cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: ADCO, Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Cart. 32 (G 136), 745 folios, f. 0501
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: Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Archives départementales de la Côte-d'Or, Cart. 32 (G 136), 745 folios, f. 0501, 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. 0501, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: http://www.wikidata.org/entity/Q15945019
description: Provenance: abbaye Saint-Étienne de Dijon
Tunable light flow control in valley photonic crystal waveguide
Creators: name: Chen, Xiao-Dong
name: Shi, Fu-Long
name: Liu, Huan
name: Lu, Jin-Cheng
name: Deng, Wei-Min
name: Dai, Jun-Yan
name: Cheng, Qiang
name: Dong, Jian-Wen
Publisher: name: arXiv
Year: 2018
Subjects: subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: The exploration of binary valley degree of freedom in topological photonic systems has inspired many intriguing optical phenomena such as photonic Hall effect, robust delay lines, and perfect out-coupling refraction. In this work, we experimentally demonstrate the tunability of light flow in a valley photonic crystal waveguide. By continuously controlling the phase difference of microwave monopolar antenna array, the flow of light can split into different directions according to the charily of phase vortex, and the splitting ratio varies smoothly from 0.9 to 0.1. Topological valley transport of edge states is also observed at photonic domain wall. Tunable edge state dispersion, i.e., from gapless valley dependent modes to gapped flat bands, is found at the photonic boundary between a valley photonic crystal waveguide and a perfect electric conductor, leading to the tunable frequency bandwidth of high transmission. Our work paves a way to the controllability and dynamic modulations of light flow in topological photonic systems.
description: 16 pages, 4 figures
Lyman alpha absorption in the nearby universe: the sightline to Q1821+643
Creators: name: Bowen, David V.
name: Pettini, Max
name: Boyle, Brian
Publisher: name: arXiv
Year: 1997
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present the first results of a survey designed to understand the origin of the Lyman alpha-forest absorption systems at low redshift. Using the WYFFOS and HYDRA multi-fibre spectrographs on the WHT and WIYN telescopes, we have identified 51 galaxies brighter than b_j=18.5 within 30 arcmins of the sightline of the QSO 1821+643. We find three galaxies within 500 h-1 kpc of the QSO sightline; the nearest galaxy is 104 h-1 kpc away from the line of sight, and is at the same redshift as a strong Lyman alpha absorption line. The remaining two galaxies have no corresponding absorption to extremely low equivalent width limits (< 0.05 Å). Beyond 500 h-1 kpc Lyman-alpha absorption lines are found at similar redshifts as several galaxies, but we show that these coincidences are likely to be accidental. Half of the Lyman alpha systems for which we could have found at least an L^* galaxy have no galaxies at the absorbers' redshifts. For the majority of the remainder, we show that any apparent association with galaxies is probably coincidental. These \lya systems are characterised by their weak equivalent widths (W_r < 0.2 Å), and we conclude that this population of absorbers is uncorrelated, or at best, weakly correlated, with galaxies.
description: New version accepted by MNRAS
Additional file 1: of Non-application of the nursing process at a hospital in Accra, Ghana: lessons from descriptive research
Creators: name: Agyeman-Yeboah, Joana
name: Kwadwo Korsah
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Molecular Biology
subject: Sociology
subject: FOS: Sociology
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Developmental Biology
subject: Marine Biology
subject: Science Policy

description: Interview guide. (DOCX 13 kb)
Additional file 2: of Are smokers who are regularly exposed to e-cigarette use by others more or less motivated to stop or to make a quit attempt? A cross-sectional and longitudinal survey
Creators: name: Jackson, Sarah
name: Beard, Emma
name: Michie, Susan
name: Shahab, Lion
name: Raupach, Tobias
name: West, Robert
name: Brown, Jamie
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Pharmacology
subject: Biotechnology
subject: Evolutionary Biology
subject: Developmental Biology
subject: Cancer
subject: Science Policy
subject: 111714 Mental Health
subject: FOS: Health sciences
subject: 110309 Infectious Diseases
subject: Computational Biology

