TY - JOUR
T1 - Isospin of intermediate mass fragments produced in peripheral, midperipheral, and central collisions from the [Formula Presented] reactions at [Formula Presented] MeV
AU - Larochelle, Y.
AU - Gingras, L.
AU - Ball, G. C.
AU - Beaulieu, L.
AU - Gagné, P.
AU - Hagberg, E.
AU - He, Z. Y.
AU - Horn, D.
AU - Laforest, R.
AU - Roy, R.
AU - St-Pierre, C.
N1 - Copyright:
Copyright 2017 Elsevier B.V., All rights reserved.
PY - 2000
Y1 - 2000
N2 - Isotopic yields of IMF’s produced in the [Formula Presented] reactions at [Formula Presented] MeV are investigated. Analysis of experimental data from the CRL-Laval [Formula Presented] multidetector array focuses on events where at least [Formula Presented] of the charge and momentum were detected for the [Formula Presented] system. Averaged isospin ratios [Formula Presented] for IMF’s with [Formula Presented] and 4 are plotted as a function of emission angle and parallel velocity in the center-of-mass frame. Results from simulations with the statistical codes SMM and GEMINI, assuming an equilibrated source, are compared to the experimental ratios. The ratios seem to indicate the presence of a midrapidity necklike structure that would produce IMF’s richer in neutrons than the two main emitters, even for very central collisions.
AB - Isotopic yields of IMF’s produced in the [Formula Presented] reactions at [Formula Presented] MeV are investigated. Analysis of experimental data from the CRL-Laval [Formula Presented] multidetector array focuses on events where at least [Formula Presented] of the charge and momentum were detected for the [Formula Presented] system. Averaged isospin ratios [Formula Presented] for IMF’s with [Formula Presented] and 4 are plotted as a function of emission angle and parallel velocity in the center-of-mass frame. Results from simulations with the statistical codes SMM and GEMINI, assuming an equilibrated source, are compared to the experimental ratios. The ratios seem to indicate the presence of a midrapidity necklike structure that would produce IMF’s richer in neutrons than the two main emitters, even for very central collisions.
UR - http://www.scopus.com/inward/record.url?scp=85035306709&partnerID=8YFLogxK
U2 - 10.1103/PhysRevC.62.051602
DO - 10.1103/PhysRevC.62.051602
M3 - Article
AN - SCOPUS:85035306709
SN - 0556-2813
VL - 62
SP - 5
JO - Physical Review C - Nuclear Physics
JF - Physical Review C - Nuclear Physics
IS - 5
ER -