cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
The Local Ecology of New Movement Organizations
Creators: name: Knudsen, Brian
Publisher: name: Carnegie Mellon University
Year: 2009
Subjects: subject: Information Systems
subject: FOS: Computer and information sciences
subject: 160510 Public Policy
subject: FOS: Political science

description: Recent scholarship from political science, urban studies, and sociology conceptualizes the city as a space of decentralized democracy – a view emphasizing localization, participation, difference, and anti-hierarchical organizational form. Instead of conceiving the city as a place of atomized individuals and a locale for market exchange, this alternative framework recognizes the city‟s role as “civitas” – a “space of active democratic citizenship” and “full human realization” based on open and free encounter and exchange with difference. The current research emerges from and fills a need within this perspective by examining how local urban contexts undergird and bolster new movement organizations (NMOs). Theory elaborates how urban density, land-use mix, and connectivity generate and enable interaction with the social diversity fundamental to decentralized and anti-hierarchical movements. In addition, theory also examines how urban walking mediates the relationships between these urban contextual traits and NMOs. Linear regression is used to assess the direct effects of density, connectivity, land-use mix, and urban walking on NMO activity (measured as human rights, environmental, and social advocacy groups), and the Sobel and Freedman-Schatzkin tests are employed to assess mediation.
Hidden Magnetism and Quantum Criticality in the Heavy Fermion Superconductor CeRhIn5
Creators: name: Park, Tuson
name: Ronning, F.
name: Yuan, H. Q.
name: Salamon, M. B.
name: Movshovich, R.
name: Sarrao, J. L.
name: Thompson, J. D.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: With understood exceptions, conventional superconductivity does not coexist with long-range magnetic order[1]. In contrast, unconventional superconductivity develops near a boundary separating magnetically ordered and magnetically disordered phases[2,3]. A maximum in the superconducting transition temperature Tc develops where this boundary extrapolates to T=0 K, suggesting that fluctuations associated with this magnetic quantum-critical point are essential for unconventional superconductivity[4,5]. Invariably though, unconventional superconductivity hides the magnetic boundary when T < Tc, preventing proof of a magnetic quantum-critical point[5]. Here we report specific heat measurements of the pressure-tuned unconventional superconductor CeRhIn5 in which we find a line of quantum-phase transitions induced inside the superconducting state by an applied magnetic field. This quantum-critical line separates a phase of coexisting antiferromagnetism and superconductivity from a purely unconventional superconducting phase and terminates at a quantum tetracritical point where the magnetic field completely suppresses superconductivity. The T->0 K magnetic field-pressure phase diagram of CeRhIn5 is well described with a theoretical model[6,7] developed to explain field-induced magnetism in the high-Tc cuprates but in which a clear delineation of quantum-phase boundaries has not been possible. These experiments establish a common relationship among hidden magnetism, quantum criticality and unconventional superconductivity in cuprate and heavy-electron systems, such as CeRhIn5.
description: journal reference added
Additional file 4 of A systematic analysis of natural α-glucosidase inhibitors from flavonoids of Radix scutellariae using ultrafiltration UPLC-TripleTOF-MS/MS and network pharmacology
Creators: name: Wang, Le
name: Tan, Nana
name: Wang, Huan
name: Hu, Jingbo
name: Diwu, Wenbo
name: Wang, Xiaoling
Publisher: name: figshare
Year: 2020
Subjects: subject: Biochemistry
subject: Space Science
subject: Molecular Biology
subject: Pharmacology
subject: Chemical Sciences not elsewhere classified
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Information Systems not elsewhere classified

