cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: Ritual & Performancekunst. Ein dialektisches Verhältnis
Creators: name: Stuckey, Lisa
Publisher: name: University Library Heidelberg
Year: 2016

description: Der Artikel behandelt die Interdependenzen zwischen Performancetheorie, Performancekunst, Ritualen und Ritualtheorie und untersucht deren gemeinsame Grundlage in ihrer Wirkung, ihrer Ästhetik und ihrem Habitus. Referenzpunkte sind Übergangsriten (Arnold van Gennep), Liminalität und Communitas (Victor W. Turner) sowie Konzepte der Ritualdynamik, um den Transfer ritueller Abläufe und rituellen Wissens in den Ausstellungsraum zu reflektieren. Welche Rolle kommen dabei der Geste, dem Körper, dem Einsatz unterschiedlicher Medien sowie Verfahren der Rhetorik zu und wie ist Agency zwischen Ritualspezialist_innen und anderen Akteur_innen verteilt? Inwiefern haben europäische und amerikanische Künstler_innen sowie Anthropolog_innen durch die kontinuierliche Bezeichnung bestimmter Praktiken als ‚schamanisch’ aktiv dazu beigetragen, dass eben diese als etwas gänzlich Fremdes verstanden und der eigenen Deutungsgewalt unterworfen werden? Dieser Artikel reflektiert kritisch den Zerfall essentialistischer Denkweisen mit Entstehung des Postkolonialismus und wie dies sich in der Kunstproduktion abzeichnet. Ebenso wird der Bedeutung rituell-performativer Versatzstücke nachgespürt, die in das Feld der Kunst transferiert werden und dort eine Dynamisierung in Form und Inhalt erfahren.
Candidates for Transiting Planets in OGLE-IV Galactic Bulge Fields
Creators: name: Mróz, M. J.
name: Pietrukowicz, P.
name: Poleski, R.
name: Udalski, A.
name: Szymański, M. K.
name: Gromadzki, M.
name: Ulaczyk, K.
name: Kozłowski, S.
name: Skowron, J.
name: Skowron, D. M.
name: Soszyński, I.
name: Mróz, P.
name: Ratajczak, M.
name: Rybicki, K. A.
name: Iwanek, P.
name: Wrona, M.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We present results of a search for transiting exoplanets in 10-yr long photometry with thousands of epochs taken in the direction of the Galactic bulge. This photometry was collected in the fourth phase of the Optical Gravitational Lensing Experiment (OGLE-IV). Our search covered approx. 222 000 stars brighter than I = 15.5 mag. Selected transits were verified using a probabilistic method. The search resulted in 99 high-probability candidates for transiting exoplanets. The estimated distances to these targets are between 0.4 kpc and 5.5 kpc, which is a significantly wider range than for previous transit searches. The planets found are Jupiter-size, with the exception of one (named OGLE-TR-1003b) located in the hot Neptune desert. If the candidate is confirmed, it can be important for studies of highly irradiated intermediate-size planets. The existing long-term, high-cadence photometry of our candidates increases the chances of detecting transit timing variations at long timescales. Selected candidates will be observed by the future NASA flagship mission, the Nancy Grace Roman Space Telescope, in its search for Galactic bulge microlensing events, which will further enhance the photometric coverage of these stars.
description: 35 pages, 13 figures, 4 tables. Published in Acta Astronomica, online catalog: https://ogledb.astrouw.edu.pl/~ogle/OCVS/
Kinetics of polarization in non-relativistic scattering
Creators: name: Milstein, A. I.
name: Salnikov, S. G.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Atomic Physics (physics.atom-ph)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: An approach is developed, which essentially simplifies derivation of kinetic equation for polarization in non-relativistic scattering. This approach is applicable for collision of projectile particles with a target for any spins of colliding particles. The most detailed consideration is performed for the case of spin 1/2 projectile particle interacting with spin 1/2 particle of a target. The solution of the kinetic equation for the case of zero initial polarization is presented.
description: 10 pages
title: Die Erotik des Papiers. Ein intimes Geständnis
Creators: name: Schildorfer, Martha M.
Publisher: name: University Library Heidelberg
Year: 2016

description: Der Dominanz digitaler Medien zum Trotz begegnet uns der Werkstoff Papier nach wie vor in den verschiedensten Aufgabenbereichen. Eine scheinbar alltägliche Episode regt an, den Blick zurück in die Geschichte zu werfen. Wann und wo wurde das Papier erfunden? Welche Bedeutung hatte es in der Gesellschaft, bevor es zur vernachlässigten Massenware und zum Recyclingmaterial wurde? Lassen Sie sich anregen, Ihre eigene Beziehung zum Papier zu hinterfragen und sie neu zu definieren!
title: Vom Nutzen der Architekturfotografie
Creators: name: Mazurova, Eva
Publisher: name: University Library Heidelberg
Year: 2016

