cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Exclusive semileptonic decays of heavy mesons in quark model
Creators: name: Melikhov, Dmitri
Publisher: name: arXiv
Year: 1996
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Semileptonic decays $D\to K,K^*,π,ρ$, $D_s\to η,η',ϕ$, and $B\to D,D^*,π,ρ$ are analyzed within the dispersion formulation of the quark model. The form factors at timelike $q$ are derived by the analytical continuation from spacelike $q$ in the form factors of the relativistic light--cone quark model. The resulting double spectral representations allow a direct calculation of the form factors in the timelike region. The results of the model are shown to be in good agreement with all available experimental data. From the analysis of the $B\to D,D^*$ decays we find $|V_{cb}|=0.037\pm 0.004$, and the $B\toπ,ρ$ decays give $|V_{ub}|=0.004\pm 0.001$.
description: revtex, 8 pages, 1 figure In this version the $V_ub$ and $V_cb$ are recalculated for $\tau_{B_0}=1.56\pm0.06$ (in previous version $\tau_{B_0}=1.50\pm0.11$ was used) and several misprints are corrected
title: ADCO, Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome VI, Cart. 190 (11 H 75), 316 folios, f. 0214v
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2012
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: 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 général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome VI, Archives départementales de la Côte-d'Or, Cart. 190 (11 H 75), 316 folios, f. 0214v, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome VI, Archives départementales de la Côte-d'Or, Cart. 190 (11 H 75), 316 folios, f. 0214v, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
title: 01_1841
Creators: name: Wesley Baldwin, John
name: Baldwin, John W.
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2018
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: L'ensemble de ces notes ont été crée par John Baldwin lors d'une de ses premières périodes de résidence à Paris. Ces documents comprennent tous les magistri qu’il avait pu rencontrer dans ses sources. Aux XIIème et XIIIème siècles, les universités n'existant pas encore, le titre de magister s'il évoque certainement une compétence n'est pas rattaché de façon systématique au passage par les écoles. De surcroît, les magistris sont le plus souvent désignés par leur seul prénom. La lecture de ces données est donc difficile et suppose un long travail pour tenter d'identifier un individu auquel on pourrait rattacher plusieurs mentions. John Baldwin avait donc renoncé à utiliser ces données pour donner un prolongement à sa magnifique étude sur les gradués d'université et leur emploi par les Capétiens et les Plantagenêts. Néanmoins, il a conservé ces données et elles sont potentiellement très utile dans le cadre de Studium, comme le sont toutes les mentions dans les volumes des Fasti Ecclesiae Gallicanae de chanoines portant ce titre de magister sans autres précisions. L'ampleur des dépouillements rend ces données très utiles et nous devons une grande reconnaissance à John Baldwin pour avoir pris la peine de faire photocopier ses fiches et de nous les avoir transmises amicalement.
Les données ainsi que les images des fiches sont accessibles sur le site Internet à l'adresse suivante : http://studium-baldwin.lamop.fr/.
Les transcriptions des fiches ont été effectuées par des étudiants de Paris 1 Panthéon - Sorbonne mais elles n'ont pas été corrigées par la suite.
description: Relation: https://lamop.hypotheses.org/
Atomic data from the Iron Project.XLIII. Transition probabilities for Fe V
Creators: name: Nahar, Sultana N.
name: Delahaye, Franck
name: Pradhan, Anil K.
name: Zeippen, C. J.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: Atomic Physics (physics.atom-ph)
subject: FOS: Physical sciences

description: An extensive set of dipole-allowed, intercombination, and forbidden transition probabilities for Fe V is presented. The Breit-Pauli R-matrix (BPRM) method is used to calculate 1.46 x 10^6 oscillator strengths for the allowed and intercombination E1 transitions among 3,865 fine-structure levels dominated by configuration complexes with n <= 10 and l <= 9. These data are complemented by an atomic structure configuration interaction (CI) calculation using the SUPERSTRUCTURE program for 362 relativistic quadrupole (E2) and magnetic dipole (M1) transitions among 65 low-lying levels dominated by the 3d^4 and 3d^ 4s configurations. Procedures have been developed for the identification of the large number of fine-structure levels and transitions obtained through the BPRM calculations. The target ion Fe VI is represented by an eigenfunction expansion of 19 fine-structure levels of 3d^3 and a set of correlation configurations. Fe V bound levels are obtained with angular and spin symmetries SLπand Jπof the (e + Fe VI) system such that 2S+1 = 5,3,1, L <= 10, J <= 8 of even and odd parities. The completeness of the calculated dataset is verified in terms of all possible bound levels belonging to relevant LS terms and transitions in correspondence with the LS terms. The fine-structure averaged relativistic values are compared with previous Opacity Project LS coupling data and other works. The 362 forbidden transition probabilities considerably extend the available data for the E2 and M1 transtions, and are in good agreement with those computed by Garstang for the 3d^4 transitions.
description: 19 pages, 1 figure. This paper marks the beginning of a large-scale effort of ab initio atomic calculations that should eventually lead to re-calculation of accurate iron opacities. Astron. Astrophys. Suppl. Ser. (in press)
title: Opstellen astronomische voorspellingen: deelrapport 2. Validatie Prospermodel
Creators: name: Coen, Leen
name: Vanlede, Joris
name: Deschamps, Maarten
name: Mostaert, Frank
Publisher: name: Flanders Hydraulics Research
Year: 2021

