Characterization of a vacuum ultraviolet light source at 118 nm

TL;DR

This paper investigates the production of 118 nm vacuum ultraviolet light via frequency tripling in xenon gas, presenting a new model to explain the observed pressure-dependent limitations in light output.

Contribution

It introduces a novel pressure broadening model to explain the limitations in 118 nm VUV light generation, improving understanding of the process.

Findings

118 nm VUV light production peaks and then decreases with pressure.

A new pressure broadening model explains the observed limitations.

Experimental setup confirms the theoretical predictions.

Abstract

Vacuum ultraviolet (VUV) light at 118 nm has been shown to be a powerful tool to ionize molecules for various gas-phase chemical studies. A convenient table top source of 118 nm light can be produced by frequency tripling 355 nm light from a Nd:YAG laser in xenon gas. This process has a low efficiency, typically producing only nJ/pulse of VUV light. Simple models of the tripling process predict the power of 118 nm light produced should increase quadratically with increasing xenon pressure. However, experimental 118 nm production has been observed to reach a maximum and then decrease to zero with increasing xenon pressure. Here, we describe the basic theory and experimental setup for producing 118 nm light and a new proposed model for the mechanism limiting the production based on pressure broadened absorption.