@article{Cha:23,
author = {Cha, S. M. and Chae, K. Y. and Abe, K. and Bae, S. and Binh, D. N. and Choi, S. H. and Duy, N. N. and Ge, Z. and
Hahn, K. I. and Hayakawa, S. and Hong, B. and Iwasa, N. and Kahl, D. and Khiem, L. H. and Kim, A. and Kim, D. and
Kim, E. J. and Kim, G. W. and Kim, M. J. and Kwak, K. and Kwag, M. S. and Lee, E. J. and Lim, S. I. and Moon, B. and
Moon, J. Y. and Park, S. Y. and Phong, V. H. and Shimizu, H. and Yamaguchi, H. and Yang, L.},
title = {Investigation of $^{22}$Mg levels via resonant scattering of $^{18}$Ne + $\alpha$},
journal = {Frontiers in Physics},
volume = {11},
year = {2023},
url = {https://www.frontiersin.org/articles/10.3389/fphy.2023.1163299},
doi = {10.3389/fphy.2023.1163299},
issn = {2296-424X},
abstract = {The $\alpha$ resonant scattering on $^{18}$Ne was measured in inverse kinematics to understand the $\alpha$-clustering of proton-rich $^{22}$Mg nucleus, performed at the CNS Radio-Isotope Beam Separator (CRIB) of Center for Nuclear Study, University of Tokyo, located at the RIBF of RIKEN Nishina Center. The excitation function of $^{22}$Mg was obtained for the excitation energies of 10--16 MeV by adopting the thick-target method. Several resonances were evident in the present work, which implies the existence of energy levels with large $\alpha$ widths. Since energy levels were not clearly observed at the astrophysically important energy range, upper limits on the $^{18}$Ne ($\alpha$, $\alpha$)$^{18}$Ne cross section were set. The astrophysical impact was also investigated by estimating the $^{18}$Ne ($\alpha$, p)$^{21}$Na cross section.}
}

@article{10.3389/fphy.2023.1189040,
author = {Kahl, Daid and Yamaguchi, Hidetoshi and Hayakawa, Seiya},
title = {Alpha clustering in nuclear astrophysics and topology},
journal = {Frontiers in Physics},
volume = {11},
year = {2023},
url = {https://www.frontiersin.org/articles/10.3389/fphy.2023.1189040},
doi = {10.3389/fphy.2023.1189040},
issn = {2296-424X}
}

@article{Yang2022,
author = {Yang, L. and Lin, C. J. and Yamaguchi, H. and Moro, A. M. and Ma, N. R. and Wang, D. X. and Cook, K. J. and Mazzocco, M. and Wen, P. W. and Hayakawa, S. and Wang, J. S. and Yang, Y. Y. and Zhang, G. L. and Huang, Z. and Inoue, A. and Jia, H. M. and Kahl, D. and Kim, A. and Kwag, M. S. and Commara, M. La and Gu, G. M. and Okamoto, S. and Parascandolo, C. and Pierroutsakou, D. and Shimizu, H. and Sun, H. H. and Wang, M. L. and Yang, F. and Zhong, F. P.},
issue = {1},
year = {2022},
volume = {13},
journal = {Nature Communications},
title = {Breakup of the proton halo nucleus 8B near barrier energies},
pages = {7193},
doi = {10.1038/s41467-022-34767-8},
abstract = {The dynamics of a nuclear open quantum system could be revealed in the correlations between the breakup fragments of halo nuclei. The breakup mechanism of a proton halo nuclear system is of particular interest as the Coulomb polarization may play an important role, which, however, remains an open question. Here we use a highly efficient silicon detector array and measure the correlations between the breakup fragments of 8B incident on 120Sn at near-barrier energies. The energy and angular correlations can be explained by a fully quantum mechanical method based on the state-of-the-art continuum discretized coupled channel calculations. The results indicate that, compared to the neutron halo nucleus 6He, 8B presents distinctive reaction dynamics: the dominance of the elastic breakup. This breakup occurs mainly via the short-lived continuum states, almost exhausts the 7Be yield, indicating the effect of Coulomb polarization on the proton halo state. The correlation information reveals that the prompt breakup mechanism dominates, occurring predominantly on the outgoing trajectory. We also show that, as a large environment, the continuum of 8B breakup may not significantly influence elastic scattering and complete fusion.}
}

@article{Hayakawa_2021,
doi = {10.3847/2041-8213/ac061f},
url = {https://doi.org/10.3847/2041-8213/ac061f},
year = 2021,
month = {jul},
publisher = {American Astronomical Society},
volume = {915},
number = {1},
pages = {L13},
author = {S. Hayakawa and M. La Cognata and L. Lamia and H. Yamaguchi and D. Kahl and K. Abe and H. Shimizu and L. Yang and O. Beliuskina and S. M. Cha and K. Y. Chae and S. Cherubini and P. Figuera and Z. Ge and M. Gulino and J. Hu and A. Inoue and N. Iwasa and A. Kim and D. Kim and G. Kiss and S. Kubono and M. La Commara and M. Lattuada and E. J. Lee and J. Y. Moon and S. Palmerini and C. Parascandolo and S. Y. Park and V. H. Phong and D. Pierroutsakou and R. G. Pizzone and G. G. Rapisarda and S. Romano and C. Spitaleri and X. D. Tang and O. Trippella and A. Tumino and N. T. Zhang},
title = {Constraining the Primordial Lithium Abundance: New Cross Section Measurement of the 7Be$\mathplus$n Reactions Updates the Total $^7$Be Destruction Rate},
journal = {The Astrophysical Journal Letters},
abstract = {The cosmological lithium problem (CLP) stems from the outstanding discrepancy between theoretical predictions and astronomical observations of primordial lithium abundances. For the radiogenic production of 7Li, 7Be plays a pivotal role in the Big Bang nucleosynthesis (BBN). Nevertheless, the data for neutron-induced 7Be destruction processes were still sparse, and especially lacked information on the contributions of transitions to the 7Li excited states. In this work, we have determined the 7BeLi, 7BeLi*, and 7BeHe reaction cross sections by means of the Trojan Horse method. The present and the previous data were analyzed together by a multichannel R-matrix fit, providing an improved uncertainty evaluation of the channel and the first-ever quantification of the contribution in the BBN-relevant energy range. We implemented the revised total reaction rate summing both the and contributions in a state-of-the-art BBN code PRIMAT. As a consequence, the present nuclear-physics data offers a reduction of the predicted 7Li abundance by about one-tenth, which would impose a stricter constraint on BBN and head us in the correct direction to the CLP solution.}
}

@article{Hu:21,
title = {Advancement of Photospheric Radius Expansion and Clocked Type-I X-Ray Burst Models with the New $^{22}\mathrm{Mg}(\ensuremath{\alpha},p)^{25}\mathrm{Al}$ Reaction Rate Determined at the Gamow Energy},
author = {Hu, J. and Yamaguchi, H. and Lam, Y. H. and Heger, A. and Kahl, D. and Jacobs, A. M. and Johnston, Z. and Xu, S. W. and Zhang, N. T. and Ma, S. B. and Ru, L. H. and Liu, E. Q. and Liu, T. and Hayakawa, S. and Yang, L. and Shimizu, H. and Hamill, C. B. and Murphy, A. St J. and Su, J. and Fang, X. and Chae, K. Y. and Kwag, M. S. and Cha, S. M. and Duy, N. N. and Uyen, N. K. and Kim, D. H. and Pizzone, R. G. and La Cognata, M. and Cherubini, S. and Romano, S. and Tumino, A. and Liang, J. and Psaltis, A. and Sferrazza, M. and Kim, D. and Li, Y. Y. and Kubono, S.},
journal = {Phys. Rev. Lett.},
volume = {127},
issue = {17},
pages = {172701},
numpages = {7},
year = {2021},
month = {Oct},
publisher = {American Physical Society},
doi = {10.1103/PhysRevLett.127.172701},
url = {https://link.aps.org/doi/10.1103/PhysRevLett.127.172701}
}

@article{Yamaguchi:20N,
author = { Hidetoshi Yamaguchi and Daid Kahl and Shigeru Kubono},
title = {CRIB: The Low Energy In-Flight RI Beam Separator},
journal = {Nuclear Physics News International},
volume = {30},
pages = {21--27},
year = {2020}
}

@article{YANG2020136045,
title = {Insight into the reaction dynamics of proton drip-line nuclear system 17F+58Ni at near-barrier energies},
journal = {Physics Letters B},
pages = {136045},
year = {2020},
issn = {0370-2693},
doi = {https://doi.org/10.1016/j.physletb.2020.136045},
url = {http://www.sciencedirect.com/science/article/pii/S0370269320308480},
author = {L. Yang and C.J. Lin and H. Yamaguchi and Jin Lei and P.W. Wen and M. Mazzocco and N.R. Ma and L.J. Sun and D.X. Wang and G.X. Zhang and K. Abe and S.M. Cha and K.Y. Chae and A. Diaz-Torres and J.L. Ferreira and S. Hayakawa and H.M. Jia and D. Kahl and A. Kim and M.S. Kwag and M. {La Commara} and R. {Navarro Pérez} and C. Parascandolo and D. Pierroutsakou and J. Rangel and Y. Sakaguchi and C. Signorini and E. Strano and X.X. Xu and F. Yang and Y.Y. Yang and G.L. Zhang and F.P. Zhong and J. Lubian},
keywords = {Weakly bound valence-proton nucleus, Reaction dynamics, Near-barrier energies},
abstract = {The mechanism of reactions with weakly-bound proton-rich nuclei at energies near the Coulomb barrier is a long-standing open question owing to the paucity of experimental data. In this study, a complete kinematics measurement was performed for the proton drip-line nucleus 17F interacting with 58Ni at four energies near the Coulomb barrier. Thanks to the powerful performance of the detector array, exhaustive information on the reaction channels, such as the differential cross sections for quasielastic scattering, exclusive and inclusive breakup, as well as for fusion-evaporation protons and alphas, was derived for the first time. The angular distributions of quasielastic scattering and exclusive breakup can be described reasonably well by the continuum-discretized coupled-channels calculations. The inclusive breakup was investigated using the three-body model proposed by Ichimura, Austern, and Vincent, and results indicate the non-elastic breakup is the dominant component. The total fusion cross sections were determined by the fusion-evaporation protons and alphas. Based on the measured exclusive breakup data, the analysis of the classical dynamical simulation code PLATYPUS demonstrates that the incomplete fusion plays a minor role. Moreover, compared with 16O+58Ni, both the reaction and total fusion cross sections of 17F+58Ni exhibit an enhancement in the sub-barrier energy region, which mainly arises from couplings to the continuum states. This work indicates that the information of full reaction channels is crucially important to comprehensively understand the reaction mechanisms of weakly bound nuclear systems.}
}

@article{Ma2019,
author = {Ma, N. R. and Yang, L. and Lin, C. J. and Yamaguchi, H.
and Wang, D. X. and Sun, L. J. and Mazzocco, M. and Jia, H. M.
and Hayakawa, S. and Kahl, D. and Cha, S. M. and Zhang, G. X.
and Yang, F. and Yang, Y. Y. and Signorini, C. and Sakaguchi, Y.
and Abe, K. and La Commara, M. and Pierroutsakou, D. and Parascandolo, C.
and Strano, E. and Kim, A. and Chae, K. Y. and Kwag, M. S.
and Zhang, G. L. and Pan, M. and Xu, X. X. and Wen, P. W.
and Zhong, F. P. and Sun, H. H. and Guo, G.},
title = {MITA: A Multilayer Ionization-chamber Telescope Array for low-energy reactions with exotic nuclei},
journal = {The European Physical Journal A},
year = {2019},
month = {Jun},
day = {07},
volume = {55},
number = {6},
pages = {87},
abstract = {We report on the development of a new, portable detector array for charged particles with a low detection threshold to study the reaction mechanisms of exotic nuclear systems at energies around the Coulomb barrier. In order to identify both light and heavy particles simultaneously, the array consists of ten units of $\Delta$E-E telescopes, where each one is made up of four detection layers: one ionization chamber, one 40 (or 60)$\mu$m double-sided silicon strip detector and two quadrant silicon detectors with thicknesses of 300$\mu$m and 1000 (or 1500)$\mu$m, respectively. The frame of the ionization chamber is innovatively designed with printed circuit boards, thus the mass of each telescopic unit was reduced significantly which eases transport and installation requirements to different radioactive ion beam lines around the globe. The commissioning experiments focused on elucidating several reaction mechanisms encountered in the 17F + 58Ni and 17F + 208Pb systems, and we demonstrated that the array has a sufficient capability to enable charged particle identification over a large range of Z. Light particles like p, d, $\alpha$ as well as heavy ions like 16O and 17F can be clearly distinguished. Considering these properties, this newly developed array enables in-depth investigation of the novel reaction mechanisms which are manifested in the collisions of exotic nuclei with differing isotopes.},
issn = {1434-601X},
doi = {10.1140/epja/i2019-12765-7},
url = {https://doi.org/10.1140/epja/i2019-12765-7}
}

@article{PhysRevC.100.024602,
title = {Elastic scattering for the $^{8}\mathrm{B}$ and $^{7}\mathrm{Be}+^{208}\mathrm{Pb}$ systems at near-Coulomb barrier energies},
author = {Mazzocco, M. and Keeley, N. and Boiano, A. and Boiano, C. and La Commara, M. and Manea, C. and Parascandolo, C. and Pierroutsakou, D. and Signorini, C. and Strano, E. and Torresi, D. and Yamaguchi, H. and Kahl, D. and Acosta, L. and Di Meo, P. and Fernandez-Garcia, J. P. and Glodariu, T. and Grebosz, J. and Guglielmetti, A. and Hirayama, Y. and Imai, N. and Ishiyama, H. and Iwasa, N. and Jeong, S. C. and Jia, H. M. and Kim, Y. H. and Kimura, S. and Kubono, S. and La Rana, G. and Lin, C. J. and Lotti, P. and Marqu\'{\i}nez-Dur\'an, G. and Martel, I. and Miyatake, H. and Mukai, M. and Nakao, T. and Nicoletto, M. and Pakou, A. and Rusek, K. and Sakaguchi, Y. and S\'anchez-Ben\'{\i}tez, A. M. and Sava, T. and Sgouros, O. and Soukeras, V. and Soramel, F. and Stiliaris, E. and Stroe, L. and Teranishi, T. and Toniolo, N. and Wakabayashi, Y. and Watanabe, Y. X. and Yang, L. and Yang, Y. Y. and Zhang, H. Q.},
journal = {Phys. Rev. C},
volume = {100},
issue = {2},
pages = {024602},
numpages = {13},
year = {2019},
month = {Aug},
publisher = {American Physical Society},
doi = {10.1103/PhysRevC.100.024602},
url = {https://link.aps.org/doi/10.1103/PhysRevC.100.024602}
}

@article{Kahl:18,
title = {First measurement of $^{30}\mathrm{S}+\alpha$ resonant elastic scattering for the $^{30}\mathrm{S}(\alpha,p)$ reaction rate},
author = {Kahl, D. and Yamaguchi, H. and Kubono, S. and Chen, A. A. and Parikh, A. and Binh, D. N. and Chen, J. and Cherubini, S. and Duy, N. N. and Hashimoto, T. and Hayakawa, S. and Iwasa, N. and Jung, H. S. and Kato, S. and Kwon, Y. K. and Nishimura, S. and Ota, S. and Setoodehnia, K. and Teranishi, T. and Tokieda, H. and Yamada, T. and Yun, C. C. and Zhang, L. Y.},
journal = {Phys. Rev. C},
volume = {97},
issue = {1},
pages = {015802},
numpages = {16},
year = {2018},
month = {Jan},
publisher = {American Physical Society},
doi = {10.1103/PhysRevC.97.015802},
url = {https://link.aps.org/doi/10.1103/PhysRevC.97.015802}
}

@article{DUY20188,
title = {Beam production of ?18Ne with in-flight method for alpha scattering at CRIB},
journal = {Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment},
volume = {897},
pages = {8 - 13},
year = {2018},
issn = {0168-9002},
doi = {https://doi.org/10.1016/j.nima.2018.04.043},
url = {http://www.sciencedirect.com/science/article/pii/S0168900218305503},
author = {N.N. Duy and K.Y. Chae and S.M. Cha and H. Yamaguchi and K. Abe and S.H. Bae and D.N. Binh and S.H. Choi and K.I. Hahn and S. Hayakawa and B. Hong and N. Iwasa and D. Kahl and L.H. Khiem and A. Kim and D.H. Kim and E.J. Kim and G.W. Kim and M.J. Kim and K. Kwak and M.S. Kwag and E.J. Lee and S.I. Lim and B. Moon and J.Y. Moon and S.Y. Park and V.H. Phong and H. Shimizu and L. Yang and Z. Ge and T.V. Nhan Hao},
keywords = {RI beam production, Alpha scatring, Inverse kinematics, Alpha cluste
},
abstract = {We conducted a measurement of 18Ne + $\alpha$ scattering in inverse kinematics,
in order to search for experimental evidence of $\alpha$-cluster structure in $^{22}$Mg above the alpha threshold
($E_\mathrm{thr}$ = 8.14MeV) and determine the astrophysical rates of the $^{18}$Ne($\alpha$, $p$)$^{21}$Na reaction under the conditions of break-out from the Hot-CNO cycle. A high intensity $^{18}$Ne beam at 2.54 AMeV was
successfully produced at CRIB (CNS Radioactive Ion Beam separator) of
the Center for Nuclear Study, the University of Tokyo.
This paper presents the in-flight production of the radioactive
18Ne beam by using the production reaction $^3$He($^{16}$O, $^{18}$Ne)$n$ with
a windowed cryogenic gas target, which was employed in the mentioned resonant $\alpha$-scattering experiment.}
}

@article{Kim2018,
author = {Kim, D.
and Kim, G. W.
and Park, S. Y.
and Kim, A.
and Hahn, K. I.
and Abe, K.
and Beliuskina, O.
and Hayakawa, S.
and Imai, N.
and Kitamura, N.
and Sakaguchi, Y.
and Yamaguchi, H.
and Cha, S. M.
and Chae, K. Y.
and Kwag, M. S.
and Hong, S. W.
and Lee, E. J.
and Lee, J. H.
and Lee, E. K.
and Moon, J. Y.
and Bae, S. H.
and Choi, S. H.
and Kubono, S.
and Panin, V.
and Wakabayashi, Y.
and Iwasa, N.
and Kahl, D.
and Chen, A. A.},
title = {Study of 19F Levels with Ex = 6.7 - 7.7 MeV by the 15N+$\alpha$ Scattering Experiment},
journal = {Journal of the Korean Physical Society},
year = {2018},
month = {Aug},
day = {01},
volume = {73},
number = {3},
pages = {265--270},
abstract = {The intense $\gamma$-rays from classical novae are emitted due to the $\beta$-decay of 18F which is produced by the Hot-CNO cycle. The reaction rate of 18F(p,$\alpha$)15O affects the prediction of the abundance of 18F. The main contribution to this reaction rate is from the resonances in 19Ne near and above the proton threshold. Hence, many experiments and theoretical works have been performed on the low-lying 18F+p resonances. One of the methods for investigating 19Ne parameters is studying the mirror nucleus 19F. $\alpha$ elastic scattering experiment was performed with a 7 MeV/u 15N beam for investigating the resonance parameters in 19F using the thick target method in inverse kinematics at the radioactive beam facility CRIB of the Center for Nuclear Study, the University of Tokyo. The excitation function of 19F was obtained for the excitation energy Ex = 6.7 - 7.7 MeV, and the parameters of the resonance states in 19F were determined using an R-matrix analysis.},
issn = {1976-8524},
doi = {10.3938/jkps.73.265},
url = {https://doi.org/10.3938/jkps.73.265}
}

@article{Cha2018,
author = {Cha, S. M.
and Chae, K. Y.
and Kim, M. J.
and Kwag, M. S.
and Lee, E. J.
and Abe, K.
and Hayakawa, S.
and Shimizu, H.
and Yamaguchi, H.
and Yang, L.
and Bae, S. H.
and Choi, S. H.
and Binh, D. N.
and Duy, N. N.
and Ge, Z.
and Phong, V. H.
and Hahn, K. I.
and Hong, B.
and Moon, B.
and Iwasa, N.
and Kahl, D.
and Khiem, L. H.
and Kim, A.
and Kim, D. H.
and Kim, G. W.
and Lim, S. I.
and Park, S. Y.
and Kim, E. J.
and Kwak, K.
and Moon, J. Y.},
title = {Study of $\alpha$-cluster Structure in 22Mg Using a Radioactive Ion Beam},
journal = {Journal of the Korean Physical Society},
year = {2018},
month = {Oct},
day = {01},
volume = {73},
number = {8},
pages = {1055--1060},
abstract = {The $\alpha$-clusterization of an atomic nucleus has been studied for a long time, even from the earliest days of nuclear physics. Our understanding of the $\alpha$-cluster structure is, however, mainly limited to the self-conjugate A = 4n (n = 2, 3, 4, ... ) light nuclei and some of the neutron-rich radionuclides such as 10Be, 11B, and 14C. In order to study the $\alpha$-cluster structure of a neutron-deficient 22Mg nucleus, we have measured the 18Ne($\alpha$, $\alpha$)18Ne scattering in inverse kinematics by using radioactive 18Ne beams and the 4He gas target at the Center for Nuclear Study radioactive ion beam separator of the University of Tokyo. Recoiling $\alpha$ particles from the scattering were detected by using silicon strip detectors, which constitute $\Delta$E-E telescopes for particle identification. By adopting a thick target method, we were able to investigate a
wide range of excitation energies $Ex$ = 9.9 - 16.5 MeV in 22Mg in this work.},
issn = {1976-8524},
doi = {10.3938/jkps.73.1055},
url = {https://doi.org/10.3938/jkps.73.1055}
}

@article{Yamaguchi:2017,
title = {Experimental investigation of a linear-chain structure in the nucleus $^{14}$C },
journal = {Physics Letters B },
volume = {766},
number = {},
pages = {11 - 16},
year = {2017},
note = {},
issn = {0370-2693},
doi = {http://dx.doi.org/10.1016/j.physletb.2016.12.050},
url = {http://www.sciencedirect.com/science/article/pii/S0370269316307961},
author = {H. Yamaguchi and D. Kahl and S. Hayakawa and Y. Sakaguchi and K. Abe and T. Nakao and T. Suhara and N. Iwasa and A. Kim and D.H. Kim and S.M. Cha and M.S. Kwag and J.H. Lee and E.J. Lee and K.Y. Chae and Y. Wakabayashi and N. Imai and N. Kitamura and P. Lee and J.Y. Moon and K.B. Lee and C. Akers and H.S. Jung and N.N. Duy and L.H. Khiem and C.S. Lee},
keywords = {Nuclear cluster},
keywords = {Linear-chain cluster state},
keywords = {Resonant elastic scattering},
keywords = {Thick-target method in inverse kinematics},
keywords = {RI beam },
abstract = {Abstract It is a well-known fact that a cluster of nucleons can be formed in the interior of an atomic nucleus, and such clusters may occupy molecular-like orbitals, showing characteristics similar to normal molecules consisting of atoms. Chemical molecules having a linear alignment are commonly seen in nature, such as carbon dioxide. A similar linear alignment of the nuclear clusters, referred to as linear-chain cluster state (LCCS), has been studied since the 1950s, however, up to now there is no clear experimental evidence demonstrating the existence of such a state. Recently, it was proposed that an excess of neutrons may offer just such a stabilizing mechanism, revitalizing interest in the nuclear LCCS, specifically with predictions for their emergence in neutron-rich carbon isotopes.
Here we present the experimental observation of $\alpha$-cluster states in the radioactive $^14$C nucleus.
Using the $^{10}$Be + $\alpha$ resonant scattering method with a radioactive beam, we observed a series of levels
which completely agree with theoretically predicted level having an explicit linear-chain cluster configuration.
We regard this as the first strong indication of the linear-chain clustered nucleus. }
}

@article{Hayakawa:16,
title = {First direct measurement of the $^{11}\mathrm{C}($\alpha$,p)^{14}\mathrm{N}$ stellar reaction by an extended thick-target method},
author = {Hayakawa, S. and Kubono, S. and Kahl, D. and Yamaguchi, H. and Binh, D. N. and Hashimoto, T. and Wakabayashi, Y. and He, J. J. and Iwasa, N. and Kato, S. and Komatsubara, T. and Kwon, Y. K. and Teranishi, T.},
journal = {Phys. Rev. C},
volume = {93},
issue = {6},
pages = {065802},
numpages = {8},
year = {2016},
month = {Jun},
publisher = {American Physical Society},
doi = {10.1103/PhysRevC.93.065802},
url = {http://link.aps.org/doi/10.1103/PhysRevC.93.065802}
}

@article{Cherubini:15,
title = {First application of the Trojan horse method with a radioactive ion beam: Study of the ${}^{18}\mathrm{F}{(p,$\alpha$)}^{15}\mathrm{O}$ reaction at astrophysical energies},
author = {Cherubini, S. and Gulino, M. and Spitaleri, C. and Rapisarda, G. G. and La Cognata, M. and Lamia, L. and Pizzone, R. G. and Romano, S. and Kubono, S. and Yamaguchi, H. and Hayakawa, S. and Wakabayashi, Y. and Iwasa, N. and Kato, S. and Komatsubara, T. and Teranishi, T. and Coc, A. and de S\'er\'eville, N. and Hammache, F. and Kiss, G. and Bishop, S. and Binh, D. N.},
journal = {Phys. Rev. C},
volume = {92},
issue = {1},
pages = {015805},
numpages = {7},
year = {2015},
month = {Jul},
publisher = {American Physical Society},
doi = {10.1103/PhysRevC.92.015805},
url = {http://link.aps.org/doi/10.1103/PhysRevC.92.015805}
}

@article{Kim:15,
title = {Measurement of the $^{14}\mathrm{O}(\alpha,p)^{17}\mathrm{F}$ cross section at ${E}_{\mathrm{c}.\mathrm{m}.}$ $\approx$2.1-5.3 MeV},
author = {Kim, A. and Lee, N. H. and Han, M. H. and Yoo, J. S. and Hahn, K. I. and Yamaguchi, H. and Binh, D. N. and Hashimoto, T. and Hayakawa, S. and Kahl, D. and Kawabata, T. and Kurihara, Y. and Wakabayashi, Y. and Kubono, S. and Choi, S. and Kwon, Y. K. and Moon, J. Y. and Jung, H. S. and Lee, C. S. and Teranishi, T. and Kato, S. and Komatsubara, T. and Guo, B. and Liu, W. P. and Wang, B. and Wang, Y.},
journal = {Phys. Rev. C},
volume = {92},
issue = {3},
pages = {035801},
numpages = {7},
year = {2015},
month = {Sep},
publisher = {American Physical Society},
doi = {10.1103/PhysRevC.92.035801},
url = {http://link.aps.org/doi/10.1103/PhysRevC.92.035801}
}

@article{2015JKPS...66..459L,
title = {Development and performance test of the analysis software for the CRIB active target},
author = {{Lee}, P. and {Lee}, C.~S. and {Moon}, J.~Y. and {Chae}, K.~Y. and {Cha},
S.~M. and {Yamaguchi}, H. and {Nakao}, T. and {Kahl}, D.~M. and {Kubono}, S. and {Cherubini}, S. and {Hayakawa}, S. and {Signorini}, C. },
journal = {Journal of Korean Physical Society},
year = {2015},
month = feb,
pages = {459-464},
volume = {66},
abstract = {Software for genuinely event-by-event analysis and event reconstruction of data obtained by using an active target
has been developed in the graphical user interface under the CERN ROOT framework.
The primary motivation for developing the software was to provide physicists
who perform experiments using an active target a more user-friendly environment for
the purpose of investigating the performance of detection systems and obtaining
ideas about physics from a large amount of experimental data. To test the performance of
the software, we analyzed experimental data from a 16N radioactive ion beam experiment for
$\alpha$-decay measurements. As a result of the analysis, we observed the Bragg curve and
measured the range of the 16N RI beam in the detector. Data were calibrated against the
calculation after comparing the Bragg curve to the one obtained from an energy loss calculation
in P-10 gas. We present a detailed description of the analysis software and its test results.},
adsurl = {http://adsabs.harvard.edu/abs/2015JKPS...66..459L},
doi = {10.3938/jkps.66.459},
keywords = {GEM-MSTPC, CRIB, MSTPC, Active target}
}

