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Related papers: Muon-induced neutrons do not explain the DAMA data

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For many years annually modulating $\sim$ keV scintillations have been observed in the DAMA/NaI and DAMA/Libra experiments. A dark matter - electron scattering interpretation is now favoured given the stringent constraints on nuclear recoil…

High Energy Physics - Phenomenology · Physics 2016-07-01 R. Foot

Background induced by neutrons in deep underground laboratories is a critical issue for all experiments looking for rare events, such as dark matter interactions or neutrinoless 2-beta decay. Neutrons can be produced either by natural…

Astrophysics · Physics 2009-06-23 V. A. Kudryavtsev , L. Pandola , V. Tomasello

A muon collider is expected to produce a high intensity neutrino beam which is an admixture of either $\nu_{\mu}+\bar{\nu_e}$ or $\bar{\nu}_{\mu} +\nu_e$ which can can be directed to underground detectors far away from the source. It will…

High Energy Physics - Phenomenology · Physics 2011-07-19 R. N. Mohapatra

We report on experimental evidence of the generation of directional muons from a laser-wakefield accelerator driven by a PW-class laser. The muons were generated following the interaction of a GeV-scale high-charge electron beam with a…

We search for dark matter (DM) with a mass [3,12] $\mathrm{GeV} / c^2$ using an exposure of 3.51 $\mathrm{t} \times \mathrm{y}$ with the XENONnT experiment.We consider spin-independent DM-nucleon interactions mediated by a heavy or light…

High Energy Physics - Experiment · Physics 2025-06-09 E. Aprile , J. Aalbers , K. Abe , S. Ahmed Maouloud , L. Althueser , B. Andrieu , E. Angelino , D. Antón Martin , F. Arneodo , L. Baudis , M. Bazyk , L. Bellagamba , R. Biondi , A. Bismark , K. Boese , A. Brown , G. Bruno , R. Budnik , C. Cai , C. Capelli , J. M. R. Cardoso , A. P. Cimental Chávez , A. P. Colijn , J. Conrad , J. J. Cuenca-García , V. D'Andrea , L. C. Daniel Garcia , M. P. Decowski , A. Deisting , C. Di Donato , P. Di Gangi , S. Diglio , K. Eitel , S. el Morabit , A. Elykov , A. D. Ferella , C. Ferrari , H. Fischer , T. Flehmke , M. Flierman , W. Fulgione , C. Fuselli , P. Gaemers , R. Gaior , M. Galloway , F. Gao , S. Ghosh , R. Giacomobono , R. Glade-Beucke , L. Grandi , J. Grigat , H. Guan , M. Guida , P. Gyorgy , R. Hammann , A. Higuera , C. Hils , L. Hoetzsch , N. F. Hood , M. Iacovacci , Y. Itow , J. Jakob , F. Joerg , Y. Kaminaga , M. Kara , P. Kavrigin , S. Kazama , M. Kobayashi , D. Koke , A. Kopec , H. Landsman , R. F. Lang , L. Levinson , I. Li , S. Li , S. Liang , Y. -T. Lin , S. Lindemann , M. Lindner , K. Liu , M. Liu , J. Loizeau , F. Lombardi , J. Long , J. A. M. Lopes , T. Luce , Y. Ma , C. Macolino , J. Mahlstedt , A. Mancuso , L. Manenti , F. Marignetti , T. Marrodán Undagoitia , K. Martens , J. Masbou , E. Masson , S. Mastroianni , A. Melchiorre , J. Merz , M. Messina , A. Michael , K. Miuchi , A. Molinario , S. Moriyama , K. Morå , Y. Mosbacher , M. Murra , J. Müller , K. Ni , U. Oberlack , B. Paetsch , Y. Pan , Q. Pellegrini , R. Peres , C. Peters , J. Pienaar , M. Pierre , G. Plante , T. R. Pollmann , L. Principe , J. Qi , J. Qin , D. Ramírez García , M. Rajado , R. Singh , L. Sanchez , J. M. F. dos Santos , I. Sarnoff , G. Sartorelli , J. Schreiner , P. Schulte , H. Schulze Eißing , M. Schumann , L. Scotto Lavina , M. Selvi , F. Semeria , P. Shagin , S. Shi , J. Shi , M. Silva , H. Simgen , C. Szyszka , A. Takeda , P. -L. Tan , D. Thers , F. Toschi , G. Trinchero , C. D. Tunnell , F. Tönnies , K. Valerius , S. Vecchi , S. Vetter , F. I. Villazon Solar , G. Volta , C. Weinheimer , M. Weiss , D. Wenz , C. Wittweg , V. H. S. Wu , Y. Xing , D. Xu , Z. Xu , M. Yamashita , L. Yang , J. Ye , L. Yuan , G. Zavattini , M. Zhong

