Cross sections and fragment distributions from neutrino-induced fission on r-process nuclei

被引:21
|
作者
Kelic, A [1 ]
Zinner, N
Kolbe, E
Langanke, K
Schmidt, KH
机构
[1] Gesell Schwerionenforsch Inst Darmstadt, D-6100 Darmstadt, Germany
[2] Aarhus Univ, Inst Phys & Astron, DK-8000 Aarhus, Denmark
[3] Univ Basel, Dept Phys, CH-4056 Basel, Switzerland
关键词
D O I
10.1016/j.physletb.2005.04.074
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We study neutrino-induced processes that might contribute to the observed patterns in the r-process abundances in low-metallicity, old galactical halo stars. The neutrino-nucleus interaction is calculated within the random phase approximation, while the decay of excited levels in the daughter nucleus is followed via the evaporation-fission code ABLA. We calculate the fission cross sections for selected neutron-rich progenitor nuclei with Z(prog) > 80. More importantly, we calculate the mass and charge distributions of the fission fragments as well as the number of neutrons set free in the neutrino-induced reactions. We particularly study a sample of nuclei with A(prog) > 200 representing r-process progenitors during their decay towards the valley of stability after the r-process freeze-out. (c) 2005 Elsevier B.V. All rights reserved.
引用
收藏
页码:48 / 58
页数:11
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