cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Additional file 1 of Safer prescription of drugs: impact of the PREFASEG system to aid clinical decision-making in primary care in Catalonia
Creators: name: Pons-Mesquida, M. Àngels
name: Oms-Arias, Míriam
name: Diogène-Fadini, Eduard
name: Figueras, Albert
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Molecular Biology
subject: Pharmacology
subject: Biotechnology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Additional file 1. Annex Table 1. Description of the types of PREFASEG alerts; Annex Table 2. Groups of pharmacological duplications included in PREFASEG in 2018; Annex Table 3. Definitions of the AEMPS safety alerts included in PREFASEG in 2018; Annex Table 4. List of drugs not recommended for use in geriatrics in 2018.
Small group elicitation session on passives and reciprocals
Creators: name: Massoma, Achille
name: Sandy, Clare S.
Publisher: name: California Language Archive, University of California, Berkeley
Year: 2022
Subjects: subject: abb

description: 'the carrying' - nominal form; BÓlÓn 'lose (misplace)' - no passive; pimbi 'get lost' - stative ('be lost'), passive, gerund, causative ('lose someone'), assocative, no applicative; 'write' - passive, associative; 'put' - no passive; 'put' - associative; 'blow' - no passive, no associative, no nominal, subjunctive; 'receive a guest' - stative, -seghe stative?, present, past, various; 'receive a guest' - no associative; 'bite' - passive, applicative, gerund, nominal; reciprocals - 'meet', 'love e.o.', 'fought e.o.', associative for 'fought'; 'hear', 'listen' - transitive, reciprocal; reciprocal - 'beat', 'kill', 'count', 'help'; associative - 'kill'; catch' - transitive, reciprocal; 'eat' - reciprocal, instrumental associative, various tenses; 'dance' - assoc/recip, assoc; 'cook' applic, applic/recip; 'take' (= leave + reciprocal) nominal; 'leave' subjunctive, stative, present, nominal; 'bring' (= arrive + reciprocal) nominal, causative; metatony w/ LMH.
Dust Destruction in Fast Shocks of Core-Collapse Supernova Remnants in the Large Magellanic Cloud
Creators: name: Williams, Brian J.
name: Borkowski, K. J.
name: Reynolds, S. P.
name: Blair, W. P.
name: Ghavamian, P.
name: Hendrick, S. P.
name: Long, K. S.
name: Points, S.
name: Raymond, J. C.
name: Sankrit, R.
name: Smith, R. C.
name: Winkler, P. F.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report observations with the MIPS instrument aboard the {\it Spitzer Space Telescope} (SST) of four supernova remnants (SNRs) believed to be the result of core-collapse SNe: N132D (0525-69.6), N49B (0525-66.0), N23 (0506-68.0), and 0453-68.5. All four of these SNRs were detected in whole at 24 $μ$m and in part at 70 $μ$m. Comparisons with {\it Chandra} broadband X-ray images show an association of infrared (IR) emission with the blast wave. We attribute the observed IR emission to dust that has been collisionally heated by electrons and ions in the hot, X-ray emitting plasma, with grain size distributions appropriate for the LMC and the destruction of small grains via sputtering by ions. As with our earlier analysis of Type Ia SNRs, models can reproduce observed 70/24 $μ$m ratios only if effects from sputtering are included, destroying small grains. We calculate the mass of dust swept up by the blast wave in these remnants, and we derive a dust-to-gas mass ratio of several times less than the often assumed value of 0.25% for the LMC. We believe that one explanation for this discrepancy could be porous (fluffy) dust grains.
description: Accepted for publication in ApJ Letters, references fixed
Further evidence for linearly-dispersive Cooper pairs
Creators: name: de Llano, M.
name: Valencia, J. J.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: A recent Bose-Einstein condensation (BEC) model of several cuprate superconductors is based on bosonic Cooper pairs (CPs) moving in 3D with a quadratic energy-momentum (dispersion) relation. The 3D BEC condensate-fraction vs. temperature (T/Tc, where Tc is the BEC transition temperature) formula poorly fits penetration-depth data for two cuprates in the range (1/2, 1]. We show how these fits are dramatically improved assuming cuprates to be quasi-2D, and how equally good fits obtain for conventional 3D and quasi-1D nanotube superconducting data, provided the correct CP dispersion is assumed in BEC at their assumed corresponding dimensionalities. This is offered as additional concrete empirical evidence for linearly-dispersive pairs in another recent BEC scenario of superconductors within which a BCS condensate turns out to be a very special case.
description: 9 pages, 1 figure
Nonlinear Diffusion Through Large Complex Networks Containing Regular Subgraphs
Creators: name: Volchenkov, D.
name: Blanchard, Ph.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: FOS: Physical sciences

description: Transport through generalized trees is considered. Trees contain the simple nodes and supernodes, either well-structured regular subgraphs or those with many triangles. We observe a superdiffusion for the highly connected nodes while it is Brownian for the rest of the nodes. Transport within a supernode is affected by the finite size effects vanishing as $N\to\infty.$ For the even dimensions of space, $d=2,4,6,...$, the finite size effects break down the perturbation theory at small scales and can be regularized by using the heat-kernel expansion.
description: 21 pages, 2 figures included
Strong large scale magnetic fields in rotating convection-driven dynamos: the important role of magnetic diffusion
Creators: name: Yan, Ming
name: Calkins, Michael A.
Publisher: name: arXiv
Year: 2021
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: Geophysics (physics.geo-ph)
subject: FOS: Physical sciences

