Light cluster production in E/A = 61 MeV 36Ar + 112,124Sn reactions
| dc.creator | Ghetti, R. | |
| dc.creator | Helgesson, J. | |
| dc.creator | Avdeichikov, V. | |
| dc.creator | Jakobsson, B. | |
| dc.creator | Colonna, N. | |
| dc.creator | Tagliente, G. | |
| dc.creator | Wilschut, H. W. | |
| dc.creator | Kravchuk, V. L. | |
| dc.date | 2005-07-22 | |
| dc.date.accessioned | 2026-07-07T05:37:37Z | |
| dc.date.available | 2026-07-07T05:37:37Z | |
| dc.description | Experimental kinetic energy distributions and small-angle two-particle correlation functions involving deuterons and tritons are compared for 36Ar+ 112,124Sn collisions at E/A = 61 MeV (i.e. for systems similar in size, but with different isospin content). A larger triton yield is observed from the more neutron-rich system, as predicted by IBUU simulations, while the emission times of the light clusters are found to be the same for the two Sn-target systems. For both systems, the time sequence tau_{d} < tau_{p} < tau_{t}, is deduced for charged particles emitted from the intermediate velocity source. | |
| dc.description | 4 pages, 3 figures, submitted to Phys. Rev. C | |
| dc.identifier | https://arxiv.org/abs/nucl-ex/0507029 | |
| dc.identifier | http://arxiv.org/abs/nucl-ex/0507029 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/81344 | |
| dc.subject | Nuclear Experiment | |
| dc.title | Light cluster production in E/A = 61 MeV 36Ar + 112,124Sn reactions | |
| dc.type | text |