2014
DOI: 10.1557/jmr.2014.108
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Temperature dependence of static and dynamic magnetic properties in NiFe/IrMn bilayer system

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Cited by 3 publications
(2 citation statements)
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“…The larger grains are magnetically ordered but still unstable that results in the presence of rotatable anisotropy at the absence of exchange bias at RT FMR data and in coercivity increase. At the temperature decrease, these larger grains become stable and begin to contribute to exchange bias instead of H RA ; this leads to H RA decrease and appearance of nonzero H EB [57]. As the temperature further decreases the smaller thermally disordered AF grains become ordered but unstable and begin to contribute to H RA so that the absolute value increases again, as seen in Figure 9b.…”
Section: Discussionmentioning
confidence: 94%
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“…The larger grains are magnetically ordered but still unstable that results in the presence of rotatable anisotropy at the absence of exchange bias at RT FMR data and in coercivity increase. At the temperature decrease, these larger grains become stable and begin to contribute to exchange bias instead of H RA ; this leads to H RA decrease and appearance of nonzero H EB [57]. As the temperature further decreases the smaller thermally disordered AF grains become ordered but unstable and begin to contribute to H RA so that the absolute value increases again, as seen in Figure 9b.…”
Section: Discussionmentioning
confidence: 94%
“…As described in [40], the FMR LW, in terms of this process, can be written in the same form as in Equation (5). On the other hand, the presence of the AF layer leads to an additional relaxation process with the Neel relaxation time τ ~exp(∆E/k B T) [36] where ∆E is K AF × V; K AF is AF anisotropy constant (3 × 10 6 erg/cm 3 for FeMn [41] and 5.25 × 10 6 erg/cm 3 for IrMn [57]); and V is the grain volume, which can be roughly evaluated as l 3 where l is the grain size from XRD data. In our case, ∆E FeMn / ∆E IrMn = 1.78, which results in a higher τ for the Co/FeMn sample and, consequently, possibly greater line broadening, even at RT.…”
Section: Discussionmentioning
confidence: 99%