# Effect of sea quarks on the single-spin asymmetries $A^{W^{\pm}}_{L}$ in   polarized pp collisions at RHIC

**Authors:** Fang Tian, Chang Gong, Bo-Qiang Ma

arXiv: 1702.07592 · 2017-03-17

## TL;DR

This paper investigates how sea quark helicity distributions influence single-spin asymmetries in W boson production during polarized proton-proton collisions at RHIC, highlighting the importance of sea quarks in nucleon spin structure.

## Contribution

It introduces a model combining valence and sea quark helicity distributions to analyze single-spin asymmetries, emphasizing the role of sea quarks in these asymmetries.

## Key findings

- Sea quark helicity distributions significantly affect $A^{W^{m 	iny f 	ext{±}}}_L$ shapes.
- $A^{W^-}_L$ is sensitive to $	riangle ar u$, while $A^{W^+}_L$ is sensitive to $	riangle ar d$.
- Experimental data constrains quark helicity distributions for both sea and valence quarks.

## Abstract

We calculate the single-spin asymmetries $A^{W^{\pm}}_{L}$ of $W^{\pm}$ bosons produced in polarized pp collisions with the valence part of the up and down quark helicity distributions modeled by the light-cone quark-spectator-diquark model while the sea part helicity distributions of the up and down quarks treated as parametrization. Comparing our results with those from experimental data at RHIC, we find that the helicity distributions of sea quarks play an important role in the determination of the shapes of $A^{W^{\pm}}_{L}$. It is shown that $A^{W^{-}}_{L}$ is sensitive to $\Delta \bar u$, while $A^{W^{+}}_{L}$ to $\Delta \bar d$ intuitively. The experimental data of the polarized structure functions and the sum of helicities are also important to constrain the sizes of quark helicity distributions both for the sea part and the valence part of the nucleon.

## Full text

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## Figures

33 figures with captions in the complete paper: https://tomesphere.com/paper/1702.07592/full.md

## References

64 references — full list in the complete paper: https://tomesphere.com/paper/1702.07592/full.md

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Source: https://tomesphere.com/paper/1702.07592