description: Title : WL Rapporten. Waterbouwkundig Laboratorium: Antwerpen Volume : PA013_2 Issue : Pagination : VIII, 15 + 17 p. bijl.
Redshift Evolution of Galaxy Cluster Densities
Creators: name: Carlberg, R. G.
name: Morris, S. L.
name: Yee, H. K. C.
name: Ellingson, E.
Publisher: name: arXiv
Year: 1996
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The number of rich galaxy clusters per unit volume is a strong function of Omega, the cosmological density parameter, and sigma_8, the linear extrapolation to z=0 of the density contrast in 8/h Mpc spheres. The CNOC cluster redshift survey provides a sample of clusters whose average mass profiles are accurately known, which enables a secure association between cluster numbers and the filtered density perturbation spectrum. We select from the CNOC cluster survey those EMSS clusters with bolometric L_x>=10^45 erg/s and a velocity dispersion exceeding 800 km/s in the redshift ranges 0.18-0.35 and 0.35-0.55. We compare the number density of these subsamples with similar samples at both high and low redshift. Using the Press-Schechter formalism and CDM style structure models, the density data are described with sigma_8=0.75+/-0.1 and Omega=0.4+/-0.2 (90% confidence). The cluster dynamical analysis gives Omega=0.2+/-0.1$ for which sigma_8=0.95+/-0.1 (90% confidence). The predicted cluster density evolution in an Ω=1 CDM model exceeds that observed by more than an order of magnitude.
description: Revised version accepted for publication in ApJLetts. 10 pages. Also available at http://manaslu.astro.utoronto.ca/~carlberg/cnoc/sigma8/s8.ps.gz
Vacuum structure and effective potential at finite temperature: a variational approach
Creators: name: Mishra, Amruta
name: Mishra, Hiranmaya
Publisher: name: arXiv
Year: 1996
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We compute the effective potential for $ϕ^4$ theory with a squeezed coherent state type of construct for the ground state. The method essentially consists in optimising the basis at zero and finite temperatures. The gap equation becomes identical to resumming the infinite series of daisy and super daisy graphs while the effective potential includes multiloop effects and agrees with that obtained through composite operator formalism at finite temperature.
description: 15 pages, Revtex, No figures, to appear in Jou. of Phys.G(Nucl. and Part. Phys.)
Formation of Disk Galaxies: On the Angular Momentum Problem, the Tully-Fisher Relation and Magnetohydrodynamics
Creators: name: Sommer-Larsen, Jesper
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Two ways of possibly solving the angular momentum problem plaguing cold dark matter (CDM) ab initio simulations of disk galaxy formation are discussed: 1) Stellar feedback processes and 2) Warm dark matter (WDM) rather than CDM. In relation to the chemical evolution of disk galaxies our simulations indicate that in case 1) the first generation of disk stars formed in disk galaxies like the Milky Way should have an abundance about two dex below solar, in fairly good agreement with the lowest observed abundance of the metal-weak tail of the Galactic thick disk. For the second case no such statements can be made without further assumptions about the star-formation history of the galaxies. We find that the I-band Tully-Fisher relation can be matched by WDM disk galaxy formation simulations provided (M/L_I) is about 0.8 for disk galaxies, which Sommer-Larsen & Dolgov (1999) argue is a reasonable value. Finally it is discussed how the magnetic field strengths observed in galactic disks can be obtained through disk galaxy formation, as an alternative to the conventional dynamo hypothesis.
description: 10 pages incl. 5 figures (Kluwer NATO format). Contribution to the Roma-Trieste Workshop 1999 "The Chemical Evolution of the Milky Way: Stars versus Clusters", Vulcano, September 20-24, 1999
The Sigma Commutator from Lattice QCD
Creators: name: Wright, Stewart V.
name: Leinweber, Derek B.
name: Thomas, Anthony W.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Nuclear Theory (nucl-th)
subject: High Energy Physics - Lattice (hep-lat)
subject: FOS: Physical sciences

description: As a direct source of information on chiral symmetry breaking within QCD, the sigma commutator is of considerable importance. Since hadron structure is a non-perturbative problem, numerical calculations on a space-time lattice are currently the only rigorous approach. With recent advances in the calculation of hadron masses within full QCD, it is of interest to see whether the sigma commutator can be calculated directly from the dependence of the nucleon mass on the input quark mass. We show that, provided the correct chiral behaviour of QCD is respected in the extrapolation to realistic quark masses, one can indeed obtain a fairly reliable determination of the sigma commutator using present lattice data. For two-flavour dynamical fermion QCD the sigma commutator lies between 45 and 55 MeV based on recent data from CP-PACS and UKQCD.
description: 4 pages, 3 figures, uses espcrc1.sty and epsfig.sty. Contribution to the proceedings of the International Conference on Quark Nuclear Physics held in Adelaide Feb. 2000
MOESM2 of High-density lipoprotein (HDL) particle size and concentration changes in septic shock patients
Creators: name: Tanaka, SĂŠbastien
name: Diallo, DĂŠvy
name: Delbosc, Sandrine
name: GenĂ¨ve, Claire
name: Zappella, Nathalie
name: Yong-Sang, Jennyfer
name: Patche, Jessica
name: Harrois, Anatole
name: Hamada, Sophie
name: Denamur, Erick
name: Montravers, Philippe
name: Duranteau, Jacques
name: Meilhac, Olivier
Publisher: name: figshare
Year: 2019
Subjects: subject: Biochemistry
subject: Medicine
subject: Cell Biology
subject: Molecular Biology
subject: Environmental Sciences not elsewhere classified
subject: Ecology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: Virology

