CERN Accelerating science

002826374 001__ 2826374
002826374 005__ 20240905092251.0
002826374 0248_ $$aoai:cds.cern.ch:2826374$$pcerncds:FULLTEXT$$pcerncds:CERN:FULLTEXT$$pcerncds:CERN
002826374 0247_ $$2DOI$$9APS$$a10.1103/PhysRevD.107.112006$$qpublication
002826374 037__ $$9arXiv$$aarXiv:2209.01177$$cphysics.ins-det
002826374 035__ $$9arXiv$$aoai:arXiv.org:2209.01177
002826374 035__ $$9Inspire$$aoai:inspirehep.net:2146298$$d2024-09-04T21:46:50Z$$h2024-09-05T02:30:44Z$$mmarcxml$$ttrue$$uhttps://inspirehep.net/api/oai2d
002826374 035__ $$9Inspire$$a2146298
002826374 041__ $$aeng
002826374 100__ $$aAgnes, P.$$uRoyal Holloway, U. of London$$uTRIUMF$$vDepartment of Physics, Royal Holloway University of London, Egham TW20 0EX, United Kingdom$$vTRIUMF, 4004 Wesbrook Mall, Vancouver, British Columbia V6T 2A3, Canada
002826374 245__ $$9arXiv$$aSensitivity projections for a dual-phase argon TPC optimized for light dark matter searches through the ionization channel
002826374 269__ $$c2022-09-02
002826374 260__ $$c2023-06-01
002826374 300__ $$a19 p
002826374 520__ $$9APS$$aDark matter lighter than <math display="inline"><mrow><mn>10</mn><mtext> </mtext><mtext> </mtext><mi>GeV</mi><mo>/</mo><msup><mi>c</mi><mn>2</mn></msup></mrow></math> encompasses a promising range of candidates. A conceptual design for a new detector, DarkSide-LowMass, is presented, based on the DarkSide-50 detector and progress toward DarkSide-20k, optimized for a low-threshold electron-counting measurement. Sensitivity to light dark matter is explored for various potential energy thresholds and background rates. These studies show that DarkSide-LowMass can achieve sensitivity to light dark matter down to the solar neutrino fog for GeV-scale masses and significant sensitivity down to <math display="inline"><mrow><mn>10</mn><mtext> </mtext><mtext> </mtext><mi>MeV</mi><mo>/</mo><msup><mi>c</mi><mn>2</mn></msup></mrow></math> considering the Migdal effect or interactions with electrons. Requirements for optimizing the detector’s sensitivity are explored, as are potential sensitivity gains from modeling and mitigating spurious electron backgrounds that may dominate the signal at the lowest energies.
002826374 520__ $$9arXiv$$aDark matter lighter than 10 GeV/c$^2$ encompasses a promising range of candidates. A conceptual design for a new detector, DarkSide-LowMass, is presented, based on the DarkSide-50 detector and progress toward DarkSide-20k, optimized for a low-threshold electron-counting measurement. Sensitivity to light dark matter is explored for various potential energy thresholds and background rates. These studies show that DarkSide-LowMass can achieve sensitivity to light dark matter down to the solar neutrino floor for GeV-scale masses and significant sensitivity down to 10 MeV/c$^2$ considering the Migdal effect or interactions with electrons. Requirements for optimizing the detector's sensitivity are explored, as are potential sensitivity gains from modeling and mitigating spurious electron backgrounds that may dominate the signal at the lowest energies.
002826374 540__ $$3preprint$$aarXiv nonexclusive-distrib 1.0$$uhttp://arxiv.org/licenses/nonexclusive-distrib/1.0/
002826374 542__ $$3publication$$dAmerican Physical Society$$f© 2023 American Physical Society$$g2023
002826374 65017 $$2arXiv$$ahep-ex
002826374 65017 $$2SzGeCERN$$aParticle Physics - Experiment
002826374 65017 $$2arXiv$$aphysics.ins-det
002826374 65017 $$2SzGeCERN$$aDetectors and Experimental Techniques
002826374 690C_ $$aCERN
002826374 690C_ $$aARTICLE
002826374 700__ $$aAhmad, I.$$uWarsaw, Copernicus Astron. Ctr.$$vAstroCeNT, Nicolaus Copernicus Astronomical Center of the Polish Academy of Sciences, 00-614 Warsaw, Poland
002826374 700__ $$aAlbergo, S.$$uMessina U.$$uINFN, Catania$$uCatania U.$$vUniversità of Catania, Catania 95124, Italy$$vINFN Catania, Catania 95121, Italy
002826374 700__ $$aAlbuquerque, I.F.M.$$uSao Paulo U.$$vInstituto de Física, Universidade de São Paulo, São Paulo 05508-090, Brazil
002826374 700__ $$aAlexander, T.$$uPNL, Richland$$vPacific Northwest National Laboratory, Richland, Washington 99352, USA
002826374 700__ $$aAlton, A.K.$$uWisconsin U., River Falls$$vPhysics Department, Augustana University, Sioux Falls, South Dakota 57197, USA
002826374 700__ $$aAmaudruz, P.$$uTRIUMF$$vTRIUMF, 4004 Wesbrook Mall, Vancouver, British Columbia V6T 2A3, Canada
002826374 700__ $$aAtzori Corona, M.$$uCagliari U.$$uINFN, Cagliari$$vPhysics Department, Università degli Studi di Cagliari, Cagliari 09042, Italy$$vINFN Cagliari, Cagliari 09042, Italy
002826374 700__ $$aAuty, D.J.$$uAlberta U.$$vDepartment of Physics, University of Alberta, Edmonton, Alberta T6G 2R3, Canada
002826374 700__ $$aAve, M.$$uSao Paulo U.$$vInstituto de Física, Universidade de São Paulo, São Paulo 05508-090, Brazil
002826374 700__ $$aAvetisov, I.Ch.$$uLomonosov Inst. Fine Chem. Tech.$$vMendeleev University of Chemical Technology, Moscow 125047, Russia
002826374 700__ $$aAvetisov, R.I.$$uLomonosov Inst. Fine Chem. Tech.$$vMendeleev University of Chemical Technology, Moscow 125047, Russia
002826374 700__ $$aAzzolini, O.$$uINFN, Legnaro$$vINFN Laboratori Nazionali di Legnaro, Legnaro (Padova) 35020, Italy
002826374 700__ $$aBack, H.O.$$uPNL, Richland$$vPacific Northwest National Laboratory, Richland, Washington 99352, USA
002826374 700__ $$aBalmforth, Z.$$uRoyal Holloway, U. of London$$vDepartment of Physics, Royal Holloway University of London, Egham TW20 0EX, United Kingdom
002826374 700__ $$aBarbarian, V.$$uSINP, Moscow$$vSkobeltsyn Institute of Nuclear Physics, Lomonosov Moscow State University, Moscow 119234, Russia
002826374 700__ $$aBarrado Olmedo, A.$$uMadrid, CIEMAT$$vCIEMAT, Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas, Madrid 28040, Spain
002826374 700__ $$aBarrillon, P.$$uMarseille, CPPM$$vCentre de Physique des Particules de Marseille, Aix Marseille Univ, CNRS/IN2P3, CPPM, Marseille, France
002826374 700__ $$aBasco, A.$$uINFN, Naples$$vINFN Napoli, Napoli 80126, Italy
002826374 700__ $$aBatignani, G.$$uINFN, Pisa$$uPisa U.$$vPhysics Department, Università degli Studi di Pisa, Pisa 56127, Italy$$vINFN Pisa, Pisa 56127, Italy
002826374 700__ $$aBerzin, E.$$uPrinceton U.$$vPhysics Department, Princeton University, Princeton, New Jersey 08544, USA
002826374 700__ $$aBondar, A.$$uNovosibirsk, IYF$$uNovosibirsk State U.$$vBudker Institute of Nuclear Physics, Novosibirsk 630090, Russia$$vNovosibirsk State University, Novosibirsk 630090, Russia
002826374 700__ $$aBonivento, W.M.$$uCagliari U.$$uINFN, Cagliari$$vINFN Cagliari, Cagliari 09042, Italy
002826374 700__ $$aBorisova, E.$$uNovosibirsk, IYF$$uNovosibirsk State U.$$vBudker Institute of Nuclear Physics, Novosibirsk 630090, Russia$$vNovosibirsk State University, Novosibirsk 630090, Russia
002826374 700__ $$aBottino, B.$$uINFN, Genoa$$uGenoa U.$$vPhysics Department, Università degli Studi di Genova, Genova 16146, Italy$$vINFN Genova, Genova 16146, Italy
002826374 700__ $$aBoulay, M.G.$$uCarleton U.$$vDepartment of Physics, Carleton University, Ottawa, Ontario K1S 5B6, Canada
002826374 700__ $$aBuccino, G.$$uGran Sasso$$vINFN Laboratori Nazionali del Gran Sasso, Assergi (AQ) 67100, Italy
002826374 700__ $$aBussino, S.$$uRome III U.$$uINFN, Rome3$$vMathematics and Physics Department, Università degli Studi Roma Tre, Roma 00146, Italy$$vINFN Roma Tre, Roma 00146, Italy
002826374 700__ $$aBusto, J.$$uMarseille, CPPM$$vCentre de Physique des Particules de Marseille, Aix Marseille Univ, CNRS/IN2P3, CPPM, Marseille, France
002826374 700__ $$aBuzulutskov, A.$$uNovosibirsk, IYF$$uNovosibirsk State U.$$vBudker Institute of Nuclear Physics, Novosibirsk 630090, Russia$$vNovosibirsk State University, Novosibirsk 630090, Russia
002826374 700__ $$aCadeddu, M.$$uCagliari U.$$uINFN, Cagliari$$vINFN Cagliari, Cagliari 09042, Italy
002826374 700__ $$aCadoni, M.$$uCagliari U.$$uINFN, Cagliari$$vPhysics Department, Università degli Studi di Cagliari, Cagliari 09042, Italy$$vINFN Cagliari, Cagliari 09042, Italy
002826374 700__ $$aCaminata, A.$$uINFN, Genoa$$vINFN Genova, Genova 16146, Italy
002826374 700__ $$aCanci, N.$$uINFN, Naples$$vINFN Napoli, Napoli 80126, Italy
002826374 700__ $$aCapra, A.$$uTRIUMF$$vTRIUMF, 4004 Wesbrook Mall, Vancouver, British Columbia V6T 2A3, Canada
002826374 700__ $$aCaprioli, S.$$uINFN, Genoa$$vINFN Genova, Genova 16146, Italy
