4.8 Article

First Dark Matter Search Results from the XENON1T Experiment

期刊

PHYSICAL REVIEW LETTERS
卷 119, 期 18, 页码 -

出版社

AMER PHYSICAL SOC
DOI: 10.1103/PhysRevLett.119.181301

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资金

  1. National Science Foundation
  2. Swiss National Science Foundation
  3. German Ministry for Education and Research
  4. Max Planck Gesellschaft
  5. Deutsche Forschungsgemeinschaft
  6. Netherlands Organisation for Scientific Research (NWO)
  7. NLeSC
  8. Weizmann Institute of Science
  9. I-CORE
  10. Pazy-Vatat
  11. Initial Training Network Invisibles (Marie Curie Actions) [PITNGA-2011-289442]
  12. Fundacao para a Ciencia e a Tecnologia
  13. Region des Pays de la Loire
  14. Knut and Alice Wallenberg Foundation
  15. Kavli Foundation
  16. Instituto Nazionale di Fisica Nucleare
  17. Wallenberg Academy Fellowship
  18. Laboratori Nazionali del Gran Sasso
  19. Direct For Mathematical & Physical Scien
  20. Division Of Physics [1413495, 1413358] Funding Source: National Science Foundation
  21. Direct For Mathematical & Physical Scien
  22. Division Of Physics [1413255, 1125897, 1209979] Funding Source: National Science Foundation

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We report the first dark matter search results from XENON1T, a similar to 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] keV(nr) energy range of interest for weakly interacting massive particle (WIMP) dark matter searches, the electronic recoil background was (1.93 +/- 0.25) x 10(-4) events/(kg x day x keV(ee)), 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/c(2), with a minimum of 7.7 x 10(-47) cm(2) for 35-GeV/c(2) WIMPs at 90% C.L.

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