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 orientation, the distance and the direction of the source.
Coalescing binaries and spherical gravitational wave detectors
Coccia E;
1996-01-01
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 orientation, the distance and the direction of the source.File in questo prodotto:
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