Massive particle pair production and oscillation in Friedman Universe: reheating energy and entropy, and cold dark matter

TL;DR

This paper models the early Universe's reheating process through massive particle pair production and oscillation driven by dark energy, linking it to dark matter formation and observable cosmological parameters.

Contribution

It introduces a novel Boltzmann-type rate equation coupled with cosmological equations to describe reheating and dark matter production in a quantum spacetime framework.

Findings

Reheating temperature consistent with tensor-to-scalar ratio constraints.

Stable massive pairs can account for cold dark matter abundance.

The model predicts a prolonged reheating episode with observable signatures.

Abstract

Suppose that the early Universe starts with a cosmological $\Lambda$-term originating from quantum spacetime at the Planck scale. Dark energy drives inflation and reheating by reducing its value for massive particle-antiparticle pairs production and oscillation, resulting in a holographic and massive pair plasma state. The back-and-forth reaction of dark energy and massive pairs slows inflation to its end and starts reheating by rapidly producing stable and unstable pairs. We introduce the Boltzmann-type rate equation describing the back-and-forth reaction. It forms a close set with Friedman equations and reheating equations for unstable pairs decay to relativistic particles. The numerical solutions show preheating, massive pairs dominated and genuine reheating episodes. We obtain the reheating temperature and entropy in terms of the tensor-to-scalar ratio $0 < r < 0.047$ consistently with observations. Stable massive pairs represent cold dark matter particles and weakly interact with dark energy. The resultant cold dark matter abundance $\Omega_c\sim 10^{-1}$ is about a constant in time.