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JUNO sensitivity to the annihilation of MeV dark matter in the galactic halo

  • The JUNO Collaboration
  • Pontificia Universidad Católica de Chile
  • Millennium Institute for SubAtomic Physics at the High-energy Frontier (SAPHIR)
  • Millennium Institute for Subatomic physics at high energy frontier (SAPHIR)
  • Université de Strasbourg
  • Pakistan Institute of Nuclear Science and Technology
  • Università degli Studi di Catania
  • III. Physikalisches Institut A
  • RWTH Aachen University
  • East China University of Science and Technology
  • University of Science and Technology of China
  • Joint Institute for Nuclear Research, Dubna
  • University of Milano
  • Department of Physics
  • Chulalongkorn University
  • Université Paris-Saclay
  • Sun Yat-Sen University
  • Department of Physics and Earth Science
  • University of Ferrara
  • University of Milano-Bicocca
  • INFN
  • Physikalisches Institut
  • University of Tübingen
  • Institute of High Energy Physics, Chinese Academy of Sciences
  • Université de Nantes
  • Department of Physics
  • National Taiwan University
  • UMR 5797
  • University of Padova
  • University Roma Tre
  • Aix-Marseille Université
  • Wuhan University
  • Politecnico di Milano

Research output: Contribution to journalArticlepeer-review

12 Citations (Scopus)

Abstract

We discuss JUNO sensitivity to the annihilation of MeV dark matter in the galactic halo via detecting inverse beta decay reactions of electron anti-neutrinos resulting from the annihilation. We study possible backgrounds to the signature, including the reactor neutrinos, diffuse supernova neutrino background, charged- and neutral-current interactions of atmospheric neutrinos, backgrounds from muon-induced fast neutrons and cosmogenic isotopes. A fiducial volume cut, as well as the pulse shape discrimination and the muon veto are applied to suppress the above backgrounds. It is shown that JUNO sensitivity to the thermally averaged dark matter annihilation rate in 10 years of exposure would be significantly better than the present-day best limit set by Super-Kamiokande and would be comparable to that expected by Hyper-Kamiokande.

Original languageEnglish
Article number001
JournalJournal of Cosmology and Astroparticle Physics
Volume2023
Issue number9
DOIs
Publication statusPublished - 1 Sept 2023
Externally publishedYes

Keywords

  • neutrino astronomy
  • neutrino detectors
  • neutrino experiments

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