Sign-Switching Dark Energy: Smooth Transitions with Recent DESI DR2 Observations

Beñat Ibarra-Uriondo; Mariam Bouhmadi-López

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arXiv · 2602.12347

Sign-Switching Dark Energy: Smooth Transitions with Recent DESI DR2 Observations

Beñat Ibarra-Uriondo·Mariam Bouhmadi-López

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Abstract

Sign-switching dark energy provides a novel mechanism for modifying the late-time expansion history of the Universe without invoking additional fields or finely tuned initial conditions. In this work, we investigate a class of background--level cosmological models in which the dark energy contribution changes sign at a transition redshift $z_\dagger$, producing a sharp deviation from standard $\Lambda$CDM dynamics. We confront these models with a comprehensive set of cosmological observations, including Planck 18 cosmic microwave background (CMB) measurements, DESI DR2 Baryonic Acoustic Oscillation (BAO) data and the Pantheon+ $\&$ SH0ES Type Ia supernova sample (SN). Using a full Markov Chain Monte Carlo (MCMC) analysis, we find that the sign-switching scenario significantly alleviates the Hubble tension while obtaining better results when statistically comparing with $\Lambda$CDM, as quantified by the Akaike and Bayesian information Criteria. Although the model is explored only at the background level, the improvement in the inferred Hubble constant demonstrates that sign-switching dark energy offers a promising and physically economical pathway toward resolving late-universe discrepancies.

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Beñat Ibarra-Uriondo, Mariam Bouhmadi-López. 2026-02-12. Sign-Switching Dark Energy: Smooth Transitions with Recent DESI DR2 Observations. https://arxiv.org/abs/2602.12347

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