Non-singular Inflation-Dark Energy Unification Model Based on Loop Quantum Cosmology and Mass-Varying Neutrinos
Zhiming Shuai, Xiangdong Zhang

TL;DR
This paper presents a non-singular cosmological model unifying inflation and dark energy within Loop Quantum Cosmology, incorporating mass-varying neutrinos to explain late-time acceleration, and validates it against observational data.
Contribution
It introduces a novel non-singular inflation-dark energy unification model based on LQC with mass-varying neutrinos, supported by observational constraints.
Findings
Quantum bounce replaces initial singularity with superinflation phase.
Model aligns well with supernova, BAO, and CMB observational data.
Neutrino coupling triggers late-time cosmic acceleration.
Abstract
Unifying the early-universe inflationary paradigm with late-time cosmic acceleration, while resolving the initial Big Bang singularity, remains one of the most profound challenges in modern cosmology. In this paper, we propose a non-singular quintessential inflation model embedded within the effective dynamics of Loop Quantum Cosmology (LQC) based on a Generalized Regularization Scheme. The quantum geometry effects naturally replace the initial singularity with a quantum bounce, followed by a phase of superinflation that sets robust initial conditions for the subsequent slow-roll inflation. To achieve a viable late-time dark energy epoch and address the coincidence problem, we introduce a coupling between the scalar field and massive neutrinos, known as Mass-Varying Neutrinos (MaVaNs). As neutrinos become non-relativistic in the post-inflationary evolution, their backreaction…
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