cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Plastic Response of a 2D Lennard-Jones amorphous solid: Detailed analysis of the local rearrangements at very slow strain-rate
Creators: name: Tanguy, Anne
name: Leonforte, Fabien
name: Barrat, J. -L.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: We analyze in details the atomistic response of a model amorphous material submitted to plastic shear in the athermal, quasistatic limit. After a linear stress-strain behavior, the system undergoes a noisy plastic flow. We show that the plastic flow is spatially heterogeneous. Two kinds of plastic events occur in the system: quadrupolar localized rearrangements, and shear bands. The analysis of the individual motion of a particle shows also two regimes: a hyper-diffusive regime followed by a diffusive regime, even at zero temperature.
title: ADCO, Ordre cistercien et abbaye de Cîteaux : comptes pour l'ordre (1337-1347), comptes du boursier (1377-1402) (11 H 1160), f. 00416
Creators: name: de la Côte-d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CBMA/CG21/F.PETOT/2017
name: Petot, Frédéric
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: comptes

description: Ordre cistercien et abbaye de Cîteaux : comptes pour l'ordre (1337-1347), comptes du boursier (1377-1402), Archives départementales de la Côte-d'Or, (11 H 1160). Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Ordre cistercien et abbaye de Cîteaux : comptes pour l'ordre (1337-1347), comptes du boursier (1377-1402), Archives départementales de la Côte-d'Or, (11 H 1160), f. 00416, in Projet CBMA - Corpus Burgundiae Medii Aevi \[Ressource en ligne\], https:// manuscrits.cbma-project.eu/
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
Using design specifications for design
Creators: name: Holtz, Neal M.
name: Fenves, Steven J(Steven Joseph)
Publisher: name: Carnegie Mellon University
Year: 1981
Subjects: subject: 90799 Environmental Engineering not elsewhere classified
subject: FOS: Environmental engineering
subject: 90599 Civil Engineering not elsewhere classified
subject: FOS: Civil engineering

description: technical report
On the Possibility of Local SR Construction
Creators: name: Kotel'nikov, G. A.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Classical Physics (physics.class-ph)
subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The violation of the invariance of the speed of light in Special Relativity has been made. The version of the theory (LSR) has been constructed in which the possibility of the superluminal motions are permitted. Some predictions of this theory are available for experimental check, for example, the measurements of aberration angles, the observation of distinctions between the redshifts in radio and optical ranges of a spectrum, the detection of superluminal objects in astrophysics and in time-flight experiments.
description: 13 pages, LaTeX, Report at the VI International Conference "Modern Problems of Natural Science", S.-Petersburg, Russia, August 21-25, 2000
title: Comprehensive Economic Development Strategy for Berkshire County, Massachusetts
Creators: name: (:Unkn) Unknown
Publisher: name: University of Massachusetts Amherst
Year: 2001
Subjects: subject: Adams
subject: Pittsfield
subject: Gravel Pit
subject: Water
subject: Sewer
subject: Economic Policy
subject: Economics
subject: Growth and Development
subject: Public Policy
subject: Urban, Community and Regional Planning
subject: Urban Studies
subject: Urban Studies and Planning

description: The Center for Economic Development at the University of Massachusetts, in Amherst, is part of the Landscape Architecture and Regional Planning Department, and is funded by the Economic Development Administration of the U.S. Department of Commerce, and the University of Massachusetts.
description: The purpose of this report was to establish the goals and objectives that would guide the Comprehensive Economic Development Strategy (CEDS) of Berkshire County, Massachusetts. These goals and objects were the result of deliberations of the countywide CEDs Coordinating Committee.
title: Histoire 08 : khWjNga
Creators: name: Jacques, Guillaume
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2015
Subjects: subject: Japhug
subject: jya
subject: text_and_corpus_linguistics
subject: language_documentation
subject: anthropological_linguistics

description: Conforms to: doi:10.34847/cocoon.49aefa90-8c1f-3ba8-a099-0ebefc6a2aa7
“Vedere” in geometria alla Scuola dell’Infanzia: attività di giustapposizione e sovrapposizione per favorire lo sviluppo della decostruzione dimensionale di figure piane.
Creators: name: Manetti, Ilaria
Publisher: name: Scuola Universitaria della Svizzera Italiana (SUPSI)
Year: 2018

