Viscous quintessence model fitted to binned SNe Ia data shows no phantom transition and lower transition redshift than DESI.
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2 Pith papers cite this work. Polarity classification is still indexing.
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A bias-controlled quasar sample of ~2000 objects demonstrates that the X-ray-to-UV luminosity relation remains constant from redshift 0.7 to 5.
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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.