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Related papers: Hunting sub-GeV dark matter with NO$\nu$A near det…

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We survey the sensitivity of past and present neutrino experiments to MeV-GeV scale dark matter, and find that these experiments possess novel sensitivity that has not yet fully explored. NO$\nu$A and BEBC are found to rule out the scalar…

High Energy Physics - Phenomenology · Physics 2020-08-12 Luca Buonocore , Patrick deNiverville , Claudia Frugiuele

We demonstrate that current and planned underground neutrino experiments could offer a powerful probe of few-MeV dark matter when combined with a nearby high-intensity low-to-medium energy electron accelerator. This experimental setup, an…

High Energy Physics - Phenomenology · Physics 2015-11-18 Eder Izaguirre , Gordan Krnjaic , Maxim Pospelov

In a broad class of consistent models, MeV to few-GeV dark matter interacts with ordinary matter through weakly coupled GeV-scale mediators. We show that a suitable meter-scale (or smaller) detector situated downstream of an electron…

High Energy Physics - Phenomenology · Physics 2014-02-05 Eder Izaguirre , Gordan Krnjaic , Philip Schuster , Natalia Toro

The proposed NEWS apparatus, a spherical detector with a small central electrode sensor operating as a proportional counter, promises to explore new swaths of the direct detection parameter space in the GeV and sub-GeV Dark Matter particle…

High Energy Physics - Phenomenology · Physics 2016-03-11 Stefano Profumo

We describe an approach to detect dark matter and other invisible particles with mass below a GeV, exploiting missing energy-momentum measurements and other kinematic features of fixed-target production. In the case of an invisibly decaying…

High Energy Physics - Phenomenology · Physics 2015-05-27 Eder Izaguirre , Gordan Krnjaic , Philip Schuster , Natalia Toro

The NuMI facility at Fermilab produces a high-intensity beam of muon neutrinos and antineutrinos, designed to study neutrino oscillations. This beam may also be a source of dark matter particles produced through a light mediator. We search…

High Energy Physics - Experiment · Physics 2025-11-13 S. Abubakar , M. Acero , B. Acharya , P. Adamson , N. Anfimov , A. Antoshkin , E. Arrieta-Diaz , L. Asquith , A. Aurisano , A. Back , N. Balashov , P. Baldi , B. A. Bambah , E. F. Bannister , A. Barros , A. Bat , T. Bezerra , V. Bhatnagar , B. Bhuyan , J. Bian , A. C. Booth , R. Bowles , B. Brahma , C. Bromberg , N. Buchanan , A. Butkevich , T. J. Carroll , E. Catano-Mur , J. P. Cesar , R. Chirco , S. Choate , B. C. Choudhary , O. T. K. Chow , A. Christensen , M. F. Cicala , T. E. Coan , T. Contreras , A. Cooleybeck , D. Coveyou , L. Cremonesi , G. S. Davies , P. F. Derwent , Z. Djurcic , K. Dobbs , D. Duenas Tonguino , E. C. Dukes , R. Ehrlich , E. Ewart , P. Filip , M. J. Frank , H. R. Gallagher , A. Giri , R. A. Gomes , M. C. Goodman , R. Group , A. Habig , F. Hakl , J. Hartnell , R. Hatcher , J. M. Hays , M. He , K. Heller , V Hewes , A. Himmel , T. Horoho , X. Huang , A. Ivanova , I. Kakorin , A. Kalitkina , D. M. Kaplan , A. Khanam , B. Kirezli , J. Kleykamp , O. Klimov , L. W. Koerner , L. Kolupaeva , R. Kralik , A. Kumar , C. D. Kuruppu , V. Kus , T. Lackey , K. Lang , J. Lesmeister , A. Lister , J. A. Lock , S. Magill , W. A. Mann , M. T. Manoharan , M. Manrique Plata , M. L. Marshak , M. Martinez-Casales , V. Matveev , A. Medhi , B. Mehta , M. D. Messier , H. Meyer , T. Miao , W. H. Miller , S. R. Mishra , R. Mohanta , A. Moren , A. Morozova , W. Mu , L. Mualem , M. Muether , C. Murthy , D. Myers , J. Nachtman , D. Naples , J. K. Nelson , O. Neogi , R. Nichol , E. Niner , A. Norman , A. Norrick , H. Oh , A. Olshevskiy , T. Olson , A. Pal , J. Paley , L. Panda , R. B. Patterson , G. Pawloski , R. Petti , L. R. Prais , A. Rafique , V. Raj , M. Rajaoalisoa , B. Ramson , B. Rebel , C. Reynolds , E. Robles , P. Roy , O. Samoylov , M. C. Sanchez , S. Sanchez Falero , P. Shanahan , P. Sharma , A. Sheshukov , Shivam , A. Shmakov , W. Shorrock , S. Shukla , I. Singh , V. Singh , S. Singh Chhibra , J. Smolik , P. Snopok , N. Solomey , A. Sousa , K. Soustruznik , M. Strait , C. Sullivan , L. Suter , A. Sutton , S. Swain , A. Sztuc , N. Talukdar , P. Tas , J. Thomas , E. Tiras , M. Titus , Y. Torun , D. Tran , J. Trokan-Tenorio , J. Urheim , B. Utt , P. Vahle , Z. Vallari , K. J. Vockerodt , A. V. Waldron , M. Wallbank , C. Weber , M. Wetstein , D. Whittington , D. A. Wickremasinghe , J. Wolcott , S. Wu , W. Wu , Y. Xiao , B. Yaeggy , A. Yahaya , A. Yankelevich , K. Yonehara , S. Zadorozhnyy , J. Zalesak , R. Zwaska