description: Il lavoro di ricerca analizza l’evoluzione della capacità di allievi della Scuola dell’Infanzia di affrontare e risolvere attività di giustapposizione e sovrapposizione in un percorso didattico, in ambito geometrico, specificatamente dedicato allo sviluppo della decostruzione dimensionale delle figure piane. Per le attività, inserite in un contesto ludico, sono stati non solo selezionati ma anche ideati materiali specifici. Le attività sono state elaborate tenendo conto di opportune variabili didattiche. Quest’ultime hanno permesso di identificare e proporre una particolare progressione delle fasi di gioco. L’analisi è stata effettuata attraverso l’osservazione partecipante. Per la raccolta dei dati ci si è serviti di rubriche valutative, appositamente stilate. Dall’analisi dei dati effettuata in modo principalmente quantitativo, è emersa un’evoluzione positiva delle capacità degli allievi di affrontare e risolvere i problemi posti. Si è notato un miglioramento più significativo nelle attività sulla giustapposizione. Grazie ad un approccio differenziato, gli allievi hanno potuto far evolvere individualmente le loro competenze e hanno potuto sviluppare la loro capacità di lavorare in modo autonomo nelle numerose sperimentazioni delle fasi di gioco. Dati i risultati, e in una prospettiva di continuità di questo approccio, sarebbe interessante poter osservarne l’incidenza a lungo termine. Relatrice: Rossana Falcade Pincolini
Gravitational Wave (GW) Classification, Space GW Detection Sensitivities and AMIGO (Astrodynamical Middle-frequency Interferometric GW Observatory)
Creators: name: Ni, Wei-Tou
Publisher: name: arXiv
Year: 2017
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: After first reviewing the gravitational wave (GW) spectral classification. we discuss the sensitivities of GW detection in space aimed at low frequency band (100 nHz-100 mHz) and middle frequency band (100 mHz-10 Hz). The science goals are to detect GWs from (i) Supermassive Black Holes; (ii) Extreme-Mass-Ratio Black Hole Inspirals; (iii) Intermediate-Mass Black Holes; (iv) Galactic Compact Binaries; (v) Stellar-Size Black Hole Binaries; and (vi) Relic GW Background. The detector proposals have arm length ranging from 100 km to 1.35x109 km (9 AU) including (a) Solar orbiting detectors and (b) Earth orbiting detectors. We discuss especially the sensitivities in the frequency band 0.1-10 microHz and the middle frequency band (0.1 Hz-10 Hz). We propose and discuss AMIGO as an Astrodynamical Middle-frequency Interferometric GW Observatory.
description: 10 pages, 2 figures, 1 table, Plenary talk given in Joint Meeting of 13th International Conference on Gravitation, Astrophysics, and Cosmology and 15th Italian-Korean Symposium on Relativistic Astrophysics, Ewha Womans University, Seoul, Korea, July 3-7, 2017
title: ADCO, Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Cart. 32 (G 136), 745 folios, f. 1341
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
name: Petot, Frédéric
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: cartulaire
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Archives départementales de la Côte-d'Or, Cart. 32 (G 136), 745 folios, f. 1341, 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. 1341, 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
Using analogical reasoning to design buildings
Creators: name: Zhao, Fang
name: Maher, Mary Lou.
name: Carnegie Mellon University.Engineering Design Research Center.
Publisher: name: Carnegie Mellon University
Year: 1988
Subjects: subject: 90799 Environmental Engineering not elsewhere classified
subject: FOS: Environmental engineering
subject: 90599 Civil Engineering not elsewhere classified
subject: FOS: Civil engineering

description: technical report
The Schur multiplier of central product of groups
Creators: name: Hatui, Sumana
name: Vermani, L. R.
name: Yadav, Manoj K.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Group Theory (math.GR)
subject: FOS: Mathematics
subject: 20J06

description: Let $G$ be a central product of two groups $H$ and $K$. We study second cohomology group of $G$, having coefficients in a divisible abelian group $D$ with trivial $G$-action, in terms of the second cohomology groups of certain quotients of $H$ and $K$. In particular, for $D = \mathbb{C}^{*}$, some of our results provide a refinement of results from [Some groups with non-trivial multiplicators, Math. Z. {\bf 120 } (1971), 307-308] and [On the Schur multiplicator of a central quotient of a direct product of groups, J. Pure Appl. Algebra {\bf 3} (1973), 73-82].
description: 10 pages, to appear in Journal of Pure and Applied Algebra
The He II Emitting Nebula N44C in the LMC: Optical/UV Spectroscopy of the Nebula and its Ionizing Star
Creators: name: Garnett, Donald R.
name: Galarza, Vanessa C.
name: Chu, You-Hua
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present HST spectroscopy and imaging, along with new ground-based spectroscopy and ROSAT HRI imaging, of the He II emitting nebula N44C and its ionizing star. A GHRS spectrogram of the ionizing star yields a spectral type of about O7 for the star. The lack of P Cygni profiles for Si IV and C IV indicates that the star is not a supergiant. The nebular abundances in the ionized gas are consistent with average abundances for LMC H II regions, with the possible exception that nitrogen may be enhanced. Enrichment by a former evolved companion star is not evident. A long-slit echelle spectrogram in H-alpha + [N II] shows no evidence for high-velocity gas in N44C. This rules out high-velocity shocks as the source of the nebular He II emission. A 108 ks ROSAT HRI image of N44C shows no X-ray point source to a 3-sigma upper limit L(X) < 10^34 erg s^-1 in the 0.1-2.0 keV band. Based on new measurements of the electron density in the He II emitting region, we derive recombination timescales of approximately 20 yrs for He^+2 and approximately 4 yrs for Ne^+4. If N44C is a fossil X-ray ionized nebula, this places severe constraints on when the putative X-ray source could have turned off. The presence of strong [Ne IV] emission in the nebula is puzzling if the ionizing source has turned off. It is possible the system is related to the Be X-ray binaries, although the O star in N44C does not show Be characteristics at the present time. Monitoring of X-rays and He II emission from the nebula, as well as a radial velocity study of the ionizing star, are needed to fully understand the emission line spectrum of N44C.
description: 37 pages, 7 figures (1 color .gif image); accepted for publication in the 10 Dec 2000 Astrophysical Journal. Complete PostScript and PDF versions can also be obtained at http://ocotillo.as.arizona.edu/~dgarnett
Emergence of Bulk CsCl Structure in (CsCl)nCs+ Cluster Ions
Creators: name: Aguado, Andres
Publisher: name: arXiv
Year: 2000
Subjects: subject: Atomic and Molecular Clusters (physics.atm-clus)
subject: FOS: Physical sciences

