THE EFFECT OF STRAIN-ENERGY ON GROWTH-RATES DURING THE OLIVINE-SPINELTRANSFORMATION AND IMPLICATIONS FOR OLIVINE METASTABILITY IN SUBDUCTING SLABS

Citation
M. Liu et al., THE EFFECT OF STRAIN-ENERGY ON GROWTH-RATES DURING THE OLIVINE-SPINELTRANSFORMATION AND IMPLICATIONS FOR OLIVINE METASTABILITY IN SUBDUCTING SLABS, J GEO R-SOL, 103(B10), 1998, pp. 23897-23909
Citations number
36
Categorie Soggetti
Geochemitry & Geophysics","Geosciences, Interdisciplinary","Astronomy & Astrophysics",Oceanografhy,"Metereology & Atmospheric Sciences
Journal title
JOURNAL OF GEOPHYSICAL RESEARCH-SOLID EARTH
ISSN journal
21699313 → ACNP
Volume
103
Issue
B10
Year of publication
1998
Pages
23897 - 23909
Database
ISI
SICI code
2169-9313(1998)103:B10<23897:TEOSOG>2.0.ZU;2-I
Abstract
We have studied growth kinetics during the transformation of Mg1.8Fe0. 2SiO4 San Carlos olivine to its high-pressure polymorphs wadsleyite (b eta phase) and ringwoodite (gamma phase) at 800 degrees-1200 degrees C and nominal pressures of 16-20 GPa. In experiments in which a large ( 500-600 mu m) olivine single crystal (contained in a matrix of either fine-grained olivine or NaCl) was transformed, reaction rims of wadsle yite/ringwoodite form on the margins of the single crystal by incohere nt grain-boundary nucleation and interface-controlled growth. Contrary to theoretical expectations, the growth rate of these reaction rims d ecreases sharply as a function of time; for instance, at 1100 degrees C and 18 GPa, growth ceases on an experimental timescale after the rim width reaches 20-25 mu m. In order to explain this observation, we de velop an elastic model based on the theory of a misfitting inclusion. Comparing the results of this model with the experimental data suggest s that elastic strain energy, which develops because of the large volu me decrease associated with the transformation, is responsible for the decreasing growth rates. On the other hand, experimental and theoreti cal results suggest that elastic strain energy is relatively unimporta nt when grains of the product phase are randomly dispersed and distinc t reaction rims do not form; this is the case when the nucleation rate is low, the growth rate is fast, and the reactant olivine is fine gra ined. On a geological timescale in subducting lithosphere, where the g rain size of the olivine is large, the growth rates of grain-boundary nucleated reaction rims are likely to be controlled by viscoelastic re laxation. Therefore current kinetic models of olivine metastability in subducting slabs, which are based on simple extrapolations of experim ental data and on the assumption that the growth rate is constant at f ixed temperature and pressure, need to be reevaluated.