A global optimisation study of the low-lying isomers of the alumina octomer (AlO)
arXiv:1810.01957 · doi:10.1016/j.cplett.2018.09.018
Abstract
We employ the Monte-Carlo Basin-Hopping (MC-BH) global optimisation technique with inter- atomic pair potentials to generate low-energy candidates of stoichiometric alumina octomers ((AlO)). The candidate structures are subsequently refined with density functional theory calculations employing hybrid functionals (B3LYP and PBE0) and a large basis set (6-311+G(d)) including a vibrational analysis. We report the discovery of a set of energetically low-lying alumina octomer clusters, including a new global minimum candidate, with shapes that are elongated rather than spherical. We find a stability limit for these and smaller-sized clusters at a temperature of K corresponding to a phase transition in liquid alumina.
arXiv comment19 pages, 9 figures, accepted for publication
References in corpus (6)
- Dust formation in the oxygen-rich AGB star IK Tau
- Aluminum-, Calcium- And Titanium-Rich Oxide Stardust In Ordinary Chondrite Meteorites
- Tracing the phase transition of Al-bearing species from molecules to dust in AGB winds. Constraining the presence of gas-phase (Al2O3)n clusters
- Automated NanoSIMS Measurements of Spinel Stardust from the Murray Meteorite
- New insights into the dust formation of oxygen-rich AGB stars
- Silicate condensation in Mira variables
Cited by in corpus (11)
- Evolution and Mass Loss of Cool Ageing Stars: a Daedalean Story
- Bottom-up dust nucleation theory in oxygen-rich evolved stars I. Aluminium oxide clusters
- Developing a self-consistent AGB wind model: II. Non-classical, non-equilibrium polymer nucleation in a chemical mixture
- ATOMIUM: ALMA tracing the origins of molecules in dust forming oxygen rich M-type stars: Motivation, sample, calibration, and initial results
- Data availability and requirements relevant for the Ariel space mission and other exoplanet atmosphere applications
- Comparison of aluminum oxide empirical potentials from cluster to nanoparticle
- Revisiting fundamental properties of TiO nanoclusters as condensation seeds in astrophysical environments
- Dust in brown dwarfs and extra-solar planets. VIII. TiO seed formation: 3D Monte Carlo versus kinetic approach
- Impact of metals on (star)dust chemistry: a laboratory astrophysics approach
- Vanadium oxide clusters in substellar atmospheres: A quantum chemical study
- The Ionization Energies of Dust-Forming Metal Oxide Clusters