Results on the Spin-Dependent Scattering of Weakly Interacting Massive Particles on Nucleons from the Run 3 Data of the LUX Experiment.
D. S. Akerib,Henrique Araujo,X. Bai,A. J. Bailey,J. Balajthy,P. Beltrame,Ethan Bernard,A. Bernstein,T. P. Biesiadzinski,E. M. Boulton,A. W. Bradley,R. Bramante,Sidney Cahn,M. C. Carmona-Benitez,C. Chan,J.J. Chapman,A.A. Chiller,C. Chiller,A. Currie,J. E. Cutter,T. J. R. Davison,L. de Viveiros,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. Kazkaz,D. Khaitan,R. Knoche,N.A. Larsen,C. Lee,B. G. Lenardo,K. T. Lesko,A. Lindote,M.I. Lopes,D.C. Malling,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,R. A. Ott,K. J. Palladino,M. Pangilinan,E. K. Pease,P. Phelps,L. Reichhart,C. Rhyne,S. Shaw,T. A. Shutt,C. Silva,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,Michael S. Witherell,F.L.H. Wolfs,K. Yazdani,Sarah Young,Chao Zhang +100 more
TLDR
The spin-dependent WIMP-neutron limit is the most sensitive constraint to date.Abstract:
We present experimental constraints on the spin-dependent WIMP (weakly interacting massive particle)-nucleon elastic cross sections from LUX data acquired in 2013. LUX is a dual-phase xenon time projection chamber operating at the Sanford Underground Research Facility (Lead, South Dakota), which is designed to observe the recoil signature of galactic WIMPs scattering from xenon nuclei. A profile likelihood ratio analysis of 1.4×10^{4} kg day of fiducial exposure allows 90% C.L. upper limits to be set on the WIMP-neutron (WIMP-proton) cross section of σ_{n}=9.4×10^{-41} cm^{2} (σ_{p}=2.9×10^{-39} cm^{2}) at 33 GeV/c^{2}. The spin-dependent WIMP-neutron limit is the most sensitive constraint to date.read more
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The waning of the WIMP? A review of models, searches, and constraints
Giorgio Arcadi,Maíra Dutra,Pradipta Ghosh,Manfred Lindner,Yann Mambrini,Mathias Pierre,Stefano Profumo,Farinaldo S. Queiroz +7 more
TL;DR: A review of the WIMP paradigm with focus on a few models which can be probed at best by these facilities, and Collider and Indirect Detection will not be neglected when they represent a complementary probe.
Journal ArticleDOI
DARWIN: towards the ultimate dark matter detector
Jelle Aalbers,F. Agostini,M. Alfonsi,F. D. Amaro,Claude Amsler,Elena Aprile,Lior Arazi,F. Arneodo,P. Barrow,Laura Baudis,Laura Baudis,M. L. Benabderrahmane,T. Berger,B. Beskers,Amos Breskin,P. A. Breur,April S. Brown,Ethan Brown,S. Bruenner,Giacomo Bruno,Ran Budnik,Lukas Bütikofer,J. Calvén,João Cardoso,D. Cichon,D. Coderre,Auke-Pieter Colijn,Jan Conrad,Jean-Pierre Cussonneau,M. P. Decowski,Sara Diglio,Guido Drexlin,Ehud Duchovni,E. Erdal,G. Eurin,A. D. Ferella,A. Fieguth,W. Fulgione,A. Gallo Rosso,P. Di Gangi,A. Di Giovanni,Michelle Galloway,M. Garbini,C. Geis,F. Glueck,L. Grandi,Z. Greene,C. Grignon,C. Hasterok,Volker Hannen,E. Hogenbirk,J. Howlett,D. Hilk,C. Hils,A. James,B. Kaminsky,Shingo Kazama,Benjamin Kilminster,A. Kish,Lawrence M. Krauss,H. Landsman,R. F. Lang,Qing Lin,F. L. Linde,Sebastian Lindemann,Manfred Lindner,J. A. M. Lopes,Marrodan T. Undagoitia,Julien Masbou,F. V. Massoli,D. Mayani,M. Messina,K. Micheneau,A. Molinario,K. Morå,E. Morteau,M. Murra,J. Naganoma,Jayden L. Newstead,Kaixuan Ni,Uwe Oberlack,P. Pakarha,Bart Pelssers,P. de Perio,R. Persiani,F. Piastra,M.-C. Piro,G. Plante,L. Rauch,S. Reichard,A. Rizzo,N. Rupp,J.M.F. dos Santos,G. Sartorelli,M. Scheibelhut,S. Schindler,Marc Schumann,Marc Schumann,Jochen Schreiner,L. Scotto Lavina,M. Selvi,P. Shagin,Miguel Silva,Hardy Simgen,P. Sissol,M. von Sivers,D. Thers,J. Thurn,A. Tiseni,Roberto Trotta,C. Tunnell,Kathrin Valerius,M. Vargas,Hongwei Wang,Yuehuan Wei,Ch. Weinheimer,T. Wester,J. Wulf,Yanxi Zhang,T. Zhu,Kai Zuber +120 more
TL;DR: DARk matter WImp search with liquid xenoN (DARWIN) as mentioned in this paper is an experiment for the direct detection of dark matter using a multi-ton liquid xenon time projection chamber at its core.
