Antiproton Spectrum Produced by Dark Matter Annihilation

  • The cross section of the process X-0X-0→gg is calculated in supersymmetry model of parti- cle physics. By means of the obtained cross section value, the estimate of source spectrum for anti- protons produced by neutralino X-0 annihilation is given. We conclude that the observation of this spectrum in the low energy region offers a possible approach to find the dark matter and the super- symmetry particle.
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SUN La-Zhen, LIU Yao-Yang and JIANG Xiang-Dong. Antiproton Spectrum Produced by Dark Matter Annihilation[J]. Chinese Physics C, 2001, 25(10): 952-957.
SUN La-Zhen, LIU Yao-Yang and JIANG Xiang-Dong. Antiproton Spectrum Produced by Dark Matter Annihilation[J]. Chinese Physics C, 2001, 25(10): 952-957. shu
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Received: 2000-12-14
Revised: 1900-01-01
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Antiproton Spectrum Produced by Dark Matter Annihilation

    Corresponding author: SUN La-Zhen,
  • Department of modern Physics, University of Science and Technology of China, Hefei 230027, china2 Institute of High Energy Physics,Academy of Sciences of China, Beijing 100039,China

Abstract: The cross section of the process X-0X-0→gg is calculated in supersymmetry model of parti- cle physics. By means of the obtained cross section value, the estimate of source spectrum for anti- protons produced by neutralino X-0 annihilation is given. We conclude that the observation of this spectrum in the low energy region offers a possible approach to find the dark matter and the super- symmetry particle.

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