Abstract
Second-order self-force computations, which will be essential in modeling extreme-mass-ratio inspirals, involve two major new difficulties that were not present at first order. One is the problem of large scales, discussed in Pound [Phys. Rev. D 92, 104047 (2015)]. Here we discuss the second difficulty, which occurs instead on small scales: if we expand the field equations in spherical harmonics, then because the first-order field contains a singularity, we require an arbitrarily large number of first-order modes to accurately compute even a single second-order mode. This is a generic feature of nonlinear field equations containing singularities, allowing us to study it in the simple context of a scalar toy model in flat space. Using that model, we illustrate the problem and demonstrate a robust strategy for overcoming it.
Cite
CITATION STYLE
Miller, J., Wardell, B., & Pound, A. (2016). Second-order perturbation theory: The problem of infinite mode coupling. Physical Review D, 94(10). https://doi.org/10.1103/PhysRevD.94.104018
Register to see more suggestions
Mendeley helps you to discover research relevant for your work.