cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Spin diffusion length of Permalloy using spin absorption in lateral spin valves
Creators: name: Sagasta, Edurne
name: Omori, Yasutomo
name: Isasa, Miren
name: Otani, YoshiChika
name: Hueso, Luis E.
name: Casanova, Fèlix
Publisher: name: arXiv
Year: 2019
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We employ the spin absorption technique in lateral spin valves to extract the spin diffusion length of Permalloy (Py) as a function of temperature and resistivity. A linear dependence of the spin diffusion length with conductivity of Py is observed, evidencing that Elliott-Yafet is the dominant spin relaxation mechanism in Permalloy. Completing the data set with additional data found in literature, we obtain $λ_{Py}= (0.91\pm 0.04) (fΩm^2)/ρ_{Py}$.
description: 8 pages, 4 figures, 2 tables
Hydrodynamics and Nucleosynthesis of Jet-Driven Supernovae II: Comparisons with Abundances of Extremely Metal-Poor Galaxies and Constraints on Supernova Progenitors
Creators: name: Leung, Shing-Chi
name: Nomoto, Ken'ichi
Publisher: name: arXiv
Year: 2023
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: The spectra of several galaxies, including extremely metal-poor galaxies (EMPGs) from the EMPRESS survey, have shown that the abundances of some Si-group elements differ from "spherical" explosion models of massive stars. This leads to the speculation that these galaxies have experienced supernova explosions with high asphericity, where mixing and fallback of the inner ejecta with the outer material leads to the distinctive chemical compositions. In this article, we consider the jet-driven supernova models by direct two-dimensional hydrodynamics simulations using progenitors about 20 -- 25 $M_{\odot}$ at zero metallicity. We investigate how the abundance patterns depend on the progenitor mass, mass cut and the asphericity of the explosion. We compare the observable with available supernova and galaxy catalogs based on $^{56}$Ni, ejecta mass, and individual element ratios. The proximity of our results with the observational data signifies the importance of aspherical supernova explosions in chemical evolution of these galaxies. Our models will provide the theoretical counterpart for understanding the chemical abundances of high-z galaxies measured by the James Webb Space Telescope.
description: 29 pages, 40 figures. Submitted to the Astrophysical Journal on Dec 21 2023, accepted on Aug 8 2024, published on Oct 18 2024
Rhynchista Rondani 1861
Creators: name: O'Hara, James E.
name: Cerretti, Pierfilippo
name: Pape, Thomas
name: Evenhuis, Neal L.
Publisher: name: Zenodo
Year: 2011
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Tachinidae
Rhynchista

description: 488. Rhynchista Rondani, 1861e: 9.
 TYPE SPECIES: Proboscina longipes Rondani, 1856, automatic [by designation of the same species (by original designation) for Proboscina Rondani, 1856].
 CURRENT STATUS: Unnecessary new replacement name for Proboscina Rondani, 1856; junior synonym of Eriothrix Meigen, 1803 [teste Herting & Dely-Draskovits (1993: 371)].
FAMILY: TACHINIDAE.
description: Published as part of O'Hara, James E., Cerretti, Pierfilippo, Pape, Thomas & Evenhuis, Neal L., 2011, 3141, pp. 1-268 in Zootaxa 3141 on page 159
Ditrichum pusillum Hampe 1867
Creators: name: Ros, Rosa M.
name: Olaf, Susana Rams
name: Eloy, Olaf Werner
name: Cerón, Eloy
Publisher: name: Zenodo
Year: 2024
Subjects: Biodiversity
Taxonomy
Plantae
Bryophyta
Bryopsida
Dicranales
Ditrichaceae
Ditrichum
Ditrichum pusillum

