Measuring the density, viscosity, and surface tension of molten titanates using electrostatic levitation in microgravity

Author:

Wilke Stephen K.12ORCID,Al-Rubkhi Abdulrahman1ORCID,Menon Vrishank1,Rafferty Jared1,Koyama Chihiro3ORCID,Ishikawa Takehiko3ORCID,Oda Hirohisa3ORCID,Hyers Robert W.45ORCID,Bradshaw Richard C.46ORCID,Kastengren Alan L.2ORCID,Kohara Shinji7ORCID,SanSoucie Michael8ORCID,Phillips Brandon8,Weber Richard12ORCID

Affiliation:

1. Materials Development, Inc 1 ., Evanston, Illinois 60202, USA

2. X-ray Science Division, Advanced Photon Source, Argonne National Laboratory 2 , Lemont, Illinois 60439, USA

3. Japan Aerospace Exploration Agency 3 , Tsukuba, Japan

4. Department of Mechanical & Materials Engineering, Worcester Polytechnic Institute 4 , Worcester, Massachusetts 01609, USA

5. RHA Materials, LLC 5 , Winchester, Massachusetts 01890, USA

6. RCB Worx Consulting 6 , Belmont, Massachusetts 02478, USA

7. Quantum Beam Diffraction Group, Center for Basic Research on Materials, National Institute for Materials Science 7 , 1-2-1 Sengen, Tsukuba, Ibaraki 305-0047, Japan

8. NASA Marshall Space Flight Center 8 , Huntsville, Alabama 35812, USA

Abstract

Rare earth and barium titanates are useful as ferroelectric, dielectric, and optical materials. Measurements of their thermophysical properties in the liquid state can help guide melt processing technologies for their manufacture and advance understanding of fragile liquids' behavior and glass formation. Here, we report the density, thermal expansion, viscosity, and surface tension of molten BaTi2O5, BaTi4O9, and 83TiO2-17RE2O3 (RE = La or Nd). Measurements were made using electrostatic levitation and droplet oscillation techniques in microgravity, which provide access to quiescent liquid droplets and deep supercooling of 510–815 K below the equilibrium melting points. Densities were measured over 900–2400 K. Viscosities were similar for all four compositions, increasing from ∼10 mPa s near 2100 K to ∼30 mPa s near 1750 K. Surface tensions were 450–490 dyn cm−1 for the rare earth titanates and 383–395 dyn cm−1 for the barium titanates; surface tensions of all compositions had small or negligible temperature dependence over 1700–2200 K. For solids recovered after melt quenching, x-ray microtomography revealed the fracture mechanics in crystalline products and minimal internal porosity in glass products, likely arising from entrapped gas bubbles. Internal microstructures were generally similar for products processed either in microgravity or in a terrestrial aerodynamic levitator.

Funder

National Aeronautics and Space Administration

Japan Society for the Promotion of Science

Publisher

AIP Publishing

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