description: Table S2. Unadjusted and adjusted associations between exposure to e-cigarette use in others and past quit attempts, high motivation to stop smoking and prospective quit attempts. (DOCX 21 kb)
A Library for Wall-Modelled Large-Eddy Simulation Based on OpenFOAM Technology
Creators: name: Mukha, Timofey
name: Rezaeiravesh, Saleh
name: Liefvendahl, Mattias
Publisher: name: arXiv
Year: 2018
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: This work presents a feature-rich open-source library for wall-modelled large-eddy simulation (WMLES), which is a turbulence modelling approach that reduces the computational cost of traditional (wall-resolved) LES by introducing special treatment of the inner region of turbulent boundary layers (TBLs). The library is based on OpenFOAM and enhances the general-purpose LES solvers provided by this software with state-of-the-art wall modelling capability. In particular, the included wall models belong to the class of wall-stress models that account for the under-resolved turbulent structures by predicting and enforcing the correct local value of the wall shear stress. A review of this approach is given, followed by a detailed description of the library, discussing its functionality and extensible design. The included wall-stress models are presented, based on both algebraic and ordinary differential equations. To demonstrate the capabilities of the library, it was used for WMLES of turbulent channel flow and the flow over a backward-facing step (BFS). For each flow, a systematic simulation campaign was performed, in order to find a combination of numerical schemes, grid resolution and wall model type that would yield a good predictive accuracy for both the mean velocity field in the outer layer of the TBLs and the mean wall shear stress. The best result was achieved using a mildly dissipative second-order accurate scheme for the convective fluxes applied on an isotropic grid with 27000 cells per $δ^3$-cube, where $δ$ is the thickness of the TBL or the half-height of the channel. An algebraic model based on Spalding's law of the wall was found to perform well for both flows. On the other hand, the tested more complicated models, which incorporate the pressure gradient in the wall shear stress prediction, led to less accurate results.
OH Satellite Line Masers and an AGN Candidate in M82
Creators: name: Seaquist, E. R.
name: Frayer, D. T.
name: Frail, D. A.
Publisher: name: arXiv
Year: 1997
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report the detection of OH satellite line masers at 1720 MHz and 1612 MHz from the nuclear region of the starburst galaxy M82. The observations were aimed at detecting 1720 MHz maser emission from the known radio emitting SNR in the nuclear region. At 1720 MHz we detect six features above the 5-sigma limit set by noise, four in emission and two in absorption. Three of the emission features appear closely associated with known discrete continuum radio sources, and one of the absorption features is precisely coincident with the discrete continuum source 44.01+59.6. The latter source also exhibits strong 1612 MHz emission at the same velocity. No other 1612 MHz features were detected. All of the 1720 MHz emission features are consistent with masers pumped by collisions with molecular hydrogen at densities between 10^3 cm^{-3} and 10^5 cm^{-3}, and T_k between 50 K and 250 K. The absorption and emission associated with the two satellite lines in 44.01+59.6, together with other evidence, points to the possibility that this source is the AGN in M82.
description: accepted ApJL
Alosa maeotica
Creators: name: Nurettin Meriç
name: Lütfiye Eryilmaz
name: Müfit Özulug
Publisher: name: Zenodo
Year: 2007
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Actinopterygii
Clupeiformes
Clupeidae
Alosa
Alosa maeotica

description: Alosa maeotica (Grimm, 1901)
Inland water: 27100-808 (1 spc.), 07.09.1974, Apolyont Lake, Bursa, N. Meriç. Istanbul Fish Market: 27100-809 (1 spc.), 28.03.1968.
description: Published as part of Nurettin Meriç, Lütfiye Eryilmaz & Müfit Özulug, 2007, A catalogue of the fishes held in the Istanbul University, Science Faculty, Hydrobiology Museum., pp. 29-54 in Zootaxa 1472 on page 29
Additional file 2 of Construction of a survival prediction model for high-and low -grade UTUC after tumor resection based on “SEER database”: a multicenter study
Creators: name: Wang, Mengmeng
name: Ren, Xin
name: Wang, Ge
name: Sun, Xiaomin
name: Tang, Shifeng
name: Zhang, Baogang
name: Xing, Xiaoming
name: Zhang, Wenfeng
name: Gao, Guojun
name: Du, Jing
name: Zhang, Shukun
name: Liu, Lijuan
name: Zheng, Xia
name: Zhang, Zhenkun
name: Sun, Changgang
Publisher: name: figshare
Year: 2021
Subjects: Medicine
Cell Biology
Biological Sciences not elsewhere classified
Information Systems not elsewhere classified
Cancer
Science Policy

