Kinematic power corrections for TMD factorization theorem of semi-inclusive deep-inelastic scattering
Sara Piloneta, Alexey Vladimirov
TL;DR
This work develops a gauge- and frame-invariant extension of the SIDIS TMD factorization theorem by summing kinematic power corrections (KPCs) that accompany the leading-twist, twist-two TMD distributions. The authors derive the complete twist-two hadron tensor within the TMD-with-KPCs framework, detailing the twist-two quark and antiquark correlators, their momentum-space representations, and the associated convolution structure that yields all SIDIS structure functions, including those activated by longitudinal photon contributions. They implement a Lorentz- and rapidity-factorization consistent convolution, with a finite integration domain in the parton momenta, and provide explicit expressions for the SIDIS structure functions in terms of twist-two TMD PDFs and FFs, connected through a common hard coefficient $C_{0, ext{DIS}}$ and rapidity scales $oldsymbol{ ext{ζ}}$, $ar{oldsymbol{ ext{ζ}}}$ (with $oldsymbol{ζ}ar{oldsymbol{ζ}}=Q^4$). Numerical studies using ART25 TMDs show KPCs contribute only a few percent at $Q\, ext{≈10 GeV}$ but can reach tens of percent at $Q\≈2$ GeV, indicating that including KPCs is essential for accurately describing current SIDIS data and potentially reconciling tensions among TMD extractions at low $Q$.
Abstract
We evaluate the complete set of kinematic power corrections (KPCs) to the leading power (LP) term of the transverse momentum dependent (TMD) factorization theorem for semi-inclusive deep-inelastic scattering (SIDIS) with a polarized target. This formulation restores the contributions of twist-two TMD distributions to all structure functions, including those that vanish at leading power, such as contributions of longitudinal photons. The resulting expressions are explicitly gauge- and frame-invariant, and inherit all key features of the standard TMD factorization framework, including the coefficient functions and the evolution equations. Numerical estimations show that KPCs contribute only a few percent at $Q\sim10$GeV, but can reach several tens of percents when $Q\sim 2$GeV. Consequently, accounting for kinematic power corrections can be vital for an accurate theoretical description of current SIDIS measurements.
