https://orcid.org/0000-0003-0181-3348
![Sample our Physical Sciences journals, sign in here to start your FREE access for 14 days]({"type":"image" , "src" : "/sda/110819/TOC-Subject-Sample-2021-Physical-Sciences.jpg"})
ABSTRACT
Magnesium ferrite (MgFe2O4) nanocrystalline samples were prepared by sol–gel method and by sintering at temperatures from 300°C to 1000°C. X-ray diffraction and electron microscopic studies showed an increase in crystallite sizes and a decrease in lattice constants at higher sintering temperatures. UV-Vis absorption measurements depicted blue shift for samples of smaller crystallite sizes (dc) with a resultant increase of the band gap energies (Eg. = 2.07 eV at dc = 49 nm to 3.10 eV at dc = 6 nm, for samples sintered at 1000°C and 300°C, respectively). Fourier transform infrared spectroscopy of the samples proved the formation of the spinel structure while energy dispersive X-ray analysis pointed out the non-stoichiometric composition, which implied the presence of vacancy type defects that could modify the structural and magnetic characteristics of the compounds. This necessitated the use of positron annihilation lifetime and coincidence Doppler broadening spectroscopic studies for defect characterisation and the results indicated distinct redistribution of cations within the unit cells, making the compound overwhelmingly turn towards a normal spinel configuration at smaller nanocrystalline sizes. Positrons were trapped in larger vacancies of increasing numbers in smaller crystallites. The vacancies turned out to be formed at the octahedral sites where the increased ionic radius of Fe3+ became large enough to reduce the occupancy significantly. Mossbauer spectra analysis indicated an increase of the ferromagnetic properties in samples sintered at higher temperatures. At 300°C and 400°C, the samples dominantly showed paramagnetic behaviour.
Acknowledgements
ARA expresses gratitude to the authorities of Saha Institute of Nuclear Physics, Kolkata for granting her permission to work there for the completion of this project. Mr Anish Karmahapatra is gratefully acknowledged for his help in getting the X-ray diffraction data. PMGN is grateful to Dr V. Prakash of Payyanur College, Kannur, Kerala and Ms Meera R. of Amrita School of Arts and Sciences, Kollam, Kerala for their help in the positron annihilation data analysis. Two of the authors (ST and NK) acknowledge the financial support received from DST-Govt. of India through Nano Mission, FIST and PURSE programs and UGC-Govt. of India through the SAP program.
Disclosure statement
No potential conflict of interest was reported by the authors.
ORCID
P. M. G. Nambissan http://orcid.org/0000-0003-0181-3348
Sabu Thomas http://orcid.org/0000-0003-4726-5746
Nandakumar Kalarikkal http://orcid.org/0000-0002-4595-6466
