cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Viscous-inviscid interaction on moving walls
Creators: name: Kirsten, Julius
Publisher: name: Imperial College London
Year: 2017

description: This thesis consists of two parts. In part I, the viscous-inviscid interaction in su- personic flows over down- and upstream moving walls is analysed. The separation is assumed to be provoked by an impinging shock or expansion wave. For large val- ues of the Reynolds number and under the assumption that the speed of the wall is [Mathematical equation appears here. To view, please open pdf attachment], the interaction is described by the classical triple deck theory. For the case [Mathematical equation appears here. To view, please open pdf attachment], the Navier-Stokes equations are analysed in a vicinity of the separation point using the method of matched asymptotic expansions. In chapter 2, the linearised interaction problem for a downstream moving wall is stud- ied and the upstream influence of small perturbations is shown to be exponentially decaying. Moreover, it is found that small perturbations to the skin friction decay alge- braically downstream. The focus then shifts towards the fully non-linear problem, when the strength of the impinging shock wave is of [Symbol appears here. To view, please open pdf attachment], and it is shown numerically that a singularity, indicative of separation, develops at the outer edge of the viscous sublayer. In chapter 3, supersonic flow over an upstream moving wall is considered for which the development of a singularity is observable in the non-linear problem, when the imping- ing shock wave is replaced by an expansion wave. Part II consists of chapter 4, in which hypersonic flows are investigated. In this case the viscous-inviscid interaction extends over the entire body surface and is described by a two-layer model. On motionless and downstream moving walls, the solution to the interaction problem near the leading edge is not unique and there exists an alge- braic upstream influence of perturbations. The associated eigenvalue problem near the leading edge is solved numerically using an iterative procedure and it is shown that the upstream influence becomes smaller as the speed of the wall is increased.
Pandora's Problem with Combinatorial Cost
Creators: name: Berger, Ben
name: Ezra, Tomer
name: Feldman, Michal
name: Fusco, Federico
Publisher: name: arXiv
Year: 2023
Subjects: subject: Data Structures and Algorithms (cs.DS)
subject: Computer Science and Game Theory (cs.GT)
subject: FOS: Computer and information sciences

description: Pandora's problem is a fundamental model in economics that studies optimal search strategies under costly inspection. In this paper we initiate the study of Pandora's problem with combinatorial costs, capturing many real-life scenarios where search cost is non-additive. Weitzman's celebrated algorithm [1979] establishes the remarkable result that, for additive costs, the optimal search strategy is non-adaptive and computationally feasible.
 We inquire to which extent this structural and computational simplicity extends beyond additive cost functions. Our main result is that the class of submodular cost functions admits an optimal strategy that follows a fixed, non-adaptive order, thus preserving the structural simplicity of additive cost functions. In contrast, for the more general class of subadditive (or even XOS) cost functions, the optimal strategy may already need to determine the search order adaptively. On the computational side, obtaining any approximation to the optimal utility requires super polynomially many queries to the cost function, even for a strict subclass of submodular cost functions.
Effects of pesticide exposure on the morphological development of the bee brain and the consequences for learning performance
Creators: name: Smith, Dylan
Publisher: name: Imperial College London
Year: 2018

