# Multi-particle and charge-dependent azimuthal correlations in heavy-ion   collisions at the Relativistic Heavy-Ion Collider

**Authors:** Bjoern Schenke, Chun Shen, Prithwish Tribedy

arXiv: 1901.04378 · 2019-04-17

## TL;DR

This paper models multi-particle azimuthal correlations in heavy-ion collisions at RHIC using a comprehensive simulation framework, providing insights into charge-dependent correlations and baseline predictions for isobar collisions.

## Contribution

It introduces a detailed simulation approach combining IP-Glasma, MUSIC, and UrQMD to study charge and momentum conservation effects on azimuthal correlations in heavy-ion collisions.

## Key findings

- Good agreement with existing charge inclusive azimuthal correlation data.
- Charge dependent two and three particle correlator results presented.
- Predictions for isobar collisions to aid Chiral Magnetic Effect searches.

## Abstract

We study multi-particle azimuthal correlations in relativistic heavy-ion collisions at a center of mass energy of 200 GeV. We use the IP-Glasma model to initialize the viscous hydrodynamic simulation MUSIC and employ the UrQMD transport model for the low temperature region of the collisions. In addition, we study effects of local charge and global momentum conservation among the sampled particles. With the exception of the lowest order three particle correlator $C_{112}$, our framework provides a good description of the existing charge inclusive azimuthal correlation data for Au+Au and U+U collisions at RHIC. We also present results for charge dependent two and three particle correlators in Au+Au and U+U collisions, and make predictions for isobar (Ru+Ru & Zr+Zr) collisions to provide a much needed baseline for the search for the Chiral Magnetic Effect at RHIC.

## Full text

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## Figures

27 figures with captions in the complete paper: https://tomesphere.com/paper/1901.04378/full.md

## References

90 references — full list in the complete paper: https://tomesphere.com/paper/1901.04378/full.md

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Source: https://tomesphere.com/paper/1901.04378