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

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2014年 / 445卷 / 01期

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

页码：L11 / L15

页数：5

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