description: Additional file 2: Appendix Table 2. A table showing the percentage of surgical procedures. Partial nephrectomy: Partial or subtotal nephrectomy (kidney or renal pelvis) or partial ureterectomy; RNU:Complete/total/simple nephrectomy - for kidney parenchyma Nephroureterectomy; Any nephrectomy: Any nephrectomy (simple, subtotal, complete, partial, total, radical) PLUS an en bloc:resection of other organ(s) (colon, bladder); Nephrectomy, NOS:Nephrectomy, NOS;Ureterectomy, NOS.
The stellar populations of the central region of M31
Creators: name: Saglia, R. P.
name: Opitsch, M.
name: Fabricius, M. H.
name: Bender, R.
name: Blana, M.
name: Gerhard, O.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We continue the analysis of the dataset of our spectroscopic observation campaign of M31, by deriving simple stellar population properties (age metallicity and alpha-elements overabundance) from the measurement of Lick/IDS absorption line indices. We describe their two-dimensional maps taking into account the dust distribution in M31. 80\% of the values of our age measurements are larger than 10 Gyr. The central 100 arcsec of M31 are dominated by the stars of the classical bulge of M31. They are old (11-13 Gyr), metal-rich (as high as [Z/H]~0.35 dex) at the center with a negative gradient outwards and enhanced in alpha-elements ([alpha/Fe]~ 0.28+- 0.01 dex). The bar stands out in the metallicity map, where an almost solar value of [Z/H] (~0.02+-0.01 dex) with no gradient is observed along the bar position angle (55.7 deg) out to 600 arcsec from the center. In contrast, no signature of the bar is seen in the age and [alpha/Fe] maps, that are approximately axisymmetric, delivering a mean age and overabundance for the bar and the boxy-peanut bulge of 10-13 Gyr and 0.25-0.27 dex, respectively. The boxy/peanut-bulge has almost solar metallicity (-0.04+- 0.01 dex). The mass-to-light ratio of the three components is approximately constant at M/LV ~ 4.4-4.7 Msol/Lsol. The disk component at larger distances is made of a mixture of stars, as young as 3-4 Gyr, with solar metallicity and smaller M/LV (~3+-0.1 Msol/Lsol). We propose a two-phase formation scenario for the inner region of M31, where most of the stars of the classical bulge come into place together with a proto-disk, where a bar develops and quickly transforms it into a boxy-peanut bulge. Star formation continues in the bulge region, producing stars younger than 10 Gyr, in particular along the bar, enhancing its metallicity. The disk component appears to build up on longer time-scales.
description: Language-edited version, Accepted for publication in A&A
The interplay between Weak and Strong Phases and Direct CP Violation from the Charmless B-meson Decays
Creators: name: Zhou, Y. F.
name: Wu, Y. L.
name: Ng, J. N.
name: Geng, C. Q.
Publisher: name: arXiv
Year: 2000
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We present a general analysis on charmless B-meson decays $B\to ππ$ and $πK$. It is noticed that the final state interactions and inelastic rescattering effects must be significant in order to understand the consistency of the current data. By using general isospin decompositions, the isospin amplitudes and the corresponding strong phases could be extracted from a global $χ^2$ fit of the experimental data. We emphasize that in general there are two, rather than one, relative strong phases in the decomposition. In the assumption of two equalstrong phases as considered in the literature, the current data, especially the ones concerning $B\to π^0 K^{0(\pm)}$decays, will imply a large isospin amplitude $|a^c_{3/2}| > 40 $, which is larger by a factor of five than the one from the naive factorization estimation. When two different strong phases are considered, all the isospin amplitudes can become, within the $1σ$-level, comparable with the theoretical values. We also show that the difference between the two strong phases cannot be too large and will be restricted by the most recent upper bound of $B\to π^0π^0$ decay. In any case, the strong phases are found to be large and the branching ratio of $B\to π^0π^0$ is likely to be enhanced by an order of magnitude in comparison with the one obtained from the naive factorization approach. Direct CP violations in all decay modes are also calculated and found to be close to the sensitivity of the present experiments.
description: 18 pages, 6 figures, Revtex, revised version to be published in PRD
Particle Swarm Optimization based search for gravitational waves from compact binary coalescences: performance improvements
Creators: name: Normandin, Marc E.
name: Mohanty, Soumya D.
name: Weerathunga, Thilina S.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: While a fully-coherent all-sky search is known to be optimal for detecting signals from compact binary coalescences (CBCs), its high computational cost has limited current searches to less sensitive coincidence-based schemes. For a network of first generation GW detectors, it has been demonstrated that Particle Swarm Optimization (PSO) can reduce the computational cost of this search, in terms of the number of likelihood evaluations, by a factor of $\approx 10$ compared to a grid-based optimizer. Here, we extend the PSO-based search to a network of second generation detectors and present further substantial improvements in its performance by adopting the local-best variant of PSO and an effective strategy for tuning its configuration parameters. It is shown that a PSO-based search is viable over the entire binary mass range relevant to second generation detectors at realistic signal strengths.
description: 12 pages, 10 figures, Clarified chirp duration, Plot labels modified
Alosa caspia subsp. nordmanni Antipa 1906
Creators: name: Nurettin Meriç
name: Lütfiye Eryilmaz
name: Müfit Özulug
Publisher: name: Zenodo
Year: 2007
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Actinopterygii
Clupeiformes
Clupeidae
Alosa
Alosa caspia
Alosa caspia nordmanni antipa, 1906

description: Alosa caspia nordmanni Antipa, 1906
Inland water: 4300-65 (6 spa), 26.01.1972, Küçükçekmece Lagoon, Istanbul, N. Meriç; 4300-61, (1 spa), 26.01.1972, Küçükçekmece Lagoon, Istanbul, N. Meriç.
description: Published as part of Nurettin Meriç, Lütfiye Eryilmaz & Müfit Özulug, 2007, A catalogue of the fishes held in the Istanbul University, Science Faculty, Hydrobiology Museum., pp. 29-54 in Zootaxa 1472 on page 29
Supersymmetry without R-Parity and without Lepton Number
Creators: name: Banks, Tom
name: Grossman, Yuval
name: Nardi, Enrico
name: Nir, Yosef
Publisher: name: arXiv
Year: 1995
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We investigate Supersymmetric models where neither R parity nor lepton number is imposed. Neutrino masses can be kept highly suppressed compared to the electroweak scale if the $μ$-terms in the superpotential are aligned with the SUSY-breaking bilinear $B$-terms. This situation arises naturally in the framework of horizontal symmetries. The same symmetries suppress the trilinear R parity violating terms in the superpotential to an acceptable level.
description: 18 pages, harvmac
The Pinch Technique at Two Loops
Creators: name: Papavassiliou, Joannis
Publisher: name: arXiv
Year: 1999
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: It is shown that the fundamental properties of gauge-independence, gauge-invariance, unitarity, and analyticity of the $S$-matrix lead to the unambiguous generalization of the pinch technique algorithm to two loops.
description: 4 pages, uses Revtex, two figures in a separate ps file
Indications on the Higgs-Boson Mass from the LEP Data
Creators: name: Consoli, M.
name: Hioki, Z.
Publisher: name: arXiv
Year: 1995
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We update our previous analysis on the Higgs mass $m_h$ and the QCD coupling $α_s(=α_s(M_z))$ by using the LEP data after the 1995 Winter Conferences. For $m_t=180$ GeV we find evidence for a rather large value of the Higgs mass in the range 500-1000 GeV, in agreement with the indications from the W mass.
description: 15 pages, LaTeX
Alosa tanaica
Creators: name: Nurettin Meriç
name: Lütfiye Eryilmaz
name: Müfit Özulug
Publisher: name: Zenodo
Year: 2007
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Actinopterygii
Clupeiformes
Clupeidae
Alosa
Alosa tanaica

