# Neon in ultrashort and intense x rays from free electron lasers

**Authors:** Christian Buth, Randolf Beerwerth, Razib Obaid, Nora Berrah, Lorenz S., Cederbaum, Stephan Fritzsche

arXiv: 1705.07521 · 2022-11-08

## TL;DR

This paper provides a detailed theoretical analysis of neon atom ionization under ultrashort, intense x-ray pulses from free electron lasers, revealing the importance of extended rate equations and uncovering new insights into ion and photon yields.

## Contribution

It introduces an extended rate-equation model for neon that includes double Auger decay and shake-off processes, connecting atomic physics with graph theory and formal languages.

## Key findings

- Plain rate equations are insufficient for accurate predictions.
- Including shake-off processes significantly affects ion yields.
- Inaccuracies in Auger decay widths have minor impact on results.

## Abstract

We theoretically examine neon atoms in ultrashort and intense x rays from free electron lasers and compare our results with data from experiments conducted at the Linac Coherent Light Source (LCLS). For this purpose, we treat in detail the electronic structure in all possible nonrelativistic cationic configurations using a relativistic multiconfiguration approach. The interaction with the x rays is described in rate-equation approximation. To understand the mechanisms of the interaction, a path analysis is devised which allows us to investigate what sequences of photoionization and decay processes lead to a specific configuration and with what probability. Thereby, we uncover a connection to the mathematics of graph theory and formal languages. In detail, we study the ion yields and find that plain rate equations do not provide a satisfactory description. We need to extend the rate equations for neon to incorporate double Auger decay of a $K$-shell vacancy and photoionization shake off for neutral neon. Shake off is included for valence and core ionization; the former has hitherto been overlooked but has important consequences for the ion yields from an x-ray energy below the core ionization threshold. Furthermore, we predict the photon yields from XUV and x-ray fluorescence; these allow one insights into the configurations populated by the interaction with the x rays. Finally, we discover that inaccuracies in those Auger decay widths employed in previous studies have only a minor influence on ion and photon yields.

## Full text

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## Figures

7 figures with captions in the complete paper: https://tomesphere.com/paper/1705.07521/full.md

## References

88 references — full list in the complete paper: https://tomesphere.com/paper/1705.07521/full.md

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Source: https://tomesphere.com/paper/1705.07521