description: Additional file 2: Figure S2. Correlation between the percentage of large and small HDL particles and LBP concentration at day 1.
A totally bounded Uniformity on coarse metric Spaces
Creators: name: Hartmann, Elisa
Publisher: name: arXiv
Year: 2017
Subjects: subject: Metric Geometry (math.MG)
subject: General Topology (math.GN)
subject: FOS: Mathematics

description: This paper presents a new version of boundary on coarse spaces. The space of ends functor maps coarse metric spaces to uniform topological spaces and coarse maps to uniformly continuous maps.
CARRERA JUDICIAL Y EVALUACION DEL DESEMPEÑO
Creators: name: Juan F. Jiménez Mayor
Publisher: name: Zenodo
Year: 2007

description: CONTENIDO: Dos pequeñas historias; I. Introducción a la evaluación del desempeño; II. Concepto y utilidad de la evaluación del desempeño; III. La evaluación del desempeño en los servidores públicos; IV. La evaluación del desempeño en el ámbito judicial; V. Justicia y rendición de cuentas; VI. Un modelo a buscar; A modo de conclusión; Fin de las historias.
Mesogenic behaviour of isomeric bent-core 6-oxoverdazyls: 1,3-vrs 1,5-substitution pattern
Creators: name: Ciastek-Iskrzycka, Sylwia
name: Gerding, Jason
name: Kaszyński, Piotr
name: Pociecha, Damian
Publisher: name: Taylor & Francis
Year: 2018
Subjects: subject: Space Science
subject: 29999 Physical Sciences not elsewhere classified
subject: FOS: Physical sciences
subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences

description: Two series of isomeric bent-core derivatives of 6-oxoverdazyl, with alkyl and partially fluorinated alkyl chains, were investigated by thermo-optical, powder X-ray diffraction and electron paramagnetic resonance methods in the pure state and binary mixtures. The results revealed that the substitution position of the arms at the verdazyl ring (1,5 vs. 1,3) strongly affects mesogenic behaviour. Steric (torsion and bending angles) and dipolar factors in both isomers are considered.
Determinant expressions of constraint polynomials and the spectrum of the asymmetric quantum Rabi model
Creators: name: Kimoto, Kazufumi
name: Reyes-Bustos, Cid
name: Wakayama, Masato
Publisher: name: arXiv
Year: 2017
Subjects: subject: Mathematical Physics (math-ph)
subject: Representation Theory (math.RT)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences
subject: FOS: Mathematics
subject: 34L40 (Primary) 81Q10, 34M05, 81S05 (Secondary)

description: The purpose of this paper is to study the exceptional eigenvalues of the asymmetric quantum Rabi models (AQRM), specifically, to determine the degeneracy of their eigenstates. Here, the Hamiltonian $H^ε_{\text{Rabi}}$ of the AQRM is defined by adding the fluctuation term $εσ_x$, with $σ_x$ being the Pauli matrix, to the Hamiltonian of the quantum Rabi model, breaking its $\mathbb{Z}_{2}$-symmetry. The spectrum of $H^ε_{\text{Rabi}}$ contains a set of exceptional eigenvalues, considered to be remains of the eigenvalues of the uncoupled bosonic mode, which are further classified in two types: Juddian, associated with polynomial eigensolutions, and non-Juddian exceptional. We explicitly describe the constraint relations for allowing the model to have exceptional eigenvalues. By studying these relations we obtain the proof of the conjecture on constraint polynomials previously proposed by the third author. In fact, we prove that the spectrum of the AQRM possesses degeneracies if and only if the parameter $ε$ is a half-integer. Moreover, we show that non-Juddian exceptional eigenvalues do not contribute any degeneracy and we characterize exceptional eigenvalues by representations of $\mathfrak{sl}_2$. Upon these results, we draw the whole picture of the spectrum of the AQRM. Furthermore, generating functions of constraint polynomials from the viewpoint of confluent Heun equations are also discussed.
description: 68 pages. The organization of the manuscript was changed to improve clarity
Characteristics and practices of school-based cluster randomised controlled trials for improving health outcomes in pupils in the United Kingdom: a methodological systematic review
Creators: name: Parker, Kitty
name: Nunns, Michael
name: Xiao, ZhiMin
name: Ford, Tamsin
name: Ukoumunne, Obioha C.
Publisher: name: Apollo - University of Cambridge Repository
Year: 2021
Subjects: Research
Child and adolescent health
Cluster randomised trials
Public health
Randomised trials
Research methods
Schools
Systematic review

