Loop quantum cosmology and its gauge-covariant avatar: a weak curvature relationship
Bao-Fei Li, Parampreet Singh

TL;DR
This paper investigates the relationship between standard loop quantum cosmology (LQC) and a gauge-covariant version (gLQC), revealing that gLQC exhibits a richer structure with higher-order quantum corrections in the weak curvature limit, including novel $ ho^{3/2}$ terms.
Contribution
It demonstrates that gLQC encompasses LQC's non-perturbative modifications and uncovers higher-order corrections, suggesting a hierarchy of quantum geometric effects in loop quantum cosmology.
Findings
gLQC recovers LQC's $ ho^2$ correction in the post-bounce branch
gLQC's pre-bounce branch exhibits a novel $ ho^{3/2}$ correction
gLQC reveals a richer structure with higher-order quantum modifications
Abstract
We explore the relationship between the effective dynamics in standard loop quantum cosmology (LQC) based on holonomies and triads obtained from gauge-fixing fluxes, and a modification of LQC based on holonomies and gauge-covariant fluxes (referred to as gLQC). Both the models yield singularity resolution via a bounce because of non-perturbative quantum geometric effects resulting in a maximum for energy density. In LQC, the bounce is extremely well captured by a term in energy density with a negative sign which emerges as a non-perturbative modification to the classical Friedmann and Raychaudhuri equations. But, details of such modifications in gLQC have remained hidden due to an arduous nature of gauge-covariant flux modifications which do not allow writing above equations in a closed form. To extract these modifications we explore the large volume, weak curvature limit for…
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