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Black hole singularities: a numerical approach | | Patrick R. Brady
; John D. Smith
; | | Date: |
28 Jun 1995 | | Journal: | Phys.Rev.Lett. 75 (1995) 1256-1259 | | Subject: | gr-qc | | Abstract: | The singularity structure of charged spherical collapse is studied by considering the evolution of the gravity-scalar field system. A detailed examination of the geometry at late times strongly suggests the validity of the mass-inflation scenario~cite{PI:90}. Although the area of the two-spheres remains finite at the Cauchy horizon, its generators are eventually focused to zero radius. Thus the null, mass-inflation singularity {em generally} precedes a crushing $r=0$ singularity deep inside the black hole core. This central singularity is spacelike. | | Source: | arXiv, gr-qc/9506067 | | Other source: | [GID 422187] pmid10060247 | | Services: | Forum | Review | PDF | Favorites | |
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