Self-force calculations with a spinning secondary
Self-force calculations with a spinning secondary
We compute the linear metric perturbation to a Schwarzschild black hole generated by a spinning compact object, specializing to circular equatorial orbits with an (anti-)aligned spin vector. We derive a two-timescale expansion of the field equations, with an attendant waveform-generation framework, that includes all effects through first postadiabatic order, and we use the Regge-Wheeler-Zerilli formalism in the frequency domain to generate waveforms that include the complete effect of the spin on the waveform phase. We perform the calculations using expansions at fixed orbital frequency, increasing the computational efficiency, and simplifying the procedure compared to previous approaches. Finally, we provide the first fully relativistic, first-principles regularization procedure for gauge invariant self-force quantities to linear order in spin. We use this procedure to produce the first strong-field, conservative self-force calculation including the spin of the secondary - computing Detweiler's redshift invariant.
Mathews, Josh
4e56c8a4-1d29-4618-a649-170f677600dd
Pound, Adam
5aac971a-0e07-4383-aff0-a21d43103a70
Wardell, Barry
70b41899-32ac-4585-888b-aaf28fd70ad5
19 April 2022
Mathews, Josh
4e56c8a4-1d29-4618-a649-170f677600dd
Pound, Adam
5aac971a-0e07-4383-aff0-a21d43103a70
Wardell, Barry
70b41899-32ac-4585-888b-aaf28fd70ad5
Mathews, Josh, Pound, Adam and Wardell, Barry
(2022)
Self-force calculations with a spinning secondary.
Physical Review D, 105 (8), [084031].
(doi:10.1103/PhysRevD.105.084031).
Abstract
We compute the linear metric perturbation to a Schwarzschild black hole generated by a spinning compact object, specializing to circular equatorial orbits with an (anti-)aligned spin vector. We derive a two-timescale expansion of the field equations, with an attendant waveform-generation framework, that includes all effects through first postadiabatic order, and we use the Regge-Wheeler-Zerilli formalism in the frequency domain to generate waveforms that include the complete effect of the spin on the waveform phase. We perform the calculations using expansions at fixed orbital frequency, increasing the computational efficiency, and simplifying the procedure compared to previous approaches. Finally, we provide the first fully relativistic, first-principles regularization procedure for gauge invariant self-force quantities to linear order in spin. We use this procedure to produce the first strong-field, conservative self-force calculation including the spin of the secondary - computing Detweiler's redshift invariant.
Text
SpinningSecondary
- Accepted Manuscript
More information
Accepted/In Press date: 25 March 2022
Published date: 19 April 2022
Identifiers
Local EPrints ID: 457507
URI: http://eprints.soton.ac.uk/id/eprint/457507
ISSN: 2470-0010
PURE UUID: 7aceaa80-14e2-425e-932b-40fa48441944
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Date deposited: 09 Jun 2022 17:10
Last modified: 17 Mar 2024 03:27
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Author:
Josh Mathews
Author:
Barry Wardell
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