Effects of Lorentz Breaking on the Accretion onto a Schwarzschild-like Black Hole

被引:18
|
作者
Yang, Rong-Jia [1 ,2 ,3 ]
Gao, He [1 ]
Zheng, Yao-Guang [1 ]
Wu, Qin [4 ]
机构
[1] Hebei Univ, Coll Phys Sci & Technol, Baoding 071002, Peoples R China
[2] Hebei Univ, Hebei Key Lab Opt Elect Informat & Mat, Baoding 071002, Peoples R China
[3] Hebei Univ, Natl Local Joint Engn Lab New Energy Photoelect D, Baoding 071002, Peoples R China
[4] Guangdong Med Univ, Sch Informat Engn, Dongguan 523808, Peoples R China
基金
中国国家自然科学基金;
关键词
accretion; mass accretion rate; Lorentz breaking; Schwarzschild-like black hole; MATTER; ENERGY;
D O I
10.1088/0253-6102/71/5/568
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
We formulate and solve the problem of spherically symmetric, steady state, adiabatic accretion onto a Schwarzschild-like black hole obtained recently. We derive the general analytic expressions for the critical points, the critical velocity, the critical speed of sound, and subsequently the mass accretion rate. The case for polytropic gas is discussed in detail. We find the parameter characterizing the breaking of Lorentz symmetry will slow down the mass accretion rate, while has no effect on the gas compression and the temperature profile below the critical radius and at the event horizon.
引用
收藏
页码:568 / 572
页数:5
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