cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Localized non-Abelian gauge fields in non-compact extra-dimensions
Creators: name: Arai, Masato
name: Blaschke, Filip
name: Eto, Minoru
name: Sakai, Norisuke
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Dynamical localization of non-Abelian gauge fields in non-compact flat $D$ dimensions is worked out. The localization takes place via a field-dependent gauge kinetic term when a field condenses in a finite region of spacetime. Such a situation typically arises in the presence of topological solitons. We construct four-dimensional low-energy effective Lagrangian up to the quadratic order in a universal manner applicable to any spacetime dimensions. We devise an extension of the $R_ξ$ gauge to separate physical and unphysical modes clearly. Out of the D-dimensional non-Abelian gauge fields, the physical massless modes reside only in the four-dimensional components, whereas they are absent in the extra-dimensional components. The universality of non-Abelian gauge charges holds due to the unbroken four-dimensional gauge invariance. We illustrate our methods with models in $D=5$ (domain walls), in $D=6$ (vortices), and in $D=7$.
description: 42 pages, 9 figures, several references are added
Acoustic insertion loss due to two dimensional periodic arrays of circular cylinders parallel to a nearby surface
Creators: name: Krynkin, Anton
name: Umnova, Olga
name: Sanchez-Perez, Juan Vicente
name: Chong, Alvin Y. B.
name: Taherzadeh, Shahram
name: Attenborough, Keith
Publisher: name: arXiv
Year: 2011
Subjects: subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: The acoustical performances of regular arrays of cylindrical elements, with their axes aligned and parallel to a ground plane, have been investigated through predictions and laboratory experiments. Semi-analytical predictions based on multiple scattering theory and numerical simulations based on a boundary element formulation have been made. Measurements have been made in an anechoic chamber using arrays of (a) cylindrical acoustically-rigid scatterers (PVC pipes) and (b) thin elastic shells. Insertion loss (IL) spectra due to the arrays have been measured without and with ground planes for several receiver heights. Data and predictions have been compared. The minima in the excess attenuation spectrum i.e., attenuation maxima due to the ground alone resulting from destructive interference between direct and ground-reflected sound waves, tend to have an adverse influence on the band gaps (BG) related to a periodic array in the free field when these two effects coincide. On the other hand, the presence of rigid ground may result in an IL for an array near the ground similar to or, in the case of the first BG, greater than that resulting from a double array, equivalent to the original array plus its ground plane mirror image, in the free field.
description: J. Acoust. Soc. Am. 130 (6), December 2011
The Hubbard model on the triangular lattice: Spiral order and spin liquid
Creators: name: Sahebsara, Peyman
name: Sénéchal, David
Publisher: name: arXiv
Year: 2007
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We investigate the half-filled Hubbard model on an isotropic triangular lattice with the variational cluster approximation. By decreasing the on-site repulsion $U$ (or equivalently increasing pressure) we go from a phase with long range, three-sublattice, spiral magnetic order, to a non-magnetic Mott insulating phase -- a spin liquid -- and then, for $U\lesssim6.7t$, to a metallic phase. Clusters of sizes 3, 6 and 15 with open boundary conditions are used in these calculations, and an extrapolation to infinite size is argued to lead to a disordered phase at $U=8t$, but to a spiral order at $U\gtrsim 12$.
description: 4 pages, 5 figures (published version)
Brief von Eduard Gans an Leopold Zunz, 31.10.1822
Creators: name: (:Unkn) Unknown
Publisher: name: Universitäts- und Landesbibliothek Sachsen-Anhalt
Year: 1822
Subjects: subject: 090

description: Einrichtung einer Unterrichtskommission bestehend aus Zunz, Rubo und Moser
Thermal radiation and entanglement in proton-proton collisions at the LHC
Creators: name: Baker, O. K.
name: Kharzeev, D. E.
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: Nuclear Experiment (nucl-ex)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: The origin of the apparent thermalization in high-energy collisions is investigated using the data of the ATLAS and CMS Collaborations at the LHC. For this purpose, we analyze the transverse momentum distributions in the following proton-proton collision processes, all at $\sqrt{s} = 13$ TeV: i) inclusive inelastic $pp$ collisions; ii) single- and double-diffractive Drell-Yan production $pp \to μ^+ μ^- X$; and iii) Higgs boson production. We confirm the relation between the effective temperature and the hard scattering scale observed at lower energies, and find that it extends even to the Higgs boson production process. In addition we find that the thermal component disappears in diffractive events (even though many charged hadrons are still produced). We discuss the implications of our study for the mechanism of multi-particle production -- in particular, we test the hypothesis about the link between quantum entanglement and thermalization in high-energy collisions.
description: 20 pages, 5 figures
Fukaya categories of the torus and Dehn surgery
Creators: name: Lekili, Yanki
name: Perutz, Timothy
Publisher: name: arXiv
Year: 2011
Subjects: subject: Symplectic Geometry (math.SG)
subject: Geometric Topology (math.GT)
subject: FOS: Mathematics

