Primordial power spectrum from Planck
Dhiraj Kumar Hazra, Arman Shafieloo, Tarun Souradeep

TL;DR
This paper reconstructs the primordial power spectrum from Planck CMB data using a modified Richardson-Lucy algorithm, identifying key features and demonstrating consistency with the standard power-law model while revealing potential hints for inflationary theories.
Contribution
The study introduces a novel reconstruction method for the primordial power spectrum from Planck data, identifying features and improving data fit beyond the power-law model.
Findings
Detected a prominent dip near f750-850 in the spectrum.
Identified a feature near f1800-2000 likely due to systematic effects.
Reconstructed spectrum improves fit to WMAP-9 data and indicates gravitational lensing evidence.
Abstract
Using modified Richardson-Lucy algorithm we reconstruct the primordial power spectrum (PPS) from Planck Cosmic Microwave Background (CMB) temperature anisotropy data. In our analysis we use different combinations of angular power spectra from Planck to reconstruct the shape of the primordial power spectrum and locate possible features. Performing an extensive error analysis we found the dip near represents the most prominent feature in the data. Feature near is detectable with high confidence only in 217 GHz spectrum and is apparently consequence of a small systematic as described in the revised Planck 2013 papers. Fixing the background cosmological parameters and the foreground nuisance parameters to their best fit baseline values, we report that the best fit power law primordial power spectrum is consistent with the reconstructed form of the PPS…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
