Abstract
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 (2.5×10-25 eV-2.5×10-21 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 Schrödinger-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 Schrödinger-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.
| Original language | English |
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| Article number | 043507 |
| Journal | Physical Review D |
| Volume | 109 |
| Issue number | 4 |
| DOIs | |
| Publication status | Published - 15 Feb 2024 |