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Osculating orbits in Schwarzschild spacetime, with an application to extreme mass-ratio inspirals

Osculating orbits in Schwarzschild spacetime, with an application to extreme mass-ratio inspirals
Osculating orbits in Schwarzschild spacetime, with an application to extreme mass-ratio inspirals
We present a method to integrate the equations of motion that govern bound, accelerated orbits in Schwarzschild spacetime. At each instant the true worldline is assumed to lie tangent to a reference geodesic, called an osculating orbit, such that the worldline evolves smoothly from one such geodesic to the next. Because a geodesic is uniquely identified by a set of constant orbital elements, the transition between osculating orbits corresponds to an evolution of the elements. In this paper we derive the evolution equations for a convenient set of orbital elements, assuming that the force acts only within the orbital plane; this is the only restriction that we impose on the formalism, and we do not assume that the force must be small. As an application of our method, we analyze the relative motion of two massive bodies, assuming that one body is much smaller than the other. Using the hybrid Schwarzschild/post-Newtonian equations of motion formulated by Kidder, Will, and Wiseman, we treat the unperturbed motion as geodesic in a Schwarzschild spacetime with a mass parameter equal to the system’s total mass. The force then consists of terms that depend on the system’s reduced mass. We highlight the importance of conservative terms in this force, which cause significant long-term changes in the time dependence and phase of the relative orbit. From our results we infer some general limitations of the radiative approximation to the gravitational self-force, which uses only the dissipative terms in the force.
1550-7998
044013-[18pp]
Pound, Adam
5aac971a-0e07-4383-aff0-a21d43103a70
Poisson, Eric
c8aa275d-6a5f-4633-9f85-3cb051641e0c
Pound, Adam
5aac971a-0e07-4383-aff0-a21d43103a70
Poisson, Eric
c8aa275d-6a5f-4633-9f85-3cb051641e0c

Pound, Adam and Poisson, Eric (2008) Osculating orbits in Schwarzschild spacetime, with an application to extreme mass-ratio inspirals. Physical Review D, 77 (4), 044013-[18pp]. (doi:10.1103/PhysRevD.77.044013).

Record type: Article

Abstract

We present a method to integrate the equations of motion that govern bound, accelerated orbits in Schwarzschild spacetime. At each instant the true worldline is assumed to lie tangent to a reference geodesic, called an osculating orbit, such that the worldline evolves smoothly from one such geodesic to the next. Because a geodesic is uniquely identified by a set of constant orbital elements, the transition between osculating orbits corresponds to an evolution of the elements. In this paper we derive the evolution equations for a convenient set of orbital elements, assuming that the force acts only within the orbital plane; this is the only restriction that we impose on the formalism, and we do not assume that the force must be small. As an application of our method, we analyze the relative motion of two massive bodies, assuming that one body is much smaller than the other. Using the hybrid Schwarzschild/post-Newtonian equations of motion formulated by Kidder, Will, and Wiseman, we treat the unperturbed motion as geodesic in a Schwarzschild spacetime with a mass parameter equal to the system’s total mass. The force then consists of terms that depend on the system’s reduced mass. We highlight the importance of conservative terms in this force, which cause significant long-term changes in the time dependence and phase of the relative orbit. From our results we infer some general limitations of the radiative approximation to the gravitational self-force, which uses only the dissipative terms in the force.

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Published date: 8 February 2008
Organisations: Applied Mathematics

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Local EPrints ID: 339869
URI: http://eprints.soton.ac.uk/id/eprint/339869
ISSN: 1550-7998
PURE UUID: f4e401cf-bc00-460a-87ed-4aa664074d9b
ORCID for Adam Pound: ORCID iD orcid.org/0000-0001-9446-0638

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Date deposited: 31 May 2012 16:00
Last modified: 15 Mar 2024 03:41

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Author: Adam Pound ORCID iD
Author: Eric Poisson

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