Spin zero Hawking radiation for non-zero-angular momentum mode

Journal Article · Fri May 15 00:00:00 EDT 2015 · AIP Conference Proceedings

DOI:https://doi.org/10.1063/1.4915699· OSTI ID:22391656

Ngampitipan, Tritos ^[1]; Bonserm, Petarpa ^[2]; Visser, Matt ^[3]

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1. Department of Physics, Chulalongkorn University, Bangkok 10330 (Thailand)
2. Department of Mathematics and Computer Science, Chulalongkorn University, Bangkok 10330 (Thailand)
3. School of Mathematics, Statistics, and Operations Research, Victoria University of Wellington, PO Box 600, Wellington 6140 (New Zealand)

Black hole greybody factors carry some quantum black hole information. Studying greybody factors may lead to understanding the quantum nature of black holes. However, solving for exact greybody factors in many black hole systems is impossible. One way to deal with this problem is to place some rigorous analytic bounds on the greybody factors. In this paper, we calculate rigorous bounds on the greybody factors for spin zero hawking radiation for non-zero-angular momentum mode from the Kerr-Newman black holes.

• OSTI ID: 22391656
• Journal Information: AIP Conference Proceedings, Vol. 1660, Issue 1; Conference: ICoMEIA 2014: International Conference on Mathematics, Engineering and Industrial Applications 2014, Penang (Malaysia), 28-30 May 2014; Other Information: (c) 2015 AIP Publishing LLC; Country of input: International Atomic Energy Agency (IAEA); ISSN 0094-243X
• Country of Publication: United States
• Language: English

Related Subjects

71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
79 ASTROPHYSICS
COSMOLOGY AND ASTRONOMY
ANALYTICAL SOLUTION
BLACK HOLES
KERR FIELD
KERR METRIC
QUANTUM MECHANICS
SPIN