Hybrid metric-Palatini Higgs inflation
Minxi He, Yusuke Mikura, Yuichiro Tada

TL;DR
This paper extends Higgs inflation within hybrid metric-Palatini gravity, exploring inflationary predictions, unitarity, and UV completions, revealing conditions for effective field theories and potential for observable cosmological signatures.
Contribution
It introduces a novel hybrid metric-Palatini Higgs inflation model with detailed inflationary and unitarity analysis, and proposes a UV extension with an additional scalar field.
Findings
Slow-roll inflation achieved with observationally consistent spectral index.
Tensor-to-scalar ratio varies with non-minimal couplings, maxing at ~10^{-3}.
UV cutoff is lower than Planck scale, but can be improved with extra scalar fields.
Abstract
We propose an extension of the Higgs inflation to the hybrid metric-Palatini gravity, where we introduce non-minimal couplings between Higgs and both the metric-type and the Palatini-type Ricci scalars. We study the inflationary phenomenology of our model and find that slow-roll inflation can be realized in the large-field regime, giving the observationally favored predictions. In particular, the scalar spectral index exhibits an attractor behavior to , while the tensor-to-scalar ratio can take an arbitrary value depending on the non-minimal coupling parameters, with the metric-Higgs limit being the maximum. We also investigate the unitarity property of our model. As the ultraviolet (UV) cutoff as a low-energy effective field theory (EFT) of this model is significantly lower than the Planck scale due to a strong curvature of field-space, we…
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Taxonomy
TopicsCosmology and Gravitation Theories · Black Holes and Theoretical Physics · Geophysics and Gravity Measurements
