2001
DOI: 10.1007/s100520100577
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Hadronic corrections at ${\cal O}(\alpha^2)$ to the energy spectrum of muon decay

Abstract: We consider the impact of O(α 2 ) hadronic corrections to the energy spectrum of the decay electron in muon decay. We find that the correction can be described, within good approximation, by a linear function in the electron energy. Explicit expressions for the form factors needed in an approach based on dispersion integrals are given. * Supported by the Deutsche Forschungsgemeinschaft.

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Cited by 22 publications
(19 citation statements)
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“…The possible contribution to the uncertainty from strong interactions is negligible in our case, since it is suppressed at least by (α/π) 2 , and the lowest order the contribution of hadronic virtual pairs was found in Ref. [36] to be small itself. An estimate of the omitted contributions by a simple counting of powers of the finestructure constant and the large logarithm is not very safe, because there could be some extra enhancement factors, like numerically large constant coefficients or powers of ln(1−x) (the latter is partially taken into account by exponentiation).…”
Section: Discussionsupporting
confidence: 53%
“…The possible contribution to the uncertainty from strong interactions is negligible in our case, since it is suppressed at least by (α/π) 2 , and the lowest order the contribution of hadronic virtual pairs was found in Ref. [36] to be small itself. An estimate of the omitted contributions by a simple counting of powers of the finestructure constant and the large logarithm is not very safe, because there could be some extra enhancement factors, like numerically large constant coefficients or powers of ln(1−x) (the latter is partially taken into account by exponentiation).…”
Section: Discussionsupporting
confidence: 53%
“…represents the electromagnetic radiative corrections, which have been calculated to Oð 2 Þ. Corrections due to the strong interaction in loops give a fractional contribution on the order of 4 Â 10 À7 [6], which is more than 2 orders of magnitude smaller than the ultimate precision goals of TWIST. The quantities , , , and , often called the Michel parameters, are bilinear combinations of the weak coupling constants and describe the shape of the decay spectrum.…”
Section: Introductionmentioning
confidence: 99%
“…Also for the amplitudes in classes I-III we rely on the dispersion relation (33) to compute the HVP in the space-like region. This method was employed, for example, to compute the hadronic corrections to muon decay [84,85] and Bhabha scattering [86][87][88]. The hadronic NNLO corrections to μ-e scattering based on the R ratio were presented in [65].…”
Section: Next-to-next-to Leading Ordermentioning
confidence: 99%