Black hole evaporation and semiclassical thin shell collapse

  title={Black hole evaporation and semiclassical thin shell collapse},
  author={Valentina Baccetti and Sebastian Murk and Daniel R. Terno},
  journal={Physical Review D},
In case of spherical symmetry the assumptions of finite-time formation of a trapped region and regularity of its boundary --- the apparent horizon --- are sufficient to identify the limiting form of the metric and the energy-momentum tensor in its vicinity. By comparison with the known results for quasi-static evaporation of black holes we complete the identification of their parameters. Consistency of the Einstein equations determines two possible types of higher-order terms in the energy… 

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