Stellar collapse without singularities?

Thomas A. Roman and Peter G. Bergmann
Phys. Rev. D 28, 1265 – Published 15 September 1983
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Abstract

For the singularity theorems of Hawking and Penrose to hold, the stress-energy tensor of matter must satisfy certain restrictions. A model is developed representing the interior of a collapsing, spherically symmetric cloud of matter, which is everywhere free of singularities, due to a relaxation of the so-called "weak energy condition." The regions of the model in which the condition must be violated, and the properties of matter and energy which result, are determined. The indications are that, at least in spherically symmetric cases involving very large masses, the energy condition must be violated in a region where the density is no larger than normal matter densities, which seems physically implausible. Hence suspending the energy conditions may not be a reasonable approach to the avoidance of singularities.

  • Received 29 November 1982

DOI:https://doi.org/10.1103/PhysRevD.28.1265

©1983 American Physical Society

Authors & Affiliations

Thomas A. Roman*

  • Department of Physics, Syracuse University, Syracuse, New York 13210 and Department of Mathematics and Physics, University of Hartford, West Hartford, Connecticut 06117

Peter G. Bergmann

  • Department of Physics, Syracuse University, Syracuse, New York 13210 and Department of Physics, New York University, New York, New York 10003

  • *Current address.

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Issue

Vol. 28, Iss. 6 — 15 September 1983

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