cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Motivationsaspekte zur Anwendung des Punktesystems der BEWIA Höchweid AG
Creators: name: Dahinden, Carla Juliette
Publisher: name: Hochschule für Angewandte Psychologie FHNW
Year: 2023
Subjects: subject: Technologieakzeptanzmodell (TAM)
subject: Job Characteristics Modell (JCM)
subject: Job Diagnostic Survey (JDS)
subject: Gruppendiskussion
subject: Einstellung
subject: Gerechtigkeit
subject: Tätigkeiten
subject: Motivationsaspekte
subject: 330 - Wirtschaft

description: Die vorliegende Bachelorarbeit untersucht die Fragestellung: Wie sollte das Punktesystem von BEWIA Höchweid AG aufgestellt sein, damit Bewohnerinnen und Bewohner motiviert sind, es zu nutzen? Die Bedürfnisse wurden anhand einer Online-Umfrage mittels Surveytool Tivian in Form einer Vollerhebung eruiert sowie anhand einer Gruppendiskussion erschlossen. Das Technologieakzeptanzmodell (TAM) sowie die Job Diagnostic Survey (JDS) legten die Grundlagen für die Erhebungsmethoden, mit Ergänzungen von weiteren Theorien wie der Gerechtigkeit oder Einstellung. Die realisierte Stichprobe bestand aus 131 Personen. Mithilfe von Häufigkeits- und Inhaltsanalysen wurde festgestellt, dass das Gemeinschaftsgefühl und die Abwicklung wichtige Bedürfnisse darstellen. Das Sammeln der Punkte selbst erweist sich ebenfalls als bedeutsamer Mehrwert.
Taylor's series expansions for real powers of functions containing squares of inverse (hyperbolic) cosine functions, explicit formulas for special partial Bell polynomials, and series representations for powers of circular constant
Creators: name: Qi, Feng
Publisher: name: arXiv
Year: 2021
Subjects: subject: Combinatorics (math.CO)
subject: Classical Analysis and ODEs (math.CA)
subject: Number Theory (math.NT)
subject: FOS: Mathematics
subject: Primary 41A58, Secondary 11B73, 33B10

description: In the paper, by virtue of expansions of two finite products of finitely many square sums, with the aid of series expansions of composite functions of (hyperbolic) sine and cosine functions with inverse sine and cosine functions, and in the light of properties of partial Bell polynomials, the author establishes Taylor's series expansions of real powers of two functions containing squares of inverse (hyperbolic) cosine functions in terms of the Stirling numbers of the first kind, presents an explicit formula of specific partial Bell polynomials at a sequence of derivatives of a function containing the square of inverse cosine function, derives several combinatorial identities involving the Stirling numbers of the first kind, demonstrates several series representations of the circular constant Pi and its real powers, recovers series expansions of positive integer powers of inverse (hyperbolic) sine functions in terms of the Stirling numbers of the first kind, and also deduces other useful, meaningful, and significant conclusions.
description: 22 pages
Observation of TeV gamma-rays from the unidentified source HESS J1841-055 with the ARGO-YBJ experiment
Creators: name: YBJ Collaboration
name: Bartoli, B.
name: Bernardini, P.
name: Bi, X. J.
name: Bolognino, I.
name: Branchini, P.
name: Budano, A.
name: Melcarne, A. K. Calabrese
name: Camarri, P.
name: Cao, Z.
name: Cardarelli, R.
name: Catalanotti, S.
name: Cattaneo, C.
name: Chen, S. Z.
name: Chen, T. L.
name: Chen, Y.
name: Creti, P.
name: Cui, S. W.
name: Dai, B. Z.
name: Staiti, G. DAli
name: DAmone, A.
name: Danzengluobu
name: De Mitri, I.
name: Piazzoli, B. DEttorre
name: Di Girolamo, T.
name: Ding, X. H.
name: Di Sciascio, G.
name: Feng, C. F.
name: Feng, Zhaoyang
name: Feng, Zhenyong
name: Galeazzi, F.
name: Giroletti, E.
name: Gou, Q. B.
name: Guo, Y. Q.
name: He, H. H.
name: Hu, Haibing
name: Hu, Hongbo
name: Huang, Q.
name: Iacovacci, M.
name: Iuppa, R.
name: James, I.
name: Jia, H. Y.
name: Labaciren
name: Li, H. J.
name: Li, J. Y.
name: Li, X. X.
name: Liguori, G.
name: Liu, C.
name: Liu, C. Q.
name: Liu, J.
name: Liu, M. Y.
name: Lu, H.
name: Ma, L. L.
name: Ma, X. H.
name: Mancarella, G.
name: Mari, S. M.
name: Marsella, G.
name: Martello, D.
name: Mastroianni, S.
name: Montini, P.
name: Ning, C. C.
name: Pagliaro, A.
name: Panareo, M.
name: Panico, B.
name: Perrone, L.
name: Pistilli, P.
name: Ruggieri, F.
name: Salvini, P.
name: Santonico, R.
name: Sbano, S. N.
name: Shen, P. R.
name: Sheng, X. D.
name: Shi, F.
name: Surdo, A.
name: Tan, Y. H.
name: Vallania, P.
name: Vernetto, S.
name: Vigorito, C.
name: Wang, B.
name: Wang, H.
name: Wu, C. Y.
name: Wu, H. R.
name: Xu, B.
name: Xue, L.
name: Yang, Q. Y.
name: Yang, X. C.
name: Yao, Z. G.
name: Yuan, A. F.
name: Zha, M.
name: Zhang, H. M.
name: Zhang, Jilong
name: Zhang, Jianli
name: Zhang, L.
name: Zhang, P.
name: Zhang, X. Y.
name: Zhang, Y.
name: Zhao, J.
name: Zhaxiciren
name: Zhaxisangzhu
name: Zhou, X. X.
name: Zhu, F. R.
name: Zhu, Q. Q.
name: Zizzi, G.
Publisher: name: arXiv
Year: 2013
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We report the observation of a very high energy γ-ray source, whose position is coincident with HESS J1841-055. This source has been observed for 4.5 years by the ARGO-YBJ experiment from November 2007 to July 2012. Its emission is detected with a statistical significance of 5.3 standard deviations. Parameterizing the source shape with a two-dimensional Gaussian function we estimate an extension σ=(0.40(+0.32,-0.22}) degree, consistent with the HESS measurement. The observed energy spectrum is dN/dE =(9.0-+1.6) x 10^{-13}(E/5 TeV)^{-2.32-+0.23} photons cm^{-2} s^{-1} TeV^{-1}, in the energy range 0.9-50 TeV. The integral γ-ray flux above 1 TeV is 1.3-+0.4 Crab units, which is 3.2-+1.0 times the flux derived by HESS. The differences in the flux determination between HESS and ARGO-YBJ, and possible counterparts at other wavelengths are discussed.
description: 17 pages, 4 figures, have been accepted for publication in ApJ
Team meets VR – Eine Konzeptentwicklung für eine Evaluation eines Virtual Reality basierten Teamtrainings in der Notfallmedizin
Creators: name: Haupt, Britta
Publisher: name: Hochschule für Angewandte Psychologie FHNW
Year: 2023
Subjects: subject: Interprofessionelle Teamarbeit
subject: Simulationstraining
subject: Virtual Reality
subject: Evaluation
subject: 150 - Psychologie

