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].
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页数:4
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