# Interpretable deep learning for nuclear deformation in heavy ion   collisions

**Authors:** Long-Gang Pang, Kai Zhou, Xin-Nian Wang

arXiv: 1906.06429 · 2019-06-26

## TL;DR

This paper demonstrates that deep convolutional neural networks can be used to infer nuclear deformation from heavy-ion collision data, revealing how different collision geometries relate to nuclear shape characteristics.

## Contribution

It introduces a novel application of DCNN and interpretation algorithms to extract and understand nuclear deformation from collision observables.

## Key findings

- DCNN successfully regresses nuclear deformation magnitude.
- Degeneracy exists between prolate-prolate and oblate-oblate collisions.
- Interpretation reveals deformation sensitivity varies with collision overlap.

## Abstract

The structure of heavy nuclei is difficult to disentangle in high-energy heavy-ion collisions. The deep convolution neural network (DCNN) might be helpful in mapping the complex final states of heavy-ion collisions to the nuclear structure in the initial state. Using DCNN for supervised regression, we successfully extracted the magnitude of the nuclear deformation from event-by-event correlation between the momentum anisotropy or elliptic flow ($v_2$) and total number of charged hadrons ($dN_{\rm ch}/d\eta$) within a Monte Carlo model. Furthermore, a degeneracy is found in the correlation between collisions of prolate-prolate and oblate-oblate nuclei. Using the Regression Attention Mask algorithm which is designed to interpret what has been learned by DCNN, we discovered that the correlation in total-overlapped collisions is sensitive to only large nuclear deformation, while the correlation in semi-overlapped collisions is discriminative for all magnitudes of nuclear deformation. The method developed in this study can pave a way for exploration of other aspects of nuclear structure in heavy-ion collisions.

## Full text

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## Figures

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## References

55 references — full list in the complete paper: https://tomesphere.com/paper/1906.06429/full.md

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Source: https://tomesphere.com/paper/1906.06429