Quartic inflation and radiative corrections with non-minimal coupling

DOI10.1088/1475-7516/2019/10/028OpenAlexW3099459526MaRDI QIDQ5067124

V. N. Şenoğuz, Nilay Bostan

Publication date: 1 April 2022

Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1907.06215

zbMATH Keywords

inflationphysics of the early universe

Mathematics Subject Classification ID

Relativity and gravitational theory (83-XX)

Related Items (5)

Non-minimally coupled quartic inflation with Coleman-Weinberg one-loop corrections in the Palatini formulation ⋮ Probing the seesaw mechanism with cosmological data ⋮ Inflation with antisymmetric tensor field: new candidates ⋮ Non-minimal (self-)running inflation: metric vs. Palatini formulation ⋮ A predictive SO(10) model

Cites Work

• On inflation with non-minimal coupling
• Superconformal inflationary \(\alpha\)-attractors
• A new improved energy-momentum tensor.
• CMB constraints on the inflaton couplings and reheating temperature in \(\alpha\)-attractor inflation
• Cosmology in scalar-tensor gravity.
• A new type of isotropic cosmological models without singularity
• MODEL DEPENDENCE OF THE NON-MINIMAL SCALAR-GRAVITON EFFECTIVE COUPLING CONSTANT IN CURVED SPACE-TIME
• The Higgs field as an inflaton
• The Scalar-Tensor Theory of Gravitation
• THE PHASE-SPACE VIEW OF INFLATION I: THE NON-MINIMALLY COUPLED SCALAR FIELD
• The Primordial Density Perturbation
• Inflationary universe: A possible solution to the horizon and flatness problems

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