description: Abstract: Background: Cluster randomised trials (CRTs) are increasingly used to evaluate non-pharmacological interventions for improving child health. Although methodological challenges of CRTs are well documented, the characteristics of school-based CRTs with pupil health outcomes have not been systematically described. Our objective was to describe methodological characteristics of these studies in the United Kingdom (UK). Methods: MEDLINE was systematically searched from inception to 30th June 2020. Included studies used the CRT design in schools and measured primary outcomes on pupils. Study characteristics were described using descriptive statistics. Results: Of 3138 articles identified, 64 were included. CRTs with pupil health outcomes have been increasingly used in the UK school setting since the earliest included paper was published in 1993; 37 (58%) studies were published after 2010. Of the 44 studies that reported information, 93% included state-funded schools. Thirty six (56%) were exclusively in primary schools and 24 (38%) exclusively in secondary schools. Schools were randomised in 56 studies, classrooms in 6 studies, and year groups in 2 studies. Eighty percent of studies used restricted randomisation to balance cluster-level characteristics between trial arms, but few provided justification for their choice of balancing factors. Interventions covered 11 different health areas; 53 (83%) included components that were necessarily administered to entire clusters. The median (interquartile range) number of clusters and pupils recruited was 31.5 (21 to 50) and 1308 (604 to 3201), respectively. In half the studies, at least one cluster dropped out. Only 26 (41%) studies reported the intra-cluster correlation coefficient (ICC) of the primary outcome from the analysis; this was often markedly different to the assumed ICC in the sample size calculation. The median (range) ICC for school clusters was 0.028 (0.0005 to 0.21). Conclusions: The increasing pool of school-based CRTs examining pupil health outcomes provides methodological knowledge and highlights design challenges. Data from these studies should be used to identify the best school-level characteristics for balancing the randomisation. Better information on the ICC of pupil health outcomes is required to aid the planning of future CRTs. Improved reporting of the recruitment process will help to identify barriers to obtaining representative samples of schools.
INDEPENDENCIA  FUNCIONAL: REQUISITO ESENCIAL DEL  PERFIL DEL JUEZ
Creators: name: Ricardo J. Moreno Ccancce
Publisher: name: Zenodo
Year: 2007

description:  SUMARIO: I.- LA CONDENA A MUERTE DE JESUS, EL AVASALLAMIENTO DE LA JUSTICIA POR LA POLITICA, II.- INDEPENDENCIA JUDICIAL EN EL PERU CONTEMPORANEO, III.INDEPENDENCIA DEL PODER JUDICIAL, IV.- INDEPENDENCIA INTERNA O FUNCIONAL DEL JUEZ, V.- LA EXCELENCIA JUDICIAL, LA ETICA JUDICIAL e INDEPENDECIA FUNCIONAL DEL JUEZ;VI.- CONCLUSIONES.
Probing the origins. I. Generalised Additive Model inference of birth radii for Milky Way stars in the solar vicinity
Creators: name: Dantas, M. L. L.
name: Smiljanic, R.
name: de Souza, R. S.
name: Tissera, P. B.
name: Magrini, L.
Publisher: name: arXiv
Year: 2025
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We employ a Generalised Additive Model (GAM) to address the limitations inherent in radial metallicity gradients predicted by chemical evolution models, thereby facilitating the estimation of birth radii for the thin disc stars in our sample based on their ages and chemical composition. We then juxtapose the birth radius predictions derived from the GAM with the calculated guiding radii, among other dynamic parameters. Metal-rich stars, formed in the inner regions of the Milky Way, seem to be predominantly churned outward. Their metal-poor counterparts, formed in the outer thin disc, exhibit the opposite behaviour. The proportion of blurred/undisturbed stars generally increases with decreasing metallicity when compared to their churned counterparts. Approximately $3/4$ of the sample has been affected by (inward or outward) churning, while the remaining $\sim 1/4$ has either been influenced by blurring or remained undisturbed. These percentages vary considerably across different metallicity-stratified groups. Also, a large age gap is identified between churned and blurred/undisturbed sub-samples within each HC-based group, being the outward-churned stars systematically the oldest, inward-churned stars the youngest, and blurred/undisturbed stars in intermediate ages. We also detect significant differences in angular momenta in the $z$ component, for stars that have either churned inward or outward, when compared to their blurred/undisturbed counterparts. Additionally, we observe the potential effects of the pericentric passage of the Sagittarius dwarf galaxy in our most metal-poor subset of stars, formed in the outer disc. Finally, we estimate that the Sun's most probable birth radius is $7.08 \pm 0.24$ kpc, with a 3$σ$ range spanning from 6.46 to 7.81 kpc, in agreement with previous studies.
description: Published in Astronomy & Astrophysics (A&A). 35 pages; 21 figures in the main text + 18 figures in the appendix. Minor formatting changes were made to the arXiv version to ensure proper compilation, but the scientific content remains unchanged. Abdriged abstract to meet arXiv's length requirements; we strongly recommend reading the full abstract. Version after language proofs
Controlled mutation in the replication of synthetic oligomers.
Creators: name: Núñez-Villanueva, Diego
name: Hunter, Christopher A
Publisher: name: Apollo - University of Cambridge Repository
Year: 2021

