The sensitivity to a cosmic stochastic background of gravitational waves of the resonant cryogenic antenna ALTAIR, operating at 1.8 kHz, is reported. An experimental upper limit of ALTAIR is compared with the upper limits given by the other detectors at lower frequencies.

Astone, P., Bassan, M., Bonifazi, P., Carelli, P., Coccia, E., Fafone, V., et al. (1999). Upper limit at 1.8 kHz for a gravitational-wave stochastic background with the ALTAIR resonant-mass detector. ASTRONOMY & ASTROPHYSICS, 343(1), 19-22.

Upper limit at 1.8 kHz for a gravitational-wave stochastic background with the ALTAIR resonant-mass detector

BASSAN, MASSIMO;COCCIA, EUGENIO;FAFONE, VIVIANA;MOLETI, ARTURO;PIZZELLA, GUIDO;
1999-01-01

Abstract

The sensitivity to a cosmic stochastic background of gravitational waves of the resonant cryogenic antenna ALTAIR, operating at 1.8 kHz, is reported. An experimental upper limit of ALTAIR is compared with the upper limits given by the other detectors at lower frequencies.
1999
Pubblicato
Rilevanza internazionale
Lettera
Nessuno
Settore FIS/01 - FISICA SPERIMENTALE
English
Con Impact Factor ISI
gravitation
Astone, P., Bassan, M., Bonifazi, P., Carelli, P., Coccia, E., Fafone, V., et al. (1999). Upper limit at 1.8 kHz for a gravitational-wave stochastic background with the ALTAIR resonant-mass detector. ASTRONOMY & ASTROPHYSICS, 343(1), 19-22.
Astone, P; Bassan, M; Bonifazi, P; Carelli, P; Coccia, E; Fafone, V; Frasca, S; Minenkov, Y; Modena, I; Modestino, P; Moleti, A; Pallottino, G; Pizzel...espandi
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/2108/23722
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