Resummed Kinetic Field Theory: a model of coupled baryonic and dark matter
Daniel Geiss, Ivan Kostyuk, Robert Lilow, Matthias Bartelmann

TL;DR
This paper extends the Kinetic Field Theory framework to include baryonic matter, enabling analytical modeling of cosmic structure formation involving both dark matter and baryons, and validates it against numerical results.
Contribution
The authors develop a combined KFT and Mesoscopic Particle Hydrodynamics approach to model coupled baryonic and dark matter dynamics in cosmic structure formation.
Findings
Accurately reproduces the suppression of small-scale structure growth.
Matches results from the numerical Boltzmann solver CLASS.
Provides a foundation for nonlinear corrections in future work.
Abstract
We present a new analytical description of cosmic structure formation in a mixture of dark and baryonic matter, using the framework of Kinetic Field Theory (KFT) -- a statistical field theory for classical particle dynamics. So far, KFT has only been able to describe a single type of particles, sufficient to consider structure growth due to the gravitational interactions between dark matter. However, the influence of baryonic gas dynamics becomes increasingly relevant when describing smaller scales. In this paper, we thus demonstrate how to extend the KFT formalism as well as a previously presented resummation scheme towards describing such mixtures of two particle species. Thereby, the gas dynamics of baryons are accounted for using the recently developed model of Mesoscopic Particle Hydrodynamics. Assuming a flat CDM Universe and a simplified model for the thermal gas…
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