description: Natural dynamos such as planets and stars generate global scale magnetic field despite the inferred presence of small scale turbulence. Such systems are known as large scale dynamos and are typically driven by convection and influenced by rotation. Previous numerical studies of rotating dynamos generally find that the large scale magnetic field becomes weaker as the flow becomes more turbulent. The underlying physical processes necessary for sustaining so-called large scale dynamos is therefore still debated. Here we use a suite of numerical simulations to show that strong large scale magnetic fields can be generated in rotating convective turbulence provided that two conditions are satisfied: (1) the flow remains rotationally constrained; and (2) magnetic diffusion is important on the small convective length scale. These findings are in agreement with previous asymptotic predictions and suggest that natural dynamos might satisfy these two conditions.
description: 6 pages, 4 figures
Additional file 1 of Cycling kinematics in healthy adults for musculoskeletal rehabilitation guidance
Creators: name: Yum, Haeun
name: Kim, Hyang
name: Lee, Taeyong
name: Park, Moon Seok
name: Lee, Seung Yeol
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Physiology
subject: FOS: Biological sciences
subject: 69999 Biological Sciences not elsewhere classified

description: Additional file 1: Supplement 1. Subjects’ data.
Tracing early structure formation with massive starburst galaxies and their implications for reionization
Creators: name: Nagamine, Kentaro
name: Cen, Renyue
name: Furlanetto, Steven R.
name: Hernquist, Lars
name: Night, Christopher
name: Ostriker, Jeremiah P.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Cosmological hydrodynamic simulations have significantly improved over the past several years, and we have already shown that the observed properties of Lyman-break galaxies (LBGs) at z=3 can be explained well by the massive galaxies in the simulations. Here we extend our study to z=6 and show that we obtain good agreement for the LBGs at the bright-end of the luminosity function (LF). Our simulations also suggest that the cosmic star formation rate density has a peak at z= 5-6, and that the current LBG surveys at z=6 are missing a significant number of faint galaxies that are dimmer than the current magnitude limit. Together, our results suggest that the universe could be reionized at z=6 by the Pop II stars in ordinary galaxies. We also estimate the LF of Lyman-alpha emitters (LAEs) at z=6 by relating the star formation rate in the simulation to the Ly-alpha luminosity. We find that the simulated LAE LFs agree with the observed data provided that the net escape fraction of Ly-alpha photon is f_{Ly-alpha} <= 0.1. We investigate two possible scenarios for this effect: (1) all sources in the simulation are uniformly dimmer by a factor of 10 through attenuation, and (2) one out of ten LAEs randomly lights up at a given moment. We show that the correlation strength of the LAE spatial distribution can possibly distinguish the two scenarios.
description: 9 pages, 4 figures. Summary of the talk given at the "First Light & Reionization" workshop at UC Irvine, May 2005. The published article is available from http://dx.doi.org/10.1016/j.newar.2005.11.002
The WZNW model on PSU(1,1|2)
Creators: name: Gotz, Gerhard
name: Quella, Thomas
name: Schomerus, Volker
Publisher: name: arXiv
Year: 2006
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Mathematical Physics (math-ph)
subject: Quantum Algebra (math.QA)
subject: FOS: Physical sciences
subject: FOS: Mathematics

description: According to the work of Berkovits, Vafa and Witten (hep-th/9902098), the non-linear sigma model on the supergroup PSU(1,1|2) is the essential building block for string theory on AdS(3)xS(3)xT(4). Models associated with a non-vanishing value of the RR flux can be obtained through a psu(1,1|2) invariant marginal deformation of the WZNW model on PSU(1,1|2). We take this as a motivation to present a manifestly psu(1,1|2) covariant construction of the model at the Wess-Zumino point, corresponding to a purely NSNS background 3-form flux. At this point the model possesses an enhanced psu(1,1|2) current algebra symmetry whose representation theory, including explicit character formulas, is developed systematically in the first part of the paper. The space of vertex operators and a free fermion representation for their correlation functions is our main subject in the second part. Contrary to a widespread claim, bosonic and fermionic fields are necessarily coupled to each other. The interaction changes the supersymmetry transformations, with drastic consequences for the multiplets of localized normalizable states in the model. It is only this fact which allows us to decompose the full state space into multiplets of the global supersymmetry. We analyze these decompositions systematically as a preparation for a forthcoming study of the RR deformation.
description: 59 pages, 2 figures, v2: a couple of typos corrected, in particular above eq. (2.26) the labels of the representations which decouple. The modifications have no affect on any of the formulas
Entanglement purification without controlled-NOT gates by using the natural dynamics of spin chains
Creators: name: Maruyama, Koji
name: Nori, Franco
Publisher: name: arXiv
Year: 2008
Subjects: subject: Quantum Physics (quant-ph)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We present a simple protocol to purify bipartite entanglement in spin-1/2 particles by utilizing only natural spin-spin interactions, i.e. those that can commonly be realized in realistic physical systems, and S_z-measurements on single spins. Even the standard isotropic Heisenberg interaction is shown to be sufficient to purify mixed state entanglement if there are at least three pairs of spins. This approach could be useful for quantum information processing in solid-state-based systems.
description: 4 figures
Small group elicitation session on gerunds versus nominals
Creators: name: Massoma, Achille
name: Sandy, Clare S.
Publisher: name: California Language Archive, University of California, Berkeley
Year: 2022
Subjects: subject: abb

