Published December 15, 2006 | Version v1
Journal article

Quantum Tunneling Radiation of Kerr-NUT Black Hole

  • 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/10.1088/0253-6102/46/6/007

Additional 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