Conversion of neutron stars to strange stars as a possible origin of gamma-ray bursts

被引:150
作者
Cheng, KS [1 ]
Dai, ZG [1 ]
机构
[1] NANJING UNIV,DEPT ASTRON,NANJING 210093,PEOPLES R CHINA
关键词
D O I
10.1103/PhysRevLett.77.1210
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
We propose that some neutron stars in low-mass x-ray binaries can accrete sufficient mass to undergo a phase transition to become strange stars. The energy released per conversion event satisfies the requirements of cosmological gamma-ray bursts, and the Lorentz factor of the resultant expanding fireball may exceed 5 x 10(3) because the strange star has very low baryon contamination. The model burst rate is consistent with observations.
引用
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页码:1210 / 1213
页数:4
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