Diffusion rates of hydrogen defect species associated with site-specific infrared spectral bands in natural olivine

Yang (Will) Li, Stephen J. Mackwell, David L. Kohlstedt

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Abstract

We investigated hydrogen transport in naturally occurring, iron-bearing samples of San Carlos olivine that were hydrogenated at confining pressures of 200 or 300 MPa and 1173 to 1303 K or dehydrogenated at room pressure and 1191 to 1358 K. Chemical diffusion coefficients were determined from diffusion profiles for individual O-H-stretching bands from series of infrared spectra in orthogonal directions across each sample. Within experimental uncertainty, the diffusivities associated with all the individual bands are in good agreement with one another in both the hydrogenation and the dehydrogenation experiments. Hydrogenation proceeds by two diffusion mechanisms, as reported previously. The faster process involves interstitial diffusion of protons coupled with a counter-flux of polarons, with proton diffusion rate-limiting hydrogenation. For this mechanism, diffusion is faster along the olivine [100] direction than along [010] and [001], consistent with the anisotropy reported for proton diffusion and conductivity in olivine. The slower process involves interstitial proton diffusion coupled with a parallel flux of metal vacancies, with vacancy diffusion rate-limiting hydrogenation. For this mechanism, diffusion is faster along [001] than along [100] and [010], consistent with the anisotropy previously reported for the diffusion of metal cations in olivine. Diffusivities from our new dehydrogenation experiments are identical in both magnitude and anisotropy to those determined in our earlier hydrogenation experiments. This agreement demonstrates the validity of studies that used the results of our hydrogenation experiments to analyze dehydrogenation profiles in olivine xenocrysts and olivine in mantle xenoliths to determine rates of magma ascent from the source regions in Earth's interior.

Original languageEnglish (US)
Article number117406
JournalEarth and Planetary Science Letters
Volume581
DOIs
StatePublished - Mar 1 2022

Bibliographical note

Funding Information:
We acknowledge technical support from Mark Zimmerman in the performance of the experiments and Jed Mosenfelder for help with the infrared spectroscopy and for valuable discussions. The manuscript was improved by insightful comments by an anonymous reviewer. This work was supported by grant EAR-1755805 from the National Science Foundation .

Publisher Copyright:
© 2022 Elsevier B.V.

Keywords

  • anisotropy
  • dehydrogenation
  • diffusion
  • hydrogenation
  • infrared
  • olivine

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