description: Ditrichum pusillum (Hedw.) Hampe
RECORDS. — Bescherelle (1882), Jelenc (1955a): La Calle. Very rare.
description: Published as part of Ros, Rosa M., Olaf, Susana Rams, Eloy, Olaf Werner & Cerón, Eloy, 2024, Revisiting the Bryophyte Checklist of Algeria: Exploring Diversity and Distribution, pp. 49-116 in Cryptogamie, Bryologie 20 (5) on page 73, DOI: 10.5252/cryptogamie-bryologie2024v45a5, http://zenodo.org/record/14593891
Removal of methylene blue from aqueous solutions using polyaniline/graphene oxide or polyaniline/reduced graphene oxide composites
Creators: name: E. A. El-Sharkaway
name: Kamel, Rasha M.
name: El-Sherbiny, Ibrahim M.
name: Gharib, Sally S.
Publisher: name: Taylor & Francis
Year: 2019
Subjects: subject: Medicine
subject: Molecular Biology
subject: Physiology
subject: FOS: Biological sciences
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: Sociology
subject: FOS: Sociology
subject: Marine Biology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: The polymeric nanocomposites polyaniline/graphene oxide (PANI/GO) and polyaniline/reduced graphene oxide (PANI/RGO) were synthesized for effective dye removal through the adsorption process. Synthesized composites were characterized by XRD, SEM, TEM and FTIR analyses. The sorption of methylene blue dye (MB) on the PANI/GO or (PANI/RGO) composites were studied as a function of contact time, concentration, temperature, adsorbent dosage and pH, and the results showed that MB sorption was dependent on pH value. The optimum concentration of the dye and the contact time for sorption of MB on PANI/GO or PANI/RGO was determined to be 270 min and 50 mg/L, respectively while the adsorbent dosage of PANI/GO and PANI/RGO were determined to be 0.4 and 0.3 g, respectively. At optimum conditions, the nature of the adsorption process have been investigated by kinetic and isotherm models. The results showed that the adsorption process followed the pseudo first-order kinetics this noticed from the higher value of correlation coefficient (R2 = 0.991) and was best suited to the Langmuir model. The maximum dye adsorption capacity of PANI/GO and PANI/RGO were estimated to be 14.2 and 19.2 mg g−1 respectively. From the results, it can be assured that the PANI/RGO is more effectively than PANI/GO for the removal of dye pollutants in water.
Minimum measurement time: lower bound on the frequency cutoff for collapse models
Creators: name: Adler, Stephen L.
name: Bassi, Angelo
name: Ferialdi, Luca
Publisher: name: arXiv
Year: 2019
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: The CSL model predicts a progressive breakdown of the quantum superposition principle, with a noise randomly driving the state of the system towards a localized one, thus accounting for the emergence of a classical world within a quantum framework. In the original model the noise is supposed to be white, but since white noises do not exist in nature, it becomes relevant to identify some of its spectral properties. Experimental data set an upper bound on its frequencies, while in this paper we bound it from below. We do so in two ways: by considering a 'minimal' measurement setup, requiring that the collapse is completed within the measurement time; and in a measurement modeling-independent way, by requiring that the fluctuations average to zero before the measurement time.
Search for Supersymmetric Dark Matter with Superfluid He3 (MACHe3)
Creators: name: Mayet, F.
name: Santos, D.
name: Bunkov, Yu. M.
name: Collin, E.
name: Godfrin, H.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: MACHe3 (MAtrix of Cells of superfluid He3) is a project of a new detector for direct Dark Matter search, using superfluid He3 as a sensitive medium. This paper presents a phenomenological study done with the DarkSUSY code, in order to investigate the discovery potential of this project of detector, as well as its complementarity with existing and planned devices.
description: 15 pages, 5 figures, submitted to Phys. Letters B, minor changes in the text
An alternative theoretical approach to describe planetary systems through a Schrodinger-type diffusion equation
Creators: name: Neto, M. de Oliveira
name: Maia, L. A.
name: Carneiro, S.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: In the present work we show that planetary mean distances can be calculated with the help of a Schrodinger-type diffusion equation. The obtained results are shown to agree with the observed orbits of all the planets and of the asteroid belt in the solar system, with only three empty states. Furthermore, the equation solutions predict a fundamental orbit at 0.05 AU from solar-type stars, a result confirmed by recent discoveries. In contrast to other similar approaches previously presented in the literature, we take into account the flatness of the solar system, by considering the flat solutions of the Schrodinger-type equation. The model has just one input parameter, given by the mean distance of Mercury.
description: 6 pages. Version accepted for publication in Chaos, Solitons & Fractals
Spectrum of the SU(3) Dirac operator on the lattice: Transition from random matrix theory to chiral perturbation theory
Creators: name: Göckeler, M.
name: Hehl, H.
name: Rakow, P. E. L.
name: Schäfer, A.
name: Wettig, T.
Publisher: name: arXiv
Year: 2001
Subjects: subject: High Energy Physics - Lattice (hep-lat)
subject: FOS: Physical sciences

description: We calculate complete spectra of the Kogut-Susskind Dirac operator on the lattice in quenched SU(3) gauge theory for various values of coupling constant and lattice size. From these spectra we compute the connected and disconnected scalar susceptibilities and find agreement with chiral random matrix theory up to a certain energy scale, the Thouless energy. The dependence of this scale on the lattice volume is analyzed. In the case of the connected susceptibility this dependence is anomalous, and we explain the reason for this. We present a model of chiral perturbation theory that is capable of describing the data beyond the Thouless energy and that has a common range of applicability with chiral random matrix theory.
description: 8 pages, RevTeX, 15 .eps figures
Ditrichum subulatum Hampe 1867
Creators: name: Ros, Rosa M.
name: Olaf, Susana Rams
name: Eloy, Olaf Werner
name: Cerón, Eloy
Publisher: name: Zenodo
Year: 2024
Subjects: Biodiversity
Taxonomy
Plantae
Bryophyta
Bryopsida
Dicranales
Ditrichaceae
Ditrichum
Ditrichum subulatum