Mirror dark matter provides a simple framework for which to explain the DAMA/Libra annual modulation signal consistently with the null results of the other direct detection experiments. The simplest possibility involves ordinary matter…

Astrophysics · Physics 2010-04-21 Paolo Ciarcelluti , Robert Foot

Xenon dual-phase time projections chambers (TPCs) have proven to be a successful technology in studying physical phenomena that require low-background conditions. With 40t of liquid xenon (LXe) in the TPC baseline design, DARWIN will have a…

Instrumentation and Detectors · Physics 2024-07-26 M. Adrover , L. Althueser , B. Andrieu , E. Angelino , J. R. Angevaare , B. Antunovic , E. Aprile , M. Babicz , D. Bajpai , E. Barberio , L. Baudis , M. Bazyk , N. Bell , L. Bellagamba , R. Biondi , Y. Biondi , A. Bismark , C. Boehm , A. Breskin , E. J. Brookes , A. Brown , G. Bruno , R. Budnik , C. Capelli , J. M. R. Cardoso , A. Chauvin , A. P. Cimental Chavez , A. P. Colijn , J. Conrad , J. J. Cuenca-García , V. D'Andrea , M. P. Decowski , A. Deisting , P. Di Gangi , S. Diglio , M. Doerenkamp , G. Drexlin , K. Eitel , A. Elykov , R. Engel , S. Farrell , A. D. Ferella , C. Ferrari , H. Fischer , M. Flierman , W. Fulgione , P. Gaemers , R. Gaior , M. Galloway , N. Garroum , S. Ghosh , F. Girard , R. Glade-Beucke , F. Glück , L. Grandi , J. Grigat , R. Größle , H. Guan , M. Guida , R. Hammann , V. Hannen , S. Hansmann-Menzemer , N. Hargittai , T. Hasegawa , C. Hils , A. Higuera , K. Hiraoka , L. Hoetzsch , M. Iacovacci , Y. Itow , J. Jakob , F. Jörg , M. Kara , P. Kavrigin , S. Kazama , M. Keller , B. Kilminster , M. Kleifges , M. Kobayashi , A. Kopec , B. von Krosigk , F. Kuger , H. Landsman , R. F. Lang , I. Li , S. Li , S. Liang , S. Lindemann , M. Lindner , F. Lombardi , J. Loizeau , T. Luce , Y. Ma , C. Macolino , J. Mahlstedt , A. Mancuso , T. Marrodán Undagoitia , J. A. M. Lopes , F. Marignetti , K. Martens , J. Masbou , S. Mastroianni , S. Milutinovic , K. Miuchi , R. Miyata , A. Molinario , C. M. B. Monteiro , K. Morå , E. Morteau , Y. Mosbacher , J. Müller , M. Murra , J. L. Newstead , K. Ni , U. G. Oberlack , I. Ostrovskiy , B. Paetsch , M. Pandurovic , Q. Pellegrini , R. Peres , J. Pienaar , M. Pierre , M. Piotter , G. Plante , T. R. Pollmann , L. Principe , J. Qi , J. Qin , M. Rajado Silva , D. Ramírez García , A. Razeto , S. Sakamoto , L. Sanchez , P. Sanchez-Lucas , J. M. F. dos Santos , G. Sartorelli , A. Scaffidi , P. Schulte , H. -C. Schultz-Coulon , H. Schulze Eißing , M. Schumann , L. Scotto Lavina , M. Selvi , F. Semeria , P. Shagin , S. Sharma , W. Shen , M. Silva , H. Simgen , R. Singh , M. Solmaz , O. Stanley , M. Steidl , P. L. Tan , A. Terliuk , D. Thers , T. Thümmler , F. Tönnies , F. Toschi , G. Trinchero , R. Trotta , C. Tunnell , P. Urquijo , K. Valerius , S. Vecchi , S. Vetter , G. Volta , D. Vorkapic , W. Wang , K. M. Weerman , C. Weinheimer , M. Weiss , D. Wenz , C. Wittweg , J. Wolf , T. Wolf , V. H. S. Wu , M. Wurm , Y. Xing , M. Yamashita , J. Ye , G. Zavattini , K. Zuber

