Séminaire / Seminar GReCO |
« Modelling the gravitational waveform for inspiralling binary systems » |
Edward Porter |
We show how re-summation techniques, such as Pade approximation, can be used to model the inspiral of a test particle into a Kerr black hole. We also look at how differential geometry can be used, not only to help model equal mass binary waveforms, but in the actual detection of gravitational wave signals. |
jeudi 13 février 2003 - 11:00 Salle des séminaires Évry Schatzman Institut d'Astrophysique de Paris |
Pages web du séminaire / Seminar's webpage |