A UNIVERSAL TREATMENT OF X-RAY AND NEUTRON-DIFFRACTION IN CRYSTALS .2. EXTINCTION

Authors
Citation
Hc. Hu, A UNIVERSAL TREATMENT OF X-RAY AND NEUTRON-DIFFRACTION IN CRYSTALS .2. EXTINCTION, Acta crystallographica. Section A, Foundations of crystallography, 53, 1997, pp. 493-504
Citations number
37
Categorie Soggetti
Crystallography
ISSN journal
01087673
Volume
53
Year of publication
1997
Part
4
Pages
493 - 504
Database
ISI
SICI code
0108-7673(1997)53:<493:AUTOXA>2.0.ZU;2-R
Abstract
Based on the formalism for calculating the integrated reflection power ratio of a plane mosaic crystal by using three dimensionless paramete rs as described in paper I [Hu (1997). Acta Cryst. A53, 000-000], exac t and universal expressions for the secondary-extinction factors in X- ray and neutron crystallography are developed that can be applied to r eflections of all possible values of extinction factor, reflection sym metry and the absorption-to-scattering cross-section ratio of the crys tal. The representation by three parameters gives a clear and definite physical meaning to the concept of extinction. The theory has been ex tended to treat the extinction of a spherical crystal, and the strikin g difference in the evaluated secondary-extinction factor between the equivalent single-plate and the exact method in the spherical-crystal treatment under theta(B) = 0 degrees is explained. As a demonstration of the feasibility of using these expressions, the diffraction data fo r LiF and MgO crystal plates measured by Lawrence [Acta Cryst. (1972), A28, 400-404; (1973), A29, 208-210] are reanalyzed by this method. Al l the reflections including the strongest ones (Y-o down to 0.026) are reanalyzed simultaneously with single-valued particle size and mosaic spread as fitting parameters and allowing for primary extinction if n ecessary. The results (R factor = 0.014 and 0.053 for LiF and MgO, res pectively) are unprecedentedly good. Furthermore, in disagreement with Lawrence, the extinction of LiF is found to be of secondary type and in the case of MgO both primary and secondary extinction should be con sidered. The analysis also shows that the formula Y similar to YpYs is valid only for very weak extinctions and that the Hamilton-Darwin equ ations are valid in a range much broader than previously anticipated.