Improved WIMP-search reach of the CDMS II germanium data.
R. Agnese,Adam Anderson,M. Asai,D. Balakishiyeva,D. Barker,R. Basu Thakur,D. A. Bauer,J. Billard,A. W. Borgland,M. A. Bowles,D. Brandt,P. L. Brink,R. Bunker,Blas Cabrera,David O. Caldwell,R. Calkins,David G. Cerdeño,H. Chagani,Yi Chen,Jodi Cooley,B. Cornell,C. H. Crewdson,P. Cushman,Miguel Daal,P. Di Stefano,T. Doughty,L. Esteban,S. Fallows,Enectali Figueroa-Feliciano,G.L. Godfrey,Sunil Golwala,J. Hall,H. R. Harris,S. A. Hertel,T. Hofer,Donald J. Holmgren,L. Hsu,Martin E. Huber,D. Jardin,A. Jastram,O. Kamaev,B. Kara,M. H. Kelsey,A. Kennedy,M. Kiveni,K. Koch,A. Leder,B. Loer,E. Lopez Asamar,P. Lukens,R. Mahapatra,Vuk Mandic,Kevin A. McCarthy,N. Mirabolfathi,Robert A. Moffatt,S. M. Oser,K. L. Page,W. A. Page,R. Partridge,M. Pepin,A. Phipps,K. Prasad,Matt Pyle,H. Qiu,W. Rau,P. Redl,A. Reisetter,Y. Ricci,H. E. Rogers,Tarek Saab,Bernard Sadoulet,J. Sander,K. Schneck,R. W. Schnee,S. Scorza,B. Serfass,B. Shank,Danielle Speller,D. Toback,S. Upadhyayula,A. N. Villano,B. Welliver,John Wilson,D. H. Wright,X. Yang,S. J. Yellin,J. J. Yen,Betty A. Young,J. Zhang +88 more
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In this article, an improved charge-pulse fitting algorithm was used to reject surface-event backgrounds in the 612 kg days germanium-detector weakly interacting massive particle (WIMP)-search exposure.Abstract:
CDMS II data from the five-tower runs at the Soudan Underground Laboratory were reprocessed with an improved charge-pulse fitting algorithm. Two new analysis techniques to reject surface-event backgrounds were applied to the 612 kg days germanium-detector weakly interacting massive particle (WIMP)-search exposure. An extended analysis was also completed by decreasing the 10 keV analysis threshold to ∼5 keV, to increase sensitivity near a WIMP mass of 8 GeV/c^2. After unblinding, there were zero candidate events above a deposited energy of 10 keV and six events in the lower-threshold analysis. This yielded minimum WIMP-nucleon spin-independent scattering cross-section limits of 1.8×10^(−44) and 1.18×10^(−41) at 90% confidence for 60 and 8.6 GeV/c^2 WIMPs, respectively. This improves the previous CDMS II result by a factor of 2.4 (2.7) for 60 (8.6) GeV/c^2 WIMPs.read more
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DarkSide-20k: A 20 tonne two-phase LAr TPC for direct dark matter detection at LNGS
