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Related papers: The XENONnT Dark Matter Experiment

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XENON10 is an experiment designed to directly detect particle dark matter. It is a dual phase (liquid/gas) xenon time-projection chamber with 3D position imaging. Particle interactions generate a primary scintillation signal (S1) and…

NEXT (Neutrino Experiment with a Xenon TPC) is a neutrinoless double beta decay experiment located at the Laboratorio Subterr\'aneo de Canfranc (LSC, Spain). Its aim is to demonstrate that the neutrino is a Majorana particle by detecting…

Instrumentation and Detectors · Physics 2022-09-21 Carmen Romo-Luque

We show that the excess in electron recoil events seen by the XENON1T experiment can be explained by relatively low-mass Luminous Dark Matter candidate. The dark matter scatters inelastically in the detector (or the surrounding rock), to…

High Energy Physics - Phenomenology · Physics 2020-10-15 Nicole F. Bell , James B. Dent , Bhaskar Dutta , Sumit Ghosh , Jason Kumar , Jayden L. Newstead

Although observations made with the CoGeNT and CDMS experiments have been interpreted as possible signals of low-mass (~7-10 GeV) dark matter particles, constraints from the XENON100 collaboration appear to be incompatible with this…

High Energy Physics - Phenomenology · Physics 2015-06-16 Dan Hooper

Dual-phase time projection chambers (TPCs) filled with the liquid noble gas xenon (LXe) are currently the most sensitive detectors searching for interactions of WIMP dark matter in a laboratory-based experiment. This is achieved by…

Instrumentation and Methods for Astrophysics · Physics 2014-08-08 Marc Schumann

The Neutrino Experiment with a Xenon TPC (NEXT) seeks to discover the neutrinoless double beta ($\beta\beta 0\nu$) decay of $^{136}$Xe using a high-pressure xenon gas time projection chamber with electroluminescent amplification. The…

Instrumentation and Detectors · Physics 2019-11-06 Justo Martín-Albo

A search for dark matter using an underground single-phase liquid xenon detector was conducted at the Kamioka Observatory in Japan, particularly for Weakly Interacting Massive Particles (WIMPs). We have used 705.9 live days of data in a…

Direct detection experiments aim at the detection of dark matter in the form of weakly interacting massive particles (WIMPs) by searching for signals from elastic dark matter nucleus scattering. Additionally, inelastic scattering in which…

High Energy Physics - Phenomenology · Physics 2020-01-08 G. Arcadi , C. Döring , C. Hasterok , S. Vogl

A multi-target detection system XAX, comprising concentric 10 ton targets of 136Xe and 129/131Xe, together with a geometrically similar or larger target of liquid Ar, is described. Each is configured as a two-phase scintillation/ionization…

Dark Matter particles can be detected directly via their elastic scattering with nuclei. Next generation experiments can eventually find physical evidences about dark matter candidates. With this motivation in mind, we have calculated the…

High Energy Physics - Phenomenology · Physics 2022-02-09 K. J. Fushimi , M. M. Saez , M. E. Mosquera , O. Civitarese

Dual-phase liquid xenon time projection chambers are the core detector elements of many experiments that conduct searches for Dark Matter and rare events, as well as in neutrino and high-energy physics. As part of this detector technology,…

A good particle candidate for Cold Dark Matter (CDM) is the supersymmetric neutralino or more generally a weakly interacting massive particle (WIMP). The expected interaction rate of WIMPs with the detector medium in the direct detection…

Instrumentation and Methods for Astrophysics · Physics 2010-02-17 V. Kozlov

The EXO-200 experiment searched for neutrinoless double-beta decay of $^{136}$Xe with a single-phase liquid xenon detector. It used an active mass of 110 kg of 80.6%-enriched liquid xenon in an ultra-low background time projection chamber…

