Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families
Shahnawaz A. Adil, Miguel A. Zapata, \"Ozg\"ur Akarsu, J. Alberto Vazquez

TL;DR
This paper introduces a background-level framework to reconstruct scalar-field potentials from dark-energy density histories, enabling comparison of analytic potential families via Bayesian evidence, and applies it to various dark-energy models.
Contribution
It develops a unified method to derive scalar-field potentials from dark-energy histories and performs Bayesian model comparison of potential families based on reconstructed potentials.
Findings
Exponential potential has highest Bayesian evidence for CPL history.
Shifted-tanh potential is strongly preferred for sign-switching dark-energy history.
Reconstructed potentials provide a dictionary linking phenomenological histories to scalar-field shapes.
Abstract
We present a unified \emph{background-level} framework that maps a prescribed late-time dark-energy density history onto an effective scalar-field description in a spatially flat FLRW universe. Working directly with , we reconstruct the associated field trajectory , and field-space potential , together with a null energy condition (NEC) consistency check. We apply the method to three benchmark histories: (i) the Chevallier--Polarski--Linder (CPL) form; (ii) a smooth mirror AdSdS sign-switching profile in which crosses zero at , interpolating between a positive late-time plateau and a negative high- plateau (CDM-like at the background level); and (iii) a shifted- emergent profile that remains positive definite and approaches at high redshift.…
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Taxonomy
TopicsCosmology and Gravitation Theories · Galaxies: Formation, Evolution, Phenomena · Dark Matter and Cosmic Phenomena
