English
 
Help Privacy Policy Disclaimer
  Advanced SearchBrowse

Item

ITEM ACTIONSEXPORT

Released

Journal Article

Gravitational spin-orbit and aligned spin1-spin2 couplings through third-subleading post-Newtonian orders

MPS-Authors
/persons/resource/persons230286

Antonelli,  Andrea
Astrophysical and Cosmological Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

/persons/resource/persons231048

Kavanagh,  Chris
Astrophysical and Cosmological Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

/persons/resource/persons231050

Khalil,  Mohammed
Astrophysical and Cosmological Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

/persons/resource/persons144501

Steinhoff,  Jan
Astrophysical and Cosmological Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

/persons/resource/persons192129

Vines,  Justin
Astrophysical and Cosmological Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

External Resource
No external resources are shared
Fulltext (restricted access)
There are currently no full texts shared for your IP range.
Fulltext (public)

2010.02018.pdf
(Preprint), 2MB

PhysRevD.102.124024.pdf
(Publisher version), 738KB

Supplementary Material (public)
There is no public supplementary material available
Citation

Antonelli, A., Kavanagh, C., Khalil, M., Steinhoff, J., & Vines, J. (2020). Gravitational spin-orbit and aligned spin1-spin2 couplings through third-subleading post-Newtonian orders. Physical Review D, 102(12): 124024. doi:10.1103/PhysRevD.102.124024.


Cite as: https://hdl.handle.net/21.11116/0000-0007-735E-F
Abstract
The study of scattering encounters continues to provide new insights into the
general relativistic two-body problem. The local-in-time conservative dynamics
of an aligned-spin binary, for both unbound and bound orbits, is fully encoded
in the gauge-invariant scattering-angle function, which is most naturally
expressed in a post-Minkowskian (PM) expansion, and which exhibits a remarkably
simple dependence on the masses of the two bodies (in terms of appropriate
geometric variables). This dependence links the PM and small-mass-ratio
approximations, allowing gravitational self-force results to determine new
post-Newtonian (PN) information to all orders in the mass ratio. In this paper,
we exploit this interplay between relativistic scattering and self-force theory
to obtain the third-subleading (4.5PN) spin-orbit dynamics for generic spins,
and the third-subleading (5PN) spin$_1$-spin$_2$ dynamics for aligned spins. We
further implement these novel PN results in an effective-one-body framework,
and demonstrate the improvement in accuracy by comparing against
numerical-relativity simulations.