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We investigate the cosmological inflation for the Einstein-Hilbert action plus the Higgs potential function and the Gauss-Bonnet term coupled with the Higgs scalar field through a dilaton-like coupling. Then, using the…

广义相对论与量子宇宙学 · 物理学 2026-05-29 Zahra Ahghari , Mehrdad Farhoudi

The Higgs field is an attractive candidate for the inflaton because it is an observationally confirmed fundamental scalar field. Importantly, it can be modeled by the most general renormalizable scalar potential. However, if the classical…

宇宙学与河外天体物理 · 物理学 2021-03-29 Martin Bojowald , Suddhasattwa Brahma , Sean Crowe , Ding Ding , Joseph McCracken

The measured masses of the Higgs boson and top quark indicate that the effective potential of the standard model either develops an unstable electroweak vacuum or stands stable all the way up to the Planck scale. In the latter case in which…

高能物理 - 唯象学 · 物理学 2015-09-15 Rong-Gen Cai , Zong-Kuan Guo , Shao-Jiang Wang

We investigate inflationary dynamics in the framework of the Einstein-Gauss-Bonnet gravity. In the model under consideration, the inflaton field is non-minimally coupled to the Gauss-Bonnet curvature invariant, so that the latter appears to…

广义相对论与量子宇宙学 · 物理学 2020-09-02 Ekaterina O. Pozdeeva , Mayukh Raj Gangopadhyay , Mohammad Sami , Alexey V. Toporensky , Sergey Yu. Vernov

We generalize the scalar-curvature coupling model ${\xi \Phi^2 R}$ of Higgs inflation to $ {\xi \Phi^a R^b} $ to study inflation. We compute the amplitude and spectral index of curvature perturbations generated during inflation and fix the…

宇宙学与河外天体物理 · 物理学 2014-03-21 Girish Chakravarty , Subhendra Mohanty , Naveen K. Singh

We critically examine the recent claim that the Standard Model Higgs boson ${\cal H}$ could drive inflation in agreement with observations if $|{\cal H}|^2$ has a strong coupling $\xi\sim 10^4$ to the Ricci curvature scalar. We first show…

高能物理 - 唯象学 · 物理学 2010-03-12 J. L. F. Barbon , J. R. Espinosa

We consider a quantum corrected inflation scenario driven by a generic GUT or Standard Model type particle model whose scalar field playing the role of an inflaton has a strong non-minimal coupling to gravity. We show that currently widely…

高能物理 - 唯象学 · 物理学 2009-01-06 A. O. Barvinsky , A. Yu. Kamenshchik , A. A. Starobinsky

We study the possibility of standard model Higgs boson acting as an inflaton field in the framework of Horava-Lifshitz Gravity. Under this framework, we showed that it is possible for the Higgs field to produce right amount of inflation and…

高能物理 - 理论 · 物理学 2011-04-25 Taotao Qiu , Debaprasad Maity

It is likely that the Higgs potential of the Standard Model is unstable, turning negative at $\phi < \Lambda \sim 10^{10}$ GeV. Here we consider whether it is possible to have Higgs Inflation on the positive stable region of the potential…

高能物理 - 唯象学 · 物理学 2023-09-14 John McDonald

The accelerated expansion of the early universe is an integral part of modern cosmology and dynamically realized by the mechanism of inflation. The simplest theoretical description of the inflationary paradigm is based on the assumption of…

高能物理 - 唯象学 · 物理学 2021-04-14 Christian F. Steinwachs

For a robust interpretation of upcoming observations from PLANCK and LHC experiments it is imperative to understand how the inflationary dynamics of a non-minimally coupled Higgs scalar field with gravity may affect the determination of the…

宇宙学与河外天体物理 · 物理学 2011-01-27 L. A. Popa , A. Caramete

The discovery of Higgs mechanism within the context of spontaneous symmetry breaking has offered a new perspective on the early time cosmic inflation and also on the relationship between elementary particles and dark energy, believed to…

高能物理 - 理论 · 物理学 2024-06-14 Manda Malekpour , Kourosh Nozari

A simple realization of inflation consists of adding the following operators to the Einstein-Hilbert action: (partial phi)^2, lambda phi^4, and xi phi^2 R, with xi a large non-minimal coupling. Recently there has been much discussion as to…

高能物理 - 唯象学 · 物理学 2010-12-01 Mark P. Hertzberg

Inflection-point inflation is an interesting possibility to realize a successful slow-roll inflation when inflation is driven by a single scalar field with its initial value below the Planck mass ($\phi_I \lesssim M_{Pl}$). In order for a…

高能物理 - 唯象学 · 物理学 2017-03-08 Nobuchika Okada , Digesh Raut

Higgs field of particle physics can play the role of the inflaton in the early universe, if it is non-minimally coupled to gravity. The Higgs inflation scenario predicts a small tensor to scalar ratio: $r\simeq 0.003$. Although this value…

高能物理 - 理论 · 物理学 2015-09-02 Sarang Zeynizadeh , Amin Rezaei Akbarieh

We propose a novel possibility for Higgs inflation where the perturbative unitarity below the Planck scale is ensured by construction and the successful predictions for inflation are accommodated. The conformal gravity coupling for the…

高能物理 - 唯象学 · 物理学 2023-10-17 Simon Cléry , Hyun Min Lee , Adriana G. Menkara

The generation of large curvature perturbations associated with the production of primordial black holes is studied in the context of a Higgs inflaton. To enable this amplification, we consider an inflationary model in which the tree-level…

高能物理 - 唯象学 · 物理学 2025-09-24 A. Tronconi , G. Venturi

The properties of the recently discovered Higgs boson together with the absence of new physics at collider experiments allows us to speculate about consistently extending the Standard Model of particle physics all the way up to the Planck…

高能物理 - 唯象学 · 物理学 2019-03-14 Javier Rubio

We study a scalar field with non-minimal kinetic coupling to itself and to the curvature. The slow rolling conditions allowing an inflationary background have been found. The quadratic and Higgs type potentials have been considered, and the…

高能物理 - 理论 · 物理学 2011-05-12 L. N. Granda

It is a longstanding desire of cosmologists, and particle physicists as well, to connect inflation to low energy physics, culminating, for instance, in what is known as Higgs inflation. The condition for the standard Higgs boson playing the…

高能物理 - 唯象学 · 物理学 2017-11-15 J. G. Ferreira , C. A. de S. Pires , J. G. Rodrigues , P. S. Rodrigues da Silva
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