INEQUALITIES. “In other words, non-baryonic DM is required for perturbations to grow sufficiently from the initial amplitude, as measured from the CMB anisotropies.”(DM = dark matter; CMB = cosmic microwave background).
https://lnkd.in/e6ifiQMn
INEQUALITIES. “In other words, non-baryonic DM is required for perturbations to grow sufficiently from the initial amplitude, as measured from the CMB anisotropies.”(DM = dark matter; CMB = cosmic microwave background).
https://lnkd.in/e6ifiQMn