Data di Pubblicazione:
2003
Abstract:
The sensitivity of standard optical schemes for the readout of weak vibrations is limited thermal and radiation pressure fluctuations induced by the small interrogation area. We propose and analyze an optical configuration allowing to overcome this problem and optimize the sensitivity of the new generation of massive gravitational wave detectors. (C) 2003 Elsevier Science B.V. All rights reserved.
Tipologia CRIS:
01.01 Articolo in rivista
Keywords:
Fabry-Perot cavity; gravitational wave detectors; thermal noise; radiation pressure; THERMAL NOISE; TEST MASSES; LASER; RADIATION; MIRROR; SPHERE
Elenco autori:
DE ROSA, Maurizio
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