Projected WIMP sensitivity of the LUX-ZEPLIN dark matter experiment
D. S. Akerib,Carl W. Akerlof,S. Alsum,Henrique Araujo,M. Arthurs,X. Bai,A. J. Bailey,J. Balajthy,S. Balashov,D. A. Bauer,J. Belle,P. Beltrame,T. Benson,Ethan Bernard,T. P. Biesiadzinski,K. E. Boast,B. Boxer,P. Brás,J. H. Buckley,Vv. Bugaev,Sergey Burdin,J. Busenitz,C. Carels,Duncan Carlsmith,Ben Carlson,M. C. Carmona-Benitez,C. Chan,J. J. Cherwinka,A. Cole,A. Cottle,W. Craddock,A. Currie,J. E. Cutter,C. E. Dahl,L.D. Viveiros,A. Dobi,J. E. Y. Dobson,E. Druszkiewicz,T. K. Edberg,W. R. Edwards,A. Fan,Simon Fayer,S. Fiorucci,T. Fruth,R. J. Gaitskell,J. Genovesi,C. Ghag,M. G. D. Gilchriese,Mgd van der Grinten,C. R. Hall,S. Hans,K. Hanzel,S. J. Haselschwardt,S. A. Hertel,Seth Hillbrand,C. Hjemfelt,Hoff,J. Y.K. Hor,D. Q. Huang,C. M. Ignarra,W. Ji,Asher Kaboth,K. Kamdin,J. Keefner,D. Khaitan,A. Khazov,Yeongduk Kim,C. D. Kocher,Elena Korolkova,H. Kraus,H.J. Krebs,L. Kreczko,Benjamin Krikler,V. A. Kudryavtsev,S. Kyre,Juhyeong Lee,B. G. Lenardo,David Leonard,K. T. Lesko,C. Levy,J. Li,J. Liao,F.-T. Liao,J. Lin,A. Lindote,R. Linehan,W. H. Lippincott,X. Liu,M.I. Lopes,B.L. Paredes,Wolfgang Lorenzon,S. Luitz,J. M. Lyle,Peter Majewski,A. Manalaysay,R. L. Mannino,C. Maupin,Daniel McKinsey,Yue Meng,E. H. Miller,J. Mock,M. E. Monzani,J. A. Morad,E. Morrison,B. J. Mount,A. Murphy,H. N. Nelson,F. Neves,J. A. Nikoleyczik,K. O'Sullivan,I. Olcina,Olevitch,K. C. Oliver-Mallory,K. J. Palladino,S. J. Patton,E. K. Pease,Bjoern Penning,A. Piepke,S. Powell,R. M. Preece,K. Pushkin,B. N. Ratcliff,J. Reichenbacher,C. Rhyne,A. Richards,J.P. Rodrigues,Richard Rosero,P. Rossiter,J.S. Saba,M. Sarychev,R. W. Schnee,Michael Schubnell,P.R. Scovell,S. Shaw,T. A. Shutt,J.J. Silk,C. Silva,K. Skarpaas,W. Skulski,M. Solmaz,V. N. Solovov,P. Sorensen,I. Stancu,M.R. Stark,T.M. Stiegler,K. Stifter,Matthew Szydagis,W. C. Taylor,R. Taylor,D. J. Taylor,D. Temples,P. A. Terman,K.J. Thomas,M. Timalsina,W. H. To,A. Tomás,T. Tope,Mani Tripathi,C. E. Tull,L. Tvrznikova,U. Utku,J. Va’vra,Antonin Vacheret,J.R. Verbus,E. Voirin,W.L. Waldron,J. R. Watson,R. C. Webb,D. White,T. J. Whitis,W. J. Wisniewski,Witherell,F.L.H. Wolfs,D. Woodward,S. D. Worm,Minfang Yeh,J. Yin,Ian S. Young +177 more
TLDR
Lux-ZEPLIN (LZ) as mentioned in this paper is a next-generation dark matter direct detection experiment that will operate 4850 feet underground at the Sanford Underground Research Facility (SURF) in Lead, South Dakota, USA using a two-phase xenon detector with an active mass of 7 tonnes.Abstract:
