Reconstruction of scalar field theories realizing inflation consistent with the Planck and BICEP2 results

DOI10.1016/j.physletb.2014.09.014zbMath1317.83097arXiv1406.2417OpenAlexW2082786033MaRDI QIDQ2355060

Kazuharu Bamba, Sergei D. Odintsov, Shin'ichi Nojiri

Publication date: 27 July 2015

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

Full work available at URL: https://arxiv.org/abs/1406.2417

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Observational and experimental questions in relativity and gravitational theory (83B05)

Related Items (9)

Hybrid inflation with Planck scale fields ⋮ Non-minimal two-loop inflation ⋮ Scalar Field Evolution at Background and Perturbation Levels for a Broad Class of Potentials ⋮ Inflationary cosmology in unimodular F(T) gravity ⋮ Dynamics of inflation and dark energy from \(F(R, \mathcal{G})\) gravity ⋮ Loop quantum cosmology scalar field models ⋮ Stabilization of Starobinsky–Vilenkin stochastic inflation by an environmental noise ⋮ On the renormalization group perspective of α-attractors ⋮ Polynomial integrals of motion in dilaton gravity theories

Cites Work

• Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests
• Unifying phantom inflation with late-time acceleration: scalar phantom-non-phantom transition model and generalized holographic dark energy

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