Journal ArticleDOI
Improved limits on scattering of weakly interacting massive particles from reanalysis of 2013 LUX data
D. S. Akerib,Henrique Araujo,X. Bai,A. J. Bailey,J. Balajthy,P. Beltrame,Ethan Bernard,A. Bernstein,T. P. Biesiadzinski,E. M. Boulton,A. W. Bradley,R. Bramante,Sidney Cahn,M. C. Carmona-Benitez,C. Chan,J.J. Chapman,A.A. Chiller,C. Chiller,A. Currie,J. E. Cutter,T. J. R. Davison,L. de Viveiros,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. Kazkaz,D. Khaitan,R. Knoche,N.A. Larsen,C. Lee,B. G. Lenardo,K. T. Lesko,A. Lindote,M.I. Lopes,D.C. Malling,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,R. A. Ott,K. J. Palladino,M. Pangilinan,E. K. Pease,P. Phelps,L. Reichhart,C. Rhyne,S. Shaw,T. A. Shutt,C. Silva,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,K. Yazdani,Sarah Young,Chao Zhang +100 more
TL;DR: This new analysis incorporates several advances: single-photon calibration at the scintillation wavelength, improved event-reconstruction algorithms, a revised background model including events originating on the detector walls in an enlarged fiducial volume, and new calibrations from decays of an injected tritium β source and from kinematically constrained nuclear recoils down to 1.1 keV.
Journal ArticleDOI
WIMP dark matter candidates and searches—current status and future prospects
TL;DR: The present experimental status of dark matter theory and experiment is overview, which includes current bounds and recent claims and hints of a possible signal in a wide range of experiments: direct detection in underground laboratories, gamma-ray, cosmic ray, x-rays, neutrino telescopes, and the LHC.
Journal ArticleDOI
First results from the CRESST-III low-mass dark matter program
A. H. Abdelhameed,G. Angloher,Peter Bauer,A. Bento,E. Bertoldo,C. Bucci,L. Canonica,A. D'Addabbo,X. Defay,S. Di Lorenzo,A. Erb,F. v. Feilitzsch,S. Fichtinger,N. Ferreiro Iachellini,A. Fuss,P. Gorla,D. Hauff,J. Jochum,A. Kinast,H. Kluck,H. Kraus,A. Langenkämper,M. Mancuso,V. Mokina,E. Mondragon,A. Münster,M. Olmi,T. Ortmann,C. Pagliarone,L. Pattavina,F. Petricca,W. Potzel,F. Pröbst,F. Reindl,J. Rothe,K. Schäffner,Jochen Schieck,V. Schipperges,D. Schmiedmayer,S. Schönert,C. Schwertner,M. Stahlberg,Leo Stodolsky,C. Strandhagen,R. Strauss,C. Türkoglu,I. Usherov,M. Willers,V. Zema +48 more
TL;DR: In this article, the authors describe the analysis of one detector operated in the first run of CRESST-III (05/2016-02/2018) achieving a nuclear recoil threshold of 30.1 eV. This result was obtained with a 23.6 g CaWO4 crystal operated as a cryogenic scintillating calorimeter.
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Dark Matter Candidates from Particle Physics and Methods of Detection
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