# Measurement of $W^{\pm}$ single spin asymmetries and $W$ cross section   ratio in polarized $p+p$ collisions at $\sqrt{s}=510$ GeV at STAR

**Authors:** Devika Gunarathne (for the STAR colloboration)

arXiv: 1702.02927 · 2019-08-14

## TL;DR

This paper reports precise measurements of $W^{}$ single spin asymmetries and cross section ratios in polarized proton-proton collisions at 510 GeV, providing insights into proton spin structure and sea quark distributions.

## Contribution

It presents the most precise $A_L^{W^}$ asymmetry results to date, with a 40% uncertainty reduction, and offers new measurements of $W$ cross section ratios at 500 and 510 GeV.

## Key findings

- Asymmetry results favor positive up antiquark polarization.
- Results are consistent with previous STAR measurements.
- New data improves constraints on proton's polarized quark distributions.

## Abstract

We present the preliminary results of measurements of single spin asymmetries, $A_L$ for $W^\pm$ boson production in longitudinally polarized p+p collisions at $\sqrt{s}=510$ GeV and measurements of cross section ratios, $\sigma _{W^+} / \sigma _{W^-}$, for $W^+,W^-$ boson production in $p+p$ collisions at $\sqrt{s}$ = 500 and 510 GeV. The asymmetry measurements are based on 246.2 pb$^{-1}$ of data taken in the RHIC 2013 run and the cross section ratio measurements are based on 102 pb$^{-1}$ of data taken during RHIC 2011 and 2012 runs by the STAR experiment. While the asymmetry results are shown as a function of the decay lepton pseudorapidity, $\eta_e$, the cross section results are shown as a function of both $\eta_e$ and W boson rapidity, $y_W$ in the mid-rapidity region ($|\eta_e|<1$). At this kinematics, $W^\pm$ single spin asymmetries provide a theoretically clean probe of the proton's polarized quark and antiquark distributions and the W cross section ratio provides sensitivity to unpolarized sea quark distributions at the scale of the W mass. The asymmetry results are consistent with recently published STAR $A^{W^\pm}_L$ results based on the data collected during RHIC 2011 and 2012 runs which showed a preference for a sizable, positive up antiquark polarization in the range $0.05 < x < 0.2$. The new preliminary results can be considered as the most precise results of $A^{W^\pm}_L$ in the world to date, with uncertainties reduced by 40\% in comparison to the published results.

## Full text

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## Figures

6 figures with captions in the complete paper: https://tomesphere.com/paper/1702.02927/full.md

## References

32 references — full list in the complete paper: https://tomesphere.com/paper/1702.02927/full.md

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Source: https://tomesphere.com/paper/1702.02927