Author:
Mombourquette Michael J.,Weil John A.
Abstract
In this paper, the second of a series devoted to developing quantitative understanding of defect species in silicates, we report ab initio self-consistent-field molecular-orbital calculations done on 10-atom and 22-atom clusters designed to simulate cation-compensated aluminum impurity centres [AlO4/M+]qt in alpha-quartz; here qt = 0 or + 1, and M = H, Li, or Na. The geometric configurations of the small models of these centres were optimized. The calculated values for total energies, various static structural parameters, electron-spin densities, net atomic charges, and orbital energies are compared with experimental data, especially those derived from electron-paramagnetic-resonance studies of hole centres and give good agreement. For example, the models predict that the holes will occur at opposite types of oxygen ions adjacent to Al3+, respectively, for uncompensated centres [AlO4]0 and for the centres [AlO4/M+]+, as is, in fact, observed. Some calculations for interstitial cations M+ and atomic hydrogen on clusters simulating large-channel c-axis oxygen sites of alpha-quartz are reported. Various reaction energies involving the aluminum centres and the interstitial species are listed.
Publisher
Canadian Science Publishing
Subject
General Physics and Astronomy
Cited by
38 articles.
订阅此论文施引文献
订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献