Numerical analysis of the performance of a resonant gravity-wave detector

Details Numerical analysis of the performance of a resonant gravity-wave detector Numerical analysis of the performance of a resonant gravity-wave detector

Sep 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989phrvd..40.1741x&link_type=abstract

Physical Review D (Particles and Fields), Volume 40, Issue 6, 15 September 1989, pp.1741-1747

Computer Science

Performance

15

Scientific paper

This paper presents the results of a detailed numerical calculation of the performance of a resonant gravitational radiation detector which uses an inductive transducer and a superconducting quantum interference device amplifier. We demonstrate the correctness of the calculations by comparing them to the present performance of the Louisiana State University antenna. We show that a standard cryogenic resonant bar detector operating at 4 K is capable of a noise temperature of less than 0.75 mK, corresponding to an rms gravitational-wave amplitude of 1.9×10-19.

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