Classical gravitational scattering at $\mathcal{O}(G^{2} S_{1}^{\infty} S_{2}^{\infty})$
Abstract
We calculate the scattering of two rotating objects with the linear-in-curvature spin-induced multipoles of Kerr black holes at and all orders in the spins of both objects. This is done including the complete set of contact terms potentially relevant to Kerr-black-hole scattering at . As such, Kerr black holes should be described by this scattering amplitude for a specific choice of values for the contact-term coefficients. The inclusion of all potential contact terms means this amplitude allows for a comprehensive search for structures emerging for certain values of the coefficients, and hence special properties that might be exhibited by Kerr-black-hole scattering. Our result can also act as a template for comparison for future computations of classical gravitational high-spin scattering.
Cite
@article{arxiv.2304.13740,
title = {Classical gravitational scattering at $\mathcal{O}(G^{2} S_{1}^{\infty} S_{2}^{\infty})$},
author = {Rafael Aoude and Kays Haddad and Andreas Helset},
journal= {arXiv preprint arXiv:2304.13740},
year = {2023}
}
Comments
16 pages