# Self amplification of channeling radiation at Bragg diffraction   conditions

**Authors:** Stasis Chuchurka, Andrei Benediktovitch, Aliaksandr Leonau, Sergey, Galyamin

arXiv: 1902.06959 · 2019-02-20

## TL;DR

This paper analyzes the potential for self-amplification of channeling radiation in crystals, showing how high electron bunch current densities and Bragg diffraction conditions can enhance X-ray emission through SASE in relativistic electron channeling.

## Contribution

It provides a theoretical analysis of conditions for SASE in channeling radiation, including the effects of crystal structure and Bragg diffraction, with numerical examples for Si, Ge, and C.

## Key findings

- Self amplification of channeling radiation is possible under high current densities.
- Bragg diffraction conditions can significantly enhance the SASE process.
- Numerical results demonstrate the feasibility in specific crystal types.

## Abstract

X-ray radiation of relativistic electrons passing through the crystal lattice (in case of channeling radiation) requires electrons with energies just from tens up to hundreds MeV, but has a drawback: low number of emitted X-ray quanta. However, the brightness of such a source could be potentially increased if the current density of the electron bunch is high enough to initiate the self amplified spontaneous emission (SASE) process. The conditions at which this phenomenon could take place for the case of axial channeling are analyzed in the present paper within the first order perturbation theory. The transition from spontaneous to SASE regime is described, the requirements for bunch current parameters initiating SASE process are determined taking into account the periodic structure of the crystal medium. It is also shown that satisfying Bragg diffraction conditions could enhance self amplification. Numerical results for the case of axial channeling in Si, Ge and C crystals are presented as an example.

## Full text

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## Figures

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## References

29 references — full list in the complete paper: https://tomesphere.com/paper/1902.06959/full.md

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Source: https://tomesphere.com/paper/1902.06959