Critical dynamics of self-gravitating Langevin particles and bacterial populations

TL;DR

This paper investigates the critical collapse dynamics of self-gravitating Langevin particles and bacterial populations modeled by generalized Smoluchowski-Poisson and Keller-Segel systems, revealing phase transitions and analogies with astrophysical objects.

Contribution

It extends the understanding of critical phenomena in these models, especially at the critical polytropic index, and draws parallels with astrophysical and biological systems.

Findings

Existence of a critical temperature and mass at the polytropic index n_3.

Collapse leads to a Dirac peak with a finite mass fraction.

Analogies between bacterial population collapse and white dwarf star limits.

Abstract

We study the critical dynamics of the generalized Smoluchowski-Poisson system (for self-gravitating Langevin particles) or generalized Keller-Segel model (for the chemotaxis of bacterial populations). These models [Chavanis & Sire, PRE, 69, 016116 (2004)] are based on generalized stochastic processes leading to the Tsallis statistics. The equilibrium states correspond to polytropic configurations with index $n$ similar to polytropic stars in astrophysics. At the critical index $n_{3}=d/(d-2)$ (where $d\ge 2$ is the dimension of space), there exists a critical temperature $\Theta_{c}$ (for a given mass) or a critical mass $M_{c}$ (for a given temperature). For $\Theta>\Theta_{c}$ or $M<M_{c}$ the system tends to an incomplete polytrope confined by the box (in a bounded domain) or evaporates (in an unbounded domain). For $\Theta<\Theta_{c}$ or $M>M_{c}$ the system collapses and forms, in a finite time, a Dirac peak containing a finite fraction $M_c$ of the total mass surrounded by a halo. This study extends the critical dynamics of the ordinary Smoluchowski-Poisson system and Keller-Segel model in $d=2$ corresponding to isothermal configurations with $n_{3}\to +\infty$. We also stress the analogy between the limiting mass of white dwarf stars (Chandrasekhar's limit) and the critical mass of bacterial populations in the generalized Keller-Segel model of chemotaxis.