cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Single-photon signals at LEP in supersymmetric models with a light gravitino
Creators: name: Lopez, J.
name: Nanopoulos, D.
name: Zichichi, A.
Publisher: name: arXiv
Year: 1996
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We study the single-photon signals expected at LEP in models with a very light gravitino. The dominant process is neutralino-gravitino production (e+e- -> chi+ G) with subsequent neutralino decay via chi->gamma+G, giving a gamma+E_miss signal. We first calculate the cross section at arbitrary center-of-mass energies and provide new analytic expressions for the differential cross section valid for general neutralino compositions. We then consider the constraints on the gravitino mass from LEP 1 and LEP161 single-photon searches, and possible such searches at the Tevatron. We show that it is possible to evade the stringent LEP 1 limits and still obtain an observable rate at LEP 2, in particular in the region of parameter space that may explain the CDF e+e+gamma+gamma+E_T,miss event. As diphoton events from neutralino pair-production would not be kinematically accessible in this scenario, the observation of whichever photonic signal will discriminate among the various light-gravitino scenarios in the literature. We also perform a Monte Carlo simulation of the expected energy and angular distributions of the emitted photon, and of the missing invariant mass expected in the events. Finally we specialize the results to the case of a recently proposed one-parameter no-scale supergravity model.
description: 31 pages, LaTeX, 14 figures (included)
title: ESLO1: entretien 073_A
Creators: name: Laboratoire Ligérien De Linguistique
name: Baude, Olivier
name: Dugua, Céline
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2015
Subjects: subject: Français
subject: fra
subject: text_and_corpus_linguistics

description: Extrait du corpus d'Orléans, réalisé dans le cadre de l'Enquête SocioLinguistique à Orléans à la fin des années 1960.
description: Conforms to: doi:10.34847/cocoon.69c4fa74-f324-3ddb-9f1a-580867fd5826
title: 02_0356
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/
Mean field theory for global binding systematics
Creators: name: Bertsch, G. F.
name: Hagino, K.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We review some possible improvements of mean field theory for application to nuclear binding systematics. Up to now, microscopic theory has been less successful than models starting from the liquid drop in describing accurately the global binding systematics. We believe that there are good prospects to develop a better global theory, using modern forms of energy density functionals and treating correlation energies systematically by the RPA.
description: RevTex, 17 pages, 5 eps figures. To be published in Yadernaya Fizika, special edition for the 90th birthday of Professor A.B. Migdal
title: ESLO1: entretien 075_A
Creators: name: Laboratoire Ligérien De Linguistique
name: Baude, Olivier
name: Dugua, Céline
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2015
Subjects: subject: Français
subject: fra
subject: text_and_corpus_linguistics

