cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: Transcription d'un entretien auprès d’une femme âgée de 32 ans allaitant son fils dans la ville de Florianopolis au Brésil
Creators: name: Campos, Danièla de Quieroz
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2017

description: Source: T-4868
description: Transcription en langue portugaise
description: L’entretien se déroule au domicile de l’informatrice qui allaite son nouveau-né âgé d’un mois et demi. L’informatrice donne le sein à son enfant depuis sa naissance. Comme son enfant n’a pas pris assez de poids, elle doit compléter l’allaitement maternel avec un lait du commerce et un sérum prescrit par le médecin. L’informatrice se confie à l’enquêtrice sur son impression d’être obligée d'utiliser un lait maternisé en complément de son lait maternel pour son enfant. La marque de lait conseillée par le médecin est citée. L’informatrice décrit l'alternance entre ses tétées et les biberons de lait du commerce. L’enquêtrice demande à l’informatrice si l’allaitement lui a causé des douleurs ou des plaies. L’informatrice répond qu’elle n’a pas rencontré ce type de problème. En revanche,elle précise avoir utilisé une téterelle. L’enquêtrice demande à l’informatrice de lui parler des conseils qu’elle a reçus de la part de son entourage. L’informatrice rapporte ceux de sa mère durant la grossesse. Elle explique que sa mère et son médecin lui ont conseillé de prendre le soleil au niveau de sa poitrine. L’informatrice explique qu’elle s’est informée sur l’allaitement à travers des lectures, des médias, et des questions qu’elle a posées aux médecins. Elle précise également avoir participé et aidé à l’organisation de cours pour les femmes enceintes. La conversation traite ensuite du sujet du colostrum. L’informatrice explique que son colostrum a été suffisant pour nourrir son enfant durant les premiers jours de sa vie. Pour l’informatrice, l’allaitement apporte à son enfant une protection à chaque tétée. L’informatrice donne les pratiques ou encore les techniques et aliments consommés pour favoriser sa production et sa montée de lait. Elle a pris soin de ses seins en ayant une bonne hygiène corporelle. L’informatrice fait le récit des premiers jours qui ont suivi la naissance de son enfant et décrit les difficultés et les douleurs liées à la césarienne auxquelles elle a été confrontée. L’informatrice évoque les sensations et les émotions qu’elle ressent lorsqu’elle allaite. Elle pense que l’allaitement maternel est meilleur pour son enfant. Pour elle, l’allaitement est plus économique que les boîtes de lait maternisé qui sont onéreuses. L’informatrice évoque également sa vie quotidienne ainsi que les endroits où elle allaite son enfant, toutefois elle explique qu’elle n’allaite pas en public. L’informatrice donne également le point de vue et la réaction des hommes de son entourage face à l’allaitement et décrit certaines situations où on lui a demandé de changer de pièce pour allaiter son enfant.
Direct Numerical Simulation of turbulent Taylor-Couette flow
Creators: name: Pirro, Davide
name: Quadrio, Maurizio
Publisher: name: arXiv
Year: 2007
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: Computational Physics (physics.comp-ph)
subject: FOS: Physical sciences

description: The direct numerical simulation (DNS) of the Taylor--Couette flow in the fully turbulent regime is described. The numerical method extends the work by Quadrio & Luchini (Eur. J. Mech. B / Fluids, v.21, pp.413--427, 2002), and is based on a parallel computer code which uses mixed spatial discretization (spectral schemes in the homogeneous directions, and fourth-order, compact explicit finite-difference schemes in the radial direction). A DNS is carried out to simulate for the first time the turbulent Taylor--Couette flow in the turbulent regime. Statistical quantities are computed to complement the existing experimental information, with a view to compare it to planar, pressure-driven turbulent flow at the same value of the Reynolds number. The main source for differences in flow statistics between plane and curved-wall flows is attributed to the presence of large-scale rotating structures generated by curvature effects.
description: To appear in European Journal of Mechanics B / Fluids
Hüsy, Jean Jacques
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1820

