Higgs inflation in Einstein-Cartan gravity
arXiv:2007.14978 · doi:10.1088/1475-7516/2021/02/008
Abstract
We study inflation driven by the Higgs field in the Einstein-Cartan formulation of gravity. In this theory, the presence of the Holst and Nieh-Yan terms with the Higgs field non-minimally coupled to them leads to three additional coupling constants. For a broad range of parameters, we find that inflation is both possible and consistent with observations. In most cases, the spectral index is given by (with the number of e-foldings) whereas the tensor-to-scalar ratio can vary between about and . Thus, there are scenarios of Higgs inflation in the Einstein-Cartan framework for which the detection of gravitational waves from inflation is possible in the near future. In certain limits, the known models of Higgs inflation in the metric and Palatini formulations of gravity are reproduced. Finally, we discuss the robustness of inflationary dynamics against quantum corrections due to the scalar and fermion fields.
26 pages, 8 figures, 1 appendix; v2: updated figures and references, added short comparison with arXiv:2007.12595, minor corrections to formulas in sections 6.2 and 6.3, other small improvements; matches published version (including erratum)
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Cited by in corpus (33)
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- Coupling Metric-Affine Gravity to a Higgs-Like Scalar Field
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- Tachyonic Preheating in Palatini Inflation
- Higgs-Modular Inflation
- Einstein-Cartan Portal to Dark Matter
- Matter matters in Einstein-Cartan gravity
- Einstein-Cartan gravity, matter, and scale-invariant generalization
- Independent connection in ACTion during inflation
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- Field redefinitions, perturbative unitarity and Higgs inflation
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- Extended interactions in the Palatini- inflation
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