@article{2014PhRvC..89a5804Z,
title = {{Investigation of the thermonuclear $^{18}$Ne({$\alpha$},p)$^{21}$Na reaction rate via resonant elastic scattering of $^{21}$Na + p}},
author = {{Zhang}, L.~Y. and {He}, J.~J. and {Parikh}, A. and {Xu}, S.~W. and
{Yamaguchi}, H. and {Kahl}, D. and {Kubono}, S. and {Mohr}, P. and
{Hu}, J. and {Ma}, P. and {Chen}, S.~Z. and {Wakabayashi}, Y. and
{Wang}, H.~W. and {Tian}, W.~D. and {Chen}, R.~F. and {Guo}, B. and
{Hashimoto}, T. and {Togano}, Y. and {Hayakawa}, S. and {Teranishi}, T. and
{Iwasa}, N. and {Yamada}, T. and {Komatsubara}, T. and {Zhang}, Y.~H. and
{Zhou}, X.~H.},
journal = {\prc},
year = {2014},
month = jan,
number = {1},
pages = {015804},
volume = {89},
abstract = {{The $^{18}$Ne({$\alpha$},p)$^{21}$Na reaction is thought to be one of the key breakout reactions from the hot CNO cycles to the rp process in type I x-ray bursts. In this work, the resonant properties of
the compound nucleus $^{22}$Mg have been investigated by measuring the resonant elastic scattering of $^{21}$Na + p. An 89-MeV $^{21}$Na radioactive beam delivered from the CNS Radioactive Ion Beam Separator bombarded an 8.8 mg/cm$^{2}$ thick polyethylene (CH$_{2}$)n target. The $^{21}$Na beam intensity was about 2{\times}10$^{5}$ pps, with a purity of about 70\% on target. The recoiled protons were measured at the center-of-mass scattering angles of {\theta}$_{c.m.}${\approx}175.2$^{\circ}$, 152.2$^{\circ}$, and 150.5$^{\circ}$ by three sets of {$\Delta$}E-E telescopes, respectively. The excitation function was obtained with the thick-target method over energies E$_{x}$($^{22}$Mg)=5.5-9.2 MeV. In total, 23 states above the proton-threshold in $^{22}$Mg were observed, and their resonant parameters were determined via an R-matrix analysis of the excitation functions. We have made several new J$^{\pi}$ assignments and confirmed some tentative assignments made in previous work. The thermonuclear $^{18}$Ne({$\alpha$},p)$^{21}$Na rate has been recalculated based on our recommended spin-parity assignments. The astrophysical impact of our new rate has been investigated through one-zone postprocessing x-ray burst calculations. We find that the $^{18}$Ne({$\alpha$},p)$^{21}$Na rate significantly affects the peak nuclear energy generation rate, reaction fluxes, and onset temperature of this breakout reaction in these astrophysical phenomena.}},
adsurl = {http://adsabs.harvard.edu/abs/2014PhRvC..89a5804Z},
archiveprefix = {arXiv},
doi = {10.1103/PhysRevC.89.015804},
eid = {015804},
eprint = {1403.4668},
keywords = {Reactions induced by unstable nuclei, Decay by proton emission, Nuclear physics aspects of novae supernovae and other explosive environments, 20\<, =A\<, =38},
owner = {daid},
primaryclass = {astro-ph.SR},
timestamp = {2014.04.24}
}

@article{Hu:14,
title = {Examination of the role of the $^{14}\mathrm{O}($\alpha${},p)^{17}\mathrm{F}$ reaction rate in type-I x-ray bursts},
author = {Hu, J. and He, J. J. and Parikh, A. and Xu, S. W. and Yamaguchi, H. and Kahl, D. and Ma, P. and Su, J. and Wang, H. W. and \
Nakao, T. and Wakabayashi, Y. and Teranishi, T. and Hahn, K. I. and Moon, J. Y. and Jung, H. S. and Hashimoto, T. and Chen, A. A. and I\
rvine, D. and Lee, C. S. and Kubono, S.},
journal = {Phys. Rev. C},
volume = {90},
issue = {2},
pages = {025803},
numpages = {7},
year = {2014},
month = {Aug},
publisher = {American Physical Society},
doi = {10.1103/PhysRevC.90.025803},
url = {http://link.aps.org/doi/10.1103/PhysRevC.90.025803}
}

@article{Jung:14,
title = {Elastic scattering of $^{25}\mathrm{Al}+p$ to explore the resonance structure in $^{26}\mathrm{Si}$},
author = {Jung, H. S. and Lee, C. S. and Kwon, Y. K. and Moon, J. Y. and Lee, J. H. and Yun, C. C. and Kim, M. J. and Hashimoto, T. a\
nd Yamaguchi, H. and Kahl, D. and Kubono, S. and Wakabayashi, Y. and Togano, Y. and Choi, Seonho and Kim, Y. H. and Kim, Y. K. and Park\
, J. S. and Kim, E. J. and Moon, C.-B. and Teranishi, T. and Iwasa, N. and Yamada, T. and Kato, S. and Cherubini, S. and Hayakawa, S. a\
nd Rapisarda, G. G.},
journal = {Phys. Rev. C},
volume = {90},
issue = {3},
pages = {035805},
numpages = {8},
year = {2014},
month = {Sep},
publisher = {American Physical Society},
doi = {10.1103/PhysRevC.90.035805},
url = {http://link.aps.org/doi/10.1103/PhysRevC.90.035805}
}

@article{PhysRevC.87.015803,
title = {{Determination of astrophysical $^{12}$N(p,$\gamma$)$^{13}$O reaction rate from the $^{2}$H($^{12}$N, $^{13}$O)n reaction and its astrophysical implications}},
author = {{Guo}, B. and {Su}, J. and {Li}, Z. and {Wang}, Y.~B. and {Yan}, S.~Q. and {Li}, Y.~J. and {Shu}, N.~C. and {Han}, Y.~L. and {Bai}, X.~X. and {Chen}, Y.~S. and {Liu}, W.~P. and {Yamaguchi}, H. and {Binh}, D.~N. and {Hashimoto}, T. and {Hayakawa}, S. and {Kahl}, D. and {Kubono}, S. and {He}, J.~J. and {Hu}, J. and {Xu}, S.~W. and {Iwasa}, N. and {Kume}, N. and {Li}, Z.},
journal = {\prc},
year = {2013},
month = nov,
pages = {015803},
volume = {87},
abstract = {The evolution of massive stars with very low-metallicities depends critically on the amount of CNO nuclides which they produce. The $^{12}$N(p,$\gamma$)$^{13}$O reaction is an important branching point in the rap processes, which are believed to be alternative paths to the slow 3α process for producing CNO seed nuclei and thus could change the fate of massive stars. In the present work, the angular distribution of the $^{2}$H($^{12}$N, $^{13}$O)n proton transfer reaction at E$_{c.m.}$=8.4 MeV has been measured for the first time. Based on the Johnson-Soper approach, the square of the asymptotic normalization coefficient (ANC) for the virtual decay of $^{13}$O$_{g.s.}$ → $^{12}$N+p was extracted to be 3.92 ± 1.47 fm$^{-1}$ from the measured angular distribution and utilized to compute the direct component in the $^{12}$N(p,$\gamma$)$^{13}$O reaction. The direct astrophysical S factor at zero energy was then found to be 0.39 ± 0.15 keV b. By considering the direct capture into the ground state of $^{13}$O, the resonant capture via the first excited state of $^{13}$O and their interference, we determined the total astrophysical S factors and rates of the $^{12}$N(p,$\gamma$)$^{13}$O reaction. The new rate is two orders of magnitude slower than that from the REACLIB compilation. Our reaction network calculations with the present rate imply that $^{12}$N(p,$\gamma$)$^{13}$O will only compete successfully with the $\beta^{+}$ decay of $^{12}$N at higher (∼2 orders of magnitude) densities than initially predicted.},
adsurl = {http://adsabs.harvard.edu/abs/2012arXiv1211.4972G},
archiveprefix = {arXiv},
doi = {10.1103/PhysRevC.87.015803},
eprint = {1211.4972},
issue = {1},
keywords = {Nuclear Experiment},
owner = {daid},
primaryclass = {nucl-ex},
timestamp = {2013.05.08}
}

@article{2013PhRvC..88a2801H,
title = {{The $^{18}$Ne({$\alpha$},p)$^{21}$Na breakout reaction in x-ray bursts: Experimental determination of spin-parities for {$\alpha$} resonances in $^{22}$Mg via resonant elastic scattering of $^{21}$Na+p}},
author = {{He}, J.~J. and {Zhang}, L.~Y. and {Parikh}, A. and {Xu}, S.~W. and {Yamaguchi}, H. and {Kahl}, D. and {Kubono}, S. and {Hu}, J. and {Ma}, P. and {Chen}, S.~Z. and {Wakabayashi}, Y. and {Sun}, B.~H. and {Wang}, H.~W. and {Tian}, W.~D. and {Chen}, R.~F. and {Guo}, B. and {Hashimoto}, T. and {Togano}, Y. and {Hayakawa}, S. and {Teranishi}, T. and {Iwasa}, N. and {Yamada}, T. and {Komatsubara}, T.},
journal = {\prc},
year = {2013},
month = jul,
number = {1},
pages = {012801},
volume = {88},
abstract = {{The $^{18}$Ne({$\alpha$},p)$^{21}$Na reaction provides a pathway for breakout from the hot CNO cycles to the rp process in type-I x-ray bursts. To better determine this astrophysical reaction rate, the resonance parameters of the compound nucleus $^{22}$Mg have been investigated by measuring the resonant elastic scattering of $^{21}$Na+p. An 89 MeV $^{21}$Na radioactive ion beam was produced at the CNS Radioactive Ion Beam Separator and bombarded an 8.8 mg/cm$^{2}$ thick polyethylene target. The recoiled protons were measured at scattering angles of {\theta}$_{c.m.}${\approx}175$^{o}$ and 152$^{o}$ by three {$\Delta$}E-E silicon telescopes. The excitation function was obtained with a thick-target method over energies E$_{x}$($^{22}$Mg) = 5.5--9.2 MeV. The resonance parameters have been determined through an R-matrix analysis. For the first time, the J$^{pi}$ values for ten states above the {$\alpha$} threshold in $^{22}$Mg have been experimentally determined in a single consistent measurement. We have made three new J$^{pi}$ assignments and confirmed seven of the ten tentative assignments in the previous work. The $^{18}$Ne({$\alpha$},p)$^{21}$Na reaction rate has been recalculated, and the astrophysical impact of our new rate has been investigated through one-zone postprocessing x-ray burst calculations. We find that the $^{18}$Ne({$\alpha$},p)$^{21}$Na rate significantly affects the peak nuclear energy generation rate and the onset temperature of this breakout reaction in these phenomena. }},
adsurl = {http://adsabs.harvard.edu/abs/2013PhRvC..88a2801H},
archiveprefix = {arXiv},
doi = {10.1103/PhysRevC.88.012801},
eid = {012801},
eprint = {1301.4283},
keywords = {Reactions induced by unstable nuclei, Decay by proton emission, Nuclear physics aspects of novae, supernovae, and other explosive environments, 20{\lt}=A{\lt}=38},
owner = {daid},
primaryclass = {astro-ph.SR},
timestamp = {2013.11.13}
}

@article{2013PhRvC..88c5801J,
title = {{Resonant scattering of $^{22}$Na + p studied by the thick-target inverse-kinematic method}},
author = {{Jin}, S.~J. and {Wang}, Y.~B. and {Su}, J. and {Yan}, S.~Q. and {Li}, Y.~J. and {Guo}, B. and {Li}, Z.~H. and {Zeng}, S. and {Lian}, G. and {Bai}, X.~X. and {Liu}, W.~P. and {Yamaguchi}, H. and {Kubono}, S. and {Hu}, J. and {Kahl}, D. and {Jung}, H.~S. and {Moon}, J.~Y. and {Lee}, C.~S. and {Teranishi}, T. and {Wang}, H.~W. and {Ishiyama}, H. and {Iwasa}, N. and {Komatsubara}, T. and {Brown}, B.~A.},
journal = {\prc},
year = {2013},
month = sep,
number = {3},
pages = {035801},
volume = {88},
abstract = {{Background: In presolar low-density graphite grains, an extraordinarily large $^{22}$Ne/$^{20}$Ne ratio or even nearly pure $^{22}$Ne is found, pointing to the condensation of radioactive $^{22}$Na in grains. Supernovae and neon-rich novae are the main events that produce $^{22}$Na via the explosive hydrogen burning process. The $^{22}$Na(p, {$\gamma$})$^{23}$Mg reaction is one of the key reactions that influences the $^{22}$Na abundance in ejecta.Purpose:The present work aims to explore the proton resonant states in $^{23}$Mg relevant to the astrophysical $^{22}$Na(p, {$\gamma$})$^{23}$Mg reaction. The determined $^{23}$Mg resonant parameters can be used to evaluate the $^{22}$Na(p, {$\gamma$})$^{23}$Mg reaction rate.Method:A low-energy $^{22}$Na radioactive ion beam is produced via the $^{1}$H($^{22}$Ne, $^{22}$Na)n reaction, and used to measure the experimental excitation function of the $^{22}$Na + p resonant scattering with a conventional thick-target inverse kinematic method. R-matrix analysis is applied to deduce the $^{23}$Mg resonance parameters from the experimental excitation function.Results: Three proton resonance states in $^{23}$Mg are observed. Spins/parities and the proton partial widths are determined. The deduced excitation energies agree with the compiled values.Conclusions: The new spin and parity assignments allow us to perform a shell-model calculation of the {$\gamma$} widths of the $^{23}$Mg resonant states for the evaluation of the $^{22}$Na(p, {$\gamma$})$^{23}$Mg astrophysical reaction rate. The two s-wave resonant states established in this work at 8.793 and 8.916 MeV in $^{23}$Mg, respectively, increase the total reaction rate by about 5\% at a temperature greater than 2 GK. }},
adsurl = {http://adsabs.harvard.edu/abs/2013PhRvC..88c5801J},
doi = {10.1103/PhysRevC.88.035801},
eid = {035801},
keywords = {Reactions induced by unstable nuclei, Elastic proton scattering, Nuclear physics aspects of novae supernovae and other explosive environments, 20\<, =A\<, =38},
owner = {daid},
timestamp = {2013.11.13}
}

@article{2013PhRvC..87c4303Y,
title = {{{$\alpha$}-resonance structure in $^{11}$C studied via resonant scattering of $^{7}$Be+{$\alpha$} and with the $^{7}$Be({$\alpha$},p) reaction}},
author = {{Yamaguchi}, H. and {Kahl}, D. and {Wakabayashi}, Y. and {Kubono}, S. and {Hashimoto}, T. and {Hayakawa}, S. and {Kawabata}, T. and {Iwasa}, N. and {Teranishi}, T. and {Kwon}, Y.~K. and {Binh}, D.~N. and {Khiem}, L.~H. and {Duy}, N.~N.},
journal = {\prc},
year = {2013},
month = mar,
number = {3},
pages = {034303},
volume = {87},
abstract = {{{\bf Background:} The resonance structure in $^{11}$C is of particular interest with regard to the astrophysical $^{7}$Be({$\alpha$},{$\gamma$}) reaction, relevant at high temperature, and to the {$\alpha$}-cluster structure in $^{11}$C.\\ {\bf Purpose:} The measurement was made to determine the unknown resonance parameters for the high excited states of $^{11}$C. In particular, the {$\alpha$}-decay width can be useful information to discuss the {$\alpha$}-cluster structure in $^{11}$C. \\{\bf Methods:} New measurements of $^{7}$Be+{$\alpha$} resonant scattering and the $^{7}$Be({$\alpha$},p)$^{10}$B reaction in inverse kinematics were performed for center-of-mass energy up to 5.5 MeV, and the resonances at excitation energies of 8.9--12.7 MeV in the compound $^{11}$C nucleus were studied. Inelastic scattering of $^{7}$Be+{$\alpha$} and the $^{7}$Be({$\alpha$},p$_{1}$)$^{10}$B$^{*}$ reaction were also studied with a simultaneous {$\gamma$}-ray measurement. The measurements were performed at the low-energy radioactive ion beam facility CRIB (CNS Radioactive Ion Beam separator) of the Center for Nuclear Study, the University of Tokyo.\\ {\bf Results}: We obtained excitation functions of $^{7}$Be({$\alpha$},{$\alpha$}$_{0}$)$^{7}$Be (elastic scattering), $^{7}$Be({$\alpha$},{$\alpha$}$_{1}$)$^{7}$Be$^{*}$ (inelastic scattering), $^{7}$Be({$\alpha$},p$_{0}$)$^{10}$B, and $^{7}$Be({$\alpha$},p$_{1}$)$^{10}$B$^{*}$. Many resonances including a new one were observed and their parameters were determined by using an R-matrix analysis.\\ {\bf Conclusions:} The resonances we observed possibly enhance the $^{7}$Be({$\alpha$},{$\gamma$}) reaction rate but with a smaller magnitude than the lower-lying resonances. A new negative-parity cluster band, similar to the one previously suggested in the mirror nucleus $^{11}$B, is proposed. }},
adsurl = {http://adsabs.harvard.edu/abs/2013PhRvC..87c4303Y},
archiveprefix = {arXiv},
doi = {10.1103/PhysRevC.87.034303},
eid = {034303},
eprint = {1212.5991},
keywords = {$^{3}$H-, $^{3}$He-, and $^{4}$He-induced reactions, Resonance reactions, Cluster models, 6{\lt}=A{\lt}=19},
owner = {daid},
primaryclass = {nucl-ex},
timestamp = {2013.05.08}
}

@article{2012PhRvC..85a5805C,
title = {{Strong $^{25}$Al+p resonances via elastic proton scattering with a radioactive $^{25}$Al beam}},
author = {{Chen}, J. and {Chen}, A.~A. and {Am{\'a}dio}, G. and {Cherubini}, S. and {Fujikawa}, H. and {Hayakawa}, S. and {He}, J.~J. and {Iwasa}, N. and {Kahl}, D. and {Khiem}, L.~H. and {Kubono}, S. and {Kurihara}, S. and {Kwon}, Y.~K. and {La Cognata}, M. and {Moon}, J.~Y. and {Niikura}, M. and {Nishimura}, S. and {Pearson}, J. and {Pizzone}, R.~G. and {Teranishi}, T. and {Togano}, Y. and {Wakabayashi}, Y. and {Yamaguchi}, H.},
journal = {\prc},
year = {2012},
month = jan,
number = {1},
pages = {015805},
volume = {85},
abstract = {{$^{25}$Al+p elastic scattering in inverse kinematics was measured to explore the level structure of $^{26}$Si above its proton threshold. The $^{2}$H($^{24}$Mg,n)$^{25}$Al reaction was used to produce a 3.4 MeV/nucleon $^{25}$Al radioactive beam with intensities of about 10$^{6}$ ions per second on target. By using a thick target of (CH$_{2}$)$_{n}$, a center-of-mass energy range of 3 MeV was scanned, reaching up to about 8.5 MeV in excitation energy in $^{26}$Si. This energy range covered the region of importance for the $^{25}$Al(p,{$\gamma$})$^{26}$Si at temperatures characteristic of explosive nucleosynthesis. Level parameters of six strong s-wave $^{25}$Al+p resonances in $^{26}$Si were extracted from fits to the measured excitation functions using the R-matrix formalism. Two new levels have been discovered, while for two others, our spin-parity assignments disagree with the results of some previous studies. Lastly, our resonance parameters for the remaining two levels are in good agreement with past experimental work, and with recent shell-model calculations. }},
adsurl = {http://adsabs.harvard.edu/abs/2012PhRvC..85a5805C},
doi = {10.1103/PhysRevC.85.015805},
eid = {015805},
keywords = {gamma transitions and level energies, Nucleosynthesis in novae, supernovae, and other explosive environments, Radiative capture, 20{\lt}=A{\lt}=38}
}

@article{2012PhRvC..85d5802J,
title = {{Experimental study of resonant states in $^{27}$P via elastic scattering of $^{26}$Si+p}},
author = {{Jung}, H.~S. and {Lee}, C.~S. and {Kwon}, Y.~K. and {Moon}, J.~Y. and {Lee}, J.~H. and {Yun}, C.~C. and {Kubono}, S. and {Yamaguchi}, H. and {Hashimoto}, T. and {Kahl}, D. and {Hayakawa}, S. and {Choi}, S. and {Kim}, M.~J. and {Kim}, Y.~H. and {Kim}, Y.~K. and {Park}, J.~S. and {Kim}, E.~J. and {Moon}, C.-B. and {Teranishi}, T. and {Wakabayashi}, Y. and {Iwasa}, N. and {Yamada}, T. and {Togano}, Y. and {Kato}, S. and {Cherubini}, S. and {Rapisarda}, G.~G.},
journal = {\prc},
year = {2012},
month = apr,
number = {4},
pages = {045802},
volume = {85},
abstract = {{Proton resonant states in $^{27}$P were studied by the resonant elastic scattering of $^{26}$Si+p with a $^{26}$Si radioactive ion beam bombarding a thick H$_{2}$ gas target with the inverse kinematics method. The properties of these resonance states are important to better constrain the production rates of the $^{26}$Si(p,{$\gamma$})$^{27}$P reaction. This is one of the astrophysically important reactions needed to understand proton-rich nucleosynthesis such as the galactic production of $^{26}$Al and energy generation in explosive stellar environments. Although there are recent studies on the resonant structure in $^{27}$P, large uncertainties remain, and only a few levels are known. In this work, resonant states were observed over the excitation energies range of 2.3 to 3.8 MeV with high statistics and without background contamination within the target. The resonance parameters were extracted by an R-matrix analysis of the excitation function. The $^{26}$Si(p,{$\gamma$})$^{27}$P stellar reaction rate has been evaluated, including high-lying resonances found in this work. }},
adsurl = {http://adsabs.harvard.edu/abs/2012PhRvC..85d5802J},
doi = {10.1103/PhysRevC.85.045802},
eid = {045802},
keywords = {Resonance reactions, gamma transitions and level energies, Nucleosynthesis in novae, supernovae, and other explosive environments, 20{\lt}=A{\lt}=38}
}

@article{2012EPJA...48...65Z,
title = {{Quasi-elastic scattering of the proton drip line nucleus $^{17}$F on $^{12}$C at 60 MeV}},
author = {{Zhang}, G.~L. and {Zhang}, C.~L. and {Zhang}, H.~Q. and {Lin}, C.~J. and {Pang}, D.~Y. and {Wu}, X.~K. and {Jia}, H.~M. and {An}, G.~P. and {Wu}, Z.~D. and {Xu}, X.~X. and {Yang}, F. and {Liu}, Z.~H. and {Kubono}, S. and {Yamaguchi}, H. and {Hayakawa}, S. and {Binh}, D.~N. and {Kwon}, Y.~K. and {Iwasa}, N. and {Mazzocco}, M. and {La Commara}, M. and {Romoli}, M. and {Signorini}, C.},
journal = {European Physical Journal A},
year = {2012},
month = may,
pages = {65},
volume = {48},
abstract = {{The quasi-elastic scattering angular distribution of the proton drip line nucleus $^{17}$F on a $^{12}$C target was measured at 60 MeV. The experimental data have been compared with the theoretical analysis based onto optical model and continuum discretized coupled channels (CDCC). The couplings between breakup and elastic scattering channels, and between inelastic and elastic scattering channels resulted very weak. In order to explore the breakup effects the total reaction cross-section was deduced from the angular distribution of the quasi-elastic scattering data, and then compared with the existing data for the other weakly and tightly bound nuclei on $^{12}$C target using a universal function. From this comparison, we concluded that the breakup effect is not important for weakly bound projectiles on the light target as obtained also with the CDCC analysis. }},
adsurl = {http://adsabs.harvard.edu/abs/2012EPJA...48...65Z},
doi = {10.1140/epja/i2012-12065-x}
}

@article{2011PhRvC..83c4306Y,
title = {{{$\alpha$} resonance structure in $^{11}$B studied via resonant scattering of $^{7}$Li+{$\alpha$}}},
author = {{Yamaguchi}, H. and {Hashimoto}, T. and {Hayakawa}, S. and {Binh}, D.~N. and {Kahl}, D. and {Kubono}, S. and {Wakabayashi}, Y. and {Kawabata}, T. and {Teranishi}, T.},
journal = {\prc},
year = {2011},
month = mar,
number = {3},
pages = {034306},
volume = {83},
abstract = {{A new measurement of {$\alpha$} resonant scattering on $^{7}$Li was performed over the excitation energy of 10.2-13.0 MeV in $^{11}$B at the low-energy RI beam facility CNS Radioactive Ion Beam separator (CRIB) of the Center for Nuclear Study (CNS), University of Tokyo. The excitation function of $^{7}$Li+{$\alpha$} at 180$^{\circ}$ in the center-of-mass system was successfully measured for the first time with the inverse kinematics method, providing important information on the {$\alpha$} cluster structure in $^{11}$B and the reaction rate of $^{7}$Li({$\alpha$},{$\gamma$}), which is relevant to the $^{11}$B production in the {$\nu$} process in core-collapse supernovae. The excitation function of the $^{7}$Li({$\alpha$},p) reaction cross section for 11.7-13.1 MeV was also measured. }},
adsurl = {http://adsabs.harvard.edu/abs/2011PhRvC..83c4306Y},
doi = {10.1103/PhysRevC.83.034306},
eid = {034306},
keywords = {$^{3}$H-, $^{3}$He-, and $^{4}$He-induced reactions, Cluster models, Resonance reactions, 6{\lt}=A{\lt}=19}
}

@article{2010.Aram.14O,
title = {Direct Measurement of the $^{14}$O($\alpha$,$\alpha$)$^{14}$O Cross Section for Astrophysically Important $^{14}$O + $\alpha$ Resonances},
author = {{Kim}, A. and {Lee}, N. H. and {Hahn}, I. S. and {Yoo}, J. S. and {Han}, M. H. and {Kubono}, S. and {Yamaguchi}, H. and {Hayakawa}, S. and {Wakabayashi}, Y. and {Binh}, D. and {Hashimoto}, H. and {Kawabata}, T. and {Kahl}, D. and {Kurihara}, Y. and {Kwon}, Y. K. and {Teranishi}, T. and {Kato}, S. and {Komatsubara}, T. and {Guo}, B. and {Bing}, G. and {Liu}, W. and {Wang}, Y.},
journal = {Journal of the Korean Physical Society},
year = {2010},
pages = {40--43},
volume = {57},
abstract = {For the study of astrophysically important states in $^{18}$Ne, the $^{14}$O($\alpha$,$\alpha$)$^{14}$O cross section was measured ininverse kinematics using a radioactive $^{14}$O beam. This reactionwas investigated for properties of resonant states of $^{18}$Ne for determining the $^{14}$O($\alpha$,p)$^{17}$F reaction rate, which isone of the most important reactions for understanding the breakoutmechanism from the Hot CNO cycle to the rp-process. Alpha inducedelastic scattering on $^{14}$O was performed using the low-energy RI beam separator at Center for Nuclear Study, in the RIKEN Accelerator Research Facility. The energy range $E_{x}= 7.2 \sim 13.1{}$ MeV of $^{18}$Ne was scanned with the thick target method. Recoiled alpha particles were measured with Si dE-E telescopes. Spins and widths of three resonances at $E_x$ = 8.6, 9.22, and 10.06 MeV were calculated using the R-matrix analysis and a new state of $^{18}$Ne at $E_{x}=12.0$ MeV was found in this experiment.},
doi = {10.3938/jkps.57.40 },
owner = {daid},
timestamp = {2010.07.17}
}

