2001
DOI: 10.1088/0953-8984/13/48/201
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Colossal-magnetoresistive manganite thin films

Abstract: Mixed-valence perovskite manganites (Re 1−x A x MnO 3 where Re=rare earth, A=alkaline earth) provide a unique opportunity to study the relationships between the structure and the magnetotransport properties due to an interplay among charge carriers, magnetic coupling, orbital ordering and structural distortion. This makes these compounds very exciting from both the basic research and from the technological view point. As the technology pursued with these materials requires film growth, extensive studies have b… Show more

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Cited by 257 publications
(238 citation statements)
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References 255 publications
(465 reference statements)
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“…As previously stated, the physical properties of magnetic thin films (Mn-based system) are strongly dependent on the strains imposed by the substrate 28 . This dependence has also been reported in the case of SRO thin films 29 where a SRO is larger than a ST O which indicates the presence of compressive in-plane stress on the SRO film.…”
Section: (A)mentioning
confidence: 94%
“…As previously stated, the physical properties of magnetic thin films (Mn-based system) are strongly dependent on the strains imposed by the substrate 28 . This dependence has also been reported in the case of SRO thin films 29 where a SRO is larger than a ST O which indicates the presence of compressive in-plane stress on the SRO film.…”
Section: (A)mentioning
confidence: 94%
“…In these regards there had been some trials in literature [4][5][6]. For example by increasing the amount of Mn 4+ through substitutions like RE/Ag [4,5], or increase in overall oxygen content [1,7], one could shift the T MI and T FM above/close to the room temperature. However one needs not only the room temperature T MI and T FM but sharper MI and FM transitions for meaningful MR at these temperature.…”
Section: Introductionmentioning
confidence: 99%
“…The occurrence of the hump and the corresponding double peaks in TCR and LFMR could possibly be due to the re-enforcement of the CO-AFMI phase due to oxygen deficiency and inhomogeneous strain. The films on STO are, as discussed earlier, under tensile strain, which favors the CO-AFMI phase and is inimical to the FMM [11]. This enhances magnetic phase fluctuations that increases the carrier scattering resulting in (i) T C >T IM , (ii) relatively broad IMT, (iii) the observed hump like feature in the (T) curve at T<T IM and (iv) the lower peak in the TCR and MR.…”
Section: Resultsmentioning
confidence: 75%
“…The lower T C /T IM in S47 is due to the presence of tensile strain that favours CO-AFM rather than FM ones [11]. However, it is interesting to note that at smaller magnetic fields (<500 Oe) the magnetic moment of L47 are smaller than that of S47 and the reverse is true at higher fields.…”
Section: Resultsmentioning
confidence: 93%
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