description: Gerund vs. nominal for 'extinguish'; gerund vs. nominal for 'eat'; 'walk' vs. 'take', gerunds and nominals; gerunds for 'take'; gerunds for 'take'; gerund for 'count'; noun for 'the washing'; gerund for 'profit'; gerund vs. noun for 'send'; gerund for 'cover' (bute), gerund vs. noun for 'have' and 'catch'; gerund for 'write'; gerund for 'put', 'sell'; gerund vs. noun for 'blow'; gerund vs. noun for 'change' vs. 'exchange'; gerund vs. noun for 'resemble'; gerund vs. noun for 'receive (guest)'; gerund vs. noun for 'try', associative, applicative; misc. tone questions from Larry; misc. tone questions from Larry; gerund vs. noun for 'block'; gerund vs. noun for 'hide'; gerund vs. noun for 'clean'; gerund vs. noun for 'forbid, refuse'; gerund vs. noun for 'know'.
Dissecting Nearby Galaxies with piXedfit: I. Spatially Resolved Properties of Stars, Dust, and Gas as Revealed by Panchromatic SED Fitting
Creators: name: Abdurro'uf
name: Lin, Yen-Ting
name: Hirashita, Hiroyuki
name: Morishita, Takahiro
name: Tacchella, Sandro
name: Akiyama, Masayuki
name: Takeuchi, Tsutomu T.
name: Wu, Po-Feng
Publisher: name: arXiv
Year: 2021
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We study spatially resolved properties (on spatial scales of $\sim 1-2$ kpc out to at least $3$ effective radii) of the stars, dust, and gas in ten nearby spiral galaxies. The properties of the stellar population and dust are derived by fitting the spatially resolved spectral energy distribution (SED) with more than 20 photometric bands ranging from far-ultraviolet to far-infrared. Our newly developed software piXedfit performs point spread function matching of images, pixel binning, and models the stellar light, dust attenuation, dust emission, and emission from a dusty torus heated by an active galactic nucleus simultaneously through the energy balance approach. With this self-consistent analysis, we present the spatially resolved version of the IRX--$β$ relation, finding that it is consistent with the relationship from the integrated photometry. We show that the old stellar populations contribute to the dust heating, which causes an overestimation of star formation rate (SFR) derived from the total ultraviolet and infrared luminosities on kpc scales. With archival high-resolution maps of atomic and molecular gas, we study the radial variation of the properties of the stellar populations (including stellar mass, age, metallicity, and SFR), dust (including dust mass, dust temperature, and abundance of polycyclic aromatic hydrocarbon), gas, as well as dust-to-stellar mass and dust-to-gas mass ratios. We observe a depletion of molecular gas mass fraction in the central region of the majority of the galaxies, suggesting that the lack of available fuel is an important factor in suppressing the specific SFR at the center.
description: 35 pages, 19 figures, 4 tables. Accepted by ApJ (results remain the same). Complementary figures to Fig. 4 (for 10 galaxies) and high resolution version of Fig. 8 are available at https://github.com/aabdurrouf/maps-nearby-galaxies
Additional file 4 of Long-term effects of alcohol consumption on cognitive function in seniors: a cohort study in China
Creators: name: Han, Lizhen
name: Jia, Jinzhu
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Pharmacology
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Additional file 4: Table S1 Results of dynamic Cox model IV (contains samples from the 1st random sample, n = 1292).
INTEGRAL observation of the accreting pulsar GX 1+4
Creators: name: Ferrigno, Carlo
name: Segreto, Alberto
name: Santangelo, Andrea
name: Wilms, Joern
name: Kreykenbohm, Ingo
name: Denis, Miroslav
name: Staubert, Ruediger
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present the results of the INTEGRAL monitoring campaign on the accreting low mass X-ray binary pulsar GX 1+4 performed during the Galactic plane scan of the INTEGRAL Core Programme. The source was observed in different luminosity states ranging from L(20-40 keV)= 1.7x10^{-10} erg/cm^2/s, to L(20-40 keV)=10.5x10^{-10} erg/cm^2/s for about 779 ks from March 2003 until October 2004. Our observations confirm the secular spin down of GX 1+4 with the spin-period varying from 139.63 s to 141.56 s. In the highest luminosity state a spin-up phase is observed. The phase-averaged spectrum of the source was modelled either with an absorbed cut-off power law or with a Comptonization model with significantly different parameters in the two brightest luminosity states. No evidence for any absorption-like feature is observed in the phase-averaged spectrum up to 110 keV. At highest luminosity, the source is found to pulsate up to 130 keV. Phase-resolved spectroscopy reveals a phase-dependent continuum and marginal evidence of an absorption feature at 34 keV in the descending part of the pulse. If interpreted as due to electron resonant cyclotron scattering, the magnetic field in the emitting region would be 2.9x10^{12}(1+z) G where z is the gravitational red shift of the emitting region. We also observed a very low luminosity state typical of this source, which lasted for about two days during which the source spectrum was modelled by a simple power-law and a pulsed signal was still detectable in the 15-100 keV energy range.
description: 15 pages, 13 figures. Accepted for publication on Astronomy and Astrophysics. Introduced language editing corrections
The cooperative effect of load and disorder in thermally activated rupture of a two-dimensional random fuse network
Creators: name: Guarino, Alessio
name: Vanel, Loïc
name: Scorretti, Riccardo
name: Ciliberto, Sergio
Publisher: name: arXiv
Year: 2006
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: A random fuse network, or equivalently a two-dimensional spring network with quenched disorder, is subjected to a constant load and thermal noise, and studied by means of numerical simulations. Rupture is thermally activated and the lifetime follows an Arrhenius law where the energy barrier is reduced by disorder. Due to the non-homogeneous distribution of forces from the stress concentration at microcrack tips, spatial correlations between rupture events appear, but they do not affect the energy barrier's dependence on the disorder; they affect only the coupling between the disorder and the applied load.
A spatio-temporal adaptive phase-field fracture method
Creators: name: Labanda, Nicolas A.
name: Espath, Luis
name: Calo, Victor Manuel
Publisher: name: arXiv
Year: 2021
Subjects: subject: Mathematical Physics (math-ph)
subject: Numerical Analysis (math.NA)
subject: FOS: Physical sciences
subject: FOS: Mathematics

