On the production and detection of gravitational waves from artificial sources

Details On the production and detection of gravitational waves from artificial sources On the production and detection of gravitational waves from artificial sources

Apr 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988opdg.rept.....d&link_type=abstract

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Astronomy and Astrophysics

Astrophysics

Detection, Gravitational Waves, Wave Generation, Gravitational Wave Antennas, Product Development

Scientific paper

It is shown that it is conceivable to build sources on Earth to produce fluxes of continuous and monochromatic gravity waves of the order of 0.001 to 0.00001 erg/s/sq cm. The obtainable frequencies are in the range 10 to the 15 to 8th power Hz, corresponding to wavelengths from 1 micron to several meters. The fluxes estimated are not far from the fluxes expected from the supernova explosions inside the bandwidth of a bar detector of the Weber type and are of the same order or higher than those expected from periodic astrophysics sources like the Crab pulsar. It is also shown that for a certain range of frequencies detectors exist with sufficient sensitivity to detect the signal.

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