description: Extrait du corpus d'Orléans, réalisé dans le cadre de l'Enquête SocioLinguistique à Orléans à la fin des années 1960.
description: Conforms to: doi:10.34847/cocoon.69c4fa74-f324-3ddb-9f1a-580867fd5826
Searching for rotation in X-COP galaxy clusters
Creators: name: Bartalesi, Tommaso
name: Ettori, Stefano
name: Nipoti, Carlo
Publisher: name: arXiv
Year: 2025
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We search for evidence of rotational support by analyzing the thermodynamic profiles of the intracluster medium (ICM) in a sample of nearby, massive galaxy clusters. For each object of the XMM-Newton Cluster Outskirts Project (X-COP) sample, we present axisymmetric models of rotating ICM with composite polytropic distributions, in equilibrium in spherically symmetric dark halos, exploring cases both with and without turbulent support in the ICM. The profile of rotation velocity and the distribution of turbulent velocity dispersion are described with flexible functional forms, consistent with the properties of synthetic clusters formed in cosmological simulations. The models are tuned via a Markov Chain Monte Carlo algorithm to reproduce the radial profiles of the thermodynamic variables as resolved in the XMM-Newton and Planck maps, and to be consistent with the mass distributions estimated either from weak lensing observations (when available) or under the assumption of a "universal" value of the baryon fraction. Our models indicate that there is room for non-negligible rotation in the ICM of massive clusters, with typical peak rotation speed 300 km/s and peak rotation-velocity-to-velocity-dispersion ratio of 0.3. According to our models, the ICM in Abell 2255 can have a rotation speed as high as 500 km/s, corresponding to a rotation-velocity-to-velocity-dispersion ratio of 0.3, at a distance of 100 kpc from the center, where the X-ray emissivity is still high. This makes Abell 2255 a very promising candidate for the presence of rotation in the ICM that could be detected with the currently operating XRISM observatory, as we demonstrate computing and analyzing a mock X-ray spectrum.
description: 25 pages, 16 figures
Collisional versus Collisionless Dark Matter
Creators: name: Moore, Ben
name: Gelato, Sergio
name: Jenkins, Adrian
name: Pearce, F. R.
name: Quilis, Vicent
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We compare the structure and substructure of dark matter halos in model universes dominated by collisional, strongly self interacting dark matter (SIDM) and collisionless, weakly interacting dark matter (CDM). While SIDM virialised halos are more nearly spherical than CDM halos, they can be rotationally flattened by as much as 20% in their inner regions. Substructure halos suffer ram-pressure truncation and drag which are more rapid and severe than their gravitational counterparts tidal stripping and dynamical friction. Lensing constraints on the size of galactic halos in clusters are a factor of two smaller than predicted by gravitational stripping, and the recent detection of tidal streams of stars escaping from the satellite galaxy Carina suggests that its tidal radius is close to its optical radius of a few hundred parsecs --- an order of magnitude smaller than predicted by CDM models but consistent with SIDM. The orbits of SIDM satellites suffer significant velocity bias $σ_{SIDM}/σ_{CDM}=0.85$ and are more circular than CDM, $β_{SIDM}} \approx 0.5$, in agreement with the inferred orbits of the Galaxy's satellites. In the limit of a short mean free path, SIDM halos have singular isothermal density profiles, thus in its simplest incarnation SIDM is inconsistent with galactic rotation curves.
description: 4 pages, submitted to ApJLetters. Further simulation details at http://www.nbody.net (www.nbody.net)
Conformal gravity: light deflection revisited and the galactic rotation curve failure
Creators: name: Campigotto, M. C.
name: Diaferio, A.
name: Fatibene, L.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We show how Conformal Gravity (CG) has to satisfy a fine-tuning condition to describe the rotation curves of disk galaxies without the aid of dark matter. Interpreting CG as a gauge natural theory yields conservation laws and their associated superpotentials without ambiguities. We consider the light deflection of a point-like lens and impose that the two Schwarzschild-like metrics with and without the lens are identical at infinite distances from the lens. The energy conservation law implies that the parameter $γ$ in the linear term of the metric has to vanish, otherwise the two metrics are physically inaccessible from each other. This linear term is responsible to mimic the role of dark matter in disk galaxies and gravitational lensing systems. Our analysis shows that removing the need of dark matter with CG thus relies on a fine-tuning condition on $γ$. We also illustrate why the results of previous investigations of gravitational lensing in CG largely disagree. These discrepancies derive from the erroneous use of the deflection angle definition adopted in General Relativity, where the vacuum solution is asymptotically flat, unlike CG. In addition, the lens mass is identified with various combinations of the metric parameters. However, these identifications are arbitrary, because the mass is not a conformally invariant quantity, unlike the conserved charge associated to the energy conservation law. Based on this conservation law and by removing the fine-tuning condition on $γ$, i.e. by setting $γ=0$, the energy difference between the metric with the point-like lens and the metric without it defines a conformally invariant quantity that can in principle be used for (1) a proper derivation of light deflection in CG, and (2) the identification of the lens mass with a function of the parameters $β$ and $k$ of the Schwarzschild-like metric.
description: 16 pages, 1 figure. Revised version according to the referees comments. The results reported in the original version remain unchanged
title: ESLO1: entretien 076_A
Creators: name: Laboratoire Ligérien De Linguistique
name: Baude, Olivier
name: Dugua, Céline
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2015
Subjects: subject: Français
subject: fra
subject: text_and_corpus_linguistics

description: Extrait du corpus d'Orléans, réalisé dans le cadre de l'Enquête SocioLinguistique à Orléans à la fin des années 1960.
description: Conforms to: doi:10.34847/cocoon.69c4fa74-f324-3ddb-9f1a-580867fd5826
Analytic perturbation theory in QCD and Schwinger's connection between the beta-function and the spectral density
Creators: name: Milton, K. A.
name: Solovtsov, I. L.
Publisher: name: arXiv
Year: 1996
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We argue that a technique called analytic perturbation theory leads to a well-defined method for analytically continuing the running coupling constant from the spacelike to the timelike region, which allows us to give a self-consistent definition of the running coupling constant for timelike momentum. The corresponding $β$-function is proportional to the spectral density, which confirms a hypothesis due to Schwinger.
description: 11 pages, 2 figures
Additional file 10: of Acute effects of combined exercise and oscillatory positive expiratory pressure therapy on sputum properties and lung diffusing capacity in cystic fibrosis: a randomized, controlled, crossover trial
Creators: name: Radtke, Thomas
name: Bรถni, Lukas
name: Bohnacker, Peter
name: Maggi-Beba, Marion
name: Fischer, Peter
name: Kriemler, Susi
name: Benden, Christian
name: Dressel, Holger
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Space Science
subject: Medicine
subject: Biotechnology
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics

description: Figure S5. Instrument inertia in cystic fibrosis sputum shear rheology measurements (DOCX 978 kb)
The Approximate Duality Gap Technique: A Unified Theory of First-Order Methods
Creators: name: Diakonikolas, Jelena
name: Orecchia, Lorenzo
Publisher: name: arXiv
Year: 2017
Subjects: subject: Optimization and Control (math.OC)
subject: Data Structures and Algorithms (cs.DS)
subject: FOS: Mathematics
subject: FOS: Computer and information sciences