description: Additional file 4. Information of nodes in the compound-target-pathway (CTP) network.
Dirac Operator Zero-modes on a Torus
Creators: name: Tenjinbayashi, Yasushi
name: Igarashi, Hiroshi
name: Fujiwara, Takanori
Publisher: name: arXiv
Year: 2005
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We study Dirac operator zero-modes on a torus for gauge background with uniform field strengths. Under the basic translations of the torus coordinates the wave functions are subject to twisted periodic conditions. In a suitable torus coordinates the zero-mode wave functions can be related to holomorphic functions of the complex torus coordinates. We construct the zero-mode wave functions that satisfy the twisted periodic conditions. The chirality and the degeneracy of the zero-modes are uniquely determined by the gauge background and are consistent with the index theorem.
description: 28 pages, 2 figures
Reconstruction of the HII Galaxy Hubble Diagram using Gaussian Processes
Creators: name: Yennapureddy, Manoj K.
name: Melia, Fulvio
Publisher: name: arXiv
Year: 2017
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The Hubble diagram constructed using HII galaxies (HIIGx) and Giant extragalactic HII regions (GEHR) as standard candles already extends beyond the current reach of Type Ia SNe. A sample of 156 HIIGx and GEHR sources has been used previously to compare the predictions of LCDM and R_h=ct, the results of which suggested that the HIIGx and GEHR sources strongly favour the latter over the former. But this analysis was based on the application of parametric fits to the data and the use of information criteria, which disfavour the less parsimonious models. In this paper, we advance the use of HII sources as standard candles by utilizing Gaussian processes (GP) to reconstruct the distance modulus representing these data without the need to pre-assume any particular model, none of which may in the end actually be the correct cosmology. In addition, this approach tightly constrains the 1 sigma confidence region of the reconstructed function, thus providing a better tool with which to differentiate between competing cosmologies. With this approach, we show that the Planck concordance model is in tension with the HII data at more than 2.5 sigma, while R_h=ct agrees with the GP reconstruction very well, particularly at redshifts > 10^{-3}.
description: 11 pages, 4 figures. Accepted for publication in JCAP
An $\dot{f}(f)$-frequency dynamics algorithm for gravitational waves
Creators: name: van Putten, Maurice H. P. M.
name: Sarkar, Abhinanda
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Coalescence of low mass compact binaries of neutron stars and black holes are primary burst sources for LIGO and VIRGO.Of importance in the early stages of observations will be the classification of candidate detections by source-type. The diversity in source parameters and serendipity in any new window of observations suggest to consider model-independent detection algorithms. Here a frequency dynamics algorithm is described which extracts a trajectory in the $\dot{f}(f)$-plane from the noisy signal. The algorithm is studied in simulated binary coalescence. Robust results are obtained with experimental noise data. Experiments show the method to be superior to matched filtering in the presence of model imperfections.
description: to appear in Rapid Commun, Phys Rev D
The Law of One Price? The Impact of IT-Enabled Markets on Consumer Search and Retailer Pricing
Creators: name: Smith, Michael
Publisher: name: Carnegie Mellon University
Year: 2001
Subjects: subject: Information Systems
subject: FOS: Computer and information sciences
subject: 160510 Public Policy
subject: FOS: Political science

description: Recent IT research has analyzed how the performance of IT-enabled markets may differ from conventional markets. This literature has made two unexpected empirical findings. First, ITenabled markets for commodity goods exhibit significant price dispersion. Second, well-known retailers in these markets appear to cooperate to set high prices. This paper presents an analytic model, and confirmatory empirical evidence, that explains this behavior as a response to the unique characteristics of consumer search in electronic markets. In conventional markets, consumer search costs are primarily a function of the consumer’s physical proximity to retailer outlets — and physical proximity is distributed relatively equally across retailers. In electronic markets, consumer search costs are primarily a function of the consumer’s mental awareness of different retailers — and this awareness is likely to be concentrated in the hands of a few retailers. Based on this model of consumer search, IT-enabled markets for commodity goods exhibit high price dispersion in equilibrium and a few well-known retailers are able to cooperate to set high prices. The predictions of the model are shown to be consistent with empirical data for 23,744 books collected from 24 Internet retailers in late 1999. Viewing consumer search in this manner provides a useful starting point for understanding the likely development of IT-enabled markets, and for understanding the importance of advertising and first-mover advantage for electronic market participants.
Redundancy effect of multisensory interactions under reduced alertness
Creators: name: Bekinschtein, Tristan
name: Ciria, Luis F.
name: Alameda, Clara
name: Zampini, Massimiliano
name: Avancini, Chiara
name: Sanabria, Daniel
Publisher: name: OSF Registries
Year: 2024
Subjects: subject: Cognitive Neuroscience
subject: Life Sciences
subject: Neuroscience and Neurobiology
subject: Cognition and Perception
subject: Social and Behavioral Sciences
subject: Psychology
subject: FOS: Psychology
subject: Brain activity
subject: Drowsiness
subject: Multisensory integration
subject: Perception
subject: Reduced alertness
subject: Redundancy effect

description: A basic principle of multisensory research posits that our ability to make adaptive responses arises from the combined action of our senses in producing a coherent multimodal representation of the external world by exploiting redundancies. This beneficial multisensory phenomenon, called the “redundancy effect”, manifests behaviourally as faster responses when two redundant stimuli (from different senses) appear together, as compared to when a single stimulus appears. Despite extensive research has repeatedly shown this effect, it is not clear whether it is modulated by the individual’s level of alertness, and if so (as hypothesised), to what extent it affects early sensory integration or later perceptual processing. In this experiment, we will combine computational modelling and EEG to determine whether audio-tactile interactions occur via similar spatiotemporal neural mechanisms under reduced alertness.
The Indian Software Services Industry: Structure and Prospects
Creators: name: Arora, Ashish
name: V.S.  Arunachalam
name: Asundi, Jai
name: Fernandes, Ronald
Publisher: name: Carnegie Mellon University
Year: 1999
Subjects: subject: Information Systems
subject: FOS: Computer and information sciences
subject: 160510 Public Policy
subject: FOS: Political science