LUX-ZEPLIN (LZ) is a next-generation dark matter direct detection experiment that will operate 4850 feet underground at the Sanford Underground Research Facility (SURF) in Lead, South Dakota, USA Using a two-phase xenon detector with an active mass of 7 tonnes, LZ will search primarily for low-energy interactions with weakly interacting massive particles (WIMPs), which are hypothesized to make up the dark matter in our galactic halo In this paper, the projected WIMP sensitivity of LZ is presented based on the latest background estimates and simulations of the detector For a 1000 live day run using a 56-tonne fiducial mass, LZ is projected to exclude at 90% confidence level spin-independent WIMP-nucleon cross sections above 14 × 10-48cm2 for a 40 GeV/c2 mass WIMP Additionally, a 5σ discovery potential is projected, reaching cross sections below the exclusion limits of recent experiments For spin-dependent WIMP-neutron(-proton) scattering, a sensitivity of 23 × 10−43 cm2 (71 × 10−42 cm2) for a 40 GeV/c2
mass WIMP is expected With underground installation well underway, LZ is on track for commissioning at SURF in 2020read more
Citations
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Journal ArticleDOI
Projected WIMP sensitivity of the XENONnT dark matter experiment
Elena Aprile,Jelle Aalbers,F. Agostini,M. Alfonsi,L. Althueser,F. D. Amaro,V. C. Antochi,E. Angelino,J. R. Angevaare,F. Arneodo,D. Barge,Laura Baudis,Boris Bauermeister,L. Bellagamba,M. L. Benabderrahmane,T. Berger,April S. Brown,Ethan Brown,S. Bruenner,Giacomo Bruno,Ran Budnik,C. Capelli,João Cardoso,D. Cichon,B. Cimmino,M. Clark,D. Coderre,Auke-Pieter Colijn,Jan Conrad,Jean-Pierre Cussonneau,M. P. Decowski,A. Depoian,P. Di Gangi,A. Di Giovanni,R. Di Stefano,Sara Diglio,A. Elykov,G. Eurin,A. D. Ferella,W. Fulgione,P. Gaemers,R. Gaior,Michelle Galloway,F. Gao,L. Grandi,C. Hasterok,C. Hils,Katsuki Hiraide,L. Hoetzsch,J. Howlett,M. Iacovacci,Yoshitaka Itow,F. Joerg,N. Kato,Shingo Kazama,Masanori Kobayashi,G. Koltman,A. Kopec,H. Landsman,R. F. Lang,L. Levinson,Qing Lin,Sebastian Lindemann,Manfred Lindner,F. Lombardi,J. Long,J. A. M. Lopes,E. López Fune,C. Macolino,J. Mahlstedt,A. Mancuso,Laura Manenti,A. Manfredini,Fabrizio Marignetti,T. Marrodán Undagoitia,K. Martens,Julien Masbou,D. Masson,S. Mastroianni,M. Messina,Kentaro Miuchi,Keita Mizukoshi,A. Molinario,K. Morå,K. Morå,Shigetaka Moriyama,Y. Mosbacher,M. Murra,J. Naganoma,Kaixuan Ni,Uwe Oberlack,K. Odgers,J. Palacio,J. Palacio,Bart Pelssers,R. Peres,J. Pienaar,V. Pizzella,Guillaume Plante,J. Qin,H. Qiu,D. Ramírez García,S. Reichard,A. Rocchetti,N. Rupp,J.M.F. dos Santos,G. Sartorelli,N. Šarčević,M. Scheibelhut,Jochen Schreiner,D. Schulte,Marc Schumann,L. Scotto Lavina,M. Selvi,F. Semeria,P. Shagin,E. Shockley,Manuel Gameiro da Silva,Hardy Simgen,Atsushi Takeda,C. Therreau,D. Thers,F. Toschi,Gian Carlo Trinchero,C. Tunnell,Kathrin Valerius,M. Vargas,G. Volta,Han Wang,Yuehuan Wei,Ch. Weinheimer,M. Weiss,D. Wenz,C. Wittweg,Z. Xu,Masaki Yamashita,Masaki Yamashita,J. Ye,G. Zavattini,Yanxi Zhang,T. Zhu,J. P. Zopounidis +141 more
TL;DR: In this paper, the authors predict the experimental background and project the sensitivity of XENONnT to the detection of weakly interacting massive particles (WIMPs) in a 4 t fiducial mass.
