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Related papers: Inert Dark Matter in Type-II Seesaw

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We extend the colored Zee-Babu model with a gauged $U(1)_{B-L}$ symmetry and a scalar singlet dark matter (DM) candidate $S$. The spontaneous breaking of $U(1)_{B-L}$ leaves a residual $Z_2$ symmetry that stabilizes the DM and generates…

High Energy Physics - Phenomenology · Physics 2018-11-14 Ran Ding , Zhi-Long Han , Li Huang , Yi Liao

We investigate the constraints on the Inert Doublet Model (IDM), a minimal extension of the Standard Model of Particle Physics featuring a scalar dark matter candidate, using data from recent and future gamma-ray observatories. The…

High Energy Physics - Phenomenology · Physics 2026-03-19 Lucca Radicce Justino , Clarissa Siqueira , Aion Viana

We study a $Z_2 \times Z'_2$ symmetric 3-Higgs Doublet Model (3HDM), wherein two of the doublets are inert and one is active (thus denoted in literature as I(2+1)HDM), yielding a two-component Dark Matter (DM) sector. The two DM candidates…

High Energy Physics - Phenomenology · Physics 2020-12-23 J. Hernandez-Sanchez , V. Keus , S. Moretti , D. Rojas-Ciofalo , D. Sokolowska

An ever-increasing body of evidence suggests that weakly interacting massive particles (WIMPs) constitute the bulk of the matter in the Universe. Experimental data, dimensional analysis and Standard Model particle physics are sufficient to…

High Energy Physics - Phenomenology · Physics 2007-05-23 F. Halzen

The document discusses a proposed extension to the Standard Model that aims to explain the presence of neutrino masses and the existence of dark matter. The model includes two potential candidates for dark matter, a vector WIMP and a…

High Energy Physics - Phenomenology · Physics 2023-09-22 Francesco Costa

While astrophysical observations imply that 85% of the matter content is unaccounted for, the nature of this dark matter (DM) component remains unknown. Weakly Interacting Massive Particles (WIMPs) - DM particles that interact at or below…

High Energy Astrophysical Phenomena · Physics 2025-07-22 Eliot Genton , Jeffrey Lazar , Carlos Argüelles , Gwenhaël de Wasseige

One of the most puzzling problems of modern physics is the identification of the nature a non-relativistic matter component present in the universe, contributing to more than 25$\%$ of the total energy budget, known as Dark Matter. Weakly…

High Energy Physics - Phenomenology · Physics 2019-01-18 Mathias Pierre

We propose a realisation of inverse seesaw model controlled by hidden $U(1)$ gauge symmetry, and discuss the impact of a bosonic dark matter (DM) candidate by imposing a $Z_2$ parity. We present the detail of scalar spectra and apply the…

High Energy Physics - Phenomenology · Physics 2019-10-25 Haiying Cai , Takaaki Nomura , Hiroshi Okada

We study a new physics scenario with two inert and one active scalar doublets, hence a 3-Higgs Doublet Model (3HDM). We impose a $Z_2 \times Z'_2$ symmetry onto such a 3HDM with one inert doublet odd under the $Z_2$ transformation and the…

High Energy Physics - Phenomenology · Physics 2023-03-29 Jaime Hernandez-Sanchez , Venus Keus , Stefano Moretti , Dorota Sokolowska

We examine the leptophilic two Higgs doublet model with fermionic dark matter, considering the range of experimental constraints on the Higgs sector. The measurements of the 125 GeV Higgs from the LHC Run-I allow us to focus on those…

High Energy Physics - Phenomenology · Physics 2015-10-28 Matthew R. Buckley , David Feld

Weakly Interacting Massive Particles (WIMPs) and axions are arguably the most compelling dark matter candidates in the literature. Could they coexist as dark matter particles? More importantly, can they be incorporated in a well motivated…

High Energy Physics - Phenomenology · Physics 2016-11-23 Alexandre Alves , Daniel A. Camargo , Alex G. Dias , Robinson Longas , Celso C. Nishi , Farinaldo S. Queiroz

We extend the two-Higgs doublet models of Type I and Type II by adding a real gauge-singlet scalar S dark matter candidate (2HDMS models). We impose theoretical constraints deriving from perturbativity, stability, unitarity and correct…

High Energy Physics - Phenomenology · Physics 2015-06-22 Aleksandra Drozd , Bohdan Grzadkowski , John F. Gunion , Yun Jiang

A number of papers attempt to explain the positron anomaly in cosmic rays, observed by PAMELA and AMS-02, in terms of dark matter (DM) decays or annihilations. However, the recent progress in cosmic gamma-ray studies challenges these…

High Energy Astrophysical Phenomena · Physics 2017-01-12 Konstantin Belotsky , Ruslan Budaev , Alexander Kirillov , Maxim Laletin

We propose a flavored $U(1)_{e\mu}$ neutrino mass and dark matter~(DM) model to explain the recent DArk Matter Particle Explorer (DAMPE) data, which feature an excess on the cosmic ray electron plus positron flux around 1.4 TeV. Only the…

High Energy Physics - Phenomenology · Physics 2018-04-09 Yi-Zhong Fan , Wei-Chih Huang , Martin Spinrath , Yue-Lin Sming Tsai , Qiang Yuan

We consider a recently proposed supersymmetric radiative seesaw model which is coupled with the minimal supergravity. The conventional R parity and $Z_2$ invariance are imposed, which ensures the existence of a multi-component dark matter…

High Energy Physics - Phenomenology · Physics 2011-12-21 Mayumi Aoki , Jisuke Kubo , Taishi Okawa , Hiroshi Takano

We use multi-component decaying dark matter (DM) scenario to explain the possible cosmic ray excesses in the positron fraction recently confirmed by AMS-02 and the total $e^+ +e^-$ flux observed by Fermi-LAT. In the two-component DM models,…

High Energy Physics - Phenomenology · Physics 2014-12-01 Chao-Qiang Geng , Da Huang , Lu-Hsing Tsai

A solution to the PAMELA positron excess with Higgsino dark matter within extended supergravity grand unified (SUGRA) models is proposed. The models are compliant with the photon constraints recently set by Fermi-LAT and produce positron as…

High Energy Physics - Phenomenology · Physics 2011-02-03 Ning Chen , Daniel Feldman , Zuowei Liu , Pran Nath , Gregory Peim

We analyze 11 years of Fermi-LAT data corresponding to the sky regions of 7 dwarf irregular (dIrr) galaxies. DIrrs are dark matter (DM) dominated systems, proposed as interesting targets for the indirect search of DM with gamma rays. The…

Cosmology and Nongalactic Astrophysics · Physics 2022-11-28 V. Gammaldi , J. Pérez-Romero , J. Coronado-Blázquez , M. Di Mauro , E. V. Karukes , M. A. Sánchez-Conde , P. Salucci

The tightening of the constraints on the standard thermal WIMP scenario has forced physicists to propose alternative dark matter (DM) models. One of the most popular alternate explanations of the origin of DM is the non-thermal production…

High Energy Physics - Phenomenology · Physics 2017-02-27 Anirban Biswas , Sandhya Choubey , Sarif Khan

Although the seesaw mechanism is a natural explanation for the small neutrino masses, there are cases when the Majorana mass terms for the right-handed neutrinos are not allowed due to symmetry. In that case, if neutrino-specific Higgs…

High Energy Physics - Phenomenology · Physics 2017-04-05 Seungwon Baek , Takaaki Nomura
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