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The performance of EXOGAM has been calculated for a Coulomb excitation experiment using a beam
of neutron-rich Ar. This experiment would aim to study the sudden onset of
collectivity for neutron-rich nuclei near the neutron magic number (at least,
on or near the stability line) of N = 28. The neutron-rich Ar isotopes such as 46Ar are
expected to be available
at an intensity level of 107 particles per second in the early stages of SPIRAL since
the noble
gases have favourable diffusion and effusion properties leading to fast and efficient extraction
from the ion source.
Rate calculations show that with the Cube-B arrangement of 4
segmented detectors it would be possible to perform a spectroscopic study of the first few
excited states of these exotic nuclei with the first low intensity beams from SPIRAL.
The detector performance was calculated for 662 keV and 1333 keV, with 0.075c, assuming that the
scattering angle of the Coulomb excited beam was measured using an ancillary detector
to within 3 degrees. Such a measurement is well within the capability of the TIARA array.
For the Cube-B and the complete 90 degree 8-detector ring, the respective
resolutions are 11.4 keV (7.6 keV) at 662 keV and 22.8 keV (14.9 keV) at 1333
keV respectively. Table 1 indicates that the extra 4
detectors in the 8-detector ring compensate for the extra distance from the
target, and hence the same overall efficiency is essentially maintained.
However, the 8-detector ring naturally exhibits less Doppler broadening. Hence,
the complete ring is likely to be the better choice for Coulomb excitation
studies that aim to measure accurately the excitation energies of nuclear
levels.
Next: Beam tracking
Up: Gamma-ray detection
Previous: Doppler correction
Wilton Catford
2000-11-03