On the pressure of collisionless particle fluids. The case of solids settling in disks

Abstract

Aims. Collections of dust, grains, and planetesimals are often treated as a pressureless fluid. We study the validity of neglecting the pressure of such a fluid by computing it exactly for the case of particles settling in a disk. Methods. We solve a modified collisionless Boltzmann equation for the particles and compute the corresponding moments of the phase space distribution: density, momentum, and pressure. Results. We find that whenever the Stokes number, defined as the ratio of the gas drag timescale to the orbital timescale, is more than 1/2, the particle fluid cannot be considered as pressureless. While we show it only in the simple case of particles settling in a laminar disk, this property is likely to remain true for most flows, including turbulent flows.

Accepted for publication as a research note in Astronomy and Astrophysics. Language edited

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• Three-Dimensional Dust Stirring by a Giant Planet Embedded in a Protoplanetary Disk
• Magnetic clumping of charged dust in the dense interstellar medium