Exact solutions for null fluid collapse
arXiv:gr-qc/9511011 · doi:10.1103/PhysRevD.53.R1759
Abstract
Exact non-static spherically symmetric solutions of the Einstein equations for a null fluid source with pressure and density related by are given. The metrics are asymptotically flat for and cosmological for . The metric is the known charged Vaidya solution. In general the metrics have multiple apparent horizons. In the long time limit, the asymptotically flat metrics are hairy black hole solutions that `fall between' the Schwarzschild and Reissner-Nordstrom metrics.
11 pages, RevTeX
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