description: The emergence of CsCl bulk structure in (CsCl)nCs+ cluster ions is investigated using a mixed quantum-mechanical/semiempirical theoretical approach. We find that rhombic dodecahedral fragments (with bulk CsCl symmetry) are more stable than rock-salt fragments after the completion of the fifth rhombic dodecahedral atomic shell. From this size (n=184) on, a new set of magic numbers should appear in the experimental mass spectra. We also propose another experimental test for this transition, which explicitely involves the electronic structure of the cluster. Finally, we perform more detailed calculations in the size range n=31--33, where recent experimental investigations have found indications of the presence of rhombic dodecahedral (CsCl)32Cs+ isomers in the cluster beams.
description: LaTeX file. 6 pages and 4 pictures. Accepted for publication in Phys. Rev. B
Treatment of engineering design constraints in a relational database
Creators: name: Fenves, Steven J(Steven Joseph)
name: Rasdorf, William John.
Publisher: name: Carnegie Mellon University
Year: 1982
Subjects: subject: 90799 Environmental Engineering not elsewhere classified
subject: FOS: Environmental engineering
subject: 90599 Civil Engineering not elsewhere classified
subject: FOS: Civil engineering

description: technical report
The Lattice $β$-function of Quantum Spin Chains
Creators: name: Crompton, P. R.
Publisher: name: arXiv
Year: 2006
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We derive the lattice $β$-function for quantum spin chains, suitable for relating finite temperature Monte Carlo data to the zero temperature fixed points of the continuum nonlinear sigma model. Our main result is that the asymptotic freedom of this lattice $β$-function is responsible for the nonintegrable singularity in $θ$, that prevents analytic continuation between $θ=0$ and $θ=π$.
description: 10 pages
Equilibrium solutions of the shallow water equations
Creators: name: Weichman, Peter B.
name: Petrich, Dean M.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: Atmospheric and Oceanic Physics (physics.ao-ph)
subject: FOS: Physical sciences

