cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Quark-Gluon-Plasma Formation at SPS Energies?
Creators: name: Werner, K.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Nuclear Theory (nucl-th)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: By colliding ultrarelativistic ions, one achieves presently energy densities close to the critical value, concerning the formation of a quark-gluon-plasma. This indicates the importance of fluctuations and the necessity to go beyond the investigation of average events. Therefore, we introduce a percolation approach to model the final stage ($τ> 1$ fm/c) of ion-ion collisions, the initial stage being treated by well-established methods, based on strings and Pomerons. The percolation approach amounts to finding high density domains, and treating them as quark-matter droplets. In this way, we have a {\bf realistic, microscopic, and Monte--Carlo based model which allows for the formation of quark matter.} We find that even at SPS energies large quark-matter droplets are formed -- at a low rate though. In other words: large quark-matter droplets are formed due to geometrical fluctuation, but not in the average event.
description: 7 Pages, HD-TVP-94-6 (1 uuencoded figure)
A quantitative discounted central limit theorem using the Fourier metric
Creators: name: Katriel, Guy
Publisher: name: arXiv
Year: 2018
Subjects: subject: Probability (math.PR)
subject: FOS: Mathematics

description: The discounted central limit theorem concerns the convergence of an infinite discounted sum of i.i.d. random variables to normality as the discount factor approaches $1$. We show that, using the Fourier metric on probability distributions, one can obtain the discounted central limit theorem, as well as a quantitative version of it, in a simple and natural way, and under weak assumptions.
Radio Constraints on the Identifications and Redshifts of Submm Galaxies
Creators: name: Smail, Ian
name: Ivison, R. J.
name: Owen, F. N.
name: Blain, A. W.
name: Kneib, J. -P.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present deep radio maps from the Very Large Array (VLA) for 16 sources detected in a sub-millimeter (submm) survey of the distant Universe. Our deep VLA 1.4-GHz maps allow us to identify radio counterparts or place stringent limits (<20uJy in the source plane) on the radio flux of the submm sources. We compare the spectral indices of our sources between 850um and 1.4GHz to empirical and theoretical models for distant starburst galaxies and active galactic nuclei (AGN) as a function of redshift. In this way we can derive redshift limits for the submm sources, even in the absence of an optical or near-infrared counterpart. We conclude that the submm population brighter than \~1mJy has a median redshift of at least ~2, more probably ~2.5-3, with almost all galaxies at z>>1. This estimate is a strong lower limit as both misidentification of the radio counterparts and non-thermal emission from an AGN will bias our redshift estimates to lower values. The high median redshift means that the submm population, if predominately powered by starbursts, contributes a substantial fraction of the total star formation density at high redshifts. A comparison of the spectral index limits with spectroscopic redshifts for proposed optical counterparts to individual submm galaxies suggests that half of the submm sources remain unidentified and thus their counterparts must be fainter than I>24.
description: In press at ApJ, 4 pages, LaTeX, 2 figures, uses emulateapj.sty
Archetypal Analysis for Sparse Representation-based Hyperspectral Sub-pixel Quantification
Creators: name: Drees, Lukas
name: Roscher, Ribana
name: Wenzel, Susanne
Publisher: name: arXiv
Year: 2018
Subjects: subject: Computer Vision and Pattern Recognition (cs.CV)
subject: FOS: Computer and information sciences

description: The estimation of land cover fractions from remote sensing images is a frequently used indicator of the environmental quality. This paper focuses on the quantification of land cover fractions in an urban area of Berlin, Germany, using simulated hyperspectral EnMAP data with a spatial resolution of 30m$\times$30m. We use constrained sparse representation, where each pixel with unknown surface characteristics is expressed by a weighted linear combination of elementary spectra with known land cover class. We automatically determine the elementary spectra from image reference data using archetypal analysis by simplex volume maximization, and combine it with reversible jump Markov chain Monte Carlo method. In our experiments, the estimation of the automatically derived elementary spectra is compared to the estimation obtained by a manually designed spectral library by means of reconstruction error, mean absolute error of the fraction estimates, sum of fractions, $R^2$, and the number of used elementary spectra. The experiments show that a collection of archetypes can be an adequate and efficient alternative to the manually designed spectral library with respect to the mentioned criteria.
Pinna rudis Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Bivalvia
Pterioida
Pinnidae
Pinna
Pinna rudis

description: Pinna rudis [spec. nov.]
P. testa sulcata: squamis fornicatis per series digestis.
Rumph. mus. t. 46. f. L. Pinna lata.
Argenv. conch. t. 25. f. F. Perna.
Habitat in O. Meridionali, Mediterraneo.
Testa rudior cornei coloris, longitudinaliter grosse sulcata s. rugosa 5 ad 8 julcis, nec alba tenuissimis numerosissimisque striis P. nobilis.
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 707, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Genome-wide identification of the SWEET gene family in Phaseolus vulgaris L. and their patterns of expression under abiotic stress
Creators: name: Du, Yanli
name: Li, Weijia
name: Geng, Jing
name: Li, Siqi
name: Zhang, Wenjing
name: Liu, Xianxian
name: Hu, Minghui
name: Zhang, Zhaoning
name: Fan, Yaru
name: Yuan, Xiankai
name: Du, Jidao
name: Zhao, Qiang
Publisher: name: Taylor & Francis
Year: 2022
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Environmental Sciences not elsewhere classified
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Plant Biology