description: Ort: Mailand
description: Verzeichnung=Description=Inventaire 05.07.2020 Automatisiert nach HAN-Import
description: Verzeichnung=Description=Inventaire ISAD(G) / HAN Katalogisierungsregeln für Archivbestände Detailliert
Galactic disk winds driven by cosmic ray pressure
Creators: name: Mao, S. Alwin
name: Ostriker, Eve C.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Cosmic ray pressure gradients transfer energy and momentum to extraplanar gas in disk galaxies, potentially driving significant mass loss as galactic winds. This may be particularly important for launching high-velocity outflows of "cool" (T < 10^4 K) gas. We study cosmic-ray driven disk winds using a simplified semi-analytic model assuming streamlines follow the large-scale gravitational potential gradient. We consider scaled Milky Way-like potentials including a disk, bulge, and halo with a range of halo velocities V_H = 50-300 km/s, and streamline footpoints with radii in the disk R_0=1-16 kpc at height 1 kpc. Our solutions cover a wide range of footpoint gas velocity u_0, magnetic-to-cosmic-ray pressure ratio, gas-to-cosmic-ray pressure ratio, and angular momentum. Cosmic ray streaming at the Alfvén speed enables the effective sound speed C_eff to increase from the footpoint to a critical point where C_eff,c = u_c ~ V_H; this differs from thermal winds in which C_eff decreases outward. The critical point is typically at a height of 1-6 kpc from the disk, increasing with V_H, and the asymptotic wind velocity exceeds the escape speed of the halo. Mass loss rates are insensitive to the footpoint values of the magnetic field and angular momentum. In addition to numerical parameter space exploration, we develop and compare to analytic scaling relations. We show that winds have mass loss rates per unit area up to ~ Pi_0 V_H^-5/3 u_0^2/3 where Pi_0 is the footpoint cosmic ray pressure and u_0 is set by the upwelling of galactic fountains. The predicted wind mass-loss rate exceeds the star formation rate for V_H < 200 km/s and u_0 = 50 km/s, a typical fountain velocity.
description: 34 pages, 12 figures, accepted to ApJ
MOESM3 of A One Health perspective to identify environmental factors that affect Rift Valley fever transmission in Gezira state, Central Sudan
Creators: name: Bashir, Rania
name: Hassan, Osama
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: Plant Biology
subject: FOS: Biological sciences
subject: Computational Biology

description: Additional file 3: Table S3. Average NDVI during 2007, 2010, and 2014 in Gezira state, Sudan.
EPOS LHC : test of collective hadronization with LHC data
Creators: name: Pierog, T.
name: Karpenko, Iu.
name: Katzy, J. M.
name: Yatsenko, E.
name: Werner, K.
Publisher: name: arXiv
Year: 2013
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: EPOS is a Monte-Carlo event generator for minimum bias hadronic interactions, used for both heavy ion interactions and cosmic ray air shower simulations. Since the last public release in 2009, the LHC experiments have provided a number of very interesting data sets comprising minimum bias p-p, p-Pb and Pb-Pb interactions. We describe the changes required to the model to reproduce in detail the new data available from LHC and the consequences in the interpretation of these data. In particular we discuss the effect of the collective hadronization in p-p scattering. A different parametrization of flow has been introduced in the case of a small volume with high density of thermalized matter (core) reached in p-p compared to large volume produced in heavy ion collisions. Both parametrizations depend only on the geometry and the amount of secondary particles entering in the core and not on the beam mass or energy. The transition between the two flow regimes can be tested with p-Pb data. EPOS LHC is able to reproduce all minimum bias
description: 27 pages, 34 figures, change to 1 column style, add ALICE data on PbPb dN/deta and link to source code
Mirabaud & Co
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1820

description: Ort: Mailand
description: Verzeichnung=Description=Inventaire 05.07.2020 Automatisiert nach HAN-Import
description: Verzeichnung=Description=Inventaire ISAD(G) / HAN Katalogisierungsregeln für Archivbestände Detailliert
Mivilee-Socin, J. J., Waren-Sensal
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1820

description: Ort: Basel
description: Verzeichnung=Description=Inventaire 05.07.2020 Automatisiert nach HAN-Import
description: Verzeichnung=Description=Inventaire ISAD(G) / HAN Katalogisierungsregeln für Archivbestände Detailliert
The Structure of Differential Invariants and Differential Cut Elimination
Creators: name: Platzer, Andre
Publisher: name: Carnegie Mellon University
Year: 1993
Subjects: subject: 89999 Information and Computing Sciences not elsewhere classified
subject: FOS: Computer and information sciences

description: The biggest challenge in hybrid systems verification is the handling of differential equations. Because computable closed-form solutions only exist for very simple differential equations, proof certificates have been proposed for more scalable verification. Search procedures for these proof certificates are still rather ad-hoc, though, because the problem structure is only understood poorly. We investigate differential invariants, which define an induction principle for differential equations and which can be checked for invariance along a differential equation just by using their differential structure, without having to solve them. We study the structural properties of differential invariants. To analyze trade-offs for proof search complexity, we identify more than a dozen relations between several classes of differential invariants and compare their deductive power. As our main results, we analyze the deductive power of differential cuts and the deductive power of differential invariants with auxiliary differential variables. We refute the differential cut elimination hypothesis and show that, unlike standard cuts, differential cuts are fundamental proof principles that strictly increase the deductive power. We also prove that the deductive power increases further when adding auxiliary differential variables to the dynamics.
GOBLET - The Global Organisation for Bioinformatics Learning, Education & Training
Creators: name: Van Gelder, Celia W.G.
name: D'Elia, Domenica
name: Korpelainen, Eija
Publisher: name: Zenodo
Year: 2021
Subjects: bioinformatics
training
education
community
trainers
network
outreach

description: GOBLET presentation at GOBLET Exhibitor Booth at ISMB/ECCB2021, 25-30 July 2021 (https://www.iscb.org/ismbeccb2021)
title: ADCO, Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome V, Cart. 189 (11 H 74), 316 folios, f. 0236r
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/2012
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire

description: Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome V, Archives départementales de la Côte-d'Or, Cart. 189 (11 H 74), 316 folios, f. 0236r, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome V, Archives départementales de la Côte-d'Or, Cart. 189 (11 H 74), 316 folios, f. 0236r, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
Nonparametric Methods in Astronomy: Think, Regress, Observe -- Pick Any Three
Creators: name: Steinhardt, Charles L.
name: Jermyn, Adam S.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: Telescopes are much more expensive than astronomers, so it is essential to minimize required sample sizes by using the most data-efficient statistical methods possible. However, the most commonly used model-independent techniques for finding the relationship between two variables in astronomy are flawed. In the worst case they can lead without warning to subtly yet catastrophically wrong results, and even in the best case they require more data than necessary. Unfortunately, there is no single best technique for nonparametric regression. Instead, we provide a guide for how astronomers can choose the best method for their specific problem and provide a python library with both wrappers for the most useful existing algorithms and implementations of two new algorithms developed here.
description: 19 pages, PASP
The semantics of scheme control-flow analysis
Creators: name: Shivers, Olin
Publisher: name: Carnegie Mellon University
Year: 2005
Subjects: subject: 89999 Information and Computing Sciences not elsewhere classified
subject: FOS: Computer and information sciences

description: Abstract: "This is a follow-up to my 1988 PLDI paper, 'Control-Flow Analysis in Scheme' [9]. I use the method of abstract semantic interpretations to explicate the control-flow analysis technique presented in that paper. I begin with a denotational semantics for CPS Scheme. I then present an alternate semantics that precisely expresses the control-flow analysis problem. I abstract this semantics in a natural way, arriving at two different semantic interpretations giving approximate solutions to the flow analysis problem, each computable at compile time.The development of the final abstract semantics provides a clear, formal description of the analysis technique presented in 'Control- Flow Analysis in Scheme.'"
Detection of a Westward Hotspot Offset in the Atmosphere of a Hot Gas Giant CoRoT-2b
Creators: name: Dang, Lisa
name: Cowan, Nicolas B.
name: Schwartz, Joel C.
name: Rauscher, Emily
name: Zhang, Michael
name: Knutson, Heather A.
name: Line, Michael
name: Dobbs-Dixon, Ian
name: Deming, Drake
name: Sundararajan, Sudarsan
name: Fortney, Jonathan J.
name: Zhao, Ming
Publisher: name: arXiv
Year: 2018
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Short-period planets exhibit day-night temperature contrasts of hundreds to thousands of degrees K. They also exhibit eastward hotspot offsets whereby the hottest region on the planet is east of the substellar point; this has been widely interpreted as advection of heat due to eastward winds. We present thermal phase observations of the hot Jupiter CoRoT-2b obtained with the IRAC instrument on the Spitzer Space Telescope. These measurements show the most robust detection to date of a westward hotspot offset of 23 $\pm$ 4 degrees, in contrast with the nine other planets with equivalent measurements. The peculiar infrared flux map of CoRoT-2b may result from westward winds due to non-synchronous rotation magnetic effects, or partial cloud coverage, that obscures the emergent flux from the planet's eastern hemisphere. Non-synchronous rotation and magnetic effects may also explain the planet's anomalously large radius. On the other hand, partial cloud coverage could explain the featureless dayside emission spectrum of the planet. If CoRoT-2b is not tidally locked, then it means that our understanding of star-planet tidal interaction is incomplete. If the westward offset is due to magnetic effects, our result represents an opportunity to study an exoplanet's magnetic field. If it has Eastern clouds, then it means that our understanding of large-scale circulation on tidally locked planets is incomplete.
description: 30 pages, 4 figures, 15 supplementary figures
RANKED CLUSTER INFLUENCE: A DEFENSE AGAINST ADVERSARIAL LABELING ATTACKS ON FAIRNESS
Creators: name: Sangeetha, Athreyan Mohana Krishnan
Publisher: name: Purdue University Graduate School
Year: 2025
Subjects: classificationCode: 461101
subject: Adversarial machine learning
classificationCode: 461199
subject: Machine learning not elsewhere classified

description: Adversarial Labeling Attacks are a proven method of degrading model metrics by flipping the labels of points in the training set or adding copies/imitations of points with the flipped label. The proposed idea is to identify the poisoned data points i.e. flipped data points using influence functions. Former ideas explored how perturbing the features of a data point in the training set influenced the loss calculation for the testing set. Now we see how perturbing the target aka flipping the label affects the loss calculation on the testing set and if we can identify the poisoned points.
Non-perturbative superpotentials across lines of marginal stability
Creators: name: Garcia-Etxebarria, Inaki
name: Uranga, Angel M.
Publisher: name: arXiv
Year: 2007
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We discuss the behaviour of non-perturbative superpotentials in 4d N=1 type II compactifications (and orientifolds thereof) near lines of marginal stability, where the spectrum of contributing BPS D-brane instantons changes discontinuously. The superpotential is nevertheless continuous, in agreement with its holomorphic dependence on the closed string moduli. The microscopic mechanism ensuring this continuity involves novel contributions to the superpotential: As an instanton becomes unstable against decay to several instantons, the latter provide a multi-instanton contribution which reconstructs that of the single-instanton before decay. The process can be understood as a non-perturbative lifting of additional fermion zero modes of an instanton by interactions induced by other instantons. These effects provide mechanisms via which instantons with U(1) symmetry can contribute to the superpotential. We provide explicit examples of these effects for non-gauge D-brane instantons, and for D-brane gauge instantons (where the motions in moduli space can be interpreted as Higgsing, or Seiberg dualities).
description: 48+1 pages, 10 figures. v2: added some refs, and rearranged a bit section 2
Brief an Max Preiswerk
Creators: name: Jung, C. G.
Publisher: name: [s.n.]
Year: 1920