description: Alosa tanaica (Grimm, 1901)
Inland water: 27200-810 (1 spc.), 20.04.1975, Manyas Lake, Balikesir, N. Meriç.
description: Published as part of Nurettin Meriç, Lütfiye Eryilmaz & Müfit Özulug, 2007, A catalogue of the fishes held in the Istanbul University, Science Faculty, Hydrobiology Museum., pp. 29-54 in Zootaxa 1472 on page 29
Regularization Ambiguity Problem for the Chern-Simons Shift
Creators: name: Nittoh, K.
name: Ebihara, T.
Publisher: name: arXiv
Year: 1998
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We consider the Chern-Simons parameter shift with the hybrid regularization consisting of the higher covariant derivative (HCD) and the Pauli-Villars (PV) regulators. We show that the shift is closely related to the parity of the regulators and get the shift and no-shift results by a suitable choice of the PV regulators. A naive treatment of the HCD term leads incorrect value of the shift.
description: 7 pages, 1 figure, latex 2e, will appear at Mod. Phys. Lett. A
Neutron Star Population Dynamics.II: 3D Space Velocities of Young Pulsars
Creators: name: Cordes, J. M.
name: Chernoff, David F.
Publisher: name: arXiv
Year: 1997
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We use astrometric, distance and spindown data on pulsars to: (1) estimate three-dimensional velocity components, birth distances from the galactic plane, and ages of individual objects; (2) determine the distribution of space velocities and the scale height of pulsar progenitors; (3) test spindown laws for pulsars; (4) test for correlations between space velocities and other pulsar parameters; and (5) place empirical requirements on mechanisms than can produce high velocity neutron stars. Our approach incorporates measurement errors, uncertainties in distances, deceleration in the Galactic potential, and differential galactic rotation. We find that the scale height of the progenitors is approximately 0.13 kpc, that the 3D velocities are distributed in two components with characteristic speeds of 175(+20,-30) km/s and 700(+200,-150) km/s representing 83% and 17% of the population respectively. These results are insensitive to the explicit relation of chronological and spindown ages. We infer that the most probable chronological ages are typically smaller than conventional spindown ages by factors as large as two. We assess mechanisms for producing high-velocity neutron stars in view of the derived velocity distribution function.
description: 54 pages, 13 Postscript figures, uses AAS LaTeX v. 4.0
VIRTIGATION lunchtime webinar slides on cross-protection: combatting plant diseases with mild virus isolates
Creators: name: Ziebell, Heiko
Publisher: name: Zenodo
Year: 2025

description: This presentation was given by VIRTIGATION partner Julius-Kühn Institute (JKI) in the frame of the project lunchtime webinar on cross-protection as a tool to combat plant diseases with mild virus isolates.The VIRTIGATION project has received funding from the European Union's Horizon 2020 research and innovation program under grant agreement No. 101000570.
Dzyaloshinskii-Moriya interaction at disordered interfaces from ab initio theory: robustness against intermixing and tunability through dusting
Creators: name: Zimmermann, Bernd
name: Legrand, William
name: Maccariello, Davide
name: Reyren, Nicolas
name: Cros, Vincent
name: Blügel, Stefan
name: Fert, Albert
Publisher: name: arXiv
Year: 2018
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: The Dzyaloshinskii-Moriya interaction (DMI), which is essential for the stabilization of topologically non-trivial chiral magnetic textures such as skyrmions, is particularly strong in heterostructures of ultra-thin magnetic materials and heavy elements. We explore by density-functional theory calculations the possibility to modify the magnetic properties at Co/Pt interfaces with chemical disorder. In these systems, we find a particular robustness of the DMI against intermixing. Upon dusting the interface with a third element (all $4d$ transition metals and B, Cu, Au and Bi), a strong reduction of the DMI is predicted. This opens up possibilities to tune the DMI through the degrees of intermixing and dusting.
Additional file 1 of Association between adverse childhood experiences and premenstrual disorders: a cross-sectional analysis of 11,973 women
Creators: name: Yang, Qian
name: Þórðardóttir, Edda Björk
name: Hauksdóttir, Arna
name: Aspelund, Thor
name: Jakobsdóttir, Jóhanna
name: Halldorsdottir, Thorhildur
name: Tomasson, Gunnar
name: Rúnarsdóttir, Harpa
name: Danielsdottir, Hilda Björk
name: Bertone-Johnson, Elizabeth R.
name: Sjölander, Arvid
name: Fang, Fang
name: Lu, Donghao
name: Valdimarsdóttir, Unnur Anna
Publisher: name: figshare
Year: 2022
Subjects: subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Neuroscience
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Cancer
subject: Science Policy
subject: Mental Health

