# $\Lambda_{c}$ Production in Au+Au Collisions at $\sqrt{s_{NN}}$ = 200   GeV measured by the STAR experiment

**Authors:** Guannan Xie (for the STAR Collaboration)

arXiv: 1704.04353 · 2019-08-13

## TL;DR

This paper reports the first measurement of $\Lambda_{c}$ baryon production in Au+Au collisions at 200 GeV, providing insights into charm quark hadronization and medium effects in heavy-ion collisions.

## Contribution

It presents the first experimental measurement of $\Lambda_{c}$ production in heavy-ion collisions at RHIC, comparing results to theoretical models of charm quark hadronization.

## Key findings

- Measured $\Lambda_{c}$/$D^0$ ratio in 10-60% central Au+Au collisions.
- Compared experimental ratio to model predictions, discussing medium effects.
- Provided new data on charm baryon production in heavy-ion environments.

## Abstract

At RHIC, enhancements in the baryon-to-meson ratio for light hadrons and hadrons containing strange quarks have been observed in central heavy-ion collisions compared to those in p+p and peripheral heavy-ion collisions in the intermediate transverse momentum ($p_T$) range (2 $<$ $p_T$ $<$ 6 GeV/$c$). This can be explained by the hadronization mechanism involving multi-parton coalescence. $\Lambda_{c}$ is the lightest charmed baryon with mass close to that of $D^0$ meson, and has an extremely short life time (c$\tau$$\sim$60 $\mu$m). Different models predict different magnitudes of enhancement in the $\Lambda_{c}$/$D^0$ ratio depending on the degree to which charm quarks are thermalized in the medium and how the coalescence mechanism is implemented.   In these proceedings, we report the first measurement of $\Lambda_{c}$ production in heavy-ion collisions using the Heavy Flavor Tracker at STAR. The invariant yield of $\Lambda_{c}$ for 3 $<$ $p_T$ $<$ 6 GeV/$c$ is measured in 10-60% central Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV. The $\Lambda_{c}$/$D^0$ ratio is compared to different model calculations, and the physics implications are discussed.

## Full text

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## Figures

5 figures with captions in the complete paper: https://tomesphere.com/paper/1704.04353/full.md

## References

14 references — full list in the complete paper: https://tomesphere.com/paper/1704.04353/full.md

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