description: von Carl [Gustav Jung]
description: *82 S 24 Öffentliche Bibliothek der Universität Basel
description: Deutsch
description: Wehr, Gerhard. - Carl Gustav Jung : Arzt - Tiefenpsychologe - Visionär : eine Bildbiographie. - Zürich : SV international / Schweizer Verlagshaus, 1989, S. 68
description: Verzeichnung=Description=Inventaire November 2017 HAN-Katalogisierungsregeln Rekatalogisierung nach Original, Standortverzeichnis und Briefkatalog
description: Verzeichnung=Description=Inventaire Februar 2024 HAN-Katalogisierungsregeln Revision nach Vorlage ben
description: Beilagen: 3 Notizblätter: 1 Zeichnung und 2 Planskizzen (Grundriss und Dachstock) des Ferienhauses, das nie realisiert wurde
Single-particle Mass Spectrometry with arrays of frequency-addressed nanomechanical resonators
Creators: name: Sage, Eric
name: Sansa, Marc
name: Fostner, Shawn
name: Defoort, Martial
name: Gély, Marc
name: Naik, Akshay K.
name: Morel, Robert
name: Duraffourg, Laurent
name: Roukes, Michael L.
name: Alava, Thomas
name: Jourdan, Guillaume
name: Colinet, Eric
name: Masselon, Christophe
name: Brenac, Ariel
name: Hentz, Sébastien
Publisher: name: arXiv
Year: 2017
Subjects: subject: Instrumentation and Detectors (physics.ins-det)
subject: FOS: Physical sciences

description: One of the main challenges to overcome to perform nanomechanical Mass Spectrometry (NEMS-MS) analysis in a practical time frame stems from the size mismatch between the analyte beam and the extremely small nanomechanical detector area. We report here the demonstration of NEMS-MS with arrays of 20 individually addressed nanomechanical resonators where the number of inputs-outputs for the whole array is the same as that of a single resonator. While all resonators within an array are interconnected via two metal levels, each resonator is designed with a distinct resonance frequency which becomes its individual address. In order to perform single-particle Mass Spectrometry, the resonance frequencies of the two first modes of each NEMS within an array are monitored simultaneously. Using such an array, mass spectra of metallic aggregates in the MDa range are acquired with more than one order of magnitude improvement in analysis time due to the increase in capture cross section compared to individual resonators. A 20 NEMS array is probed in 150ms with the same mass limit of detection as a single resonator. Spectra acquired with a conventional Time- of-Flight (TOF) mass spectrometer in the same system show excellent agreement. As individual information for each resonator within the array is retained, the array becomes a particle imager, each resonator acting as a pixel. With this technique, we demonstrate how Mass Spectrometry Imaging (MSI) at the single particle level becomes possible by mapping a 4cm-particle beam in the MDa range and above.
Karte an Otto Duthaler
Creators: name: Jung, C. G.
Publisher: name: [s.n.]
Year: 1920

description: von C[arl] [Gustav Jung]
description: *82 S 24 Öffentliche Bibliothek der Universität Basel
description: Deutsch
description: Wehr, Gerhard. - Carl Gustav Jung : Arzt - Tiefenpsychologe - Visionär : eine Bildbiographie. - Zürich : SV international / Schweizer Verlagshaus, 1989, S. 68
description: Verzeichnung=Description=Inventaire November 2017 HAN-Katalogisierungsregeln Rekatalogisierung nach Original, Standortverzeichnis und Briefkatalog
Influence of galactic arm scale dynamics on the molecular composition of the cold and dense ISM I. Observed abundance gradients in dense clouds
Creators: name: Ruaud, M.
name: Wakelam, V.
name: Gratier, P.
name: Bonnell, I. A.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Aims. We study the effect of large scale dynamics on the molecular composition of the dense interstellar medium during the transition between diffuse to dense clouds. Methods. We followed the formation of dense clouds (on sub-parsec scales) through the dynamics of the interstellar medium at galac- tic scales. We used results from smoothed particle hydrodynamics (SPH) simulations from which we extracted physical parameters that are used as inputs for our full gas-grain chemical model. In these simulations, the evolution of the interstellar matter is followed for ~50 Myr. The warm low-density interstellar medium gas flows into spiral arms where orbit crowding produces the shock formation of dense clouds, which are held together temporarily by the external pressure. Results. We show that depending on the physical history of each SPH particle, the molecular composition of the modeled dense clouds presents a high dispersion in the computed abundances even if the local physical properties are similar. We find that carbon chains are the most affected species and show that these differences are directly connected to differences in (1) the electronic fraction, (2) the C/O ratio, and (3) the local physical conditions. We argue that differences in the dynamical evolution of the gas that formed dense clouds could account for the molecular diversity observed between and within these clouds. Conclusions. This study shows the importance of past physical conditions in establishing the chemical composition of the dense medium.
description: 15 pages, 15 figures
Twisted Bhargava Cubes
Creators: name: Gan, Wee Teck
name: Savin, Gordan
Publisher: name: arXiv
Year: 2013
Subjects: subject: Number Theory (math.NT)
subject: Rings and Algebras (math.RA)
subject: FOS: Mathematics
subject: 11S90, 17A75, 17C40

