Finding origins of CMB anomalies in the inflationary quantum fluctuations

Abstract

In this paper, we present compelling evidence for the parity asymmetry (a discrete symmetry that is separate from isotropy) in the Cosmic Microwave Background (CMB) map, measured through two-point temperature correlations. This parity asymmetric CMB challenges our understanding of the quantum physics of the early Universe rather than LCDM ($\Lambda$ Cold-Dark-Matter). We commence by conducting a comprehensive analysis of the Planck CMB, focusing on the distribution of power in low-multipoles and temperature anticorrelations at parity conjugate points in position space. We find tension with the near scale-invariant power-law power spectrum of Standard Inflation (SI), with p-values of the order $\mathcal{O}\left( 10^{-4}-10^{-3} \right)$. Alternatively, we explore the framework of direct-sum inflation (DSI), where a quantum fluctuation arises as a direct-sum of two components evolving forward and backward in time at parity conjugate points in physical space. We found that DSI is consistent with data on parity asymmetry, the absence of power at $\theta>60^{\circ}$, and power suppression at low-even-multipoles, which are major data anomalies in the SI. Furthermore, we discover that the parameters characterizing the hemispherical power asymmetry anomaly become statistically insignificant when the large SI quadrupole amplitude is reduced to align with the data. DSI explains this low quadrupole with a p-value of $3.5\%$, 39 times higher than SI. Combining statistics from parameters measuring parity and low-$\ell$ angular power spectrum, we find that DSI is 50-650 times more probable than SI. In summary, our investigation suggests that CMB temperature fluctuations exhibit homogeneity and isotropy but parity-asymmetric consistent with predictions of DSI. This observation provides tantalizing evidence for the quantum mechanical nature of gravity.