Black Hole Spectroscopy, Final System Parameters

Details Black Hole Spectroscopy, Final System Parameters Black Hole Spectroscopy, Final System Parameters

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012aps..apr.r7005l&link_type=abstract

American Physical Society, APS April Meeting 2012, March 31-Apr 3, 2012, abstract #R7.005

Physics

Scientific paper

Given a gravitational wave signal containing merger and ring-down, we present a method for estimating the start of ring-down, and extracting quasi-normal mode information from the signal. The application of this method to numerical relativity waveforms may reveal information about the source generating the gravitational waves beyond the final mass and spin of the black hole. We investigate the potential for recovering the system's initial and final parameters from these modes.

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