description: Replication of sequence information with mutation is the molecular basis for the evolution of functional biopolymers. Covalent template-directed synthesis has been used to replicate sequence information in synthetic oligomers, and the covalent base-pairs used in these systems provide an opportunity to manipulate the outcome of the information transfer process through the use of traceless linkers. Two new types of covalent base-pair have been used to introduce mutation in the replication of an oligotriazole, where information is encoded as the sequence of benzoic acid and phenol monomer units. When a benzoic acid-benzoic acid base-pairing system was used, a direct copy of a benzoic acid homo-oligomer template was obtained. When a phenol-benzoic acid base-pairing system was used, a reciprocal copy, the phenol homo-oligomer, was obtained. The two base-pairing systems are isosteric, so they can be used interchangeably, allowing direct and reciprocal copying to take place simultaneously on the same template strand. As a result, it was possible to introduce mutations in the replication process by spiking the monomer used for direct copying with the monomer used for reciprocal copying. The mutation rate is determined precisely by the relative proportions of the two monomers. The ability to introduce mutation at a controlled rate is a key step in the development of synthetic systems capable of evolution, which requires replication with variation.
Additional file 2: of Host genetics influence the rumen microbiota and heritable rumen microbial features associate with feed efficiency in cattle
Creators: name: Li, Fuyong
name: Li, Changxi
name: Chen, Yanhong
name: Liu, Junhong
name: Zhang, Chunyan
name: Irving, Barry
name: Fitzsimmons, Carolyn
name: Plastow, Graham
name: Guan, Le
Publisher: name: figshare
Year: 2019
Subjects: subject: Space Science
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Evolutionary Biology
subject: Chemical Sciences not elsewhere classified
subject: Ecology
subject: Biological Sciences not elsewhere classified

description: Table S2. Diet information for animal experiments. (DOCX 17 kb)
UCLA Beekeeping Program Proposal: Assessing Student Interest and Building a Framework for a Campus Apiary
Creators: name: Glory Thai
Publisher: name: figshare
Year: 2018
Subjects: subject: 160802 Environmental Sociology
subject: FOS: Sociology
subject: 50203 Environmental Education and Extension
subject: FOS: Earth and related environmental sciences
subject: 160810 Urban Sociology and Community Studies

description: Research paper detailing our methodology, findings, and conclusions.
Neutron Star Structure and the Equation of State
Creators: name: Lattimer, J. M.
name: Prakash, M.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: The structure of neutron stars is considered from theoretical and observational perspectives. We demonstrate an important aspect of neutron star structure: the neutron star radius is primarily determined by the behavior of the pressure of matter in the vicinity of nuclear matter equilibrium density. In the event that extreme softening does not occur at these densities, the radius is virtually independent of the mass and is determined by the magnitude of the pressure. For equations of state with extreme softening, or those that are self-bound, the radius is more sensitive to the mass. Our results show that in the absence of extreme softening, a measurement of the radius of a neutron star more accurate than about 1 km will usefully constrain the equation of state. We also show that the pressure near nuclear matter density is primarily a function of the density dependence of the nuclear symmetry energy, while the nuclear incompressibility and skewness parameters play secondary roles. In addition, we show that the moment of inertia and the binding energy of neutron stars, for a large class of equations of state, are nearly universal functions of the star's compactness. These features can be understood by considering two analytic, yet realistic, solutions of Einstein's equations, due, respectively, to Buchdahl and Tolman. We deduce useful approximations for the fraction of the moment of inertia residing in the crust, which is a function of the stellar compactness and, in addition, the presssure at the core-crust interface.
description: 51 pages, 10 figures, submitted to ApJ
Dynamical properties of dissipative XYZ Heisenberg lattices
Creators: name: Rota, Riccardo
name: Minganti, Fabrizio
name: Biella, Alberto
name: Ciuti, Cristiano
Publisher: name: arXiv
Year: 2017
Subjects: subject: Quantum Physics (quant-ph)
subject: Other Condensed Matter (cond-mat.other)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: We study dynamical properties of dissipative XYZ Heisenberg lattices where anisotropic spin-spin coupling competes with local incoherent spin flip processes. In particular, we explore a region of the parameter space where dissipative magnetic phase transitions for the steady state have been recently predicted by mean-field theories and exact numerical methods. We investigate the asymptotic decay rate towards the steady state both in 1D (up to the thermodynamical limit) and in finite-size 2D lattices, showing that critical dynamics does not occur in 1D, but it can emerge in 2D. We also analyze the behavior of individual homodyne quantum trajectories, which well reveal the nature of the transition.
title: ESLO1: conversation téléphonique 319_C
Creators: name: Laboratoire Ligérien De Linguistique
name: Baude, Olivier
name: Dugua, Céline
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2015
Subjects: subject: Français
subject: fra
subject: text_and_corpus_linguistics

