4.7 Article

Study of the electromagnetic background in the XENON100 experiment

期刊

PHYSICAL REVIEW D
卷 83, 期 8, 页码 -

出版社

AMER PHYSICAL SOC
DOI: 10.1103/PhysRevD.83.082001

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资金

  1. National Science Foundation [PHY-03-02646, PHY-04-00596]
  2. CAREER [PHY-0542066]
  3. Department of Energy [DE-FG02-91ER40688]
  4. Swiss National Foundation SNF [20-118119]
  5. Volkswagen Foundation
  6. FCT [PTDC/FIS/100474/2008]
  7. Direct For Mathematical & Physical Scien
  8. Division Of Physics [0904224] Funding Source: National Science Foundation
  9. Division Of Physics
  10. Direct For Mathematical & Physical Scien [0705337] Funding Source: National Science Foundation
  11. Fundação para a Ciência e a Tecnologia [PTDC/FIS/100474/2008] Funding Source: FCT

向作者/读者索取更多资源

The XENON100 experiment, located at the Laboratori Nazionali del Gran Sasso, aims to directly detect dark matter in the form of weakly interacting massive particles via their elastic scattering off xenon nuclei. We present a comprehensive study of the predicted electronic recoil background coming from radioactive decays inside the detector and shield materials and intrinsic radioactivity in the liquid xenon. Based on GEANT4 Monte Carlo simulations using a detailed geometry together with the measured radioactivity of all detector components, we predict an electronic recoil background in the energy region of interest and 30 kg fiducial mass of less than 10(-2) events . kg(-1) . day(-1) . keV(-1), consistent with the experiment's design goal. The predicted background spectrum is in very good agreement with the data taken during the commissioning of the detector in Fall 2009.

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