The Source of Anomalous Positrons in the Cosmic Rays Above 10GeV

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CHEN Feng-Zhi, NIE Chuan-Hui and WANG Ping. The Source of Anomalous Positrons in the Cosmic Rays Above 10GeV[J]. Chinese Physics C, 1991, 15(6): 504-509.
CHEN Feng-Zhi, NIE Chuan-Hui and WANG Ping. The Source of Anomalous Positrons in the Cosmic Rays Above 10GeV[J]. Chinese Physics C, 1991, 15(6): 504-509. shu
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Received: 1900-01-01
Revised: 1900-01-01
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The Source of Anomalous Positrons in the Cosmic Rays Above 10GeV

    Corresponding author: CHEN Feng-Zhi,
  • Department of Physics,Anhui Normal University,Wuhu 2410001 Institute of High Energy Physics,Academia Sinica,Beijing 100039

Abstract: We suggest that the heavy neutral lepton in a specific version of SU(3)L×U(1) model can not only act as dark matter but also provide with a source of anomalous positrons in the cosmic rays above 10GeV.

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