On the global visibility of the singularity in quasi-spherical collapse.

DOI10.1023/A:1018813108516zbMath1047.83514arXivgr-qc/9806055MaRDI QIDQ1807287

S. S. Deshingkar, Sanjay Jhingan, Pankaj S. Joshi

Publication date: 18 November 1999

Published in: General Relativity and Gravitation (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/gr-qc/9806055

Mathematics Subject Classification ID

Black holes (83C57) Space-time singularities, cosmic censorship, etc. (83C75)

Related Items (6)

CAN WE SEE NAKED SINGULARITIES? ⋮ On the visibility of singularities in general relativity and modified gravity theories ⋮ RECENT DEVELOPMENTS IN GRAVITATIONAL COLLAPSE AND SPACETIME SINGULARITIES ⋮ Role of initial data in higher dimensional quasi-spherical gravitational collapse ⋮ Asymptotically FRW black holes ⋮ Time dependent geometry in massive gravity

Cites Work

• A class of inhomogeneous cosmological models
• Non-radiative solutions of Einstein's equations for dust
• Cosmic censorship and the role of pressure in gravitational collapse
• The final fate of spherical inhomogeneous dust collapse
• The Large Scale Structure of Space-Time
• Naked strong curvature singularities in Szekeres spacetimes

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