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Interpretation of Gravitational-Wave Observations
Abstract
If Weber's gravitational-wave observations are interpreted in terms of a source at the Galactic center, both the intensity and the frequency of the waves are more reasonable if the source is assumed to emit in a synchrotron mode (narrow angles, high harmonics). Although presently studied sources for such modes are astrophysically unsatisfactory---high-energy, nearly circular, scattering orbits---other possible sources are under study.
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Cited by
Arvanitaki, A., Dimopoulos, S., Dubovsky, S., Kaloper, N., & March-Russell, J. (2010) · Physical Review D · doi:10.1103/physrevd.81.123530 · Cited by 1,941
Rotating Black Holes: Separable Wave Equations for Gravitational and Electromagnetic Perturbations
Teukolsky, S. A. (1972) · Physical Review Letters · doi:10.1103/physrevlett.29.1114 · Cited by 1,045
Black holes, gravitational waves and fundamental physics: a roadmap
Askar, A., Belczynski, C., Bertone, G., Bon, E., Blas, D., Brito, R., Bulik, T., Burrage, C., Byrnes, C. T., Caprini, C., et al. (2019) · Classical and Quantum Gravity · doi:10.1088/1361-6382/ab0587 · Cited by 744
Floating Orbits, Superradiant Scattering and the Black-hole Bomb
PRESS, W. H., & TEUKOLSKY, S. A. (1972) · Nature · doi:10.1038/238211a0 · Cited by 729
Exploring the string axiverse with precision black hole physics
Arvanitaki, A., & Dubovsky, S. (2011) · Physical Review D · doi:10.1103/physrevd.83.044026 · Cited by 667
Metadata
- Authors
- Misner, C. W.
- Venue
- Physical Review Letters
- Publisher
- American Physical Society (APS)
- Published
- 1972-04-10
- Volume
- 28
- Issue
- 15
- Pages
- 994-997
- ISSN
- 0031-9007 (ISSN-L)
- OpenAlex
- W2045989665
- Cited by
- 203
- References
- 0
- FWCI
- 16.98
- Type
- journal article
- Language
- en
- Open access
- closed
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