description: A statistical method for calculating equilibrium solutions of the shallow water equations, a model of essentially 2-d fluid flow with a free surface, is described. The model contains a competing acoustic turbulent {\it direct} energy cascade, and a 2-d turbulent {\it inverse} energy cascade. It is shown, nonetheless that, just as in the corresponding theory of the inviscid Euler equation, the infinite number of conserved quantities constrain the flow sufficiently to produce nontrivial large-scale vortex structures which are solutions to a set of explicitly derived coupled nonlinear partial differential equations.
description: 4 pages, no figures. Submitted to Physical Review Letters
Connection between jets, winds and accretion in T Tauri stars: the X-shooter view
Creators: name: Nisini, B.
name: Antoniucci, S.
name: Alcala', J. M.
name: Giannini, T.
name: Manara, C. F.
name: Natta, A.
name: Fedele, D.
name: Biazzo, K.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We have analysed the [OI]6300 A line in a sample of 131 young stars with discs in the Lupus, Chamaeleon and signa Orionis star forming regions, observed with the X-shooter spectrograph at VLT. The stars have mass accretion rates spanning from 10^{-12} to 10^{-7} Mo/yr. The line profile was deconvolved into a low velocity component (LVC, < 40 km/s) and a high velocity component (HVC, > 40 km/s ), originating from slow winds and high velocity jets, respectively. The LVC is by far the most frequent component, with a detection rate of 77%, while only 30% of sources have a HVC. The [OI]6300 luminosity of both the LVC and HVC, when detected, correlates with stellar and accretion parameters of the central sources (i.e. Lstar , Mstar , Lacc , Macc), with similar slopes for the two components. The line luminosity correlates better with the accretion luminosity than with the stellar luminosity or stellar mass. We suggest that accretion is the main drivers for the line excitation and that MHD disc-winds are at the origin of both components. In the sub-sample of Lupus sources observed with ALMA a relationship is found between the HVC peak velocity and the outer disc inclination angle, as expected if the HVC traces jets ejected perpendicularly to the disc plane. Mass loss rates measured from the HVC span from ~ 10^{-13} to ~10^{-7} Mo/yr. The corresponding Mloss/Macc ratio ranges from ~0.01 to ~0.5, with an average value of 0.07. However, considering the upper limits on the HVC, we infer a ratio < 0.03 in more than 40% of sources. We argue that most of these sources might lack the physical conditions needed for an efficient magneto-centrifugal acceleration in the star-disc interaction region. Systematic observations of populations of younger stars, that is, class 0/I, are needed to explore how the frequency and role of jets evolve during the pre-main sequence phase.
description: 15 pages, 14 figures, Accepted for publication in A&A
Nonanalyticities of entropy functions of finite and infinite systems
Creators: name: Casetti, Lapo
name: Kastner, Michael
Publisher: name: arXiv
Year: 2006
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: In contrast to the canonical ensemble where thermodynamic functions are smooth for all finite system sizes, the microcanonical entropy can show nonanalytic points also for finite systems, even if the Hamiltonian is smooth. The relation between finite and infinite system nonanalyticities is illustrated by means of a simple classical spin-like model which is exactly solvable for both, finite and infinite system sizes, showing a phase transition in the latter case. The microcanonical entropy is found to have exactly one nonanalytic point in the interior of its domain. For all finite system sizes, this point is located at the same fixed energy value $ε_{c}^{finite}$, jumping discontinuously to a different value $ε_{c}^{infinite}$ in the thermodynamic limit. Remarkably, $ε_{c}^{finite}$ equals the average potential energy of the infinite system at the phase transition point. The result, supplemented with results on nonanalyticities of the microcanonical entropy for other models, indicates that care is required when trying to infer infinite system properties from finite system nonanalyticities.
description: 4 pages, 1 figure
Holography of D-Brane Reconnection
Creators: name: Berg, Marcus
name: Hohm, Olaf
name: Samtleben, Henning
Publisher: name: arXiv
Year: 2006
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Gukov, Martinec, Moore and Strominger found that the D1-D5-D5' system with the D5-D5' angle at 45 degrees admits a deformation "rho" preserving supersymmetry. Under this deformation, the D5-branes and D5'-branes reconnect along a single special Lagrangian manifold. We construct the near-horizon limit of this brane setup (for which no supergravity solution is currently known), imposing the requisite symmetries perturbatively in the deformation rho. Reducing to the three-dimensional effective gauged supergravity, we compute the scalar potential and verify the presence of a deformation with the expected properties. We compute the conformal dimensions as functions of rho. This spectrum naturally organizes into N=3 supermultiplets, corresponding to the 3/16 preserved by the brane system. We give some remarks on the symmetric orbifold CFT for Q_D5=Q_D5', outline the computation of rho-deformed correlators in this theory, and probe computations in our rho-deformed background.
description: 33 pages, 5 figures
title: Histoire 08 : kWmtChW
Creators: name: Jacques, Guillaume
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2015
Subjects: subject: Japhug
subject: jya
subject: text_and_corpus_linguistics
subject: language_documentation
subject: anthropological_linguistics

description: Conforms to: doi:10.34847/cocoon.49aefa90-8c1f-3ba8-a099-0ebefc6a2aa7
Constraints on Cosmological Anisotropy out to z=1 from Supernovae Ia
Creators: name: Kolatt, Tsafrir S.
name: Lahav, Ofer
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: A combined sample of 79 high and low redshift supernovae Ia (SNe) is used to set constraints on the degree of anisotropy in the Universe out to $z\simeq1$. First we derive the global most probable values of matter density $Ω_M $, the cosmological constant $Ω_Λ$, and the Hubble constant $H_0$, and find them to be consistent with the published results from the two data sets of Riess et al. 1998 (R98) and Perlmutter et al. 1999 (P99). We then examine the Hubble diagram (HD, i.e., the luminosity-redshift relation) in different directions on the sky by utilising spherical harmonic expansion. In particular, via the analysis of the dipole anisotropy, we divide the sky into the two hemispheres that yield the most discrepant of the three cosmological parameters, and the scatter $χ^2_{\rm HD}$ in each case. The most discrepant values roughly move along the locus $-4Ω_M +3 Ω_Λ = 1$ (cf. P99), but by no more than $Δ\approx 2.5$ along this line. For a perfect FRW universe, Monte Carlo realizations that mimic the current set of SNe yield values higher than the measured $Δ$ in $\sim 1/5$ of the cases. We discuss implications for the validity of the Cosmological Principle, and possible calibration problems in the SNe data sets.
description: 6 pages, submitted to MNRAS
Miglioramento di un sistema di misura del tiro nell’hockey su ghiaccio
Creators: name: Dotti, Zaccheo
Publisher: name: Scuola Universitaria della Svizzera Italiana (SUPSI)
Year: 2018

