cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Dark Energy in the Dark Ages
Creators: name: Linder, Eric V.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Non-negligible dark energy density at high redshifts would indicate dark energy physics distinct from a cosmological constant or ``reasonable'' canonical scalar fields. Such dark energy can be constrained tightly through investigation of the growth of structure, with limits of \la2% of total energy density at z\gg1 for many models. Intermediate dark energy can have effects distinct from its energy density; the dark ages acceleration can be constrained to last less than 5% of a Hubble e-fold time, exacerbating the coincidence problem. Both the total linear growth, or equivalently σ_8, and the shape and evolution of the nonlinear mass power spectrum for z<2 (using the Linder-White nonlinear mapping prescription) provide important windows. Probes of growth, such as weak gravitational lensing, can interact with supernovae and CMB distance measurements to scan dark energy behavior over the entire range z=0-1100.
description: 6 pages, 5 figures; figure added, minor edits to match Astropart.Phys. version
On the existence of a first order phase transition at small vacuum angle $θ$ in the $CP^3$ model
Creators: name: Olejnik, S.
name: Schierholz, G.
Publisher: name: arXiv
Year: 1993
Subjects: subject: High Energy Physics - Lattice (hep-lat)
subject: FOS: Physical sciences

description: We examine the phase structure of the $CP^3$ model as a function of $θ$ in the weak coupling regime. It is shown that the model has a first order phase transition at small $θ$. We pay special attention to the extrapolation of the data to the infinite volume. It is found that the critical value of $θ$ decreases towards zero as $β$ is taken to infinity.
description: 3 pages, DESY 93-177, talk presented by G. Schierholz at Lattice93
Case Study : The merger between Renault and Nissan
Creators: name: Benoit Lamarsaude
Publisher: name: figshare
Year: 2018
Subjects: subject: 160607 International Relations
subject: FOS: Political science

description: This paper describes the negotiations to form the Renault-Nissan alliance. Many observers doubted that the companies would reach agreement in 1999, let alone develop a partnership lauded throughout the auto industry fifteen years later. Firstly, the analysis focus on the key elements of this negotiation, developing the three dimensions: who?, what? and how?. Secondly the conduct of negotiations ,from the first contact of the two companies to the signed agreement, is described and discussed. Finally, as a conclusion, this paper ends on the learning we can pull from this case.
DESARROLLO DE HABILIDADES COGNITIVAS A TRAVÉS DE JUEGOS DE MESA: ANÁLISIS DE BLACK ROSE WARS: REBIRTH, CATAN Y PANDEMIC
Creators: name: Fallon Lopez Neumann, Elfriede Kristall
Publisher: name: UNITEPC
Year: 2024

description: En los últimos años los juegos de mesa han demostrado ser una valiosa herramienta para el aprender y desarrollar diferentes habilidades cognitivas. Investigaciones en el campo de la psicología y la educación destacan cómo la estructura y dinámica de los juegos de mesa no solo entretienen, sino que también facilitan el aprendizaje y la práctica de habilidades cognitivas y socioemocionales, como el trabajo en equipo, la toma de decisiones estratégicas y la gestión de recursos (Gobet et al., 2012). En este resumen extendido se analizarán estos tres juegos de mesa: Black Rose Wars: Rebirth, Catan y Pandemic, con el fin examinar como pueden ayudar a desarrollar diferentes habilidades cognitivas siguiendo la teoría de las inteligencias múltiples de Howard Gardner (1983). Según esta teoría, todas las personas poseen diferentes tipos de inteligencias, y estas pueden aprender a través de la práctica.
Code_Aster : collaborative innovation at EDF
Creators: name: Benoit Lamarsaude
Publisher: name: figshare
Year: 2018
Subjects: subject: 150307 Innovation and Technology Management
subject: FOS: Economics and business

description: Code_Aster is a computation software by finite elements used and developed by EDF to numerical simulation purposes used in the design of structures for over 25 years. In 2001 EDF decides to distribute this software under public license. Unusual for a program of this scale, this decision stems from a desire to EDF always evolve and innovate through the tool used by all engineering services. This paper describes how the organization implemented and adjusted over the years has enabled it to become a benchmark software. The observation is particularly focused on the elements favoring the emergence of innovations through this project.
Crossing conditions in coupled cluster theory
Creators: name: Kjønstad, Eirik F.
name: Myhre, Rolf H.
name: Martinez, Todd J.
name: Koch, Henrik
Publisher: name: arXiv
Year: 2017
Subjects: subject: Chemical Physics (physics.chem-ph)
subject: FOS: Physical sciences

