Neutrino mixing and nucleosynthesis in core-collapse supernovae -: art. no. 51

被引：110

作者：

Balantekin, AB

Yüksel, H

机构：

[1] Univ Wisconsin, Dept Phys, Madison, WI 53706 USA

[2] Tohoku Univ, Dept Phys, Sendai, Miyagi 980, Japan

[3] Tohoku Univ, Nucl Theory Grp, Sendai, Miyagi 980, Japan

来源：

NEW JOURNAL OF PHYSICS | 2005年 / 7卷

关键词：

D O I：

10.1088/1367-2630/7/1/051

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

A simple description of core-collapse supernovae is given. Properties of the neutrino-driven wind, neutrino fluxes and luminosities, reaction rates and the equilibrium electron fraction in supernova environments are discussed. Neutrino mixing and neutrino interactions that are relevant to core-collapse supernovae are briefly reviewed. The values of electron fraction under several evolution scenarios that may impact rapid neutron-capture process (r-process) nucleosynthesis are calculated.

引用

页数：18

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