description: Kolumne zu Architektur mit einer Rezension von: Angelika Fitz, Gabriele Lenz (Hg./Ed.), Vom Nutzen der Architekturfotografie/Architectural Photography and its Uses, Birkhäuser Verlag, 288 Seiten, Abbildungen. Preis: € [D] 49.95, ISBN: 9783035605860.
Memory-efficient w-projection with the fast Gauss transform
Creators: name: Bannister, Keith W.
name: Cornwell, Tim J.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: We describe a method performing w-projection using the fast Gauss transform of Strain (1991). We derive the theoretical performance, and simulate the actual performance for a range of w for a canonical array. While our implementation is dominated by overheads, we argue that this approach could for the basis of a higher-performing algorithms with particular application to the Square Kilometer Array.
description: 12 pages, 5 figures. Accepted for publication in MNRAS
Chemical Abundances in Field Red Giants from High-Resolution H-Band Spectra using the APOGEE Spectral Linelist
Creators: name: Smith, Verne V.
name: Cunha, Katia
name: Shetrone, Matthew D.
name: Meszaros, Szabolcs
name: Prieto, Carlos Allende
name: Bizyaev, Dmitry
name: Perez, Ana Garcia
name: Majewski, Steven R.
name: Schiavon, Ricardo
name: Holtzman, Jon
name: Johnson, Jennifer A.
Publisher: name: arXiv
Year: 2012
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: High-resolution H-band spectra of five bright field K, M, and MS giants, obtained from the archives of the Kitt Peak National Observatory (KPNO) Fourier Transform Spectrometer (FTS), are analyzed to determine chemical abundances of 16 elements. The abundances were derived via spectrum synthesis using the detailed linelist prepared for the SDSS III Apache Point Galactic Evolution Experiment (APOGEE), which is a high-resolution near-infrared spectroscopic survey to derive detailed chemical abundance distributions and precise radial velocities for 100,000 red giants sampling all Galactic stellar populations. Measured chemical abundances include the cosmochemically important isotopes 12C, 13C, 14N, and 16O, along with Mg, Al, Si, K, Ca, Ti, V, Cr, Mn, Fe, Co, Ni, and Cu. A comparison of the abundances derived here with published values for these stars reveals consistent results to ~0.1 dex. The APOGEE spectral region and linelist is, thus, well-suited for probing both Galactic chemical evolution, as well as internal nucleosynthesis and mixing in populations of red giants using high-resolution spectroscopy.
description: Accepted for publication in The Astrophysical Journal. 42 pages, 12 figures
Carex canescens
Creators: name: Becherer
Publisher: name: Zenodo
Year: 1956
Subjects: Biodiversity
Taxonomy

description: P. canescens X recta Cat. 94. Zu streichen.
description: Published as part of Becherer, 1956, Florae Vallesiacae Supplementum, pp. 1-556 in Denkschriften der Schweizerischen Naturforschenden Gesellschaft 71 on pages 1-556
Elektronentranslation in Atom-Atom-Stössen bei niedriger Energie
Creators: name: Menzel, Thomas
Publisher: name: Hannover : Universität Hannover
Year: 2000
Subjects: subject: Atom-atom-collisions
subject: integral cross-sections
subject: electron translation
subject: Atom-Atom-Stoß
subject: S-Matrix
subject: Streuquerschnitt
subject: Dewey Decimal Classification::500 | Naturwissenschaften::530 | Physik

description: [no abstract]
NLTE water lines in Betelgeuse-like atmospheres
Creators: name: Lambert, Julien
name: Josselin, Eric
name: Ryde, Nils
name: Faure, Alexandre
Publisher: name: arXiv
Year: 2013
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: The interpretation of water lines in red supergiant stellar atmospheres has been much debated over the past decade. The introduction of the so-called MOLspheres to account for near-infrared "extra" absorption has been controversial. We propose that non-LTE effects should be taken into account before considering any extra-photospheric contribution. After a brief introduction on the radiative transfer treatment and the inadequacy of classical treatments in the case of large-scale systems such as molecules, we present a new code, based on preconditioned Krylov subspace methods. Preliminary results suggest that NLTE effects lead to deeper water bands, as well as extra cooling.
description: 9 pages, 5 figures, Proceedings of the Betelgeuse Workshop, Paris, 2012
title: Otto Springer, Die Flußnamen Württembergs und Badens
Creators: name: Weisgerber, Leo
Publisher: name: University Library Heidelberg
Year: 2016

description: Rezension zu: Otto Springer, Die Flußnamen Württembergs und Badens. (Tübinger germanistische Arbeiten Bd. XI.) Stuttgart 1930, Verlag W. Kohlhammer. XVI, 257 S., 3 Karten.
title: Walter Schmid, Norisches Eisen
Creators: name: Reinecke, Paul
Publisher: name: University Library Heidelberg
Year: 2016

description: Rezension zu: Walter Schmid, Norisches Eisen (Beiträge zur Geschichte des österreichischen Eisenwesens, im Aufträge der Österreichisch-Alpinen Montangesellschaft herausgegeben, Abt. I, Heft 2). Berlin-Wien 1932, Verlag Julius Springer, Düsseldorf, Verlag Stahleisen m. b. H.
title: Miles Burkitt and V. Gordon Childe, A Chronological Table of Prehistory
Creators: name: Reinecke, Paul
Publisher: name: University Library Heidelberg
Year: 2016

description: Rezension zu: Miles Burkitt and V. Gordon Childe, A Chronological Table of Prehistory. Sonderabdruck aus Antiquity VI 1932, S. 185—205, mit einer Tafel in Umschlag, Gloucester, 2s 6d (durch den Assistant Editor der „Antiquity“, 24 Parkend Road, Gloucester, England, erhältlich).
TSEP: Threshold-sensitive Stable Election Protocol for WSNs
Creators: name: Kashaf, A.
name: Javaid, N.
name: Khan, Z. A.
name: Khan, I. A.
Publisher: name: arXiv
Year: 2012
Subjects: subject: Networking and Internet Architecture (cs.NI)
subject: FOS: Computer and information sciences

