Thawing k-essence dark energy in the PAge space
Zhiqi Huang

TL;DR
This paper investigates thawing k-essence dark energy models within the PAge parameter space, demonstrating that theoretical priors significantly enhance cosmological parameter constraints from future cosmic shear data.
Contribution
It introduces a general framework for analyzing thawing k-essence models in PAge space and quantifies the improvement in parameter estimation when applying the theoretical prior.
Findings
Thawing k-essence models cluster in a narrow band in PAge space.
Theoretical prior improves the figure of merit by a factor of 3.3.
Simulation of cosmic shear data demonstrates the benefit of the prior.
Abstract
A broad class of dark energy models can be written in the form of k-essence, whose Lagrangian density is a two-variable function of a scalar field and its kinetic energy . In the thawing scenario, the scalar field becomes dynamic only when the Hubble friction drops below its mass scale in the late universe. Thawing k-essence dark energy models can be randomly sampled by generating the Taylor expansion coefficients of its Lagrangian density from random matrices \cite{thaws}. Ref. \cite{thaws} points out that the non-uniform distribution of effective equation of state parameters of thawing k-essence model can be used to improve the statistics of model selection. The present work studies the statistics of thawing k-essence in a more general framework that is Parameterized by the Age of the universe (PAge)…
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