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Family of regular interiors for nonrotating black holes withT00=T11

2002/02/28 by E. Elizalde, Emilio Elizalde, S. R. Hildebrandt +1 · 3 citations
Mathematics · Physics and Astronomy · #Algorithm #Astrophysical Phenomena and Observations #Black Holes and Theoretical Physics #Black hole (networking) #Computer science #Core (optical fiber) #Cosmology and Gravitation Theories #Energy (signal processing) #Generalization #Mathematical analysis #Mathematical physics #Mathematics #Order (exchange) #Physics #Pure mathematics #Quantum mechanics #Tensor (intrinsic definition) #Type (biology) #astro-ph #gr-qc #hep-th #math-ph #math.MP

paper · pdf · doi:10.1103/physrevd.65.124024

published as Phys.Rev. D65 (2002) 124024 · 31 pages, 1 figure, version to appear in Physical Review D

arxiv created 2002/04/17 · openalex publication_date 2002/06/18 · arxiv updated 2009/11/30 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

We find the general solution for the spacetimes describing the interior of static black holes with an equation of state of the type T00=T11 (T being the stress-energy tensor). This form is the one expected from taking into account different quantum effects associated with strong gravitational fields. We recover all the particular examples found in the literature. We remark that all the solutions found follow the natural scheme of an interior core linked smoothly with the exterior solution by a transient region. We also discuss their local energy properties and give the main ideas involved in a possible generalization of the scheme in order to include other realistic types of sources.

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