CNS Radio Isotope Beam separator (CRIB)
CRIB can produce low energy (<10 MeV/u) radio isotope (RI) beam
from the stable nuclei beam accelerated at an AVF cyclotron (K=70)
by in-flight method.
Using two dipole magnets, produced particles are separated,
and we can obtain various radioisotopes as secondary beams.
A Wien filter, installed downstream of the two dipole magnets,
gives further separation according to the velocity of the beam.
With the latest technology of the heavy-ion source and accelerator,
this facility can provide intense and good-quality RI beams,
which are applicable for various fields of physics research,
especially for the nuclear astrophysics.
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RI Beam Production
The RI beam is produced at the primary target,
usually by a reaction of a stable nuclei beam and
gas of light elements (solid targets such as beryllium are also used).
The primary beam current is typically a few 100 pnA.
The RI beam energy is relatively low (<10 MeV/u),
and typical intensity is 104 to 106 particles per second.
RI beams produced at CRIB until 2007
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primary beam
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secondary beam
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10B
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11C, 12N, 10C
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20Ne
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21Na, 22Mg
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18O
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17N, 18F, 18N
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14N
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14O, 13N
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24Mg
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25Al,26Si
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7Li
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7Be, 8Li
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40Ar
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39Ar
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6Li
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8B
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28Si
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30S
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Separation by Dipoles
CRIB has two dipole magnets, called D1 and D2.
The momentum of the secondary beam is analyzed in D1,
and reaches at the momentum dispersive focal plane, called
F1. At F1, the momentum of the particle is selected (usually &Delta p/p ~ 1%)
by a movable slit.
Then, the beam is focused achromatically at the second focal plane, F2.
Specifications for the dipole section
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Orbit radius
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84-98 cm
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Maximum energy
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110Z2/A MeV
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Maximum magnetic rigidity
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1.1 T m
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Analyzable energy range
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30%
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Solid angle acceptance
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5.6 msr
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| Resolution
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1/850
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Momentum dispersion
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~0
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