Abstract
Co2 (OH) AsO4 has been prepared by hydrothermal synthesis and characterized from x-ray and neutron powder diffraction. The structure consists of a three-dimensional framework in which Co (1) O 5 -trigonal bipyramid dimers and Co (2) O6-octahedra chains are simultaneously present. The magnetic structure has been determined by neutron (D2B and D1B) powder-diffraction data. Below 22 K, the Co2 (OH) AsO4 phase shows an incommensurate antiferromagnetic structure along the b direction. The propagation vector (0,δ,0) is temperature dependent with a value of δ=0.430 at the lowest temperature (1.8 K). Magnetization measurements of Co2 (OH) AsO4 show a complex magnetic behavior with the presence of three different signals. Between 6 and 21 K, a strong dependence of the magnetic field is observed with a shift of the inflexion point associated to the three-dimensional antiferromagnetic ordered from 18 K at 1 kOe to 20.1 K at 90 kOe. The small splitting observed in the zero-field-cooled-field-cooled curves at low temperatures is characteristic of ferromagnetic interactions but saturation is not reached even up to 90 kOe. Heat-capacity measurements show an unusual dependence on the magnetic field for antiferromagnetic transitions with a jump at the Neél temperature quite small (2 J/Kmol). The magnetic contribution exhibits a λ -type anomaly associated to the three-dimensional antiferromagnetic ordering. Surprisingly, the λ anomaly grows with the magnetic field and becomes better defined. Neutron powder diffraction in different fields shows a magnetic phase transition. The incommensurate magnetic structure evolves at low temperatures toward a collinear AF phase for fields higher than 35 kOe. © 2010 The American Physical Society.
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CITATION STYLE
De Pedro, I., Rojo, J. M., Rodríguez Fernández, J., Fernández-Díaz, M. T., & Rojo, T. (2010). Sinusoidal magnetic structure in a three-dimensional antiferromagnetic Co2 (OH ) AsO4: Incommensurate-commensurate magnetic phase transition. Physical Review B - Condensed Matter and Materials Physics, 81(13). https://doi.org/10.1103/PhysRevB.81.134431
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