Published October 7, 2004
| Version v1
Journal article
How classical are TeV-scale black holes?
Creators
- 1. Department of Physics and Astronomy, University of Mississippi, PO Box 1848, University, MS 38677-1848 (United States)
- 2. Department of Physics, University of Lethbridge, 4401 University Drive, Lethbridge, Alberta T1K 3M4 (Canada)
Description
We show that the Hawking temperature and the entropy of black holes are subject to corrections from two sources: the generalized uncertainty principle and thermal fluctuations. Both effects increase the temperature and decrease the entropy, resulting in faster decay and 'less classical' black holes. We discuss the implications of these results for TeV-scale black holes that are expected to be produced at future colliders
Availability note (English)
Available online at http://stacks.iop.org/0264-9381/21/4511/cqg4_19_001.pdf or at the Web site for the journal Classical and Quantum Gravity (ISSN 1361-6382) http://www.iop.org/Additional details
Identifiers
- URL
- http://stacks.iop.org/0264-9381/21/4511/cqg4_19_001.pdf; http://www.iop.org/;
- DOI
- 10.1088/0264-9381/21/19/001;
- PII
- S0264-9381(04)79156-X;
Publishing Information
- Journal Title
- Classical and Quantum Gravity
- Journal Volume
- 21
- Journal Issue
- 19
- Journal Page Range
- p. 4511-4522
- ISSN
- 0264-9381
- CODEN
- CQGRDG
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 36029492
- Subject category
- S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS;
- Descriptors DEI
- BLACK HOLES; ENTROPY; FLUCTUATIONS; TEMPERATURE DEPENDENCE; TEV RANGE; UNCERTAINTY PRINCIPLE
- Descriptors DEC
- ENERGY RANGE; PHYSICAL PROPERTIES; THERMODYNAMIC PROPERTIES; VARIATIONS