description: Extrait du corpus d'Orléans, réalisé dans le cadre de l'Enquête SocioLinguistique à Orléans à la fin des années 1960.
description: Conforms to: doi:10.34847/cocoon.69c4fa74-f324-3ddb-9f1a-580867fd5826
Ruination in Wounded Baghdad: Visualizing and Problematizing the Spatialization of Destruction
Creators: name: Al-Shamali, Farah
Publisher: name: figshare
Year: 2024
Subjects: classificationCode: 470206
subject: Cultural studies of nation and region
classificationCode: 440612
subject: Urban geography
classificationCode: 470208
subject: Culture, representation and identity
classificationCode: 369999
subject: Other creative arts and writing not elsewhere classified

description: Considering Baghdadi urbanity today translates into contending with spatial destruction and what that leaves behind as far as the spirit of the wounded city. Going beyond the mere physical, pain that is exacted onto space is imprinted upon the psyche of streets and alleyways so much so that the relationship becomes a perplexing one. Place and people alike are beckoned into attempting to reckon and engage with the wound. It has become part of the spatial fabric and so must be looked at as such. History and historiography have additionally illustrated topological ruin that had been visited upon the capital since its founding. Journeying through the recent past and present requires addressing this accumulated spatial confusion. It means taking in the place-based nuances that are as psychogeographical as they are arbitrary. Iraqi creatives have done this repeatedly by rendering the hurt and settling it into their outputs. The problematization of space in this sense is an opportunity to, as the city fell into a new pattern of being, migrate the politics of the situation into a poetics. Disastrous violence essentially fashions a different character. It is only in this way that the cycle of devastation may physically cease to arrest and interrupt existence when it is allowed into the fold of the spatial everyday. It is then that urban life may find a new tone and tenor not merely surviving but allowing woundedness to have potentiality.
title: ADCO, Comptes du Petit-Cîteaux (1477-1491) (11 H 1179), f. 00500
Creators: name: de la Côte d'Or, Archives départementales
name: Petot, Frédéric
name: Archives Départementales De La Côte-D'Or
name: Archives Départementales De La Côte D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CBMA/CG21/F.PETOT/2019
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: cartulaire
subject: Chartes de la Bourgogne du Moyen Âge
subject: comptes

description: Comptes du Petit-Cîteaux (1477-1491), Archives départementales de la Côte-d'Or, (11 H 1179). Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Comptes du Petit-Cîteaux (1477-1491), Archives départementales de la Côte-d'Or, (11 H 1179), f. 00500, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https://manuscrits.cbma-project.eu/
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
Peculiar modules for 4-ended tangles
Creators: name: Zibrowius, Claudius
Publisher: name: arXiv
Year: 2017
Subjects: subject: Geometric Topology (math.GT)
subject: Quantum Algebra (math.QA)
subject: Symplectic Geometry (math.SG)
subject: FOS: Mathematics

description: With a 4-ended tangle $T$, we associate a Heegaard Floer invariant $\operatorname{CFT^\partial}(T)$, the peculiar module of $T$. Based on Zarev's bordered sutured Heegaard Floer theory, we prove a glueing formula for this invariant which recovers link Floer homology $\operatorname{\widehat{HFL}}$. Moreover, we classify peculiar modules in terms of immersed curves on the 4-punctured sphere. In fact, based on an algorithm of Hanselman, Rasmussen and Watson, we prove general classification results for the category of curved complexes over a marked surface with arc system. This allows us to reinterpret the glueing formula for peculiar modules in terms of Lagrangian intersection Floer theory on the 4-punctured sphere. We then study some applications: firstly, we show that peculiar modules detect rational tangles. Secondly, we give short proofs of various skein exact triangles. Thirdly, we compute the peculiar modules of the 2-stranded pretzel tangles $T_{2n,-(2m+1)}$ for $n,m>0$ using nice diagrams. We then observe that these peculiar modules enjoy certain symmetries which imply that mutation of the tangles $T_{2n,-(2m+1)}$ preserves $δ$-graded, and for some orientations even bigraded link Floer homology.
description: 83 pages, many PSTricks figures. Only minor changes to v2. This version of the paper has been accepted by the Journal of Topology for publication
Electromagnetic moments of relativistic higher spin baryons
Creators: name: Pascalutsa, V.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We point out a source of ambiguities in the measurements of the electromagnetic moments of spin-3/2 baryons which rely on relativistic Lagrangian models. An anambiguous relation between the parameters of the spin-3/2 electromagnetic Lagrangian and the electromagnetic moments of the spin-3/2 particle exits in general only for on-shell situation, while the measurements are done on ``virtual'' baryons.
description: 4 pages, 2 figures; contribution to the proceedings of the International Conference on Quark Nuclear Physics (Adelaide, February 2000)
Control of excitonic absorption by thickness variation in few-layer GaSe
Creators: name: Budweg, Arne
name: Yadav, Dinesh
name: Grupp, Alexander
name: Leitenstorfer, Alfred
name: Trushin, Maxim
name: Pauly, Fabian
name: Brida, Daniele
Publisher: name: arXiv
Year: 2017
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: We control the thickness of GaSe on the level of individual layers and study the corresponding optical absorption via highly sensitive differential transmission measurements. Suppression of excitonic transitions is observed when the number of layers is smaller than a critical value of 8. Through ab-initio modelling we are able to link this behavior to a fundamental change in the band structure that leads to the formation of a valence band shaped as an inverted Mexican hat in thin GaSe. The thickness-controlled modulation of the optical properties provides attractive resources for the development of functional optoelectronic devices based on a single material.
French court-aires with their ditties Englished: how language influences text settings in the 17th century French air de cour
Creators: name: KATHRYN JANE SULLIVAN
Publisher: name: Monash University
Year: 2019
Subjects: subject: 190409 Musicology and Ethnomusicology
subject: FOS: Arts (arts, history of arts, performing arts, music)