002826374 700__ $$aCaravati, M.$$uCagliari U.$$uINFN, Cagliari$$vINFN Cagliari, Cagliari 09042, Italy
002826374 700__ $$aCárdenas-Montes, M.$$uMadrid, CIEMAT$$vCIEMAT, Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas, Madrid 28040, Spain
002826374 700__ $$aCargioli, N.$$uCagliari U.$$uINFN, Cagliari$$vPhysics Department, Università degli Studi di Cagliari, Cagliari 09042, Italy$$vINFN Cagliari, Cagliari 09042, Italy
002826374 700__ $$aCarlini, M.$$uGran Sasso$$vINFN Laboratori Nazionali del Gran Sasso, Assergi (AQ) 67100, Italy
002826374 700__ $$aCastello, P.$$uCagliari U.$$uINFN, Cagliari$$vDepartment of Electrical and Electronic Engineering, Università degli Studi di Cagliari, Cagliari 09123, Italy$$vINFN Cagliari, Cagliari 09042, Italy
002826374 700__ $$aCataudella, V.$$uNaples U.$$uINFN, Naples$$vINFN Napoli, Napoli 80126, Italy$$vPhysics Department, Università degli Studi “Federico II” di Napoli, Napoli 80126, Italy
002826374 700__ $$aCavalcante, P.$$uGran Sasso$$vINFN Laboratori Nazionali del Gran Sasso, Assergi (AQ) 67100, Italy
002826374 700__ $$aCavuoti, S.$$uNaples U.$$uINFN, Naples$$uCapodimonte Observ.$$vINFN Napoli, Napoli 80126, Italy$$vPhysics Department, Università degli Studi “Federico II” di Napoli, Napoli 80126, Italy$$vINAF Osservatorio Astronomico di Capodimonte, 80131 Napoli, Italy
002826374 700__ $$aCebrian, S.$$uZaragoza U.$$vCentro de Astropartículas y Física de Altas Energías, Universidad de Zaragoza, Zaragoza 50009, Spain
002826374 700__ $$aCela Ruiz, J.M.$$uMadrid, CIEMAT$$vCIEMAT, Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas, Madrid 28040, Spain
002826374 700__ $$aChashin, S.$$uSINP, Moscow$$vSkobeltsyn Institute of Nuclear Physics, Lomonosov Moscow State University, Moscow 119234, Russia
002826374 700__ $$aChepurnov, A.$$uSINP, Moscow$$vSkobeltsyn Institute of Nuclear Physics, Lomonosov Moscow State University, Moscow 119234, Russia
002826374 700__ $$aChyhyrynets, E.$$uINFN, Legnaro$$vINFN Laboratori Nazionali di Legnaro, Legnaro (Padova) 35020, Italy
002826374 700__ $$aCicalò, C.$$uCagliari U.$$uINFN, Cagliari$$vINFN Cagliari, Cagliari 09042, Italy
002826374 700__ $$aCifarelli, L.$$uPurdue U.$$uBologna U.$$uINFN, Bologna$$vDepartment of Physics and Astronomy, Università degli Studi di Bologna, Bologna 40126, Italy$$vINFN Bologna, Bologna 40126, Italy
002826374 700__ $$aCintas, D.$$uZaragoza U.$$vCentro de Astropartículas y Física de Altas Energías, Universidad de Zaragoza, Zaragoza 50009, Spain
002826374 700__ $$aCocco, V.$$uCagliari U.$$uINFN, Cagliari$$vINFN Cagliari, Cagliari 09042, Italy
002826374 700__ $$aConde Vilda, E.$$uMadrid, CIEMAT$$vCIEMAT, Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas, Madrid 28040, Spain
002826374 700__ $$aConsiglio, L.$$uGran Sasso$$vINFN Laboratori Nazionali del Gran Sasso, Assergi (AQ) 67100, Italy
002826374 700__ $$aCopello, S.$$uINFN, Genoa$$uGenoa U.$$vPhysics Department, Università degli Studi di Genova, Genova 16146, Italy$$vINFN Genova, Genova 16146, Italy
002826374 700__ $$aCovone, G.$$uNaples U.$$uINFN, Naples$$vINFN Napoli, Napoli 80126, Italy$$vPhysics Department, Università degli Studi “Federico II” di Napoli, Napoli 80126, Italy
002826374 700__ $$aCross, S.$$uRutherford$$vScience & Technology Facilities Council (STFC), Rutherford Appleton Laboratory, Technology, Harwell Oxford, Didcot OX11 0QX, United Kingdom
002826374 700__ $$aCzubak, M.$$uJagiellonian U.$$vM. Smoluchowski Institute of Physics, Jagiellonian University, 30-348 Krakow, Poland
002826374 700__ $$aCzudak, P.$$uJagiellonian U.$$vM. Smoluchowski Institute of Physics,Jagiellonian University,30-348 Krakow,Poland
002826374 700__ $$aD'Aniello, M.$$uNaples U.$$uINFN, Naples$$vDepartment of Strutture per l’Ingegneria e l’Architettura, Università degli Studi “Federico II” di Napoli, Napoli 80131, Italy
002826374 700__ $$aD'Auria, S.$$uINFN, Milan$$vINFN Milano, Milano 20133, Italy
002826374 700__ $$aDa Rocha Rolo, M.D.$$uINFN, Turin$$vINFN Torino, Torino 10125, Italy
002826374 700__ $$aDadoun, O.$$uParis U., VI-VII$$vLPNHE, CNRS/IN2P3, Sorbonne Université, Université Paris Diderot, Paris 75252, France
002826374 700__ $$aDaniel, M.$$uMadrid, CIEMAT$$vCIEMAT, Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas, Madrid 28040, Spain
002826374 700__ $$aDavini, S.$$uINFN, Genoa$$vINFN Genova, Genova 16146, Italy
002826374 700__ $$aDe Candia, A.$$uNaples U.$$uINFN, Naples$$vINFN Napoli, Napoli 80126, Italy$$vPhysics Department, Università degli Studi “Federico II” di Napoli, Napoli 80126, Italy
002826374 700__ $$aDe Cecco, S.$$uINFN, Rome$$uRome U.$$vPhysics Department, Sapienza Università di Roma, Roma 00185, Italy$$vINFN Sezione di Roma, Roma 00185, Italy
002826374 700__ $$aDe Falco, A.$$uCagliari U.$$uINFN, Cagliari$$vPhysics Department, Università degli Studi di Cagliari, Cagliari 09042, Italy$$vINFN Cagliari, Cagliari 09042, Italy
002826374 700__ $$aDe Filippis, G.$$uNaples U.$$uINFN, Naples$$vINFN Napoli, Napoli 80126, Italy$$vPhysics Department, Università degli Studi “Federico II” di Napoli, Napoli 80126, Italy
002826374 700__ $$aDe Gruttola, D.$$uINFN, Naples$$uSalerno U.$$uINFN, Salerno$$vINFN Salerno, Salerno 84084, Italy$$vPhysics Department, Università degli Studi di Salerno, Salerno 84084, Italy
002826374 700__ $$aDe Pasquale, S.$$uINFN, Naples$$uSalerno U.$$uINFN, Salerno$$vINFN Salerno, Salerno 84084, Italy$$vPhysics Department, Università degli Studi di Salerno, Salerno 84084, Italy
002826374 700__ $$aDe Rosa, G.$$uNaples U.$$uINFN, Naples$$vINFN Napoli, Napoli 80126, Italy$$vPhysics Department, Università degli Studi “Federico II” di Napoli, Napoli 80126, Italy
002826374 700__ $$aDellacasa, G.$$uINFN, Turin$$vINFN Torino, Torino 10125, Italy
002826374 700__ $$aDerbin, A.V.$$uSt. Petersburg, INP$$vSaint Petersburg Nuclear Physics Institute, Gatchina 188350, Russia
002826374 700__ $$aDevoto, A.$$uCagliari U.$$uINFN, Cagliari$$vPhysics Department, Università degli Studi di Cagliari, Cagliari 09042, Italy$$vINFN Cagliari, Cagliari 09042, Italy
002826374 700__ $$aDi Capua, F.$$uNaples U.$$uINFN, Naples$$vINFN Napoli, Napoli 80126, Italy$$vPhysics Department, Università degli Studi “Federico II” di Napoli, Napoli 80126, Italy
002826374 700__ $$aDi Noto, L.$$uINFN, Genoa$$vINFN Genova, Genova 16146, Italy
002826374 700__ $$aDi Stefano, P.$$uQueen's U., Kingston$$vDepartment of Physics, Engineering Physics and Astronomy, Queen’s University, Kingston, Ontario K7L 3N6, Canada
002826374 700__ $$aDionisi, C.$$uINFN, Rome$$uRome U.$$vPhysics Department, Sapienza Università di Roma, Roma 00185, Italy$$vINFN Sezione di Roma, Roma 00185, Italy
002826374 700__ $$aDolganov, G.$$uKurchatov Inst., Moscow$$vNational Research Centre Kurchatov Institute, Moscow 123182, Russia
002826374 700__ $$aDordei, F.$$uCagliari U.$$uINFN, Cagliari$$vINFN Cagliari, Cagliari 09042, Italy
002826374 700__ $$aDoria, L.$$uMainz U., Inst. Kernphys.$$vInstitut für Kernphysik, Johannes Gutenberg-Universität Mainz, D-55128 Mainz, Germany
002826374 700__ $$aErjavec, T.$$uUC, Davis$$vDepartment of Physics, University of California, Davis, California 95616, USA
002826374 700__ $$aFernandez Diaz, M.$$uMadrid, CIEMAT$$vCIEMAT, Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas, Madrid 28040, Spain
002826374 700__ $$aFiorillo, G.$$uNaples U.$$uINFN, Naples$$vINFN Napoli, Napoli 80126, Italy$$vPhysics Department, Università degli Studi “Federico II” di Napoli, Napoli 80126, Italy
002826374 700__ $$aFranceschi, A.$$uFrascati$$vINFN Laboratori Nazionali di Frascati, Frascati 00044, Italy
002826374 700__ $$aFranchini, P.$$uLancaster U.$$uRoyal Holloway, U. of London$$vPhysics Department, Lancaster University, Lancaster LA1 4YB, United Kingdom$$vDepartment of Physics, Royal Holloway University of London, Egham TW20 0EX, United Kingdom
002826374 700__ $$aFranco, D.$$uAPC, Paris$$vAPC, Université de Paris, CNRS, Astroparticule et Cosmologie, Paris F-75013, France
002826374 700__ $$aFrolov, E.$$uNovosibirsk, IYF$$uNovosibirsk State U.$$vBudker Institute of Nuclear Physics, Novosibirsk 630090, Russia$$vNovosibirsk State University, Novosibirsk 630090, Russia
002826374 700__ $$aFunicello, N.$$uINFN, Naples$$uSalerno U.$$uINFN, Salerno$$vINFN Salerno, Salerno 84084, Italy$$vPhysics Department, Università degli Studi di Salerno, Salerno 84084, Italy
002826374 700__ $$aGabriele, F.$$uCagliari U.$$uINFN, Cagliari$$vINFN Cagliari, Cagliari 09042, Italy
