Thermal Expansion and Response to Pressure of Double-ReO3-Type Fluorides NaMVF6(M = Nb, Ta)

Anthony J. Lloyd, Eric B. Masterson, Samuel J. Baxter, Jamie J. Molaison, António M. Dos Santos, Angus P. Wilkinson

Research output: Contribution to journalArticlepeer-review

7 Scopus citations

Abstract

Several II-IV double-ReO3-type (DROT) fluorides are known to exhibit strong negative thermal expansion (NTE) over a wide temperature range while retaining a cubic structure down to 120 K or lower. CaZrF6, CaNbF6, CaTiF6, and MgZrF6, embody these properties. In contrast to the behavior of these II-IV materials, the I-V DROT material, NaSbF6, has been reported to display a phase transition from rhombohedral to cubic above 300 K and positive thermal expansion both above and below the transition. In this work, NaNbF6 and NaTaF6 are shown to undergo first-order cubic-to-rhombohedral transitions on cooling to ∼130 K. Above this transition, NaNbF6 shows modest NTE between 160 and 250 K, whereas NaTaF6 exhibits near-zero thermal expansion over the range 210-270 K. These I-V systems are elastically softer than their II-IV counterparts, with a zero pressure bulk modulus, K0, of 14.6(8) GPa and first derivative of the bulk modulus with respect to pressure, K0′, of -18(3) for cubic NaNbF6, and K0 = 14.47(3) GPa and K0′= -21.56(7) for cubic NaTaF6. When subject to ∼0.3 GPa at 300 K, both compounds exhibit a phase transition from Fm3¯ m to R3¯. The R3¯ phases exhibit negative linear compressibility over a limited pressure range. A further transition with phase coexistence occurs at ∼2.5-3.0 GPa for NaNbF6 and ∼4.5 GPa for NaTaF6. Compression of NaNbF6 in helium at room temperature and below provides no evidence for helium penetration into the structure to form a perovskite with helium on the A-site, as was previously reported for CaZrF6.

Original languageEnglish
Pages (from-to)13979-13987
Number of pages9
JournalInorganic Chemistry
Volume59
Issue number19
DOIs
StatePublished - Oct 5 2020

Funding

We are grateful for experimental assistance from the staff of beamline 17- BM at the Advanced Photon Source and both the sample environment team, and instrument staff of the SNAP beamline, at the Spallation Neutron Source. The work at Georgia Tech was partially financially supported under NSF DMR-1607316 and NSF DMR-2002739. The research made use of the Advanced Photon Source, a U.S. Department of Energy (DOE) Office of Science User Facility operated for the DOE Office of Science by Argonne National Laboratory under Contract No. DE-AC02-06CH11357. A portion of this research used resources at the Spallation Neutron Source, a DOE Office of Science User Facility operated by the Oak Ridge National Laboratory.

FundersFunder number
National Science Foundation2002739, DMR-1607316, 1607316, DMR-2002739
U.S. Department of Energy
Office of Science
Argonne National LaboratoryDE-AC02-06CH11357

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