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Absolute optical rotation of CsLiB 6 O 10
Author(s) -
HerrerosCedrés Javier,
Kaminsky Werner,
HernándezRodriguez Cecilio
Publication year - 2005
Publication title -
journal of applied crystallography
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.429
H-Index - 162
ISSN - 1600-5767
DOI - 10.1107/s0021889805009908
Subject(s) - refractive index , optical rotation , rotation (mathematics) , bar (unit) , wavelength , electron density , optics , chemistry , crystal (programming language) , materials science , crystallography , analytical chemistry (journal) , physics , electron , mathematics , geometry , quantum mechanics , meteorology , chromatography , computer science , programming language
The optical rotation (OR) of CsLiB 6 O 10 (CLBO, space group ) along the a axis has been determined by the HAUP method [Kobayashi & Uesu (1983). J Appl. Cryst. 16 , 204–211] at a wavelength of 632.8 nm and by the TILTER method [Kaminsky & Glazer (1996). Ferroelectrics , 183 , 133–141] at 532 nm and 650 nm. The respective rotatory powers were found to be 17 (1), 24 (2) and 19 (2)° mm −1 . The absolute chirality has been established by comparing Bijvoet differences, { hkl } and {}, on the same crystal on which OR was measured. Atomic positions and electron density Fourier peak heights were exploited as input for semi‐empirical calculations of refractive indices and OR, using WinOPTACT [Glazer (2002). J. Appl. Cryst. 35 , 652] with only one free parameter fitted to match the average refractive index.
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