description: Ditrichum subulatum Hampe
RECORDS. — Bescherelle (1882): Kabylie. Bescherelle (1882), Jelenc (1955a): La Calle; Philippeville. Corbière (1889), Jelenc (1955a): Blida, aux Chênes-Lièges, bord d‘un ruisselet, 600 m. Jelenc (1954b, 1955a, 1967): Massif de l‘Akfadou, sources sous les Zéens. Jelenc (1955a): Bône; Édough; Kabylie du Djurdjura, Aït Daoud; La Réghaia. Rare.
description: Published as part of Ros, Rosa M., Olaf, Susana Rams, Eloy, Olaf Werner & Cerón, Eloy, 2024, Revisiting the Bryophyte Checklist of Algeria: Exploring Diversity and Distribution, pp. 49-116 in Cryptogamie, Bryologie 20 (5) on page 73, DOI: 10.5252/cryptogamie-bryologie2024v45a5, http://zenodo.org/record/14593891
The Role of Magnetic Field Geometry in the Evolution of Neutron Star Merger Accretion Discs
Creators: name: Christie, I. M.
name: Lalakos, A.
name: Tchekhovskoy, A.
name: Fernández, R.
name: Foucart, F.
name: Quataert, E.
name: Kasen, D.
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Neutron star mergers are unique laboratories of accretion, ejection, and r-process nucleosynthesis. We used 3D general relativistic magnetohydrodynamic simulations to study the role of the post-merger magnetic geometry in the evolution of merger remnant discs around stationary Kerr black holes. Our simulations fully capture mass accretion, ejection, and jet production, owing to their exceptionally long duration exceeding $4$ s. Poloidal post-merger magnetic field configurations produce jets with energies $E_\mathrm{jet} \sim (4{-}30)\times10^{50}$ erg, isotropic equivalent energies $E_\mathrm{iso}\sim(4{-}20)\times10^{52}$ erg, opening angles $θ_\mathrm{jet}\sim6{-}13^\circ$, and durations $t_j\lesssim1$ s. Accompanying the production of jets is the ejection of $f_\mathrm{ej}\sim30{-}40\%$ of the post-merger disc mass, continuing out to times $> 1$ s. We discover that a more natural, purely toroidal post-merger magnetic field geometry generates large-scale poloidal magnetic flux of alternating polarity and striped jets. The first stripe, of $E_\mathrm{jet}\simeq2\times10^{48}\,\mathrm{erg}$, $E_\mathrm{iso}\sim10^{51}$ erg, $θ_\mathrm{jet}\sim3.5{-}5^\circ$, and $t_j\sim0.1$ s, is followed by $\gtrsim4$ s of striped jet activity with $f_\mathrm{ej}\simeq27\%$. The dissipation of such stripes could power the short gamma-ray burst (sGRB) prompt emission. Our simulated jet energies and durations span the range of sGRBs. We find that although the blue kilonova component is initially hidden from view by the red component, it expands faster, outruns the red component, and becomes visible to off-axis observers. In comparison to GW 170817/GRB 170817A, our simulations under-predict the mass of the blue relative to red component by a factor of few. Including the dynamical ejecta and neutrino absorption may reduce this tension.
description: 14 pages, 12 figures
The longicorn beetles (Coleoptera, Cerambycidae) of the Bureinskii State Nature Reserve, Khabarovskii Krai, Russia
Creators: name: N.S. Anisimov
name: Bezborodov, Vitaly
name: Koshkin, Evgeny
Publisher: name: figshare
Year: 2019
Subjects: subject: Zoology
subject: FOS: Biological sciences

description: In the Bureinskii State Nature Reserve and in adjacent territories 45 species of the Cerambycidae family from 31 genera of 14 tribes of 5 subfamilies were registered. 22 species are listed for the first time for the fauna of the study area: Rhagium inquisitor (Linnaeus, 1758), Rh. heyrovskyi Podany, 1964, Pachyta lamed (Linnaeus, 1758), Evodinellus borealis (Gyllenhal, 1827), Brachyta variabilis (Gebler, 1817), B. sachalinensis Matsumura, 1911, Nivellia extensa (Gebler, 1833), Anastrangalia renardi (Gebler, 1848), Leptura duodecimguttata Fabricius, 1801, Tetropium gracilicorne Reitter, 1889, Trichoferus campestris (Faldermann, 1835), Semanotus undatus (Linnaeus, 1758), Callidium chlorizans (Solsky, 1871), C. violaceum (Linnaeus, 1758), Xylotrechus altaicus (Gebler, 1836), Clytus arietoides Reitter, 1899, Mesosa myops (Dalman, 1817), Monochamus impluviatus Motschulsky, 1859, Lamia textor (Linnaeus, 1758), Pogonocherus fasciculatus (DeGeer, 1775), Acanthocinus carinulatus (Gebler, 1833), Saperda interrupta Gebler, 1825; 13 genera: Rhagium Fabricius, 1775, Pachyta Dejean, 1821, Evodinellus Plavilstshikov, 1915, Tetropium Kirby, 1837, Trichoferus Wollaston, 1854, Semanotus Mulsant, 1839, Callidium Fabricius, 1775, Xylotrechus Chevrolat, 1860, Clytus  Laicharting, 1784, Mesosa Latreille, 1829, Lamia Fabricius, 1775, Pogonocherus Mulsant, 1821, Acanthocinus Dejean, 1821; 7 tribes: Tetropiini Seidlitz, 1891, Hesperophanini Mulsant, 1839, Callidiini Kirby, 1837, Mesosini Mulsant, 1839, Lamiini Latreille, 1825, Pogonocherini Mulsant, 1839, Acanthocinini Blanchard, 1845. The most diverse are Lepturinae (24 species), followed by Lamiinae (10), Cerambycinae (7), Spondylidinae (3) and Necydalinae (1). The species with a Transpalearctic range are predominant – 25 (55,6%). The eastern Palearctic type of range includes 11 species (24,4%), to the East Asian species – 5 species (11,1%), to the Holarctic type – 4 species (8,9%). Most of the beetles of the reserve are trophically associated with the dominant here coniferous woody vegetation – 24 species (53,3%). Are able to populate both coniferous and deciduous woody plants – 9 species (20%). Only deciduous trees and shrubs inhabit 8 species (17,8%), of which Trichoferus campestris (Faldermann, 1835) is able to develop also on grassy (аstragalus). One species (2,2%) is associated exclusively with herbaceous plants – Brachyta interrogationis (Linnaeus, 1758).
The Initial Mass Function of Stars: Evidence for Uniformity in Variable Systems
Creators: name: Kroupa, Pavel
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The distribution of stellar masses that form in one star-formation event in a given volume of space is called the initial mass function (IMF). The IMF has been estimated from low-mass brown dwarfs to very massive stars. Combining IMF estimates for different populations in which the stars can be observed individually unveils an extraordinary uniformity of the IMF. This general insight appears to hold for populations including present-day star formation in small molecular clouds, rich and dense massive star-clusters forming in giant clouds, through to ancient and metal-poor exotic stellar populations that may be dominated by dark matter. This apparent universality of the IMF is a challenge for star formation theory because elementary considerations suggest that the IMF ought to systematically vary with star-forming conditions.
description: 32 pages, all 6 figures are in colour, published in Science
Saprobius Rondani 1880
Creators: name: O'Hara, James E.
name: Cerretti, Pierfilippo
name: Pape, Thomas
name: Evenhuis, Neal L.
Publisher: name: Zenodo
Year: 2011
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Sphaeroceridae
Saprobius

