Quantum Radiation of General Nonstationary Black Holes
arXiv:gr-qc/0612174 · doi:10.1209/0295-5075/85/30007
Abstract
This paper has been withdrawn by the authors. Quantum radiative characteristics of 4D semi-classical nonstationary black holes in the general case are investigated by using the method of generalized tortoise coordinate transformation. It is generally shown that the temperature and the shape of the event horizon of this kind of black holes depend on both the time and different angles. Further, we discover that there is a certain relationship that is ignored before between thermal radiation and non-thermal radiation of black holes, which is that the chemical potential in thermal radiation spectrum is equal to the highest energy of the negative energy state of particles in non-thermal radiation for 4D semi-classical nonstationary black holes. Also, we show that the deduced general results can be applied to different concrete conditions.
arXiv commentThis paper has been revised and will appear in EPL (Europhysics Letters)
References in corpus (14)
- Gauss-Bonnet Black Holes in AdS Spaces
- A Note on Thermodynamics of Black Holes in Lovelock Gravity
- Cardy-Verlinde Formula and Thermodynamics of Black Holes in de Sitter Spaces
- Massive Complex Scalar Field in a Kerr-Sen Black Hole Background: Exact Solution of Wave Equation and Hawking Radiation
- Massive complex scalar field in the Kerr-Sen geometry: Exact solution of wave equation and Hawking radiation
- Hawking Radiation of Dirac Particles in a Variable-mass Kerr Space-time
- Topological Gauge Theory Of General Weitzenbock Manifolds Of Dislocations In Crystals
- Unified Expressions Of All Integral Variational Principles
- Hawking Radiation of a Non-stationary Kerr-Newman Black Hole: Spin-Rotation Coupling Effect
- Addendum: Hawking Radiation of Photons in a Variable-mass Kerr Black Hole
- Exact Solutions to Sourceless Charged Massive Scalar Field Equation on Kerr-Newman Background
- Solution Of Wheeler-De Witt Equation, Potential Well And Tunnel Effect
- Generalization of Classical Statistical Mechanics to Quantum Mechanics and Stable Property of Condensed Matter
- Thermal radiation in non-static curved spacetimes: quantum mechanical path integrals and configuration space topology