Phase transitions in self-gravitating systems and bacterial populations with a screened attractive potential
arXiv:1001.1942 · doi:10.1103/PhysRevE.81.051103
Abstract
We consider a system of particles interacting via a screened Newtonian potential and study phase transitions between homogeneous and inhomogeneous states in the microcanonical and canonical ensembles. Like for other systems with long-range interactions, we obtain a great diversity of microcanonical and canonical phase transitions depending on the dimension of space and on the importance of the screening length. We also consider a system of particles in Newtonian interaction in the presence of a ``neutralizing background''. By a proper interpretation of the parameters, our study describes (i) self-gravitating systems in a cosmological setting, and (ii) chemotaxis of bacterial populations in the original Keller-Segel model.
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- Instability of a uniformly collapsing cloud of classical and quantum self-gravitating Brownian particles
- Inhomogeneous Tsallis distributions in the HMF model
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- Random transitions described by the stochastic Smoluchowski-Poisson system and by the stochastic Keller-Segel model
- Thermodynamics of the HMF model with a magnetic field
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