Crystallographic and magnetic structure of SrCoO2.5 brownmillerite:: Neutron study coupled with band-structure calculations
Crystallographic and magnetic structure of SrCoO2.5 brownmillerite:: Neutron study coupled with band-structure calculations
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DOI:
10.1103/physrevb.78.054404
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发表时间:
2008-08-01
影响因子:
3.7
通讯作者:
Rivas, J.
中科院分区:
文献类型:
--
作者:
Munoz, A.;de la Calle, C.;Rivas, J.
A study of the crystallographic and magnetic structure of SrCoO(2.5) with a brownmillerite-type structure has been carried out from neutron powder-diffraction (NPD) measurements at temperatures ranging from 10 to 623 K, across the Neel temperature (T(N)=537 K) of this anti ferromagnetic oxide. The study has been complemented with differential scanning calorimeter (DSC), dc susceptibility and magnetization measurements. Although the refinement of the crystal structure from NPD data is possible in the orthorhombic Pnma and Ima2 space groups, the support of ab-initio band-structure calculations has allowed us to select, without ambiguity, the Ima2 space group as the ground state for SrCoO(2.5) brownmillerite. In Ima2 the crystallographic structure of SrCoO(2.5) is described as layers of corner-sharing Co1O(6) octahedra alternating along the a axis with layers of vertex-sharing Co2O(4) tetrahedra, conforming chains running along the [0 0 1] direction. The magnetic structure below T(N)=537 K is G-type with the magnetic moments directed along the c axis. This magnetic arrangement is stable from T(N) down to 10 K. At T=10 K, the magnetic moment values for Co1 and Co2 atoms are 3.12(13) mu B and 2.88(14) mu B, respectively, compatible with a Co(2+)L state, where L stands for a ligand hole. The magnetic susceptibility curves show, below 200 K, a divergence of zero-field cooling and field cooling curves, displaying broad maxima which are interpreted as due to the presence of ferromagnefic clusters embedded into an anti ferromagnetic matrix. These inhomogeneities are inherent to the synthesis process, by quenching microcrystalline samples of SrCoO(3-x) composition from high temperature, where cubic, ferromagnetic perovskites have been identified by diffraction methods.