Addendum: Fitting the DESI BAO data with dark energy driven by the Cohen-Kaplan-Nelson bound

Abstract

Motivated by the recent Year-2 data release of the DESI collaboration, we update our results on time-varying dark energy models driven by the Cohen-Kaplan-Nelson bound. The previously found preference of time-dependent dark energy models compared to ΛCDM is further strengthend by the new data release. For our particular models, we find that this preference increases up to ≈ 2.6 σ depending on the used supernova dataset.