The evaporation of charged black holes
Google (United States) · Google DeepMind (United Kingdom) · +3 more institutions
Abstract
A bstract Charged particle emission from black holes with sufficiently large charge is exponentially suppressed. As a result, such black holes are driven towards extremality by the emission of neutral Hawking radiation. Eventually, an isolated black hole gets close enough to extremality that the gravitational backreaction of a single Hawking photon becomes important, and the quantum field theory in curved spacetime approximation breaks down. To proceed further, we need to use a quantum theory of gravity. We make use of recent progress in our understanding of the quantum-gravitational thermodynamics of near-extremal black holes to compute the corrected spectrum for both neutral and charged Hawking radiation,…
Citation impact
- FWCI
- 103.27
- Percentile
- 100%
- References
- 90
Authors
4- ARAdam R. Brown
Google (United States), Google DeepMind (United Kingdom), Stanford University
- LVLuca V. Iliesiu
Center for Theoretical Physics, Stanford University
- GPGeoff Penington
Center for Theoretical Physics
- MUMykhaylo UsatyukCorresponding
Center for Theoretical Physics, Kavli Institute for Theoretical Sciences
Topics & keywords
- Hawking radiation
- Semiclassical physics
- Black hole (networking)
- Micro black hole
- Charged black hole
- Angular momentum
- Photon
- Black hole thermodynamics
Funding
- NSNational Science FoundationAwards: PHY-2309135, 0002563, 2309135, PHY-2210452
- UDU.S. Department of EnergyAwards: DE-FOA-0002563, DE-SC0019380, PHY-2210452
- ACAspen Center for PhysicsAward: PHY-2210452
- SFSimonsen FoundationAwards: 994312, 216179
- SNSchweizerischer Nationalfonds zur Förderung der Wissenschaftlichen ForschungAwards: PHY-2210452, PHY-2309135
- OOOffice of the Chief Information OfficerAwards: DE-FOA-0002563, DE-SC0025522, DE-SC0019380
- KIKavli Institute for Theoretical Physics, University of California, Santa BarbaraAwards: PHY-2309135, 216179, PHY-2210452, 2309135
- AFAir Force Office of Scientific ResearchAwards: FA9550-, FA9550-22-1-0098, FA9550