description: 493. Saprobius Rondani, 1880a: 11.
 ORIGINALLY INCLUDED SPECIES: Borborus nigriceps Rondani, 1880; Borborus nitidus Meigen, 1830 (with Borborus hamatus Haliday, 1833 var. in synonymy); Borborus nervosus Meigen, 1835.
 TYPE SPECIES: Borborus nitidus Meigen, 1830, by subsequent designation (Norrbom & Kim, 1985: 185).
 CURRENT STATUS: Junior synonym of Crumomyia Macquart, 1835 [teste Rohaček (2001: 58)].
FAMILY: SPHAEROCERIDAE.
 [Sarchophaga]  Rondani in Osculati , 1850: 240.
 CURRENT STATUS: Incorrect subsequent spelling of Sarcophaga Meigen, 1826.
FAMILY: SARCOPHAGIDAE.
REMARKS: Criteria for making this name available as an emendation were not found to be fulfilled in this work.
 494. Sarcopaga Rondani, 1856: 85.
 CURRENT STATUS: Unjustified emendation of Sarcophaga Meigen, 1826; junior synonym of Sarcophaga Meigen, 1826. New synonymy.
FAMILY: SARCOPHAGIDAE.
REMARKS: Name made available as an emendation by virtue of similar spelling changes in two or more names from “ph” to “p” in the same work.
description: Published as part of O'Hara, James E., Cerretti, Pierfilippo, Pape, Thomas & Evenhuis, Neal L., 2011, 3141, pp. 1-268 in Zootaxa 3141 on pages 160-161
Additional file 3 of Notch1 activation of Jagged1 contributes to differentiation of mesenchymal stem cells into endothelial cells under cigarette smoke extract exposure
Creators: name: Cheng, Yi
name: Gu, Wen
name: Zhang, Guorui
name: Guo, Xuejun
Publisher: name: figshare
Year: 2022
Subjects: subject: Biochemistry
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Pharmacology
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer
subject: Hematology

description: Additional file 3. The original western blot images of β-actin.
title: A place for (almost) every thing and everything in its place: phonotactic effects on phonological development in Italian
Creators: name: Cucinelli, Alex
Publisher: name: Memorial University of Newfoundland
Year: 2020

description: In learning their first language(s), children must acquire a phonemic inventory, a syllable shape (e.g., CV, CVC, CCV), and an understanding of which phonemes can occupy which positions within the syllable or word. In hierarchical representations, this can be accounted for through constraints on dependency relationships, where the specification of segmental features in dependent positions captures marked options. This thesis examines the phonological development of four Italian-learning children, whose overall behaviour aligns with implicational relationships proposed in the literature. I account for their behaviour through hierarchically organized prosodic and segmental representations which reflect claims based on the notion of markedness. These representations incorporate the prediction that early stages of acquisition and typologically ubiquitous syllable shapes represent unmarked options, while syllable shapes learned relatively late and those only allowed in typologically rare languages constitute more marked options. By investigating prosodic development alongside segmental development in Italian, this thesis contributes novel observations concerning the markedness of prosodic dependency in reference to sonority and place or articulation, for example: liquid+consonant, strident+consonant coda-onset clusters and consonant+liquid onset clusters all imply homorganic nasal+consonant coda-onset clusters, which also means that complex onsets imply coda-onset clusters, both in child grammars and in the typology of adult grammars.
Additional file 1: of Person-centred, integrated and pro-active care for multi-morbid elderly with advanced care needs: a propensity score-matched controlled trial
Creators: name: G. Berntsen
name: M. Dalbakk
name: J. Hurley
name: T. Bergmo
name: B. Solbakken
name: L. Spansvoll
name: J. Bellika
name: S. SkrĂ¸Vseth
name: T. Brattland
name: M. Rumpsfeld
Publisher: name: figshare
Year: 2019
Subjects: subject: Biochemistry
subject: Medicine
subject: Cell Biology
subject: Developmental Biology
subject: Cancer
subject: Science Policy
subject: 111714 Mental Health
subject: FOS: Health sciences
subject: Computational Biology