description: This paper is a companion to the authors' forthcoming work extending Heegaard Floer theory from closed 3-manifolds to compact 3-manifolds with two boundary components via quilted Floer cohomology. We describe the first interesting case of this theory: the invariants of 3-manifolds bounding S^2 union T^2, regarded as modules over the Fukaya category of the punctured 2-torus. We extract a short proof of exactness of the Dehn surgery triangle in Heegaard Floer homology. We show that A-infinity structures on the graded algebra A formed by the cohomology of two basic objects in the Fukaya category of the punctured 2-torus are governed by just two parameters (m^6,m^8), extracted from the Hochschild cohomology of A. For the Fukaya category itself, m^6 is nonzero.
description: 29 pages, 2 figures, a footnote added
Supplementary document for Enhanced performance of amplified spontaneous emission in Dion-Jacobson phase quasi-2D perovskite by facilitating carrier co-radiation - 7060309.pdf
Creators: name: Zhang, Yuan
name: Dong, Zhiwei
name: Guo, Xiwei
name: Hu, Yongsheng
name: Zhang, Zhibin
name: DENG, YANYAN
name: Zhang, Yong
name: Men, Zhuowu
name: Geng, Chong
name: yulei, Wang
Publisher: name: Optica Publishing Group
Year: 2024
Subjects: Uncategorized

description: Supplemental Document
High precision study of B*B pi coupling in unquenched QCD
Creators: name: Ohki, Hiroshi
name: Matsufuru, Hideo
name: Onogi, Tetsuya
Publisher: name: arXiv
Year: 2007
Subjects: subject: High Energy Physics - Lattice (hep-lat)
subject: FOS: Physical sciences

description: The B* B pi coupling is a fundamental parameter of chiral effective Lagrangian with heavy-light mesons and can constrain the B->pi l nu form factor in the soft pion limit which will be useful for precise determination of |Vub|. We compute the B* B pi coupling with the static heavy quark and the O(a)-improved Wilson light quark. Simulations are carried out with n_f=2 unquenched 12^3x24 lattices at beta=1.80 generated by CP-PACS collaboration. Following the quenched study by Negishi et al., we employ the all-to-all propagator with 200 low eigenmodes as well as HYP smeared link to improve the statistical accuracy.
description: 7 pages, 5 figures, talk presented at the XXV International Symposium on Lattice Field Theory, July 30 - August 4, 2007, Regensburg, Germany Journal-ref: PoS(LATTICE 2007)365
title: Lyman break galaxies and the Ly alpha forest
Creators: name: Kollmeier, JA
name: Weinberg, DH
name: Dave, R
name: Katz, N
Publisher: name: University of Massachusetts Amherst
Year: 2003
Subjects: subject: galaxies : high-redshift
subject: quasars : absorption lines
subject: Astrophysics and Astronomy

description: This is the pre-published version harvested from ArXiv. The published version is located at http://iopscience.iop.org/0004-637X/594/1/75/
description: We use hydrodynamic cosmological simulations to predict correlations between Lyα forest absorption and the galaxy distribution at redshift z 3. The probability distribution function (PDF) of Lyα flux decrements shifts systematically toward higher values in the vicinity of galaxies, reflecting the overdense environments in which these galaxies reside. The predicted signal remains strong in spectra smoothed over 50-200 km s-1, allowing tests with moderate-resolution quasar spectra. The strong bias of high-redshift galaxies toward high-density regions imprints a clear signature on the flux PDF, but the predictions are not sensitive to galaxy baryon mass or star formation rate, and they are similar for galaxies and dark matter halos. The dependence of the flux PDF on galaxy proximity is sensitive to redshift determination errors, with rms errors of 150-300 km s-1 substantially weakening the predicted trends. On larger scales, the mean galaxy overdensity in a cube of 5 or 10 h-1 Mpc (comoving) is strongly correlated with the mean Lyα flux decrement on a line of sight through the cube center. The slope of the correlation is ~3 times steeper for galaxies than for dark matter as a result of galaxy bias. The predicted large-scale correlation is in qualitative agreement with recently reported observational results. However, observations also show a drop in the average absorption in the immediate vicinity of galaxies, which our models do not predict even if we allow the galaxies or active galactic nuclei within them to be ionizing sources. This decreased absorption could be a signature of galaxy feedback on the surrounding intergalactic medium, perhaps via galactic winds. We find that a simplified "wind" model that eliminates neutral hydrogen in spheres around the galaxies can marginally explain the data. However, because peculiar velocities allow gas at large distances to produce saturated absorption at the galaxy redshift, these winds (or any other feedback mechanism) must extend to comoving radii of ~1.5 h-1 Mpc to reproduce the observations. We also discuss the possibility that extended Lyα emission from the target galaxies "fills in" the expected Lyα forest absorption at small angular separations.
Steady State Thermodynamics for Heat Conduction -- Microscopic Derivation
Creators: name: Komatsu, Teruhisa S.
name: Nakagawa, Naoko
name: Sasa, Shin-ichi
name: Tasaki, Hal
Publisher: name: arXiv
Year: 2007
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: Starting from microscopic mechanics, we derive thermodynamic relations for heat conducting nonequilibrium steady states. The extended Clausius relation enables one to experimentally determine nonequilibrium entropy to the second order in the heat current. The associated Shannon-like microscopic expression of the entropy is suggestive. When the heat current is fixed, the extended Gibbs relation provides a unified treatment of thermodynamic forces in linear nonequilibrium regime.
description: 4 pages, version 1 contains a flaw, which has been fixed in version 2. version 3 is much easier to read. In the final version 4, which is going to appear in PRL, ref. 10 was added and some improvments were made
New Ideas for Brain Modelling 5
Creators: name: Greer, Kieran
Publisher: name: arXiv
Year: 2018
Subjects: subject: Artificial Intelligence (cs.AI)
subject: FOS: Computer and information sciences

