It's not ${\sigma }_8$ : constraining the non-linear matter power spectrum with the Dark Energy Survey Year-5 supernova sample

The weak gravitational lensing magnification of Type Ia supernovae (SNe Ia) is sensitive to the matter power spectrum on scales $k>1h$ Mpc${}^{-1}$, making it unwise to interpret SNe Ia lensing in terms of power on linear scales. We compute the probability density function of SNe Ia magnification as a function of standard cosmological parameters, plus an empirical parameter $A_{\mathrm{m}\mathrm{o}\mathrm{d}}$ which describes the suppression or enhancement of matter power on non-linear scales compared to a cold dark matter only model. While baryons are expected to enhance power on the scales relevant to SN Ia lensing, other physics such as neutrino masses or non-standard dark matter may suppress power. Using the Dark Energy Survey Year-5 sample, we find $A_{\mathrm{m}\mathrm{o}\mathrm{d}}=0.77_{-0.40}^{+0.69}$ (68% credible interval around the median). Although the median is consistent with unity there are hints of power suppression, with $A_{\mathrm{m}\mathrm{o}\mathrm{d}}<1.09$ at 68% credibility.