description: L’obiettivo del presente progetto consiste nel migliorare un sistema di misura del tiro nell’hockey su ghiaccio, allestito da Deluigi e Dotti, al fine si predisporre di un sistema di misura che permetta all’utente (giocatore) di migliorare il proprio tiro. Si è focalizzato il lavoro sulla verifica della possibilità di ricavare i valori di forza impressa al bastone e degli impatti (paletta-ghiaccio e paletta-disco), mediante la misura delle deformazioni con estensimetri montati sui due assi del manico del bastone. L’analisi in frequenza di misurazioni di tiro reali, abbinate all’applicazione di filtri passa-alto e passa-banda permette di isolare gli istanti esatti d’impatto tra la paletta e il ghiaccio e tra la paletta e il disco. Sono state svolte delle misurazioni in laboratorio per determinare lo spettro di vibrazione del bastone e per calibrare in forza gli estensimetri, sia staticamente che dinamicamente. La calibrazione statica è stata svolta con una cella di carico, mentre la calibrazione dinamica mediante l’utilizzo di un martello strumentato, con il quale è possibile misurare la forza d’impatto.
The Critical Point Equation And Contact Geometry
Creators: name: Ghosh, Amalendu
name: Patra, Dhriti Sundar
Publisher: name: arXiv
Year: 2017
Subjects: subject: Differential Geometry (math.DG)
subject: FOS: Mathematics
subject: 53C25, 53C20, 53C15

description: In this paper, we consider the CPE conjecture in the frame-work of $K$-contact and $(κ, μ)$-contact manifolds. First, we prove that if a complete $K$-contact metric satisfies the CPE is Einstein and is isometric to a unit sphere $S^{2n+1}$. Next, we prove that if a non-Sasakian $ (κ, μ) $-contact metric satisfies the CPE, then $ M^{3} $ is flat and for $ n > 1 $, $ M^{2n+1} $ is locally isometric to $ E^{n+1}\times S^{n}(4)$.
description: In the published version there was a sign error in Eq. (1.3). We have fixed it here
Introduction to hypocoercive methods and applications for simple linear inhomogeneous kinetic models
Creators: name: Hérau, Frédéric
Publisher: name: arXiv
Year: 2017
Subjects: subject: Analysis of PDEs (math.AP)
subject: Spectral Theory (math.SP)
subject: FOS: Mathematics

description: In this lectures given at the Morning side center of Mathematics in October 2016, we present in a very simple framework Hilbertian hypocoercive methods in the case of 1d kinetic inhomogeneous equations, and some illustrations concerning short time or long time behavior in a linear or non-linear perturbative setting
Higher Dipole Bands in the NLC Accelerating Structure
Creators: name: Adolphsen, C.
name: Bane, K. L. F.
name: Dolgashev, V. A.
name: Ko, K.
name: Li, Z.
name: Miller, R.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Accelerator Physics (physics.acc-ph)
subject: FOS: Physical sciences

description: We show that scattering matrix calculations for dipole modes between 23-43 GHz for the 206 cell detuned structure (DS) are consistent with finite element calculations and results of the uncoupled model. In particular, the rms sum wake for these bands is comparable to that of the first dipole band. We also show that for RDDS1 uncoupled wakefield calculations for higher bands are consistent with measurements. In particular, a clear 26 GHz signal in the short range wake is found in both results.
description: 3 pages, 7 figures, submitted to LINAC2000 as TUA18, 21-28 August, Monterey, CA
title: ADCO, Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome IX, Cart. 193 (11 H 78), f. 0227v
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: LaMOP
subject: cartulaire
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge

description: Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome IX, Archives départementales de la Côte-d'Or, Cart. 193 (11 H 78), f. 0227v, 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 IX, Archives départementales de la Côte-d'Or, Cart. 193 (11 H 78), f. 0227v, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
Tools and techniques for knowledge-based expert systems for engineering design
Creators: name: Maher, Mary Lou
name: Fenves, Steven J(Steven Joseph)
name: Duvvuru  Sriram
Publisher: name: Carnegie Mellon University
Year: 1984
Subjects: subject: 90799 Environmental Engineering not elsewhere classified
subject: FOS: Environmental engineering
subject: 90599 Civil Engineering not elsewhere classified
subject: FOS: Civil engineering

description: technical report
Brave art: Scottish identity and stand-up comedy
Creators: name: Silveira, Carolina
Publisher: name: Zenodo
Year: 2024

