4.4 Article

The neutron background of the XENON100 dark matter search experiment

出版社

IOP Publishing Ltd
DOI: 10.1088/0954-3899/40/11/115201

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资金

  1. NSF
  2. DOE
  3. SNF
  4. UZH
  5. FCT
  6. Region des Pays de la Loire
  7. STCSM
  8. NSFC
  9. DFG
  10. Stichting voor Fundamenteel Onderzoek der Materie (FOM)
  11. Max Planck Society
  12. Weizmann Institute of Science
  13. LNGS
  14. STFC [ST/K001426/1, ST/K006770/1] Funding Source: UKRI
  15. Direct For Mathematical & Physical Scien
  16. Division Of Physics [1206061] Funding Source: National Science Foundation
  17. Division Of Physics
  18. Direct For Mathematical & Physical Scien [1104740] Funding Source: National Science Foundation
  19. Science and Technology Facilities Council [ST/K006770/1 DMUK, ST/K006770/1, 1376100, ST/K001426/1] Funding Source: researchfish

向作者/读者索取更多资源

TheXENON100 experiment, installed underground at the LaboratoriNazionali del Gran Sasso, aims to directly detect dark matter in the form of weakly interacting massive particles (WIMPs) via their elastic scattering off xenon nuclei. This paper presents a study on the nuclear recoil background of the experiment, taking into account neutron backgrounds from (alpha, n) reactions and spontaneous fission due to natural radioactivity in the detector and shield materials, as well as muon-induced neutrons. Based on MonteCarlo simulations and using measured radioactive contaminations of all detector components, we predict the nuclear recoil backgrounds for the WIMP search results published by theXENON100 experiment in 2011 and 2012, 0.11(-0.04)(+0.08) events and 0.17(-0.07)(+0.12) events, respectively, and conclude that they do not limit the sensitivity of the experiment.

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