description: Die vorliegende Bachelorarbeit befasst sich mit einer Konzeptentwicklung und -gestaltung für eine Evaluation im Rahmen eines neuartigen Simulationstrainings für interprofessionelle Teamarbeit mit Einsatz von Virtual Reality (VR) Technologie. In interprofessionellen Teams im Gesundheitswesen spielen verschiedene Elemente eine wichtige Rolle, um den hoch komplexen und dynamischen Arbeitsalltag möglichst gut zu koordinieren und die Patientensicherheit sicherzustellen. Damit das VR-basierte Teamtraining zukünftig effektiv gestaltet und eingesetzt werden kann, benötigt es eine Evaluation. Dazu braucht es ein Konzept, um Anhaltspunkte zu haben, wie vorgegangen wird und was zu beachten ist. Diese einzelnen Schritte wie die Auswahl geeigneter Variablen und deren Messinstrumente für die Evaluation werden im Bericht erarbeitet. Sie dienen der Veranschaulichung des Prozesses.
The Framework of Mechanics for Dynamic Behaviors of Fractional-Order Stochastic Dynamic Systems
Creators: name: Ren, Ruibin
name: Yuan, George Xianzhi
Publisher: name: arXiv
Year: 2021
Subjects: subject: Dynamical Systems (math.DS)
subject: Probability (math.PR)
subject: Chaotic Dynamics (nlin.CD)
subject: FOS: Mathematics
subject: FOS: Physical sciences
subject: I.6.1; I.6.3; J.2; K.6.4
subject: 26A33, 34F15, 34K37, 37A50, 37H05, 70k30, 82C31

description: The goal of this paper is to establish a general framework for dynamic behaviors of coupled fractional-order stochastic dynamic systems of particles by using star-coupled models. In particular, the general mechanics on the dynamic behaviors related to the stochastic resonance (SR) phenomenon of a star-coupled harmonic oscillator subject to multiplicative fluctuation and periodic force in viscous media are established by considering couplings, memory effects, the occurring of synchronization linked to the occurring of SR induced. The multiplicative noise is modeled as dichotomous noise and the memory of viscous media is characterized by fractional power kernel function. By using the Shapiro-Loginov formula and Laplace transform, the analytical expressions for the first moment of the steady state response, the stability and relationship between the system response and the system parameters in the long-time limit in terms of systems'asymptotic stability are also established. All theoretical analyses are supported by the corresponding numerical simulations, and thus it seems that the results established in this paper would provide a possible fundamental mathematical framework for the study of Schumpeter's theory on the economic development under the innovation and capital paradigm and related disciplines. In particular, the framework established by this paper allows us at the first time logically concluding that in general, the ratio for SMEs grow up successfully is less than one third, this is consistent with what the market has been observed commonly, and the similar conclusion available from the existing literature today.
description: 29 pages, 20 figures
The 2012 Hubble Ultra Deep Field (UDF12): Observational Overview
Creators: name: Koekemoer, Anton M.
name: Ellis, Richard S
name: McLure, Ross J.
name: Dunlop, James S.
name: Robertson, Brant E
name: Ono, Yoshiaki
name: Schenker, Matthew A.
name: Ouchi, Masami
name: Bowler, Rebecca A. A.
name: Rogers, Alexander B.
name: Curtis-Lake, Emma
name: Schneider, Evan
name: Charlot, Stephane
name: Stark, Daniel P.
name: Furlanetto, Steven R.
name: Cirasuolo, Michele
name: Wild, V.
name: Targett, T.
Publisher: name: arXiv
Year: 2012
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We present the 2012 Hubble Ultra Deep Field campaign (UDF12), a large 128-orbit Cycle 19 \HST\ program aimed at extending previous WFC3/IR observations of the UDF by quadrupling the exposure time in the F105W filter, imaging in an additional F140W filter, and extending the F160W exposure time by 50%. The principal scientific goal of this project is to determine whether galaxies reionized the universe; our observations are designed to provide a robust determination of the star formation density at $z$$\,\gtrsim\,$8, improve measurements of the ultraviolet continuum slope at $z$$\,\sim\,7\,-\,$8, facilitate the construction of new samples of $z$$\,\sim\,9\,-\,$10 candidates, and enable the detection of sources up to $z$$\,\sim\,$12. For this project we committed to combining these and other WFC3/IR imaging observations of the UDF area into a single homogeneous dataset, to provide the deepest near-infrared observations of the sky currently achievable. In this paper we present the observational overview of the project, motivated by its scientific goals, and describe the procedures used in reducing the data as well as the final products that are produced. We have used the most up up-to-date methods for calibrating and combining the images, in particular paying attention to correcting several instrumental effects. We release the full combined mosaics, comprising a single, unified set of mosaics of the UDF, providing the deepest near-infrared blank-field view of the universe obtained to date, reaching magnitudes as deep as AB$\,\sim\,$30 in the near-infrared, and yielding a legacy dataset on this field of lasting scientific value to the community.
description: 16 pages, 9 figures, submitted to ApJS
Additional file 1 of Medical education during the COVID-19 pandemic: lessons for the orthopedic departments
Creators: name: Vahdati, Zahra
name: Nematian, Hossein
name: Farhoud, Amir Reza
name: Tahmasebi, Mohammad Naghi
name: Rahimi-Dehgolan, Shahram
name: Mortazavi, Seyed Mohammad Javad
name: Kamrani, Reza Shahryar
name: Zanjani, Leila Oryadi
name: Golbakhsh, Mohammad Reza
name: Seraj, Roya Nasl
name: Nabian, Mohammad Hossein
Publisher: name: figshare
Year: 2023
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy

