Detectability of gravitational wave events by spherical resonant-mass antennas

Details Detectability of gravitational wave events by spherical resonant-mass antennas Detectability of gravitational wave events by spherical resonant-mass antennas

1996-02-09

arxiv.org/abs/gr-qc/9602018v2

Phys.Rev.D54:2409-2420,1996

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

39 pages, 4 EPS Figures, some additional SNRs for secular instabilities, some changes to LIGO SNRs, Appendix added on the asym

Scientific paper

10.1103/PhysRevD.54.2409

We have calculated signal-to-noise ratios for eight spherical resonant-mass antennas interacting with gravitational radiation from inspiralling and coalescing binary neutron stars and from the dynamical and secular bar-mode instability of a rapidly rotating star. We find that by using technology that could be available in the next several years, spherical antennas can detect neutron star inspiral and coalescence at a distance of 15 Mpc and the dynamical bar-mode instability at a distance of 2 Mpc.

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