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Investigation of lattice dynamics, magnetism and electronic transport in $\beta$-Na$_{0.33}$V$_2$O$_{5}$

Authors :
Shukla, Rishabh
Ulrich, Clemens
Dhaka, R. S.
Source :
Physical Review B, 106, 125148 (2022)
Publication Year :
2022

Abstract

We investigate the electronic and magnetic properties as well as lattice dynamics and spin-phonon coupling of $\beta$-Na$_{0.33}$V$_2$O$_5$ using temperature-dependent Raman scattering, dc-magnetization and dc-resistivity, x-ray photoemission, and absorption spectroscopy. The Rietveld refinement of XRD pattern with space group C2/m confirms the monoclinic structure. The analysis of temperature-dependent Raman spectra in a temperature range of 13--673~K reveals an anharmonic dependence of the phonon frequency and full width at half maximum, which is accredited to the symmetric phonon decay. However, below about 40 K, the hardening of the phonon frequency beyond anharmonicity is attributed to the spin-phonon coupling. Interestingly, the estimated effective magnetic moment $\mu_{\rm eff}=$ 0.63~$\mu_B$ from the magnetization data manifests a mixed-valence state of V ions in 4+ (18$\pm$1\%) and 5+ (82$\pm$1\%). A similar ratio of V$^{4+}$ to V$^{5+}$ is also observed in the x-ray photoemission and x-ray absorption near-edge spectra and that is found to be consistent with the sample stoichiometry. In addition, the V$^{4+}$ ions are distributed between different vanadium (V1 and V3) sites. The analysis of extended x-ray absorption fine structure at different V-sites gives the corresponding V--O bond lengths, which are utilized in the assignment of Raman modes. Moreover, the temperature-dependent resistivity resembles a semiconducting behavior where the charge carrier transport is facilitated by the band conduction at higher temperatures and via hopping $\le$260~K.<br />Comment: to be published in PRB

Details

Database :
arXiv
Journal :
Physical Review B, 106, 125148 (2022)
Publication Type :
Report
Accession number :
edsarx.2205.06019
Document Type :
Working Paper
Full Text :
https://doi.org/10.1103/PhysRevB.106.125148