002826374 700__ $$aGahan, D.$$uCagliari U.$$uINFN, Cagliari$$vPhysics Department, Università degli Studi di Cagliari, Cagliari 09042, Italy$$vINFN Cagliari, Cagliari 09042, Italy
002826374 700__ $$aGalbiati, C.$$uPrinceton U.$$uGran Sasso$$uINFN, Aquila$$uRome U., Tor Vergata$$vPhysics Department, Princeton University, Princeton, New Jersey 08544, USA$$vGran Sasso Science Institute, L’Aquila 67100, Italy$$vINFN Laboratori Nazionali del Gran Sasso, Assergi (AQ) 67100, Italy
002826374 700__ $$aGallina, G.$$uPrinceton U.$$vPhysics Department, Princeton University, Princeton, New Jersey 08544, USA
002826374 700__ $$aGallus, G.$$uCagliari U.$$uINFN, Cagliari$$vDepartment of Electrical and Electronic Engineering, Università degli Studi di Cagliari, Cagliari 09123, Italy$$vINFN Cagliari, Cagliari 09042, Italy
002826374 700__ $$aGarbini, M.$$uEnrico Fermi Ctr., Rome$$uINFN, Bologna$$vMuseo Storico della Fisica e Centro Studi e Ricerche Enrico Fermi, Roma 00184, Italy$$vINFN Bologna, Bologna 40126, Italy
002826374 700__ $$aGarcia Abia, P.$$uMadrid, CIEMAT$$vCIEMAT, Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas, Madrid 28040, Spain
002826374 700__ $$aGendotti, A.$$uZurich, ETH$$vInstitute for Particle Physics, ETH Zürich, Zürich 8093, Switzerland
002826374 700__ $$aGhiano, C.$$uGran Sasso$$vINFN Laboratori Nazionali del Gran Sasso, Assergi (AQ) 67100, Italy
002826374 700__ $$aGiampaolo, R.A.$$uINFN, Turin$$uINFN, Aquila$$uRome U., Tor Vergata$$vINFN Torino, Torino 10125, Italy$$vGran Sasso Science Institute, L’Aquila 67100, Italy
002826374 700__ $$aGiganti, C.$$uParis U., VI-VII$$vLPNHE, CNRS/IN2P3, Sorbonne Université, Université Paris Diderot, Paris 75252, France
002826374 700__ $$aGiorgi, M.A.$$uPisa U.$$uINFN, Pisa$$vPhysics Department, Università degli Studi di Pisa, Pisa 56127, Italy$$vINFN Pisa, Pisa 56127, Italy
002826374 700__ $$aGiovanetti, G.K.$$uWilliams Coll.$$vWilliams College, Physics Department, Williamstown, Massachusetts 01267 USA
002826374 700__ $$aGoicoechea Casanueva, V.$$uHawaii U.$$vDepartment of Physics and Astronomy, University of Hawai’i, Honolulu, Hawaii 96822, USA
002826374 700__ $$aGola, A.$$uFond. Bruno Kessler, Trento$$uTrento U.$$vTrento Institute for Fundamental Physics and Applications, Povo 38123, Italy$$vFondazione Bruno Kessler, Povo 38123, Italy
002826374 700__ $$aGorman, D.$$uRutherford$$vScience & Technology Facilities Council (STFC), Rutherford Appleton Laboratory, Technology, Harwell Oxford, Didcot OX11 0QX, United Kingdom
002826374 700__ $$aGraciani Diaz, R.$$uBarcelona U.$$vUniversiatat de Barcelona, Barcelona E-08028, Catalonia, Spain
002826374 700__ $$aGrauso, G.$$uINFN, Naples$$vINFN Napoli, Napoli 80126, Italy
002826374 700__ $$aGrilli di Cortona, G.$$uFrascati$$vINFN Laboratori Nazionali di Frascati, Frascati 00044, Italy
002826374 700__ $$aGrobov, A.$$uKurchatov Inst., Moscow$$uMoscow Phys. Eng. Inst.$$vNational Research Centre Kurchatov Institute, Moscow 123182, Russia$$vNational Research Nuclear University MEPhI, Moscow 115409, Russia
002826374 700__ $$aGromov, M.$$uSINP, Moscow$$uDubna, JINR$$vSkobeltsyn Institute of Nuclear Physics, Lomonosov Moscow State University, Moscow 119234, Russia$$vJoint Institute for Nuclear Research, Dubna 141980, Russia
002826374 700__ $$aGuan, M.$$uBeijing, Inst. High Energy Phys.$$vInstitute of High Energy Physics, Beijing 100049, China
002826374 700__ $$aGuerzoni, M.$$uINFN, Bologna$$vINFN Bologna, Bologna 40126, Italy
002826374 700__ $$aGulino, M.$$uSplit Tech. U.$$uINFN, LNS$$vEngineering and Architecture Faculty, Università di Enna Kore, Enna 94100, Italy$$vINFN Laboratori Nazionali del Sud, Catania 95123, Italy
002826374 700__ $$aGuo, C.$$uBeijing, Inst. High Energy Phys.$$vInstitute of High Energy Physics, Beijing 100049, China
002826374 700__ $$aHackett, B.R.$$uPNL, Richland$$vPacific Northwest National Laboratory, Richland, Washington 99352, USA
002826374 700__ $$aHall, J.B.$$uPrinceton U.$$vPhysics Department, Princeton University, Princeton, New Jersey 08544, USA
002826374 700__ $$aHallin, A.L.$$uAlberta U.$$vDepartment of Physics, University of Alberta, Edmonton, Alberta T6G 2R3, Canada
002826374 700__ $$aHamer, A.$$uU. Edinburgh$$uRoyal Holloway, U. of London$$vDepartment of Physics, Royal Holloway University of London, Egham TW20 0EX, United Kingdom$$vSchool of Physics and Astronomy, University of Edinburgh, Edinburgh EH9 3FD, United Kingdom
002826374 700__ $$aHelton, H.$$uPrinceton U.$$vPhysics Department, Princeton University, Princeton, New Jersey 08544, USA
002826374 700__ $$aHaranczyk, M.$$uJagiellonian U.$$vM. Smoluchowski Institute of Physics, Jagiellonian University, 30-348 Krakow, Poland
002826374 700__ $$aHessel, T.$$uAPC, Paris$$vAPC, Université de Paris, CNRS, Astroparticule et Cosmologie, Paris F-75013, France
002826374 700__ $$aHill, S.$$uRoyal Holloway, U. of London$$vDepartment of Physics, Royal Holloway University of London, Egham TW20 0EX, United Kingdom
002826374 700__ $$aHorikawa, S.$$uINFN, Aquila$$uL'Aquila U.$$uGran Sasso$$vUniversità degli Studi dell’Aquila, L’Aquila 67100, Italy$$vINFN Laboratori Nazionali del Gran Sasso, Assergi (AQ) 67100, Italy
002826374 700__ $$aHubaut, F.$$uMarseille, CPPM$$vCentre de Physique des Particules de Marseille, Aix Marseille Univ, CNRS/IN2P3, CPPM, Marseille, France
002826374 700__ $$aHugues, T.$$uWarsaw, Copernicus Astron. Ctr.$$vAstroCeNT, Nicolaus Copernicus Astronomical Center of the Polish Academy of Sciences, 00-614 Warsaw, Poland
002826374 700__ $$aHungerford, E.V.$$uHouston U.$$vDepartment of Physics, University of Houston, Houston, Texas 77204, USA
002826374 700__ $$aIanni, An.$$uPrinceton U.$$uGran Sasso$$vPhysics Department, Princeton University, Princeton, New Jersey 08544, USA$$vINFN Laboratori Nazionali del Gran Sasso, Assergi (AQ) 67100, Italy
002826374 700__ $$aIppolito, V.$$uINFN, Rome$$vINFN Sezione di Roma, Roma 00185, Italy
002826374 700__ $$aJillings, C.$$uSNOLAB, Lively$$uLaurentian U.$$vSNOLAB, Lively, Ontario P3Y 1N2, Canada$$vDepartment of Physics and Astronomy, Laurentian University, Sudbury, Ontario P3E 2C6, Canada
002826374 700__ $$aKachru, P.$$uINFN, Aquila$$uRome U., Tor Vergata$$uGran Sasso$$vGran Sasso Science Institute, L’Aquila 67100, Italy$$vINFN Laboratori Nazionali del Gran Sasso, Assergi (AQ) 67100, Italy
002826374 700__ $$aKemp, A.A.$$uQueen's U., Kingston$$vDepartment of Physics, Engineering Physics and Astronomy, Queen’s University, Kingston, Ontario K7L 3N6, Canada
002826374 700__ $$aKendziora, C.L.$$uFermilab$$vFermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
002826374 700__ $$aKeppel, G.$$uINFN, Legnaro$$vINFN Laboratori Nazionali di Legnaro, Legnaro (Padova) 35020, Italy
002826374 700__ $$aKhomyakov, A.V.$$uLomonosov Inst. Fine Chem. Tech.$$vMendeleev University of Chemical Technology, Moscow 125047, Russia
002826374 700__ $$aKimura, M.$$uWarsaw, Copernicus Astron. Ctr.$$vAstroCeNT, Nicolaus Copernicus Astronomical Center of the Polish Academy of Sciences, 00-614 Warsaw, Poland
002826374 700__ $$aKochanek, I.$$uGran Sasso$$vINFN Laboratori Nazionali del Gran Sasso, Assergi (AQ) 67100, Italy
002826374 700__ $$aKondo, K.$$uGran Sasso$$vINFN Laboratori Nazionali del Gran Sasso, Assergi (AQ) 67100, Italy
002826374 700__ $$aKorga, G.$$uRoyal Holloway, U. of London$$vDepartment of Physics, Royal Holloway University of London, Egham TW20 0EX, United Kingdom
002826374 700__ $$aKoulosousas, S.$$uRoyal Holloway, U. of London$$vDepartment of Physics, Royal Holloway University of London, Egham TW20 0EX, United Kingdom
002826374 700__ $$aKubankin, A.$$uBelgorod State U.$$vRadiation Physics Laboratory, Belgorod National Research University, Belgorod 308007, Russia
002826374 700__ $$aKuss, M.$$uINFN, Pisa$$vINFN Pisa, Pisa 56127, Italy
002826374 700__ $$aKuźniak, M.$$uWarsaw, Copernicus Astron. Ctr.$$vAstroCeNT, Nicolaus Copernicus Astronomical Center of the Polish Academy of Sciences, 00-614 Warsaw, Poland
002826374 700__ $$aLa Commara, M.$$uNaples U.$$uINFN, Naples$$vINFN Napoli, Napoli 80126, Italy$$vPharmacy Department, Università degli Studi “Federico II” di Napoli, Napoli 80131, Italy
002826374 700__ $$aLai, M.$$uCagliari U.$$uINFN, Cagliari$$vPhysics Department, Università degli Studi di Cagliari, Cagliari 09042, Italy$$vINFN Cagliari, Cagliari 09042, Italy
002826374 700__ $$aLe Guirriec, E.$$uMarseille, CPPM$$vCentre de Physique des Particules de Marseille, Aix Marseille Univ, CNRS/IN2P3, CPPM, Marseille, France