description: Additional file 1: Supplementary methods, Categorization of covariates. Figure S1. Flow chat. Figure S2. Distribution of ACE score. Figure S3. Standardized risk of PMDs over the total number of ACEs. Table S1. Required minimum frequency of events for ascertainment of ACEs. Table S2. Associations of accumulative ACEs with PMDs: complete-case analysis. Table S3. Associations of ACEs with premenstrual symptom score. Table S4. Associations of the number of ACEs with probable cases of PMDs, stratified by age group.
Associative photoproduction of charmed particles near threshold
Creators: name: Rekalo, Michail P.
name: Tomasi-Gustafsson, Egle
Publisher: name: arXiv
Year: 2000
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We calculate the cross section and the beam asymmetry for exclusive photoproduction of charmed particles near threshold ($γ+p\to Λ_c^+ +\bar{D^0}$), in the framework of an effective Lagrangian model. We discuss the sensitivity of these observables to the magnetic moment of the $Λ_c$ baryon and of the coupling constant in the $pΛ_c D$ vertex. We show that exclusive measurements allow, in principle, to determine the magnetic moments of charmed baryons.
description: 4 pages 4 figures
Renormalization of non-singlet quark operator matrix elements for deep-inelastic scattering
Creators: name: Van Thurenhout, Sam
name: Moch, Sven-Olaf
Publisher: name: arXiv
Year: 2021
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We introduce a new method for calculating the mixing matrix for non-singlet quark operators including total derivatives, based solely on their renormalization structure in the chiral limit. As input, the method requires the well-known forward anomalous dimensions, which determine the evolution of parton distribution functions, and a calculation of the matrix elements of operators without total derivatives. Assuming a large number of quark flavors $n_f$, we are able to calculate the mixing matrix to fifth order in the strong coupling $α_s$ in the $\overline{\mbox{MS}}$-scheme.
description: 14 pages, LaTeX, 1 figure, Proceedings to Matter To The Deepest 2021, journal version
Cortázar: Figuras y Límites
Creators: name: Eduardo G., González
name: González, Eduardo G.
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2021
Subjects: Literatura argentina
Experimentación
"Rayuela"

description: Notas: Texto escrito en Bennington College (EEUU, Vermont).
description: Source: Num.Ref. : JC-CAR-12.052
description: Source: Localización del archivo: Centre de Recherches Latino-Américaines (CRLA–Archivos, ITEM UMR8132). MSHS - Bât. A5, 1er étage 5 rue Théodore Lefebvre - TSA21103. 86073 Poitiers cedex 9.
description: Bibliographic citation: González, Eduardo G., « Cortázar: figuras y límites », Modern Language Notes, 89, núm. 2 (1974) , p. 232-249.
Working Group Summary: Pion-Nucleon Coupling Constant
Creators: name: Sainio, M. E.
Publisher: name: arXiv
Year: 1999
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: A brief introduction to different determinations of the piNN coupling constant is given, and some comments on the topics discussed in the working group are made.
description: 6 pages, 3 figures, 8th International Symposium on Meson-Nucleon Physics and the Structure of the Nucleon, Zuoz, Switzerland, Aug. 15-21, 1999
Curating a connected community in virtual space: Solomon Islands Research Mentoring Tok Stori
Creators: name: Sanga, Kabini
name: Reynolds, M
name: Malefoasi, A
name: Paulsen, I
Publisher: name: Open Access Te Herenga Waka-Victoria University of Wellington
Year: 2024
Subjects: classificationCode: 39
subject: Education
classificationCode: 3903
subject: Education systems
classificationCode: 3902
subject: Education policy, sociology and philosophy

