کد مقاله کد نشریه سال انتشار مقاله انگلیسی نسخه تمام متن
4741644 1641515 2014 11 صفحه PDF دانلود رایگان
عنوان انگلیسی مقاله ISI
Effects of pressure and temperature on the silicon diffusivity of pyrope-rich garnet
ترجمه فارسی عنوان
اثرات فشار و دما بر نفوذ سیلیکون گارنت غنی از خاکپور
موضوعات مرتبط
مهندسی و علوم پایه علوم زمین و سیارات فیزیک زمین (ژئو فیزیک)
چکیده انگلیسی


• Arrhenius parameters in Si diffusion rates in pyrope-rich garnet were determined.
• Si diffusion is the slowest in the major constituent elements in the garnet.
• Si diffusion controls the rates of plastic deformation in the garnet.
• Si diffusion rates in garnet are similar with those in wadsleyite and ringwoodite.
• Separation of subducted oceanic crust from underlying peridotite layer may not occur.

We have determined the pressure and temperature dependencies of Si volume diffusion rates in a single crystal of Pyp75Alm15Gr10 garnet at 6–25 GPa and 1400–1800 °C by the 29Si tracer diffusion method. High-pressure experiments were conducted using the Kawai-type multi-anvil high-pressure apparatus. Diffusion profiles were obtained using secondary ion mass spectrometry in the depth-profiling mode. The Si diffusion coefficient in garnet (Dgt) is expressed by the Arrhenius equation: Dgt = D0 exp(−(E∗ + PV∗)/RT), with log10D0 = −7.1 ± 1.7 m2/s, E∗ = 345 ± 56 kJ/mol, and V∗ = 4.7 ± 0.5 cm3/mol. Si diffusion seems to be the slowest in the major constituent elements in a pyrope-rich garnet and control rates of plastic deformation. The comparison between Si diffusion rates in garnet and wadsleyite/ringwoodite suggests that garnet has similar or slightly lower strength (at most ∼2 times) compared with wadsleyite, and has similar or slightly higher strength (at most ∼3 times) compared with ringwoodite at temperatures ranging from 900 to 1300 °C. Thus, strength contrast between subducted oceanic crust and underlying peridotite layer may be small at the mantle transition zone conditions. This result suggests that the separation of subducted oceanic crust from an underlying peridotite layer may not occur.

ناشر
Database: Elsevier - ScienceDirect (ساینس دایرکت)
Journal: Physics of the Earth and Planetary Interiors - Volume 226, January 2014, Pages 28–38
نویسندگان
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