description: Let G be a reductive group and P=MN a maximal parabolic subgroup. The group M acts, by conjugation, on N/[N,N]. It is well known that, over an algebraically closed field, the group M acts transitively on a Zariski open set. However, over a general field, the structure of orbits may be quite non-trivial. A description may involve unexpected invariants. A notable example is when G is a split, simply connected group of type D_4, and P is the maximal parabolic corresponding to the branching point of the Dynkin diagram. The space N/[N,N] is also known as the Bhargava cube, and it was the starting point of his investigations of prehomogeneous spaces. We consider a version of this problem for the triality D_4.
Collegii Musici Protocollum. Angefangen den 10.t Augusti A.o 1708 : Enthaltend Alles dasjenige, was von jeweiligen Membris desselbigen, von Zeit zu Zeit per Majora ist geschlossen worden
Creators: name: Collegium Musicum Basiliensis
Publisher: name: [s.n.]
Year: 1708

description: Protokolle auf original gezählten Seiten 1-309: erster Eintrag 10.t August 1708, letzter Eintrag Xbris 1760. Im hinteren Teil des Bandes (S. 316-356) alfabetisches Stichwortregister mit Seitenverweisen.
description: Collegium Musicum Basiliensis
description: S. V = Titelseite
description: Allgemeine Musikgesellschaft Basel
description: Deutsch
description: Verzeichnung=Description=Inventaire August 2023 HAN-Katalogisierungsregeln rpf
title: Analysis of the Pressures in the Crown-Wall of Rubble-Mound Breakwaters under Tsunami Actions, Based on Laboratory Experiments
Creators: name: Aniel-Quiroga, Íñigo
name: Vidal, César
name: Lara, Javier L.
name: González, Mauricio
Publisher: name: Bundesanstalt für Wasserbau
Year: 2019

description: Presented at: Coastal Structures Conference 2019, Hannover, Germany, September 30th – October 2nd, 2019
Entangling photons using a charged quantum dot in a microcavity
Creators: name: Hu, C. Y.
name: Munro, W. J.
name: Rarity, J. G.
Publisher: name: arXiv
Year: 2007
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We present two novel schemes to generate photon polarization entanglement via single electron spins confined in charged quantum dots inside microcavities. One scheme is via entangled remote electron spins followed by negatively-charged exciton emissions, and another scheme is via a single electron spin followed by the spin state measurement. Both schemes are based on giant circular birefringence and giant Faraday rotation induced by a single electron spin in a microcavity. Our schemes are deterministic and can generate an arbitrary amount of multi-photon entanglement. Following similar procedures, a scheme for a photon-spin quantum interface is proposed.
description: 4 pages, 4 figures
title: ADCO, Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Cart. 32 (G 136), 745 folios, f. 0412
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: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire

description: Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Archives départementales de la Côte-d'Or, Cart. 32 (G 136), 745 folios, f. 0412, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Archives départementales de la Côte-d'Or, Cart. 32 (G 136), 745 folios, f. 0412, 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 seductive appeal of thin clients
Creators: name: Niraj  Tolia
name: Andersen, David G.
name: M  Satyanarayanan
Publisher: name: Carnegie Mellon University
Year: 2008
Subjects: subject: 89999 Information and Computing Sciences not elsewhere classified
subject: FOS: Computer and information sciences

description: Abstract: "Interest in thin clients is very high today because of frustration with the growing total cost of ownership of personal computers. Unfortunately, thin clients may not meet the usability goal of crisp interactive response. This paper shows that the adequacy of thin-client computing is highly variable, and depends on both the application and the available network quality. For intensely interactive applications, the tight control of end-to-end network latency required by thin clients may be hard to guarantee at large scale. The paper advocates the concept of stateless thick clients, and describes how they may reduce total cost of ownership while preserving good interactive performance."
Self-interacting dark matter constraints in a thick dark disk scenario
Creators: name: Vattis, Kyriakos
name: Koushiappas, Savvas M.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: A thick dark matter disk is predicted in cold dark matter simulations as the outcome of the interaction between accreted satellites and the stellar disk in Milky Way sized halos. We study the effects of a self-interacting thick dark disk on the energetic neutrino flux from the Sun. We find that for particle masses between 100 GeV and 1 TeV and dark matter annihilation to heavy leptons either the self-interaction may not be strong enough to solve the small scale structure motivation or a dark disk cannot be present in the Milky Way.
description: 6 pages, 5 figures
Staub & Co
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1820

