ELECTRIC CHARGE ESTIMATION OF A NEWBORN BLACK HOLE

被引:6
作者
Baushev, Anton [1 ,2 ]
Chardonnet, Pascal [2 ]
机构
[1] Joint Inst Nucl Res, Bogoliubov Lab Theoret Phys, Dubna 141980, Moscow Region, Russia
[2] Univ Savoie, Lab Annecy Le Vieux Phys Theor, F-74941 Annecy Le Vieux, France
来源
INTERNATIONAL JOURNAL OF MODERN PHYSICS D | 2009年 / 18卷 / 13期
基金
俄罗斯基础研究基金会;
关键词
Black hole; electric charge; classical electrodynamics;
D O I
10.1142/S0218271809015771
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Though a black hole can theoretically possess a very big charge (Q/root GM similar or equal to 1), the charge of the real astrophysical black holes is usually considered to be negligible. This supposition is based on the fact that an astrophysical black hole is always surrounded by some plasma, which is a very good conductor. However, it disregards the fact that black holes usually have some angular momentum, which can be interpreted as their rotation of a sort. If in the plasma surrounding the hole there is some magnetic field, it leads to electric field creation and, consequently, charge separation. In this article we estimate the upper limit of the electric charge of stellar mass astrophysical black holes. We have considered a new black hole formation process and shown that the charge of a newborn black hole can be significant (similar to 10(13) C). Though the obtained charge of an astrophysical black hole is big, the charge-to-mass ratio is small, Q/root GM similar to 10(-7), and it is not enough to affect significantly either the gravitational field of the star or the dynamics of its collapse.
引用
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页码:2035 / 2045
页数:11
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