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This work studies the fundamental connection between lattice strain and magnetic anisotropy in the ferromagnetic semiconductor (Ga,Mn)As. The first chapters provide a general introduction into the material system and a detailed description of the growth process by molecular beam epitaxy. A finite element simulation formalism is developed to model the strain distribution in (Ga,Mn)As nanostructures is introduced and its predictions verified by high-resolution x-ray diffraction methods. The influence of lattice strain on the magnetic anisotropy is explained by an magnetostatic model. A possible device application is described in the closing chapter.
The present thesis is concerned with molecular beam epitaxy of magnetite (Fe3O4) thin films on semiconducting substrates and the characterization of their structural, chemical, electronic, and magnetic properties. Magnetite films could successfully be grown on ZnO substrates with high structural quality and atomically abrupt interfaces. The films are structurally almost completely relaxed exhibiting nearly the same in-plane and out-of-plane lattice constants as in the bulk material. Films are phase-pure and show only small deviations from the ideal stoichiometry at the surface and in some cases at the interface. Growth proceeds via wetting layer plus island mode and results in a domain structure of the films. Upon coalescence of growing islands twin-boundaries (rotational twinning) and anti-phase boundaries are formed. The overall magnetization is nearly bulk-like, but shows a slower approach to saturation, which can be ascribed to the reduced magnetization at anti-phase boundaries. However, the surface magnetization which was probed by x-ray magnetic circular dichroism was significantly decreased and is ascribed to a magnetically inactive layer at the surface. Such a reduced surface magnetization was also observed for films grown on InAs and GaAs. Magnetite could also be grown with nearly ideal iron-oxygen stoichiometry on InAs substrates. However, interfacial reactions of InAs with oxygen occur and result in arsenic oxides and indium enrichment. The grown films are of polycrystalline nature. For the fabrication of Fe3O4/GaAs films, a postoxidation of epitaxial Fe films on GaAs was applied. Growth proceeds by a transformation of the topmost Fe layers into magnetite. Depending on specific growth conditions, an Fe layer of different thickness remains at the interface. The structural properties are improved in comparison with films on InAs, and the resulting films are well oriented along [001] in growth direction. The magnetic properties are influenced by the presence of the Fe interface layer as well. The saturation magnetization is increased and the approach to saturation is faster than for films on the other substrates. We argue that this is connected to a decreased density of anti-phase boundaries because of the special growth method. Interface phases, viz. arsenic and gallium oxides, are quantified and different growth conditions are compared with respect to the interface composition.
In this work the epitaxial growth and characterization of the half-metallic ferromagnet NiMnSb was presented. NiMnSb crystallizes in the C1b structure which is similar to the zinc blende structure from widely used III-V semiconductors. One special property of NiMnSb is the theoretical 100% spin-polarization at the Fermi edge. This makes it a perfect candidate for spintronic experiments and the material of choice for building novel spintronic devices. Another important topic in this work were the magnetic properties of NiMnSb, especially the low magnetic damping of the grown thin films. All grown layers were fabricated with the technique of MBE. The layer stacks for all different experiments and devices were grown on InP substrate in (001) or (111)B orientation. Before the NiMnSb layer a buffer layer of undoped (In,Ga)As was grown. Additional for some samples on InP(111)B, a Si doped (In,Ga)As layer was grown on top of the undoped (In,Ga)As layer. The dopant concentration of this n-doped layer was determined by ETCH-CV. All layers were investigated by structural and the NiMnSb layer additional by magnetic properties. For the structural investigation the in-situ technique RHEED and ex-situ tool HRXRD were used. RHEED observations showed a good quality of the grown buffer and half-metallic ferromagnet layers on both orientations. These results were strengthened by the HRXRD measurement. The vertical lattice constant could be determined. The received value of a(NiMnSb_vertical) = 5.925 Å for NiMnSb on InP(001) is in good agreement to the value a(NiMnSb_Lit) = 5.903 Å found in literature [Cas55]. For NiMnSb on InP(111)B a vertical lattice constant of a(NiMnSb_vertikal) = 6.017 Å could be determined. The horizontal lattice constant of the buffer and the half-metallic ferromagnet layer could be determined as the same of the substrate. For NiMnSb this conclusion is only valid up to a thickness of ≈40nm. To increase this maximum thickness, NiMnSb samples were grown on InP(001) substrates and capped with Ti/Au layers. Afterwards a reciprocal space map of the (533) reflex was drawn with GIXRD at the synchrotron beamline BW2 of HASYLAB [Kum07]. It has been shown that the critical thickness is more than doubled by depositing a Ti/Au capping directly after growth of NiMnSb without breaking the ultrahigh vacuum (UHV). The magnetic properties were determined with FMR experiments and SQUID measurements. The received magnetic damping parameter α from a 40nm thick NiMnSb layer on InP(001) could be determined to 3.19e−3 along [1-10]. The resulting line width of our NiMnSb layers on InP(001) is more than 4.88 times smaller than measured before [Hei04]. Another result is the direction dependence of the damping. It has been measured that the difference of the damping is changed by more than 42% when rotating the applied field by 45° from [1-10] to [100].With SQUID we measured a saturation magnetization of a 40nm thick NiMnSb layer as 4µB. NiMnSb layers on InP(111)B substrate where also measured with FMR with a surprising result. These layers not only showed a decreasing in the anisotropy field with increasing thickness but also an uniaxial anisotropy. This behaviour can be explained with defects on these samples. With an AFM triangle-like defects were measured. These defects originated from the buffer layer and influenced the magnetic properties. Another part of this work is dedicated to the behaviour of NiMnSb at temperatures around 80K. With our samples, no phase transition can be observed in the data of the Hall, anomalous Hall term and resistivity. The last part of this work discusses different spintronic devices build with our NiMnSb layers. In a first device the magnetization acts on the current. This Giant Magneto Resistance (GMR) device consisted of InP:S(001) - 180nm undoped (In,Ga)As - 40nm NiMnSb - 10nm Cu - 6nm NiFe - 10nm Ru in current perpendicular to plane (CPP) geometry. We received a Magneto-Resistance-Ratio of 3.4%. In a second device the current acts on the magnetization and makes use of the spin torque phenomena. This so called Spin Torque Oscillator (STO) emitted frequencies in the GHz range (13.94GHz - 14.1GHz). The last fabricated device is based on the magnetic vortex phenomena. For switching the core polarity the gyrotropic frequencies f + = 254MHz f − = 217MHz and a total static magnetic field of only mµ0H = 65mT were necessary. The reversal efficiency has been determined as better than 99% [Lou09].