Abstract:The large scale structures observed in cosmic maps correspond to super-horizon (causally disconnected) perturbations in the early Universe that are usually attributed to scale invariant adiabatic modes from cosmic Inflation. Here, we interpret discrepant measurements of the expansion rate H 0 (the so called Hubble tension) as super-horizon perturbations and show that they are neither adiabatic nor scale invariant. We argue that these measurements indicate that cosmic expansion originates from gravitational col… Show more
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