description: We derive the crossing conditions at conical intersections between electronic states in coupled cluster theory, and show that if the coupled cluster Jacobian matrix is nondefective, two (three) independent conditions are correctly placed on the nuclear degrees of freedom for an inherently real (complex) Hamiltonian. Calculations using coupled cluster theory on an $2 {^{1}}A' / 3 {^{1}}A'$ conical intersection in hypofluorous acid illustrate the nonphysical artifacts associated with defects at accidental same-symmetry intersections. In particular, the observed intersection seam is folded about a space of the correct dimensionality, indicating that minor modifications to the theory are required for it to provide a correct description of conical intersections in general. We find that an accidental symmetry allowed $1 {^{1}}A" / 2 {^{1}}A"$ intersection in hydrogen sulfide is properly described, showing no artifacts as well as linearity of the energy gap to first order in the branching plane.
description: 9 pages and 4 figures
Information dynamics in quantum theory
Creators: name: Garbaczewski, Piotr
Publisher: name: arXiv
Year: 2006
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Shannon entropy and Fisher information functionals are known to quantify certain information-theoretic properties of continuous probability distributions of various origins. We carry out a systematic study of these functionals, while assuming that the pertinent probability density has a quantum mechanical appearance $ρ\doteq |ψ|^2$, with $ψ\in L^2(R)$. Their behavior in time, due to the quantum Schrödinger picture evolution-induced dynamics of $ρ(x,t)$ is investigated as well, with an emphasis on thermodynamical features of quantum motion.
description: 11 pages
Formation of the first star clusters and massive star binaries by fragmentation of filamentary primordial gas clouds
Creators: name: Hirano, Shingo
name: Yoshida, Naoki
name: Sakurai, Yuya
name: Fujii, Michiko S.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We perform a set of cosmological simulations of early structure formation with incorporating baryonic streaming motions. We present a case where a significantly elongated gas cloud with $\sim\!10^4\,$solar masses (${\rm M_\odot}$) is formed in a pre-galactic ($\sim\!10^7\,{\rm M_\odot}$) dark halo. The gas streaming into the halo compresses and heats the massive filamentary cloud to a temperature of $\sim\!10,000\,$Kelvin. The gas cloud cools rapidly by atomic hydrogen cooling, and then by molecular hydrogen cooling down to $\sim\!400\,$Kelvin. The rapid decrease of the temperature and hence of the Jeans mass triggers fragmentation of the filament to yield multiple gas clumps with a few hundred solar masses. We estimate the mass of the primordial star formed in each fragment by adopting an analytic model based on a large set of radiation hydrodynamics simulations of protostellar evolution. The resulting stellar masses are in the range of $\sim\!50$-$120\,{\rm M_\odot}$. The massive stars gravitationally attract each other and form a compact star cluster. We follow the dynamics of the star cluster using a hybrid $N$-body simulation. We show that massive star binaries are formed in a few million years through multi-body interactions at the cluster center. The eventual formation of the remnant black holes will leave a massive black hole binary, which can be a progenitor of strong gravitational wave sources similar to those recently detected by the Advanced Laser Interferometer Gravitational-Wave Observatory (LIGO).
description: 13 pages, 11 figures, 2 tables, accepted to ApJ
Alice: The Rosetta Ultraviolet Imaging Spectrograph
Creators: name: Stern, S. A.
name: Slater, D. C.
name: Scherrer, J.
name: Stone, J.
name: Versteeg, M.
name: A'Hearn, M. F.
name: Bertaux, J. L.
name: Feldman, P. D.
name: Festou, M. C.
name: Parker, J. Wm.
name: Siegmund, O. H. W.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We describe the design, performance and scientific objectives of the NASA-funded ALICE instrument aboard the ESA Rosetta asteroid flyby/comet rendezvous mission. ALICE is a lightweight, low-power, and low-cost imaging spectrograph optimized for cometary far-ultraviolet (FUV) spectroscopy. It will be the first UV spectrograph to study a comet at close range. It is designed to obtain spatially-resolved spectra of Rosetta mission targets in the 700-2050 A spectral band with a spectral resolution between 8 A and 12 A for extended sources that fill its ~0.05 deg x 6.0 deg field-of-view. ALICE employs an off-axis telescope feeding a 0.15-m normal incidence Rowland circle spectrograph with a concave holographic reflection grating. The imaging microchannel plate detector utilizes dual solar-blind opaque photocathodes (KBr and CsI) and employs a 2 D delay-line readout array. The instrument is controlled by an internal microprocessor. During the prime Rosetta mission, ALICE will characterize comet 67P/Churyumov-Gerasimenko's coma, its nucleus, and the nucleus/coma coupling; during cruise to the comet, ALICE will make observations of the mission's two asteroid flyby targets and of Mars, its moons, and of Earth's moon. ALICE has already successfully completed the in-flight commissioning phase and is operating normally in flight. It has been characterized in flight with stellar flux calibrations, observations of the Moon during the first Earth fly-by, and observations of comet Linear T7 in 2004 and comet 9P/Tempel 1 during the 2005 Deep Impact comet-collision observing campaign
description: 11 pages, 7 figures
High-resolution TNG spectra of T Tauri stars: Near-IR GIANO observations of the young variables XZ Tau and DR Tau
Creators: name: Antoniucci, S.
name: Nisini, B.
name: Biazzo, K.
name: Giannini, T.
name: Lorenzetti, D.
name: Sanna, N.
name: Harutyunyan, A.
name: Origlia, L.
name: Oliva, E.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We used the TNG/GIANO instrument to obtain near-IR high-resolution spectra (R~50000) of XZ Tau and DR Tau, two actively accreting T Tauri stars classified as EXors. The analysis of the observed features provides information on the properties of the inner disk, the accretion columns, and the winds. Both sources display composite HI line profiles, with contributions from both accreting gas and high-velocity winds. These lines become more symmetric and narrower with increasing upper energy, which may be interpreted in terms of two components with different decrements or imputed to self-absorption effects. XZ Tau shows a relatively high state of activity with respect to literature observations. The variation of the HeI 1.08um line blue-shifted absorption suggests that the inner wind has undergone a dramatic change in its velocity structure, connected with a recent accretion event. DR Tau has a more stable wind as its HeI 1.08um absorption is stable in time in spite of strong variability of the emission component. The IR veiling can be interpreted as due to blackbody emission at temperatures of 1600K for XZ Tau and 2300K DR Tau, with emitting areas ~30 times larger than the star. For XZ Tau these conditions are consistent with emission from the inner rim of the dusty disk, while for DR Tau the fairly high temperature may suggest an origin from a thick gaseous disk within the dust sublimation radius. Strong and broad metallic lines, mainly from CI and FeI, are detected in XZ Tau, similar to those observed in other EXor sources during burst phases. DR Tau shows weaker and narrower metallic lines, despite its larger accretion luminosity. This suggests that accretion is not the only driver of metallic line excitation. Our observations show the potential of wide-band, high-resolution near-IR spectroscopy to simultaneously probe the phenomena that occur in the star-disk interaction region.
description: 15 pages, accepted by A&A
Case Study : 2016 Future Supply Chain
Creators: name: Benoit Lamarsaude
Publisher: name: figshare
Year: 2018
Subjects: subject: 150309 Logistics and Supply Chain Management
subject: FOS: Economics and business
subject: 10206 Operations Research
subject: FOS: Mathematics

