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Preprint . 1992
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Cauchy horizon singularity without mass inflation

descriptionPublicationkeyboard_double_arrow_right Article , Preprint 15 May 1993Embargo end date: 01 Jan 1992 English Publisher:American Physical Society (APS)Journal:Physical Review D, volume 47, pages 4,239-4,243 (issn: 0556-2821, Copyright policy )Funded by:NSERC | unidentified
Authors: Brady, P. R.; Nunez, D.; Sinha, S.;

doi: 10.1103/physrevd.47.4239 , 10.48550/arxiv.gr-qc/9211026

pmid: 10015419

arXiv: gr-qc/9211026

Cauchy horizon singularity without mass inflation

Abstract

A perturbed Reissner-Nordstr��m-de Sitter solution is used to emphasize the nature of the singularity along the Cauchy horizon of a charged spherically symmetric black hole. For these solutions, conditions may prevail under which the mass function is bounded and yet the curvature scalar $R_{��������} R^{��������}$ diverges.

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Keywords

Astrophysics (astro-ph), FOS: Physical sciences, General Relativity and Quantum Cosmology (gr-qc), Astrophysics, General Relativity and Quantum Cosmology

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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
26
Top 10%
Top 10%
Top 10%
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