Displaying similar documents to “The laser interferometer gravitational wave observatory project LIGO”

VIRGO: a wide band gravitational wave detector

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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Gravitational radiation from accreting neutron stars

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...

Theory of spacecraft Doppler tracking

Massimo Tinto (1997)

Banach Center Publications

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We present a review of the spacecraft Doppler tracking technique used in broad band searches for gravitational waves in the millihertz frequency band. After deriving the transfer functions of a gravitational wave pulse and of the noise sources entering into the Doppler observable, we summarize the upper limits for the amplitudes of gravitational wave bursts, continuous, and of a stochastic background estimated by Doppler tracking experiments.

Stellar pulsations and gravitational waves

Kostas Kokkotas (1997)

Banach Center Publications

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Pulsating stars are important sources of information for astrophysics. Nearly every star undergoes some kind of pulsation from the early stages of its formation until the very late ones i.e. the catastrophic creation of a supercompact object (white dwarf, neutron star or black hole). Pulsations of supercompact objects are of great importance for relativistic astrophysics since these pulsations are accompanied by the emission of gravitational radiation. In this review we shall discuss...