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dc.contributorNISTen_US
dc.contributorBrown Universityen_US
dc.contributorNISTen_US
dc.contributor.authorBurton, Bejnamin P.
dc.contributor.authorvan de Walle, Axel
dc.contributor.authorkattner, Ursula
dc.contributor.otherbenjamin.burton@nist.goven_US
dc.date.accessioned2014-11-20T17:12:49Z
dc.date.available2014-11-20T17:12:49Z
dc.date.issued2014-11-20
dc.identifier.citationJournal of Applied Physics 100, 113528 (2006).en_US
dc.identifier.urihttp://hdl.handle.net/11256/116
dc.description.abstractFirst principles phase diagram calculations were performed for the wurtzite-structure quasibinary systems AlN–GaN, GaN–InN, and AlN–InN. Cluster expansion Hamiltonians that excluded, and included, excess vibrational contributions to the free energy, Fvib, were evaluated. Miscibility gaps are predicted for all three quasibinaries, with consolute points, XC,TC , for AlN–GaN, GaN–InN, and AlN–InN equal to 0.50, 305 K , 0.50, 1850 K , and 0.50, 2830 K without Fvib, and 0.40, 247 K , 0.50, 1620 K , and 0.50, 2600 K with Fvib, respectively. In spite of the very different ionic radii of Al, Ga, and In, the GaN–InN and AlN–GaN diagrams are predicted to be approximately symmetric.en_US
dc.relation.uri10.1063/1.2372309en_US
dc.subjectAlN-GaN; GaN-InN; AlN-InN; First Principles Phase Diagram Calculation; Excess vibrational entropyen_US
dc.titleFirst principles phase diagram calculations for the wurtzite-structure systems AlN-GaN, GaN-InN, and AlN-InNen_US


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