cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
3. Designing a Base Funding to Support the Research Workforce
Creators: name: , Baisden
Publisher: name: Zenodo
Year: 2022
Subjects: Science Policy
Aotearoa New Zealand
Research Funding

description: Previous briefs addressing Te Ara Paerangi Future Pathways Green Paper evolve from awareness that the pandemic has raised serious concerns about the sustainability of today’s research institutions and funding systems. Aotearoa’s highly contestable funding raises concerns that our system may be among the most unstable internationally and prone to the problems observed in increasingly hypercompetitive research systems worldwide. Hypercompetition is associated with poor behaviours and mediocrity, undermines diversity, equity and inclusion (DEI), and reduces the likelihood of funding innovative projects and careers. How can we build more collaborative, connected careers within research systems appropriate for taking society on innovative journeys to solve the biggest challenges such as climate change and protecting endangered biodiversity? This paper and previous work describes analysis to arrive at design suggestions for an innovative base funding proposal that better achieves the historical intentions to meet national research needs that have evolved considerably over 30 years. The proposed system would reallocate existing and possibly additional government funding to support 30–50% of researchers’ salaries and related costs. The intent is to enhance the overall well being of the research workforce and knowledge systems by creating or incentivising a number of features that overcome current dilemmas, improving the responsiveness, connectivity and use of research within Aotearoa New Zealand, though self-organisation following Ostrom’s principles of common resource pool allocation. The proposed scheme has advantages over the current highly contestable system, and is expected to outperform tenure-driven systems.
Schnell-Griot & Co
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1820

description: Ort: Triest
description: Verzeichnung=Description=Inventaire 05.07.2020 Automatisiert nach HAN-Import
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Schönauer, J. G
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1820

description: Ort: Nürnberg
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Particle-number conservation in static-path approximation for thermal superfluid systems
Creators: name: Kaneko, K.
name: Schiller, A.
Publisher: name: arXiv
Year: 2007
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: By applying particle-number projection to the static-path approximation (SPA), the heat capacity and the breakdown of pairing correlations are investigated in the thermally excited, superfluid systems 172Yb, 94Mo, and 56Fe. For the heavy nucleus 172Yb, the heat capacities in both the SPA and the number-projected SPA (NPSPA) exhibit an S shape; the difference between the SPA and NPSPA heat-capacity curves is not very large and the particle-number projection thereby enhances the S shape already seen in the SPA. The temperature at which the S-shape of heat capacity curve occurs parallels the temperature of the breakdown of pairing correlations as indicated by the effective pairing gap. However, for the comparatively lighter nuclei 94Mo and 56Fe, the SPA does not produce an S-shaped heat capacity on its own; only after particle-number projection the S shape appears in the heat-capacity curve. For 94Mo, we compare the NPSPA result with thermal odd-even mass differences, which are regarded as a direct measure of the pairing gap.
description: 7 pages, 5 figures, accepted for publication in Phys. Rev. C
Sharp bounds for higher linear syzygies and classifications of projective varieties
Creators: name: Han, Kangjin
name: Kwak, Sijong
Publisher: name: arXiv
Year: 2013
Subjects: subject: Algebraic Geometry (math.AG)
subject: Commutative Algebra (math.AC)
subject: FOS: Mathematics
subject: Primary 14N05, 13D02, 14N25, Secondary 51N35

description: In the present paper, we consider upper bounds of higher linear syzygies i.e. graded Betti numbers in the first linear strand of the minimal free resolutions of projective varieties in arbitrary characteristic. For this purpose, we first remind `Partial Elimination Ideals (PEIs)' theory and introduce a new framework in which one can study the syzygies of embedded projective schemes well using PEIs theory and the reduction method via inner projections. Next we establish fundamental inequalities which govern the relations between the graded Betti numbers in the first linear strand of an algebraic set $X$ and those of its inner projection $X_q$. Using these results, we obtain some natural sharp upper bounds for higher linear syzygies of any nondegenerate projective variety in terms of the codimension with respect to its own embedding and classify what the extremal case and next-to-extremal case are. This is a generalization of Castelnuovo and Fano's results on the number of quadrics containing a given variety and another characterization of varieties of minimal degree and del Pezzo varieties from the viewpoint of `syzygies'. Note that our method could be also applied to get similar results for more general categories (e.g. connected in codimension one algebraic sets).
description: 22 pages, 7 figures, comments are welcomed
Schmidt, J. B
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1820

