Exact solution of a static charged sphere in general relativity
Keyword(s):
The Self
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An exact solution of the field equations of general relativity is obtained for a static, spherically symmetric distribution of charge and mass which can be matched with the Reissner–Nordström metric at the boundary. The self-energy contributions to the total gravitational mass are computed retaining only the first order terms in the gravitational constant.
1996 ◽
Vol 11
(30)
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pp. 2409-2415
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2008 ◽
Vol 23
(38)
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pp. 3247-3263
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1963 ◽
Vol 59
(4)
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pp. 739-741
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1970 ◽
Vol 3
(2)
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pp. 149-165
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2011 ◽
Vol 20
(11)
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pp. 2239-2252
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