Journal ArticleDOI
Direct Detection of WIMP Dark Matter: Concepts and Status
TL;DR: In this article, the concepts of direct detection of dark matter in the form of Weakly Interacting Massive Particles (WIMPs) in ultra-sensitive detectors located in underground laboratories are reviewed.
Journal ArticleDOI
Projected WIMP Sensitivity of the XENONnT Dark Matter Experiment
Elena Aprile,Jelle Aalbers,F. Agostini,M. Alfonsi,L. Althueser,F. D. Amaro,V. C. Antochi,E. Angelino,J. R. Angevaare,F. Arneodo,D. Barge,Laura Baudis,Boris Bauermeister,L. Bellagamba,M. L. Benabderrahmane,T. Berger,April S. Brown,Ethan Brown,S. Bruenner,Giacomo Bruno,Ran Budnik,C. Capelli,João Cardoso,D. Cichon,B. Cimmino,Michael Ryan Clark,D. Coderre,Auke-Pieter Colijn,Jan Conrad,Jean-Pierre Cussonneau,M. P. Decowski,A. Depoian,P. Di Gangi,A. Di Giovanni,R. Di Stefano,Sara Diglio,A. Elykov,G. Eurin,A. D. Ferella,W. Fulgione,P. Gaemers,R. Gaior,Michelle Galloway,F. Gao,L. Grandi,C. Hasterok,C. Hils,Katsuki Hiraide,L. Hoetzsch,J. Howlett,M. Iacovacci,Yoshitaka Itow,F. Joerg,N. Kato,Shingo Kazama,Masanori Kobayashi,G. Koltman,A. Kopec,H. Landsman,R. F. Lang,L. Levinson,Qing Lin,Sebastian Lindemann,Manfred Lindner,F. Lombardi,J. Long,J.A.M. Lopes,E. López Fune,C. Macolino,Joern Mahlstedt,A. Mancuso,Laura Manenti,A. Manfredini,Fabrizio Marignetti,T. Marrodán Undagoitia,Kalen Martens,Julien Masbou,D. Masson,S. Mastroianni,M. Messina,Kentaro Miuchi,Keita Mizukoshi,A. Molinario,K. Morå,S. Moriyama,Y. Mosbacher,M. Murra,J. Naganoma,Kaixuan Ni,Uwe Oberlack,K. Odgers,J. Palacio,Bart Pelssers,R. Peres,J. Pienaar,V. Pizzella,Guillaume Plante,J. Qin,H. Qiu,D. Ramírez García,S. Reichard,A. Rocchetti,N. Rupp,J.M.F. dos Santos,G. Sartorelli,N. Šarčević,M. Scheibelhut,Jochen Schreiner,D. Schulte,Marc Schumann,L. Scotto Lavina,M. Selvi,F. Semeria,P. Shagin,E. Shockley,Manuel Gameiro da Silva,Hardy Simgen,Atsushi Takeda,C. Therreau,D. Thers,F. Toschi,G. C. Trinchero,C. Tunnell,K. Valerius,M. Vargas,G. Volta,Hulin Wang,Yuehuan Wei,Ch. Weinheimer,M. Weiss,D. Wenz,C. Wittweg,Z. Xu,Masaki Yamashita,J. Ye,Guido Zavattini,Y. Zhang,T. Zhu,J. P. Zopounidis +138 more
TL;DR: In this article, the authors predict the experimental background and project the sensitivity of XENONnT to the detection of weakly interacting massive particles (WIMPs) using the profile construction method, in order to ensure proper coverage.
