MG14 - Talk detail |
Participant |
d'Ambrosi, Giuseppe | |||||||
Institution |
Nikhef - Science Park 105 - Amsterdam - Noord Holland - Netherland | |||||||
Session |
BH4 |
Accepted |
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Order |
Time |
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Talk |
Oral abstract |
Title |
Ballistic orbits for gravitational waves | |||||
Coauthors | ||||||||
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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Pdf file |
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Session |
GW1 |
Accepted |
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Order |
Time |
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Talk |
Poster abstract |
Title |
Ballistic orbits for gravitational waves | |||||
Coauthors | ||||||||
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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Pdf file |
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