Radiation Ball as a Black Hole
arXiv:hep-th/0310185
Abstract
A structure of the radiation-ball which is identified as a Schwarzschild black hole is found out by investigating the backreaction of Hawking radiation into space-time. The structure consists of the radiation which is gravitationally bounded in the ball and of a singularity. The entropy of the radiation in the ball is proportional to the surface-area of the ball and nearly equals to the Bekenstein entropy. The Hawking radiation is regarded as a leak-out from the ball. There arises no information paradox because there exists no horizon in the structure.
12 pages, 3 figures
References in corpus (6)
- Black Hole Entropy in Canonical Quantum Gravity and Superstring Theory
- Stretched horizons, quasiparticles and quasinormal modes
- Electroweak Baryogenesis by Black Holes
- Spherical Domain Wall formed by Field Dynamics of Hawking Radiation and Structure Near Horizon
- Electroweak/GUT Domain Wall by Hawking Radiation: Baryogenesis and Dark Matter from Several Hundred kg Black Holes
- Spherical Domain Wall formed by Field Dynamics of Hawking Radiation and Spontaneous Charging-up of Black Hole