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Gravitational collapse of a Brownian gas

Tom 66 / 2004

Clément Sire, Pierre-Henri Chavanis Banach Center Publications 66 (2004), 287-304 MSC: 92-xx, 85-xx, 35-xx, 82-xx. DOI: 10.4064/bc66-0-20

Streszczenie

We investigate a model describing the dynamics of a gas of self-gravitating Brownian particles. This model can also have applications for the chemotaxis of bacterial populations. We focus here on the collapse phase obtained at sufficiently low temperature//energy and on the post-collapse regime following the singular time where the central density diverges. Several analytical results are illustrated by numerical simulations.

Autorzy

  • Clément SireLaboratoire de Physique Théorique (UMR 5152 du CNRS)
    Université
    Paul Sabatier
    118, route de Narbonne
    31062 Toulouse Cedex 4, France
    e-mail
  • Pierre-Henri ChavanisLaboratoire de Physique Théorique (UMR 5152 du CNRS)
    Université
    Paul Sabatier
    118, route de Narbonne
    31062 Toulouse Cedex 4, France
    e-mail

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