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相关论文: Dark Matter and Muon $g-2$ Anomaly via Scale Symme…

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Extending the spacetime symmetries of standard model (SM) by scale invariance (SI) may address the Higgs naturalness problem. In this article we attempt to embed accidental dark matter (DM) into SISM, requiring that the symmetry protecting…

高能物理 - 唯象学 · 物理学 2015-12-09 Jun Guo , Zhaofeng Kang

We investigate the phenomenology of an extension of the Standard Model (SM) by a non-abelian gauge group $SU(2)_{HS}$ where all SM particles are singlets under this gauge group, and a new scalar representation $\phi$ that is singlet under…

高能物理 - 唯象学 · 物理学 2021-10-27 Nabil Baouche , Amine Ahriche , Gaber Faisel , Salah Nasri

We consider a simple scalar dark matter model within the frame of gauged $L_{\mu}-L_{\tau}$ symmetry. A gauge boson $Z'$ as well as two scalar fields $S$ and $\Phi$ are introduced to the Standard Model (SM). $S$ and $\Phi$ are SM singlet…

高能物理 - 唯象学 · 物理学 2022-04-19 XinXin Qi , AiGeng Yang , Wei Liu , Hao Sun

We explore the idea of accidental dark matter (aDM) stability in the scale invariant local $U(1)_{B-L}$ model, which is a theory for neutrino and at the same time radiatively breaks scale invariance via quantum mechanical dynamics in the…

高能物理 - 唯象学 · 物理学 2015-08-04 Jun Guo , Zhaofeng Kang , P. Ko , Yuta Orikasa

We investigate single and two-component scalar dark matter scenarios in classically scale invariant standard model which is free of the hierarchy problem in the Higgs sector. We show that despite the very restricted space of parameters…

高能物理 - 唯象学 · 物理学 2016-05-04 Karim Ghorbani , Hossein Ghorbani

We propose a minimal model for the cosmic coincidence problem $\Omega_{\rm DM}/\Omega_B \sim 5$ and neutrino mass in a type-II seesaw scenario. We extend the standard model of particle physics with a $\rm SU(2)$ singlet leptonic Dirac…

高能物理 - 唯象学 · 物理学 2021-11-30 Nimmala Narendra , Narendra Sahu , Sujay Shil

The most recent results of searches at the LHC for the Higgs boson h have turned up possible hints of such a particle with mass m_h about 125 GeV consistent with standard model (SM) expectations. This has many potential implications for the…

高能物理 - 唯象学 · 物理学 2012-06-08 Xiao-Gang He , Bo Ren , Jusak Tandean

The Standard Model (SM) plus a real gauge-singlet scalar field dubbed darkon (SM+D) is the simplest model possessing a weakly interacting massive particle (WIMP) dark-matter candidate. In this model, the parameters are constrained from dark…

高能物理 - 唯象学 · 物理学 2015-03-18 Yi Cai , Xiao-Gang He , Bo Ren

We present a model explaining both the 4.2 $\sigma$ muon $g-2$ anomaly and the relic density of dark matter (DM) in which DM interacts with the Standard Model (SM) via a scalar portal boson $\varphi$ carrying both dark and SM leptonic…

高能物理 - 唯象学 · 物理学 2022-07-08 S. N. Gninenko , N. V. Krasnikov

We consider a scalar dark matter model, the SM4+D, consisting of the standard model with four generations (SM4) and a real gauge-singlet scalar called darkon, D, as the weakly interacting massive particle (WIMP) dark-matter (DM) candidate.…

高能物理 - 唯象学 · 物理学 2014-11-20 Xiao-Gang He , Shu-Yu Ho , Jusak Tandean , Ho-Chin Tsai

We consider a classically scale invariant version of the Standard Model, extended by an extra dark $SU(2)_X$ gauge group. Apart from the dark gauge bosons and a dark scalar doublet which is coupled to the Standard Model Higgs through a…

高能物理 - 唯象学 · 物理学 2016-02-03 Alexandros Karam , Kyriakos Tamvakis

We investigate and compare two simple models of dark matter (DM): a vector and a scalar DM model. Both models require the presence of two physical Higgs bosons $h_1$ and $h_2$ which come from mixed components of the standard Higgs doublet…

高能物理 - 唯象学 · 物理学 2019-01-16 Duarte Azevedo , Mateusz Duch , Bohdan Grzadkowski , Da Huang , Michal Iglicki , Rui Santos

We study the phenomenology of a vector dark matter (VDM) in a $U(1)_X$ gauged extension of the Standard Model (SM) which is connected to the type II seesaw framework via the Higgs portal. When this $U(1)_X$ symmetry is spontaneously broken…

高能物理 - 唯象学 · 物理学 2024-08-06 Nandini Das , Tapoja Jha , Dibyendu Nanda

We propose a two-component asymmetric FIMP (feebly interacting massive particle) dark matter (DM) model in which both DM candidates are real scalar fields. The model is an extension of the Standard Model (SM) by two scalar DM components and…

高能物理 - 唯象学 · 物理学 2026-05-26 S. Peyman Zakeri

We discuss a number of experimental constraints on Weinberg's Higgs portal model. In this framework, the standard model (SM) particle spectrum is extended to include one complex scalar field S and one Dirac fermion \psi. These new fields…

We consider isosinglet scalar extension of a model with a Higgs democracy - multihiggs extension of the SM where each quark and lepton has its own Higgs isodoublet. The addition of light isosinglet scalar allows to solve both muon…

高能物理 - 唯象学 · 物理学 2017-10-18 N. V. Krasnikov

We present a new model of "Stealth Dark Matter": a composite baryonic scalar of an $SU(N_D)$ strongly-coupled theory with even $N_D \geq 4$. All mass scales are technically natural, and dark matter stability is automatic without imposing an…

We discuss the dynamics and phenomenology of an oscillating scalar field coupled to the Higgs boson that accounts for the dark matter in the Universe. The model assumes an underlying scale invariance such that the scalar field only acquires…

高能物理 - 唯象学 · 物理学 2018-05-25 Catarina Cosme , João G. Rosa , O. Bertolami

In the context of a two-Higgs doublet model, supplemented by an additional light pseudoscalar Higgs boson and a stable isosinglet fermion, we consider the possibility of addressing simultaneously the discrepancy from the standard…

高能物理 - 唯象学 · 物理学 2022-09-14 Giorgio Arcadi , Abdelhak Djouadi , Farinaldo Queiroz

We propose and study a purely inelastic scalar dark matter model, where two real scalars-dark matter $\phi_1$ and its excited partner $\phi_2$ interact with the Standard Model via a Higgs portal. After mass diagonalization, only inelastic…

高能物理 - 唯象学 · 物理学 2025-08-20 Jinhui Guo , Jia Liu , Chenhao Peng , Xiao-Ping Wang
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