Propagation Estimates for the Boson Star Equation
Sébastien Breteaux, Jérémy Faupin, Viviana Grasselli
TL;DR
This work studies propagation for the boson-star equation $i\partial_t\psi=(\langle\nabla\rangle+w*|\psi|^2)\psi$ in $\mathbb{R}^d$, addressing how fast the quantum state can disperse for general two-body potentials $w$ decomposed as a finite signed measure plus a bounded function. It develops a comprehensive well-posedness theory (local and global) in varied function spaces (including Lorentz and weighted Sobolev spaces) and proves sharp maximal-velocity bounds that match the light-speed limit with exponentially small remainders. In the short-range setting, the paper establishes scattering to free dynamics, wave-operator invertibility in weighted spaces, and asymptotic phase-space propagation and minimal-velocity estimates, linking long-time behavior to the momentum of scattering states. The results provide a rigorous, quantitative picture of propagation and dispersive decay for pseudo-relativistic boson stars, with implications for mean-field limits and gravitational models of boson stars. The methods combine fixed-point, dispersive, Lorentz-space inequalities, and modern ASTLO/phase-space techniques to handle nonlinear, nonlocal interactions and time-dependent effective Hamiltonians. The work thus advances understanding of causality-like propagation and long-time scattering in nonlinear, nonlocal quantum dynamics.
Abstract
We consider the boson star equation with a general two-body interaction potential $w$ and initial data $ψ_0$ in a Sobolev space. Under general assumptions on $w$, namely that $w$ decomposes as a sum of a finite, signed measure and an essentially bounded function, we prove that the (local in time) solution cannot propagate faster than the speed of light, up to a sharp exponentially small remainder term. If $w$ is short-range and $ψ_0$ is regular and small enough, we prove in addition asymptotic phase-space propagation estimates and minimal velocity estimates for the (global in time) solution, depending on the momentum of the scattering state associated to $ψ_0$.
