cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: Der Einfluss der Fischerei auf Natur, Umwelt und biologische Vielfalt
Creators: name: Arlinghaus, Robert
name: Brinker, Alexander
name: Wolter, Christian
Publisher: name: Zeitschrift für Fischerei
Year: 2020

description: Die Leopoldina Nationale Akademie der Wissenschaften legte im Jahr 2020 eine Analyse zur Biodiversitätskrise in terrestrischen und aquatischen Ökosystemen vor. Die in diesem normativen Bericht getätigten Aussagen zur Rolle und Bedeutung der Fischerei und Aquakultur beim Rückgang der Biodiversität werden in vorliegendem Beitrag einer kritischen Bewertung unterzogen. Im Ergebnis wird konstatiert, dass das Management der globalen Fischerei in den letzten Jahren eine deutliche Verbesserung erfahren hat und dass die Aquakultur vielfach zu den ressourcenschonendsten Erzeugungsmethoden tierischen Proteins gehört. Beide Fischereizweige, Aquakultur und Fischerei, sind wesentlich für die weltweite Lebensmittelversorgung mit tierischem Protein, auch und insbesondere in den Entwicklungsländern. Heute wird die Mehrzahl der genutzten marinen Fischbestände, die 79 % des globalen Fangertrags liefern, nachhaltig bewirtschaftet. Während die Fischerei einen dominierenden Einfluss auf Biomasse und Größenstruktur von marinen Fischpopulationen ausübt, sind in Binnengewässern hingegen weit überwiegend andere Faktoren als die Fischerei als Haupteinflussfaktor auf die Biodiversität anzusehen. Dementsprechend trägt eine veränderte Managementpraxis der Binnenfischerei kaum zum Stopp der Biodiversitätskrise bei, wohingegen die Senkung der Fischereisterblichkeit in übernutzten marinen Fischbeständen Abundanz und Größenstruktur der Fischpopulationen anheben dürfte. Insgesamt hat der Leopoldina-Bericht die Charakterisierung der Fischerei- und Aquakultureffekte und die Möglichkeiten des Fischereimanagements auf die Biodiversität ungenau und zu pessimistisch widergegeben.
description: Zeitschrift für Fischerei, Nr. 1 (2020)
Geochemistry constrains global hydrology on Early Mars
Creators: name: Kite, Edwin S.
name: Daswani, Mohit Melwani
Publisher: name: arXiv
Year: 2019
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Geophysics (physics.geo-ph)
subject: FOS: Physical sciences

description: Ancient hydrology is recorded by sedimentary rocks on Mars. The most voluminous sedimentary rocks that formed during Mars' Hesperian period are sulfate-rich rocks, explored by the $Opportunity$ rover from 2004-2012 and soon to be investigated by the $Curiosity$ rover at Gale crater. A leading hypothesis for the origin of these sulfates is that the cations were derived from evaporation of deep-sourced groundwater, as part of a global circulation of groundwater. Global groundwater circulation would imply sustained warm Earthlike conditions on Early Mars. Global circulation of groundwater including infiltration of water initially in equilibrium with Mars' CO$_2$ atmosphere implies subsurface formation of carbonate. We find that the CO$_2$ sequestration implied by the global groundwater hypothesis for the origin of sulfate-rich rocks on Mars is 30-5000 bars if the $Opportunity$ data are representative of Hesperian sulfate-rich rocks, which is so large that (even accounting for volcanic outgassing) it would bury the atmosphere. This disfavors the hypothesis that the cations for Mars' Hesperian sulfates were derived from upwelling of deep sourced groundwater. If, instead, Hesperian sulfate-rich rocks are approximated as pure Mg-sulfate (no Fe), then the CO$_2$ sequestration is 0.3-400 bars. The low end of this range is consistent with the hypothesis that the cations for Mars' Hesperian sulfates were derived from upwelling of deep sourced groundwater. In both cases, carbon sequestration by global groundwater circulation actively works to terminate surface habitability, rather than being a passive marker of warm Earthlike conditions. $Curiosity$ will soon be in a position to discriminate between these two hypotheses. Our work links Mars sulfate cation composition, carbon isotopes, and climate change.
description: Accepted by Earth & Planetary Science Letters. 5 figures
Additional file 1: of Immature O-glycans recognized by the macrophage glycoreceptor CLEC10A (MGL) are induced by 4-hydroxy-tamoxifen, oxidative stress and DNA-damage in breast cancer cells
Creators: name: Anna-Katharina Kurze
name: Buhs, Sophia
name: Eggert, Dennis
name: Oliveira-Ferrer, Leticia
name: Müller, Volkmar
name: Niendorf, Axel
name: Wagener, Christoph
name: Nollau, Peter
Publisher: name: figshare
Year: 2019
Subjects: subject: Biophysics
subject: Biochemistry
subject: Space Science
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Pharmacology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Cancer
subject: Hematology
subject: Plant Biology
subject: Computational Biology

