Active-sterile neutrino conversion: consequences for the r-process and supernova neutrino detection

被引：77

作者：

Fetter, J

McLaughlin, GC ^{[1
]}

Balantekin, AB

Fuller, GM

机构：

[1] N Carolina State Univ, Dept Phys, Raleigh, NC 27695 USA

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

[3] Univ Calif San Diego, Dept Phys, La Jolla, CA 92093 USA

来源：

ASTROPARTICLE PHYSICS | 2003年 / 18卷 / 05期

基金：

美国国家科学基金会;

关键词：

D O I：

10.1016/S0927-6505(02)00156-1

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We examine active-sterile neutrino conversion in the late time post-core-bounce supernova environment. By including the effect of feedback on the Mikheyev-Smirnov-Wolfenstein (MSW) conversion potential, we obtain a large range of neutrino mixing parameters which produce a favorable environment for the r-process. We look at the signature of this effect in the current generation of neutrino detectors now coming on line. We also investigate the impact of the neutrino-neutrino forward-scattering-induced potential on the MSW conversion. (C) 2002 Elsevier Science B.V. All rights reserved.

引用

页码：433 / 448

页数：16

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