Date of Original Version

3-30-2011

Type

Article

Rights Management

Copyright 2011 IOP Publishing Ltd and SISSA

Abstract or Description

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.

DOI

http://dx.doi.org/10.1088/1475-7516/2011/03/009

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Published In

Journal of Cosmology and Astroparticle Physics, 2011.