Neutrino-matter interactions in the context of core-collapse supernovae

被引：8

作者：

Burrows, A ^{[1
]}

机构：

[1] Univ Arizona, Dept Astron, Tucson, AZ 85721 USA

来源：

PROGRESS IN PARTICLE AND NUCLEAR PHYSICS, VOL 46: RADIOACTIVE BEAMS IN NUCLEAR AND ASTROPHYSICS | 2001年 / 46卷

关键词：

D O I：

10.1016/S0146-6410(01)00108-9

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 processes determine the viability of the neutrino-driven mechanism of core-collapse supernova explosions. Here, I list and discuss some of the various neutrino scattering, absorption. and production processes that collectively determine the outcome of core collapse, the creation of neutron stars, the ejection of the stellar mantle, and the cooling of protoneutron stars. These are the essential inputs into the radiation/hydrodynamics codes with which astrophysicists simulate the supernova phenomenon. Hence, understanding these processes is a crucial prerequisite to the further advancement of supernova theory.

引用

页码：59 / 71

页数：13

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