description: How pesticides contribute towards insect pollinator declines is a question of global ecological and economic importance. In social bees, a critical but understudied step in evaluating pesticide risk is to understand how contaminated food brought back to the colony can affect developing individuals. Within social bee colonies individuals are likely to be exposed to pesticides during two principal developmental stages - brood (larval & pupal) and early adulthood. Understanding how the developmental timing of pesticide exposure affects adult phenotypes is important in revealing the stages at which workers are most vulnerable to exposure and thus uncovers windows of susceptibility in colony development. This thesis investigates how exposure to a neurotoxic pesticide in a major insect pollinator ¬– the bumblebee (Bombus terrestris audax), at different key developmental stages affects learning behaviour at two adult ages, and links variation in learning performance with volumetric changes in brain development. In Chapter 2 I investigate the olfactory learning behaviour of individuals, finding that older bees have reduced learning performance, whether exposed during brood or early-adult development. In chapter 3 I present the development of a new method for exploring morphological variation in tiny soft tissue structures using micro-Computed tomography and image analysis. In Chapters 4 and 5 I apply this new protocol to investigate the volume of the major brain neuropils of individual workers that were experimentally treated and assessed for learning performance in Chapter 2. I find that exposure during either developmental phase can impede growth of the structures associated with olfactory learning and that these reductions in volume correlate with impaired learning performance. My findings show that in response to pesticde exposure during brood development or early adulthood, bumblebee colonies can produce workers with developmentally and functionally impaired brains. This is worrying as it suggests that social bee colonies foraging on pesticide contaminated food may be producing a behaviourally impaired workforce.
Magnetic field decay and period evolution of the source RX J0720.4-3125
Creators: name: Popov, S. B.
name: Konenkov, D. Yu.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We studied possible evolution of the rotational period and the magnetic field of the X-ray source RX J0720.4-3125 assuming this source to be an isolated neutron star accreting from the interstellar medium. Magnetic field of the source is estimated to be $10^6 - 10^9$ Gs (most probably $\approx 2\cdot 10^8$ Gs), and it is difficult to explain the observable rotational period 8.38 s without invoking hypothesis of the magnetic field decay. We used the model of ohmic decay of the crustal magnetic field. The estimates of the accretion rate ($10^{-14} - 10^{-16} M_\odot/yr$), velocity of the source relative to the interstellar medium ($10 - 50 $ km/s), the neutron star age ($2\cdot 10^9 - 10^{10}$ yrs) are obtained.
description: 9 pages, 3 PostScript figures
Three-dimensional modeling of mass transfer in close binary systems with non-synchronous rotation
Creators: name: Bisikalo, D. V.
name: Boyarchuk, A. A.
name: Kuznetsov, O. A.
name: Chechetkin, V. M.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present the results of three-dimensional numerical simulations of mass transfer in semi-detached binary systems in which the mass-losing star is rotating. The cases of aligned and misaligned non-synchronous rotation of the donor star are considered; the resulting flow patterns are compared to the synchronous case. The main properties of the flow, such as the formation of an circumbinary envelope, the absence of a "hot spot" on the edge of the accretion disk, and the formation of a shock wave along the flow edge, are qualitatively similar to those obtained earlier. For the case of misaligned, non-synchronous rotation, the behavior of the disk and surrounding matter in established flow regime reflects changes in the boundary conditions at the surface of the donor star; in other words, a "driven disk" model is realized in the calculations.
description: LaTeX, 22 pages, accepted for publication in Astronomy Reports
Additional file 2: of Genomic profiles of primary and metastatic esophageal adenocarcinoma identified via digital sorting of pure cell populations: results from a case report
Creators: name: Isidori, Federica
name: Malvi, Deborah
name: Fittipaldi, Silvia
name: Forcato, Claudio
name: Bozzarelli, Isotta
name: Sala, Claudia
name: Raulli, Giovanni
name: D’Errico, Antonia
name: Fiorentino, Michelangelo
name: Seri, Marco
name: Kausilia Krishnadath
name: Bonora, Elena
name: Mattioli, Sandro
Publisher: name: figshare
Year: 2018
Subjects: subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: Cancer

description: Figure S1. Plots of Copy Number Analysis and phylogenetic tree using WES data. A 18 Mb region on chromosome 6 (q21-22.33) is indicated (red box), where CNV analysis identified a copy gain in PT (A) and M1 (B), as reported in Additional file 1: Table S2. (C) In the second chest metastasis (M2) a focal amplification was detected in the 6q22.33 region, spanning RNF146 and ECHDC1 genes (black arrowhead). (D) SNPhylo analysis results, showing the genetic distance between the three tumor samples. Numbers indicate the branch length from central node. The distance between two tumors is equal to the sum of their branch length. Analysis was performed according to [6]. (PDF 137 kb)
UniverseMachine: The Correlation between Galaxy Growth and Dark Matter Halo Assembly from z=0-10
Creators: name: Behroozi, Peter
name: Wechsler, Risa
name: Hearin, Andrew
name: Conroy, Charlie
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present a method to flexibly and self-consistently determine individual galaxies' star formation rates (SFRs) from their host haloes' potential well depths, assembly histories, and redshifts. The method is constrained by galaxies' observed stellar mass functions, SFRs (specific and cosmic), quenched fractions, UV luminosity functions, UV-SM relations, IRX-UV relations, auto- and cross-correlation functions (including quenched and star-forming subsamples), and quenching dependence on environment; each observable is reproduced over the full redshift range available, up to 01 correlates strongly with halo mass; quenched fractions at fixed halo mass decrease with increasing redshift; massive quenched galaxies reside in higher-mass haloes than star-forming galaxies at fixed galaxy mass; star-forming and quenched galaxies' star formation histories at fixed mass differ most at z<0.5; satellites have large scatter in quenching timescales after infall, and have modestly higher quenched fractions than central galaxies; Planck cosmologies result in up to 0.3 dex lower stellar mass-halo mass ratios at early times; and, nonetheless, stellar mass-halo mass ratios rise at z>5. Also presented are revised stellar mass-halo mass relations for all, quenched, star-forming, central, and satellite galaxies; the dependence of star formation histories on halo mass, stellar mass, and galaxy SSFR; quenched fractions and quenching timescale distributions for satellites; and predictions for higher-redshift galaxy correlation functions and weak lensing surface densities. The public data release (DR1) includes the massively parallel (>10^5 cores) implementation (the UniverseMachine), the newly compiled and remeasured observational data, derived galaxy formation constraints, and mock catalogues including lightcones.
description: 51 pages; MNRAS accepted. Updated data and code available at http://www.peterbehroozi.com/data.html
Stable measurement-induced Floquet enriched topological order
Creators: name: Vu, DinhDuy
name: Lavasani, Ali
name: Lee, Jong Yeon
name: Fisher, Matthew P. A.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Quantum Physics (quant-ph)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: The Floquet code utilizes a periodic sequence of two-qubit measurements to realize the topological order. After each measurement round, the instantaneous stabilizer group can be mapped to a honeycomb toric code, explaining the topological feature. The code also possesses a time-crystal order - the $e-m$ transmutation after every cycle, breaking the Floquet symmetry of the measurement schedule. This behavior is distinct from the stationary topological order realized in either random circuits or time-independent Hamiltonian. Therefore, the resultant phase belongs to the overlap between the classes of Floquet enriched topological orders and measurement-induced phases. In this work, we construct a continuous path interpolating between the Floquet and toric codes, focusing on the transition between the time-crystal and stationary topological phases. We show that this transition is characterized by a divergent length scale. We also add single-qubit perturbations to the model and obtain a richer two-dimensional parametric phase diagram of the Floquet code, showing the stability of the Floquet enriched topological order.
description: 6+8 pages, 13 figures
Emberiza familiaris Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Aves
Passeriformes
Emberizidae
Emberiza
Emberiza familiaris

