How Gaussian can the Sky be? Primordial Non-Gaussianity from Quantum Information
Cesar Gomez, Raul Jimenez

TL;DR
This paper introduces a quantum information framework to analyze primordial non-Gaussianities in the early universe, revealing quantum-originated effects like clock bias that influence the distribution of primordial fluctuations.
Contribution
It presents a model-independent quantum estimation approach to quantify non-Gaussianities, linking them to quantum properties of the early universe and identifying a novel clock bias effect.
Findings
Primordial non-Gaussianities include squeezed and equilateral shapes.
The squeezed non-Gaussianity relates to the spectral index as $f_{NL} o n_s - 1$.
A new quantum clock bias effect impacts the spectral tilt and running, potentially measurable.
Abstract
Using the quantum information picture to describe the early universe as a time dependent quantum density matrix, with time playing the role of a stochastic variable, we compute the non-gaussian features in the distribution of primordial fluctuations. We use a quasi de Sitter model to compute the corresponding quantum Fisher information function as the second derivative of the relative entanglement entropy for the density matrix at two different times. We define the curvature fluctuations in terms of the time quantum estimator. Using standard quantum estimation theory we compute the non-gaussian features in the statistical distribution of primordial fluctuations. Our approach is model independent and only relies on the existence of a quasi de Sitter phase. We show that there are primordial non-gaussianities, both in the form of squeezed and equilateral shapes. The squeezed limit gives a…
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.
