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Related papers: A Warped Model of Dark Matter

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We discuss a model of dark matter consisting of high energy anti-electron-neutrinos with leptonic force, which is produced by the conserved leptonic charge $g_\ell$ associated with Lee-Yang's $U_1$ gauge symmetry. Based on…

High Energy Physics - Phenomenology · Physics 2021-09-21 Jong-Ping Hsu , Leonardo Hsu

We show that models with exotic leptons transforming as E ~ (1,3,-1) under the standard model gauge symmetry are well suited for generating neutrino mass via a radiative inverse seesaw. This approach realizes natural neutrino masses and…

High Energy Physics - Phenomenology · Physics 2015-06-04 Sandy S. C. Law , Kristian L. McDonald

It is possible that the strongest interactions between dark matter and the Standard Model occur via the neutrino sector. Unlike gamma rays and charged particles, neutrinos provide a unique avenue to probe for astrophysical sources of dark…

High Energy Physics - Phenomenology · Physics 2023-11-07 Carlos A. Argüelles , Diyaselis Delgado , Avi Friedlander , Ali Kheirandish , Ibrahim Safa , Aaron C. Vincent , Henry White

The annihilation of TeV-scale leptophilic dark matter into electron-positron pairs (hereafter $e^+e^-$) will produce a sharp cutoff in the local cosmic-ray $e^+e^-$ spectrum at an energy matching the dark matter mass. At these high…

High Energy Physics - Phenomenology · Physics 2023-11-07 Isabelle John , Tim Linden

We present a model in which the dark matter particle is frozen-in at MeV scale. In this model, the mediator between the standard model sector and the dark sector can automatically provide a self-interaction for dark matter. The interaction…

High Energy Physics - Phenomenology · Physics 2018-12-17 Haipeng An , Ran Huo , Wanqiang Liu

In this paper we develop a Markov Chain Monte Carlo code to study the dark matter properties in interpreting the recent observations of cosmic ray electron/positron excesses. We assume that the dark matter particles couple dominantly to…

Cosmology and Nongalactic Astrophysics · Physics 2010-01-20 Jie Liu , Qiang Yuan , Xiaojun Bi , Hong Li , Xinmin Zhang

In the cosmological paradigm, cold dark matter dominates the mass content of the Universe and is present at every scale. Candidates for dark mater include many extensions of the standard model, with a Weakly Interacting Massive Particle…

High Energy Astrophysical Phenomena · Physics 2019-08-13 Matthieu Vivier

We propose an extension of the standard model with a B-L global symmetry that is broken softly at the TeV scale. The neutrinos acquire masses through a type-II seesaw while the lepton (L) asymmetry arises in the {\it singlet sector} but…

High Energy Physics - Phenomenology · Physics 2010-05-27 John McDonald , Narendra Sahu , Utpal Sarkar

We construct a simple U(1) hidden sector model of metastable dark matter that could explain excess 511 keV gamma rays from the galactic center as observed by INTEGRAL, through inelastic scattering of dark matter followed by its decay.…

High Energy Physics - Phenomenology · Physics 2015-06-04 James M. Cline , Andrew R. Frey

We present a new paradigm for dark matter in which a dark matter asymmetry is established in the early universe that is then transferred to ordinary matter. We show this scenario can fit naturally into weak scale physics models, with a dark…

High Energy Physics - Phenomenology · Physics 2011-09-13 Matthew R. Buckley , Lisa Randall

A triplet dark matter candidate from thermal leptogenesis is considered with building a model. The model is based on the standard two Higgs doublet model and seesaw mechanism with Higgs triplets. The parameters (couplings and masses) are…

High Energy Physics - Phenomenology · Physics 2014-04-24 Jae Ho Heo , C. S. Kim

High energy particles are produced by the annihilation of dark matter particles in our galaxy. These are presently searched for using balloon-borne antiproton and positron detectors and large area, deep underground neutrino telescopes. Dark…

High Energy Physics - Phenomenology · Physics 2016-09-01 F. Halzen , J. E Jacobsen

We consider a model of dark matter whose most prominent signature is a monochromatic flux of TeV neutrinos from the galactic center. As an example of a general scenario, we consider a specific model where the dark matter is a fermion in the…

High Energy Physics - Phenomenology · Physics 2009-08-14 Adam Falkowski , Jose Juknevich , Jessie Shelton

Dark energy and dark matter constitute 95% of the observable Universe. Yet the physical nature of these two phenomena remains a mystery. Einstein suggested a long-forgotten solution: gravitationally repulsive negative masses, which drive…

General Physics · Physics 2018-12-05 J. S. Farnes

For explaining the AMS-02 cosmic positron excess, which was recently reported, we consider a scenario of thermally produced and decaying dark matter (DM) into the standard model (SM) leptons with an extremely small decay rate, \Gamma_{DM}…

High Energy Physics - Phenomenology · Physics 2014-05-02 Ki-Young Choi , Bumseok Kyae , Chang Sub Shin

By extending the Standard Model with singlet-doublet fermions and triplet scalars, all odd under a new $Z_2$ symmetry, we introduce a radiative seesaw model that can simultaneously account for dark matter, explain the existence of neutrino…

High Energy Physics - Phenomenology · Physics 2019-09-16 J. Fiaschi , M. Klasen , S. May

Many difficulties are encountered when attempting to pinpoint a common origin for several observed astrophysical anomalies, and when assessing their tension with existing exclusion limits. These include systematic uncertainties affecting…

High Energy Physics - Phenomenology · Physics 2016-08-25 M. A. Deliyergiyev

We consider models of decaying spin-1 dark matter whose dominant coupling to the standard model sector is through a dark-Higgs Yukawa portal connecting a TeV-scale vector-like lepton to the standard model (right-handed) electron. Below the…

High Energy Physics - Phenomenology · Physics 2021-02-24 Cédric Delaunay , Teng Ma , Yotam Soreq

We show how the problem of small neutrino masses and suppressed proton decay can be simultaneously resolved in 6-D universal extra dimension models (UED) with a low fundamental scale using extended gauge groups that contain the local $B-L$…

High Energy Physics - Phenomenology · Physics 2009-11-07 R. N. Mohapatra , A. Perez-Lorenzana

We present a minimal left-right dark matter framework that can simultaneously explain the recently observed 3.55 keV X-ray line from several galaxy clusters and gauge coupling unification at high energy scale. Adopting a minimal dark matter…

High Energy Physics - Phenomenology · Physics 2017-12-27 Debasish Borah , Arnab Dasgupta , Sudhanwa Patra