Spin induced multipole moments for the gravitational wave flux from binary inspirals to third Post-Newtonian order
General Relativity and Quantum Cosmology2011-03-30v2Cosmology and Nongalactic AstrophysicsHigh Energy Physics - PhenomenologyHigh Energy Physics - Theory
Using effective field theory techniques we calculate the source multipole moments needed to obtain the spin contributions to the power radiated in gravitational waves from inspiralling compact binaries to third Post-Newtonian order (3PN). The multipoles depend linearly and quadratically on the spins and include both spin(1)spin(2) and spin(1)spin(1) components. The results in this paper provide the last missing ingredient required to determine the phase evolution to 3PN including all spin effects which we will report in a separate paper.
@article{arxiv.1007.1312,
title = {Spin induced multipole moments for the gravitational wave flux from binary inspirals to third Post-Newtonian order},
author = {Rafael A. Porto and Andreas Ross and Ira Z. Rothstein},
journal= {arXiv preprint arXiv:1007.1312},
year = {2011}
}