TY - JOUR A1 - Di Sante, Domenico A1 - Erdmenger, Johanna A1 - Greiter, Martin A1 - Matthaiakakis, Ioannis A1 - Meyer, René A1 - Fernandez, David Rodríguez A1 - Thomale, Ronny A1 - van Loon, Erik A1 - Wehling, Tim T1 - Turbulent hydrodynamics in strongly correlated Kagome metals JF - Nature Communications N2 - A current challenge in condensed matter physics is the realization of strongly correlated, viscous electron fluids. These fluids can be described by holography, that is, by mapping them onto a weakly curved gravitational theory via gauge/gravity duality. The canonical system considered for realizations has been graphene. In this work, we show that Kagome systems with electron fillings adjusted to the Dirac nodes provide a much more compelling platform for realizations of viscous electron fluids, including non-linear effects such as turbulence. In particular, we find that in Scandium Herbertsmithite, the fine-structure constant, which measures the effective Coulomb interaction, is enhanced by a factor of about 3.2 as compared to graphene. We employ holography to estimate the ratio of the shear viscosity over the entropy density in Sc-Herbertsmithite, and find it about three times smaller than in graphene. These findings put the turbulent flow regime described by holography within the reach of experiments. Viscous electron fluids are predicted in strongly correlated systems but remain challenging to realize. Here, the authors predict enhanced effective Coulomb interaction and reduced ratio of the shear viscosity over entropy density in a Kagome metal, inferring turbulent flow of viscous electron fluids. KW - coupling-constant dependence KW - shear viscosity KW - electron KW - resistance Y1 - 2020 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:bvb:20-opus-230380 VL - 11 ER - TY - JOUR A1 - Kim, N. Y. A1 - Kusudo, K. A1 - Löffler, A. A1 - Höfling, S. A1 - Forchel, A. A1 - Yamamoto, Y. T1 - Exciton-polariton condensates near the Dirac point in a triangular lattice JF - New Journal of Physics N2 - Dirac particles, massless relativistic entities, obey linear energy dispersions and hold important implications in particle physics. The recent discovery of Dirac fermions in condensed matter systems including graphene and topological insulators has generated a great deal of interest in exploring the relativistic properties associated with Dirac physics in solid-state materials. In addition, there are stimulating research activities to engineer Dirac particles, elucidating their exotic physical properties in a controllable setting. One of the successful platforms is the ultracold atom-optical lattice system, whose dynamics can be manipulated and probed in a clean environment. A microcavity exciton-polariton-lattice system offers the advantage of forming high-orbital condensation in non-equilibrium conditions, which enables one to explore novel quantum orbital order in two dimensions. In this paper, we experimentally construct the band structures near Dirac points, the vertices of the first hexagonal Brillouin zone with exciton-polariton condensates trapped in a triangular lattice. Due to the finite spectral linewidth, the direct map of band structures at Dirac points is elusive; however, we identify the linear part above Dirac points and its associated velocity value is similar to ~0.9-2 x \(10^8 cm s^{-1}\), consistent with the theoretical estimate \(1 x 10^8 cm s^{-1}\) with a \(2 \mu m\) lattice constant. We envision that the exciton-polariton condensates in lattices would be a promising solid-state platform, where the system order parameter can be accessed in both real and momentum spaces. KW - Bose-Einstein condensation KW - carbon nanotubes KW - graphene KW - electron KW - dynamics KW - fermions KW - trap KW - gas Y1 - 2013 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:bvb:20-opus-123103 SN - 1367-2630 VL - 15 IS - 035032 ER - TY - THES A1 - Parragh, Nicolaus T1 - Strongly Correlated Multi-Orbital Systems : A Continuous-Time Quantum Monte Carlo Analysis T1 - Stark korrelierte Vielteilchensysteme : Eine Zeitkontinuum-Quanten-Monte-Carlo-Analyse N2 - In this thesis I present results concerning realistic calculations of correlated fermionic many-body systems. One of the main objectives of this work was the implementation of a hybridization expansion continuous-time quantum Monte Carlo (CT-HYB) algorithm and of a flexible self-consistency loop based on the dynamical mean-field theory (DMFT). DMFT enables us to treat strongly correlated electron systems numerically. After the implementation and extensive testing of the program we investigated different problems to answer open questions concerning correlated systems and their numerical treatment. N2 - Die vorliegende Dissertation beschäftigt sich mit der numerischen Berechnung von realistischen stark korrelierten