description: We present an energy-preserving mechanic formulation for dynamic quasi-brittle fracture in an Eulerian-Lagrangian formulation, where a second-order phase-field equation controls the damage evolution. The numerical formulation adapts in space and time to bound the errors, solving the mesh-bias issues these models typically suffer. The time-step adaptivity estimates the temporal truncation error of the partial differential equation that governs the solid equilibrium. The second-order generalized-$α$ time-marching scheme evolves the dynamic system. We estimate the temporal error by extrapolating a first-order approximation of the present time-step solution using previous ones with backward difference formulas; the estimate compares the extrapolation with the time-marching solution. We use an adaptive scheme built on a residual minimization formulation in space. We estimate the spatial error by enriching the discretization with elemental bubbles; then, we localize an error indicator norm to guide the mesh refinement as the fracture propagates. The combined space and time adaptivity allows us to use low-order linear elements in problems involving complex stress paths. We efficiently and robustly use low-order spatial discretizations while avoiding mesh bias in structured and unstructured meshes. We demonstrate the method's efficiency with numerical experiments that feature dynamic crack branching, where the capacity of the adaptive space-time scheme is apparent. The adaptive method delivers accurate and reproducible crack paths on meshes with fewer elements.
description: Preprint
Dolichogenidea infima
Creators: name: Fernandez-Triana, Jose
name: Sakagami, Kota
name: Shimizu, So
Publisher: name: Zenodo
Year: 2018
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Braconidae
Dolichogenidea
Dolichogenidea infima

description: D. infima (Haliday, 1834): Propodeum mostly polished and without areola (only small rugae above nucha); ovipositor sheath much shorter (approximately 0.5 times) than metatibia.
description: Published as part of Fernandez-Triana, Jose, Sakagami, Kota & Shimizu, So, 2018, Dolichogenidea maetoi sp. nov. (Hymenoptera: Braconidae) from Japan, the first parasitoid wasp recorded from Hyblaea fortissima (Lepidoptera), pp. 167-175 in Acta Entomologica Musei Nationalis Pragae 58 (1) on page 172, DOI: 10.2478/aemnp-2018-0014, http://zenodo.org/record/3699178
Memory and compiler optimizations for low-power and -energy
Creators: name: Zendra, Olivier
Publisher: name: arXiv
Year: 2006
Subjects: subject: Programming Languages (cs.PL)
subject: Performance (cs.PF)
subject: FOS: Computer and information sciences

description: Embedded systems become more and more widespread, especially autonomous ones, and clearly tend to be ubiquitous. In such systems, low-power and low-energy usage get ever more crucial. Furthermore, these issues also become paramount in (massively) multi-processors systems, either in one machine or more widely in a grid. The various problems faced pertain to autonomy, power supply possibilities, thermal dissipation, or even sheer energy cost. Although it has since long been studied in harware, energy optimization is more recent in software. In this paper, we thus aim at raising awareness to low-power and low-energy issues in the language and compilation community. We thus broadly but briefly survey techniques and solutions to this energy issue, focusing on a few specific aspects in the context of compiler optimizations and memory management.
description: ICOOOLPS'2006 was co-located with the 20th European Conference on Object-Oriented Programming (ECOOP'2006)
Concentration inequalities and asymptotic results for ratio type empirical processes
Creators: name: Giné, Evarist
name: Koltchinskii, Vladimir
Publisher: name: arXiv
Year: 2006
Subjects: subject: Probability (math.PR)
subject: FOS: Mathematics
subject: 60E15 (Primary) 60F17, 60F15, 62G08, 68T10 (Secondary)