description: Ort: Triest
description: Verzeichnung=Description=Inventaire 05.07.2020 Automatisiert nach HAN-Import
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Vector leptoquark mass limits and branching ratios of $ K_L^0, B^0, B_s \to l^+_i l^-_j $ decays with account of fermion mixing in leptoquark currents
Creators: name: Smirnov, A. D.
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: The contributions of the vector leptoquarks of Pati-Salam type to the branching ratios of $K_L^0, B^0, B_s \to l \, l^{\prime}$ decays are calculated with account of the fermion mixing in the leptoguark currents of the general type. Using the general parametrizations of the mixing matrices the lower vector leptoquark mass limit $ m_V > 86 \,\, TeV $ is found from the current experimental data on these decays. The branching ratios of the decays $B^0, B_s \to l \, l^{\prime}$ predicted at $m_V = 86 \,\, TeV$ are calculated. These branching ratios for the decays $ B^0, B_s \to μ^+ μ^-, e μ$ are close to the experimental data whereas those for the decays $B^0 \to e^+ e^-, e τ, μτ$, and $B_s \to e^+ e^-$ are by order of $2\div4$ less than their current experimental limits. For the decays $B_s \to e τ, μτ$ these branching ratios are of order $10^{-10}$ and $10^{-9}$ respectively. The predicted branching ratios will be usefull in the current and future experimental searches for these decays.
description: 10 pages, 1 table, minor corrections, final version for publication in Modern Physics Letters A
Mez, Gebrüder
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1820

description: Ort: Freiburg i. Br.
description: Verzeichnung=Description=Inventaire 05.07.2020 Automatisiert nach HAN-Import
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title: Design Verification of Afsluitdijk Renovation with Large Scale Tests
Creators: name: Klein Breteler, Mark
name: Ockeloen, Wouter
name: Boerma, Emiel
name: Kuiper, Coen
Publisher: name: Bundesanstalt für Wasserbau
Year: 2019

description: Presented at: Coastal Structures Conference 2019, Hannover, Germany, September 30th – October 2nd, 2019
Another Look at the Ho-Lee Bond Option Pricing Model
Creators: name: Kim, Young Shin
name: Stoyanov, Stoyan
name: Rachev, Svetlozar
name: Fabozzi, Frank J.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Mathematical Finance (q-fin.MF)
subject: FOS: Economics and business

description: In this paper, we extend the classical Ho-Lee binomial term structure model to the case of time-dependent parameters and, as a result, resolve a drawback associated with the model. This is achieved with the introduction of a more flexible no-arbitrage condition in contrast to the one assumed in the Ho-Lee model.
Merger of black hole and neutron star in general relativity: Tidal disruption, torus mass, and gravitational waves
Creators: name: Shibata, Masaru
name: Taniguchi, Keisuke
Publisher: name: arXiv
Year: 2007
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We systematically perform the merger simulation of black hole-neutron star (BH-NS) binaries in full general relativity, focusing on the case that the NS is tidally disrupted. We prepare BH-NS binaries in a quasicircular orbit as the initial condition in which the BH is modeled by a nonspinning moving puncture. For modeling the NS, we adopt the $Γ$-law equation of state with $Γ=2$ and the irrotational velocity field. We change the BH mass in the range $M_{\rm BH} \approx 3.3$--$4.6M_{\odot}$, while the rest mass of the NS is fixed to be $M_{*}=1.4 M_{\odot}$ (i.e., the NS mass $M_{\rm NS} \approx 1.3M_{\odot}$). The radius of the corresponding spherical NS is set in the range $R_{\rm NS} \approx 12$--15 km (i.e., the compactness $GM_{\rm NS}/R_{\rm NS}c^2 \approx 0.13$--0.16). We find for all the chosen initial conditions that the NS is tidally disrupted near the innermost stable circular orbit. For the model of $R_{\rm NS}=12$ km, more than 97 % of the rest mass is quickly swallowed into the BH and the resultant torus mass surrounding the BH is less than $0.04M_{\odot}$. For the model of $R_{\rm NS} \approx 14.7$ km, by contrast, the torus mass is about $0.16M_{\odot}$ for the BH mass $\approx 4M_{\odot}$. The thermal energy of the material in the torus increases by the shock heating occurred in the collision between the spiral arms, resulting in the temperature $10^{10}$--$10^{11}$ K. (.. omission ..) We also present gravitational waveforms during the inspiral, tidal disruption of the NS, and subsequent evolution of the disrupted material. (.. omission ..)
description: 20 pages
Schultze & Co
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1820

description: Ort: Frankfurt a. M.
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Schulthess, Caspar, & Co
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1820