description: This paper describes a process for combining patterns and features, to guide a search process and make predictions. It is based on the functionality that a human brain might have, which is a highly distributed network of simple neuronal components that can apply some level of matching and cross-referencing over retrieved patterns. The process uses memory in a dynamic way and it is directed through the pattern matching. The paper firstly describes the mechanisms for neuronal search, memory and prediction. The paper then presents a formal language for defining cognitive processes, that is, pattern-based sequences and transitions. The language can define an outer framework for concept sets that are linked to perform the cognitive act. The language also has a mathematical basis, allowing for the rule construction to be consistent. Now, both static memory and dynamic process hierarchies can be built as tree structures. The new information can also be used to further integrate the cognitive model and the ensemble-hierarchy structure becomes an essential part. A theory about linking can suggest that nodes in different regions link together when generally they represent the same thing.
title: Enhanced methods for surface current estimation from X-band radar data
Creators: name: Li, Yi
Publisher: name: Memorial University of Newfoundland
publisherIdentifier: https://ror.org/04haebc03
publisherIdentifierScheme: ROR
Year: 2025

description: Estimating ocean surface currents accurately is crucial for a wide range of applications, including marine navigation, environmental monitoring, and coastal management. Traditional methods for measuring surface currents face challenges such as limited spatial coverage and sensitivity to environmental noise, making the development of more accurate and robust techniques a pressing need in oceanography. This thesis focuses on improving the accuracy and robustness of ocean surface current estimation using X-band radar image sequences by introducing two novel algorithms. In the first part of this thesis, a Symmetry of Doppler Shifts (SDS) method is introduced for retrieving surface current information from radar images. The method focuses on extracting the wave angular frequencies and corresponding wavenumbers from the radar image sequences. Then, Doppler shifts are calculated based on wavevectors that exhibit symmetry with respect to the origin in the wavenumber plane. These Doppler shifts are used to estimate both the speed and direction of surface currents. Simulations with synthetic data show that the SDS method achieves a root mean square error (RMSE) of 0.13 m/s for current speed and 1.4° for direction. The results indicate that the method performs with accuracy comparable to existing techniques under simulated conditions. The second part of this research builds on the SDS method by integrating it with an enhanced Polar Current Shell (PCS) algorithm. The improvements include the application of Kernel Density Estimation (KDE) for noise filtering, interquartile range filtering to remove outliers, and symmetry-based noise reduction. The modified PCS method also employs a single curve-fitting process, analyzing all wavenumbers in the PCS domain collectively rather than individually. The improved algorithm was validated with both simulated data and real-world radar data from a Decca radar (2008) and a Koden radar (2017). Results show that the modified PCS method reduces the RMSE for speed by 0.06 m/s and direction by 3.8° for the Decca radar, and by 0.02 m/s for speed and 4.6° for direction for the Koden radar, compared to the original PCS method.
The Source of Ionization along the Magellanic Stream
Creators: name: Bland-Hawthorn, J.
name: Sutherland, R.
name: Agertz, O.
name: Moore, B.
Publisher: name: arXiv
Year: 2007
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Since its discovery in 1996, the source of the bright H-alpha emission (up to 750 mR) along the Magellanic Stream has remained a mystery. There is no evidence of ionising stars within the HI stream, and the extended hot halo is far too tenuous to drive strong shocks into the clouds. We now present a hydrodynamical model that explains the known properties of the H-alpha emission and provides new insights on the lifetime of the Stream clouds. The upstream clouds are gradually disrupted due to their interaction with the hot halo gas. The clouds that follow plough into gas ablated from the upstream clouds, leading to shock ionisation at the leading edges of the downstream clouds. Since the following clouds also experience ablation, and weaker H-alpha (100-200 mR) is quite extensive, a disruptive cascade must be operating along much of the Stream. In our model, the clouds are evolving on timescales of 100-200 Myr, such that the Stream must be replenished by the Magellanic Clouds at a fairly constant rate. The ablated material falls onto the Galaxy as a warm drizzle which suggests that diffuse ionized gas at 10**4 K may be an important constituent of galactic accretion. The observed HI emission provides a new constraint on the rate of disruption of the Stream and, consequently, the infall rate of metal-poor gas onto the Galaxy. When the ionized component of the Stream is fully accounted for, the rate of gas accretion is 0.4 Msun/yr, roughly twice the rate deduced from HI observations alone.
description: 5 pages, 4 figures; high quality preprint and simulations available at http://www.aao.gov.au/astro/MS
Supplementary document for Photoluminescence properties of two-dimensional semiconductor heterointerfaces - 7045924.pdf
Creators: name: Yan, Shancheng
name: Liu, Hao
name: Chen, Liping
name: Chen, Tianhong
name: Wang, Kaili
name: Jin, Zhihan
name: Tan, Chee Leong
name: Shi, Yi
Publisher: name: Optica Publishing Group
Year: 2024
Subjects: Uncategorized

