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General Solution for Self-Gravitating Spherical Null Dust

A. Mikovic
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Abstract

We find the general solution of equations of motion for self-gravitating spherical null dust as a perturbative series in powers of the outgoing matter energy-momentum tensor, with the lowest order term being the Vaidya solution for the ingoing matter. This is done by representing the null-dust model as a 2d dilaton gravity theory, and by using a symmetry of a pure 2d dilaton gravity to fix the gauge. Quantization of this solution would provide an effective metric which includes the back-reaction for a more realistic black hole evaporation model than the evaporation models studied previously.

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BibTeXRIS

A. Mikovic. 1997-05-13. General Solution for Self-Gravitating Spherical Null Dust. https://doi.org/10.1103/physrevd.56.r6067

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