description: Sugar Will Eventually be Exported Transporters (SWEET) proteins function as sugar transporters that play key roles in plant growth, development, and biotic and abiotic stress responses. However, little is known about the SWEET gene family in common bean (Phaseolus vulgaris L.). In this study, 24 putative PvSWEET genes were identified. They can be categorized into four subgroups based on a phylogenetic analysis, exon–intron structure, cis-regulatory elements, and MEME motifs. A collinearity analysis showed that three pairs of segmental duplicated events were identified. The Phytozome database showed that 16 PvSWEET genes were highly expressed in reproductive organs. PvSWEET5 was expressed the most highly in all the tissues tested, while PvSWEET8/9/10/13 were undetectable in the datasets. The results of qRT-PCR analysis showed that PvSWEET24 was significantly up-regulated following treatment with NaCl, CdCl2, and HgCl2, whereas the PvSWEET5 and PvSWEET20 genes displayed a specific negative response to CdCl2 stress. Collectively, this study provides comprehensive information for the role of SWEET gene family in common bean and lays a solid foundation to elucidate the biological function of the PvSWEET gene family, as well as provide insights into the correlation between the PvSWEET genes and responses to metal stresses.
The Balian-Brézin Method in Relativistic Quantum Mechanics
Creators: name: Jean, H. -C.
name: Payne, G. L.
name: Polyzou, W. N.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Nuclear Theory (nucl-th)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The method suggested by Balian and Brézin for treating angular momentum reduction in the Faddeev equations is shown to be applicable to the relativistic three-body problem.
description: 14 pages in LaTeX
On localizing and concentrating electromagnetic fields
Creators: name: Harrach, Bastian
name: Lin, Yi-Hsuan
name: Liu, Hongyu
Publisher: name: arXiv
Year: 2018
Subjects: subject: Analysis of PDEs (math.AP)
subject: FOS: Mathematics

description: We consider field localizing and concentration of electromagnetic waves governed by the time-harmonic anisotropic Maxwell system in a bounded domain. It is shown that there always exist certain boundary inputs which can generate electromagnetic fields with energy localized/concentrated in a given subdomain while nearly vanishing in another given subdomain. The theoretical results may have potential applications in telecommunication, inductive charging and medical therapy. We also derive a related Runge approximation result for the time-harmonic anisotropic Maxwell system with partial boundary data.
Pinna nobilis Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Bivalvia
Pterioida
Pinnidae
Pinna
Pinna nobilis

description: Pinna nobilis [spec. nov.]
P. testa striata: squamis canaliculato tubulosis subimbricatis.
Bonan. recr. 2. f. 24.
Argenv. conch. t. 25. f. B.
Habitat in M. Mediterraneo.
Varietates potius quam distinctae species sunt sex priores hujus generis.
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 707, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
title: Investigation of Complex Formation by Oligomers of Cytosine and Guanosine
Creators: name: Davis, Steven Roberts
Publisher: name: Old Dominion University
publisherIdentifier: https://ror.org/04zjtrb98
publisherIdentifierScheme: ROR
Year: 1987

description: Duplex formation between oligo(C:G) n where n=3 to 4 was shown not to occur under conditions favorable for duplex formation between poly G and poly C. Instead, a stable guano sine self-structure was found to form which a Tm of 50°C for (Gp)3 and 80°C for (Gp)4 at strand concentrations of 10-5M in 1M NaCl. Neither a duplex nor a self-structure formed in the absence of salt.

Oligomers of guanosine and cytosine were obtained by basic hydrolysis and separated according to chain length using DEAE Sephadex column chromatography. Separation of cytosine oligomers with chain lengths up to eight bases and oligomers of guanosine up to four bases was achieved. A brown oxidation product formed during the hydrolysis of poly G but did not occur when the reaction solutions were purged with He prior to hydrolysis.
Combinatorial and algebraic perspectives on the marginal independence structure of Bayesian networks
Creators: name: Deligeorgaki, Danai
name: Markham, Alex
name: Misra, Pratik
name: Solus, Liam
Publisher: name: arXiv
Year: 2022
Subjects: subject: Methodology (stat.ME)
subject: Algebraic Geometry (math.AG)
subject: Combinatorics (math.CO)
subject: Statistics Theory (math.ST)
subject: Machine Learning (stat.ML)
subject: FOS: Computer and information sciences
subject: FOS: Mathematics
subject: 62R01, 62H22, 60J22, 13F65, 62D20, 05C75

