On the Mass and the States of the Dark Mater Partcles

  • We discuss a category of stable dark matter particles which are weakly interacting and related to the superstructure of the universe.These particles may be degenerate fermions and the bosons near a high temperature state.In both cases,we deduce that the particle mass is ~10-1eV and the absolute value of its chemical potential is <<10-1eV.This result is not in contradiction with the dip phenomena of the ultra high energy primary cosmic ray spectrum at ~1015eV and ~1018eV.
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  • [1] 黄无量,高能物理与核物理,20(1996)409.[2]R.B.Tully,Ap.J.,303(1986)25;Ap.J.,323(1986)1.[3]M.J.Geler et al.,Science,246(1989)897.[4]T.J.Broadhurst et al.,Nature,343(1990)726.[5]L.D.Landau et al.,Statistical Physics,Pergamon Press,London,1958.[6]黄无量,高能物理与核物理,15(1991)1135.[7]S.Weinberg,Gravitation and Cosmology,J.Wiley,New York,1972.
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Huang Wuliang. On the Mass and the States of the Dark Mater Partcles[J]. Chinese Physics C, 1997, 21(4): 316-321.
Huang Wuliang. On the Mass and the States of the Dark Mater Partcles[J]. Chinese Physics C, 1997, 21(4): 316-321. shu
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Received: 1900-01-01
Revised: 1900-01-01
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On the Mass and the States of the Dark Mater Partcles

    Corresponding author: Huang Wuliang,
  • Institute of High Energy Physics,The Chinese Academy of Sciences,Beijing 100039

Abstract: We discuss a category of stable dark matter particles which are weakly interacting and related to the superstructure of the universe.These particles may be degenerate fermions and the bosons near a high temperature state.In both cases,we deduce that the particle mass is ~10-1eV and the absolute value of its chemical potential is <<10-1eV.This result is not in contradiction with the dip phenomena of the ultra high energy primary cosmic ray spectrum at ~1015eV and ~1018eV.

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