description: Emberiza familiaris [spec. nov.]
E. griseo-maculata, apicibus rectricum albis, dorso postico flavo.
Motacilla capite & rostro nigro, uropygio luteo. Osb. iter. 102.
Habitat in Asia.
Corpus magnitudine Ligurini, supra cinereum maculis fuscis, subtus cinereum. Dorsum sub alis & versus caudam flavum. Tectrices caudae albae.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 178, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Additional file 1: of Functional study of CHS gene family members in citrus revealed a novel CHS gene affecting the production of flavonoids
Creators: name: Zhibin Wang
name: Qibin Yu
name: Wanxia Shen
name: Choaa El Mohtar
name: Xiaochun Zhao
name: Gmitter, Fredrick
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Space Science
subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Evolutionary Biology
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: Developmental Biology
subject: Science Policy
subject: Plant Biology

description: Table S1. Identify homology of CHS or CHS-like genes considered in Fig. 1. Table S2. Information of the CHS candidate genes and primers used for expression analysis. Table S3. Standard curve used in flavonoids detection. (DOCX 127 kb)
The Mass Of Black Holes in the Nuclei Of Spirals
Creators: name: Salucci, Paolo
name: Ratnam, Charu
name: Monaco, Pierluigi
name: Danese, Luigi
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We use rotation curve kinematics of 1000 spiral galaxies to investigate if these galaxies could host BH (Black Hole) remnants that once powered the QSO phenomenon. The rotation curves of both early and late-type spirals are used to place upper limits on the BH mass. We find that the central objects in spirals are 10-100 times less massive than those detected in ellipticals, suggesting that the contribution to the QSO phenomenon by the BH remnants hosted in these objects is negligible. The upper limits on the mass of the BHs resident in late type spirals are stringent: $M_{BH}\leq 10^{6}-10^{7} M_{\odot}$, indicating that only low luminosity activity possibly occurred in these objects.
description: 12 pages, revised version, in press on MN
Two-point correlation function of high-redshift objects: an explicit formulation on a light-cone hypersurface
Creators: name: Yamamoto, Kazuhiro
name: Suto, Yasushi
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: While all the cosmological observations are carried out on a light-cone, the null hypersurface of an observer at z=0, the clustering statistics has been properly defined only on the constant-time hypersurface. We develop a theoretical formulation for a two-point correlation function on the light-cone, and derive a practical approximate expression relevant to the discussion of clustering of high-redshift objects at large separations. As a specific example, we present predictions of the two-point correlation function for the Durham/AAT, SDSS and 2dF quasar catalogues. We also briefly discuss the effects of adopted luminosity function, cosmological parameters and bias models on the correlation function on the light-cone.
description: 21 pages, 5 figures, ApJ in press
Inclusive J/$ψ$ production at forward and backward rapidity in p-Pb collisions at $\sqrt{s_{\rm NN}}$ = 8.16 TeV
Creators: name: ALICE Collaboration
Publisher: name: arXiv
Year: 2018
Subjects: subject: Nuclear Experiment (nucl-ex)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: Inclusive J/$ψ$ production is studied in p-Pb interactions at a centre-of-mass energy per nucleon-nucleon collision $\sqrt{s_{\rm NN}}=8.16$ TeV, using the ALICE detector at the CERN LHC. The J/$ψ$ meson is reconstructed, via its decay to a muon pair, in the centre-of-mass rapidity intervals $2.03
description: 24 pages, 8 captioned figures, 1 table, authors from page 19, published, figures at http://aliceinfo.cern.ch/ArtSubmission/node/4284
3D Printing Lattice Based Pressure Sensors for Human Health and Performance Monitoring
Creators: name: Stein, Emily
Publisher: name: Stanford Digital Repository
Year: 2025
Subjects: subject: 3D printing
subject: Dielectrics
subject: Capacitive pressure sensors