description: Supplementary Material 1
Learning controllers for performance through LMI regions
Creators: name: Bisoffi, Andrea
name: De Persis, Claudio
name: Tesi, Pietro
Publisher: name: arXiv
Year: 2021
Subjects: subject: Systems and Control (eess.SY)
subject: Dynamical Systems (math.DS)
subject: Optimization and Control (math.OC)
subject: FOS: Electrical engineering, electronic engineering, information engineering
subject: FOS: Mathematics

description: In an open-loop experiment, an input sequence is applied to an unknown linear time-invariant system (in continuous or discrete time) affected also by an unknown-but-bounded disturbance sequence (with an energy or instantaneous bound); the corresponding state sequence is measured. The goal is to design directly from the input and state sequences a controller that enforces a certain performance specification on the transient behaviour of the unknown system. The performance specification is expressed through a subset of the complex plane where closed-loop eigenvalues need to belong, a so called LMI region. For this control design problem, we provide here convex programs to enforce the performance specification from data in the form of linear matrix inequalities (LMI). For generic LMI regions, these are sufficient conditions to assign the eigenvalues within the LMI region for all possible dynamics consistent with data, and become necessary and sufficient conditions for special LMI regions. In this way, we extend classical model-based conditions from a seminal work in the literature to the setting of data-driven control from noisy data. Through two numerical examples, we investigate how these data-based conditions compare with each other.
Chords of 2-factors in planar cubic bridgeless graphs
Creators: name: Diwan, Ajit
Publisher: name: arXiv
Year: 2021
Subjects: subject: Combinatorics (math.CO)
subject: FOS: Mathematics
subject: 05C70 05C10 05C15

description: We show that every edge in a 2-edge-connected planar cubic graph is either contained in a 2-edge-cut or is a chord of some cycle that is contained in a 2-factor of the graph. As a consequence, we show that every edge in a cyclically 4-edge-connected planar cubic graph, except $K_2^3$ and $K_4$, is contained in a perfect matching whose removal disconnects the graph. We obtain a complete characterization of 2-edge-connected planar cubic graphs that have an edge such that every 2-factor containing the edge is a Hamiltonian cycle, and also of those that have an edge such that the complement of every perfect matching containing the edge is a Hamiltonian cycle. Another immediate consequence of the main result is that for any two edges contained in a facial cycle of a 2-edge-connected planar cubic graph, there exists a 2-factor in the graph such that both edges are contained in the same cycle of the 2-factor. We conjecture that this property holds for any two edges in a 2-edge-connected planar cubic graph, and prove it for planar cubic bipartite graphs. The main result is proved in the dual form by showing that every plane triangulation admits a vertex 3-coloring such that no face is monochromatic and there is exactly one specified edge between a specified pair of color classes.
Additional file 2 of Medical education during the COVID-19 pandemic: lessons for the orthopedic departments
Creators: name: Vahdati, Zahra
name: Nematian, Hossein
name: Farhoud, Amir Reza
name: Tahmasebi, Mohammad Naghi
name: Rahimi-Dehgolan, Shahram
name: Mortazavi, Seyed Mohammad Javad
name: Kamrani, Reza Shahryar
name: Zanjani, Leila Oryadi
name: Golbakhsh, Mohammad Reza
name: Seraj, Roya Nasl
name: Nabian, Mohammad Hossein
Publisher: name: figshare
Year: 2023
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy

description: Supplementary Material 2
KRAS mutation testing in colorectal cancer as an example of the pathologist's role in personalized targeted therapy: a practical approach
Creators: name: Domagala, Pawel
name: Hybiak, Jolanta
name: Sulzyc-Bielicka, Violetta
name: Cybulski, Cezary
name: Rys, Janusz
name: Domagala, Wenancjusz
Publisher: name: arXiv
Year: 2013
Subjects: subject: Genomics (q-bio.GN)
subject: FOS: Biological sciences