description: Wireless Sensor Networks (WSNs) are expected to find wide applicability and increasing deployment in near future. In this paper, we propose a new protocol, Threshold Sensitive Stable Election Protocol (TSEP), which is reactive protocol using three levels of heterogeneity. Reactive networks, as opposed to proactive networks, respond immediately to changes in relevant parameters of interest. We evaluate performance of our protocol for a simple temperature sensing application and compare results of protocol with some other protocols LEACH, DEEC, SEP, ESEP and TEEN. And from simulation results it is observed that protocol outperforms concerning life time of sensing nodes used.
description: 10th IEEE International Conference on Frontiers of Information Technology (FIT 12), 2012
Simulated Radio and Neutrino Imaging of a Microquasar
Creators: name: Smponias, Theodoros
Publisher: name: arXiv
Year: 2023
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Microquasar stellar systems emit electromagnetic radiation and high-energy particles. Thanks to their location within our own galaxy, they can be observed in high detail. Still, many of their inner workings remain elusive; hence, simulations, as the link between observations and theory, are highly useful. In this paper, both high-energy particle and synchrotron radio emissions from simulated microquasar jets are calculated using special relativistic imaging. A finite ray speed imaging algorithm is employed on hydrodynamic simulation data, producing synthetic images seen from a stationary observer. A hydrodynamical model is integrated in the above emission models. Synthetic spectra and maps are then produced that can be compared to observations from detector arrays. As an application, the model synthetically observes microquasars during an episodic ejection at two different spatio-temporal scales: one on the neutrino emission region scale and the other on the synchrotron radio emission scale. The results are compared to the sensitivity of existing detectors.
Thermal noise investigations in gravitational wave research
Creators: name: Ribichini, Luciano
Publisher: name: Hannover : Gottfried Wilhelm Leibniz Universität Hannover
Year: 2007
Subjects: subject: Pendulum
subject: etalon
subject: coating
subject: Dewey Decimal Classification::500 | Naturwissenschaften::530 | Physik

description: [no abstract]
The Nonlinear Schrödinger Equation in the Finite Line
Creators: name: Ramos, Juan I.
name: Villatoro, Francisco R.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Pattern Formation and Solitons (nlin.PS)
subject: Mathematical Physics (math-ph)
subject: Computational Physics (physics.comp-ph)
subject: FOS: Physical sciences
subject: 35C08, 65M06, 78A60

description: A numerical study of the nonlinear Schrödinger (NLS) equation subject to homogeneous Dirichlet, Neumann and Robin boundary conditions in the finite line is presented. The results are compared with both the exact analytical ones for the initial-value problem (IVP) of the NLS equation and the numerical ones for periodic boundary conditions. It is shown that initial solutions obtained by truncating the exact N-soliton solution of the IVP of the NLS equation into a finite interval develop solitary waves that behave as solitons, even after collisions with the boundaries. For periodic and homogeneous Dirichlet and Neumann boundary conditions, it is observed that the interaction between solitons and boundaries is equivalent to the collision between solitons in IVP or quarterplane problems. It is shown that for homogeneous Robin boundary conditions, boundary layers that trap and delay the soliton are formed at the boundaries. Phase diagrams for the soliton amplitude at the boundary points and for the soliton's maximum amplitude show a recurrent phenomenon, and are similar to those of the cubic Duffing equation. It is also shown that the phase diagrams are strong functions of the parameter that defines the Robin boundary conditions. A method of images, similar to the one used in potential theory, is developed for the NLS equation in the quarterplane with homogeneous Dirichlet and Neumann boundary conditions at the finite boundary.
Archimedean-type force in a cosmic dark fluid: III. Big Rip, Little Rip and Cyclic solutions
Creators: name: Balakin, Alexander B.
name: Bochkarev, Vladimir V.
Publisher: name: arXiv
Year: 2012
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We analyze late-time evolution of the Universe in the framework of the self-consistent model, in which the dark matter is influenced by the Archimedean-type force proportional to the four-gradient of the dark energy pressure. The dark energy is considered as a fluid with the equation of state of the relaxation type, which takes into account a retardation of the dark energy response to the Universe accelerated expansion. The dark matter is guided by the Archimedean-type force, which redistributes the total energy of the dark fluid between two its constituents, dark energy and dark matter, in the course of the Universe accelerated expansion. We focus on the constraints for the dark energy relaxation time parameter, for the dark energy equation of state parameter, and for the Archimedean-type coupling constants, which guarantee the Big Rip avoidance. In particular, we show that the Archimedean-type coupling protects the Universe from the Big Rip scenario with asymptotically infinite negative dark energy pressure, and that the Little Rip is the fate of the Universe with the Archimedean-type interaction inside the dark fluid.
description: 17 pages, 3 figures, accepted for publication in Physical Review D
HST Fine Guidance Sensor Parallaxes for Four Classical Novae
Creators: name: Harrison, Thomas E.
name: Bornak, Jillian
name: McArthur, Barbara E.
name: Benedict, G. Fritz
Publisher: name: arXiv
Year: 2013
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We have used data obtained with the Fine Guidance Sensors on the Hubble Space Telescope to derive precise astrometric parallaxes for four classical novae: V603 Aql, DQ Her, GK Per, and RR Pic. All four objects exceeded the Eddington limit at visual maximum. Re-examination of the original light curve data for V603 Aql and GK Per has led us to conclude that their visual maxima were slightly brighter than commonly assumed. With known distances, we examine the various maximum magnitude--rate of decline (MMRD) relationships that have been established for classical novae. We find that these four objects show a similar level of scatter about these relationships as seen in larger samples of novae whose distances were determined using indirect techniques. We also examine the nebular expansion parallax method, and find that it fails for three of the four objects. In each case it was possible to find an explanation for the failure of that technique to give precise distance estimates. DQ Her appears to suffer from an anomalously high extinction when compared to field stars on its sight line. We suggest that this is likely due to local material, which may also be the source of the IRAS detections of this object.
description: Accepted in the Astrophysical Journal
Rapid convergence of the Weinberg expansion of the deuteron stripping amplitude
Creators: name: Pang, D. Y.
name: Timofeyuk, N. K.
name: Johnson, R. C.
name: Tostevin, J. A.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Nuclear Theory (nucl-th)
subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: Theories of $(d,p)$ reactions frequently use a formalism based on a transition amplitude that is dominated by the components of the total three-body scattering wave function where the spatial separation between the incoming neutron and proton is confined by the range of the $n$-$p$ interaction, $V_{np}$. By comparison with calculations based on the CDCC method we show that the $(d,p)$ transition amplitude is dominated by the first term of the expansion of the three-body wave function in a complete set of Weinberg states. We use the \nuc{132}{Sn}(d,p)\nuc{133} {Sn} reaction at 30 and 100 MeV as examples of contemporary interest. The generality of this observed dominance and its implications for future theoretical developments are discussed.
description: 6 pages, 4 figures, Physical Review C - Accepted
On the mechanism of elasto-inertial turbulence
Creators: name: Dubief, Yves
name: Terrapon, Vincent E.
name: Soria, Julio
Publisher: name: arXiv
Year: 2013
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: Elasto-inertial turbulence is a new state of turbulence found in flows with polymer additives . The dynamics of turbulence generated and controlled by such additives is investigated from the perspective of the coupling between polymer dynamics and flow structures. Direct numerical simulations of channel flow with Reynolds numbers ranging from 1000 to 6000 (based on the bulk and the channel height) are used to study the formation and dynamics of elastic instabilities and their effects on the flow. The resulting mechanism of interactions between polymer dynamics and the flow helps resolve a long-standing controversy in the understanding of polymer drag reduction and explains the phenomenon of early turbulence, or onset of turbulence at lower Reynolds numbers than for Newtonian flows, previously observed in polymeric flows. Polymers also point out an interesting analogy with the forward and backward energy cascade in two-dimensional turbulence.
description: Submitted to Physics of Fluids. In honor of Parviz Moin 60th Birthday
Rotating dark matter admixed neutron stars
Creators: name: Cronin, John
name: Zhang, Xinyang
name: Kain, Ben
Publisher: name: arXiv
Year: 2023
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We study rotating compact stars that are mixtures of the ordinary nuclear matter in a neutron star and fermionic dark matter. After deriving equations describing a slowly rotating system made up of an arbitrary number of perfect fluids, we specialize to the two-fluid case, where the first fluid describes ordinary matter and the second fluid describes dark matter. Electromagnetic observations of the moment of inertia and angular momentum directly probe ordinary matter and not dark matter. Upon taking this into account, we show that the I-Love-Q relations for dark matter admixed neutrons stars can deviate significantly from the standard single-fluid relationships.
description: 16 pages, 3 figures
Typicality à la Russell in set theory
Creators: name: Tzouvaras, Athanassios
Publisher: name: arXiv
Year: 2023
Subjects: subject: Logic (math.LO)
subject: FOS: Mathematics
subject: 03E45, 03E47

