Thermodynamics of the pseudobinary GaAs1-xBix (0 ≤ x ≤ 1) alloys studied by different exchange-correlation functionals, special quasi-random structures and Monte Carlo simulations
2015 (English)In: Computational Condensed Matter, ISSN 2352-2143, Vol. 5, 7-13 p.Article in journal (Refereed) PublishedText
GaAs<inf>1-x</inf>Bi<inf>x</inf> alloys have useful properties for many optoelectronic applications. Although the crystal growth by molecular beam epitaxy is influenced by kinetics, it is also important to understand the thermodynamics of the alloys. The Gibbs formation energies and the immiscibility curve of the totally disordered GaAs<inf>1-x</inf>Bi<inf>x</inf> (0 ≤ x ≤ 1) are determined using special quasi-random structures (SQS) of different sizes, different exchange-correlation functionals and Monte Carlo simulations. The local density approximation gives slightly larger mixing enthalpies and smaller Bi solubilities than the generalized gradient approximation for the GaAs<inf>1-x</inf>Bi<inf>x</inf> alloys, if the semiconducting GaAs and metallic Ga and Bi are reference states. The 64 and 512 atom SQS give similar mixing enthalpies, except at x = 0.5, where as eight atom SQS overestimate the mixing enthalpy significantly. The disordered alloys are more stable than the most stable ordered phases except at very low temperatures. The spinodal transformation temperature corresponds approximately to the latest experimental results, if the separated systems can conform to their own lattice constants. The spinodal transformation temperature is decreased very significantly, if the decomposing phases are constrained to maintain lattice coherence with the substrate. The strain energies of the alloys and decomposing phases are large also at the surfaces.
Place, publisher, year, edition, pages
Elsevier, 2015. Vol. 5, 7-13 p.
Bismide, Gallium arsenide, Gibbs free energy, Immiscibility, Spinodal decomposition, Surface
Other Materials Engineering
IdentifiersURN: urn:nbn:se:kth:diva-181836DOI: 10.1016/j.cocom.2015.09.002ScopusID: 2-s2.0-84942316925OAI: oai:DiVA.org:kth-181836DiVA: diva2:902419
QC 201602112016-02-112016-02-052016-02-11Bibliographically approved