description: We consider the problem of estimating the marginal independence structure of a Bayesian network from observational data, learning an undirected graph we call the unconditional dependence graph. We show that unconditional dependence graphs of Bayesian networks correspond to the graphs having equal independence and intersection numbers. Using this observation, a Gröbner basis for a toric ideal associated to unconditional dependence graphs of Bayesian networks is given and then extended by additional binomial relations to connect the space of all such graphs. An MCMC method, called GrUES (Gröbner-based Unconditional Equivalence Search), is implemented based on the resulting moves and applied to synthetic Gaussian data. GrUES recovers the true marginal independence structure via a penalized maximum likelihood or MAP estimate at a higher rate than simple independence tests while also yielding an estimate of the posterior, for which the $20\%$ HPD credible sets include the true structure at a high rate for data-generating graphs with density at least $0.5$.
description: 54 pages, 13 figures, 3 tables
The Origin of Recombining Plasma and the Detection of the Fe-K Line in the Supernova Remnant W28
Creators: name: Okon, Hiromichi
name: Uchida, Hiroyuki
name: Tanaka, Takaaki
name: Matsumura, Hideaki
name: Tsuru, Takeshi Go
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Overionized recombining plasmas (RPs) have been discovered from a dozen of mixed- morphology (MM) supernova remnants (SNRs). However their formation process is still under debate. As pointed out by many previous studies, spatial variations of plasma temperature and ionization state provide clues to understand the physical origin of RPs. We report on a spatially resolved X-ray spectroscopy of W28, which is one of the largest MM SNRs found in our Galaxy. Two observations with Suzaku XIS cover the center of W28 to the northeastern rim where the shock is interacting with molecular clouds. The X-ray spectra in the inner regions are well reproduced by a combination of two-RP model with different temperatures and ionization states, whereas that in northeastern rim is explained with a single-RP model. Our discovery of the RP in the northeastern rim suggests an effect of thermal conduction between the cloud and hot plasma, which may be the production process of the RP. The X-ray spectrum of the north- eastern rim also shows an excess emission of the Fe I Kα line. The most probable process to explain the line would be inner shell ionization of Fe in the molecular cloud by cosmic-ray particles accelerated in W28.
description: 9 page, 6 figures, 4 tables, accepted in PASJ on February 8, 2018
Additional file 1 of Development and validation of a distributed representation model of Japanese high-dimensional administrative claims data for clinical epidemiology studies
Creators: name: Matsui, Hiroki
name: Fushimi, Kiyohide
name: Yasunaga, Hideo
Publisher: name: figshare
Year: 2025
Subjects: Medicine
Biotechnology
Biological Sciences not elsewhere classified
Information Systems not elsewhere classified
Mathematical Sciences not elsewhere classified
Hematology

description: Supplementary Material 1.
Comparison of 2D and 3D models of flow structure in semidetached binaries
Creators: name: Bisikalo, D. V.
name: Boyarchuk, A. A.
name: Chechetkin, V. M.
name: Kuznetsov, O. A.
name: Molteni, D.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present the results of systematic comparison of 2D and 3D numerical models of mass transfer in semidetached binaries. It is shown that only for case of γ\sim 1 (near-isothermal case) the obtained 2D and 3D solutions are qualitatively similar. For higher value of γthe 3D flow structure is drastically changed and for γ=1.2 the accretion disk is not formed in the system. Numerical results show that for case of γ=1.2 the 2D and 3D solutions are different. We discuss the spiral-shaped shock waves obtained in numerical models. It is shown that these shocks are not intrinsic spirals and are caused by collisions of the gaseous flows in the system.
description: LaTeX, 18 pages, 11 eps-figures, Astron. Reports, in press
Mytilus ruber Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Bivalvia
Mytiloida
Mytilidae
Mytilus
Mytilus ruber