description: This paper offers a look at the work carried out in 2008 by the Global Commerce Initiative and Cap Gemini on the future of the supply chain in the medium term. First we resent the key ideas of the paper CGI and Cap Gemini. We present and detail two examples of process developments in the fields of evolution cites the report of CGI and Cap Gemini. These examples are the management of fluctuating demand and reverse logistics. Both are these real cases from the indemnisaton chain of an insurance company. Theimplementation of the conditions and benefits are presented and discussed. We show the relevance of the concepts of logistics in areas that are not natively considered as such.
Note Regarding Clearance of Telegram for Warsaw Embassy
Creators: name: United States. Department Of State
Publisher: name: The University of Texas at Austin
Year: 1964
Subjects: Box 200 Folder 8
Box 200 Folder 08
Poland -- Politics and government -- 1945-1980
Poland -- Relations -- United States

description: Note to Bundy from Read with enclosed telegram detailing necessary White House clearance prior to transmission.
title: ADCO, Cartulaire de Cîteaux pour les domaines de Beaune (XVe siècle), Cart. 177 (11 H 289), 197 folios, f. 0331
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2015
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: cartulaire
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Cartulaire de Cîteaux pour les domaines de Beaune (XVe siècle), Archives départementales de la Côte-d'Or, Cart. 177 (11 H 289), 197 folios, f. 0331, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire de Cîteaux pour les possessions d’Izeure (XVe siècle), Archives départementales de la Côte-d'Or, Cart. 177 (11 H 289), 197 folios, f. 0331, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
Bound states in the continuum in a single-level Fano-Anderson model
Creators: name: Longhi, Stefano
Publisher: name: arXiv
Year: 2006
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Bound states in the continuum (BIC) are shown to exist in a single-level Fano-Anderson model with a colored interaction between the discrete state and a tight-binding continuum, which may describe mesoscopic electron or photon transport in a semi-infinite one-dimensional lattice. The existence of BIC is explained in the lattice realization as a boundary effect induced by lattice truncation.
description: 5 figures (submitted for publication)
Sonate : [fis-moll für Klavier] : [Op. 1]
Creators: name: Weber, Gustav
Publisher: name: [s.n.]
Year: 1845