description: Capacitive pressure sensors have generated significant interest for applications in human health and performance monitoring. A wide range of potential applications require low cost, compliant sensors that can be tuned to appropriate sensing regimes and sensitivities. Previous literature has shown that microstructuring the dielectric layers of sensors can provide significant increases in sensitivity and that dielectric geometry can directly impact sensor range and performance. Leveraging advances in high resolution 3D printing we have developed a new method for fabricating elastomeric lattices with highly tunable geometric properties for use as capacitive pressure sensor dielectrics. We characterized the impact of microstructure geometry on the capacitive pressure sensors’ mechanical performance and developed a new set of analytical equations suitable for the lattice geometries to predict the capacitance response and sensitives of microstructured sensors under external pressure. This work covers 1) design rationale of lattice unit cells, 2) an analytical expression that directly predicts the capacitance response, and 3) 3D printing elastomeric lattice dielectric layers, which taken together serve as a framework and starting point to design and fabricate capacitive pressure sensors for various biomedical applications as well as for human health and performance monitoring.
title: ADCO, Sixième cartulaire de Saint-Étienne de Dijon (1662), Cart. 30 (G 133), 441 folios, f. 402
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2012
name: Petot, Frédéric
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: cartulaire
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge

description: Sixième cartulaire de Saint-Étienne de Dijon (1662), Archives départementales de la Côte-d'Or, Cart. 30 (G 133), 441 folios, f. 402, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Sixième cartulaire de Saint-Étienne de Dijon (1662), Archives départementales de la Côte-d'Or, Cart. 30 (G 133), 441 folios, f. 402, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https://manuscrits.cbma-project.eu/
description: Provenance: abbaye Saint-Étienne de Dijon
description: Provenance: http://www.wikidata.org/entity/Q15945019
Exploration of Sustainable Logistics Service Quality Evaluation Indicator System-Taking China as an Example
Creators: name: Sifan, Zhang
name: Yan, Jiang
Publisher: name: Zenodo
Year: 2024

description: Due to the deterioration of the natural environment, the acceleration of market globalization, and the deepening of health and equity awareness, the public attaches increasing importance to sustainable development. Decarburization and sustainability have become an inevitable trend in the development of the logistics industry. However, research on sustainable logistics service quality in academia is fragmented, and emerging market countries, including China, lack evaluation tools for sustainable logistics service quality. To fill this gap, a systematic review of domestic and international studies on logistics service quality is conducted, and a sustainable logistics service quality evaluation tool covering the environment, economy, society, and enterprise is proposed based on the theory of "triple bottom line" and expert evaluation. The results suggest that Chinese logistics service providers should focus on using environmentally friendly packaging materials, strengthening green technology innovation, and promoting the continuous optimization of logistics costs. They should also focus on employee training and rights protection, and actively fulfill their social responsibilities to build a sustainable competitive advantage in logistics services.
Emberiza militaris Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Aves
Passeriformes
Emberizidae
Emberiza
Emberiza militaris

description: Emberiza militaris [spec. nov.]
E. fusca, pectore gula humerisque sanguineis.
Turdus ater, pectore coccineo. Mus. Ad. Fr. 1. p. 18. Chin. Lagerstr. 12.
Rubicilla fusca major. Edw. av. 82. t. 82.
Habitat in America, Asia.
Magnitudo Sturni. Color supra e scolopacino fuscus, subtus sanguineus. Rostrum basi subcalvum. Remiges fuscae: 1, 2 margine exteriore griseae. Rectrices aequales, fuscae: apice fasciis pallidioribus variae.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 178, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Integer quantum Hall transition on a tight-binding lattice
Creators: name: Puschmann, Martin
name: Cain, Philipp
name: Schreiber, Michael
name: Vojta, Thomas
Publisher: name: arXiv
Year: 2018
Subjects: subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: FOS: Physical sciences

