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The Higgs effective potential becomes unstable at approximately $10^{11}$ GeV, and if only standard model interactions are considered, the lifetime $\tau$ of the electroweak vacuum turns out to be much larger than the age of the Universe…

高能物理 - 唯象学 · 物理学 2019-06-26 Vincenzo Branchina , Eloisa Bentivegna , Filippo Contino , Dario Zappalà

The quadratic divergences of the Higgs mass may be cancelled either accidentally or by the exchange of some new particles. Alternatively its impact on naturalness may be weakened by raising the Higgs mass, which requires changing the…

高能物理 - 唯象学 · 物理学 2008-11-26 Riccardo Barbieri , Lawrence J. Hall , Vyacheslav S. Rychkov

It has been suggested that electroweak symmetry breaking in the Standard Model may be natural if the Standard Model merges into a conformal field theory (CFT) at short distances. In such a scenario the Higgs mass would be protected from…

高能物理 - 唯象学 · 物理学 2014-01-22 Gustavo Marques Tavares , Martin Schmaltz , Witold Skiba

We explore a simple and predictive dark matter scenario involving a complex scalar field, $\phi$, coupled to the Higgs portal with no additional field content. In the UV, the field possesses a global $U(1)$ symmetry which is broken by mass…

高能物理 - 唯象学 · 物理学 2025-08-01 Dan Hooper , Gordan Krnjaic , Duncan Rocha , Subhojit Roy

We study a model where quintessence potential $e^{-\xi\phi}$ coupled to Higgs potential. We calculate the evolution of the quintessence, and track the running of the effective Higgs self-coupling. We find it slightly larger than that of the…

高能物理 - 唯象学 · 物理学 2019-02-27 Chengcheng Han , Shi Pi , Misao Sasaki

We consider scenarios where the inflaton field decays dominantly to a hidden dark matter (DM) sector. By studying the typical behavior of the Standard Model (SM) Higgs field during inflation, we derive a relation between the primordial…

宇宙学与河外天体物理 · 物理学 2019-10-16 Tommi Tenkanen

The standard model Higgs boson can serve as the inflaton field of slow roll inflationary models provided it exhibits a large non-minimal coupling with the gravitational scalar curvature. The Higgs boson self interactions and its couplings…

高能物理 - 唯象学 · 物理学 2009-11-05 T. E. Clark , Boyang Liu , S. T. Love , T. ter Veldhuis

We consider classically scale-invariant extensions of the Standard Model (CSI ESM) which stabilise the Higgs potential and have good dark matter candidates. In this framework all mass scales, including electroweak and dark matter masses,…

高能物理 - 唯象学 · 物理学 2016-02-19 Valentin V. Khoze , Christopher McCabe , Gunnar Ro

In models with an extended Higgs sector, such as the (N)MSSM, scalar states mix with one another. Yet, the concept of Higgs mixing is problematic at the radiative level, since it introduces both a scheme and a gauge dependence. In…

高能物理 - 唯象学 · 物理学 2020-12-30 Florian Domingo , Sebastian Paßehr

In a previous work, a classically scale invariant extension of the standard model was proposed, as a potential candidate for resolving the hierarchy problem, by minimally introducing a complex gauge singlet scalar, and generating radiative…

高能物理 - 唯象学 · 物理学 2014-07-31 Arsham Farzinnia , Jing Ren

Since the current evidence of its existence is revealed only through its gravitational influence, the way dark matter couples to gravity must be then of primary importance. Here, unlike the standard model sector which is typically coupled…

高能物理 - 唯象学 · 物理学 2020-10-21 Hemza Azri , Adil Jueid , Canan Karahan , Salah Nasri

Motivated by the null results of current dark matter searches and the small-scale problems, we study a dark sector charged by a spontaneous broken gauge $U(1)'$. To explore the parameter space of this model, in addition to the consideration…

高能物理 - 唯象学 · 物理学 2024-07-30 Song Li , Jin Min Yang , Mengchao Zhang , Rui Zhu

A version of the Standard Model is considered, where the electroweak symmetry breaking is provided by cosmological initial data given for the zeroth Fourier harmonic of the Higgs field $<\phi>$. The initial data symmetry breaking mechanism…

高能物理 - 唯象学 · 物理学 2008-01-14 A. B. Arbuzov , L. A. Glinka , V. N. Pervushin

We find the approximate solutions for the Higgs masses and couplings in the NMSSM with exact and softly broken PQ--symmetry. The obtained solutions indicate that there exists a mass hierarchy in the Higgs spectrum which is caused by the…

高能物理 - 唯象学 · 物理学 2007-05-23 R. Nevzorov , D. J. Miller

Black holes, dark energy, and the Higgs field are all currently established, exciting, and mysterious, each in its own way. Cosmological data show that dark energy may evolve with time. The electroweak phase transition during stellar…

宇宙学与河外天体物理 · 物理学 2025-02-11 Steve P. Ahlen , James W. Rohlf , Gregory Tarlé

In the high-scale (split) MSSM, the measured Higgs mass sets an upper bound on the supersymmetric scalar mass scale MSUSY around $10^{11}$ ($10^{8}$) GeV, for $\tan\beta$ in the standard range and the central value of the top quark mass…

高能物理 - 唯象学 · 物理学 2018-09-24 Jae-hyeon Park

A hierarchically small weak scale does not generally coincide with enhanced symmetry, but it may still be exceptional with respect to vacuum energy. By analyzing the classical vacuum energy as a function of parameters such as the Higgs…

高能物理 - 唯象学 · 物理学 2019-04-09 Clifford Cheung , Prashant Saraswat

We investigate inflationary Higgs dynamics and constraints on the Standard Model parameters assuming the Higgs potential, computed to next-to-next leading order precision, is not significantly affected by new physics. For a high…

高能物理 - 唯象学 · 物理学 2015-06-19 Kari Enqvist , Tuukka Meriniemi , Sami Nurmi

We consider the classically scale invariant Higgs-dilaton model of dynamical symmetry breaking extended with an extra scalar field that plays the role of dark matter. The Higgs boson is light near a critical boundary between different…

高能物理 - 唯象学 · 物理学 2022-06-01 Kristjan Kannike , Niko Koivunen , Aleksei Kubarski , Luca Marzola , Martti Raidal , Alessandro Strumia , Venno Vipp

We investigate the electroweak vacuum stability in an extended version of the Standard Model which incorporates two additional singlet scalar fields and three right handed neutrinos. One of these extra scalars plays the role of dark matter…

高能物理 - 唯象学 · 物理学 2018-05-02 Purusottam Ghosh , Abhijit Kumar Saha , Arunansu Sil