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Published June 2013 | public
Journal Article

Refractive index and optical dispersion of In_2O_3, InBO_3 and gahnite

Abstract

Refractive indices of In_2O_3, In_(2−x)Sn_xO_3, InBO_3 and 2 different gahnite crystals (Zn_(0.95)Fe_(0.05)Al_2O_4 and Zn_(0.91)Mg_(0.04)Mn_(0.03)Fe_(0.03)Al_(1.99)Fe_(0.01)O_4) were measured at wavelengths of 435.8–643.8 nm and were used to calculate n (n_D) at λ = 589.3 nm and (n_∞) at λ = ∞ with the one-term Sellmeier equation 1/(n^2 − 1) = −A/λ^2 + B. Total polarizabilities, α_(total), were calculated from n_∞ and the Lorenz–Lorentz equation. Refractive indices, n_D and dispersion values, A, are, respectively, 2.093 and 133 × 10^(−16) m^2 for In_2O_3; 2.0755 and 138 × 10^(−16) m^2 for In_(2−x)Sn_xO_3; 1.7995 and 56 × 10^(−16) m^2 for Zn_(0.95)Fe_(0.05)Al_2O_4; 1.7940 and 57 × 10^(−16) m^2 for Zn_(0.91)Mg_(0.04)Mn_(0.03)Fe_(0.03)Al_(1.99)Fe_(0.01)O_4 and n_o = 1.8782 and n_e = 1.7756 and 〈63〉 × 10^(−16) m^2 for InBO_3. The lack of consistency of the polarizabilities of Zn^(2+) in ZnO and In^(3+) in In_2O_3 with the Zn_(2+) and In3+ polarizabilities in other Zn- and In-containing compounds is correlated with structural strain and very high dispersion of ZnO and In_2O_3.

Additional Information

© 2013 Elsevier Ltd. Received 14 February 2013. Accepted 18 February 2013. Available online 28 February 2013. We are indebted to Chi Ma at the Caltech Analytical Facility for microprobe analyses of the In2O3, InBO3 and gahnite samples and to Dieter Dettmar for skillful preparation of crystal prisms. Brian Cook originally provided the specimen of gahnite1 from his mine and Prof. Robert Dymek originally provided the specimen and analysis of gahnite2 from the Harvard mineral collection. The analyses were supported, in part, by the National Science Foundation grant EAR-0947956 to GRR. Work at Oregon State University was supported by National Science Foundation grant DMR-0804167 to MAS.

Additional details

Created:
August 22, 2023
Modified:
October 24, 2023