PIRSA:13030093

Video URL

https://pirsa.org/13030093

A Self-consistent Model of the Black Hole Evaporation

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

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

          @misc{ scivideos_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 for Theoretical Physics},
            year = {2013},
            month = {mar},
            note = {PIRSA:13030093 see, \url{https://scivideos.org/pirsa/13030093}}
          }

Yuki Yokokura RIKEN

Talk numberPIRSA:13030093
DOI10.48660/13030093
Source RepositoryPIRSA
Collection
Talk Type Scientific Series
Subject

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)