Detectability of gravitational wave events by spherical resonant-mass antennas
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 bar-mode instability of a rapidly rotating star. We find that by using technology only slightly beyond that already demonstrated, spherical antennas can detect these astronomical phenomena at realistic distances.Keywords
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