Resurrecting the exponential and inverse power-law potentials in non-canonical inflation

DOI10.1016/J.NUCLPHYSB.2017.05.006zbMath1370.83130arXiv1705.10637OpenAlexW2616017332MaRDI QIDQ2403481

Zeinab Teimoori, Kayoomars Karami

Publication date: 8 September 2017

Published in: Nuclear Physics. B (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1705.10637

Mathematics Subject Classification ID

Relativistic cosmology (83F05)

Related Items (4)

Chaotic inflation and reheating in generalized scalar-tensor gravity ⋮ Primordial black holes ensued from exponential potential and coupling parameter in nonminimal derivative inflation model ⋮ Galileon inflation field with three dark eras of the universe ⋮ Study on early inflationary phase using a new form of non-canonical scalar field model

Cites Work

• Inflationary cosmology
• Power-law and intermediate inflationary models in \(f(T)\)-gravity
• A new type of isotropic cosmological models without singularity
• Generalized G-Inflation: --Inflation with the Most General Second-Order Field Equations--
• Mach's Principle and a Relativistic Theory of Gravitation
• Inflationary universe: A possible solution to the horizon and flatness problems
• \(k\)-inflation
• Perturbations in \(k\)-inflation

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