Neutron star tidal disruption in mixed binaries: The imprint of the equation of state
Neutron star tidal disruption in mixed binaries: The imprint of the equation of state
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DOI：
10.1103/physrevd.81.064026
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发表时间：
2009-12
影响因子：
5
通讯作者：
V. Ferrari;L. Gualtieri;F. Pannarale
中科院分区：
文献类型：
--
作者：
V. Ferrari;L. Gualtieri;F. Pannarale
我们研究了黑洞-中子星合并双星中子星的潮汐扰动。对于描述中子星内部物质的几个状态方程和一组大的双星参数，我们计算了恒星被黑洞潮汐场破坏的临界轨道距离。当破坏发生在恒星到达最内部稳定的圆形轨道之前，引力
We study the tidal disruption of neutron stars in black hole-neutron star coalescing binaries. We calculate the critical orbital separation at which the star is disrupted by the black hole tidal field for several equations of state describing the matter inside the neutron star, and for a large set of the binary parameters. When the disruption occurs before the star reaches the innermost stable circular orbit, the gravitational