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Radiating collapse solutions

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Abstract

Exact gravitational collapse solutions with shear and radial heat flow are obtained by integrating a field equation. Junction conditions which match the collapse solutions to an exterior Vaidya metric show that, at the boundary, the pressure is proportional to the magnitude of the heat flow vector.

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References

  1. Misner, C. W., and Sharp, D. H. (1965).Phys. Lett.,15, 279.

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  3. Vaidya, P. C. (1953).Nature,171, 260.

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  4. Lindquist, R. W., Schwartz, R. A., and Misner, C. W. (1965).Phys. Rev.,137, B1364.

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Authors and Affiliations

  1. Physics Department, University of Windsor, Windsor, Ontario

    E. N. Glass

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  1. E. N. Glass
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Glass, E.N. Radiating collapse solutions. Gen Relat Gravit 21, 733–740 (1989). https://doi.org/10.1007/BF00759082

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  • DOI: https://doi.org/10.1007/BF00759082

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