2-PROTON CORRELATION-FUNCTIONS FOR EQUILIBRIUM AND NONEQUILIBRIUM EMISSION

被引：26

作者：

GONG, WG

GELBKE, CK

CARLIN, N

DESOUZA, RT

KIM, YD

LYNCH, WG

MURAKAMI, T

POGGI, G

SANDERSON, D

TSANG, MB

XU, HM

FIELDS, DE

KWIATKOWSKI, K

PLANETA, R

VIOLA, VE

YENNELLO, SJ

PRATT, S

机构：

[1] INDIANA UNIV,INDIANA UNIV CYCLOTRON FACIL,BLOOMINGTON,IN 47405

[2] INDIANA UNIV,DEPT CHEM,BLOOMINGTON,IN 47405

[3] INDIANA UNIV,DEPT PHYS,BLOOMINGTON,IN 47405

[4] UNIV WISCONSIN,DEPT PHYS,MADISON,WI 53706

[5] UNIV WISCONSIN,DEPT PHYS & ASTRON,MADISON,WI 53706

来源：

PHYSICS LETTERS B | 1990年 / 246卷 / 1-2期

关键词：

D O I：

10.1016/0370-2693(90)91301-Q

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Two-proton correlation functions are compared for equilibrium and non-equilibrium emission processes investigated, respectively, in "reverse kinematics" for the reactions 129XE+27Al and 129Xe+122Sn at E A = 31 MeV and in "forward kinematics" for the reaction 14N+197Au at E A = 75 MeV. Observed differences in the shapes of the correlation functions are understood in terms of the different time scales for equilibrium and preequilibrium emission. Transverse and longitudinal correlation functions are very similar. © 1990.

引用

页码：21 / 25

页数：5

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