Flux-balance laws in scalar self-force theory
Alexander M. Grant, Jordan Moxon

TL;DR
This paper develops a new method using symplectic currents to derive flux-balance laws for all constants of motion, including the Carter constant, in scalar self-force theory within Kerr spacetime.
Contribution
It introduces a novel approach employing symplectic currents and symmetry operators to derive flux-balance laws for all constants of motion in Kerr spacetime.
Findings
Derived flux-balance laws for all constants of motion in Kerr spacetime.
Presented a new approach using symplectic currents and symmetry operators.
Focused on scalar self-force, with implications for gravitational case.
Abstract
The motion of a radiating point particle can be represented by a series of geodesics whose "constants" of motion evolve slowly with time. The evolution of these constants of motion can be determined directly from the self-force equations of motion. In the presence of spacetime symmetries, the situation simplifies: there exist not only constants of motion conjugate to these symmetries, but also conserved currents whose fluxes can be used to determine their evolution. Such a relationship between point-particle motion and fluxes of conserved currents is a flux-balance law. However, there exist constants of motion that are not related to spacetime symmetries, the most notable example of which is the Carter constant in the Kerr spacetime. In this paper, we first present a new approach to flux-balance laws for spacetime symmetries, using the techniques of symplectic currents and symmetry…
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Taxonomy
TopicsAstrophysical Phenomena and Observations · Geophysics and Sensor Technology · Pulsars and Gravitational Waves Research
