English
 
User Manual Privacy Policy Disclaimer Contact us
  Advanced SearchBrowse

Item

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

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.

Item is

Basic

show hide
Item Permalink: http://hdl.handle.net/11858/00-001M-0000-0023-F7C1-4 Version Permalink: http://hdl.handle.net/11858/00-001M-0000-0024-2661-8
Genre: Journal Article

Files

show Files
hide Files
:
1104.5659.pdf (Preprint), 423KB
Name:
1104.5659.pdf
Description:
File downloaded from arXiv at 2014-10-21 11:22
Visibility:
Public
MIME-Type / Checksum:
application/pdf / [MD5]
Technical Metadata:
Copyright Date:
-
Copyright Info:
-
:
PhysRevD.84.064041.pdf (Any fulltext), 510KB
Name:
PhysRevD.84.064041.pdf
Description:
-
Visibility:
Public
MIME-Type / Checksum:
application/pdf / [MD5]
Technical Metadata:
Copyright Date:
-
Copyright Info:
-
License:
-

Locators

show

Creators

show
hide
 Creators:
Blanchet, Luc1, Author
Buonanno, A.2, 3, Author              
Faye, Guillaume, Author
Affiliations:
1IAP, ou_persistent22              
2Astrophysical and Cosmological Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, ou_1933290              
3University of Maryland, ou_persistent22              

Content

show
hide
Free keywords: General Relativity and Quantum Cosmology, gr-qc
 Abstract: 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.

Details

show
hide
Language(s):
 Dates: 2011-04-292011-09-122011
 Publication Status: Published in print
 Pages: Minor corrections. To be published in Physical Review D
 Publishing info: -
 Table of Contents: -
 Rev. Method: -
 Identifiers: arXiv: 1104.5659
URI: http://arxiv.org/abs/1104.5659
DOI: 10.1103/PhysRevD.84.064041
 Degree: -

Event

show

Legal Case

show

Project information

show

Source 1

show
hide
Title: Physical Review D
  Other : Phys. Rev. D.
Source Genre: Journal
 Creator(s):
Affiliations:
Publ. Info: Lancaster, Pa. : American Physical Society
Pages: - Volume / Issue: 84 (6) Sequence Number: 064041 Start / End Page: - Identifier: ISSN: 0556-2821
CoNE: /journals/resource/111088197762258