First Dark Matter Search Results from the XENON1T Experiment

Open Access
Authors
  • F.D. Amaro
  • M. Anthony
  • F. Arneodo
  • P. Barrow
  • L. Baudis
  • B. Bauermeister
  • M.L. Benabderrahmane
  • T. Berger
  • P.A. Breur
  • A. Brown
  • A. Brown
  • S. Bruenner
  • G. Bruno
  • R. Budnik
  • L. Bütikofer
  • J. Calvén
  • J.M.R. Cardoso
  • M. Cervantes
  • D. Cichon
  • D. Coderre
  • A.P. Colijn
  • J. Conrad
  • J.P. Cussonneau
  • M.P. Decowski
  • P. de Perio
  • P. Di Gangi
  • A. Di Giovanni
  • S. Diglio
  • G. Eurin
  • J. Fei
  • A.D. Ferella
  • A. Fieguth
  • W. Fulgione
  • A. Gallo Rosso
  • M. Galloway
  • F. Gao
  • M. Garbini
  • R. Gardner
  • C. Geis
  • L.W. Goetzke
  • L. Grandi
  • Z. Greene
  • C. Grignon
  • C. Hasterok
  • E. Hogenbirk
  • A. Tiseni
  • XENON Collaboration
Publication date 03-11-2017
Journal Physical Review Letters
Article number 181301
Volume | Issue number 119 | 18
Number of pages 6
Organisations
  • Faculty of Science (FNWI) - Institute of Physics (IoP) - Institute for High Energy Physics (IHEF)
Abstract
We report the first dark matter search results from XENON1T, a ∼2000−kg-target-mass dual-phase (liquid-gas) xenon time projection chamber in operation at the Laboratori Nazionali del Gran Sasso in Italy and the first ton-scale detector of this kind. The blinded search used 34.2 live days of data acquired between November 2016 and January 2017. Inside the (1042±12)−kg fiducial mass and in the [5,40]  keVnr energy range of interest for weakly interacting massive particle (WIMP) dark matter searches, the electronic recoil background was (1.93±0.25)×10−4  events/(kg×day×keVee), the lowest ever achieved in such a dark matter detector. A profile likelihood analysis shows that the data are consistent with the background-only hypothesis. We derive the most stringent exclusion limits on the spin-independent WIMP-nucleon interaction cross section for WIMP masses above 10  GeV/c2, with a minimum of 7.7×10−47  cm2 for 35−GeV/c2 WIMPs at 90% C.L.
Document type Article
Language English
Published at https://doi.org/10.1103/PhysRevLett.119.181301
Downloads
PhysRevLett.119.181301 (Final published version)
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