description: This article examines the relationship between academic mentoring and tok stori, a Melanesian orality, in a digital environment. This relationship is significant where dispersal is an unintended consequence of the way development aid intersects with academic opportunities for scholars from less developed countries, and, consequently, country-focused academic communities remain undeveloped as education becomes individualised. This situation occurs despite the fact that the self is social and education is a common good in many contexts, such as Solomon Islands in Melanesia. Using the contributions of participants in the Solomon Islands Research Mentoring Tok Stori (SIRMT), we discuss the various kinds of support and outcomes that become possible when deliberate attempts are made to create a connected community through mentoring in virtual space. Among the findings are the significance of mentorship to personal and academic growth, the potential of deliberate community building through virtual means in Solomon Islands and virtual tok stori as a catalyst to developments the physical world.
Continuous condensation in nanogrooves
Creators: name: Malijevský, Alexandr
Publisher: name: arXiv
Year: 2018
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: We consider condensation in a capillary groove of width $L$ and depth $D$, formed by walls that are completely wet (contact angle $θ=0$), which is in a contact with a gas reservoir of the chemical potential $μ$. On a mesoscopic level, the condensation process can be described in terms of the midpoint height $\ell$ of a meniscus formed at the liquid-gas interface. For macroscopically deep grooves ($D\to\infty$), and in the presence of long-range (dispersion) forces, the condensation corresponds to a second order phase transition, such that $\ell\sim (μ_{cc}-μ)^{-1/4}$ as $μ\toμ_{cc}^-$ where $μ_{cc}$ is the chemical potential pertinent to capillary condensation in a slit pore of width $L$. For finite values of $D$, the transition becomes rounded and the groove becomes filled with liquid at a chemical potential higher than $μ_{cc}$ with a difference of the order of $D^{-3}$. For sufficiently deep grooves, the meniscus growth initially follows the power-law $\ell\sim (μ_{cc}-μ)^{-1/4}$ but this behaviour eventually crosses over to $\ell\sim D-(μ-μ_{cc})^{-1/3}$ above $μ_{cc}$, with a gap between the two regimes shown to be $\barδμ\sim D^{-3}$. Right at $μ=μ_{cc}$, when the groove is only partially filled with liquid, the height of the meniscus scales as $\ell^*\sim (D^3L)^{1/4}$. Moreover, the chemical potential (or pressure) at which the groove is half-filled with liquid exhibits a non-monotonic dependence on $D$ with a maximum at $D\approx 3L/2$ and coincides with $μ_{cc}$ when $L\approx D$. Finally, we show that condensation in finite grooves can be mapped on the condensation in capillary slits formed by two asymmetric (competing) walls a distance $D$ apart with potential strengths depending on $L$.
The first Pontryagin class of a quadratic Lie 2-algebroid
Creators: name: Sheng, Yunhe
Publisher: name: arXiv
Year: 2018
Subjects: subject: Differential Geometry (math.DG)
subject: Mathematical Physics (math-ph)
subject: Category Theory (math.CT)
subject: Symplectic Geometry (math.SG)
subject: FOS: Mathematics
subject: FOS: Physical sciences

description: In this paper, first we give a detailed study on the structure of a transitive Lie 2-algebroid and describe a transitive Lie 2-algebroid using a morphism from the tangent Lie algebroid TM to a strict Lie 3-algebroid constructed from derivations. Then we introduce the notion of a quadratic Lie 2-algebroid and define its first Pontryagin class, which is a cohomology class in H^5(M). Associated to a CLWX 2-algebroid, there is a quadratic Lie 2-algebroid naturally. Conversely, we show that the first Pontryagin class of a quadratic Lie 2-algebroid is the obstruction class of the existence of a CLWX-extension. Finally we construct a quadratic Lie 2-algebroid from a trivial principle 2-bundle with a Gamma-connection and show that its first Pontryagin class is trivial.
description: 28 pages
Dissipation of a tide in a differentially rotating star
Creators: name: Talon, Suzanne
name: Kumar, Pawan
Publisher: name: arXiv
Year: 1997
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The orbital period of the binary pulsar PSR J0045-7319, which is located in our neighbouring galaxy the Small Magellanic Cloud (SMC), appears to be decreasing on a timescale of half a million year. This timescale is more than two orders of magnitude smaller than what is expected from the standard theory of tidal dissipation. Kumar and Quataert (1997a) proposed that this rapid evolution can be understood provided that the neutron star's companion, a main sequence B-star, has set up significant differential rotation. They showed that the spin synchronization time for the B-star is similar to the orbit circularization time, whereas the time to synchronize the surface rotation is much shorter, and thus significant differential rotation in the star is indeed expected. However, their calculation did not include the various processes that can redistribute angular momentum in the star, possibly forcing it into solid body rotation; in that case the dissipation of the tide would not be enhanced. The goal of this paper is to include the redistribution of angular momentum in the B-star due to meridional circulation and shear stresses and to calculate the resulting rotation profile as a function of time. We find that although angular momentum redistribution is important, the B-star continues to have sufficient differential rotation so that tidal waves are entirely absorbed as they arrive at the surface. The mechanism proposed by Kumar and Quataert to speed up the orbital evolution of the SMC binary pulsar should therefore work as suggested.
description: 7 pages, LaTeX, 4 figures, Submitted to ApJ. Replaces astro-ph/9707309 (minor changes)
D2.5 Final Report on Project Impact
Creators: name: Geser, Guntram
name: Hollander, Hella
Publisher: name: Zenodo
Year: 2017

description: This report is a deliverable (D2.5) of the project ARIADNE - Advanced Research Infrastructure for Archaeological Dataset Networking in Europe that has been funded under the European Community’s Seventh Framework Programme. The document reports the final results of Task 2.5:  Impact Evaluation.