description: Figures S1,S2 show the PL mapping of the four heterojunctions, respectively, and Figure S3 shows a schematic of the synthesis method for Te nanosheets
title: ADCO, Cartulaire des Dominicains de Dijon (1286), Cart. 221 (H 53), 170 folios, f. 0157
Creators: name: de la Côte d'Or, Archives départementales
name: Petot, Frédéric
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2012
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: cartulaire
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge

description: Cartulaire des Dominicains de Dijon (1286), Archives départementales de la Côte-d'Or, Cart. 221 (H 53), 170 folios. Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire des Dominicains de Dijon (1286), Archives départementales de la Côte-d'Or, Cart. 221 (H 53), 170 folios, f. 0157, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: Dijon
description: Provenance: http://www.wikidata.org/entity/Q7003
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb15250518p
description: Provenance: http://www.idref.fr/02643413X/id
description: Provenance: https://www.geonames.org/6453767
Additional file 2: of Views and perceptions of Australian physiotherapists and physiotherapy students about the potential implementation of physiotherapist prescribing in Australia: a survey protocol
Creators: name: T. Noblet
name: J. Marriot
name: T. Jones
name: C. Dean
name: A. Rushton
Publisher: name: figshare
Year: 2018
Subjects: subject: Biophysics
subject: Pharmacology
subject: Biotechnology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy

description: Online Information and Consent Form. (DOCX 16 kb)
Observational constraints on scalar field models of dark energy with barotropic equation of state
Creators: name: Sergijenko, Olga
name: Durrer, Ruth
name: Novosyadlyj, Bohdan
Publisher: name: arXiv
Year: 2011
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We constrain the parameters of dynamical dark energy in the form of a classical or tachyonic scalar field with barotropic equation of state jointly with other cosmological ones using the combined datasets which include the CMB power spectra from WMAP7, the baryon acoustic oscillations in the space distribution of galaxies from SDSS DR7, the power spectrum of luminous red galaxies from SDSS DR7 and the light curves of SN Ia from 2 different compilations: Union2 (SALT2 light curve fitting) and SDSS (SALT2 and MLCS2k2 light curve fittings). It has been found that the initial value of dark energy equation of state parameter is constrained very weakly by most of the data while the rest of main cosmological parameters are well constrained: their likelihoods and posteriors are similar, have the forms close to Gaussian (or half-Gaussian) and their confidential ranges are narrow. The most reliable determinations of the best fitting value and $1σ$ confidence range for the initial value of dark energy equation of state parameter were obtained from the combined datasets including SN Ia data from the full SDSS compilation with MLCS2k2 fitting of light curves. In all such cases the best fitting value of this parameter is lower than the value of corresponding parameter for current epoch. Such dark energy loses its repulsive properties and in future the expansion of the Universe will change into contraction. We also perform an error forecast for the Planck mock data and show that they narrow essentially the confidential ranges of cosmological parameters values, moreover, their combination with SN SDSS compilation with MLCS2k2 light curve fitting may exclude the fields with initial equation of state parameter $>-0.1$ at 2$σ$ confidential level.
description: 26 pages, 13 figures, 4 tables, accepted for publication in JCAP
Two dimensional collective electron magnetotransport, oscillations and chaos in a semiconductor superlattice
Creators: name: Bonilla, L. L.
name: Carretero, M.
name: Segura, A.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Chaotic Dynamics (nlin.CD)
subject: FOS: Physical sciences

