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相关论文: Higgs Inflation and the Electroweak Gauge Sector

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Slow-roll inflation requires the inflaton field to have an exceptionally flat potential, which combined with measurements of the scale of inflation demands some degree of fine-tuning. Alternatively, the flatness of the potential could be…

高能物理 - 唯象学 · 物理学 2015-06-23 Djuna Croon , Veronica Sanz

Models of axion inflation based on a single cosine potential require the axion decay constant $f$ to be super-Planckian in size. However, $f > M_{Pl}$ is disfavored by the Weak Gravity Conjecture (WGC). It is then pertinent to ask if one…

高能物理 - 唯象学 · 物理学 2019-06-10 Pran Nath , Maksim Piskunov

The observed value of the Higgs mass indicates the possibility that there is no supersymmetry below the Planck scale and that the Higgs can play the role of the inflaton. We examine the general structure of the saddle point inflation in…

高能物理 - 唯象学 · 物理学 2015-09-09 Yuta Hamada , Hikaru Kawai , Kiyoharu Kawana

We discuss the phenomenological implications of hybrid natural inflation models in which the inflaton is a pseudo-Goldstone boson but inflation is terminated by a second scalar field. A feature of the scheme is that the scale of breaking of…

高能物理 - 唯象学 · 物理学 2014-11-20 Graham G Ross , Gabriel German

The constraint on the mass of Higgs field in the Standard Model at the minimal interaction with the gravity is derived in the form of lower bound $m_H> 150$ GeV by the strict requirement of decoupling the Higgs boson from the inflation of…

广义相对论与量子宇宙学 · 物理学 2010-05-10 V. V. Kiselev , S. A. Timofeev

We find that the triplet Higgs of the Type II seesaw mechanism can simultaneously generate the neutrino masses and observed baryon asymmetry, while playing a role in inflation. We survey the allowed parameter space and determine that this…

高能物理 - 唯象学 · 物理学 2022-04-20 Neil D. Barrie , Chengcheng Han , Hitoshi Murayama

In the composite Higgs models, originally proposed by Georgi and Kaplan, the Higgs boson is a pseudo Nambu-Goldstone boson (pNGB) of spontaneous breaking of a global symmetry. In the minimal version of such models, global SO(5) symmetry is…

高能物理 - 唯象学 · 物理学 2016-08-03 Shinya Kanemura , Kunio Kaneta , Naoki Machida , Shinya Odori , Tetsuo Shindou

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 may affect the degeneracy of the inflationary…

宇宙学与河外天体物理 · 物理学 2009-10-29 L. A. Popa

We investigate a simple model to explain inflation, neutrino masses and dark matter simultaneously. This is based on the so-called radiative seesaw model proposed by Ma in order to explain neutrino masses and dark matter by introducing a…

高能物理 - 唯象学 · 物理学 2015-06-12 Shinya Kanemura , Toshinori Matsui , Takehiro Nabeshima

In this talk, I shall focus on theories beyond the Standard Model which predict massive neutrinos. Hybrid inflation emerges naturally in these theories: the slow-rolling inflaton field is a gauge singlet which couples with a GUT Higgs field…

高能物理 - 唯象学 · 物理学 2007-05-23 Rachel Jeannerot

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

Models addressing the naturalness of a light Higgs boson typically employ symmetries, either bosonic or fermionic, to stabilize the Higgs mass. We consider a setup with the minimal amount of symmetries: four shift symmetries acting on the…

高能物理 - 唯象学 · 物理学 2015-06-24 Ian Low

We study the possibility that the Higgs and the inflaton are the same single field or cousins arising from the extra space components of some higher-dimensional gauge field. We take 5D supersymmetric gauge theory with a matter compactified…

高能物理 - 理论 · 物理学 2009-11-19 Takeo Inami , Yoji Koyama , C. S. Lim , Shie Minakami

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

Composite Higgs models can trivially satisfy precision-electroweak and flavour constraints by simply having a large spontaneous symmetry breaking scale, f > 10 TeV. This produces a 'split' spectrum, where the strong sector resonances have…

高能物理 - 唯象学 · 物理学 2015-06-23 James Barnard , Tony Gherghetta , Tirtha Sankar Ray , Andrew Spray

Higgs inflation uses the gauge variant Higgs field as the inflaton. During inflation the Higgs field is displaced from its minimum, which results in associated Goldstone bosons that are apparently massive. Working in a minimally coupled…

高能物理 - 唯象学 · 物理学 2012-07-31 Sander Mooij , Marieke Postma

We study inflation driven by a slow-rolling inflaton field, characterised by a quadratic potential, and incorporating radiative corrections within the context of supergravity. In this model the energy scale of inflation is not overly…

高能物理 - 唯象学 · 物理学 2011-02-16 Gabriel German , Graham Ross , Subir Sarkar

We study the post-inflationary dynamics of the Standard Model Higgs and a real singlet scalar $s$, coupled together through a renormalizable coupling $\lambda_{sh}h^2s^2$, in a $Z_2$ symmetric model that may explain the observed dark matter…

宇宙学与河外天体物理 · 物理学 2014-09-08 Kari Enqvist , Sami Nurmi , Tommi Tenkanen , Kimmo Tuominen

This work explores the possibility of inflation in a scale-symmetric extension of the Standard Model Higgs sector, where the Higgs field $\phi_1$ is coupled to a singlet scalar, the dilaton $\phi_0$. The two-scalar theory is formulated…

高能物理 - 唯象学 · 物理学 2026-04-01 Z. Lalak , P. Michalak

We investigate inflation driven by the Higgs boson in the Palatini formulation of General Relativity. Our analysis primarily focuses on a small non-minimal coupling of the Higgs field to gravity in the range $0<\xi\lesssim 1$. We…

高能物理 - 唯象学 · 物理学 2023-06-07 Arthur Poisson , Inar Timiryasov , Sebastian Zell
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