description: Gustav Weber
description: Öffentliche Bibliothek der Universität Basel
description: Digitalisierung=Digitization=Numérisation September 2023 TIFF
description: Verzeichnung=Description=Inventaire 2009 Übernahme Rekatalogis. AK UB durch Medea 2002-2005
Quantum Quenches and Relaxation Dynamics in the Thermodynamic Limit
Creators: name: Mallayya, Krishnanand
name: Rigol, Marcos
Publisher: name: arXiv
Year: 2017
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Quantum Gases (cond-mat.quant-gas)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We implement numerical linked cluster expansions (NLCEs) to study dynamics of lattice systems following quantum quenches, and focus on a hard-core boson model in one-dimensional lattices. We find that, in the nonintegrable regime and within the accessible times, local observables exhibit exponential relaxation. We determine the relaxation rate as one departs from the integrable point and show that it scales quadratically with the strength of the integrability breaking perturbation. We compare the NLCE results with those from exact diagonalization calculations on finite chains with periodic boundary conditions, and show that NLCEs are far more accurate.
description: 5 pages, 3 figures, as published
Scientific performance analysis of the SYZ telescope design vs. the RC telescope design
Creators: name: Ma, Donglin
name: Cai, Zheng
Publisher: name: arXiv
Year: 2017
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: Recently, Su et al. (2016) propose a telescope design, referred as the "SYZ" design, for Chinese new project of a 12m optical-infrared telescope. The SYZ telescope design consists of three aspheric mirrors with non-zero power, including a relay mirror below the primary mirror. SYZ design yields a good imaging quality and has a relatively flat field curvature at Nasmyth focus. To evaluate the science-compatibility of this three-mirror telescope, in this paper, we thoroughly compare the performance of SYZ design with that of Ritchey-Chrétien (RC) design, a conventional two-mirror telescope design. Further, we propose the Observing Information Throughput ($OIT$) as a metric for quantitatively evaluating the telescopes' science performance. We find that although a SYZ telescope yields a superb imaging quality over a large field of view, a two-mirror (RC) telescope design holds a higher overall throughput, a better diffraction-limited imaging quality in the central field of view (FOV$<5'$) which is better for the performance of extreme Adaptive Optics (AO), and a generally better scientific performance with a higher $OIT$ value.
description: 10 pages, 7 figures; submitted
Radio continuum monitoring of the extreme carbon star IRC+10216
Creators: name: Menten, K. M.
name: Reid, M. J.
name: Kruegel, E.
name: Claussen, M. J.
name: Sahai, R.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We describe Very Large Array observations of the extreme carbon star IRC+10216 at 8.4, 14.9, and 22.5 GHz made over a two year period. We find possible variability correlated with the infrared phase and a cm- to sub-millimeter wavelength spectral index very close to 2. The variability, observed flux densities, and upper limit on the size are consistent with the emission arising from the stellar photosphere or a slightly larger radio photosphere.
description: 9 pages, incl. 4 figures. To appear in Astronomy & Astrophysics
Message Regarding Verbatim Text from President Concerning President Zawadzki
Creators: name: United States. Department Of State
Publisher: name: The University of Texas at Austin
Year: 1964
Subjects: Box 200 Folder 8
Box 200 Folder 08
Poland -- Politics and government -- 1945-1980
Poland -- Relations -- United States

description: Message stating verbatim text to be delivered on behalf of President following the death of Aleksandr Zawadzki.
Stability of cosmic structures in scalar-tensor theories of gravity
Creators: name: Panotopoulos, Grigoris
name: Rincon, Angel
Publisher: name: arXiv
Year: 2017
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: In the present work we study a concrete model of Scalar--Tensor theory of gravity characterized by two free parameters, and compare its predictions against observational data and constraints coming from supernovae, solar system tests as well as the stability of cosmic structures. First an exact analytical solution at the background level is obtained. Then using that solution the expression for the turnaround radius is computed. Finally we show graphically how current data and limits put bounds on the parameters of the model at hand.
description: v2: 6 pages, 6 figures, references added, improved introduction, to appear in: The European Physical Journal C
The Isgur-Wise Function
Creators: name: Kenway, R. D.
Publisher: name: arXiv
Year: 1993
Subjects: subject: High Energy Physics - Lattice (hep-lat)
subject: FOS: Physical sciences

description: After a brief introduction to the Heavy-Quark Effective Theory (HQET), I review the extraction of the Isgur-Wise function from lattice QCD calculations of the matrix elements for semi-leptonic decays of heavy-light pseudoscalar mesons both into pseudoscalar and into vector mesons. This work is beginning to test the heavy-quark spin-flavour symmetries around the charm mass and to indicate the size of $O(1/m_c)$ corrections. An alternative approach to put the HQET on the lattice offers the prospect of computing the Isgur-Wise function directly.
description: 6 pages, uuencoded compressed tar postscript file, Edinburgh preprint 93/535, Talk presented at LATTICE 93 Dallas
Baryogenesis from Oscillations of Charmed or Beautiful Baryons
Creators: name: Aitken, Kyle
name: McKeen, David
name: Nelson, Ann E.
name: Neder, Thomas
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We propose a model for CP violating oscillations of neutral, heavy-flavored baryons into antibaryons at rates which are within a few orders of magnitude of their lifetimes. The flavor structure of the baryon violation suppresses neutron oscillations and baryon number violating nuclear decays to experimentally allowed rates. We also propose a scenario for producing such baryons in the early Universe via the out-of-equilibrium decays of a neutral particle, after hadronization but before nucleosynthesis. We find parameters where CP violating baryon oscillations at a temperature of a few MeV could result in the observed asymmetry between baryons and antibaryons. Furthermore, part of the relevant parameter space for baryogenesis is potentially testable at Belle II via decays of heavy flavor baryons into an exotic neutral fermion. The model introduces four new particles: three light Majorana fermions and a colored scalar. The lightest of these fermions is typically long lived on collider timescales and may be produced in decays of bottom and possibly charmed hadrons.
description: 15 pages, 6 figures
Extrinsic Parameter Calibration for Line Scanning Cameras on Ground Vehicles with Navigation Systems Using a Calibration Pattern
Creators: name: Wendel, Alexander
name: Underwood, James
Publisher: name: arXiv
Year: 2017
Subjects: subject: Robotics (cs.RO)
subject: Computer Vision and Pattern Recognition (cs.CV)
subject: FOS: Computer and information sciences

