Search for Electronic Recoil Event Rate Modulation with 4 Years of XENON100 Data

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
  • E. 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
  • D. Franco
  • W. Fulgione
  • A. Gallo Rosso
  • M. Galloway
  • F. Gao
  • M. Garbini
  • C. Geis
  • L.W. Goetzke
  • Z. Greene
  • C. Grignon
  • C. Hasterok
  • E. Hogenbirk
  • R. Itay
  • B. Kaminsky
  • XENON Collaboration
Publication date 10-03-2017
Journal Physical Review Letters
Article number 101101
Volume | Issue number 118 | 10
Number of pages 6
Organisations
  • Faculty of Science (FNWI) - Institute of Physics (IoP) - Institute for High Energy Physics (IHEF)
Abstract

We report on a search for electronic recoil event rate modulation signatures in the XENON100 data accumulated over a period of 4 yr, from January 2010 to January 2014. A profile likelihood method, which incorporates the stability of the XENON100 detector and the known electronic recoil background model, is used to quantify the significance of periodicity in the time distribution of events. There is a weak modulation signature at a period of 431-14+16 day in the low energy region of (2.0-5.8) keV in the single scatter event sample, with a global significance of 1.9σ; however, no other more significant modulation is observed. The significance of an annual modulation signature drops from 2.8σ, from a previous analysis of a subset of this data, to 1.8σ with all data combined. Single scatter events in the low energy region are thus used to exclude the DAMA/LIBRA annual modulation as being due to dark matter electron interactions via axial vector coupling at 5.7σ.

Document type Article
Note © 2017 American Physical Society
Language English
Published at https://doi.org/10.1103/PhysRevLett.118.101101
Other links https://www.scopus.com/pages/publications/85015038881
Downloads
PhysRevLett.118.101101 (Final published version)
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