Abstract

Hydrated singly charged magnesium ions Mg+(H2O)n, n ≤ 5, in the gas phase are ideal model systems to study photochemical hydrogen evolution since atomic hydrogen is formed over a wide range of wavelengths, with a strong cluster size dependence. Mass selected clusters are stored in the cell of an Fourier transform ion cyclotron resonance mass spectrometer at a temperature of 130 K for several seconds, which allows thermal equilibration via blackbody radiation. Tunable laser light is used for photodissociation. Strong transitions to D1–3 states (correlating with the 3s-3px,y,z transitions of Mg+) are observed for all cluster sizes, as well as a second absorption band at 4–5 eV for n = 3-5. Due to the lifted degeneracy of the 3px,y,z energy levels of Mg+, the absorptions are broad and red shifted with increasing coordination number of the Mg+ center, from 4.5 eV for n = 1 to 1.8 eV for n = 5. In all cases, H atom formation is the dominant photochemical reaction channel. Quantum chemical calculations using the full range of methods for excited state calculations reproduce the experimental spectra and explain all observed features. In particular, they show that H atom formation occurs in excited states, where the potential energy surface becomes repulsive along the O⋅⋅⋅H coordinate at relatively small distances. The loss of H2O, although thermochemically favorable, is a minor channel because, at least for the clusters n = 1-3, the conical intersection through which the system could relax to the electronic ground state is too high in energy. In some absorption bands, sequential absorption of multiple photons is required for photodissociation. For n = 1, these multiphoton spectra can be modeled on the basis of quantum chemical calculations.

Highlights

  • Hydrated magnesium ions represent an interesting system to understand the mechanisms of hydrogen production via catalysis on metal centers1–7 as well as corrosion effects.8 At the same time, they play a role in processes in the Earth’s and other planets’ upper atmosphere where magnesium is present due to the influx of interplanetary particles.9,10 Hydrated metal ions M+(H2O)n are well-defined moieties to study the transition of various properties from a metal atom solvated by a single water molecule to bulk behavior.11–14 There has been a long history of studies on microhydrated metal ions in the gas phase over the last decades

  • Relative photodissociation cross sections were measured for Mg+(H2O)1-5 clusters in the range of 0.6–5.0 eV

  • The results are overall in good agreement with the theoretical predictions, as well as earlier experiments,20 the dissociation bands all seem to be shifted to the red, especially in the case of the Mg+(H2O)3 cluster

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Summary

INTRODUCTION

Hydrated magnesium ions represent an interesting system to understand the mechanisms of hydrogen production via catalysis on metal centers as well as corrosion effects. At the same time, they play a role in processes in the Earth’s and other planets’ upper atmosphere where magnesium is present due to the influx of interplanetary particles. Hydrated metal ions M+(H2O)n are well-defined moieties to study the transition of various properties from a metal atom solvated by a single water molecule to bulk behavior. There has been a long history of studies on microhydrated metal ions in the gas phase over the last decades. The existence of a hydrated electron and a Mg di-cation was proclaimed for n ≥ 8.30 Siu and Liu explained the minimum cluster size for the hydrogen loss reaction based on ab initio molecular dynamics calculations and investigated the influence of the coordination number on the process.. The existence of a hydrated electron and a Mg di-cation was proclaimed for n ≥ 8.30 Siu and Liu explained the minimum cluster size for the hydrogen loss reaction based on ab initio molecular dynamics calculations and investigated the influence of the coordination number on the process.32 They explained the switch off for the hydrogen loss process for larger clusters due to the barrier increase when the solvated electron moves beyond the third solvation shell.. Theoretical calculations are used to model the spectra and to explain the observed reactions on excited state potential energy surfaces

EXPERIMENTAL AND THEORETICAL METHODS
Experimental photodissociation spectra
Modeled photoabsorption spectra
Photodissociation modeling
CONCLUSIONS
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