description: Line scanning cameras, which capture only a single line of pixels, have been increasingly used in ground based mobile or robotic platforms. In applications where it is advantageous to directly georeference the camera data to world coordinates, an accurate estimate of the camera's 6D pose is required. This paper focuses on the common case where a mobile platform is equipped with a rigidly mounted line scanning camera, whose pose is unknown, and a navigation system providing vehicle body pose estimates. We propose a novel method that estimates the camera's pose relative to the navigation system. The approach involves imaging and manually labelling a calibration pattern with distinctly identifiable points, triangulating these points from camera and navigation system data and reprojecting them in order to compute a likelihood, which is maximised to estimate the 6D camera pose. Additionally, a Markov Chain Monte Carlo (MCMC) algorithm is used to estimate the uncertainty of the offset. Tested on two different platforms, the method was able to estimate the pose to within 0.06 m / 1.05$^{\circ}$ and 0.18 m / 2.39$^{\circ}$. We also propose several approaches to displaying and interpreting the 6D results in a human readable way.
description: Published in MDPI Sensors, 30 October 2017
Global Generalized Bianchi Identities for Invariant Variational Problems on Gauge-natural Bundles
Creators: name: Palese, M.
name: Winterroth, E.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Mathematical Physics (math-ph)
subject: High Energy Physics - Theory (hep-th)
subject: Differential Geometry (math.DG)
subject: FOS: Physical sciences
subject: FOS: Mathematics
subject: 58A20;58A32;58E30;58E40;58J10;58J70

description: We derive both {\em local} and {\em global} generalized {\em Bianchi identities} for classical Lagrangian field theories on gauge-natural bundles. We show that globally defined generalized Bianchi identities can be found without the {\em a priori} introduction of a connection. The proof is based on a {\em global} decomposition of the {\em variational Lie derivative} of the generalized Euler--Lagrange morphism and the representation of the corresponding generalized Jacobi morphism on gauge-natural bundles. In particular, we show that {\em within} a gauge-natural invariant Lagrangian variational principle, the gauge-natural lift of infinitesimal principal automorphism {\em is not} intrinsically arbitrary. As a consequence the existence of {\em canonical} global superpotentials for gauge-natural Noether conserved currents is proved without resorting to additional structures.
description: 24 pages, minor changes, misprints corrected, a misprint in the coordinate expression of the Jacobi morphism corrected; final version to appear in Arch. Math. (Brno)
Memo Regarding Conversation with Norman Cousins
Creators: name: United States. Department Of State
Publisher: name: The University of Texas at Austin
Year: 1965
Subjects: Box 200 Folder 8
Box 200 Folder 08
Poland -- Politics and government -- 1945-1980
Poland -- Relations -- United States

description: Memo to Read from Bundy detailing conversation with Norman Cousins regarding elements of telephonic report, Polish positions, and ICC status.
title: 02_1560
Creators: name: Wesley Baldwin, John
name: Baldwin, John W.
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2018
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: L'ensemble de ces notes ont été crée par John Baldwin lors d'une de ses premières périodes de résidence à Paris. Ces documents comprennent tous les magistri qu’il avait pu rencontrer dans ses sources. Aux XIIème et XIIIème siècles, les universités n'existant pas encore, le titre de magister s'il évoque certainement une compétence n'est pas rattaché de façon systématique au passage par les écoles. De surcroît, les magistris sont le plus souvent désignés par leur seul prénom. La lecture de ces données est donc difficile et suppose un long travail pour tenter d'identifier un individu auquel on pourrait rattacher plusieurs mentions. John Baldwin avait donc renoncé à utiliser ces données pour donner un prolongement à sa magnifique étude sur les gradués d'université et leur emploi par les Capétiens et les Plantagenêts. Néanmoins, il a conservé ces données et elles sont potentiellement très utile dans le cadre de Studium, comme le sont toutes les mentions dans les volumes des Fasti Ecclesiae Gallicanae de chanoines portant ce titre de magister sans autres précisions. L'ampleur des dépouillements rend ces données très utiles et nous devons une grande reconnaissance à John Baldwin pour avoir pris la peine de faire photocopier ses fiches et de nous les avoir transmises amicalement.
Les données ainsi que les images des fiches sont accessibles sur le site Internet à l'adresse suivante : http://studium-baldwin.lamop.fr/.
Les transcriptions des fiches ont été effectuées par des étudiants de Paris 1 Panthéon - Sorbonne mais elles n'ont pas été corrigées par la suite.
description: Relation: https://lamop.hypotheses.org/
The Little Cub: Discovery of an Extremely Metal-Poor Star-Forming Galaxy in the Local Universe
Creators: name: Hsyu, Tiffany
name: Cooke, Ryan J.
name: Prochaska, J. Xavier
name: Bolte, Michael
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We report the discovery of the Little Cub, an extremely metal-poor star-forming galaxy in the local Universe, found in the constellation Ursa Major (a.k.a. the Great Bear). We first identified the Little Cub as a candidate metal-poor galaxy based on its Sloan Digital Sky Survey photometric colors, combined with spectroscopy using the Kast spectrograph on the Shane 3-m telescope at Lick Observatory. In this letter, we present high-quality spectroscopic data taken with the Low Resolution Imaging Spectrometer at Keck Observatory, which confirm the extremely metal-poor nature of this galaxy. Based on the weak [O III] 4363 Angstrom emission line, we estimate a direct oxygen abundance of 12 + log(O/H) = 7.13 +/- 0.08, making the Little Cub one of the lowest metallicity star-forming galaxies currently known in the local Universe. The Little Cub appears to be a companion of the spiral galaxy NGC 3359 and shows evidence of gas stripping. We may therefore be witnessing the quenching of a near-pristine galaxy as it makes its first passage about a Milky Way-like galaxy.
description: 8 pages, 3 figures, Accepted for publication in the Astrophysical Journal Letters
Note Regarding Bundy's Documentation of Conversation with Norman Cousins
Creators: name: United States. Department Of State
Publisher: name: The University of Texas at Austin
Year: 1965
Subjects: Box 200 Folder 8
Box 200 Folder 08
Poland -- Politics and government -- 1945-1980
Poland -- Relations -- United States

