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Related papers: Bounds on Light Dark Matter

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In the cosmological paradigm, cold dark matter (DM) dominates the mass content of the Universe and is present at every scale. Candidates for DM include many extensions of the standard model, such as weakly interacting massive particles…

High Energy Astrophysical Phenomena · Physics 2019-08-13 Benjamin Zitzer

In the past few years, many mesoscale systems have been proposed as possible detectors of sub-GeV dark matter particles. In this work, we point out the feasibility of probing dark matter-nucleon scattering cross section using…

High Energy Physics - Phenomenology · Physics 2023-11-15 Anirban Das , Noah Kurinsky , Rebecca K. Leane

Massive particles with self interactions of the order of 0.2 barn/GeV are intriguing Dark Matter candidates from an astrophysical point of view. Current and past experiments for direct detection of massive Dark Matter particles are focusing…

Instrumentation and Methods for Astrophysics · Physics 2017-03-17 F. Nozzoli

Warm dark matter (WDM) might more easily account for small scale clustering measurements than the heavier particles typically invoked in Lambda cold dark matter (LCDM) cosmologies. In this paper, we consider a Lambda WDM cosmology in which…

Astrophysics · Physics 2009-11-11 Casey R. Watson , John F. Beacom , Hasan Yuksel , Terry P. Walker

Searches for Dark Matter at the LHC are commonly described in terms of simplified models with scalar, pseudo-scalar, vector and axial-vector mediators. In this work we explore the constraints imposed on such models from the observed Dark…

High Energy Physics - Phenomenology · Physics 2016-03-30 Tristan du Pree , Kristian Hahn , Philip Harris , Christos Roskas

We test the luminosity function of Milky Way satellites as a constraint for the nature of Dark Matter particles. We perform dissipationless high-resolution N-body simulations of the evolution of Galaxy-sized halo in the standard Cold Dark…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-14 Andrea V. Maccio' , Fabio Fontanot

Constraints on the indirect detection of dark matter are usually obtained from observations of astrophysical objects -- the Galactic Center, dwarf galaxies, M31, etc. Here we propose instead to look for the annihilation or decay of dark…

High Energy Physics - Phenomenology · Physics 2021-10-27 Teresa Marrodán Undagoitia , Werner Rodejohann , Tim Wolf , Carlos E. Yaguna

Resonantly produced sterile neutrinos are considered an attractive dark matter (DM) candidate only requiring a minimal, well motivated extension to the standard model of particle physics. With a particle mass restricted to the keV range,…

Cosmology and Nongalactic Astrophysics · Physics 2016-05-25 Aurel Schneider

In the conventional cosmology masses of the stable supersymmetric relics, candidates for the dark matter (DM) particles, should be typically below 1 TeV. This is in conflict with the LHC bounds on the low energy SUSY. However, in…

High Energy Physics - Phenomenology · Physics 2022-09-21 E. V. Arbuzova

Leptophilic sub-MeV spin-zero dark matter (DM) decays into photons via one-loop processes, a scenario that has been in part overlooked in current literature. In this work, we provide updated and comprehensive upper limits on scalar,…

High Energy Physics - Phenomenology · Physics 2025-09-30 Gabriele Montefalcone , Gilly Elor , Kimberly K. Boddy , Nicola Bellomo

We investigate the sensitivities of upcoming MeV gamma-ray telescopes to sterile neutrino dark matter in the mass range $(0.2-100)\,{\rm MeV}$. Sterile neutrinos in this regime can produce observable photon signals through radiative…

High Energy Physics - Phenomenology · Physics 2026-04-22 Shivam Gola , Akash Kumar Saha , Manibrata Sen

We present a comprehensive review of keV-scale sterile neutrino Dark Matter, collecting views and insights from all disciplines involved - cosmology, astrophysics, nuclear, and particle physics - in each case viewed from both theoretical…