description: We present a general technique for the analysis of first-order methods. The technique relies on the construction of a duality gap for an appropriate approximation of the objective function, where the function approximation improves as the algorithm converges. We show that in continuous time enforcement of an invariant that this approximate duality gap decreases at a certain rate exactly recovers a wide range of first-order continuous-time methods. We characterize the discretization errors incurred by different discretization methods, and show how iteration-complexity-optimal methods for various classes of problems cancel out the discretization error. The techniques are illustrated on various classes of problems -- including convex minimization for Lipschitz-continuous objectives, smooth convex minimization, composite minimization, smooth and strongly convex minimization, solving variational inequalities with monotone operators, and convex-concave saddle-point optimization -- and naturally extend to other settings.
description: In SIAM Journal on Optimization. The most recent version corrected a few typos
Properties of superdeformed fission isomers in the cranked relativistic Hartree-Bogoliubov theory
Creators: name: Afanasjev, A. V.
name: Ring, P.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: The rotational and deformation properties of superdeformed fission isomers in the $A\sim 240$ mass region have been investigated within the framework of the cranked relativistic Hartree-Bogoliubov theory. The dependence of the results of the calculations on the parametrization of the RMF Lagrangian has been studied. The rotational properties are best described by the NL1 force.
description: 5 pages, uses epsf.sty and hip-artc.sty, 1 PostScript figure, contribution to the Proceedings of the International Symposium on Exotic Nuclear Structures, May 15-20, 2000, Debrecen, Hungary
title: ESLO1: entretien 078_A
Creators: name: Laboratoire Ligérien De Linguistique
name: Baude, Olivier
name: Dugua, Céline
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2015
Subjects: subject: Français
subject: fra
subject: text_and_corpus_linguistics

description: Extrait du corpus d'Orléans, réalisé dans le cadre de l'Enquête SocioLinguistique à Orléans à la fin des années 1960.
description: Conforms to: doi:10.34847/cocoon.69c4fa74-f324-3ddb-9f1a-580867fd5826
Additional file 3: of Genome sequencing analysis of Streptomyces coelicolor mutants that overcome the phosphate-depending vancomycin lethal effect
Creators: name: Santos-Beneit, Fernando
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Space Science
subject: Microbiology
subject: FOS: Biological sciences
subject: Evolutionary Biology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: Computational Biology

description: Table S2. Analysis of the effect of coupling SCO1212 and SCO1213 to pVJ and pVJc on the growth of the next strains: SC100 (S. coelicolor M145-pVJ-1212; isolate 1), SC101 (S. coelicolor M145-pVJ-1212; isolate 2), SC102 (S. coelicolor M145-pVJc-1212; isolate 1), SC103 (S. coelicolor M145-pVJc-1212; isolate 2), SC104 (S. coelicolor M145-pVJ-1213; isolate 1), SC105 (S. coelicolor M145-pVJ-1213; isolate 2), SC106 (S. coelicolor M145-pVJc-1213; isolate 1), SC107 (S. coelicolor M145-pVJc-1213; isolate 2) in DifcoNA (with or without 1% K2HPO4 addition) and different concentrations of lysozyme, vancomycin and teicoplanin. The concentration of the compounds is shown as Îźg per mL. (DOCX 15 kb)
Formation and evolution of disk galaxies within cold dark matter halos
Creators: name: Avila-Reese, V.
name: Firmani, C.
name: Klypin, A.
name: Kravtsov, A. V.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present results of extensive model calculations of disk galaxy evolution within an hierarchical inside-out formation scenario. We first compare properties of the dark halos identified in a cosmological N-body simulation with predictions of a seminumerical method based on an extended collapse model and find a good agreement. We also study the properties of the halos in dependence on their environment. We then describe detailed modelling of the formation and evolution of disks within the growing isolated cold dark matter halos and predictions for the main properties, correlations and evolutionary features of normal disk galaxies. The possible shortcomings of the scenario are discussed.
description: 4 pages. To appear in "Cosmic Evolution and Galaxy Formation: Structure, Interactions and Feedback", Eds. J.Franco, E.Terlevich, O.Lopez-Cruz, I.Aretxaga, ASP Conf. Series
title: ESLO1: entretien 079_A
Creators: name: Laboratoire Ligérien De Linguistique
name: Baude, Olivier
name: Dugua, Céline
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2015
Subjects: subject: Français
subject: fra
subject: text_and_corpus_linguistics

