Cosmological simulations of mixed ultralight dark matter

The era of precision cosmology allows us to test the composition of the dark matter. Mixed ultralight or fuzzy dark matter (FDM) is a cosmological model with dark matter composed of a combination of particles of mass m <= 10-20 eV, with an astrophysical de Broglie wavelength, and particles with a negligible wavelength sharing the properties of cold dark matter (CDM). In this work, we simulate cosmological volumes with a dark matter wave function for the ultralight component coupled gravitationally to CDM particles. We investigate the impact of a mixture of CDM and FDM in various proportions (0%, 1%, 10%, 50%, 100%) and for ultralight particle masses ranging over five orders of magnitude (2.5x 10-25 eV-2.5 x 10-21 eV). To track the evolution of density perturbations in the nonlinear regime, we adapt the simulation code AxioNyx to solve the CDM dynamics coupled to a FDM wave function obeying the Schrodinger-Poisson equations. We obtain the nonlinear power spectrum and study the impact of the wave effects on the growth of structure on different scales. We confirm that the steady-state solution of the Schrodinger-Poisson system holds at the center of halos in the presence of a CDM component when it composes 50% or less of the dark matter but find no stable density core when the FDM accounts for 10% or less of the dark matter. We implement a modified friends -of -friends halo finder and find good agreement between the observed halo abundance and the predictions from the adapted halo model AxionHMCode.