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  Gravitational-Wave Phasing of Compact Binary Systems to the Fourth-and-a-Half post-Newtonian Order

Blanchet, L., Faye, G., Henry, Q., Larrouturou, F., & Trestini, D. (in preparation). Gravitational-Wave Phasing of Compact Binary Systems to the Fourth-and-a-Half post-Newtonian Order.

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Item Permalink: https://hdl.handle.net/21.11116/0000-000D-13E8-8 Version Permalink: https://hdl.handle.net/21.11116/0000-000D-13EB-5
Genre: Paper

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2304.11185.pdf (Preprint), 205KB
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 Creators:
Blanchet, Luc, Author
Faye, Guillaume, Author
Henry, Quentin1, Author           
Larrouturou, François, Author
Trestini, David, Author
Affiliations:
1Astrophysical and Cosmological Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, ou_1933290              

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Free keywords: General Relativity and Quantum Cosmology, gr-qc,Astrophysics, Cosmology and Extragalactic Astrophysics, astro-ph.CO, Astrophysics, High Energy Astrophysical Phenomena, astro-ph.HE,High Energy Physics - Theory, hep-th
 Abstract: The inspiral phase of gravitational waves emitted by spinless compact binary
systems is derived through the fourth-and-a-half post-Newtonian (4.5PN) order
beyond quadrupole radiation, and the leading amplitude mode ($\ell$, m) = (2,
2) is obtained at 4PN order. We also provide the radiated flux, as well as the
phase in the stationary phase approximation. Rough numerical estimates for the
contribution of each PN order are provided for typical systems observed by
current and future gravitational wave detectors.

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 Dates: 2023-04-212023-04-25
 Publication Status: Not specified
 Pages: 9 pages, 1 table. v2: reference of the companion paper updated
 Publishing info: -
 Table of Contents: -
 Rev. Type: -
 Identifiers: arXiv: 2304.11185
 Degree: -

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