Cosmic Acceleration with Torsion and Non-metricity in Friedmann-like Universes
Damianos Iosifidis

TL;DR
This paper derives a generalized cosmic acceleration equation incorporating torsion and non-metricity in FLRW universes, exploring their effects on the universe's expansion rate.
Contribution
It presents the most general form of the acceleration equation with torsion and non-metricity in FLRW spacetimes, extending standard cosmological models.
Findings
Conditions for torsion and non-metricity to accelerate expansion
Conditions for torsion and non-metricity to decelerate expansion
Generalized acceleration equation including non-Riemannian degrees of freedom
Abstract
Starting from the generalized Raychaudhuri equation with torsion and non-metricity, and considering an FLRW spacetime we derive the most general form of acceleration equation in the presence of torsion and non-metricity. That is we derive the cosmic acceleration equation when the nonRiemannian degrees of freedom are also taken into account. We then discuss some conditions under which torsion and non-metricity accelerate/decelerate the expansion rate of the Universe.
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