中文
相关论文

相关论文: Higgs-Inflaton Mixing and Vacuum Stability

200 篇论文

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 investigate the role of the Higgs field as a fundamental scalar in the Standard Model within the framework of modular inflation models, where a modulus field acts as the inflaton and its interactions are governed by an underlying modular…

高能物理 - 唯象学 · 物理学 2025-08-06 Shuntaro Aoki , Hajime Otsuka , Ryota Yanagita

If Higgs is a spectator scalar, i.e. if it is not directly coupled to the inflaton, superhorizon Higgs modes must have been exited during inflation. Since Higgs is unstable its decay into photons is expected to seed superhorizon photon…

广义相对论与量子宇宙学 · 物理学 2018-04-11 Ali Kaya

In the standard model the (Brout-Englert-)Higgs quartic coupling becomes negative at high energies rendering our current electroweak vacuum metastable, but with an instability timescale much longer than the age of the Current Universe.…

高能物理 - 唯象学 · 物理学 2019-02-20 David Rodriguez-Roman , Malcolm Fairbairn

The measurement of the trilinear and quartic Higgs self-couplings is necessary for the reconstruction of the Higgs potential. This way the Higgs mechanism as the origin of electroweak symmetry breaking can be tested. The couplings are…

高能物理 - 唯象学 · 物理学 2015-03-17 Ramona Grober , Margarete Muhlleitner

Higgs G-inflation is an inflation model that takes advantage of a Galileon-like derivative coupling. It is a non-renormalizable operator and is strongly coupled at high energy scales. Perturbative analysis does not have a predictive power…

高能物理 - 唯象学 · 物理学 2015-05-20 Kohei Kamada

We study the effects of the Higgs directly coupled to the inflaton on the primordial power spectrum. The quadratic coupling between the Higgs and the inflaton stabilizes the Higgs in the electroweak vacuum during inflation by inducing a…

高能物理 - 唯象学 · 物理学 2015-12-04 Jinn-Ouk Gong , Chengcheng Han , Shi Pi

In this work, we investigated the electroweak vacuum instability during or after inflation. In the inflationary Universe, i.e., de Sitter space, the vacuum field fluctuations $\left< {\delta \phi }^{ 2 } \right>$ enlarge in proportion to…

高能物理 - 唯象学 · 物理学 2017-08-09 Kazunori Kohri , Hiroki Matsui

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

During inflation in the early universe, the Higgs field continuously acquires long-wave quantum fluctuations. They accumulate to yield a non-vanishing value with an exponentially large correlation length. We study consequences of such Higgs…

高能物理 - 唯象学 · 物理学 2012-10-30 Taro Kunimitsu , Jun'ichi Yokoyama

The Higgs field of the pure Standard Model can lead to the inflationary expansion of the early Universe if it is non-minimally coupled to gravity. The model predicts Cosmic Microwave Background (CMB) parameters in perfect agreement with the…

高能物理 - 唯象学 · 物理学 2013-10-09 Fedor Bezrukov

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 the augmentation of the Standard Model (SM) with another $SU(2)$ Higgs doublet and right-handed neutrinos. The second Higgs doublet ($\Phi_2$) is defined to be odd under the $Z_2$ symmetry, and hence, the lightest stable neutral…

高能物理 - 唯象学 · 物理学 2026-02-03 Seong Chan Park , Shilpa Jangid

We study cosmological gravitational particle production (CGPP) in Higgs inflation, wherein the inflaton is a scalar field with quartic self-coupling $\lambda$ and a nonminimal coupling to gravity $\xi$, and which may, but need not be, the…

高能物理 - 唯象学 · 物理学 2025-10-29 Tammi Chowdhury , Leah Jenks , Edward W. Kolb , Evan McDonough

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

In the absence of new physics around $10^{10}$ GeV, the electroweak vacuum is at best metastable. This represents a major challenge for high scale inflationary models as, during the early rapid expansion of the universe, it seems difficult…

高能物理 - 唯象学 · 物理学 2018-01-17 Xavier Calmet , Iberê Kuntz , Ian G. Moss

We consider a possibility that the Higgs field in the Standard Model (SM) serves as an inflaton when its value is around the Planck scale. We assume that the SM is valid up to an ultraviolet cutoff scale \Lambda, which is slightly below the…

高能物理 - 唯象学 · 物理学 2014-02-11 Yuta Hamada , Hikaru Kawai , Kin-ya Oda

An elementary Higgs boson, which is the remnant of the spontaneous symmetry breaking mechanism in the Standard Model, remains one of the most elusive particles. If a Higgs boson candidate is found at future accelerators, it becomes…

高能物理 - 唯象学 · 物理学 2007-05-23 P. Osland , P. N. Pandita

The direct coupling between the Higgs field and the spacetime curvature, if finely tuned, is known to stabilize the Higgs boson mass. The fine-tuning is soft because the Standard Model (SM) parameters are subject to no fine-tuning thanks to…

高能物理 - 唯象学 · 物理学 2015-11-04 Beste Korutlu

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