Extremal Black Holes as Relativistic Systems with Kepler Dynamics

TL;DR

This paper demonstrates that extremal black hole binaries can exhibit Kepler-like elliptical orbits within relativistic Hamiltonian frameworks, extending classical orbital dynamics to relativistic black hole systems.

Contribution

It establishes the existence of Kepler-like dynamics in relativistic black hole binaries with electric charge and scalar hair, using Hamiltonian methods up to high post-Newtonian orders.

Findings

Kepler-like Hamiltonians exist for extremal black hole binaries.

Explicit canonical transformations relate these Hamiltonians to the classical Kepler problem.

Kepler-like dynamics hold for arbitrary mass ratios and in the test-mass limit.

Abstract

The recent detection of gravitational waves emanating from inspiralling black hole binaries has triggered a renewed interest in the dynamics of relativistic two-body systems. The conservative part of the latter are given by Hamiltonian systems obtained from so called post-Newtonian expansions of the general relativistic description of black hole binaries. In this paper we study the general question of whether there exist relativistic binaries that display Kepler-like dynamics with elliptical orbits. We show that an orbital equivalence to the Kepler problem indeed exists for relativistic systems with a Hamiltonian of a Kepler-like form. This form is realised by extremal black holes with electric charge and scalar hair to at least first order in the post-Newtonian expansion for arbitrary mass ratios and to all orders in the post-Newtonian expansion in the test-mass limit of the binary. Moreover, to fifth post-Newtonian order, we show that Hamiltonians of the Kepler-like form can be related explicitly through a canonical transformation and time reparametrization to the Kepler problem, and that all Hamiltonians conserving a Laplace-Runge-Lenz-like vector are related in this way to Kepler.