Axion emissivity from the conversion of a neutron star into a strange star

被引：1
作者：
Sub, IS [1 ]
Lee, CH
机构：
[1] Hanyang Univ, Res Inst Nat Sci, Seoul 133791, South Korea
[2] Hanyang Univ, Dept Phys, Seoul 133791, South Korea
来源：
PHYSICS LETTERS B | 1998年 / 432卷 / 1-2期
关键词：
axions; astrophysics; neutron stars; strange star;
D O I：
10.1016/S0370-2693(98)00597-8
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The conversion of neutron matter into strange matter in a neutron star occurs through the non-leptonic weak-interaction process. We study the energy loss of the neutron star by the emission of axions in that process. Owing to that process, the neutron star will liberate the energy which can in no way be negligible as an axion burst. (C) 1998 EIsevier Science B.V. All rights reserved.
引用
收藏
页码：145 / 150
页数：6
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