description: We adjust the notion of typicality originated with Russell, which was introduced and studied in a previous paper for general first-order structures, to make it expressible in the language of set theory. The adopted definition of the class ${\rm NT}$ of nontypical sets comes out as a natural strengthening of Russell's initial definition, which employs properties of small (minority) extensions, when the latter are restricted to the various levels $V_ζ$ of $V$. This strengthening leads to defining ${\rm NT}$ as the class of sets that belong to some countable ordinal definable set. It follows that ${\rm OD}\subseteq {\rm NT}$ and hence ${\rm HOD}\subseteq {\rm HNT}$. It is proved that the class ${\rm HNT}$ of hereditarily nontypical sets is an inner model of ${\rm ZF}$. Moreover the (relative) consistency of $V\neq {\rm NT}$ is established, by showing that in many forcing extensions $M[G]$ the generic set $G$ is a typical element of $M[G]$, a fact which is fully in accord with the intuitive meaning of typicality. In particular it is consistent that there exist continuum many typical reals. In addition it follows from a result of Kanovei and Lyubetsky that ${\rm HOD}\neq {\rm HNT}$ is also relatively consistent. In particular it is consistent that ${\cal P}(ω)\cap {\rm OD}\subsetneq{\cal P}(ω)\cap {\rm NT}$. However many questions remain open, among them the consistency of ${\rm HOD}\neq {\rm HNT}\neq V$, ${\rm HOD}={\rm HNT}\neq V$ and ${\rm HOD}\neq {\rm HNT}= V$.
description: 15 pages
Optimal diffusive search: nonequilibrium resetting versus equilibrium dynamics
Creators: name: Evans, Martin R.
name: Majumdar, Satya N.
name: Mallick, Kirone
Publisher: name: arXiv
Year: 2012
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: We study first-passage time problems for a diffusive particle with stochastic resetting with a finite rate $r$. The optimal search time is compared quantitatively with that of an effective equilibrium Langevin process with the same stationary distribution. It is shown that the intermittent, nonequilibrium strategy with non-vanishing resetting rate is more efficient than the equilibrium dynamics. Our results are extended to multiparticle systems where a team of independent searchers, initially uniformly distributed with a given density, looks for a single immobile target. Both the average and the typical survival probability of the target are smaller in the case of nonequilibrium dynamics.
description: 15 pages, 2 figures, submitted to Journal of Physics A: Mathematical and Theoretical
Eine Quelle quantenentarteter Gase für die Atominterferometrie
Creators: name: Zaiser, Maic
Publisher: name: Hannover : Gottfried Wilhelm Leibniz Universität Hannover
Year: 2010
Subjects: subject: Atominterferometrie
subject: quantenentartete atomare Gase
subject: optische Dipolfallen
subject: Atom interferometry
subject: quantum degenerate atomic gases
subject: optical dipole traps
subject: Dewey Decimal Classification::500 | Naturwissenschaften::530 | Physik

