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arxiv: 1203.2962 · v2 · pith:WKFPNWUGnew · submitted 2012-03-13 · 🌀 gr-qc · astro-ph.CO· astro-ph.HE· hep-ph· hep-th

Spin induced multipole moments for the gravitational wave amplitude from binary inspirals to 2.5 Post-Newtonian order

classification 🌀 gr-qc astro-ph.COastro-ph.HEhep-phhep-th
keywords spinamplitudegravitationalmomentsmultipoleorderpost-newtonianwave
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Using the NRGR effective field theory formalism we calculate the remaining source multipole moments necessary to obtain the spin contributions to the gravitational wave amplitude to 2.5 Post-Newtonian (PN) order. We also reproduce the tail contribution to the waveform linear in spin at 2.5PN arising from the nonlinear interaction between the current quadrupole and the mass monopole.

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