@phdthesis{SanchezBarriga2010,
  author    = {S{\´a}nchez-Barriga, Jaime},
  title     = {A photoemission study of quasiparticle excitations, electron-correlation effects and magnetization dynamics in thin magnetic systems},
  url       = {http://nbn-resolving.de/urn:nbn:de:kobv:517-opus-48499},
  school      = {Universit{\"a}t Potsdam},
  year      = {2010},
  abstract  = {This thesis is focused on the electronic, spin-dependent and dynamical properties of thin magnetic systems. Photoemission-related techniques are combined with synchrotron radiation to study the spin-dependent properties of these systems in the energy and time domains. In the first part of this thesis, the strength of electron correlation effects in the spin-dependent electronic structure of ferromagnetic bcc Fe(110) and hcp Co(0001) is investigated by means of spin- and angle-resolved photoemission spectroscopy. The experimental results are compared to theoretical calculations within the three-body scattering approximation and within the dynamical mean-field theory, together with one-step model calculations of the photoemission process. From this comparison it is demonstrated that the present state of the art many-body calculations, although improving the description of correlation effects in Fe and Co, give too small mass renormalizations and scattering rates thus demanding more refined many-body theories including nonlocal fluctuations. In the second part, it is shown in detail monitoring by photoelectron spectroscopy how graphene can be grown by chemical vapour deposition on the transition-metal surfaces Ni(111) and Co(0001) and intercalated by a monoatomic layer of Au. For both systems, a linear E(k) dispersion of massless Dirac fermions is observed in the graphene pi-band in the vicinity of the Fermi energy. Spin-resolved photoemission from the graphene pi-band shows that the ferromagnetic polarization of graphene/Ni(111) and graphene/Co(0001) is negligible and that graphene on Ni(111) is after intercalation of Au spin-orbit split by the Rashba effect. In the last part, a time-resolved x-ray magnetic circular dichroic-photoelectron emission microscopy study of a permalloy platelet comprising three cross-tie domain walls is presented. It is shown how a fast picosecond magnetic response in the precessional motion of the magnetization can be induced by means of a laser-excited photoswitch. From a comparision to micromagnetic calculations it is demonstrated that the relatively high precessional frequency observed in the experiments is directly linked to the nature of the vortex/antivortex dynamics and its response to the magnetic perturbation. This includes the time-dependent reversal of the vortex core polarization, a process which is beyond the limit of detection in the present experiments.},
  language  = {en}
}
@phdthesis{Shaw2024,
  author    = {Shaw, Vasundhara},
  title     = {Cosmic-ray transport and signatures in their local environment},
  doi       = {10.25932/publishup-62019},
  url       = {http://nbn-resolving.de/urn:nbn:de:kobv:517-opus4-620198},
  school      = {Universit{\"a}t Potsdam},
  pages     = {143},
  year      = {2024},
  abstract  = {The origin and structure of magnetic fields in the Galaxy are largely unknown. What is known is that they are essential for several astrophysical processes, in particular the propagation of cosmic rays. Our ability to describe the propagation of cosmic rays through the Galaxy is severely limited by the lack of observational data needed to probe the structure of the Galactic magnetic field on many different length scales. This is particularly true for modelling the propagation of cosmic rays into the Galactic halo, where our knowledge of the magnetic field is particularly poor. In the last decade, observations of the Galactic halo in different frequency regimes have revealed the existence of out-of-plane bubble emission in the Galactic halo. In gamma rays these bubbles have been termed Fermi bubbles with a radial extent of ≈ 3 kpc and an azimuthal height of ≈ 6 kpc. The radio counterparts of the Fermi bubbles were seen by both the S-PASS telescopes and the Planck satellite, and showed a clear spatial overlap. The X-ray counterparts of the Fermi bubbles were named eROSITA bubbles after the eROSITA satellite, with a radial width of ≈ 7 kpc and an azimuthal height of ≈ 14 kpc. Taken together, these observations suggest the presence of large extended Galactic Halo Bubbles (GHB) and have stimulated interest in exploring the less explored Galactic halo. In this thesis, a new toy model (GHB model) for the magnetic field and non-thermal electron distribution in the Galactic halo has been proposed. The new toy model has been used to produce polarised synchrotron emission sky maps. Chi-square analysis was used to compare the synthetic skymaps with the Planck 30 GHz polarised skymaps. The obtained constraints on the strength and azimuthal height were found to be in agreement with the