APA

(2026). Hawking Radiation from near extremal black holes. Perimeter Institute. https://pirsa.org/26040070

MLA

Hawking Radiation from near extremal black holes. Perimeter Institute, Apr. 28, 2026, https://pirsa.org/26040070

BibTex

@misc{ pirsa_PIRSA:26040070,
  doi = {10.48660/26040070},
  url = {https://pirsa.org/26040070},
  author = {},
  keywords = {Cosmology},
  language = {en},
  title = {Hawking Radiation from near extremal black holes},
  publisher = {Perimeter Institute},
  year = {2026},
  month = {apr},
  note = {PIRSA:26040070 see, \url{https://pirsa.org}}
}
            

Abstract

Over the last few years it has been understood that black holes sufficiently close to extremality receive large quantum corrections that modify their thermodynamic properties. In this talk I will explain how these large quantum corrections modify the real time dynamics of near-extremal black holes. In particular, the spectrum of emitted Hawking radiation differs drastically from the predictions of QFT in curved spacetime.
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