English
 
Help Privacy Policy Disclaimer
  Advanced SearchBrowse

Item

ITEM ACTIONSEXPORT

Released

Journal Article

Trapped Electrons at the Amorphous Solid Water/Vacuum Interface as Possible Reactants in a Water Splitting Reaction

MPS-Authors
/persons/resource/persons183254

King,  Sarah B.
Physical Chemistry, Fritz Haber Institute, Max Planck Society;

/persons/resource/persons22225

Wegkamp,  Daniel
Physical Chemistry, Fritz Haber Institute, Max Planck Society;

/persons/resource/persons81302

Richter,  Clemens
Physical Chemistry, Fritz Haber Institute, Max Planck Society;

/persons/resource/persons22250

Wolf,  Martin
Physical Chemistry, Fritz Haber Institute, Max Planck Society;

/persons/resource/persons22128

Stähler,  Julia
Physical Chemistry, Fritz Haber Institute, Max Planck Society;

External Resource
No external resources are shared
Fulltext (restricted access)
There are currently no full texts shared for your IP range.
Fulltext (public)
There are no public fulltexts stored in PuRe
Supplementary Material (public)
There is no public supplementary material available
Citation

King, S. B., Wegkamp, D., Richter, C., Wolf, M., & Stähler, J. (2017). Trapped Electrons at the Amorphous Solid Water/Vacuum Interface as Possible Reactants in a Water Splitting Reaction. The Journal of Physical Chemistry C, 121(13), 7379-7386. doi:10.1021/acs.jpcc.7b01459.


Cite as: https://hdl.handle.net/11858/00-001M-0000-002D-4035-F
Abstract
The dynamics and energetics of electrons in water impacts diverse fields, from electrochemistry to astrochemistry. In the present experiments, long-lived, low-energy, electronic states are observed at the amorphous solid water (ASW)/vacuum interface with decay times on the order of seconds, orders of magnitude longer than solvated electron states observed in the ASW bulk. The formation, relaxation, and reactivity of these trapped electrons were investigated using two-photon photoemission of >15 bilayers of amorphous D2O adsorbed on the Cu(111) surface. The decay time of the trapped electron signal is approximately 16 s. This extraordinarily long lifetime allows for a reaction between trapped electrons and the ASW surface, producing hydroxide anions and molecular hydrogen at the interface. This reaction is observed by a decrease of the trapped electron population and a concomitant increase of the work function during ultraviolet light exposure. The low-energy electron reactivity at the ASW/vacuum interface has profound implications for astrochemistry due to the prevalence of ASW in space.