description: Ort: Neapel
description: Verzeichnung=Description=Inventaire 05.07.2020 Automatisiert nach HAN-Import
description: Verzeichnung=Description=Inventaire ISAD(G) / HAN Katalogisierungsregeln für Archivbestände Detailliert
The Role of Software Architecture in Requirements Engineering
Creators: name: Garlan, David
Publisher: name: Carnegie Mellon University
Year: 1969
Subjects: subject: 89999 Information and Computing Sciences not elsewhere classified
subject: FOS: Computer and information sciences

description: Problem Space versus Solution Space Requirements engineering is concerned fundamen tally with the shape of the problem space. Its primary goal is to determine the dimensions of the problem that the software system is to solve. In contrast, software architecture is concerned with the shape of the solution space. Its primary goal is to determine the structure of a solution to a problem posed by a set of requirements. Thus, understanding the role of software architecture in requirements engineering is largely a matter of understanding the dynamic relationship between identification of a problem to be solved and a description of its solution.
Exoplanet HD209458b: inflated hydrogen atmosphere but no sign of evaporation
Creators: name: Ben-Jaffel, Lotfi
Publisher: name: arXiv
Year: 2007
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Many extrasolar planets orbit closely to their parent star. Their existence raises the fundamental problem of loss and gain in their mass. For exoplanet HD209458b, reports on an unusually extended hydrogen corona and a hot layer in the lower atmosphere seem to support the scenario of atmospheric inflation by the strong stellar irradiation. However, difficulties in reconciling evaporation models with observations call for a reassessment of the problem. Here, we use HST archive data to report a new absorption rate of ~8.9% +/- 2.1% by atomic hydrogen during the HD209458b transit, and show that no sign of evaporation could be detected for the exoplanet. We also report evidence of time variability in the HD209458 Lyman-a flux, a variability that was not accounted for in previous studies, which corrupted their diagnostics. Mass loss rates thus far proposed in the literature in the range 5x(10^{10}-10^{11} g s^{-1}) must induce a spectral signature in the Lyman-a line profile of HD209458 that cannot be found in the present analysis. Either an unknown compensation effect is hiding the expected spectral feature or else the mass loss rate of neutrals from HD209458 is modest.
description: corrected for typos. Published 2007 December 10 in ApjL
Phase transition for the system of small volume in the $ϕ^4$ theory in the Tsallis nonextensive statistics
Creators: name: Ishihara, Masamichi
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 studied the effects of the nonextensivity on the phase transition for the system of small volume $V$ in the $ϕ^4$ theory in the Tsallis nonextensive statistics of entropic parameter $q$ and temperature $T$, when the deviation from the Boltzmann-Gibbs statistics, $|q-1|$, is small. We calculated the condensate and the mass to the order $q-1$ with the normalized $q$-expectation value under the massless free particle approximation. The following facts were found. The condensate $Φ$ divided by $v$, $Φ/v$, at $q$ is smaller than that at $q'$ for $q>q'$ as a function of $T_{\mathrm{ph}}/v$ which is the physical temperature $T_{\mathrm{ph}}$ divided by $v$, where $T_{\mathrm{ph}}$ at $q=1$ coincides with $T$ and $v$ is the value of the condensate at $T=0$. The mass decreases, reaches minimum, and increases after that, as $T_{\mathrm{ph}}$ increases. The mass at $q>1$ is lighter than the mass at $q=1$ at low physical temperature and heavier than the mass at $q=1$ at high physical temperature. The effects of the nonentensivity on the physical quantity as a function of $T_{\mathrm{ph}}$ become strong as $|q-1|$ increases. The results indicate the significance of the definition of the expectation value, the definition of the physical temperature, and the constraints for the density operator, when the terms including the volume of the system are not negligible.
description: 11 pages, 6 figures
Observation of Poincaré-Andronov-Hopf bifurcation in cyclotron maser emission from plasma magnetic trap
Creators: name: Shalashov, A. G.
name: Gospodchikov, E. D.
name: Izotov, I. V.
name: Mansfeld, D. A.
name: Skalyga, V. A.
name: Tarvainen, O.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Plasma Physics (physics.plasm-ph)
subject: FOS: Physical sciences