@article{2009PhRvC..80a5801H,
title = {{Investigation of excited states in $^{22}$Mg via resonant elastic scattering of $^{21}$Na+p and its astrophysical implications}},
author = {{He}, J.~J. and {Kubono}, S. and {Teranishi}, T. and {Hu}, J. and {Notani}, M. and {Baba}, H. and {Nishimura}, S. and {Moon}, J.~Y. and {Nishimura}, M. and {Iwasaki}, H. and {Yanagisawa}, Y. and {Hokoiwa}, N. and {Kibe}, M. and {Lee}, J.~H. and {Kato}, S. and {Gono}, Y. and {Lee}, C.~S.},
journal = {\prc},
year = {2009},
month = jul,
number = {1},
pages = {015801},
volume = {80},
abstract = {{The excited states in $^{22}$Mg have been investigated by the resonant elastic scattering of $^{21}$Na+p. A 4.0 MeV/nucleon $^{21}$Na beam was separated by the Center for Nuclear Study (CNS) radioactive ion beam separator (CRIB) and then used to bombard a thick (CH$_{2}$)$_{n}$ target. The energy spectra of recoiled protons were measured at scattering angles of {\theta}$_{c.m.}${\approx}172$^{\circ}$,146$^{\circ}$, and 134$^{\circ}$, respectively. A wide energy-range of excitation function in $^{22}$Mg (up to E$_{x}$\approx{}8.9 MeV) was obtained simultaneously with a thick-target method, and a state at 7.06 MeV was newly observed. The resonant parameters were deduced from an R-matrix analysis of the center-of-mass (c.m.) differential cross-section data with a SAMMY-M6-BETA code. The astrophysical resonant reaction rate for the $^{18}$Ne({$\alpha$},p)$^{21}$Na reaction was recalculated based on the present parameters. Generally speaking, the present rates are much smaller than the previous ones. }},
adsurl = {http://adsabs.harvard.edu/abs/2009PhRvC..80a5801H},
doi = {10.1103/PhysRevC.80.015801},
eid = {015801},
keywords = {Reactions induced by unstable nuclei, Decay by proton emission, Nuclear physics aspects of novae, supernovae, and other explosive environments, 20{\lt}=A{\lt}=38}
}

@article{2009PhLB..672..230Y,
title = {{Low-lying non-normal parity states in $^{8}$B measured by proton elastic scattering on $^{7}$Be}},
author = {{Yamaguchi}, H. and {Wakabayashi}, Y. and {Kubono}, S. and {Amadio}, G. and {Fujikawa}, H. and {Teranishi}, T. and {Saito}, A. and {He}, J.~J. and {Nishimura}, S. and {Togano}, Y. and {Kwon}, Y.~K. and {Niikura}, M. and {Iwasa}, N. and {Inafuku}, K. and {Khiem}, L.~H.},
journal = {Physics Letters B},
year = {2009},
month = feb,
pages = {230-234},
volume = {672},
abstract = {{A new measurement of proton resonance scattering on $^{7}$Be was performed up to the center-of-mass energy of 6.7 MeV using the low-energy RI beam facility CRIB (CNS Radioactive Ion Beam separator) at the Center for Nuclear Study of the University of Tokyo. The excitation function of $^{7}$Be+p elastic scattering above 3.5 MeV was measured successfully for the first time, providing important information about the resonance structure of the $^{8}$B nucleus. The resonances are related to the reaction rate of $^{7}$Be(p,{$\gamma$})$^{8}$B, which is the key reaction in solar $^{8}$B neutrino production. Evidence for the presence of two negative parity states is presented. One of them is a 2$^{-}$ state observed as a broad s-wave resonance, the existence of which had been questionable. Its possible effects on the determination of the astrophysical S-factor of $^{7}$Be(p,{$\gamma$})$^{8}$B at solar energy are discussed. The other state had not been observed in previous measurements, and its spin and parity were determined as 1$^{-}$. }},
adsurl = {http://adsabs.harvard.edu/abs/2009PhLB..672..230Y},
archiveprefix = {arXiv},
doi = {10.1016/j.physletb.2009.01.033},
eprint = {0810.3363},
keywords = {Resonance reactions, 6{$\lt$}=A{$\lt$}=19, Spin, parity, and isobaric spin, Solar neutrinos},
primaryclass = {nucl-ex}
}

@article{2008EPJA...36....1H,
title = {{A study of the proton resonant property in $^{22}$Mg by elastic scattering of $^{21}$Na + p and its astrophysical implication in the $^{18}$Ne({$\alpha$}, p)$^{21}$Na reaction rate}},
author = {{He}, J.~J. and {Kubono}, S. and {Teranishi}, T. and {Notani}, M. and {Baba}, H. and {Nishimura}, S. and {Moon}, J.~Y. and {Nishimura}, M. and {Michimasa}, S. and {Iwasaki}, H. and {Yanagisawa}, Y. and {Hokoiwa}, N. and {Kibe}, M. and {Lee}, J.~H. and {Kato}, S. and {Gono}, Y. and {Lee}, C.~S.},
journal = {European Physical Journal A},
year = {2008},
month = apr,
pages = {1-5},
volume = {36},
abstract = {{Proton resonances in $^{22}$Mg have been investigated by the resonant elastic scattering of $^{21}$Na + p. The $^{21}$Na beam with a mean energy of 4.00 MeV/nucleon was separated by the CNS radioactive-ion-beam separator (CRIB) and bombarded a thick (CH$_{2}$)$_{n}$ target. The energy spectra of recoiled protons were measured at scattering angles of {\theta}$_{c.m.}$ {\approx} 172$^{\circ}$ , 146$^{\circ}$ , respectively. Several excited states observed before have been confirmed including two states (at 6.616, 6.796 MeV) observed at TRIUMF. A new state at 7.06 MeV has been observed, and another new one at 7.28 MeV is tentatively identified due to its low statistics. The proton resonant parameters were deduced from an R-matrix analysis of the differential cross-section data with a SAMMY-M6-BETA code. The astrophysical implication for the $^{18}$Ne({$\alpha$}, p)$^{21}$Na reaction has been briefly discussed. }},
adsurl = {http://adsabs.harvard.edu/abs/2008EPJA...36....1H},
doi = {10.1140/epja/i2007-10554-7},
keywords = {25.60.-t Reaction induced by unstable nuclei, 23.50.+z Decay by proton emission, 26.50.+x Nuclear physics aspects of novae, supernovae, and other explosive environments}
}

@article{2008NIMPA.589..150Y,
title = {{Development of a cryogenic gas target system for intense radioisotope beam production at CRIB}},
author = {{Yamaguchi}, H. and {Wakabayashi}, Y. and {Amadio}, G. and {Hayakawa}, S. and {Fujikawa}, H. and {Kubono}, S. and {He}, J.~J. and {Kim}, A. and {Binh}, D.~N.},
journal = {Nuclear Instruments and Methods in Physics Research A},
year = {2008},
month = may,
pages = {150-156},
volume = {589},
abstract = {{A cryogenic gas target system was developed for the radioisotope (RI) beam production at CNS Radio Isotope Beam separator (CRIB). Hydrogen gas was cooled to 85 90 K using liquid nitrogen and used as a secondary beam production target having a thickness of 2.3mg/cm$^{2}$. An intense $^{7}$Be beam (2{\times}10$^{8}$ particles per second) was successfully produced using this target. We observed a density-reduction effect at the gas target for high-current primary beams with about 7.5 W heat deposition. One main feature of the target system is forced circulation of the target gas. We have found that the circulation of the target gas at a rate of 55 standard liters per minute (slm) was effective in eliminating the density reduction. The extent to which the forced flow can prevent the density reduction had not been known well. In this work, the relation between the density reduction and the forced circulation rate was quantitatively studied. }},
adsurl = {http://adsabs.harvard.edu/abs/2008NIMPA.589..150Y},
doi = {10.1016/j.nima.2008.02.013}
}

@article{2007PhRvC..76e5802H,
title = {{Investigation of structure in $^{23}$Al via resonant proton scattering of $^{22}$Mg+p and the $^{22}$Mg(p,{$\gamma$})$^{23}$Al astrophysical reaction rate}},
author = {{He}, J.~J. and {Kubono}, S. and {Teranishi}, T. and {Notani}, M. and {Baba}, H. and {Nishimura}, S. and {Moon}, J.~Y. and {Nishimura}, M. and {Iwasaki}, H. and {Yanagisawa}, Y. and {Hokoiwa}, N. and {Kibe}, M. and {Lee}, J.~H. and {Kato}, S. and {Gono}, Y. and {Lee}, C.~S.},
journal = {\prc},
year = {2007},
month = nov,
number = {5},
pages = {055802},
volume = {76},
abstract = {{Proton resonant states in $^{23}$Al have been investigated for the first time by the resonant elastic and inelastic scattering of $^{22}$Mg+p with a $^{22}$Mg beam at 4.38 MeV/nucleon bombarding a thick (CH$_{2}$)$_{n}$ target. The low-energy $^{22}$Mg beam was separated by the CNS radioactive ion beam separator (CRIB). The energy spectra of recoiled protons were measured at average scattering angles of {\theta}$_{lab}${\approx}4$^{\circ}$,17$^{\circ}$ and 23$^{\circ}$. A new state has been observed at E$_{x}$=3.00 MeV with a spin-parity assignment of (3/2$^{+}$). In addition, resonant inelastic scattering has populated three more states at excitation energies of 3.14, 3.26, and 3.95 MeV, with proton decay to the first excited state in Mg22 being observed. The new state at 3.95 MeV has been assigned a spin-parity of J$^{\pi}$=(7/2$^{+}$). The resonant parameters were determined by an R-matrix analysis of the excitation functions with a SAMMY-M6-BETA code. The core-excited structure of $^{23}$Al is discussed within a shell-model picture. The stellar reaction rate of the $^{22}$Mg(p,{$\gamma$})$^{23}$Al reaction has been reevaluated, and the revised total reaction rate is about 40\% greater than the previous result for temperatures beyond T$_{9}$=0.3. }},
adsurl = {http://adsabs.harvard.edu/abs/2007PhRvC..76e5802H},
doi = {10.1103/PhysRevC.76.055802},
eid = {055802},
keywords = {Reactions induced by unstable nuclei, Decay by proton emission, Nuclear physics aspects of novae, supernovae, and other explosive environments, 20{\lt}=A{\lt}=38}
}

@article{2007PhLB..650..129T,
title = {{Single-particle resonance levels in $^{14}$O examined by $^{13}$N+p elastic resonance scattering}},
author = {{Teranishi}, T. and {Kubono}, S. and {Yamaguchi}, H. and {He}, J.~J. and {Saito}, A. and {Fujikawa}, H. and {Amadio}, G. and {Niikura}, M. and {Shimoura}, S. and {Wakabayashi}, Y. and {Nishimura}, S. and {Nishimura}, M. and {Moon}, J.~Y. and {Lee}, C.~S. and {Odahara}, A. and {Sohler}, D. and {Khiem}, L.~H. and {Li}, Z.~H. and {Lian}, G. and {Liu}, W.~P.},
journal = {Physics Letters B},
year = {2007},
month = jun,
pages = {129-134},
volume = {650},
abstract = {{Single-particle properties of low-lying resonance levels in $^{14}$O have been studied efficiently by utilizing a technique of proton elastic resonance scattering with a $^{13}$N secondary beam and a thick proton target. The excitation functions for the N13+p elastic scattering were measured over a wide energy range of E$_{cm}$=0.4--3.3 MeV and fitted with an R-matrix calculation. A clear assignment of J$^{\pi}$=2$^{-}$ has been made for the level at E$_{x}$=6.767(11) MeV in $^{14}$O for the first time. The excitation functions show a signature of a new 0$^{-}$ level at E$_{x}$=5.71(2) MeV with {$\Gamma$}=400(100) keV. The excitation energies and widths of the $^{14}$O levels are discussed in conjunction with the spectroscopic structure of A=14 nuclei with T=1. }},
adsurl = {http://adsabs.harvard.edu/abs/2007PhLB..650..129T},
doi = {10.1016/j.physletb.2007.05.013},
keywords = {Spin, parity, and isobaric spin, Spectroscopic factors and asymptotic normalization coefficients, Resonance reactions, 6{\lt}=A{\lt}=19}
}

@article{2005NIMPA.539...74Y,
title = {{Low-energy radioisotope beam separator CRIB}},
author = {{Yanagisawa}, Y. and {Kubono}, S. and {Teranishi}, T. and {Ue}, K. and {Michimasa}, S. and {Notani}, M. and {He}, J.~J. and {Ohshiro}, Y. and {Shimoura}, S. and {Watanabe}, S. and {Yamazaki}, N. and {Iwasaki}, H. and {Kato}, S. and {Kishida}, T. and {Morikawa}, T. and {Mizoi}, Y.
},
journal = {Nuclear Instruments and Methods in Physics Research A},
year = {2005},
month = feb,
pages = {74-83},
volume = {539},
abstract = {A low-energy in-flight type RI beam separator, called CRIB, has been installed for nuclear physics and nuclear astrophysics by the Center for Nuclear Study, the University of Tokyo in the RIKEN Accelerator Research Facility. It consists of a double achromatic system and an Wien filter. It is capable of providing RI beams at 5?10 MeV/nucleon. Since CRIB has been developed in the end of 2000, many proton-rich RI beams were successfully produced via the (p,n), (d,t), and (3He,n) reactions in inverse kinematics. In this paper, the design of the separator and its performance are discussed including the method of RI-beam production at low energies.},
adsurl = {http://adsabs.harvard.edu/abs/2005NIMPA.539...74Y},
doi = {10.1016/j.nima.2004.09.041}
}

@article{2003PhLB..556...27T,
title = {{Study of resonance states in $^{12}$N using a radioactive ion beam of $^{11}$C}},
author = {{Teranishi}, T. and {Kubono}, S. and {Shimoura}, S. and {Notani}, M. and {Yanagisawa}, Y. and {Michimasa}, S. and {Ue}, K. and {Iwasaki}, H. and {Kurokawa}, M. and {Satou}, Y. and {Morikawa}, T. and {Saito}, A. and {Baba}, H. and {Lee}, J.~H. and {Lee}, C.~S. and {F{\"u}l{\"o}p}, Z. and {Kato}, S.},
journal = {Physics Letters B},
year = {2003},
month = mar,
pages = {27-32},
volume = {556},
abstract = {{Resonance states in $^{12}$N were studied by using the resonance elastic scattering of $^{11}$C+p with a low-energy radioactive ion beam of $^{11}$C at 3.5 MeV/nucleon and a thick (CH$_{2}$)$_{n}$ target. The $^{11}$C beam was separated by a newly installed CNS radioactive ion beam separator (CRIB). The energy spectrum of recoil protons was measured at laboratory scattering angles around {\theta}$_{LAB}$=0$^{\circ}$ to identify resonance states in $^{12}$N. The spin-parity values of J$^{\pi}$=3$^{-}$ and (2)$^{+}$ have been determined for the levels at the excitation energies of E$_{x}$=3.1 and 3.6 MeV in $^{12}$N, respectively, suggesting a small contribution of the 3.1-MeV level to the $^{11}$C(p,{$\gamma$})$^{12}$N stellar reaction. }},
adsurl = {http://adsabs.harvard.edu/abs/2003PhLB..556...27T},
doi = {10.1016/S0370-2693(03)00098-4}
}

@article{2002EPJA...13..217K,
title = {{New low-energy RIB separator CRIB for nuclear astrophysics}},
author = {{Kubono}, S. and {Yanagisawa}, Y. and {Teranishi}, T. and {Kato}, S. and {Kishida}, Y. and {Michimasa}, S. and {Ohshiro}, Y. and {Shimoura}, S. and {Ue}, K. and {Watanabe}, S. and {Yamazaki}, N.},
journal = {European Physical Journal A},
year = {2002},
pages = {217-220},
volume = {13},
abstract = {{An in-flight RIB separator at low energies, which is the first extensive separator at low energies, called CRIB, is just under construction at CNS. This consists of a double-achromatic magnetic separator, a window-less gas target, and a Wien filter. Some characteristics of the CRIB are described. Possible experimental plans are also discussed in our nuclear astrophysics project for the study of the explosive hydrogen burning process, especially on the onset mechanism. }},
adsurl = {http://adsabs.harvard.edu/abs/2002EPJA...13..217K}
}

@article{Yamag:ESSENA23,
author = {{Yamaguchi, H.} and {Hayakawa, S.} and {Ma, N.R.} and {Shimizu, H.} and {Okawa, K.} and {Zhang, Q.} and {Yang, L.} and {Kahl, D.} and {La Cognata, M.} and {Lamia, L.} and {Abe, K.} and {Beliuskina, O.} and {Cha, S.M.} and {Chae, K.Y.} and {Cherubini, S.} and {Figuera, P.} and {Ge, Z.} and {Gulino, M.} and {Hu, J.} and {Inoue, A.} and {Iwasa, N.} and {Kim, A.} and {Kim, D.} and {Kiss, G.} and {Kubono, S.} and {La Commara, M.} and {Lattuada, M.} and {Lee, E.J.} and {Moon, J.Y.} and {Palmerini, S.} and {Parascandolo, C.} and {Park, S.Y.} and {Phong, V.H.} and {Pierroutsakou, D.} and {Pizzone, R.G.} and {Rapisarda, G.G.} and {Romano, S.} and {Spitaleri, C.} and {Tang, X.D.} and {Trippella, O.} and {Tumino, A.} and {Zhang, N.T.} and {Lam, Y.H.} and {Heger, A.} and {Jacobs, A.M.} and {Xu, S.W.} and {Ma, S.B.} and {Ru, L.H.} and {Liu, E.Q.} and {Liu, T.} and {Hamill, C.B.} and {Murphy, A. St J.} and {Su, J.} and {Fang, X.} and {Kwag, M.S.} and {Duy, N.N.} and {Uyen, N.K.} and {Kim, D.H.} and {Liang, J.} and {Psaltis, A.} and {Sferrazza, M.} and {Johnston, Z.} and {Li, Y.Y.}},
title = {RIB induced reactions: Studying astrophysical reactions with low-energy RI beam at CRIB},
doi = {10.1051/epjconf/202327501015},
url = {https://doi.org/10.1051/epjconf/202327501015},
journal = {EPJ Web Conf.},
year = 2023,
volume = 275,
pages = {01015}
}

@article{Okawa:ESSENA23,
author = {{Okawa, Kodai} and {Kim, Minju} and {Chae, Kyungyuk} and {Hayakawa, Seiya} and {Adachi, Satoshi} and {Cha, Soomi} and {Chillery, Thomas William} and {Furuno, Tatsuya} and {Gu, Gyungmo} and {Hanai, Shutaro} and {Imai, Nobuaki} and {Kahl, David} and {Kawabata, Takahiro} and {Kim, Chanhee} and {Kim, Dahee} and {Kim, Sohyun} and {Kubono, Shigeru} and {Kwag, Minsik} and {Li, Jiatai} and {Ma, Nanru} and {Michimasa, Shin\'{}ichiro} and {Nguyen Kim, Uyen} and {Nguyen Ngoc, Duy} and {Sakanashi, Kohsuke} and {Shimizu, Hideki} and {Sirbu, Oana} and {Yamaguchi, Hidetoshi} and {Yokoyama, Rin} and {Zhang, Qian}},
title = {Direct measurement of the $^{26}$Si($\alpha$, $p$)$^{29}$P reaction at CRIB for the nucleosynthesis in the X-ray bursts},
doi = {10.1051/epjconf/202327502009},
url = {https://doi.org/10.1051/epjconf/202327502009},
journal = {EPJ Web Conf.},
year = 2023,
volume = 275,
pages = {02009}
}

@article{Yamaguchi:NIC16,
author = {{Yamaguchi, H.} and {Hayakawa, S.} and {Ma, N.R.} and {Shimizu, H.} and {Okawa, K.} and {Yang, L.} and {Kahl, D.} and {La Cognata, M.} and {Lamia, L.} and {Abe, K.} and {Beliuskina, O.} and {Cha, S.M.} and {Chae, K.Y.} and {Cherubini, S.} and {Figuera, P.} and {Ge, Z.} and {Gulino, M.} and {Hu, J.} and {Inoue, A.} and {Iwasa, N.} and {Kim, A.} and {Kim, D.} and {Kiss, G.} and {Kubono, S.} and {La Commara, M.} and {Lattuada, M.} and {Lee, E.J.} and {Moon, J.Y.} and {Palmerini, S.} and {Parascandolo, C.} and {Park, S.Y.} and {Phong, V. H.} and {Pierroutsakou, D.} and {Pizzone, R.G.} and {Rapisarda, G.G.} and {Romano, S.} and {Spitaleri, C.} and {Tang, X.D.} and {Trippella, O.} and {Tumino, A.} and {Zhang, N.T.} and {Lam, Y.H.} and {Heger, A.} and {Jacobs, A.M.} and {Xu, S.W.} and {Ma, S.B.} and {Ru, L.H.} and {Liu, E.Q.} and {Liu, T.} and {Hamill, C.B.} and {St J. Murphy, A.} and {Su, J.} and {Fang, X.} and {Kwag, M.S.} and {Duy, N.N.} and {Uyen, N.K.} and {Kim, D.H.} and {Liang, J} and {Psaltis, A.} and {Sferrazza, M.} and {Johnston, Z.} and {Li, Y.Y.}},
title = {Experimental studies on astrophysical reactions at the low-energy RI beam separator CRIB},
doi = {10.1051/epjconf/202226003003},
url = {https://doi.org/10.1051/epjconf/202226003003},
journal = {EPJ Web Conf.},
year = 2022,
volume = 260,
pages = {03003}
}

@article{Hu:NIC16,
author = {{Hu, J.} and {Yamaguchi, H.} and {Lam, Y.H.} and {Heger, A.} and {Kahl, D.} and {Jacobs, A.M.} and {Johnston, Z.} and {Xu, S.W.} and {Zhang, N.T.} and {Ma, S.B.} and {Ru, L.H.} and {Liu, E.Q.} and {Liu, T.} and {Hayakawa, S.} and {Yang, L.} and {Shimizu, H.} and {Hamill, C.B.} and {Murphy, A. StJ.} and {Su, J.} and {Fang, X.} and {Chae, K.Y.} and {Kwag, M.S.} and {Cha, S.M.} and {Duy, N.N.} and {Uyen, N.K.} and {Kim, D.H.} and {Pizzone, R.G.} and {La Cognata, M.} and {Cherubini, S.} and {Romano, S.} and {Tumino, A.} and {Liang, J.} and {Psaltis, A.} and {Sferrazza, M.} and {Kim, D.} and {Li, Y.Y.} and {Kubono, S.}},
title = {First measurement of 25Al+p resonant scattering relevant to the astrophysical reaction $^{22}$Mg($\alpha$, $p$)$^{25}$Al},
doi = {10.1051/epjconf/202226005001},
url = {https://doi.org/10.1051/epjconf/202226005001},
journal = {EPJ Web Conf.},
year = 2022,
volume = 260,
pages = {05001}
}

@article{Gulino:20,
doi = {10.1088/1742-6596/1610/1/012005},
url = {https://doi.org/10.1088/1742-6596/1610/1/012005},
year = 2020,
month = {},
publisher = {{IOP} Publishing},
volume = {1610},
pages = {012005},
author = {M.~Gulino and S.~Cherubini and S.~Kubono and L.~Lamia and M.~L. Cognata and R.~G. Pizzone,
H.~Yamaguchi and S.~Hayakawa and Y.~Wakabayashi and N.~Iwasa and S.~Kato and T.~Komatsubara,
T.~Teranishi and A.~Coc and N.~de~S{\'{e}}r{\'{e}}ville and F.~Hammache and G.~Kiss,
S.~Bishop and D.~N. Binh and B.~Roeder and L.~Trache and R.~Tribble and C.~Spitaleri},
title = {Application of Trojan horse method to radioactive ion beams induced reactions},
journal = {Journal of Physics: Conference Series},
abstract = {}
}

@article{Hayakawa:20,
author = { S. Hayakawa and M. La Cognata and L. Lamia and H. Shimizu and L. Yang and H. Yamaguchi and K. Abe and O. Beliuskina and S. M. Cha and K. Y. Chae and S. Cherubini and P. Figuera and Z. Ge and M. Gulino and J. Hu and A. Inoue and N. Iwasa and D. Kahl and A. Kim and D. H. Kim and G. Kiss and S. Kubono and M. La Commara and M. Lattuada and E. J. Lee and J. Y. Moon and S. Palmerini and C. Parascandolo and S. Y. Park and D. Pierroutsakou and R. G. Pizzone and G. G. Rapisarda and S. Romano and C. Spitaleri and X. D. Tang and O. Trippella and A. Tumino and P. Vi and N. T. Zhang},
title = {Experimental Study on the $^7$Be($n$, $p$)$^7$Li and the $^7$Be($n$,$\alpha$)$^4$He Reactions for Cosmological Lithium Problem},
journal = {JPS Conf. Proc.},
volume = {31},
pages = {011036},
year = {2020},
doi = {10.7566/JPSCP.31.011036},
url = {https://journals.jps.jp/doi/abs/10.7566/JPSCP.31.011036},
eprint = {https://journals.jps.jp/doi/pdf/10.7566/JPSCP.31.011036}
}

@article{Shimizu:20,
author = { H. Shimizu and D. Kahl and H. Yamaguchi and K. Abe and O. Beliuskina and S. M. Cha and K. Y. Chae and A. A. Chen and Z. Ge and S. Hayakawa and N. Imai and N. Iwasa and A. Kim and D. H. Kim and M. J. Kim and S. Kubono and M. S. Kawag and J. Liang and J. Y. Moon and S. Nishimura and S. Oka and S. Y. Park and A. Psaltis and T. Teranishi and Y. Ueno and L. Yang},
title = {Study on $^{26m}$Al($p$, $\gamma$) Reaction at the SNe Temperature},
journal = {JPS Conf. Proc.},
volume = {31},
pages = {011073},
year = {2020},
doi = {10.7566/JPSCP.31.011073},
url = {https://journals.jps.jp/doi/abs/10.7566/JPSCP.31.011073},
eprint = {https://journals.jps.jp/doi/pdf/10.7566/JPSCP.31.011073}
}

@article{Yamaguchi:20c,
author = { H.~Yamaguchi and S.~Hayakawa and L.~Yang and H.~Shimizu and D.~Kahl and T.~Suhara and N.~Iwasa and
S.~M. Cha and M.~S. Kwag and J.~H. Lee and E.~J. Lee and K.~Y. Chae and A.~Kim and D.~H. Kim and
Y.~Wakabayashi and N.~Imai and N.~Kitamura and P.~Lee and J.~Y. Moon and K.~B. Lee and
C.~Akers and N.~N. Duy and L.~H. Khiem and C.~S. Lee},
title = {Studies nuclear astrophysics
and nuclear clustering with low-energy RI beams at CRIB},
journal = {JPS Conf. Proc.},
volume = {32},
pages = {010055},
year = {2020},
doi = {10.7566/JPSCP.32.010055}
}

