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Black Holes, Moduli, and Long-Range Forces

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arxiv 2006.09378 v2 pith:GGTWTOQU submitted 2020-06-16 hep-th gr-qc

classification hep-thgr-qc
keywords blackextremalholeholeslargemodulireissner-nordstromvanishing
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It is well known that an identical pair of extremal Reissner-Nordstrom 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-Nordstrom black hole is a charged, spherically symmetric black hole with vanishing surface gravity or vanishing horizon area. Analogous results hold for black branes.

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Cited by 1 Pith paper

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  1. Co-Scaling and Alignment of Electric and Magnetic Towers

    hep-th 2025-05 conditional novelty 7.0 of 10

    Electric and magnetic BPS towers in 5d supergravity are conjectured to co-scale and align, and a new S-map is conjectured to characterize the magnetic infinity cone of a Calabi-Yau threefold.

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