Abstract
Abstract
In this paper, we present compelling evidence for the parity asymmetry (a discrete
symmetry separate from isotropy) in the Cosmic Microwave Background (CMB) map, measured through
two-point temperature correlations. Any asymmetry associated with discrete symmetries, such as
parity, challenges our understanding of quantum physics associated with primordial physics rather
than LCDM (Λ Cold-Dark-Matter) itself. 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
𝒪(10-4 - 10-3). 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. This mechanism
results in a parity-asymmetric scale-dependent power spectrum, particularly prominent at
low-multipoles, without any additional free model parameters. Our findings indicate that DSI is
consistent with data on parity asymmetry, the absence of power at θ > 60°, and power
suppression at low-even-multipoles which are major data anomalies in the SI model. 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-ℓ angular power spectrum, we find that
DSI is 50-650 times more probable than SI. In summary, our investigation suggests that while CMB temperature fluctuations exhibit homogeneity and isotropy, they also display parity-asymmetric
behavior consistent with predictions of DSI. This observation provides a tantalizing evidence for
the quantum mechanical nature of gravity.
Cited by
2 articles.
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