fermionischen Vielteilchensystemen. Die Hauptzielsetzung dieser Arbeit war die Implementierung und das Testen einer zeitkontinuum Quanten Monte Carlo Methode in der Hybridisierungsentwicklung und einer flexiblen selbstkonsistenten Schleife basierend auf der dynamischen Molekularfeldtheorie die es uns ermöglicht solch stark korrelierte Systeme zu berechnen. Nach der Implementierung wurde das Programm ausführlich getest und es wurden Studien an unterschiedlichen Problemen durchgeführt. In Kapitel 1 werde ich das Anderson St¨orstellen-Problem und verschiedene Lösungsansätze für dieses Problem vorstellen. Besonderes Augenmerk werde ich auf den speziellen Lösungsansatz legen den ich implementiert habe. Am Ende des Kapitels werde ich Benchmark-Ergebnisse präsentieren. ... KW - Monte-Carlo-Simulation KW - Elektron KW - Vielteilchen KW - Quanten-Monte-Carlo-Analyse KW - electron KW - many body KW - quantum Monte Carlo KW - Vielteilchensystem KW - Fermionensystem KW - Starke Kopplung Y1 - 2013 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:bvb:20-opus-85253 ER - TY - JOUR A1 - Vainio, Rami A1 - Valtonen, Eino A1 - Heber, Bernd A1 - Malandraki, Olga E. A1 - Papaioannou, Athanasios A1 - Klein, Karl-Ludwig A1 - Afanasiev, Alexander A1 - Agueda, Neus A1 - Aurass, Henry A1 - Battarbee, Markus A1 - Braune, Stephan A1 - Dröge, Wolfgang A1 - Ganse, Urs A1 - Hamadache, Clarisse A1 - Heynderickx, Daniel A1 - Huttunen-Heikinmaa, Kalle A1 - Kiener, Jürgen A1 - Kilian, Patrick A1 - Kopp, Andreas A1 - Kouloumvakos, Athanasios A1 - Maisala, Sami A1 - Mishev, Alexander A1 - Miteva, Rosita A1 - Nindos, Alexander A1 - Oittinen, Tero A1 - Raukunen, Osku A1 - Riihonen, Esa A1 - Rodriguez-Gasen, Rosa A1 - Saloniemi, Oskari A1 - Sanahuja, Blai A1 - Scherer, Renate A1 - Spanier, Felix A1 - Tatischeff, Vincent A1 - Tziotziou, Kostas A1 - Usoskin, Ilya G. A1 - Vilmer, Nicole T1 - The first SEPServer event catalogue similar to ~68-MeV solar proton events observed at 1 AU in 1996-2010 JF - Journal of Space Weather and Space Climate N2 - SEPServer is a three-year collaborative project funded by the seventh framework programme (FP7-SPACE) of the European Union. The objective of the project is to provide access to state-of-the-art observations and analysis tools for the scientific community on solar energetic particle (SEP) events and related electromagnetic (EM) emissions. The project will eventually lead to better understanding of the particle acceleration and transport processes at the Sun and in the inner heliosphere. These processes lead to SEP events that form one of the key elements of space weather. In this paper we present the first results from the systematic analysis work performed on the following datasets: SOHO/ERNE, SOHO/EPHIN, ACE/EPAM, Wind/WAVES and GOES X-rays. A catalogue of SEP events at 1 AU, with complete coverage over solar cycle 23, based on high-energy (similar to 68-MeV) protons from SOHO/ERNE and electron recordings of the events by SOHO/EPHIN and ACE/EPAM are presented. A total of 115 energetic particle events have been identified and analysed using velocity dispersion analysis (VDA) for protons and time-shifting analysis (TSA) for electrons and protons in order to infer the SEP release times at the Sun. EM observations during the times of the SEP event onset have been gathered and compared to the release time estimates of particles. Data from those events that occurred during the European day-time, i.e., those that also have observations from ground-based observatories included in SEPServer, are listed and a preliminary analysis of their associations is presented. We find that VDA results for protons can be a useful tool for the analysis of proton release times, but if the derived proton path length is out of a range of 1 AU < s less than or similar to 3 AU, the result of the analysis may be compromised, as indicated by the anti-correlation of the derived path length and release time delay from the associated X-ray flare. The average path length derived from VDA is about 1.9 times the nominal length of the spiral magnetic field line. This implies that the path length of first-arriving MeV to deka-MeV protons is affected by interplanetary scattering. TSA of near-relativistic electrons results in a release time that shows significant scatter with respect to the EM emissions but with a trend of being delayed more with increasing distance between the flare and the nominal footpoint of the Earth-connected field line. KW - radio emissions (dynamic) KW - projects KW - advanced composition explorer KW - wind spacecraft KW - stereo mission KW - alpha monitor KW - electron KW - plasma KW - radio KW - spectrometer KW - heliosphere KW - instrument KW - radiation KW - flares Y1 - 2013 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:bvb:20-opus-122847 SN - 2115-7251 VL - 3 IS - A12 ER -