Pith. sign in

REVIEW 3 cited by

Regular black holes and their singular families

Not yet reviewed by Pith; the record is open.

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 2503.13133 v1 pith:LTROW4VG submitted 2025-03-17 gr-qc hep-th

Regular black holes and their singular families

classification gr-qc hep-th
keywords blackholesregularsingularclasscounterpartscurvaturemass
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
0 comments
read the original abstract

Regular black holes without curvature singularity can arise in Einstein gravity with appropriate matter energy-momentum tensor. We show that these regular solutions represent only a special case of a much broader family of black holes with a free mass parameter. The regularity is achieved only at a specific mass value, and any deviation from the fine-tuned parameter inevitably results in curvature singularity. As a concrete example, we consider nonlinear electrodynamics (NLED) as matter sources. A new NLED theory is proposed that is a generalization of the Bardeen class and the Hayward class. New regular black holes and their singular counterparts are obtained. Significant distinctions between regular black holes and their singular counterparts are analyzed. These findings provide new insights into regular black holes.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 3 Pith papers

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

  1. Charging up regular black holes

    gr-qc 2026-07 accept novelty 6.0

    Charged Bardeen and Hayward metrics become singular under deformed Einstein–Maxwell equations; more stringent regularity conditions are derived and improved regular charged metrics are constructed.

  2. Shadow signatures and energy accumulation in Lorentzian-Euclidean black holes

    gr-qc 2026-01 unverdicted novelty 5.0

    Lorentzian-Euclidean black holes produce excess inner-shadow intensity and accumulate energy at the horizon with backreaction unlike stable light rings.

  3. Dark matter production from evaporation of regular primordial black holes

    hep-ph 2025-10 unverdicted novelty 5.0

    Regular primordial black holes can evaporate completely like singular ones and yield the observed dark matter density under modified cosmological constraints.