description: This paper reports on the results of research on the Indian software industry, carried out at Carnegie Mellon University. We use a variety of sources, including a questionnaire survey of Indian software firms, and field visits and interviews with industry participants, observers, and US based clients. The Indian software industry is remarkable in a number of respects. It is service rather than product oriented, heavily export oriented, and is largely managed by professional and entrepreneurial managements. Also, domestic market experience and expertise appears to have very little benefits for successful importers. Although the industry has grown in spectacular fashion, sustaining this performance will pose a number of challenges. In order to counteract the widely reported shortages of skilled software professionals and the possible competition from other low wage, human capital rich countries, Indian firms are trying to move up the value chain by acquiring deeper knowledge of business domains and management capability, and to reduce costs by developing superior methodologies and tools. Whether and how many firms will be a key test of the management skills and willingness to invest along a number of dimensions. From a social perspective, the disconnect between domestic and export markets is a major challenge, but one that the growing diffusion of computers and the improvement of the communication infrastructure should make easier to confront. In the end, the greatest impact the software industry is likely to have on the Indian economy is indirect, in its role as an exemplar of the new business organisational form and as an inspiration to other entrepreneurs.
Properties of the electrostatically driven helical plasma state
Creators: name: Akçay, Cihan
name: Finn, John M.
name: Nebel, Richard A.
name: Barnes, Daniel C.
name: Martin, Neal
Publisher: name: arXiv
Year: 2017
Subjects: subject: Plasma Physics (physics.plasm-ph)
subject: FOS: Physical sciences

description: A novel plasma state has been found [C.~Akçay, J.~Finn, R.~Nebel and D.~Barnes, Phys.~Plasmas \textbf{24}, 052503 (2017)] in the presence of a uniform applied axial magnetic field in periodic cylindrical geometry. This state is driven by external electrostatic fields provided by helical electrodes, and depends on radius $r
Pairing correlations in N~Z pf-shell nuclei
Creators: name: Langanke, K.
name: Dean, D. J.
name: Koonin, S. E.
name: Radha, P. B.
Publisher: name: arXiv
Year: 1996
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We perform Shell Model Monte Carlo calculations to study pair correlations in the ground states of $N=Z$ nuclei with masses A=48-60. We find that $T=1$, $J^π=0^+$ proton-neutron correlations play an important, and even dominant role, in the ground states of odd-odd $N=Z$ nuclei, in agreement with experiment. By studying pairing in the ground states of $^{52-58}$Fe, we observe that the isovector proton-neutron correlations decrease rapidly with increasing neutron excess. In contrast, both the proton, and trivially the neutron correlations increase as neutrons are added. We also study the thermal properties and the temperature dependence of pair correlations for $^{50}$Mn and $^{52}$Fe as exemplars of odd-odd and even-even $N=Z$ nuclei. While for $^{52}$Fe results are similar to those obtained for other even-even nuclei in this mass range, the properties of $^{50}$Mn at low temperatures are strongly influenced by isovector neutron-proton pairing. In coexistence with these isovector pair correlations, our calculations also indicate an excess of isoscalar proton-neutron pairing over the mean-field values. The isovector neutron-proton correlations rapidly decrease with temperatures and vanish for temperatures above $T=700$ keV, while the isovector correlations among like nucleons persist to higher temperatures. Related to the quenching of the isovector proton-neutron correlations, the average isospin decreases from 1, appropriate for the ground state, to 0 as the temperature increases.
The formation of urea in space I. Ion-molecule, neutral-neutral, and radical gas-phase reactions
Creators: name: Brigiano, Flavio Siro
name: Jeanvoine, Yannick
name: Largo, Antonio
name: Spezia, Riccardo
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Chemical Physics (physics.chem-ph)
subject: FOS: Physical sciences
subject: 85-08