The report addresses the project objectives and the framework of the impact evaluation, summarises the overall results, and gives recommendations for ARIADNE and other stakeholders with a focus on potential further advances.
Visualization and analysis of continuous glucose monitoring data based on self-monitoring.
Creators: name: Yating Ke
Publisher: name: The University of North Carolina at Chapel Hill University Libraries
Year: 2024

description: Diabetes as a chronic disease affecting multiple age groups has been increasing in prevalence in recent years. This trend highlights the growing need for effective blood glucose monitoring in the wider population. Based on the continuous development of continuous glucose monitoring devices and the fact that daily glucose monitoring remains an important component in controlling the progression of the disease, the aim of this study was to develop an intuitive glucose visualization tool that utilizes continuous glucose test data to facilitate patient self-monitoring, self-management and support clinical decision-making at a potential level. By combining a user-friendly interface with advanced data analytics, the tool aims to empower patients in their daily diabetes management while providing valuable insights for medical review.
Additional file 1: of Effectiveness of contrast-associated acute kidney injury prevention methods; a systematic review and network meta-analysis
Creators: name: Ahmed, Khalid
name: McVeigh, Terri
name: Cerneviciute, Raminta
name: Mohamed, Sara
name: Tubassam, Mohammad
name: Karim, Mohammad
name: Walsh, Stewart
Publisher: name: figshare
Year: 2018
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics

description: Analysis flow chart and statistical approach. (DOCX 125 kb)
Production of a chaotic squeezed state from a ``pion liquid" and overbunching of identical pion correlations
Creators: name: Andreev, I. V.
name: Weiner, R. M.
Publisher: name: arXiv
Year: 1995
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: It is shown that a one to one correspondence between quantum fields in two different "phases" as might be realized for pions produced from a "hadron liquid" leads to squeezed states. The single and double inclusive cross sections for at chaotic superposition of such states are calculated. The correlation of identical pions is overbunched in comparison with canonical Bose-Einstein correlations.
description: Latex File, 6 pages
Alosa agone
Creators: name: Nurettin Meriç
name: Lütfiye Eryilmaz
name: Müfit Özulug
Publisher: name: Zenodo
Year: 2007
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Actinopterygii
Clupeiformes
Clupeidae
Alosa
Alosa agone

description: Alosa agone (Scopoli, 1786)
Sea of Marmara: 4400-66 (2 spc.), 30.09.1967, M. Demir; 4400-60 (1 spa), 30.09.1967, M. Demir; 4400-677 (1 spa), 17.04.1992, Front of Gônen Stream, trawl, 33 m, L. Eryilmaz. Aegean Sea: 4400-67 (4 spc.), 18.01.1969, Kusadasi Fish Market.
description: Published as part of Nurettin Meriç, Lütfiye Eryilmaz & Müfit Özulug, 2007, A catalogue of the fishes held in the Istanbul University, Science Faculty, Hydrobiology Museum., pp. 29-54 in Zootaxa 1472 on page 29
The pinch technique at two-loops: The case of mass-less Yang-Mills theories
Creators: name: Papavassiliou, Joannis
Publisher: name: arXiv
Year: 1999
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The generalization of the pinch technique beyond one loop is presented. It is shown that the crucial physical principles of gauge-invariance, unitarity, and gauge-fixing-parameter independence single out at two loops exactly the same algorithm which has been used to define the pinch technique at one loop, without any additional assumptions. The two-loop construction of the pinch technique gluon self-energy, and quark-gluon vertex are carried out in detail for the case of mass-less Yang-Mills theories, such as perturbative QCD. We present two different but complementary derivations. First we carry out the construction by directly rearranging two-loop diagrams. The analysis reveals that, quite interestingly, the well-known one-loop correspondence between the pinch technique and the background field method in the Feynman gauge persists also at two-loops. The renormalization is discussed in detail, and is shown to respect the aforementioned correspondence. Second, we present an absorptive derivation, exploiting the unitarity of the $S$-matrix and the underlying BRS symmetry; at this stage we deal only with tree-level and one-loop physical amplitudes. The gauge-invariant sub-amplitudes defined by means of this absorptive construction correspond precisely to the imaginary parts of the $n$-point functions defined in the full two-loop derivation, thus furnishing a highly non-trivial self-consistency check for the entire method. Various future applications are briefly discussed.
description: 29 pages, uses Revtex, 22 Figures in a separate ps file
A ring in a shell: the large-scale 6D structure of the Vela OB2 complex
Creators: name: Cantat-Gaudin, T.
name: Mapelli, M.
name: Balaguer-Núñez, L.
name: Jordi, C.
name: Sacco, G.
name: Vallenari, A.
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: The Vela OB2 association is a group of 10 Myr stars exhibiting a complex spatial and kinematic substructure. The all-sky Gaia DR2 catalogue contains proper motions, parallaxes (a proxy for distance) and photometry that allow us to separate the various components of Vela OB2. We characterise the distribution of the Vela OB2 stars on a large spatial scale, and study its internal kinematics and dynamic history. We make use of Gaia DR2 astrometry and published Gaia-ESO Survey data. We apply an unsupervised classification algorithm to determine groups of stars with common proper motions and parallaxes. We find that the association is made up of a number of small groups, with a total current mass over 2330 Msun. The three-dimensional distribution of these young stars trace the edge of the gas and dust structure known as the IRAS Vela Shell across 180 pc and shows clear signs of expansion. We propose a common history for Vela OB2 and the IRAS Vela Shell. The event that caused the expansion of the shell happened before the Vela OB2 stars formed, imprinted the expansion in the gas the stars formed from, and most likely triggered star formation.
description: Accepted by A&A (02 November 2018), 13 pages, 9+2 figures
Self-dual vortex-like configurations in SU(2) Yang-Mills Theory
Creators: name: Gonzalez-Arroyo, A.
name: Montero, A.
Publisher: name: arXiv
Year: 1998
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: High Energy Physics - Lattice (hep-lat)
subject: FOS: Physical sciences

