Viscous quintessence model fitted to binned SNe Ia data shows no phantom transition and lower transition redshift than DESI.
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Forecasts show that ~66 optical GRBs can achieve σ_w ≈ 0.47 in wCDM using Dainotti relations, matching Planck precision and enabling independent high-redshift tests of dark energy.
citing papers explorer
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Interpretation of the binned SNe Ia Master Sample data via a scalar quintessence component: phantom transition?
Viscous quintessence model fitted to binned SNe Ia data shows no phantom transition and lower transition redshift than DESI.
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Gamma-Ray Bursts as an Independent High-Redshift Probe of Dark Energy
Forecasts show that ~66 optical GRBs can achieve σ_w ≈ 0.47 in wCDM using Dainotti relations, matching Planck precision and enabling independent high-redshift tests of dark energy.