The final fate of spherical inhomogeneous dust collapse: II. Initial data and causal structure of the singularity

DOI10.1088/0264-9381/13/11/019zbMath0869.53060arXivgr-qc/9604046OpenAlexW2031762837MaRDI QIDQ5689719

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Publication date: 2 September 1997

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/gr-qc/9604046

zbMATH Keywords

Einstein equations spherical collapse Tolman-Bondi metric inhomogeneous dust

Mathematics Subject Classification ID

Black holes (83C57) Applications of differential geometry to physics (53Z05) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Space-time singularities, cosmic censorship, etc. (83C75) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Equations of motion in general relativity and gravitational theory (83C10)

Related Items (8)

CAN WE SEE NAKED SINGULARITIES? ⋮ Can we distinguish black holes from naked singularities by the images of their accretion disks? ⋮ A non-static quantum inspired spacetime in \(f(R)\) gravity: gravity's rainbow ⋮ GRAVITATIONAL COLLAPSE WITH TANGENTIAL PRESSURE ⋮ Complete solutions to the metric of spherically collapsing dust in an expanding spacetime with a cosmological constant ⋮ Critical phenomena in gravitational collapse ⋮ Critical phenomena in gravitational collapse ⋮ ANALYSIS OF TRAPPED SURFACES IN HIGHER DIMENSIONAL DUST COLLAPSE

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