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Electromagnetic self-force on a static charge in Schwarzschild-de Sitter spacetimes

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arxiv 1307.8342 v1 pith:HIIZHGXN submitted 2013-07-31 gr-qc

Electromagnetic self-force on a static charge in Schwarzschild-de Sitter spacetimes

classification gr-qc
keywords cosmologicalchargeself-forceconstantpositivealwaysblackhole
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We compute the self-force acting on an electric charge at rest in Schwarzschild-de Sitter spacetimes, allowing the cosmological constant to be either positive or negative. In the case of a positive cosmological constant, we show that the self-force is always positive, representing a repulsion from the black hole, and monotonically decreasing with increasing distance from the black hole. The spectrum of results is richer in the case of a negative cosmological constant. Here the self-force is not always positive --- it is negative when the black-hole and cosmological scales are comparable and the charge is close to the black hole --- and not always monotonically decreasing --- it is actually monotonically increasing when the cosmological scale is sufficiently small compared to the black-hole scale. The self-force also approaches a constant asymptotic value when the charge is moved to large cosmological distances; this feature can be explained in terms of an interaction between the charge and the conformal boundary at infinity, which acts as a grounded conductor.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Self-Forces as Nonlocal Probes of Gravastar Interiors

    gr-qc 2026-07 conditional novelty 7.0

    For charges held near a gravastar, the self-force carries information about the interior, giving explicitly computable differences from the black-hole case.

  2. Self-Forces as Nonlocal Probes of Gravastar Interiors

    gr-qc 2026-07 conditional novelty 6.0

    Static scalar and electric charges near a thin-shell gravastar experience self-forces different from those near a black hole, with analytic leading-order formulas.