description: Extrait du corpus d'Orléans, réalisé dans le cadre de l'Enquête SocioLinguistique à Orléans à la fin des années 1960.
description: Conforms to: doi:10.34847/cocoon.69c4fa74-f324-3ddb-9f1a-580867fd5826
Figure-of-eight velocity curves: UGC10205
Creators: name: Vega, J. C.
name: Corsini, E. M.
name: Pizzella, A.
name: Bertola, F.
Publisher: name: arXiv
Year: 1997
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We measured the velocity curve and the velocity dispersion profile of the ionized gas along the major axis of the edge-on galaxy UGC~10205. The observed kinematics extends up to about 40 arcsec from the nucleus. In the inner 13 arcsec of this early-type spiral three kinematically distinct gaseous components are present. We disentangle a fast-rotating and a slow-rotating component. They give to the UGC10205 velocity curve a ``figure-of-eight'' appearance. A third velocity component is also detected on the southeast side of the galaxy. Possibly it is produced by gas in non-circular motions.
description: 8 pages, 3 figures, Latex macro A&A and psfig macro to insert figures
MOESM1 of A new GIS model for ecologically suitable distributions of medicinal plants
Creators: name: Wu, Jie
name: Li, Xiwen
name: Huang, Linfang
name: Meng, Xiangxiao
name: Hu, Haoyu
name: Luo, Lu
name: Chen, Shilin
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Chemical Sciences not elsewhere classified
subject: Ecology
subject: FOS: Biological sciences
subject: Biological Sciences not elsewhere classified
subject: Mathematical Sciences not elsewhere classified

description: Additional file 1: Table S1. Calculation of Euclidean distance. Table S2. Classification of raster. Table S3. Calculation of suitable soil. Table S4. Summary of published species.
Cosmic Strings in Theories With Dynamical Symmetry Breaking
Creators: name: Brandenberger, R.
name: Huang, T.
name: Yang, K.
name: Zhang, X.
Publisher: name: arXiv
Year: 1996
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We study the classical cosmic string solution in a theory with dynamical $U(1)$ symmetry breaking. We calculate the energy per unit length of the string and compare it to that obtained in a model with a fundamental Higgs. We find that the predictions of the standard Abelian Higgs model are quite stable towards the addition of higher dimension operators expected in the effective Lagrangian for the order parameter in a model with dynamical symmetry breaking, at least for small coupling constant $λ$.
description: 10 pages, 3 figures, uses LATEX
title: ESLO1: entretien 080_A
Creators: name: Laboratoire Ligérien De Linguistique
name: Baude, Olivier
name: Dugua, Céline
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2015
Subjects: subject: Français
subject: fra
subject: text_and_corpus_linguistics

description: Extrait du corpus d'Orléans, réalisé dans le cadre de l'Enquête SocioLinguistique à Orléans à la fin des années 1960.
description: Conforms to: doi:10.34847/cocoon.69c4fa74-f324-3ddb-9f1a-580867fd5826
Good Research Practice Courses
Creators: name: Center For Reproducible Science
name: Gonzalez, Gorka Fraga
name: Held, Leonhard
name: Wiel, Hester Vd
name: Molo, Fabio
name: Schwab, Simon
name: Furrer, Eva
name: Heyard, Rachel
Publisher: name: OSF
Year: 2018
Subjects: Good research practice
Reproducibility

description: This repository contains the full course materials which we designed and teach at the University of Zurich.
Bulk-edge correspondence and new topological phases in periodically driven spin-orbit coupled materials in the low frequency limit
Creators: name: Saxena, Ruchi
name: Rao, Sumathi
name: Kundu, Arijit
Publisher: name: arXiv
Year: 2017
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We study the topological phase transitions induced in spin-orbit coupled materials with buckling like silicene, germanene, stanene, etc, by circularly polarised light, beyond the high frequency regime, and unearth many new topological phases. These phases are characterised by the spin-resolved topological invariants, $C_0^\uparrow$, $C_0^\downarrow$, $C_π^\uparrow$ and $C_π^\downarrow$, which specify the spin-resolved edge states traversing the gaps at zero quasi-energy and the Floquet zone boundaries respectively. We show that for each phase boundary, and independently for each spin sector, the gap closure in the Brillouin zone occurs at a high symmetry point.
title: ESLO1: entretien 081_A
Creators: name: Laboratoire Ligérien De Linguistique
name: Baude, Olivier
name: Dugua, Céline
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2015
Subjects: subject: Français
subject: fra
subject: text_and_corpus_linguistics

description: Extrait du corpus d'Orléans, réalisé dans le cadre de l'Enquête SocioLinguistique à Orléans à la fin des années 1960.
description: Conforms to: doi:10.34847/cocoon.69c4fa74-f324-3ddb-9f1a-580867fd5826
THE LIVED COMMUNICATION EXPERIENCES OF SPECIAL EDUCATION TEACHERS AT MILLER COUNTY SCHOOLS
Creators: name: SALES, ROM KENNETH BUGLOSA
Publisher: name: Zenodo
Year: 2023

