cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Sprache und Bewegung. Förderung der pragmatisch-kommunikativen Kompetenzen im Zyklus 2 mit Bewegungseinheiten des Karten-Sets Mvly
Creators: name: Andermatt, Andrea
Publisher: name: Zenodo
Year: 2022
Subjects: Sonderpädagogik
Masterarbeit
pragmatisch-kommunikative Kompetenzen
Zyklus 2
Karten-Set Mvly

description: In dieser qualitativ orientierten empirischen Arbeit wird die Auswirkung einer bewegungsorientierten Intervention auf einen Teilbereich der pragmatisch-kommunikativen Kompetenzen, das Aufrechthalten eines Gesprächs, untersucht. Im Fokus standen zwei Schüler_innen aus dem Zyklus 2. Mithilfe einer Prä-Post-Testung wurden die Daten der Entwicklungen in den pragmatisch-kommunikativen Kompetenzen und der Bewegung gesammelt, verglichen und interpretiert. Als Fördermethode der zehnwöchigen Intervention dienten die Bewegungswahrnehmungsübungen und Bewegungsspiele des KartenSets Mvly. Die Datenauswertung zeigt eine durchaus positive Entwicklung im fokussierten Teilbereich der pragmatisch-kommunikativen Kompetenzen, auch wenn diese nicht eindeutig ausgefallen sind. Weiterführende Forschung in diesem Bereich könnte eine breite abgestützte Studie sein, um aufschlussreichere Daten über das Fördern der Basiskompetenzen im Zyklus 2 zu gewinnen.
title: Zum Andenken an Ernst Mayer-Graf, 8. September 1907-16. August 1956
title: Gedenkfeier anlässlich der Bestattung Montag, den 20. August 1956 im Krematorium in Zürich
titleType: Subtitle
Creators: name: (:Unkn) Unknown
Publisher: name: Zentralbibliothek Zürich
Year: 1956
Subjects: subject: 920 Biografien, Genealogie, Insignien
subject: Nachruf
subject: Meyer-Graf, Ernst
subject: Sankt Gallen

description: Enthält: Einleitung und Besinnungsworte von Pfarrer Hannes Reimann, Zürich-Enge; Gedenkworte von Herrn J. L. Duvoisin, Präsident und Delegierter des Verwaltungsrates der Esso Standard (Switzerland)
Co-nonsolvency of PNiPAM at the transition between solvation mechanisms
Creators: name: Bischofberger, Irmgard
name: Calzolari, Davide C. E.
name: Trappe, Veronique
Publisher: name: arXiv
Year: 2014
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: We investigate the co-nonsolvency of poly-N-isopropyl acrylamide (PNiPAM) in different water-alcohol mixtures and show that this phenomenon is due to two distinct solvation contributions governing the phase behavior of PNiPAM in the water-rich and alcohol-rich regime respectively. While hydrophobic hydration is the predominant contribution governing the phase behavior of PNiPAM in the water-rich regime, the mixing contributions governing the phase behavior of classical polymer solutions determine the phase behavior of PNiPAM in the alcohol-rich regime. This is evidenced by distinct scaling relations denoting the energetic state of the aqueous medium as a key parameter for the phase behavior of PNiPAM in the water-rich regime, while the volume fractions of respectively water, alcohol and PNiPAM become relevant parameters in the alcohol-rich regime. Adding alcohol to water decreases the energetics of the aqueous medium, which gradually suppresses hydrophobic hydration, while adding water to alcohol decreases the solvent quality. Consequently, PNiPAM is insoluble in the intermediate range of solvent composition, where neither hydrophobic hydration nor the mixing contributions prevail. This accounts for the co-nonsolvency phenomenon observed for PNiPAM in water-alcohol mixtures.
LFV couplings of the extra gauge boson Z' and leptonic decay and production of pseudoscalar mesons
Creators: name: Yue, Chong-Xing
name: Cui, Man-Lin
Publisher: name: arXiv
Year: 2014
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Considering the constraints of the lepton flavor violating (LFV) processes $μ\rightarrow 3e$ and $τ\rightarrow3μ$ on the LFV couplings $Z'\ell_{i}\ell_{j}$, in the contexts of the $E_{6}$ models, the left-right (LR) models, the "alternative" left-right (ALR) models and the 331 models, we investigate the contributions of the extra gauge boson $Z'$ to the decay rates of the processes $\ell_{i}\rightarrow\ell_{j}ν_{\ell}ν_{\ell}$, $τ\rightarrowμP $ and $P\rightarrow μe$ with $P=π^{0},η$ and $η'$. Our numerical results show that the maximal values of the branching ratios for these processes are not dependent on the $Z'$ mass $M_{Z'}$ at leader order. The extra gauge boson $Z'_{X}$ predicted by the $E_{6}$ models can make the maximum value of the branching ratio $Br(τ\rightarrowμν_{\ell}ν_{\ell})$ reach $1.1\times10^{-7}$. All $Z'$ models considered in this paper can produce significant contributions to the process $τ\rightarrowμP$. However, the value of $Br(P\rightarrowμe)$ is far below its corresponding experimental upper bound.
description: 14 pages, 2 figures; matches published version
Using Red Clump Stars to Decompose the Galactic Magnetic Field with Distance
Creators: name: Pavel, Michael D.
Publisher: name: arXiv
Year: 2014
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: A new method for measuring the large-scale structure of the Galactic magnetic field is presented. The Galactic magnetic field has been probed through the Galactic disk with near-infrared starlight polarimetry, however the distance to each background star is unknown. Using red clump stars as near-infrared standard candles, this work presents the first attempt to decompose the line of sight structure of the sky-projected Galactic magnetic field. Two example lines-of-sight are decomposed: toward a field with many red clump stars and toward a field with few red clump stars. A continuous estimate of magnetic field orientation over several kiloparsecs of distance is possible in the field with many red clump stars, while only discrete estimates are possible in the sparse example. toward the Outer Galaxy, there is a continuous field orientation with distance that shows evidence of perturbation by the Galactic warp. toward the Inner Galaxy, evidence for a large-scale change in the magnetic field geometry is consistent with models of magnetic field reversals, independently derived from Faraday rotation studies. A photo-polarimetric method for identifying candidate intrinsically polarized stars is also presented. The future application of this method to large regions of the sky will begin the process of mapping the Galactic magnetic field in a way never before possible.
description: 11 pages, 8 figures, 2 tables, accepted for publication in The Astronomical Journal