description: Mytilus ruber [spec. nov.]
M. testa rugosa, valvulis obliquis postice dilatatis, margine cardinali apicem aequante.
Argenv. conch. t. 25. f. Q?
Habitat in O. australiore.
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 706, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
A gas-rich nuclear bar fuelling a powerful central starburst in NGC 2782
Creators: name: Jogee, Shardha
name: Kenney, Jeffrey D. P.
name: Smith, Beverly J.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present evidence that the peculiar interacting starburst galaxy NGC 2782 (Arp 215) harbors a gas-rich nuclear stellar bar feeding an M82-class powerful central starburst, from a study based on OVRO CO (J=1->0) data, WIYN BVR & Halpha observations, along with available NIR images, a 5 GHz RC map and HST images. NGC 2782 harbors a clumpy, bar-like CO feature of radius ~ 7.5'' (1.3 kpc) which leads a nuclear stellar bar of similar size. The nuclear CO bar is massive: it contains ~2.5x10**9 M_sun of molecular gas, which makes up ~ 8 % of the dynamical'mass present within a 1.3 kpc radius. Within the CO bar, emission peaks in two extended clumpy lobes which lie on opposite sides of the nucleus, separated by ~ 6'' (1 kpc). Between the CO lobes, in the inner 200 pc radius, resides a powerful central starburst which is forming stars at a rate of 3 to 6 M_sun yr-1. While circular motions dominate the CO velocity field, the CO lobes show weak bar-like streaming motions on the leading side of the nuclear stellar bar, suggestive of gas inflow. We estimate semi-analytically the gravitational torque from the nuclear stellar bar on the gas, and suggest large gas inflow rates from the CO lobes into the central starburst. These observations, which are amongst the first ones showing a nuclear stellar bar fuelling molecular gas into an intense central starburst, are consistent with simulations and theory which suggest that nuclear bars provide an efficient way of transporting gas closer to the galactic center to fuel central activity. Furthermore, several massive clumps are present at low radii, and dynamical friction might produce further gas inflow. We suggest that the nuclear molecular gas bas and central activity will be very short-lived, likely disappearing within 5x10**8 years.
description: Accepted by the Astrophysical Journal, 10 pages, Latex with emulateapj.sty, apjfonts.sty, 10 postscript & 2 gif figures
Additional file 1: of Factors affecting interspecific differences in genetic divergence among populations of Anolis lizards in Cuba
Creators: name: Cádiz, Antonio
name: Nagata, Nobuaki
name: Díaz, Luis
name: Suzuki-Ohno, Yukari
name: Lázaro Echenique-Díaz
name: Akashi, Hiroshi
name: Makino, Takashi
name: Masakado Kawata
Publisher: name: figshare
Year: 2018
Subjects: subject: Genetics
subject: FOS: Biological sciences
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: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: Inorganic Chemistry
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology

description: Table S1. (a) Location data and GenBank accession numbers of the Cuban specimens used in this study. (b) Regional sampling data. Table S2. GenBank sequence accession numbers of the non-Cuban specimens used in this study. Table S3. Description of Unique Type in Cuba Anoles. Table S4. Environmental variables for each locality. Table S5. Results of a phylogenetic generalized least squares (PGLS) analysis for the final model using both nuclear DNA (nDNA) and mitochondrial DNA (mtDNA) (a) and only mtDNA (b). (DOC 627 kb)
Threshold Two-Pion Photo- and Electroproduction: More neutrals than expected
Creators: name: Bernard, V.
name: Kaiser, N.
name: Meißner, Ulf-G.
name: Schmidt, A.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Nuclear Theory (nucl-th)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We present an exploratory study of two pion photo-- and electroproduction off the nucleon in the threshold region. To calculate the pertinent amplitudes, we make use of heavy baryon chiral perturbation theory. We show that due to finite chiral loops the production cross section for final states with two neutral pions is considerably enhanced. The experimental implications are briefly discussed.
description: 23pp, plain TeX, 11 figures available upon request, CRN 94/14
Static density response of one-dimensional soft bosons across the clustering transition
Creators: name: Teruzzi, Martina
name: Pini, Davide
name: Rossotti, Stefano
name: Galli, Davide Emilio
name: Bertaina, Gianluca
Publisher: name: arXiv
Year: 2018
Subjects: subject: Quantum Gases (cond-mat.quant-gas)
subject: FOS: Physical sciences

description: One-dimensional bosons interacting via a soft-shoulder potential are investigated at zero temperature. The flatness of the potential at short distances introduces a typical length, such that, at relatively high densities and sufficiently strong interactions, clusters are formed, even in the presence of a completely repulsive potential. We evaluate the static density response function of this system across the transition from the liquid to the cluster liquid phases. Such quantity reveals the density modulations induced by a weak periodic external potential, and is maximal at the clustering wavevector. It is known that this response function is proportional to the static structure factor in the classical regime at high temperature, while for this zero-temperature quantum systems, we extract it from the dynamical structure factor evaluated with quantum Monte Carlo methods.
description: 7 pages, 3 figures. Proceedings of the "Recent Progress in Many-Body Theories" international conference, Pohang, South Korea, 2017
Provably Convergent Plug & Play Linearized ADMM, applied to Deblurring Spatially Varying Kernels
Creators: name: Laroche, Charles
name: Almansa, Andrés
name: Coupeté, Eva
name: Tassano, Matias
Publisher: name: arXiv
Year: 2022
Subjects: subject: Computer Vision and Pattern Recognition (cs.CV)
subject: Optimization and Control (math.OC)
subject: Applications (stat.AP)
subject: FOS: Computer and information sciences
subject: FOS: Mathematics

