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  Energy and periastron advance of compact binaries on circular orbits at the fourth post-Newtonian order

Bernard, L., Blanchet, L., Bohe, A., Faye, G., & Marsat, S. (2017). Energy and periastron advance of compact binaries on circular orbits at the fourth post-Newtonian order. Physical Review D, 95(4): 044026. doi:10.1103/PhysRevD.95.044026.

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Datensatz-Permalink: http://hdl.handle.net/11858/00-001M-0000-002C-3F1A-4 Versions-Permalink: http://hdl.handle.net/11858/00-001M-0000-002E-2BE3-B
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 Urheber:
Bernard, Laura, Autor
Blanchet, Luc, Autor
Bohe, Alejandro1, Autor              
Faye, Guillaume, Autor
Marsat, Sylvain1, Autor              
Affiliations:
1Astrophysical and Cosmological Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, ou_1933290              

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Schlagwörter: General Relativity and Quantum Cosmology, gr-qc
 Zusammenfassung: In this paper, we complete our preceding work on the Fokker Lagrangian describing the dynamics of compact binary systems at the fourth post-Newtonian (4PN) order in harmonic coordinates. We clarify the impact of the non-local character of the Fokker Lagrangian or the associated Hamiltonian on both the conserved energy and the relativistic periastron precession for circular orbits. We show that the non-locality of the action, due to the presence of the tail effect at the 4PN order, gives rise to an extra contribution to the conserved integral of energy with respect to the Hamiltonian computed on shell, which was not taken into account in our previous work. We also provide a direct derivation of the periastron advance by taking carefully into account this non-locality. We then argue that the infra-red (IR) divergences in the calculation of the gravitational part of the action are problematic, which motivates us to introduce a second ambiguity parameter, in addition to the one already assumed previously. After fixing these two ambiguity parameters by requiring that the conserved energy and the relativistic periastron precession for circular orbits are in agreement with numerical and analytical gravitational self-force calculations, valid in the limiting case of small mass ratio, we find that our resulting Lagrangian is physically equivalent to the one obtained in the ADM Hamiltonian approach.

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 Datum: 2016-10-252017-01-062017
 Publikationsstatus: Im Druck publiziert
 Seiten: 30 pages, 1 figure
 Ort, Verlag, Ausgabe: -
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 Identifikatoren: arXiv: 1610.07934
URI: http://arxiv.org/abs/1610.07934
DOI: 10.1103/PhysRevD.95.044026
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Titel: Physical Review D
  Andere : Phys. Rev. D.
Genre der Quelle: Zeitschrift
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Ort, Verlag, Ausgabe: Lancaster, Pa. : American Physical Society
Seiten: - Band / Heft: 95 (4) Artikelnummer: 044026 Start- / Endseite: - Identifikator: ISSN: 0556-2821
CoNE: /journals/resource/111088197762258