# First, second, third and fourth flow harmonics of deuterons and protons   in Au+Au reactions at 1.23 A GeV

**Authors:** Paula Hillmann, Jan Steinheimer, Tom Reichert, Vincent Gaebel, Marcus, Bleicher, Sukanya Sombun, Christoph Herold, Ayut Limphirat

arXiv: 1907.04571 · 2020-04-22

## TL;DR

This study uses the UrQMD model to analyze flow harmonics of deuterons and protons in Au+Au collisions at 1.23 AGeV, showing deuteron formation via coalescence and its impact on flow measurements, with implications for the HADES experiment.

## Contribution

It extends UrQMD to include deuteron formation by coalescence and demonstrates its effectiveness in describing flow data at GSI energies, highlighting the role of light cluster formation.

## Key findings

- Deuteron flow data are well described with a hard equation of state.
- Light cluster formation significantly affects proton flow results.
- Flow scaling relations like v3 ~ v1v2 and v4 ~ v2^2 are confirmed.

## Abstract

We explore the directed, elliptic, triangular and quadrangular flow of deuterons in Au+Au reactions at a beam energy of 1.23 AGeV within the UrQMD approach. These investigations are of direct relevance for the HADES experiment at GSI that has recently presented first data on the flow of light clusters in Au+Au collisions at 1.23 AGeV. To address the deuteron flow, UrQMD has been extended to include deuteron formation by coalescence. We find that this ansatz provides a very good description of the measured deuteron flow data, if a hard equation of state is used for the simulation. In addition we show that light cluster formation has a sizable impact on the proton flow and has to be taken into account to obtain reliable results in the forward/backward region. Based on the observed scaling of the flow, which is a natural result of coalescence, we conclude that deuteron production at GSI energies is a final state recombination effect. Finally, we also discuss the scaling relations of the higher order flow components up to $v_4$. We show that $v_3 \sim v_1v_2$ and $v_4 \sim v_2^2$ as function of transverse momentum and that the integrated $v_2^2 \sim v_4$ over the investigated energy range from $E_{lab}$=0.1 AGeV to 40 AGeV.

## Full text

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## Figures

19 figures with captions in the complete paper: https://tomesphere.com/paper/1907.04571/full.md

## References

62 references — full list in the complete paper: https://tomesphere.com/paper/1907.04571/full.md

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Source: https://tomesphere.com/paper/1907.04571