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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

A search for sub-GeV dark matter produced from collisions of the Fermilab 8 GeV Booster protons with a steel beam dump was performed by the MiniBooNE-DM Collaboration using data from $1.86 \times 10^{20}$ protons on target in a dedicated…

The MiniBooNE-DM collaboration searched for vector-boson mediated production of dark matter using the Fermilab 8 GeV Booster proton beam in a dedicated run with $1.86 \times 10^{20}$ protons delivered to a steel beam dump. The MiniBooNE…

We study the sensitivity to sub-GeV dark sectors of high energy ($ \geq100$ GeV) proton fixed target experiments such as the Main Injector and the future Long-Baseline Neutrino Facility (LBNF). We focus on off-axis detectors since they have…

High Energy Physics - Phenomenology · Physics 2017-08-02 Claudia Frugiuele

In a dedicated run where protons from the Fermilab Booster were delivered directly to the steel beam dump of the Booster Neutrino Beamline (BNB), the MiniBooNE detector was used to search for the production of sub-GeV dark matter particles…

High Energy Physics - Experiment · Physics 2020-01-29 Alexis A. Aguilar-Arevalo

Cosmology observations indicate that our universe is composed of 25% dark matter (DM), yet we know little about its microscopic properties. Whereas the gravitational interaction of DM is well understood, its interaction with the Standard…

High Energy Physics - Experiment · Physics 2015-01-05 R. T. Thornton , MiniBooNE-DM collaboration

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

We consider the sensitivity of fixed-target neutrino experiments at the luminosity frontier to light stable states, such as those present in models of MeV-scale dark matter. To ensure the correct thermal relic abundance, such states must…

High Energy Physics - Phenomenology · Physics 2015-03-19 Patrick deNiverville , Maxim Pospelov , Adam Ritz

We analyze the prospects for detection of light sub-GeV dark matter produced in experiments designed to study the properties of neutrinos, such as MiniBooNE, T2K, SHiP, DUNE etc. We present an improved production model, when dark matter…

High Energy Physics - Phenomenology · Physics 2017-02-15 Patrick deNiverville , Chien-Yi Chen , Maxim Pospelov , Adam Ritz

We present a first search for dark-trident scattering in a neutrino beam using a data set corresponding to $7.2 \times 10^{20}$ protons on target taken with the MicroBooNE detector at Fermilab. Proton interactions in the neutrino target at…

High Energy Physics - Experiment · Physics 2024-05-17 MicroBooNE collaboration , P. Abratenko , O. Alterkait , D. Andrade Aldana , L. Arellano , J. Asaadi , A. Ashkenazi , S. Balasubramanian , B. Baller , G. Barr , D. Barrow , J. Barrow , V. Basque , O. Benevides Rodrigues , S. Berkman , A. Bhanderi , A. Bhat , M. Bhattacharya , M. Bishai , A. Blake , B. Bogart , T. Bolton , J. Y. Book , M. B. Brunetti , L. Camilleri , Y. Cao , D. Caratelli , F. Cavanna , G. Cerati , A. Chappell , Y. Chen , J. M. Conrad , M. Convery , L. Cooper-Troendle , J. I. Crespo-Anadon , R. Cross , M. Del Tutto , S. R. Dennis , P. Detje , A. Devitt , R. Diurba , Z. Djurcic , R. Dorrill , K. Duffy , S. Dytman , B. Eberly , P. Englezos , A. Ereditato , J. J. Evans , R. Fine , O. G. Finnerud , B. T. Fleming , W. Foreman , D. Franco , A. P. Furmanski , F. Gao , D. Garcia-Gamez , S. Gardiner , G. Ge , S. Gollapinni , E. Gramellini , P. Green , H. Greenlee , L. Gu , W. Gu , R. Guenette , P. Guzowski , L. Hagaman , O. Hen , C. Hilgenberg , G. A. Horton-Smith , Z. Imani , B. Irwin , M. S. Ismail , C. James , X. Ji , J. H. Jo , R. A. Johnson , Y. J. Jwa , D. Kalra , N. Kamp , G. Karagiorgi , W. Ketchum , M. Kirby , T. Kobilarcik , I. Kreslo , M. B. Leibovitch , I. Lepetic , J. -Y. Li , K. Li , Y. Li , K. Lin , B. R. Littlejohn , H. Liu , W. C. Louis , X. Luo , C. Mariani , D. Marsden , J. Marshall , N. Martinez , D. A. Martinez Caicedo , S. Martynenko , A. Mastbaum , I. Mawby , N. McConkey , V. Meddage , J. Micallef , K. Miller , K. Mistry , T. Mohayai , A. Mogan , M. Mooney , A. F. Moor , C. D. Moore , L. Mora Lepin , M. M. Moudgalya , S. Mulleria Babu , D. Naples , A. Navrer-Agasson , N. Nayak , M. Nebot-Guinot , J. Nowak , N. Oza , O. Palamara , N. Pallat , V. Paolone , A. Papadopoulou , V. Papavassiliou , H. Parkinson , S. F. Pate , N. Patel , Z. Pavlovic , E. Piasetzky , I. Pophale , X. Qian , J. L. Raaf , V. Radeka , A. Rafique , M. Reggiani-Guzzo , L. Ren , L. Rochester , J. Rodriguez Rondon , M. Rosenberg , M. Ross-Lonergan , C. Rudolph von Rohr , I. Safa , G. Scanavini , D. W. Schmitz , A. Schukraft , W. Seligman , M. H. Shaevitz , R. Sharankova , J. Shi , E. L. Snider , M. Soderberg , S. Soldner-Rembold , J. Spitz , M. Stancari , J. St. John , T. Strauss , A. M. Szelc , W. Tang , N. Taniuchi , K. Terao , C. Thorpe , D. Torbunov , D. Totani , M. Toups , Y. -T. Tsai , J. Tyler , M. A. Uchida , T. Usher , B. Viren , M. Weber , H. Wei , A. J. White , S. Wolbers , T. Wongjirad , M. Wospakrik , K. Wresilo , W. Wu , E. Yandel , T. Yang , L. E. Yates , H. W. Yu , G. P. Zeller , J. Zennamo , C. Zhang

