Primordial quantum nonequilibrium and large-scale cosmic anomalies
Samuel Colin, Antony Valentini

TL;DR
This paper proposes that incomplete quantum relaxation during a pre-inflationary phase could explain large-scale anomalies in the CMB, using the de Broglie-Bohm framework and numerical simulations.
Contribution
It introduces a novel quantum nonequilibrium scenario during pre-inflation that can account for observed cosmic anomalies, supported by numerical modeling.
Findings
Power deficit with inverse-tangent shape in the primordial spectrum
Ability to produce observed magnitude of power deficit
Potential explanation for large-scale anisotropy
Abstract
We study incomplete relaxation to quantum equilibrium at long wavelengths, during a pre-inflationary phase, as a possible explanation for the reported large-scale anomalies in the cosmic microwave background (CMB). Our scenario makes use of the de Broglie-Bohm pilot-wave formulation of quantum theory, in which the Born probability rule has a dynamical origin. The large-scale power deficit could arise from incomplete relaxation for the amplitudes of the primordial perturbations. We show, by numerical simulations for a spectator scalar field, that if the pre-inflationary era is radiation dominated then the deficit in the emerging power spectrum will have a characteristic shape (an inverse-tangent dependence on wavenumber k, with oscillations). It is found that our scenario is able to produce a power deficit in the observed region and of the observed (approximate) magnitude for an…
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