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Phys. Rev. B 73, 014105 (2006) [7 pages]

High-pressure phases in SnO2 to 117 GPa

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Sean R. Shieh*
Department of Earth Sciences, National Cheng Kung University, Taiwan 701

Atsushi Kubo and Thomas S. Duffy
Department of Geosciences, Princeton University, Princeton, New Jersey 08544, USA

Vitali B. Prakapenka and Guoyin Shen
GeoSoilEnviroCARS, University of Chicago, Chicago, Illinos 60637, USA

Received 25 August 2005; revised 28 October 2005; published 13 January 2006

X-ray diffraction of SnO2 (cassiterite) at high pressures and temperatures demonstrates the existence of four phase transitions to 117 GPa. The observed sequence of phases for SnO2 is rutile-type (P42∕mnm)→CaCl2-type(Pnnm)→pyrite-type(Pa3̅ )→ZrO2 orthorhombic phase I (Pbca)→cotunnite-type (Pnam). Our observations of the first three phases are generally in agreement with earlier studies. The orthorhombic phase I and cotunnite-type structure (orthorhombic phase II) were observed in SnO2 for the first time. The Pbca phase is found at 50–74 GPa during room-temperature compression. The cotunnite-type structure was synthesized when SnO2 was compressed to 74 GPa and heated at 1200 K. The cotunnite-type form was observed during compression between 54–117 GPa with additional laser heating carried out at 91 and 111 GPa. Fitting the pressure-volume data for the high-pressure phases to the second-order Birch-Murnaghan equation of state yields a bulk modulus of 259(26) GPa for the Pbca phase and 417(7) GPa for the cotunnite-type phase.

© 2006 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevB.73.014105
DOI:
10.1103/PhysRevB.73.014105
PACS:
62.50.+p, 61.10.Nz, 61.50.Ks, 64.10.+h

*Present address: Department of Earth Sciences, University of Western Ontario, Ontario, N6A 5B7.

Present address: HPCAT, Advanced Photon Source, ANL, Argonne, IL 60439.