description: Understanding how words and music combine to produce a song has occupied musicians and poets for centuries. The relationships that words and music form make the task of achieving such an understanding complex and never ending, but important to pursue, because of the centrality of song as a mode of human expression. This thesis examines the relationship between text and music in the seventeenth-century French air de cour and how an attempt to translate them into English diminished their aesthetic potency. Central to this thesis is a case study of Edward Filmer’s 1629 collection French court-aires with their ditties Englished.
Size conservation emerges spontaneously in biomolecular condensates formed by scaffolds and surfactant clients
Creators: name: Sanchez-Burgos, Ignacio
name: Joseph, Jerelle A.
name: Collepardo-Guevara, Rosana
name: Espinosa, Jorge R.
Publisher: name: Apollo - University of Cambridge Repository
Year: 2021
Subjects: Article
/639/766/747
/631/57/2266
article

description: Funder: Junior Research Fellow at Kings College
description: Funder: Ernest Oppenheimer Memorial Trust; doi: http://dx.doi.org/10.13039/501100009978
description: Abstract: Biomolecular condensates are liquid-like membraneless compartments that contribute to the spatiotemporal organization of proteins, RNA, and other biomolecules inside cells. Some membraneless compartments, such as nucleoli, are dispersed as different condensates that do not grow beyond a certain size, or do not present coalescence over time. In this work, using a minimal protein model, we show that phase separation of binary mixtures of scaffolds and low-valency clients that can act as surfactants—i.e., that significantly reduce the droplet surface tension—can yield either a single drop or multiple droplets that conserve their sizes on long timescales (herein ‘multidroplet size-conserved’ scenario’), depending on the scaffold to client ratio. Our simulations demonstrate that protein connectivity and condensate surface tension regulate the balance between these two scenarios. The multidroplet size-conserved scenario spontaneously arises at increasing surfactant-to-scaffold concentrations, when the interfacial penalty for creating small liquid droplets is sufficiently reduced by the surfactant proteins that are preferentially located at the interface. In contrast, low surfactant-to-scaffold concentrations enable continuous growth and fusion of droplets without restrictions. Overall, our work proposes one thermodynamic mechanism to help rationalize how size-conserved coexisting condensates can persist inside cells—shedding light on the roles of protein connectivity, binding affinity, and droplet composition in this process.
Examples of legal text
Creators: name: Perehudoff, Katrina
Publisher: name: figshare
Year: 2018
Subjects: subject: 111799 Public Health and Health Services not elsewhere classified
subject: FOS: Health sciences

description: This Annex presents an overview of innovative text for access to medicines identified in national UHC legislation. The legal texts below have been edited for clarity. The original texts in the national language and English can be found the respective country profiles in our online appendix.
Original article: Legislating for universal access to medicines: A rights-based cross-national comparison of UHC laws in 16 health systemsAuthors: S. Katrina Perehudoff, Nikita V. Alexandrov, Hans V. Hogerzeil Date: 14 June 2018
Improved Spin Basis for Angular Correlation Studies in Single Top Quark Production at the Tevatron
Creators: name: Mahlon, Gregory
name: Parke, Stephen
Publisher: name: arXiv
Year: 1996
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We show in single top quark production that the spin of the top quark is correlated with the direction of the d-type quark in the event. For single top production in the W* channel, the d-type quark comes dominantly from the antiproton at the Tevatron, whereas for the W-gluon fusion channel the spectator jet is the d-type quark the majority of the time at this machine. Our results are that 98% of the top quarks from the W* process have their spins in the antiproton direction, and 96% of the top quarks in the W-gluon fusion process have their spins in the spectator jet direction. We also compare with the more traditional, but less effective, helicity basis. The direction of the top quark spin is reflected in angular correlations in its decay products.
description: 19 pages, LaTeX, 6 postscript figures included. Final version, as will appear in Phys. Rev. D
Is occupational physical activity associated with mortality in UK Biobank?
Creators: name: Pearce, Matthew
name: Strain, Tessa
name: Wijndaele, Katrien
name: Sharp, Stephen J.
name: Mok, Alexander
name: Brage, Søren
Publisher: name: Apollo - University of Cambridge Repository
Year: 2021
Subjects: Research
Paradox
Labour
Heavy
Leisure-time