description: Many organic molecules have been observed in the interstellar medium thanks to advances in radioastronomy, and very recently the presence of urea was also suggested. While those molecules were observed, it is not clear what the mechanisms responsible to their formation are. In fact, if gas-phase reactions are responsible, they should occur through barrierless mechanisms (or with very low barriers). In the past, mechanisms for the formation of different organic molecules were studied, providing only in a few cases energetic conditions favorable to a synthesis at very low temperature. A particularly intriguing class of such molecules are those containing one N--C--O peptide bond, which could be a building block for the formation of biological molecules. Urea is a particular case because two nitrogen atoms are linked to the C--O moiety. Thus, motivated also by the recent tentative observation of urea, we have considered the synthetic pathways responsible to its formation. We have studied the possibility of forming urea in the gas phase via different kinds of bi-molecular reactions: ion-molecule, neutral, and radical. In particular we have focused on the activation energy of these reactions in order to find possible reactants that could be responsible for to barrierless (or very low energy) pathways. We have used very accurate, highly correlated quantum chemistry calculations to locate and characterize the reaction pathways in terms of minima and transition states connecting reactants to products. Most of the reactions considered have an activation energy that is too high; but the ion-molecule reaction between NH$_2$OH$_2^+$ and formamide is not too high. These reactants could be responsible not only for the formation of urea but also of isocyanic acid, which is an organic molecule also observed in the interstellar medium.
description: 9 pages + 8 pages of appendix
A Class of Cosmological Matrix Models
Creators: name: Li, Miao
Publisher: name: arXiv
Year: 2005
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We discuss a class of matrix models describing cosmology with a light-like singularity, generalizing the model proposed by Craps et al. in hep-th/0506180.
description: 12 pages, harvmac, v2: final version published in Phys. Lett. B
title: Rapport de voyage, Ile de France (1926) : Ligne de New-York, 1957, voyage n°24
Creators: name: De Beaudean, Raoul
name: Delafon, Michel
name: Nadal, Jean
name: Tournyol du Clos, Guy
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2024
Subjects: subject: Compagnie Générale Transatlantique
subject: Transports maritimes - Histoire
subject: Marine marchande
subject: Journaux de bord

description: Chapitrage : Rapport général / du capitaine - Rapport du commissaire - Rapport du second - Rapport de l'officier de sécurité - Rapport de l'officier de navigation - Rapport du médecin - Rapport contentieux
description: Source: French Lines & Compagnies, 1997 004 5072-16
description: Coverage: 1957-08-16/1957-08-31
title: 01_0937
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/
Refraction in exoplanet atmospheres: Photometric signatures, implications for transmission spectroscopy, and search in Kepler data
Creators: name: Alp, Dennis
name: Demory, Brice-Olivier
Publisher: name: arXiv
Year: 2017
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Refraction deflects photons that pass through atmospheres, which affects transit light curves. Refraction thus provides an avenue to probe physical properties of exoplanet atmospheres and to constrain the presence of clouds and hazes. In addition, an effective surface can be imposed by refraction, thereby limiting the pressure levels probed by transmission spectroscopy. The main objective of the paper is to model the effects of refraction on photometric light curves for realistic planets and to explore the dependencies on atmospheric physical parameters. We also explore under which circumstances transmission spectra are significantly affected by refraction. Finally, we search for refraction signatures in photometric residuals in Kepler data. We use the model of Hui & Seager (2002) to compute deflection angles and refraction transit light curves, allowing us to explore the parameter space of atmospheric properties. The observational search is performed by stacking large samples of transit light curves from Kepler. We find that out-of-transit refraction shoulders are the most easily observable features, which can reach peak amplitudes of ~10 parts per million (ppm) for planets around Sun-like stars. More typical amplitudes are a few ppm or less for Jovians and at the sub-ppm level for super-Earths. Interestingly, the signal-to-noise ratio of any refraction residuals for planets orbiting Sun-like hosts are expected to be similar for planets orbiting red dwarfs. We also find that the maximum depth probed by transmission spectroscopy is not limited by refraction for weakly lensing planets, but that the incidence of refraction can vary significantly for strongly lensing planets. We find no signs of refraction features in the stacked Kepler light curves, which is in agreement with our model predictions.
description: Accepted for publication in A&A
A Case for an Atmosphere on Super-Earth 55 Cancri e
Creators: name: Angelo, Isabel
name: Hu, Renyu
Publisher: name: arXiv
Year: 2017
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: One of the primary questions when characterizing Earth-sized and super-Earth-sized exoplanets is whether they have a substantial atmosphere like Earth and Venus or a bare-rock surface like Mercury. Phase curves of the planets in thermal emission provide clues to this question, because a substantial atmosphere would transport heat more efficiently than a bare-rock surface. Analyzing phase curve photometric data around secondary eclipse has previously been used to study energy transport in the atmospheres of hot Jupiters. Here we use phase curve, Spitzer time-series photometry to study the thermal emission properties of the super-Earth exoplanet 55 Cancri e. We utilize a semi-analytical framework to fit a physical model to the infrared photometric data at 4.5 micron. The model uses parameters of planetary properties including Bond albedo, heat redistribution efficiency (i.e., ratio between radiative timescale and advective timescale of the atmosphere), and atmospheric greenhouse factor. The phase curve of 55 Cancri e is dominated by thermal emission with an eastward-shifted hot spot. We determine the heat redistribution efficiency to be ~1.47, which implies that the advective timescale is on the same order as the radiative timescale. This requirement cannot be met by the bare-rock planet scenario because heat transport by currents of molten lava would be too slow. The phase curve thus favors the scenario with a substantial atmosphere. Our constraints on the heat redistribution efficiency translate to an atmospheric pressure of ~1.4 bar. The Spitzer 4.5-micron band is thus a window into the deep atmosphere of the planet 55 Cancri e.
description: Accepted for publication on AJ
Hydrogen refuelling station with integrated metal hydride compressor: layout features and experience of two-year operation
Creators: name: Lototskyy, Mykhaylo
name: Davids, Moegamat
name: Swanepoel, Dana
name: Louw, Gerhard
name: Klochko, Yevgeniy
name: Smith, Fahmida
name: Haji, Fatema
name: Tolj, Ivan
name: Cordellia, Sita
name: Linkov, Vladimir
Publisher: name: Zenodo
Year: 2018