description: When quantized, traces of classically chaotic single particle systems include eigenvalue statistics and scars in eigenfuntions. Since 2001, many theoretical and experimental works have argued that classically chaotic single electron dynamics influences and controls collective electron transport. For transport in semiconductor superlattices under tilted magnetic and electric fields, these theories rely on a reduction to a one-dimensional self-consistent drift model. A two-dimensional theory based on self-consistent Boltzmann transport does not support that single electron chaos influences collective transport. This theory agrees with existing experimental evidence of current self-oscillations, predicts spontaneous collective chaos via a period doubling scenario and it could be tested unambiguously by measuring the electric potential inside the superlattice under a tilted magnetic field.
description: 10 pages, 6 figures, PRE
The link between chemical anomalies along the red giant branch and the horizontal branch extension in globular clusters
Creators: name: Carretta, Eugenio
name: Recio-Blanco, Alejandra
name: Gratton, Raffaele G.
name: Piotto, Giampaolo
name: Bragaglia, Angela
Publisher: name: arXiv
Year: 2007
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We find a strong correlation between the extension of the Na-O anticorrelation observed in red giant branch (RGB) stars and the high temperature extension of the horizontal branch (HB) blue tails of Galactic globular clusters (GCs). The longer is the O-depleted tail of the Na-O anticorrelation observed in the RGB stars, the higher is the maximum temperature reached by the bluest HB stars in the GC. This result provides a clear, empirical evidence of a link between the extension of the HB and the presence of star-to-star abundance variations of proton-capture elements in GC stars. We discuss the possible interpretation of this correlation.
description: Comments: 6 pages, 1 figure, uses emulateapj.cls; accepted for publication in the Astrophysical Journal Letters
title: ADCO, Cartulaire des Dominicains de Dijon (1286), Cart. 221 (H 53), 170 folios, f. 0122
Creators: name: de la Côte d'Or, Archives départementales
name: Petot, Frédéric
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2012
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: cartulaire
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Cartulaire des Dominicains de Dijon (1286), Archives départementales de la Côte-d'Or, Cart. 221 (H 53), 170 folios. Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire des Dominicains de Dijon (1286), Archives départementales de la Côte-d'Or, Cart. 221 (H 53), 170 folios, f. 0122, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb15250518p
description: Provenance: http://www.idref.fr/02643413X/id
description: Provenance: https://www.geonames.org/6453767
description: Provenance: Dijon
description: Provenance: http://www.wikidata.org/entity/Q7003
title: Avant-propos_Le Salon de Grenoble 1904
Creators: name: AmateurS
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020

description: Avant-propos
description: ID_PARA_00900
Additional file 1 of An explainable artificial intelligence framework for risk prediction of COPD in smokers
Creators: name: Wang, Xuchun
name: Qiao, Yuchao
name: Cui, Yu
name: Ren, Hao
name: Zhao, Ying
name: Linghu, Liqin
name: Ren, Jiahui
name: Zhao, Zhiyang
name: Chen, Limin
name: Qiu, Lixia
Publisher: name: figshare
Year: 2023
Subjects: subject: Artificial Intelligence and Image Processing
subject: FOS: Computer and information sciences

description: Additional file 1: Supplementary Table S1. Sampling process of survey subjects for COPD surveillance in China. Supplementary Table S2. Parameter setting. Supplementary Table S3. Detection rate of COPD with categorical variable of different populations. Supplementary Table S4. Detection rate of COPD with continuous variable of different populations. Supplementary Table S5. Sample situation. Supplementary Table S6. Distribution of train/test data.
Chemo-kinematics of the Milky Way from the SDSS-III MARVELS Survey
Creators: name: Grieves, Nolan
name: Ge, Jian
name: Thomas, Neil
name: Willis, Kevin
name: Ma, Bo
name: Lorenzo-Oliveira, Diego
name: Queiroz, A. B. A.
name: Ghezzi, Luan
name: Chiappini, Cristina
name: Anders, Friedrich
name: Dutra-Ferreira, Letícia
name: de Mello, Gustavo F. Porto
name: Santiago, Basílio X.
name: da Costa, Luiz N.
name: Ogando, Ricardo L. C.
name: del Peloso, E. F.
name: Tan, Jonathan C.
name: Schneider, Donald P.
name: Pepper, Joshua
name: Stassun, Keivan G.
name: Zhao, Bo
name: Bizyaev, Dmitry
name: Pan, Kaike
Publisher: name: arXiv
Year: 2018
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Combining stellar atmospheric parameters, such as effective temperature, surface gravity, and metallicity, with barycentric radial velocity data provides insight into the chemo-dynamics of the Milky Way and our local Galactic environment. We analyze 3075 stars with spectroscopic data from the Sloan Digital Sky Survey III (SDSS-III) MARVELS radial velocity survey and present atmospheric parameters for 2343 dwarf stars using the spectral indices method, a modified version of the equivalent width method. We present barycentric radial velocities for a sample of 2610 stars with a median uncertainty of 0.3 km s$^{-1}$. We determine stellar ages using two independent methods and calculate ages for 2335 stars with a maximum-likelihood isochronal age-dating method and for 2194 stars with a Bayesian age-dating method. Using previously published parallax data we compute Galactic orbits and space velocities for 2504 stars to explore stellar populations based on kinematic and age parameters. This study combines good ages and exquisite velocities to explore local chemo-kinematics of the Milky Way, which complements many of the recent studies of giant stars with the APOGEE survey, and we find our results to be in agreement with current chemo-dynamical models of the Milky Way. Particularly, we find from our metallicity distributions and velocity-age relations of a kinematically-defined thin disk that the metal rich end has stars of all ages, even after we clean the sample of highly eccentric stars, suggesting that radial migration plays a key role in the metallicity scatter of the thin disk. All stellar parameters and kinematic data derived in this work are catalogued and published online in machine-readable form.
description: 22 pages, 28 figures, Accepted by MNRAS 2018 August 31
Sigma and Pion Decays of Mixed Heavy Hybrids
Creators: name: Kisslinger, Leonard S.
name: Krute, Dara J.
Publisher: name: arXiv
Year: 2011
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We estimate the relative branching ratio of $σ$ to 2$π$ for the decay of the $Ψ'(2S)$, which we have found to be a mixed charm and hybrid charmonium meson. The external field method and correlators from a previous calculation are used to estimate these decays. We find the $σ$ to 2$π$ branching ratio for $Ψ'(2S)$ to the $J/Ψ(1S)$ decay to be 0.98, in agreement with an experiment at IHEP-BES.
description: 8 pages, 6 figures
Supplementary document for Photoluminescence properties of two-dimensional semiconductor heterointerfaces - 7078630.pdf
Creators: name: Liu, Hao
name: Chen, Liping
name: Chen, Tianhong
name: Wang, Kaili
name: Jin, Zhihan
name: Tan, Chee Leong
name: Shi, Yi
name: Yan, Shancheng
Publisher: name: Optica Publishing Group
Year: 2024
Subjects: Uncategorized

