Orateur
David Trestini
(IAP et LUTH)
Description
We compute the gravitational waves generated by compact binary systems in a class of massless scalar-tensor (ST) theories to the 1.5 post-Newtonian order beyond the standard quadrupole radiation in general relativity (GR). Using (and adapting) the multipolar-post-Minkowskian and post-Newtonian formalism in GR we obtain in particular the tail and non-linear memory terms associated with the dipole radiation in ST theory. The multipole moments and GW flux are derived for general orbits and compared to previous results in the literature. In the case of quasi-circular orbits, we present ready-to-use templates for the data analysis of detectors.
Authors
David Trestini
(IAP et LUTH)
Luc Blanchet
(C.N.R.S.)
Laura Bernard