2009
DOI: 10.1016/j.nuclphysb.2009.01.001
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Third-order QCD corrections to the charged-current structure function

Abstract: We compute the coefficient function for the charge-averaged W ± -exchange structure function F 3 in deep-inelastic scattering (DIS) to the third order in massless perturbative QCD. Our new threeloop contribution to this quantity forms, at not too small values of the Bjorken variable x, the dominant part of the next-to-next-to-next-to-leading order corrections. It thus facilitates improved determinations of the strong coupling α s and of 1/Q 2 power corrections from scaling violations measured in neutrino-nucle… Show more

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Cited by 109 publications
(127 citation statements)
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“…The calculation of these functions in dimensional regularization is a standard way to determine the splitting functions governing the scale dependence (evolution) of the perturbatively incalculable but process-independent parton and fragmentation distributions. The coefficient functions (partonic cross sections) for DIS and SIA, together with those for inclusive lepton-pair and Higgs-boson production in hadron collisions, facilitate studies of the analytic structure of QCD corrections at and beyond the next-to-next-to-leading order (NNLO) of the renormalization-group improved perturbative expansion [2][3][4][5][6][7][8][9][10][11][12][13][14][15][16], an accuracy that is harder to achieve for less inclusive quantities.…”
Section: Introductionmentioning
confidence: 99%
“…The calculation of these functions in dimensional regularization is a standard way to determine the splitting functions governing the scale dependence (evolution) of the perturbatively incalculable but process-independent parton and fragmentation distributions. The coefficient functions (partonic cross sections) for DIS and SIA, together with those for inclusive lepton-pair and Higgs-boson production in hadron collisions, facilitate studies of the analytic structure of QCD corrections at and beyond the next-to-next-to-leading order (NNLO) of the renormalization-group improved perturbative expansion [2][3][4][5][6][7][8][9][10][11][12][13][14][15][16], an accuracy that is harder to achieve for less inclusive quantities.…”
Section: Introductionmentioning
confidence: 99%
“…The above (spin-averaged) splitting functions are presently known to n = 2 [1,2], i.e., the nextto-next-to-leading order (NNLO ≡ N 2 LO). The coefficient functions for the most important structure functions (including F 3 for charge-averaged W -exchange) have also been fully computed to order α 3 s [3][4][5], while the less important chargeasymmetry W -cases are available only through a couple of low-integer Mellin-N moments [6,7]. The frontier in the present massless case are now the α 4 s corrections, for which first results have been obtained at the lowest value of N [8,9].…”
Section: Introductionmentioning
confidence: 99%
“…to NNLO [4,5,6,7]. For photon and charged current W ± -boson exchange, even the hard corrections at order O(α s 3 ) have been obtained [8,9]. For completeness, we also mention that the approach to polarized DIS is completely analogous.…”
Section: Deep-inelastic Scatteringmentioning
confidence: 99%