Palatini double-well and Coleman-Weinberg potentials with non-minimal coupling
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Publication:5026124
DOI10.1088/1475-7516/2021/04/042zbMath1485.83123arXiv2009.04406OpenAlexW3156604001MaRDI QIDQ5026124
Publication date: 7 February 2022
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2009.04406
Relativistic cosmology (83F05) Quantization of the gravitational field (83C45) Symmetry breaking in quantum theory (81R40) Gravitational energy and conservation laws; groups of motions (83C40)
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
- Non-minimal (self-)running inflation: metric vs. Palatini formulation
- Tracing the high energy theory of gravity: an introduction to Palatini inflation
- Field theories with « Superconductor » solutions
- THE PHASE-SPACE VIEW OF INFLATION I: THE NON-MINIMALLY COUPLED SCALAR FIELD
- Higgs inflation with loop corrections in the Palatini formulation
- Coleman-Weinberg linear inflation: metric vs. Palatini formulation
- Quantum corrections to quartic inflation with a non-minimal coupling: metric vs. Palatini
- Higgs inflation at the hilltop
- Palatini inflation in models with an R2 term
- Inflationary predictions of double-well, Coleman-Weinberg, and hilltop potentials with non-minimal coupling
- Scalar-tensor linear inflation
- Dynamically induced Planck scale and inflation in the Palatini formulation
- Higgs inflation in metric and Palatini formalisms: required suppression of higher dimensional operators
- Quadratic, Higgs and hilltop potentials in Palatini gravity
- The Primordial Density Perturbation
- Inflationary universe: A possible solution to the horizon and flatness problems
- Nonminimal Coleman-Weinberg inflation with an R2 term
- Preheating in Palatini Higgs inflation