description: Let $\mathcal{F}$ be a class of measurable functions on a measurable space $(S,\mathcal{S})$ with values in $[0,1]$ and let \[P_n=n^{-1}\sum_{i=1}^nδ_{X_i}\] be the empirical measure based on an i.i.d. sample $(X_1,...,X_n)$ from a probability distribution $P$ on $(S,\mathcal{S})$. We study the behavior of suprema of the following type: \[\sup_{r_n
description: Published at http://dx.doi.org/10.1214/009117906000000070 in the Annals of Probability (http://www.imstat.org/aop/) by the Institute of Mathematical Statistics (http://www.imstat.org)
Generation of a superposition of odd photon number states for quantum information networks
Creators: name: Neergaard-Nielsen, J. S.
name: Nielsen, B. Melholt
name: Hettich, C.
name: Moelmer, K.
name: Polzik, E. S.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We report on the experimental observation of quantum-network-compatible light described by a non-positive Wigner function. The state is generated by photon subtraction from a squeezed vacuum state produced by a continuous wave optical parametric amplifier. Ideally, the state is a coherent superposition of odd photon number states, closely resembling a superposition of weak coherent states (a Schroedinger cat), with the leading contribution from a single photon state in the low parametric gain limit. Light is generated in a nearly perfect spatial mode with a Fourier-limited frequency bandwidth which matches well atomic quantum memory requirements. The source is also characterized by high spectral brightness with about 10,000 and more events per second routinely generated. The generated state of light is the ultimate input state for testing quantum memories, quantum repeaters and linear optics quantum computers.
description: 5 pages, 3 figures; added and updated references, minor clarifications in the text
Additional file 1 of Effectiveness and experiences of the Extension for Community Healthcare Outcomes (ECHO) Model in developing competencies among healthcare professionals: a mixed methods systematic review protocol
Creators: name: Chicoine, Gabrielle
name: Côté, José
name: Pepin, Jacinthe
name: Fontaine, Guillaume
name: Maheu-Cadotte, Marc-André
name: Hong, Quan Nha
name: Rouleau, Geneviève
name: Ziegler, Daniela
name: Jutras-Aswad, Didier
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: Science Policy

description: Additional file 1: Examples of educational methods delivered in implementations of ECHO-affiliated programs. Table 1. The ECHO Model educational theories, principles and methods with concrete examples of delivery.
Modelling segregation of flowing bidisperse granular mixtures varying simultaneously in size and density
Creators: name: Duan, Yifei
name: Umbanhowar, Paul B.
name: Ottino, Julio M.
name: Lueptow, Richard M.
Publisher: name: arXiv
Year: 2020
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: Flowing granular materials segregate due to differences in particle size (driven by percolation) and density (driven by buoyancy). Modelling the segregation of mixtures of large/heavy particles and small/light particles is challenging due to the opposing effects of the two segregation mechanisms. Using discrete element method (DEM) simulations of combined size and density segregation we show that the segregation velocity is well described by a model that depends linearly on the local shear rate and quadratically on the species concentration. Concentration profiles predicted by incorporating this segregation velocity model into a continuum advection-diffusion-segregation transport model match DEM simulation results well for a wide range of particle size and density ratios. Most surprisingly, the DEM simulations and the segregation velocity model both show that the segregation direction for a range of size and density ratios depends on the local species concentration. This leads to a methodology to determine the combination of particle size ratio, density ratio, and particle concentration for which a bidisperse mixture will not segregate.
Dolichogenidea interpolata
Creators: name: Fernandez-Triana, Jose
name: Sakagami, Kota
name: Shimizu, So
Publisher: name: Zenodo
Year: 2018
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Braconidae
Dolichogenidea
Dolichogenidea interpolata

description: D. interpolata (Papp, 1975): Flagellomeres 14 length 1.4–1.5 times its width; ovipositor sheath much longer (1.5–1.6 times) than metatibia.
description: Published as part of Fernandez-Triana, Jose, Sakagami, Kota & Shimizu, So, 2018, Dolichogenidea maetoi sp. nov. (Hymenoptera: Braconidae) from Japan, the first parasitoid wasp recorded from Hyblaea fortissima (Lepidoptera), pp. 167-175 in Acta Entomologica Musei Nationalis Pragae 58 (1) on page 172, DOI: 10.2478/aemnp-2018-0014, http://zenodo.org/record/3699178
Deformable Scintillation Dosimeter I: Challenges and Implementation using Computer Vision Techniques
Creators: name: Cloutier, Emily
name: Archambault, Louis
name: Beaulieu, Luc
Publisher: name: arXiv
Year: 2021
Subjects: subject: Medical Physics (physics.med-ph)
subject: FOS: Physical sciences

