Instability of a uniformly collapsing cloud of classical and quantum self-gravitating Brownian particles
Pierre-Henri Chavanis

TL;DR
This paper analyzes the stability and nonlinear evolution of a collapsing cloud of self-gravitating particles, comparing classical and quantum models, and introduces new equations and criteria for structure formation in such systems.
Contribution
It derives a new density contrast evolution equation in a collapsing frame and compares stability criteria with classical approaches, also extending to quantum Bose-Einstein condensates.
Findings
Different stability criteria from Jeans analysis.
Self-similar solutions for nonlinear regime.
Quantum effects modeled by nonlinear mean field equations.
Abstract
We study the growth of perturbations in a uniformly collapsing cloud of self-gravitating Brownian particles. This problem shares analogies with the formation of large-scale structures in a universe experiencing a "big-crunch" or with the formation of stars in a molecular cloud experiencing gravitational collapse. Starting from the barotropic Smoluchowski-Poisson system, we derive a new equation describing the evolution of the density contrast in the comoving (collapsing) frame. This equation can serve as a prototype to study the process of self-organization in complex media with structureless initial conditions. We solve this equation analytically in the linear regime and compare the results with those obtained by using the "Jeans swindle" in a static medium. The stability criteria, as well as the laws for the time evolution of the perturbations, are different. The Jeans criterion is…
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