CL-36 (N,P)S-36 CROSS-SECTION FROM 25 MEV TO 800 KEV AND THE NUCLEOSYNTHESIS OF THE RARE ISOTOPE S-36

被引:17
|
作者
KOEHLER, PE
GRAFF, SM
OBRIEN, HA
GLEDENOV, YM
POPOV, YP
机构
[1] LOS ALAMOS NATL LAB, DIV PHYS, LOS ALAMOS, NM 87545 USA
[2] DUBNA JOINT NUCL RES INST, NEUTRON PHYS LAB, DUBNA, RUSSIA
来源
PHYSICAL REVIEW C | 1993年 / 47卷 / 05期
关键词
D O I
10.1103/PhysRevC.47.2107
中图分类号
O57 [原子核物理学、高能物理学];
学科分类号
070202 ;
摘要
We have measured the (Cl(n,p)S)-Cl-36-S-36 cross section from thermal energy to approximately 800 keV. Parameters for eight resonances between 900 eV and 70 keV were determined in a multilevel fit to our data which also included information from published (S(p, gamma)Cl)-S-36-Cl-37 measurements. The (Cl(n,p)S)-Cl-36-S-36 reaction can play a critical role in the production of the rare isotope S-36 in explosive nucleosynthesis and s-process calculations. The astrophysical rate for this reaction was calculated from our measured cross sections and was found to be significantly smaller than the theoretical rate used in previous nucleosynthesis calculations. We discuss the impact of this result on the nucleosynthesis of S-36.
引用
收藏
页码:2107 / 2112
页数:6
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