description: Stand-up comedy remains a prevalent form of entertainment in Scotland, with comedians drawing sell-out crowds, and comedy making up the biggest section of the Edinburgh Fringe Festival programme. Moreover, stand-up comedy is recognised by many academics as a form of social commentary that can affirm or subvert cultural norms, or at the very least, provide a social thermometer that tells us what is going on in society. Research on Scottish stand-up comedy can therefore shed a light on how contemporary Scottish identity is constructed and understood. Yet, despite its popularity and potential social significance, few studies have focused on Scottish comedy to date, and none have chosen to analyse Scottish stand-up comedy specifically. The present research addresses this gap and uses discourse analysis to understand how Scottish stand-up comedy articulates representations of contemporary Scottish and British identities. The data for this study includes live comedy performances at the Edinburgh Fringe as well as interviews with stand-up comedians to gain a deeper insight. The findings show that Scotland is largely framed as a postcolonial nation with distinct values (inclusive, left-wing, egalitarian), particularly in comparison to ‘Brexit’ England. Despite this emphasis on civic nationalism, there are intersectional differences in how people experience Scottish identity, particularly for Scots positioned outside traditional white, heterosexual masculinity, who have to work harder to belong. The Edinburgh Fringe brings to the fore questions of belonging and exclusion as Scots make up a relatively small proportion of the comedy offering. Yet, the Fringe is also identified as a carnivalesque space with subversive potential. By disrupting the taken for granted, and highlighting possibilities for change, Scottish stand-up comedians at the Fringe engage in the political work of (de-)constructing the boundaries of identity and belonging.
Effect of risk perception on epidemic spreading in temporal networks
Creators: name: Moinet, Antoine
name: Barrat, Alain
name: Satorras, Romualdo Pastor
Publisher: name: arXiv
Year: 2017
Subjects: subject: Physics and Society (physics.soc-ph)
subject: FOS: Physical sciences

description: Many progresses in the understanding of epidemic spreading models have been obtained thanks to numerous modeling efforts and analytical and numerical studies, considering host populations with very different structures and properties, including complex and temporal interaction networks. Moreover, a number of recent studies have started to go beyond the assumption of an absence of coupling between the spread of a disease and the structure of the contacts on which it unfolds. Models including awareness of the spread have been proposed, to mimic possible precautionary measures taken by individuals that decrease their risk of infection, but have mostly considered static networks. Here, we adapt such a framework to the more realistic case of temporal networks of interactions between individuals. We study the resulting model by analytical and numerical means on both simple models of temporal networks and empirical time-resolved contact data. Analytical results show that the epidemic threshold is not affected by the awareness but that the prevalence can be significantly decreased. Numerical studies highlight however the presence of very strong finite-size effects, in particular for the more realistic synthetic temporal networks, resulting in a significant shift of the effective epidemic threshold in the presence of risk awareness. For empirical contact networks, the awareness mechanism leads as well to a shift in the effective threshold and to a strong reduction of the epidemic prevalence.
Stability of products of equivalence relations
Creators: name: Marrakchi, Amine
Publisher: name: arXiv
Year: 2017
Subjects: subject: Dynamical Systems (math.DS)
subject: Operator Algebras (math.OA)
subject: FOS: Mathematics
subject: 37A20, 46L10, 46L36

description: An ergodic p.m.p. equivalence relation $ \mathcal{R}$ is said to be stable if $\mathcal{R} \cong \mathcal{R} \times \mathcal{R}_0$ where $\mathcal{R}_0$ is the unique hyperfinite ergodic type $\mathrm{II}_1$ equivalence relation. We prove that a direct product $\mathcal{R} \times \mathcal{S}$ of two ergodic p.m.p. equivalence relations is stable if and only if one of the two components $\mathcal{R}$ or $\mathcal{S}$ is stable. This result is deduced from a new local characterization of stable equivalence relations. The similar question on McDuff $\mathrm{II}_1$ factors is also discussed and some partial results are given.
description: 14 pages
Coupled bulk and brane fields about a de Sitter brane
Creators: name: Cardoso, Antonio
name: Koyama, Kazuya
name: Mennim, Andrew
name: Seahra, Sanjeev S.
name: Wands, David
Publisher: name: arXiv
Year: 2006
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We consider the evolution of a bulk scalar field in anti-de Sitter (AdS) spacetime linearly coupled to a scalar field on a de Sitter boundary brane. We present results of a spectral analysis of the system, and find that the model can exhibit both bound and continuum resonant modes. We find that zero, one, or two bound states may exist, depending upon the masses of the brane and bulk fields relative to the Hubble length and the AdS curvature scale and the coupling strength. In all cases, we find a critical coupling above which there exists a tachyonic bound state. We show how the 5-dimensional spectral results can be interpreted in terms of a 4-dimensional effective theory for the bound states. We find excellent agreement between our analytic results and the results of a new numerical code developed to model the evolution of bulk fields coupled to degrees of freedom on a moving brane. This code can be used to model the behaviour of braneworld cosmological perturbations in scenarios for which no analytic results are known.
description: 16 pages, 10 figures; minor ammendments to the text, typos corrected including a misprint in Eq. (102), reference added
Fully Resolved Numerical Simulations of Fused Deposition Modeling. Part I-Fluid Flow
Creators: name: Xia, Huanxiong
name: Lu, Jiacai
name: Dabiri, Sadegh
name: Tryggvason, Gretar
Publisher: name: arXiv
Year: 2017
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: Purpose - This paper presents a first step toward developing a comprehensive methodology for fully resolved numerical simulations of fusion deposition modeling. Design/methodology/approach - A front-tracking/finite volume method previously developed for simulations of multiphase flows is extended to model the injection of hot polymer and its cooling down. Findings - The accuracy and convergence properties of the new method are tested by grid refinement and the method is shown to produce convergent solutions for the shape of the filament, the temperature distribution, contact area and reheat region when new filaments are deposited on top of previously laid down filaments. Research limitations/implications - The present paper focuses on modeling the fluid flow and the cooling. The modeling of solidification, volume changes and residual stresses will be described in Part II. Practical implications - The ability to carry our fully resolved numerical simulations of the fusion deposition process is expected to help explore new deposition strategies and to provide the "ground truth" for the development of reduced order models. Originality/value - The present paper is the first fully resolved simulation of the deposition in fusion filament modeling.
description: Accepted by Rapid Prototyping Journal
Carnet nº 13, commencé à Hiroshima (p. 7)
Creators: name: Péraire, Lucien
name: CNRS
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2023