Journal ArticleDOI
The LUX-ZEPLIN (LZ) experiment
D. S. Akerib,Carl W. Akerlof,D. Yu. Akimov,A. Alquahtani,S. Alsum,T. J. Anderson,N. Angelides,Henrique Araujo,A. Arbuckle,J. E. Armstrong,M. Arthurs,H. Auyeung,X. Bai,A. J. Bailey,J. Balajthy,S. Balashov,J. Bang,M.J. Barry,J. Barthel,D. Bauer,Peter Bauer,A. Baxter,J. Belle,P. Beltrame,J. R. Bensinger,T. Benson,Ethan Bernard,Ethan Bernard,Adam Bernstein,A. Bhatti,A. Biekert,A. Biekert,T. P. Biesiadzinski,B. Birrittella,K. E. Boast,Alexander Bolozdynya,E. M. Boulton,E. M. Boulton,B. Boxer,R. Bramante,S. Branson,P. Brás,Martin Breidenbach,J. H. Buckley,V. Bugaev,R. Bunker,Sergey Burdin,J. Busenitz,J. S. Campbell,C. Carels,Duncan Carlsmith,Ben Carlson,M. C. Carmona-Benitez,Michele Cascella,C. Chan,J. J. Cherwinka,A. A. Chiller,C. Chiller,N. I. Chott,A. Cole,J. P. Coleman,David Colling,R. Conley,A. Cottle,R. Coughlen,W. Craddock,D. Curran,A. Currie,J. E. Cutter,J.P. da Cunha,C. E. Dahl,C. E. Dahl,S. Dardin,Sridhara Dasu,J. C. Davis,T. J. R. Davison,L. de Viveiros,N. Decheine,A. Dobi,J. E. Y. Dobson,E. Druszkiewicz,A. Dushkin,T. K. Edberg,W. R. Edwards,B. N. Edwards,J. Edwards,M. Elnimr,W. T. Emmet,S. R. Eriksen,C. H. Faham,A. Fan,Simon Fayer,S. Fiorucci,Henning Flaecher,I. M. Fogarty Florang,P. Ford,V. B. Francis,F. Froborg,T. Fruth,R. J. Gaitskell,N.J. Gantos,D. Garcia,A. Geffre,V. M. Gehman,R. Gelfand,J. Genovesi,R.M. Gerhard,C. Ghag,Eli Gibson,M. G. D. Gilchriese,S. Gokhale,Bhawna Gomber,T. G. Gonda,A. Greenall,S. Greenwood,G. Gregerson,M. G. D. van der Grinten,Carl Gwilliam,C. R. Hall,D.S. Hamilton,S. Hans,K. Hanzel,T. Harrington,A. Harrison,C. Hasselkus,S. J. Haselschwardt,D. Hemer,S. A. Hertel,John Heise,Seth Hillbrand,O. Hitchcock,C. Hjemfelt,M. Hoff,B. Holbrook,E. Holtom,J. Y.K. Hor,M. Horn,D. Q. Huang,T.W. Hurteau,C. M. Ignarra,M. N. Irving,R. G. Jacobsen,R. G. Jacobsen,O. Jahangir,S. N. Jeffery,W. Ji,Mikkel B. Johnson,J. Johnson,P. Johnson,W. G. Jones,A. C. Kaboth,A. C. Kaboth,A. Kamaha,K. Kamdin,K. Kamdin,V. Kasey,Kareem Kazkaz,J. Keefner,D. Khaitan,M. Khaleeq,A. Khazov,A.V. Khromov,I. Khurana,Yeongduk Kim,W. T. Kim,C. D. Kocher,A. Konovalov,L. Korley,Elena Korolkova,M. Koyuncu,J. Kras,H. Kraus,S. Kravitz,H.J. Krebs,L. Kreczko,Benjamin Krikler,V. A. Kudryavtsev,A. V. Kumpan,S. Kyre,A. Lambert,B. Landerud,N. A. Larsen,A. Laundrie,E. Leason,H. S. Lee,Juhyeong Lee,C. Lee,B. G. Lenardo,David Leonard,R. Leonard,K. T. Lesko,C. Levy,J. Li,Yunpeng Liu,J. Liao,F.-T. Liao,J. Lin,J. Lin,A. Lindote,R. Linehan,W. H. Lippincott,R. Liu,X. Liu,C. Loniewski,M.I. Lopes,B. Lopez Paredes,Wolfgang Lorenzon,D. Lucero,S. Luitz,J. M. Lyle,Candace Lynch,P. Majewski,J. Makkinje,D.C. Malling,A. Manalaysay,Laura Manenti,R. L. Mannino,N. Marangou,D. Markley,P. MarrLaundrie,T.J. Martin,M. F. Marzioni,C. Maupin,C. T. McConnell,Daniel McKinsey,Daniel McKinsey,J. McLaughlin,Dongming Mei,Yue