# Light (anti)nuclei production in Cu+Cu collisions at   $\sqrt{s_{\rm{NN}}}=200$GeV

**Authors:** Liu Feng-Xian, Chen Gang, She Zhi-Lei, Zhou Dai-Mei, Xie Yi-Long

arXiv: 1906.02592 · 2021-02-23

## TL;DR

This study investigates light (anti)nuclei production in Cu+Cu collisions at 200 GeV using a phase-space coalescence model, revealing strong centrality dependence and mass scaling properties consistent with experimental data.

## Contribution

It introduces a combined PACIAE and coalescence model approach to analyze (anti)nuclei yields and their dependence on collision centrality and mass in high-energy heavy-ion collisions.

## Key findings

- Yields decrease rapidly with increasing centrality.
- Antinucleus to nucleus ratios remain constant across centralities.
- Yields exhibit mass scaling properties.

## Abstract

The production of light (anti)nuclei have been investigated using the dynamically constrained phase-space coalescence model based on the final-state hadrons generated by the PACIAE model in Cu+Cu collisions at $\sqrt{s_{\rm{NN}}}=200$GeV with $|\eta|<0.5$ and $0<p_T<8$GeV/c. The results show that there is a strong centrality dependence of yields of $\rm d$, $\rm\overline d$, $\rm ^3He$, $\rm^3\overline {He}$, $\rm ^4He$, and $\rm^4\overline {He}$, i.e., their yields decrease rapidly with the increase of centrality, and the greater the mass is, the greater the dependence shows; whereas their ratio of antinucleus to nucleus and coalescence parameter $B_A$ remain constant as the centrality increases. In addition, the yields of (anti)nuclei are strongly dependent on the mass of the (anti)nuclei, indicating that the (anti)nuclei produced have mass scaling properties in high-energy heavy-ion collisions. Our results are consistent with the STAR experimental data.

## Full text

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## Figures

5 figures with captions in the complete paper: https://tomesphere.com/paper/1906.02592/full.md

## References

40 references — full list in the complete paper: https://tomesphere.com/paper/1906.02592/full.md

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Source: https://tomesphere.com/paper/1906.02592