Response of the Mario SCHENBERG gravitational wave detector to signals from a black hole ringdown

Details Response of the Mario SCHENBERG gravitational wave detector to signals from a black hole ringdown Response of the Mario SCHENBERG gravitational wave detector to signals from a black hole ringdown

Feb 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005tmgm.meet.2019c&link_type=abstract

The Tenth Marcel Grossmann Meeting. Proceedings of the MG10 Meeting held at Brazilian Center for Research in Physics (CBPF), Rio

Physics

Scientific paper

In this work we calculate the performance of the Mario Schenberg gravitational wave detector to observe black hole's ringdown waveform. This kind of signal is originated from a black hole (BH) perturbation. The waveform looks like damped sinusoid that can be calculated analytically using BH perturbation theory. We simulated ringdown waveforms, introduced them on Schenberg model and obtained results which show that the detector will be sensitive enough to observe this kind of signals in a radius of ~ 20kpc.

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