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Charged Fermions and Strong Cosmic Censorship

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arxiv 1811.10629 v3 pith:7IPY6YJA submitted 2018-11-26 gr-qc hep-thmath-phmath.MP

Charged Fermions and Strong Cosmic Censorship

classification gr-qc hep-thmath-phmath.MP
keywords censorshipcosmicstrongblackfermionicholessittercharge
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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It was recently shown that the Strong Cosmic Censorship conjecture might be violated for near-extremally-charged black holes in de Sitter space. Here, we extend our study to charged fermionic fields in the exterior of Reissner-Nordstr\"{o}m-de Sitter black holes. We identify three families of modes; one related to the photon sphere, a second related to the de Sitter horizon and a third which dominates near extremality. We show that for near-extremally-charged black holes there is a critical fermionic charge below which Strong Cosmic Censorship may potentially be violated. Surprisingly enough, as one approaches extremality even more, violation of Strong Cosmic Censorship may occur even beyond the critical fermionic charge.

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Cited by 1 Pith paper

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  1. Scalar perturbations and strong cosmic censorship in a regular ABGB-de Sitter black hole spacetime

    gr-qc 2026-07 conditional novelty 6.0

    In regular ABGB-de Sitter black holes, near-extremal scalar perturbations decay fast enough (β>1/2) to violate strong cosmic censorship, and adding scalar mass can push the regularity parameter past β=1.