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相关论文: Towards a classification of UV completable Higgs i…

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We investigate the UV-completion of the Higgs inflation in the metric and the Palatini formalisms. It is known that the cutoff scales for the perturbative unitarity of these inflation models become much smaller than the Planck scale to be…

高能物理 - 唯象学 · 物理学 2022-05-27 Yusuke Mikura , Yuichiro Tada

We re-examine the predictiveness of single-field inflationary models and discuss how an unknown UV completion can complicate determining inflationary model parameters from observations, even from precision measurements. Besides the usual…

高能物理 - 唯象学 · 物理学 2015-07-21 C. P. Burgess , Subodh P. Patil , Michael Trott

Higgs inflation is known to be a minimal extension of the Standard Model allowing for the description of the early Universe inflation. This model is considered as an effective field theory since it has a relatively low cutoff scale, thus…

高能物理 - 理论 · 物理学 2021-03-22 Alexey S. Koshelev , Anna Tokareva

In the Higgs inflation scenario the Higgs field is strongly coupled to the Ricci scalar in order to drive primordial inflation. However, in its original form in pure metric formulation of gravity, the ultraviolet (UV) cutoff of the Higgs…

高能物理 - 唯象学 · 物理学 2011-04-19 Florian Bauer , Durmus A. Demir

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…

高能物理 - 理论 · 物理学 2023-05-30 Minxi He , Yusuke Mikura , Yuichiro Tada

In new Higgs inflation the Higgs kinetic terms are non-minimally coupled to the Einstein tensor, allowing the Higgs field to play the role of the inflaton. The new interaction is non-renormalizable, and the model only describes physics…

高能物理 - 唯象学 · 物理学 2018-03-13 Jacopo Fumagalli , Sander Mooij , Marieke Postma

The predictions of Standard Model Higgs inflation are in excellent agreement with the Planck data, without the need for new fields. However, consistency of the theory requires the presence of (unknown) threshold corrections. These modify…

高能物理 - 唯象学 · 物理学 2017-03-15 Jacopo Fumagalli , Marieke Postma

In a recently proposed scenario for primordial inflation, where the Standard Model (SM) Higgs boson plays a role of the inflation field, an effective field theory (EFT) approach is the most convenient for working out the consequences of…

高能物理 - 唯象学 · 物理学 2015-05-20 R. Horvat

This paper studies the quantum corrections to the Higgs inflation model in the context of the Einstein-Cartan (E-C) gravity in the large-$ N $ limit with $N$ being the number of real scalar components in Higgs. Recently, it is realized that…

高能物理 - 唯象学 · 物理学 2024-01-05 Minxi He , Kohei Kamada , Kyohei Mukaida

The present measurement of the standard model (SM) parameters suggests that the Higgs effective potential has a maximum at the intermediate scale, and the electroweak (EW) vacuum is not absolutely stable. The simplest possibility for…

高能物理 - 唯象学 · 物理学 2022-11-08 Wen Yin

We consider a simple extension of the Standard Model Higgs inflation with one new real scalar field which preserves unitarity up to the Planck scale. The new scalar field (called sigma) completes in the ultraviolet the theory of Higgs…

高能物理 - 唯象学 · 物理学 2011-01-28 Gian F. Giudice , Hyun Min Lee

We derive a Higgs inflationary model in the context of a complex geometrical scalar-tensor theory of gravity. In this model the Higgs inflaton scalar field has geometrical origin playing the role of the Weyl scalar field in the original…

广义相对论与量子宇宙学 · 物理学 2020-07-14 José Edgar Madriz Aguilar , J. Zamarripa , M. Montes , C. Romero

Scalar field models of inflation based on a large nonminimal coupling to gravity xi, in particular, Higgs inflation, may violate unitarity at an energy scale ~ M_p / xi << M_p. In this case the model is incomplete at energy scales relevant…

高能物理 - 唯象学 · 物理学 2010-12-01 Rose N. Lerner , John McDonald

We analyse the self-consistency of inflation in the Standard Model, where the Higgs field has a large non-minimal coupling to gravity. We determine the domain of energies in which this model represents a valid effective field theory as a…

高能物理 - 唯象学 · 物理学 2011-03-07 F. Bezrukov , A. Magnin , M. Shaposhnikov , S. Sibiryakov

For inflation driven by the Higgs field coupled non-minimally to gravity, we study the cutoff energy scale above which perturbation theory breaks down. Employing the metric formulation, we first give an overview of known results and then…

高能物理 - 唯象学 · 物理学 2023-07-18 Georgios K. Karananas , Mikhail Shaposhnikov , Sebastian Zell

Models of inflation in which the Higgs field is non-minimally coupled to gravity lead, after a recaling of the metric, to a complicated expression for the potential of the inflaton field. Nevertheless, this potential produces the desired…

高能物理 - 理论 · 物理学 2022-06-08 Noureddine Mohammedi

We discuss a simple unitarization of Higgs inflation that is genuinely weakly coupled up to Planckian energies. A large non-minimal coupling between the Higgs and the Ricci curvature is induced dynamically at intermediate energies, as a…

高能物理 - 唯象学 · 物理学 2015-01-12 J. L. F. Barbon , J. A. Casas , J. Elias-Miro , J. R. Espinosa

Extensions of the Standard Model and general relativity featuring a UV fixed point can leave observable implications at accessible energies. Although mass parameters such as the Planck scale can appear through dimensional transmutation, all…

高能物理 - 唯象学 · 物理学 2019-09-13 Alberto Salvio

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…

高能物理 - 唯象学 · 物理学 2021-10-22 Mikhail Shaposhnikov , Andrey Shkerin , Inar Timiryasov , Sebastian Zell

It is an interesting question whether low energy degrees of freedom may be responsible for early universe inflation. To examine this, here we present a simple version of Higgs-inflation with minimal coupling to gravity and a quadratic…

高能物理 - 唯象学 · 物理学 2012-08-10 Mark P. Hertzberg
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