002826374 700__ $$aLeason, E.$$uRoyal Holloway, U. of London$$vDepartment of Physics, Royal Holloway University of London, Egham TW20 0EX, United Kingdom
002826374 700__ $$aLi, X.$$uPrinceton U.$$vPhysics Department, Princeton University, Princeton, New Jersey 08544, USA
002826374 700__ $$aLidey, L.$$uPNL, Richland$$vPacific Northwest National Laboratory, Richland, Washington 99352, USA
002826374 700__ $$aLipp, J.$$uRutherford$$vScience & Technology Facilities Council (STFC), Rutherford Appleton Laboratory, Technology, Harwell Oxford, Didcot OX11 0QX, United Kingdom
002826374 700__ $$aLissia, M.$$uCagliari U.$$uINFN, Cagliari$$vINFN Cagliari, Cagliari 09042, Italy
002826374 700__ $$aLongo, G.$$uNaples U.$$uINFN, Naples$$vINFN Napoli, Napoli 80126, Italy$$vPhysics Department, Università degli Studi “Federico II” di Napoli, Napoli 80126, Italy
002826374 700__ $$aLuzzi, L.$$uMadrid, CIEMAT$$vCIEMAT, Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas, Madrid 28040, Spain
002826374 700__ $$aMacfadyen, O.$$uRoyal Holloway, U. of London$$vDepartment of Physics, Royal Holloway University of London, Egham TW20 0EX, United Kingdom
002826374 700__ $$aMachulin, I.N.$$uKurchatov Inst., Moscow$$uMoscow Phys. Eng. Inst.$$vNational Research Centre Kurchatov Institute, Moscow 123182, Russia$$vNational Research Nuclear University MEPhI, Moscow 115409, Russia
002826374 700__ $$aManthos, I.$$uBirmingham U.$$vSchool of Physics and Astronomy, University of Birmingham, Edgbaston, B15 2TT, Birmingham, United Kingdom
002826374 700__ $$aMapelli, L.$$uPrinceton U.$$vPhysics Department, Princeton University, Princeton, New Jersey 08544, USA
002826374 700__ $$aMargotti, A.$$uINFN, Bologna$$vINFN Bologna, Bologna 40126, Italy
002826374 700__ $$aMari, S.M.$$uRome III U.$$uINFN, Rome3$$vMathematics and Physics Department, Università degli Studi Roma Tre, Roma 00146, Italy$$vINFN Roma Tre, Roma 00146, Italy
002826374 700__ $$aMariani, C.$$uVirginia Tech.$$vVirginia Tech, Blacksburg, Virginia 24061, USA
002826374 700__ $$aMaricic, J.$$uHawaii U.$$vDepartment of Physics and Astronomy, University of Hawai’i, Honolulu, Hawaii 96822, USA
002826374 700__ $$aMarini, A.$$uINFN, Genoa$$uGenoa U.$$vPhysics Department, Università degli Studi di Genova, Genova 16146, Italy$$vINFN Genova, Genova 16146, Italy
002826374 700__ $$aMartínez, M.$$uZaragoza U.$$uARAID, Zaragoza$$vCentro de Astropartículas y Física de Altas Energías, Universidad de Zaragoza, Zaragoza 50009, Spain$$vFundación ARAID, Universidad de Zaragoza, Zaragoza 50009, Spain
002826374 700__ $$aMartoff, C.J.$$uTemple U.$$vDepartment of Physics, University of Liverpool, The Oliver Lodge Laboratory, Liverpool L69 7ZE, United Kingdom
002826374 700__ $$aMasoni, A.$$uCagliari U.$$uINFN, Cagliari$$vINFN Cagliari, Cagliari 09042, Italy
002826374 700__ $$aMavrokoridis, K.$$uLiverpool U.$$vDepartment of Physics, University of Liverpool, The Oliver Lodge Laboratory, Liverpool L69 7ZE, United Kingdom
002826374 700__ $$aMazzi, A.$$uFond. Bruno Kessler, Trento$$uTrento U.$$vTrento Institute for Fundamental Physics and Applications, Povo 38123, Italy$$vFondazione Bruno Kessler, Povo 38123, Italy
002826374 700__ $$aMcDonald, A.B.$$uQueen's U., Kingston$$vDepartment of Physics, Engineering Physics and Astronomy, Queen’s University, Kingston, Ontario K7L 3N6, Canada
002826374 700__ $$aMessina, A.$$uINFN, Rome$$uRome U.$$vPhysics Department, Sapienza Università di Roma, Roma 00185, Italy$$vINFN Sezione di Roma, Roma 00185, Italy
002826374 700__ $$aMilincic, R.$$uHawaii U.$$vDepartment of Physics and Astronomy, University of Hawai’i, Honolulu, Hawaii 96822, USA
002826374 700__ $$aMoggi, A.$$uINFN, Pisa$$vINFN Pisa, Pisa 56127, Italy
002826374 700__ $$aMoharana, A.$$uINFN, Aquila$$uRome U., Tor Vergata$$uGran Sasso$$vGran Sasso Science Institute, L’Aquila 67100, Italy$$vINFN Laboratori Nazionali del Gran Sasso, Assergi (AQ) 67100, Italy
002826374 700__ $$aMonroe, J.$$uRoyal Holloway, U. of London$$vDepartment of Physics, Royal Holloway University of London, Egham TW20 0EX, United Kingdom
002826374 700__ $$aMorrocchi, M.$$uINFN, Pisa$$uPisa U.$$vPhysics Department, Università degli Studi di Pisa, Pisa 56127, Italy$$vINFN Pisa, Pisa 56127, Italy
002826374 700__ $$aMozhevitina, E.N.$$uLomonosov Inst. Fine Chem. Tech.$$vMendeleev University of Chemical Technology, Moscow 125047, Russia
002826374 700__ $$aMróz, T.$$uJagiellonian U.$$vM. Smoluchowski Institute of Physics, Jagiellonian University, 30-348 Krakow, Poland
002826374 700__ $$aMuratova, V.N.$$uSt. Petersburg, INP$$vSaint Petersburg Nuclear Physics Institute, Gatchina 188350, Russia
002826374 700__ $$aMuscas, C.$$uCagliari U.$$uINFN, Cagliari$$vDepartment of Electrical and Electronic Engineering, Università degli Studi di Cagliari, Cagliari 09123, Italy$$vINFN Cagliari, Cagliari 09042, Italy
002826374 700__ $$aMusico, P.$$uINFN, Genoa$$vINFN Genova, Genova 16146, Italy
002826374 700__ $$aNania, R.$$uINFN, Bologna$$vINFN Bologna, Bologna 40126, Italy
002826374 700__ $$aNapolitano, T.$$uFrascati$$vINFN Laboratori Nazionali di Frascati, Frascati 00044, Italy
002826374 700__ $$aNessi, M.$$uCERN$$vCERN, European Organization for Nuclear Research 1211 Geneve 23, Switzerland, CERN
002826374 700__ $$aNieradka, G.$$uWarsaw, Copernicus Astron. Ctr.$$vAstroCeNT, Nicolaus Copernicus Astronomical Center of the Polish Academy of Sciences, 00-614 Warsaw, Poland
002826374 700__ $$aNikolopoulos, K.$$uBirmingham U.$$vSchool of Physics and Astronomy, University of Birmingham, Edgbaston, B15 2TT, Birmingham, United Kingdom
002826374 700__ $$aNikulin, I.$$uBelgorod State U.$$vRadiation Physics Laboratory, Belgorod National Research University, Belgorod 308007, Russia
002826374 700__ $$aNowak, J.$$uLancaster U.$$vPhysics Department, Lancaster University, Lancaster LA1 4YB, United Kingdom
002826374 700__ $$aOlchansky, K.$$uTRIUMF$$vTRIUMF, 4004 Wesbrook Mall, Vancouver, British Columbia V6T 2A3, Canada
002826374 700__ $$aOleinik, A.$$uBelgorod State U.$$vRadiation Physics Laboratory, Belgorod National Research University, Belgorod 308007, Russia
002826374 700__ $$aOleynikov, V.$$uNovosibirsk, IYF$$uNovosibirsk State U.$$vBudker Institute of Nuclear Physics, Novosibirsk 630090, Russia$$vNovosibirsk State University, Novosibirsk 630090, Russia
002826374 700__ $$aOrgantini, P.$$uPrinceton U.$$uGran Sasso$$vPhysics Department, Princeton University, Princeton, New Jersey 08544, USA$$vINFN Laboratori Nazionali del Gran Sasso, Assergi (AQ) 67100, Italy
002826374 700__ $$aOrtiz de Solórzano, A.$$uZaragoza U.$$vCentro de Astropartículas y Física de Altas Energías, Universidad de Zaragoza, Zaragoza 50009, Spain
002826374 700__ $$aPagani, L.$$uUC, Davis$$vDepartment of Physics, University of California, Davis, California 95616, USA
002826374 700__ $$aPallavicini, M.$$uINFN, Genoa$$uGenoa U.$$vPhysics Department, Università degli Studi di Genova, Genova 16146, Italy$$vINFN Genova, Genova 16146, Italy
002826374 700__ $$aPandola, L.$$uINFN, LNS$$vINFN Laboratori Nazionali del Sud, Catania 95123, Italy
002826374 700__ $$aPantic, E.$$uUC, Davis$$vDepartment of Physics, University of California, Davis, California 95616, USA
002826374 700__ $$aPaoloni, E.$$uINFN, Pisa$$uPisa U.$$vPhysics Department, Università degli Studi di Pisa, Pisa 56127, Italy$$vINFN Pisa, Pisa 56127, Italy
002826374 700__ $$aPaternoster, G.$$uFond. Bruno Kessler, Trento$$uTrento U.$$vTrento Institute for Fundamental Physics and Applications, Povo 38123, Italy$$vFondazione Bruno Kessler, Povo 38123, Italy
002826374 700__ $$aPegoraro, P.A.$$uCagliari U.$$uINFN, Cagliari$$vDepartment of Electrical and Electronic Engineering, Università degli Studi di Cagliari, Cagliari 09123, Italy$$vINFN Cagliari, Cagliari 09042, Italy
002826374 700__ $$aPelczar, K.$$uJagiellonian U.$$vM. Smoluchowski Institute of Physics, Jagiellonian University, 30-348 Krakow, Poland
002826374 700__ $$aPellegrino, C.$$uINFN, Bologna$$vINFN Bologna, Bologna 40126, Italy
002826374 700__ $$aPerotti, F.$$uMilan Polytechnic$$uINFN, Milan$$vINFN Milano, Milano 20133, Italy$$vCivil and Environmental Engineering Department, Politecnico di Milano, Milano 20133, Italy
002826374 700__ $$aPesudo, V.$$uMadrid, CIEMAT$$vCIEMAT, Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas, Madrid 28040, Spain
