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

页码：257 / 259

页数：3

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