期刊
PHYSICAL REVIEW D
卷 97, 期 10, 页码 -出版社
AMER PHYSICAL SOC
DOI: 10.1103/PhysRevD.97.104034
关键词
-
资金
- European Regional Development Fund [POIG. 02.01.00-12-023/08]
- Narodowe Centrum Nauki Grant [DEC-2012/06/A/ST2/00397]
- [K/DSC/004356]
We obtain from the first principles a general-relativistic Keplerian rotation law for self-gravitating disks around spinning black boles. This is an extension of a former rotation law that was designed mainly for toroids around spinless black holes. We integrate numerically axial stationary Einstein equations with self-gravitating disks around spinless or spinning black holes; that includes the first ever integration of the Keplerian selfgravitating tori. This construction can be used for the description of tight black hole-torus systems produced during coalescences of two neutron stars or modelling of compact active galactic nuclei.
作者
我是这篇论文的作者
点击您的名字以认领此论文并将其添加到您的个人资料中。
推荐
暂无数据