Black holes, moduli, and long-range forces
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Abstract It is well known that an identical pair of extremal Reissner-Nordström black holes placed a large distance apart will exert no force on each other. In this paper, I establish that the same result holds in a very large class of two-derivative effective theories containing an arbitrary number of gauge fields and moduli, where the appropriate analog of an extremal Reissner-Nordström black hole is a charged, spherically symmetric black hole with vanishing surface gravity or vanishing horizon area. Analogous results hold for black branes.
2014 ◽
Vol 29
(36)
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pp. 1450191
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2016 ◽
Vol 12
(S324)
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pp. 351-352
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Vol 26
(13)
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pp. 1750151
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1999 ◽
Vol 14
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pp. 1951-1960
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2019 ◽
Vol 17
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pp. 69-78
1997 ◽
Vol 06
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pp. 563-573
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