Two-fluid dark matter models

TL;DR

This paper explores a two-fluid dark matter model where dark matter consists of two non-interacting fluids with different velocities, leading to anisotropic pressure profiles and potential implications for galaxy rotation curves and cosmology.

Contribution

It introduces a novel two-fluid dark matter model with anisotropic pressures and derives equilibrium equations and velocity profiles, including cosmological implications.

Findings

Density profiles and tangential velocities obtained numerically.

Model isotropizes over large time scales.

Potential to explain galaxy rotation curves.

Abstract

We investigate the possibility that dark matter is a mixture of two non-interacting perfect fluids, with different four-velocities and thermodynamic parameters. The two-fluid model can be described as an effective single anisotropic fluid, with distinct radial and tangential pressures. The basic equations describing the equilibrium structure of the two-fluid dark matter model, and of the tangential velocity of test particles in stable circular orbits, are obtained for the case of a spherically symmetric static geometry. By assuming a non-relativistic kinetic model for the dark matter particles, the density profile and the tangential velocity of the dark matter mixture are obtained by numerically integrating the gravitational field equations. The cosmological implications of the model are also briefly considered, and it is shown that the anisotropic two-fluid model isotropizes in the large time limit.