2004
DOI: 10.1103/physrevb.70.052403
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Magnetocrystalline and magnetoelastic basal plane anisotropies inHoLusuperlattices

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Cited by 16 publications
(27 citation statements)
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“…This affects the exchange interaction and, hence, the type of magnetic order and transition temperatures in ML structures [16][17][18]. Additionally, combined with hybridization effects, symmetry breaking and epitaxial strain influence the magnetic anisotropy and magnetoelastic interactions [19], giving rise to a different magnetic behavior compared to that of thick films.…”
Section: Introductionmentioning
confidence: 99%
“…This affects the exchange interaction and, hence, the type of magnetic order and transition temperatures in ML structures [16][17][18]. Additionally, combined with hybridization effects, symmetry breaking and epitaxial strain influence the magnetic anisotropy and magnetoelastic interactions [19], giving rise to a different magnetic behavior compared to that of thick films.…”
Section: Introductionmentioning
confidence: 99%
“…At a glance, the MEL constants associated to the tetragonal MS mode ε α2 are around about an order of magnitude larger than those associated to the volume expansion ε α1 . The quick analysis of the α-MEL constants reveals the following key features: (1) The tetragonal MS mode is considerably more efficient than the volume expansion mode in decreasing the sixfold magnetic anisotropic energy, since it turns out that M 10, being fully coherent with a prior study of the impact that an in-plane compression epitaxial strain has upon the sixfold magnetic anisotropy [47]. (2) The uniaxial magnetic anisotropy increases rapidly under the appearance of ε α2 ; notice that M 2 α2 = 0.9 GPa and the ratio M 7.9.…”
Section: Thermal Analysis Of the Volume And Tetragonal Magnetostrmentioning
confidence: 77%
“…(11), replicates a change of sign in K 6,eff 6 as H is swept in the [Ho 85 /Lu 15 ] 50 superlattice (SL), in which the SFT was first observed [21], the first aspect we must consider is the influence that the finite size [50] of the Ho layers has upon the MEL constants. Thus, as an earlier study [47] has shown, the development of typical epitaxial strains in multilayered rare earth based systems originated a negligible alteration, if any at all, in the γ -MEL constants, however, the α-MEL ones experienced an appreciable strain-induced modification, which is in a general case modelled as follows [23]:…”
Section: Spin-flop Transition Model In Holmium: Competing Mel Anmentioning
confidence: 99%
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“…Here we report on the distinctive way in which finite-size and the spin's dimensionality effects determine the MAE in ultrathin layers. Taking RE superlattices (SLs) as a model system [33], which is featured by the precise modeling of their MAE [29,30], we demonstrate that the two dimensionality of the spin system in ultrathin RE layers imprints a universal, rank-independent temperature scaling on the MAE constant as a quadratic power law of the reduced magnetization, in agreement with early predictions [34].We have investigated two ultrathin strain-alike RE-based SLs, mainly, [Dy 8±1 /Sc 8±1 ] 50 and [Ho 8±1 /Lu 18±2 ] 75 , hereafter referred to as Dy/Sc and Ho/Lu SLs, where the subindexes indicate the number of monolayers (MLs) in each layer, and 50 and 75 refer to the number of repetitions of the Dy/Sc and Ho/Lu bilayers, respectively. Both SLs were grown by a molecular beam epitaxy technique in a Balzers UMS630 facility, with a base pressure of better than 2 × 10 −10 mbar and deposited onto epi-polished (1120)-oriented Al 2 O 3 substrates, following well-established growth techniques [35,36].…”
mentioning
confidence: 99%