Cosmic gravitational emissions having the character of noise

Details Cosmic gravitational emissions having the character of noise Cosmic gravitational emissions having the character of noise

Feb 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978mvsfa..19..118s&link_type=abstract

Moskovskii Universitet, Vestnik, Seriia III - Fizika, Astronomiia, vol. 19, Jan.-Feb. 1978, p. 118-121. In Russian.

Mathematics

Logic

1

Astronomical Models, Cosmic Noise, Gravitational Waves, Gravitons, Plasma Radiation, Pulsars, Binary Stars, Flux Density, Galaxies, High Temperature Plasmas, Noise Spectra

Scientific paper

The paper investigates the possibility of detecting gravitational-wave noise produced by the spontaneous creation of gravitons during the expansion of the universe. Three types of possible mechanisms yielding random gravitational radiation are considered, and windows where predicted relict radiation might be washed over by emissions of another source are indicated. The first two mechanisms are in connection with the emission of gravitational waves by the cosmological plasma, while the third mechanism considers gravitational radiation from the aggregate of pulsars of the Galaxy.

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