# Interpretation of the unpolarized azimuthal asymmetries in SIDIS

**Authors:** Albi Kerbizi (on behalf of the COMPASS Collaboration)

arXiv: 1812.07477 · 2018-12-19

## TL;DR

This paper investigates azimuthal asymmetries in SIDIS to extract quark transverse momentum information, highlighting the importance of subtracting vector meson decay contributions for accurate measurements.

## Contribution

It demonstrates that accounting for exclusive vector meson decay contamination is essential for correctly interpreting azimuthal asymmetries in SIDIS data.

## Key findings

- Large differences between data and Monte Carlo at high momentum fractions.
- Contamination from vector meson decays significantly affects azimuthal asymmetries.
- Subtracting vector meson contributions improves the extraction of intrinsic transverse momentum.

## Abstract

The measurement of azimuthal modulations in hadron leptoproduction on unpolarized nucleons allows to get information on the intrinsic transverse momentum $\langle k_T^2 \rangle$ of quarks in a nucleon through both the Cahn effect and the Boer-Mulders function. We have compared the azimuthal asymmetries in the cross section of $160\, \rm{GeV}/c$ muons scattered off an unpolarised deuteron target as measured by COMPASS with a Monte Carlo program, based on the ${}^3P_0$ model of quark anti-quark pair production at string breaking, which accounts for the Cahn effect. Large differences have been observed between data and Monte Carlo, in particular at large values of the fraction of the longitudinal momentum of the fragmenting quark carried by the produced hadron. We found out that most of these differences are due to pions from exclusive vector mesons contaminating the SIDIS sample, which also exhibit large azimuthal modulations. Using the measurements of the exclusive reaction $\mu N\rightarrow \mu' \, \rho\, N$ we had done in 2006, we can reproduce reasonably well the observed differences. Subtracting the contribution of hadrons produced in the decay of exclusive vector mesons from the SIDIS unpolarised azimuthal asymmetries is therefore a prerequisite condition for extracting $\langle k_T^2 \rangle$ and the Boer-Mulders function.

## Full text

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## Figures

11 figures with captions in the complete paper: https://tomesphere.com/paper/1812.07477/full.md

## References

9 references — full list in the complete paper: https://tomesphere.com/paper/1812.07477/full.md

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Source: https://tomesphere.com/paper/1812.07477