description: Identifying targets for personalized targeted therapy is the pathologist's domain and a treasure. For decades, pathologists have had to learn, understand, adopt and implement many new laboratory techniques as they arrived on the scene. Pathologists successfully integrate the results of those tests into final pathology reports that were, and still are, the basis of clinical therapeutic decisions. The molecular methods are different but no more difficult to comprehend in the era of "kit procedures". Pathologists have the knowledge and expertise to identify particular gene mutations using the appropriate molecular tests currently available. This review focuses on the most important recent developments in KRAS mutation testing in metastatic colorectal cancer (CRC), and shows that a pathologist is involved in 10 stages of this procedure. Recent studies have shown that highly sensitive, simple, reliable and rapid assays may significantly improve the identification of CRC patients resistant to anti-EGFR therapy. Thus, direct sequencing does not seem to be an optimal procedure of KRAS testing for clinical purposes. Twelve currently available high-sensitivity diagnostic assays (with the CE-IVD mark) for KRAS mutation testing are briefly described and compared. The suggested pathology report content for somatic mutation tests is described. In conclusion, evidence is presented that sending away paraffin blocks with tumor tissue for KRAS mutation testing may not be in the best interest of patients. Instead, an evidence-based approach indicates that KRAS mutation testing should be performed in pathology departments, only with the use of CE-IVD/FDA-approved KRAS tests, and with the obligatory, periodic participation in the KRAS EQA scheme organized by the European Society of Pathology as an independent international body.
description: 20 pages, 2 figures, 2 tables, 140 references
title: "Arbeit statt Arbeitslosigkeit finanzieren" – Förderung eines dauerhaften sozialen Arbeitsmarktes
title: Stellungnahme zur Anhörung des Ausschusses für Arbeit, Gesundheit und Soziales des Landtags Nordrhein-Westfalen am 26.8.2015
titleType: AlternativeTitle
Creators: name: Knuth, Matthias
Publisher: name: DuEPublico: Duisburg-Essen Publications Online, University of Duisburg-Essen, Germany
Year: 2018

description: Kurz gefasst
Der Vorrang der Vermittlung in den allgemeinen Arbeitsmarkt vor einer geförderten Beschäftigung ist selbstverständlich. Verstärkter Personaleinsatz kann dabei kostengünstiger sein als Eingliederungszuschüsse.
Vorrangige Orientierung auf den allgemeinen Arbeitsmarkt und die Stärkung und Verstetigung von Alternativen für die dauerhaft vom Arbeitsmarkt Ausgegrenzten sind keine Gegensätze. Außer für rentennahe Altersjahrgänge sollte die individuelle Förderung jedoch befristet bleiben.
Übergangschancen in den allgemeinen Arbeitsmarkt und ungeförderte Beschäftigung können voraussichtlich gesteigert werden, wenn die geförderte Beschäftigung als „Sozialer Arbeitsmarkt“ unter Beteiligung von privatwirtschaftlichen Unternehmen, Sozialunternehmen und Beschäftigungsträgern marktnah ausgestaltet wird. Die Beteiligung insbesondere der Privatwirtschaft muss erarbeitet werden; sie ergibt sich nicht von selbst. Der Wiederaufbau von Sozialunternehmen verlangt strukturelle Unterstützung.
Alle Arbeitgeber des Sozialen Arbeitsmarktes brauchen stabile und verlässliche Rahmenbedingungen. Hierzu gehören flankierende Dienstleistungen zur Integration der Geförderten (Coaching, Gesundheitsförderung), arbeitsbegleitende Qualifizierung und die strategische Berücksichtigung bei der öffentlichen Auftragsvergabe.
Der „Passiv-Aktiv-Transfer“ kann selbst bei bestehenden Beschränkungen im Eingliederungstitel das mögliche Finanzierungsvolumen für die Förderung von Arbeitsverhältnissen nach § 16e verdoppeln bis verdreifachen.
Die Kommunen sind zentrale Partner eines Sozialen Arbeitsmarktes. Sie werden diese Rolle nur wahrnehmen wollen, wenn die Ersparnis von passiven Leistungen bei der Anrechnung von Einkommen und Vermögen auf die Bedarfe zwischen den Finanzierungsanteilen des Bundes und der Kommunen künftig vom ersten Euro an anteilig erfolgt.
Der Begriff der Langzeitarbeitslosigkeit als Zugangskriterium zum Sozialen Arbeitsmarkt ist unzureichend; die bestehenden Ergänzungen um Vermittlungshemmnisse und Negativprognose laufen der Orientierung auf den allgemeinen Arbeitsmarkt zuwider. Es sollte eine SGB II-spezifische Kombination von Merkmalen als Indikator der Förderbarkeit entwickelt werden.
Electron acceleration to relativistic energies at a strong quasi-parallel shock wave
Creators: name: Masters, A.
name: Stawarz, L.
name: Fujimoto, M.
name: Schwartz, S. J.
name: Sergis, N.
name: Thomsen, M. F.
name: Retinò, A.
name: Hasegawa, H.
name: Lewis, G. R.
name: Coates, A. J.
name: Canu, P.
name: Dougherty, M. K.
Publisher: name: arXiv
Year: 2013
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Plasma Physics (physics.plasm-ph)
subject: Space Physics (physics.space-ph)
subject: FOS: Physical sciences

description: Electrons can be accelerated to ultrarelativistic energies at strong (high-Mach number) collisionless shock waves that form when stellar debris rapidly expands after a supernova. Collisionless shock waves also form in the flow of particles from the Sun (the solar wind), and extensive spacecraft observations have established that electron acceleration at these shocks is effectively absent whenever the upstream magnetic field is roughly parallel to the shock surface normal (quasi-parallel conditions). However, it is unclear whether this magnetic dependence of electron acceleration also applies to the far stronger shocks around young supernova remnants, where local magnetic conditions are poorly understood. Here we present Cassini spacecraft observations of an unusually strong solar system shock wave (Saturn's bow shock) where significant local electron acceleration has been confirmed under quasi-parallel magnetic conditions for the first time, contradicting the established magnetic dependence of electron acceleration at solar system shocks. Furthermore, the acceleration led to electrons at relativistic energies (~MeV), comparable to the highest energies ever attributed to shock-acceleration in the solar wind. These observations demonstrate that at high-Mach numbers, like those of young supernova remnant shocks, quasi-parallel shocks become considerably more effective electron accelerators.
description: 16 pages, 4 figures, accepted for publication in Nature Physics. Following journal guidelines, this is the submitted version (the accepted version will be uploaded 6 months after publication)
Colored HOMFLY polynomials as multiple sums over paths or standard Young tableaux
Creators: name: Anokhina, A.
name: Mironov, A.
name: Morozov, A.
name: Morozov, An.
Publisher: name: arXiv
Year: 2013
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Geometric Topology (math.GT)
subject: Quantum Algebra (math.QA)
subject: FOS: Physical sciences
subject: FOS: Mathematics

