# Fluctuations and clustering of multiplicity in collisions of   relativistic ions

**Authors:** Maciej Rybczynski, Zbigniew Wlodarczyk

arXiv: 1904.01366 · 2020-02-19

## TL;DR

This paper explains the non-monotonic fluctuations in particle multiplicity in relativistic ion collisions through particle clustering, revealing collective behavior and self-organization in hadronic matter.

## Contribution

It introduces a cluster-based explanation for multiplicity fluctuations, contrasting with traditional string-hadronic models, and characterizes clusters as quasi-neutral gases with collective properties.

## Key findings

- Multiplicity fluctuations are explained by particle clustering.
- Clusters exhibit collective behavior with a characteristic Debye length.
- The model reproduces observed non-monotonic fluctuation patterns.

## Abstract

We discuss the recently measured event-by-event multiplicity fluctuations in relativistic heavy-ion collisions. It is shown that the observed non-monotonic behaviour of the scaled variance of multiplicity distribution as a function of collision centrality (such effect is not observed in a widely used string-hadronic models of nuclear collisions) can be fully explained by the correlations between produced particles promoting cluster formation. We define a cluster as a quasi-neutral gas of charged and neutral particles which exhibits collective behaviour. The characteristic space scale of this shielding is the Debye length. Multiplicity distribution in a cluster is given by Negative Binomial distribution while the rest (reservoir), treated as a superposition of elementary collisions, is described by Binomial distribution. The ability to generate spatial structures (cluster phase) sign the propensity to self-organize of hadronic matter.

## Full text

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## Figures

11 figures with captions in the complete paper: https://tomesphere.com/paper/1904.01366/full.md

## References

40 references — full list in the complete paper: https://tomesphere.com/paper/1904.01366/full.md

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Source: https://tomesphere.com/paper/1904.01366