@article{Inoue_2020,
doi = {10.1088/1742-6596/1643/1/012049},
url = {https://doi.org/10.1088/1742-6596/1643/1/012049},
year = 2020,
month = {dec},
publisher = {{IOP} Publishing},
volume = {1643},
pages = {012049},
author = {Azusa Inoue and Atsushi Tamii and Phaikying Chan and Seiya Hayakawa and Nobuyuki Kobayashi and Yukie Maeda and Kotaro Nonaka and Tatsushi Shima and Hideki Shimizu and Dinh Trong Tran and Xuan Wang and Hidetoshi Yamaguchi and Lei Yang and Zaihong Yang},
title = {Study of the contribution of the 7Be(d, p) reaction to the 7Li problem in the Big-Bang Nucleosynthesis},
journal = {Journal of Physics: Conference Series},
abstract = {Our research goal is to measure the cross section of the 7Be(d, p) reaction to find a solution for the cosmological the 7Li problem, which is an overestimation of the primordial 7Li abundance in the standard Big-Bang nucleosynthesis (BBN) model. We developed a method to produce an unstable 7Be target to measure the reaction in normal kinematics in a high-resolution measurement. We performed an experiment to produce the 7Be target and also to measure the cross section of the 7Be(d, p)8Be reaction with the produced 7Be target at the tandem facility, Kobe University. A 2.36 MeV proton beam irradiated a Li target to transmute 7Li particles to 7Be particles via the 7Li(p, n)7Be reaction. We produced 2.6×10$^{13}$ 7Be particles in the target after two days’ proton irradiation. After the target production, the beam ion was changed to deuterons with energies of 0.6, 1.0, and 1.6 MeV to measure the 7Be(d, p) reaction. The outgoing protons were measured by two $\Delta E-E$ silicon telescopes placed at 30$^{o}$ and 45$^{o}$. We report the preliminary results of this experiment, including the 7Be(d, p) cross section.}
}

@article{Yamaguchi_2020,
doi = {10.1088/1742-6596/1643/1/012069},
url = {https://doi.org/10.1088/1742-6596/1643/1/012069},
year = 2020,
month = {dec},
publisher = {{IOP} Publishing},
volume = {1643},
pages = {012069},
author = {G. Yamaguchi and S. Hayakawa and N.R. Ma and H. Shimizu and L. Yang and D. Kahl and K. Abe and T. Suhara and N. Iwasa and A. Kim and D.H. Kim and S.M. Cha and M.S. Kwag and J.H. Lee and E.J. Lee and K.Y. Chae and Y. Wakabayashi and N. Imai and N. Kitamura and P. Lee and J.Y. Moon and K.B. Lee and C. Akers and H.S. Jung and N.N. Duy and L.H. Khiem and C.S. Lee and S. Cherubini and M. Gulino and C. Spitaleri and G.G. Rapisarda and La Cognata and L. Lamia and S. Romano and A. Coc and N. de Sereville and F. Hammache and G. Kiss and S. Bishop and T. Teranishi and T. Kawabata and Y.K. Kwon and D.N. Binh},
title = {Experiments on astrophysical reactions with low-energy unstable nuclei beams at {CRIB}},
journal = {Journal of Physics: Conference Series},
abstract = {Studies on nuclear astrophysics, nuclear structure, and other interests have been performed using the radioactive-isotope (RI) beams at the low-energy RI beam separator CRIB, operated by Center for Nuclear Study (CNS), the University of Tokyo. The elastic resonant scattering is a striking tool to study astrophysical reactions and nuclear clusters. In particular, when it is coupled with a thick target and inverse kinematics, the measurement can be very efficient and even feasible with RI beams. By measuring resonant scattering, we can study the properties of resonant states which could play an important role in the astrophysical reaction, or have an exotic nuclear structure. The 10Be+α elastic scattering has been measured at CRIB, and three resonances which are in agreement with the prediction of a linear-chain structure by Suhara-En’yo were observed, giving a strong indication of the existence of such an exotic structure. Measurements based on the indirect technique of the reaction measurement, such as the Trojan horse method, have also been performed at CRIB.}
}

@article{Mazzocco_2020,
doi = {10.1088/1742-6596/1643/1/012096},
url = {https://doi.org/10.1088/1742-6596/1643/1/012096},
year = 2020,
month = {dec},
publisher = {{IOP} Publishing},
volume = {1643},
pages = {012096},
author = {M Mazzocco and N Keeley and A Boiano and C Boiano and M La Commara and A Lagni and C Manea and C Parascandolo and D Pierroutsakou and C Signorini and E Strano and D Torresi and H Yamaguchi and D Kahl and L Acosta and Di Meo and J P Fernandez-Garcia and T Glodariu and J Grebosz and A Guglielmetti and Y Hirayama and N Imai and H Ishiyama and N Iwasa and S C Jeong and H M Jia and Y H Kim and S Kimura and S Kubono and G La Rana and C J Lin and P Lotti and G Marqu{\'{\i}}nez-Duran and I Martel and H Miyatake and M Mukai and T Nakao and M Nicoletto and A Pakou and K Rusek and Y Sakaguchi and A M S{\'{a}}nchez-Ben{\'{\i}}tez and T Sava and O Sgouros and V Soukeras and F Soramel and E Stiliaris and L Stroe and T Teranishi and N Toniolo and Y Wakabayashi and Y X Watanabe and L Yang and Y Y Yang and H Q Zhang},
title = {Direct processes for the systems $^7$Be, $^8$B + $^{208}$Pb at Coulomb barrier energies},
journal = {Journal of Physics: Conference Series},
abstract = {The elastic scattering process for the nuclear reactions induced by the Radioactive Ion Beams 7Be and 8B on a 208Pb target was measured for the first time in the energy range around the Coulomb barrier. Extensive theoretical calculations within the framework of the optical model were performed. An excellent agreement between experimental data and theoretical predictions was achieved for the reaction 7Be + 208Pb, while a comprehensive understanding of the reaction dynamics induced by the more exotic projectile 8B is still far to be reached. Predictions of the cross section for the breakup for both systems will also be given.}
}

@inproceedings{Yamaguchi:NIC15,
author = {Yamaguchi, H.
and Hayakawa, S.
and Yang, L.
and Shimizu, H.
and Kahl, D.},
editor = {Formicola, Alba
and Junker, Matthias
and Gialanella, Lucio
and Imbriani, Gianluca},
title = {Study on Explosive Nucleosynthesis with Low-Energy RI Beams at CRIB},
booktitle = {Nuclei in the Cosmos XV},
year = {2019},
publisher = {Springer International Publishing},
address = {Cham},
pages = {265--268},
abstract = {Studies on nuclear astrophysics and nuclear structure have been performed using the radioactive-isotope (RI) beams at the low-energy RI beam separator CRIB of the University of Tokyo. Recent studies on astrophysical reactions in high-temperature stellar environments at CRIB are discussed. We conducted a series of {\$}{\$}{\backslash}alpha {\$}{\$}resonant scattering measurements with RI beams and the thick-target method, mainly to evaluate astrophysical reaction rates of {\$}{\$}{\backslash}alpha {\$}{\$}-induced reactions. Experimental projects based on other experimental techniques, such as the Trojan horse method or RI-implanted target, are also ongoing.},
isbn = {978-3-030-13876-9}
}

@inproceedings{Hayakawa:NIC15,
author = {Hayakawa, S.
and Abe, K.
and Beliuskina, O.
and Cha, S. M.
and Chae, K. Y.
and Cherubini, S.
and Figuera, P.
and Ge, Z.
and Gulino, M.
and Hu, J.
and Inoue, A.
and Iwasa, N.
and Kahl, D.
and Kim, A.
and Kim, D. H.
and Kiss, G. G.
and Kubono, S.
and La Cognata, M.
and La Commara, M.
and Lamia, L.
and Lattuada, M.
and Lee, E. J.
and Moon, J. Y.
and Palmerini, Sara
and Parascandolo, C.
and Park, S. Y.
and Pierroutsakou, D.
and Pizzone, Rosario Gianluca
and Rapisarda, G. G.
and Romano, S.
and Shimizu, H.
and Spitaleri, C.
and Tang, Xiaodong
and Trippella, O.
and Tumino, Aurora
and Vi, P.
and Yamaguchi, H.
and Yang, L.
and Zhang, N. T.},
editor = {Formicola, Alba
and Junker, Matthias
and Gialanella, Lucio
and Imbriani, Gianluca},
title = {Cross Section Measurements of the 7Be(n,p)7Li and the 7Be(n,$\alpha$)4He Reactions Covering the Big-Bang Nucleosynthesis Energy Range by the Trojan Horse Method at CRIB},
booktitle = {Nuclei in the Cosmos XV},
year = {2019},
publisher = {Springer International Publishing},
address = {Cham},
pages = {33--37},
abstract = {We performed indirect measurements of the neutron-induced reactions {\$}{\$}^{\{}7{\}}{\$}{\$}Be(n,p){\$}{\$}^{\{}7{\}}{\$}{\$}Li and {\$}{\$}^{\{}7{\}}{\$}{\$}Be(n,{\$}{\$}{\backslash}mathsf {\backslash}alpha {\$}{\$}){\$}{\$}^{\{}4{\}}{\$}{\$}He simultaneously by the Trojan Horse method relevant to the cosmological {\$}{\$}^7{\$}{\$}Li problem. Preliminary excitation functions for {\$}{\$}(n,p{\_}0){\$}{\$}and {\$}{\$}(n,{\backslash}alpha ){\$}{\$}are basically consistent with the previous studies, and new information about the {\$}{\$}(n,p{\_}1){\$}{\$}contribution suggests possible enhancement of the total reaction rate.},
isbn = {978-3-030-13876-9}
}

@inproceedings{Lamia:NIC15,
author = {Lamia, L.
and Spitaleri, C.
and Mazzocco, M.
and Hayakawa, S.
and Bertulani, C. A.
and Boiano, A.
and Boiano, C.
and Broggini, Carlo
and Caciolli, Antonio
and Depalo, Rosanna
and Galtarossa, F.
and Guardo, G. L.
and Gulino, M.
and Kubono, S.
and La Cognata, M.
and La Commara, M.
and La Rana, G.
and Lattuada, M.
and Menegazzo, Roberto
and Pakou, A.
and Parascandolo, C.
and Piatti, D.
and Pierroutsakou, D.
and Pizzone, Rosario Gianluca
and Romano, S.
and Rapisarda, G. G.
and Sergi, M. L.
and Sgouros, O.
and Soramel, F.
and Soukeras, V.
and Strano, E.
and Torresi, D.
and Tumino, Aurora
and Yamaguchi, H.
and Villante, F. L.
and Zhang, G. L.},
editor = {Formicola, Alba
and Junker, Matthias
and Gialanella, Lucio
and Imbriani, Gianluca},
title = {The Cosmologically Relevant $^7$Be($n$,$\alpha$)$^4$He Reaction in View of the Recent THM Investigations},
booktitle = {Nuclei in the Cosmos XV},
year = {2019},
publisher = {Springer International Publishing},
address = {Cham},
pages = {53--56},
abstract = {The cosmologically relevant $^7$Be($n$,$\alpha$)$^4$He has been matter of recent studies aimed at contributing to the long-standing Li-problem. Here a brief description of the twin THM investigations will be shown and the main results discussed.},
isbn = {978-3-030-13876-9}
}

@article{La_Commara_2018,
doi = {10.1088/1742-6596/966/1/012010},
url = {https://doi.org/10.1088%2F1742-6596%2F966%2F1%2F012010},
year = 2018,
month = {feb},
publisher = {{IOP} Publishing},
volume = {966},
pages = {012010},
author = {M. La Commara and M. Mazzocco and A. Boiano and C. Boiano and C. Manea and C. Parascandolo and D. Pierroutsakou and C. Signorini and E. Strano and D. Torresi and H. Yamaguchi and D. Kahl and P. Di Meo and J. Grebosz and N. Imai and Y. Hirayama and H. Ishiyama and N. Iwasa and S.C. Jeong and H.M. Jia and Y.H. Kim and S. Kimura and S. Kubono and C.J. Lin and H. Miyatake and M. Mukai and T. Nakao and M. Nicoletto and Y. Sakaguchi and A.M. S{\'{a}}nchez-Ben{\'{\i}}tez and F. Soramel and T. Teranishi and Y. Wakabayashi and Y.X. Watanabe and L. Yang and Y.Y. Yang},
title = {$^8$B+$^{208}$Pb Elastic Scattering at Coulomb Barrier Energies},
journal = {Journal of Physics: Conference Series},
abstract = {The scattering process of weakly-bound nuclei at Coulomb barrier energies provides deep insights on
the reaction dynamics induced by exotic nuclei. Within this framework, we measured for the first time the scattering process of the short-lived Radioactive Ion Beam (RIB) 8B (Sp = 0.1375 MeV) from a 208Pb target at 50 MeV beam energy.
The 8B RIB was produced by means of the in-flight facility CRIB (RIKEN, Japan) with an average intensity on target of 10 kHz and a purity about 25%.
Elastically scattering ions were detected in the angular range \theta c.m.
= 10°-160$^\circ$ by
means of the detector array EXPADES. A preliminary optical model analysis indicates a total reaction cross section of about 1 b, a value, once reduced, 2-3 times larger than those obtained for the reactions induced by the stable weakly-bound projectiles 6,7Li on a 208Pb
target in the energy range around the Coulomb barrier.}
}

@article{Kahl:OMEG17,
author = {Kahl,D. and Shimizu,H. and Yamaguchi,H. and Abe,K. and Beliuskina,O. and Cha,S. M. and Chae,K. Y. and Chen,A. A. and Ge,Z. and Hayakawa,S. and Imai,N. and Iwasa,N. and Kim,A. and Kim,D. H. and Kim,M. J. and Kubono,S. and Kwag,M. S. and Liang,J. and Moon,J. Y. and Nishimura,S. and Oka,S. and Park,S. Y. and Psaltis,A. and Teranishi,T. and Ueno,Y. and Yang,L. },
title = {Impact of the $^{26m}$Al($p$, $\gamma$)reaction to galactic 2$^{26}$Al yield},
journal = {AIP Conference Proceedings},
volume = {1947},
number = {1},
pages = {020003},
year = {2018},
doi = {10.1063/1.5030807},
url = {https://aip.scitation.org/doi/abs/10.1063/1.5030807},
eprint = {https://aip.scitation.org/doi/pdf/10.1063/1.5030807},
abstract = { Astrophysical observables that are directly linked to nuclear physics inputs provide critical and stringent constraints on nucleosynthetic models. As 26Al was the first specific radioactivity observed in the Galaxy, its origin has fascinated the nuclear astrophysics community for nearly forty years.
Despite extensive research, the precise origins of 26Al remain elusive.
At present, the sum of all putative stellar contributions generally overestimates the 26Al mass in the
interstellar medium. Among the many reactions that influence the yield of 26Al, radiative proton capture on its isomer
26mAl is one of the least constrained reactions by experimental data. To this end, we developed a 26Al isomeric beam and performed proton elastic scattering to search for low-spin states in 27Si. The experimental method and the preliminary results of this on-going study will be presented.
}
}

@article{Hayakawa:OMEG17,
author = {Hayakawa,S. and Abe,K. and Beliuskina,O. and Cha,S. M. and Chae,K. Y. and Cherubini,S. and
Figuera,P. and Ge,Z. and Gulino,M. and Hu,J. and Inoue,A. and Iwasa,N. and Kahl,D. and Kim,A. and Kim,D. H. and Kiss,G.
and Kubono,S. and La Cognata,M. and La Commara,M. and Lamia,L. and Lattuada,M. and Lee,E. J. and Moon,J. Y. and
Palmerini,S. and Parascandolo,C. and Park,S. Y. and Pierroutsakou,D. and Pizzone,R. G. and Rapisarda,G. G. and Romano,S.
and Shimizu,H. and Spitaleri,C. and Tang,X. D. and Trippella,O. and Tumino,A. and Vi,P. and Yamaguchi,H. and Yang,L. and Zhang,N. T. },
title = {Measurements of the neutron-induced reactions on 7Be with CRIB by the Trojan Horse method},
journal = {AIP Conference Proceedings},
volume = {1947},
number = {1},
pages = {020011},
year = {2018},
doi = {10.1063/1.5030815},
url = {https://aip.scitation.org/doi/abs/10.1063/1.5030815},
eprint = { https://aip.scitation.org/doi/pdf/10.1063/1.5030815},
abstract = { The cosmological 7Li problem has been one of the big issues left in the standard Big-Bang nucleosynthesis (BBN) model. In order to determine the radiogenic 7Li abundance by the BBN, it is important to know the production and the destruction rate of 7Be rather than 7Li itself. We performed indirect measurements
of the relevant neutron-induced reactions 7Be(n, p)7Li and 7Be(n, $\alpha$)4He simultaneously by the Trojan Horse Method (THM) via the three-body reactions 7Be(d,7Lip)1H and
7Be(d, $\alpha \alpha$)1H. A 7Be radioactive-isotope (RI) beam at 3.16
MeV/u was produced at Center-for-Nuclear-Study RI Beam (CRIB) separator. The Q-value spectra shows the evidence of the three-body channels of interest. We confirmedthat the THM was applicable to the present measurements by the momentum distributions of the spectator proton. Preliminary excitation functions are roughly consistent with the previous studies, moreover providing new data in the BBN energy range, and suggesting that new information about the 7Be(n, p1)7Li* contribution may be obtained by carrying out a further data analysis. }
}

@article{Yamaguchi:OMEG2017,
author = {Yamaguchi,H. and Kahl,D. and Hayakawa,S. and Yang,L. and Shimizu,H. and Sakaguchi,Y. and Abe,K. and Wakabayashi,Y. and Hashimoto,T. and Nakao,T. and Kubono,S. and Suhara,T. and Iwasa,N. and Kim,A. and Kim,D. H. and Cha,S. M. and Kwag,M. S. and Lee,J. H. and Lee,E. J. and Chae,K. Y. and Imai,N. and Kitamura,N. and Lee,P. and Moon,J. Y. and Lee,K. B. and Akers,C. and Jung,H. S. and Duy,N. N. and Khiem,L. H. and Lee,C. S. and Cherubini,S. and Gulino,M. and Spitaleri,C. and Rapisarda,G. G. and Cognata,M. La and Lamia,L. and Romano,S. and Coc,A. and de Sereville,N. and Hammache,F. and Kiss,G. and Bishop,S. and Teranishi,T. and Kawabata,T. and Kwon,Y. K. and Binh,D. N. },
title = {Indirect studies on astrophysical reactions at the low-energy RI beam separator CRIB},
journal = {AIP Conference Proceedings},
volume = {1947},
number = {1},
pages = {020022},
year = {2018},
doi = {10.1063/1.5030826},
url = {https://aip.scitation.org/doi/abs/10.1063/1.5030826 },
eprint = { https://aip.scitation.org/doi/pdf/10.1063/1.5030826 },
abstract = { Studies on nuclear astrophysics, nuclear structure, and other interests have been performed using the radioactive-isotope (RI) beams at the low-energy RI beam separator CRIB, operated by Center for Nuclear Study (CNS), the University of Tokyo. A type of measurement to study astophysical reactions at CRIB is by the elast$\alpha$,$\gamma$ resonant scattering with the thick-target method in inverse kinematics. An example is the α resonant scattering with 7Be beam, related to the astrophysical 7Be($\alpha$,$\gamma$) reactions, which is relevant in the hot p-p chain and $\nu$p-process in supernovae. Other α resonant scattering measurements with 30S, 10Be, 15O, and 18Ne beams have been performed at CRIB, using the thick-target method. There have also been measurements based on other experimental methods. The first Trojan horse method (THM) measurement using an RI beam has been performed at CRIB, to study the 18F(p, $\alpha$)15O reaction at astrophysical energies via the three body reaction 2H(18F, $\alpha$15O)n. The 18F(p, $\alpha$)15O reaction rate is crucial to understand the 511-keV $\gamam$-ray production in nova explosion phenomena, and we successfully evaluated the reactio cross section at novae temperature and below experimentally for the first time. }
}

@article{Yamaguchi,
author = {{Yamaguchi, H.} and {Hayakawa, S.} and {Yang, L.} and {Shimizu, H.} and {Kahl, D.}},
title = {Direct measurements and detection techniques with low-energy RIBs},
doi = {10.1051/epjconf/201818401017},
url = {https://doi.org/10.1051/epjconf/201818401017},
journal = {EPJ Web Conf.},
year = 2018,
volume = 184,
pages = {01017}
}

@article{Inoue:18,
author = {{Inoue, A.} and {Tamii, A.} and {Abe, K.} and {Adachi, S.} and {Aoi, N.} and {Asai, M.} and {Fukuda, M.} and {Gey, G.} and {Hashimoto, T.} and {Ideguchi, E.} and {Isaak, J.} and {Kobayashi, N.} and {Maeda, Y.} and {Makii, H.} and {Matsuta, K.} and {Mihara, M.} and {Miura, M.} and {Shima, T.} and {Shimizu, H.} and {Tang, R.} and {Dinh Trong, T.} and {Yamaguchi, H.} and {Yang, L.}},
title = {Study of the contribution of the 7Be(d, p) reaction to the 7Li problem in the Big-Bang Nucleosynthesis},
doi = {10.1051/epjconf/201818402007},
url = {https://doi.org/10.1051/epjconf/201818402007},
journal = {EPJ Web Conf.},
year = 2018,
volume = 184,
pages = {02007}
}

@article{Shimizu:18,
author = {{Shimizu, H.} and {Kahl, D.} and {Yamaguchi, H.} and {Abe, K.} and {Beliuskina, O.} and {Cha, S. M.} and {Chae, K. Y.} and {Chen, A. A.} and {Ge, Z.} and {Hayakawa, S.} and {Imai, N.} and {Iwasa, N.} and {Kim, A.} and {Kim, D. H.} and {Kim, M. J.} and {Kubono, S.} and {Kawag, M. S.} and {Liang, J.} and {Moon, J. Y.} and {Nishimura, S.} and {Oka, S.} and {Park, S. Y.} and {Psaltis, A.} and {Teranishi, T.} and {Ueno, Y.} and {Yang, L.}},
title = {Isomeric $^{26}$Al beam production with CRIB},
doi = {10.1051/epjconf/201818402013},
url = {https://doi.org/10.1051/epjconf/201818402013},
journal = {EPJ Web Conf.},
year = 2018,
volume = 184,
pages = {02013}
}

@article{Gulino:18,
author = {{Gulino, Marisa} and {Cherubini, Silvio} and {Gabriele Rapisarda, Giuseppe} and {Kubono, Shigeru} and {Lamia, Livio} and {La Cognata, Marco} and {Gianluca Pizzone, Rosario} and {Yamaguchi, Hidetoshi} and {Hayakawa, Seya} and {Wakabayashi, Yasuo} and {Iwasa, Naohito} and {Kato, Seigo} and {Komatsubara, Tetsuro} and {Teranishi, Takashi} and {Coc, Alain} and {de S\'er\'eville, Nicolas} and {Hammache, Fairouz} and {Kiss, Gabor} and {Bishop, Shawn} and {Nguyen Binh, Dam} and {Roeder, Brian} and {Trache, Livius} and {Tribble, Robert} and {Spart\`a, Roberta} and {Indelicato, Iolanda} and {Spitaleri, Claudio}},
title = {Trojan Horse Method experiments with radioactive ion beams},
doi = {10.1051/epjconf/201818401008},
url = {https://doi.org/10.1051/epjconf/201818401008},
journal = {EPJ Web Conf.},
year = 2018,
volume = 184,
pages = {01008}
}

@article{Strano:18,
author = {{Strano, E.} and {Mazzocco, M.} and {Boiano, A.} and {Boiano, C.} and {La Commara, M.} and {Manea, C.} and {Parascandolo, C.} and {Pierroutsakou, D.} and {Signorini, C.} and {Torresi, D.} and {Yamaguchi, H.} and {Kahl, D.} and {Acosta, L.} and {Di Meo, P.} and {Fernandez-Garcia, J.P.} and {Glodariu, T.} and {Grebosz, J.} and {Guglielmetti, A.} and {Imai, N.} and {Hirayama, Y.} and {Ishiyama, H.} and {Iwasa, N.} and {Jeong, S.C.} and {Jia, H.M.} and {Keeley, N.} and {Kim, Y.H.} and {Kimura, S.} and {Kubono, S.} and {Lay, J.A.} and {Lin, C.J.} and {Marquinez-Duran, G.} and {Marte, I.} and {Miyatake, H.} and {Mukai, M.} and {Nakao, T.} and {Nicoletto, M.} and {Pakou, A.} and {Rusek, K.} and {Sakaguchi, Y.} and {Sanchez-Benitez, A.M.} and {Sava, T.} and {Sgouros, O.} and {Stefanini, C.} and {Soramel, F.} and {Soukeras, V.} and {Stiliaris, E.} and {Stroe, L.} and {Teranishi, T.} and {Toniolo, N.} and {Wakabayashi, Y.} and {Watanabe, Y.X.} and {Yang, L.} and {Yang, Y.Y.}},
title = {$^7$Be and $^8$B reaction dynamics at Coulomb barrier energies},
doi = {10.1051/epjconf/201818402015},
url = {https://doi.org/10.1051/epjconf/201818402015},
journal = {EPJ Web Conf.},
year = 2018,
volume = 184,
pages = {02015}
}

@article{Mazzocco_2018,
doi = {10.1088/1742-6596/1078/1/012013},
url = {https://doi.org/10.1088%2F1742-6596%2F1078%2F1%2F012013},
year = 2018,
month = {aug},
publisher = {{IOP} Publishing},
volume = {1078},
pages = {012013},
author = {M Mazzocco and A Boiano and C Boiano and M La Commara and C Manea and C Parascandolo and D Pierroutsakou and C Signorini and E Strano and D Torresi and H Yamaguchi and D Kahl and L Acosta and P Di Meo and J P Fernandez-Garcia and T Glodariu and J Grebosz and A Guglielmetti and N Imai and Y Hirayama and H Ishiyama and N Iwasa and S C Jeong and H M Jia and N Keeley and Y H Kim and S Kimura and S Kubono and J A Lay and C J Lin and G Marquinez-Duran and I Martel and H Miyatake and M Mukai and T Nakao and M Nicoletto and A Pakou and K Rusek and Y Sakaguchi and A M S{\'{a}}nchez-Ben{\'{\i}}tez and T Sava and O Sgouros and F Soramel and V Soukeras and E Stiliaris and L Stroe and T Teranishi and N Toniolo and Y Wakabayashi and Y X Watanabe and L Yang and Y Y Yang},
title = {Reaction Dynamics for the Systems 7Be, 8B $\mathplus$ 208Pb at Coulomb Barrier Energies},
journal = {Journal of Physics: Conference Series},
abstract = {In this contribution we describe the first results obtained for the investigation of the elastic scattering process in the reactions induced by the Radioactive Ion Beams 7Be and 8B on a 208Pb target at Coulomb barrier energies. The experimental data were analyzed within the framework of the optical model in order to extract the total reaction cross section. The comparison with data available in literature for reactions induced on 208Pb by light ions in the mass range A = 6-8 shows that the loosely-bound 8B has the largest reactivity.}
}

@article{Hayakawa:NIC2016,
author = { S. Hayakawa and C. Spitaleri and N. Burtebayev and A. Aimaganbetov and S.V. Artemov and P. Figuera and M. Fisichella and G.L. Guardo and S. Igamov and I. Indelicato and G.G. Kiss and S. Kubono and M. La Cognata and L. Lamia and M. Lattuada and M. Nassurlla and E. Piasecki and G.G. Rapisarda and S. Romano and S.B. Sakuta and A. TrzciAska and A. Tumino and A. Urkinbayev and T. Zholdybayev},
title = {Trojan Horse Method for the Oxygen-Burning Process Reactions},
booktitle = {Proceedings of the 14th International Symposium on Nuclei in the Cosmos (NIC2016)},
pages = {020406},
year = {2017},
journal = {JPS Conf. Proc.},
volume = {14},
doi = {10.7566/JPSCP.14.020406},
url = {https://journals.jps.jp/doi/abs/10.7566/JPSCP.14.020406},
eprint = {https://journals.jps.jp/doi/pdf/10.7566/JPSCP.14.020406}
}