description: If a knot is represented by an m-strand braid, then HOMFLY polynomial in representation R is a sum over characters in all representations Q\in R^{\otimes m}. Coefficients in this sum are traces of products of quantum R-matrices along the braid, but these matrices act in the space of intertwiners, and their size is equal to the multiplicity M_{RQ} of Q in R^{\otimes m}. If R is the fundamental representation R=[1], then M_{[1] Q} is equal to the number of paths in representation graph, which lead from the fundamental vertex [1] to the vertex Q. In the basis of paths the entries of the m-1 relevant R-matrices are associated with the pairs of paths and are non-vanishing only when the two paths either coincide or differ by at most one vertex; as a corollary R-matrices consist of just 1x1 and 2x2 blocks, given by very simple explicit expressions. If cabling method is used to color the knot with the representation R, then the braid has m|R| strands, Q have a bigger size m|R|, but only paths passing through the vertex R are included into the sums over paths which define the products and traces of the m|R|-1 relevant R-matrices. In the case of SU(N) this path sum formula can also be interpreted as a multiple sum over the standard Young tableaux. By now it provides the most effective way for evaluation of the colored HOMFLY polynomials, conventional or extended, for arbitrary braids.
description: 12 pages
title: Abbau der Langzeitarbeitslosigkeit
title: Stellungnahme zur Öffentlichen Anhörung des Ausschusses für Arbeit und Soziales im Deutschen Bundestag vom 18. Mai 2015
titleType: AlternativeTitle
Creators: name: Bosch, Gerhard
Publisher: name: DuEPublico: Duisburg-Essen Publications Online, University of Duisburg-Essen, Germany
Year: 2018

description: Kurz gefasst
Im Wirtschaftsaufschwung 2005 bis 2008 konnte die Zahl der Langzeitarbeitslosen deutlich verringert werden. Seitdem stagniert sie trotz der weiterhin erfreulichen Beschäftigungszunahme auf einem hohen Niveau knapp über der Millionengrenze. Rund 500.000 Personen sind mehr als zwei Jahre arbeitslos.
Angesichts der Vielfältigkeit der Problemlagen und auch der unterschiedlichen Potenziale der betroffenen Personen kann sie nur mit einem Bündel von Instrumenten bekämpft werden, die auf den Einzelfall zugeschnitten werden müssen. 
Langzeitarbeitslose sollten nicht pauschal öffentlich geförderter Beschäftigung zugeordnet werden, sondern die Arbeitsmarktpolitik muss einen stärkeren Beitrag zur Qualifizierung von Arbeitslosen leisten. Denn der Arbeitsmarkt für einfache Tätigkeiten ist immer enger geworden und Arbeitslose ohne Berufsausbildung haben aufgrund des „Überangebots“ von gering qualifizierten Arbeitskräften ohne zusätzliche Qualifikation kaum Integrationschancen.
Der bisherige de facto Vorrang der Vermittlung führte dazu, dass gerade die arbeitsmarktnahen und weiterbildungsgeeigneten An- und Ungelernten vermittelt wurden. Diese Gruppe muss langfristig auf qualifizierteren Arbeitsplätzen eingesetzt werden, um für die anderen Langzeitarbeitslosen die einfachen Arbeitsplätze freizumachen. 
Die beiden Bundes-Programme zur Bekämpfung der Langzeitarbeitslosigkeit sind zu begrüßen. Die neuen Elemente - Betriebsakquise, Coaching, Gesundheitsförderung - hätte man allerdings geeigneter an die Regelförderung (§16e SGB II "Förderung von Arbeitsverhältnissen") anbinden können. Denn damit steht ein ausbaufähiges Instrument zur Verfügung, das Arbeitgebern jeglicher Art (Privatwirtschaft, Beschäftigungsträger, Soziale Unternehmen) offensteht.
Vesselness features and the inverse compositional AAM for robust face recognition using thermal IR
Creators: name: Ghiass, Reza Shoja
name: Arandjelovic, Ognjen
name: Bendada, Hakim
name: Maldague, Xavier
Publisher: name: arXiv
Year: 2013
Subjects: subject: Computer Vision and Pattern Recognition (cs.CV)
subject: FOS: Computer and information sciences