description: Ort: Zürich
description: Verzeichnung=Description=Inventaire 05.07.2020 Automatisiert nach HAN-Import
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Width-Dependent Band Gap in Armchair Graphene Nanoribbons Reveals Fermi Level Pinning on Au(111)
Creators: name: Merino-Díez, Néstor
name: Garcia-Lekue, Aran
name: Carbonell-Sanromà, Eduard
name: Li, Jingcheng
name: Corso, Martina
name: Colazzo, Luciano
name: Sedona, Francesco
name: Sánchez-Portal, Daniel
name: Pascual, Jose I.
name: de Oteyza, Dimas G.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We report on the energy level alignment evolution of valence and conduction bands of armchair-oriented graphene nanoribbons (aGNR) as their band gap shrinks with increasing width. We use 4,4-dibromo-para-terphenyl as molecular precursor on Au(111) to form extended poly-para-phenylene nanowires, which can be fused sideways to form atomically precise aGNRs of varying widths. We measure the frontier bands by means of scanning tunneling spectroscopy, corroborating that the nanoribbons band gap is inversely proportional to their width. Interestingly, valence bands are found to show Fermi level pinning as the band gap decreases below a threshold value around 1.7 eV. Such behavior is of critical importance to understand the properties of potential contacts in graphene nanoribbon-based devices. Our measurements further reveal a particularly interesting system for studying Fermi level pinning by modifying an adsorbates band gap while maintaining an almost unchanged interface chemistry defined by substrate and adsorbate.
Throughput Maximization in Wireless Powered Communication Networks
Creators: name: Ju, Hyunsgsik
name: Zhang, Rui
Publisher: name: arXiv
Year: 2013
Subjects: subject: Information Theory (cs.IT)
subject: FOS: Computer and information sciences

description: This paper studies the newly emerging wireless powered communication network (WPCN) in which one hybrid access point (H-AP) with constant power supply coordinates the wireless energy/information transmissions to/from distributed users that do not have energy sources. A "harvest-then-transmit" protocol is proposed where all users first harvest the wireless energy broadcast by the H-AP in the downlink (DL) and then send their independent information to the H-AP in the uplink (UL) by time-division-multiple-access (TDMA). First, we study the sum-throughput maximization of all users by jointly optimizing the time allocation for the DL wireless power transfer versus the users' UL information transmissions given a total time constraint based on the users' DL and UL channels as well as their average harvested energy values. By applying convex optimization techniques, we obtain the closed-form expressions for the optimal time allocations to maximize the sum-throughput. Our solution reveals "doubly near-far" phenomenon due to both the DL and UL distance-dependent signal attenuation, where a far user from the H-AP, which receives less wireless energy than a nearer user in the DL, has to transmit with more power in the UL for reliable information transmission. Consequently, the maximum sum-throughput is achieved by allocating substantially more time to the near users than the far users, thus resulting in unfair rate allocation among different users. To overcome this problem, we furthermore propose a new performance metric so-called common-throughput with the additional constraint that all users should be allocated with an equal rate regardless of their distances to the H-AP. We present an efficient algorithm to solve the common-throughput maximization problem. Simulation results demonstrate the effectiveness of the common-throughput approach for solving the new doubly near-far problem in WPCNs.
description: 26 pages, 12 figures
Schwartz-Carlins, Notaire
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1820

description: Ort: Huningue
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Schmid, J. J., I.U.L
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1820

description: Ort: Basel
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Testing a new luminosity/redshift indicator for $γ$-ray bursts
Creators: name: Zhang, Zhi-Bin
name: Xie, Guang-Zhong
Publisher: name: arXiv
Year: 2007
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have tested a relative spectral lag (RSL) method suggested earlier as a luminosity/redshift (or distance) estimator, using the generalized method by Schaefer & Collazzi. We find the derivations from the luminosity/redshift-RSL (L/R-RSL) relation are comparable with the corresponding observations. Applying the luminosity-RSL relation to two different GRB samples, we find that there exist no violators from the generalized test, namely the Nakar & Piran test and Li test. We also find that about 36 per cent of Schaefer's sample are outliers for the L/R-RSL relation within 1$σ$ confidence level, but no violators at 3$σ$ level within the current precision of L/R-RSL relation. An analysis of several potential outliers for other luminosity relations shows they can match the L/R-RSL relation well within an acceptable uncertainty. All the coincident results seem to suggest that this relation could be a potential tool for cosmological study.
description: 7 pages, 6 figures and 1 table; Comments are welcome
Schlatter & Schnell
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1820

