Neutrino-induced reaction rates for r-process nuclei -: art. no. 055803

被引:48
作者
Hektor, A [1 ]
Kolbe, E
Langanke, K
Toivanen, J
机构
[1] Univ Aarhus, Inst Phys & Astron, DK-8000 Aarhus C, Denmark
[2] Univ Basel, Dept Phys & Astron, CH-4003 Basel, Switzerland
来源
PHYSICAL REVIEW C | 2000年 / 61卷 / 05期
关键词
D O I
10.1103/PhysRevC.61.055803
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
Neutrino-induced charged- and neutral-current reactions play an important role during and after the r process, if the latter occurs in an environment with extreme neutrino fluxes such as the neutrino-driven wind model or neutron star mergers. Therefore consistent r-process simulations require the knowledge of neutrino-nucleus reaction rates for very neutron-rich nuclei. The neutrino reactions can excite the daughter nucleus above the neutron threshold, which are quite low for r-process nuclei. Thus the daughter nucleus will decay by emission of one or several neutrons. We have calculated the relevant total and partial neutron spallation cross sections for r-process nuclei with neutron numbers N=41-135. Our calculations are bayed on the random phase approximation and consider allowed as well as forbidden transitions.
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页数:10
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