Simple, efficient method of calculating the Detweiler-Whiting singular field to very high order
Simple, efficient method of calculating the Detweiler-Whiting singular field to very high order
Most self-force calculations rely, in one way or another, on representations of a particle's Detweiler-Whiting singular field. We present a simple method of calculating the singular field to high order in a local expansion in powers of distance from the particle. As a demonstration, we compute the singular field to 14th order in distance, 10 orders beyond the previous state of the art, in the simple case of a scalar charge in circular orbit around a Schwarzschild black hole. We provide the result in both a four-dimensional form and a decomposed form suitable for use in an m-mode puncture scheme. Our method should have applications in overcoming bottlenecks in current self-force calculations at both first and second orders in perturbation theory.
Bourg, Patrick
7243e5d7-edd5-4066-89d3-f8357dbde8f8
Pound, Adam
5aac971a-0e07-4383-aff0-a21d43103a70
Upton, Samuel D.
f0ff8ac2-2ef0-4a99-b2d6-e55772f34dcf
Panosso Macedo, Rodrigo
9abb6bca-fc8d-4038-bc79-225d0bae4c00
4 October 2024
Bourg, Patrick
7243e5d7-edd5-4066-89d3-f8357dbde8f8
Pound, Adam
5aac971a-0e07-4383-aff0-a21d43103a70
Upton, Samuel D.
f0ff8ac2-2ef0-4a99-b2d6-e55772f34dcf
Panosso Macedo, Rodrigo
9abb6bca-fc8d-4038-bc79-225d0bae4c00
Bourg, Patrick, Pound, Adam, Upton, Samuel D. and Panosso Macedo, Rodrigo
(2024)
Simple, efficient method of calculating the Detweiler-Whiting singular field to very high order.
Physical Review D, 110 (8), [084007].
(doi:10.1103/PhysRevD.110.084007).
Abstract
Most self-force calculations rely, in one way or another, on representations of a particle's Detweiler-Whiting singular field. We present a simple method of calculating the singular field to high order in a local expansion in powers of distance from the particle. As a demonstration, we compute the singular field to 14th order in distance, 10 orders beyond the previous state of the art, in the simple case of a scalar charge in circular orbit around a Schwarzschild black hole. We provide the result in both a four-dimensional form and a decomposed form suitable for use in an m-mode puncture scheme. Our method should have applications in overcoming bottlenecks in current self-force calculations at both first and second orders in perturbation theory.
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Submitted date: 17 April 2024
Accepted/In Press date: 16 August 2024
Published date: 4 October 2024
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© 2024 American Physical Society.
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Local EPrints ID: 494082
URI: http://eprints.soton.ac.uk/id/eprint/494082
ISSN: 2470-0010
PURE UUID: e3ca1089-3ae5-459c-b689-d466c30b348a
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Date deposited: 23 Sep 2024 16:41
Last modified: 12 Nov 2024 03:15
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Author:
Patrick Bourg
Author:
Samuel D. Upton
Author:
Rodrigo Panosso Macedo
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