Bifurcation from the Kurth solution in galactic dynamics
Markus Kunze, Rafael Ortega
TL;DR
The paper analyzes the nonlinear gravitational Vlasov-Poisson system near the Kurth equilibrium by constructing an explicit, infinite-dimensional family of weak static states $f_\Gamma$ that share the Kurth density $\rho_{\mathrm{Kurth}}$. It recasts the uniform-density constraint as an Abel-type integral equation for a profile $\varphi$, solving it via a one-dimensional operator framework involving $I^{1/2}$, $K_\Gamma$, and $S_\Gamma$ and obtaining a corresponding $\Phi_\Gamma$. The authors prove $f_\Gamma\to f_{\mathrm{Kurth}}$ in $L^1$ as $\Gamma\to1$, and each static state is surrounded by time-periodic weak solutions, revealing a rich bifurcation structure. By convexity, these equilibria lead to an infinite-dimensional continuum of steady states, all with the same density and with associated periodic perturbations, highlighting a large abundance of equilibria near the Kurth state and offering potential links to Osipkov-Merritt models.
Abstract
It will be shown that there exists an infinite-dimensional continuum ${\cal C}$ of weak static solutions of the Vlasov-Poisson system that bifurcates from the Kurth solution. Each $f_\ast\in {\cal C}$ has the charge density $ρ_{f_\ast}=ρ_{\rm Kurth}$, and (like the Kurth solution itself) each $f_\ast$ is surrounded by time-periodic weak solutions.