description: Note from Bundy detailing conversation with Norman Cousins regarding conversations with the North Vietnamese.
Digitisation in the forest-based sector. State of technology and opportunities for innovation
Creators: name: Kies, Uwe
name: Lengefeld, Andreas Kleinschmit Von
Publisher: name: Zenodo
Year: 2018
Subjects: industry 4.0
forest-based sector
digital transformation

description: Disruptive technologies pave the way for the 4th industrial revolution and to tremendous changes in production and manufacturing. How is the forest-based sector prepared for these changes and what are the opportunities for growth and innovation? Presentation at the Club du Bois at the European Parliament, Brussels, 10 Jan 2018, hosted by CEI-Bois, EPF, EOS www.clubdubois.eu
title: 01_0739
Creators: name: Wesley Baldwin, John
name: Baldwin, John W.
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2018
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: L'ensemble de ces notes ont été crée par John Baldwin lors d'une de ses premières périodes de résidence à Paris. Ces documents comprennent tous les magistri qu’il avait pu rencontrer dans ses sources. Aux XIIème et XIIIème siècles, les universités n'existant pas encore, le titre de magister s'il évoque certainement une compétence n'est pas rattaché de façon systématique au passage par les écoles. De surcroît, les magistris sont le plus souvent désignés par leur seul prénom. La lecture de ces données est donc difficile et suppose un long travail pour tenter d'identifier un individu auquel on pourrait rattacher plusieurs mentions. John Baldwin avait donc renoncé à utiliser ces données pour donner un prolongement à sa magnifique étude sur les gradués d'université et leur emploi par les Capétiens et les Plantagenêts. Néanmoins, il a conservé ces données et elles sont potentiellement très utile dans le cadre de Studium, comme le sont toutes les mentions dans les volumes des Fasti Ecclesiae Gallicanae de chanoines portant ce titre de magister sans autres précisions. L'ampleur des dépouillements rend ces données très utiles et nous devons une grande reconnaissance à John Baldwin pour avoir pris la peine de faire photocopier ses fiches et de nous les avoir transmises amicalement.
Les données ainsi que les images des fiches sont accessibles sur le site Internet à l'adresse suivante : http://studium-baldwin.lamop.fr/.
Les transcriptions des fiches ont été effectuées par des étudiants de Paris 1 Panthéon - Sorbonne mais elles n'ont pas été corrigées par la suite.
description: Relation: https://lamop.hypotheses.org/
Memorandum of Conversation Regarding Security, Non-Proliferation, and the German Problem
Creators: name: United States. Department Of State
Publisher: name: The University of Texas at Austin
Year: 1965
Subjects: Box 200 Folder 8
Box 200 Folder 08
Poland -- Politics and government -- 1945-1980
Poland -- Relations -- United States

description: Memorandum of conversation regarding need to find permanent solution to problems of Central Europe.
Broadening of the chiral critical region in a hydrodynamically expanding medium
Creators: name: Herold, Christoph
name: Bleicher, Marcus
name: Nahrgang, Marlene
name: Steinheimer, Jan
name: Limphirat, Ayut
name: Kobdaj, Chinorat
name: Yan, Yupeng
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We investigate higher cumulants of the sigma field as the chiral order parameter at the QCD phase transition. We derive a thermodynamic expression for the skewness and kurtosis from susceptibilities and use these to determine $Sσ$ and $κσ^2$ for the sigma field in equilibrium. In a next step, we study the behavior of these cumulants in both an equilibrated static medium and an expanding medium resembling the hydrodynamic stage of a heavy-ion collision. For the latter one, we find a significant broadening of the critical region.
description: 7 pages, 3 figures, accepted for publication in EPJ A
Note Regarding Enclosed Conversation Between President and Polish Ambassador Drozniak
Creators: name: United States. Department Of State
Publisher: name: The University of Texas at Austin
Year: 1965
Subjects: Box 200 Folder 8
Box 200 Folder 08
Poland -- Politics and government -- 1945-1980
Poland -- Relations -- United States