description: Ort: Lindau
description: Verzeichnung=Description=Inventaire 05.07.2020 Automatisiert nach HAN-Import
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Relativistic jet feedback II: Relationship to gigahertz peak spectrum and compact steep spectrum radio galaxies
Creators: name: Bicknell, Geoffrey V.
name: Mukherjee, Dipanjan
name: Wagner, Alexander Y.
name: Sutherland, Ralph S.
name: Nesvadba, Nicole P. H.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We propose that Gigahertz Peak Spectrum (GPS) and Compact Steep Spectrum (CSS) radio sources are the signposts of relativistic jet feedback in evolving galaxies. Our simulations of relativistic jets interacting with a warm, inhomogeneous medium, utilize cloud densities and velocity dispersions in the range derived from optical observations, show that free-free absorption can account for the $\sim \rm GHz$ peak frequencies and low frequency power laws inferred from the radio observations. These new computational models replace the power-law model for the free-free optical depth in the \citep{bicknell97a} model by a more fundamental model involving disrupted log-normal distributions of warm gas. One feature of our new models is that at early stages, the low frequency spectrum is steep but progressively flattens as a result of a broader distribution of optical depths, suggesting that the steep low frequency spectra discovered by \citet{callingham17a} may possibly be attributed to young sources. We also investigate the inverse correlation between peak frequency and size and find that the initial location on this correlation is determined by the average density of the warm ISM. The simulated sources track this correlation initially but eventually fall below it, indicating the need for a more extended ISM than presently modelled. GPS and CSS sources can potentially provide new insights into the phenomenon of AGN feedback since their peak frequencies and spectra are indicative of the density, turbulent structure and distribution of gas in the host galaxy.
description: Accepted for publication in Monthly Notices of the Royal Astronomical Society
Growth of Primitive Elements in Free Groups
Creators: name: Puder, Doron
name: Wu, Conan
Publisher: name: arXiv
Year: 2013
Subjects: subject: Group Theory (math.GR)
subject: Combinatorics (math.CO)
subject: FOS: Mathematics
subject: 20E05 (Primary) 05A16 (Secondary)

description: In the free group $F_k$, an element is said to be primitive if it belongs to a free generating set. In this paper, we describe what a generic primitive element looks like. We prove that up to conjugation, a random primitive word of length $N$ contains one of the letters exactly once asymptotically almost surely (as $N \to \infty$). This also solves a question from the list `Open problems in combinatorial group theory' [Baumslag-Myasnikov-Shpilrain 02']. Let $p_{k,N}$ be the number of primitive words of length $N$ in $F_k$. We show that for $k \ge 3$, the exponential growth rate of $p_{k,N}$ is $2k-3$. Our proof also works for giving the exact growth rate of the larger class of elements belonging to a proper free factor.
description: 20 pages, 2 figures. A few minor improvements of the introduction of ideas
Vassal, R., & Comp
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1820

description: Ort: Le Hâvre
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Poisson brackets in Hydrodynamics
Creators: name: Kolev, Boris
Publisher: name: arXiv
Year: 2007
Subjects: subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences
subject: 53D20 53D17 37K05 37K65

description: This paper investigates different Poisson structures that have been proposed to give a Hamiltonian formulation to evolution equations issued from fluid mechanics. Our aim is to explore the main brackets which have been proposed and to discuss the difficulties which arise when one tries to give a rigorous meaning to these brackets. Our main interest is in the definition of a valid and usable bracket to study rotational fluid flows with a free boundary. We discuss some results which have emerged in the literature to solve some of the difficulties that arise. It appears to the author that the main problems are still open.
Nonrelativistic hydrodynamics from quantum field theory: (I) Normal fluid composed of spinless Schrödinger fields
Creators: name: Hongo, Masaru
Publisher: name: arXiv
Year: 2018
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We provide a complete derivation of hydrodynamic equations for nonrelativistic systems based on quantum field theories of spinless Schrödeinger fields, assuming that an initial density operator takes a special form of the local Gibbs distribution. The constructed optimized/renormalized perturbation theory for real-time evolution enables us to separately evaluate dissipative and nondissipative parts of constitutive relations. It is shown that the path-integral formula for local thermal equilibrium together with the symmetry properties of the resulting action---the nonrelativistic diffeomorphism and gauge symmetry in the thermally emergent Newton-Cartan geometry---provides a systematic way to derive the nondissipative part of constitutive relations. We further show that dissipative parts are accompanied with the entropy production operator together with two kinds of fluctuation theorems by the use of which we derive the dissipative part of constitutive relations and the second law of thermodynamics. After obtaining the exact expression for constitutive relations, we perform the derivative expansion and derive the first-order hydrodynamic (Navier-Stokes) equation with the Green-Kubo formula for transport coefficients.
description: 36 pages, 4 figures
Simultaneous multiwavelength observations of V404 Cygni during its 2015 June outburst decay strengthen the case for an extremely energetic jet-base
Creators: name: Maitra, Dipankar
name: Scarpaci, John F.
name: Grinberg, Victoria
name: Reynolds, Mark T.
name: Markoff, Sera
name: Maccarone, Thomas J.
name: Hynes, Robert I.
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We present results of multiband optical photometry of the black hole X-ray binary system V404 Cygni obtained using Wheaton College Observatory's 0.3m telescope, along with strictly simultaneous INTEGRAL and Swift observations during 2015 June 25.15--26.33 UT, and 2015 June 27.10--27.34 UT. These observations were made during the 2015 June outburst of the source when it was going through an epoch of violent activity in all wavelengths ranging from radio to $γ$-rays. The multiwavelength variability timescale favors a compact emission region, most likely originating in a jet outflow, for both observing epochs presented in this work. The simultaneous INTEGRAL/Imager on Board the Integral Satellite (IBIS) 20--40 keV light curve obtained during the June 27 observing run correlates very strongly with the optical light curve, with no detectable delay between the optical bands as well as between the optical and hard X-rays. The average slope of the dereddened spectral energy distribution was roughly flat between the $I_C$- and $V$-bands during the June 27 run, even though the optical and X-ray flux varied by $>$25$\times$ during the run, ruling out an irradiation origin for the optical and suggesting that the optically thick to optically thin jet synchrotron break during the observations was at a frequency larger than that of $V$-band, which is quite extreme for X-ray binaries. These observations suggest that the optical emission originated very close to the base of the jet. A strong H$α$ emission line, probably originating in a quasi-spherical nebula around the source, also contributes significantly in the $R_C$-band. Our data, in conjunction with contemporaneous data at other wavelengths presented by other groups, strongly suggest that the jet-base was extremely compact and energetic during this phase of the outburst.
description: 15 pages, 2 tables, 5 figures. Accepted for publication in ApJ
Usteri-von Muralt, J. M
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1820