002826374 700__ $$aPiacentini, S.$$uRome U.$$uINFN, Rome$$vPhysics Department, Sapienza Università di Roma, Roma 00185, Italy$$vINFN Sezione di Roma, Roma 00185, Italy
002826374 700__ $$aPietropaolo, F.$$uCERN$$vCERN, European Organization for Nuclear Research 1211 Geneve 23, Switzerland, CERN
002826374 700__ $$aPino, N.$$uMessina U.$$uINFN, Catania$$uCatania U.$$vUniversità of Catania, Catania 95124, Italy$$vINFN Catania, Catania 95121, Italy
002826374 700__ $$aPira, C.$$uINFN, Legnaro$$vINFN Laboratori Nazionali di Legnaro, Legnaro (Padova) 35020, Italy
002826374 700__ $$aPocar, A.$$uMassachusetts U., Amherst$$vAmherst Center for Fundamental Interactions and Physics Department, University of Massachusetts, Amherst, Massachusetts 01003, USA
002826374 700__ $$aPoehlmann, D.M.$$uUC, Davis$$vDepartment of Physics, University of California, Davis, California 95616, USA
002826374 700__ $$aPordes, S.$$uFermilab$$vFermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
002826374 700__ $$aPralavorio, P.$$uMarseille, CPPM$$vCentre de Physique des Particules de Marseille, Aix Marseille Univ, CNRS/IN2P3, CPPM, Marseille, France
002826374 700__ $$aPrice, D.$$uManchester U.$$vDepartment of Physics and Astronomy, The University of Manchester, Manchester M13 9PL, United Kingdom
002826374 700__ $$aRaffaelli, F.$$uINFN, Pisa$$vINFN Pisa, Pisa 56127, Italy
002826374 700__ $$aRagusa, F.$$uINFN, Milan$$uMilan U.$$vPhysics Department, Università degli Studi di Milano, Milano 20133, Italy$$vINFN Milano, Milano 20133, Italy
002826374 700__ $$aRamachers, Y.$$uCoventry U.$$vUniversity of Warwick, Department of Physics, Coventry CV47AL, United Kingdom
002826374 700__ $$aRamirez, A.$$uHouston U.$$vDepartment of Physics, University of Houston, Houston, Texas 77204, USA
002826374 700__ $$aRazeti, M.$$uCagliari U.$$uINFN, Cagliari$$vINFN Cagliari, Cagliari 09042, Italy
002826374 700__ $$aRazeto, A.$$uGran Sasso$$vINFN Laboratori Nazionali del Gran Sasso, Assergi (AQ) 67100, Italy
002826374 700__ $$aRenshaw, A.L.$$uHouston U.$$vDepartment of Physics, University of Houston, Houston, Texas 77204, USA
002826374 700__ $$aRescigno, M.$$uINFN, Rome$$vINFN Sezione di Roma, Roma 00185, Italy
002826374 700__ $$aResnati, F.$$uCERN$$vCERN, European Organization for Nuclear Research 1211 Geneve 23, Switzerland, CERN
002826374 700__ $$aRetiere, F.$$uTRIUMF$$vTRIUMF, 4004 Wesbrook Mall, Vancouver, British Columbia V6T 2A3, Canada
002826374 700__ $$aRignanese, L.P.$$uINFN, Bologna$$uPurdue U.$$uBologna U.$$vDepartment of Physics and Astronomy, Università degli Studi di Bologna, Bologna 40126, Italy$$vINFN Bologna, Bologna 40126, Italy
002826374 700__ $$aRipoli, C.$$uINFN, Salerno$$uSalerno U.$$uINFN, Naples$$vINFN Salerno, Salerno 84084, Italy$$vPhysics Department, Università degli Studi di Salerno, Salerno 84084, Italy
002826374 700__ $$aRivetti, A.$$uINFN, Turin$$vINFN Torino, Torino 10125, Italy
002826374 700__ $$aRoberts, A.$$uLiverpool U.$$vDepartment of Physics, University of Liverpool, The Oliver Lodge Laboratory, Liverpool L69 7ZE, United Kingdom
002826374 700__ $$aRoberts, C.$$uLiverpool U.$$vDepartment of Physics and Astronomy, The University of Manchester, Manchester M13 9PL, United Kingdom
002826374 700__ $$aRode, J.$$uParis U., VI-VII$$uAPC, Paris$$vAPC, Université de Paris, CNRS, Astroparticule et Cosmologie, Paris F-75013, France$$vLPNHE, CNRS/IN2P3, Sorbonne Université, Université Paris Diderot, Paris 75252, France
002826374 700__ $$aRogers, G.$$uBirmingham U.$$vSchool of Physics and Astronomy, University of Birmingham, Edgbaston, B15 2TT, Birmingham, United Kingdom
002826374 700__ $$aRomero, L.$$uMadrid, CIEMAT$$vCIEMAT, Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas, Madrid 28040, Spain
002826374 700__ $$aRossi, M.$$uINFN, Genoa$$uGenoa U.$$vPhysics Department, Università degli Studi di Genova, Genova 16146, Italy$$vINFN Genova, Genova 16146, Italy
002826374 700__ $$aRubbia, A.$$uZurich, ETH$$vInstitute for Particle Physics, ETH Zürich, Zürich 8093, Switzerland
002826374 700__ $$aSadashivajois, S.$$uRoyal Holloway, U. of London$$vDepartment of Physics, Royal Holloway University of London, Egham TW20 0EX, United Kingdom
002826374 700__ $$aSaffold, T.R.$$uWilliams Coll.$$vWilliams College, Physics Department, Williamstown, Massachusetts 01267 USA
002826374 700__ $$aSamoylov, O.$$uDubna, JINR$$vJoint Institute for Nuclear Research, Dubna 141980, Russia
002826374 700__ $$aSandford, E.$$uManchester U.$$vDepartment of Physics and Astronomy, The University of Manchester, Manchester M13 9PL, United Kingdom
002826374 700__ $$aSanfilippo, S.$$uINFN, LNS$$vINFN Laboratori Nazionali del Sud, Catania 95123, Italy
002826374 700__ $$aSantone, D.$$uRoyal Holloway, U. of London$$vDepartment of Physics, Royal Holloway University of London, Egham TW20 0EX, United Kingdom
002826374 700__ $$aSantorelli, R.$$uMadrid, CIEMAT$$vCIEMAT, Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas, Madrid 28040, Spain
002826374 700__ $$aSavarese, C.$$uPrinceton U.$$vPhysics Department, Princeton University, Princeton, New Jersey 08544, USA
002826374 700__ $$aScapparone, E.$$uINFN, Bologna$$vINFN Bologna, Bologna 40126, Italy
002826374 700__ $$aScioli, G.$$uPurdue U.$$uBologna U.$$uINFN, Bologna$$vDepartment of Physics and Astronomy, Università degli Studi di Bologna, Bologna 40126, Italy$$vINFN Bologna, Bologna 40126, Italy
002826374 700__ $$aSemenov, D.A.$$uSt. Petersburg, INP$$vSaint Petersburg Nuclear Physics Institute, Gatchina 188350, Russia
002826374 700__ $$aShchagin, A.$$uBelgorod State U.$$vRadiation Physics Laboratory, Belgorod National Research University, Belgorod 308007, Russia
002826374 700__ $$aSheshukov, A.$$uDubna, JINR$$vJoint Institute for Nuclear Research, Dubna 141980, Russia
002826374 700__ $$aSimeone, M.$$uNaples U.$$uINFN, Naples$$vINFN Napoli, Napoli 80126, Italy$$vChemical, Materials, and Industrial Production Engineering Department, Università degli Studi “Federico II” di Napoli, Napoli 80126, Italy
002826374 700__ $$aSkensved, P.$$uQueen's U., Kingston$$vDepartment of Physics, Engineering Physics and Astronomy, Queen’s University, Kingston, Ontario K7L 3N6, Canada
002826374 700__ $$aSkorokhvatov, M.D.$$uKurchatov Inst., Moscow$$uMoscow Phys. Eng. Inst.$$vNational Research Centre Kurchatov Institute, Moscow 123182, Russia$$vNational Research Nuclear University MEPhI, Moscow 115409, Russia
002826374 700__ $$aSmirnov, O.$$uDubna, JINR$$vJoint Institute for Nuclear Research, Dubna 141980, Russia
002826374 700__ $$aSmirnova, T.$$uKurchatov Inst., Moscow$$vNational Research Centre Kurchatov Institute, Moscow 123182, Russia
002826374 700__ $$aSmith, B.$$uTRIUMF$$vTRIUMF, 4004 Wesbrook Mall, Vancouver, British Columbia V6T 2A3, Canada
002826374 700__ $$aSokolov, A.$$uNovosibirsk, IYF$$uNovosibirsk State U.$$vBudker Institute of Nuclear Physics, Novosibirsk 630090, Russia$$vNovosibirsk State University, Novosibirsk 630090, Russia
002826374 700__ $$aSpangenberg, M.$$uCoventry U.$$vUniversity of Warwick, Department of Physics, Coventry CV47AL, United Kingdom
002826374 700__ $$aStefanizzi, R.$$uCagliari U.$$uINFN, Cagliari$$vPhysics Department, Università degli Studi di Cagliari, Cagliari 09042, Italy$$vINFN Cagliari, Cagliari 09042, Italy
002826374 700__ $$aSteri, A.$$uCagliari U.$$uINFN, Cagliari$$vINFN Cagliari, Cagliari 09042, Italy
002826374 700__ $$aStracka, S.$$uINFN, Pisa$$vINFN Pisa, Pisa 56127, Italy
002826374 700__ $$aStrickland, V.$$uCarleton U.$$vDepartment of Physics, Carleton University, Ottawa, Ontario K1S 5B6, Canada
002826374 700__ $$aStringer, M.$$uQueen's U., Kingston$$vDepartment of Physics, Engineering Physics and Astronomy, Queen’s University, Kingston, Ontario K7L 3N6, Canada
002826374 700__ $$aSulis, S.$$uCagliari U.$$uINFN, Cagliari$$vDepartment of Electrical and Electronic Engineering, Università degli Studi di Cagliari, Cagliari 09123, Italy$$vINFN Cagliari, Cagliari 09042, Italy
002826374 700__ $$aSung, A.$$uPrinceton U.$$vPhysics Department, Princeton University, Princeton, New Jersey 08544, USA
002826374 700__ $$aSuvorov, Y.$$uNaples U.$$uINFN, Naples$$uKurchatov Inst., Moscow$$vNational Research Centre Kurchatov Institute, Moscow 123182, Russia$$vINFN Napoli, Napoli 80126, Italy$$vPhysics Department, Università degli Studi “Federico II” di Napoli, Napoli 80126, Italy
002826374 700__ $$aSzelc, A.M.$$uU. Edinburgh$$vSchool of Physics and Astronomy, University of Edinburgh, Edinburgh EH9 3FD, United Kingdom
002826374 700__ $$aTürkoğ, C.
