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相关论文: On stability of electroweak vacuum during inflatio…

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The recently suggested Festina-Lente (FL) bound provides a lower bound on the masses of ${\rm U(1)}$ charged particles in terms of the positive vacuum energy. Since the charged particle masses in the Standard Model (SM) are generated by the…

高能物理 - 唯象学 · 物理学 2022-02-17 Sung Mook Lee , Dhong Yeon Cheong , Sang Chul Hyun , Seong Chan Park , Min-Seok Seo

We study the effect of inflation on gaugino condensation in supergravity. Unless the Hubble scale H is significantly below the gaugino condensation scale, the gaugino condensate is a dynamical variable which cannot be integrated out. For a…

高能物理 - 理论 · 物理学 2010-02-01 Oleg Lebedev , Chloe Papineau , Marieke Postma

Using a new approach to the analysis of false vacuum decay based on the so-called tunneling potential, we develop a general method to find scalar potentials with a false vacuum with exactly solvable decay at the semi-classical level,…

高能物理 - 理论 · 物理学 2021-09-15 J. R. Espinosa , J. -F. Fortin , J. Huertas

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

Small evaporating black holes were proposed to be dangerous inducing fast decay of the electroweak false vacuum. We observe that the flat-spectrum matter perturbations growing at the post-inflationary matter dominated stage can produce such…

宇宙学与河外天体物理 · 物理学 2017-10-20 Dmitry Gorbunov , Dmitry Levkov , Alexander Panin

We revisit the compatibility between the chaotic inflation, which provides a natural solution to the initial condition problem, and the metastable electroweak vacuum, which is suggested by the results of LHC and the current mass…

高能物理 - 唯象学 · 物理学 2016-11-22 Masahiro Kawasaki , Kyohei Mukaida , Tsutomu T. Yanagida

In the present paper we discuss how trans-Planckian physics affects inflationary vacuum fluctuations and primordial density perturbations. The trans-Planckian problem during inflation has been widely discussed in literature, but it is still…

高能物理 - 理论 · 物理学 2019-08-21 Hiroki Matsui

In the conventional metric formulation of gravity, the Higgs Inflation model violates unitarity in the electroweak vacuum in Higgs scattering at the energy scale $\Lambda \sim M_{Pl}/\xi$, where $\xi \sim 10^4$ is the non-minimal coupling…

高能物理 - 唯象学 · 物理学 2021-05-05 J. McDonald

We consider a model of D-term inflation in which the inflaton coincides with the standard Higgs doublet. Non-renormalizable terms are controlled by a discrete R-symmetry of the superpotential. We consider radiative corrections to the scalar…

高能物理 - 唯象学 · 物理学 2010-05-25 K. Tamvakis

It is known that the Higgs potential in the Standard Model can drive a successful inflation as long as the Higgs field couples non-minimally to gravity. It is then inevitable to take into account the loop corrections of the Standard Model…

高能物理 - 唯象学 · 物理学 2020-05-04 Po-Wen Chang , Cheng-Wei Chiang , Kin-Wang Ng

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 inflation within a model framework where the Higgs boson arises as a pseudo-Goldstone boson associated with the breaking of a global symmetry at a scale significantly larger than the electroweak one. We show that in such a model…

高能物理 - 唯象学 · 物理学 2017-02-15 Tommi Alanne , Francesco Sannino , Tommi Tenkanen , Kimmo Tuominen

The Standard Model Higgs becomes tachyonic at high energy scales according to current measurements. This unstable regime of the Higgs potential can be realized in the early Universe during high scale inflation, potentially with catastrophic…

高能物理 - 唯象学 · 物理学 2023-01-24 Bibhushan Shakya

If the inflationary phase lasted longer than the minimal period, the length scales observed today originate from modes that were smaller than the Planck length during inflation. It was recently argued that this "trans-Planckian problem" can…

宇宙学与河外天体物理 · 物理学 2020-03-25 Tommi Tenkanen

By ignoring the local density fluctuations, we construct an uniform Higgs-field's (inflaton's) quantum theory with varying effective Planck constant ($\hbar_{v}(t) \propto R(t)^{-3}$) for the evolution of the dark energy density during the…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Wei Yuan , Yu-xin Liu

We discuss models where the Higgs boson of the electroweak standard model plays the role of the inflaton. We focus on the question of the violation of perturbative unitarity due to the coupling of the Higgs boson either to the Ricci scalar…

高能物理 - 唯象学 · 物理学 2011-02-16 Michael Atkins , Xavier Calmet

In the context of the Higgs model involving gauge and Yukawa interactions with the spontaneous gauge symmetry breaking, we consider $\lambda \phi^4$ inflation with non-minimal gravitational coupling, where the Higgs field is identified as…

高能物理 - 唯象学 · 物理学 2015-09-23 Nobuchika Okada , Digesh Raut

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

It is possible that the expansion of the universe began with an inflationary phase, in which the inflaton driving the process also was a Higgs field capable of stabilizing magnetic monopoles in a grand-unified gauge theory. If so, then the…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Alfred Scharff Goldhaber

We propose a possibility that the inflaton potential is significantly modified after inflation due to heavy field dynamics. During inflation there may be a heavy scalar field stabilized at a value deviated from the low-energy minimum. As…

高能物理 - 唯象学 · 物理学 2016-02-24 Naoya Kitajima , Fuminobu Takahashi
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