English
 
Help Privacy Policy Disclaimer
  Advanced SearchBrowse

Item

ITEM ACTIONSEXPORT
  Gravitational Spin-Orbit Coupling through Third-Subleading Post-Newtonian Order: From First-Order Self-Force to Arbitrary Mass Ratios

Antonelli, A., Kavanagh, C., Khalil, M., Steinhoff, J., & Vines, J. (2020). Gravitational Spin-Orbit Coupling through Third-Subleading Post-Newtonian Order: From First-Order Self-Force to Arbitrary Mass Ratios. Physical Review Letters, 125: 011103. doi:10.1103/PhysRevLett.125.011103.

Item is

Files

show Files
hide Files
:
2003.11391.pdf (Preprint), 643KB
Name:
2003.11391.pdf
Description:
File downloaded from arXiv at 2020-11-24 13:24
OA-Status:
Visibility:
Public
MIME-Type / Checksum:
application/pdf / [MD5]
Technical Metadata:
Copyright Date:
-
Copyright Info:
-
:
10.1103_PhysRevLett.125.011103.pdf (Publisher version), 351KB
Name:
10.1103_PhysRevLett.125.011103.pdf
Description:
Open Access
OA-Status:
Visibility:
Public
MIME-Type / Checksum:
application/pdf / [MD5]
Technical Metadata:
Copyright Date:
-
Copyright Info:
-

Locators

show

Creators

show
hide
 Creators:
Antonelli, Andrea1, Author           
Kavanagh, Chris1, Author           
Khalil, Mohammed1, Author           
Steinhoff, Jan1, Author           
Vines, Justin1, Author           
Affiliations:
1Astrophysical and Cosmological Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, ou_1933290              

Content

show
hide
Free keywords: General Relativity and Quantum Cosmology, gr-qc
 Abstract: Exploiting simple yet remarkable properties of relativistic gravitational
scattering, we use first-order self-force (linear-in-mass-ratio) results to
obtain arbitrary-mass-ratio results for the complete third-subleading
post-Newtonian (4.5PN) corrections to the spin-orbit sector of spinning-binary
conservative dynamics, for generic (bound or unbound) orbits and spin
orientations. We thereby improve important ingredients of models of
gravitational waves from spinning binaries, and we demonstrate the improvement
in accuracy by comparing against aligned-spin numerical simulations of binary
black holes.

Details

show
hide
Language(s):
 Dates: 2020-03-252020-06-192020
 Publication Status: Issued
 Pages: 8 pages, 2 figures. v2: matches version accepted in PRL
 Publishing info: -
 Table of Contents: -
 Rev. Type: -
 Identifiers: arXiv: 2003.11391
DOI: 10.1103/PhysRevLett.125.011103
 Degree: -

Event

show

Legal Case

show

Project information

show

Source 1

show
hide
Title: Physical Review Letters
  Abbreviation : Phys. Rev. Lett.
Source Genre: Journal
 Creator(s):
Affiliations:
Publ. Info: Woodbury, N.Y. : American Physical Society
Pages: - Volume / Issue: 125 Sequence Number: 011103 Start / End Page: - Identifier: ISSN: 0031-9007
CoNE: https://pure.mpg.de/cone/journals/resource/954925433406_1