description: Plug & Play methods combine proximal algorithms with denoiser priors to solve inverse problems. These methods rely on the computability of the proximal operator of the data fidelity term. In this paper, we propose a Plug & Play framework based on linearized ADMM that allows us to bypass the computation of intractable proximal operators. We demonstrate the convergence of the algorithm and provide results on restoration tasks such as super-resolution and deblurring with non-uniform blur.
Fine structure of the red clump in Local Group galaxies
Creators: name: Girardi, Leo
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Some fine structures can nowadays be identified in the high-quality colour-magnitude diagrams (CMD) of Local Group galaxies. The clump of red giants, for instance, may present a significant colour spread, and extensions to both brighter and fainter luminosities. Such features are predicted by population synthesis models which consider stars in the complete relevant ranges of ages and metallicities, and are potentially useful for constraining the star formation histories of the parent galaxies over scales of gigayears. We briefly comment the cases of fields in the Magellanic Clouds, M31, and the local CMD from Hipparcos.
description: To appear in Proc. of the VLT Opening Symposium (Parallel Workshop 2: Star-Way to the Universe)
A Black-Hole Excision Scheme for General Relativistic Core-Collapse Supernova Simulations
Creators: name: Sykes, B.
name: Mueller, B.
name: Cordero-Carrión, I.
name: Cerdá-Durán, P.
name: Novak, J.
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: Fallback supernovae and the collapsar scenario for long-gamma ray burst and hypernovae have received considerable interest as pathways to black-hole formation and extreme transient events. Consistent simulations of these scenarios require a general relativistic treatment and need to deal appropriately with the formation of a singularity. Free evolution schemes for the Einstein equations can handle the formation of black holes by means of excision or puncture schemes. However, in constrained schemes, which offer distinct advantages in long-term numerical stability in stellar collapse simulations over well above $10^{4}$ light-crossing time scales, the dynamical treatment of black-hole spacetimes is more challenging. Building on previous work on excision in conformally flat spacetimes, we here present the implementation of a black-hole excision scheme for supernova simulations with the CoCoNuT-FMT neutrino transport code. We describe in detail a choice of boundary conditions that ensures long-time numerical stability, and also address upgrades to the hydrodynamics solver that are required to stably evolve the relativistic accretion flow onto the black hole. The scheme is currently limited to a spherically symmetric metric, but the hydrodynamics can be treated multi-dimensionally. For demonstration, we present a spherically symmetric simulation of black-hole formation in an $85 M_\odot$ star, as well as a two-dimensional simulation of the fallback explosion of the same progenitor. These extend past 9s and 0.3s after black-hole formation, respectively.
description: 19 pages, 12 figures. Accepted by PRD. Updated to correct typographical error in funding acknowledgements
Exotic Magnetism and Spin-Orbit Assisted Mott Insulating State in a $3d-5d$ Double Perovskite
Creators: name: Cavichini, A. S.
name: Orlando, M. T.
name: Depianti, J. B.
name: Passamai, J. L.
name: Damay, F.
name: Porcher, F.
name: Granado, E.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: The magnetic structure of Ca$_2$MnReO$_6$ double perovskite is investigated by neutron powder diffraction and bulk magnetization, showing dominant non-collinear Mn magnetic moments [$4.35(7)$ $μ_B$] that are orthogonally aligned with the small Re moments [$0.22(4)$ $μ_B$]. $Ab$-initio electronic structure calculations show that the strong spin-orbit coupling for Re $5d$ electrons combined with a relatively modest on-site Coulomb repulsion ($U_{eff}^{Re} \gtrsim 0.6$ eV) is sufficient to render this material insulating. This is a rare example of spin-orbit assisted Mott insulator outside the realm of iridates, with remarkable magnetic properties.
description: 7 pages, 5 figures, 2 tables
Complex cyanides as chemical clocks in hot cores
Creators: name: Allen, V.
name: van der Tak, F. F. S.
name: Walsh, C.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: In the high-mass star-forming region G35.20-0.74N, small scale (about 800 AU) chemical segregation has been observed in which complex organic molecules containing the CN group are located in a small location. We aim to determine the physical origin of the large abundance difference (about 4 orders of magnitude) in complex cyanides within G35.20-0.74 B, and we explore variations in age, gas and dust temperature, and gas density. We performed gas-grain astrochemical modeling experiments with exponentially increasing (coupled) gas and dust temperature rising from 10 to 500 K at constant H$_2$ densities of 10$^7$, 10$^8$, and 10$^9$ cm$^{-3}$. We tested the effect of varying the initial ice composition, cosmic-ray ionization rate, warm-up time (over 50, 200, and 1000 kyr), and initial (10, 15, and 25 K) and final temperatures (300 and 500 K). Varying the initial ice compositions within the observed and expected ranges does not noticeably affect the modeled abundances indicating that the chemical make-up of hot cores is determined in the warm-up stage. Complex cyanides vinyl and ethyl cyanide (CH$_2$CHCN and C$_2$H$_5$CN, respectively) cannot be produced in abundances (versus H$_2$) greater than 5x10$^{-10}$ for CH$_2$CHCN and 2x10$^{-10}$ for C$_2$H$_5$CN with a fast warm-up time (52 kyr), while the lower limit for the observed abundance of C$_2$H$_5$CN toward source B3 is 3.4x10$^{-10}$. Complex cyanide abundances are reduced at higher initial temperatures and increased at higher cosmic-ray ionization rates. Reproducing the observed abundances toward G35.20-0.74 Core B3 requires a fast warm-up at a high cosmic-ray ionization rate (1x10$^{-16}$ s$^{-1}$) at a high gas density (>10$^9$ cm$^{-3}$). G35.20-0.74 source B3 only needs to be about 2000 years older than B1/B2 for the observed chemical difference to be present. (This abstract has been shortened)
description: 14 pages (plus 11 pages appendices), 12 figures main text
Additional file 1 of Effects of moving cupping therapy for plaque psoriasis: study protocol for a randomized multicenter clinical trial
Creators: name: Xing, Meng
name: Yan, Xiaoning
name: Yang, Suqing
name: Li, Linge
name: Gong, Liping
name: Liu, Hongxia
name: Xu, Rong
name: Chen, Jie
name: Ying, Luo
name: Zhao, Yiding
name: An, Yuepeng
name: Liu, Yang
name: Huang, Gang
name: Guo, Fei
name: Yin, Qingfeng
name: Wang, Ruiping
name: Li, Bin
name: Li, Xin
Publisher: name: figshare
Year: 2020
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Information Systems not elsewhere classified
subject: Mathematical Sciences not elsewhere classified
subject: Developmental Biology
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Additional file 1. SPIRIT 2013 Checklist.
Additional file 8: of A mathematical model of CO2, O2 and N2 exchange during venovenous extracorporeal membrane oxygenation
Creators: name: Joyce, Christopher
name: Shekar, Kiran
name: Cook, David
Publisher: name: figshare
Year: 2018
Subjects: subject: Molecular Biology
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Developmental Biology

