Constraints on Dark Matter-Dark Energy Scattering from ACT DR6 CMB Lensing
arxiv(2024)
Abstract
The predicted present-day amplitude of matter fluctuations based on cosmic
microwave background (CMB) anisotropy data has sometimes been found discrepant
with more direct measurements of late-time structure. This has motivated many
extensions to the standard cosmological model, including kinetic interactions
between dark matter and dark energy that introduce a drag force slowing the
growth of structure at late times. Exploring this scenario, we develop a model
for quasi-linear scales in the matter power spectrum by calculating the
critical overdensity in the presence of this interaction and a varying dark
energy equation of state. We explicitly avoid modeling or interpretation of
data on non-linear scales in this model (such as use of ΛCDM-calibrated
priors), which would require numerical simulations. We find that the presence
of the drag force hinders halo formation, thus increasing the deviation from
ΛCDM in the mildly non-linear regime. We use CMB lensing observations
from the sixth data release of the Atacama Cosmology Telescope up to L=1250
(in combination with Planck, Sloan Digital Sky Survey, and 6dFGS data) to
derive the strongest constraints to date on the amplitude of the drag term,
finding the dimensionless interaction strength
Γ_DMDE/(H_0ρ_c)<0.831 (2.81) at the 68% (95%)
confidence level. The inclusion of non-linear corrections improves our
constraints by about 35% compared to linear theory. Our results do not exclude
the best-fit values of Γ_DMDE found in previous studies using
information from galaxy weak lensing, though we find no statistical preference
for the dark matter-dark energy kinetic interactions over ΛCDM. We
implement our model in a publicly available fork of the Boltzmann code CLASS at
https://github.com/fmccarthy/Class_DMDE.
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