description: Even though the integer quantum Hall transition has been investigated for nearly four decades its critical behavior remains a puzzle. The best theoretical and experimental results for the localization length exponent $ν$ differ significantly from each other, casting doubt on our fundamental understanding. While this discrepancy is often attributed to long-range Coulomb interactions, Gruzberg et al. [Phys. Rev. B 95, 125414 (2017)] recently suggested that the semiclassical Chalker-Coddington model, widely employed in numerical simulations, is incomplete, questioning the established central theoretical results. To shed light on the controversy, we perform a high-accuracy study of the integer quantum Hall transition for a microscopic model of disordered electrons. We find a localization length exponent $ν=2.58(3)$ validating the result of the Chalker-Coddington network.
description: 10 pages, 9 figures
Cosmological Magnetic Fields Limits in an Inhomogeneous Universe
Creators: name: Blasi, Pasquale
name: Burles, Scott
name: Olinto, Angela V.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We study the effect of inhomogeneities in the matter distribution of the universe on the Faraday rotation of light from distant QSOs and derive new limits on the cosmological magnetic field. The matter distribution in the Universe is far from being homogeneous and, for the redshifts of interest to rotation measures (RM), it is well described by the observed Ly-$α$ forest. We use a log-normal distribution to model the Ly-$α$ forest and assume that a cosmological magnetic field is frozen into the plasma and is therefore a function of the density inhomogeneities. The Ly-$α$ forest results are much less sensitive to the cosmological magnetic field coherence length than those for a homogeneous universe and show an increase in the magnitude of the expected RM for a given field by over an order of magnitude. The forest also introduces a large scatter in RM for different lines-of-sight with a highly non-gaussian tail that renders the variance and the mean RM impractical for setting limits. The $median|{\rm RM}|$ is a better statistical indicator which we use to derive the following limits using the observed RM for QSOs between $z = 0$ and $z = 2.5$. We set $Ω_b h^2 = 0.02$ and get for cosmological fields coherent accross the present horizon, $B_{H_0^{-1}} \la 10^{-9}$ G in the case of a Ly-$α$ forest which is stronger than the limit for a homogeneous universe, $B_{H_0^{-1}}^h \la 2 \times 10^{-8}$ G; while for 50 Mpc coherence length, the inhomogeneous case gives $B_{50 {\rm Mpc}} \la 6 \times 10^{-9}$ G while the homogeneous limit is $B_{50 {\rm Mpc}}^h \la 10^{-7}$ G and for coherence length equal to the Jeans length, $B_{λ_J} \la 10^{-8}$ G for the Ly-$α$ case while $B_{λ_J}^h \la 10^{-6}$ G.
description: submitted to ApJL
Warped discs and the directional stability of jets in Active Galactic Nuclei
Creators: name: Natarajan, Priyamvada
name: Armitage, Philip J.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Warped accretion discs in Active Galactic Nuclei (AGN) exert a torque on the black hole that tends to align the rotation axis with the angular momentum of the outer disc. We compute the magnitude of this torque by solving numerically for the steady state shape of the warped disc, and verify that the analytic solution of Scheuer and Feiler (1996) provides an excellent approximation. We generalise these results for discs with strong warps and arbitrary surface density profiles, and calculate the timescale on which the black hole becomes aligned with the angular momentum in the outer disc. For massive holes and accretion rates of the order of the Eddington limit the alignment timescale is always short (less than a Myr), so that jets accelerated from the inner disc region provide a prompt tracer of the angular momentum of gas at large radii in the disc. Longer timescales are predicted for low luminosity systems, depending on the degree of anisotropy in the disc's hydrodynamic response to shear and warp, and for the final decay of modest warps at large radii in the disc that are potentially observable via VLBI. We discuss the implications of this for the inferred accretion history of those Active Galactic Nuclei whose jet directions appear to be stable over long timescales. The large energy deposition rate at modest disc radii during rapid realignment episodes should make such objects transiently bright at optical and infrared wavelengths.
description: MNRAS, in press. Revised to match accepted version, with one new figure showing alignment timescale as a function of black hole mass
An Application of Computable Distributions to the Semantics of Probabilistic Programs
Creators: name: Huang, Daniel
name: Morrisett, Greg
name: Spitters, Bas
Publisher: name: arXiv
Year: 2018
Subjects: subject: Programming Languages (cs.PL)
subject: FOS: Computer and information sciences

description: In this chapter, we explore how (Type-2) computable distributions can be used to give both (algorithmic) sampling and distributional semantics to probabilistic programs with continuous distributions. Towards this end, we sketch an encoding of computable distributions in a fragment of Haskell and show how topological domains can be used to model the resulting PCF-like language. We also examine the implications that a (Type-2) computable semantics has for implementing conditioning. We hope to draw out the connection between an approach based on (Type-2) computability and ordinary programming throughout the chapter as well as highlight the relation with constructive mathematics (via realizability).
description: Accepted as contribution to "Foundations of Probabilistic Programming"
Additional file 3: of Association of different iron deficiency cutoffs with adverse outcomes in chronic kidney disease
Creators: name: Eisenga, Michele
name: Nolte, Ilja
name: Meer, Peter Van Der
name: Bakker, Stephan
name: Gaillard, Carlo
Publisher: name: figshare
Year: 2018
Subjects: subject: Biochemistry
subject: Medicine
subject: Biotechnology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Marine Biology