002826374 700__ $$aTürkoğlu, C.$$uWarsaw, Copernicus Astron. Ctr.$$vAstroCeNT, Nicolaus Copernicus Astronomical Center of the Polish Academy of Sciences, 00-614 Warsaw, Poland
002826374 700__ $$aTartaglia, R.$$uGran Sasso$$vINFN Laboratori Nazionali del Gran Sasso, Assergi (AQ) 67100, Italy
002826374 700__ $$aTaylor, A.$$uLiverpool U.$$vDepartment of Physics, University of Liverpool, The Oliver Lodge Laboratory, Liverpool L69 7ZE, United Kingdom
002826374 700__ $$aTaylor, J.$$uLiverpool U.$$vDepartment of Physics, University of Liverpool, The Oliver Lodge Laboratory, Liverpool L69 7ZE, United Kingdom
002826374 700__ $$aTedesco, S.$$uINFN, Turin$$uPolytech. Turin$$vINFN Torino, Torino 10125, Italy$$vDepartment of Electronics and Communications, Politecnico di Torino, Torino 10129, Italy
002826374 700__ $$aTestera, G.$$uINFN, Genoa$$vINFN Genova, Genova 16146, Italy
002826374 700__ $$aThieme, K.$$uHawaii U.$$vDepartment of Physics and Astronomy, University of Hawai’i, Honolulu, Hawaii 96822, USA
002826374 700__ $$aThorpe, T.N.$$uUCLA$$vPhysics and Astronomy Department, University of California, Los Angeles, California 90095, USA
002826374 700__ $$aTonazzo, A.$$uAPC, Paris$$vAPC, Université de Paris, CNRS, Astroparticule et Cosmologie, Paris F-75013, France
002826374 700__ $$aTorres-Lara, S.$$uHouston U.$$vDepartment of Physics, University of Houston, Houston, Texas 77204, USA
002826374 700__ $$aTricomi, A.$$uMessina U.$$uINFN, Catania$$uCatania U.$$vUniversità of Catania, Catania 95124, Italy$$vINFN Catania, Catania 95121, Italy
002826374 700__ $$aUnzhakov, E.V.$$uSt. Petersburg, INP$$vSaint Petersburg Nuclear Physics Institute, Gatchina 188350, Russia
002826374 700__ $$aVallivilayil John, T.$$uINFN, Aquila$$uRome U., Tor Vergata$$uGran Sasso$$vGran Sasso Science Institute, L’Aquila 67100, Italy$$vINFN Laboratori Nazionali del Gran Sasso, Assergi (AQ) 67100, Italy
002826374 700__ $$aVan Uffelen, M.$$uMarseille, CPPM$$vCentre de Physique des Particules de Marseille, Aix Marseille Univ, CNRS/IN2P3, CPPM, Marseille, France
002826374 700__ $$aViant, T.$$uZurich, ETH$$vInstitute for Particle Physics, ETH Zürich, Zürich 8093, Switzerland
002826374 700__ $$aViel, S.$$uCarleton U.$$vDepartment of Physics, Carleton University, Ottawa, Ontario K1S 5B6, Canada
002826374 700__ $$aVishneva, A.$$uDubna, JINR$$vJoint Institute for Nuclear Research, Dubna 141980, Russia
002826374 700__ $$aVogelaar, R.B.$$uVirginia Tech.$$vVirginia Tech, Blacksburg, Virginia 24061, USA
002826374 700__ $$aVossebeld, J.$$uLiverpool U.$$vDepartment of Physics, University of Liverpool, The Oliver Lodge Laboratory, Liverpool L69 7ZE, United Kingdom
002826374 700__ $$aWada, M.$$uWarsaw, Copernicus Astron. Ctr.$$uCagliari U.$$vPhysics Department, Università degli Studi di Cagliari, Cagliari 09042, Italy$$vAstroCeNT, Nicolaus Copernicus Astronomical Center of the Polish Academy of Sciences, 00-614 Warsaw, Poland
002826374 700__ $$aWalczak, M.B.$$uWarsaw, Copernicus Astron. Ctr.$$vAstroCeNT, Nicolaus Copernicus Astronomical Center of the Polish Academy of Sciences, 00-614 Warsaw, Poland
002826374 700__ $$aWang, Y.$$uBeijing, Inst. High Energy Phys.$$uBeijing, GUCAS$$vUniversity of Chinese Academy of Sciences, Beijing 100049, China$$vInstitute of High Energy Physics, Beijing 100049, China
002826374 700__ $$aWesterdale, S.$$uUC, Riverside$$uPrinceton U.$$vPhysics Department, Princeton University, Princeton, New Jersey 08544, USA$$vDepartment of Physics and Astronomy, University of California, Riverside, California 92507, USA
002826374 700__ $$aWheadon, R.J.$$uINFN, Turin$$vINFN Torino, Torino 10125, Italy
002826374 700__ $$aWilliams, L.$$uLewis - Clark Coll.$$vDepartment of Physics and Engineering, Fort Lewis College, Durango, Colorado 81301, USA
002826374 700__ $$aWingerter-Seez, I.$$uMarseille, CPPM$$vCentre de Physique des Particules de Marseille, Aix Marseille Univ, CNRS/IN2P3, CPPM, Marseille, France
002826374 700__ $$aWojaczyński, R.$$uWarsaw, Copernicus Astron. Ctr.$$vAstroCeNT, Nicolaus Copernicus Astronomical Center of the Polish Academy of Sciences, 00-614 Warsaw, Poland
002826374 700__ $$aWojcik, Ma.M.$$uJagiellonian U.$$vM. Smoluchowski Institute of Physics, Jagiellonian University, 30-348 Krakow, Poland
002826374 700__ $$aWojcik, Ma.$$uLodz, Tech. U.$$vInstitute of Applied Radiation Chemistry, Lodz University of Technology, 93-590 Lodz, Poland
002826374 700__ $$aWright, T.$$uVirginia Tech.$$vVirginia Tech, Blacksburg, Virginia 24061, USA
002826374 700__ $$aXie, Y.$$uBeijing, Inst. High Energy Phys.$$uBeijing, GUCAS$$vUniversity of Chinese Academy of Sciences, Beijing 100049, China$$vInstitute of High Energy Physics, Beijing 100049, China
002826374 700__ $$aYang, C.$$uBeijing, Inst. High Energy Phys.$$uBeijing, GUCAS$$vUniversity of Chinese Academy of Sciences, Beijing 100049, China$$vInstitute of High Energy Physics, Beijing 100049, China
002826374 700__ $$aZabihi, A.$$uWarsaw, Copernicus Astron. Ctr.$$vAstroCeNT, Nicolaus Copernicus Astronomical Center of the Polish Academy of Sciences, 00-614 Warsaw, Poland
002826374 700__ $$aZakhary, P.$$uWarsaw, Copernicus Astron. Ctr.$$vAstroCeNT, Nicolaus Copernicus Astronomical Center of the Polish Academy of Sciences, 00-614 Warsaw, Poland
002826374 700__ $$aZani, A.$$uINFN, Milan$$vINFN Milano, Milano 20133, Italy
002826374 700__ $$aZichichi, A.$$uPurdue U.$$uBologna U.$$uINFN, Bologna$$vDepartment of Physics and Astronomy, Università degli Studi di Bologna, Bologna 40126, Italy$$vINFN Bologna, Bologna 40126, Italy
002826374 700__ $$aZuzel, G.$$uJagiellonian U.$$vM. Smoluchowski Institute of Physics, Jagiellonian University, 30-348 Krakow, Poland
002826374 700__ $$aZykova, M.P.$$uLomonosov Inst. Fine Chem. Tech.$$vMendeleev University of Chemical Technology, Moscow 125047, Russia
002826374 710__ $$gGlobal Argon Dark Matter Collaboration
002826374 773__ $$c112006$$mpublication$$n11$$pPhys. Rev. D$$v107$$xPhys. Rev. D 107, 112006 (2023)$$y2023
002826374 8564_ $$uhttps://lss.fnal.gov/archive/2022/pub/fermilab-pub-22-658-nd-ppd.pdf$$yFermilab Library Server
002826374 8564_ $$82387561$$s66962$$uhttps://cds.cern.ch/record/2826374/files/neutrino_cevns_ne2.png$$y00003 Coherent elastic neutrino-nucleus scattering background from all sources ($pp$ neutrinos not visible), zoomed into \emph{(top)} \SIrange{0}{50}{\el} and \emph{(bottom)} \SIrange{0}{5}{\el}.
002826374 8564_ $$82387562$$s1897334$$uhttps://cds.cern.ch/record/2826374/files/2209.01177.pdf$$yFulltext
002826374 8564_ $$82387563$$s75391$$uhttps://cds.cern.ch/record/2826374/files/exclusion_migdal.png$$y00010 Projected \NinetyPerCentCL\ upper limits on the spin-independent DM-nucleon scattering cross section for \DSLMExposure\ exposure: \emph{(Top, left)} with and without binomial quenching fluctuations. \emph{(Top, right)} with varying thresholds and background rates. \emph{(Bottom, left)} including the Migdal effect. \emph{(Bottom, right)} attempting to model and fit \SE\ backgrounds (see \refeqn{eq:se_spectra}) at varying impurity concentrations relative to \DSf, $\eta$. Unless otherwise stated, projections assume binomial quenching fluctuations and an \ce{^39Ar} activity of \DSfUArArThreeNineActivityOverTen. The neutrino fog in \LAr\ with index $n$ representing the resulting impediment to a $3\sigma$ \DM\ observation is shown in shades of gray, calculated to $\text{m}_\chi\SI{=100}{\MeV\per\square\c}$~\cite{ohareNewDefinitionNeutrino2021}. Current limits are shown from CRESST-III~\cite{petriccaFirstResultsLowmass2020}, \DSf~\cite{ds50SearchLowmassDark2022,ds50Migdal2022}, and \XENONOT~\cite{aprile_light_2019,aprileSearchLightDark2019}.
002826374 8564_ $$82387564$$s82981$$uhttps://cds.cern.ch/record/2826374/files/discovery_nuclearscattering.png$$y00014 Projected \emph{(Top)} \NinetyPerCentCL\ exclusion curves for the spin-independent \DM-nucleon scattering cross section with \DSfUArArThreeNineActivityOverTen\ of \ce{^39Ar}, compared to (solid) current and (dashed) projected limits. \emph{(Bottom)} $3\sigma$ significance evidence contours with a (dashed) \num{2} or (dotted) \SI{4}{\el} threshold and (thick) \DSfUArArThreeNineActivityOverOneHundredVal\ or (thin) \DSfUArArThreeNineActivityOverTen\ of \ce{^39Ar}. Binomial quenching fluctuations and \SI{1}{\tonne\year} exposures are assumed. The neutrino fog in \LAr, with $n$ denoting the impediment to a $3\sigma$ \DM\ observation, is in gray~\cite{ohareNewDefinitionNeutrino2021}. Limits from CRESST-III~\cite{petriccaFirstResultsLowmass2020}, \DSf~\cite{ds50SearchLowmassDark2022}, and \XENONOT~\cite{aprile_light_2019} are shown, along with DAMIC-1K~\cite{damiccollaborationConstraintsLightDark2019}, NEWS-G, and SuperCDMS~\cite{supercdmscollaborationProjectedSensitivitySuperCDMS2017} projections.
002826374 8564_ $$82387565$$s57176$$uhttps://cds.cern.ch/record/2826374/files/bkgd_summary.png$$y00004 Backgrounds from \grs, \isotope{39}{Ar}, and \CEnNS, compared to \DSf. \DM\ spectra for are shown at \numlist{2.5;5;10}\,\si{\GeV\per\square\c} masses with spin-independent nucleon-scattering cross section \mbox{$\sigma_\text{SI}=\SI{e-44}{\square\cm}$}.
002826374 8564_ $$82387566$$s81946$$uhttps://cds.cern.ch/record/2826374/files/exclusion_projection.png$$y00013 Projected \emph{(Top)} \NinetyPerCentCL\ exclusion curves for the spin-independent \DM-nucleon scattering cross section with \DSfUArArThreeNineActivityOverTen\ of \ce{^39Ar}, compared to (solid) current and (dashed) projected limits. \emph{(Bottom)} $3\sigma$ significance evidence contours with a (dashed) \num{2} or (dotted) \SI{4}{\el} threshold and (thick) \DSfUArArThreeNineActivityOverOneHundredVal\ or (thin) \DSfUArArThreeNineActivityOverTen\ of \ce{^39Ar}. Binomial quenching fluctuations and \SI{1}{\tonne\year} exposures are assumed. The neutrino fog in \LAr, with $n$ denoting the impediment to a $3\sigma$ \DM\ observation, is in gray~\cite{ohareNewDefinitionNeutrino2021}. Limits from CRESST-III~\cite{petriccaFirstResultsLowmass2020}, \DSf~\cite{ds50SearchLowmassDark2022}, and \XENONOT~\cite{aprile_light_2019} are shown, along with DAMIC-1K~\cite{damiccollaborationConstraintsLightDark2019}, NEWS-G, and SuperCDMS~\cite{supercdmscollaborationProjectedSensitivitySuperCDMS2017} projections.
