Deutsch
 
Hilfe Datenschutzhinweis Impressum
  DetailsucheBrowse

Datensatz

DATENSATZ AKTIONENEXPORT
Zur Ablage hinzufügen
  FreigabegeschichteDetailsÜbersicht

Freigegeben
Zeitschriftenartikel

Tail-induced spin-orbit effect in the gravitational radiation of compact binaries

MPG-Autoren
/persons/resource/persons127862

Buonanno,  A.
Astrophysical and Cosmological Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;
University of Maryland;

Externe Ressourcen
Es sind keine externen Ressourcen hinterlegt
Volltexte (beschränkter Zugriff)
Für Ihren IP-Bereich sind aktuell keine Volltexte freigegeben.
Volltexte (frei zugänglich)

1104.5659.pdf
(Preprint), 423KB

PhysRevD.84.064041.pdf
(beliebiger Volltext), 510KB

Ergänzendes Material (frei zugänglich)
Es sind keine frei zugänglichen Ergänzenden Materialien verfügbar
Zitation

Blanchet, L., Buonanno, A., & Faye, G. (2011). Tail-induced spin-orbit effect in the gravitational radiation of compact binaries. Physical Review D, 84(6): 064041. doi:10.1103/PhysRevD.84.064041.


Zitierlink: https://hdl.handle.net/11858/00-001M-0000-0023-F7C1-4
Zusammenfassung
Gravitational waves contain tail effects which are due to the back-scattering of linear waves in the curved space-time geometry around the source. In this paper we improve the knowledge and accuracy of the two-body inspiraling post-Newtonian (PN) dynamics and gravitational-wave signal by computing the spin-orbit terms induced by tail effects. Notably, we derive those terms at 3PN order in the gravitational-wave energy flux, and 2.5PN and 3PN orders in the wave polarizations. This is then used to derive the spin-orbit tail effects in the phasing through 3PN order. Our results can be employed to carry out more accurate comparisons with numerical-relativity simulations and to improve the accuracy of analytical templates aimed at describing the whole process of inspiral, merger and ringdown.