We discuss the interaction of the gravitational waveform emitted by a coalescing binary during its inspiral phase with the two lowest-order quadrupole modes of a resonant spherical mass. We find that a large spherical detector can determine the chirp mass, the orbit inclination, the distance and the direction of the source.

Coalescing binary features measurable with a spherical gravitational wave detector

Coccia E;
1996

Abstract

We discuss the interaction of the gravitational waveform emitted by a coalescing binary during its inspiral phase with the two lowest-order quadrupole modes of a resonant spherical mass. We find that a large spherical detector can determine the chirp mass, the orbit inclination, the distance and the direction of the source.
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Utilizza questo identificativo per citare o creare un link a questo documento: http://hdl.handle.net/20.500.12571/2760
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