Probing strange stars with advanced gravitational wave detectors

被引:16
|
作者
Moraes, Pedro H. R. S. [1 ]
Miranda, Oswaldo D. [1 ]
机构
[1] Inst Nacl Pesquisas Espaciais, Div Astrofis, BR-12227010 Sao Jose Dos Campos, SP, Brazil
关键词
gravitational waves; binaries: general; gamma-ray burst: general; stars: neutron; GAMMA-RAY BURST; EQUATION-OF-STATE; NEUTRON-STAR; NUCLEAR-EQUATION; COMPACT BINARIES; MAGNETIC-FIELDS; GIANT FLARE; GRB; 051103; MASS; REPEATER;
D O I
10.1093/mnrasl/slu124
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
When a neutron star is squeezed to huge densities, it can be converted to a strange star. Using the event/year rate of a neutron star-strange star binary system, we show that the operational phase of advanced gravitational wave detectors might show some evidence that such strange stars do exist. Moreover, we argue that such a system could be a plausible progenitor to GRB 051103 and GRB 070201. In the last run of the Laser Interferometer Gravitational-Wave Observatory (LIGO), no gravitational wave signal was found for these gamma-ray bursts, and a conclusive explanation for this needs to be found.
引用
收藏
页码:L11 / L15
页数:5
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