Non-minimally coupled Natural Inflation: Palatini and Metric formalism with the recent BICEP/Keck
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Publication:5882763
DOI10.1088/1475-7516/2023/02/063OpenAlexW4322626010MaRDI QIDQ5882763
Publication date: 17 March 2023
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2209.02434
Cites Work
- Higgs inflation: consistency and generalisations
- Variational formulation of general relativity from 1915 to 1925 Palatini's method discovered by Einstein in 1925
- A new improved energy-momentum tensor.
- Linear inflation from quartic potential
- Cosmology in scalar-tensor gravity.
- Natural inflation with hidden scale invariance
- A natural inflation inspired model
- THE PHASE-SPACE VIEW OF INFLATION I: THE NON-MINIMALLY COUPLED SCALAR FIELD
- Higgs inflation with loop corrections in the Palatini formulation
- Resurrecting Quadratic Inflation with a non-minimal coupling to gravity
- Coleman-Weinberg linear inflation: metric vs. Palatini formulation
- Higgs inflation at the hilltop
- Inflationary predictions of double-well, Coleman-Weinberg, and hilltop potentials with non-minimal coupling
- Scalar-tensor linear inflation
- Natural inflation with a nonminimal coupling to gravity
- Higgs inflation in metric and Palatini formalisms: required suppression of higher dimensional operators
- Scalar-tensor extension of natural inflation
- Quadratic, Higgs and hilltop potentials in Palatini gravity
- The Primordial Density Perturbation
- Inflationary universe: A possible solution to the horizon and flatness problems
- Preheating in Palatini Higgs inflation
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