Particle dark matter could have a mass anywhere from that of ultralight candidates, $m_\chi\sim 10^{-21}\,$eV, to scales well above the GeV. Conventional laboratory searches are sensitive to a range of masses close to the weak scale, while…

High Energy Physics - Phenomenology · Physics 2019-09-13 Rodrigo Alonso , Diego Blas , Peter Wolf

The next generation of neutrino telescopes will feature unprecedented sensitivities in the detection of neutrinos. Here we study the capabilities of a large-scale neutrino telescope, like the fully-operating KM3NeT experiment in the near…

High Energy Physics - Phenomenology · Physics 2023-08-16 L. Salvador Miranda , S. Basegmez du Pree , K. C. Y. Ng , A. Cheek , C. Arina

The astrophysics community is considering plans for a variety of gamma-ray telescopes (including ACT and GRIPS) in the energy range 1--100 MeV, which can fill in the so-called "MeV gap" in current sensitivity. We investigate the utility of…

Cosmology and Nongalactic Astrophysics · Physics 2015-09-15 Kimberly K. Boddy , Jason Kumar

The existence of dark matter is undisputed, while the nature of it is still unknown. Explaining dark matter with the existence of a new unobserved particle is among the most promising possible solutions. Recently dark matter candidates in…

Instrumentation and Detectors · Physics 2017-12-12 Alexander Baehr , Holger Kluck , Jelena Ninkovic , Jochen Schieck , Johannes Treis

Light dark matter is a compelling experimental target in light of stringent constraints on heavier WIMPs. However, for a sub-MeV WIMP, the universe is sufficiently well understood at temperatures below 10 MeV that there is no room for it to…

High Energy Physics - Phenomenology · Physics 2018-03-02 Daniel Green , Surjeet Rajendran

It was recently shown that standard sub-GeV dark matter candidates can be effectively probed by large neutrino observatories via annual modulation of the total photomultiplier hit rate. That work focused on the production of light by the…

High Energy Physics - Phenomenology · Physics 2025-12-17 Lillian Santos-Olmsted , Rebecca K. Leane , Carlos Blanco , John F. Beacom

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

Sub-GeV Dark Matter particles upscattered by cosmic rays gain enough kinetic energy to pass the thresholds of large volume detectors on Earth. We then use public Super-Kamiokande and MiniBooNE data to derive a novel limit on the scattering…

High Energy Physics - Phenomenology · Physics 2019-05-15 Yohei Ema , Filippo Sala , Ryosuke Sato

Assuming that dark matter particles interact with quarks via a GeV-scale mediator, we study dark matter production in fixed target collisions. The ensuing signal in a neutrino near detector consists of neutral-current events with an energy…

High Energy Physics - Phenomenology · Physics 2015-06-23 Bogdan A. Dobrescu , Claudia Frugiuele

Direct detection strategies are proposed for dark matter particles with MeV to GeV mass. In this largely unexplored mass range, dark matter scattering with electrons can cause single-electron ionization signals, which are detectable with…

High Energy Physics - Phenomenology · Physics 2012-06-01 Rouven Essig , Jeremy Mardon , Tomer Volansky

We propose a new method to detect sub-GeV dark matter, through their scatterings from free leptons and the resulting kinematic shifts. Specially, such an experiment can detect dark matter interacting solely with muons. The experiment…

High Energy Physics - Phenomenology · Physics 2023-10-12 Alim Ruzi , Chen Zhou , Xiaohu Sun , Dayong Wang , Siguang Wang , Yong Ban , Yajun Mao , Qite Li , Qiang Li

Dark matter with mass below about a GeV is essentially unobservable in conventional direct detection experiments. However, newly proposed technology will allow the detection of single electron events in semiconductor materials with…

High Energy Physics - Phenomenology · Physics 2012-11-13 Peter W. Graham , David E. Kaplan , Surjeet Rajendran , Matthew T. Walters

Highly energetic proton/electron beam fixed target experiments extends an opportunity to probe the sub-GeV dark matter and associated interactions. In this work we have explored the sensitivity of DUNE for sub-GeV leptophobic dark matter…

High Energy Physics - Phenomenology · Physics 2020-12-03 Sabeeha Naaz , Jyotsna Singh , R. B. Singh

Sterile neutrinos with the mass in the keV range are interesting warm dark matter (WDM) candidates. The restrictions on their parameters (mass and mixing angle) obtained by current X-ray missions (XMM-Newton or Chandra) can only be improved…

Astrophysics · Physics 2008-11-26 Alexey Boyarsky , Jan Willem den Herder , Andrey Neronov , Oleg Ruchayskiy
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