Structure of liquid tricalcium aluminate

James W. E. Drewitt, Adrian C. Barnes, Sandro Jahn, Simon C. Kohn, Michael J. Walter, Alexey N. Novikov, Daniel R. Neuville, Henry E. Fischer, and Louis Hennet
Phys. Rev. B 95, 064203 – Published 1 February 2017

Abstract

The atomic-scale structure of aerodynamically levitated and laser-heated liquid tricalcium aluminate (Ca3Al2O6) was measured at 2073(30) K by using the method of neutron diffraction with Ca isotope substitution (NDIS). The results enable the detailed resolution of the local coordination environment around calcium and aluminum atoms, including the direct determination of the liquid partial structure factor, SCaCa(Q), and partial pair distribution function, gCaCa(r). Molecular dynamics (MD) simulation and reverse Monte Carlo (RMC) refinement methods were employed to obtain a detailed atomistic model of the liquid structure. The composition Ca3Al2O6 lies at the CaO-rich limit of the CaO:Al2O3 glass-forming system. Our results show that, although significantly depolymerized, liquid Ca3Al2O6 is largely composed of AlO4 tetrahedra forming an infinite network with a slightly higher fraction of bridging oxygen atoms than expected for the composition. Calcium-centered polyhedra exhibit a wide distribution of four- to sevenfold coordinated sites, with higher coordinated calcium preferentially bonding to bridging oxygens. Analysis of the MD configuration reveals the presence of 10% unconnected AlO4 monomers and Al2O7 dimers in the liquid. As the CaO concentration increases, the number of these isolated units increases, such that the upper value for the glass-forming composition of CaO:Al2O3 liquids could be described in terms of a percolation threshold at which the glass can no longer support the formation of an infinitely connected AlO4 network.

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  • Received 9 December 2016

DOI:https://doi.org/10.1103/PhysRevB.95.064203

©2017 American Physical Society

Physics Subject Headings (PhySH)

Condensed Matter, Materials & Applied Physics

Authors & Affiliations

James W. E. Drewitt1,*, Adrian C. Barnes2, Sandro Jahn3, Simon C. Kohn1, Michael J. Walter1, Alexey N. Novikov4,5, Daniel R. Neuville4, Henry E. Fischer6, and Louis Hennet5

  • 1School of Earth Sciences, University of Bristol, Wills Memorial Building, Queens Road, Bristol, BS8 1RJ, United Kingdom
  • 2H H Wills Physics Laboratory, University of Bristol, Bristol, BS8 1TL, United Kingdom
  • 3Institute of Geology and Mineralogy, University of Cologne, Zuelpicher Str. 49b, 50674 Cologne, Germany
  • 4Institut de Physique du Globe de Paris, CNRS-IPGP, Géomatériaux, Sorbonne Paris Cité, 1 rue Jussieu, 75005 Paris, France
  • 5Conditions Extrêmes et Matériaux : Haute Température et Irradiation, CEMHTI-CNRS, Université d'Orléans, 1d avenue de la Recherche Scientifique, 45071 Orléans cedex 2, France
  • 6Institut Laue-Langevin, 71 avenue des Martyrs, CS 20156, 38042 Grenoble cedex 9, France

  • *james.drewitt@bristol.ac.uk

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Vol. 95, Iss. 6 — 1 February 2017

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