Gravitational Microlenses as Natural Amplifiers of Gravitational Radiation

Details Gravitational Microlenses as Natural Amplifiers of Gravitational Radiation Gravitational Microlenses as Natural Amplifiers of Gravitational Radiation

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998tx19.confe.468z&link_type=abstract

Abstracts of the 19th Texas Symposium on Relativistic Astrophysics and Cosmology, held in Paris, France, Dec. 14-18, 1998. Eds.:

Astronomy and Astrophysics

Astrophysics

Scientific paper

We consider gravitational microlenses as a natural amplifiers of gravitational radiation. We discuss the properties of astrophysical sources of gravitational radiation which demonstrate the essential amplification for VIRGO (LIGO) and LISA detectors respectively. We obtain that the astrophysical sources of gravitational radiation would be amplified essentially for LISA detector, but the influence on the estimated rate is not great for LIGO (VIRGO) detector. We estimate a propability of a great amplification of gravitational waves by binary gravitational lenses. Thus, using gravitational wave detector we could detect much more distant sources of gravitational radiation which are amplified by gravitational microlenses.

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