Metric perturbations from eccentric orbits on a Schwarzschild black hole: I. Odd-parity Regge-Wheeler to Lorenz gauge transformation and two new methods to circumvent the Gibbs phenomenon
Seth Hopper, Charles R. Evans

TL;DR
This paper develops new frequency domain methods to accurately compute odd-parity metric perturbations caused by eccentric orbits around Schwarzschild black holes, overcoming Gibbs phenomenon issues.
Contribution
It introduces two novel techniques, partial annihilator and extended particular solutions, to transfer frequency domain solutions to the time domain without Gibbs artifacts.
Findings
Successfully computed odd-parity gauge generator and metric perturbations.
Demonstrated effectiveness of new methods in avoiding Gibbs phenomenon.
Laid groundwork for future even-parity perturbation calculations.
Abstract
We calculate the odd-parity, radiative () parts of the metric perturbation in Lorenz gauge caused by a small compact object in eccentric orbit about a Schwarzschild black hole. The Lorenz gauge solution is found via gauge transformation from a corresponding one in Regge-Wheeler gauge. Like the Regge-Wheeler gauge solution itself, the gauge generator is computed in the frequency domain and transferred to the time domain. The wave equation for the gauge generator has a source with a compact, moving delta-function term and a discontinuous non-compact term. The former term allows the method of extended homogeneous solutions to be applied (which circumvents the Gibbs phenomenon). The latter has required the development of new means to use frequency domain methods and yet be able to transfer to the time domain while avoiding Gibbs problems. Two new methods are developed to achieve…
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