description: This phenomenological study was conducted to shed light on the lived communication experiences of the special education teachers at Miller County Schools. The qualitative approach used unstructured interviews to give a voice to the five respondents. The question prompts were based on the observation of self-contained and inclusive classes, IEP meetings, and parent conferences. Making sense of the lived communicative experiences of the special education teachers, the concept of cognizant-sensitive communication emerged. My inquiry revealed that cognizant-sensitive communication in special education allows for improving students’ achievement in case it constitutes the essential basis of all teaching, learning and communication processes. Cognizant-sensitive communication strategies allow appropriate approaches and emphasize the value of equality as conditions necessary to create a full-fledged process of communication, teaching and learning with students with special needs. Teacher-parent communication highlighted the need of understanding, building relationships, and truthful feedback. On the other hand, the inside and outside the classroom communication challenges revealed five themes, namely: misunderstanding; behavioral issues; lack of response; unclear understanding of the children’s special needs, and struggle to adapt to the changes. Recommendations and solutions to the communication challenges outlined the last two themes consisting of awareness and sensitivity and prioritizing students’ interests. Hence, cognizant-sensitive communication was theorized. It refers to the process where the messenger delves deeper into the abilities, thoughts, interests, and even limitations of the receiver to formulate, select, structure, and relay the message. This phenomenon is common among the lived communication experiences of the special education teachers.
Conservative descent for semi-orthogonal decompositions
Creators: name: Bergh, Daniel
name: Schnürer, Olaf M.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Algebraic Geometry (math.AG)
subject: FOS: Mathematics

description: Motivated by the local flavor of several well-known semi-orthogonal decompositions in algebraic geometry, we introduce a technique called conservative descent, which shows that it is enough to establish these decompositions locally. The decompositions we have in mind are those for projectivized vector bundles and blow-ups, due to Orlov, and root stacks, due to Ishii and Ueda. Our technique simplifies the proofs of these decompositions and establishes them in greater generality for arbitrary algebraic stacks.
description: Final version
title: ESLO1: entretien 083_A
Creators: name: Laboratoire Ligérien De Linguistique
name: Baude, Olivier
name: Dugua, Céline
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2015
Subjects: subject: Français
subject: fra
subject: text_and_corpus_linguistics

description: Extrait du corpus d'Orléans, réalisé dans le cadre de l'Enquête SocioLinguistique à Orléans à la fin des années 1960.
description: Conforms to: doi:10.34847/cocoon.69c4fa74-f324-3ddb-9f1a-580867fd5826
Time-odd mean fields in the rotating frame: microscopic nature of nuclear magnetism
Creators: name: Afanasjev, A. V.
name: Ring, P.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: The microscopic role of nuclear magnetism in rotating frame is investigated for the first time in the framework of the cranked relativistic mean field theory. It is shown that nuclear magnetism modifies the expectation values of single-particle spin, orbital and total angular momenta along the rotational axis effectively creating additional angular momentum. This effect leads to the increase of kinematic and dynamic moments of inertia at given rotational frequency and has an impact on effective alignments.
description: 16 pages, 4 figures, submitted to Physical Review C
Additional file 2: of Genome sequencing analysis of Streptomyces coelicolor mutants that overcome the phosphate-depending vancomycin lethal effect
Creators: name: Santos-Beneit, Fernando
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Space Science
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Molecular Biology
subject: Biotechnology
subject: Evolutionary Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: 60506 Virology
subject: Computational Biology

description: Table S1. Analysis of the growth of L2 and L4 complemented strains grown in DifcoNA (with or without 1% K2HPO4 addition) and different concentrations of lysozyme, vancomycin and teicoplanin. The concentration of the compounds is shown as Îźg per mL. (DOCX 16 kb)
Омана планування: класифікація
Creators: name: Shatilova, Oleksandra
Publisher: name: figshare
Year: 2024
Subjects: classificationCode: 520104
subject: Industrial and organisational psychology (incl. human factors)

description: Шатілова О. Омана планування: класифікація. Вектори соціальної, організаційної та економічної психології : тези доп. IIІ Міжнар. наук.-практ. конф., м. Київ, 23 лют. 2024 р. Київ, 2024. С. 330–332. URL: https://doi.org/10.6084/m9.figshare.25412191
title: ESLO1: entretien 082_A
Creators: name: Laboratoire Ligérien De Linguistique
name: Baude, Olivier
name: Dugua, Céline
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2015
Subjects: subject: Français
subject: fra
subject: text_and_corpus_linguistics

