We report on a search for weakly interacting massive particles (WIMPs) using 278.8 days of data collected with the XENON1T experiment at LNGS. XENON1T utilizes a liquid xenon time projection chamber with a fiducial mass of (1.30 +/- 0.01) ton, resulting in a 1.0 ton yr exposure. The energy region of interest, [1.4; 10.6] keV(ee) ([4.9; 40.9] keV(nr)), exhibits an ultralow electron recoil background rate of [82(-3)(+5) (syst) +/- 3 stat)] events/ton yr keV(ee)). No significant excess over background is found, and a profile likelihood analysis parametrized in spatial and energy dimensions excludes new parameter space for the WIMP-nucleon spin-independent elastic scatter cross section for WIMP masses above 6 GeV/c(2), with a minimum of 4.1 x 10(-47) cm(2) at 30 GeV/c(2) and a 90% confidence level.
Journal article
Dark Matter Search Results from a One Ton-Year Exposure of XENON1T
Physical Review Letters, Vol.121(11), 111302
12/Sep/2018
Abstract
Details
- Title
- Dark Matter Search Results from a One Ton-Year Exposure of XENON1T
- Creators
- XENON Dark Matter Research Project (Institution)E. Aprile (null) - Columbia UniversityJ. Aalbers (null) - University of AmsterdamF. Agostini (null) - INFN Sezione di BolognaM. Alfonsi (null) - Johannes Gutenberg University MainzL. Althueser (null) - University of MünsterF. D. Amaro (null) - Universidade de CoimbraM. Anthony (null) - Columbia UniversityF. Arneodo (null) - New York University Abu DhabiL. Baudis (null) - University of ZurichB. Bauermeister (null) - Stockholm UniversityM. L. Benabderrahmane (null) - New York University Abu DhabiT. Berger (null) - Rensselaer Polytechnic InstituteP. A. Breur (null) - University of AmsterdamA. Brown (null) - University of AmsterdamA. Brown (null) - University of ZurichE. Brown (null) - Rensselaer Polytechnic InstituteS. Bruenner (null) - Max Planck Institute for Nuclear PhysicsG. Bruno (null) - New York University Abu DhabiR. Budnik (null) - 972WIS_INST___88C. Capelli (null) - University of ZurichJ. M. R. Cardoso (null) - Universidade de CoimbraD. Cichon (null) - Max Planck Institute for Nuclear PhysicsD. Coderre (Corresponding Author) - University of FreiburgA. P. Colijn (null) - University of AmsterdamJ. Conrad (null) - Stockholm UniversityJ. P. Cussonneau (null) - Université Bretagne LoireM. P. Decowski (null) - University of AmsterdamP. de Perio (null) - Columbia UniversityP. Di Gangi (null) - INFN Sezione di BolognaA. Di Giovanni (null) - New York University Abu DhabiS. Diglio (null) - Université Bretagne LoireA. Elykov (null) - University of FreiburgG. Eurin (null) - Max Planck Institute for Nuclear PhysicsJ. Fei (null) - University of California, San DiegoA. D. Ferella (null) - Stockholm UniversityA. Fieguth (null) - University of MünsterW. Fulgione (null) - Osservatorio Astrofisico di TorinoA. Gallo Rosso (null) - Istituto Nazionale di Fisica Nucleare, Gran Sasso Sci InstM. Galloway (null) - University of ZurichF. Gao (null) - Columbia UniversityM. Garbini (null) - INFN Sezione di BolognaH. Qiu (null) - 972WIS_INST___88R. Itay (null) - 972WIS_INST___88G. Koltman (null) - 972WIS_INST___88H. Landsman (null) - 972WIS_INST___88L. Levinson (null) - 972WIS_INST___91A. Manfredini (null) - 972WIS_INST___88N. Priel (null) - 972WIS_INST___122H. Wang (null) - 972WIS_INST___99Y. Zhang (null) - The Weizmann Institute of Science
- Resource Type
- Journal article
- Publication Details
- Physical Review Letters, Vol.121(11), 111302; 12/Sep/2018
- Number of pages
- 8
- Language
- English
- DOI
- https://doi.org/10.1103/PhysRevLett.121.111302
- Grant note
- We gratefully acknowledge support from the National Science Foundation, Swiss National Science Foundation, German Ministry for Education and Research, Max Planck Gesellschaft, Deutsche Forschungsgemeinschaft, Netherlands Organisation for Scientific Research (NWO), NLeSC, Weizmann Institute of Science, I-CORE, Pazy-Vatat, Initial Training Network Invisibles (Marie Curie Actions, No. PITNGA-2011-289442), Fundacao para a Ciencia e a Tecnologia, Region des Pays de la Loire, Knut and Alice Wallenberg Foundation, Kavli Foundation, and Istituto Nazionale di Fisica Nucleare. Data processing is performed using infrastructures from the Open Science Grid and European Grid Initiative. We are grateful to Laboratori Nazionali del Gran Sasso for hosting and supporting the XENON project.
- Record Identifier
- 993261838403596
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