| Home > Publications database > Gravitational radiation from inspiralling compact objects: Spin-spin effects completed at the next-to-leading post-Newtonian order |
| Journal Article | PUBDB-2021-03486 |
; ;
2021
Inst.
Melville, NY
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Please use a persistent id in citations: doi:10.1103/PhysRevD.104.024037 doi:10.3204/PUBDB-2021-03486
Report No.: DESY-21-039; arXiv:2103.14612
Abstract: Using the gravitational potential and source multipole moments bilinear in the spins, first computed to next-to-leading order (NLO) in the post-Newtonian expansion within the effective field theory (EFT) framework, we complete here the derivation of the dynamical invariants and flux-balance equations, including energy and angular momentum. We use these results to calculate spin-spin effects in the orbital frequency and accumulated phase to NLO for circular orbits. We also derive the linear momentum and center-of-mass fluxes and associated kick velocity, to the highest relevant post-Newtonian order. We explicitly demonstrate the equivalence between the quadratic-in-spin source multipoles obtained using the EFT formalism and those rederived later with more traditional tools, leading to perfect agreement for spin-spin radiative observables to NLO among both approaches.
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Preprint
Gravitational radiation from inspiralling compact objects: Spin-spin effects completed at the next-to-leading post-Newtonian order
1-39 (2021) [10.3204/PUBDB-2021-01827]
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