description: Ort: Zürich
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How to switch on and off a Gamma-ray burst through a magnetar
Creators: name: Bernardini, M. G.
name: Campana, S.
name: Ghisellini, G.
name: D'Avanzo, P.
name: Burlon, D.
name: Covino, S.
name: Ghirlanda, G.
name: Melandri, A.
name: Salvaterra, R.
name: Vergani, S. D.
name: D'Elia, V.
name: Fugazza, D.
name: Sbarufatti, B.
name: Tagliaferri, G.
Publisher: name: arXiv
Year: 2013
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: One of the most elusive features of Gamma Ray Bursts (GRBs) is the sporadic emission prior to the main prompt event observed in at least $\sim 15\%$ of cases. These precursors have spectral and temporal properties similar to the main prompt emission, and smaller, but comparable, energetics. They are separated from the main event by a quiescent time that may be extremely long and, in some cases, more than one precursor has been observed in the same burst. Precursors are still a puzzle: despite many attempts none of the proposed models can account for all the observed features. Based on the complete sample of bright long GRBs observed by Swift (BAT6), we propose a new scenario for which precursors are explained by assuming that the central GRB engine is a newly born magnetar. In this model the precursor and the prompt emission arise from accretion of matter onto the surface of the magnetar. The accretion process can be halted by the centrifugal drag exerted by the rotating magnetosphere onto the in-falling matter, allowing for multiple precursors and very long quiescent times.
description: 10 pages, 4 figures, 3 tables
Vischer & Sohn
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1820

description: Ort: Basel
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The Impact of Rotation on the Evolution of Low-Mass Stars
Creators: name: Brown, D.
name: Salaris, M.
Publisher: name: arXiv
Year: 2007
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: High precision photometry and spectroscopy of low-mass stars reveal a variety of properties standard stellar evolution cannot predict. Rotation, an essential ingredient of stellar evolution, is a step towards resolving the discrepancy between model predictions and observations. The first rotating stellar model, continuously tracing a low-mass star from the pre-main sequence onto the horizontal branch, is presented. The predicted luminosity functions of globular clusters and surface rotation velocities on the horizontal branch are discussed.
description: 5 pages, 6 figures, to be published in the Proceedings of the Conference 'Unsolved Problems in Stellar Physics', Cambridge, 2-6 July 2007
title: ADCO, Cartulaire de Cîteaux pour les possessions d’Izeure (XVe siècle), Cart. 178 (11 H 80), 82 folios, f. 0035
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
name: Petot, Frédéric
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire

description: Cartulaire de Cîteaux pour les possessions d’Izeure (XVe siècle), Archives départementales de la Côte-d'Or, Cart. 178 (11 H 80), 82 folios, f. 0035, 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. 178 (11 H 80), 82 folios, f. 0035, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
Schaezler, Joh. Lorenz
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1820

description: Ort: Augsburg
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On the radion mediation of the Supersymmetry breaking in N=2, D=5 Supergravity Orbifolds
Creators: name: Diamandis, G. A.
name: Georgalas, B. C.
name: Kouroumalou, P.
name: Lahanas, A. B.
Publisher: name: arXiv
Year: 2007
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We discuss the on-shell N=1 Supersymmetric coupling of brane chiral multiplets in the context of N=2, D=5 Supergravity compactified on $S_1/Z_2$ orbifolds. Assuming a constant superpotential on the hidden brane we study the transmission of the supersymmetry breaking to the visible brane. We find that to lowest order in the five dimensional Newton's constant $k_5^2$ and gravitino mass $m_{3/2}^2$ the spinor field of the radion multiplet is responsible of inducing positive one-loop squared masses $m_ϕ^2 \sim {m_{3/2}^2} / (M_{Planck}^2 R^2)$ to the scalar fields which are localized on the visible brane with $R$ the length scale of the fifth dimension. Considering a cubic superpotential on the visible brane we also find that non-vanishing soft trilinear scalar couplings $A$ are induced given by $A=3m_ϕ^2/m_{3/2}$.
description: 14 pages, 2 figures, version to appear in Physics Letters B
Corrective Re-gridding Techniques for Non-Uniform Sampling in Time Domain Terahertz Spectroscopy
Creators: name: Potts, A. M.
name: Mai, T. T.
name: Warren, M. T.
name: Aguilar, R. Valdés
Publisher: name: arXiv
Year: 2017
Subjects: subject: Optics (physics.optics)
subject: Other Condensed Matter (cond-mat.other)
subject: FOS: Physical sciences