Upward-going stopping muons initiated by atmospheric \numu and \anumu interactions in the rock below the Soudan 2 detector have been isolated, together with a companion sample of neutrino-induced single muons, created within the detector,…

High Energy Physics - Experiment · Physics 2008-11-26 2 Collaboration , W. W. M. Allison

A weakly interacting massive particle (WIMP) weighing only a few GeV has been invoked as an explanation for the signal from the DAMA/LIBRA experiment. We show that the data from DAMA/LIBRA are now powerful enough to strongly constrain the…

High Energy Physics - Phenomenology · Physics 2009-06-30 Spencer Chang , Aaron Pierce , Neal Weiner

We introduce and study the first class of signals that can probe the dark matter in Mesogenesis which will be observable at current and upcoming large volume neutrino experiments. The well-motivated Mesogenesis scenario for generating the…

High Energy Physics - Phenomenology · Physics 2024-01-26 Joshua Berger , Gilly Elor

The neutrino experiment KARMEN is situated at the beam stop neutrino source ISIS. It provides nu_mu's, nu_e's and nu_mu_bar's in equal intensities from the pi+ mu+ decay at rest. The oscillation channels nu_mu->nu_e and nu_mu_bar->nu_e_bar…

High Energy Physics - Experiment · Physics 2012-08-27 KARMEN Collaboration

This article describes the Monte Carlo simulation used to interpret the measurement of the muon-induced neutron flux in the Boulby Underground Laboratory (North Yorkshire, UK), recently performed using a large scintillator veto deployed…

High Energy Physics - Experiment · Physics 2011-05-23 A. Lindote , H. M. Araujo , V. A. Kudryavtsev , M. Robinson

The Large Volume Detector (LVD), hosted in the INFN Laboratori Nazionali del Gran Sasso, is triggered by atmospheric muons at a rate of $\sim 0.1$~Hz. The data collected over almost a quarter of century are used to study the muon intensity…

Upward-going muons observed by the Super-Kamiokande detector are produced by high-energy atmospheric neutrinos which interact in rock around the detector. Those which pass completely through the detector have a mean parent neutrino energy…

High Energy Physics - Experiment · Physics 2019-08-14 A. Habig

[Background] Long-Baseline experiments such as T2K, NOvA or the planned Deep Underground Neutrino Experiment (DUNE) require theoretical descriptions of the complete event in a neutrino-nucleus reaction. Since nuclear targets are used this…

Nuclear Theory · Physics 2017-07-26 U. Mosel , K. Gallmeister

The DAMA/LIBRA collaboration has detected an annual modulation of the recoil rate in NaI crystals with the phase expected for WIMP scattering events. This signal is dramatically inconsistent with upper limits from other experiments for…

Cosmology and Nongalactic Astrophysics · Physics 2010-09-14 Douglas P. Finkbeiner , Tongyan Lin , Neal Weiner

We consider a model where neutrinos interact with weakly interacting massive particles (WIMPs) as a possible explanation for the production of NuTeV's anomalous dimuon events. This model naturally produces the features reported by NuTeV,…

High Energy Physics - Phenomenology · Physics 2011-07-05 Andrew Alton , Thomas Alexander

ArgoNeuT, or Argon Neutrino Test, is a 170 liter liquid argon time projection chamber designed to collect neutrino interactions from the NuMI beam at Fermi National Accelerator Laboratory. ArgoNeuT operated in the NuMI low-energy beam line…

Accelerator-based experiments reliant on charged pion and kaon decays to produce muon-neutrino beams also deliver an associated powerful flux of muons. Therefore, these experiments can additionally be sensitive to light new particles that…

High Energy Physics - Phenomenology · Physics 2023-11-21 Cari Cesarotti , Yonatan Kahn , Gordan Krnjaic , Duncan Rocha , Joshua Spitz