NEUTRON CAPTURE RATES AND r-PROCESS NUCLEOSYNTHESIS

被引：0

作者：

Surman, R. A. ^{[1
]}

Mumpower, M. R. ^{[2
]}

McLaughlin, G. C. ^{[2
]}

Sinclair, R. ^{[3
]}

Hix, W. R. ^{[3
]}

Jones, K. L. ^{[3
]}

机构：

[1] Union Coll, Dept Phys & Astron, Schenectady, NY 12308 USA

[2] North Carolina State Univ, Dept Phys, Raleigh, NC 27695 USA

[3] Univ Tennessee, Dept Phys, Knoxville, TN 37996 USA

来源：

CAPTURE GAMMA-RAY SPECTROSCOPY AND RELATED TOPICS | 2013年

基金：

美国国家科学基金会;

关键词：

NUCLEI; WINDS;

D O I：

暂无

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：

Simulations of r-process nucleosynthesis require nuclear physics information for thousands of neutron-rich nuclear species from the line of stability to the neutron drip line. While arguably the most important pieces of nuclear data for the r-process are the masses and beta decay rates, individual neutron capture rates can also be of key importance in setting the final r-process abundance pattern. Here we consider the influence of neutron capture rates in forming the A similar to 80 and rare earth peaks.

引用

页码：304 / 313

页数：10

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