APA

Yokokura, Y. (2013). A Self-consistent Model of the Black Hole Evaporation. Perimeter Institute. https://pirsa.org/13030093

MLA

Yokokura, Yuki. A Self-consistent Model of the Black Hole Evaporation. Perimeter Institute, Mar. 07, 2013, https://pirsa.org/13030093

BibTex

@misc{ pirsa_PIRSA:13030093,
  doi = {10.48660/13030093},
  url = {https://pirsa.org/13030093},
  author = {Yokokura, Yuki},
  keywords = {Quantum Gravity},
  language = {en},
  title = {A Self-consistent Model of the Black Hole Evaporation},
  publisher = {Perimeter Institute},
  year = {2013},
  month = {mar},
  note = {PIRSA:13030093 see, \url{https://pirsa.org}}
}
            

Abstract

We construct a self-consistent model which describes a black hole from formation to evaporation including the back reaction from the Hawking radiation. In the case where a null shell collapses, at the beginning the evaporation occurs, but it stops eventually, and a horizon and singularity appear. On the other hand, in the generic collapse process of a continuously distributed null matter, the black hole evaporates completely without forming a macroscopically large horizon nor singularity. We also find a stationary solution in the heat bath, which can be regarded as a normal thermodynamic object. (hep-th: 1302.4733)