Article ID Journal Published Year Pages File Type
8156937 Journal of Magnetism and Magnetic Materials 2014 6 Pages PDF
Abstract
We report ferromagnetism in pure and Cu-doped tin oxide (SnO2) nanowires grown on silicon substrate using a thermal evaporation process at atmospheric pressure. Scanning electron microscopy (SEM) and transmission electron microscopy (TEM) images indicated the growth of wire-like nanostructures on silicon substrate with average diameter of 30-110 nm and length of 60-100 µm. The EDX spectra confirmed the growth of pure and Cu-doped SnO2 nanowires with Cu concentration of 0.25 at%, 0.5 at% and 2 at%. X-ray diffraction study revealed that as-grown nanowires have a tetragonal rutile structure of SnO2, without any secondary phase and were polycrystalline in nature. The room temperature photoluminescence (PL) spectra of as-grown nanowires showed strong emission at 590 nm and 600 nm originated due to oxygen vacancies and defect-related electronic states in the band gap. The ferromagnetism was observed in the pure and Cu-doped SnO2 nanowires at room temperature as well as at lower temperature of 5 K. At room temperature (300 K), pure SnO2 nanowires were ferromagnetic with a very small saturation magnetization (Ms) of ~0.06 emu/g, a remanent magnetization (Mr) of ~16.67% of Ms, and a coercivity of ~101 Oe while the nanowires doped with 0.25 at%, 0.5 at% and 2 at% of Cu were ferromagnetic with a saturation magnetization of ~10.25 emu/g, ~11.64 emu/g and 15.65 emu/g, a remanent magnetization of ~31.70%, ~46.13% and 56.29% of Ms, and a coercivity of ~162 Oe, ~181 Oe and 273 Oe, respectively. The magnetization of as-grown nanowires increases from 0.06 emu/g to 15.65 emu/g with increase in Cu-dopant concentration from 0 at% to 2 at%. Electron Spin Resonance (ESR) spectra also confirmed the room temperature ferromagnetism in Cu-doped SnO2 nanowires. The origin of room temperature ferromagnetism can be attributed to both surface defects and oxygen vacancies.
Related Topics
Physical Sciences and Engineering Physics and Astronomy Condensed Matter Physics
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