Published April 7, 2002
| Version v1
Journal article
Gravitational waves from inspiralling binary black holes
Description
Binary black holes are the most promising candidate sources for the first generation of earth-based interferometric gravitational-wave detectors. We summarize and discuss the state-of-the-art analytical techniques developed during the last few years to better describe the late dynamical evolution of binary black holes of comparable masses
Availability note (English)
Available online at http://stacks.iop.org/0264-9381/19/1267/q20705.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/0264-9381/19/1267/q20705.pdf; http://www.iop.org/;
- PII
- S0264-9381(02)31383-2;
Publishing Information
- Journal Title
- Classical and Quantum Gravity
- Journal Volume
- 19
- Journal Issue
- 7
- Journal Page Range
- p. 1267-1278
- ISSN
- 0264-9381
- CODEN
- CQGRDG
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 34031412
- Subject category
- S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS;
- Descriptors DEI
- BLACK HOLES; GRAVITATIONAL WAVE DETECTORS; GRAVITATIONAL WAVES; INTERFEROMETRY; STAR EVOLUTION
- Descriptors DEC
- MEASURING INSTRUMENTS; RADIATION DETECTORS