Conversion of neutrinos in dense plasmas

被引：7
|
作者：
Bingham, R
Cairns, RA
Dawson, JM
Dendy, RO
LashmoreDavies, CN
Tystovich, VN
机构：
[1] UNIV ST ANDREWS,SCH MATH & COMP SCI,ST ANDREWS KY16 9SS,FIFE,SCOTLAND
[2] UNIV ST ANDREWS,SCH MATH & COMPUTAT SCI,ST ANDREWS KY16 9SS,FIFE,SCOTLAND
[3] UNIV CALIF LOS ANGELES,DEPT PHYS,LOS ANGELES,CA 90024
[4] UKAEA,ABINGDON OX14 3DB,OXON,ENGLAND
[5] RUSSIAN ACAD SCI,INST GEN PHYS,MOSCOW,RUSSIA
来源：
PHYSICS LETTERS A | 1997年 / 232卷 / 3-4期
关键词：
D O I：
10.1016/S0375-9601(97)00364-2
中图分类号：
O4 [物理学];
学科分类号：
0702 ;
摘要：
The conversion of electron neutrinos into either a tan or muon neutrino in a dense plasma, such as in the solar interior, is shown to be described by the Weber equation. We show that the problem is related to propagation through a potential barrier and is identical to classical mode conversion problems in inhomogeneous fluids and plasmas, (C) 1997 Elsevier Science B,V.
引用
收藏
页码：257 / 259
页数：3
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