@article{Yamaguchi:NIC2016,
author = { H. Yamaguchi and D. Kahl and S. Hayakawa and Y. Sakaguchi and K. Abe and H. Shimuzu and Y. Wakabayashi and T. Hashimoto and S. Cherubini and M. Gulino and C. Spitaleri and G. G. Rapisarda and M. La Cognata and L. Lamia and S. Romano and S. Kubono and N. Iwasa and T. Teranishi and T. Kawabata and Y. K. Kwon and D. N. Binh and L. H. Khiem and N. N. Duy and S. Kato and T. Komatsubara and A. Coc and N. de Sereville and F. Hammache and G. Kiss and S. Bishop},
title = {Experimental Studies of Light-Ion Nuclear Reactions Using Low-Energy RI Beams},
booktitle = {Proceedings of the 14th International Symposium on Nuclei in the Cosmos (NIC2016)},
year = {2017},
journal = {JPS Conf. Proc.},
volume = {14},
pages = {010503},
doi = {10.7566/JPSCP.14.010503},
url = {https://journals.jps.jp/doi/abs/10.7566/JPSCP.14.010503},
eprint = {https://journals.jps.jp/doi/pdf/10.7566/JPSCP.14.010503}
}

@article{Gulino:NIC2016,
author = { Marisa Gulino and Silvio Cherubini and Claudio Spitaleri and Giuseppe Gabriele Rapisarda and Marco La Cognata and Livio Lamia and Rosario Gianluca Pizzone and Stefano Romano and Shigeru Kubono and Hidetoshi Yamaguchi and Seya Hayakawa and Yasuo Wakabayashi and Naohito Iwasa and Seigo Kato and Tetsuro Komatsubara and Takashi Teranishi and Alain Coc and Nicolas de Sereville and Fairouz Hammache and Gabor Kiss and Shawn Bishop and Dam Nguyen Binh},
title = {The $^{18}$F($n$,$\alpha$) Reaction: First Study of $n$-Induced Reaction on a Radioactive Nucleus Using the Trojan Horse Method},
booktitle = {Proceedings of the 14th International Symposium on Nuclei in the Cosmos (NIC2016)},
year = {2017},
journal = {JPS Conf. Proc.},
volume = {14},
pages = {021104},
doi = {10.7566/JPSCP.14.021104},
url = {https://journals.jps.jp/doi/abs/10.7566/JPSCP.14.021104},
eprint = {https://journals.jps.jp/doi/pdf/10.7566/JPSCP.14.021104}
}

@article{Kahl:NIC2016,
author = { D. Kahl and A. A. Chen and S. Kubono and H. Yamaguchi and D. N. Binh and J. Chen and
S. Cherubini and N. N. Duy and T. Hashimoto and S. Hayakawa and N. Iwasa and H. S. Jung and
S. Kato and Y. K. Kwon and S. Nishimura and S. Ota and K. Setoodehnia and T. Teranishi and H. Tokieda and T. Yamada
and C. C. Yun and L. Y. Zhang},
title = {$^{30}$S($\alpha$, $p$) Thermonuclear Reaction Rate from Experimental Level Structure of $^{34}$Ar},
year = {2017},
journal = {JPS Conf. Proc.},
doi = {10.7566/JPSCP.14.020510},
url = {https://journals.jps.jp/doi/abs/10.7566/JPSCP.14.020510},
eprint = {https://journals.jps.jp/doi/pdf/10.7566/JPSCP.14.020510}
}

@article{Abe:NIC2016,
author = { K. Abe and S. Hayakawa and H. Yamaguchi and L. Lamia},
title = {Feasibility Study for the $^7$Be+n Reaction Measurements by Trojan Horse Method at CRIB},
booktitle = {Proceedings of the 14th International Symposium on Nuclei in the Cosmos (NIC2016)},
year = {2017},
journal = {JPS Conf. Proc.},
volume = {14},
pages = {020507},
doi = {10.7566/JPSCP.14.020507},
url = {https://journals.jps.jp/doi/abs/10.7566/JPSCP.14.020507},
eprint = {https://journals.jps.jp/doi/pdf/10.7566/JPSCP.14.020507}
}

@article{Yamaguchi:C2016,
doi = {10.1088/1742-6596/863/1/012025},
url = {https://doi.org/10.1088%2F1742-6596%2F863%2F1%2F012025},
year = 2017,
month = {jun},
publisher = {{IOP} Publishing},
volume = {863},
pages = {012025},
author = {H Yamaguchi and D Kahl and S Hayakawa and Y Sakaguchi and K Abe and T Nakao and T Suhara and N Iwasa and A Kim and D H Kim and S M Cha and M S Kwag and J H Lee and E J Lee and K Y Chae and Y Wakabayashi and N Imai and N Kitamura and P Lee and J Y Moon and K B Lee and C Akers and H S Jung and N N Duy and L H Khiem and C S Lee},
title = {Study on $\alpha$-cluster levels in non-4n nuclei using low-energy {RI} beams},
journal = {Journal of Physics: Conference Series},
abstract = {Alpha resonant scattering is a simple and promising method to study $\alpha$-cluster structure in nuclei. It has several good features which enable us to perform measurements with short-lived and relatively low-intense RI beams. Several measurements on alpha resonant scattering have been carried out at CRIB (CNS Radioactive Ion Beam separator), which is a low-energy RI beam separator at Center for Nuclear Study (CNS) of the University of Tokyo. Recent $\alpha$ resonant scattering studies at CRIB, using 7Li, 7Be and 10Be beams with a helium gas target, are discussed.}
}

@article{Kahl:2017a,
author = {{Kahl, D.} and {Shimizu, H.} and {Yamaguchi, H.} and {Abe, K.} and {Beliuskina, O.} and {Cha, S. M.} and {Chae, K. Y.} and {Chen, A. A.} and {Ge, Z.} and {Hayakawa, S.} and {Imai, N.} and {Iwasa, N.} and {Kim, A.} and {Kim, D. H.} and {Kim, M. J.} and {Kubono, S.} and {Kwag, M. S.} and {Liang, J.} and {Moon, J. Y.} and {Nishimura, S.} and {Oka, S.} and {Park, S. Y.} and {Psaltis, A.} and {Teranishi, T.} and {Ueno, Y.} and {Yang, L.}},
title = {Isomer beam elastic scattering: $^{26m}$Al($p$, $p$) for astrophysics},
doi = {10.1051/epjconf/201716501030},
url = {https://doi.org/10.1051/epjconf/201716501030},
journal = {EPJ Web Conf.},
year = 2017,
volume = 165,
pages = {01030}
}

@article{Yamaguchi:2017a,
author = {{Yamaguchi, H.} and {Kahl, D.} and {Hayakawa, S.} and {Yang, L.} and {Shimizu, H.} and {Sakaguchi, Y.} and {Abe, K.} and {Nakao, T.} and {Suhara, T.} and {Iwasa, N.} and {Kim, A.} and {Kim, D.H.} and {Cha, S.M.} and {Kwag, M.S.} and {Lee, J.H.} and {Lee, E.J.} and {Chae, K.Y.} and {Wakabayashi, Y.} and {Imai, N.} and {Kitamura, N.} and {Lee, P.} and {Moon, J.Y.} and {Lee, K.B.} and {Akers, C.} and {Jung, H.S.} and {Duy, N.N.} and {Khiem, L.H.} and {Lee, C.S.} and {Hashimoto, T.} and {Kubono, S.} and {Kawabata, T.} and {Teranishi, T.} and {Kwon, Y.K.} and {Binh, D.N.}},
title = {Nuclear astrophysics projects at the low-energy RI beam separator CRIB},
doi = {10.1051/epjconf/201716501056},
url = {https://doi.org/10.1051/epjconf/201716501056},
journal = {EPJ Web Conf.},
year = 2017,
volume = 165,
pages = {01056}
}

@article{Wang:2016,
author = {{Wang, Y.B.} and {Jin, S.J.} and {Jing, L.} and {Han, Z.Y.} and {Bai, X.X.} and {Guo, B.} and {Li, Y.J.} and {Li, Z.H.} and {Lian, G.} and {Su, J.} and {Sun, L.J.} and {Yan, S.Q.} and {Zeng, S.} and {Liu, W.P.} and {Yamaguchi, H.} and {Kubono, S.} and {Hu, J.} and {Kahl, D.} and {He, J.J} and {Wang, J.S.} and {Tang, X.D.} and {Xu, S.W.} and {Ma, P.} and {Zhang, N.T.} and {Bai, Z.} and {Huang, M.R.} and {Jia, B.L.} and {Jin, S.L.} and {Ma, J.B.} and {Ma, S.B.} and {Ma, W.H.} and {Yang, Y.Y.} and {Zhang, L.Y.} and {Jung, H.S.} and {Moon, J.Y.} and {Lee, C.S.} and {Teranishi, T.} and {Wang, H.W.} and {Ishiyama, H.} and {Iwasa, N.} and {Komatsubara, T.} and {Brown, B.A.}},
title = {Two measurements of the 22Na+p resonant scattering via thick-target inverse-kinematics method},
doi = {10.1051/epjconf/201610904010},
url = {https://doi.org/10.1051/epjconf/201610904010},
journal = {EPJ Web of Conferences},
year = 2016,
volume = 109,
pages = {04010}
}

@article{Yamaguchi:SEA2016,
title = {Overview of the activities at the low-energy beam separator CRIB},
year = 2016,
volume = {39C},
pages = {358},
author = {H. Yamaguchi and D. Kahl and S. Hayakawa and L. Yang and Y. Sakaguchi and
K. Abe and H. Shimizu and CRIB Collaboration},
journal = {Il Nuovo Cimento},
doi = {10.1393/ncc/i2016-16358-x}
}

@article{Kahl:SEA2016,
title = {Explosive destruction of $^{26}$Al},
year = 2016,
volume = {39C},
pages = {362},
author = {D. Kahl and H. Yamaguchi and H. Shimizu and K. Abe and O. Beliuskina and S. M. Cha and
K.Y. Chae and Z. Ge and S. Hayakawa and M.S. Kwag and D. H. Kim and J. Y. Moon and
S.Y. Park and L. Yang},
journal = {Il Nuovo Cimento},
doi = {10.1393/ncc/i2016-16371-1}
}

@article{Cha:SEA2016,
title = {Study of $\alpha$ cluster structure in $^{22}$Mg},
year = 2016,
volume = {39C},
pages = {371},
author = {S.M. Cha and K.Y. Chae and K. Abe and S.H. Bae and S.H. Choi and D.N. Binh and N.N. Duy and
K.I. Hahn and S. Hayakawa and B. Hong and H.S. Jung and D. Kahl and L.H. Khiem and A. Kim and
D.H. Kim and E.J. Kim and G.W. Kim and M.J. Kim and K.J. Kwag and M.S. Kwag and Y.K. Kwon and
C.S. Lee and E.J. Lee and S.I. Lim and B. Moon and J.Y. Moon and T. Nakao and S.Y. Park and
H. Shimizu and H. Yamaguchi and L. Yang and G. Zhuang},
journal = {Il Nuovo Cimento},
doi = {10.1393/ncc/i2016-16371-1}
}

@article{2015aris.confa0011Y,
title = {{Studies on Nuclear Astrophysics and Exotic Structure at the Low-Energy RI Beam Facility CRIB}},
author = {{Yamaguchi}, H. and {Kahl}, D. and {Hayakawa}, S. and {Sakaguchi}, Y. and {Nakao},
T. and {Wakabayashi}, Y. and {Hashimoto}, T. and {Teranishi}, T. and {Kubono}, S. and {Cherubini}, S.
and {Mazzocco}, M. and {Signorini}, C. and {Gulino}, M. and {Di Pietro}, A. and {Figuera}, P. and {La Cognata}, M.
and {Lattuada}, M. and {Spitaleri}, C. and {Torresi}, D. and {Lee}, P.~S. and {Lee}, C.~S. and {Komatsubara}, T.
and {Iwasa}, N. and {Okoda}, Y. and {Pierroutsakou}, D. and {Parascandolo}, C. and {La Commara}, M.
and {Strano}, E. and {Boiano}, C. and {Boiano}, A. and {Manea}, C. and {S{\'a}nchez-Ben{\'i}tez}, A.~M.
and {Miyatake}, H. and {Watanabe}, Y.~X. and {Ishiyama}, H. and {Jeong}, S.~C. and {Imai}, N. and {Hirayama}, Y.
and {Kimura}, S. and {Mukai}, M. and {Kim}, Y.~H. and {Lin}, C.~J. and {Jia}, H.~M. and {Yan}, L.
and {Yang}, Y.~Y. and {Kawabata}, T. and {Kwon}, Y.~K. and {Binh}, D.~N. and {Khiem}, L.~H. and {Duy}, N.~N. },
journal = {The Physical Society of Japan Conference Proceedings},
year = {2015},
pages = {010011},
volume = {6},
abstract = {Studies on nuclear astrophysics, resonant structure, and nuclear reaction are going on at CRIB (CNS Radioactive Ion
Beam separator), a low-energy RI beam separator operated by Center for Nuclear Study (CNS), the University of Tokyo.
Two major methods used at CRIB to study nuclear reactions of astrophysical relevance are the resonant scattering,
and direct measurements of ($\alpha$,p) reactions using a thick-gas target. Several experiments for decay measurements and
reaction mechanism are also performed using low-energy RI beams at CRIB. Some of the results from recent experiments at CRIB are discussed.},
adsurl = {http://adsabs.harvard.edu/abs/2015aris.confa0011Y},
doi = {10.7566/JPSCP.6.010011},
eid = {010011}
}

@article{2015AIPC.1645..387S,
title = {{{$\beta$}-delayed {$\alpha$} decay of $^{16}$N and the $^{12}$C({$\alpha$}, {$\gamma$})$^{16}$O
cross section at astrophysical energies: A new experimental approach}},
author = {{Sanfilippo}, S. and {Cherubini}, S. and {Hayakawa}, S. and
{Di Pietro}, A. and {Figuera}, P. and {Gulino}, M. and {La Cognata}, M. and
{Lattuada}, M. and {Spitaleri}, C. and {Yamaguchi}, H. and {Kahl}, D. and
{Nakao}, T. and {Kubono}, S. and {Wakabayashi}, Y. and {Hashimoto}, T. and
{Iwasa}, N. and {Okoda}, Y. and {Ushio}, K. and {Teranishi}, T. and
{Mazzocco}, M. and {Signorini}, C. and {Torresi}, D. and {Moon}, J.~Y. and
{Komatsubara}, T. and {Lee}, P.~S. and {Chae}, K.~Y. and {Gwak}, M.~S.},
journal = {American Institute of Physics Conference Series},
year = {2015},
month = feb,
pages = {387-391},
volume = {1645},
abstract = {{The $^{12}$C ({$\alpha$},{$\gamma$})$^{16}$O reaction at energies
corresponding to the quiescent helium burning in massive stars is
regarded as one of the most important processes in nuclear astrophysics.
Although this process has being studied for over four decades, our
knowledge of its cross section at the energies of interest for
astrophysics is still widely unsatisfactory. Indeed, no experimental
data are available around 300 keV and in the energy region of
astrophysical interest extrapolations are performed using some
theoretical approaches, usually R-matrix calculations. Consequently, the
published astrophysical factors range from 1 to 288 keVb for
S$_{E1}$(300) and 7 to 120 keVb for S$_{E2}$(300),
especially because of the unknown contribution coming from subthreshold
resonances. To improve the reliability of these extrapolations, data
from complementary experiments, such as elastic and quasi-elastic
{$\alpha$} scattering on $^{12}$C , {$\alpha$}-transfer reactions to
$^{16}$O , and $^{16}$N decay are usually included in the
analysis. Here the {$\beta$}-delayed {$\alpha$} decay of $^{16}$N is
used to infer information on the $^{12}$C
({$\alpha$},{$\gamma$})$^{16}$O reaction and a new experimental
technique is suggested.
}},
adsurl = {http://adsabs.harvard.edu/abs/2015AIPC.1645..387S},
doi = {10.1063/1.4909607},
series = {American Institute of Physics Conference Series}
}

@article{Yamaguchi:14c,
author = {H Yamaguchi and D Kahl and T Nakao and Y Wakabayashi and T Hashimoto and S Hayakawa and T Kawabata and T Teranishi and Y K Kwon and D N
Binh and L H Khiem and N N Duy and S Kubono and T Suhara and Y Kanada-En'yo and J Y Moon and A Kim and N Iwasa and P S Lee and K Y Chae and S M
Cha and M S Gwak and D H Kim and E Milman},
title = {Nuclear clusters studied with alpha resonant scatterings using RI beams at CRIB},
journal = {Journal of Physics: Conference Series},
volume = {569},
number = {1},
pages = {012019},
url = {http://stacks.iop.org/1742-6596/569/i=1/a=012019},
year = {2014},
abstract = {Alpha resonant scattering is a simple and promising method to study alpha-cluster structure in nuclei. It has several good features which enable us to
perform measurements with short-lived and relatively low-intense RI beams. Several measurements on alpha resonant scattering have been carried out at CRIB
(CNS Radioactive Ion Beam separator), which is a low-energy RI beam separator at Center for Nuclear Study (CNS)
of the University of Tokyo. Recent alpha resonant scattering studies at CRIB, using 7Li, 7Be and 10Be beams with a helium gas target, are discussed.}
}

@article{Kahl:OMEG12,
author = {Kahl, D. and Hashimoto, T. and Duy, N. N. and Kubono, S. and Yamaguchi, H. and
Binh, D. N. and Chen, A. A. and Cherubini, S. and Hayakawa, S. and He, J. J. and Ishiyama, H. and
Iwasa, N. and Khiem, L. H. and Kwon, Y. K. and Michimasa, S. and Nakao, T. and Ota, S. and Teranishi,
T. and Tokieda, H. and Wakabayashi, Y. and Yamada, T. and Zhang, L. Y.},
title = {Active target studies of the $\alpha p$-process at CRIB},
journal = {AIP Conference Proceedings},
year = {2014},
volume = {1594},
number = {},
pages = {163-170},
url = {http://scitation.aip.org/content/aip/proceeding/aipcp/10.1063/1.4874062},
doi = {http://dx.doi.org/10.1063/1.4874062}
}

@article{He:OMEG12,
author = {He, J. J. and Hu, J. and Zhang, L. Y. and Xu, S. W. and Parikh, A. and Yamaguchi, H. and
Kahl, D. and Ma, P. and Chen, S. Z. and Su, J. and Wakabayashi, Y. and Togano, Y. and Hayakawa, S. and
Wang, H. W. and Tian, W. D. and Chen, R. F. and Guo, B. and Nakao, T. and Teranishi, T. and Moon, J. Y.
and Jung, H. S. and Hashimoto, T. and Chen, A. A. and Irvine, D. and Hahn, K. I. and Iwasa, N. and
Yamada, T. and Komatsubara, T. and Lee, C. S. and Kubono, S.},
title = {Astrophysics studies relevant to stellar x-ray bursts},
journal = {AIP Conference Proceedings},
year = {2014},
volume = {1594},
number = {},
pages = {176-183},
url = {http://scitation.aip.org/content/aip/proceeding/aipcp/10.1063/1.4874064},
doi = {http://dx.doi.org/10.1063/1.4874064}
}

@article{Cherubini:OMEG12,
author = {Cherubini, S. and Gulino, M. and Spitaleri, C. and La Cognata, M. and Lamia, L. and
Puglia, S. and Rapisarda, G. and Romano, S. and Kubono, S. and Yamaguchi, H. and Binh, D. and Hayakawa,
S. and Kurihara, Y. and Wakabayashi, Y. and Bishop, S. and Coc, A. and De S\'{e}r\'{e}ville, N. and Hammache, F.},
title = {First results of Trojan horse method using radioactive ion beams:
18F(p,$\alpha$)
at astrophysical energies},
journal = {AIP Conference Proceedings},
year = {2014},
volume = {1594},
number = {},
pages = {184-189},
url = {http://scitation.aip.org/content/aip/proceeding/aipcp/10.1063/1.4874065},
doi = {http://dx.doi.org/10.1063/1.4874065}
}

@article{Yamaguchi:OMEG12,
author = {Yamaguchi, H. and Kahl, D. and Nakao, T. and Wakabayashi, Y. and Kubano, S. and
Hashimoto, T. and Hayakawa, S. and Kawabata, T. and Iwasa, N. and Teranishi, T. and
Kwon, Y. K. and Binh, D. N. and Khiem, L. H. and Duy, N. G.},
title = {Alpha resonant scattering for astrophysical reaction studies},
journal = {AIP Conference Proceedings},
year = {2014},
volume = {1594},
number = {},
pages = {220-225},
url = {http://scitation.aip.org/content/aip/proceeding/aipcp/10.1063/1.4874072},
doi = {http://dx.doi.org/10.1063/1.4874072}
}

@article{Yamaguchi:13c,
title = {Recent developments and research projects at the low-energy RI beam facility CRIB },
journal = {Nuclear Instruments and Methods in Physics Research Section B: Beam Interactions with Materials and Atoms },
volume = {317},
number = {},
pages = { 664--667 },
year = {2013},
note = {},
issn = {0168-583X},
doi = {http://dx.doi.org/10.1016/j.nimb.2013.05.090},
author = {H. Yamaguchi and D. Kahl and T. Nakao and Y. Wakabayashi and S. Kubono and T. Hashimoto and S. Hayakawa and
T. Kawabata and N. Iwasa and T. Teranishi and Y.K. Kwon and D.N. Binh and L.H. Khiem and N.N. Duy}
}

@article{2012AIPC.1484...25B,
title = {{Measurement of $^{21}$Na({$\alpha$},p)$^{24}$Mg stellar reaction using a $^{21}$Na RI-beam}},
author = {{Binh}, D.~N. and {Kubono}, S. and {Yamaguchi}, H. and {Hayakawa}, S. and {Hashimoto}, T. and {Kahl}, D. and {Teranishi}, T. and {Iwasa}, N. and {Kato}, S. and {Khiem}, L.~H. and {Tho}, N.~T. and {Wakabayashi}, Y.
},
journal = {American Institute of Physics Conference Series},
year = {2012},
month = nov,
pages = {25-30},
volume = {1484},
abstract = {{We performed an experiment of the $^{21}$Na({$\alpha$}p)$^{24}$Mg reaction for the first time by a direct measurement with a thick target method. The studied energy was covered for high temperature conditions in X-ray bursts and core-collapse supernovae. The $^{21}$Na({$\alpha$}p)$^{24}$Mg reaction could make a branch of the extended {$\alpha$}p-process and could be important to understand the production of $^{22}$Na during the hydrogen explosion at high temperature, like in X-ray bursts, and the $^{44}$Ti production from core-collapse supernovae. }},
adsurl = {http://adsabs.harvard.edu/abs/2012AIPC.1484...25B},
doi = {10.1063/1.4763367},
editor = {{Kubono}, S. and {Hayakawa}, T. and {Kajino}, T. and {Miyatake}, H. and {Motobayashi}, T. and {Nomoto}, K.},
keywords = {alpha particle-nucleus reactions, nuclei with mass number 20 to 38, supernovae},
owner = {daid},
series = {American Institute of Physics Conference Series},
timestamp = {2013.05.08}
}

@article{2012AIPC.1484..454H,
title = {{Direct measurement of the $^{18}$Ne({$\alpha$},p)$^{21}$Na reaction}},
author = {{Hashimoto}, T. and {Kubono}, S. and {Yamaguchi}, H. and {Hayakawa}, S. and {Kahl}, D.~M. and {Ota}, S. and {Michimasa}, S. and {Tokieda}, H. and {Ishiyama}, H. and {Watanabe}, Y.~X. and {Hirayama}, Y. and {Imai}, N. and {Miyatake}, H. and {Jeong}, S.~C. and {Yamaguchi}, K. and {Arai}, I. and {Komatsubara}, T. and {Fukuda}, T. and {Mizoi}, Y. and {Das}, S.~K. and {Iwasa}, N. and {Yamada}, T. and {Chen}, A.~A. and {He}, J.~J.},
journal = {American Institute of Physics Conference Series},
year = {2012},
month = nov,
pages = {454-456},
volume = {1484},
abstract = {{The excitation fuction of the $^{18}$Ne({$\alpha$},p)$^{21}$Na reaction in was directry measured using a new active target detector system. We are analyzing accumulated data. We will report the result of the development of the GEM - MSTPC and the preliminary results of the $^{18}$Ne({$\alpha$},p)$^{21}$Na a experiment. }},
adsurl = {http://adsabs.harvard.edu/abs/2012AIPC.1484..454H},
doi = {10.1063/1.4763451},
editor = {{Kubono}, S. and {Hayakawa}, T. and {Kajino}, T. and {Miyatake}, H. and {Motobayashi}, T. and {Nomoto}, K.},
keywords = {alpha particle-nucleus reactions, nuclear energy levels, Level density, Transfer reactions},
owner = {daid},
series = {American Institute of Physics Conference Series},
timestamp = {2013.05.08}
}

@article{2012AIPC.1484..445H,
title = {{Direct measurement of the breakout reaction $^{11}$C({$\alpha$},p)$^{14}$N in explosive hydrogen-burning process}},
author = {{Hayakawa}, S. and {Kubono}, S. and {Kahl}, D. and {Yamaguchi}, H. and {Binh}, D.~N. and {Hashimoto}, T. and {Wakabayashi}, Y. and {He}, J.~J. and {Iwasa}, N. and {Kato}, S. and {Komatsubara}, T. and {Kwon}, Y.~K. and {Teranishi}, T. and {Wanajo}, S.},
journal = {American Institute of Physics Conference Series},
year = {2012},
month = nov,
pages = {445-447},
volume = {1484},
abstract = {{We determined the $^{11}$C({$\alpha$},p)$^{14}$N reaction rate relevant to the nucleosynthesis in explosive hydrogen-burning stars. The measurement was performed by means of the thick target method in inverse kinematics with $^{11}$C RI beams. We derived the excitation functions for the ground-state transition and excited-state transitions using time-of-flight information for the first time. The present reaction rate is compared to the previous one. }},
adsurl = {http://adsabs.harvard.edu/abs/2012AIPC.1484..445H},
doi = {10.1063/1.4763448},
editor = {{Kubono}, S. and {Hayakawa}, T. and {Kajino}, T. and {Miyatake}, H. and {Motobayashi}, T. and {Nomoto}, K.},
keywords = {alpha particle-nucleus reactions, nucleosynthesis, stellar internal processes, Stellar hydrogen burning, Nucleosynthesis in novae, supernovae, and other explosive environments, Stellar structure, interiors, evolution, nucleosynthesis, ages},
owner = {daid},
series = {American Institute of Physics Conference Series},
timestamp = {2013.05.08}
}

@article{2012AIPC.1498..339H,
title = {{Direct measurement of the $^{11}$C({$\alpha$},p)$^{14}$N reaction at CRIB: A path from pp-chain to CNO}},
author = {{Hayakawa}, S. and {Kubono}, S. and {Kahl}, D. and {Yamaguchi}, H. and {Binh}, D.~N. and {Hashimoto}, T. and {Wakabayashi}, Y. and {He}, J.~J. and {Iwasa}, N. and {Kato}, S. and {Komatsubara}, T. and {Kwon}, Y.~K. and {Teranishi}, T. and {Wanajo}, S.},
journal = {American Institute of Physics Conference Series},
year = {2012},
month = nov,
pages = {339-343},
volume = {1498},
abstract = {{We determined the total reaction rate of the $^{11}$C({$\alpha$},p)$^{14}$N reaction relevant to the nucleosynthesis in explosive hydrogen-burning stars. The measurement was performed by means of the thick target method in inverse kinematics with $^{11}$C RI beams. We performed the identification of the ground-state transition and excited-state transitions using time-of-flight information for the first time. }},
adsurl = {http://adsabs.harvard.edu/abs/2012AIPC.1498..339H},
doi = {10.1063/1.4768515},
editor = {{Trache}, L. and {Gina Isar}, P.},
keywords = {alpha particle-nucleus reactions, nucleosynthesis, $^{3}$H-, $^{3}$He-, and $^{4}$He-induced reactions, Stellar hydrogen burning, Stellar structure, interiors, evolution, nucleosynthesis, ages},
owner = {daid},
series = {American Institute of Physics Conference Series},
timestamp = {2013.05.08}
}