description: Figure S5. Shows the “Effect of FOXYO2 on PaCO2”. (PDF 76 kb)
Mesons and the Structure of Nucleons
Creators: name: Koepf, W.
name: Henley, E. M.
name: Alberg, M.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Nuclear Theory (nucl-th)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The role of mesons, particularly the pion, in the structure of nucleons is reviewed and investigated. Since quark-antiquark pairs are likely to ``transform" into mesons at large distances, mesons are expected to contribute to nucleon structure. Their effects on the Gottfried sum rule, on the strangeness content of the nucleon, and on the spin of the nucleon are discussed.
description: 15 pages, TeX file followed by 3 uuencoded PostScript figures (optional), DOE/ER/40427-08-N94
MOESM1 of Small size fullerenol nanoparticles suppress lung metastasis of breast cancer cell by disrupting actin dynamics
Creators: name: Qin, Yanxia
name: Chen, Kui
name: Gu, Weihong
name: Dong, Xinghua
name: Lei, Ruihong
name: Chang, Yanan
name: Bai, Xue
name: Xia, Shibo
name: Zeng, Li
name: Zhang, Jiaxin
name: Ma, Sihan
name: Li, Juan
name: Li, Shan
name: Xing, Gengmei
Publisher: name: figshare
Year: 2018
Subjects: subject: Biophysics
subject: Space Science
subject: Medicine
subject: Cell Biology
subject: Molecular Biology
subject: Pharmacology
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer
subject: Plant Biology
subject: FOS: Biological sciences

description: Additional file 1. Additional figures.
Implementation of a geometrically and energetically constrained mesoscale eddy parameterization in an ocean circulation model
Creators: name: Mak, Julian
name: Maddison, James R.
name: Marshall, David P.
name: Munday, David R.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Atmospheric and Oceanic Physics (physics.ao-ph)
subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: The global stratification and circulation of the ocean and their sensitivities to changes in forcing depend crucially on the representation of the mesoscale eddy field. Here, a geometrically informed and energetically constrained parameterization framework for mesoscale eddies --- termed GEOMETRIC --- is proposed and implemented in three-dimensional primitive equation channel and sector models. The GEOMETRIC framework closes mesoscale eddy fluxes according to the standard Gent--McWilliams scheme, but with the eddy transfer coefficient constrained by the depth-integrated eddy energy field, provided through a prognostic eddy energy budget evolving with the mean state. It is found that coarse resolution calculations employing GEOMETRIC broadly reproduce model sensitivities of the eddy permitting reference calculations in the emergent circumpolar transport, meridional overturning circulation profile and the depth-integrated eddy energy signature; in particular, eddy saturation emerges in the sector configuration. Some differences arise, attributed here to the simple prognostic eddy energy budget employed, to be improved upon in future investigations. The GEOMETRIC framework thus proposes a shift in paradigm, from a focus on how to close for eddy fluxes, to focusing on the representation of eddy energetics.
description: 19 pages, 9 figures, submitted to Journal of Physical Oceanography; comments welcome. (Copyright statement: see section 7a of https://www.ametsoc.org/ams/index.cfm/publications/ethical-guidelines-and-ams-policies/ams-copyright-policy/)
Modeling Three-dimensional Invasive Solid Tumor Growth in Heterogeneous Microenvironment under Chemotherapy
Creators: name: Xie, Hang
name: Jiao, Yang
name: Fan, Qihui
name: Hai, Miaomiao
name: Yang, Jiaen
name: Hu, Zhijian
name: Yang, Yue
name: Shuai, Jianwei
name: Chen, Guo
name: Liu, Ruchuan
name: Liu, Liyu
Publisher: name: arXiv
Year: 2018
Subjects: subject: Tissues and Organs (q-bio.TO)
subject: Populations and Evolution (q-bio.PE)
subject: FOS: Biological sciences

