Possibility of detecting superlong gravitational waves

Details Possibility of detecting superlong gravitational waves Possibility of detecting superlong gravitational waves

Feb 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978azh....55...65s&link_type=abstract

Astronomicheskii Zhurnal, vol. 55, no. 1, 1978, p. 65-68. In Russian.

Physics

Optics

8

Binary Stars, Gravitational Waves, Long Wave Radiation, Radiation Detectors, Supermassive Stars, Electromagnetic Pulses, Propagation Modes, Pulsars, Stellar Mass, Supergiant Stars

Scientific paper

The effect of superlong gravitational waves on the propagation of electromagnetic pulses is analyzed. The change in period of pulses transmitted with constant period through a gravitational wave field is calculated in a geometrical optics approximation. Conditions under which detection of gravitational waves from binaries is possible by studying the phase modulation of transmitted pulses are derived. It is shown that it might be possible to detect gravitational radiation from binary superstars whose masses are about 10 billion solar masses.

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