Craig E. Aalseth,Fabio Acerbi,P. Agnes,Ivone F. M. Albuquerque,Thomas Alexander,Andrea Alici,A. K. Alton,Pietro Antonioli,Silvia Arcelli,Raffaele Ardito,I. J. Arnquist,D. M. Asner,M. Ave,H. O. Back,A. Barrado Olmedo,G. Batignani,E. Bertoldo,S. Bettarini,Maria Giuseppina Bisogni,V. Bocci,A.E. Bondar,A.E. Bondar,G. Bonfini,W. Bonivento,M. Bossa,B. Bottino,M. G. Boulay,R. Bunker,S. Bussino,A. Buzulutskov,A. Buzulutskov,M. Cadeddu,Mariano Cadoni,A. Caminata,N. Canci,A. Candela,C. Cantini,M. Caravati,M. Cariello,M. Carlini,M. Carpinelli,A. Castellani,S. Catalanotti,Vittorio Cataudella,P. Cavalcante,Stefano Cavuoti,R. Cereseto,A. S. Chepurnov,C. Cicalo,L. Cifarelli,Mauro Citterio,A. G. Cocco,Manuel Colocci,S. Corgiolu,Giovanni Covone,Paolo Crivelli,I. D'Antone,M. D'Incecco,D. D'Urso,M. Da Rocha Rolo,M. K. Daniel,S. Davini,A. de Candia,S. De Cecco,M. De Deo,G. De Filippis,G. De Guido,G. De Rosa,G. Dellacasa,M. Della Valle,Pierfranco Demontis,A. V. Derbin,A. Devoto,F. Di Eusanio,G. Di Pietro,C. Dionisi,A. Dolgov,I. Dormia,S. Dussoni,A. Empl,M. Fernandez Diaz,Alessandro Ferri,C. Filip,G. Fiorillo,K. Fomenko,D. Franco,George E. Froudakis,F. Gabriele,Andrea Gabrieli,Cristiano Galbiati,P. Garcia Abia,A. Gendotti,Aldo Ghisi,Stefano Giagu,P. Giampa,G. Gibertoni,C. Giganti,Mario Giorgi,G. K. Giovanetti,M. L. Gligan,Alberto Gola,O. Gorchakov,A. M. Goretti,F. Granato,Marco Grassi,Jay W. Grate,G. Y. Grigoriev,M. Gromov,Min-Xin Guan,Marcelo Braga Bueno Guerra,M. Guerzoni,Marisa Gulino,R. K. Haaland,A. L. Hallin,B. Harrop,Eric W. Hoppe,S. Horikawa,B. Hosseini,D. Hughes,Paul H. Humble,E. V. Hungerford,An. Ianni,C. J. Jillings,T. N. Johnson,K. Keeter,C. L. Kendziora,S. Kim,G. Koh,D. Korablev,G. Korga,A. S. Kubankin,M. Kuss,M. Kuźniak,M. La Commara,B. Lehnert,Xiujiang Li,M. Lissia,G. U. Lodi,Ben Loer,Giuseppe Longo,P. F. Loverre,Rudi Lussana,Lelio Luzzi,Yanhui Ma,A. A. Machado,I. N. Machulin,I. N. Machulin,A. Mandarano,L. Mapelli,M. Marcante,M. Marcante,Anselmo Margotti,Stefano Maria Mari,Mario Mariani,J. Maricic,C. J. Martoff,Michele Mascia,M. Mayer,A. B. McDonald,Andrea Messina,P. D. Meyers,R. Milincic,A. Moggi,Stefania Moioli,Jocelyn Monroe,A. Monte,Matteo Morrocchi,B. J. Mount,W. Mu,V. N. Muratova,S. Murphy,Paolo Musico,Rosario Nania,A. Navrer Agasson,I. Nikulin,V. Nosov,V. Nosov,A. O. Nozdrina,A. O. Nozdrina,N. N. Nurakhov,A. Oleinik,V. Oleynikov,V. Oleynikov,M. Orsini,Fausto Ortica,L. Pagani,Marco Pallavicini,Simonetta Palmas,Luciano Pandola,E. Pantic,E. Paoloni,Giovanni Paternoster,V. Pavletcov,F. Pazzona,S. J. M. Peeters,K. Pelczar,Laura A. Pellegrini,N. Pelliccia,Federico Perotti,R. Perruzza,V. Pesudo,Claudio Piemonte,Fabrizio Giulio Luca Pilo,A. Pocar,T. Pollmann,Davide Portaluppi,D. A. Pugachev,H. Qian,B. Radics,F. Raffaelli,Francesco Ragusa,M. Razeti,A. Razeto,V. Regazzoni,V. Regazzoni,C. Regenfus,B. Reinhold,A. L. Renshaw,M. Rescigno,F. Retiere,Q. Riffard,Angelo