S-PASS radio observations. The upper, lower and best-fit values obtained from the above chi-squared analysis were used to generate three separate toy models. These three models were used to propagate ultra-high energy cosmic rays. This study was carried out for two potential sources, Centaurus A and NGC 253, to produce magnification maps and arrival direction skymaps. The simulated arrival direction skymaps were found to be consistent with the hotspots of Centaurus A and NGC 253 as seen in the observed arrival direction skymaps provided by the Pierre Auger Observatory (PAO). The turbulent magnetic field component of the GHB model was also used to investigate the extragalactic dipole suppression seen by PAO. UHECRs with an extragalactic dipole were forward-tracked through the turbulent GHB model at different field strengths. The suppression in the dipole due to the varying diffusion coefficient from the simulations was noted. The results could also be compared with an analytical analogy of electrostatics. The simulations of the extragalactic dipole suppression were in agreement with similar studies carried out for galactic cosmic rays.},
  language  = {en}
}
@phdthesis{Lengefeld2010,
  author    = {Lengefeld, Jan},
  title     = {Zirkulardichroismus-Messungen mit Synchrotronstrahlung am BESSY : M{\"o}glichkeiten und Grenzen bei der Untersuchung biologischer Proben},
  url       = {http://nbn-resolving.de/urn:nbn:de:kobv:517-opus-44263},
  school      = {Universit{\"a}t Potsdam},
  year      = {2010},
  abstract  = {In dieser Arbeit wurden die M{\"o}glichkeiten und Grenzen f{\"u}r Zirkulardichroismus-Messungen mit Synchrotronstrahlung untersucht. Dazu wurde ein Messaufbau f{\"u}r Zirkulardichroismus-Messungen an zwei Strahlrohren am Berliner Elektronenspeicherring f{\"u}r Synchrotronstrahlung eingesetzt, die f{\"u}r Messungen im Bereich des ultravioletten Lichts geeignet sind. Eigenschaften der Strahlrohre und des Messaufbau wurden in einigen wichtigen Punkten mit kommerziellen Zirkulardichroismus-Spektrometern verglichen. Der Schwerpunkt lag auf der Ausdehnung des zug{\"a}nglichen Wellenl{\"a}ngenbereichs unterhalb von 180 nm zur Untersuchung des Zirkulardichroismus von Proteinen in diesem Bereich. In diesem Bereich ist es nicht nur die Lichtquelle sondern vor allem die Absorption des Lichts durch Wasser, die den Messbereich bei der Messung biologischer Proben in w{\"a}ssriger L{\"o}sung einschr{\"a}nkt. Es wurden Bedingungen gefunden, unter denen der Messbereich auf etwa 160 nm, in einigen F{\"a}llen bis auf 130 nm ausgedehnt werden konnte. Dazu musste die Pfadl{\"a}nge deutlich reduziert werden und verschieden Probenk{\"u}vetten wurden getestet. Der Einfluss der dabei auftretenden Spannungsdoppelbrechung in den Probenk{\"u}vetten auf das Messsignal konnte mit einem alternativen Messaufbau deutlich reduziert werden. Systematische Fehler im Messsignal und auftretende Strahlensch{\"a}den begrenzen jedoch die Zuverl{\"a}ssigkeit der gemessenen Spektren. Bei Proteinfilmen schr{\"a}nkt die Absorption von Wasser den Messbereich kaum ein. Es wurden jedoch meist deutliche Unterschiede zwischen den Spektren von Proteinfilmen und den Spektren von Proteinen in w{\"a}ssriger L{\"o}sung festgestellt. Solange diese Unterschiede nicht minimiert werden k{\"o}nnen, stellen Proteinfilme keine praktikable Alternative zu Messungen in w{\"a}ssriger L{\"o}sung dar.},
  language  = {de}
}
@phdthesis{Henneberg2004,
  author    = {Henneberg, Oliver},
  title     = {In-situ Untersuchungen zur Entstehung von Oberfl{\"a}chengittern in Polymeren},
  url       = {http://nbn-resolving.de/urn:nbn:de:kobv:517-0001331},
  school      = {Universit{\"a}t Potsdam},
  year      = {2004},
  abstract  = {In festen azobenzenhaltigen Polymeren wurde bei Bestrahlung mit blauem Licht ein makroskopischer Materialtransport beobachtet. Um die Dynamik der Gitterentstehung zu verfolgen, wurde am Speicherring f{\"u}r Synchrotronstrahlung ein Gitterschreibaufbau errichtet. Damit konnte erstmals in dieser Arbeit die Gitterbildungsgeschwindigkeit in-situ simultan mit R{\"o}ntgen- und Lichtstreuung untersucht werden. Mit Hilfe einer speziellen Anpassung der R{\"o}ntgenstreutheorie konnten sehr gute {\"U}bereinstimmungen von theoretischen Berechnungen mit den Messergebnissen erzielt werden. Dabei konnte nachgewiesen werden, dass sich zeitgleich mit einem Oberfl{\"a}chengitter auch ein Dichtegitter entwickelt. Durch die Trennung beider Streuanteile ließ sich die Dynamik der Strukturentstehungen bestimmen. Des weiteren konnte erstmals mit Hilfe der Photoelektronenspektroskopie die molekulare Orientierung an der Oberfl{\"a}che eines Oberfl{\"a}chengitters nachgewiesen werden. Die Bewegungsursache kann auf einen Impuls{\"u}bertrag w{\"a}hrend der Isomerisierung zur{\"u}ckgef{\"u}hrt werden, w{\"a}hrend die Bewegungsrichtung durch den elektrischen Feldvektor festgelegt wird. Die Theorie der Gitterentstehung konnte verbessert werden.},
  language  = {de}
}