description: Plastic scintillation detectors are increasingly used to measure dose distributions in the context of radiotherapy treatments. Their water-equivalence, real-time response and high spatial resolution distinguish them from traditional detectors, especially in complex irradiation geometries. Their range of applications could be further extended by embedding scintillators in a deformable matrix mimicking anatomical changes. In this work, we characterized signal variations arising from the translation and rotation of scintillating fibers with respect to a camera. Corrections are proposed using stereo vision techniques and two sCMOS complementing a CCD camera. The study was extended to the case of a prototype real-time deformable dosimeter comprising an array of 19 scintillating. The signal to angle relationship follows a gaussian distribution (FWHM = 52°) whereas the intensity variation from radial displacement follows the inverse square law. Tracking the position and angle of the fibers enabled the correction of these spatial dependencies. The detecting system provides an accuracy and precision of respectively 0.008 cm and 0.03 cm on the position detection. This resulted in an uncertainty of 2° on the angle measurement. Displacing the dosimeter by $\pm$3 cm in depth resulted in relative intensities of 100$\pm$10% (mean $\pm$ standard deviation) to the reference position. Applying corrections reduced the variations thus resulting in relative intensities of 100$\pm$1%. Similarly, for lateral displacements of $\pm$3 cm, intensities went from 98$\pm$3% to 100$\pm$1% after the correction. Therefore, accurate correction of the signal collected by a camera imaging the output of scintillating elements in a 3D volume is possible. This work paves the way to the development of real-time scintillator-based deformable dosimeters.
Additional file 2 of Effectiveness and experiences of the Extension for Community Healthcare Outcomes (ECHO) Model in developing competencies among healthcare professionals: a mixed methods systematic review protocol
Creators: name: Chicoine, Gabrielle
name: Côté, José
name: Pepin, Jacinthe
name: Fontaine, Guillaume
name: Maheu-Cadotte, Marc-André
name: Hong, Quan Nha
name: Rouleau, Geneviève
name: Ziegler, Daniela
name: Jutras-Aswad, Didier
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: Science Policy

description: Additional file 2. Recommended items to address in a systematic review protocol from the Preferred Reporting Items for Systematic review and Meta-Analysis Protocols (PRISMA-P) 2015 checklist [47].
Planetary Companions around Three Intermediate-Mass G and K Giants: 18 Del, xi Aql, and HD 81688
Creators: name: Sato, Bun'ei
name: Izumiura, Hideyuki
name: Toyota, Eri
name: Kambe, Eiji
name: Ikoma, Masahiro
name: Omiya, Masashi
name: Masuda, Seiji
name: Takeda, Yoichi
name: Murata, Daisuke
name: Itoh, Yoichi
name: Ando, Hiroyasu
name: Yoshida, Michitoshi
name: Kokubo, Eiichiro
name: Ida, Shigeru
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report the detection of 3 new extrasolar planets from the precise Doppler survey of G and K giants at Okayama Astrophysical Observatory. The host stars, namely, 18 Del (G6 III), xi Aql (K0 III) and HD 81688 (K0 III-IV), are located at the clump region on the HR diagram with estimated masses of 2.1-2.3 M_solar. 18 Del b has a minimum mass of 10.3 M_Jup and resides in a nearly circular orbit with period of 993 days, which is the longest one ever discovered around evolved stars. xi Aql b and HD 81688 b have minimum masses of 2.8 and 2.7 M_Jup, and reside in nearly circular orbits with periods of 137 and 184 days, respectively, which are the shortest ones among planets around evolved stars. All of the substellar companions ever discovered around possible intermediate-mass (1.7-3.9 M_solar) clump giants have semimajor axes larger than 0.68 AU, suggesting the lack of short-period planets. Our numerical calculations suggest that Jupiter-mass planets within about 0.5 AU (even up to 1 AU depending on the metallicity and adopted models) around 2-3 M_solar stars could be engulfed by the central stars at the tip of RGB due to tidal torque from the central stars. Assuming that most of the clump giants are post-RGB stars, we can not distinguish whether the lack of short-period planets is primordial or due to engulfment by central stars. Deriving reliable mass and evolutionary status for evolved stars is highly required for further investigation of formation and evolution of planetary systems around intermediate-mass stars.
description: 28 pages, 9 figures, accepted for publication in PASJ
Dolichogenidea jaroshevskyi
Creators: name: Fernandez-Triana, Jose
name: Sakagami, Kota
name: Shimizu, So
Publisher: name: Zenodo
Year: 2018
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Braconidae
Dolichogenidea
Dolichogenidea jaroshevskyi