description: Abstract: Background: Current physical activity guidelines do not distinguish between activity accumulated in different behavioural domains but some studies suggest that occupational physical activity (OPA) may not confer health benefits and could even be detrimental. The purpose of this study was to investigate associations between OPA and mortality outcomes. Methods: From baseline (2006–2010), 460,901 UK Biobank participants (aged 40–69 years) were followed for a median 12.0 (IQR: 11.3–12.7) years. OPA was categorised by cross-tabulating degree of manual work and walking/standing work amongst those in paid employment (n = 267,765), and combined with categories of occupational status for those not in paid employment (n = 193,136). Cox proportional hazards models were used to estimate sex-stratified hazard ratios (HR) and 95% confidence intervals (CI) for mortality from all causes, CVD, and cancer by occupational group, and for working hours/week and non-occupational physical activity stratified by occupational group. Models included adjustment for age and a range of lifestyle, socio-economic and health-related covariates. Results: During 5,449,989 person-years of follow-up, 28,740 deaths occurred. Compared to those reporting no heavy manual or walking/standing work (e.g. sedentary office workers) and adjusting for covariates, retirement was associated with lower mortality in women (HR = 0.62, CI: 0.53–0.72) and men (HR = 0.80, CI: 0.71–0.90), whereas unemployment was associated with higher mortality in men only (HR = 1.24, CI: 1.07–1.45). Within the working population, there was no evidence of differences in all-cause, CVD or cancer mortality by OPA group when comparing those reporting higher levels of OPA to the lowest OPA reference group for both women and men. Working < 35 h/week versus 35–40 h/week was associated with lower mortality in women (HR = 0.85, CI: 0.79–0.92) and men (HR = 0.83, CI: 0.78–0.89), with no interaction by OPA. Non-occupational physical activity was associated with lower mortality in working women (HR = 0.89 per 5 kJ/day/kg, CI: 0.84–0.95) and men (HR = 0.87 per 5 kJ/day/kg, CI: 0.84–0.91), with no interaction by OPA group. Conclusions: Jobs classified as higher levels of OPA may not be as active as reported, or the types of physical activity performed in those jobs are not health-enhancing. Irrespective of OPA category or employment status, non-occupational physical activity appears to provide health benefits.
Effect of magnetic field on neutrino annihilation efficiency in gamma-ray bursts
Creators: name: Du, Shuang
name: Peng, Fang-Kun
name: Long, Guang-Bo
name: Li, Miao
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Neutrino annihilation process on a hyperaccreting disk is one of the leading models to explain the generation of relativistic jets of gamma-ray bursts (GRBs). However, there is still uncertainty regarding the NAE of neutron star-accretion disc (NS-disc) system because of complicated microphysics processes and effects of strong magnetic field. In this paper, we investigate the NAE by assuming that the prompt jet of GRB 070110 is driven by neutrino pair annihilation in the NS-disc system. Our calculation shows $η_{ν\barν}> 1.2 \times 10^{-3}$ under the estimated accretion rate $\dot{M}\simeq 0.04\rm M_{\odot}\cdot s^{-1}$. Independent of the detailed accretion disc models, our result shows that the magnetic field may play an important role in the neutrino annihilation process on the hyperaccreting magnetized accretion disc. Compared with the theoretical value of $η_{\rm ν\barν}$ of the nonmagnetized BH-disc system, the NAE should increase significantly in the case of the NS-disc system if the GRB is powered by magnetar-disc system.
description: Fixed some mistakes, 5 pages, 3 figures,MNRAS published
The Progenitor Masses of Wolf-Rayet Stars and Luminous Blue Variables Determined from Cluster Turn-offs. I. Results from 19 OB Associations in the Magellanic Clouds
Creators: name: Massey, Philip
name: Waterhouse, Elizabeth
name: DeGioia-Eastwood, Kathleen
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We combine new CCD UBV photometry and spectroscopy with that from the literature to investigate 19 Magellanic Cloud OB associations that contain Wolf-Rayet (WR) and other types of evolved massive stars. Our spectroscopy reveals a wealth of newly identified interesting objects, including early O-type supergiants, a high mass double-lined binary in the SMC, and, in the LMC, a newly confirmed LBV (R 85), a newly discovered WR star (Sk-69 194), and a newly found luminous B[e] star (LH85-10). We use the data to evaluate the extent that each association is coeval, and for the ones with little age spread, determine the turn-off masses of the unevolved stars, as a means of finding the progenitor masses of LBVs and WRs. Our data is also used to find the (minimum) bolometric corrections that apply to these evolved objects. We find that WRs in the SMC come from only the highest mass stars (>70Mo), while in the LMC the WNEs come from a wide range of masses---possibly all stars with masses >30Mo pass though a WNE stage at LMC metallicities. In both the SMC and LMC the WCs appear to come from the same mass range as do the WNs, a finding that has important implications for interpreting the WC/WN ratio among Local Group galaxies. LBVs appear to come from the very highest mass stars. The Ofpe/WN9 stars, sometimes implicated in the "LBV phenonomon" come from very modest mass stars, 25-35Mo, suggesting a different origin for their variability. The BCs of WRs are considerably more negative than those of O-type stars, with BC(WNE)=-6.0 mag and BC(WC4)=-5.5mag; more modest values are found for the Ofpe/WN9 stars (-2 to -4 mag). These findings are consistent with recent analysis done with Hillier's "standard model".
description: To appear in the Astronomical Journal. Also available from ftp://gemini.tuc.noao.edu/pub/massey/mcwr.ps.Z