The swallowing of a quark star by a black hole

被引：34

作者：

Kluzniak, W

Lee, WH

机构：

[1] Copernicus Astron Ctr, PL-00716 Warsaw, Poland

[2] Zielona Gora Univ, Inst Astron, PL-65265 Zielona Gora, Poland

[3] Univ Nacl Autonoma Mexico, Inst Astron, Mexico City 04510, DF, Mexico

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2002年 / 335卷 / 01期

关键词：

dense matter; gravitational waves; hydrodynamics; binaries : close; stars : general; gamma-rays : bursts;

D O I：

10.1046/j.1365-8711.2002.05819.x

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

In three-dimensional smooth particle hydrodynamic simulations of the coalescence of a quark star with a pseudo-Newtonian black hole all of the quark matter is quickly accreted by the black hole. The Madsen-Caldwell-Friedman argument against the existence of quark stars may need to be re-examined.

引用

收藏

页码：L29 / L32

页数：4

相关论文

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