description: [no abstract]
title: ÐÐ½Ð¾Ð³Ð¾Ð¿Ð¾ÑÐ¾ÑÐ½Ð¾Ðµ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð½Ð° ÑÐ·ÑÐºÐµ C#
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: Ð¢ÑÑÐ°Ð»ÑÑÑÐº, ÐÐ¾Ð½ÑÑÐ°Ð½ÑÐ¸Ð½
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2025
Subjects: ÐÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐ·ÑÐºÐ¸
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description: Ð ÑÑÐµÐ±Ð½Ð¾Ð¼ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ð¸ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑÑÑ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÑÑÐµÐ´ÑÑÐ²Ð° Ð¼Ð½Ð¾Ð³Ð¾Ð¿Ð¾ÑÐ¾ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð½Ð° Ð¡#. ÐÑÐ´ÐµÐ»ÑÐ½ÑÐµ ÑÐ°Ð·Ð´ÐµÐ»Ñ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¿Ð¾ÑÐ¾ÐºÐ¾Ð² Thread, Ð·Ð°Ð´Ð°Ñ Task, ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ PLINQ Ð¸ Parallel, Ð° ÑÐ°ÐºÐ¶Ðµ ÑÑÐµÐ´ÑÑÐ²Ð°Ð¼ ÑÐ¸Ð½ÑÑÐ¾Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¸ Ð°ÑÐ¸Ð½ÑÑÐ¾Ð½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ. ÐÐ¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÐ¸ Ð¸ Ð¾Ð³ÑÐ°Ð½Ð¸ÑÐµÐ½Ð¸Ñ ÑÑÐµÐ´ÑÑÐ² Ð¿Ð°ÑÐ°Ð»Ð»ÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð½Ð° Ð¡# Ð¸Ð»Ð»ÑÑÑÑÐ¸ÑÑÑÑÑÑ Ð¿ÑÐ¸Ð¼ÐµÑÐ°Ð¼Ð¸ ÐºÐ¾Ð´Ð° Ð¸ Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ð¼Ð¸ Ð·Ð°Ð´Ð°Ð½Ð¸ÑÐ¼Ð¸.
Exploring factors contributing to young workers’ vulnerability to work-related harm
Creators: name: Manglicmot, Manfred
name: Cotton, Olivia
name: Chen, Sonia
name: Crawford, Joanne
Publisher: name: Open Access Victoria University of Wellington | Te Herenga Waka
Year: 2021
Subjects: subject: 220299 History and Philosophy of Specific Fields not elsewhere classified
subject: FOS: Philosophy, ethics and religion
subject: Sociology
subject: FOS: Sociology
subject: 150399 Business and Management not elsewhere classified
subject: FOS: Economics and business

description: New Zealand has experienced significant increases in youth employment rates in the last 20 years with 40 per cent of people employed part-time. This age group has been associated with the second-highest rate of injury claims. At the current time, there is limited information on why young workers in New Zealand are more vulnerable to work-related harm. This project aimed to explore this with a convenience sample of young workers using an online survey. Participants represented a diverse ethnic population but the sample was predominately female. In total, 32.7 per cent of respondents had received no occupational health and safety (OHS) training when starting work. Fifty-seven per cent of the sample thought that OHS was valued by their employer. Interestingly, 63 per cent of the sample said they would be confident about speaking up about an OHS issue with most being willing to speak to their manager. In relation to stress, the analysis identified that there was an association between feeling stressed and being unable to follow OHS protocols (p=0.05). While this was a small exploratory study, suggestions made to improve OHS include clear and open communication between workers and employers, improved access to OHS resources and continuous and in-depth training.
Exploring factors contributing to young workers’ vulnerability to work-related harm
Creators: name: Manglicmot, Manfred
name: Cotton, Olivia
name: Chen, Sonia
name: Crawford, Joanne
Publisher: name: Open Access Te Herenga Waka-Victoria University of Wellington
Year: 2021
Subjects: classificationCode: 500299
subject: History and philosophy of specific fields not elsewhere classified
classificationCode: 441099
subject: Sociology not elsewhere classified
classificationCode: 359999
subject: Other commerce, management, tourism and services not elsewhere classified