description: We report the first experimental evidence of a controlled transition from the generation of periodic bursts of electromagnetic emission into continuous wave regime of a cyclotron maser formed in magnetically confined non-equilibrium plasmas. The kinetic cyclotron instability of the extraordinary wave of weakly inhomogeneous magnetized plasma is driven by the anisotropic electron population resulting from electron cyclotron plasma heating in MHD-stable minimum-B open magnetic trap.
description: This is an author-created version of an article submitted for publication in Physical Review Letters
Excitons and cavity polaritons for ultracold atoms in an optical lattice
Creators: name: Zoubi, Hashem
name: Ritsch, Helmut
Publisher: name: arXiv
Year: 2007
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We study the resonant electronic excitation dynamics for ultracold atoms trapped in a deep optical lattice prepared in a Mott insulator state. Excitons in these artificial crystals are similar to Frenkel excitons in Noble atom or molecular crystals. They appear when the atomic excited state line width is smaller than the exciton band width generated by dipole-dipole coupling. When the atoms are placed within a cavity the electronic excitations and the quantized cavity mode get coupled. In the collective strong coupling regime excitations form two branches of cavity polaritons with Rabi splitting larger than the atomic and the cavity line width. To demonstrate their properties we calculate the transmission, reflection, and absorption spectra for an incident weak probe field, which show resonances at the polariton frequencies.
description: 9 pages, 9 figures
Trivial and Non-trivial Superconductivity in dsDNA
Creators: name: Simchi, Hamidreza
Publisher: name: arXiv
Year: 2018
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: A double-stranded DNA (dsDNA) is modeled by two coupled one-dimensional Kitaev's chain and the topological superconductivity is studied. It is shown that the zero energy mode exists under some specific conditions. The wave function of zero mode is calculated and it is shown that the Majorana quasi-particles exist on the ends of each strand. By calculating the winding number, we show that the topological phase transition can happen if the hopping integral between two strands is very smaller than the pairing potential between the Cooper pairs. It means that the dsDNA behaves as a trivial superconductor, commonly, but single-stranded DNA (or two coupled ssDNA with very small hopping between them) may behave as a non-trivial superconductor. Finally, we suggest an experimental setup for probable detection of Majorana quasi-particle in DNA.
title: Η σημασία των διατροφικών συμπληρωμάτων στην υγεία του ανθρώπου
title: The importance of nutritional supplements in human health
titleType: AlternativeTitle
Creators: name: Μπουνιαλέτου, Αθανασία
Publisher: name: Πανεπιστήμιο Δυτικής Αττικής
Year: 2021
Subjects: Διατροφικά συμπληρώματα

description: Το θέμα της παρούσας πτυχιακής εργασίας είναι η επίδραση των διατροφικών συμπληρωμάτων στην ανθρώπινη υγεία. Τα διατροφικά συμπληρώματα χρησιμοποιούνται για να συμπληρώσουν τα κενά στην ανθρώπινη διατροφή όταν αυτή είναι ελλιπής. Έχει θεσπιστεί ένα αυστηρό νομοθετικό πλαίσιο ώστε να εξασφαλιστεί ότι ο καταναλωτής δεν παραπλανάτε και ότι γνωρίζει ότι το διατροφικό συμπλήρωμα δεν είναι φάρμακο και για αυτό δεν υφίσταται τους ίδιους ποιοτικούς ελέγχους με τα φάρμακα. Έχει γίνει ένας μεγάλος αριθμός επιστημονικών ερευνών που εξετάζουν τη χρήση τους στον αθλητισμό και στην αντιμετώπιση του υποσιτισμού, καθώς και τη θεραπευτική δράση τους στην πρόληψη και τη θεραπεία του καρκίνου, των καρδιαγγειακών προβλημάτων, οστεοπαθολογικών καταστάσεων, σακχαρώδη διαβήτη τύπου ΙΙ, υποχοληστερολαιμίας, συνδρόμου του ευερέθιστου εντέρου, ψυχολογικών διαταραχών και της όρασης. Η χρήση τους όμως θέλει προσοχή γιατί η υπερκατανάλωση αλλά και η νοθεία μπορεί να δημιουργήσουν σοβαρά προβλήματα.
On operator-valued monotone independence
Creators: name: Hasebe, Takahiro
name: Saigo, Hayato
Publisher: name: arXiv
Year: 2013
Subjects: subject: Operator Algebras (math.OA)
subject: FOS: Mathematics

description: We investigate operator-valued monotone independence, a noncommutative version of independence for conditional expectation. First we introduce operator-valued monotone cumulants to clarify the whole theory and show the moment-cumulant formula. As an application, one can obtain an easy proof of Central Limit Theorem for operator-valued case. Moreover, we prove a generalization of Muraki's formula for the sum of independent random variables and a relation between generating functions of moments and cumulants.
description: Proof of Theorem 3.4 is explained
Tauenstein, zum Steinernen Ecken
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1820

description: Ort: Zürich
description: Verzeichnung=Description=Inventaire 05.07.2020 Automatisiert nach HAN-Import
description: Verzeichnung=Description=Inventaire ISAD(G) / HAN Katalogisierungsregeln für Archivbestände Detailliert
Stierlin, Jacob Friedrich, jünger
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1820

description: Ort: Ebingen
description: Verzeichnung=Description=Inventaire 05.07.2020 Automatisiert nach HAN-Import
description: Verzeichnung=Description=Inventaire ISAD(G) / HAN Katalogisierungsregeln für Archivbestände Detailliert
Thuret & Co
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1820

