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arXiv · 2303.01108

Evolution of complex magnetic phases and metal-insulator transition through Nb substitution in La$_{0.5}$Sr$_{0.5}$Co$_{1-x}$Nb$_x$O$_3$

Abstract

We report the evolution of structural, magnetic, transport, and electronic properties of bulk polycrystalline La$_{0.5}$Sr$_{0.5}$Co$_{1-x}$Nb$_x$O$_3$ ($x =$ 0.025--0.25) samples. The Rietveld refinement of the x-ray diffraction patterns with R$\bar3$c space group reveals that the lattice parameters and rhombohedral distortion monotonously increase with the Nb$^{5+}$(4$d^0$) substitution ($x$). The magnetic susceptibility exhibits a decrease in the magnetic ordering temperature and net magnetization with $x$, which manifests that the Nb substitution dilutes the ferromagnetic (FM) double exchange interaction and enhances the antiferromagnetic (AFM) super-exchange interaction. Interestingly, for the $x>$ 0.1 samples the FM order is completely suppressed and the emergence of a glassy state is clearly evident. Moreover, the decrease in the coercivity (H$\rm_{C}$) and remanence (M$\rm_{r}$) with $x$ in the magnetic isotherms measured at 5~K further confirms the dominance of AFM interactions and reduction of FM volume fraction for the $x>$ 0.1 samples. More interestingly, we observe resistivity minima for the $x=$ 0.025 and 0.05 samples, which are analyzed using the quantum corrections in the conductivity, and found that the weak localization effect dominates over the renormalized electron-electron interactions in the 3D limit. Further, a semiconducting resistivity behavior is obtained for $x>$ 0.05, which follows the Arrhenius law at high temperatures ($\sim$160--320~K), and the 3D-variable range hopping prevails in the low-temperature region ($<$160~K). The core-level photoemission spectra confirm the valence state of constituent elements and the absence of Co$^{2+}$ is discernible.

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Rishabh Shukla, R. S. Dhaka. 2023-03-02. Evolution of complex magnetic phases and metal-insulator transition through Nb substitution in La$_{0.5}$Sr$_{0.5}$Co$_{1-x}$Nb$_x$O$_3$. https://doi.org/10.1103/physrevb.107.165108

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