No description available.

No description available.

No description available.

No description available.

Since many years, the importance of thin layers increases for lots of technical uses. Beginning in the field of microelectronics, the use of thin layers spread increasingly to other areas. Coatings for surface refining and optimisation of the mechanical properties for material engineering, customisation of the surface chemistry in catalysts, as well influencing of the transmission and reflection characteristics of surfaces in optics are only some examples of the high scientific and economic weight of the thin layer technology. Thin magnetic layers are the basis of many known storage media ranging from the tape recorder to the hard disk up to the credit card. Nowadays, these thin layers again gain interest in the research field of nanoelectronics as ultrathin layers. So-called spinvalve-read/write heads being already installed in actual hard disks use the Tunnel Magneto Resistance effect for a significant rise in memory density synonymous capacity. Such read/writeheads consist of a magnetic layersystem. This use of the magnetic as well as the electric characteristics of the electrons is called spintronics. The iron oxide magnetite exhibits a high iron portion, is strong antiferrimagnetic and has a high Curie-temperature. Since many years, it is used as a magnetic pigment on already mentioned magnetic tapes. Literature [1, 2, 3, 4] considers ultrathin epitaxial layers of magnetite on magnesium oxide for uses in the spintronics as a most promising candidate, because it inheres a complete spin polarisation at Fermi-level. Moreover, thin magnetite layers serve in the chemical industry as a catalyst in the Haber- Bosch-procedure and to the dehydration of ethylbenzene to styrene. Being already used and considered to be of ongoing interest, ultrathin magnetite layers offer a wide range of technological applications in many modern industrial and scientific fields. Because there is, nevertheless, a variety of other iron oxide (cf. chapter 4), it is a matter to determine the special growth conditions of magnetite. These ultrathin iron oxide layers were grown reactively on the (001)-surfaces of the magnesium oxide substrate by molecular beam epitaxy. Besides, the surface is examined by the diffraction of low-energy electrons concerning its crystalline structure. X-ray photo electron spectroscopy approaching the stochiometry completes these first characterisations. Other investigations are carried out at HASYLAB / DESY in Hamburg by X-ray reflectivity and X-ray diffraction. The exact thickness of the layers, its crystal properties in bulk, as well as the thickness of the crystalline portion of the layers can be determined among other features of the system. The evaluation of XRR-and XRD-investigations is done via simulations with in chapter 5 introduced software packages. The reader finds the theoretical backgrounds to the used techniques in chapter 3. The experimental setups in Osnabr¨uck and Hamburg as well as the backgrounds to the preparation are presented in chapter 5. Because the formation of the different iron oxides is described in literature [5, 6, 7, 8] as mostly depending on annealing temperatures, the experimental results in chapter 6 are graded accordingly. The dependence on temperature, layer thickness and annealing time should be examined for the iron oxides possible on this substrate. The aim of this work is the preparation of ultrathin epitaxial iron oxide layers with thicknesses up to few nanometers. The main goal is to find the growth parameters for ultrathin crystalline magnetite layers.

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This work investigates the growth dynamic of the reactive molecular beam epitaxy of Fe3O4 films, and its impact on the cation distribution as well as on the magnetic and structural properties at the surface and the interfaces. In order to study the structure and composition of Fe3O4 films during growth, time-resolved high-energy x-ray diffraction (tr-HEXRD) and time-resolved hard x-ray photoelectron spectroscopy (tr-HAXPES) measurements are used to monitor the deposition process of Fe3O4 ultrathin films on SrTiO3(001), MgO(001) and NiO/MgO(001). For Fe3O4\SrTiO3(001) is found that the film first grows in a disordered island structure, between thicknesses of 1.5nm to 3nm in FeO islands and finally in the inverse spinel structure of Fe3O4, displaying (111) nanofacets on the surface. The films on MgO(001) and NiO/MgO(001) show a similar result, with the exception that the films are not disordered in the early growth stage, but form islands which immediately exhibit a crystalline FeO phase up to a thickness of 1nm. After that, the films grown in the inverse spinel structure on both MgO(001) and NiO/MgO(001). Additionally, the tr-HAXPES measurements of Fe3O4/SrTiO3(001) demonstrate that the FeO phase is only stable during the deposition process, but turns into a Fe3O4 phase when the deposition is interrupted. This suggests that this FeO layer is a strictly dynamic property of the growth process, and might not be retained in the as-grown films. In order to characterize the as-grown films, a technique is introduced to extract the cation depth distribution of Fe3O4 films from magnetooptical depth profiles obtained by fitting x-ray resonant magnetic reflectivity (XRMR) curves. To this end, x-ray absorption (XAS) and x-ray magnetic circular dichroism (XMCD) spectra are recorded as well as XRMR curves to obtain magnetooptical depth profiles. To attribute these magnetooptical depth profiles to the depth distribution of the cations, multiplet calculations are fitted to the XMCD data. From these calculations, the cation contributions at the three resonant energies of the XMCD spectrum can be evaluated. Recording XRMR curves at those energies allows to resolve the magnetooptical depth profiles of the three iron cation species in Fe3O4. This technique is used to resolve the cation stoichiometry at the surface of Fe3O4/MgO(001) films and at the interfaces of Fe3O4/MgO(001) and Fe3O4/NiO. The first unit cell of the Fe3O4(001) surface shows an excess of Fe3+ cations, likely related to a subsurface cation-vacancy reconstruction of the Fe3O4(001) surface, but the magnetic order of the different cation species appears to be not disturbed in this reconstructed layer. Beyond this layer, the magnetic order of all three iron cation species in Fe3O4/MgO(001) is stable for the entire film with no interlayer or magnetic dead layer at the interface. For Fe3O4/NiO films, we unexpectedly observe a magnetooptical absorption at the Ni L3 edge in the NiO film corresponding to a ferromagnetic order throughout the entire NiO film, which is antiferromagnetic in the bulk. Additionally, the magnetooptical profiles indicate a single intermixed layer containing both Fe2+ and Ni2+ cations.

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