@article{2012AIPC.1484..240H,
title = {{Study of resonant scattering of $^{21}$Na+p relevant to astrophysical $^{18}$Ne({$\alpha$},p)$^{21}$Na reaction}},
author = {{He}, J.~J. and {Zhang}, L.~Y. and {Xu}, S.~W. and {Chen}, S.~Z. and {Hu}, J. and {Ma}, P. and {Chen}, R.~F. and {Yamaguchi}, H. and {Kubono}, S. and {Hashimoto}, T. and {Kahl}, D. and {Hayakawa}, S. and {Wakabayashi}, Y. and {Togano}, Y. and {Wang}, H.~W. and {Tian}, W.~D. and {Guo}, B. and {Teranishi}, T. and {Iwasa}, N. and {Yamada}, T. and {Komatsubara}, T.},
journal = {American Institute of Physics Conference Series},
year = {2012},
month = nov,
pages = {240-245},
volume = {1484},
abstract = {{Astrophysical $^{18}$Ne({$\alpha$},p)$^{21}$Na reaction is one of the most probable breakout routes, which lead to the rp-process from the hot-CNO cycle, converting the initial CNO elements into heavier elements in Type I x-ray bursters. Presently, there is no much experimental cross-section data reported at the energy of astrophysical interest, and resonant spectroscopic information in compound $^{22}$Mg is scarce as well. The experiment has been carried out by using the CNS radioactive ion beam separator (CRIB). Resonant properties in $^{22}$Mg have been studied via the resonant elastic scattering of $^{21}$Na+p, and cross section of the time-reversal reaction of $^{21}$Na(p,{$\alpha$})$^{18}$Ne been measured simultaneously. A wide excitation energy region up to Ex \~{} 9.5 MeV in $^{22}$Mg has been scanned with a thick-target method. Some preliminary results will be reported. }},
adsurl = {http://adsabs.harvard.edu/abs/2012AIPC.1484..240H},
doi = {10.1063/1.4763401},
editor = {{Kubono}, S. and {Hayakawa}, T. and {Kajino}, T. and {Miyatake}, H. and {Motobayashi}, T. and {Nomoto}, K.},
keywords = {alpha particle-nucleus scattering, nucleosynthesis, X-ray sources (astronomical)},
owner = {daid},
series = {American Institute of Physics Conference Series},
timestamp = {2013.05.08}
}

@article{2012AIPC.1484..307J,
title = {{Study of proton resonance structure in $^{27}$P via resonant elastic scattering of $^{26}$Si+p}},
author = {{Jung}, H.~S. and {Lee}, C.~S. and {Kwon}, Y.~K. and {Moon}, J.~Y. and {Lee}, J.~H. and {Yun}, C.~C. and {Kubono}, S. and {Yamaguchi}, H. and {Hashimoto}, T. and {Kahl}, D. and {Hayakawa}, S. and {Choi}, S. and {Kim}, M.~J. and {Kim}, Y.~H. and {Kim}, Y.~K. and {Park}, J.~S. and {Kim}, E.~J. and {Moon}, C.-B. and {Teranishi}, T. and {Wakabayashi}, Y. and {Iwasa}, N. and {Yamada}, T. and {Togano}, Y. and {Kato}, S. and {Cherubini}, S. and {Rapisarda}, G.~G.},
journal = {American Institute of Physics Conference Series},
year = {2012},
month = nov,
pages = {307-312},
volume = {1484},
abstract = {{A measurement of resonant elastic scattering of $^{26}$Si+p was performed with a thick target using a $^{26}$Si radioactive ion beam at the CRIB (CNS Radioactive Ion Beam separator) of the Center for Nuclear Study (CNS), the University of Tokyo. The excitation function of $^{27}$P was measured successfully with the inverse kinematics method through a covered the range of excitation energies from Ex \~{} 2.3 to 3.8 MeV, providing information about the resonance structure of this nucleus. The properties of these resonances are important to better determine the production rates of $^{26}$Si(p,g)$^{27}$P reaction, which is one of the astrophysically important nuclear reactions to understand the production of the $^{26}$Al. Some new resonant states have been investigated, and determined their resonance parameters, such as excitation energies, proton partial widths, and spin-parities by R-matrix calculation. }},
adsurl = {http://adsabs.harvard.edu/abs/2012AIPC.1484..307J},
doi = {10.1063/1.4763412},
editor = {{Kubono}, S. and {Hayakawa}, T. and {Kajino}, T. and {Miyatake}, H. and {Motobayashi}, T. and {Nomoto}, K.},
keywords = {nuclear energy levels, nuclear resonance scattering, nuclear spin, nuclei with mass number 20 to 38, proton radiative capture, proton-nucleus scattering, Spin, parity, and isobaric spin, Level density, Resonance reactions, Elastic proton scattering, Radiative capture, 20{\lt}=A{\lt}=38},
owner = {daid},
series = {American Institute of Physics Conference Series},
timestamp = {2013.05.08}
}

@article{2012nuco.confE.200J,
title = {{Experimental study of resonant states in $^{26}$Si and $^{27}$P via elastic scattering of $^{25}$Al+p and $^{26}$Si+p}},
author = {{Jung}, H.~S. and {Lee}, C.~S. and {Moon}, J.~Y. and {Kwon}, Y.~K. and {Lee}, J.~H. and {Yun}, C.~C. and {Kubono}, S. and {Yamaguchi}, H. and {Kahl}, D.},
journal = {Proceedings of Science},
year = {2012},
pages = {200:1-6},
volume = {NIC XII},
abstract = {The rapid proton capture process (rp process) is a dominant reaction sequence in explosive hydrogen burning that synthesizes heavier elements, especially proton-rich unstable nuclides. Therefore, accurate thermonuclear reaction rates for (p,$\gamma$) reactions on the rp process path are essential for an understanding of the nucleosynthesis processes and energy production. We studied proton resonant states in $^{26}$Si and $^{27}$P via elastic scattering in inverse kinematics at the low-energy RI beam facility CRIB (CNS Radioactive Ion Beam separator), University of Tokyo. By using a thick H$_{2}$ gas target, excitation energies range of 6.8 to 8.2 MeV in $^{26}$Si and 2.3 to 3.8 MeV in $^{27}$P were scanned, respectively. Several resonances above the proton threshold level were observed with high statistics and free from any background contribution in the target. Their resonance parameters were subsequently extracted by an R-matrix analysis; these are important to better constrain the production rates of the $^{25}$Al(p,$\gamma$)$^{26}$Si and $^{26}$Si(p,$\gamma$)$^{27}$P reactions.},
owner = {daid},
timestamp = {2013.05.08},
url = {http://pos.sissa.it/archive/conferences/146/200/NIC\%20XII_200.pdf}
}

@article{2012nuco.confE.201K,
title = {{Measurement of the $^{30}$S + $\alpha$ system for type I X-ray bursts}},
author = {{Kahl}, D. and {Chen}, A.~A. and {Kubono}, S. and {Hashimoto}, T. and {Binh}, D.~N. and {Chen}, J. and {Cherubini}, S. and {Duy}, N.~N. and {Hayakawa}, S. and {Iwasa}, N. and {Jung}, H.~S. and {Kato}, S. and {Kwon}, Y.~K. and {Michimasa}, S. and {Nishimura}, S. and {Ota}, S. and {Setoodehnia}, K. and {Teranishi}, T. and {Tokieda}, H. and {Yamada}, T. and {Yamaguchi}, H. and {Yun}, C.~C. and {Zhang}, L.~Y.},
journal = {Proceedings of Science},
year = {2012},
pages = {201:1-5},
volume = {NIC XII},
abstract = {The $^{30}$S($\alpha$,\,p) reaction is considered to be important in the nuclear trajectory to higher mass in type I X-ray bursts. The reaction flow encounters a bottle-neck at $^{30}$S, owing to the competition of photo-disintegration with further proton capture, and because the half-life of this isotope is on the order of the burst rise timescale. Different burst simulations by various researchers indicate the ($\alpha$,\,p) reaction may by-pass this waiting point, depending on the stellar reaction rate, which has not previously been measured experimentally, and the structure of the compound nucleus $^{34}$Ar is not well understood above the alpha-threshold. The $^{30}$S($\alpha$,\,p) reaction could explain rare bolometrically double-peaked burst profiles, appears to make a considerable contribution to the overall energy generation, and affects the neutron star crustal composition for the recurrent inertia required in burst models to reproduce astronomical observations. Using a low-energy $^{30}$S radioactive ion beam and an active target technique (a helium gas mixture serves as both a target gas and a detector fill gas), we acquired data on both alpha elastic scattering of $^{30}$S as well as the $^{30}$S($\alpha$,\,p) reaction simultaneously at relevant energies for X-ray bursts. We present for the first time the status of the data analysis and the preliminary results of this research.},
owner = {daid},
timestamp = {2013.05.08},
url = {http://pos.sissa.it/archive/conferences/146/201/NIC\%20XII_201.pdf}
}

@article{2012AIPC.1484..189K,
title = {{Experimental challenge to nuclear physics problems in the {$\nu$}p-process}},
author = {{Kubono}, S. and {Binh}, D.~N. and {Hayakawa}, S. and {Hashimoto}, T. and {Kahl}, D.~M. and {Yamaguchi}, H. and {Wakabayashi}, Y. and {Teranishi}, T. and {Iwasa}, N. and {Komatsubara}, T. and {Kato}, S. and {Chen}, A. and {Cherubini}, S. and {Choi}, S.~H. and {Hahn}, I.~S. and {He}, J.~J. and {Khiem}, L.~H. and {Lee}, C.~S. and {Kwon}, Y.~K. and {Wanajo}, S. and {Janka}, H.-T.},
journal = {American Institute of Physics Conference Series},
year = {2012},
month = nov,
pages = {189-196},
volume = {1484},
abstract = {{Astrophysical stellar reactions at extremely high temperatures involve a variety of problems both in nuclear reactions and nuclear structures. Specifically, the problems in the {$\nu$}pprocess were discussed in this talk based on our recent experimental results with low-energy RI beams and a simulation study. The {$\nu$}p-process is one of the key processes for investigating the mechanism of type II supernovae, and the process could be possibly responsible for ''the excess production'' of p-nuclei around mass 90-100. Alpha cluster resonances have been discovered experimentally to play a crucial role for the stellar ({$\alpha$}, p) reactions just above the alpha threshold. Neutron induced reactions in the proton-rich nuclear regions in the {$\nu$}p-process are also suggested to play an important role, which involve nuclear structures of high level density at high excitation energies, probably giant resonances. The discussion also covered the p-nuclei production through the {$\nu$}p-process at around mass 100. }},
adsurl = {http://adsabs.harvard.edu/abs/2012AIPC.1484..189K},
doi = {10.1063/1.4763394},
editor = {{Kubono}, S. and {Hayakawa}, T. and {Kajino}, T. and {Miyatake}, H. and {Motobayashi}, T. and {Nomoto}, K.},
keywords = {alpha particle-nucleus reactions, giant resonances, nuclear cluster model, nuclear density, nuclear energy levels, nuclear mass, nuclear reaction theory, nuclear structure theory, supernovae, Properties of nuclei; nuclear energy levels, Binding energies and masses, Level density, Cluster models, Nuclear reaction models and methods, Giant resonances, $^{3}$H-, $^{3}$He-, and $^{4}$He-induced reactions, Nucleosynthesis in novae, supernovae, and other explosive environments, Nuclear physics aspects of novae, supernovae, and other explosive environments, Supernovae},
owner = {daid},
series = {American Institute of Physics Conference Series},
timestamp = {2013.05.08}
}

@article{2012PThPS.196..346K,
title = {{Alpha-Cluster Dominance in the {$\alpha$}p Process in Explosive Hydrogen Burning}},
author = {{Kubono}, S. and {Dam}, N. and {Hayakawa}, S. and {Hashimoto}, H. and {Kahl}, D. and {Yamaguchi}, H. and {Wakabayashi}, Y. and {Teranishi}, T. and {Iwasa}, N. and {Komatsubara}, T. and {Kato}, S. and {Chen}, A. and {Cherubini}, S. and {Choi}, S. and {Hahn}, I. and {He}, J. and {Le}, H.~K. and {Lee}, C. and {Kwon}, Y. and {Wanajo}, S. and {Janka}, H.},
journal = {Progress of Theoretical Physics Supplement},
year = {2012},
pages = {346-351},
volume = {196},
abstract = {{Nucleosynthesis by alpha particles and heavier 4n nuclei are of great interest as they would involve nuclear cluster resonances. The role of nuclear clustering is discussed for nucleosynthesis with the Cluster Nucleosynthesis Diagram (CND) proposed before, especially those involving alpha induced reactions, based on our recent works of ({$\alpha$},p) reactions with low energy RI beams. We present experimental results that alpha resonances play a crucial role for the ({$\alpha$},p) reaction cross sections. Molecular resonances are also briefly discussed along this line for O- and C-burning. }},
adsurl = {http://adsabs.harvard.edu/abs/2012PThPS.196..346K},
owner = {daid},
timestamp = {2013.05.08}
}

@article{2012AIPC.1484..365K,
title = {{Measurement of $^{25}$Al+p resonant elastic scattering for studying the $^{25}$Al(p,{$\gamma$})$^{26}$Si}},
author = {{Kwon}, Y.~K. and {Lee}, C.~S. and {Jung}, H.~S. and {Moon}, J.~Y. and {Lee}, J.~H. and {Yun}, C.~C. and {Kubono}, S. and {Yamaguchi}, H. and {Hashimoto}, T. and {Kahl}, D. and {Hayakawa}, S. and {Choi}, S. and {Kim}, M.~J. and {Kim}, Y.~H. and {Kim}, Y.~K. and {Park}, J.~S. and {Kim}, E.~J. and {Moon}, C.-B. and {Teranishi}, T. and {Wakabayashi}, Y. and {Iwasa}, N. and {Yamada}, T. and {Togano}, Y. and {Kato}, S. and {Cherubini}, S. and {Rapisarda}, G.~G.},
journal = {American Institute of Physics Conference Series},
year = {2012},
month = nov,
pages = {365-368},
volume = {1484},
abstract = {{Proton resonant states in $^{26}$Si have been studied by the resonant elastic scattering of $^{25}$Al+p with a $^{25}$Al radioactive ion beam at 2.863 MeV/nucleon bombarding a thick H$_{2}$ gas target with the inverse kinematics method at the low-energy RI beam facility CRIB (CNS Radioactive Ion Beam separator), University of Tokyo. The properties of these resonance states are important to better determine the production rates of $^{25}$Al(p,{$\gamma$})$^{26}$Si reaction, which is one of the astrophysically important nuclear reactions to understand the production of the ground state of $^{26}$Al, the emitter of its characteristic 1.809-MeV gamma-ray, under the explosive stellar environments such as novae and X-ray bursts. In this work, several resonances above the proton threshold level have been observed with a high statistics and background free through a covered the range of excitation energies from Ex \~{} 6.8 to 8.2 MeV. }},
adsurl = {http://adsabs.harvard.edu/abs/2012AIPC.1484..365K},
doi = {10.1063/1.4763422},
editor = {{Kubono}, S. and {Hayakawa}, T. and {Kajino}, T. and {Miyatake}, H. and {Motobayashi}, T. and {Nomoto}, K.},
keywords = {nuclear energy levels, nuclei with mass number 20 to 38, proton radiative capture, proton-nucleus scattering, Level density, Elastic proton scattering, Radiative capture, 20{\lt}=A{\lt}=38},
owner = {daid},
series = {American Institute of Physics Conference Series},
timestamp = {2013.05.08}
}

@article{2012AIPC.1484...19W,
title = {{Indirect measurements of reactions in hot p-p chain and CNO cycles}},
author = {{Wang}, Y.~B. and {Guo}, B. and {Jin}, S.~J. and {Li}, Z.~H. and {Binh}, D.~N. and {Hashimoto}, H. and {Hayakawa}, S. and {He}, J.~J. and {Hu}, J. and {Iwasa}, N. and {Kahl}, D.~M. and {Kubono}, S. and {Kume}, N. and {Li}, E.~T. and {Li}, Y.~J. and {Liu}, X. and {Su}, J. and {Xu}, S.~W. and {Yamaguchi}, H. and {Yan}, S.~Q. and {Zeng}, S. and {Bai}, X.~X. and {Lian}, G. and {Wang}, B.~X. and {Liu}, W.~P.},
journal = {American Institute of Physics Conference Series},
year = {2012},
month = nov,
pages = {19-24},
volume = {1484},
abstract = {{Several reactions have been experimentally studied, including the $^{12}$N(d,n)$^{13}$O and the ones induced by the $^{3}$He+$^{12}$C entrance channel. The former was carried out at the CRIB facility of University of Tokyo, aiming to indirectly determine the astrophysical reaction rates of the $^{12}$N(p,{$\gamma$})$^{13}$O reaction. For the $^{3}$He+$^{12}$C entrance channel, many excited states of several nuclei are populated and the angular distribution of each state is being analyzed. }},
adsurl = {http://adsabs.harvard.edu/abs/2012AIPC.1484...19W},
doi = {10.1063/1.4763366},
editor = {{Kubono}, S. and {Hayakawa}, T. and {Kajino}, T. and {Miyatake}, H. and {Motobayashi}, T. and {Nomoto}, K.},
keywords = {deuteron-nucleus reactions, heavy ion-nucleus scattering, nuclear energy levels, nuclei with mass number 6 to 19, proton radiative capture, Level density, Angular distribution and correlation measurements, Radiative capture, Elastic and quasielastic scattering, 6{\lt}=A{\lt}=19, Elementary particle processes},
owner = {daid},
series = {American Institute of Physics Conference Series},
timestamp = {2013.05.08}
}

@article{2012AIPC.1484..225Y,
title = {{Alpha-induced reaction studies using low-energy RI beams at CRIB}},
author = {{Yamaguchi}, H. and {Kahl}, D. and {Hu}, J. and {Kubono}, S. and {Hayakawa}, S. and {Hashimoto}, T.},
journal = {American Institute of Physics Conference Series},
year = {2012},
month = nov,
pages = {225-231},
volume = {1484},
abstract = {{CRIB (CNS Radioactive Ion Beam separator) is a low-energy RI beam separator at the Center for Nuclear Study (CNS) of the University of Tokyo. Studies on proton and alpha resonance scatterings, ({$\alpha$}, p) reactions, and other types of measurements ({$\beta$}-decay lifetimes etc.) have been performed using RI beams at CRIB, motivated by interests on astrophysical reactions and exotic nuclear structure. Among the studies at CRIB, the measurement of $^{7}$Li+{$\alpha$}/$^{7}$Be+{$\alpha$} resonant scatterings are presented. }},
adsurl = {http://adsabs.harvard.edu/abs/2012AIPC.1484..225Y},
doi = {10.1063/1.4763399},
editor = {{Kubono}, S. and {Hayakawa}, T. and {Kajino}, T. and {Miyatake}, H. and {Motobayashi}, T. and {Nomoto}, K.},
keywords = {alpha particle-nucleus scattering, nuclear resonance scattering, nuclear structure, nuclei with mass number 6 to 19, Resonance reactions, Elastic and inelastic scattering, 6{\lt}=A{\lt}=19, Elementary particle processes},
owner = {daid},
series = {American Institute of Physics Conference Series},
timestamp = {2013.05.08}
}

@article{2012nuco.confE.244Y,
title = {{Recent astrophysical studies at the low-energy RI beam separator CRIB}},
author = {{Yamaguchi}, H. and {Kahl}, D. and {Nakao}, T. and {Kubono}, S},
journal = {Proceedings of Science},
year = {2012},
pages = {244:1-6},
volume = {NIC XII},
abstract = {CRIB (CNS Radioactive Ion Beam separator) is a low-energy RI beam separator at Center for Nuclear Study (CNS) of the University of Tokyo. Studies on proton and alpha resonance scatterings, ($\alpha$,p) reactions, and other types of measurements ( $\beta$-decay lifetimes etc.) have been performed using RI beams at CRIB, motivated by interests on astrophysical reactions and exotic nuclear structure. Among the studies at CRIB, the measurement of $^{7}$Be+$\alpha$ resonant scattering is presented.},
owner = {daid},
timestamp = {2013.05.08},
url = {http://pos.sissa.it/archive/conferences/146/244/NIC\%20XII_244.pdf}
}

@article{2012nuco.confE.186Z,
title = {{Experimental Study of the Key $^{18}$Ne($\alpha$,p)$^{21}$Na reaction}},
author = {{Zhang}, L.~Y. and {He}, J.~J. and {Xu}, S.~W. and {Yamaguchi}, H. and {Kubono}, S. and {Wakabayashi}, Y. and {Chen}, S.~Z. and {Hu}, J. and {Ma}, P. and {Togano}, Y. and {Hashimoto}, T. and {Kahl}, D. and {Teranishi}, T. and {Chen}, R.~F. and {Wang}, H.~W. and {Tian}, W.~D. and {Guo}, B. and {Hayakawa}, S. and {Iwasa}, N. and {Yamada}, T. and {Komatsubara}, T.},
journal = {Proceedings of Science},
year = {2012},
pages = {186:1-5},
volume = {NIC XII},
abstract = {The $^{18}$Ne($\alpha$, p)$^{21}$Na reaction is thought to be one of the key breakout reaction from the hot CNO cycle to the rp-process in X-ray bursts. We investigated the resonant properties of the compoundnucleus $^{22}$Mg by measuring the resonant elastic scattering of $^{21}$Na+p. An 89 MeV $^{21}$Na radioactive beam was produced by CRIB and then bombarded a 93-$\mu$m-thick polyethylene target. The $^{21}$Na beam intensity was about 2$\times$10$^{5}$ pps, with a purity of about 70\% on the target. The recoiled protons were measured by three sets of $\Delta$E-E telescope respectively. A wide excitation energy range of 5.5-9.2 MeV in $^{22}$Mg was scanned with a thick-target method. Some preliminary results are shown.},
owner = {daid},
timestamp = {2013.05.08},
url = {http://pos.sissa.it/archive/conferences/146/186/NIC\%20XII_186.pdf}
}

@article{2010AIPC.1269..387B,
title = {{Direct Measurement of $^{21}$Na+{$\alpha$} Stellar Reaction}},
author = {{Binh}, D.~N. and {Kubono}, S. and {Yamaguchi}, H. and {Hayakawa}, S. and {Hashimoto}, T. and {Kahl}, D. and {Teranishi}, T. and {Iwasa}, N. and {Kume}, N. and {Kato}, S. and {Khiem}, L.~H. and {Tho}, N.~T. and {Wakabayashi}, Y.},
journal = {American Institute of Physics Conference Series},
year = {2010},
month = aug,
pages = {387-389},
volume = {1269},
abstract = {The measurement of the resonant alpha scattering and the $^{21}$Na($\alpha$, p) reaction were performed for the first time in inverse kinematics with the thick target method using a $^{21}$Na radioisotope (RI) beam. This paper reports the current result of alpha scattering measurement and its astrophysics implication.},
adsurl = {http://adsabs.harvard.edu/abs/2010AIPC.1269..387B},
booktitle = {American Institute of Physics Conference Series},
doi = {10.1063/1.3485175},
editor = {{I.~Tanihara, H.~J.~Ong, A.~Tamii, T.~Kishimoto, T.~Kajino, S.~Kubono, \& T.~Shima}},
keywords = {radioactive ion beams, nucleosynthesis, beta-decay, gamma-rays, Sources of radioactive nuclei, Cosmic ray nucleosynthesis, Relation with nuclear matrix elements and nuclear structure, gamma-ray},
owner = {daid},
timestamp = {2012.04.18}
}

@article{2010NuPhA.834..667C,
title = {{Study of astrophysically important states in $^{26}$Si with the p($^{27}$Si,$^{26}$Si$^{*}$)d reaction and the p($^{25}$Al,p)$^{25}$Al elastic scattering}},
author = {{Chen}, J. and {Chen}, A.~A. and {Schatz}, H. and {Kubono}, S. and {Reyes}, A.~B. and {Smith}, A. and {Wales}, B. and {Ouellet}, C. and {Kahl}, D. and {Redondo}, D.~G. and {Lorusso}, G. and {Lenestour}, J. and {Conca}, J.~P. and {Smith}, K. and {Amthor}, M. and {Matos}, M. and {Yamaguchi}, H. and {Iwasa}, N. and {Hayakawa}, S. and {Michimasa}, S. and {Teranishi}, T. and {Kurihawa}, Y. and {Wakabayashi}, Y.},
journal = {Nuclear Physics A},
year = {2010},
month = mar,
pages = {667-669},
volume = {834},
abstract = {The astrophysically important states in $^{26}$Si have been studied with different reactions because of their dominant contribution to the $^{25}$Al(p,$\gamma$)$^{26}$Si reaction rate at nova temperatures. We performed two different experiments to study the states of interest in $^{26}$Si, with the aim of reducing the main uncertainty in the current $^{25}$Al(p,$\gamma$)$^{26}$Si rate by determining the level parameters of the dominant states more accurately. One is the p($^{27}$Si,$^{26}$Si$^{*}$)d experiment at NSCL, in which we measured the gamma-ray decays from the excited states in $^{26}$Si. The other one is the $^{25}$Al+p elastic scattering experiment with CRIB at RIKEN.},
adsurl = {http://adsabs.harvard.edu/abs/2010NuPhA.834..667C},
doi = {10.1016/j.nuclphysa.2010.01.119},
owner = {daid},
timestamp = {2012.04.18}
}

@article{2010AIPC.1269..104H,
title = {{Direct measurement of the $^{11}$C({$\alpha$}, p)$^{14}$N stellar reaction at CRIB}},
author = {{Hayakawa}, S. and {Kubono}, S. and {Hashimoto}, T. and {Yamaguchi}, H. and {Binh}, D.~N. and {Kahl}, D.~M. and {Wakabayashi}, Y. and {Iwasa}, N. and {Kume}, N. and {Miura}, I. and {Teranishi}, T. and {He}, J.~J. and {Kwon}, Y.~K. and {Komatsubara}, T. and {Kato}, S. and {Wanajo}, S. },
journal = {American Institute of Physics Conference Series},
year = {2010},
month = aug,
pages = {104-109},
volume = {1269},
abstract = {The first direct measurement of the $^{11}$C($\alpha$, p)$^{14}$N reaction cross section of astrophysical interest has been performed for the center-of-mass energies from 1 to 4.5 MeV with the CRIB (Center for Nuclear Study Radioactive Ion Beam separator). We successfully distinguished the transition to the ground state of $^{14}$N and that to the second excited state with a comparable yield. The resonant shapes in the preliminary excitation function for the ground state transition have been confirmed to be consistent with the ones from the time-reversal reaction data of previous experiments.},
adsurl = {http://adsabs.harvard.edu/abs/2010AIPC.1269..104H},
doi = {10.1063/1.3485120},
editor = {{I.~Tanihara, H.~J.~Ong, A.~Tamii, T.~Kishimoto, T.~Kajino, S.~Kubono, \& T.~Shima}},
keywords = {radioactive ion beams, supernovae, cyclotrons, telescopes, Sources of radioactive nuclei, Nuclear physics aspects of novae, supernovae, and other explosive environments, Cyclotrons, Astronomical and space-research instrumentation},
owner = {daid},
series = {American Institute of Physics Conference Series},
timestamp = {2012.04.18}
}