We study the sensitivity of the Fermilab Short-Baseline Neutrino (SBN) experiments, MicroBooNE, ICARUS, and SBND, to MeV- to GeV-scale inelastic dark matter interacting through a dark photon mediator. These models provide interesting…

High Energy Physics - Phenomenology · Physics 2021-11-03 Brian Batell , Joshua Berger , Luc Darmé , Claudia Frugiuele

A proposal submitted to the FNAL PAC is described to search for light sub-GeV WIMP dark matter at MiniBooNE. The possibility to steer the beam past the target and into an absorber leads to a significant reduction in neutrino background,…

Dark Matter (DM) comprising particles in the mass range of a few MeV to GeV is waiting to be explored, given the many theoretical models accommodating cosmological abundance. We hereby propose an experiment with the LHC proton beam of 7 TeV…

High Energy Physics - Experiment · Physics 2016-09-04 Ashok Kumar , Archana Sharma

Accelerator-based neutrino experiments with high-intensity proton beams and advanced detector technologies provide a powerful and complementary approach to probing physics beyond the Standard Model. The MiniBooNE experiment at Fermilab…

High Energy Physics - Phenomenology · Physics 2026-03-30 Bhaskar Dutta , Debopam Goswami , Aparajitha Karthikeyan , Vishvas Pandey , Zahra Tabrizi , Adrian Thompson , Richard G. Van de Water

High-luminosity fixed-target neutrino experiments present a new opportunity to search for light sub-GeV dark matter and associated new forces. We analyze the physics reach of these experiments to light leptophobic dark states coupled to the…

High Energy Physics - Phenomenology · Physics 2014-12-31 Brian Batell , Patrick deNiverville , David McKeen , Maxim Pospelov , Adam Ritz

Neutrino and dark matter experiments with large-volume ($\gtrsim 1$ ton) detectors can provide excellent sensitivity to signals induced by energetic light dark matter coming from the present universe. Taking boosted dark matter as a…

High Energy Physics - Phenomenology · Physics 2020-07-16 Doojin Kim , Pedro A. N. Machado , Jong-Chul Park , Seodong Shin

We propose a new approach to search for light dark matter (DM), with keV-GeV mass, via inelastic nucleus scattering at large-volume neutrino detectors such as Borexino, DUNE, Super-K, Hyper-K, and JUNO. The approach uses inelastic nuclear…

High Energy Physics - Phenomenology · Physics 2024-10-21 Bhaskar Dutta , Wei-Chih Huang , Doojin Kim , Jayden L. Newstead , Jong-Chul Park , Iman Shaukat Ali

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

Short-baseline neutrino (SBN) facilities are optimal for new-physics searches, including the possible production of new particles in and along the neutrino beamline. One such class of models considers states that are created by neutrino…

High Energy Physics - Phenomenology · Physics 2025-07-11 Bhaskar Dutta , Debopam Goswami , Aparajitha Karthikeyan , Kevin J. Kelly

Core-collapse supernovae, among the universe's most energetic events, offer a novel window into the dark sector by potentially producing a flux of boosted dark matter (BDM). We explore the potential to detect the BDM produced by supernovae…

High Energy Physics - Phenomenology · Physics 2025-06-23 Badal Bhalla , Fazlollah Hajkarim , Doojin Kim , Kuver Sinha
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