| Home > Publications database > Gravitational radiation from inspiralling compact objects: Spin effects to the fourth post-Newtonian order |
| Journal Article | PUBDB-2022-07502 |
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2022
Inst.
Melville, NY
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Please use a persistent id in citations: doi:10.1103/PhysRevD.106.L101501 doi:10.3204/PUBDB-2022-07502
Report No.: DESY-22-004; ET-0001A-22; arXiv:2201.05138
Abstract: The linear- and quadratic-in-spin contributions to the binding potential and gravitational-wave flux from binary systems are derived to next-to-next-to-leading order in the post-Newtonian (PN) expansion of general relativity, including finite-size and tail effects. The calculation is carried out through the worldline effective field theory framework. We find agreement in the overlap with the available PN and self-force literature. As a direct application, we complete the knowledge of spin effects in the evolution of the orbital phase for aligned-spin circular orbits to fourth PN order. We estimate the impact in the number of accumulated gravitational-wave cycles and find they make a significant contribution for next-generation observatories. The results presented here will therefore play an important role in providing reliable physical interpretation of gravitational-wave signals from spinning binaries with future gravitational-wave detectors such as LISA and the Einstein Telescope.
Keyword(s): spin: effect ; higher-order: 4 ; gravitational radiation: flux ; binary ; general relativity ; orbit: circle ; overlap ; Einstein Telescope ; LISA ; effective field theory ; finite size ; expansion: higher-order
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Gravitational radiation from inspiralling compact objects: Spin effects to fourth Post-Newtonian order
[10.3204/PUBDB-2022-00119]
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