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Related papers: Nonabelian dark matter: models and constraints

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The possibility of explaining the positron and electron excess recently found by the PAMELA and ATIC collaborations in terms of dark matter (DM) annihilation has attracted considerable attention. Models surviving bounds from, e.g,…

Astrophysics · Physics 2010-04-15 Lars Bergstrom , Gianfranco Bertone , Torsten Bringmann , Joakim Edsjo , Marco Taoso

A recent model of dark energy and dark matter was proposed, involving a new gauge group $SU(2)_Z$ whose coupling grows strong at a scale $\Lambda_Z \sim 10^{-3} eV$, a result which is obtained from a simple assumption that its initial value…

High Energy Physics - Phenomenology · Physics 2008-03-27 P. Q. Hung

The correlation between Higgs-like scalars and light dark matter is an interesting topic, especially now that a $125 GeV$ Higgs was discovered and dark matter (DM) searches got negative results. The $95 GeV$ excess reported by the CMS…

High Energy Physics - Phenomenology · Physics 2024-01-01 Weichao Li , Haoxue Qiao , Kun Wang , Jingya Zhu

We propose a scalar-mediated Self-Interacting Dark Matter (SIDM) model to address small-scale structure anomalies such as the core-cusp and diversity problems. The model is composed by a leptophilic scalar mediator and a pseudo-Dirac dark…

High Energy Physics - Phenomenology · Physics 2026-05-05 Zihan Wang

A few multiplets that can be added to the SM contain a lightest neutral component which is automatically stable and provides allowed DM candidates with a non-standard phenomenology. Thanks to coannihilations, a successful thermal abundance…

High Energy Physics - Phenomenology · Physics 2009-10-09 Marco Cirelli , Nicolao Fornengo , Alessandro Strumia

We propose a radiative seesaw model with a light dark matter candidate (DM) under modular $A_4$ and gauged $U(1)_{B-L}$ symmetries, in which neutrino masses are generated via one-loop level, and we have a bosonic DM candidate $\sim 0.01-50$…

High Energy Physics - Phenomenology · Physics 2021-08-24 Keiko I. Nagao , Hiroshi Okada

The nature of dark matter (DM) particles and the mechanism that provides their measured relic abundance are currently unknown. In this paper we investigate inert scalar and vector like fermion doublet DM candidates with a charge asymmetry…

High Energy Physics - Phenomenology · Physics 2015-05-30 Chiara Arina , Narendra Sahu

We observe that in SUSY models with non-universal GUT scale gaugino mass parameters, raising the GUT scale SU(2) gaugino mass |M_2| from its unified value results in a smaller value of -m_{H_u}^2 at the weak scale. By the electroweak…

High Energy Physics - Phenomenology · Physics 2008-11-26 Howard Baer , Azar Mustafayev , Heaya Summy , Xerxes Tata

The proposal of a galactic population of intermediate mass black holes (IMBHs), forming dark matter (DM) ``mini-spikes'' around them, has received considerable attention in recent years. In fact, leading in some scenarios to large…

Cosmology and Nongalactic Astrophysics · Physics 2010-04-15 Torsten Bringmann , Julien Lavalle , Pierre Salati

The $W$-boson mass, which was recently measured at FermiLab with an unprecedented precision, suggests the presence of new multiplets beyond the Standard Model (SM). One of the minimal extensions of the SM is to introduce an additional…

High Energy Physics - Phenomenology · Physics 2022-09-07 Yi-Zhong Fan , Tian-Peng Tang , Yue-Lin Sming Tsai , Lei Wu

A model of dark matter (DM) that communicates with the Standard Model (SM) exclusively through suppressed dimension five operator is discussed. The SM is augmented with a symmetry $U(1)_X \otimes Z_2$, where $U(1)_X$ is gauged and broken…

High Energy Physics - Phenomenology · Physics 2021-02-03 Basabendu Barman , Subhaditya Bhattacharya , Bohdan Grzadkowski

We propose a gauged $U(1)_{B-L}$ extension of the standard model (SM) to explain simultaneously the light neutrino masses and dark matter (DM). The generation of neutrino masses occurs through a variant of type-II seesaw mechanism in which…

High Energy Physics - Phenomenology · Physics 2020-02-18 Satyabrata Mahapatra , Nimmala Narendra , Narendra Sahu

The particle origin of dark matter (DM) remains elusive despite decades of direct, indirect, and collider searches. Several groups have reported a $\gamma$-ray excess toward the Galactic Centre, commonly referred to as the Galactic Centre…

High Energy Physics - Phenomenology · Physics 2025-12-01 Jordan Koechler , Mattia Di Mauro

Some extensions of the Standard Model provide Dark Matter candidate particles which can have a dominant coupling with the lepton sector of the ordinary matter. Thus, such Dark Matter candidate particles ($\chi^{0}$) can be directly detected…

The cosmic-ray excess observed by PAMELA in the positron fraction and by FERMI and HESS in the electron + positron flux can be interpreted in terms of DM annihilations or decays into leptonic final states. Final states into tau's or 4mu…

High Energy Physics - Phenomenology · Physics 2010-02-24 Patrick Meade , Michele Papucci , Alessandro Strumia , Tomer Volansky

We study the CDF $W$-mass, muon $g-2$, and dark matter observables in a local $U(1)_{L_\mu-L_\tau}$ model in which the new particles include three vector-like leptons ($E_1,~ E_2,~ N$), a new gauge boson $Z'$, a scalar $S$ (breaking…

High Energy Physics - Phenomenology · Physics 2023-01-04 Quan Zhou , Xiao-Fang Han

We consider a minimal renormalizable and gauge invariant dark matter (DM) model, in which the singlet fermion DM has only axial couplings to a new pseudoscalar mediator. The mixing between the pseudoscalar mediator and the standard model…

High Energy Physics - Phenomenology · Physics 2017-04-12 Seungwon Baek , P. Ko , Jinmian Li

Annihilating dark matter (DM) models based on a scalar hidden sector with Higgs portal-like couplings to the Standard Model are considered as a possible explanation for recently observed cosmic ray excesses. Two versions of the model are…

High Energy Physics - Phenomenology · Physics 2015-05-13 Kazunori Kohri , John McDonald , Narendra Sahu

Recently, it has been shown that electrons and positrons from dark matter (DM) annihilations provide an excellent fit to the Fermi, PAMELA, and HESS data. Using this DM model, which requires an enhancement of the annihilation cross section…

High Energy Astrophysical Phenomena · Physics 2009-11-20 Anders Pinzke , Christoph Pfrommer , Lars Bergstrom

This work investigates the allowed parameter spaces of a simplified dark matter (DM) model characterized by a spin-0 mediator with masses in the low to intermediate range ($ < $ 10 GeV). We systematically divide the parameter space into…

High Energy Physics - Phenomenology · Physics 2025-03-21 Lipika Kolay , Soumitra Nandi