description: Time domain terahertz spectroscopy typically uses mechanical delay stages that inherently suffer from non-uniform sampling positions. We review, simulate, and experimentally test the ability of corrective cubic spline and Shannon re-gridding algorithms to mitigate the inherent sampling position noise. We present simulations and experimental results that show re-gridding algorithms can increase the signal to noise ratio within the frequency range of 100 GHz to 2 THz. We also predict that re-gridding corrections will become increasingly important to both spectroscopy and imaging as THz technology continues to improve and higher frequencies become experimentally accessible.
description: 10 pages, 3 figures
Shock waves from heavy-quark mesons in AdS/CFT
Creators: name: Gubser, Steven S.
name: Pufu, Silviu S.
name: Yarom, Amos
Publisher: name: arXiv
Year: 2007
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We calculate the far-field stress-energy tensor of a quark gluon plasma due to a heavy-quark meson moving through it, using a semi-classical description in string theory of the meson as a string hanging into anti-de Sitter space. We find that these mesons create a shock wave but no diffusion wake, in contrast to single heavy quarks described via a trailing string, where the diffusion wake is strong. If thermal QCD responds similarly to heavy quarks and heavy quarkonia, the presence or suppression of the diffusion wake constitutes a prediction which can in principle be checked in heavy-ion collisions.
description: 22 pages
The Wolf Within
Creators: name: Iliano  Cervesato
Publisher: name: Carnegie Mellon University
Year: 1985
Subjects: subject: 89999 Information and Computing Sciences not elsewhere classified
subject: FOS: Computer and information sciences

description: A formal specification of a security protocol cannot be limited to listing the messages exchanged. In MSR, each construct is associated with typing and data access specification (DAS) rules, which describe under which circumstances a principal can access keys and other information. A protocol specification is completed with a description of the intruder in the style of Dolev and Yao, the wolf in the protocol world. In this paper, we show that the protocol determines the intruder: the wolf is deep within. More precisely we show that the Dolev-Yao intruder rules can be automatically reconstructed from the DAS rules, and that the DAS rules can themselves be inferred from annotated typing declarations for the various message constructors.
Mean Occupation Function of High Redshift Quasars from the Planck Cluster Catalog
Creators: name: Chakraborty, Priyanka
name: Chatterjee, Suchetana
name: Dutta, Alankar
name: Myers, Adam D.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We characterise the distribution of quasars within dark matter halos using a direct measurement technique for the first time at redshifts as high as $z \sim 1$. Using the Planck Sunyaev-Zeldovich (SZ) catalogue for galaxy groups and the Sloan Digital Sky Survey (SDSS) DR12 quasar dataset, we assign host clusters/groups to the quasars and make a measurement of the mean number of quasars within dark matter halos as a function of halo mass. We find that a simple power-law fit of $\log\left = (2.11 \pm 0.01) \log (M) -(32.77 \pm 0.11)$ can be used to model the quasar fraction in dark matter halos. This suggests that the quasar fraction increases monotonically as a function of halo mass even to redshifts as high as $z\sim 1$.
description: Accepted for publication in PASP
Charmless 3-body B Decays: Resonant and Nonresonant Contributions
Creators: name: Cheng, Hai-Yang
Publisher: name: arXiv
Year: 2007
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: Charmless 3-body decays of $B$ mesons are studied using a simple model based on the framework of the factorization approach. We have identified a large source of the nonresonant signal in the matrix elements of scalar densities, e.g. $$. This explains the dominance of the nonresonant background in $B\to KKK$ decays, the sizable nonresonant fraction of order $(35\sim 40)%$ in $K^-π^+π^-$ and $\bar K^0π^+π^-$ modes and the smallness of nonresonant rates in $B\to πππ$ decays. We have computed the resonant and nonresonant contributions to charmless 3-body decays and determined the rates for the quasi-two-body decays $B\to VP$ and $B\to SP$. Time-dependent CP asymmetries $\sin2β_{\rm eff}$ and $A_{CP}$ in $K^+K^-K_S,K_SK_SK_S,K_Sπ^+π^-$ and $K_Sπ^0π^0$ modes are estimated.
description: 8 pages, talk presented at 4th International Conference on Flavor Physics (ICFP 2007), Beijing, China, Sept 24-28, 2007; add references and the new BaBar measurement of B^0 to K^+ pi^- pi^0
Scherer & Finguerlin
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1820