description: New Zealand has experienced significant increases in youth employment rates in the last 20 years with 40 per cent of people employed part-time. This age group has been associated with the second-highest rate of injury claims. At the current time, there is limited information on why young workers in New Zealand are more vulnerable to work-related harm. This project aimed to explore this with a convenience sample of young workers using an online survey. Participants represented a diverse ethnic population but the sample was predominately female. In total, 32.7 per cent of respondents had received no occupational health and safety (OHS) training when starting work. Fifty-seven per cent of the sample thought that OHS was valued by their employer. Interestingly, 63 per cent of the sample said they would be confident about speaking up about an OHS issue with most being willing to speak to their manager. In relation to stress, the analysis identified that there was an association between feeling stressed and being unable to follow OHS protocols (p=0.05). While this was a small exploratory study, suggestions made to improve OHS include clear and open communication between workers and employers, improved access to OHS resources and continuous and in-depth training.
Physical origin of satellite in photoemission of doped graphene: An ab-initio GW plus cumulant study
Creators: name: Lischner, Johannes
name: Vigil-Fowler, Derek
name: Louie, Steven G.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: We calculate the photoemission spectra of suspended and epitaxial doped graphene using an ab initio cumulant expansion of the Green's function based on the GW self-energy. Our results are compared to experiment and to standard GW calculations. For doped graphene on a silicon carbide substrate, we find, in contrast to earlier calculations, that the spectral function from GW only does not reproduce experimental satellite properties. However, ab initio GW plus cumulant theory combined with an accurate description of the substrate screening results in good agreement with experiment, but gives no plasmaron (i.e., no extra well-defined excitation satisfying Dyson's equation).
description: 5 pages, accepted to Phys. Rev. Lett
Third generation stellar models for asteroseismology of hot B subdwarf stars. A test of accuracy with the pulsating eclipsing binary PG 1336--018
Creators: name: Van Grootel, Valerie
name: Charpinet, Stephane
name: Brassard, Pierre
name: Fontaine, Gilles
name: Green, Elizabeth M.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Context. Asteroseismic determinations of structural parameters of hot B subdwarfs (sdB) have been carried out for more than a decade now. These analyses rely on stellar models whose reliability for the required task needs to be evaluated critically. Aims. We present new models of the so-called third generation (3G) dedicated to the asteroseismology of sdB stars. These parameterized models are complete static structures suitable for analyzing both p- and g-mode pulsators, contrary to the former second generation (2G) models that were limited to p-modes. While the reliability of the 2G models has been successfully verified in the past, this important test still has to be conducted on the 3G structures. Methods. The close eclipsing binary PG 1336-018 provides a unique opportunity to test the reliability of sdB models. We compared the structural parameters of the sdB component in PG 1336-018 obtained from asteroseismology based on the 3G models, with those derived independently from the modeling of the reflection/irradiation effect and the eclipses observed in the light curve. Results. The stellar parameters inferred from asteroseismology using the 3G models are found to be remarkably consistent with both the preferred orbital solution obtained from the binary light curve modeling and the updated spectroscopic estimates for the surface gravity of the star. We also show that the uncertainties on the input physics included in stellar models have no noticeable impact, at the current level of accuracy, on the structural parameters derived by asteroseismology. Conclusions. The stellar models presently used to carry out quantitative seismic analyses of sdB stars are reliable for the task. The stellar parameters inferred by this technique, at least for those that could be tested (M*, R*, and log g), appear to be both very precise and accurate, as no significant systematic effect has been found.
description: 26 pages
title: Renate Rolle, Vjačeslav Ju. Murcin und Andrej Ju. Alekseev, Königskurgan Čertomlyk. Ein skythischer Grabhügel des 4. vorchristlichen Jahrhundert
Creators: name: Schwarzmaier, Agnes
Publisher: name: University Library Heidelberg
Year: 2016

description: Rezension zu: Renate Rolle, Vjačeslav Ju. Murcin und Andrej Ju. Alekseev, Königskurgan Čertomlyk. Ein skythischer Grabhügel des 4. vorchristlichen Jahrhunderts. Hamburger Forschungen zur Archäologie, Band 1. Herausgegeben von Hans Georg Niemeyer und Renate Rolle. Verlag Philipp von Zabern, Mainz 1998. Teilband I (Textteil): VIII, 222 Seiten, 40 Abbildungen, 52 Tafeln; Teilband II (Katalog): IX, 41 Seiten, 65 Schwarzweißund 30 Farbtafeln; Teilband III (Beilagen): IV, 236 Seiten, 61 Abbildungen, 23 Schwarzweiß- und 3 Farbtafeln (Teilbände II und III zusammengebunden).
The QGP dynamics in relativistic heavy-ion collisions
Creators: name: Bratkovskaya, E. L.
name: Cassing, W.
name: Konchakovski, V. P.
name: Linnyk, O.
name: Ozvenchuk, V.
name: Toneev, V. D.
name: Voronyuk, V.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: The dynamics of partons and hadrons in relativistic nucleus-nucleus collisions is analyzed within the novel Parton-Hadron-String Dynamics (PHSD) transport approach, which is based on a dynamical quasiparticle model for the partonic phase (DQPM) including a dynamical hadronization scheme. The PHSD model reproduces a large variety of observables from SPS to LHC energies, e.g. the quark-number scaling of elliptic flow, transverse mass and rapidity spectra of charged hadrons, dilepton spectra, open and hidden charm production, collective flow coefficients etc., which are associated with the observation of a sQGP. The highlights of the latest results on collective flow are presented and open questions/perspectives are discussed.
description: 8 pages, 4 figures, contribution to the Proceedings of the Kruger-2012 International Workshop on Discovery Physics at the LHC (Kruger National park in South Africa, December 3-7, 2012)
Salix cinerea
Creators: name: Becherer
Publisher: name: Zenodo
Year: 1956
Subjects: Biodiversity
Taxonomy

