Destroying the Kerr–Newman–MOG black hole with charged scalar field

In this paper, we investigate the weak cosmic censorship conjecture (WCCC) for the Kerr Newman modified gravity black hole (KN–MOG–BH) by examining its interaction with charged scalar fields. Neglecting backreaction effects, we first show that the scalar test fields with frequencies just above the superradiance threshold can overspin/overcharge both extremal and nearly extremal KN–MOG–BHs, leading to the formation of naked singularities. Next, we incorporate backreaction effects, assuming that the event horizon’s angular velocity rises prior to the test field’s absorption. We show that backreaction prevents overspinning/overcharging in the extremal KN–MOG–BH, whereas in the nearly extremal case, it fails to stop the black hole from being overspun/overcharged.

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Publication Details

Journal
Modern Physics Letters A
Published
2026-01-08
DOI
https://doi.org/10.1142/s0217732326500227
Primary Topic
Black Holes and Theoretical Physics
Type
article
Field-Weighted Citation Impact
0.00
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article

Destroying the Kerr–Newman–MOG black hole with charged scalar field

Ayyesha K. Ahmed, A. R. Kashif, Waqar Ahmad
Modern Physics Letters A
Black Holes and Theoretical Physics
article

Destroying the Kerr–Newman–MOG black hole with charged scalar field

Ayyesha K. Ahmed, A. R. Kashif, Waqar Ahmad
article en

Abstract

In this paper, we investigate the weak cosmic censorship conjecture (WCCC) for the Kerr Newman modified gravity black hole (KN–MOG–BH) by examining its interaction with charged scalar fields. Neglecting backreaction effects, we first show that the scalar test fields with frequencies just above the superradiance threshold can overspin/overcharge both extremal and nearly extremal KN–MOG–BHs, leading to the formation of naked singularities. Next, we incorporate backreaction effects, assuming that the event horizon’s angular velocity rises prior to the test field’s absorption. We show that backreaction prevents overspinning/overcharging in the extremal KN–MOG–BH, whereas in the nearly extremal case, it fails to stop the black hole from being overspun/overcharged.

Modern Physics Letters AVol. 41(07)
Capital University of Science and Technology (PK)
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Black Holes and Theoretical Physics
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