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相关论文: Natural Higgs Inflation, Gauge Coupling Unificatio…

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Several authors have recently argued that a satisfactory inflationary scenario can be implemented in the Standard Model (SM) by introducing a strong non-minimal coupling of the Higgs doublet to gravity. It is shown here that type I seesaw…

高能物理 - 唯象学 · 物理学 2009-12-02 Nobuchika Okada , Mansoor Ur Rehman , Qaisar Shafi

We investigate the dependency of Higgs inflation on the non-renormalisable matching between the low energy Standard Model limit and the inflationary regime at high energies. We show that for the top mass range $m_t \gtrsim 171.8$ GeV the…

宇宙学与河外天体物理 · 物理学 2016-08-17 Vera-Maria Enckell , Kari Enqvist , Sami Nurmi

We have realized non-minimal Higgs inflation and standard hybrid inflation in the supersymmetric flipped $SU(5)$ model with $U(1)_R$ symmetry using the no-scale form of the K\"{a}hler potential. In non-minimal Higgs inflation the waterfall…

高能物理 - 唯象学 · 物理学 2021-10-12 Mian Muhammad Azeem Abid , Maria Mehmood , Mansoor Ur Rehman , Qaisar Shafi

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

Higgs inflation can occur if the Standard Model (SM) is a self-consistent effective field theory up to inflationary scale. This leads to a lower bound on the Higgs boson mass, $M_h \geq M_{\text{crit}}$. If $M_h$ is more than a few hundreds…

高能物理 - 唯象学 · 物理学 2015-06-19 Fedor Bezrukov , Mikhail Shaposhnikov

An extension of the Standard Model with three right-handed neutrinos and a simple invisible axion model can account for all experimentally confirmed signals of new physics (neutrino oscillations, dark matter and baryon asymmetry) in…

高能物理 - 唯象学 · 物理学 2019-02-06 Alberto Salvio

We briefly review several Higgs inflation models and discuss their cosmological implications. We first classify the inflation models according to the predicted value of the tensor-to-scalar ratio: (i) $r = {\cal O}(0.01-0.1)$, (ii) $r =…

高能物理 - 唯象学 · 物理学 2015-06-01 Fuminobu Takahashi

We consider the inflation model generated by the Standard Model (SM) Higgs boson having a strong non-minimal curvature coupling. This model suggests the range of the Higgs mass $135.6\; {\rm GeV} \lesssim M_H\lesssim 184.5\;{\rm GeV}$…

高能物理 - 理论 · 物理学 2015-05-20 Andrei O. Barvinsky

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

A non-minimal coupling xi of the Standard Model Higgs field to gravity can give rise to inflation, but large xi is required and thus leads to a violation of perturbative unitarity at Mp/xi, which is well below the inflationary scale…

高能物理 - 唯象学 · 物理学 2014-03-24 Kyle Allison

Supersymmetric Unified theories which incorporate a renormalizable Type I seesaw mechanism for small neutrino masses can also provide slow roll inflection point inflation along a flat direction associated with a gauge invariant combination…

高能物理 - 唯象学 · 物理学 2012-09-21 Charanjit S. Aulakh , Ila Garg

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

Renormalisation group analysis with the present measurements of the top quark mass $m_t = 172.69\pm 0.30$ GeV indicates that the Standard Model (SM) Higgs potential becomes unstable at energy scales $\sim 10^{10}$ GeV. This may be…

高能物理 - 唯象学 · 物理学 2024-02-26 Shinsuke Kawai , Nobuchika Okada , Qaisar Shafi

We analyse one-loop radiative corrections to the inflationary potential in the theory, where inflation is driven by the Standard Model Higgs field. We show that inflation is possible provided the Higgs mass m_H lies in the interval…

高能物理 - 唯象学 · 物理学 2010-05-28 Fedor L. Bezrukov , Amaury Magnin , Mikhail Shaposhnikov

A minimal extension of the Standard Model (SM) with a single new mass scale and providing a complete and consistent picture of particle physics and cosmology up to the Planck scale is presented. We add to the SM three right-handed…

高能物理 - 唯象学 · 物理学 2017-02-22 Guillermo Ballesteros , Javier Redondo , Andreas Ringwald , Carlos Tamarit

Higgs inflation is attractive because it identifies the inflaton with the electroweak Higgs boson. In this work, we construct a new class of supersymmetric Higgs inflationary models in the no-scale supergravity with an SU(5) GUT group.…

高能物理 - 唯象学 · 物理学 2015-01-22 John Ellis , Hong-Jian He , Zhong-Zhi Xianyu

We consider the possibility to observationally differentiate the Standard Model (SM) Higgs driven inflation with non-minimal couplingto gravity from other variants of SM Higgs inflation based on the scalar field theories with non-canonical…

宇宙学与河外天体物理 · 物理学 2015-05-28 L. A. Popa

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 derive a Higgs inflationary model in the context of holographic cosmology, where we consider a universe filled with a Higgs field non-minimally coupled to gravity in a slow-roll regime. The amplitude of density (scalar) perturbations is…

广义相对论与量子宇宙学 · 物理学 2021-01-28 Aatifa Bargach , Farida Bargach , Mariam Bouhmadi-López , Taoufik Ouali

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

广义相对论与量子宇宙学 · 物理学 2018-02-27 Jan Kwapisz , Krzysztof A. Meissner
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