description: The PACT care model. A stronger and more detailed qualitative description of the PACT intervention. (DOCX 210 kb)
Quenching as a Contest between Galaxy Halos and their Central Black Holes
Creators: name: Chen, Zhu
name: Faber, S. M.
name: Koo, David. C.
name: Somerville, Rachel S.
name: Primack, Joel R.
name: Dekel, Avishai
name: Rodríguez-Puebla, Aldo
name: Guo, Yicheng
name: Barro, Guillermo
name: Kocevski, Dale D.
name: van der Wel, A.
name: Woo, Joanna
name: Bell, Eric F.
name: Fang, Jerome J.
name: Ferguson, Henry C.
name: Giavalisco, Mauro
name: Huertas-Company, Marc
name: Jiang, Fangzhou
name: Kassin, Susan
name: Lin, Lin
name: Liu, Fengshan
name: Luo, Yifei
name: Luo, Zhijian
name: Pacifici, Camilla
name: Pandya, Viraj
name: Salim, Samir
name: Shu, Chenggang
name: Tacchella, Sandro
name: Terrazas, Bryan A.
name: Yesuf, Hassen M.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Existing models of galaxy formation have not yet explained striking correlations between structure and star-formation activity in galaxies, notably the sloped and moving boundaries that divide star-forming from quenched galaxies in key structural diagrams. This paper uses these and other relations to ``reverse-engineer'' the quenching process for central galaxies. The basic idea is that star-forming galaxies with larger radii (at a given stellar mass) have lower black-hole masses due to lower central densities. Galaxies cross into the green valley when the cumulative effective energy radiated by their black hole equals $\sim4\times$ their halo-gas binding energy. Since larger-radii galaxies have smaller black holes, one finds they must evolve to higher stellar masses in order to meet this halo-energy criterion, which explains the sloping boundaries. A possible cause of radii differences among star-forming galaxies is halo concentration. The evolutionary tracks of star-forming galaxies are nearly parallel to the green-valley boundaries, and it is mainly the sideways motions of these boundaries with cosmic time that cause galaxies to quench. BH-scaling laws for star-forming, quenched, and green-valley galaxies are different, and most BH mass growth takes place in the green valley. Implications include: the radii of star-forming galaxies are an important second parameter in shaping their black holes; black holes are connected to their halos but in different ways for star-forming, quenched, and green-valley galaxies; and the same BH-halo quenching mechanism has been in place since $z \sim 3$. We conclude with a discussion of black hole-galaxy co-evolution, the origin and interpretation of BH scaling laws.
description: 45 pages, 20 figures, 2 tables, accepted for publication in ApJ
Path-based Explanation for Knowledge Graph Completion
Creators: name: Chang, Heng
name: Ye, Jiangnan
name: Avila, Alejo Lopez
name: Du, Jinhua
name: Li, Jia
Publisher: name: arXiv
Year: 2024
Subjects: subject: Machine Learning (cs.LG)
subject: Artificial Intelligence (cs.AI)
subject: Social and Information Networks (cs.SI)
subject: FOS: Computer and information sciences

description: Graph Neural Networks (GNNs) have achieved great success in Knowledge Graph Completion (KGC) by modelling how entities and relations interact in recent years. However, the explanation of the predicted facts has not caught the necessary attention. Proper explanations for the results of GNN-based KGC models increase model transparency and help researchers develop more reliable models. Existing practices for explaining KGC tasks rely on instance/subgraph-based approaches, while in some scenarios, paths can provide more user-friendly and interpretable explanations. Nonetheless, the methods for generating path-based explanations for KGs have not been well-explored. To address this gap, we propose Power-Link, the first path-based KGC explainer that explores GNN-based models. We design a novel simplified graph-powering technique, which enables the generation of path-based explanations with a fully parallelisable and memory-efficient training scheme. We further introduce three new metrics for quantitative evaluation of the explanations, together with a qualitative human evaluation. Extensive experiments demonstrate that Power-Link outperforms the SOTA baselines in interpretability, efficiency, and scalability.
description: Accepted by KDD 2024
Three-dimensional theory for interaction between atomic ensembles and free-space light
Creators: name: Duan, L. -M.
name: Cirac, J. I.
name: Zoller, P.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Atomic ensembles have shown to be a promising candidate for implementations of quantum information processing by many recently-discovered schemes. All these schemes are based on the interaction between optical beams and atomic ensembles. For description of these interactions, one assumed either a cavity-QED model or a one-dimensional light propagation model, which is still inadequate for a full prediction and understanding of most of the current experimental efforts which are actually taken in the three-dimensional free space. Here, we propose a perturbative theory to describe the three-dimensional effects in interaction between atomic ensembles and free-space light with a level configuration important for several applications. The calculations reveal some significant effects which are not known before from the other approaches, such as the inherent mode-mismatching noise and the optimal mode-matching conditions. The three-dimensional theory confirms the collective enhancement of the signal-to-noise ratio which is believed to be one of the main advantage of the ensemble-based quantum information processing schemes, however, it also shows that this enhancement need to be understood in a more subtle way with an appropriate mode matching method.
description: 16 pages, 9 figures
Thermodynamics of SU(3) gauge theory on anisotropic lattices
Creators: name: PACS Collaboration
name: Namekawa, Y.
name: Aoki, S.
name: Burkhalter, R.
name: Ejiri, S.
name: Fukugita, M.
name: Hashimoto, S.
name: Ishizuka, N.
name: Iwasaki, Y.
name: Kanaya, K.
name: Kaneko, T.
name: Kuramashi, Y.
name: Lesk, V.
name: Okamoto, M.
name: Okawa, M.
name: Taniguchi, Y.
name: Ukawa, A.
name: Yoshié, T.
Publisher: name: arXiv
Year: 2001
Subjects: subject: High Energy Physics - Lattice (hep-lat)
subject: FOS: Physical sciences

description: Finite temperature SU(3) gauge theory is studied on anisotropic lattices using the standard plaquette gauge action. The equation of state is calculated on $16^{3} \times 8$, $20^{3} \times 10$ and $24^{3} \times 12$ lattices with the anisotropy $ξ\equiv a_s / a_t = 2$, where $a_s$ and $a_t$ are the spatial and temporal lattice spacings. Unlike the case of the isotropic lattice on which $N_t=4$ data deviate significantly from the leading scaling behavior, the pressure and energy density on an anisotropic lattice are found to satisfy well the leading $1/N_t^2$ scaling from our coarsest lattice, $N_t/ξ=4$. With three data points at $N_t/ξ=4$, 5 and 6, we perform a well controlled continuum extrapolation of the equation of state. Our results in the continuum limit agree with a previous result from isotropic lattices using the same action, but have smaller and more reliable errors.
description: RevTeX, 21 pages, 17 PS figures. A quantitative test about the benefit of anisotropic lattices added, minor errors corrected. Final version for PRD
Additional file 1: of Sarcopenia as a predictor of hospitalization among older people: a systematic review and meta-analysis
Creators: name: Zhang, Xiaoming
name: Zhang, Wenwu
name: Wang, Conghua
name: Tao, Wuyuan
name: Dou, Qingli
name: Yang, Yunzhi
Publisher: name: figshare
Year: 2018
Subjects: Medicine
Biological Sciences not elsewhere classified
Information Systems not elsewhere classified
Developmental Biology
Cancer
Science Policy

