The Gravitational Wave Antennas Explorer And Nautilus: A Progress Report

We report the most recent results obtained with the two cryogenic gravitational wave (g.w.) detectors of the Rome group. A new cross correlation measurement of stochastic background is described, as well as a test of Newton inverse square law at laboratory distances. We then give a preview of sensit...

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Detalles Bibliográficos
Autores principales: Bassan, Massimo, Astone, P, Cosmelli,C, Frasca, S, Pallottino, G V, Coccia, E, Minenkov, Y, Modena, I, Moleti, A, Pizzella, G, Bonifazi, P, Terenzi, R, Visco, M, Carelli, P, Fafone, V, Marini, A, Mauceli, E, Modestino, G, Papa, M A, Ronga, F, Votano, L
Lenguaje:eng
Publicado: 2000
Materias:
General Relativity and Cosmology
Detectors and Experimental Techniques
Acceso en línea:http://cds.cern.ch/record/2288303
Descripción
Sumario:We report the most recent results obtained with the two cryogenic gravitational wave (g.w.) detectors of the Rome group. A new cross correlation measurement of stochastic background is described, as well as a test of Newton inverse square law at laboratory distances. We then give a preview of sensitivity enhancement expected with the new setup of Explorer and with possible, future upgrades of Nautilus

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