description: D. jaroshevskyi (Tobias, 1976): Flagellomeres 15 cubic; propodeum slightly sculptured in lower half [apparently without defined areola, but the descriptions consulted (PAPP 1981, TOBIAS 1986) are not clear about that].
description: Published as part of Fernandez-Triana, Jose, Sakagami, Kota & Shimizu, So, 2018, Dolichogenidea maetoi sp. nov. (Hymenoptera: Braconidae) from Japan, the first parasitoid wasp recorded from Hyblaea fortissima (Lepidoptera), pp. 167-175 in Acta Entomologica Musei Nationalis Pragae 58 (1) on page 173, DOI: 10.2478/aemnp-2018-0014, http://zenodo.org/record/3699178
Defect-driven antiferromagnetic domain walls in CuMnAs films
Creators: name: Reimers, Sonka
name: Kriegner, Dominik
name: Gomonay, Olena
name: Carbone, Dina
name: Krizek, Filip
name: Novak, Vit
name: Campion, Richard P.
name: Maccherozzi, Francesco
name: Bjorling, Alexander
name: Amin, Oliver J.
name: Barton, Luke X.
name: Poole, Stuart F.
name: Omari, Khalid A.
name: Michalicka, Jan
name: Man, Ondrej
name: Sinova, Jairo
name: Jungwirth, Tomas
name: Wadley, Peter
name: Dhesi, Sarnjeet S.
name: Edmonds, Kevin W.
Publisher: name: arXiv
Year: 2021
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: Efficient manipulation of antiferromagnetic (AF) domains and domain walls has opened up new avenues of research towards ultrafast, high-density spintronic devices. AF domain structures are known to be sensitive to magnetoelastic effects, but the microscopic interplay of crystalline defects, strain and magnetic ordering remains largely unknown. Here, we reveal, using photoemission electron microscopy combined with scanning X-ray diffraction imaging and micromagnetic simulations, that the AF domain structure in CuMnAs thin films is dominated by nanoscale structural twin defects. We demonstrate that microtwin defects, which develop across the entire thickness of the film and terminate on the surface as characteristic lines, determine the location and orientation of 180 degree and 90 degree domain walls. The results emphasize the crucial role of nanoscale crystalline defects in determining the AF domains and domain walls, and provide a route to optimizing device performance.
On the Evolution of Thermonuclear Flames on Large Scales
Creators: name: Zhang, Ju
name: Messer, O. E. Bronson
name: Khokhlov, Alexei M.
name: Plewa, Tomasz
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The thermonuclear explosion of a massive white dwarf in a Type Ia supernova explosion is characterized by vastly disparate spatial and temporal scales. The extreme dynamic range inherent to the problem prevents the use of direct numerical simulation and forces modelers to resort to subgrid models to describe physical processes taking place on unresolved scales. We consider the evolution of a model thermonuclear flame in a constant gravitational field on a periodic domain. The gravitational acceleration is aligned with the overall direction of the flame propagation, making the flame surface subject to the Rayleigh-Taylor instability. The flame evolution is followed through an extended initial transient phase well into the steady-state regime. The properties of the evolution of flame surface are examined. We confirm the form of the governing equation of the evolution suggested by Khokhlov (1995). The mechanism of vorticity production and the interaction between vortices and the flame surface are discussed. The results of our investigation provide the bases for revising and extending previous subgrid-scale model.
description: 15 pages, 22 postscript figures. Accepted for publication by the Astrophysical Journal. High resolution figures can be found at http://flash.uchicago.edu/~zhang/research_paper.html
Berry Phase in the Gravitational Quantum Well and the Seiberg-Witten map
Creators: name: Bastos, C.
name: Bertolami, O.
Publisher: name: arXiv
Year: 2006
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We explicitly compute the geometrical Berry phase for the noncommutative gravitational quantum well for different SW maps. We find that they lead to different partial contributions to the Berry phase. For the most general map we obtain that $Δγ(S)\simη^3$, in a segment S of the path in the configuration space where $\sqrtη$ is the fundamental momentum scale for the noncommutative gravitational quantum well. For the full closed path, we find, through an explicit computation, that $γ(C)=0$. This result is consistent with the fact that physical properties are independent of the SW map and shows that these maps do not introduce degeneracies or level crossing in the noncommutative extensions of the gravitational quantum well.
description: 10 pages. Extended discussion and change in title
Small group elicitation session on tense-aspect and gerunds
Creators: name: Massoma, Achille
name: Sandy, Clare S.
Publisher: name: California Language Archive, University of California, Berkeley
Year: 2022
Subjects: subject: abb

description: Modals with Greg - might, almost, already; "he already/almost fell" - can use 'bak' in place of 'baa' in biclausal but not in monoclausal construction; tense/aspect - "He was falling", "He was dying"; tense/aspect - "We have fallen", "We were falling", "We had fallen", etc; tense/aspect - "He almost fell", "He almost died", "He almost laughed", "He had already laughed"; "I almost came to your house", "I almost ate the apple", "I almost build a house"; "I haven't finished (present perfect?)", "I didn't finish", "I hadn't finished", "I wasn't finishing"; tense/aspect - "I haven't finished" (work) (today); tense/aspect - "I haven't finished counting crabs, counting the teachers"; copulas and auxiliaries with Rachele, vowel harmony with 'be la'; "I could have gone", "I was able to go" (today) (and I did); "I should go", "I have to go", "I have to have to go"; applicative of 'sell'; gerund and nominal forms of 'call', 'sell'; gerund and nominal forms of 'have', 'catch', 'buy'; 'his arrest' vs. 'the arresting of him'.
Additional file 3 of Effectiveness and experiences of the Extension for Community Healthcare Outcomes (ECHO) Model in developing competencies among healthcare professionals: a mixed methods systematic review protocol
Creators: name: Chicoine, Gabrielle
name: Côté, José
name: Pepin, Jacinthe
name: Fontaine, Guillaume
name: Maheu-Cadotte, Marc-André
name: Hong, Quan Nha
name: Rouleau, Geneviève
name: Ziegler, Daniela
name: Jutras-Aswad, Didier
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: Science Policy

description: Additional file 3. Complete search strategy for the electronic databases.
Numerical solution of perturbed Kepler problem using a split operator technique
Creators: name: Balaraman, G. S.
name: Vrinceanu, D.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Computational Physics (physics.comp-ph)
subject: Atomic Physics (physics.atom-ph)
subject: FOS: Physical sciences

