CMB parity asymmetry from unitary quantum gravitational physics

TL;DR

This paper proposes a quantum gravitational framework that naturally explains the observed parity asymmetry in the CMB, providing strong Bayesian evidence favoring this model over standard inflationary theories.

Contribution

It introduces a unitary quantum field theory in curved spacetime incorporating parity and time-reversal, explaining CMB anomalies as a consequence of quantum gravity effects.

Findings

Bayes factor exceeds 650, favoring the new model

Predicts parity asymmetry as a natural outcome of cosmic expansion

Provides evidence for quantum gravitational origins of CMB anomalies

Abstract

Longstanding anomalies in the Cosmic Microwave Background (CMB), including the low quadrupole moment and hemispherical power asymmetry, have recently been linked to an underlying parity asymmetry. We show here how this parity asymmetry naturally arises within a quantum framework that explicitly incorporates the construction of a geometric quantum vacuum based on parity ($\mathcal{P}$) and time-reversal ($\mathcal{T}$) transformations. This elegant framework restores unitarity in quantum field theory in curved spacetime (QFTCS). When applied to inflationary quantum fluctuations, this unitary QFTCS formalism predicts parity asymmetry as a natural consequence of cosmic expansion, which inherently breaks time-reversal symmetry. Observational data strongly favor this unitary QFTCS approach, with a Bayes factor, the ratio of marginal likelihoods associated with the model given the data $p\left( M\vert D \right)$, exceeding 650 times that of predictions from the standard inflationary framework. This Bayesian approach contrasts with the standard practice in the CMB community, which evaluates $p\left( D\vert M \right)$, the likelihood of the data under the model, which undermines the importance of low-$\ell$ physics. Our results, for the first time, provide compelling evidence for the quantum gravitational origins of CMB parity asymmetry on large scales.