Meng,E. H. Miller,Z. J. Minaker,E. Mizrachi,J. Mock,J. Mock,D. Molash,A. Monte,M. E. Monzani,J. A. Morad,E. Morrison,B. J. Mount,A. St. J. Murphy,D. Naim,A. Naylor,C. Nedlik,C. Nehrkorn,H. N. Nelson,J. Nesbit,F. Neves,J. A. Nikkel,J. A. Nikoleyczik,A. Nilima,J. O'Dell,H. Oh,F. G. O'Neill,K. O’Sullivan,K. O’Sullivan,I. Olcina,M. A. Olevitch,K. C. Oliver-Mallory,K. C. Oliver-Mallory,L. Oxborough,A. Pagac,D. Pagenkopf,S. Pal,K. J. Palladino,V. M. Palmaccio,J. Palmer,M. Pangilinan,S. J. Patton,E. K. Pease,Bjoern Penning,G. Pereira,C. Pereira,I. B. Peterson,A. Piepke,S. Pierson,S. Powell,R. M. Preece,K. Pushkin,Y. Qie,M. Racine,B. N. Ratcliff,J. Reichenbacher,L. Reichhart,C. Rhyne,A. Richards,Q. Riffard,Q. Riffard,G. R. C. Rischbieter,J.P. Rodrigues,H. J. Rose,Richard Rosero,P. Rossiter,R. Rucinski,G. Rutherford,D. Rynders,J.S. Saba,L. Sabarots,D. Santone,M. Sarychev,A. B.M.R. Sazzad,R. W. Schnee,Michael Schubnell,P. R. Scovell,Mary Severson,D. Seymour,S. Shaw,G. W. Shutt,T. A. Shutt,J. J. Silk,C. Silva,K. Skarpaas,W. Skulski,A. R. Smith,Richard J. Smith,Richard J. Smith,R. E. Smith,J. So,M. Solmaz,V. N. Solovov,P. Sorensen,V.V. Sosnovtsev,I. Stancu,M.R. Stark,S. Stephenson,N. Stern,A. Stevens,T.M. Stiegler,K. Stifter,R. Studley,T. J. Sumner,K. Sundarnath,P. Sutcliffe,N. Swanson,Matthew Szydagis,M. Tan,W. C. Taylor,Robert A. Taylor,D. J. Taylor,D. Temples,B. P. Tennyson,P. A. Terman,K.J. Thomas,J. Thomson,D. R. Tiedt,M. Timalsina,W. H. To,A. Tomás,T. Tope,Mani Tripathi,D. R. Tronstad,C. E. Tull,W. Turner,L. Tvrznikova,L. Tvrznikova,M. Utes,U. Utku,S. Uvarov,J. Va’vra,Antonin Vacheret,A. Vaitkus,J.R. Verbus,T. Vietanen,E. Voirin,C. O. Vuosalo,S. Walcott,W.L. Waldron,Kathrin C. Walker,J. J. Wang,Ren-Jie Wang,L. Wang,Yufeng Wang,J. R. Watson,J. R. Watson,J. Migneault,S. Weatherly,R. C. Webb,Wenzhao Wei,M. R. While,Ross G. White,J. T. White,D. White,T. J. Whitis,T. J. Whitis,W. J. Wisniewski,K. Wilson,M. S. Witherell,M. S. Witherell,F.L.H. Wolfs,J. D. Wolfs,D. Woodward,S. D. Worm,X. Xiang,Q. Xiao,Jilei Xu,Minfang Yeh,J. Yin,Ian S. Young,Chao Zhang +398 more
TL;DR: The design and assembly of the LUX-ZEPLIN experiment, a direct detection search for cosmic WIMP dark matter particles, is described and its key design features and requirements are described.
Journal ArticleDOI
Global analyses of Higgs portal singlet dark matter models using GAMBIT
Peter Athron,Peter Athron,Csaba Balázs,Csaba Balázs,Ankit Beniwal,Sanjay Bloor,José Eliel Camargo-Molina,Jonathan M. Cornell,Ben Farmer,Andrew Fowlie,Andrew Fowlie,Andrew Fowlie,Tomás E. Gonzalo,Felix Kahlhoefer,Anders Kvellestad,Anders Kvellestad,Gregory D. Martinez,Pat Scott,Aaron C. Vincent,Sebastian Wild,Martin White,Martin White,Anthony G. Williams,Anthony G. Williams +23 more
TL;DR: In this article, the authors present global analyses of effective Higgs portal dark matter models in the frequentist and Bayesian statistical frameworks and use GAMBIT to determine the preferred mass and coupling ranges for models with vector, Majorana and Dirac fermion dark matter.