description: Here, we present the details about layout and operation of the H2 refuelling station at Impala Platinum refineries in Springs, South Africa, since its start-up in October 2015 (officially launched on March 31, 2016). The station provides H2 dispensing at the pressure up to 185 bar and uses pipeline H2 (P~50 bar) available at the customer site. H2 compression to P=200 bar with productivity up to 13 Nm3/h is provided by the integrated 1-stage metal hydride (MH) H2 compressor which uses steam (T~130 °C) for the heating
 and circulating water (T~20 °C) for the cooling; both steam and water are also available from the customer infrastructure. The station also includes H2 dispenser, buffer tank (standard gas cylinder pack), and control block on the basis of Siemens Program Logic Controller (PLC) which provides fully automated system operation. Switching H2 and steam / water flows is carried out with the help of remotely controlled, pneumatically actuated valves and auxiliary check valves. The H2 discharge line is also equipped with a
 safety relief valve for H2 venting if overpressure (>210 bar) takes place. Additionally, at P=200 bar the control block switches the system into standby mode when both MH compression modules are cooled down and their gas manifolds are connected to the H2 supply line. The H2 dispensing is independent on the compressor operation and takes from 6 to 15 minutes.
Directed flow in heavy-ion collisions and its implications for astrophysics
Creators: name: Ivanov, Yuri B.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Nuclear Theory (nucl-th)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: Analysis of directed flow ($v_1$) of protons, antiprotons and pions in heavy-ion collisions is performed in the range of collision energies $\sqrt{s_{NN}}$ = 2.7--39 GeV. Simulations have been done within a three-fluid model employing a purely hadronic equation of state (EoS) and two versions of the EoS with deconfinement transitions: a first-order phase transition and a smooth crossover transition. The crossover EoS is unambiguously preferable for the description of experimental data at lower collision energies $\sqrt{s_{NN}}\leq$ 20 GeV. However, at higher collision energies $\sqrt{s_{NN}}\geq$ 20 GeV the purely hadronic EoS again becomes advantageous. This indicates that the deconfinement EoS in the quark-gluon sector should be stiffer at high baryon densities than those used in the calculation. The latter finding is in agreement with that discussed in astrophysics in connection with existence of hybrid stars with masses up to about two solar masses.
description: 7 pages, 3 figures. Contribution to Proceedings of the Conference "Compact Stars in the QCD Phase Diagram VI", Dubna, Sept. 26-29, 2017. arXiv admin note: substantial text overlap with arXiv:1601.03902
Low-energy interaction of composite spin-half systems with scalar and vector fields
Creators: name: Phillips, D. R.
name: Birse, M. C.
name: Wallace, S. J.
Publisher: name: arXiv
Year: 1996
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We consider a composite spin-half particle moving in spatially-varying scalar and vector fields. The vector field is assumed to couple to a conserved charge, but no assumption is made about either the structure of the composite or its coupling to the scalar field. A general form for the piece of the spin-orbit interaction of the composite with the scalar and vector fields which is first-order in momentum transfer ${\bf Q}$ and second-order in the fields is derived.
description: 10 pages, RevTeX
The Indian Software Industry and Its Prospects
Creators: name: Arora, Ashish
Publisher: name: Carnegie Mellon University
Year: 2006
Subjects: subject: Information Systems
subject: FOS: Computer and information sciences
subject: 160510 Public Policy
subject: FOS: Political science