@article{2010AIPC.1269..424K,
title = {{$^{30}$S({$\alpha$}, p) in X-Ray Bursts at CRIB}},
author = {{Kahl}, D. and {Chen}, A.~A. and {Kubono}, S. and {Binh}, D.~N. and {Chen}, J. and {Hashimoto}, T. and {Hayakawa}, S. and {Kaji}, D. and {Kim}, A. and {Kurihara}, Y. and {Lee}, N.~H. and {Nishimura}, S. and {Ohshiro}, Y. and {Setoodeh Nia}, K. and {Wakabayashi}, Y. and {Yamaguchi}, H.},
journal = {American Institute of Physics Conference Series},
year = {2010},
month = aug,
pages = {424-426},
volume = {1269},
abstract = {Over the past three years, we have worked on developing a well-characterized $^{30}$S radioactive beam to be used in a future experiment aiming to directly measure the $^{30}$S($\alpha$, p) stellar reaction rate within the Gamow window of Type I X-ray bursts.},
adsurl = {http://adsabs.harvard.edu/abs/2010AIPC.1269..424K},
archiveprefix = {arXiv},
doi = {10.1063/1.3485188},
editor = {{I.~Tanihara, H.~J.~Ong, A.~Tamii, T.~Kishimoto, T.~Kajino, S.~Kubono, \& T.~Shima}},
eprint = {1010.4958},
keywords = {X-ray sources (astronomical), radioactive ion beams, magnetic moments, X-ray sources; X-ray bursts, Sources of radioactive nuclei, Electric and magnetic fields},
owner = {daid},
primaryclass = {nucl-ex},
series = {American Institute of Physics Conference Series},
timestamp = {2012.04.18}
}

@article{2010AIPC.1213..208K,
title = {{$^{30}$S Beam Development and X-ray Bursts}},
author = {{Kahl}, D. and {Chen}, A.~A. and {Kubono}, S. and {Binh}, D.~N. and {Chen}, J. and {Hashimoto}, T. and {Hayakawa}, S. and {Kaji}, D. and {Kim}, A. and {Kurihara}, Y. and {Lee}, N.~H. and {Ohshiro}, Y. and {Nishimura}, S. and {Setoodeh Nia}, K. and {Wakabayashi}, Y. and {Yamaguchi}, H.},
journal = {American Institute of Physics Conference Series},
year = {2010},
month = mar,
pages = {208-214},
volume = {1213},
abstract = {Over the past three years, we have worked on developing a well-characterized $^{30}$S radioactive beam to be used in a future experiment aiming to directly measure to extrapolate the $^{30}$S($\alpha$,p) stellar reaction rate within the Gamow window of Type I X-ray bursts. The importance of the $^{30}$S($\alpha$,p) reaction to X-ray bursts is discussed. Given the astrophysical motivation, the successful results of and challenges involved in the production of a low-energy $^{30}$S beam are detailed. Finally, an overview of our future plans regarding this on-going project are presented.},
adsurl = {http://adsabs.harvard.edu/abs/2010AIPC.1213..208K},
archiveprefix = {arXiv},
doi = {10.1063/1.3362583},
editor = {{C.~Spitaleri, C.~Rolfs, \& R.~G.~Pizzone}},
eprint = {1010.4928},
keywords = {X-ray sources (astronomical), radioactive ion beams, heavy ion-nucleus reactions, counters, X-ray sources; X-ray bursts, Sources of radioactive nuclei, Heavy-particle decay, Gas-filled counters: ionization chambers, proportional, and avalanche counters},
owner = {daid},
primaryclass = {nucl-ex},
series = {American Institute of Physics Conference Series},
timestamp = {2012.04.18}
}

@article{2010NuPhA.834..647K,
title = {{Nuclear Clusters in Astrophysics}},
author = {{Kubono}, S. and {Binh}, D.~N. and {Hayakawa}, S. and {Hashimoto}, H. and {Kahl}, D. and {Wakabayashi}, Y. and {Yamaguchi}, H. and {Teranishi}, T. and {Iwasa}, N. and {Komatsubara}, T. and {Kato}, S. and {Khiem}, L.~H. },
journal = {Nuclear Physics A},
year = {2010},
month = mar,
pages = {647-650},
volume = {834},
abstract = {The role of nuclear clustering is discussed for nucleosynthesis in stellar evolution with Cluster Nucleosynthesis Diagram (CND) proposed before. Special emphasis is placed on $\alpha$-induced stellar reactions together with molecular states for O and C burning.},
adsurl = {http://adsabs.harvard.edu/abs/2010NuPhA.834..647K},
doi = {10.1016/j.nuclphysa.2010.01.113}
}

@article{2010AIPC.1224..475K,
title = {{Nuclear Astrophysics Programs with Low-Energy RI Beams at CRIB}},
author = {{Kubono}, S. and {Binh}, D.~N. and {Hayakawa}, S. and {Hashimoto}, T. and {Kahl}, D.~M. and {Yamaguchi}, H. and {Wakabayashi}, Y. and {Teranishi}, T. and {Iwasa}, N. and {Komatsubara}, T. and {Kato}, S. and {Khiem}, L.~H.},
journal = {American Institute of Physics Conference Series},
year = {2010},
month = apr,
pages = {475-481},
volume = {1224},
abstract = {Nuclear astrophysics activities with CNS RI beam separator (CRIB) are reported together with the present status of the CRIB facility which is supported by the AVF upgrade project for the total development of the low-energy RIB facility. The activities include direct and indirect measurements of stellar reactions especially relevant to explosive burning processes such as nova and supernovae. Some recent results are discussed together with a scope of the facility.},
adsurl = {http://adsabs.harvard.edu/abs/2010AIPC.1224..475K},
doi = {10.1063/1.3431454},
editor = {{Y.~E.~Penionzhkevich \& S.~M.~Lukyanov}},
keywords = {radioactive ion beams, nucleosynthesis, cyclotrons, heavy ion-nucleus reactions, Reaccelerated radioactive beams, Weak interaction and neutrino induced processes, galactic radioactivity, Cyclotrons, Hard scattering in relativistic heavy ion collisions},
owner = {daid},
series = {American Institute of Physics Conference Series},
timestamp = {2012.04.18}
}

@article{2010AIPC.1269..262Y,
title = {{Studies of alpha-induced astrophysical reactions at CRIB}},
author = {{Yamaguchi}, H. and {Hashimoto}, T. and {Hayakawa}, S. and {Binh}, D.~N. and {Kahl}, D. and {Kubono}, S.},
journal = {American Institute of Physics Conference Series},
year = {2010},
month = aug,
pages = {262-267},
volume = {1269},
abstract = {CRIB (CNS Radioactive Ion Beam separator ) is a low-energy RI beam separator at the Center for Nuclear Study (CNS) of the University of Tokyo. Using the RI beams at CRIB, many measurements on proton alpha resonance scatterings, ($\alpha$,p) reactions, and others were performed in recent years mainly for studying astrophysical reactions and exotic nuclear structure. Among them, the results on the $^{7}$Li+$\alpha$ resonance scatterings are presented.},
adsurl = {http://adsabs.harvard.edu/abs/2010AIPC.1269..262Y},
doi = {10.1063/1.3485145},
editor = {{I.~Tanihara, H.~J.~Ong, A.~Tamii, T.~Kishimoto, T.~Kajino, S.~Kubono, \& T.~Shima}},
keywords = {radioactive ion beams, nuclear resonance reactions, quadrupole moments, atomic collisions, Radioactive wastes, waste disposal, Other resonances, Electromagnetic moments, Elastic and inelastic scattering},
owner = {daid},
series = {American Institute of Physics Conference Series},
timestamp = {2012.04.18}
}

@article{2010AIPC.1235..247Y,
title = {{Nuclear Astrophysics and Structure Studies Using Low-energy RI Beams at CRIB}},
author = {{Yamaguchi}, H. and {Hashimoto}, T. and {Hayakawa}, S. and {Binh}, D.~N. and {Kahl}, D. and {Kubono}, S.},
journal = {American Institute of Physics Conference Series},
year = {2010},
month = may,
pages = {247-252},
volume = {1235},
abstract = {CRIB (CNS Radioactive Ion Beam separator) is a low-energy RI beam separator at the Center for Nuclear Study (CNS) of the University of Tokyo. Using the RI beams at CRIB, Many measurements on proton and alpha resonance scatterings, ($\alpha$,p) reactions, and others were peformed in recent years, mainly for studying astrophysical reactions and exotic nuclear structure. Among them, the results on the $^{7}$Be+p and $^{7}$Li+$\alpha$ resonance scatterings are presented.},
adsurl = {http://adsabs.harvard.edu/abs/2010AIPC.1235..247Y},
doi = {10.1063/1.3442603},
keywords = {nuclear structure, separation, proton scattering, alpha particle-nucleus reactions, neutrinos, Collective levels, Isotope separation and enrichment, Elastic proton scattering, Elastic and inelastic scattering, Neutrino scattering},
owner = {daid},
series = {American Institute of Physics Conference Series},
timestamp = {2012.04.18}
}

@article{2010nuco.confE.214Y,
title = {{Alpha-induced astrophysical reactions studied at CRIB}},
author = {{Yamaguchi}, H. and {Hashimoto}, T. and {Hayakawa}, S. and {Dam Nguyen}, B. and {Kahl}, D. and {Kubono}, S.},
journal = {Proceedings of Science},
year = {2010},
pages = {214:1-6},
volume = {NIC-XI},
abstract = {CRIB (CNS Radioactive Ion Beam separator) is a low-energy RI beam separator at the Center for Nuclear Study (CNS) of the University of Tokyo. Studies on proton and alpha resonance scatterings, ($\alpha$,\,p) reactions, and other types of measurements ( $\beta$-decay lifetimes etc.) have been performed using RI beams at CRIB, motivated by interests on astrophysical reactions and exotic nuclear structure. Among the studies at CRIB, the measurement of $^{7}$Li+$\alpha$ resonant scattering is presented.},
adsurl = {http://adsabs.harvard.edu/abs/2010nuco.confE.214Y},
owner = {daid},
timestamp = {2013.05.08},
url = {http://pos.sissa.it/archive/conferences/100/214/NIC%20XI_214.pdf}
}

@article{2009AIPC.1120..189Y,
title = {{Nuclear Astrophysical studies using low-energy RI beams at CRIB}},
author = {{Yamaguchi}, H. and {Wakabayashi}, Y. and {Hayakawa}, S. and {Binh}, D.~N. and {Kahl}, D. and {Kurihara}, Y. and {Kubono}, S. and {Teranishi}, T. and {He}, J.~J. and {Kwon}, Y.~K. and {Nishimura}, S. and {Togano}, Y. and {Iwasa}, N. and {Niikura}, M. and {Khiem}, L.~H.},
journal = {American Institute of Physics Conference Series},
year = {2009},
month = may,
pages = {189-193},
volume = {1120},
abstract = {CRIB (CNS Radioactive Ion Beam separator) is a low-energy RI beam separator at the Center for Nuclear Study (CNS) of the University of Tokyo, used for various studies covering nuclear-astrophysical topics. An application of the RI beam at CRIB for the astrophysical studies is a new measurement of the proton resonance scattering on $^{7}$Be. The measurement was performed up to the excitation energy of 6.8 MeV, ans the excitation function above 3.5 MeV was successfully measured for the first time, providing important information about the reaction rate of $^{7}$Be(p,$\gamma$)$^{8}$B, which is the key reaction in the solar $^{8}$B neutrino production. A preliminary result of the $^{7}$Be+p experiment is presented.},
adsurl = {http://adsabs.harvard.edu/abs/2009AIPC.1120..189Y},
doi = {10.1063/1.3141645},
keywords = {Solar neutrinos, Low and intermediate energy heavy-ion reactions, Cyclotrons, Gas-filled counters: ionization chambers, proportional, and avalanche counters, Astronomical and space-research instrumentation},
owner = {daid},
timestamp = {2012.04.18}
}

@article{2008nuco.confE.153C,
title = {{Study of astrophysically important states in $^{26}$Si with the p($^{25}$Al,p)$^{25}$Al elastic scattering}},
author = {{Chen}, J. and {Chen}, A.~A. and {Amadio}, G. and {Bazin}, D. and {Becerril Reyes}, A.~D. and {Amthor}, A.~M. and {Cherubini}, S. and {Galaviz Redondo}, D. and {Gade}, A. and {Glasmacher}, T. and {Fujikawa}, H. and {Iwasa}, N. and {He}, J.~J. and {Hayakawa}, S. and {Kahl}, D. and {Khiem}, L.~H. and {Kubono}, S. and {Kurihara}, Y. and {Kwon}, Y.~K. and {Lorusso}, G. and {Matos}, M. and {Moon}, J.~Y. and {Niikura}, M. and {Nishimura}, S. and {Odahara}, A. and {Ouellet}, C.~V. and {Pearson}, J. and {Pereira}, J. and {Pizzone}, R.~G. and {Sidoti}, A. and {Schatz}, H. and {Smith}, K. and {Teranishi}, T. and {Togano}, Y. and {Wales}, B. and {Wakabayashi}, Y. and {Yamaguchi}, Y. and {Zegers}, R. },
journal = {Proceedings of Science},
year = {2008},
pages = {153:1-5},
volume = {NIC X},
abstract = {The radioisotope $^{26}$Al is an important probe of the interstellar medium of our galaxy, but its production is now still not well determined partially due to the lack of knowledge of the important states in $^{26}$Si, which dominate the large uncertainty in the $^{25}$Al(p,$\gamma$)$^{26}$Si reaction rate at nova temperatures. We give an update on two experiments that were performed to study these states. One is a measurement of the $^{27}$Si(p,d)$^{26}$Si$^{*}$ reaction at the NSCL, and the other one is a measurement of the $^{25}$Al+p elastic scattering with the CRIB facility at RIKEN.},
adsurl = {http://adsabs.harvard.edu/abs/2008nuco.confE.153C},
owner = {daid},
timestamp = {2012.04.18},
url = {http://pos.sissa.it/archive/conferences/053/153/NIC\%20X_153.pdf}
}

@article{2008nuco.confE.171K,
title = {{Astrophysical (alpha,p) cross section technique and $^{30}$S RIB Development}},
author = {{Kahl}, D. and {Chen}, A.~A. and {Binh}, D.~N. and {Chen}, J. and {Hashimoto}, T. and {Hayakawa}, S. and {Kim}, A. and {Kubono}, S. and {Kurihara}, Y. and {Lee}, N.~H. and {Michimasa}, S. and {Nishimura}, S. and {Ouellet}, C.~V. and {Setoodehnia}, K. and {Wakabayashi}, Y. and {Yamaguchi}, H.},
journal = {Proceedings of Science},
year = {2008},
pages = {171:1-5},
volume = {NIC X},
abstract = {The present work reports the results of $^{30}$S radioactive beam development for a future experiment directly measuring data to extrapolate the $^{30}$S($\alpha$,p) stellar reaction rate in Type I X-ray bursts, a phenomena where nuclear explosions occur repeatedly on the surface of accreting neutron stars. We produce the radioactive ion $^{30}$S via the $^{3}$He($^{28}$Si,$^{30}$S)n reaction, by bombarding a cryogenically cooled target of $^{3}$He at 400 Torr and 80 K with $^{28}$Si beams of 6.9 and 7.54 MeV/u. In order to perform a successful future experiment which allows us to calculate the stellar $^{30}$S($\alpha$,p) reaction rate, Hauser-Feshbach calculations indicate we require a $^{30}$S beam of $\sim 10^{5}$ particles per second (pps) at $\sim$ 32 MeV. Based on our recent beam development experiments in 2006 and 2008, it is believed that such a beam may be fabricated in 2009 according to the results presented. We plan to measure the $^{4}$He($^{30}$S,p) cross-section at astrophysical energies in 2009, and some brief remarks on the planned ($\alpha$,p) technique are also elucidated.},
adsurl = {http://adsabs.harvard.edu/abs/2008nuco.confE.171K},
archiveprefix = {arXiv},
booktitle = {Nuclei in the Cosmos (NIC X)},
eprint = {0904.2067},
owner = {daid},
timestamp = {2012.04.18},
url = {http://pos.sissa.it/archive/conferences/053/171/NIC\%20X_171.pdf}
}

@article{2008ASPC..393..219K,
title = {{Radioactive $^{30}$S Beam to Study X-Ray Bursts}},
author = {{Kahl}, D. and {Chen}, A.~A. and {Chen}, J. and {Hayakawa}, S. and {Kim}, A. and {Kubono}, S. and {Michimasa}, S. and {Setoodehnia}, K. and {Wakabayashi}, Y. and {Yamaguchi}, H.},
journal = {Astronomical Society of the Pacific Conference Series},
year = {2008},
month = aug,
pages = {219-222},
volume = {393},
abstract = {The understanding of energy generation in Type I X-ray bursts will be enhanced by a direct measurement of the nuclear reaction cross section $^{30}$S($\alpha$,p)$^{33}$Cl. Models of this explosive stellar nucleosynthesis are constrained by the observations of bursts with multiple peaks in their bolometric luminosity. A recent model by Fisker, Thielemann, & Wiescher (2004) gives a theoretical basis for a nuclear waiting point at $^{30}$S in order to explain these observations. In order to experimentally test the predictions of this model, the authors undertook two days of $^{30}$S radioactive ion beam (RIB) development in December 2006 in preparation for a 2008 experiment directly measuring the $\alpha$($^{30}$S,p) cross section.},
adsurl = {http://adsabs.harvard.edu/abs/2008ASPC..393..219K},
booktitle = {New Horizons in Astronomy},
editor = {{A.~Frebel, J.~R.~Maund, J.~Shen, \& M.~H.~Siegel}},
owner = {daid},
timestamp = {2012.04.18},
url = {http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008ASPC..393..219K&link_type=ARTICLE&db_key=AST}
}

@article{2006EPJA...27S.327K,
title = {{Nuclear astrophysics at the east drip line}},
author = {{Kubono}, S. and {Teranishi}, T. and {Notani}, M. and {Yamaguchi}, H. and {Saito}, A. and {He}, J.~J. and {Wakabayashi}, Y. and {Fujikawa}, H. and {Amadio}, G. and {Baba}, H. and {Fukuchi}, T. and {Shimoura}, S. and {Michimasa}, S. and {Nishimura}, S. and {Nishimura}, M. and {Gono}, Y. and {Odahara}, A. and {Kato}, S. and {Moon}, J.~Y. and {Lee}, J.~H. and {Kwon}, Y.~K. and {Lee}, C.~S. and {Hahn}, K.~I. and {F{\"u}l{\"o}p}, Z. and {Guimar Aes}, V. and {Lichtenthaler}, R.
},
journal = {European Physical Journal A},
year = {2006},
month = mar,
pages = {327-332},
volume = {27},
abstract = {{In the first half of the paper, the nuclear astrophysics activities in Japan, especially in experimental studies are briefly overviewed. A variety of beams have been developed and used for nuclear astrophysics experiments in Japan. The activities include the RI beam facilities at low energies by the in-flight method at the Center for Nuclear Study (CNS), University of Tokyo and by the ISOL-based method at the JAERI tandem facility, and the RI beam facility at intermediate energies at RIKEN. Other activities include a study of the $^{12}$C({$\alpha$},{$\gamma$})$^{16}$O reaction exclusively at the tandem accelerator at the Kyushu University, and studies at the neutron facility at Tokyo Institute of Technology and at the photon facility at AIST (Sanso-ken). Research opportunities in the future at RIBF, J-PARC, and SPRING8 are also discussed. A discussion on the research activities at CNS has been specifically extended in the latter half, including various possibilities in collaboration at the RI beam factory at RIKEN. }},
adsurl = {http://adsabs.harvard.edu/abs/2006EPJA...27S.327K},
doi = {10.1140/epja/i2006-08-050-5},
keywords = {25.70.Ef Resonances, 25.60.-t Reactions induced by unstable nuclei, 26.30.+k Nucleosynthesis in novae, supernovae and other explosive environments, 29.25.Rm Sources of radioactive nuclei}
}

@article{2003NuPhA.718..207T,
title = {{Experimental studies using a low-energy RI beam separator at CNS}},
author = {{Teranishi}, T. and {Kubono}, S. and {Shimoura}, S. and {Notani}, M. and {Yanagisawa}, Y. and {Michimasa}, S. and {Ue}, K. and {Iwasaki}, H. and {Kurokawa}, M. and {Satou}, Y. and {Morikawa}, T. and {Saito}, A. and {Baba}, H. and {Lee}, J.~H. and {Lee}, C.~S. and {F{\"u}l{\"o}p}, Z. and {Kato}, S.},
journal = {Nuclear Physics A},
year = {2003},
month = may,
pages = {207-213},
volume = {718},
abstract = {{Radioactive-ion (RI) beams of $^{10}$C, $^{14}$O, $^{12N}$ and $^{11}$C with energies low 10 A MeV were produced by using a low-energy in-flight RI beam separator newly constructed by CNS, University of Tokyo. Using the $^{12}$N and $^{11}$C beams, some resonance states were identified in the proton elastic scattering $^{12}$N+p and $^{11}$C+p, respectively. }},
adsurl = {http://adsabs.harvard.edu/abs/2003NuPhA.718..207T},
doi = {10.1016/S0375-9474(03)00716-4}
}

@article{2011APS..DNP.FG005J,
title = {{Measurement of $^{26}$Si+p resonant elastic scattering for studying the $^{26}$Si(p,{$\gamma$})$^{27}$P reaction}},
author = {{Jung}, H.~S. and {Kwon}, Y.~K. and {Moon}, J.~Y. and {Lee}, J.~H. and {Yun}, C.~C. and {Lee}, C.~S. and {Choi}, S. and {Kim}, M.~J. and {Kim}, Y.~H. and {Kim}, Y.~K. and {Park}, J.~S. and {Kim}, E.~J. and {Moon}, C.~B. and {Kubono}, S. and {Yamaguchi}, H. and {Kahl}, D. and {Teranishi}, T. and {Wakabayshi}, Y. and {Iwasa}, N. and {Togano}, Y. and {Cherubini}, S.},
journal = {APS Division of Nuclear Physics Meeting Abstracts},
year = {2011},
month = oct,
pages = {F5},
abstract = {Proton resonant states in $^{27}$P have been studied by the resonant elastic scattering of $^{26}$Si+p with a $^{26}$Si radioactive ion beam at 3.039 MeV/u bombarding a thick H2 gas target with the inverse kinematics method at the low-energy RI beam facility CRIB at CNS, University of Tokyo. The properties of these resonance states are important to better determine the production rates of $^{26}$Si(p,$\gamma$)$^{27}$P reaction which is one of the atrophysically important reactions to understand the production of the ground state of $^{26}$Al under the explosive stellar environments at higher temperature. In this work, some new states have been observed with a high statistics and background free through a covered the range of excitation energies from Ex = 2.3 to 3.8 MeV. The resonant parameters of those states, were determined by an R-matrix analysis of the excitation functions.},
adsurl = {http://adsabs.harvard.edu/abs/2011APS..DNP.FG005J},
url = {http://meeting.aps.org/Meeting/DNP11/Event/150795}
}

@article{2009APS..HAW.LG004B,
title = {{Direct Measurement of $^{21}$Na+{$\alpha$} Stellar Reaction}},
author = {{Binh Dam}, N. and {Yamaguchi}, H. and {Wakabayashi}, Y. and {Hayakawa}, S. and {Hashimoto}, T. and {Kahl}, D. and {Kubono}, S. and {Le}, H.~K. and {Nguyen}, T.~T. and {Iwasa}, N. and {Kume}, N. and {Kato}, S. and {Teranishi}, T.},
journal = {APS Meeting Abstracts},
year = {2009},
month = oct,
pages = {L4},
abstract = {Nucleosynthesis of $^{22}$Na is an interesting subject because of possible {$\gamma$}-ray observation and isotopic anomalies in presolar grain. $^{22}$Na would have been mainly produced in the NeNa cycle. At high temperature conditions, $^{21}$Na({$\alpha$},p)$^{24}$Mg reaction could play a significant role to make flow from the NeNa cycle to the next MgAl cycle and beyond. Clearly, the $^{21}$Na({$\alpha$},p)$^{24}$Mg stellar reaction would bypass $^{22}$Na, resulting in reduction of $^{22}$Na production, therefore, it is strongly coupled to the Ne-E problem. It could be also important to understand the early stage of the rp-process. Experiment was performed using a 39 MeV $^{21}$Na radioactive beam obtained by the CNS Radio Isotope Beam separator CRIB of the University of Tokyo. Both protons and alphas were measured from {$\alpha$}+$^{21}$Na scattering with a thick $^{4}$He gas target.},
adsurl = {http://adsabs.harvard.edu/abs/2009APS..HAW.LG004B},
owner = {daid},
timestamp = {2012.04.18},
url = {http://meetings.aps.org/link/BAPS.2009.HAW.LG.4}
}

@article{2009APS..HAW.BG002H,
title = {{Study of the $^{14}$O + {$\alpha$} reaction at low energy}},
author = {{Hashimoto}, T. and {Kubono}, S. and {Yamaguchi}, H. and {Hayakawa}, S. and {Dam}, N.~B. and {Kahl}, D. and {Kawabata}, T. and {Wakabayashi}, Y. and {Lee}, N.~H. and {Kim}, A. and {Han}, M.~H. and {Yoo}, J.~S. and {Hahn}, K.~I. and {Kwon}, Y.~K. and {Lee}, C.~S. and {Teranishi}, T. and {Kato}, S. and {Komatsubara}, T. and {Wang}, B.~X. and {Guo}, B. and {Bing}, G. and {Wang}, Y.~B. and {Liu}, W.~P.},
journal = {APS Meeting Abstracts},
year = {2009},
month = oct,
pages = {B2},
abstract = {The $^{14}$O($\alpha$, p)$^{17}$F stellar reaction is one of the key reactions for the breakout from the Hot--CNO cycle to the rp--process. Since the cross sections depends on the product of $\alpha$ and proton widths of the intermediate states in $^{18}$Ne, it is important to determine these widths. We performed an experiment of the $^{14}$O + $\alpha$ scattering with a thick target method at the CNS Radioactive Ion Beam (CRIB) facility. The experiment was carried out using a thick Helium gas target and position sensitive silicon telescopes. This measurement provides an excitation function of $^{14}$O + $\alpha$ scattering for an energy range of E$_{cm}$ = 1.7 -- 5.9 MeV. We will concentrate on the elastic scattering channel in this presentation, since the $\alpha$-cluster structure in $^{18}$Ne above the $\alpha$--threshold would play an important role for the stellar reaction. Several $\alpha$--resonances were observed in the present experiment. The experimental result will be presented, and the $\alpha$ cluster structure in $^{18}$Ne and the significance to the stellar reaction will be discussed.},
adsurl = {http://adsabs.harvard.edu/abs/2009APS..HAW.BG002H},
owner = {daid},
timestamp = {2012.04.18},
url = {http://meetings.aps.org/link/BAPS.2009.HAW.BG.2}
}

@article{2009APS..HAW.LG006H,
title = {{Direct Measurement of the $^{11}$C($\alpha$,p)$^{14}$N Reaction}},
author = {{Hayakawa}, S. and {Kubono}, S. and {Yamaguchi}, H. and {Hashimoto}, T. and {Binh}, D.~N. and {Kahl}, D. and {Wakabayashi}, Y. and {Iwasa}, N. and {Kume}, N. and {Miura}, Y. and {Teranishi}, T. and {He}, J.~J. and {Kwon}, Y.~K. and {Komatsubara}, T. and {Kato}, S. and {Wanajo}, S. },
journal = {APS Meeting Abstracts},
year = {2009},
month = oct,
pages = {L6},
abstract = {A recent simulation of the rp-process in neutrino-driven winds in type II supernovae ($\nu$p-process) suggests that the $^{11}$C($\alpha$,p)$^{14}$N reaction could be an important breakout pass from the pp-chain region to the CNO region. However, there are only very limited experimental information of the reaction cross section available from the time-reverse reaction studies. In order to determine the reaction rate of $^{11}$C($\alpha$,p)$^{14}$N, a direct measurement by means of the thick-target inverse-kinematics method has recently been performed using low-energy $^{11}$C beams from the CNS Radioactive Ion Beam (CRIB) separator, a $^{4}$He gas target and $\delta$E-E position-sensitive silicon telescopes at three downstream angles. The experiment covered E$_{CM}$ = 0.5--5 MeV corresponding to the stellar temperature of 1.5--7 GK. The obtained reaction cross section including some resonances and transitions to the excited states of $^{14}$N will be reported.},
adsurl = {http://adsabs.harvard.edu/abs/2009APS..HAW.LG006H},
owner = {daid},
timestamp = {2012.04.18},
url = {http://meetings.aps.org/link/BAPS.2009.HAW.LG.6}
}