description: Search strategy of PubMed research report. (DOCX 13 kb)
Third-order relativistic hydrodynamics: dispersion relations and transport coefficients of a dual plasma
Creators: name: Diles, Saulo M.
name: Mamani, Luis A. H.
name: Miranda, Alex S.
name: Zanchin, Vilson T.
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Hydrodynamics is nowadays understood as an effective field theory that describes the dynamics of the long-wavelength and slow-time fluctuations of an underlying microscopic theory. In this work we extend the relativistic hydrodynamics to third order in the gradient expansion for neutral fluids in a general curved spacetime of $d$ dimensions. We find 58 new transport coefficients, 19 due to third-order scalar corrections and 39 due to tensorial corrections. In the particular case of a conformal fluid, the number of new transport coefficients is reduced to 19, all of them due to third-order tensorial corrections. The dispersion relations of linear fluctuations in the third-order relativistic hydrodynamics is obtained, both in the rest frame of the fluid and in a general moving frame. As an application we obtain some of the transport coefficients of a relativistic conformal fluid in three dimensions by using the AdS/CFT correspondence. These transport coefficients are extracted from the dispersion relations of the linear fluctuations. The gravity dual of the fluctuations in this conformal fluid is described by the gravitational perturbations of four-dimensional anti-de Sitter black branes, which are solutions of the Einstein equations with a negative cosmological constant. To find the hydrodynamic quasinormal modes (QNMs) of the scalar sector we use the SUSY quantum mechanics of the gravitational perturbations of four-dimensional black branes. Such a symmetry allows us to find the wavefunction of the scalar (or sound) sector in the hydrodynamic limit directly from the wavefunction of the vector (or shear) sector, which is usually easier to be found because the perturbation wave equations for the vector sector are much simpler than the ones for the scalar sector.
description: 41 pages, 1 figure
Drepanocladus aduncus Warnst.
Creators: name: Ros, Rosa M.
name: Olaf, Susana Rams
name: Eloy, Olaf Werner
name: Cerón, Eloy
Publisher: name: Zenodo
Year: 2024
Subjects: Biodiversity
Taxonomy
Plantae
Bryophyta
Bryopsida
Hypnales
Amblystegiaceae
Drepanocladus
Drepanocladus aduncus

description: Drepanocladus aduncus (Hedw.) Warnst.
RECORDS. — Bescherelle (1882), Jelenc (1955a): Kabylie du Djurdjura, Tala Ghizan; Kabylie du Djurdjura, Igoulmimen. Corbière (1904): Constantine, bords asséchés de l’étang supérieur du djebel Ouasch, 1180 m. Jelenc (1955a): Atlas de Blida, oued el Kebir. Constantine; Gorges de la Chiffa; Kabylie du Djurdjura, Aït Idjer; Kabylie du Djurdjura, Akfadou; Kabylie du Djurdjura, Akfadou au lac Noir, 1430 m; Kabylie du Djurdjura, Tirourda; La Réghaia; Maison-Carrée; Monts de Constantine. Boukhatem et al. (2017): El-Kala National Park, Tonga lake watershed. Mazari & Boulaacheb (2023): Setif, Megriss Mountain. Frequent.
COMMENT
Drepanocladus aduncus var. laxus Schimp. ex Jelenc nom. inval. was reported from Algeria (Constantine) by Jelenc (1955a). According to Ros et al. (2013), its identity is difficult to assess because in his taxonomic study Żarnowiec (2001), was not able to locate the type.
description: Published as part of Ros, Rosa M., Olaf, Susana Rams, Eloy, Olaf Werner & Cerón, Eloy, 2024, Revisiting the Bryophyte Checklist of Algeria: Exploring Diversity and Distribution, pp. 49-116 in Cryptogamie, Bryologie 20 (5) on pages 73-74, DOI: 10.5252/cryptogamie-bryologie2024v45a5, http://zenodo.org/record/14593891
Additional file 2: of Person-centred, integrated and pro-active care for multi-morbid elderly with advanced care needs: a propensity score-matched controlled trial
Creators: name: G. Berntsen
name: M. Dalbakk
name: J. Hurley
name: T. Bergmo
name: B. Solbakken
name: L. Spansvoll
name: J. Bellika
name: S. SkrĂ¸Vseth
name: T. Brattland
name: M. Rumpsfeld
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Cancer
subject: Science Policy

description: Supplementary analyses. This file includes additional tables showing: Crude results for all outcomes. Pooled adjusted results for all outcomes, showing I2 (the heterogeneity index across sites), with outlier-sites first included and then excluded. The Kaplan-Meier plot for mortality, with outlier sites excluded. (DOCX 53 kb)
Semi-Arid Agriculture in West Bengal (A Case Study)
Creators: name: Chaudhuri, Saroj Kanti
name: Chaudhuri, Saroj Kanti
Publisher: name: Unknown
Year: 1971
Subjects: Crop Production/Industries
Environmental Economics and Policy

