Abstract
The origin of the long-wavelength incommensurate magnetic structure of is discussed considering possible interchains super-superexchange paths. The experimental value of the propagation vector with can be reproduced only if one considers the next-nearest super-superexchange interaction. A spin-dimer analysis using the extended Huckel tight-binding method confirms that, despite longer interatomic Co-Co distances, the latter interaction is indeed much stronger. The stability of the observed structure with respect to certain commensurate states is discussed.
- Received 20 November 2008
DOI:https://doi.org/10.1103/PhysRevB.80.172405
©2009 American Physical Society