002826374 8564_ $$82387567$$s60302$$uhttps://cds.cern.ch/record/2826374/files/sensitivity_vs_ar39.png$$y00006 Median \NinetyPerCentCL\ upper limits and $1\sigma$ expectation band on \DSLowMassMidMass\ \DM\ at varying \isotope{39}{Ar} activity.
002826374 8564_ $$82387568$$s72704$$uhttps://cds.cern.ch/record/2826374/files/se_spectra.png$$y00007 \SE\ spectra scaled from \DSf\ using \refeqn{eq:se_spectra} and \refeqn{eq:se_scaling}, for different electron amplification factors \gTwo, excess noise factor $F$, and impurity scaling factors $\eta$. Backgrounds from other sources are shown for comparison, assuming a \DSfUArArThreeNineActivityOverTen\ \isotope{39}{Ar} activity.
002826374 8564_ $$82387569$$s134088$$uhttps://cds.cern.ch/record/2826374/files/exclusion_electronscattering.png$$y00015 Projected \emph{(left)} \NinetyPerCentCL\ exclusion curves and \emph{(right)} $3\sigma$ significance evidence contours for \DM-electron couplings with \emph{(top)} light and \emph{(bottom)} heavy mediators. Bands show \SI{1}{\tonne\year} contours with \SIrange{7.3}{73}{\micro\becquerel\per\kg} of \ce{^39Ar}. Limits are shown from \DSf~\cite{ds50electronic2022}, SENSEI~\cite{barakSENSEIDirectDetectionResults2020}, XENON10~\cite{essigNewConstraintsProspects2017}, and \XENONOT~\cite{aprile_light_2019}. Thick lines show $\bar{\sigma}_e$ giving the relic \DM\ abundance through freeze-in or freeze-out production mechanisms, from \refcite{essigDirectDetectionSubGeV2016}.
002826374 8564_ $$82387570$$s87480$$uhttps://cds.cern.ch/record/2826374/files/exclusion_scenarios.png$$y00009 Projected \NinetyPerCentCL\ upper limits on the spin-independent DM-nucleon scattering cross section for \DSLMExposure\ exposure: \emph{(Top, left)} with and without binomial quenching fluctuations. \emph{(Top, right)} with varying thresholds and background rates. \emph{(Bottom, left)} including the Migdal effect. \emph{(Bottom, right)} attempting to model and fit \SE\ backgrounds (see \refeqn{eq:se_spectra}) at varying impurity concentrations relative to \DSf, $\eta$. Unless otherwise stated, projections assume binomial quenching fluctuations and an \ce{^39Ar} activity of \DSfUArArThreeNineActivityOverTen. The neutrino fog in \LAr\ with index $n$ representing the resulting impediment to a $3\sigma$ \DM\ observation is shown in shades of gray, calculated to $\text{m}_\chi\SI{=100}{\MeV\per\square\c}$~\cite{ohareNewDefinitionNeutrino2021}. Current limits are shown from CRESST-III~\cite{petriccaFirstResultsLowmass2020}, \DSf~\cite{ds50SearchLowmassDark2022,ds50Migdal2022}, and \XENONOT~\cite{aprile_light_2019,aprileSearchLightDark2019}.
002826374 8564_ $$82387571$$s49744$$uhttps://cds.cern.ch/record/2826374/files/sensitivity_vs_expo.png$$y00012 Median \NinetyPerCentCL\ upper limit and $1\sigma$ expectation band for \SI{5}{\GeV\per\square\c} \DM\ at varying exposure.
002826374 8564_ $$82387572$$s82338$$uhttps://cds.cern.ch/record/2826374/files/sensitivity_quenchingfluctuatoins.png$$y00008 Projected \NinetyPerCentCL\ upper limits on the spin-independent DM-nucleon scattering cross section for \DSLMExposure\ exposure: \emph{(Top, left)} with and without binomial quenching fluctuations. \emph{(Top, right)} with varying thresholds and background rates. \emph{(Bottom, left)} including the Migdal effect. \emph{(Bottom, right)} attempting to model and fit \SE\ backgrounds (see \refeqn{eq:se_spectra}) at varying impurity concentrations relative to \DSf, $\eta$. Unless otherwise stated, projections assume binomial quenching fluctuations and an \ce{^39Ar} activity of \DSfUArArThreeNineActivityOverTen. The neutrino fog in \LAr\ with index $n$ representing the resulting impediment to a $3\sigma$ \DM\ observation is shown in shades of gray, calculated to $\text{m}_\chi\SI{=100}{\MeV\per\square\c}$~\cite{ohareNewDefinitionNeutrino2021}. Current limits are shown from CRESST-III~\cite{petriccaFirstResultsLowmass2020}, \DSf~\cite{ds50SearchLowmassDark2022,ds50Migdal2022}, and \XENONOT~\cite{aprile_light_2019,aprileSearchLightDark2019}.
002826374 8564_ $$82387573$$s135265$$uhttps://cds.cern.ch/record/2826374/files/discovery_electronscattering.png$$y00016 Projected \emph{(left)} \NinetyPerCentCL\ exclusion curves and \emph{(right)} $3\sigma$ significance evidence contours for \DM-electron couplings with \emph{(top)} light and \emph{(bottom)} heavy mediators. Bands show \SI{1}{\tonne\year} contours with \SIrange{7.3}{73}{\micro\becquerel\per\kg} of \ce{^39Ar}. Limits are shown from \DSf~\cite{ds50electronic2022}, SENSEI~\cite{barakSENSEIDirectDetectionResults2020}, XENON10~\cite{essigNewConstraintsProspects2017}, and \XENONOT~\cite{aprile_light_2019}. Thick lines show $\bar{\sigma}_e$ giving the relic \DM\ abundance through freeze-in or freeze-out production mechanisms, from \refcite{essigDirectDetectionSubGeV2016}.
002826374 8564_ $$82387574$$s81271$$uhttps://cds.cern.ch/record/2826374/files/qy_curves.png$$y00001 Ionization yield models assumed in these studies for (top) nuclear recoils and (bottom) electronic recoils. Bands show $\pm1\sigma$ uncertainty from the fit to constraints.
002826374 8564_ $$82387575$$s79638$$uhttps://cds.cern.ch/record/2826374/files/exclusion_sefits.png$$y00011 Projected \NinetyPerCentCL\ upper limits on the spin-independent DM-nucleon scattering cross section for \DSLMExposure\ exposure: \emph{(Top, left)} with and without binomial quenching fluctuations. \emph{(Top, right)} with varying thresholds and background rates. \emph{(Bottom, left)} including the Migdal effect. \emph{(Bottom, right)} attempting to model and fit \SE\ backgrounds (see \refeqn{eq:se_spectra}) at varying impurity concentrations relative to \DSf, $\eta$. Unless otherwise stated, projections assume binomial quenching fluctuations and an \ce{^39Ar} activity of \DSfUArArThreeNineActivityOverTen. The neutrino fog in \LAr\ with index $n$ representing the resulting impediment to a $3\sigma$ \DM\ observation is shown in shades of gray, calculated to $\text{m}_\chi\SI{=100}{\MeV\per\square\c}$~\cite{ohareNewDefinitionNeutrino2021}. Current limits are shown from CRESST-III~\cite{petriccaFirstResultsLowmass2020}, \DSf~\cite{ds50SearchLowmassDark2022,ds50Migdal2022}, and \XENONOT~\cite{aprile_light_2019,aprileSearchLightDark2019}.
002826374 8564_ $$82387576$$s443368$$uhttps://cds.cern.ch/record/2826374/files/DS-LM_drawing.png$$y00000 Conceptual detector design: a \DSLMTargetActiveMass\ dual-phase \LArTPC\ in an acrylic vessel, viewed by two photosensor arrays via \DSLMPDMOffset\ ``buffer vetoes'', in a \UAr\ ``bath veto'' in a cryostat, immersed in a water tank (not shown).
002826374 8564_ $$82387577$$s57463$$uhttps://cds.cern.ch/record/2826374/files/veto_edep.png$$y00005 Energy deposited in (blue) the \PDM\ buffer veto and (green) bath veto for simulated \grs\ from the photoelectronics with \SI{<3}{\keV} single-scatters in the \TPC\ fiducial volume, considering both vetoes independently.
002826374 8564_ $$82387578$$s36126$$uhttps://cds.cern.ch/record/2826374/files/xyresolution.png$$y00002 Horizontal position resolution \XYResolutionSymbol\ as a function of signal size. Between \SIrange{1}{15}{\el}, \XYResolutionSymbol\ is between \SIrange{2}{7}{\cm}. The dark line shows the median \XYResolutionSymbol, and the lighter band is the $1\sigma$ confidence belt from simulation statistics.
002826374 8564_ $$82390179$$s1502130$$uhttps://cds.cern.ch/record/2826374/files/91ce6168799b33f720d8ae133fe8e56d.pdf$$yFulltext
002826374 8564_ $$82459629$$s49744$$uhttps://cds.cern.ch/record/2826374/files/w12_sensitivity_vs_expo.png$$y00012 Median \NinetyPerCentCL\ upper limit and $1\sigma$ expectation band for \SI{5}{\GeV\per\square\c} \DM\ at varying exposure.
002826374 8564_ $$82459630$$s57463$$uhttps://cds.cern.ch/record/2826374/files/w5_veto_edep.png$$y00005 Energy deposited in (blue) the \PDM\ buffer veto and (green) bath veto for simulated \grs\ from the photoelectronics with \SI{<3}{\keV} single-scatters in the \TPC\ fiducial volume, considering both vetoes independently.
002826374 8564_ $$82459631$$s134088$$uhttps://cds.cern.ch/record/2826374/files/w15_exclusion_electronscattering.png$$y00015 Projected \emph{(left)} \NinetyPerCentCL\ exclusion curves and \emph{(right)} $3\sigma$ significance evidence contours for \DM-electron couplings with \emph{(top)} light and \emph{(bottom)} heavy mediators. Bands show \SI{1}{\tonne\year} contours with \SIrange{7.3}{73}{\micro\becquerel\per\kg} of \ce{^39Ar}. Limits are shown from \DSf~\cite{ds50electronic2022}, SENSEI~\cite{barakSENSEIDirectDetectionResults2020}, XENON10~\cite{essigNewConstraintsProspects2017}, and \XENONOT~\cite{aprile_light_2019}. Thick lines show $\bar{\sigma}_e$ giving the relic \DM\ abundance through freeze-in or freeze-out production mechanisms, from \refcite{essigDirectDetectionSubGeV2016}.
002826374 8564_ $$82459632$$s135265$$uhttps://cds.cern.ch/record/2826374/files/w16_discovery_electronscattering.png$$y00016 Projected \emph{(left)} \NinetyPerCentCL\ exclusion curves and \emph{(right)} $3\sigma$ significance evidence contours for \DM-electron couplings with \emph{(top)} light and \emph{(bottom)} heavy mediators. Bands show \SI{1}{\tonne\year} contours with \SIrange{7.3}{73}{\micro\becquerel\per\kg} of \ce{^39Ar}. Limits are shown from \DSf~\cite{ds50electronic2022}, SENSEI~\cite{barakSENSEIDirectDetectionResults2020}, XENON10~\cite{essigNewConstraintsProspects2017}, and \XENONOT~\cite{aprile_light_2019}. Thick lines show $\bar{\sigma}_e$ giving the relic \DM\ abundance through freeze-in or freeze-out production mechanisms, from \refcite{essigDirectDetectionSubGeV2016}.