description: Ort: Paris
description: Verzeichnung=Description=Inventaire 05.07.2020 Automatisiert nach HAN-Import
description: Verzeichnung=Description=Inventaire ISAD(G) / HAN Katalogisierungsregeln für Archivbestände Detailliert
The Use of MMR and Diversity-Based Reranking in Document Reranking and Summarization
Creators: name: Carbonell, Jaime G.
name: Goldstein, Jade
Publisher: name: Carnegie Mellon University
Year: 1997
Subjects: subject: 89999 Information and Computing Sciences not elsewhere classified
subject: FOS: Computer and information sciences

description: This paper presents a method for combining query-relevance with information-novelty in the context of text retrieval and summarization. The Maximal Marginal Relevance (MMR) criterion strives to reduce redundancy while maintaining query relevance in re-ranking retrieved documents and in selecting appropriate passages for text summarization. Preliminary results indicate some benefits for MMR diversity ranking in document retrieval and in single document summarization. The latter are borne out by the recent results of the SUMMAC conference in the evaluation of summarization systems. However, the clearest advantage is demonstrated in constructing non-redundant multi-document summaries, where MMR results are clearly superior to non-MMR passage selection.
Nivel de contaminación de residuos textiles en el municipio de La Plata Huila, 2023_1
Creators: name: Sanza Chavaco, Britney Vanessa
name: Cáceres Ramírez, Dayana
Publisher: name: Zenodo, Curso Seminario de Investigación. Universidad Surcolombiana, La Plata
Year: 2023
Subjects: Contaminación ambiental
Contaduría ambiental
Industria textil

description: Estudiante de cuarto semestre del programa de Contaduría Pública, en la sede La Plata, de la Universidad Surcolombiana 2023_2.

El sector textil ha sido nombrado como una de las actividades más antiguas e influyentes en el desarrollo industrial, esto se ha desarrollado significativamente en todo el mundo debido a contribuciones significativas al empleo, la modernización, la tecnología y la economía en general; la industria textil es una industria compleja porque depende de múltiples industrias, como la agricultura, la química y demás procesos para la fabricación de una prenda de vestir, sin embargo, los distribuidores, agentes de suministro y corredores del sector textil promueven las compras y ventas de dichos productos, basándose que desde el año 2000, las industrias de la moda de todo el mundo han duplicado las ventas, siendo  influenciadas por el fenómeno de la moda rápida, esto se refiere a la ropa hecha para imitar la pasarela y las tendencias de la marca de lujo, el propósito de la moda rápida se da “gracias a la fabricación barata, el consumo rápido y frecuente de prendas de corta duración” según (Juezas, M, 2022,Pag. 42); es decir que debe venderse en un período de tiempo muy corto y a un precio muy económico, lo cual suele ser muy atractivo para los consumidores, porque pueden actualizar constantemente el armario a un precio muy asequible y siempre llevar las últimas tendencias de moda, lo cual genera un consumismo constante entre la población; sin darnos cuenta de la contaminación para el entorno ambiental y social que se presenta al generar cierta cantidad de residuos textiles.
title: Effect of Venting Holes to Relieve Wave Impact Pressures on Flood Gates with Overhangs
Creators: name: Hofland, Bas
name: Passos, Marlon
name: de Almeida, Ermano
Publisher: name: Bundesanstalt für Wasserbau
Year: 2019

description: Presented at: Coastal Structures Conference 2019, Hannover, Germany, September 30th – October 2nd, 2019
Effects of exciton-plasmon strong coupling on third harmonic generation of WS2 monolayer at periodic plasmonic interfaces
Creators: name: Sukharev, Maxim
name: Pachter, Ruth
Publisher: name: arXiv
Year: 2017
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: We study theoretically optical response of WS2 monolayer located near periodic metal nanostructured arrays in two and three dimensions. The emphasis of simulations is on the strong coupling regime of excitons supported by WS2 and surface plasmon-polaritons supported by various periodic plasmonic interfaces. It is demonstrated that a monolayer of WS2 placed in a close proximity of periodic arrays of either slits or holes results in a Rabi splitting of the corresponding surface plasmon-polariton resonance as revealed in calculated transmission and reflection spectra. The nonlinear regime, at which the monolayer of WS2 exhibits the third harmonic generation is studied in details. It is shown that at the strong coupling regime the third harmonic signal is significantly affected by plasmon-polaritons and the symmetry of hybrid exciton-plasmon modes. It is also shown that the local electromagnetic field induced by plasmons is the major contributor to the enhancement of the third harmonic signal in three dimensions. The local electromagnetic fields resulted from the third harmonic generation are greatly localized and highly sensitive to the environment making it a great tool for nano-probes.
Deciding between the Covariance Analytical Approach and the Change-Score Approach in Two Wave Panel Data
Creators: name: Köhler, Carmen
name: Hartig, Johannes
name: Schmid, Christine
Publisher: name: Taylor & Francis
Year: 2020
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Science Policy

