Neutrino opacities in nuclear matter

被引：204

作者：

Burrows, Adam ^{[1
]}

Reddy, Sanjay

Thompson, Todd A.

机构：

[1] Univ Arizona, Steward Observ, Tucson, AZ 85721 USA

[2] Los Alamos Natl Lab, Div Theoret, Los Alamos, NM 87544 USA

[3] Univ Calif Berkeley, Dept Astron, Berkeley, CA 94720 USA

[4] Univ Calif Berkeley, Theoret Astrophys Ctr, Berkeley, CA 94720 USA

来源：

NUCLEAR PHYSICS A | 2006年 / 777卷

基金：

美国国家航空航天局;

关键词：

supernovae; neutrino interactions; neutrino spectra; protoneutron stars; kinetic theory;

D O I：

10.1016/j.nuclphysa.2004.06.012

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-matter cross sections and interaction rates are central to the core-collapse supernova phenomenon and, very likely, to the viability of the explosion mechanism itself. In this paper, we describe the major neutrino scattering, absorption, and production processes that together influence the outcome of core collapse and the cooling of protoneutron stars. One focus is on energy redistribution and many-body physics, but our major goal is to provide a useful resource for those interested in supernova neutrino microphysics. (c) 2004 Elsevier B.V. All rights reserved.

引用

页码：356 / 394

页数：39

共 69 条

[51] STELLAR CORE COLLAPSE - A BOLTZMANN TREATMENT OF NEUTRINO-ELECTRON SCATTERING [J].