In Einstein-Cartan gravity, non-interacting holographic dark energy with Hubble cutoff acquires a torsion scalar that scales as a^{-3} and shifts its equation of state from dust-like to values near -1, enabling acceleration.
Frenkel, “ ¨Uber die von der molekularkinetischen Theorie der W¨ arme geforderte Bewegung von in ruhenden Fl¨ ussigkeiten suspendierten Teilchen, Z
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Holographic Dark Energy with Hubble Radius as an Infrared Cutoff in Einstein-Cartan Gravity
In Einstein-Cartan gravity, non-interacting holographic dark energy with Hubble cutoff acquires a torsion scalar that scales as a^{-3} and shifts its equation of state from dust-like to values near -1, enabling acceleration.