description: Over the course of the last decade, infrared (IR) and particularly thermal IR imaging based face recognition has emerged as a promising complement to conventional, visible spectrum based approaches which continue to struggle when applied in the real world. While inherently insensitive to visible spectrum illumination changes, IR images introduce specific challenges of their own, most notably sensitivity to factors which affect facial heat emission patterns, e.g. emotional state, ambient temperature, and alcohol intake. In addition, facial expression and pose changes are more difficult to correct in IR images because they are less rich in high frequency detail which is an important cue for fitting any deformable model. We describe a novel method which addresses these challenges. To normalize for pose and facial expression changes we generate a synthetic frontal image of a face in a canonical, neutral facial expression from an image of the face in an arbitrary pose and facial expression. This is achieved by piecewise affine warping which follows active appearance model (AAM) fitting. This is the first publication which explores the use of an AAM on thermal IR images; we propose a pre-processing step which enhances detail in thermal images, making AAM convergence faster and more accurate. To overcome the problem of thermal IR image sensitivity to the pattern of facial temperature emissions we describe a representation based on reliable anatomical features. In contrast to previous approaches, our representation is not binary; rather, our method accounts for the reliability of the extracted features. This makes the proposed representation much more robust both to pose and scale changes. The effectiveness of the proposed approach is demonstrated on the largest public database of thermal IR images of faces on which it achieved 100% identification, significantly outperforming previous methods.
The debris disk around gamma Doradus resolved with Herschel
Creators: name: Broekhoven-Fiene, Hannah
name: Matthews, Brenda C.
name: Kennedy, Grant M.
name: Booth, Mark
name: Sibthorpe, Bruce
name: Lawler, Samantha M.
name: Kavelaars, J. J.
name: Wyatt, Mark C.
name: Qi, Chenruo
name: Koning, Alice
name: Su, Kate Y. L.
name: Rieke, George H.
name: Wilner, David J.
name: Greaves, Jane S.
Publisher: name: arXiv
Year: 2012
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We present observations of the debris disk around gamma Doradus, an F1V star, from the Herschel Key Programme DEBRIS (Disc Emission via Bias-free Reconnaissance in the Infrared/Submillimetre). The disk is well-resolved at 70, 100 and 160 micron, resolved along its major axis at 250 micron, detected but not resolved at 350 micron, and confused with a background source at 500 micron. It is one of our best resolved targets and we find it to have a radially broad dust distribution. The modelling of the resolved images cannot distinguish between two configurations: an arrangement of a warm inner ring at several AU (best-fit 4 AU) and a cool outer belt extending from ~55 to 400 AU or an arrangement of two cool, narrow rings at ~70 AU and ~190 AU. This suggests that any configuration between these two is also possible. Both models have a total fractional luminosity of ~10^{-5} and are consistent with the disk being aligned with the stellar equator. The inner edge of either possible configuration suggests that the most likely region to find planets in this system would be within ~55 AU of the star. A transient event is not needed to explain the warm dust's fractional luminosity.
description: 12 pages, 6 figures, accepted for publication in ApJ
Gustav Keckeis, 1884-1967
Creators: name: Balthasar, Hans Urs Von
name: Füglister, Robert
name: Balmer, Hans Rudolf
Publisher: name: [Verlag nicht ermittelbar]
Year: 1967
Subjects: subject: 070 Publizistische Medien, Journalismus, Verlagswesen
subject: 920 Biografien, Genealogie, Insignien
subject: Nachruf
subject: Keckeis, Gustav
subject: Basel

description: Inhalt: Reden an der Abdankungsfeier in Basel - Nachrufe auf den Verstorbenen (in der Presse) - Gustav Keckeis in der Erinnerung einiger Freunde (Ausschnitte aus Briefen)
Coreless planar transformer for hard-switching applications
Creators: name: Hackel, Jonathan
Publisher: name: TU Dortmund
Year: 2023
Subjects: subject: Hard switching
subject: Inductive feed forward
subject: Coreless planar transformer
subject: 620
subject: Transformator
subject: Störgrößenaufschaltung
subject: Schaltvorgang
subject: Halbleiter
subject: Elektromagnetische Induktion
subject: Simulation

description: Leistungshalbleiter werden meist in schaltenden Anwendungen eingesetzt. Hartes Schalten ist hierfür ein gängiges und einfaches Funktionsprinzip, insbesondere bei induktiven Lasten. Hier können durch Verkürzung der Übergangsdauer zwischen Spannung und Strom die Schaltverluste reduziert werden. Die Nachteile schnellerer Übergänge in hart schaltenden Anwendungen sind in der Regel höhere Überschwingungen und außerdem die Erzeugung von elektromagnetischen Störungen. Die maximale Überspannung wird hierbei durch die Sperrspannung des Halbleiters begrenzt. Ein gängiger Ansatz zur Reduzierung der Überspannungen für einen Leistungshalbleiter ist die Minimierung der Induktivität im Leistungspfad. Ein in Reihe mit den Leistungsanschlüssen des Halbleiters geschalteter Transformator kann jedoch für verschiedene Anwendungen von Vorteil sein. Insbesondere die hohen Stromgradienten bei schnellen, harten Schaltvorgängen sorgt für eine hohe, und somit gut nutzbare Ausgangsspannung des Transformators. In dieser Arbeit wird ein neues Design eines kernlosen Planartransformators vorgestellt. Eine hohe magnetische Kopplung und ein einstellbares Übersetzungsverhältnis sowie eine besonders hohe Bandbreite sorgen dafür, dass die Induktivität in Reihe mit dem Halbleiter minimal gehalten werden kann. Der zweischichtige Aufbau ist zudem für verschiedene Substrate, insbesondere Leiterplatten, geeignet. Ein bis zur ersten Resonanzfrequenz gültiges Simulationsmodell des neuen Übertragerdesigns wurde erstellt und verifiziert. Die Anwendung, für die der Übertrager in dieser Arbeit hauptsächlich eingesetzt wird, ist das induktive Feed-Forward-Verfahren. Diese Methode zur Steuerung von Leistungshalbleitern beschleunigt das Umschalten in hart schaltenden Anwendungen. Die Methode wird analysiert und Verbesserungen für eine Auswahl von Leistungshalbleiter-Designs werden vorgeschlagen und verifiziert. Weiterhin wird die Ansteuerungsmethode modifiziert, um symmetrische Stromgradienten in parallel geschalteten Leistungshalbleitern zu erreichen. Außerdem wird der Übertrager vergleichbar zu einer Rogowski-Spule als Stromsensor genutzt, um die hohen Stromgradienten beim Schalten zu charakterisieren. Es wird gezeigt, dass durch verpolung der Sekundärwicklung das induktive Feed-Forward-Verfahren zur Verlangsamung des Schaltvorganges eingesetzt werden kann. In der letzten in dieser Arbeit vorgestellten Anwendung wird der Übertrager zur Erzeugung einer isolierten Versorgungsspannung für die Gate Ansteuerung eingesetzt. Die Anwendung ist besonders vorteilhaft, wenn eine negative Versorgungsspannung erforderlich ist, z.B. aufgrund einer niedrigen Schwellspannung.
Influence of Microfluidic Standards on Organs-on-Chips
Creators: name: Batista, Elsa
name: Van Heeren,
name: Ogheard, Florestan
name: Silverio, Vania
name: Kaal, Joris
name: Verplank, Nicolas
Publisher: name: Zenodo
Year: 2022
Subjects: microfluidics
standards
supply chain

