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Cosmological consequences of a scalar field with oscillating equation of state. III. Unifying inflation with dark energy and small tensor-to-scalar ratio
Phys. Rev. D 103, 123545 – Published 25 June, 2021
DOI: https://doi.org/10.1103/PhysRevD.103.123545
Abstract
We investigate the inflationary consequences of the oscillating dark energy model proposed by Tián [Phys. Rev. D 101, 063531 (2020), which aims to solve the cosmological coincidence problem with a multiaccelerating 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 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 circumstantial evidence for the MAU. After the end of inflation, the scalar field rolls toward infinity instead of a local minimum, and meanwhile its equation of state is oscillating with an average value larger than . In this framework, we show that gravitational particle creation at the end of inflation is capable of reheating the Universe.
Physics Subject Headings (PhySH)
See Also
Cosmological consequences of a scalar field with oscillating equation of state: A possible solution to the fine-tuning and coincidence problems
Cosmological consequences of a scalar field with oscillating equation of state. IV. Primordial nucleosynthesis and the deuterium problem
Article Text
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