Pulsar kicks from neutrino oscillations -: art. no. 061302

被引：74

作者：

Kusenko, A ^{[1
]}

Segrè, G

机构：

[1] Univ Calif Los Angeles, Dept Phys & Astron, Los Angeles, CA 90095 USA

[2] Univ Penn, Dept Phys, Philadelphia, PA 19104 USA

来源：

PHYSICAL REVIEW D | 1999年 / 59卷 / 06期

关键词：

D O I：

10.1103/PhysRevD.59.061302

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Neutrino oscillations can explain the observed motion of pulsars. We show that two different models of neutrino emission from a cooling neutron star are in good quantitative agreement and predict the same order of magnitude for the pulsar kick velocity, consistent with the data. [S0556-2821(99)50206-3].

引用

页数：4

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