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相关论文: Are $R^2$- and Higgs-inflations really unlikely?

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We investigate whether Higgs inflation can occur in the Standard Model starting from natural initial conditions or not. The Higgs has a non-minimal coupling to the Ricci scalar. We confine our attention to the regime where quantum Einstein…

高能物理 - 唯象学 · 物理学 2016-02-16 Alberto Salvio , Anupam Mazumdar

We examine the class of initial conditions which give rise to inflation. Our analysis is carried out for several popular models including: Higgs inflation, Starobinsky inflation, chaotic inflation, axion monodromy inflation and…

广义相对论与量子宇宙学 · 物理学 2018-11-07 Swagat S. Mishra , Varun Sahni , Alexey V. Toporensky

We study initial conditions for inflation in scenarios where the inflaton potential has a plateau shape. Such models are those most favored by Planck data and can be obtained in a large number of model classes. As a representative example,…

宇宙学与河外天体物理 · 物理学 2020-04-29 Tommi Tenkanen , Eemeli Tomberg

We consider Higgs inflation with an $\alpha R^2$ term. It adds a new scalar degree of freedom, which leads to a two-field model of inflation. We do a complete slow-roll analysis of the three-dimensional parameter space of the $R^2$…

宇宙学与河外天体物理 · 物理学 2020-01-22 Vera-Maria Enckell , Kari Enqvist , Syksy Rasanen , Lumi-Pyry Wahlman

It is known that the Higgs potential becomes flat around the Planck scale under the assumption that the Standard Model is valid up to very high scale. Taking this into account, we revisit the Higgs inflation scenario and find that the…

高能物理 - 唯象学 · 物理学 2015-04-23 Yuta Hamada

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

Inflation based on scalar fields which are non-minimally coupled to gravity has been proposed as a way to unify inflation with weak-scale physics, with the inflaton being identified with the Higgs boson or other weak-scale scalar article.…

高能物理 - 唯象学 · 物理学 2010-04-30 Rose N. Lerner , John McDonald

We rebut the recent claim (arXiv:0912.5463) that Einstein-frame scattering in the Higgs inflation model is unitary above the cut-off energy Lambda ~ Mp/xi. We show explicitly how unitarity problems arise in both the Einstein and Jordan…

高能物理 - 唯象学 · 物理学 2014-11-20 C. P. Burgess , Hyun Min Lee , Michael Trott

For the central values of the relevant experimental inputs, that is the strong coupling constant and the top quark and Higgs masses, the effective Higgs potential displays two minima, one at the electroweak scale and a deeper one at high…

高能物理 - 唯象学 · 物理学 2026-02-04 Isabella Masina , Mariano Quiros

We consider $R^2$ inflation in the Palatini gravity assuming the existence of scalar fields, coupled to gravity in the most general manner. These theories, in the Einstein frame, and for one scalar field $h$, share common features with $K$…

广义相对论与量子宇宙学 · 物理学 2020-04-08 Ioannis D. Gialamas , A. B. Lahanas

We derive one- and two-loop renormalization group equations (RGEs) of Higgs-$R^2$ inflation. This model has a non-minimal coupling between the Higgs and the Ricci scalar and a Ricci scalar squared term on top of the standard model. The RGEs…

高能物理 - 唯象学 · 物理学 2021-03-17 Yohei Ema , Kyohei Mukaida , Jorinde van de Vis

We consider models of chaotic inflation driven by the real parts of a conjugate pair of Higgs superfields involved in the spontaneous breaking of a grand unification symmetry at a scale assuming its supersymmetric value. Employing quadratic…

高能物理 - 唯象学 · 物理学 2018-01-30 C. Pallis

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

Within the Standard Model, the current Higgs and top quark data favor metastability of the electroweak vacuum, although the uncertainties are still significant. The true vacuum is many orders of magnitude deeper than ours and the barrier…

高能物理 - 唯象学 · 物理学 2015-06-11 Oleg Lebedev , Alexander Westphal

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

We construct a chaotic inflation model in which the Higgs fields play the role of the inflaton in the standard model as well as in the singlet extension of the supersymmetric standard model. The key idea is to allow a non-canonical kinetic…

高能物理 - 唯象学 · 物理学 2011-02-15 Kazunori Nakayama , Fuminobu Takahashi

We consider models of chaotic inflation driven by the real parts of a conjugate pair of Higgs superfields involved in the spontaneous breaking of a grand unification symmetry at a scale assuming its supersymmetric value. We combine a…

高能物理 - 唯象学 · 物理学 2016-01-22 C. Pallis

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

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

Recently there was an extensive discussion of Higgs inflation in the theory with the potential \lambda(\phi^2-v^2)^2 and nonminimal coupling to gravity {\xi\over 2}\phi^2R, for \xi >> 1 and v<< 1. We extend this investigation to the…

高能物理 - 理论 · 物理学 2015-03-17 Andrei Linde , Mahdiyar Noorbala , Alexander Westphal
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