description: We show that there are solutions of the SU(2) Yang-Mills classical equations of motion in R^4, which are self-dual and vortex-like(fluxons). The action density is concentrated along a thick two-dimensional wall (the world sheet of a straight infinite vortex line). The configurations are constructed from self-dual R^2 x T^2 configurations.
description: latex2e file. 10 pages 2 figures
Is the LMC Microlensing Due to an Intervening Dwarf Galaxy?
Creators: name: The MACHO Collaboration
name: Alcock, C.
name: Allsman, R. A.
name: Alves, D. R.
name: Axelrod, T. S.
name: Becker, A.
name: Bennett, D. P.
name: Cook, K. H.
name: Freeman, K. C.
name: Griest, K.
name: Lehner, M. J.
name: Marshall, S. L.
name: Minniti, D.
name: Peterson, B. A.
name: Pratt, M. R.
name: Quinn, P. J.
name: Rodgers, A. W.
name: Rorabeck, A.
name: Stubbs, C. W.
name: Sutherland, W.
name: Tomaney, A.
name: Vandehei, T.
name: Welch, D. L.
Publisher: name: arXiv
Year: 1997
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The recent suggestion that the microlensing events observed towards the Large Magellanic Cloud are due to an intervening Sgr-like dwarf galaxy is examined. A search for foreground RR Lyrae in the MACHO photometry database yields 20 stars whose distance distribution follow the expected halo density profile. Cepheid and red giant branch clump stars in the MACHO database are consistent with membership in the LMC. There is also no evidence in the literature for a distinct kinematic population, for intervening gas, or for the turn-off of such a hypothetical galaxy. We conclude that if the lenses are in a foreground galaxy, it must be a particularly dark galaxy.
description: 11 pages, 4 PostScript figures, uses aaspp4.sty. Submitted to The Astrophysical Journal Letters
Dancers/Archivists: Community Archiving Practices Among Country Dancers
Creators: name: Dean, Carrie
Publisher: name: The University of North Carolina at Chapel Hill University Libraries
Year: 2024
Subjects: country dance

description: Country dancing is a niche form of folk dance which, nevertheless, continues to flourish today. Country dance practitioners have unique information needs which are not met by traditional institutions, as well as a strong desire to preserve their dance form for future generations. As such, they have developed a variety of methods to preserve country dance ephemera and make it accessible to the broader dance community. This study describes some of these methods and how they have evolved in the digital age based on semi-structured interviews with country dance practitioners who have contributed to these efforts through the lens of community archiving.
The effect of ionic versus covalent functionalization of polyoxometalate hybrid materials with coordinating subunits on their stability and interaction with DNA
Creators: name: Nowicka, Daria
name: Marcinkowski, Dawid
name: Vadra, Nahir
name: Szymańska, Martyna
name: Kubicki, Maciej
name: Consiglio, Giuseppe
name: Drożdż, Wojciech
name: Stefankiewicz, Artur R.
name: Patroniak, Violetta
name: Fik-Jaskółka, Marta
name: Gorczyński, Adam
Publisher: name: Zenodo
Year: 2024

description: Inorganic-organic hybrid materials that combine both Polyoxometalates (POMs) and metal ion coordinating subunits (CSUs) represent promising multifunctional materials. Though their individual components are often biologically active, utilization of hybrid materials in bioassays significantly depends on the functionalization method and thus resulting stability of the system. Quite intriguingly, these aspects were very scarcely studied in hybrid materials based on Wells-Dawson POM (WD POM) scaffold and remain unknown. We chose two model WD POM hybrid systems to establish how the functionalization mode (ionic vs covalent) affects their stability in biological medium and interaction with nucleic acids. The synthetic scope and limitations of the covalent POM-terpyridine hybrids were demonstrated and compared with the ionic Complex-Decorated Surfactant Encapsulated-Clusters (CD-SECs) hybrids. The nature of POM and CSU binding can be utilized to modulate the stability of the hybrid and the extent of DNA binding. The above systems show the potential to behave as the model cargo-platforms of potential utilization in medicine and pharmacy.
description: We express gratitude to Dr. Aleksandra Bocian for help in synthesis of ionic hybrids H1ion -H7ion. This work was supported by the National Science Centre, Poland (grant numbers UMO-2022/45/N/ST4/00632 (D.N.), UMO-2022/45/N/ST4/00344 (D.M.), UMO-2019/32/C/ST4/00565 (W.D.), UMO-2022/47/B/ST4/02310 (V.P.)). Daria Nowicka is a scholarship holder of the Adam Mickiewicz University in Poznan Foundation for the academic year 2023/2024. MFJ: the work was supported by IDUB-UAM (project no. 038/04/NŚ/0023).