Stellar (n,GAMMA;) cross sections of neutron-rich nuclei

被引:0
|
作者
Marganiec, J. [1 ]
Dillmann, I. [1 ]
Pardo, C. Domingo [1 ]
Kaeppeler, F. [1 ]
机构
[1] GSI Helmholtzzent Schwerionenforsch GmbH, Planckstr 1, D-64291 Darmstadt, Germany
关键词
s process; r process; Nuclear astrophysics; Stellar nucleosynthesis; NUCLEOSYNTHESIS;
D O I
10.1063/1.3362587
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The present measurements were performed by means of the activation technique. Neutrons were produced at the Karlsruhe Van de Graaff accelerator via the Li-7(p,n)Be-7 reaction. For proton energies just above threshold, one obtains a neutron spectrum similar to a Maxwellian distribution for kT = 25 keV. This quasi-stellar neutron spectrum allowed us to measure the Maxwellian, averaged cross sections directly. The experimental results of Yb-174,Yb-176, W-184,W-186, Os-190,Os-192 Pt-196,Pt-198, and Hg-202 were extrapolated from kT = 25 keV to lower and higher temperatures.
引用
收藏
页码:219 / +
页数:2
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