We report on the cooling at liquid-helium temperature of our 2270 kg 5056 Al bar at CERN. The liquid-helium container had been filled up to 1500 liters ensuring to keep the antenna cold for more than one month. The antenna is equipped with a resonant capacitive transducer operating at constant electrical charge with a FET low-noise amplifier. The transducer is tuned to the antenna within less than I Hz and the two normal-mode frequencies are ν−=908.160 Hz and ν+=924.234 Hz with an applied electrical field in the transducer of 106 V/m. The corresponding overall merit factors areQ −=5.20·106 andQ +=7.25·106. The transducer has been tested up to an electrical field of 6·106 V/m: in this condition we have βQ≈104. The antenna has been in operation for several weeks giving, for the Brownian noise, values in agreement with the calculated values. We report also on the results of tests performed on a DC SQUID, whose input was connected to a commercial capacitor via a transformer with turn ratio of 1000.

Initial Operation at Liquid-Helium Temperature of the M=2270 kg Al 5056 Gravitational-Wave Antenna of the Rome Group / Amaldi, Edoardo; P., Bonifazi; F., Bronzini; P., Carelli; M. G., Castellano; G., Cavallari; E., Coccia; Cosmelli, Carlo; V., Foglietti; R., Habel; I., Modena; Y., Ogawa; Pallottino, Giovanni Vittorio; Pizzella, Guido; Rapagnani, Piero; Ricci, Fulvio; G., Vannaroni. - In: LA RIVISTA DEL NUOVO CIMENTO DELLA SOCIETÀ ITALIANA DI FISICA. - ISSN 0393-697X. - 7:3(1984), pp. 338-354. [10.1007/BF02507677]

Initial Operation at Liquid-Helium Temperature of the M=2270 kg Al 5056 Gravitational-Wave Antenna of the Rome Group.

AMALDI, Edoardo;COSMELLI, Carlo;PALLOTTINO, Giovanni Vittorio;PIZZELLA, Guido;RAPAGNANI, Piero;RICCI, Fulvio;
1984

Abstract

We report on the cooling at liquid-helium temperature of our 2270 kg 5056 Al bar at CERN. The liquid-helium container had been filled up to 1500 liters ensuring to keep the antenna cold for more than one month. The antenna is equipped with a resonant capacitive transducer operating at constant electrical charge with a FET low-noise amplifier. The transducer is tuned to the antenna within less than I Hz and the two normal-mode frequencies are ν−=908.160 Hz and ν+=924.234 Hz with an applied electrical field in the transducer of 106 V/m. The corresponding overall merit factors areQ −=5.20·106 andQ +=7.25·106. The transducer has been tested up to an electrical field of 6·106 V/m: in this condition we have βQ≈104. The antenna has been in operation for several weeks giving, for the Brownian noise, values in agreement with the calculated values. We report also on the results of tests performed on a DC SQUID, whose input was connected to a commercial capacitor via a transformer with turn ratio of 1000.
1984
astronomical observations (listed by technique of observation); experimental tests of general relativity and observations of gravitational radiation
01 Pubblicazione su rivista::01a Articolo in rivista
Initial Operation at Liquid-Helium Temperature of the M=2270 kg Al 5056 Gravitational-Wave Antenna of the Rome Group / Amaldi, Edoardo; P., Bonifazi; F., Bronzini; P., Carelli; M. G., Castellano; G., Cavallari; E., Coccia; Cosmelli, Carlo; V., Foglietti; R., Habel; I., Modena; Y., Ogawa; Pallottino, Giovanni Vittorio; Pizzella, Guido; Rapagnani, Piero; Ricci, Fulvio; G., Vannaroni. - In: LA RIVISTA DEL NUOVO CIMENTO DELLA SOCIETÀ ITALIANA DI FISICA. - ISSN 0393-697X. - 7:3(1984), pp. 338-354. [10.1007/BF02507677]
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11573/78070
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