Cosmological Evolution in the $GL(4,\mathbb{R})$ Yang-Mills Theory of Gravity: Resolving the JWST Early Galaxy Crisis and Late-Time Acceleration
Yi Yang, Wai Bong Yeung

TL;DR
This paper proposes a gauge-theoretic gravity model based on $GL(4, ext{R})$ Yang-Mills theory that explains early universe expansion and late-time acceleration without scalar fields or a cosmological constant.
Contribution
It introduces a novel gauge-theoretic gravity framework that naturally accounts for cosmic evolution, resolving the JWST galaxy crisis and late-time acceleration without ad hoc scalar fields.
Findings
Achieves a singularity-free coasting expansion $a(t) \,\propto\, t$, addressing early galaxy formation.
Transitions to a vacuum state with residual torsion, leading to late-time exponential acceleration.
Eliminates the need for scalar fields or a cosmological constant in cosmological modeling.
Abstract
We investigate the cosmological implications of the Yang-Mills gauge theory of gravity. A long-standing theoretical challenge in standard cosmology is the reliance on ad hoc rolling scalar fields (e.g., the inflaton or quintessence) to drive early-time inflation and late-time acceleration, despite their unknown particle physics origins. In this work, by treating the affine connection as a gauge field and the world metric as a non-dynamical background, we derive an exact expansion history that strictly eliminates the need for any rolling scalar fields or a cosmological constant. The dynamics are governed solely by the Yang-Mills field strength squared. We demonstrate that the early Universe exhibits a singularity-free coasting expansion , resolving the JWST high-redshift galaxy crisis by granting significantly more time for early structure formation. As…
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