Cosmological consequences of a scalar field with oscillating equation of state. III. Unifying inflation with dark energy and small tensor-to-scalar ratio
S. X. Tian, Zong-Hong Zhu

TL;DR
This paper explores a scalar field model unifying inflation and dark energy, predicting an extremely small tensor-to-scalar ratio and suggesting gravitational particle creation as a reheating mechanism, consistent with current observations.
Contribution
It introduces a generalized oscillating dark energy model that naturally predicts a very small tensor-to-scalar ratio, aligning with observational constraints and providing a new perspective on inflation and dark energy unification.
Findings
Predicts tensor-to-scalar ratio r~10^{-7} consistent with Planck data.
Proves r<0.01 in a generalized model, supporting the smallness of primordial gravitational waves.
Suggests gravitational particle creation can reheat the universe after inflation.
Abstract
We investigate the inflationary consequences of the oscillating dark energy model proposed by Ti\'an [\href{https://doi.org/10.1103/PhysRevD.101.063531}{Phys. Rev. D {\bf 101}, 063531 (2020)}], which aims to solve the cosmological coincidence problem with multi-accelerating Universe (MAU). We point out that the inflationary dynamics belong to slow-roll inflation. The spectral index of scalar perturbations and the tensor-to-scalar ratio are shown to be consistent with current \textit{Planck} measurements. Especially, this model predicts , which is far below the observation limits. This result motivates us to explore the smallness of in the general MAU. We propose a quintessential generalization of the original model and prove in general. The null detection to date of primordial gravitational waves provides a circumstantial evidence for the MAU. After the…
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