A new-type antenna for continuous gravitational radiation

Details A new-type antenna for continuous gravitational radiation A new-type antenna for continuous gravitational radiation

Mar 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992rsci...63.1880s&link_type=abstract

Review of Scientific Instruments (ISSN 0034-6748), vol. 63, March 1992, p. 1880-1883.

Physics

1

Antenna Design, Gravitational Wave Antennas, Pulsars, Cryogenic Equipment, Finite Element Method, Q Factors, Stellar Radiation, Tuning

Scientific paper

A new-type disk antenna has been developed to search for continuous gravitational waves emitted from millisecond and submillisecond pulsars. The antenna not only has a wide tunable range of the eigenfrequency that covers down to almost half of the original frequency of the quadrupole mode, but also is easily tuned to an objective frequency with an accuracy of 4 x 10 exp -5 at 4.2 K. The mechanical quality factor has reached 3.0 x 10 exp 7 at 4.2 K in an antenna made of A15056.

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