Hawking radiation from dynamical horizons
arXiv:1204.1530 · doi:10.1103/PhysRevD.87.084051
Abstract
In completely local settings, we establish that a dynamically evolving black hole horizon can be assigned a Hawking temperature. Moreover, we calculate the Hawking flux and show that the radius of the horizon shrinks.
5 Pages
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- Marginally Trapped Surfaces in Spherical Gravitational Collapse
- Quantum radiation of Kerr black hole in de Sitter background
- Estimation of temperature of cosmological apparent horizons: a new approach
- Spherical trapped surfaces in n-dimensional general relativity
- Evaporation of Primordial Black Holes in a Thermal Universe: A Thermofield Dynamics Approach
- Gravitational thermodynamics and universal holographic duality in dynamical spacetimes