The EXPLORER gravitational wave detector has been recently improved. The antenna has been equipped with a new read-out. The use of a new transducer, characterized by a very small gap, and a dc-Squid with a high coupling, led to a better sensitivity and a larger bandwidth. In the first six months of the year 2000, an effective temperature of 3 mK and a bandwidth of almost 8 Hz were reached. Further improvements are expected. The new experimental configuration appears also very promising for use in the ultra-cryogenic antenna NAUTILUS.

Recent improvements on the EXPLORER gravitational wave antenna

Castellano M G;
2002

Abstract

The EXPLORER gravitational wave detector has been recently improved. The antenna has been equipped with a new read-out. The use of a new transducer, characterized by a very small gap, and a dc-Squid with a high coupling, led to a better sensitivity and a larger bandwidth. In the first six months of the year 2000, an effective temperature of 3 mK and a bandwidth of almost 8 Hz were reached. Further improvements are expected. The new experimental configuration appears also very promising for use in the ultra-cryogenic antenna NAUTILUS.
2002
R. Cianci, R. Collina, M. Francaviglia, P. Fré
Recent developments in general relativity
Recent developments in general relativity. 14th SIGRAV Conference on General Relativity and Gravitational Physics
397
401
88-470-0162-5
18-22 sept. 2000
Genova, Italy
19
none
Astone, P; Bassan, M; Bonifazi, P; Carelli, P; Castellano, MARIA GABRIELLA; Cavallari, G; Coccia, E; Cosmelli, C; D'Antonio, S; Fafone, V; Minenkov, Y...espandi
273
info:eu-repo/semantics/conferenceObject
04 Contributo in convegno::04.01 Contributo in Atti di convegno
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/20.500.14243/206950
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