description: A systematic understanding of the evolution and growth dynamics of invasive solid tumors in response to different chemotherapy strategies is crucial for the development of individually optimized oncotherapy. Here, we develop a hybrid three-dimensional (3D) computational model that integrates pharmacokinetic model, continuum diffusion-reaction model and discrete cell automaton model to investigate 3D invasive solid tumor growth in heterogeneous microenvironment under chemotherapy. Specifically, we consider the effects of heterogeneous environment on drug diffusion, tumor growth, invasion and the drug-tumor interaction on individual cell level. We employ the hybrid model to investigate the evolution and growth dynamics of avascular invasive solid tumors under different chemotherapy strategies. Our simulations reproduce the well-established observation that constant dosing is generally more effective in suppressing primary tumor growth than periodic dosing, due to the resulting continuous high drug concentration. In highly heterogeneous microenvironment, the malignancy of the tumor is significantly enhanced, leading to inefficiency of chemotherapies. The effects of geometrically-confined microenvironment and non-uniform drug dosing are also investigated. Our computational model, when supplemented with sufficient clinical data, could eventually lead to the development of efficient in silico tools for prognosis and treatment strategy optimization.
description: 41 pages, 8 figures
title: ADCO, Cartulaire de Cîteaux pour les possessions d’Izeure (XVe siècle), Cart. 178 (11 H 80), 82 folios, f. 0155
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: Petot, Frédéric
name: CG21/F.PETOT/2015
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire

description: Cartulaire de Cîteaux pour les possessions d’Izeure (XVe siècle), Archives départementales de la Côte-d'Or, Cart. 178 (11 H 80), 82 folios, f. 0155, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire de Cîteaux pour les possessions d’Izeure (XVe siècle), Archives départementales de la Côte-d'Or, Cart. 178 (11 H 80), 82 folios, f. 0155, 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
title: Цифровизация в свете этики:  за и против
Creators: name: Волохова, Н.
name: Подгорный, Б.
Publisher: name: Новгородский государственный университет имени Ярослава Мудрого (НовГУ)
Year: 2021

description: Современная мировая ситуация, связанная с пандемией коронавируса, поновому нивелирует отношение человека к привычным аспектам жизни. Это прослеживается абсолютно во всех сферах и говорят об этом представители всех профессий: политики, медики, психологи, философы, экономисты, программисты и пр. Особое место отводится применению цифровых технологий. Цифровизация становится главным условием качественного дистанцирования, одним из главных механизмов борьбы с пандемией. Цель статьи – определить дихотомическую сущность этической составляющей как важнейшей личностной компоненты современного информационного общества, где приоритетное место отдано процессам цифровизации.
Additional file 6: of Lung fluid biomarkers for acute respiratory distress syndrome: a systematic review and meta-analysis
Creators: name: Wang, Yishan
name: Wang, Huijuan
name: Zhang, Chunfang
name: Zhang, Chao
name: Yang, Huqin
name: Gao, Ruiyue
name: Tong, Zhaohui
Publisher: name: figshare
Year: 2019
Subjects: Medicine
Cell Biology
Biological Sciences not elsewhere classified
Science Policy