description: Supplemental information
Additional file 2: of Midwivesâ experience of their education, knowledge and practice around immersion in water for labour or birth
Creators: name: Lewis, Lucy
name: Hauck, Yvonne
name: Butt, Janice
name: Western, Chloe
name: Overing, Helen
name: Corrinne Poletti
name: Priest, Jessica
name: Hudd, Dawn
name: Thomson, Brooke
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy

description: Focus group questions. (DOCX 12 kb)
The enigma of GCIRS 3 - Constraining the properties of the mid-infrared reference star of the central parsec of the Milky Way with optical long baseline interferometry
Creators: name: Pott, J. -U.
name: Eckart, A.
name: Glindemann, A.
name: Schodel, R.
name: Viehmann, T.
name: Robberto, M.
Publisher: name: arXiv
Year: 2007
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: GCIRS3 is the most prominent MIR source in the central pc of the Galaxy. NIR spectroscopy failed to solve the enigma of its nature. The properties of extreme individual objects of the central stellar cluster contribute to our knowledge of star and dust formation close to a supermassive black hole. We initiated an interferometric experiment to understand IRS3 and investigate its properties as spectroscopic and interferometric reference star at 10um. VISIR imaging separates a compact source from diffuse, surrounding emission. The VLTI/MIDI instrument was used to measure visibilities at 10mas resolution of that compact 10um source, still unresolved by a single VLT. Photometry data were added to enable simple SED- and full radiative transfer-models of the data. The luminosity and size estimates show that IRS3 is probably a cool carbon star enshrouded by a complex dust distribution. Dust temperatures were derived. The coinciding interpretation of multiple datasets confirm dust emission at several spatial scales. The IF data resolve the innermost area of dust formation. Despite observed deep silicate absorption towards IRS3 we favor a carbon rich chemistry of the circumstellar dust shell. The silicate absorption most probably takes place in the outer diffuse dust, which is mostly ignored by MIDI measurements. This indicates physically and chemically distinct conditions of the local dust, changing with the distance to IRS3. We have demonstrated that optical long baseline interferometry at infrared wavelengths is an indispensable tool to investigate sources at the Galactic Center. Our findings suggest further studies of the composition of interstellar dust and the shape of the 10um silicate feature at this outstanding region.
description: accepted by A&A, now in press; 19 pages, 22 figures, 5 tables
Additional file 1 of ACYP2 contributes to malignant progression of glioma through promoting Ca2+ efflux and subsequently activating c-Myc and STAT3 signals
Creators: name: Li, Mengdan
name: Ruan, Banjun
name: Wei, Jing
name: Yang, Qi
name: Chen, Mingwei
name: Ji, Meiju
name: Hou, Peng
Publisher: name: figshare
Year: 2020
Subjects: subject: Biophysics
subject: Biochemistry
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Pharmacology
subject: Chemical Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer
subject: Hematology

description: Additional file 1: Table S1. The primers used in this study for RT-PCR or qRT-PCR assays. Table S2. The short tandem repeat (STR) profiles of human glioma cell lines used in this study. Table S3. The sequences of siRNAs/shRNAs used in this study. Table S4. The primers used in this study for plasmid construction. Table S5. The antibodies used in this study.
Individual Vortex Manipulation and Stick-Slip Motion in Periodic Pinning Arrays
Creators: name: Ma, X.
name: Reichhardt, C. J. O.
name: Reichhardt, C.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: We numerically examine the manipulation of vortices interacting with a moving trap representing a magnetic force tip translating across a superconducting sample containing a periodic array of pinning sites. As a function of the tip velocity and coupling strength, we find five distinct dynamic phases, including a decoupled regime where the vortices are dragged a short distance within a pinning site, an intermediate coupling regime where vortices in neighboring pinning sites exchange places, an intermediate trapping regime where individual vortices are dragged longer distances and exchange modes of vortices occur in the surrounding pins, an intermittent multiple trapping regime where the trap switches between capturing one or two vortices, and a strong couping regime in which the trap permanently captures and drags two vortices. In some regimes we observe the counterintuitive behavior that slow moving traps couple less strongly to vortices than faster moving traps; however, the fastest moving traps are generally decoupled. The different phases can be characterized by the distances the vortices are displaced and the force fluctuations exerted on the trap. We find different types of stick-slip motion depending on whether vortices are moving into and out of pinning sites, undergoing exchange, or performing correlated motion induced by vortices outside of the trap. Our results are general to the manipulation of other types of particle-based systems interacting with periodic trap arrays, such as colloidal particles or certain types of frictional systems.
description: 10 pages, 13 figures
Additional file 1: of Understanding medical travel from a source country perspective: a cross sectional study of the experiences of medical travelers from the Maldives
Creators: name: Suzana, Mariyam
name: Walls, Helen
name: Smith, Richard
name: Hanefeld, Johanna
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Medicine
subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Science Policy
subject: 60506 Virology

