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Axial vector transition form factors in holographic QCD and their contribution to the anomalous magnetic moment of the muon

机译:全息QCD的轴向矢量转变形式因子及其对μ子异常磁矩的贡献

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We evaluate axial vector transition form factors in holographic QCD models that have been shown to reproduce well recent experimental and theoretical results for the pion transition form factor. Comparing with L3 data on f 1 → γ γ * we find remarkable agreement regarding the shape of single-virtual form factors. In the double-virtual case, the holographic results differ strongly from a simple dipole form, and this has an important impact on the corresponding estimate of the axial vector contribution to the anomalous magnetic moment of the muon a μ through hadronic light-by-light scattering. We demonstrate that hard-wall models satisfy the Melnikov-Vainshtein short-distance constraint for the latter, if and only if the infinite tower of axial vector states is included. The results for a μ , however, are strongly dominated by the first few resonances. Numerically, these results turn out to be surprisingly large: ( 2.9 – 4.1 ) × 10 ? 10 in the hard-wall models, 57%–58% of which are due to the longitudinal contribution, which is the one responsible for the Melnikov-Vainshtein short-distance constraint. Rescaling the holographic result to obtain an optimal fit of L3 data, but then matching only 52% of the asymptotic constraint, the result is reduced to 2.2 ( 5 ) × 10 ? 10 , which is still significantly larger than most previous phenomenological estimates of the axial vector exchange contribution.
机译:我们评估全息QCD模型中的轴向矢量转变形式因子,该模型已被证明为再现最近的孔过渡外形的实验和理论结果。与F 1→γγ*上的L3数据进行比较,我们找到了关于单虚拟形式因子的形状的显着协议。在双虚拟情况下,全息结果从简单的偶极形式均匀地不同,这对轴向向量贡献的相应估计对通过HODRONIC亮光的轴向μm的异常磁矩的相应估计产生了重要的影响散射。我们展示了硬墙模型满足后者的梅尔尼科夫-Vainshtein短距离约束,如果包括轴向载体状态的无限塔架。然而,μ的结果由前几个共振强烈主导。在数值上,这些结果结果令人惊讶的是:(2.9 - 4.1)×10? 10在硬墙模型中,57%-58%的纵向贡献是纵向贡献,这是梅尔尼科夫 - VainShtein短距离约束的负责。重新加入全息结果以获得L3数据的最佳拟合,但随后仅匹配52%的渐近约束,结果减少到2.2(5)×10? 10,其仍然显着大于最先前的轴向矢量交流贡献的现象估计。

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