@article{2009APS..HAW.KG003W,
title = {{Beta-decay measurement of $^{46}$Cr}},
author = {{Wakabayashi}, Y. and {Yamaguchi}, H. and {Hashimoto}, T. and {Hayakawa}, S. and {Kurihara}, Y. and {Binh}, D.~N. and {Kahl}, D. and {Kubono}, S. and {Nishimura}, S. and {Gono}, Y. and {Suga}, M. and {Fujita}, Y.},
journal = {APS Meeting Abstracts},
year = {2009},
month = oct,
pages = {K3},
abstract = {For the rapid proton capture process (rp-process) in X-ray bursts and the core-collapse stage of supernovae, proton-rich pf-shell nuclei far from the line of stability play important roles. Studies of the feeding ratios and half-lives of the $\beta$ and electron capture decays of these proton-rich pf-shell nuclei are of great astrophysical interest not only for nucleo synthesis but also for Fermi and Gamow-Teller transition study. The experiment to measure the half life of $\beta$ decay of $^{46}$Cr was performed using the low-energy RI beam separator (CRIB) of the Center for Nuclear Study (CNS), University of Tokyo. The $^{46}$Cr particles were produced by the $^{36}$Ar + $^{12}$C fusion reaction. A natural C foil of 0.56 mg/cm$^{2}$ was installed as the primary target. The $^{36}$Ar primary beam was accelerated up to 3.6 MeV/nucleon by the RIKEN AVF cyclotron. A double sided Si strip detector (DSSD) of 500-$\mu$m thickness was used as a $\beta$-ray detector. A Si detector of 1.5-mm thickness was placed just behind the DSSD for a $\beta$-ray detector. To measure $\beta$-delayed $\gamma$ rays, 3 clover and 1 coaxial Ge detectors were set around the target chamber. The beam was pulsed to measure the half life of the $\beta$ decay of $^{46}$Cr. The $\beta$-delayed $\gamma$ ray of $^{46}$Cr was observed in this experiment. The experimental result will be discussed.},
adsurl = {http://adsabs.harvard.edu/abs/2009APS..HAW.KG003W},
owner = {daid},
timestamp = {2013.05.08},
url = {http://meetings.aps.org/link/BAPS.2009.HAW.KG.3}
}

@article{2010.CNS.Hashimoto,
title = {Present status of the direct measurement of the $^{18}$Ne($\alpha$,\,p) reaction cross section using the GEM-MSTPC},
author = {{Hashimoto}, T. and {Kubono}, S. and {Yamaguchi}, H. and {Hayakawa}, S. and {Kahl}, D. and {Ota}, S. and {Michimasa}, S. and {Tokieda}, H. and {Yamaguchi}, K. and {Arai}, I. and {Komatsubara}, T. and {Ishiyama}, H. and {Watanabe}, Y.~X. and {Miyatake}, H. and {Hirayama}, Y. and {Imai}, N. and {Jeong}, S.~C. and {Mizoi}, Y. and {Das}, S.~K. and {Fukuda}, T. and {Makii}, H. and {Wakabayashi}, Y. and {Iwasa}, N. and {Yamada}, T. and {Chen}, A.~A. and {He}, J.~J.},
journal = {Center for Nuclear Study Annual Report 2010},
year = {2012},
pages = {3-4},
volume = {CNS-REP-88},
owner = {daid},
timestamp = {2012.04.17},
url = {http://www.cns.s.u-tokyo.ac.jp/archive/annual/ann10.pdf}
}

@article{2010.CNS.Ota,
title = {CNS Active Target Development and Test Experiment at HIMAC},
author = {{Ota}, S. and {Michimasa}, S. and {Gunji}, T. and {Yamaguchi}, H. and {Tokieda}, H. and {Hashimoto}, T. and {Akimoto}, R. and {Kahl}, D. and {Dozono}, M. and {Hayakawa}, S. and {Kawase}, S. and {Kikuchi}, Y. and {Maeda}, Y. and {Matsubara}, H. and {Otsu}, H. and {Kubono}, S. and {Hamagaki}, H and {Uesaka}, T. },
journal = {Center for Nuclear Study Annual Report 2010},
year = {2012},
pages = {46-47},
volume = {CNS-REP-88},
owner = {daid},
timestamp = {2012.04.17},
url = {http://www.cns.s.u-tokyo.ac.jp/archive/annual/ann10.pdf}
}

@article{2010.CNS.Yamaguchi,
title = {Excitation functions of $^{7}$Be+$\alpha$ elastic and inelastic scattering cross sections},
author = {{Yamaguchi}, H. and {Hashimoto}, T. and {Hayakawa}, S. and {Binh}, D.~N. and {Kahl}, D. and {Kubono}, S. and {Kawabata}, T. and {Teranishi}, T. and {Wakabayashi}, Y. and {Iwasa}, N. and {Miura}, Y. and {Kwon}, Y.~K. and {Khiem}, L.~H. and {Duy}, N.~N.},
journal = {Center for Nuclear Study Annual Report 2010},
year = {2012},
pages = {1-2},
volume = {CNS-REP-88},
owner = {daid},
timestamp = {2012.04.17},
url = {http://www.cns.s.u-tokyo.ac.jp/archive/annual/ann10.pdf}
}

@article{2009.CNS.Binh,
title = {Multichannel R-matrix analysis for an alpha scattering in inverse kinematics using a $^{21}$Na radioisotope beam},
author = {{Binh}, D.~N. and {Khiem}, L.~H. and {Tho}, N.~T. and {Kubono}, S. and {Yamaguchi}, H. and {Wakabayashi}, Y. and {Hayakawa}, S. and {Kahl}, D. and {Hashimoto}, T. and {Teranishi}, T. and {Kato}, S. and {Iwasa}, N.},
journal = {Center for Nuclear Study Annual Report 2009},
year = {2011},
pages = {5-6},
volume = {CNS-REP-86},
owner = {daid},
timestamp = {2011.02.02},
url = {http://www.cns.s.u-tokyo.ac.jp/archive/annual/ann09.pdf}
}

@article{2009.CNS.Hashimoto,
title = {Present status of the direct measurement of the $^{18}$Ne($\alpha$,\,p) reaction cross section using the GEM-MSTPC},
author = {{Hashimoto}, T. and {Kubono}, S. and {Yamaguchi}, H. and {Hayakawa}, S. and {Kahl}, D. and {Ota}, S. and {Michimasa}, S. and {Tokieda}, H. and {Yamaguchi}, K. and {Arai}, I. and {Komatsubara}, T. and {Ishiyama}, H. and {Watanabe}, Y.~X. and {Miyatake}, H. and {Hirayama}, Y. and {Imai}, N. and {Jeong}, S.~C. and {Mizoi}, Y. and {Das}, S.~K. and {Fukuda}, T. and {Makii}, H. and {Wakabayashi}, Y. and {Iwasa}, N. and {Yamada}, T. and {Chen}, A.~A. and {He}, J.~J.},
journal = {Center for Nuclear Study Annual Report 2009},
year = {2011},
pages = {9-10},
volume = {CNS-REP-86},
owner = {daid},
timestamp = {2011.02.02},
url = {http://www.cns.s.u-tokyo.ac.jp/archive/annual/ann09.pdf}
}

@article{2009.CNS.Seiya,
title = {First direct measurement of the $^{11}$C($\alpha$,p)$^{14}$N stellar reaction},
author = {{Hayakawa}, S. and {Kubono}, S. and {Hashimoto}, T. and {Yamaguchi}, H. and {Binh}, D.~N. and {Kahl}, D. and {Wakabayashi}, Y. and {Iwasa}, N. and {Kume}, N. and {Miura}, I. and {Teranishi}, T. and {He}, J.~J. and {Kwon}, Y.~K. and {Komatsubara}, T. and {Kato}, S. and {Wanajo}, S.},
journal = {Center for Nuclear Study Annual Report 2009},
year = {2011},
pages = {7-8},
volume = {CNS-REP-86},
owner = {daid},
timestamp = {2011.02.02},
url = {http://www.cns.s.u-tokyo.ac.jp/archive/annual/ann09.pdf}
}

@article{CNS.2009.daid,
title = {$^{30}$S Beam Production and RI Beam Modeling at CRIB},
author = {{Kahl}, D and {Chen}, A.~A. and {Kubono}, S. and {Binh}, D.~N. and {Chen}, J. and {Hashimoto}, T. and {Hayakawa}, S. and {Iwasa}, N. and {Kaji}, D. and {Kim}, A. and {Kurihara}, Y. and {Lee}, N.~H. and {Mazzocco}, M. and {Nishimura}, S. and {Ohshiro}, Y. and {Setoodehnia}, K. and {Wakabayashi}, Y. and {Yamaguchi}, H.},
journal = {Center for Nuclear Study Annual Report 2009},
year = {2011},
pages = {11-12},
volume = {CNS-REP-86},
owner = {daid},
timestamp = {2011.02.02},
url = {http://www.cns.s.u-tokyo.ac.jp/archive/annual/ann09.pdf}
}

@article{2009.CNS.Guo,
title = {Indirect measurement of astrophysical $^{12}$N(p,\,$\gamma$)$^{13}$O reaction rate},
author = {{Liu}, W.~P. and {Guo}, B. and {Su}, J. and {Li}, Z.~H. and {Binh}, D.~N. and {Han}, Y.~L. and {Hashimoto}, T. and {Hayakawa}, S. and {He}, J.~J. and {Hu}, J. and {Iwasa}, N. and {Kahl}, D.~M. and {Kubono}, S. and {Kume}, N. and {Li}, Y.~J. and {Li}, Z.~H. and {Wang}, Y.~B. and {Xu}, S.~W. and {Yamaguchi}, H. and {Yan}, S.~Q. and {Bai}, X.~X. and {Lian}, G. and {Wang}, B.~X. and {Zeng}, S.},
journal = {Center for Nuclear Study Annual Report 2009},
year = {2011},
pages = {15-16},
volume = {CNS-REP-86},
owner = {daid},
timestamp = {2011.02.02},
url = {http://www.cns.s.u-tokyo.ac.jp/archive/annual/ann09.pdf}
}

@article{2009.CNS.Ota,
title = {New Intergroup Collaboration for Development of GEM-TPC Active Target},
author = {{Ota}, S. and {Michimasa}, S. and {Gunji}, T. and {Yamaguchi}, H. and {Akimoto}, R. and {Hashimoto}, T. and {Kahl}, D. and {Hayakawa}, S. and {Tokieda}, H. and {Kawase}, S. and {Tsuji}, T. and {Kubono}, S. and {Hamagaki}, H and {Uesaka}, T.
},
journal = {Center for Nuclear Study Annual Report 2009},
year = {2011},
pages = {57-58},
volume = {CNS-REP-86},
owner = {daid},
timestamp = {2011.02.02},
url = {http://www.cns.s.u-tokyo.ac.jp/archive/annual/ann09.pdf}
}

@article{2009.CNS.Teranishi,
title = {Test measurement of $^{17}$Ne+p resonance elastic scattering},
author = {{Teranishi}, T. and {Kubono}, S. and {Yamaguchi}, H. and {Hashimoto}, T. and {Hayakawa}, S. and {Kurihara}, Y. and {Binh}, D.~N. and {Kahl}, D. and {Wakabayashi}, Y. and {Khiem}, L.~H. and {Cuong}, P.~V. and {Watanabe}, S. and {Goto}, A.
},
journal = {Center for Nuclear Study Annual Report 2009},
year = {2011},
pages = {17-18},
volume = {CNS-REP-86},
owner = {daid},
timestamp = {2011.02.02},
url = {http://www.cns.s.u-tokyo.ac.jp/archive/annual/ann09.pdf}
}

@article{2009.CNS.Bayashi,
title = {Beta-decay measurement of $^{46}$Cr},
author = {{Wakabayashi}, Y. and {Yamaguchi}, H. and {Hashimoto}, T. and {Hayakawa}, S. and {Kurihara}, Y. and {Binh}, D.~N. and {Kahl}, D. and {Nishimura}, S. and {Gono}, Y. and {Fujita}, Y. and {Kubono}, S.},
journal = {Center for Nuclear Study Annual Report 2009},
year = {2011},
pages = {13-15},
volume = {CNS-REP-86},
owner = {daid},
timestamp = {2011.02.02},
url = {http://www.cns.s.u-tokyo.ac.jp/archive/annual/ann09.pdf}
}

@article{2009.CNS.Yamaguchi,
title = {Measurement of alpha resonance scattering on $^{7}$Be},
author = {{Yamaguchi}, H. and {Hashimoto}, T. and {Hayakawa}, S. and {Binh}, D.~N. and {Kahl}, D. and {Kubono}, S. and {Kawabata}, T. and {Wakabayashi}, Y. and {Iwasa}, N. and {Miura}, Y. and {Kwon}, Y.~K. and {Khiem}, L.~H. and {Duy}, N.~N. and {Teranishi}, T.},
journal = {Center for Nuclear Study Annual Report 2009},
year = {2011},
pages = {1-2},
volume = {CNS-REP-86},
owner = {daid},
timestamp = {2011.02.02},
url = {http://www.cns.s.u-tokyo.ac.jp/archive/annual/ann09.pdf}
}

@article{2009.CNS.Yamaguchi2,
title = {R-matrix analysis on the excitation function of $^{7}$Li+$\alpha$ elastic scattering},
author = {{Yamaguchi}, H. and {Hashimoto}, T. and {Hayakawa}, S. and {Binh}, D.~N. and {Kahl}, D. and {Kubono}, S. and {Wakabayashi}, Y. and {Kawabata}, T. and {Teranishi}, T.},
journal = {Center for Nuclear Study Annual Report 2009},
year = {2011},
pages = {3-4},
volume = {CNS-REP-86},
owner = {daid},
timestamp = {2011.02.02},
url = {http://www.cns.s.u-tokyo.ac.jp/archive/annual/ann09.pdf}
}

@article{2008.CNS.Binh,
title = {Alpha Resonant Scattering Measurement Using a $^{21}$Na Radioactive Beam},
author = {{Binh}, D.~N. and {Khiem}, L.~H. and {Tho}, N.~T. and {Kubono}, S. and {Yamaguchi}, H. and {Wakabayashi}, Y. and {Hayakawa}, S. and {Kahl}, D. and {Hashimoto}, T. and {Teranishi}, T. and {Kato}, S. and {Iwasa}, N. and {Kume}, N.},
journal = {Center for Nuclear Study Annual Report 2008},
year = {2010},
pages = {19-20},
volume = {CNS-REP-83},
owner = {daid},
timestamp = {2011.02.02},
url = {http://www.cns.s.u-tokyo.ac.jp/archive/annual/ann08.pdf}
}

@article{2008.CNS.Jun,
title = {Update: study of astrophysically important states in $^{26}$Si using the $^{25}$Al+p elastic scattering with CRIB},
author = {{Chen}, J. and {Chen}, A.~A. and {Kubono}, S. and {Yamaguchi}, H. and {Amadio}, G. and {Cherubini}, S. and {La Cognata}, M. and {Fujikawa}, H. and {Hayakawa}, S. and {Iwasa}, N. and {He}, J.~J. and {Kahl}, D. and {Khiem}, L.~H. and {Kurihara}, Y. and {Kwon}, Y.~K. and {Moon}, J.~Y. and {Niikura}, M. and {Nishimura}, S. and {Odahara}, A. and {Pearson}, J. and {Pizzone}, R. and {Saito}, A. and {Signorini}, C. and {Teranishi}, T. and {Togano}, Y. and {Wakabayashi}, Y.},
journal = {Center for Nuclear Study Annual Report 2008},
year = {2010},
pages = {21-22},
volume = {CNS-REP-83},
owner = {daid},
timestamp = {2011.02.02},
url = {http://www.cns.s.u-tokyo.ac.jp/archive/annual/ann08.pdf}
}

@article{2008.CNS.Seiya,
title = {Practical Designing of the Direct Measurement of the Astrophysical Reaction $^{11}$C($\alpha$,p)$^{14}$N},
author = {{Hayakawa}, S. and {Kubono}, S. and {Hashimoto}, T. and {Yamaguchi}, H. and {Binh}, D.~N. and {Kahl}, D.~M. and {Wakabayashi}, Y. and {Iwasa}, N. and {Kume}, N. and {Miura}, I. and {Teranishi}, T. and {He}, J.~J. and {Kwon}, Y.~K. and {Komatsubara}, T. and {Kato}, S. and {Wanajo}, S.},
journal = {Center for Nuclear Study Annual Report 2008},
year = {2010},
pages = {9-10},
volume = {CNS-REP-83},
owner = {daid},
timestamp = {2011.02.02},
url = {http://www.cns.s.u-tokyo.ac.jp/archive/annual/ann08.pdf}
}

@article{2009.RAPR.daid,
title = {Progress in $^{30}$S Beam Development for a Measurement of $^{4}$He($^{30}$S,\,p)},
author = {{Kahl}, D. and {Chen}, A.~A. and {Kubono}, S. and {Binh}, D.~N. and {Chen}, J. and {Hashimoto}, T. and {Hayakawa}, S. and {Kaji}, D. and {Kim}, A. and {Kurihara}, Y. and {Lee}, N.~H. and {Michimasa}, S. and {Nishimura}, S. and {Ohshiro}, Y. and {Setodeh nia}, K. and {Wakabayashi}, Y. and {Yamaguchi}, H.},
journal = {RIKEN Accelerator Progress Report 2009},
year = {2010},
pages = {30},
volume = {43},
owner = {daid},
timestamp = {2012.04.17},
url = {http://www.nishina.riken.jp/researcher/APR/Document/2009.pdf}
}

@article{2008.CNS.Namee,
title = {Study of the $^{14}$N($\alpha$, $\alpha$)$^{14}$N, $^{14}$N($\alpha$,p)$^{17}$O, and $^{14}$N($\alpha$,d)$^{16}$O reactions using a $^{14}$N beam in the inverse kinematics for astrophysics experiments},
author = {{Lee}, N.~H. and {Kubono}, S. and {Yamaguchi}, H. and {Hashimoto}, T. and {Kawabata}, T. and {Wakabayashi}, Y. and {Hayakawa}, S. and {Kurihara}, Y. and {Dam}, Nugyen Binh and {Kahl}, D.~M. and {Ternanishi}, T. and {Kato}, S. and {Komatsubara}, T. and {Han}, M.~H. and {Kim}, A. and {Yoo}, J.~S. and {Hahn}, K.~I. and {Kwon}, Y.~W. and {Guo}, B. and {Wang}, B. X. and {Wang}, Y. B.},
journal = {Center for Nuclear Study Annual Report 2008},
year = {2010},
pages = {11-12},
volume = {CNS-REP-83},
owner = {daid},
timestamp = {2011.02.02},
url = {http://www.cns.s.u-tokyo.ac.jp/archive/annual/ann08.pdf}
}

@article{2008.CNS.Bayashi,
title = {Beta-decay half life of $^{46}$Cr},
author = {{Wakabayashi}, Y. and {Yamaguchi}, H. and {Hashimoto}, T. and {Hayakawa}, S. and {Kurihara}, Y. and {Binh}, D.~N. and {Kahl}, D. and {Nishimura}, S. and {Gono}, Y. and {Suga}, M. and {Fujita}, Y. and {Kubono}, S.},
journal = {Center for Nuclear Study Annual Report 2008},
year = {2010},
pages = {25-26},
volume = {CNS-REP-83},
owner = {daid},
timestamp = {2011.02.02},
url = {http://www.cns.s.u-tokyo.ac.jp/archive/annual/ann08.pdf}
}

@article{2009.RAPR.yamag,
title = {New measurement of resonance scattering of alpha particles on $^{7}$Li},
author = {{Yamaguchi}, H. and {Hashimoto}, T. and {Binh}, D.~N. and {Kahl}, D. and {Hayakawa}, S. and {Wakabayashi}, Y. and {Kawabata}, T. and {Teranishi}, T.},
journal = {RIKEN Accelerator Progress Report 2009},
year = {2010},
pages = {31},
volume = {43},
owner = {daid},
timestamp = {2012.04.17},
url = {http://www.nishina.riken.jp/researcher/APR/Document/2009.pdf}
}

@article{2008.CNS.Yamaguchi,
title = {New measurement of alpha resonance scattering on $^{7}$Li},
author = {{Yamaguchi}, H. and {Hashimoto}, T. and {Hayakawa}, S. and {Binh}, D.~N. and {Kahl}, D. and {Kubono}, S. and {Wakabayashi}, Y. and {Kawabata}, T. and {Teranishi}, T.},
journal = {Center for Nuclear Study Annual Report 2008},
year = {2010},
pages = {5-6},
volume = {CNS-REP-83},
owner = {daid},
timestamp = {2011.02.02},
url = {http://www.cns.s.u-tokyo.ac.jp/archive/annual/ann08.pdf}
}

@article{2007.CNS.Jun,
title = {Study of Astrophysically Important States in $^{26}$Si through Elastic Scattering with CRIB},
author = {{Chen}, J. and {Chen}, A.~A. and {Kubono}, S. and {Yamaguchi}, H. and {Amadio}, G. and {Cherubini}, S. and {La Cognata}, M. and {Fujikawa}, H. and {Hayakawa}, S. and {Iwasa}, N. and {He}, J.~J. and {Kahl}, D. and {Khiem}, L.~H. and {Kurihara}, Y. and {Kwon}, Y.~K. and {Moon}, J.~Y. and {Niikura}, M. and {Nishimura}, S. and {Odahara}, A. and {Pearson}, J. and {Pizzone}, R. and {Saito}, A. and {Signorini}, C. and {Teranishi}, T. and {Togano}, Y. and {Wakabayashi}, Y.},
journal = {Center for Nuclear Study Annual Report 2007},
year = {2009},
pages = {3-4},
volume = {CNS-REP-80},
owner = {daid},
timestamp = {2011.02.02},
url = {http://www.cns.s.u-tokyo.ac.jp/archive/annual/ann07.pdf}
}

@article{2008.RAPR.Jun,
title = {Study of astrophysically important states in $^{26}$Si via the p($^{25}$Al, p)$^{25}$Al elastic scattering},
author = {{Chen}, J. and {Chen}, A.~A. and {Kubono}, S. and {Yamaguchi}, H. and {Amadio}, G. and {Cherubini}, S. and {La Cognata}, M. and {Fujikawa}, H. and {Hayakawa}, S. and {Iwasa}, N. and {He}, J.~J. and {Kahl}, D. and {Khiem}, L.~H. and {Kurihara}, Y. and {Kwon}, Y.~K. and {Moon}, J.~Y. and {Niikura}, M. and {Nishimura}, S. and {Odahara}, A. and {Pearson}, J. and {Pizzone}, R. and {Saito}, A. and {Signorini}, C. and {Teranishi}, T. and {Togano}, Y. and {Wakabayashi}, Y.},
journal = {RIKEN Accelerator Progress Report 2008},
year = {2009},
pages = {21},
volume = {42},
owner = {daid},
timestamp = {2011.02.02},
url = {http://www.nishina.riken.jp/researcher/APR/Document/2008.pdf}
}

@article{CNS.2007.daid,
title = {$^{30}$S Beam Production with CRIB: Analysis of 2006 Data and Preliminary Experimental Results from 2008},
author = {{Kahl}, D and {Chen}, A.~A. and {Binh}, D.~N. and {Chen}, J. and {Hashimoto}, T. and {Hayakawa}, S. and {Kubono}, S. and {Kurihara}, Y. and {Lee}, N.~H. and {Michimasa}, S. and {Nishimura}, S. and {Ouellet}, C.~V. and {Setoodehnia}, K. and {Wakabayashi}, Y. and {Yamaguchi}, H.},
journal = {Center for Nuclear Study Annual Report 2007},
year = {2009},
pages = {9-10},
volume = {CNS-REP-80},
owner = {daid},
timestamp = {2011.02.02},
url = {http://www.cns.s.u-tokyo.ac.jp/archive/annual/ann07.pdf}
}

@article{2008.RAPR.daid,
title = {$^{30}$S Beam Development with CRIB},
author = {{Kahl}, D. and {Chen}, A.~A. and {Dam}, N.~B. and {Chen}, J. and {Hashimoto}, T. and {Hayakawa}, S. and {Kim}, A. and {Kubono}, S. and {Kurihara}, Y. and {Lee}, N.~H. and {Michimasa}, S. and {Nishimura}, S. and {Ouellet}, C.~V. and {Setodeh nia}, K. and {Wakabayashi}, Y. and {Yamaguchi}, H.},
journal = {RIKEN Accelerator Progress Report 2008},
year = {2009},
pages = {20},
volume = {42},
owner = {daid},
timestamp = {2011.02.02},
url = {http://www.nishina.riken.jp/researcher/APR/Document/2008.pdf}
}

@article{2008.RAPR.Bayashi,
title = {Half life measurement of $^{46}$Cr},
author = {{Wakabayashi}, Y. and {Yamaguchi}, H. and {Hashimoto}, T. and {Hayakawa}, H. and {Kurihara}, Y. and {Nishimura}, S. and {Binh}, D.~N. and {Kahl}, D. and {Suga}, M. and {Gono}, Y. and {Fujita}, Y. and {Kubono}, S.},
journal = {RIKEN Accelerator Progress Report 2008},
year = {2009},
pages = {19},
volume = {42},
owner = {daid},
timestamp = {2011.02.02},
url = {http://www.nishina.riken.jp/researcher/APR/Document/2008.pdf}
}

@article{2006.CNS.Jun,
title = {Study of Astrophysically Important States in $^{26}$Si through Elastic Scattering with CRIB},
author = {{Chen}, J. and {Chen}, A.~A. and {Kubono}, S. and {Yamaguchi}, H. and {Amadio}, G. and {Cherubini}, S. and {La Cognata}, M. and {Fujikawa}, H. and {Hayakawa}, S. and {Iwasa}, N. and {He}, J.~J. and {Kahl}, D. and {Khiem}, L.~H. and {Kurihara}, Y. and {Kwon}, Y.~K. and {Moon}, J.~Y. and {Niikura}, M. and {Nishimura}, S. and {Odahara}, A. and {Pearson}, J. and {Pizzone}, R. and {Saito}, A. and {Signorini}, C. and {Teranishi}, T. and {Togano}, Y. and {Wakabayashi}, Y.},
journal = {Center for Nuclear Study Annual Report 2006},
year = {2007},
pages = {3-4},
volume = {CNS-REP-76},
owner = {daid},
timestamp = {2011.02.02},
url = {http://www.cns.s.u-tokyo.ac.jp/archive/annual/ann06.pdf}
}

@article{2007.CNS.daid,
title = {On the Waiting Point at A=30 in X-ray Bursts: $^{30}$S($\alpha$,p)$^{33}$Cl with CRIB},
author = {{Kahl}, D. and {Chen}, A.~A. and {Chen}, J. and {Hayakawa}, S. and {Kim}, A. and {Kubono}, S. and {Michimasa}, S. and {Setoodehnia}, K. and {Wakabayashi}, Y. and {Yamaguchi}, H.},
journal = {Center for Nuclear Study Annual Report 2006},
year = {2007},
pages = {1-2},
volume = {CNS-REP-76},
owner = {daid},
timestamp = {2011.02.02},
url = {http://www.cns.s.u-tokyo.ac.jp/archive/annual/ann06.pdf}
}

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