2002
DOI: 10.1016/s0039-6028(02)01888-5
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Theoretical and experimental energy barriers associated with the incorporation of excess As into GaAs()

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Cited by 4 publications
(4 citation statements)
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“…The interaction energy between the cluster and the Ga atom is defined as the total energy of the system minus the sum of the total energies of the separated reactants ͑i.e., the Ga atom infinitely far away from the respective cluster͒. The applied method is similar to our earlier calculations, [10][11][12] in which, however, the surfaces had been left unreconstructed. Our calculations are performed with the GAUSSIAN 94 program package 13 on a Fujitsu VP parallel vector computer.…”
Section: Methodsmentioning
confidence: 95%
“…The interaction energy between the cluster and the Ga atom is defined as the total energy of the system minus the sum of the total energies of the separated reactants ͑i.e., the Ga atom infinitely far away from the respective cluster͒. The applied method is similar to our earlier calculations, [10][11][12] in which, however, the surfaces had been left unreconstructed. Our calculations are performed with the GAUSSIAN 94 program package 13 on a Fujitsu VP parallel vector computer.…”
Section: Methodsmentioning
confidence: 95%
“…In this way a cage forms (one Ga atom: half cage; two Ga atoms: full cage) which stabilizes the interstitial As atom, as described before [20]. Now, the main difference between our model [26] and a model described by Suda and Otsuka [11] is that we regard the escape of the As 2 molecule from the interstitial position as the thermodynamically activated process, since the activation energy in our model (~68 meV) is comparable with the kinetic energy of particles at the considered growth temperature range (40-70 meV). In contrast to our model, Suda and Otsuka considered the desorption of As from adsorption layer, which requires an activation energy at least one order of magnitude higher (~1 eV) than thermal energies.…”
Section: Introductionmentioning
confidence: 92%
“…The energy of the system was calculated by DFT/B3LYP/6-31++G method. The applied method is similar to that used in our earlier calculations [20,26,27]. The calculations are performed with the GAUSSIAN 03 program package [28] on a SunFire 15000 supercomputer.…”
Section: Introductionmentioning
confidence: 99%
“…the Ga atom infinitely far away from the respective cluster, for details see [32]). The applied method is similar to our earlier calculations [34][35][36] in which, however, the surface had been left unreconstructed. All ab-initio calculations were performed with the GAUSSIAN 94 program package [37].…”
Section: Antisite Defectsmentioning
confidence: 99%