description: Ort: Le Hâvre
description: Verzeichnung=Description=Inventaire 05.07.2020 Automatisiert nach HAN-Import
description: Verzeichnung=Description=Inventaire ISAD(G) / HAN Katalogisierungsregeln für Archivbestände Detailliert
Structural parameters of 11 faint Galactic globular clusters derived with 2MASS
Creators: name: Bonatto, C.
name: Bica, E.
Publisher: name: arXiv
Year: 2007
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The determination of structural parameters of 11 faint Galactic globular clusters that, in most cases, had not been previously studied in this context. The clusters are IC1257, Lynga7, Terzan4, Terzan10, BH176, ESO452-SC11, ESO280-SC08, 2MASS-GC01, 2MASS-GC02, GLIMPSE-C01 and AL3, which are projected not far from the central region of the Galaxy. Field-star contamination is significant in the colour-magnitude diagrams. Stellar radial number-density and surface-brightness profiles are built with 2MASS photometry that, for the present clusters, corresponds basically to giant-branch stars. Field-star decontamination is essential for clusters in dense fields. With decontaminated photometry we also compute the total MV of four such globular clusters, using M4 as a template. King-like functions are fitted to the radial profiles, from which the core, half-light, half-star count and tidal radii are derived, together with the concentration parameter. Parameters derived here are compared to the equivalent ones of other Galactic globular clusters available in the literature. Structural parameters and luminosity of most of the faint globular clusters dealt with in this paper are consistent with those of Palomar-like (low-mass and loose structure) globular clusters. This work helps to improve coverage of the globular cluster parameter space.
description: 11 pages, 9 figs. Accepted by A&A
Nonstationary analogue black holes
Creators: name: Eskin, Gregory
Publisher: name: arXiv
Year: 2013
Subjects: subject: Mathematical Physics (math-ph)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Analysis of PDEs (math.AP)
subject: FOS: Physical sciences
subject: FOS: Mathematics

description: We study the existence of analogue nonstationary spherically symmetric black holes. The prime example is the acoustic model (cf. [V], [U]). We consider also a more general class of metrics that could be useful in other physical models of analogue black and white holes. We give examples of the appearance of black holes and of disappearance of white holes. We also discuss the relation between the apparent and the event horizons for the case of analogue black holes. In the end we study the inverse problem of determination of black or white holes by boundary measurements for the spherically symmetric nonstationary metrics.
Structure of the Scalars
Creators: name: Pennington, M. R.
Publisher: name: arXiv
Year: 2007
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The PDG Tables list more scalar mesons than can fit into one quark model nonet: indeed, even more than can belong to two multiplets. Consequently, some of these must be states beyond the quark model. So which of these is ${\bar q}q$ or ${\bar{qq}}qq$ or multi-meson molecule or largely glue? How experiment can help us distinguish between these possibilities is discussed.
description: 12 pages, 5 figures. Invited talk at MENU 2007, 11th International Conference on Meson-Nucleon Physics and the Structure of the Proton, September 10-14, 2007, IKP, Forschungzentrum J\"ulich, Germany
The Robot is the Tether: Active, Adaptive Power Routing for Modular Robots With Unary Inter-robot Connectors
Creators: name: Campbell, Jason
name: Padmanabhan  Pillai
name: Goldstein, Seth C.
Publisher: name: Carnegie Mellon University
Year: 1979
Subjects: subject: 89999 Information and Computing Sciences not elsewhere classified
subject: FOS: Computer and information sciences

description: This paper describes a novel approach to powering a radical type of microrobot. Our long-term aim is to enable the construction of ensembles of millions of coordinated nearspherical, submillimeter microrobots. Both the large number of potential simultaneous neighbors of each robot (12) and the difficulty of fine actuation at such small scales preclude the use of complex connectors previously developed in many modular robotics efforts. Instead, we propose to leverage multirobot cooperation to simplify the mechanics of modular robot docking. In our approach, the robots actively cooperate to route virtual power busses (both supply and ground) to all the robots in the ensemble using only unary (single conductor) electrical connectors between robots. A unary connector allows for larger tolerances in engagement angle, simplifies robot manufacture, speeds reconfiguration, and maximizes the proportion of the connector surface area useful for carrying current. The algorithms we present permit a robot ensemble to efficiently harvest and distribute power from sources discovered in the environment and/or carried by the ensemble. We evaluate these algorithms in a variety of simulated deployment conditions and report on the impact of hardware defects, limited on-board power storage, and the ensemble-environment interface.
Particle energization through time-periodic helical magnetic fields
Creators: name: Mitra, Dhrubaditya
name: Brandenburg, Axel
name: Dasgupta, Brahmananda
name: Niklasson, Eyvind
name: Ram, Abhay
Publisher: name: arXiv
Year: 2013
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Chaotic Dynamics (nlin.CD)
subject: Space Physics (physics.space-ph)
subject: FOS: Physical sciences

description: We solve for the motion of charged particles in a helical time-periodic ABC (Arnold-Beltrami-Childress) magnetic field. The magnetic field lines of a stationary ABC field with coefficients $A=B=C=1$ are chaotic, and we show that the motion of a charged particle in such a field is also chaotic at late times with positive Lyapunov exponent. We further show that in time-periodic ABC fields, the kinetic energy of a charged particle can increase indefinitely with time. At late times the mean kinetic energy grows as a power law in time with an exponent that approaches unity. For an initial distribution of particles, whose kinetic energy is uniformly distributed within some interval, the PDF of kinetic energy is, at late times, close to a Gaussian but with steeper tails.
description: uses Revtex 4 instead of Revtex 4-1