학술논문
Gravity in binary systems at the fifth and sixth post-Newtonian order
Document Type
Working Paper
Author
Source
Subject
Language
Abstract
Binary sources of gravitational waves in the early inspiral phase are accurately described by a post-Newtonian expansion in small velocity and weak interaction. We compute the conservative dynamics to fifth and partial sixth order using a non-relativistic effective field theory. We give predictions for central observables and determine the required coefficients for the construction of an Effective One-Body Hamiltonian, extending the applicability of our results to the late inspiral and merger phases.
Comment: 10 pages, 1 figure. Contribution to the proceedings of Loops and Legs in Quantum Field Theory - LL2022
Comment: 10 pages, 1 figure. Contribution to the proceedings of Loops and Legs in Quantum Field Theory - LL2022