Non-constancy and the Effect of Nuclear Environment of K-Factors in p-N(A) Drell-Yan Process

  • Based on the next leading order (NLO) perturbative QCD calculation and adopted parton distribution functions from double Q2 rescaling model (DQ2RM) in nuclei, we have discussed the variation of K-factors in p N(A) Drell-Yan process. Our results show that K-factors could not be treated as constants as usual, but are varied markedly with the kinimatic variable xT(A). In the ISR and SppS energy regions, when 2×10-3≤ xT(A)<1, K-factors decrease markedly as xT(A) becomes smaller, but after xT(A)<2×10-3, Their values increase rapidly as xT(A) further decrease. K-factor has a little dependence on nucleon number A of a nuclei also, and their effects are more clear in small xT(A) region. These observations are important for stringent test of some models and some physical quanties with Drell-Yan (Drell-Yan like) process in super high energy regions.
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LIU ChunXiu, HE ZhenMin, DUAN ChunGui and PENG HongAn. Non-constancy and the Effect of Nuclear Environment of K-Factors in p-N(A) Drell-Yan Process[J]. Chinese Physics C, 2000, 24(2): 131-139.
LIU ChunXiu, HE ZhenMin, DUAN ChunGui and PENG HongAn. Non-constancy and the Effect of Nuclear Environment of K-Factors in p-N(A) Drell-Yan Process[J]. Chinese Physics C, 2000, 24(2): 131-139. shu
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Received: 1998-12-02
Revised: 1900-01-01
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Non-constancy and the Effect of Nuclear Environment of K-Factors in p-N(A) Drell-Yan Process

    Corresponding author: LIU ChunXiu,
  • Department of Physics, Shandong University, Ji’nan 250100, China2 Department of Physics, Hebei Teacher′s University, Shijiazhuang 050016, China3 Department of Physics, Peking University, Beijing 100871, China

Abstract: Based on the next leading order (NLO) perturbative QCD calculation and adopted parton distribution functions from double Q2 rescaling model (DQ2RM) in nuclei, we have discussed the variation of K-factors in p N(A) Drell-Yan process. Our results show that K-factors could not be treated as constants as usual, but are varied markedly with the kinimatic variable xT(A). In the ISR and SppS energy regions, when 2×10-3≤ xT(A)<1, K-factors decrease markedly as xT(A) becomes smaller, but after xT(A)<2×10-3, Their values increase rapidly as xT(A) further decrease. K-factor has a little dependence on nucleon number A of a nuclei also, and their effects are more clear in small xT(A) region. These observations are important for stringent test of some models and some physical quanties with Drell-Yan (Drell-Yan like) process in super high energy regions.

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