description: Table S3. Association of different cutoff values of ferritin and TSAT, adjusted for age and sex, with respect to risk of anemia in CKD patients (based on eGFR 30 mg/24 h or albumin-to-creatinine ratio ≥ 30 mg/g). (PDF 226 kb)
Towards Entanglement Entropy of Random Large-N Theories
Creators: name: Shao, Siqi
name: Komijani, Yashar
Publisher: name: arXiv
Year: 2023
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: A large class of strongly correlated quantum systems can be described in certain large-N limits by quadratic in field actions along with self-consistency equations that determine the two-point functions. We use the replica approach and the notion of shifted Matsubara frequency to compute von Neumann and Rényi entanglement entropies for generic bi-partitioning of such systems. We argue that the von Neumann entropy can be computed from equilibrium spectral functions w/o partitioning, while the Rényi entropy requires re-calculating the spectrum in the interacting case. We demonstrate the flexibility of the method by applying it to examples of a two-site problem in presence of decoherence, and coupled Sachdev-Ye-Kitaev models.
Locally Biased Galaxy Formation and Large Scale Structure
Creators: name: Narayanan, Vijay K.
name: Berlind, Andreas
name: Weinberg, David H.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We examine the influence of the morphology-density(MD) relation and a wide range of simple models for biased galaxy formation on statistical measures of large scale structure. We contrast the behavior of local biasing models, in which the efficiency of galaxy formation is determined by density, geometry, or velocity dispersion of the local mass distribution, with that of non-local biasing models, in which galaxy formation is modulated coherently over scales larger than the galaxy correlation length. If morphological segregation of galaxies is governed by a local MD relation, then the correlation function of E/S0 galaxies should be steeper and stronger than that of spiral galaxies on small scales, as observed, while on large scales the correlation functions of E/S0 and spiral galaxies should have the same shape but different amplitudes. Similarly, all of our local bias models produce scale-independent amplification of the correlation function and power spectrum in the linear and mildly non-linear regimes; only a non-local biasing mechanism can alter the shape of the power spectrum on large scales. Moments of the biased galaxy distribution retain the hierarchical pattern of the mass moments, but biasing alters the values and scale-dependence of the hierarchical amplitudes S3 and S4. Pair-weighted moments of the galaxy velocity distribution are sensitive to the details of the biasing prescription. The non-linearity of the relation between galaxy density and mass density depends on the biasing prescription and the smoothing scale, and the scatter in this relation is a useful diagnostic of the physical parameters that determine the bias. Although the sensitivity of galaxy clustering statistics to the details of biasing is an obstacle to testing cosmological models, it is an asset for testing galaxy formation theories.
description: 47 pages including 17 Figures, submitted to ApJ
title: ADCO, Cartulaire de l'office de la Porte de l'abbaye de Cîteaux, Registrum possessionum porte Cistercii (début XVe siècle), Cart. 172 (11 H 69), 115 folios, f. 0048
Creators: name: de la Côte d'Or, Archives départementales
name: CG21/F.PETOT/2012
name: Petot, Frédéric
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire

description: Cartulaire de l'office de la Porte de l'abbaye de Cîteaux, Registrum possessionum porte Cistercii (début XVe siècle), Archives départementales de la Côte-d'Or, Cart. 172 (11 H 69), 115 folios, f. 0048, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire de l'office de la Porte de l'abbaye de Cîteaux, Registrum possessionum porte Cistercii (début XVe siècle), Archives départementales de la Côte-d'Or, Cart. 172 (11 H 69), 115 folios, f. 0048, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
Third family of compact stars within a nonlocal chiral quark model equation of state
Creators: name: Alvarez-Castillo, D. E.
name: Blaschke, D. B.
name: Grunfeld, A. G.
name: Pagura, V. P.
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: A class of hybrid compact star equations of state is investigated that joins by a Maxwell construction a low-density phase of hadronic matter, modeled by a relativistic meanfield approach with excluded nucleon volume, with a high-density phase of color superconducting two-flavor quark matter, described within a nonlocal covariant chiral quark model. We find the conditions on the vector meson coupling in the quark model under which a stable branch of hybrid compact stars occurs in the cases with and without diquark condensation. We show that these hybrid stars do not form a third family disconnected from the second family of ordinary neutron stars unless additional (de)confining effects are introduced with a density-dependent bag pressure. A suitably chosen density dependence of the vector meson coupling assures that at the same time the $2~$M$_\odot$ maximum mass constraint is fulfilled on the hybrid star branch. A twofold interpolation method is realized which implements both, the density dependence of a confining bag pressure at the onset of the hadron-to-quark matter transition as well as the stiffening of quark matter at higher densities by a density-dependent vector meson coupling. For three parametrizations of this class of hybrid equation of state the properties of corresponding compact star sequences are presented, including mass twins of neutron and hybrid stars at 2.00, 1.39 and 1.20 $M_\odot$, respectively. The sensitivity of the hybrid equation of state and the corresponding compact star sequences to variations of the interpolation parameters at the 10% level is investigated and it is found that the feature of third family solutions for compact stars is robust against such a variation. This advanced description of hybrid star matter allows to interpret GW170817 as a merger not only of two neutron stars but also of a neutron star with a hybrid star or of two hybrid stars.
description: 20 pages, 17 figures, 2 tables, largely extended version
Gizli kürtaj nasıl yapılır 0553 366 23 76
Creators: name: Kürtaj ilacı 0553 366 23 76, Düşük hapi 0553 366 23 76
Publisher: name: figshare
Year: 2024
Subjects: classificationCode: 320219
subject: Paramedicine
classificationCode: 310303
subject: Ecological physiology
classificationCode: 310301
subject: Behavioural ecology

