Speaker
Andreas Martin Maier
(DESY)
Description
The dynamics of binary black hole and neutron star systems in the early inspiral phase are well described by a post-Newtonian expansion in small velocities and weak coupling. Adopting nonrelativistic effective field theory techniques known from quarkonium systems this expansion can be formulated in terms of multiloop Feynman diagrams. I discuss results for the complete fifth and partial sixth order corrections.
Primary authors
Andreas Martin Maier
(DESY)
Prof.
Gerhard Schäfer
(Friedrich-Schiller-Universität Jena)
Prof.
Johannes Blümlein
(DESY)
Peter Marquard
(DESY)