Rivetti,Simone Rizzardini,Aldo Romani,L. Romero,B. Rossi,N. Rossi,André Rubbia,D. Sablone,Piero Salatino,O. Samoylov,E. Sanchez Garcia,W. Sands,S. Sanfilippo,Marco Sant,R. Santorelli,C. Savarese,Eugenio Scapparone,B. Schlitzer,Gilda Scioli,E. Segreto,Allen Seifert,D. A. Semenov,A.V. Shchagin,L. Shekhtman,L. Shekhtman,E. Shemyakina,E. Shemyakina,A. Sheshukov,Marino Simeone,P. N. Singh,P. Skensved,M. D. Skorokhvatov,M. D. Skorokhvatov,O. Smirnov,G. Sobrero,Andrey Sokolov,Andrey Sokolov,A. Sotnikov,F. Speziale,R. Stainforth,C. Stanford,Giuseppe Baldovino Suffritti,Y. Suvorov,Y. Suvorov,R. Tartaglia,G. Testera,A. Tonazzo,Alberto Tosi,P. Trinchese,E. V. Unzhakov,Annalisa Vacca,E. Vázquez-Jáuregui,Monica Verducci,T. Viant,Federica Villa,A. Vishneva,B. Vogelaar,M. Wada,J. Wahl,J. Walding,Hui Wang,Yuting Wang,Alan Watson,S. Westerdale,Richard M. Williams,Marcin Wójcik,S. Wu,X. Xiang,Xiang Xiao,Chung-Yao Yang,Z. Ye,A. Yllera de Llano,Franco Zappa,G. Zappalà,G. Zappalà,Caoxiang Zhu,Antonino Zichichi,M. Zullo,A. Zullo,G. Zuzel +300 more
TL;DR: The DarkSide-20k detector as discussed by the authors is a direct WIMP search detector using a two-phase Liquid Argon Time Projection Chamber (LAr TPC) with an active mass of 23 t (20 t).
Journal ArticleDOI
The dawn of FIMP Dark Matter : A review of models and constraints
TL;DR: In this article, the authors present an overview of scenarios where the observed dark matter (DM) abundance consists of Feebly Interacting Massive Particles (FIMPs), produced nonthermally by the so-called freeze-in mechanism.
Journal ArticleDOI
Dark Matter Search Results from the PICO-2L C3F8 Bubble Chamber.
C. Amole,Miguel Ardid,David M. Asner,D. Baxter,E. Behnke,P. S. Bhattacharjee,H. Borsodi,M. Bou-Cabo,S. J. Brice,Daniel Broemmelsiek,K. Clark,J. I. Collar,P. S. Cooper,M. Crisler,C. E. Dahl,C. E. Dahl,S. Daley,Madhusmita Das,F. Debris,N. Dhungana,J. Farine,Ivan Felis,R. Filgas,M. Fines-Neuschild,Francoise Girard,G. Giroux,M. Hai,J. Hall,O. Harris,C. M. Jackson,M. Jin,C. B. Krauss,M. Lafrenière,M. Laurin,I. Lawson,I. Levine,W. H. Lippincott,E. Mann,J. P. Martin,Deepam Maurya,Pitam Mitra,R. Neilson,R. Neilson,A. J. Noble,A. Plante,R. B. Podviianiuk,Shashank Priya,A. E. Robinson,M. Ruschman,O. Scallon,O. Scallon,S. Seth,Andrew Sonnenschein,N. Starinski,I. Stekl,E. Vázquez-Jáuregui,E. Vázquez-Jáuregui,J. Wells,U. Wichoski,V. Zacek,Jie Zhang +60 more
TL;DR: These data provide the most sensitive direct detection constraints on WIMP-proton spin-dependent scattering to date, with significant sensitivity at low W IMP masses for spin-independent WIMp-nucleon scattering.
