Quasi-normal modes of stars and black holes.
Kokkotas, Kostas D., Schmidt, Bernd G. (1999)
Living Reviews in Relativity [electronic only]
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Kokkotas, Kostas D., Schmidt, Bernd G. (1999)
Living Reviews in Relativity [electronic only]
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Bernard Schutz (1997)
Banach Center Publications
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Neutron stars may emit steady gravitational wave signals that will be among the first kinds of gravitational wave signals that the new generation of interferometric detectors will search for. I consider here the possibility that accreting neutron stars may be driven into the steady emission of gravitational waves. I estimate the amplitudes that the waves may have if the accretion takes place at the Eddington limit, such as may happen when a neutron star spirals inside a giant star in...
Sathyaprakash, B.S., Schutz, Bernard F. (2009)
Living Reviews in Relativity [electronic only]
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C. V. Heer, J. A. Little, J. R. Bupp (1968)
Annales de l'I.H.P. Physique théorique
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B. Caron, A. Dominjon, C. Drezen, Raffaele Flaminio, X. Grave, F. Marion, L. Massonnet, C. Mehmel, R. Morand, B. Mours, V. Sannibale, M. Yvert, D. Babusci, S. Bellucci, G. Candusso, G. Giordano, G. Matone, L. Dognin, J. Mackowski, M. Napolitano, L. Pinard, F. Barone, E. Calloni, L. Di Fiore, A. Grado, L. Milano, G. Russo, S. Solimeno, M. Barsuglia, V. Brisson, F. Cavalier, M. Davier, P. Hello, F. LeDiberder, P. Marin, M. Taubman, F. Bondu, A. Brillet, F. Cleva, H. Heitmann, L. Latrach, C. Man, Pham-Tu Manh, J. Vinet, C. Boccara, Ph. Gleyzes, V. Loriette, J. Roger, G. Cagnoli, L. Gammaitoni, J. Kovalik, F. Marchesoni, M. Punturo, M. Bernardini, S. Braccini, C. Bradaschia, R. Del Fabbro, R. DeSalvo, A. Di Virgilio, I. Ferrante, F. Fidecaro, A. Gennai, A. Giassi, A. Giazotto, L. Holloway, P. La Penna, G. Losurdo, F. Palla, Pani Hui-Bao, A. Pasqualetti, D. Passuello, R. Poggiani, G. Torelli, Zhang Zhou, E. Majorana, P. Puppo, P. Rapagnani, F. Ricci (1997)
Banach Center Publications
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Theocharis Apostolatos (1997)
Banach Center Publications
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According to general relativity, a binary consisting of spinning bodies will precess due to spin-orbit and spin-spin coupling. The corresponding modulation of its gravitational waves might be a serious problem for detecting such waves with simple post-Newtonian templates. A new family of templates that takes into account the complications arising from the orbital precession is proposed and its application and performance are discussed.
James Blackburn (1997)
Banach Center Publications
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The Laser Interferometer Gravitational Wave Observatory (LIGO) will search for direct evidence of gravitational waves emitted by astrophysical sources in accord with Einstein’s General Theory of Relativity. State of the art laser interferometers located in Hanford, Washington and Livingston Parish, Louisiana will unambiguously measure the infinitesimal displacements of isolated test masses which convey the signature of these gravitational waves. The initial implementation of LIGO will...
R. N. Ibragimov (2012)
Mathematical Modelling of Natural Phenomena
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A linear, uniformly stratified ocean model is used to investigate propagation of baroclinic Kelvin waves in a cylindrical basin. It is found that smaller wave amplitudes are inherent to higher mode individual terms of the obtained solutions that are also evanescent away of a costal line toward the center of the circular basin. It is also shown that the individual terms if the obtained solutions can be visualized as spinning patterns in rotating stratified fluid confined in a circular...
Alkahby, H.Y. (1996)
International Journal of Mathematics and Mathematical Sciences
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