Perovskite solid solutions–a Monte Carlo study of the deep earth analogue (K, Na)MgF3
- Авторы: Tealdi C.1, Lavrentiev M.Y.2, Mohn C.E.3, Allan N.L.4
-
Учреждения:
- Department of Chemistry
- United Kingdom Atomic Energy Authority
- Centre for Earth Evolution and Dynamics (CEED)
- School of Chemistry
- Выпуск: Том 57, № 2 (2016)
- Страницы: 257-266
- Раздел: Article
- URL: https://bakhtiniada.ru/0022-4766/article/view/159358
- DOI: https://doi.org/10.1134/S0022476616020037
- ID: 159358
Цитировать
Аннотация
Understanding the behaviour of solid solutions over wide ranges of temperature and pressure remains a major challenge to both theory and experiment. Here we report a detailed exchange Monte Carlo study using a classical ionic model of the model perovskite parascandolaite-neighborite (K,Na)MgF3 solid solution and its end-members for temperatures in the range 300-1000 K and pressures from 0-8 GPa. Full account is taken of the local environment of the individual cations, clustering and thermal effects. Properties considered include the crystal structure, phase transitions, the thermodynamics of mixing and the non-ideality of the solid solution. Clustering of the potassium ions is examined via a short-range order parameter. Where experimental data are available for comparison, agreement is very good.
Ключевые слова
Об авторах
C. Tealdi
Department of Chemistry
Email: mikhail.lavrentiev@ukaea.uk
Италия, Pavia
M. Lavrentiev
United Kingdom Atomic Energy Authority
Автор, ответственный за переписку.
Email: mikhail.lavrentiev@ukaea.uk
Великобритания, Abingdon
C. Mohn
Centre for Earth Evolution and Dynamics (CEED)
Email: mikhail.lavrentiev@ukaea.uk
Норвегия, Oslo
N. Allan
School of Chemistry
Email: mikhail.lavrentiev@ukaea.uk
Великобритания, Bristol
Дополнительные файлы
