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Related papers: Confronting $\gamma$-rays from singlet fermionic c…

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Due to their proximity, high dark-matter content, and apparent absence of non-thermal processes, Milky Way dwarf spheroidal satellite galaxies (dSphs) are excellent targets for the indirect detection of dark matter. Recently, eight new dSph…

High Energy Astrophysical Phenomena · Physics 2015-08-18 LAT Collaboration , The DES Collaboration , A. Drlica-Wagner , A. Albert , K. Bechtol , M. Wood , L. Strigari , M. Sanchez-Conde , L. Baldini , R. Essig , J. Cohen-Tanugi , B. Anderson , R. Bellazzini , E. D. Bloom , R. Caputo , C. Cecchi , E. Charles , J. Chiang , A. de Angelis , S. Funk , P. Fusco , F. Gargano , N. Giglietto , F. Giordano , S. Guiriec , M. Gustafsson , M. Kuss , F. Loparco , P. Lubrano , N. Mirabal , T. Mizuno , A. Morselli , T. Ohsugi , E. Orlando , M. Persic , S. Raino , N. Sehgal , F. Spada , D. J. Suson , G. Zaharijas , S. Zimmer , T. Abbott , S. Allam , E. Balbinot , A. H. Bauer , A. Benoit-Levy , R. A. Bernstein , G. M. Bernstein , E. Bertin , D. Brooks , E. Buckley-Geer , D. L. Burke , A. Carnero Rosell , F. J. Castander , R. Covarrubias , C. B. D'Andrea , L. N. da Costa , D. L. DePoy , S. Desai , H. T. Diehl , C. E Cunha , T. F. Eifler , J. Estrada , A. E. Evrard , A. Fausti Neto , E. Fernandez , D. A. Finley , B. Flaugher , J. Frieman , E. Gaztanaga , D. Gerdes , D. Gruen , R. A. Gruendl , G. Gutierrez , K. Honscheid , B. Jain , D. James , T. Jeltema , S. Kent , R. Kron , K. Kuehn , N. Kuropatkin , O. Lahav , T. S. Li , E. Luque , M. A. G. Maia , M. Makler , M. March , J. Marshall , P. Martini , K. W. Merritt , C. Miller , R. Miquel , J. Mohr , E. Neilsen , B. Nord , R. Ogando , J. Peoples , D. Petravick , A. Pieres , A. A. Plazas , A. Queiroz , A. K. Romer , A. Roodman , E. S. Rykoff , M. Sako , E. Sanchez , B. Santiago , V. Scarpine , M. Schubnell , I. Sevilla , R. C. Smith , M. Soares-Santos , F. Sobreira , E. Suchyta , M. E. C. Swanson , G. Tarle , J. Thaler , D. Thomas , D. Tucker , A. Walker , R. H. Wechsler , W. Wester , P. Williams , B. Yanny , J. Zuntz

A recent study of gamma-ray data from the Galactic Center motivates the investigation of light (~7-10 GeV) particle dark matter models featuring tau lepton pairs as dominant annihilation final state. The Lepton-Specific two-Higgs-doublet…

High Energy Physics - Phenomenology · Physics 2015-05-28 M. S. Boucenna , S. Profumo

The presence of dark matter is nowadays widely supported by a large body of astronomical and cosmological observations. A large amount of dark matter is expected to be present in the central region of the Milky Way. Very-high-energy (>100…

High Energy Astrophysical Phenomena · Physics 2019-08-14 Lucia Rinchiuso , Emmanuel Moulin , Aion Viana , Christopher Van Eldik , Johannes Veh

We present an analysis of the Dark S3 model in the heavy DM mass region, this model features an S3 symmetric extension of the scalar sector of the SM including a scalar $SU(2)$ doublet dark matter candidate. We use publicly available tools…

High Energy Physics - Phenomenology · Physics 2020-08-28 C. Espinoza , M. Mondragón

We discuss a supersymmetric model for cogenesis of dark and baryonic matter where the dark matter (DM) has mass in the 8-10 GeV range as indicated by several direct detection searches including most recently the CDMS experiment with the…

High Energy Physics - Phenomenology · Physics 2015-06-15 Rouzbeh Allahverdi , Bhaskar Dutta , Rabindra N. Mohapatra , Kuver Sinha

We have analysed the early LHC signatures of the minimal supergravity (mSUGRA) model. Our emphasis is on the 7 - $TeV$ run corresponding to an integrated luminosity of $\sim 1.0 ~fb^{-1}$ although we have also discussed briefly the…