description: Table S1. Providers and destinations frequented by Maldivian medical travelers, 2013. (DOCX 17 kb)
Selecting the rank of truncated SVD by Maximum Approximation Capacity
Creators: name: Frank, Mario
name: Buhmann, Joachim M.
Publisher: name: arXiv
Year: 2011
Subjects: subject: Information Theory (cs.IT)
subject: Machine Learning (cs.LG)
subject: Machine Learning (stat.ML)
subject: FOS: Computer and information sciences

description: Truncated Singular Value Decomposition (SVD) calculates the closest rank-$k$ approximation of a given input matrix. Selecting the appropriate rank $k$ defines a critical model order choice in most applications of SVD. To obtain a principled cut-off criterion for the spectrum, we convert the underlying optimization problem into a noisy channel coding problem. The optimal approximation capacity of this channel controls the appropriate strength of regularization to suppress noise. In simulation experiments, this information theoretic method to determine the optimal rank competes with state-of-the art model selection techniques.
description: 7 pages, 5 figures; Will be presented at the IEEE International Symposium on Information Theory (ISIT) 2011. The conference version has only 5 pages. This version has an extended appendix
Temporal scaling of the growth dependent radiative properties of microalgae
Creators: name: Zhao, J. M.
name: Ma, C. Y.
name: Liu, L. H.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Biological Physics (physics.bio-ph)
subject: FOS: Physical sciences

description: The radiative properties of microalgae are basic parameters for analyzing light field distribution in photobioreactors (PBRs). With the growth of microalgae cell, their radiative properties will vary with growth time due to accumulation of pigment and lipid, cell division and metabolism. In this work, we report both experimental and theoretical evidence of temporal scaling behavior of the growth dependent radiative properties of microalgae cell suspensions. A new concept, the temporal scaling function (TSF), defined as the ratio of absorption or scattering cross-sections at growth phase to that at stationary phase, is introduced to characterize the temporal scaling. The temporal evolution and temporal scaling characteristics of the absoroption and scattering cross-sections of three example microalgae species, Chlorella vulgaris, Chlorella pyrenoidosa, and Chlorella protothecoides, were experimentally studied at spectral range 380 to 850 nm. It is shown that the TSFs of the absorption and scattering cross-sections for different microalgae species are approximately constant at different wavelength, which confirms theoretical predictions very well. With the aid of the temporal scaling relation, the radiative properties of microalgae at any growth time can be calculated based on those measured at stationary phase. The findings of this work will help the understanding of time dependent radiative properties of microalgae and facilitate their applications in light field analysis in PBRs design.
description: 24 pages, 9 figures, submitted to JQSRT on Dec 28, 2017
title: ADCO, Cinquième cartulaire de Saint-Étienne de Dijon (1664), Cart. 28 (G 132), 258 folios, f. 00080
Creators: name: de la Côte d'Or, Archives départementales
name: Petot, Frédéric
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2012
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire
subject: LaMOP

description: Cinquième cartulaire de Saint-Étienne de Dijon (1664), Archives départementales de la Côte-d'Or, Cart. 28 (G 132), 258 folios, f. 00080, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cinquième cartulaire de Saint-Étienne de Dijon (1664), Archives départementales de la Côte-d'Or, Cart. 28 (G 132), 258 folios, f. 00080, 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
title: Article_Bulletin mensuel de la réunion d'amateurs du chien de police 1923
Creators: name: AmateurS
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020

description: ID_ARTI_00164
Tail effects in the third post-Newtonian gravitational wave energy flux of compact binaries in quasi-elliptical orbits
Creators: name: Arun, K G
name: Blanchet, Luc
name: Iyer, Bala R
name: Qusailah, Moh'd S S
Publisher: name: arXiv
Year: 2007
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: The far-zone flux of energy contains hereditary (tail) contributions that depend on the entire past history of the source. Using the multipolar post-Minkowskian wave generation formalism, we propose and implement a semi-analytical method in the frequency domain to compute these contributions from the inspiral phase of a binary system of compact objects moving in quasi-elliptical orbits up to 3PN order. The method explicitly uses the quasi-Keplerian representation of elliptical orbits at 1PN order and exploits the doubly periodic nature of the motion to average the 3PN fluxes over the binary's orbit. Together with the instantaneous (non-tail) contributions evaluated in a companion paper, it provides crucial inputs for the construction of ready-to-use templates for compact binaries moving on quasi-elliptic orbits, an interesting class of sources for the ground based gravitational wave detectors such as LIGO and Virgo as well as space based detectors like LISA.
description: 32 pages, 10 figures. Minor changes in text throughout. Matches the published version
Australian Educators’ Use of Children’s Heritage Language in Early Childhood Services: Facilitators and Barriers
Creators: name: Tang, Mingjun
Publisher: name: Macquarie University
Year: 2024
Subjects: classificationCode: 390302
subject: Early childhood education

