Dynamics of reheating in loop quantum cosmology
Yogesh, Bao-Fei Li, Mayukh R. Gangopadhyay, and Anzhong Wang
APS Open Sci. 1, 000120 (2026) - Published 2 September, 2026
In loop quantum cosmology (LQC), the initial singularity is replaced by a quantum bounce, leading to a universal postbounce evolution characterized by three distinct epochs: bouncing, transition, and slow-roll inflation, before the hot big-bang universe starts. While the generic nature of inflation in the presence of an inflaton field in LQC is well established, the subsequent reheating phase—the process that thermalizes the universe and marks the beginning of the hot big bang—has remained unexplored in this quantum gravitational framework. This paper presents the first comprehensive integration of the (generalized) reheating mechanism into the LQC paradigm. Using the power law plateau potential and comparing predictions with the latest Planck 2018 and ACT 2025 data, we demonstrate that the inclusion of a reheating phase with a generic equation of state is fully consistent with the cosmological constraints. In addition, using the observational data for the amplitude and spectral index of the scalar perturbations and the tensor-to-scalar ratio, we also constrain the total number of e-folds from the bounce to the present day and find a lower bound, which is less constrained than that obtained previously from the fitting of the high- cosmic microwave background temperature power spectrum (TT), the polarization data (TT, TE, EE), and the low- polarization data (lowP). We also show that at the horizon crossing, there exist six independent algebraic equations, which uniquely determine six physical parameters, once the amplitude and the power spectral index of the pivot mode of the scalar perturbations are provided. Three of the six parameters form a complete set of the initial conditions at the horizon crossing and uniquely determine the entire evolution of the universe, including both the pre- and postbounce phases, through the modified Friedmann and Klein-Gordon equations of LQC. This is sharply in contrast to the case without considering the reheating phase.