High Energy Physics - Phenomenology · Physics 2017-02-10 R. Adhikari , M. Agostini , N. Anh Ky , T. Araki , M. Archidiacono , M. Bahr , J. Baur , J. Behrens , F. Bezrukov , P. S. Bhupal Dev , D. Borah , A. Boyarsky , A. de Gouvea , C. A. de S. Pires , H. J. de Vega , A. G. Dias , P. Di Bari , Z. Djurcic , K. Dolde , H. Dorrer , M. Durero , O. Dragoun , M. Drewes , G. Drexlin , Ch. E. Düllmann , K. Eberhardt , S. Eliseev , C. Enss , N. W. Evans , A. Faessler , P. Filianin , V. Fischer , A. Fleischmann , J. A. Formaggio , J. Franse , F. M. Fraenkle , C. S. Frenk , G. Fuller , L. Gastaldo , A. Garzilli , C. Giunti , F. Glück , M. C. Goodman , M. C. Gonzalez-Garcia , D. Gorbunov , J. Hamann , V. Hannen , S. Hannestad , S. H. Hansen , C. Hassel , J. Heeck , F. Hofmann , T. Houdy , A. Huber , D. Iakubovskyi , A. Ianni , A. Ibarra , R. Jacobsson , T. Jeltema , J. Jochum , S. Kempf , T. Kieck , M. Korzeczek , V. Kornoukhov , T. Lachenmaier , M. Laine , P. Langacker , T. Lasserre , J. Lesgourgues , D. Lhuillier , Y. F. Li , W. Liao , A. W. Long , M. Maltoni , G. Mangano , N. E. Mavromatos , N. Menci , A. Merle , S. Mertens , A. Mirizzi , B. Monreal , A. Nozik , A. Neronov , V. Niro , Y. Novikov , L. Oberauer , E. Otten , N. Palanque-Delabrouille , M. Pallavicini , V. S. Pantuev , E. Papastergis , S. Parke , S. Pascoli , S. Pastor , A. Patwardhan , A. Pilaftsis , D. C. Radford , P. C. -O. Ranitzsch , O. Rest , D. J. Robinson , P. S. Rodrigues da Silva , O. Ruchayskiy , N. G. Sanchez , M. Sasaki , N. Saviano , A. Schneider , F. Schneider , T. Schwetz , S. Schönert , S. Scholl , F. Shankar , R. Shrock , N. Steinbrink , L. Strigari , F. Suekane , B. Suerfu , R. Takahashi , N. Thi Hong Van , I. Tkachev , M. Totzauer , Y. Tsai , C. G. Tully , K. Valerius , J. W. F. Valle , D. Venos , M. Viel , M. Vivier , M. Y. Wang , C. Weinheimer , K. Wendt , L. Winslow , J. Wolf , M. Wurm , Z. Xing , S. Zhou , K. Zuber

Within the Minimal Supersymmetric Standard Model (MSSM) we systematically investigate the bounds on the mass of the lightest neutralino. We allow for non-universal gaugino masses and thus even consider massless neutralinos, while assuming…

High Energy Physics - Phenomenology · Physics 2010-04-23 H. K. Dreiner , S. Heinemeyer , O. Kittel , U. Langenfeld , A. M. Weber , G. Weiglein

In recent work, it has been argued that multi-TeV masses for scalar superpartners are not unnatural. Indeed, they appear to have significant phenomenological virtues. Here we explore the implications of such `focus point' supersymmetry for…

High Energy Physics - Phenomenology · Physics 2009-09-25 Jonathan L. Feng , Konstantin T. Matchev , Frank Wilczek

Dark matter and neutrinos provide the two most compelling pieces of evidence for new physics beyond the Standard Model of Particle Physics but they are often treated as two different sectors. In this paper, we consider how neutrino…

High Energy Physics - Phenomenology · Physics 2018-05-28 Andres Olivares-Del Campo , Sergio Palomares-Ruiz , Silvia Pascoli

As one of the fundamental unknowns of our Universe, the mass of dark matter remains to be a topic of great interest. We consider the possibility of a time-variation of the dark matter mass. We study the cosmological constraints on a model…

Cosmology and Nongalactic Astrophysics · Physics 2025-04-01 Amlan Chakraborty , Anirban Das , Subinoy Das , Shiv K. Sethi

We apply phase-space density considerations to obtain lower bounds on the mass of sterile neutrino as dark matter candidate. The bounds are different for non-resonant production, resonant production in the presence of lepton asymmetry and…

High Energy Physics - Phenomenology · Physics 2009-12-04 D. Gorbunov , A. Khmelnitsky , V. Rubakov

The impacts of the light sterile neutrino hypothesis in particle physics and cosmology are reviewed. The observed short baseline neutrino anomalies challenging the standard explanation of neutrino oscillations within the framework of three…

High Energy Physics - Phenomenology · Physics 2019-06-05 Sin Kyu Kang

We estimate the gamma ray fluxes from the residual annihilations of Dark Matter particles having a mass mdm \in [MeV, O(GeV)] and compare them to observations. We find that particles lighter than O(100 MeV) are excluded unless their cross…

Astrophysics · Physics 2008-11-26 C. Boehm , T. A. Ensslin , J. Silk

The existence of dark matter was suggested, using simple gravitational arguments, seventy years ago. Although we are now convinced that most of the mass in the Universe is indeed some non-luminous matter, we still do not know its…

High Energy Physics - Phenomenology · Physics 2009-11-10 Carlos Munoz
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