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Journal ArticleDOI
Review of Particle Physics
Keith A. Olive,Kaustubh Agashe,Claude Amsler,Mario Antonelli,Jean-Francois Arguin,D. M. Asner,Howard Baer,H. R. Band,R. M. Barnett,T. Basaglia,Christian W. Bauer,J. J. Beatty,V. L. Belousov,J. Beringer,G. Bernardi,Siegfried Bethke,H. Bichsel,Otmar Biebel,E. Blucher,S. Blusk,Gustaaf Brooijmans,Oliver Buchmueller,Volker D. Burkert,M A Bychkov,Robert N. Cahn,Marcela Carena,Marcela Carena,Augusto Ceccucci,Alessandro Cerri,Debadi Chakraborty,Mingshui Chen,R. S. Chivukula,K. Copie,G. A. Cowan,O. I. Dahl,Giancarlo D'Ambrosio,Thibault Damour,Daniel de Florian,A. de Gouvea,Thomas DeGrand,P. de Jong,G. Dissertori,Bogdan A. Dobrescu,Michael Doser,Manuel Drees,Herbert K. Dreiner,D. A. Edwards,Semen Eidelman,Jens Erler,Jens Erler,V. V. Ezhela,W. Fetscher,Brian D. Fields,B. Foster,B. Foster,A Freitas,Thomas K. Gaisser,H. R. Gallagher,L. A. Garren,H J Gerber,G. Gerbier,Timothy Gershon,Tony Gherghetta,Sunil Golwala,M. C. Goodman,Christoph Grab,Andrei Gritsan,C. Grojean,D. E. Groom,Martin Grunewald,Martin Grunewald,Atul Gurtu,Atul Gurtu,Th. Gutsche,Howard E. Haber,Howard E. Haber,K. Hagiwara,C. Hanhart,Shoji Hashimoto,Yoshinari Hayato,K. G. Hayes,M. Heffner,B. K. Heltsley,Juan José Hernández-Rey,Ken Ichi Hikasa,A Höcker,Jamie Holder,A Holtkamp,Joey Huston,John David Jackson,Kurtis F Johnson,T. R. Junk,Marumi Kado,Marumi Kado,D. Karlen,Uli Katz,S. R. Klein,Eberhard Klempt,R. Kowalewski,Frank Krauss,Michal Kreps,B. Krusche,Yu V. Kuyanov,Younghoon Kwon,Ofer Lahav,Jack Laiho,Paul Langacker,Andrew R. Liddle,Zoltan Ligeti,Chi Lin,T. M. Liss,L. S. Littenberg,K. S. Lugovsky,S. B. Lugovsky,Fabio Maltoni,T Mannel,Aneesh V. Manohar,William J. Marciano,Alan D. Martin,A. Masoni,John Matthews,David Milstead,Paolo Molaro,Klaus Mönig,Filip Moortgat,M. J. Mortonson,M. J. Mortonson,Hitoshi Murayama,Hitoshi Murayama,Hitoshi Murayama,Koji Nakamura,Meenakshi Narain,Paolo Nason,S. Sánchez Navas,Matthias Neubert,P. Nevski,Y. Nir,Luc Pape,J. A. Parsons,C. Patrignani,John A. Peacock,M. Pennington,S. T. Petcov,S. T. Petcov,A. Piepke,A Pomarol,Arnulf Quadt,Stuart Raby,Jonas Rademacker,Georg G. Raffelt,B. N. Ratcliff,Paul William Richardson,Andreas Ringwald,Stefan Roesler,S. Rolli,Anatoli Romaniouk,L. J. Rosenberg,Jonathan L. Rosner,G Rybka,C.T. Sachrajda,Y. Sakai,Gavin P. Salam,Gavin P. Salam,Subir Sarkar,Subir Sarkar,Fabio Sauli,O. Schneider,Kate Scholberg,Douglas Scott,Vivek Sharma,Stephen R. Sharpe,M. Silari,Torbjörn Sjöstrand,Peter Skands,Peter Skands,J. G. Smith,George F. Smoot,George F. Smoot,George F. Smoot,S. M. Spanier,H. Spieler,Christian Spiering,Achim Stahl,Todor Stanev,Sophia L. Stone,T. Sumiyoshi,Michael Syphers,F Takahashi,Masaharu Tanabashi,John Terning,L. Tiator,Maksym