Instrumentation and Detectors · Physics 2022-02-23 N. Ackerman , J. Albert , M. Auger , D. J. Auty , I. Badhrees , P. S. Barbeau , L. Bartoszek , E. Baussan , V. Belov , C. Benitez-Medina , T. Bhatta , M. Breidenbach , T. Brunner , G. F. Cao , W. R. Cen , C. Chambers , B. Cleveland , R. Conley , S. Cook , M. Coon , W. Craddock , A. Craycraft , W. Cree , T. Daniels , L. Darroch , S. J. Daugherty , J. Daughhetee , C. G. Davis , J. Davis , S. Delaquis , A. Der Mesrobian-Kabakian , R. deVoe , T. Didberidze , J. Dilling , A. Dobi , A. G. Dolgolenko , M. J. Dolinski , M. Dunford , J. Echevers , L. Espic , W. Fairbank , D. Fairbank , J. Farine , W. Feldmeier , S. Feyzbakhsh , P. Fierlinger , K. Fouts , D. Franco , D. Freytag , D. Fudenberg , P. Gautam , G. Giroux , R. Gornea , K. Graham , G. Gratta , C. Hagemann , C. Hall , K. Hall , G. Haller , E. V. Hansen , C. Hargrove , R. Herbst , S. Herrin , J. Hodgson , M. Hughes , A. Iverson , A. Jamil , C. Jessiman , M. J. Jewell , A. Johnson , T. N. Johnson , S. Johnston , A. Karelin , L. J. Kaufman , R. Killick , T. Koffas , S. Kravitz , R. Krücken , A. Kuchenkov , K. S. Kumar , Y. Lan , A. Larson , D. S. Leonard , F. Leonard , F. LePort , G. S. Li , S. Li , Z. Li , C. Licciardi , Y. H. Lin , D. Mackay , R. MacLellan , M. Marino , J. -M. Martin , Y. Martin , T. McElroy , K. McFarlane , T. Michel , B. Mong , D. C. Moore , K. Murray , R. Neilson , O. Njoya , O. Nusair , K. O'Sullivan , A. Odian , I. Ostrovskiy , C. Ouellet , A. Piepke , A. Pocar , C. Y. Prescott , K. Pushkin , F. Retiere , A. Rivas , A. L. Robinson , E. Rollin , P. C. Rowson , M. P. Rozo , J. Runge , J. J. Russell , S. Schmidt , A. Schubert , D. Sinclair , K. Skarpaas , S. Slutsky , E. Smith , A. K. Soma , V. Stekhanov , V. Strickland , M. Swift , M. Tarka , J. Todd , T. Tolba , D. Tosi , T. I. Totev , R. Tsang , K. Twelker , B. Veenstra , V. Veeraraghavan , J. -L. Vuilleumier , J. -M. Vuilleumier , M. Wagenpfeil , A. Waite , J. Walton , T. Walton , K. Wamba , J. Watkins , M. Weber , L. J. Wen , U. Wichoski , M. Wittgen , J. Wodin , J. Wood , G. Wrede , S. X. Wu , Q. Xia , L. Yang , Y. -R. Yen , O. Ya Zeldovich , T. Ziegler

We consider models of xenophobic dark matter, in which isospin-violating dark matter-nucleon interactions significantly degrade the response of xenon direct detection experiments. For models of near-maximal xenophobia, with…

High Energy Physics - Phenomenology · Physics 2013-08-09 Jonathan L. Feng , Jason Kumar , David Sanford

Dark matter can scatter and excite a nucleus to a low-lying excitation in a direct detection experiment. This signature is distinct from the canonical elastic scattering signal because the inelastic signal also contains the energy deposited…

High Energy Physics - Phenomenology · Physics 2016-05-24 Christopher McCabe

We have witnessed the beginning of an era where dark matter and neutrino detectors can probe similar new physics phenomena. Motivated by the low-energy electron recoil spectrum observed by the dark matter experiment, XENON1T, at Gran Sasso…

High Energy Physics - Phenomenology · Physics 2020-12-02 Manfred Lindner , Yann Mambrini , Tessio B. de Melo , Farinaldo S. Queiroz

The quest for the particle nature of dark matter is one of the big open questions of modern physics. A well motivated candidate for dark matter is the so-called WIMP - a weakly interacting massive particle. Recently several theoretically…

Models of nuclear dark matter propose that the dark sector contains large composite states consisting of dark nucleons in analogy to Standard Model nuclei. We examine the direct detection phenomenology of a particular class of nuclear dark…

High Energy Physics - Phenomenology · Physics 2017-11-01 A. Butcher , R. Kirk , J. Monroe , S. M. West
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