The final fate of spherical inhomogeneous dust collapse

DOI10.1088/0264-9381/13/3/019zbMath0849.53069arXivgr-qc/9409062OpenAlexW3105919049MaRDI QIDQ4873097

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Publication date: 10 November 1996

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

Full work available at URL: https://arxiv.org/abs/gr-qc/9409062

zbMATH Keywords

black holenaked singularitystrong curvature naked singularitiesgravitational collapse of a spherically symmetric inhomogeneous dust cloudinitial density and velocity distributionsTolman-Bondi metric

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)

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