Journal Article PUBDB-2021-03486

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Gravitational radiation from inspiralling compact objects: Spin-spin effects completed at the next-to-leading post-Newtonian order

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2021
Inst. Melville, NY

Physical review / D 104(2), 024037 () [10.1103/PhysRevD.104.024037]
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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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Note: Phys. Rev. D 104, 024037 (2021). 39 pages. 1 ancillary file (wl format)

Contributing Institute(s):
  1. Theoretische Astroteilchenphysik (Z_THAT)
Research Program(s):
  1. 611 - Fundamental Particles and Forces (POF4-611) (POF4-611)
  2. LHCtoLISA - Precision Gravity: From the LHC to LISA (817791) (817791)
  3. EXC 2121 - Das Quantisierte Universum (390833306) (390833306)
Experiment(s):
  1. No specific instrument

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Gravitational radiation from inspiralling compact objects: Spin-spin effects completed at the next-to-leading post-Newtonian order
1-39 () [10.3204/PUBDB-2021-01827]  GO OpenAccess  Download fulltext Files  Download fulltextFulltext by arXiv.org BibTeX | EndNote: XML, Text | RIS


 Record created 2021-08-23, last modified 2025-07-16


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