# QCD analysis of non-singlet structure functions at NNLO accuracy, based   on the Laplace transform

**Authors:** Maral Salajegheh, S. Mohammad Moosavi Nejad, Abolfazl Mirjalili, S., Atashbar Tehrani

arXiv: 1904.03439 · 2020-06-09

## TL;DR

This paper employs Laplace transform techniques to analyze non-singlet quark distributions and nucleon structure functions at NNLO accuracy, incorporating target mass and higher twist corrections, and compares results with contemporary PDFs and experimental data.

## Contribution

It introduces a novel application of Laplace transforms combined with Jacobi polynomial expansion for NNLO QCD analysis of non-singlet structure functions, including target mass and higher twist effects.

## Key findings

- Results agree well with recent experimental data.
- Comparison with modern PDF sets shows consistency.
- Method provides a precise framework for structure function analysis.

## Abstract

In this work, using the Laplace transformation technique we present our results for non-singlet quark distributions as well as nucleon structure function $F_2(x,Q^2)$ in unpolarized case at next-to-next-to-leading order (NNLO) QCD accuracy. We shall particularly compare our results for the sets of valence-quark parton distribution functions with the contemporary collaborations like CT14, CT18, MMHT14, MKAM16 and NNPDF. To construct the nucleon structure function we employ the expansion of Jacobi polynomials which is a suitable transform to convert the results of non-singlet structure function from the Laplace $s$-space to Bjorken $x$-space. We shall also consider the contributions of target mass correction as well as the higher twist effects at large-$x$ region for the proton and deuteron structure functions. Our results for the unpolarized quark distribution functions and nucleon structure functions are in good agreement with recent theoretical models and available experimental data.

## Full text

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## Figures

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## References

89 references — full list in the complete paper: https://tomesphere.com/paper/1904.03439/full.md

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Source: https://tomesphere.com/paper/1904.03439