# Extracting the strangeness freeze-out temperature from net-Kaon data at   RHIC

**Authors:** Rene Bellwied, Jacquelyn Noronha-Hostler, Paolo Parotto, Israel, Portillo Vazquez, Claudia Ratti, Jamie Stafford

arXiv: 1904.12711 · 2019-04-30

## TL;DR

This paper investigates the freeze-out temperature of strange particles at RHIC, finding it to be higher than that of light particles, supported by model calculations, experimental data, and preliminary spectra analysis.

## Contribution

It introduces evidence for a separate, higher freeze-out temperature for strange particles compared to light particles at RHIC.

## Key findings

- Strangeness freeze-out temperature is 10-15 MeV higher than light freeze-out temperature.
- Model calculations and experimental data support a two freeze-out temperature scenario.
- Preliminary Lambda spectra suggest a higher freeze-out temperature is favored.

## Abstract

Using the moments of the net-kaon distribution calculated within a state of-the-art hadron resonance gas model compared to experimental data from STAR's Beam Energy Scan, we find that the extracted strange freeze-out temperature is incompatible with the light one extracted from net-proton and net-charge fluctuations. Additionally predictions for net-$Lambda$ fluctuations are made that also appear to be consistent with a higher freeze-out temperature for strange particles. This strangeness freeze-out temperature is roughly $10-15$ MeV higher than the corresponding light freeze-out temperature. We also discuss cross-susceptibilities using different identified particles, which may be a further test of this two freeze-out temperature picture. Finally, we lay out the necessary updates needed in relativistic hydrodynamic models to take into account for this two freeze-out temperature scenario and present preliminary results of $\Lambda$ spectra at RHIC for AuAu $\sqrt{s_{NN}}=200$ GeV collisions that indicate a higher freeze-out temperature is preferred.

## Full text

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## Figures

6 figures with captions in the complete paper: https://tomesphere.com/paper/1904.12711/full.md

## References

62 references — full list in the complete paper: https://tomesphere.com/paper/1904.12711/full.md

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Source: https://tomesphere.com/paper/1904.12711