High Energy Physics - Phenomenology · Physics 2014-11-21 Nabanita Bhattacharyya , Amitava Datta , Sujoy Poddar

We examine the status of benchmark simplified dark matter models that have been proposed to explain the GeV gamma-ray Galactic Center excess. We constrain the available parameter space using updated observations from indirect detection,…

High Energy Physics - Phenomenology · Physics 2026-05-25 Yongao Hu , Cari Cesarotti , Tracy R. Slatyer

Recent experiments have measured the Galactic $\gamma$-ray diffuse emission up to PeV energies, opening a window to study acceleration of Galactic cosmic rays and their propagation up to the cosmic-ray knee. Furthermore, these observations…

High Energy Astrophysical Phenomena · Physics 2025-09-12 Manuel Rocamora , Pedro De La Torre Luque , Miguel A. Sánchez-Conde

The inert doublet model, a minimal extension of the Standard Model by a second Higgs doublet, is one of the simplest and most attractive scenarios that can explain the dark matter. In this paper, we demonstrate the existence of a new viable…

High Energy Physics - Phenomenology · Physics 2011-04-20 Laura Lopez-Honorez , Carlos E. Yaguna

A light singlino is a promising candidate for dark matter, and a light higgsino is natural in the parameter space of the NMSSM. We study the combined constraints on this scenario resulting from the dark matter relic density, the most recent…

High Energy Physics - Phenomenology · Physics 2018-09-26 Ulrich Ellwanger , Cyril Hugonie

The particle-physics nature of dark matter (DM) remains one of the central open questions in modern physics. A widely used framework to investigate DM properties is provided by simplified models (DMSimps), which extend the Standard Model…

High Energy Physics - Phenomenology · Physics 2025-10-13 Mattia Di Mauro , Bohan Xie

Dark matter decay or annihilation may produce monochromatic signals in the gamma-ray energy range. In this work we argue that there are strong theoretical motivations for studying these signals in the framework of gravitino dark matter…

The relationship between the degree of fine-tuning in Electroweak Symmetry Breaking (EWSB) and the discoverability of dark matter in current and next generation direct detection experiments is investigated in the context of two unified…

High Energy Physics - Phenomenology · Physics 2015-06-11 Pearl Sandick

High energy ${\gamma}$-rays are powerful probes in the search for annihilations of dark matter (DM) par- ticles in dense environments. In several DM particle models their annihilation produces characteristic features such as lines, bumps or…

High Energy Astrophysical Phenomena · Physics 2019-08-15 Louise Oakes , Aion Viana , Emmanuel Moulin , Lucia Rinchiuso , Ullrich Schwanke , Marco Cirelli , Paolo Panci , Filippo Sala , Joseph Silk , Marco Taoso

We outline the unique opportunities and challenges in the search for "ultraheavy" dark matter candidates with masses between roughly $10~{\rm TeV}$ and the Planck scale $m_{\rm pl} \approx 10^{16}~{\rm TeV}$. This mass range presents a wide…

We calculate direct detection constraints on inelastic dark matter (DM) for a scalar portal scenario with leptophilic couplings. The p-wave velocity suppression of the annihilation cross section of scalar-mediated inelastic Dirac DM implies…

High Energy Physics - Phenomenology · Physics 2026-04-17 I. V. Voronchikhin , D. V. Kirpichnikov

The H.E.S.S. experiment is an array of four identical imaging atmospheric Cherenkov telescopes in the Southern hemisphere, designed to observe very high energy gamma-rays (E > 100 GeV). These high energy gamma-rays can be used to search for…

High Energy Astrophysical Phenomena · Physics 2011-11-28 A. Viana

We consider the possibility that neutrino masses arise from the exchange of dark matter states. We examine in detail the phenomenology of fermionic dark matter in the singlet-triplet scotogenic reference model. We explore the case of…

High Energy Physics - Phenomenology · Physics 2024-01-24 Anirban Karan , Soumya Sadhukhan , José W. F. Valle

We propose a minimal scenario for light thermal dark matter (DM) in sub-GeV to GeV range by incorporating a scalar singlet DM in a type-I seesaw scenario extended by an additional Higgs doublet $\phi_2$. The latter permits efficient…

High Energy Physics - Phenomenology · Physics 2025-07-16 Debasish Borah , Pritam Das , Satyabrata Mahapatra , Narendra Sahu

Recently, the HESS telescope has observed a gamma-ray spectrum from the galactic center extending to at least $\sim$10 TeV. Although it has been suggested that this could be the product of annihilating dark matter particles, the candidates…

High Energy Physics - Phenomenology · Physics 2009-11-10 Dan Hooper , John March-Russell