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High-pressure compressibility and vibrational properties of (Ca,Mn)CO3

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Published/Copyright: November 30, 2016
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Abstract

Knowledge of potential carbon carriers such as carbonates is critical for our understanding of the deep-carbon cycle and related geological processes within the planet. Here we investigated the high-pressure behavior of (Ca,Mn)CO3 up to 75 GPa by synchrotron single-crystal X-ray diffraction, laser Raman spectroscopy, and theoretical calculations. MnCO3-rich carbonate underwent a structural phase transition from the CaCO3-I structure into the CaCO3-VI structure at 45–48 GPa, while CaCO3-rich carbonate transformed into CaCO3-III and CaCO3-VI at approximately 2 and 15 GPa, respectively. The equation of state and vibrational properties of MnCO3-rich and CaCO3-rich carbonates changed dramatically across the phase transition. The CaCO3-VI-structured CaCO3-rich and MnCO3-rich carbonates were stable at room temperature up to at least 53 and 75 GPa, respectively. The addition of smaller cations (e.g., Mn2+, Mg2+, and Fe2+) can enlarge the stability field of the CaCO3-I phase as well as increase the pressure of the structural transition into the CaCO3-VI phase.

Acknowledgments

We acknowledge R. McCarty, X. Wu, P. Dera, and R. Jones for experimental assistance and helpful discussion. W.L. Mao acknowledges support from the Geophysics Program at NSF (EAR 1446969) and the Deep Carbon Observatory. R. Caracas acknowledges computational support from eDARI under grant stl2816 and from PSMN of ENS Lyon, and financial support from the PICS program of CNRS and the Deep Carbon Observatory. D.W. Fan acknowledges financial support from the National Natural Science Foundation of China (41374107), and the Youth Innovative Technology Talents Program of Institute of Geochemistry, Chinese Academy of Sciences. Portions of this work were performed at Geo-SoilEnviroCARS (Sector 13) and HPCAT (Sector 16), Advanced Photon Source (APS), Argonne National Laboratory. Use of the COMPRES-GSECARS gas loading system was supported by COMPRES under NSF Cooperative Agreement EAR 11-57758 and by GSECARS through NSF grant EAR-1128799 and DOE grant DE-FG02-94ER14466. HPCAT operations are supported by DOE-NNSA under Award No. DE-NA0001974 and DOE-BES under Award No. DE-FG02-99ER45775, with partial instrumentation funding by NSF. The Advanced Photon Source, a U.S. Department of Energy (DOE) Office of Science User Facility is operated for the DOE Office of Science by Argonne National Laboratory under Contract No. DE-AC02-06CH11357. Data used in this study are available upon request from J. Liu (E-mail:) and R. Caracas (E-mail: ).

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Received: 2016-2-27
Accepted: 2016-7-25
Published Online: 2016-11-30
Published in Print: 2016-12-1

© 2016 by Walter de Gruyter Berlin/Boston

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