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A neutral Dirac fermion is supplied as a singlet within the context of the standard model (SM) and is considered as a dark matter (DM) candidate near electroweak scale (10-1000 GeV) with nonzero magnetic dipole moment. The Dirac particles…

高能物理 - 唯象学 · 物理学 2010-09-17 Jae Ho Heo

The scotogenic model is a well motivated scenario that provides both an explanation for neutrino masses and for dark matter. We focus on a real scalar dark matter candidate in this model, produced through standard thermal freeze-out. We…

高能物理 - 唯象学 · 物理学 2022-05-18 Ivania M. Ávila , Giovanna Cottin , Marco A. Díaz

We investigate a model of dark sector based on non-Abelian $SU(2)_D$ gauge symmetry. This dark gauge symmetry is broken into discrete $Z_2$ via vacuum expectation values of two real triplet scalars, and an $SU(2)_D$ doublet Dirac fermion…

高能物理 - 唯象学 · 物理学 2021-05-26 P. Ko , Takaaki Nomura , Hiroshi Okada

The non-observation of dark matter (DM) by direct detection experiments suggests that any new interaction of DM with the Standard Model (SM) should be very weak. One of the simplest scenarios to achieve this is a dark sector that is charged…

高能物理 - 唯象学 · 物理学 2019-07-26 Patrick Foldenauer

A simple and well-motivated explanation for the origin of dark matter is that it consists of thermal relic particles that get their mass entirely through electroweak symmetry breaking. The simplest models implementing this possibility…

高能物理 - 唯象学 · 物理学 2007-05-23 Philip C. Schuster , Natalia Toro

We test the dark photon as a portal connecting to the dark sector in the case of Dirac fermion and complex scalar dark matter with masses up to 1 TeV. Both the dark photon and the $Z$ boson contribute to the dark matter annihilation and…

高能物理 - 唯象学 · 物理学 2026-04-10 X. G. Wang , B. M. Loizos , A. W. Thomas

The notion of U(1) lepton number (which may only be softly broken) is applied to models of dark matter which interacts with leptons. Previous scotogenic models of Majorana or Dirac neutrino mass are shown to be derivable in this framework…

高能物理 - 唯象学 · 物理学 2020-09-02 Ernest Ma

Kinetic heating of old cold neutron stars, via the scattering of dark matter with matter in the star, provides a promising way to probe the nature of dark matter interactions. We consider a dark matter candidate that is a Standard Model…

高能物理 - 唯象学 · 物理学 2025-10-24 Nicole F. Bell , Giorgio Busoni , Avirup Ghosh

We discuss the extent to which models of Weakly Interacting Massive Particle (WIMP) Dark Matter (DM) at and above the electroweak scale can be probed conclusively in future high energy and astroparticle physics experiments. We consider…

高能物理 - 唯象学 · 物理学 2019-02-14 Michael J. Baker , Andrea Thamm

The problem of the dark matter in the universe is reviewed. A short history of the subject is given, and several of the most obvious particle candidates for dark matter are identified. Particular focus is given to weakly interacting,…

高能天体物理现象 · 物理学 2012-06-15 Lars Bergström

We explore a gauged $U(1)_{B-L}$ extension of standard model with inclusion of three right-handed neutrinos of exotic $B-L$ charges to cancel the gauge anomaly. Non-trivial transformation of new particles under $B-L$ symmetry forbids the…

高能物理 - 唯象学 · 物理学 2022-07-13 Subhasmita Mishra , Nimmala Narendra , Prafulla Kumar Panda , Nirakar Sahoo

GeV-scale thermal dark matter (DM) is highly constrained by the null results of both direct and indirect detection experiments, especially in the context of simplified models. In this work, we study the interplay of collider, direct and…

高能物理 - 唯象学 · 物理学 2026-04-22 D. Alonso-González , D. Cerdeño , P. Foldenauer , J. M. No

We present a model for dark matter with extra spatial dimensions in which Standard-Model (SM) fermions have localized wave functions. The underlying gauge group is $G_{\rm SM} \otimes {\rm U}(1)_z$, and the dark matter particle is a…

高能物理 - 唯象学 · 物理学 2021-12-21 S. Girmohanta , R. Shrock

We investigate an extension of the standard model (SM) with a singlet fermionic dark matter (DM) particle which interacts with the SM sector through a real singlet scalar. The presence of a new scalar provides the possibility of generating…

高能物理 - 唯象学 · 物理学 2015-06-18 Tai Li , Yu-Feng Zhou

We formulate a predictive model of fermion masses and mixings based on a $\Delta(27)$ family symmetry. In the quark sector the model leads to the viable mixing inspired texture where the Cabibbo angle comes from the down quark sector and…

高能物理 - 唯象学 · 物理学 2018-06-13 Nicolás Bernal , A. E. Cárcamo Hernández , Ivo de Medeiros Varzielas , Sergey Kovalenko

We propose a model in which the origin of neutrino mass is dependent on the existence of dark matter. Neutrinos acquire mass at the three-loop level and the dark matter is the neutral component of a fermion triplet. We show that…

高能物理 - 唯象学 · 物理学 2015-06-19 Amine Ahriche , Chian-Shu Chen , Kristian L. McDonald , Salah Nasri

The scotogenic model defines a framework for radiative neutrino masses and provides a viable dark matter candidate. Since the scotogenic dark matter is leptophilic, indirect searches appear as an especially interesting possibility. Here we…

高能物理 - 唯象学 · 物理学 2026-05-14 Ricardo Cepedello , Pablo de la Torre , Manuel Masip

We take into account a generic form of a Dirac fermionic dark matter (DM), which communicates with the Standard Model quarks via a scalar mediator, in a model-independent way. Four special interaction scenarios are investigated, where one…

高能物理 - 唯象学 · 物理学 2013-06-19 Ho-Chin Tsai , Kwei-Chou Yang

We propose a minimal model where a dark sector, odd under a $\mathcal{Z}_2$ discrete symmetry, is the seed of lepton number violation in the neutrino sector at the loop level, in the context of the linear seesaw mechanism. Neutrino mass…

高能物理 - 唯象学 · 物理学 2023-07-19 A. Batra , H. B. Câmara , F. R. Joaquim

We discuss singlet fermion dark matter within a left-right symmetric model promoting baryon and lepton numbers as separate gauge symmetries. We add a simple Dirac fermionic dark matter singlet under $SU(2)_{L,R}$ with nonzero and equal…

高能物理 - 唯象学 · 物理学 2016-06-29 Sudhanwa Patra , Soumya Rao
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