description: 0553 366 23 76 HIZLI VE GİZLİ GÖNDERİM
Müşteri mahremiyetinizi ön planda tutarak, talebiniz üzerine Cytotec ilacını hızlı ve gizli bir şekilde size ulaştırıyoruz. Paketinizin içeriği dışarıdan anlaşılmayacak şekilde paketlenir ve size özel teslimatla en kısa sürede elinize ulaşır.
Physics of the Merging Clusters Cygnus A, A3667, and A2065
Creators: name: Markevitch, M.
name: Sarazin, C. L.
name: Vikhlinin, A.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present ASCA gas temperature maps of the nearby merging galaxy clusters Cygnus A, A3667, and A2065. Cygnus A appears to have a particularly simple merger geometry that allows an estimate of the subcluster collision velocity from the observed temperature variations. We estimate it to be ~2000 km/s. Interestingly, this is similar to the free-fall velocity that the two Cygnus A subclusters should have achieved at the observed separation, suggesting that merger has been effective in dissipating the kinetic energy of gas halos into thermal energy, without channeling its major fraction elsewhere (e.g., into turbulence). In A3667, we may be observing a spatial lag between the shock front seen in the X-ray image and the corresponding rise of the electron temperature. A lag of the order of hundreds of kiloparsecs is possible due to the combination of thermal conduction and a finite electron-ion equilibration time. Forthcoming better spatial resolution data will allow a direct measurement of these phenomena using such lags. A2065 has gas density peaks coincident with two central galaxies. A merger with the collision velocity estimated from the temperature map should have swept away such peaks if the subcluster total mass distributions had flat cores in the centers. The fact that the peaks have survived (or quickly reemerged) suggests that the gravitational potential also is strongly peaked. Finally, the observed specific entropy variations in A3667 and Cygnus A indicate that energy injection from a single major merger may be of the order of the full thermal energy of the gas. We hope that these order of magnitude estimates will encourage further work on hydrodynamic simulations, as well as more quantitative representation of the simulation results.
description: Corrected the Cyg-A figure (errors shown were 1-sigma not 90%); text unchanged. ApJ in press. Latex, 5 pages, 3 figures (2 color), uses emulateapj.sty
The Mixtures and the Neural Critics: On the Pointwise Mutual Information Profiles of Fine Distributions
Creators: name: Czyż, Paweł
name: Grabowski, Frederic
name: Vogt, Julia E.
name: Beerenwinkel, Niko
name: Marx, Alexander
Publisher: name: ETH Zurich
Year: 2023
Subjects: Machine Learning (stat.ML)
Information Theory (cs.IT)
Machine Learning (cs.LG)
FOS: Computer and information sciences

description: Mutual information quantifies the dependence between two random variables and remains invariant under diffeomorphisms. In this paper, we explore the pointwise mutual information profile, an extension of mutual information that maintains this invariance. We analytically describe the profiles of multivariate normal distributions and introduce the family of fine distributions, for which the profile can be accurately approximated using Monte Carlo methods. We then show how fine distributions can be used to study the limitations of existing mutual information estimators, investigate the behavior of neural critics used in variational estimators, and understand the effect of experimental outliers on mutual information estimation. Finally, we show how fine distributions can be used to obtain model-based Bayesian estimates of mutual information, suitable for problems with available domain expertise in which uncertainty quantification is necessary.
description: arXiv
Cardiopulmonary resuscitation quality parameters from motion capture data using Differential Evolution fitting of sinusoids
Creators: name: Lins, Christian
name: Eckhoff, Daniel
name: Klausen, Andreas
name: Hellmers, Sandra
name: Hein, Andreas
name: Fudickar, Sebastian
Publisher: name: arXiv
Year: 2018
Subjects: subject: Neural and Evolutionary Computing (cs.NE)
subject: FOS: Computer and information sciences

