TY - JOUR
T1 - Pressure-induced Pbca-P21/c phase transition of natural orthoenstatite
T2 - The effect of high temperature and its geophysical implications
AU - Zhang, Jin S.
AU - Reynard, Bruno
AU - Montagnac, Gilles
AU - Bass, Jay D.
N1 - Funding Information:
This work was supported by the National Science Foundation (NSF) under Grant EAR07-38871 , Consortium for Materials Properties Research in Earth Sciences (COMPRES) under NSF Cooperative Agreement EAR 11-57758 , and an international cooperative program between University of Illinois at Urbana-Champaign and Centre National de la Recherche Scientifique (CNRS), France . The Raman facility in Lyon is supported by Institut National des Sciences de l’Univers . We also thank Hervé Cardon for the help to our experiment. We are grateful to George Rossman (Caltech) and George Harlow ( Am. Museum of Natural History ) for providing samples.
PY - 2014/3
Y1 - 2014/3
N2 - In-situ high-pressure (P) high-temperature (T) Raman spectroscopy has been used to investigate the effect of temperature on the high-pressure phase transition of Mg-rich orthoenstatite (OEN) to a newly-discovered P21/c phase (HPCEN2) up to 673K and 18.2(10)GPa. Two natural orthoenstatite samples were used in this study: near end-member Mg orthoenstatite (Zabargad Island, Egypt), and Al+Fe-bearing orthoenstatite (San Carlos, Arizona). For San Carlos OEN (SC-OEN), the experiment was performed at room temperature, 373, 573 and 673K; For Zabargad Island OEN (Zabg OEN), experiments were performed at 573 and 673K. The three phases OEN, HPCEN2, and another high-pressure phase with space group C2/c (denoted by HPCEN) are readily distinguished by a characteristic doublet, triplet, or singlet, respectively, in the 660-680cm-1 range. Similarly, splitting of a peak near 1100cm-1 is indicative of an OEN→HPCEN2 transition. For both samples, no phase other than OEN and HPCEN2 was observed within the investigated P-T range. The recovered products after slow cooling for over 24h from 673K and 16.6(9)GPa were OEN. The Clapeyron slope (dP/dT) of this transition is bracketed between +0.020 to -0.0026GPa/K for Zabg-OEN, and +0.0023 to -0.0049GPa/K for SC-OEN. Our results suggest a possible stability field for HPCEN2 at the bottom of the upper mantle.
AB - In-situ high-pressure (P) high-temperature (T) Raman spectroscopy has been used to investigate the effect of temperature on the high-pressure phase transition of Mg-rich orthoenstatite (OEN) to a newly-discovered P21/c phase (HPCEN2) up to 673K and 18.2(10)GPa. Two natural orthoenstatite samples were used in this study: near end-member Mg orthoenstatite (Zabargad Island, Egypt), and Al+Fe-bearing orthoenstatite (San Carlos, Arizona). For San Carlos OEN (SC-OEN), the experiment was performed at room temperature, 373, 573 and 673K; For Zabargad Island OEN (Zabg OEN), experiments were performed at 573 and 673K. The three phases OEN, HPCEN2, and another high-pressure phase with space group C2/c (denoted by HPCEN) are readily distinguished by a characteristic doublet, triplet, or singlet, respectively, in the 660-680cm-1 range. Similarly, splitting of a peak near 1100cm-1 is indicative of an OEN→HPCEN2 transition. For both samples, no phase other than OEN and HPCEN2 was observed within the investigated P-T range. The recovered products after slow cooling for over 24h from 673K and 16.6(9)GPa were OEN. The Clapeyron slope (dP/dT) of this transition is bracketed between +0.020 to -0.0026GPa/K for Zabg-OEN, and +0.0023 to -0.0049GPa/K for SC-OEN. Our results suggest a possible stability field for HPCEN2 at the bottom of the upper mantle.
KW - High-pressure clinoenstatite
KW - High-pressure phase transition
KW - Orthoenstatite
KW - Raman spectroscopy
KW - Upper mantle
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U2 - 10.1016/j.pepi.2013.09.008
DO - 10.1016/j.pepi.2013.09.008
M3 - Article
AN - SCOPUS:84897045927
SN - 0031-9201
VL - 228
SP - 150
EP - 159
JO - Physics of the Earth and Planetary Interiors
JF - Physics of the Earth and Planetary Interiors
ER -