Non-minimal (self-)running inflation: metric vs. Palatini formulation
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Publication:2024183
DOI10.1007/JHEP01(2021)011zbMath1459.83073arXiv1912.10038MaRDI QIDQ2024183
Publication date: 3 May 2021
Published in: Journal of High Energy Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1912.10038
Relativistic cosmology (83F05) Renormalization group methods applied to problems in quantum field theory (81T17) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Astrophysical cosmology (85A40)
Related Items (16)
Dynamically induced Planck scale and inflation in the Palatini formulation ⋮ Palatini R 2 quintessential inflation ⋮ β-function reconstruction of Palatini inflationary attractors ⋮ Constant-roll in the Palatini-R2 models ⋮ Initial conditions for plateau inflation: a case study ⋮ Extended interactions in the Palatini-R2inflation ⋮ New class of hybrid metric-Palatini scalar-tensor theories of gravity ⋮ Tracing the high energy theory of gravity: an introduction to Palatini inflation ⋮ Implications of Palatini gravity for inflation and beyond ⋮ Possible discrepancies between cosmological and electroweak observables in Higgs inflation ⋮ Slow-roll inflation in Palatini \(F(R)\) gravity ⋮ Multiple point criticality principle and Coleman-Weinberg inflation ⋮ Gravitational dark matter production in Palatini preheating ⋮ Palatini double-well and Coleman-Weinberg potentials with non-minimal coupling ⋮ Inflation and Reheating in f(R,h) theory formulated in the Palatini formalism ⋮ Tachyonic preheating in Palatini R 2 inflation
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