Theoretical priors in scalar-tensor cosmologies: Thawing quintessence

Abstract

The late time acceleration of the Universe can be characterized in terms of an extra, time dependent, component of the universe -- dark energy. The simplest proposal for dark energy is a scalar-tensor theory -- quintessence -- which consists of a scalar field, $\varphi$, whose dynamics is solely dictated by its potential, $V(\varphi )$. Such a theory can be uniquely characterized by the equation of state of the scalar field energy momentum-tensor. We find the time dependence of the equation of state for a broad family of potentials and, using this information, we propose an analytic prior distribution for the most commonly used parametrization. We show that this analytic prior can be used to accurately predict the distribution of observables for the next generation of cosmological surveys. Including the theoretical priors in the comparison with observations considerably improves the constraints on the equation of state.

V1: 13 pages, 11 figures, comments welcome; V2: 14 pages, 11 figures, minor clarifications added, accepted for publication in PRD

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Cited by in corpus (14)

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• Cosmological constraints on Galileon dark energy with broken shift symmetry
• Improving data-driven model-independent reconstructions and updated constraints on dark energy models from Horndeski cosmology
• Cosmological consequences of a scalar field with oscillating equation of state. II. Oscillating scaling and chaotic accelerating solutions
• Statistics of Thawing K-essence Dark Energy Models
• Thawing Quintessence: Priors, evidence, and likely trajectories
• Theoretical priors in scalar-tensor cosmologies: Shift-symmetric Horndeski models
• Geometry vs growth: Internal consistency of the flat ΛCDM model with KiDS-1000
• Dark energy constraints in light of theoretical priors