description: Extrait du corpus d'Orléans, réalisé dans le cadre de l'Enquête SocioLinguistique à Orléans à la fin des années 1960.
description: Conforms to: doi:10.34847/cocoon.69c4fa74-f324-3ddb-9f1a-580867fd5826
Compact groups from semi-analytical models of galaxy formation -- VI: Evolution of the two first-ranked galaxies
Creators: name: Zandivarez, A.
name: Diaz-Gimenez, E.
Publisher: name: arXiv
Year: 2025
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: [Abridged] Compact groups (CGs) of galaxies have proven to be unique environments for studying galaxy interactions. We propose a detailed analysis of the galaxy evolution to disentangle the relationship between the two first-ranked galaxies in CGs throughout their history as a function of the assembly channels of their hosts. Our study was performed from a semi-analytical point of view, using more than 20000 CGs. We based our analysis on studying the first- (1R) and second-ranked (2R) galaxies in CGs, where the ranking is determined using the galaxy stellar mass. The 1R galaxies have significantly reduced their star-forming capacity over time, reaching a quenching stage and often becoming bulge-dominated or elliptical. Notably, this transformation occurred earlier for 1R galaxies in early-formed CGs (around 5 to 8 Gyrs ago), while those in recently-formed CGs experienced this change more recently (around 2 to 3 Gyrs ago). The analysis of the time evolution of a variant of the Tremaine & Richstone statistics showed that the 1R galaxy in early-formed CGs began to stand out for its dominant properties around 6 Gyrs ago, almost 5 Gyrs earlier than the 1R inhabiting recently formed CGs. We observed that a large majority of the 1R galaxies have experienced at least one major merger event during their life, while we observed this only for a third of 2R galaxies. The 1R galaxies can also display several of these events and most of their last major merger events can be described as the addition of a progenitor that is the second most massive galaxy in their surroundings at the time of the merger. We find that the semi-analytical framework explored in this work describes a scenario where galaxy mergers are the main driving force in shaping the properties of the 1R galaxies in CGs. We note that this scenario is especially intensive when those galaxies inhabit CGs that had formed early on.
description: 13 pages, 7 figures, 1 table, accepted for publication in A&A
The Mass-To-Light Function: Antibias and Omega_m
Creators: name: Bahcall, N. A.
name: Cen, R.
name: Davé, R.
name: Ostriker, J. P.
name: Yu, Q.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We use large-scale cosmological simulations to estimate the mass-to-light ratio of galaxy systems as a function of scale, and compare the results with observations of galaxies, groups, clusters, and superclusters of galaxies. We find remarkably good agreement between observations and simulations. Specifically, we find that the simulated mass-to-light ratio increases with scale on small scales and flattens to a constant value on large scales, as suggested by observations. We find that while mass typically follows light on large scales, high overdensity regions --- such as rich clusters and superclusters of galaxies --- exhibit higher M/L_B values than average, while low density regions exhibit lower M/L_B values; high density regions are thus antibiased in M/L_B, with mass more strongly concentrated than blue light. This is true despite the fact that the galaxy mass density is unbiased or positively biased relative to the total mass density in these regions. The M/L_B antibias is likely due to the relatively old age of the high density regions, where light has declined significantly since their early formation time, especially in the blue band which traces recent star formation. Comparing the simulated results with observations, we place a powerful constraint on the mass density of the universe; using, for the first time, the entire observed mass-to-light function, from galaxies to superclusters, we find Omega =0.16+/-0.05.
description: 26 pages, 4 figs, minor changes, to be published in ApJ, Vol.541 (Oct.1, 2000)
On gauging finite subgroups
Creators: name: Tachikawa, Yuji
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We study in general spacetime dimension the symmetry of the theory obtained by gauging a non-anomalous finite normal Abelian subgroup $A$ of a $Γ$-symmetric theory. Depending on how anomalous $Γ$ is, we find that the symmetry of the gauged theory can be i) a direct product of $G=Γ/A$ and a higher-form symmetry $\hat A$ with a mixed anomaly, where $\hat A$ is the Pontryagin dual of $A$; ii) an extension of the ordinary symmetry group $G$ by the higher-form symmetry $\hat A$; iii) or even more esoteric types of symmetries which are no longer groups. We also discuss the relations to the effect called the $H^3(G,\hat A)$ symmetry localization obstruction in the condensed-matter theory and to some of the constructions in the works of Kapustin-Thorngren and Wang-Wen-Witten.
description: 26 pages; v3: numerous minor improvements suggested by an anonymous referee; v2: minor improvement in Sec. 2.6.1
Additional file 1: of â Doing hymen reconstructionâ : an analysis of perceptions and experiences of Flemish gynaecologists
Creators: name: Leye, Els
name: Emilomo Ogbe
name: Heyerick, Maaike
Publisher: name: figshare
Year: 2018
Subjects: subject: Cell Biology
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Developmental Biology

description: Questionnaire in English. (PDF 71 kb)
MOESM2 of A new GIS model for ecologically suitable distributions of medicinal plants
Creators: name: Wu, Jie
name: Li, Xiwen
name: Huang, Linfang
name: Meng, Xiangxiao
name: Hu, Haoyu
name: Luo, Lu
name: Chen, Shilin
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Molecular Biology
subject: Biotechnology
subject: Environmental Sciences not elsewhere classified
subject: Ecology
subject: FOS: Biological sciences
subject: Biological Sciences not elsewhere classified

