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Reconstructing dark energy with fewer assumptions

astro-ph.CO · 2026-06-04 · unverdicted · novelty 5.0

Bin-wise uncorrelated reconstruction from DESI/SDSS BAO and Pantheon+/Union3.1/DES-Dovekie supernovae yields dark energy density peaking then declining and equation of state oscillating with phantom crossing near z~0.7, consistent across datasets at moderate significance.

Neutrino mass constraints in interacting dark energy models after DESI DR2

astro-ph.CO · 2026-06-03 · unverdicted · novelty 4.0

Upper bounds on total neutrino mass in four phenomenological interacting dark energy models are derived from DESI DR2 BAO plus CMB and SNIa data, showing strong dependence on the interaction term form and statistical preference for models that tighten the bound below the oscillation lower limit.

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