We describe the cryogenic resonant gravitational wave detector of the Rome group, named Explorer, and report on its long term operation with sensitivity for short bursts in the range h 17- l0>< 10' 19. Ex- plorer has mass M =2270 kg and is equipped with a resonant capacitive transducer followed by a dc su- perconducting quantum interference device amplifier. It has been operated at T:2.6 K in a cryostat cooled with superfluid helium. With a transducer voltage bias of 320 V (E =6. 15 MV/m) the two reso- nant modes have frequencies of 904.7 and 921.3 Hz with coupled quality factors, respectively, of 0.77X 10° and l.0>< 10°. The description of the experimental apparatus and of its calibration is followed by the analysis of the noise and the calculation of the expected sensitivity of the detector: h :8 X 10*" (under the assumption of bursts with duration of 1 ms). We then describe the data acquisition system and the techniques of data analysis, discussing the filtering algorithms. The last section reports the ex- perimental results obtained during the operation of the detector from May 1990 to December 1991. During this period the data were recorded for more than two-thirds of the total time: we show the dis- tributions of the data and the hourly averages of the sensitivity. The data taken from May 1991 to De- cember l99l have also been used to establish a new improved upper limit for the rate and strength of gravitational wave pulses; at h =2><lOT17, for example, there are no more than 0.5 events/day as aver- aged over a period of 134 days.
Long-term operation of the Rome" Explorer" cryogenic gravitational wave detector
1993
Abstract
We describe the cryogenic resonant gravitational wave detector of the Rome group, named Explorer, and report on its long term operation with sensitivity for short bursts in the range h 17- l0>< 10' 19. Ex- plorer has mass M =2270 kg and is equipped with a resonant capacitive transducer followed by a dc su- perconducting quantum interference device amplifier. It has been operated at T:2.6 K in a cryostat cooled with superfluid helium. With a transducer voltage bias of 320 V (E =6. 15 MV/m) the two reso- nant modes have frequencies of 904.7 and 921.3 Hz with coupled quality factors, respectively, of 0.77X 10° and l.0>< 10°. The description of the experimental apparatus and of its calibration is followed by the analysis of the noise and the calculation of the expected sensitivity of the detector: h :8 X 10*" (under the assumption of bursts with duration of 1 ms). We then describe the data acquisition system and the techniques of data analysis, discussing the filtering algorithms. The last section reports the ex- perimental results obtained during the operation of the detector from May 1990 to December 1991. During this period the data were recorded for more than two-thirds of the total time: we show the dis- tributions of the data and the hourly averages of the sensitivity. The data taken from May 1991 to De- cember l99l have also been used to establish a new improved upper limit for the rate and strength of gravitational wave pulses; at h =2>I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
