Astronomy and Astrophysics – Astronomy
Scientific paper
Aug 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991nyasa.631..156f&link_type=abstract
(Nonlinear problems in relativity and cosmology; Proceedings of the 6th Florida Workshop in Nonlinear Astronomy, Gainesville, Oc
Astronomy and Astrophysics
Astronomy
9
Equations Of State, Gravitational Collapse, Gravitational Waves, Laser Interferometry, Signal To Noise Ratios, Stellar Cores, Finite Difference Theory, Supernovae
Scientific paper
Detailed finite-difference calculations of axisymmetric stellar-core collapse designed to determine the gravitational radiation waveforms were performed. The resulting waveforms are interpreted in the context of the most advanced detectors envisioned from the proposed Laser-Interferometer Gravitational-wave Observatory (LIGO). It is assumed that, to be considered detectable, a burst of gravitational radiation must be responsible for on average at least three event per year whose SNR has less than 5 percent probability of being generated by detector noise. With this criterion, it is found that gravitational radiation from axisymmetric stellar-core collapse is not detectable by the proposed LIGO detectors.
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