2015
DOI: 10.1038/nmat4341
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Spatially resolved ultrafast magnetic dynamics initiated at a complex oxide heterointerface

Abstract: Diffraction is used to determine the spatial and temporal evolution of the magnetic disordering. We observe a magnetic melt front that grows from the substrate interface into the film, at a speed that suggests electronically driven propagation.Light control and ultrafast phase front propagation at hetero-interfaces may lead to new opportunities in optomagnetism, for example by driving domain wall motion to transport information across suitably designed devices. 3/25! ! !In transition metal oxides, rearrangemen… Show more

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Cited by 119 publications
(112 citation statements)
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References 45 publications
(49 reference statements)
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“…4 that the IMT and the emergence of itinerant charges may be driving rearrangements also in the magnetic and structural properties in the nickelate film. This analysis substantiates our earlier proposal of a phase transition driven by charge redistribution [8]. Furthermore, we can safely exclude a propagating acoustic (strain) wave as a driving force for the observed dynamics.…”
Section: /16supporting
confidence: 91%
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“…4 that the IMT and the emergence of itinerant charges may be driving rearrangements also in the magnetic and structural properties in the nickelate film. This analysis substantiates our earlier proposal of a phase transition driven by charge redistribution [8]. Furthermore, we can safely exclude a propagating acoustic (strain) wave as a driving force for the observed dynamics.…”
Section: /16supporting
confidence: 91%
“…Ref. 8), and the structural phase front propagating at about 4·10 3 m/s (black data points, extracted from off-resonant x-ray diffraction presented in Fig. 1), equal to the NdNiO 3 speed of sound (grey solid line).…”
Section: /16mentioning
confidence: 99%
“…Experimentally, a nonequilibrium distribution of acoustic phonons, which we denote by n B (ω q ), can be generated by ultrafast strain of interfaces [6,7,[28][29][30]. A periodic driving of such nonequilibrium phonons is necessary to establish a steadystate non-thermal phononic distribution, otherwise the phonons would relax back to equilibrium.…”
Section: A Boltzmann Formalismmentioning
confidence: 99%
“…Although acoustic phonons do not couple directly to light, they can be excited by rapidly applying lattice strain via an interface or via piezoelectric forces [7,[28][29][30]. The small energies required to excite acoustic phonons, as compared to optical phonons, generate less heating.…”
Section: Introductionmentioning
confidence: 99%
“…The combination of an element selective excitation with an element selective probe offers new paths for unraveling the fundamental mechanisms that drive magnetization loss by separately addressing the weight of possible contributions in this complex problem. Important classes of magnetic materials, in this respect, are ferrites [8,9] and transition metal (TM) rare-earth (RE) compounds [10][11][12][13]. Beyond their applicative interest, the (O-mediated) TM-TM coupling in magnetic oxides and the (5d-mediated) 3d-4f coupling in TM-RE compounds make these materials ideal candidates for resonant-pump resonant-probe magnetization dynamics studies.…”
Section: Introductionmentioning
confidence: 99%