description: An efficient geometric integrator is proposed for solving the perturbed Kepler motion. This method is stable and accurate over long integration time, which makes it appropriate for treating problems in astrophysics, like solar system simulations, and atomic and molecular physics, like classical simulations of highly excited atoms in external fields. The key idea is to decompose the hamiltonian in solvable parts and propagate the system according to each term. Two case studies, the Kepler atom in an uniform field and in a monochromatic field, are presented and the errors are analyzed.
description: 17 pages, 5 figures, submitted to the Journal of Computational Physics
Arc-minute-scale studies of the interstellar gas towards HESS$\,$J1804$-$216: Still an unidentified TeV $γ$-ray source
Creators: name: Feijen, K.
name: Rowell, G.
name: Einecke, S.
name: Braiding, C.
name: Burton, M. G.
name: Maxted, N.
name: Voisin, F.
name: Wong, G. F.
Publisher: name: arXiv
Year: 2020
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: The Galactic TeV $γ$-ray source HESS$\,$J1804$-$216 is currently an unidentified source. In an attempt to unveil its origin, we present here the most detailed study of interstellar gas using data from the Mopra Southern Galactic Plane CO Survey, 7 and 12$\,$mm wavelength Mopra surveys and Southern Galactic Plane Survey of HI. Several components of atomic and molecular gas are found to overlap HESS$\,$J1804$-$216 at various velocities along the line of sight. The CS(1-0) emission clumps confirm the presence of dense gas. Both correlation and anti-correlation between the gas and TeV $γ$-ray emission have been identified in various gas tracers, enabling several origin scenarios for the TeV $γ$-ray emission from HESS$\,$J1804$-$216. For a hadronic scenario, SNR$\,$G8.7$-$0.1 and the progenitor SNR of PSR$\,$J1803$-$2137 require cosmic ray (CR) enhancement factors of $\mathord{\sim} 50$ times the solar neighbour CR flux value to produce the TeV $γ$-ray emission. Assuming an isotropic diffusion model, CRs from both these SNRs require a slow diffusion coefficient, as found for other TeV SNRs associated with adjacent ISM gas. The morphology of gas located at 3.8$\,$kpc (the dispersion measure distance to PSR$\,$J1803$-$2137) tends to anti-correlate with features of the TeV emission from HESS$\,$J1804$-$216, making the leptonic scenario possible. Both pure hadronic and pure leptonic scenarios thus remain plausible.
description: 29 pages, 23 figures, 5 tables, accepted for publication in PASA
Dolichogenidea jilinensis Chen & Song 2004
Creators: name: Fernandez-Triana, Jose
name: Sakagami, Kota
name: Shimizu, So
Publisher: name: Zenodo
Year: 2018
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Braconidae
Dolichogenidea
Dolichogenidea jilinensis

description: D. jilinensis Chen & Song, 2004: Pterostigma brown; propodeum mostly smooth, with only a small trace of posterior areola carinae near nucha.
description: Published as part of Fernandez-Triana, Jose, Sakagami, Kota & Shimizu, So, 2018, Dolichogenidea maetoi sp. nov. (Hymenoptera: Braconidae) from Japan, the first parasitoid wasp recorded from Hyblaea fortissima (Lepidoptera), pp. 167-175 in Acta Entomologica Musei Nationalis Pragae 58 (1) on page 173, DOI: 10.2478/aemnp-2018-0014, http://zenodo.org/record/3699178
Additional file 4 of Effectiveness and experiences of the Extension for Community Healthcare Outcomes (ECHO) Model in developing competencies among healthcare professionals: a mixed methods systematic review protocol
Creators: name: Chicoine, Gabrielle
name: Côté, José
name: Pepin, Jacinthe
name: Fontaine, Guillaume
name: Maheu-Cadotte, Marc-André
name: Hong, Quan Nha
name: Rouleau, Geneviève
name: Ziegler, Daniela
name: Jutras-Aswad, Didier
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: Science Policy

description: Additional file 4: Example of a matrix for integrating the QUAN and QUAL findings of the review, inspired from Candy et al. (2011) [74]. Table 3. Tabulation of critical factors (1 - …) drawn from the QUAL findings (themes), categorized according to nature of factors [34], with each ECHO program components/characteristics and effect size (E) on healthcare professionals’ competency development.
The Size of the Cooling Region of Hot Gas in Two Elliptical Galaxies
Creators: name: Bregman, Joel N.
name: Otte, Birgit
name: Miller, Eric D.
name: Irwin, Jimmy A.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Some early-type galaxies show OVI emission, a tracer of gas at 10^5.5 K, and a predicted product of gas cooling from the X-ray emitting temperatures. We studied the spatial extent and velocity structure of this cooling gas by obtaining spectra of the OVI doublet in NGC 4636 and NGC 5846 with the Far Ultraviolet Spectroscopic Explorer. For NGC 4636, the central LWRS pointing shows that the OVI lines are double-peaked and symmetrical about the systemic velocity of the galaxy, with a separation of 210 km/s. A LWRS observation 30" from the center failed to show additional OVI emission. For NGC 5846, three spectra were obtained with 4" x 20" apertures (MDRS) at the center and 4" to the east and west of the center. The OVI line flux seen in the previous LWRS is contained in the sum of the smaller apertures, with most of the flux in a single non-central MDRS aperture, suggesting a size for the emission < 0.5 kpc; the emission consists of a blue and red peak. For both galaxies, the OVI velocity structure is similar to that of the optical [NII] emission and is consistent with rotation. The compactness and velocity structure of the OVI emission rules out cooling flow models with broadly distributed mass drop-out but is consistent with cooling flow models where the cooling occurs primarily in the central region. The 1E4 K gas may be the end state of the OVI gas.
description: 17 pages, 5 figures