002826374 8564_ $$82459633$$s57176$$uhttps://cds.cern.ch/record/2826374/files/w4_bkgd_summary.png$$y00004 Backgrounds from \grs, \isotope{39}{Ar}, and \CEnNS, compared to \DSf. \DM\ spectra for are shown at \numlist{2.5;5;10}\,\si{\GeV\per\square\c} masses with spin-independent nucleon-scattering cross section \mbox{$\sigma_\text{SI}=\SI{e-44}{\square\cm}$}.
002826374 8564_ $$82459634$$s443368$$uhttps://cds.cern.ch/record/2826374/files/w0_DS-LM_drawing.png$$y00000 Conceptual detector design: a \DSLMTargetActiveMass\ dual-phase \LArTPC\ in an acrylic vessel, viewed by two photosensor arrays via \DSLMPDMOffset\ ``buffer vetoes'', in a \UAr\ ``bath veto'' in a cryostat, immersed in a water tank (not shown).
002826374 8564_ $$82459635$$s77363$$uhttps://cds.cern.ch/record/2826374/files/w10_exclusion_migdal.png$$y00010 Projected \NinetyPerCentCL\ upper limits on the spin-independent DM-nucleon scattering cross section for \DSLMExposure\ exposure: \emph{(Top, left)} with and without binomial quenching fluctuations. \emph{(Top, right)} with varying thresholds and background rates. \emph{(Bottom, left)} including the Migdal effect. \emph{(Bottom, right)} attempting to model and fit \SE\ backgrounds (see \refeqn{eq:se_spectra}) at varying impurity concentrations relative to \DSf, $\eta$. Unless otherwise stated, projections assume binomial quenching fluctuations and an \ce{^39Ar} activity of \DSfUArArThreeNineActivityOverTen. The neutrino fog in \LAr\ with index $n$ representing the resulting impediment to a $3\sigma$ \DM\ observation is shown in shades of gray, calculated to $\text{m}_\chi\SI{=100}{\MeV\per\square\c}$~\cite{ohareNewDefinitionNeutrino2021}. Current limits are shown from CRESST-III~\cite{petriccaFirstResultsLowmass2020}, \DSf~\cite{ds50SearchLowmassDark2022,ds50Migdal2022}, and \XENONOT~\cite{aprile_light_2019,aprileSearchLightDark2019}.
002826374 8564_ $$82459636$$s72704$$uhttps://cds.cern.ch/record/2826374/files/w7_se_spectra.png$$y00007 \SE\ spectra scaled from \DSf\ using \refeqn{eq:se_spectra} and \refeqn{eq:se_scaling}, for different electron amplification factors \gTwo, excess noise factor $F$, and impurity scaling factors $\eta$. Backgrounds from other sources are shown for comparison, assuming a \DSfUArArThreeNineActivityOverTen\ \isotope{39}{Ar} activity.
002826374 8564_ $$82459637$$s79638$$uhttps://cds.cern.ch/record/2826374/files/w11_exclusion_sefits.png$$y00011 Projected \NinetyPerCentCL\ upper limits on the spin-independent DM-nucleon scattering cross section for \DSLMExposure\ exposure: \emph{(Top, left)} with and without binomial quenching fluctuations. \emph{(Top, right)} with varying thresholds and background rates. \emph{(Bottom, left)} including the Migdal effect. \emph{(Bottom, right)} attempting to model and fit \SE\ backgrounds (see \refeqn{eq:se_spectra}) at varying impurity concentrations relative to \DSf, $\eta$. Unless otherwise stated, projections assume binomial quenching fluctuations and an \ce{^39Ar} activity of \DSfUArArThreeNineActivityOverTen. The neutrino fog in \LAr\ with index $n$ representing the resulting impediment to a $3\sigma$ \DM\ observation is shown in shades of gray, calculated to $\text{m}_\chi\SI{=100}{\MeV\per\square\c}$~\cite{ohareNewDefinitionNeutrino2021}. Current limits are shown from CRESST-III~\cite{petriccaFirstResultsLowmass2020}, \DSf~\cite{ds50SearchLowmassDark2022,ds50Migdal2022}, and \XENONOT~\cite{aprile_light_2019,aprileSearchLightDark2019}.
002826374 8564_ $$82459638$$s60302$$uhttps://cds.cern.ch/record/2826374/files/w6_sensitivity_vs_ar39.png$$y00006 Median \NinetyPerCentCL\ upper limits and $1\sigma$ expectation band on \DSLowMassMidMass\ \DM\ at varying \isotope{39}{Ar} activity.
002826374 8564_ $$82459639$$s81271$$uhttps://cds.cern.ch/record/2826374/files/w1_qy_curves.png$$y00001 Ionization yield models assumed in these studies for (top) nuclear recoils and (bottom) electronic recoils. Bands show $\pm1\sigma$ uncertainty from the fit to constraints.
002826374 8564_ $$82459640$$s82338$$uhttps://cds.cern.ch/record/2826374/files/w8_sensitivity_quenchingfluctuatoins.png$$y00008 Projected \NinetyPerCentCL\ upper limits on the spin-independent DM-nucleon scattering cross section for \DSLMExposure\ exposure: \emph{(Top, left)} with and without binomial quenching fluctuations. \emph{(Top, right)} with varying thresholds and background rates. \emph{(Bottom, left)} including the Migdal effect. \emph{(Bottom, right)} attempting to model and fit \SE\ backgrounds (see \refeqn{eq:se_spectra}) at varying impurity concentrations relative to \DSf, $\eta$. Unless otherwise stated, projections assume binomial quenching fluctuations and an \ce{^39Ar} activity of \DSfUArArThreeNineActivityOverTen. The neutrino fog in \LAr\ with index $n$ representing the resulting impediment to a $3\sigma$ \DM\ observation is shown in shades of gray, calculated to $\text{m}_\chi\SI{=100}{\MeV\per\square\c}$~\cite{ohareNewDefinitionNeutrino2021}. Current limits are shown from CRESST-III~\cite{petriccaFirstResultsLowmass2020}, \DSf~\cite{ds50SearchLowmassDark2022,ds50Migdal2022}, and \XENONOT~\cite{aprile_light_2019,aprileSearchLightDark2019}.
002826374 8564_ $$82459641$$s36126$$uhttps://cds.cern.ch/record/2826374/files/w2_xyresolution.png$$y00002 Horizontal position resolution \XYResolutionSymbol\ as a function of signal size. Between \SIrange{1}{15}{\el}, \XYResolutionSymbol\ is between \SIrange{2}{7}{\cm}. The dark line shows the median \XYResolutionSymbol, and the lighter band is the $1\sigma$ confidence belt from simulation statistics.
002826374 8564_ $$82459642$$s82981$$uhttps://cds.cern.ch/record/2826374/files/w14_discovery_nuclearscattering.png$$y00014 Projected \emph{(Top)} \NinetyPerCentCL\ exclusion curves for the spin-independent \DM-nucleon scattering cross section with \DSfUArArThreeNineActivityOverTen\ of \ce{^39Ar}, compared to (solid) current and (dashed) projected limits. \emph{(Bottom)} $3\sigma$ significance evidence contours with a (dashed) \num{2} or (dotted) \SI{4}{\el} threshold and (thick) \DSfUArArThreeNineActivityOverOneHundredVal\ or (thin) \DSfUArArThreeNineActivityOverTen\ of \ce{^39Ar}. Binomial quenching fluctuations and \SI{1}{\tonne\year} exposures are assumed. The neutrino fog in \LAr, with $n$ denoting the impediment to a $3\sigma$ \DM\ observation, is in gray~\cite{ohareNewDefinitionNeutrino2021}. Limits from CRESST-III~\cite{petriccaFirstResultsLowmass2020}, \DSf~\cite{ds50SearchLowmassDark2022}, and \XENONOT~\cite{aprile_light_2019} are shown, along with DAMIC-1K~\cite{damiccollaborationConstraintsLightDark2019}, NEWS-G, and SuperCDMS~\cite{supercdmscollaborationProjectedSensitivitySuperCDMS2017} projections.
002826374 8564_ $$82459643$$s87480$$uhttps://cds.cern.ch/record/2826374/files/w9_exclusion_scenarios.png$$y00009 Projected \NinetyPerCentCL\ upper limits on the spin-independent DM-nucleon scattering cross section for \DSLMExposure\ exposure: \emph{(Top, left)} with and without binomial quenching fluctuations. \emph{(Top, right)} with varying thresholds and background rates. \emph{(Bottom, left)} including the Migdal effect. \emph{(Bottom, right)} attempting to model and fit \SE\ backgrounds (see \refeqn{eq:se_spectra}) at varying impurity concentrations relative to \DSf, $\eta$. Unless otherwise stated, projections assume binomial quenching fluctuations and an \ce{^39Ar} activity of \DSfUArArThreeNineActivityOverTen. The neutrino fog in \LAr\ with index $n$ representing the resulting impediment to a $3\sigma$ \DM\ observation is shown in shades of gray, calculated to $\text{m}_\chi\SI{=100}{\MeV\per\square\c}$~\cite{ohareNewDefinitionNeutrino2021}. Current limits are shown from CRESST-III~\cite{petriccaFirstResultsLowmass2020}, \DSf~\cite{ds50SearchLowmassDark2022,ds50Migdal2022}, and \XENONOT~\cite{aprile_light_2019,aprileSearchLightDark2019}.
002826374 8564_ $$82459644$$s81946$$uhttps://cds.cern.ch/record/2826374/files/w13_exclusion_projection.png$$y00013 Projected \emph{(Top)} \NinetyPerCentCL\ exclusion curves for the spin-independent \DM-nucleon scattering cross section with \DSfUArArThreeNineActivityOverTen\ of \ce{^39Ar}, compared to (solid) current and (dashed) projected limits. \emph{(Bottom)} $3\sigma$ significance evidence contours with a (dashed) \num{2} or (dotted) \SI{4}{\el} threshold and (thick) \DSfUArArThreeNineActivityOverOneHundredVal\ or (thin) \DSfUArArThreeNineActivityOverTen\ of \ce{^39Ar}. Binomial quenching fluctuations and \SI{1}{\tonne\year} exposures are assumed. The neutrino fog in \LAr, with $n$ denoting the impediment to a $3\sigma$ \DM\ observation, is in gray~\cite{ohareNewDefinitionNeutrino2021}. Limits from CRESST-III~\cite{petriccaFirstResultsLowmass2020}, \DSf~\cite{ds50SearchLowmassDark2022}, and \XENONOT~\cite{aprile_light_2019} are shown, along with DAMIC-1K~\cite{damiccollaborationConstraintsLightDark2019}, NEWS-G, and SuperCDMS~\cite{supercdmscollaborationProjectedSensitivitySuperCDMS2017} projections.
002826374 8564_ $$82459645$$s66962$$uhttps://cds.cern.ch/record/2826374/files/w3_neutrino_cevns_ne2.png$$y00003 Coherent elastic neutrino-nucleus scattering background from all sources ($pp$ neutrinos not visible), zoomed into \emph{(top)} \SIrange{0}{50}{\el} and \emph{(bottom)} \SIrange{0}{5}{\el}.
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