description: P. cinerea X puberula - NachE. Schmid:Branson, Fully, Sitten, Oranges, Siders, Raron, Visp, Mörel, Deisch, Binneggen. (Vgl. E. Schmid bei A. Becherer in Ber. Schweiz.Bot. Ges. 4l, S. 316 [1932] und H. Frey Lit. 1935, passim.)
description: Published as part of Becherer, 1956, Florae Vallesiacae Supplementum, pp. 1-556 in Denkschriften der Schweizerischen Naturforschenden Gesellschaft 71 on pages 1-556
Observations of the WASP-2 System by the APOSTLE Program
Creators: name: Becker, Andrew C.
name: Kundurthy, Praveen
name: Agol, Eric
name: Barnes, Rory
name: Williams, Benjamin F.
name: Rose, Amy E.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: We present transit observations of the WASP-2 exoplanet system by the Apache Point Survey of Transit Lightcurves of Exoplanets (APOSTLE) program. Model fitting to these data allows us to improve measurements of the hot-Jupiter exoplanet WASP-2b and its orbital parameters by a factor of ~2 over prior studies; we do not find evidence for transit depth variations. We do find reduced chi^2 values greater than 1.0 in the observed minus computed transit times. A sinusoidal fit to the residuals yields a timing semi-amplitude of 32 seconds and a period of 389 days. However, random rearrangements of the data provide similar quality fits, and we cannot with certainty ascribe the timing variations to mutual exoplanet interactions. This inconclusive result is consistent with the lack of incontrovertible transit timing variations (TTVs) observed in other hot-Jupiter systems. This outcome emphasizes that unique recognition of TTVs requires dense sampling of the libration cycle (e.g. continuous observations from space-based platforms). However, even in systems observed with the Kepler spacecraft, there is a noted lack of transiting companions and TTVs in hot-Jupiter systems. This result is more meaningful, and indicates that hot-Jupiter systems, while they are easily observable from the ground, do not appear to be currently configured in a manner favorable to the detection of TTVs. The future of ground-based TTV studies may reside in resolving secular trends, and/or implementation at extreme quality observing sites to minimize atmospheric red noise.
description: ApJ Letters, accepted
Actions, Quotients and Lattices of Locally Compact Quantum Groups
Creators: name: Brannan, Michael
name: Chirvasitu, Alexandru
name: Viselter, Ami
Publisher: name: Deutsche Mathematiker-Vereinigung
Year: 2020

description: We prove a number of property (T) permanence results for locally compact quantum groups under exact sequences and the presence of invariant states, analogous to their classical versions. Along the way we characterize the existence of invariant weights on quantum homogeneous spaces of quotient type, and relate invariant states for LCQG actions on von Neumann algebras to invariant vectors in canonical unitary implementations, providing an application to amenability. Finally, we introduce a notion of lattice in a locally compact quantum group, noting examples provided by Drinfeld doubles of compact quantum groups. We show that property (T) lifts from a lattice to the ambient LCQG, just as it does classically, thus obtaining new examples of non-classical, non-compact, non-discrete LCQGs with property (T).
description: DOCUMENTA MATHEMATICA, Vol 25 (2020), p. 2553-2582
On the zero modes of the Faddev-Popov operator in the Landau gauge
Creators: name: Landim, R. R.
name: Vilar, L. C. Q.
name: Ventura, O. S.
name: Lemes, V. E. R.
Publisher: name: arXiv
Year: 2012
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Following Henyey procedure, we construct examples of zero modes of the Faddev-Popov operator in the Landau gauge in Euclidean space in D dimensions, for both SU(2) and SU(3 groups. We consider gauge field configurations $A^a_μ$ which give rise to a field strength, $F^a_{μν} =\partial_μA^a_ν-\partial_νA^a_μ+ f^{abc}A^b_μA^c_ν$, whose nonlinear term, $ f^{abc}A^b_μA^c_ν$, turns out to be nonvanishing. To our knowledge, this is the first time where such a non-abelian configuration is explicitly obtained in the case of SU(3) in 4D.
description: 14 page,no figures
title: Barbara Pferdehirt, Römische Militärdiplome und Entlassungsurkunden in der Sammlung des Römisch- Germanischen Zentralmuseums
Creators: name: Eck, Werner
Publisher: name: University Library Heidelberg
Year: 2016

description: Rezension zu: Barbara Pferdehirt, Römische Militärdiplome und Entlassungsurkunden in der Sammlung des Römisch-Germanischen Zentralmuseums, Teil I und II, Verlag des Römisch-Germanischen Zentralmuseums. In Kommission bei Rudolf Habelt Bonn, Mainz 2004. 217 Seiten, 138 Tafeln schwarzweiß, 4 Farbtafeln.
title: Yann Le Bohec, avec la collaboration de Catherine Wolff (Hrsg.), Les légions de Rome sous le Haut-Empire
Creators: name: Birley, Anthony R.
Publisher: name: University Library Heidelberg
Year: 2016

description: Rezension zu: Yann Le Bohec, avec la collaboration de Catherine Wolff (Hrsg.), Les légions de Rome sous le Haut-Empire. Actes du Congrès de Lyon (17 – 19 septembre 1998). Verlag De Boccard, Paris 2000. 2 Bände, 754 Seiten, zahlreiche Abbildungen im Text.
title: Susanna Künzl, Die Trierer Spruchbecherkeramik. Dekorierte Schwarzfirniskeramik des 3. und 4. Jahrhunderts n. Chr.
Creators: name: Lenz, Karl Heinz
Publisher: name: University Library Heidelberg
Year: 2016

description: Rezensionn zu: Susanna Künzl, Die Trierer Spruchbecherkeramik. Dekorierte Schwarzfirniskeramik des 3. und 4. Jahrhunderts n. Chr. Trierer Zeitschrift für Geschichte und Kunst des Trierer Landes und seiner Nachbargebiete, Beiheft 21. Hrsg. vom Rheinischen Landesmuseum Trier. Selbstverlag des Rheinischen Landesmuseums Trier, Trier 1997. 292 Seiten, 16 Typentafeln, 71 weitere Tafeln.
title: Jonathan Edmonson, Trinidad Nogales Basarrate und Walter Trillmich, Imagen y memoria. Monumentos funerarios con retratos en la Colonia Augusta Emerita
Creators: name: Caballos Rufino, Antonio
Publisher: name: University Library Heidelberg
Year: 2016

