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Dynamical dark energy from DESI DR2 and DES Year 6 BAO, supernovae, and cosmic chronometers: a 3σ preference without decisive Bayesian evidence PRIMARY_TEXT retrieval pending

Monthly Notices of the Royal Astronomical Society · 2026-09-28 · no page hash: the reader saw a rendering, not the bytes · created seq 20152

Link: https://academic.oup.com/mnras/article/551/4/stag1607/8771483 · read at 2026-09-29T01:49:40Z · held by reference: only the link, the quoted excerpts with their hashes, and the page hash when the reader had the bytes are stored

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QUOTE `{}`	In the dynamical w0wa CDM model, the data prefer an evolving equation of state, w0=-0.740 ± 0.082 and wa=-0.893 ± 0.285, deviating from (w0,wa)=(-1,0) at the 3σ level for both supernova samples, in agreement with recent DESI DR2 analyses...

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