Journal ArticleDOI
Dark Matter Search Results from the Complete Exposure of the PICO-60 C$_3$F$_8$ Bubble Chamber
C. Amole,M. Ardid,I. J. Arnquist,D. M. Asner,D. Baxter,E. Behnke,M. Bressler,B. Broerman,G. Cao,Chujie Chen,U. Chowdhury,Karl J. Clark,J. I. Collar,P. S. Cooper,C. B. Coutu,C. Cowles,M. B. Crisler,G. Crowder,N. A. Cruz-Venegas,C. E. Dahl,Mala Das,S. Fallows,J. Farine,Ivan Felis,R. Filgas,F. Girard,G. Giroux,J. Hall,C. Hardy,O. Harris,T. Hillier,Eric W. Hoppe,C. M. Jackson,M. Jin,L. Klopfenstein,T. Kozynets,C. B. Krauss,M. Laurin,I. Lawson,A. Leblanc,Ilan Levine,C. Licciardi,W. H. Lippincott,B. Loer,F. Mamedov,P. Mitra,C. D. Moore,T. Nania,R. Neilson,A. J. Noble,P. Oedekerk,Amber M. Ortega,M.-C. Piro,A. Plante,R. Podviyanuk,Shashank Priya,A. E. Robinson,S. Sahoo,O. Scallon,Satyajit Seth,A. Sonnenschein,N. Starinski,I. Stekl,T. Sullivan,F. Tardif,E. Vázquez-Jáuregui,N. Walkowski,E. Weima,U. Wichoski,K. Wierman,Yongke Yan,V. Zacek,Jie Zhang +72 more
TL;DR: The PICO Collaboration as discussed by the authors has been supported by the Canada Foundation for Innovation and the Province of Ontario Ministry of Research and Innovation, with underground access provided by Vale at the Creighton mine site.
Journal ArticleDOI
Low-mass dark matter search with CDMSlite
R. Agnese,Adam Anderson,T. Aralis,Tsuguo Aramaki,I. J. Arnquist,W. Baker,D. Balakishiyeva,D. Barker,R. Basu Thakur,D. A. Bauer,T. Binder,M. A. Bowles,P. L. Brink,R. Bunker,Blas Cabrera,David O. Caldwell,R. Calkins,C. Cartaro,David G. Cerdeño,Yu Kai Chang,H. Chagani,Yi Chen,Jodi Cooley,B. Cornell,P. Cushman,Miguel Daal,P. Di Stefano,T. Doughty,L. Esteban,E. Fascione,Enectali Figueroa-Feliciano,Matthew Fritts,G. Gerbier,M. Ghaith,G.L. Godfrey,Sunil Golwala,J. Hall,H. R. Harris,Ziqing Hong,Eric W. Hoppe,L. Hsu,Martin E. Huber,V. Iyer,D. Jardin,A. Jastram,Chitrasen Jena,M. H. Kelsey,A. Kennedy,A. Kubik,Noah Kurinsky,A. Leder,B. Loer,E. Lopez Asamar,P. Lukens,D. MacDonell,R. Mahapatra,Vuk Mandic,N. Mast,E. H. Miller,N. Mirabolfathi,Robert A. Moffatt,Bedangadas Mohanty,J. D. Morales Mendoza,J. K. Nelson,John L. Orrell,S. M. Oser,K. L. Page,W. A. Page,R. Partridge,M. Pepin,M. Peñalver Martinez,A. Phipps,S. S. Poudel,Matt Pyle,H. Qiu,W. Rau,P. Redl,A. Reisetter,T. Reynolds,Amy Roberts,A. E. Robinson,H. E. Rogers,Tarek Saab,Bernard Sadoulet,J. Sander,K. Schneck,R. W. Schnee,S. Scorza,Kartik Senapati,B. Serfass,Danielle Speller,M. Stein,J. Street,Hiromasa Tanaka,D. Toback,R. Underwood,A. N. Villano,B. von Krosigk,B. Welliver,John Wilson,M. J. Wilson,D. H. Wright,S. J. Yellin,J. J. Yen,Betty A. Young,X. Zhang,Xingbo Zhao +106 more
TL;DR: The SuperCDMS experiment at the Soudan Underground Laboratory was designed to directly detect weakly interacting massive particles (WIMPs) that may constitute the dark matter in our Galaxy as discussed by the authors.
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