4.7 Article

Emission of single and few electrons in XENON1T and limits on light dark matter

期刊

PHYSICAL REVIEW D
卷 106, 期 2, 页码 -

出版社

AMER PHYSICAL SOC
DOI: 10.1103/PhysRevD.106.022001

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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. Helmholtz Association
  7. Dutch Research Council (NWO)
  8. Weizmann Institute of Science
  9. Israeli Science Foundation
  10. Fundacao para a Ciencia e a Tecnologia
  11. Region des Pays de la Loire
  12. Knut and Alice Wallenberg Foundation
  13. Kavli Foundation
  14. JSPS Kakenhi in Japan
  15. Istituto Nazionale di Fisica Nucleare
  16. European Union [860881]
  17. SURF Cooperative
  18. Marie Curie Actions (MSCA) [860881] Funding Source: Marie Curie Actions (MSCA)

向作者/读者索取更多资源

This paper examines the origins of delayed single- and few-electron emissions in dual-phase time projection chambers. After removing correlated backgrounds, the observed event rates for 1 to 5 electrons are <30 events/(electron x kg x day). The study also derives 90% confidence upper limits for dark matter-electron scattering, electric dipole, magnetic dipole, anapole interactions, as well as exclusion of new parameter space for dark photons and solar dark photons.
Delayed single- and few-electron emissions plague dual-phase time projection chambers, limiting their potential to search for light-mass dark matter. This paper examines the origins of these events in the XENON1T experiment. Characterization of the intensity of delayed electron backgrounds shows that the resulting emissions are correlated, in time and position, with high-energy events and can effectively be vetoed. In this work we extend previous S2-only analyses down to a single electron. From this analysis, after removing the correlated backgrounds, we observe rates <30 events/(electron x kg x day) in the region of interest spanning 1 to 5 electrons. We derive 90% confidence upper limits for dark matter-electron scattering, first direct limits on the electric dipole, magnetic dipole, and anapole interactions, and bosonic dark matter models, where we exclude new parameter space for dark photons and solar dark photons.

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