description: How will microfluidic standards improve and ease organ-on-chip development and studies ? By the Improvement of device
 availability, reliability and accessibility; by encouraging large-scale adoption; by speeding up development; by improving time-to-market; by lower production costs
A new group of doubly charmed molecule with $T$-doublet charmed meson pair
Creators: name: Wang, Fu-Lai
name: Chen, Rui
name: Liu, Xiang
Publisher: name: arXiv
Year: 2021
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Inspired by the observation of the doubly charmed tetraquark state $T_{cc}^+$ at the LHCb Collaboration, we systematically study the $S$-wave interactions between a pair of charmed mesons ($D_{1},\,D_{2}^{\ast}$) in the $T$-doublet, where we adopt the one-boson-exchange model and consider both the $S$-$D$ wave mixing and coupled channel effects. Our numerical results suggest that the prime doubly charmed molecular tetraquark candidates are the $S$-wave $D_1D_1$ state with $I(J^P)=0(1^+)$, the $S$-wave $D_1{D}_2^{\ast}$ states with $I(J^P)=0(1^+,\,2^+,\,3^+)$, and the $S$-wave ${D}_2^{\ast}{D}_2^{\ast}$ states with $I(J^P)=0(1^+,\,3^+)$. The $S$-wave $D_1D_1$ state with $I(J^P)=1(2^+)$, the $S$-wave $D_1{D}_2^{\ast}$ state with $I(J^P)=1(3^+)$, and the $S$-wave ${D}_2^{\ast}{D}_2^{\ast}$ state with $I(J^P)=1(4^+)$ may be the possible isovector doubly charmed molecular tetraquark candidates. We expect the experiments like the LHCb or Belle II collaborations to search for these predicted doubly charmed molecular tetraquarks near the $D_1D_1$, $D_1D_2^*$, and $D_2^*D_2^*$ thresholds in future.
description: 14 pages, 7 tables, and 5 figures
Integrable Flows for Starlike Curves in Centroaffine Space
Creators: name: Calini, Annalisa
name: Ivey, Thomas
name: Beffa, Gloria Mari
Publisher: name: arXiv
Year: 2013
Subjects: subject: Exactly Solvable and Integrable Systems (nlin.SI)
subject: Analysis of PDEs (math.AP)
subject: Differential Geometry (math.DG)
subject: FOS: Physical sciences
subject: FOS: Mathematics

description: We construct integrable hierarchies of flows for curves in centroaffine ${\mathbb R}^3$ through a natural pre-symplectic structure on the space of closed unparametrized starlike curves. We show that the induced evolution equations for the differential invariants are closely connected with the Boussinesq hierarchy, and prove that the restricted hierarchy of flows on curves that project to conics in ${\mathbb{RP}}^2$ induces the Kaup-Kuperschmidt hierarchy at the curvature level.
title: Biological [and Conference] Opinion on the Proposed Implementation of a Program for the Issuance of Permits for Research and Enhancement Activities on Cetaceans in the Arctic, Atlantic, Indian, Pacific, and Southern Oceans
titleType: Other
Creators: name: United States. National Marine Fisheries Service
Publisher: name: United States. National Marine Fisheries Service
Year: 2019

description: ESA Section 7 Consultation ; OPR-2018-00019
Synthesis and characterisation of the geometric ferroelectric LaTaO₄
Creators: name: Howieson, Grant William
Publisher: name: The University of St Andrews
Year: 2022

description: LaTaO₄ is one of very few reported n=2 Carpy-Galy oxides. It is isostructural to the BaMF₄ fluorides which were subject of much prior study due to their ferroelectric and multiferroic properties. Previous studies of LaTaO₄ have been consistent in their conclusion that it can adopt either a low temperature non-polar monoclinic, or high temperature polar orthorhombic phase, with the monoclinic – orthorhombic transition temperature (Tₘ₋ₒ) being dependent on the preparation method. Recent studies, however, have reported an unidentified dielectric anomaly in the orthorhombic phase which alludes to an additional subtle structural transition above Tₘ₋ₒ. Powder neutron (PND) and electron diffraction studies have revealed that the previously unidentified dielectric anomaly denotes a transition between an incommensurately modulated and unmodulated orthorhombic (Cmc2₁) structure at ~503 K. The phase transition sequence is re-investigated in light of this new modulated phase, with resonant ultrasound (RUS) and Raman spectroscopy being utilised to elucidate the dynamics of transition and show the incommensurate – commensurate transition to be unusually 1ˢᵗ order, but nearly continuous (tri-critical). Refinement of PND data in the Cmc2₁(α00)0s0 superspace group, indicates a modulation wavevector q = (0.456 0 0) at 483 K. The modulation arises from a variation in La³⁺ positions and octahedral tilts which propagate along the polar a-axis and is speculated to arise as a mechanism to improve overall bonding environment of La³⁺. Electron microscopy reveals that the modulation arises from partially ordered sub-units, which are 2.5× and 3× expansions of the original orthorhombic cell. A model has been constructed which combines the local structural origin with the observed macroscopic modulation, where sub-units partially order with an average periodicity of ~11a (~0.456 a*). Previous studies report a relationship between the stability of each phase of LaTaO₄ and A-cation size. To explore the possibility that the modulation arises purely by an A-cation size effect, the series La₁₋ₓLnₓTaO₄ is synthesized, where Ln = Ce³⁺, Pr³⁺ and Nd³⁺ (0 ≤ x ≤ 0.3). Doping with these isovalent cations shows a general trend of stabilisation of the low temperature phases with decreasing average A-cation radii; the effect is amplified in Ce³⁺-doped samples and preliminary analysis suggests that this is due to a mix of oxidation states and the associated inter- and de-intercalation of interstitial oxygens during thermal cycling.
Decelerated invasion and waning moon patterns in public goods games with delayed distribution
Creators: name: Szolnoki, Attila
name: Perc, Matjaz
Publisher: name: arXiv
Year: 2013
Subjects: subject: Physics and Society (physics.soc-ph)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Social and Information Networks (cs.SI)
subject: Populations and Evolution (q-bio.PE)
subject: FOS: Physical sciences
subject: FOS: Computer and information sciences
subject: FOS: Biological sciences