description: The manuscript focuses on effects in nonrandomized studies with two outcome measurement occasions and one explanatory variable, and in which groups already differ at the pretest. Such study designs are often encountered in educational and instructional research. Two prominent approaches to estimate effects are (1) covariance analytical approaches and (2) latent change-score models. In current practice, both approaches are applied interchangeably, without a clear rationale for when to use which approach. The aim of this contribution is to outline under which conditions the approaches produce unbiased estimates of the instruction effect. We present a theoretical data generating model in which we decompose the variances of the relevant variables, and examine under which data generating conditions the estimated instruction effect is unbiased. We show that, under specific assumptions, both methods can be used to answer the general question of whether instruction has an effect. Another implication from the results is that practitioners need to consider which underlying data generating assumptions the approaches make, since a violation of those assumptions will lead to biased effects. Based on our results, we give recommendations for preferable research designs.
How would surround vehicles move? A Unified Framework for Maneuver Classification and Motion Prediction
Creators: name: Deo, Nachiket
name: Rangesh, Akshay
name: Trivedi, Mohan M.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Computer Vision and Pattern Recognition (cs.CV)
subject: FOS: Computer and information sciences

description: Reliable prediction of surround vehicle motion is a critical requirement for path planning for autonomous vehicles. In this paper we propose a unified framework for surround vehicle maneuver classification and motion prediction that exploits multiple cues, namely, the estimated motion of vehicles, an understanding of typical motion patterns of freeway traffic and inter-vehicle interaction. We report our results in terms of maneuver classification accuracy and mean and median absolute error of predicted trajectories against the ground truth for real traffic data collected using vehicle mounted sensors on freeways. An ablative analysis is performed to analyze the relative importance of each cue for trajectory prediction. Additionally, an analysis of execution time for the components of the framework is presented. Finally, we present multiple case studies analyzing the outputs of our model for complex traffic scenarios
description: Accepted for publication in IEEE transactions on Intelligent Vehicles
Vassal, R., & Comp
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1820

description: Ort: Paris
description: Verzeichnung=Description=Inventaire 05.07.2020 Automatisiert nach HAN-Import
description: Verzeichnung=Description=Inventaire ISAD(G) / HAN Katalogisierungsregeln für Archivbestände Detailliert
The stable magnetic field of the fullly-convective star V374 Peg
Creators: name: Morin, J.
name: Donati, J. -F.
name: Forveille, T.
name: Delfosse, X.
name: Dobler, W.
name: Petit, P.
name: Jardine, M. M.
name: Cameron, A. C.
name: Albert, L.
name: Manset, N.
name: Dintrans, B.
name: Chabrier, G.
name: Valenti, J. A.
Publisher: name: arXiv
Year: 2007
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report in this paper phase-resolved spectropolarimetric observations of the rapidly-rotating fully-convective M4 dwarf V374 Peg, on which a strong, mainly axisymmetric, large-scale poloidal magnetic field was recently detected. In addition to the original data set secured in 2005 August, we present here new data collected in 2005 September and 2006 August. From the rotational modulation of unpolarised line profiles, we conclude that starspots are present at the surface of the star, but their contrast and fractional coverage are much lower than those of non-fully convective active stars with similar rotation rate. Applying tomographic imaging on each set of circularly polarised profiles separately, we find that the large-scale magnetic topology is remarkably stable on a timescale of 1 yr; repeating the analysis on the complete data set suggests that the magnetic configuration is sheared by very weak differential rotation (about 1/10th of the solar surface shear) and only slightly distorted by intrinsic variability. This result is at odds with various theoretical predictions, suggesting that dynamo fields of fully-convective stars should be mostly non-axisymmetric unless they succeed at triggering significant differential rotation.
description: 12 pages, 11 figures, 1 table. Accepted for publication in MNRAS
The Use of MMR and Diversity-Based Reranking for Reodering Documents and Producing Summaries
Creators: name: Carbonell, Jaime G.
name: Goldstein, Jade
Publisher: name: Carnegie Mellon University
Year: 1981
Subjects: subject: 89999 Information and Computing Sciences not elsewhere classified
subject: FOS: Computer and information sciences

description: This paper presents a method for combining query-relevance with information-novelty in the context of text retrieval and summarization. The Maximal Marginal Relevance (MMR) criterion strives to reduce redundancy while maintaining query relevance in re-ranking retrieved documents and in selecting appropriate passages for text summarization. Preliminary results indicate some benefits for MMR diversity ranking in document retrieval and in single document summarization. The latter are borne out by the recent results of the SUMMAC conference in the evaluation of summarization systems. However, the clearest advantage is demonstrated in constructing non-redundant multi-document summaries, where MMR results are clearly superior to non-MMR passage selection.