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Ab initio prediction of quadruple perovskites with half-metallic ferrimagnetism and high Curie temperatures

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Abstract

CaCu3Fe2Re2O12, a quadruple perovskite (QP) with the chemical formula AA’3B2B’2O12, shows half-metallic ferrimagnetism with large magnetization and a high Curie temperature (TC). Here we investigated a series of QPs using density functional theory and Monte Carlo simulations. We found that all compounds are ferrimagnetic with substituted A2+ (A=Ca, Sr, Ba, Pb) ions exhibiting high Tc (above 405 K), and the A3+ (A=Sc, Y, La ) substituted ones yielding even higher TC (above 502 K). By examining interatomic exchange parameters, we found that the antiferromagnetic exchange couplings between Re and Cu as well as Re and Fe are responsible for this very high Curie temperature. For the compounds with A3+ substitution, electron doping in bands around the Fermi level dominated by the Re ions strengthen the Re-Cu and Re-Fe exchange interactions, which cause an increase in the TC. This work demonstrates a design strategy of enhancing the spin ordering temperature by replacing A-site non-magnetic ions.

Presenters

  • duo wang

    Physics and Astronomy, Uppsala University, Department of Physics and Astronomy, Uppsala University

Authors

  • duo wang

    Physics and Astronomy, Uppsala University, Department of Physics and Astronomy, Uppsala University

  • Monirul Shaikh

    Physics and Nanotechnology, SRM Institute of Science and Technology, Dept. of Physics and Nanotechnology, SRM Institute of Science and Technology

  • Saurabh Ghosh

    Physics and Nanotechnology, SRM Institute of Science and Technology, Department of Physics and Nanotechnology, SRM Institute of Science and Technology, Kattankulathur 603 203, Tamil Nadu, India, Dept. of Physics and Nanotechnology, SRM Institute of Science and Technology, Department of Physics and Nanotechnology, SRM Institute of Science and Technology, Kattankulathur - 603 203, Tamil Nadu, India

  • Biplab Sanyal

    Physics and Astronomy, Uppsala University, Uppsala University, Department of Physics and Astronomy, Uppsala University