description: India’s emergence as a major exporter of software services in less than a decade and a half has excited debate about the causes of its success and ignited hopes for similar success in other industries. The subsequent growth of exports of other business services appears to validate the belief of some observers that India’s software success would have broader benefits for the Indian economy. Despite this, there is a perennial undercurrent of concern about the prospects of the Indian software industry. The causes for concern are not difficult to find. Wages for software professionals have consistently risen year over year and employee attrition remains a persistent problem for companies. Indian exports continue to be mostly services with a modest technology content and there is little evidence of successful product development. Add to these the ever present possibility of China (or Eastern Europe or the Philippines) emerging as potent rivals, and there is much to be concerned about. This paper will briefly describe its growth and evolution, identify the major factors that contributed to its success, and some possible ones that were not important. The prospects of the industry are next and in this context this paper shall summarize the available evidence on the extent to which India and Indian firms are participating in software innovation. This will lead to an assessment of whether the industry has and can provide higher value added products and services.
Gas in Galaxies
Creators: name: Bland-Hawthorn, J.
name: Reynolds, R. J.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The interstellar medium (ISM) can be thought of as the galactic atmosphere which fills the space between stars. When clouds within the ISM collapse, stars are born. When the stars die, they return their matter to the surrounding gas. Therefore the ISM plays a vital role in galactic evolution. The medium includes starlight, gas, dust, planets, comets, asteroids, fast moving charged particles (cosmic rays) and magnetic fields. The gas can be further divided into hot, warm and cold components, each of which appear to exist over a range of densities, and therefore pressures. Remarkably, the diverse gas components, cosmic rays, magnetic fields and starlight all have very roughly the same energy density of about 1 eV cm$^{-3}$. All the major constituents (or phases) of the interstellar medium appear to be identified now, although complete multi-phase studies are extremely difficult beyond a few thousand parsecs from the Sun. The interstellar medium is a highly complex environment which does not lend itself to simple analysis. However, this has not stopped astrophysicists from producing basic models of the ISM in order to make sense of the great wealth of data coming in from ground-based telescopes and from satellites.
description: 8 pages of text, 6 figures; Encyclopaedia of Astronomy & Astrophysics, MacMillan and Institute of Physics Publishing, to appear Sept 2000
Scaling Behavior of Angular Dependent Resistivity in CeCoIn$_5$: Possible Evidence for d-Wave Density Waves
Creators: name: Hu, T.
name: Xiao, H.
name: Sayles, T. A.
name: Maple, M. B.
name: Maki, Kazumi
name: Dora, B.
name: Almasan, C. C.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: In-plane angular dependent resistivity ADR was measured in the non-Fermi liquid regime of CeCoIn$_5$ single crystals at temperatures $T \le 20$ K and in magnetic fields $H$ up to 14 T. Two scaling behaviors were identified in low field region where resistivity shows T-linear dependence, separated by a critical angle $θ_{c}$ which is determined by the anisotropy of CeCoIn$_5$; i.e., ADR depends only on the perpendicular (parallel) field component below (above) $θ_c$. These scaling behaviors and other salient features of ADR are consistent with d-wave density waves.
Stochastic representation of the effects of micromixing on soot in turbulent non-premixed flames
Creators: name: Gkantonas, Savvas
name: Mastorakos, Epaminondas
Publisher: name: Apollo - University of Cambridge Repository
Year: 2023

description: The impact of small-scale mixing and scalar dissipation rate (SDR) fluctuations on the evolution of soot particle size distribution (PSD) dynamics in non-premixed turbulent flames is investigated within the context of Large Eddy Simulation (LES). To accomplish this, a stochastic approach based on a physicochemical sectional model, spatially homogeneous Conditional Moment Closure (CMC) and a stochastic differential equation for the SDR are employed, mimicking the function of an LES sub-grid scale combustion model. The results reveal the influence of SDR fluctuations on the probability density function (PDF) and the dynamic behaviour of gas-phase species and soot PSD moments, emphasising the importance of micromixing, the LES resolution, and the underlying assumptions regarding particle transport. This study provides a framework for better understanding the effectiveness of presumed PDF sub-grid scale combustion models in describing soot evolution.
Why should I care? On the incentives of transparency in research with human subjects
Creators: name: Krebs, Christine Renate
name: Toro, Frederico Grasso
name: Churakova, Olga
Publisher: name: Zenodo
Year: 2024
Subjects: Transparency as a means of demonstrating research integrity
Research Data Management
Personal data
Transparency
Open Science services

description: This poster presents insights from our survey on the local requirements on Open Science support services. Further, we use the research data lifecycle to demonstrate what Open Science means in general, and what research data management means specifically in every stage for researchers. Additionally, we will highlight at each stage the resulting benefits for researchers.
Bound states of the two-dimensional Dirac equation for an energy-dependent hyperbolic Scarf potential
Creators: name: Schulze-Halberg, A.
name: Roy, P.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Quantum Physics (quant-ph)
subject: Other Condensed Matter (cond-mat.other)
subject: High Energy Physics - Theory (hep-th)
subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: We study the two-dimensional massless Dirac equation for a potential that is allowed to depend on the energy and on one of the spatial variables. After determining a modified orthogonality relation and norm for such systems, we present an application involving an energy-dependent version of the hyperbolic Scarf potential. We construct closed-form bound state solutions of the associated Dirac equation.
The Impact of Web-Based Risk Calculators on Health Risk Perceptions and Information Processing
Creators: name: Harle, Christopher
Publisher: name: Carnegie Mellon University
Year: 2008
Subjects: subject: Information Systems
subject: FOS: Computer and information sciences
subject: 160510 Public Policy
subject: FOS: Political science