description: We study the evolution of cooperation in the spatial public goods game, focusing on the effects that are brought about by the delayed distribution of goods that accumulate in groups due to the continuous investments of cooperators. We find that intermediate delays enhance network reciprocity because of a decelerated invasion of defectors, who are unable to reap the same high short-term benefits as they do in the absence of delayed distribution. Long delays, however, introduce a risk because the large accumulated wealth might fall into the wrong hands. Indeed, as soon as the curvature of a cooperative cluster turns negative, the engulfed defectors can collect the heritage of many generations of cooperators, and by doing so start a waning moon pattern that nullifies the benefits of decelerated invasion. Accidental meeting points of growing cooperative clusters may also act as triggers for the waning moon effect, thus linking the success of cooperators with their propensity to fail in a rather bizarre way. Our results highlight that "investing into the future" is a good idea only if that future is sufficiently near and not likely to be burdened by inflation.
description: 4 two-column pages, 5 figures; accepted for publication in Physical Review E
Does Complexity Equal Anything?
Creators: name: Belin, Alexandre
name: Myers, Robert C.
name: Ruan, Shan-Ming
name: Sárosi, Gábor
name: Speranza, Antony J.
Publisher: name: arXiv
Year: 2021
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We present a new infinite class of gravitational observables in asymptotically Anti-de Sitter space living on codimension-one slices of the geometry, the most famous of which is the volume of the maximal slice. We show that these observables display universal features for the thermofield-double state: they grow linearly in time at late times and reproduce the switch-back effect in shock wave geometries. We argue that any member of this class of observables is an equally viable candidate as the extremal volume for a gravitational dual of complexity.
description: 6 pages + appendices, 3 figures; v2 minor edits and title change - version as in PRL
Standardization of chemical prefixes, CURIEs, URIs, and semantic mappings
Creators: name: Hoyt, Charles Tapley
Publisher: name: Zenodo
Year: 2023

description: Chemistry ontologies and semantic web resources typically use URIs and compact URIs (CURIEs) to encode references to chemical entities and concepts. However, due to a lack of standardization, several different URIs or CURIEs could refer to the same entity in the same semantic resource. For example, alsterpaullone can be referenced by many URIs (http://purl.obolibrary.org/obo/CHEBI_138488, https://identifiers.org/CHEBI:138488, etc.). Similarly, it can be referenced by many different CURIEs (CHEBI:138488, CHEBIID:138488, etc.). This talk covers the Bioregistry (https://bioregistry.io, https://github.com/biopragmatics/bioregistry), an external, community-driven registry prefixes for chemical ontologies and their associated metadata which can be used to standardize CURIEs and URIs. Further, the Bioregistry provides a set of tools to aid in standardization, validation, and integration of data, knowledge, and models.
Simulations of magnetic fields in isolated disk galaxies
Creators: name: Pakmor, R.
name: Springel, V.
Publisher: name: arXiv
Year: 2012
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Magnetic fields are known to be dynamically important in the interstellar medium of our own Galaxy, and they are ubiquitously observed in diffuse gas in the halos of galaxies and galaxy clusters. Yet, magnetic fields have typically been neglected in studies of the formation of galaxies, leaving their global influence on galaxy formation largely unclear. We extend our MHD implementation in the moving-mesh code Arepo to cosmological problems which include radiative cooling and the formation of stars. In particular, we replace our previously employed divergence cleaning approach with a Powell 8-wave scheme, which turns out to be significantly more stable, even in very dynamic environments. We verify the improved accuracy through simulations of the MRI in accretion disks, that reproduce its correct linear growth rate. Using this new MHD code, we simulate the formation of isolated disk galaxies similar to the Milky Way using idealized initial conditions with and without magnetic fields. We find that the magnetic field is quickly amplified in the initial starburst and the differential rotation of the forming disk until it eventually saturates when it becomes comparable to the thermal pressure. The additional pressure component leads to a lower star formation rate at late times compared to simulations without magnetic fields, and induces changes in the spiral arm structures of the gas disk. In addition, we observe highly magnetized fountain-like outflows from the disk. These results are robust with numerical resolution and are largely independent of the initial magnetic seed field assumed in the initial conditions, as the amplification process is rapid and self-regulated. Our findings suggest an important influence of magnetic fields on galaxy formation and evolution, cautioning against their neglect in theoretical models of structure formation.
description: 19 pages, 15 figures, submitted to MNRAS, comments welcome