description: Note from Edmund Glenn concerning attached documents expressing details of conversation between President and Polish Ambassador and the President's documented remarks.
Was the Milky Way Bulge Formed From The Buckling Disk Instability, Hierarchical Collapse, Accretion of Clumps, or All of the Above?
Creators: name: Nataf, David M.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: The assembly of the Milky Way bulge is an old topic in astronomy, one now in a period of renewed and rapid development. The dominant scenario for bulge formation is that of the Milky Way as a nearly pure disk galaxy, with the inner disk having formed a bar and buckled. This can potentially explain virtually all bulge stars with [Fe/H] ~ -0.50.
description: 13 pages, 5 figures, accepted for publication in PASA
A Mathematician's Viewpoint to Bell's theorem: In Memory of Walter Philipp
Creators: name: Khrennikov, Andrei
Publisher: name: arXiv
Year: 2006
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: In this paper dedicated to the memory of Walter Philipp, we formalize the rules of classical$\to$ quantum correspondence and perform a rigorous mathematical analysis of the assumptions in Bell's NO-GO arguments.
Memorandum of Conversation Regarding Presidential Discussion as Confidential Discussion
Creators: name: United States. Department Of State
Publisher: name: The University of Texas at Austin
Year: 1965
Subjects: Box 200 Folder 8
Box 200 Folder 08
Poland -- Politics and government -- 1945-1980
Poland -- Relations -- United States

description: Memorandum of conversation detailing exchanged words between the President and Polish Ambassador Drozniak, part 1 of 3.
Memorandum of Conversation Regarding Presidential Discussion of Vietnam
Creators: name: United States. Department Of State
Publisher: name: The University of Texas at Austin
Year: 1965
Subjects: Box 200 Folder 8
Box 200 Folder 08
Poland -- Politics and government -- 1945-1980
Poland -- Relations -- United States

description: Memorandum of conversation detailing exchanged words between the President and Polish Ambassador Drozniak, part 2 of 3.
Recovering the Inflationary Potential and Primordial Power Spectrum With a Slow Roll Prior: Methodology and Application to WMAP 3 Year Data
Creators: name: Peiris, Hiranya
name: Easther, Richard
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We introduce a new method for applying an inflationary prior to a cosmological dataset that includes relations between observables at arbitrary order in the slow roll expansion. The process is based on the inflationary flow equations, and the slow roll parameters appear explicitly in the cosmological parameter set. We contrast our method to other ways of imposing an inflationary prior on a cosmological dataset, and argue that this method is ideal for use with heterogeneous datasets. In particular, it would be well suited to exploiting any direct detection of fundamental tensor modes by a BBO-style mission. To demonstrate the practical use of this method we apply it to the WMAPI+All dataset, and the newly released WMAPII dataset on its own and together with the SDSS data. We find that all basic classes of single field inflationary models are still allowed at the 1-2sigma level, but the overall parameter space is sharply constrained. In particular, we find evidence that the combination of WMAPII+SDSS is sensitive to effects arising from terms that are quadratic in the two leading-order slow roll parameters.
description: v2 adds references and fixes typos. New explanatory material added clarifying effects that depend on terms that are second order in the slow roll parameters, and the impact of the beam parametrization and SZ prior on the central value of n_s v3: Added refs, minor clarifications, title modified. In press with JCAP v4: New figures, with minor smoothing artifacts removed. Matches published version. v5 Fixed typo in caption of Figure 5
A review of heavy-heavy spectroscopy
Creators: name: Davies, C. T. H.
Publisher: name: arXiv
Year: 1993
Subjects: subject: High Energy Physics - Lattice (hep-lat)
subject: FOS: Physical sciences

description: Calculations of the heavy-heavy spectrum present a good opportunity for precision tests of QCD using lattice techniques. All methods make use of a non-relativistic expansion of the action and its systematic improvement to remove lattice artefacts. There was convincing demonstration this year that these methods work and that the associated perturbation theory is well-behaved. Comparison to experimental results yields an accurate value for the lattice spacing, a, a key result in the determination of α_{s}, and (for the first time this year) the mass of the b quark (4.7(1) GeV).
description: talk at Lattice'93, Dallas. 6 pages of latex espcrc2.sty needed and figures on request
The Pristine survey III: Spectroscopic confirmation of an efficient search for extremely metal-poor stars
Creators: name: Youakim, K.
name: Starkenburg, E.
name: Aguado, D. S.
name: Martin, N. F.
name: Fouesneau, M.
name: Hernández, J. I. González
name: Prieto, C. Allende
name: Bonifacio, P.
name: Gentile, M.
name: Kielty, C.
name: Côté, P.
name: Jablonka, P.
name: McConnachie, A.
name: Janssen, R. Sánchez
name: Tolstoy, E.
name: Venn, K.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The Pristine survey is a narrow-band, photometric survey focused around the wavelength region of the Ca II H & K absorption lines, designed to efficiently search for extremely metal-poor stars. In this work, we use the first results of a medium-resolution spectroscopic follow-up to refine the selection criteria for finding extremely metal-poor stars ($\textrm{[Fe/H]} \leq -3.0$) in the Pristine survey. We consider methods by which stars can be selected from available broad-band and infrared photometry plus the additional Pristine narrow-band photometry. The spectroscopic sample presented in this paper consists of 205 stars in the magnitude range $14 < V < 18$. Applying the photometric selection criteria cuts the sample down to 149 stars, and from these we report a success rate of 70% for finding stars with $\textrm{[Fe/H]} \leq -2.5$ and 22% for finding stars with $\textrm{[Fe/H]} \leq -3.0$. These statistics compare favourably with other surveys that search for extremely metal-poor stars, namely an improvement by a factor of $\sim 4-5$ for recovering stars with $\textrm{[Fe/H]} \leq -3.0$. In addition, Pristine covers a fainter magnitude range than its predecessors, and can thus probe deeper into the Galactic halo.
description: 14 pages, 6 figures, 4 tables, full version of Table 1 available on-line only, accepted for publication in MNRAS
Improvements to ATLAS primary vertexing reconstruction for LHC Run 3
Creators: name: Lee, Graham
name: Cairo, Valentina
name: Casper, Dave
name: Pettersson, Nora Emilia
name: Danninger, Matthias
Publisher: name: Zenodo
Year: 2019

