Light particle probes of expansion and temperature evolution: Coalescence model analyses of heavy ion collisions at 47A MeV - art. no. 034607

Citation
K. Hagel et al., Light particle probes of expansion and temperature evolution: Coalescence model analyses of heavy ion collisions at 47A MeV - art. no. 034607, PHYS REV C, 6203(3), 2000, pp. 4607
Citations number
88
Categorie Soggetti
Physics
Journal title
PHYSICAL REVIEW C
ISSN journal
05562813 → ACNP
Volume
6203
Issue
3
Year of publication
2000
Database
ISI
SICI code
0556-2813(200009)6203:3<4607:LPPOEA>2.0.ZU;2-R
Abstract
The reactions C-12 + Sn-116, Ne-22 + Ag, Ar-40 + Mo-100, and Zn-64 + Y-89 h ave been studied at 47A MeV projectile energy. For these reactions the most violent collisions lend to increasing amounts of fragment and light partic le emission as the projectile mass increases. This is consistent with quant um molecular dynamics (QMD) model simulations of the collisions. Moving sou rce fits to the light charged particle data have been used to gain a global view of the evolution of the particle emission,Comparisons of the multipli cities and spectra of light charged particles emitted in the reactions with the four different projectiles indicate a common emission mechanism for ea rly emitted ejectiles even though the deposited excitation energies differ greatly. The spectra for such ejectiles can be characterized as emission in the nucleon-nucleon frame. Evidence that the He-3 yield is dominated by th is type of emission and the role of the collision dynamics in determining t he H-3/He-3 yield ratio are discussed. Self-consistent coalescence model an alyses are applied to the light cluster yields, in an attempt to probe emit ter source sizes and to follow the evolution of the temperatures and densit ies from the time of first particle emission to equilibration. These analys es exploit correlations between ejectile energy and emission time, suggeste d by the QMD calculations. In this analysis the degree of expansion of the emitting system is found to increase with increasing projectile mass. The d ouble isotope yield ratio temperature drops as the system expands. Average densities as low as 0.36 rho(0) are reached at a time near 100 fm/c after c ontact. Calorimetric methods were used to derive the mass and excitation en ergy of the excited nuclei which are present after preequilibrium emission. The derived masses range from 102 to 116 u and the derived excitation ener gies increase from 2.6 to 6.9 MeV/nucleon with increasing projectile mass. A caloric curve is derived for these expanded A similar to 110 nuclei. This caloric curve exhibits a plateau at temperatures near 7 MeV. The plateau e xtends from similar to 3.5 to 6.9 MeV/nucleon excitation energy.