# Modeling the large-scale power deficit with smooth and discontinuous primordial spectra

## TL;DR

This paper explores cosmological models with a large-scale power deficit in the primordial spectrum, fitting new parameters to various data sets, and finds evidence for a significant reduction in power at large scales around 350 Mpc.

## Contribution

It introduces a modified primordial power spectrum with a large-scale deficit and analyzes its statistical significance across multiple cosmological data sets.

## Key findings

- Evidence for a sharp power reduction at ~350 Mpc scale
- Motivations for models breaking scalar-tensor consistency
- Statistical support for a large-scale power deficit

## Abstract

We investigate a set of cosmological models for which the primordial power spectrum has a large-scale power deficit. The standard power-law spectrum is subject to long-wavelength modifications described by some new parameters, resulting in corrections to the anisotropies in the cosmic microwave background. The new parameters are fitted to different data sets: temperature only, temperature and polarization, the low-redshift determination of $H_0$, and baryonic acoustic oscillations. We discuss the statistical significance of the modified spectra, from both frequentist and Bayesian perspectives. Our analysis suggests motivations for considering models that break scalar-tensor consistency, or models with negligible power in the far super-Hubble limit. We present what appears to be substantial evidence for a new scale around 350 Mpc above which the primordial (scalar) power spectrum is sharply reduced by about 20%.