Abstract

We present a general method for obtaining the quantum chromodynamical radiative corrections to the higher-twist (power-suppressed) contributions to inclusive deep-inelastic scattering in terms of light-cone correlation functions of the fundamental fields of quantum chromodynamics. Using this procedure, we calculate the previously unknown O(αs){\cal O}(\alpha_s) corrections to the twist-three part of the spin scaling function gT(xB,Q2)(=g1(xB,Q2)+g2(xB,Q2))g_T(x_B,Q^2) (=g_1(x_B,Q^2)+g_2(x_B,Q^2)) and the corresponding forward Compton amplitude ST(ν,Q2)S_T(\nu,Q^2). Expanding our result about the unphysical point xB=x_B=\infty, we arrive at an operator product expansion of the nonlocal product of two electromagnetic current operators involving twist-two and -three operators valid to O(αs){\cal O}(\alpha_s) for forward matrix elements. We find that the Wandzura-Wilczek relation between g1(xB,Q2)g_1(x_B,Q^2) and the twist-two part of gT(xB,Q2)g_T(x_B,Q^2) is respected in both the singlet and non-singlet sectors at this order, and argue its validity to all orders. The large-NcN_c limit does not appreciably simplify the twist-three Wilson coefficients.Comment: 41 pages, 9 figures, corrected minor erro

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