On the oscillation-driven cosmological expansion at the post-inflationary stage

DOI10.1134/S0202289317010078zbMath1369.83109arXiv1611.03734OpenAlexW2565131940MaRDI QIDQ2398810

V. A. Koutvitsky, Eugene M. Maslov

Publication date: 21 August 2017

Published in: Gravitation \& Cosmology (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1611.03734

zbMATH Keywords

oscillation-driven cosmological expansionpost-inflationary stage

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Space-time singularities, cosmic censorship, etc. (83C75) Exact solutions to problems in general relativity and gravitational theory (83C15)

Related Items (2)

Perturbation approach to the Hill equation with a slowly varying parameter with application to the inflationary cosmology ⋮ Novel CMB constraints on the α parameter in alpha-attractor models

Cites Work

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• The singular Hill equation and generalized Lindemann-Stieltjes method
• Inflation with oscillations
• A new type of isotropic cosmological models without singularity
• Parametric instability of the real scalar pulsons
• Late-time oscillatory behaviour for self-gravitating scalar fields
• Instability of coherent states of a real scalar field
• Inflation without Slow Roll

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