description: Additional file 2. Minimum Standards of Reporting Checklist.
title: ESLO1: entretien 084_A
Creators: name: Laboratoire Ligérien De Linguistique
name: Baude, Olivier
name: Dugua, Céline
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2015
Subjects: subject: Français
subject: fra
subject: text_and_corpus_linguistics

description: Extrait du corpus d'Orléans, réalisé dans le cadre de l'Enquête SocioLinguistique à Orléans à la fin des années 1960.
description: Conforms to: doi:10.34847/cocoon.69c4fa74-f324-3ddb-9f1a-580867fd5826
Motion Tomography of a single trapped ion
Creators: name: Poyatos, J. F.
name: Walser, R.
name: Cirac, J. I.
name: Zoller, P.
name: Blatt, R.
Publisher: name: arXiv
Year: 1996
Subjects: subject: Atomic Physics (physics.atom-ph)
subject: FOS: Physical sciences

description: A method for the experimental reconstruction of the quantum state of motion for a single trapped ion is proposed. It is based on the measurement of the ground state population of the trap after a sudden change of the trapping potential. In particular, we show how the Q function and the quadrature distribution can be measured directly. In an example we demonstrate the principle and analyze the sensibility of the reconstruction process to experimental uncertainties as well as to finite grid limitations. Our method is not restricted to the Lamb-Dicke Limit and works in one or more dimensions.
description: 4 pages, Revtex format, 4 postscript figures, changed typographical errors
title: ESLO1: entretien 085_A
Creators: name: Laboratoire Ligérien De Linguistique
name: Baude, Olivier
name: Dugua, Céline
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2015
Subjects: subject: Français
subject: fra
subject: text_and_corpus_linguistics

description: Extrait du corpus d'Orléans, réalisé dans le cadre de l'Enquête SocioLinguistique à Orléans à la fin des années 1960.
description: Conforms to: doi:10.34847/cocoon.69c4fa74-f324-3ddb-9f1a-580867fd5826
Additional file 1: of Evaluation of the reliability, usability, and applicability of AMSTAR, AMSTAR 2, and ROBIS: protocol for a descriptive analytic study
Creators: name: Gates, Allison
name: Gates, Michelle
name: Gonรงalo Duarte
name: Cary, Maria
name: Becker, Monika
name: Prediger, Barbara
name: Vandermeer, Ben
name: Fernandes, Ricardo
name: Pieper, Dawid
name: Hartling, Lisa
Publisher: name: figshare
Year: 2018
Subjects: subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Items and response options on the AMSTAR, AMSTAR 2, and ROBIS tools. Provides an overview of the items and response options on the AMSTAR, AMSTAR 2, and ROBIS tools. (DOCX 20 kb)
title: ESLO1: entretien 087_A
Creators: name: Laboratoire Ligérien De Linguistique
name: Baude, Olivier
name: Dugua, Céline
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2015
Subjects: subject: Français
subject: fra
subject: text_and_corpus_linguistics

description: Extrait du corpus d'Orléans, réalisé dans le cadre de l'Enquête SocioLinguistique à Orléans à la fin des années 1960.
description: Conforms to: doi:10.34847/cocoon.69c4fa74-f324-3ddb-9f1a-580867fd5826
Queues on a dynamically evolving graph
Creators: name: Mandjes, Michel
name: Starreveld, Nicos
name: Bekker, René
Publisher: name: arXiv
Year: 2017
Subjects: subject: Probability (math.PR)
subject: FOS: Mathematics

description: This paper considers a population process on a dynamically evolving graph, which can be alternatively interpreted as a queueing network. The queues are of infinite-server type, entailing that at each node all customers present are served in parallel. The links that connect the queues have the special feature that they are unreliable, in the sense that their status alternates between 'up' and 'down'. If a link between two nodes is down, with a fixed probability each of the clients attempting to use that link is lost; otherwise the client remains at the origin node and reattempts using the link (and jumps to the destination node when it finds the link restored). For these networks we present the following results: (a) a system of coupled partial differential equations that describes the joint probability generating function corresponding to the queues' time-dependent behavior (and a system of ordinary differential equations for its stationary counterpart), (b) an algorithm to evaluate the (time-dependent and stationary) moments, and procedures to compute user-perceived performance measures which facilitate the quantification of the impact of the links' outages, (c) a diffusion limit for the joint queue length process.We include explicit results for a series relevant special cases, such as tandem networks and symmetric fully connected networks.
Baryogenesis from baryon number violating scalar interactions
Creators: name: Bowes, J. P.
name: Volkas, R. R.
Publisher: name: arXiv
Year: 1996
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: In the following work we consider the possibility of explaining the observed baryon number asymmetry in the universe from simple baryon number violating modifications, involving massive scalar bosons, to the Standard Model. In these cases baryon number violation is mediated through a combination of Yukawa and scalar self-coupling interactions. Starting with a previously compiled catalogue of baryon-number violating extensions of the Standard Model, we identify the minimal subsets which can induce a $B-L$ asymmetry and thus be immune to sphaleron washout. For each of these models, we identify the region of parameter space that leads to the production of a baryon number asymmetry of the correct order of magnitude.
description: 14 pages, 3 Postscript figures
title: ESLO1: entretien 086_A
Creators: name: Laboratoire Ligérien De Linguistique
name: Baude, Olivier
name: Dugua, Céline
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2015
Subjects: subject: Français
subject: fra
subject: text_and_corpus_linguistics

