Gravitational radiation from inspiralling compact objects: Spin effects to the fourth post-Newtonian order
| Autor: | Porto Pereira, Rafael Alejandro, Yang, Zixin, Cho, Gihyuk |
|---|---|
| Jazyk: | angličtina |
| Rok vydání: | 2022 |
| Předmět: |
High Energy Physics - Theory
higher-order: 4 LISA spin: effect gravitational radiation: flux binary orbit: circle FOS: Physical sciences General Relativity and Quantum Cosmology (gr-qc) expansion: higher-order 4 [higher-order] General Relativity and Quantum Cosmology effect [spin] Einstein Telescope effective field theory higher-order [expansion] High Energy Physics - Theory (hep-th) finite size general relativity overlap ddc:530 flux [gravitational radiation] circle [orbit] |
| Zdroj: | Physical review / D 106(10), L101501 (2022). doi:10.1103/PhysRevD.106.L101501 |
| DOI: | 10.3204/pubdb-2022-07502 |
| Popis: | Physical review / D 106(10), L101501 (2022). doi:10.1103/PhysRevD.106.L101501 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. Published by Inst., Melville, NY |
| Databáze: | OpenAIRE |
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