# System size scan of D meson $R_\text{AA}$ and $v_n$ using PbPb, XeXe,   ArAr, and OO collisions at LHC

**Authors:** Roland Katz, Caio A. G. Prado, Jacquelyn Noronha-Hostler, Alexandre A., P. Suaide

arXiv: 1907.03308 · 2020-10-07

## TL;DR

This study predicts how D meson suppression and flow vary across different collision systems at the LHC, revealing complex dependencies on system size, geometry, and collision centrality, with implications for understanding quark-gluon plasma properties.

## Contribution

It introduces a systematic system size scan at the LHC using advanced modeling to explore D meson observables across multiple collision systems, highlighting non-trivial effects.

## Key findings

- Nuclear modification factor approaches unity in smaller systems.
- v2 remains similar across different system sizes in central collisions.
- D meson v2 is sensitive to nuclear deformation in XeXe collisions.

## Abstract

Experimental measurements indicate no suppression (e.g. $R_\text{pPb} \sim 1$) but a surprisingly large D meson $v_2$ was measured in pPb collisions. In order to understand these results we use Trento+v-USPhydro+DAB-MOD to make predictions and propose a system size scan at the LHC involving $^{208}$PbPb, $^{129}$XeXe, $^{40}$ArAr, and $^{16}$OO collisions. We find that the nuclear modification factor approaches unity as the system size is decreased, but nonetheless, in the 0-10% most central collisions $v_2\{2\}$ is roughly equivalent regardless of system size. These results arise from a rather non-trivial interplay between the shrinking path length and the enhancement of eccentricities in small systems at high multiplicity. Finally, we also find a surprising sensitivity of D mesons $v_2\{2\}$ in 0-10% at $p_T = 2-10$ GeV to the slight deformation of $^{129}$Xe recently found at LHC.

## Full text

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## Figures

11 figures with captions in the complete paper: https://tomesphere.com/paper/1907.03308/full.md

## References

101 references — full list in the complete paper: https://tomesphere.com/paper/1907.03308/full.md

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Source: https://tomesphere.com/paper/1907.03308