description: Cardiopulmonary resuscitation (CPR) is alongside electrical defibrillation the most crucial countermeasure for sudden cardiac arrest, which affects thousands of individuals every year. In this paper, we present a novel approach including sinusoid models that use skeletal motion data from an RGB-D (Kinect) sensor and the Differential Evolution (DE) optimization algorithm to dynamically fit sinusoidal curves to derive frequency and depth parameters for cardiopulmonary resuscitation training. It is intended to be part of a robust and easy-to-use feedback system for CPR training, allowing its use for unsupervised training. The accuracy of this DE-based approach is evaluated in comparison with data of 28 participants recorded by a state-of-the-art training mannequin. We optimized the DE algorithm hyperparameters and showed that with these optimized parameters the frequency of the CPR is recognized with a median error of $\pm 2.9$ compressions per minute compared to the reference training mannequin.
description: Final paper, 22 pages
Observation of plaid-like spin splitting in a noncoplanar antiferromagnet
Creators: name: Zhu, Yu-Peng
name: Chen, Xiaobing
name: Liu, Xiang-Rui
name: Liu, Yuntian
name: Liu, Pengfei
name: Zha, Heming
name: Qu, Gexing
name: Hong, Caiyun
name: Li, Jiayu
name: Jiang, Zhicheng
name: Ma, Xiao-Ming
name: Hao, Yu-Jie
name: Zhu, Ming-Yuan
name: Liu, Wenjing
name: Zeng, Meng
name: Jayaram, Sreehari
name: Lenger, Malik
name: Ding, Jianyang
name: Mo, Shu
name: Tanaka, Kiyohisa
name: Arita, Masashi
name: Liu, Zhengtai
name: Ye, Mao
name: Shen, Dawei
name: Wrachtrup, Jörg
name: Huang, Yaobo
name: He, Rui-Hua
name: Qiao, Shan
name: Liu, Qihang
name: Liu, Chang
Publisher: name: arXiv
Year: 2023
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Spatial, momentum and energy separation of electronic spins in condensed matter systems guides the development of novel devices where spin-polarized current is generated and manipulated. Recent attention on a set of previously overlooked symmetry operations in magnetic materials leads to the emergence of a new type of spin splitting, enabling giant and momentum-dependent spin polarization of energy bands on selected antiferromagnets. Despite the ever-growing theoretical predictions, the direct spectroscopic proof of such spin splitting is still lacking. Here, we provide solid spectroscopic and computational evidence for the existence of such materials. In the noncoplanar antiferromagnet MnTe$_2$, the in-plane components of spin are found to be antisymmetric about the high-symmetry planes of the Brillouin zone, comprising a plaid-like spin texture in the antiferromagnetic (AFM) ground state. Such an unconventional spin pattern, further found to diminish at the high-temperature paramagnetic state, stems from the intrinsic AFM order instead of spin-orbit coupling (SOC). Our finding demonstrates a new type of quadratic spin texture induced by time-reversal breaking, placing AFM spintronics on a firm basis and paving the way for studying exotic quantum phenomena in related materials.
description: Version 3, 49 pages, 4 main figures, 13 extended data figures and 2 extended data tables. Nature in press (2024)
Emberiza psittacea Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Aves
Passeriformes
Emberizidae
Emberiza
Emberiza psittacea

description: Emberiza psittacea [spec. nov.]
E. cinereo-fusca, alis fulvis, rectricibus duabus longissimis.
Fringilla brasiliensis. Seb. mus. 1 p. 103. t. 66. f. 5.
Habitat in America australi.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 178, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
The FLOODLABEL as a social innovation in flood risk management to increase homeowners' resilience
Creators: name: Meyer, Helene
name: Hartmann, Thomas
Publisher: name: TU Dortmund
Year: 2023
Subjects: subject: flood prevention
subject: flood risk management
subject: resilience
subject: self-precaution
subject: social innovation
subject: 710

description: In flood risk management awareness has been growing that the responsibility for coping with a flood cannot be assumed by the government alone. Homeowners need to be actively involved in flood risk management by taking responsibility; for this, they need empowerment and support to take adequate precautions. If homeowners implement precautionary measures, they can mitigate damage caused by floods and thus increase their resilience. This requires an appropriate risk communication strategy with the population. The FLOODLABEL in Germany informs and prompts homeowners to take precautionary measures. The Flood Competence Center developed the FLOODLABEL. This study employs the analytical framework of social innovation as the FLOODLABEL has some characteristics of social innovation. This study first explores the FLOODLABEL, which constitutes social innovation in flood risk management, and therefore characterizes the five development phases and their successes and challenges as social innovation. Second, it tries to understand and reflect upon the current stage of the FLOODLABEL as a social innovation in Germany and seeks to learn from this tool about the potential drivers associated with the process of implementation. Third, there is potential to gather a better understanding of other social innovations in flood risk management.
description: Journal of flood risk management;