description: Result of subgroup analysis for diagnosis. (DOCX 14 kb)
Impact of the form of weighted networks on the quantum extreme reservoir computation
Creators: name: Hayashi, Aoi
name: Sakurai, Akitada
name: Nishio, Shin
name: Munro, William J.
name: Nemoto, Kae
Publisher: name: arXiv
Year: 2022
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: The quantum extreme reservoir computation (QERC) is a versatile quantum neural network model that combines the concepts of extreme machine learning with quantum reservoir computation. Key to QERC is the generation of a complex quantum reservoir (feature space) that does not need to be optimized for different problem instances. Originally, a periodically-driven system Hamiltonian dynamics was employed as the quantum feature map. In this work we capture how the quantum feature map is generated as the number of time-steps of the dynamics increases by a method to characterize unitary matrices in the form of weighted networks. Furthermore, to identify the key properties of the feature map that has sufficiently grown, we evaluate it with various weighted network models that could be used for the quantum reservoir in image classification situations. At last, we show how a simple Hamiltonian model based on a disordered discrete time crystal with its simple implementation route provides nearly-optimal performance while removing the necessity of programming of the quantum processor gate by gate.
description: 9 pages, 5 figures
The impact of viscosity on the morphology of gaseous flows in semidetached binary systems
Creators: name: Bisikalo, D. V.
name: Boyarchuk, A. A.
name: Kuznetsov, O. A.
name: Chechetkin, V. M.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Results of 3D gas dynamical simulation of mass transfer in binaries are presented for systems with various values of viscosity. Analysis of obtained solutions shows that in the systems with low value of viscosity the flow structure is qualitatively similar to one for systems with high viscosity. Presented calculations confirm that there is no shock interaction between the stream from L1 and the forming accretion disk (`hot spot') at any value of viscosity.
description: LaTeX, 18 pages, 15 eps-figures, Astron. Reports, in press
Dynamical friction and the evolution of satellites in virialized halos: the theory of linear response
Creators: name: Colpi, Monica
name: Mayer, Lucio
name: Governato, Fabio
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The evolution of a small satellite inside a more massive truncated isothermal spherical halo is studied using both the Theory of Linear Response for dynamical friction and N-Body simulations. The analytical approach includes the effects of the gravitational wake, of the tidal deformation and the shift of the barycenter of the primary, so unifying the local versus global interpretation of dynamical friction. Sizes, masses, orbital energies and eccentricities are chosen as expected in hierarchical clustering models. We find that in general the drag force in self-gravitating backgrounds is weaker than in uniform media and that the orbital decay is not accompanied by a significant circularization. We also show that the dynamical friction time scale is weakly dependent on the initial circularity. We provide a fitting formula for the decay time that includes the effect of mass and angular momentum loss. Live satellites with dense cores can survive disruption up to an Hubble time within the primary, notwithstanding the initial choice of orbital parameters. Dwarf spheroidal satellites of the Milky Way, like Sagittarius A and Fornax, have already suffered mass stripping and, with their present masses, the sinking times exceed 10 Gyr even if they are on very eccentric orbits.
description: 27 pages including 9 figures. Accepted for publication in the Astrophysical Journal. Part 2, issue November 10 1999, Volume 525
The Propagators of Gauge Bosons on a lattice
Creators: name: Preparata, B. G.
name: XUE, She-Sheng
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Lattice (hep-lat)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We analyse the problem of the generation of mass in the gauge boson sector on the (Planck) lattice. We obtain a dynamical scenario quite similar to the popular Higgs-mechanism, with the important difference that no Higgs-type excitation is present in our theory. By fixing the mass of the $Z^\circ$-boson and the renormalized gauge couplings at their experimental values, we get for the top quark mass $m_t\simeq 149$GeV and for the $ρ$-parameter the very small value $ρ\sim 10^{-6}$.
description: to appear in Phys. Lett. 10 pages (TeX) and 1 figure, MITH 93/11
MOESM3 of Hapke-based computational method to enable unmixing of hyperspectral data of common salts
Creators: name: Howari, Fares
name: Gheorge Acbas
name: Nazzal, Yousef
name: AlAydaroos, Fatima
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Medicine
subject: Molecular Biology
subject: Physiology
subject: FOS: Biological sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Inorganic Chemistry

description: Additional file 3. Simulation of reflection spectra for non-intimate linear mixture for comparison.
Gradients of Absorption Line Strengths in Elliptical Galaxies
Creators: name: Kobayashi, Chiaki
name: Arimoto, Nobuo
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have re-studied line-strength gradients of 80 elliptical galaxies. Typical metallicity gradients are d[Fe/H]/dlogr = -0.3. The metallicity gradients do not correlate with any physical properties of galaxies, including central and mean metallicities, central velocity dispersions sigma0, absolute B-magnitudes MB, absolute effective radii Re, and dynamical masses of galaxies. By using the metallicity gradients, we have calculated mean stellar metallicities for individual ellipticals. Typical mean stellar metallicities are = -0.3. The mean metallicities correlate well with sigma0 and dynamical masses, though relations for MB and Re include significant scatters. We find fundamental planes defined by surface brightnesses SBe, , and Re (or MB), and the scatters of which are much smaller than those of the -Re (or MB) relations. The -sigma0 relation is nearly in parallel to the [Fe/H]0- sigma0 relation but systematically lower by 0.3 dex. The metallicity-mass relation, or equivalently, the color-magnitude relation holds not only for the central part but also for the whole part of galaxies. Using Mg2 and Fe1, we find = +0.2 in most of ellipticals. shows no correlation with galaxy mass tracers. This can be most naturally explained if the star formation had stopped in ellipticals before the bulk of Type Ia supernovae began to explode. Ellipticals can have significantly different metallicity gradients and even if they have the same galaxy mass. This may result from galaxy mergers, but no evidence is found from presently available data to support the same origin for metallicity gradients, the scatters around metallicity-mass relation, and dynamical disturbances. This may suggest that the scatters have their origin at the formation epoch of galaxies.
description: 33 pages LaTeX, 18 PostScript figures, Accepted for publication in the Astrophysical Journal
Pinna saccata Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Bivalvia
Pterioida
Pinnidae
Pinna
Pinna saccata

description: Pinna saccata [spec. nov.]
P. testa laevi saccata erectiuscula subfastigiata.
Rumph. mus. t. 46. f. N. Pinna alba.
Gvalt. test. t. 79. f. F.
Habitat in M. Mediterraneo, Indico.
Pinnae neque vita fortasse posset servari a Polypo octopodia, nisi opera Cancri Pinnotheris. Amoen. acad. 2. p. 48.
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 707, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206