Reconstructing Quintessence

TL;DR

This paper uses an Effective Field Theory approach to reconstruct quintessence dark energy models from cosmological data, testing model properties without assuming specific scalar potential forms.

Contribution

It introduces a model-independent reconstruction method for quintessence using current cosmological data, constraining dark energy properties across redshifts without potential assumptions.

Findings

Standard cosmology remains favored by data.

Deviations from the ΛCDM expansion are below 10% at z<1.5.

Current data can test quintessence properties without potential assumptions.

Abstract

We present an Effective Field Theory based reconstruction of quintessence models of dark energy directly from cosmological data. We show that current cosmological data possess enough constraining power to test several quintessence model properties for redshifts $z\in [0,1.5]$ with no assumptions about the behavior of the scalar field potential. We use measurements of the cosmic microwave background, supernovae distances, and the clustering and lensing of galaxies to constrain the evolution of the dark energy equation of state, Swampland Conjectures, the shape of the scalar field reconstructed potential, and the structure of its phase space. The standard cosmological model still remains favored by data and, within quintessence models, deviations from its expansion history are bounded to be below the 10% level at 95% confidence at any redshift below $z=1.5$.