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arXiv · gr-qc/9602018

Detectability of gravitational wave events by spherical resonant-mass antennas

Gregory M. Harry·Thomas R. Stevenson·Ho Jung Paik
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Abstract

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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Gregory M. Harry, Thomas R. Stevenson, Ho Jung Paik. 1996-05-13. Detectability of gravitational wave events by spherical resonant-mass antennas. https://doi.org/10.1103/physrevd.54.2409

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