Published July 21, 2005
| Version v1
Journal article
Intermediate asymptotics of the Kerr quasinormal spectrum
Creators
- 1. Racah Institute of Physics, Hebrew University, Jerusalem 91904 (Israel)
- 2. Physics Faculty, Weizmann Institute, Rehovot 76100 (Israel)
Description
We study analytically the quasinormal mode spectrum of near-extremal (rotating) Kerr black holes. We find an analytic expression for these black-hole resonances in terms of the black-hole physical parameters: its Bekenstein-Hawking temperature, TBH, and its horizon's angular velocity, Ω. The expression is valid in the intermediate asymptotic regime 1 << vertical bar ω vertical bar << T-1BH. (letter to the editor)
Availability note (English)
Available online at http://stacks.iop.org/0264-9381/22/L71/cqg5_14_l01.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/0264-9381/22/L71/cqg5_14_l01.pdf; http://www.iop.org/;
- DOI
- 10.1088/0264-9381/22/14/L01;
- PII
- S0264-9381(05)00319-9;
Publishing Information
- Journal Title
- Classical and Quantum Gravity
- Journal Volume
- 22
- Journal Issue
- 14
- Journal Page Range
- p. L71-L75
- ISSN
- 0264-9381
- CODEN
- CQGRDG
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 36101535
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Descriptors DEI
- ANGULAR VELOCITY; BLACK HOLES; ENERGY SPECTRA; KERR METRIC; RESONANCE
- Descriptors DEC
- METRICS; SPECTRA; VELOCITY