description: created: 16-10-1930
The Radio Structure of the Supernova Remnant MSH14-63
Creators: name: dickel, John R.
name: Strom, Richard G.
name: Milne, D. K.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: G315.4-2.3 is an extended shell supernova remnant (SNR) with some characteristics of evolutionarily young remnants and some of older ones. To further elucidate some of its characteristics, we present imaging and polarimetry of this SNR at a frequency of 1.34 GHz with a resolution of 8 arcsec made with the Australia Telescope Compact Array. The indicators of youth are: Morphologically, the radio emission arises in a smooth shell without the fine scale filaments seen in the optical. Many of the optical filaments are Balmer dominated. Where measurable, the orientation of the magnetic field appears to be radial with respect to the center of the remnant. There may have been a supernova in that region in AD185. Indications of older age include: Particularly in RCW86, the bright optical nebula in the southwestern corner of this extended SNR, but also in other locations there are several filaments with bright [S II] emission representative of older shocked filaments in radiative equilibrium. If the remnant lies at the kinematical distance of 2.8 kpc, it has a diameter of 37 pc which would be large for a remnant less than two thousand years old. The remnant seems to be expanding inside a cavity outlined by infrared emission and so it could well be young and large. Where it is encountering the walls of the cavity it is slowing rapidly and we observe the radiative filaments. RCW86 itself is encountering a dense clump of material but may also be the remains of a more compact lump of ejecta ploughing into the surroundings.
description: 15 pages in AAS LaTeX 5.0, 5 figures (2 parts in JPEG, 6 in GIF, 4 in eps), accepted by ApJ
title: Histoire 08 : kWqhi
Creators: name: Jacques, Guillaume
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2015
Subjects: subject: Japhug
subject: jya
subject: text_and_corpus_linguistics
subject: language_documentation
subject: anthropological_linguistics

description: Conforms to: doi:10.34847/cocoon.49aefa90-8c1f-3ba8-a099-0ebefc6a2aa7
The use of LISP for computer-aided design systems
Creators: name: Holtz, Neal M.
name: Rasdorf, William John.
Publisher: name: Carnegie Mellon University
Year: 1982
Subjects: subject: 90799 Environmental Engineering not elsewhere classified
subject: FOS: Environmental engineering
subject: 90599 Civil Engineering not elsewhere classified
subject: FOS: Civil engineering

description: technical report
Conservative Algorithms for Non-Maxwellian Plasma Kinetics
Creators: name: Le, H. P.
name: Cambier, J. -L.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Plasma Physics (physics.plasm-ph)
subject: Computational Physics (physics.comp-ph)
subject: FOS: Physical sciences

description: We present a numerical model and a set of conservative algorithms for Non-Maxwellian plasma kinetics with inelastic collisions. These algorithms self-consistently solve for the time evolution of an isotropic electron energy distribution function interacting with an atomic state distribution function of an arbitrary number of levels through collisional excitation, deexcitation, as well as ionization and recombination. Electron-electron collisions, responsible for thermalization of the electron distribution, are also included in the model. The proposed algorithms guarantee mass/charge and energy conservation in a single step, and is applied to the case of non-uniform gridding of the energy axis in the phase space of the electron distribution function. Numerical test cases are shown to demonstrate the accuracy of the method and its conservation properties.
Non-linear Development of Secular Gravitational Instability in Protoplanetary Disks
Creators: name: Tominaga, Ryosuke T.
name: Inutsuka, Shu-ichiro
name: Takahashi, Sanemichi Z.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: We perform non-linear simulation of secular gravitational instability (GI) in protoplanetary disks that has been proposed as a mechanism of the planetesimal formation and the multiple ring formation. Since the timescale of the growth of the secular GI is much longer than the Keplerian rotation period, we develop a new numerical scheme for a long term calculation utilizing the concept of symplectic integrator. With our new scheme, we first investigate the non-linear development of the secular GI in a disk without a pressure gradient in the initial state. We find that the surface density of dust increases by more than a factor of one hundred while that of gas does not increase even by a factor of two, which results in the formation of dust-dominated rings. A line mass of the dust ring tends to be very close to the critical line mass of a self-gravitating isothermal filament. Our results indicate that the non-linear growth of the secular GI provides a powerful mechanism to concentrate the dust. We also find that the dust ring formed via the non-linear growth of the secular GI migrates inward with a low velocity, which is driven by the self-gravity of the ring. We give a semi-analytical expression for the inward migration speed of the dusty ring.
description: 29 pages, 18 figures, accepted for publication in Publications of the Astronomical Society of Japan
title: Histoire 08 : qaCti
Creators: name: Jacques, Guillaume
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2015
Subjects: subject: Japhug
subject: jya
subject: text_and_corpus_linguistics
subject: language_documentation
subject: anthropological_linguistics

