Neutral current induced neutrino oscillations in a supernova

被引：135

作者：

Kusenko, A ^{[1
]}

Segre, G ^{[1
]}

机构：

[1] UNIV PENN,DEPT PHYS & ASTRON,PHILADELPHIA,PA 19104

来源：

PHYSICS LETTERS B | 1997年 / 396卷 / 1-4期

关键词：

D O I：

10.1016/S0370-2693(97)00121-4

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Neutral currents induced matter oscillations of electroweak-active (anti-)neutrinos to sterile neutrinos can explain the observed motion of pulsars. In contrast to a recently proposed explanation of the pulsar birth velocities based on the v(mu,tau) <--> v(e) oscillations, the heaviest neutrino (either active or sterile) would have to have mass of order several keV. (C) 1997 Elsevier Science B.V.

引用

页码：197 / 200

页数：4

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