Post-inflationary phases stiffer than radiation and Palatini formulation

DOI10.1088/1361-6382/ab52a8zbMath1478.83251arXiv1905.06182OpenAlexW3098561190MaRDI QIDQ5160112

Massimo Giovannini

Publication date: 28 October 2021

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1905.06182

zbMATH Keywords

inflationquintessencecosmological perturbationsCMBPalatini formulationhigher-order gravitational theories

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Geometrodynamics and the holographic principle (83E05) Quantization of the gravitational field (83C45)

Related Items (10)

Dynamically induced Planck scale and inflation in the Palatini formulation ⋮ Relic gravitons from stiff curvature perturbations ⋮ Palatini R ² quintessential inflation ⋮ β-function reconstruction of Palatini inflationary attractors ⋮ Palatini approach and large-scale magnetogenesis ⋮ Tracing the high energy theory of gravity: an introduction to Palatini inflation ⋮ Implications of Palatini gravity for inflation and beyond ⋮ Gravitational dark matter production in Palatini preheating ⋮ Inflation and Reheating in f(R,h) theory formulated in the Palatini formalism ⋮ Tachyonic preheating in Palatini R ² inflation

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