description: Conforms to: doi:10.34847/cocoon.49aefa90-8c1f-3ba8-a099-0ebefc6a2aa7
Stable Monolayer alpha-Phase of CdTe: Strain-Dependent Properties
Creators: name: Unsal, Elif
name: Senger, Ramazan T.
name: Sahin, Hasan
Publisher: name: arXiv
Year: 2017
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: CdTe is a well known and widely used binary compound for optoelectronic applications. In this study, we propose the thinnest, free standing monolayer of CdTe which holds the tetragonal-PbO (alpha-PbO) symmetry. The structural, electronic, vibrational and strain dependent properties are investigated by means of first principles calculations based on density functional theory. Our results demonstrate that the monolayer alpha-CdTe is a dynamically stable and mechanically flexible material. It is found that the thinnest monolayer crystal of CdTe is a semiconductor with a direct band gap of 1.95 eV, which corresponds to red light in the visible spectrum. Moreover, it is found that the band gap can be tunable under biaxial strain. With its strain-controllable direct band gap within the visible spectrum, stable alpha-phase of monolayer CdTe is a suitable candidate for optoelectronic device applications.
Seminario.La importancia de la nutrición durante el envejecimiento
Creators: name: Medina Ponce, Ángel Jonatan
name: Estévez Torres, Kevin
Publisher: name: Zenodo
Year: 2024

description: Seminario impartido el 14 de marzo de 2024 como material de prácticas de aula de la asignatura 42417 - Cuidados Enfermeros en el Envejecimiento. Grado en Enfermería.Sede Gran Canaria
Elastic contact to nearly incompressible coatings -- Stiffness enhancement and elastic pile-up
Creators: name: Barthel, Etienne
name: Perriot, Antoine
name: Chateauminois, Antoine
name: Frétigny, Christian
Publisher: name: arXiv
Year: 2006
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: We have recently proposed an efficient computation method for the frictionless linear elastic axisymmetric contact of coated bodies [A. Perriot and E. Barthel, J. Mat. Res. 19 (2004) 600]. Here we give a brief description of the approach. We also discuss implications of the results for the instrumented indentation data analysis of coated materials. Emphasis is laid on incompressible or nearly incompressible materials (Poisson ratio $ν>0.4$): we show that the contact stiffness rises much more steeply with contact radius than for more compressible materials and significant elastic pile-up is evidenced. In addition the dependence of the penetration upon contact radius increasingly deviates from the homogeneous reference case when the Poisson ratio increases. As a result, this algorithm may be helpful in instrumented indentation data analysis on soft and nearly incompressible layers.
A Novel Detection Strategy for Nonlinear Frequency-Division Multiplexing
Creators: name: Civelli, Stella
name: Forestieri, Enrico
name: Secondini, Marco
Publisher: name: arXiv
Year: 2017
Subjects: subject: Information Theory (cs.IT)
subject: FOS: Computer and information sciences

description: A novel decision feedback detection strategy exploiting a causality property of the nonlinear Fourier transform is introduced. The novel strategy achieves a considerable performance improvement compared to previously adopted strategies in terms of Q-factor.
description: The work has been submitted to the Optical Fiber Communication (OFC) Conference 2018
The use of artificial intelligence techniques in preliminary structural design
Creators: name: Fenves, Steven J.(Steven Joseph)
name: Maher, Mary Lou
Publisher: name: Carnegie Mellon University
Year: 1981
Subjects: subject: 90799 Environmental Engineering not elsewhere classified
subject: FOS: Environmental engineering
subject: 90599 Civil Engineering not elsewhere classified
subject: FOS: Civil engineering

description: technical report
Measurement of air shower cores to study the cosmic ray composition in the knee energy region
Creators: name: Amenomori, M.
name: Ayabe, S.
name: Caidong
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Since 1996, a hybrid experiment consisting of an emulsion chamber and a burst detector array and the Tibet-II air shower array has been operated at Yangbajing (4300 m above sea level) in Tibet. This experiment can detect air-shower cores, called burst events, accompanied by air showers in excess of about 100 TeV. Using the burst event data observed by this experiment, we discuss the primary cosmic ray composition around the knee in comparison with the Monte Carlo simulations. In this paper, we show that all the features of burst events are wholly compatible with the heavy enriched composition in the knee energy region.
description: 20 pages, 21 figures, to appear in Physical Review D