description: Every day, millions of Americans use the Internet to obtain health information. To satisfy this demand, organizations deliver a variety of content that promotes awareness and education and informs health-related decision making. Given advances in web technology, new statistical models of disease, and the shift towards shared patient decision making, these e-health services are increasingly complex. Through applications such as personal health records and “health risk calculators” Internet users can obtain personalized and interactive feedback about their current health state, model-based predictions about their future health, and tailored education about healthy behavior. While providing the public with more content to inform health-related decisions is an appropriate goal, research in health psychology and behavioral decision making suggest the importance of clearly understanding the perceptual and behavioral responses when laypersons are presented with statistical results and personalized risk information. Little research has studied how web-based personalized and interactive health applications actually impact the beliefs and behavior of users. In two separate experiments, we measured the effect of a type 2 diabetes “risk calculator” website on user information processing and subjective risk perceptions about diabetes. In the first experiment, 100 middle-aged and elderly adults were randomized to one of three conditions in order to determine how personalized risk estimates and interactive risk feedback influenced information usage and beliefs about future diabetes onset. Results showed that personalization and interactive features did not lead to increases in information utilization as expected. Instead, we show in some cases personalization actually reduced the amount of information accessed and the extent to which users attended to and carefully considered health risk content. The experiment did show that personalization was related to modest increases in the accuracy of absolute diabetes risk estimates but did not motivate significant changes in relative or affective risk perceptions. A second study of 34 university staff members was qualitatively suggestive of similar results. Future work is needed to further understand the behavioral implications when complex statistical models are integrated with publicly available health information websites. This may aid the design of health information applications and ensure that providers of these tools are effectively motivating improved awareness and education about health risks.
Photon electroproduction off nuclei in the $Δ$-resonance region
Creators: name: Pasquini, B.
Publisher: name: arXiv
Year: 1996
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: The cross section for the $A(e,e'γ)A$ reaction is calculated, investigating the contribution from the nuclear target with respect to the radiative corrections from the electron. The reaction mechanism is studied for photon emission in the $Δ$-resonance region, varying the scattering geometry and analyzing the most favourable kinematical conditions to extract information on the nuclear system.
description: 10 pages, LaTeX, 6 figures available from the author
Tachina civilis Rondani 1859
Creators: name: Sforzi, Alessandra
name: Sommaggio, Daniele
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Rhinophoridae
Tachina
Tachina civilis

description: Tachina civilis Rondani, 1859
ORIGINAL DESCRIPTION: 1859b: 194 (key), 199 (description).
 TYPE LOCALITY: “ in Apennino parmensi, … in Etruria (= Tuscany), … ab Insubria [Parmese Apennines, … Etruria (= Tuscany) … Insubria (= Lombardy) (Italy)]”.
 TYPE MATERIAL: 1 ♂, syntype (MZUF: Box 13): Tachina Mgn / civilis Rnd., ♂ / 682; 2 ♀♀, syntypes (one missing right mid-leg, the other covered with mold) (MZUF: Box 13): Tachina Mgn / civilis Rnd., ♀ / 682; 1 ♂, syntype (missing left mid-leg) (MZUF: Box D): Tachina civilis Rnd., 258, ♂, Parma / 393 258; 1 ♂, syntype (missing left mid-leg, abdomen partially eaten by dermestids) (MSNC: Box DIPTERA Ex collezione Rondani - I): Tachina civilis Rnd. 76 ♂ Parma / Coll. Rondani, scatola n° 1, posiz. G-6 / Museo di Storia Naturale Università di Pisa, Calci (PI) ex collezione Rondani.
 CURRENT STATUS: valid species, as Exorista (Ptilotachina) civilis (Herting & Dely-Draskovits 1993: 125, Pape et al. 1995: 16, O’Hara et al. 2009: 94, 2020: 399, Cerretti 2010: 101).
 REMARKS: Rondani (1859b: 199) described both sexes of Tachina civilis without specifying the exact number of specimens and not giving a range of lengths: “ marem unicum legi … alterum a D. Piccioli … lectum, et foeminam a D. De-Cristofori ab Insubria [I collected a single male … the other collected by D. Piccioli, and the female by D. De-Cristofori from Insubria]”. We found five syntypes in this study.
description: Published as part of Sforzi, Alessandra & Sommaggio, Daniele, 2021, Catalog of the Diptera types described by Camillo Rondani, pp. 1-438 in Zootaxa 4989 (1) on page 357, DOI: 10.11646/zootaxa.4989.1.1, http://zenodo.org/record/4980621
How Generic are the Robust Theoretical Aspects of Jamming in Hard Sphere Models?
Creators: name: Parisi, Giorgio
name: Pollack, Yoav G.
name: Procaccia, Itamar
name: Rainone, Corrado
name: Singh, Murari
Publisher: name: arXiv
Year: 2017
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: In very recent work the mean field theory of the jamming transition in infinite dimensional hard spheres models was presented. Surprisingly, this theory predicts quantitatively numerically determined characteristics of jamming in two and three dimensions. This is a rare and unusual finding. Here we argue that this agreement in non-generic: only for hard sphere models it happens that sufficiently close to jamming the effective interactions are in agreement with mean-field theory, justifying the truncation of many body interactions (which is the exact protocol in infinite dimensions). Any softening of the bare hard sphere interactions results in effective interactions that are not mean-field all the way to jamming, making the discussed phenomenon non generic.
description: Supplementary Material added. Keywords: Amorphous, Soft Matter, force\-law, hard spheres, soft spheres, jamming, colloids, simulation, Emergent interactions
title: ADCO, Septième cartulaire de Saint-Étienne de Dijon (1661-1665), Cart. 29 (G 134), 996 folios, f. 0733
Creators: name: de la Côte d'Or, Archives départementales
name: Petot, Frédéric
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2012
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: cartulaire
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge

