riassunto2

BH4 - Gravitational fields with sources: From compact objects to black holes

Speaker

d'Ambrosi, Giuseppe

Coauthors

Talk Title

Ballistic orbits for gravitational waves

Abstract

Among the sources of gravitational waves worth modelling there are Extreme Mass Ratio binaries. In order to understand the dynamics during their coalescence, we describe a special class of ballistic geodesics in Schwarzschild space-time. These orbits are in 1-1 correspondence, and completely degenerate in energy and angular momentum, with stable circular orbits. From these special orbits we derive analytic expressions for the source terms in the Regge-Wheeler and Zerilli-Moncrief radiative equations for a point-particle, and compute the gravitational waves emitted during the infall in an Extreme Mass Ratio black-hole binary coalescence. Results of these calculations and the waveforms obtained are then discussed, showing limits and applicability of the method."

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