2004
DOI: 10.1103/physreve.69.066109
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Postcollapse dynamics of self-gravitating Brownian particles and bacterial populations

Abstract: We address the postcollapse dynamics of a self-gravitating gas of Brownian particles in D dimensions in both canonical and microcanonical ensembles. In the canonical ensemble, the postcollapse evolution is marked by the formation of a Dirac peak with increasing mass. The density profile outside the peak evolves self-similarly with decreasing central density and increasing core radius. In the microcanonical ensemble, the postcollapse regime is marked by the formation of a "binarylike" structure surrounded by an… Show more

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Cited by 57 publications
(47 citation statements)
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“…If the free energy possesses several local minima, the choice of the equilibrium state depends on a complicated notion of basin of attraction (for self-gravitating Brownian particles [ 28 , 29 ] the free energy is not bounded from below. In that case, the system can either relax towards a local minimum of free energy F at fixed mass – when it exists – or collapse to a Dirac peak [ 30 ], leading to a divergence of the free energy ). According to the preceding results, we conclude that dynamical stability with respect to the generalized mean field Smoluchowski equation and generalized thermodynamical stability in the canonical ensemble coincide.…”
Section: Macroscopic Description: Average Dynamicsmentioning
confidence: 99%
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“…If the free energy possesses several local minima, the choice of the equilibrium state depends on a complicated notion of basin of attraction (for self-gravitating Brownian particles [ 28 , 29 ] the free energy is not bounded from below. In that case, the system can either relax towards a local minimum of free energy F at fixed mass – when it exists – or collapse to a Dirac peak [ 30 ], leading to a divergence of the free energy ). According to the preceding results, we conclude that dynamical stability with respect to the generalized mean field Smoluchowski equation and generalized thermodynamical stability in the canonical ensemble coincide.…”
Section: Macroscopic Description: Average Dynamicsmentioning
confidence: 99%
“…for all perturbations δρ that conserve mass. Using Equation (30), the condition of thermodynamical stability can also be written as…”
Section: Thermodynamical Stabilitymentioning
confidence: 99%
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“…The Smoluchowski-Poisson system has been studied in [16,[58][59][60][61][62]. The screened Smoluchowski-Poisson system and the modified Smoluchowski-Poisson system have been studied in [63,64].…”
Section: Self-gravitating Brownian Particlesmentioning
confidence: 99%
“…The local well-posedness of (1.1)-(1.6) has been investigated in [15] and [10]. Explicit solutions describing the pre-collapse and post-collapse dynamics have been obtained in [7,8,17,18] for a spherically symmetric distribution of matter.…”
Section: Introduction Let B Denote the Open Ball In Rmentioning
confidence: 99%