Inclusive η′ Production in B Decays and the Enhancement Due to Charged Technipions

  • We calculate the new contribuhons to the charmless B decay B→Xsη′ via the QCD gluon anomaly and the enhanced b→sg decay due to the charged technipions appeared in Technicolor Model. Widen the considered paraxneter space the new physics contribuhon can result in a large enhancement to the inclusive η′ produchon and in tUrn to account for the CLEO data of Br(B→η′Xs).
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  • [1] CLEO Collaborahon, Browder T E et a]. phys. Rev. Lett., 1998, 81. 17862 Halperin I, Zhitnistsky A. Phys. Rev. Lett., 1998, 80:438;Halperin I,Zhitnitsky A, Phys. Rev., 1997, D56:7247 3 Atwood D D, Soni A, Phys. Lett, 1997, B405:150; Fritzsch H. Phys. Lett. 1997, B415:83 4 Hou W S, Tseng B. Phys. Rev. Lett., 1997, 80:4345 Kagan A L, Petrov A A. hep–ph / 9707354 6 Yuan F, Chao K T. Phys. Rev., 1997, D56: R2459 7 Du D S, Kim C S, Yang Y D. Phys. Lett., 1998, B426: 133; Ahmady M R. Kou E, Sugamoto A. Phys.Rev., 1998, D58: 0140158 Hou W S. Nucl. Phys., 1988, B308:5619 Farhi E, Susskind L. Phys. Rev., 1979 D20:340410 Ellis J, Gailaard M K, Nanopoulous D V et al. Nucl. Phys. 1981, B187:541; Eichten E, Hinchilffe I, LaneK et al. Rev. Mod. Phys., 1984, 56: 579; Phys. Rev., 1986, D34: 1547; For the Current status ofTechnicolor Theories see paper: X Lane, ICHEP96, 1996, 367–37811 Lü C D, Xiao Z J. Phys. Rev. 1996, D53:2529 12 CLEO Collaborahon, Coan T E et al. Phys. Rev. Lett, 1998, 80: 1150
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Lu Gongru, Xiao Zhenjun, Guo Hongkai and Lv Linxia. Inclusive η′ Production in B Decays and the Enhancement Due to Charged Technipions[J]. Chinese Physics C, 1999, 23(12): 1158-1162.
Lu Gongru, Xiao Zhenjun, Guo Hongkai and Lv Linxia. Inclusive η′ Production in B Decays and the Enhancement Due to Charged Technipions[J]. Chinese Physics C, 1999, 23(12): 1158-1162. shu
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Received: 1998-10-05
Revised: 1900-01-01
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Inclusive η′ Production in B Decays and the Enhancement Due to Charged Technipions

    Corresponding author: Lu Gongru,
  • Departwnt of Physics, Henan Normal University, Xinxiang,453002

Abstract: We calculate the new contribuhons to the charmless B decay B→Xsη′ via the QCD gluon anomaly and the enhanced b→sg decay due to the charged technipions appeared in Technicolor Model. Widen the considered paraxneter space the new physics contribuhon can result in a large enhancement to the inclusive η′ produchon and in tUrn to account for the CLEO data of Br(B→η′Xs).

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