description: The increasing track multiplicity in ATLAS poses new challenges for primary vertex reconstruction software, where it is expected to reach over 70 inelastic proton-proton collisions per beam crossing during Run-2 of the LHC and even more extreme vertex density in the next upcoming Runs. In order to address these challenges, two new tools were adapted. The first is the Gaussian track density seed finder, a simple yet powerful analytic model of the track density along the beam axis in order to locate candidate vertices The second is the Adaptive Multi Vertex Finder, a global approach to vertex finding and fitting, which deploys the same adaptive vertex fitting technique as the Iterative Vertex Finder algorithm used in Run-2. This allows vertices to compete for nearby tracks in parallel, in order to take into account the vertex structure of the event. This talk summarises the optimization and expected performance of the Adaptive Multi Vertex Finder algorithm and software, for conditions foreseen for Run-3 of the LHC. These studies are coupled to a newly optimised vertexing seeder algorithm and further performance studies in the ITk scenario.
General linear-optical quantum state generation scheme: Applications to maximally path-entangled states
Creators: name: VanMeter, N. M.
name: Lougovski, P.
name: Uskov, D. B.
name: Kieling, K.
name: Eisert, J.
name: Dowling, Jonathan P.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We introduce schemes for linear-optical quantum state generation. A quantum state generator is a device that prepares a desired quantum state using product inputs from photon sources, linear-optical networks, and postselection using photon counters. We show that this device can be concisely described in terms of polynomial equations and unitary constraints. We illustrate the power of this language by applying the Grobner-basis technique along with the notion of vacuum extensions to solve the problem of how to construct a quantum state generator analytically for any desired state, and use methods of convex optimization to identify bounds to success probabilities. In particular, we disprove a conjecture concerning the preparation of the maximally path-entangled |n,0)+|0,n) (NOON) state by providing a counterexample using these methods, and we derive a new upper bound on the resources required for NOON-state generation.
description: 5 pages, 2 figures
Installing and administrating the ATLAS Metadata Interface (AMI) ecosystem
Creators: name: Odier, Jerome
name: Fulachier, Jerome Henri
name: Lambert, Fabian
Publisher: name: Zenodo
Year: 2019

description: ATLAS Metadata Interface (AMI) is a generic ecosystem for metadata aggregation, transformation and cataloging. Benefiting from about 20 years of feedback in the LHC context, the second major version was released in 2018. This poster describes how to install and administrate AMI version 2. A particular focus is given to the registration of existing databases in AMI, the adding of additional metadata and the generation of high level HTML 5 search interfaces using a dedicated wizard. Finally, this poster shows how to extend AMI by writing server-side Java commands, tasks and client-side HTML 5 applications.
Faecal contamination and foraging behaviour from Parasite insight: assessing fitness costs, infection risks and foraging benefits relating to gastrointestinal nematodes in wild mammalian herbivores
Creators: name: Coulson, Graeme
name: Cripps, Jemma K.
name: Garnick, Sarah
name: Bristow, Verity
name: Beveridge, Ian
Publisher: name: The Royal Society
Year: 2018
Subjects: subject: Ecology
subject: FOS: Biological sciences
subject: Health Care
subject: Diseases
subject: 111706 Epidemiology
subject: FOS: Health sciences
subject: 60801 Animal Behaviour

description: The influence of faecal contamination on foraging behaviour in free-ranging eastern grey kangaroos (Macropus giganteus)
The Finite Temperature Phase Transition in the Lattice SU(2)-Higgs Model
Creators: name: Farakos, K.
name: Kajantie, K.
name: Rummukainen, K.
name: Shaposhnikov, M.
Publisher: name: arXiv
Year: 1993
Subjects: subject: High Energy Physics - Lattice (hep-lat)
subject: FOS: Physical sciences

description: We study the finite temperature transition of SU(2)-Higgs model with lattice Monte Carlo techniques. We use dimensional reduction to transform the original 4-dimensional SU(2)-gauge + fundamental Higgs theory to an effective 3-dimensional SU(2) + adjoint Higgs + fundamental Higgs model. The simulations were performed with Higgs masses of 35 and 80 GeV; in both cases we observe a stronger first order transition than the perturbation theory predicts, indicating that the dynamics of the transition strongly depend on non-perturbative effects.
description: 3 pages postscript, contribution to the Lattice 93-conference, Dallas, USA, October 1993, preprint IUHET-266