Detectability of the gravitational wave signal from a close neutron star binary with mass transfer

Details Detectability of the gravitational wave signal from a close neutron star binary with mass transfer Detectability of the gravitational wave signal from a close neutron star binary with mass transfer

Aug 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992apj...394..586j&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 394, no. 2, Aug. 1, 1992, p. 586-591.

Statistics

Computation

22

Binary Stars, Gravitational Waves, Neutron Stars, Stellar Mass Accretion, Computational Astrophysics, Laser Interferometry, Mass Transfer, Signal To Noise Ratios, Stellar Models

Scientific paper

Two simple analytical model of a neutron star binary with mass transfer corresponding to different equations of state are developed. The members of the binary are assumed to move along Newtonian orbits, and the quadrupole formula is used to determine gravitational radiation. The detectability of the gravitational wave signal from such a system by laser interferometers with optimal linear filtering is calculated.

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