Electronic structure and magnetic properties of RMnX (R= Mg, Ca, Sr, Ba, Y; X= Si, Ge) studied by KKR method

Abstract

Electronic structure calculations, using the charge and spin self-consistent Korringa- Kohn-Rostoker (KKR) method, have been performed for several RMnX compounds (R = Mg, Ca, Sr, Ba, Y; X = Si, Ge) of the CeFeSi-type structure. The origin of their magnetic properties has been investigated emphasizing the role of the Mn sublattice. The significant influence of the Mn-Mn and Mn-X interatomic distances on the Mn magnetic moment value is delineated from our computations, supporting many neutron diffraction data. We show that the marked change of μMn with the Mn-Mn and Mn-X distances resulted from a redistribution between spin-up and spin-down d-Mn DOS rather than from different fillings of the Mn 3d-shell. Bearing in mind that the neutron diffraction data reported for the RMnX compounds are rather scattered, the KKR computations of μMn are in fair agreement with the experimental values. Comparing density of states near EF obtained in different magnetic orderings, one can notice that the entitled RMnX systems seem to 'adapt' their magnetic structures to minimize the DOS in the vicinity of the Fermi level. Noteworthy, the SrMnGe antiferromagnet exhibits a pseudo-gap behaviour at EF, suggesting anomalous electron transport properties. In addition, the F-AF transition occurring in the disordered La1-xYxMnSi alloy for the 0.8<x<1 range is well supported by the DOS features of La0.2Y0.8MnSi. In contrast to the investigated RMnX compounds, YFeSi was found to be non-magnetic, which is in excellent agreement with the experimental data.

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