APA

Baccetti, V. (2017). Effects of black hole radiation: horizon avoidance. Perimeter Institute. https://pirsa.org/17110094

MLA

Baccetti, Valentina. Effects of black hole radiation: horizon avoidance. Perimeter Institute, Nov. 10, 2017, https://pirsa.org/17110094

BibTex

@misc{ pirsa_PIRSA:17110094,
  doi = {10.48660/17110094},
  url = {https://pirsa.org/17110094},
  author = {Baccetti, Valentina},
  keywords = {Quantum Gravity},
  language = {en},
  title = {Effects of black hole radiation: horizon avoidance},
  publisher = {Perimeter Institute},
  year = {2017},
  month = {nov},
  note = {PIRSA:17110094 see, \url{https://pirsa.org}}
}
            

Abstract

Event horizons are the defining feature of classical black holes. They are the key ingredient of the information loss paradox which, as paradoxes in quantum foundations, is built on a combination of predictions of quantum theory and counterfactual classical features. Within the semi-classical theory we investigate the possibility that black hole radiation still does not allow for a finite time crossing of the Schwarzschild radius of collapsing matter as seen by distant observers. The exact form of the pre-Hawking radiation is not yet settled, and we make only minimal assumptions about its nature.