Evidence of a truncated spectrum in the angular correlation function of the cosmic microwave background
Fulvio Melia, Martin Lopez-Corredoira

TL;DR
The paper presents evidence that the lack of large-angle correlations in the CMB can be explained by a non-zero minimum wavenumber, challenging standard inflationary models and suggesting alternative early Universe scenarios.
Contribution
It introduces a cutoff in the primordial power spectrum to explain CMB anomalies, providing strong observational evidence against zero minimum wavenumber in inflation.
Findings
Planck data rules out zero k_min at >8 sigma confidence
A non-zero k_min indicates a maximum wavelength at decoupling
Results challenge the standard inflationary paradigm
Abstract
The lack of large-angle correlations in the fluctuations of the cosmic microwave background (CMB) conflicts with predictions of slow-roll inflation. But though probabilities (< 0.24%) for the missing correlations disfavor the conventional picture at > 3 sigma, factors not associated with the model itself may be contributing to the tension. Here we aim to show that the absence of large-angle correlations is best explained with the introduction of a non-zero minimum wavenumber k_min for the fluctuation power spectrum P(k). We assume that quantum fluctuations were generated in the early Universe with a well-defined power spectrum P(k), though with a cutoff k_min not equal to 0. We then re-calculate the angular correlation function of the CMB and compare it with Planck observations. The Planck 2013 data rule out a zero k_min at a confidence level exceeding 8 sigma. Whereas purely slow-roll…
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