description: The Early Years Learning Framework V2.0 (EYLF) provides the foundation for centre-based early childhood learning and teaching across Australia. The EYLF explicitly recommends practices for educators, such as learning some key words from children’s heritage language (HL) and using those words when talking to children. Despite clear national endorsement and advice, there are inconsistencies in the use of HL with children in Australian early childhood services. This study aimed to examine the facilitators and barriers to educators’ use of HL with multilingual children and parents in early childhood services.
A mixed-method approach was employed in this study. An online survey captured information on educators’ demographics, self-reported fluency in languages other than English (multilingual competence) and use of HL with children and parents. Open questions from the online survey provided insights into the benefits and challenges of using HL, as well as solutions, as identified by educators. An interview then allowed for an in-depth discussion. Analysis of closed questions indicated a significant association between educators’ reported language fluency and use of HL with multilingual children and parents. Semantic analysis of open-ended survey questions revealed that although educators recognised the importance of using HL in promoting a sense of belonging for children, they faced significant challenges, such as a lack of proficiency in HL, parent’s aspirations for using English with children and colleague’s negative attitude towards multilingualism. Five themes emerged after the thematic analysis of interviews with four highly educated multilingual educators: centre’s culture, language (mis) match, parents’ characteristics, educator's philosophy, and professional role. This study reveals the important role of educators’ multilingual competence and a whole-centre approach in supporting multilingual families, where staff team, leaders and management at the centre have to work collaboratively on endorsing multilingualism. Recommendations for multilingualism in the Australian early childhood workforce are discussed.
Additional file 2 of ACYP2 contributes to malignant progression of glioma through promoting Ca2+ efflux and subsequently activating c-Myc and STAT3 signals
Creators: name: Li, Mengdan
name: Ruan, Banjun
name: Wei, Jing
name: Yang, Qi
name: Chen, Mingwei
name: Ji, Meiju
name: Hou, Peng
Publisher: name: figshare
Year: 2020
Subjects: subject: Biophysics
subject: Biochemistry
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Pharmacology
subject: Chemical Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer
subject: Hematology

description: Additional file 2: Figure S1. ACYP2 knockdown in glioma cells were confirmed by qRT-PCR assay. Figure S2. ACYP2 knockdown inhibits migration and invasion abilities of glioma cells. Figure S3. Ectopic expression of ACYP2 in SHG44 and A172 cells promoted cell migration and invasion compared to the control. Figure S4. The effect of ACYP2 knockdown on Ca2+ levels in endoplasmic reticulum (ER) in glioma cells. Figure S5. BAPTA-AM treatment reverses inhibitory effect of ACYP2 depletion on glioma cell migration. Figure S6. Calpeptin treatment reverses inhibitory effect of ACYP2 depletion on glioma cell migration. Figure S7. The effect of ACYP2 knockdown on the activity of NFATc1 in glioma cells. Figure S8. qRT-PCR was used to determine the effect of ACYP2 knockdown on the expression of NF-kB’s downstream targets (Bcl-xL and Bcl-2) in the indicated cells. Figure S9. qRT-PCR was used to determine the effect of ACYP2 knockdown on the expression of c-Myc’s downstream targets (E2F2 and cyclin E) and p-STAT3’s downstream targets (c-Fos and c-Jun). Figure S10. Cells transfected with the indicated constructs were treated with the vehicle or Stattic, and the MTT assay was then carried out to evaluate their effect on cell proliferation. Figure S11. qRT-PCR assay was performed to determine mRNA expression levels of PMCA1–4 in the indicated glioma cell lines.
Boundary Regularity for Asymptotically Hyperbolic Metrics with Smooth Weyl Curvature
Creators: name: Jin, Xiaoshang
Publisher: name: arXiv
Year: 2018
Subjects: subject: Differential Geometry (math.DG)
subject: FOS: Mathematics

description: In this paper, we study the regularity of asymptotically hyperbolic metrics with Einstein condition near boundary and Weyl curvature smooth enough in arbitrary dimension. Following Michael Anderson's method, we show that $C^{m,α}$ conformally compact Riemannian metrics with Einstein equation vanishing to finite order near boundary have conformal compactifications that are $C^{m+2,α}$ up to the boundary when Weyl curvature is in $C^{m,α}$ and the boundary metric is in $C^{m+2,α}$ where $m\geq 3.$
description: 24 pages