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相关论文: False Vacuum Higgs Inflation and the Graviweak Uni…

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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

We consider a minimal classically scale-invariant extension of the Standard Model. In this theory, the Higgs mechanism is triggered and the electroweak symmetry breaking is generated radiatively by the Coleman-Weinberg sector which is…

高能物理 - 唯象学 · 物理学 2015-06-17 Valentin V. Khoze

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

We study gravitational interaction of Higgs boson through the unique dimension-4 operator $\xi H^\dag H R$, with $H$ the Higgs doublet and $R$ the Ricci scalar curvature. We analyze the effect of this dimensionless nonminimal coupling $\xi$…

广义相对论与量子宇宙学 · 物理学 2014-06-16 Jing Ren , Zhong-Zhi Xianyu , Hong-Jian He

Extrapolating the Standard Model Higgs potential at high energies, we study the barrier between the electroweak and Planck scale minima. The barrier arises by taking the central values of the relevant experimental inputs, that is the strong…

高能物理 - 唯象学 · 物理学 2024-11-27 Isabella Masina , Mariano Quiros

We consider the Higgs inflation in the extension of the Standard Model with two Higgs doublets coupled to gravity non-minimally. In the presence of an approximate global U(1) symmetry in the Higgs sector, both radial and angular modes of…

高能物理 - 唯象学 · 物理学 2015-06-04 Jinn-Ouk Gong , Sin Kyu Kang , Hyun Min Lee

For a narrow band of values of the top quark and Higgs boson masses, the Standard Model Higgs potential develops a false minimum at energies of about $10^{16}$ GeV, where primordial Inflation could have started in a cold metastable state. A…

高能物理 - 唯象学 · 物理学 2013-05-30 Isabella Masina , Alessio Notari

For a narrow band of values of the top quark and Higgs boson masses, the Standard Model Higgs potential develops a shallow local minimum at energies of about $10^{16}$ GeV, where primordial inflation could have started in a cold metastable…

宇宙学与河外天体物理 · 物理学 2014-06-11 Isabella Masina

We construct a new inflation model in which the standard model Higgs boson couples minimally to gravity and acts as the inflaton. Our construction of Higgs inflation incorporates the standard model with Einstein gravity which exhibits…

宇宙学与河外天体物理 · 物理学 2014-11-04 Zhong-Zhi Xianyu , Hong-Jian He

If the Standard Model is valid up to very high energies it is known that the Higgs potential can develop a local minimum at field values around $10^{15}-10^{17}$ GeV, for a narrow band of values of the top quark and Higgs masses. We show…

高能物理 - 唯象学 · 物理学 2013-05-30 Isabella Masina , Alessio Notari

We propose a model for cosmic inflation which is based on an effective description of strongly interacting, nonsupersymmetric matter within the framework of dynamical Abelian projection and centerization. The underlying gauge symmetry is…

高能物理 - 唯象学 · 物理学 2009-11-07 Ralf Hofmann , Mathias Th. Keil

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

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

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

We have recently suggested [1,2] that Inflation could have started in a local minimum of the Higgs potential at field values of about $10^{15}-10^{17}$ GeV, which exists for a narrow band of values of the top quark and Higgs masses and thus…

高能物理 - 唯象学 · 物理学 2015-06-04 Isabella Masina , Alessio Notari

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

This thesis presents a possible inflation scenario as a consequence of non-minimal gravitational couplings in the Conformal Standard Model. That model consists, in comparison to the SM, of additional right-chiral neutrinos and a complex…

广义相对论与量子宇宙学 · 物理学 2019-11-13 Jan Henryk Kwapisz

Higgs inflation with a Gauss-Bonnet term is studied in the Einstein frame. Our model features two coupling functions, $\Omega^2(\phi)$ and $\omega(\phi)$, coupled to the Ricci scalar and Gauss-Bonnet combinations. We found a special…

广义相对论与量子宇宙学 · 物理学 2024-03-26 Seoktae Koh , Seong Chan Park , Gansukh Tumurtushaa

The Higgs inflation scenario is an approach to realize the cosmic inflation, where the Higgs boson plays a role of the inflaton. In the minimal model, it would be difficult to satisfy theoretical constraints from vacuum stability and…

高能物理 - 唯象学 · 物理学 2014-05-23 Toshinori Matsui

The quartic and trilinear Higgs field couplings to an additional real scalar are renormalizable, gauge and Lorentz invariant. Thus, on general grounds, one expects such couplings between the Higgs and an inflaton in quantum field theory. In…

高能物理 - 唯象学 · 物理学 2018-12-26 Yohei Ema , Mindaugas Karciauskas , Oleg Lebedev , Stanislav Rusak , Marco Zatta