# Effective decrease of photoelectric emission threshold from gold plated   surfaces

**Authors:** Peter J Wass, Daniel Hollington, Timothy J Sumner, Fangchao Yang and, Markus Pfeil

arXiv: 1901.01057 · 2019-07-08

## TL;DR

This study investigates how gold-plated surfaces can emit photoelectrons at lower photon energies than expected, revealing practical insights for satellite charge neutralization applications.

## Contribution

It provides detailed measurements of photoelectric emission from gold surfaces with varying roughness and develops a model to simulate the process accurately.

## Key findings

- Quantum yields up to 44 ppm observed
- Photoemission occurs at photon energies below gold's nominal work function
- Surface roughness and long-term effects influence emission efficiency

## Abstract

Many applications require charge neutralisation of isolated test bodies and this has been successfully done using photoelectric emission from surfaces which are electrically benign(gold) or superconducting (niobium). Gold surfaces nominally have a high work function ($\sim 5.1$\,eV)which should require deep UV photons for photoemission. In practice it has been found that it can be achieved with somewhat lower energy photons with indicative work functions of ($ 4.1-4.3$\,eV). A detailed working understanding of the process is lacking and this work reports on a study of the photoelectric emission properties of 4.6x4.6 cm^2 gold plated surfaces, representative of those used in typical satellite applications with a film thickness of 800 nm, and measured surface roughnesses between 7 and 340 nm. Various UV sources with photon energies from 4.8 to 6.2 eV and power outputs from 1 nW to 1000 nW, illuminated a ~0.3 cm^2 of the central surface region at angles of incidence from 0 to 60 degrees.   Final extrinsic quantum yields in the range 10 ppm to 44 ppm were reliably obtained during 8 campaigns, covering a ~3 year period, but with intermediate long-term variations lasting several weeks and, in some cases, bake-out procedures at up to 200 C. Experimental results were obtained in a vacuum system with a baseline pressure of ~10^{-7} mbar at room temperature. A working model, designed to allow accurate simulation of any experimental configuration, is proposed.

## Full text

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## Figures

26 figures with captions in the complete paper: https://tomesphere.com/paper/1901.01057/full.md

## References

47 references — full list in the complete paper: https://tomesphere.com/paper/1901.01057/full.md

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Source: https://tomesphere.com/paper/1901.01057