Displaying similar documents to “Frequency of oscillations of a synchronous motor”

The laser interferometer gravitational wave observatory project LIGO

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...

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.