description: Septième cartulaire de Saint-Étienne de Dijon (1661-1665), Archives départementales de la Côte-d'Or, Cart. 29 (G 134), 996 folios, f. 0733, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Septième cartulaire de Saint-Étienne de Dijon (1661-1665), Archives départementales de la Côte-d'Or, Cart. 29 (G 134), 996 folios, f. 0733, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https://manuscrits.cbma-project.eu/
description: Provenance: abbaye Saint-Étienne de Dijon
description: Provenance: http://www.wikidata.org/entity/Q15945019
The Impact of State Enterprise Zones on Urban Housing Markets
Creators: name: Engberg, John
name: Greenbaum, Robert
Publisher: name: Carnegie Mellon University
Year: 1999
Subjects: subject: Information Systems
subject: FOS: Computer and information sciences
subject: 160510 Public Policy
subject: FOS: Political science

description: State-sponsored enterprise zones are a major economic development tool for over forty states. In many cases, the impact of these geographically targeted tax-based policies has never been evaluated. One roadblock to evaluation is the difficulty of controlling for the persistent effect of distressed local economic conditions while searching for possible programmatic effects. We examine the impact of enterprise zone programs on a variety of local economic growth rates in Florida, Pennsylvania and Virginia. We focus on housing prices because they capitalize expected long run changes in prosperity. We find that the states established zones in very distressed areas. The housing markets in zone areas are surprisingly strong following zone designation, in spite of continued weak income and employment growth. Estimates that distinguish the programmatic impact from differences arising due to pre-designation conditions indicate that two of the programs stimulated housing demand as measured by increases in home ownership and occupancy rates. However, the programs’ negative impact on labor market conditions offset the increased demand, causing housing prices to remain stable.
Superconductivity in the Nb-Ru-Ge $σ$-Phase
Creators: name: Carnicom, Elizabeth M.
name: Xie, Weiwei
name: Sobczak, Zuzanna
name: Kong, Tai
name: Klimczuk, Tomasz
name: Cava, Robert J.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: We show that the previously unreported ternary $σ$-phase material Nb$_{20.4}$Ru$_{5.7}$Ge$_{3.9}$ is a superconductor with a critical temperature of 2.2 K. Temperature-dependent magnetic susceptibility, resistance, and specific heat measurements were used to characterize the superconducting transition. The Sommerfeld constant $γ$ for Nb$_{20.4}$Ru$_{5.7}$Ge$_{3.9}$ is 91 mJ mol-f.u.$^{-1}$K$^{-2}$ and the specific heat anomaly at the superconducting transition, $Δ$C/$γ$T$_c$, is approximately 1.38. The zero-temperature upper critical field ($μ_0$H$_{c2}$(0)) was estimated to be 2 T by resistance data. Field-dependent magnetization data analysis estimated $μ_0$H$_{c1}$(0) to be 5.5 mT. Thus, the characterization shows Nb$_{20.4}$Ru$_{5.7}$Ge$_{3.9}$ to be a type II BCS superconductor. This material appears to be the first reported ternary phase in the Nb-Ru-Ge system, and the fact that there are no previously reported binary Nb-Ru, Nb-Ge, or Ru-Ge $σ$-phases shows that all three elements are necessary to stabilize the material. A $σ$-phase in the Ta-Ru-Ge system was synthesized but did not display superconductivity above 1.7 K, which suggests that electron count cannot govern the superconductivity observed. Preliminary characterization of a possible superconducting $σ$-phase in the Nb-Ru-Ga system is also reported.
description: 7 pages, 8 figures, 3 tables