Estimate of BR(B -> X_s gamma) at O(alpha_s^2)

Estimate of BR(B -> X_s gamma) at O(alpha_s^2)
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DOI:
10.1103/physrevlett.98.022002
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发表时间:
2006-09
影响因子:
8.6
通讯作者:
M. Misiak;H. Asatrian;K. Bieri;M. Czakon;A. Czarnecki;T. Ewerth;A. Ferroglia;P. Gambino;M. Gorbahn;C. Greub;U. Haisch;A. Hovhannisyan;T. Hurth;A. Mitov;Poghosyan;M. Ślusarczyk;M. Steinhauser
M. Misiak;H. Asatrian;K. Bieri;M. Czakon;A. Czarnecki;T. Ewerth;A. Ferroglia;P. Gambino;M. Gorbahn;C. Greub;U. Haisch;A. Hovhannisyan;T. Hurth;A. Mitov;Poghosyan;M. Ślusarczyk;M. Steinhauser
中科院分区:
物理与天体物理1区
文献类型:
--
作者:
M. Misiak;H. Asatrian;K. Bieri;M. Czakon;A. Czarnecki;T. Ewerth;A. Ferroglia;P. Gambino;M. Gorbahn;C. Greub;U. Haisch;A. Hovhannisyan;T. Hurth;A. Mitov;Poghosyan;M. Ślusarczyk;M. Steinhauser

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结合我们对弱辐射B介子衰变的各种O(α_s^2)修正的结果,我们能够给出QCD中次-次-首阶分支比的第一个估计。在B介子静止系中,当E_gamma > 1.6 GeV时,我们发现BR(B -> X_s gamma)=(3.15 +_ 0.23)x 10^-4.四种不确定度:非摄动不确定度(5%)、参数不确定度(3%)、高阶不确定度(3%)和mc插值模糊度(3%)被正交相加以获得总误差。
Combining our results for various O(alpha_s^2) corrections to the weak radiative B-meson decay, we are able to present the first estimate of the branching ratio at the next-to-next-to-leading order in QCD. We find BR(B -> X_s gamma) = (3.15 +_ 0.23) x 10^-4 for E_gamma > 1.6 GeV in the B-meson rest frame. The four types of uncertainties: non-perturbative (5%), parametric (3%), higher-order (3%) and m_c-interpolation ambiguity (3%) have been added in quadrature to obtain the total error.