Titov,N. P. Tkachenko,Nils A. Tornqvist,Daniel Tovey,German Valencia,G. Venanzoni,Manuella Vincter,Petr Vogel,Andreas Vogt,S. P. Wakely,Wolfgang Walkowiak,C. W. Walter,D. R. Ward,Georg Weiglein,David H. Weinberg,E. J. Weinberg,Martin White,Martin White,L. R. Wiencke,C. G. Wohl,Lincoln Wolfenstein,J. Womersley,C. L. Woody,Ron L. Workman,A. Yamamoto,W-M. Yao,G P Zeller,Oleg Zenin,Jie Zhang,Ren-Yuan Zhu,Frank Zimmermann,P A Zyla,G. Harper,V. S. Lugovsky,P. Schaffner +225 more
TL;DR: The review as discussed by the authors summarizes much of particle physics and cosmology using data from previous editions, plus 3,283 new measurements from 899 Japers, including the recently discovered Higgs boson, leptons, quarks, mesons and baryons.
Journal ArticleDOI
Asymptotic formulae for likelihood-based tests of new physics
TL;DR: In this paper, the authors describe likelihood-based statistical tests for use in high energy physics for the discovery of new phenomena and for construction of confidence intervals on model parameters, focusing on the properties of the test procedures that allow one to account for systematic uncertainties.
Journal ArticleDOI
Results from a Search for Dark Matter in the Complete LUX Exposure
D. S. Akerib,S. Alsum,Henrique Araujo,X. Bai,A. J. Bailey,J. Balajthy,P. Beltrame,Ethan Bernard,A. Bernstein,T. P. Biesiadzinski,E. M. Boulton,R. Bramante,P. Brás,D. Byram,Sidney Cahn,M. C. Carmona-Benitez,C. Chan,A.A. Chiller,C. Chiller,A. Currie,J. E. Cutter,T. J. R. Davison,A. Dobi,J. E. Y. Dobson,E. Druszkiewicz,B. N. Edwards,C. H. Faham,S. Fiorucci,R. J. Gaitskell,V. M. Gehman,C. Ghag,K.R. Gibson,M. G. D. Gilchriese,C. R. Hall,M. Hanhardt,S. J. Haselschwardt,S. A. Hertel,D. P. Hogan,M. Horn,D. Q. Huang,C. M. Ignarra,M. Ihm,R.G. Jacobsen,W. Ji,K. Kamdin,K. Kazkaz,D. Khaitan,R. Knoche,N.A. Larsen,C. Lee,B. G. Lenardo,K. T. Lesko,A. Lindote,M.I. Lopes,A. Manalaysay,R. L. Mannino,M. F. Marzioni,Daniel McKinsey,D. M. Mei,J. Mock,M. Moongweluwan,J. A. Morad,A. St. J. Murphy,C. Nehrkorn,H. N. Nelson,F. Neves,K. O’Sullivan,K. C. Oliver-Mallory,K. J. Palladino,E. K. Pease,P. Phelps,L. Reichhart,C. Rhyne,S. Shaw,T. A. Shutt,C. Silva,M. Solmaz,V. N. Solovov,P. Sorensen,S. Stephenson,T. J. Sumner,Matthew Szydagis,D. J. Taylor,W. C. Taylor,B. P. Tennyson,P. A. Terman,D. R. Tiedt,W. H. To,Mani Tripathi,L. Tvrznikova,S. Uvarov,J.R. Verbus,R. C. Webb,J. T. White,T. J. Whitis,M. S. Witherell,F.L.H. Wolfs,Jilei Xu,K. Yazdani,Sarah Young,Chao Zhang +100 more
TL;DR: This search yields no evidence of WIMP nuclear recoils and constraints on spin-independent weakly interacting massive particle (WIMP)-nucleon scattering using a 3.35×10^{4} kg day exposure of the Large Underground Xenon experiment are reported.
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