Origin of the large-scale galaxy peculiar velocity field: a minimal isocurvature model

Abstract

The galaxy peculiar velocity field (velocity relative to the uniform Hubble law expansion) seems to have a large r.m.s. value, ∼500 km s⁻¹, and a large coherence length ≳=50 Mpc. It is difficult to account for this in the standard model inspired by inflation, where galaxies and clusters of galaxies grow by gravity out of initially adiabatic fluctuations in the distribution of mass now dominated by weakly interacting cold dark matter^1,2. A model that does seem to work assumes that, at high redshift, mass was uniform and the baryon number was inhomogeneous, a stationary random process. This produces in the late Universe a baryon distribution with a power spectrum proportional to the initial value at short wavelength, a prominent peak in the spectrum at the matter-radiation Jeans length, and a sharp cutoff at longer wavelengths. Here I report how this spectrum normalized by the observed galaxy clustering can produce by gravity the large velocity field with large coherence length needed without excessively perturbing the microwave background.