A TEST OF THE IMPORTANCE OF WEAK REFLECTIONS IN RESOLVING A SPACE-GROUP AMBIGUITY INVOLVING THE PRESENCE OR ABSENCE OF AN INVERSION CENTER

Citation
D. Kassner et al., A TEST OF THE IMPORTANCE OF WEAK REFLECTIONS IN RESOLVING A SPACE-GROUP AMBIGUITY INVOLVING THE PRESENCE OR ABSENCE OF AN INVERSION CENTER, Acta crystallographica. Section B, Structural science, 49, 1993, pp. 646-654
Citations number
27
Categorie Soggetti
Crystallography
ISSN journal
01087681
Volume
49
Year of publication
1993
Part
4
Pages
646 - 654
Database
ISI
SICI code
0108-7681(1993)49:<646:ATOTIO>2.0.ZU;2-W
Abstract
The structure of margarite, CaAl2[Al2Si2O10](OH)2, has been reported i n space group C2/c, and in the corresponding non-centrosymmetric space group Cc. Previous refinements of margarite in space group Cc were ma rred by strong correlations affecting parameters that are inversion re lated in C2/c. Refinement of single-crystal X-ray diffraction data, co llected with synchrotron radiation, converged without large correlatio ns in Cc. The refinement was based on 4056 F(obs), without merging Fri edel pairs, including all the weak reflections (R = 0.027). No atom in Cc is removed further than 0.08 angstrom from its corresponding posit ion in C2/c. The R in space group C2/c, after merging of the Friedel m ates, was 0.059 (2658 F(obs)). For the weak F(obs) the disagreement in space group C2/c is much worse than in Cc. This agrees with the wamin g that it is the weak F(obs) which are most sensitive to small non-cen trosymmetric distortions [Schomaker & Marsh (1979). Acta Cryst. B35, 1 933-1934]. Removing weak F(obs) from the data results in a data set re sembling one that could have been collected using an X-ray tube (with omission of weak F(obs)). In the Cc model without weak F(obs) many of the correlation coefficients rose dramatically to values over 0.9, and consequently difficulties occurred in converging the refinement and t he estimated standard deviations increased fourfold compared to the va lues obtained for refinement of the full data set. Therefore, if one w ishes to resolve a space-group ambiguity: (1) one should collect preci se data, and especially collect as many weak reflections as precisely as possible; (2) one should include all reflections in the refinement, even if this raises the R value - a more complete data set, with a hi gher R value may be more important in establishing the symmetry than a smaller data set with a lower R value; (3) when measuring at a synchr otron one should use a wavelength which emphasizes the anomalous-dispe rsion contribution in order to make the differences between the Friede l pairs more significant.