PIRSA:11050011

Video URL

https://pirsa.org/11050011

Modeling the evaporation of mini black holes

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

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

          @misc{ scivideos_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 for Theoretical Physics},
            year = {2011},
            month = {may},
            note = {PIRSA:11050011 see, \url{https://scivideos.org/pirsa/11050011}}
          }

Elizabeth Winstanley University of Sheffield

Talk numberPIRSA:11050011
DOI10.48660/11050011
Source RepositoryPIRSA
Collection
Talk Type Scientific Series
Subject

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.