Dark Energy as Double N-Flation--Observational Predictions
J. Richard Gott, III, Zachary Slepian

TL;DR
This paper introduces a unified model linking dark energy and inflation through a double N-flation potential, deriving observational predictions for dark energy behavior, and suggesting it can be tested with upcoming experiments.
Contribution
It proposes a novel double-field inflationary model that connects inflation and dark energy, providing explicit formulas for dark energy evolution and observational predictions.
Findings
Derived a formula for dark energy equation of state evolution.
Numerical solutions support the slow-roll approximation for dark energy.
Model is testable with future observational data, especially related to inflationary parameters.
Abstract
We propose a simple model for dark energy useful for comparison with observations. It is based on the idea that dark energy and inflation should be caused by the same physical process. As motivation, we note that Linde's simple chaotic inflation produces values of and , which are consistent with the WMAP 1-sigma error bars. We therefore propose with and , where and the reduced Planck mass is set to unity. The field drives inflation and has damped by now (), while is currently rolling down its potential to produce dark energy. Using this model, we derive the formula via the slow-roll approximation. Our numerical results from exact and self-consistent…
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