Sudheendra, L. ; Raju, A. R. ; Rao, C. N. R. (2003) A systematic study of four series of electron-doped rare earth manganates, LnxCa1−xMnO3 (Ln=La, Nd, Gd and Y) over the x=0.02-0.25 composition range Journal of Physics: Condensed Matter, 15 (6). pp. 895-905. ISSN 0953-8984
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Official URL: http://iopscience.iop.org/0953-8984/15/6/316?fromS...
Related URL: http://dx.doi.org/10.1088/0953-8984/15/6/316
Abstract
Electrical and magnetic properties of four series of manganates LnxCa1−xMnO3 (Ln=La, Nd, Gd and Y) have been studied in the electron-doped regime (x=0.02-0.25) in order to investigate the various inter-dependent phenomena such as ferromagnetism, phase separation and charge ordering. The general behaviour of all four series of manganates is similar, with some of the properties showing a dependence on the average radius of the A-site cations, <rA> and cation size disorder. Thus, all the compositions show an increase in magnetization at 100-120 K (TM) for x<xmax, the magnetization increasing with increasing x. The value of xmax increases with decreasing <rA>, probably due to the increased phase separation induced by site disorder. This is also reflected in the larger width of the hysteresis loops at T<TM for small x or <rA>. In this regime, the electrical resistivity decreases with increasing x, but remains low and nearly constant, T>TM. The percolative nature of the conduction mechanism at T<TM is substantiated by the fit of the conductivity data to the scaling law, σ∝|xc−x|p, where p is in the 2-4 range. When x>xmax, the materials become antiferromagnetic (AFM) and charge-ordered at a temperature TCA, accompanied by a marked increase in resistivity. The value of TCA increases with increasing <rA> and x (up to x=0.3). Thus, all four series of manganates are characterized by a phase-separated regime between x=0.02 and 0.1-0.15 and an AFM charge-ordered regime at x>0.1-0.15.
Item Type: | Article |
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Source: | Copyright of this article belongs to Institute of Physics. |
ID Code: | 44726 |
Deposited On: | 23 Jun 2011 05:52 |
Last Modified: | 23 Jun 2011 05:52 |
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