EFT of Dark Energy with Cosmic Chronometers: Reconstructing Background EFT Functions
Fumiya Okamatsu, Kazufumi Takahashi

TL;DR
This paper presents a method to reconstruct the background effective field theory functions of dark energy directly from cosmic chronometer data, enabling model-independent testing of dark energy models including mbda CDM.
Contribution
It introduces a novel approach to derive EFT functions from observational data without assuming specific cosmological models, facilitating broader tests of dark energy theories.
Findings
Reconstructed EFT functions from cosmic chronometer data.
Demonstrated application to constrain quintessence models.
Enabled model-independent testing of mbda CDM and other dark energy models.
Abstract
The effective field theory (EFT) of dark energy provides a model-independent framework for studying cosmology within scalar-tensor theories. In this work, we explore how the time evolution of the cosmological background, inferred from cosmic chronometer measurements of the Hubble parameter, can be used to reconstruct the relevant EFT functions. Our approach enables the direct determination of these EFT functions from observational data without assuming any specific cosmological model. This makes it possible to test the background evolution of a wide range of dark energy models, including the CDM model. We further demonstrate how the reconstructed EFT functions can be applied to constrain concrete theories, such as the quintessence model.
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