Gravitational wave scintillation by a stellar cluster

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dc.creatorCongedo, G.
dc.creatorDe Paolis, F.
dc.creatorLongo, P.
dc.creatorNucita, A. A.
dc.creatorVetrugno, D.
dc.date2006-10-27
dc.date.accessioned2026-07-07T11:00:02Z
dc.date.available2026-07-07T11:00:02Z
dc.descriptionThe diffraction effects on gravitational waves propagating through a stellar cluster are analyzed in the relevant approximation of Fresnel diffraction limit. We find that a gravitational wave scintillation effect - similar to the radio source scintillation effect - comes out naturally, implying that the gravitational wave intensity changes in a characteristic way as the observer moves.
dc.description9 pages, in press in IJMP D
dc.identifierhttps://arxiv.org/abs/astro-ph/0610830
dc.identifierhttp://arxiv.org/abs/astro-ph/0610830
dc.identifierInt.J.Mod.Phys.D15:1937-1946,2006
dc.identifierdoi:10.1142/S0218271806009248
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/187605
dc.subjectAstrophysics
dc.titleGravitational wave scintillation by a stellar cluster
dc.typetext

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