Rare Radiative Decay b→X<SUB>s</SUB>γ in the Technicolor with Scalars Model

XIONG ZhaoHua; CHEN HeSheng; LU Liang; LU GongRu

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2024年10月30日

Chinese Physics C> 2000, Vol. 24> Issue(8) : 711-718

Rare Radiative Decay b→X_sγ in the Technicolor with Scalars Model

Institute of High Energy Physics,The Chinese Academy of Sciences,Beijing 100039,China2 Department of Physics,Henan Normal University,Xinxiang 453002,China

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Abstract：
The O(α_s) correction to the inclusive decay of b→X sγ is calculated in the technicolor model with scalars. We find that the deviation of the decay width from the standard model prediction can be reduced by as much as 50% when ALEPH experimental value is used. In particular,the CLEO measurement which corresponds to the 33% reduction gives more stringent constraint on the parameter space in the technicolor with scalars model than B-B mixing. The model predictions can be observable in the forthcoming few years with upgraded CLEO detector and B-factories.

References

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XIONG ZhaoHua, CHEN HeSheng, LU Liang and LU GongRu. Rare Radiative Decay b→X_sγ in the Technicolor with Scalars Model[J]. Chinese Physics C, 2000, 24(8): 711-718.

XIONG ZhaoHua, CHEN HeSheng, LU Liang and LU GongRu. Rare Radiative Decay b→X_sγ in the Technicolor with Scalars Model[J]. Chinese Physics C, 2000, 24(8): 711-718. shu

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Received: 1999-06-28
Revised: 1900-01-01

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沈阳化工大学材料科学与工程学院沈阳 110142

Rare Radiative Decay b→X_sγ in the Technicolor with Scalars Model

Corresponding author: XIONG ZhaoHua,

Institute of High Energy Physics,The Chinese Academy of Sciences,Beijing 100039,China2 Department of Physics,Henan Normal University,Xinxiang 453002,China

Received Date: 1999-06-28
Accepted Date: 1900-01-01
Available Online: 2000-08-05

Abstract: The O(α_s) correction to the inclusive decay of b→X sγ is calculated in the technicolor model with scalars. We find that the deviation of the decay width from the standard model prediction can be reduced by as much as 50% when ALEPH experimental value is used. In particular,the CLEO measurement which corresponds to the 33% reduction gives more stringent constraint on the parameter space in the technicolor with scalars model than B-B mixing. The model predictions can be observable in the forthcoming few years with upgraded CLEO detector and B-factories.