description: Rezension zu: Jonathan Edmonson, Trinidad Nogales Basarrate und Walter Trillmich, Imagen y memoria. Monumentos funerarios con retratos en la Colonia Augusta Emerita. Madrid, Real Academia de la Historia y Museo Nacional de Arte Romano. Bibliotheca Archaeologica Hispana, Band 10; zugleich Monografías Emeritenses, Band 6. Fundaciones de Estudios Romanos, BBVA, Ramón Areces y Caja Madrid, Diputación de Badajoz y Caja Duero, 2001. 253 Seiten, 71 und 27 Abbildungen, 8 Tafeln.
Finding extraterrestrial life using ground-based high-resolution spectroscopy
Creators: name: Snellen, Ignas
name: de Kok, Remco
name: Poole, Rudolf Le
name: Brogi, Matteo
name: Birkby, Jayne
Publisher: name: arXiv
Year: 2013
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Exoplanet observations promise one day to unveil the presence of extraterrestrial life. Atmospheric compounds in strong chemical disequilibrium would point to large-scale biological activity just as oxygen and methane do in the Earth's atmosphere. The cancellation of both the Terrestrial Planet Finder and Darwin missions means that it is unlikely that a dedicated space telescope to search for biomarker gases in exoplanet atmospheres will be launched within the next 25 years. Here we show that ground-based telescopes provide a strong alternative for finding biomarkers in exoplanet atmospheres through transit observations. Recent results on hot Jupiters show the enormous potential of high-dispersion spectroscopy to separate the extraterrestrial and telluric signals making use of the Doppler shift of the planet. The transmission signal of oxygen from an Earth-twin orbiting a small red dwarf star is only a factor 3 smaller than that of carbon monoxide recently detected in the hot Jupiter tau Bootis b, albeit such a star will be orders of magnitude fainter. We show that if Earth-like planets are common, the planned extremely large telescopes can detect oxygen within a few dozen transits. Ultimately, large arrays of dedicated flux collector telescopes equipped with high-dispersion spectrographs can provide the large collecting area needed to perform a statistical study of life-bearing planets in the solar neighborhood.
description: 22 pages, 3 figures; published in ApJ
title: Manfred K.H. Eggert, Archäologie. Grundzüge einer Historischen Kulturwissenschaft
Creators: name: Fernández-Götz, Manuel A.
Publisher: name: University Library Heidelberg
Year: 2016

description: Rezension zu: Manfred K.H. Eggert, Archäologie. Grundzüge einer Historischen Kulturwissenschaft. Verlag A. Francke, Tübingen und Basel 2006. XIV sowie 305 Seiten, 27 Abbildungen.
Online_supplementary_file_1.docx
Creators: name: Watts, Christina
Publisher: name: figshare
Year: 2023
Subjects: Public health not elsewhere classified

description: Online supplementary file for Watts C, Jones M, Lindorff K, Freeman B. How tobacco companies use the revolving door between government and industry to influence policymaking: an Australian case study. Public Health Res Pract. 2023; Online early publication. https://doi.org/10.17061/phrp33122305
title: Christa Landwehr, Die römischen Skulpturen von Caesarea Mauretaniae. Band III. Idealplastik. Bacchus und Gefolge – Masken – Fabelwesen – Tiere – Bukranien – nicht benennbare Figuren
Creators: name: Fuchs, Michaela
Publisher: name: University Library Heidelberg
Year: 2016

description: Christa Landwehr, Die römischen Skulpturen von Caesarea Mauretaniae. Band III. Idealplastik. Bacchus und Gefolge – Masken – Fabelwesen – Tiere – Bukranien – nicht benennbare Figuren. Aufnahmen von Florian Kleinefenn. Mit Beiträgen von Rita Amedick, Dagmar Grassinger und Adrian Zimmermann. Philipp von Zabern, Mainz 2006. XVI und 127 Seiten, 11 Abbildungen, 80 Tafeln sowie 32 Beilagen.
Constraining the Interiors of Asteroids Through Close Encounters
Creators: name: Dinsmore, Jack T
name: de Wit, Julien
Publisher: name: arXiv
Year: 2022
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Knowledge of the interior density distribution of an asteroid can reveal its composition and constrain its evolutionary history. However, most asteroid observational techniques are not sensitive to interior properties. We investigate the interior constraints accessible through monitoring variations in angular velocity during a close encounter. We derive the equations of motion for a rigid asteroid's orientation and angular velocity to arbitrary order and use them to generate synthetic angular velocity data for a representative asteroid on a close Earth encounter. We develop a toolkit AIME (Asteroid Interior Mapping from Encounters) which reconstructs asteroid density distribution from these data, and we perform injection-retrieval tests on these synthetic data to assess AIME's accuracy and precision. We also perform a sensitivity analysis to asteroid parameters (e.g., asteroid shape and orbital elements), observational set-up (e.g., measurement precision and cadence), and the mapping models used. We find that high precision in rotational period estimates (<~0.27 seconds) are necessary for each cadence, and that low perigees (<~18 Earth radii) are necessary to resolve large-scale density non-uniformities to uncertainties ~0.1% of the local density under some models.
description: 17 pages, 14 figures. This is a pre-copyedited, author-produced PDF of an article accepted for publication in MNRAS following peer review