description: This paper attempts to indicate the state of agriculture in a semi0arid region within an irrigated zone in an agriculturally advanced district, namely, Burdwan. While the semi-arid region consists of Asansol zone, the remaining part of the district comes under the irrigated zone which enjoys the facilities of canal irrigation from long past. While the district is said to be the most agriculturally advanced district in West Bengal, the agricultural condition of the purely rain-fed area in the same district needs much consideration in the context of overall 'green revolution'. The total operational area of the semi-arid zone is 1,40,520 acres which is as much as 30 percent of the total operational area of the district.
Removal of methylene blue from aqueous solutions using polyaniline/graphene oxide or polyaniline/reduced graphene oxide composites
Creators: name: E. A. EL-Sharkaway
name: Kamel, Rasha M.
name: EL-Sherbiny, Ibrahim M.
name: Gharib, Sally S.
Publisher: name: Taylor & Francis
Year: 2019
Subjects: subject: Medicine
subject: Molecular Biology
subject: Physiology
subject: FOS: Biological sciences
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: Sociology
subject: FOS: Sociology
subject: Marine Biology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: The polymeric nanocomposites polyaniline/graphene oxide (PANI/GO) and polyaniline/reduced graphene oxide (PANI/RGO) were synthesized for effective dye removal through adsorption process. Synthesized composites were characterized by XRD, SEM, TEM and FTIR analyses. The sorption of methylene blue dye (MB) on the PANI/GO or (PANI/RGO) composites were studied as a function of contact time, concentration, temperature, adsorbent dosage and pH, and the results showed that MB sorption was dependent on pH value. The optimum concentration of the dye and the contact time for sorption of MB on PANI/GO or PANI/RGO was determined to be 270 min and 50 mg/L, respectively while the adsorbent dosage of PANI/GO and PANI/RGO were determined to be 0.4 and 0.3 g, respectively. At optimum conditions, the nature of the adsorption process have been investigated by kinetic and isotherm models. The results showed that the adsorption process followed pseudo first order kinetics this noticed from the higher value of correlation coefficient (R2 = 0.991) and was best suited to the Langmuir model. The maximum dye adsorption capacity of PANI/GO and PANI/RGO were estimated to be 14.2 and 19.2 g-1 respectively. From the results, it can be assured that the PANI/RGO is more effectively than PANI/GO for the removal of dye pollutants in water.
The Dirac Operator in a Fermion Bag Background in 1+1 Dimensions and Generalized Supersymmetric Quantum Mechanics
Creators: name: Feinberg, Joshua
Publisher: name: arXiv
Year: 2001
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We show that the spectral theory of the Dirac operator $D = i\delsl-σ(x) -iπ(x)\gam_5$ in a static background $(σ(x),π(x))$ in 1+1 space-time dimensions, is underlined by a certain generalization of supersymmetric quantum mechanics, and explore its consequences.
description: latex, 18 pages
Sarcophila Rondani 1856
Creators: name: O'Hara, James E.
name: Cerretti, Pierfilippo
name: Pape, Thomas
name: Evenhuis, Neal L.
Publisher: name: Zenodo
Year: 2011
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Sarcophagidae
Sarcophila

description: 495. Sarcophila Rondani, 1856: 86.
 ORIGINALLY INCLUDED SPECIES: Musca latifrons Fallén, 1817.
 TYPE SPECIES: Musca latifrons Fallén, 1817, by original designation.
 CURRENT STATUS: Valid genus [teste Pape (1996: 166)].
FAMILY: SARCOPHAGIDAE.
description: Published as part of O'Hara, James E., Cerretti, Pierfilippo, Pape, Thomas & Evenhuis, Neal L., 2011, 3141, pp. 1-268 in Zootaxa 3141 on page 161
Encalypta trachymitria Ripart
Creators: name: Ros, Rosa M.
name: Olaf, Susana Rams
name: Eloy, Olaf Werner
name: Cerón, Eloy
Publisher: name: Zenodo
Year: 2024
Subjects: Biodiversity
Taxonomy
Plantae
Bryophyta
Bryopsida
Pottiales
Encalyptaceae
Encalypta
Encalypta trachymitria

description: Encalypta trachymitria Ripart
Encalypta rhaptocarpa var. leptodon Lindb.
Nomenclature follows Fedosov (2012).
RECORDS. — Jelenc (1955a): Dra el Arba; Kabylie des Babor, cap Aokas. Rare.
description: Published as part of Ros, Rosa M., Olaf, Susana Rams, Eloy, Olaf Werner & Cerón, Eloy, 2024, Revisiting the Bryophyte Checklist of Algeria: Exploring Diversity and Distribution, pp. 49-116 in Cryptogamie, Bryologie 20 (5) on page 74, DOI: 10.5252/cryptogamie-bryologie2024v45a5, http://zenodo.org/record/14593891
The Language of Dialogue Is Complex
Creators: name: Robertson, Alexander
name: Aiello, Luca Maria
name: Quercia, Daniele
Publisher: name: arXiv
Year: 2019
Subjects: subject: Computers and Society (cs.CY)
subject: Computation and Language (cs.CL)
subject: Social and Information Networks (cs.SI)
subject: FOS: Computer and information sciences

