Tension between SN and BAO: current status and future forecasts
Celia Escamilla-Rivera, Ruth Lazkoz, Vincenzo Salzano, Irene Sendra

TL;DR
This paper examines the current and future tensions between supernovae and baryon acoustic oscillation data in constraining dark energy models, highlighting the impact of priors and the benefits of a low-correlation parametrization.
Contribution
It provides a comprehensive analysis of the tension between SNeIa and BAO data using simulations and explores the effects of priors and parametrization choices on dark energy constraints.
Findings
Tension depends on priors for Omega_m and Omega_b.
Forecasts show BAO data will become more constraining.
Low correlation parametrization narrows parameter errors.
Abstract
Using real and synthetic Type Ia SNe (SNeIa) and baryon acoustic oscillations (BAO) data representing current observations forecasts, this paper investigates the tension between those probes in the dark energy equation of state (EoS) reconstruction considering the well known CPL model and Wang's low correlation reformulation. In particular, here we present simulations of BAO data from both the the radial and transverse directions. We also explore the influence of priors on Omega_m and Omega_b on the tension issue, by considering 1-sigma deviations in either one or both of them. Our results indicate that for some priors there is no tension between a single dataset (either SNeIa or BAO) and their combination (SNeIa+BAO). Our criterion to discern the existence of tension (sigma-distance) is also useful to establish which is the dataset with most constraining power; in this respect SNeIa…
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