The spectrum of gravitational radiation from binary systems

Details The spectrum of gravitational radiation from binary systems The spectrum of gravitational radiation from binary systems

Apr 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987azh....64..438l&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 64, Mar.-Apr. 1987, p. 438-442. In Russian.

Mathematics

Logic

10

Binary Stars, Gravitational Waves, Stellar Evolution, Background Radiation, Milky Way Galaxy, Monte Carlo Method

Scientific paper

The evolution of low- and intermediate-mass stars has been simulated by using Monte Carlo methods. The spectrum of the gravitational radiation background from binaries in our Galaxy is obtained. The metric strain amplitude as high as h ≡ 10-19.5 is attainable at frequencies of about 10-4Hz. It is shown that the gravitational wave background from binaries exceeds some known GWB cosmological origin at 10-8 - 1 Hz.

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