The quantum cosmological tilt and the origin of dark matter
Cesar Gomez, Raul Jimenez

TL;DR
This paper explores how quantum effects influence the tilt of the primordial power spectrum, revealing a transition from red to blue tilt that could explain the formation of primordial black holes as dark matter candidates.
Contribution
It introduces a non-perturbative quantum analysis of the power spectrum tilt, showing a scale-dependent transition that supports primordial black hole formation.
Findings
Quantum tilt transitions from red to blue at small scales.
Supports formation of primordial black holes with masses up to 10^{20} grams.
Provides a quantum Fisher information framework for tilt dependence.
Abstract
A promising candidate for cold dark matter is primordial black holes (PBH) formed from strong primordial quantum fluctuations. A necessary condition for the formation of PBH's is a change of sign in the tilt governing the anomalous scale invariance of the power spectrum from red at large scales into blue at small scales. Non-perturbative information on the dependence of the power spectrum tilt on energy scale can be extracted from the quantum Fisher information measuring the energy dependence of the quantum phases defining the de Sitter vacua. We show that this non-perturbative quantum tilt goes from a red tilted phase, at large scales, into a blue tilted phase at small scales converging to in the UV. This allows the formation of PBH's in the range of masses .
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