Preliminary results on the operation of a 2270 kg cryogenic gravitational-wave antenna with a resonant capacitive transducer and a d.c. ... View Full Text


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Article Info

DATE

1986-07

AUTHORS

E. Amaldi, C. Cosmelli, G. V. Pallottino, G. Pizzella, P. Rapagnani, F. Ricci, P. Bonifazi, M. G. Castellano, P. Carelli, V. Foglietti, G. Cavallari, E. Coccia, I. Modena, R. Habel

ABSTRACT

In November 1985 the gravitational-wave antenna of the Rome group, installed at CERN, has started operating. It consists of a 5056 aluminium cilinder 3 m long, 2270 kg heavy, cooled at 4.2 K. The antenna vibrations are detected by means of a resonant capacitive transducer that together with the bar makes a two-coupled-oscillator system. The low-noise amplification is obtained with a d.c. SQUID amplifier. The frequencies of the two resonant modes are:v-=907.116 Hz andv+=923.083 Hz, with merit factorsQ−=3.2·106 andQ+=5.6·106. The sensitivity to short gravitational bursts, expressed in terms of effective noise temperature, is 18 mK. This corresponds to a change in the metric tensor whose Fourier transform isH=1.1·10−21 Hz−1. For monochromatic waves the antenna is sensitive (SNR=1) toh∼2·10−25 in a band width of about 1/3 Hz, with a three months integration time. More... »

PAGES

829-845

Identifiers

URI

http://scigraph.springernature.com/pub.10.1007/bf02558082

DOI

http://dx.doi.org/10.1007/bf02558082

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1043053451


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