Hawking radiation is corpuscular
arXiv:1606.01790 · doi:10.1140/epjc/s10052-016-4233-3
Abstract
The total number of Hawking quanta emitted during the evaporation of a Schwarzschild black hole is proportional to the square of the initial mass or, equivalently, to the Bekenstein entropy. This simple, but little appreciated, fact is interpreted in terms of the recent discovery of black hole soft hair.
arXiv comment6 pages, v.3: added reference
References in corpus (16)
- Soft Hair on Black Holes
- On BMS Invariance of Gravitational Scattering
- BMS supertranslations and Weinberg's soft graviton theorem
- Symmetries of asymptotically flat 4 dimensional spacetimes at null infinity revisited
- BMS charge algebra
- Semiclassical Virasoro Symmetry of the Quantum Gravity S-Matrix
- Supertranslations and Superrotations at the Black Hole Horizon
- Conserved charges of the extended Bondi-Metzner-Sachs algebra
- Black Hole's 1/N Hair
- The Hawking cascade from a black hole is extremely sparse
- Classical Limit of Black Hole Quantum N-Portrait and BMS Symmetry
- Non-Thermal Corrections to Hawking Radiation Versus the Information Paradox
- Thermality of the Hawking flux
- Entropy budget for Hawking evaporation
- Entropy/information flux in Hawking radiation
- Gravitational Memory Charges of Supertranslation and Superrotation on Rindler Horizons
Cited by in corpus (9)
- Soft hairy horizons in three spacetime dimensions
- Matter and gravitons in the gravitational collapse
- Zero Mass Remnant as an Asymptotic State of Hawking Evaporation
- Strong Coupling and Classicalization
- A Complementary Third Law for Black Hole Thermodynamics
- Unitarity and Page curve for evaporation of 2D AdS black holes
- Quantum information in Hawking radiation
- Unitary toy qubit transport model for black hole evaporation
- Total spectral distributions from Hawking radiation