Published December 15, 2006
| Version v1
Journal article
Quantum Tunneling Radiation of Kerr-NUT Black Hole
Creators
- 1. College of Physics Science and Technology, Shenyang Normal University, Shenyang 110034 (China)
- 2. Institute of Theoretical Physics, China West Normal University, Nanchong 637002 (China)
- 3. Department of Preparatory Courses, Shenyang Institute of Engineering, Shenyang 110136 (China)
Description
Based on particles in a dynamical geometry, extending the Parikh's method of quantum tunneling radiation, we deeply investigate the quantum tunneling radiation of Kerr-NUT black hole. When self-gravitating action, energy conservation, and angular momentum conservation are taken into account, the emission rate of the particle on the event horizon is related to the change of Bekenstein-Hawking entropy and the emission spectrum is not precisely thermal, but is consistent with an underlying unitary theory.
Availability note (English)
Available from http://dx.doi.org/10.1088/0253-6102/46/6/007Additional details
Identifiers
Publishing Information
- Journal Title
- Communications in Theoretical Physics
- Journal Volume
- 46
- Journal Issue
- 6
- Journal Page Range
- p. 991-994
- ISSN
- 0253-6102
INIS
- Country of Publication
- China
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 42056857
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ANGULAR MOMENTUM; BLACK HOLES; EMISSION SPECTRA; ENERGY CONSERVATION; TUNNEL EFFECT
- Descriptors DEC
- SPECTRA