In this talk I will review the self-force approach to calculating gravitational radiation and associated quantities for a small compact body moving on a hyperbolic geodesic around a large black hole. I will present the latest gravitational self-force (GSF) calculations and comparisons with post-Minkowskian (PM), post-Newontian and numerical relativity results. I will also discuss how a resummation for PM results can be used to improve the convergence in the strong-field.
De Donato Bini
De Pierpaolo Mastrolia
De Marie-Anne Bizouard
De Alessandro Nagar
De Simon Maenaut
De Keefe Mitman
De Simone Albanesi
De Manuela Campanelli
De Marc Henneaux
De Niels Warburton
De Sergiu Klainerman
De Rod Gover
De Jérémie Szeftel
