4.7 Article

Dark photon search in the mass range between 1.5 and 3.4 GeV/c

期刊

PHYSICS LETTERS B
卷 774, 期 -, 页码 252-257

出版社

ELSEVIER
DOI: 10.1016/j.physletb.2017.09.067

关键词

Dark photon search; Initial state radiation; BESIII

资金

  1. National Key Basic Research Program of China [2015CB856700]
  2. National Natural Science Foundation of China (NSFC) [11235011, 11335008, 11425524, 11625523, 11635010]
  3. Chinese Academy of Sciences (CAS) Large-Scale Scientific Facility Program
  4. CAS Center for Excellence in Particle Physics (CCEPP)
  5. Joint Large-Scale Scientific Facility Fund of the NSFC
  6. Joint Large-Scale Scientific Facility Funds of the CAS [U1332201, U1532257, U1532258, KJCX2-YW-N29, KJCX2-YW-N45, QYZDJ-SSW-SLH003]
  7. 100 Talents Program of CAS
  8. National 1000 Talents Program of China
  9. Shanghai Key Laboratory for Particle Physics and Cosmology
  10. German Research Foundation DFG [CRC 1044, FOR 2359]
  11. Istituto Nazionale di Fisica Nucleare, Italy
  12. Koninklijke Nederlandse Akademie van Wetenschappen (KNAW) [530-4CDP03]
  13. Ministry of Development of Turkey [DPT2006K-120470]
  14. National Science and Technology fund
  15. Swedish Resarch Council
  16. U.S. Department of Energy [DE-FG02-05ER41374, DE-SC-0010118, DE-SC-0010504, DE-SC-0012069]
  17. University of Groningen (RuG)
  18. Helmholtzzentrum fuer Schwerionenforschung GmbH (GSI), Darmstadt
  19. WCU Program of National Research Foundation of Korea [R32-2008-000-10155-0]
  20. INPAC

向作者/读者索取更多资源

Using a data set of 2.93 fb taken at a center-of-mass energy root s = 3.773 GeV with the BESIII detector at the BEPCII collider, we perform a search for an extra U(1) gauge boson, also denoted as a dark photon. We examine the initial state radiation reactions e(+)e(-) -> e(+)e(-) gamma(ISR) and e(+)e(-) -> mu(+)mu(-) gamma(ISR) for this search, where the dark photon would appear as an enhancement in the invariant mass distribution of the leptonic pairs. We observe no obvious enhancement in the mass range between 1.5 and 3.4 GeV/c(2) and set a 90% confidence level upper limit on the mixing strength of the dark photon and the Standard Model photon. We obtain a competitive limit in the tested mass range. (c) 2017 The Author(s). Published by Elsevier B.V.

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