Inflation and late-time acceleration from a double-well potential with cosmological constant
Jaume de Haro, Emilio Elizalde

TL;DR
This paper proposes a cosmological model without a big bang singularity, featuring an inflationary phase, a phase transition, reheating, and a smooth transition to the standard Lambda-CDM universe.
Contribution
It introduces a novel non-singular universe model with a double-well potential and cosmological constant that unifies early inflation and late-time acceleration.
Findings
Achieves a non-singular universe with inflation and late acceleration
Reheats the universe to MeV temperatures after phase transition
Smoothly matches the standard Lambda-CDM cosmology
Abstract
A model of a universe without big bang singularity is presented, which displaysanearly inflationary period ending just before a phase transition to a deflationary epoch. The model produces enough heavy particles so as to reheat the universe at temperatures in the MeV regime. After the reheating, it smoothly matches the standard CDM scenario.
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