description: Extrait du corpus d'Orléans, réalisé dans le cadre de l'Enquête SocioLinguistique à Orléans à la fin des années 1960.
description: Conforms to: doi:10.34847/cocoon.69c4fa74-f324-3ddb-9f1a-580867fd5826
On the origin of the color Tully-Fisher and color-magnitude relations of disk galaxies
Creators: name: Avila-Reese, V.
name: Firmani, C.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We propose and show that the dependence of the internal face-on dust absorption upon B-band luminosity reported by Wang & Heckman (1996) for a sample of late-type galaxies may explain the empirical color-magnitude and color Tully-Fisher relations of disk galaxies. Thus, in order to explain these relations, it is not necessary to evoke star formation and gas infall efficiencies dependent on the mass of the galaxy system. After applying the Wang & Heckman's luminosity-dependent extinction to hierarchical inside-out galaxy formation and evolution models where the star formation and gas infall efficiencies do not significantly depend on mass, we succesfully predict the observed Tully-Fisher relations in the H and B bands as well as the color-magnitude relation.
description: 1 page. To appear in ``Cosmic Evolution and Galaxy Formation: Structure, Interactions and Feedback'', Eds. J.Franco, E.Terlevich, O.Lopez-Cruz, I.Aretxaga, ASP Conf. Series
CoCCoA: Complex Chemistry in hot Cores with ALMA. The chemical evolution of acetone from ice to gas
Creators: name: Chen, Y.
name: Garrod, R. T.
name: Rachid, M.
name: van Dishoeck, E. F.
name: Brogan, C. L.
name: Loomis, R.
name: Lipnicky, A.
name: McGuire, B. A.
Publisher: name: arXiv
Year: 2025
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Chemical Physics (physics.chem-ph)
subject: FOS: Physical sciences

description: Acetone (CH3COCH3) is one of the most abundant three-carbon oxygen-bearing complex organic molecules (O-COMs) that have been detected in space. Recently, acetone ice has been reported as (tentatively) detected toward B1-c, which enables the gas-to-ice comparison of its abundances. The detection of acetone ice warrants a more systematic study of its gaseous abundances which is currently lacking. Therefore, we conducted systematic measurements of acetone gas in a dozen hot cores observed by the CoCCoA survey and investigate the chemical evolution from ice to gas of acetone in protostellar systems. We fit the ALMA spectra to determined the column density, excitation temperature, and line width of acetone, along with propanal (C2H5CHO), ketene (CH2CO), and propyne (CH3CCH), which might be chemically linked with acetone. We found that the observed gas abundances of acetone are surprisingly high compared to those of two-carbon O-COMs, while aldehydes are overall less abundant than other O-COMs (e.g., alcohols, ethers, and esters). This may suggest specific formation or destruction mechanisms that favor the production of ethers, esters, and ketones over aldehydes. The derived physical properties suggest that acetone, propanal, and ketene have the same origin from hot cores as other O-COMs, while propyne tends to trace the more extended outflows. The acetone-to-methanol ratios are higher in ice than in gas by one order of magnitude, hinting at gas-phase reprocessing after sublimation. There are several suggested formation pathways of acetone (in both ice and gas) from acetaldehyde (CH3CHO), ketene, and propylene (C3H6). The observed ratios between acetone and the relevant species are rather constant across the sample, and can be well reproduced by astrochemical simulations, but more investigations are needed to draw solid conclusions.
description: Accepted for publication in A&A. Main text: 14 pages, 9 figures, 1 table; appendix: 19 pages, 14 figures, 2 tables
Adiabatic mechanism of the multiply charged ion production by a laser field through ATI states of an atom
Creators: name: Kuchiev, M. Yu.
Publisher: name: arXiv
Year: 1996
Subjects: subject: Atomic Physics (physics.atom-ph)
subject: FOS: Physical sciences

description: ATI can be followed by an inelastic collision of the ionized electron with the parent atomic particle resulting in an excitation of the ion. It may be a continuum state excitation producing the doubly charged ion or a discrete state which also enhances the doubly charged ion production. Absorption of a few quanta above the atomic threshold is sufficient to make this mechanism work. As a result the two-electron processes can take place even in moderate fields. The example of two-electron excitations of He atoms in a 780 nm laser field with intensity above $ 10^{14}$W/cm$^2$ is discussed
description: 12 pages, Revtex, 1 Postscript figure. Accepted for publication in Phys.Lett.A