Effective Dynamics for Weakly Interacting Bosons in an Iterated High-Density Thermodynamic Limit
Daniele Ferretti, Kalle Koskinen
TL;DR
This work analyzes the time evolution of a weakly interacting Bose gas on a 3D torus in a high-density thermodynamic limit with coupling scaled as $1/\rho$. Adopting a grand canonical Fock-space framework and Weyl coherence, it derives a fluctuation dynamics around a time-dependent Hartree condensate and proves that, for each fixed time in a finite interval, the one-particle density matrix converges to the Hartree condensate projector in the iterated limit $L\to\infty$ followed by $\rho\to\infty$. The convergence is quantified in trace (and Hilbert-Schmidt) norm, with a rate governed by the initial quasi-vacuum’s tail and energy quasi-self-consistency, under quasi-complete Bose-Einstein condensation. The results establish a rigorous link between microscopic many-body dynamics and nonlinear Hartree evolution in a thermodynamic torus setting, including controlled fluctuations and energy consistency, and highlight the importance of limit ordering in deriving effective condensate dynamics. Overall, the paper advances mathematical understanding of Bose gases in the high-density regime by providing a robust, quantitative derivation of Hartree dynamics as the emergent macroscopic description.
Abstract
We study the time evolution of weakly interacting Bose gases on a three-dimensional torus of arbitrary volume. The coupling constant is supposed to be inversely proportional to the density, which is considered to be large and independent of the particle number. We take into account a class of initial states exhibiting quasi-complete Bose-Einstein condensation. For each fixed time in a finite interval, we prove the convergence of the one-particle reduced density matrix towards the projection onto the normalised order parameter describing the condensate - evolving according to the Hartree equation - in the iterated limit where the volume (and therefore the particle number), and subsequently the density go to infinity. The rate of convergence depends only on the density and on the decay of both the expected number of particles and the energy of the initial quasi-vacuum state.
