PIRSA:14070019

Video URL

https://pirsa.org/14070019

Asymmetric Hawking Radiation : Baryogenesis from Hawking Radiation

Hook, A. (2014). Asymmetric Hawking Radiation : Baryogenesis from Hawking Radiation. Perimeter Institute for Theoretical Physics. https://pirsa.org/14070019

Hook, Anson. Asymmetric Hawking Radiation : Baryogenesis from Hawking Radiation. Perimeter Institute for Theoretical Physics, Jul. 29, 2014, https://pirsa.org/14070019 

          @misc{ scivideos_PIRSA:14070019,
            doi = {10.48660/14070019},
            url = {https://pirsa.org/14070019},
            author = {Hook, Anson},
            keywords = {Particle Physics},
            language = {en},
            title = {Asymmetric Hawking Radiation : Baryogenesis from Hawking Radiation},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2014},
            month = {jul},
            note = {PIRSA:14070019 see, \url{https://scivideos.org/index.php/pirsa/14070019}}
          }

Anson Hook University of Maryland, College Park

Talk numberPIRSA:14070019
DOI10.48660/14070019
Source RepositoryPIRSA
Collection
Talk Type Scientific Series
Subject

Abstract

We show that in the presence of a chemical potential, black hole evaporation generates baryon number. If the inflaton or Ricci scalar is derivatively coupled to the B-L current, the expansion of the universe acts as a chemical potential and splits the energy levels of particles and their anti-particles. The asymmetric Hawking radiation of primordial black holes can thus be used to generate a B-L asymmetry. If dark matter is produced by the same mechanism, the coincidence between the mass density of visible and dark matter can be naturally explained.