PIRSA:11050011 Scientific Series Strong Gravity

DOI10.48660/11050011

Series: Strong Gravity

Winstanley, E. (2011). Modeling the evaporation of mini black holes. Perimeter Institute. https://pirsa.org/11050011

Winstanley, Elizabeth. Modeling the evaporation of mini black holes. Perimeter Institute, May. 06, 2011, https://pirsa.org/11050011 

@misc{ pirsa_PIRSA:11050011,
  doi = {10.48660/11050011},
  url = {https://pirsa.org/11050011},
  author = {Winstanley, Elizabeth},
  keywords = {Strong Gravity},
  language = {en},
  title = {Modeling the evaporation of mini black holes},
  publisher = {Perimeter Institute},
  year = {2011},
  month = {may},
  note = {PIRSA:11050011 see, \url{https://pirsa.org}}
}

Abstract

TeV-scale models of quantum gravity predict the formation of mini black holes at the Large Hadron Collider. If these black holes can be treated, at least for part of their evolution, as semi-classical objects, they will emit Hawking radiation. In this talk we review the modeling of this evaporation process, particularly for the case when the black hole is rotating. A detailed understanding of the Hawking radiation is necessary for accurate simulations of black hole events at the LHC.

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