description: Integrative Complexity (IC) is a psychometric that measures the ability of a person to recognize multiple perspectives and connect them, thus identifying paths for conflict resolution. IC has been linked to a wide variety of political, social and personal outcomes but evaluating it is a time-consuming process requiring skilled professionals to manually score texts, a fact which accounts for the limited exploration of IC at scale on social media.We combine natural language processing and machine learning to train an IC classification model that achieves state-of-the-art performance on unseen data and more closely adheres to the established structure of the IC coding process than previous automated approaches. When applied to the content of 400k+ comments from online fora about depression and knowledge exchange, our model was capable of replicating key findings of prior work, thus providing the first example of using IC tools for large-scale social media analytics.
description: 12 pages, 9 figures, 10 tables
Impacts of packed bed polydispersity and deformation on fine particle transport
Creators: name: Vyas, Dhairya R.
name: Gao, Song
name: Umbanhowar, Paul B.
name: Ottino, Julio M.
name: Lueptow, Richard M.
Publisher: name: arXiv
Year: 2024
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: Static granular packings play a central role in numerous industrial applications and natural settings. In these situations, fluid or fine particle flow through a bed of static particles is heavily influenced by the narrowest passage connecting the pores of the packing, commonly referred to as pore throats or constrictions. Existing studies predominantly assume monodisperse rigid particles, but this is an oversimplification of the problem. In this work, we illustrate the connection between pore throat size, polydispersity, and particle deformation. Simple analytical expressions are provided to link these properties of the packing, followed by examples from Discrete Element Method (DEM) simulations of fine particle percolation demonstrating the impact of polydispersity and particle deformation. Our intent is to emphasize the substantial impact of polydispersity and particle deformation on constriction size, underscoring the importance of accounting for these effects in particle transport in granular packings.
Supplementary document for High-performance, on-chip speckle spectrometer using two-dimensional silicon photonic disordered microring lattice - 6324573.pdf
Creators: name: Lin, Zhongjin
name: Yu, Shangxuan
name: Chen, Yuxuan
name: Cai, Wangning
name: Lin, Becky
name: Song, Jinxiang
name: MITCHELL, MATTHEW
name: Hammood, Mustafa
name: Jhoja, Jaspreet
name: Jaeger, Nicolas
Publisher: name: Optica Publishing Group
Year: 2023
Subjects: Uncategorized

description: Supplemental
The prevalence of pseudo-bulges in the Auriga simulations
Creators: name: Gargiulo, Ignacio D.
name: Monachesi, Antonela
name: Gómez, Facundo A.
name: Grand, Robert J. J.
name: Marinacci, Federico
name: Pakmor, Rüdiger
name: White, Simon D. M.
name: Bell, Eric F.
name: Fragkoudi, Francesca
name: Tissera, Patricia
Publisher: name: arXiv
Year: 2019
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We study the galactic bulges in the Auriga simulations, a suite of thirty cosmological magneto-hydrodynamical zoom-in simulations of late-type galaxies in Milky Way-sized dark matter haloes performed with the moving-mesh code AREPO. We aim to characterize bulge formation mechanisms in this large suite of galaxies simulated at high resolution in a fully cosmological context. The bulges of the Auriga galaxies show a large variety in their shapes,sizes and formation histories. According to observational classification criteria, such as Sersic index and degree of ordered rotation, the majority of the Auriga bulges can be classified as pseudo-bulges, while some of them can be seen as composite bulges with a classical component; however, none can be classified as a classical bulge. Auriga bulges show mostly an in-situ origin, 21 percent of them with a negligible accreted fraction (facc < 0.01). In general,their in-situ component was centrally formed, with 75 percent of the bulges forming most of their stars inside the bulge region at z=0. Part of their in-situ mass growth is rapid and is associated with the effects of mergers, while another part is more secular in origin. In 90 percent of the Auriga bulges, the accreted bulge component originates from less than four satellites.We investigate the relation between the accreted stellar haloes and the bulges of the Auriga simulations. The total bulge mass shows no correlation with the accreted stellar halo mass, as in observations. However, the accreted mass of bulges tends to correlate with their respective accreted stellar halo mass.
description: 21 pages, 14 figures
title: Deep Learning for Hyperbolic Conservation Laws with Non‐convex Flux
Creators: name: Minbashian, Hadi
name: Giesselmann, Jan
Publisher: name: Wiley‐VCH
Year: 2024

description: In this work, we investigate the capabilities of deep neural networks for solving hyperbolic conservation laws with non‐convex flux functions. The behaviour of solutions to these problems depends on the underlying small‐scale regularization. In many applications concerning phase transition phenomena, the regularization terms consist of diffusion and dispersion which are kept in balance in the limit. This may lead to the development of both classical and non‐classical (or undercompressive) shock waves at the same time which makes the development of approximation schemes that converge towards the appropriate weak solution of these problems challenging. Here, we consider a scalar conservation law with cubic flux function as a toy model and present preliminary results of an ongoing work to study the capabilities of a deep learning algorithm called PINNs proposed in [1] for solving this problem. It consists of a feed‐forward network with a hyperbolic tangent activation function along with an additional layer to enforce the differential equation.
Effects of Relativistic Expansion on the Late-time Supernova Light Curves
Creators: name: Iwamoto, Koichi
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The effects of relativistic expansion on the late-time supernova light curves are investigated analytically, and a correction term to the (quasi-)exponential decay is obtained by expanding the observed flux in terms of (β), where (β) is the maximum velocity of the ejecta divided by the speed of light (c). It is shown that the Doppler effect brightens the light curve owing to the delayed decay of radioactive nuclei as well as to the Lorentz boosting of the photon energies. The leading correction term is quadratic in (β), thus being proportional to (E_{\rm k}/(M_{\rm ej} c^2)), where (E_{\rm k}) and (M_{\rm ej}) are the kinetic energy of explosion and the ejecta mass. It is also shown that the correction term evolves as a quadratic function of time since the explosion. The relativistic effect is negligibly small at early phases, but becomes of considerable size at late phases. In particular, for supernove having a very large energy(hypernova) or exploding in a jet-like or whatever non-spherical geometry, (^{56})Ni is likely to be boosted to higher velocities and then we might see an appreciable change in flux. However, the actual size of deviation from the (quasi-)exponential decay will be uncertain, depending on other possible effects such as ionization freeze-out and contributions from other energy sources that power the light curve.
description: 12 pages including 2 figures, submitted to ApJL