description: Figure S1. Positivity for CLEC10A ligands correlates with the secretory phase in human endometrium samples. Figure S2. Phagocytosis of CFSE-labelled MCF7cells by macrophages. Figure S3. Zeocin leads to accumulation of CLEC10A ligands in the endosomal/lysosomal pathway and in autophagosomes. Figure S4. Effects of tamoxifen, zeocin and hydrogen peroxide on cell viability of breast cancer cell lines. Figure S5. Scratch assay of 4-hydroxy-tamoxifen-, zeocin- and hydrogen peroxide treated breast cancer cell lines. Figure S6. Independent reproduction of western blots and mRNA expression analysis of mucin 1 (MUC1), COSMC and T-synthase (T-Syn) in MCF7 and T47D cells. Figure S7. Immunofluorescence of GalNT2 and GalNT6 in T47D breast cancer cells. Table S1. Clinico-pathological characteristics of the 146 invasive ductal breast carcinomas. Table S2. Antibodies and the corresponding dilutions used for western blot and immunofluorescence. (PDF 2784 kb)
Benin Agriculture Productivity and profitability Measurement
Creators: name: Constant, Labintan Adeniyi
name: Shijun, Ding
name: Constant, Labintan Adeniyi
name: Shijun, Ding
Publisher: name: Unknown
Year: 2012
Subjects: subject: Productivity Analysis
subject: Agricultural-Productivity- Profitability-Benin-Reform

description: This paper explored the Benin agricultural productivity and profitability under occurred reform since 1961 to 2008. Productivity and profitability has been evaluated using the new approach developed by O’Donnell(2008).In the approach Productivity is obtain using Hick Moorsteen index decomposition into Technical Change, mix Efficiency change and Scale Efficiency Change while Profitability is obtain using productivity and Term of Trade product. To achieved the purpose of this paper, agricultural output-input quantity and prices data have been collected from FAO stat, Benin Country FAO statistical database and Benin National Agricultural Institute Database during the period 1961-2008. All data are computing using the DPIN software developed by O’Donnell (2010). It is found that since the country national independency in 1961, Benin agriculture productivity has decreased. The decreased has been more significant after the sector liberalization while the term of trade has been much improved and profitability increased. This situation explains that after the liberalization, competiveness has decreased and monopolization increased. It can be conclude that most private stakeholder involve in the sector during post liberalization has earn more profit than invest to contribute at the sector productivity growth. The paper indentify that the country doesn’t improved agricultural productivity after the sector liberalization in opposite to the normal figure that liberalization will stimulate technology transfer and development which will improve productivity. The situation will then highlight policies maker to identify news strategy which can help to optimize the production and agriculture resources efficiency.
title: Zeitschrift für Fischerei – Deutschlands erste Open-Access Fachzeitschrift für alle Belange der Fischerei
Creators: name: Arlinghaus, Robert
Publisher: name: Zeitschrift für Fischerei
Year: 2020

description: Die Zeitschrift für Fischerei (Kurztitel FischZeit) ist eine wissenschaftliche Fachzeitschrift für alle Bereiche der Fischerei in Binnengewässern, Küstengewässern und dem Meer. Sie berücksichtigt alle Themen, die die Erwerbs-, Freizeit- und Subsistenzfischerei, die Aquakultur sowie den Fischarten- und Gewässerschutz in Binnen- und Meeresökosystemen berühren. Die FischZeit publiziert Fachbeiträge aus unterschiedlichen Disziplinen (Natur- und Sozialwissenschaften) und legt Wert auf den konkreten Anwendungsbezug. Dementsprechend ist ein wesentliches Kennzeichen der FischZeit die Publikation von Fachbeiträgen, die wissenschaftlichen Standards entsprechen, aber gleichzeitig Lösungen für die Praxis anbieten. Alle Manuskripte durchlaufen nach der Einreichung einen wissenschaftlichen Begutachtungsprozess, an deren Ende auch die Ablehnung einmal eingereichter Manuskripte stehen kann.
description: Zeitschrift für Fischerei, Nr. 1 (2020)
MOESM3 of Investigation into limiting dilution and tick transmissibility phenotypes associated with attenuation of the S24 vaccine strain
Creators: name: Mans, Ben
name: Ronel Pienaar
name: P. Christo Troskie
name: Combrink, Michael
Publisher: name: figshare
Year: 2019
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Additional file 3: Table S3. Summary of the mapping coverages obtained for the major chromosomes de novo assembled for various B. bovis clones.
TeV String State Excitation via High Energy Cosmic Neutrinos
Creators: name: Friess, Joshua J.
name: Han, Tao
name: Hooper, Dan
Publisher: name: arXiv
Year: 2002
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Astrophysics (astro-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We construct the open-string scattering amplitudes for neutrino-gluon collisions and evaluate the high energy neutrino-nucleon scattering cross section via string state excitations in the TeV string-scale scenario. We find that the neutrino-gluon scattering is the dominant contribution, 5-10 times larger than neutrino-quark processes, though black hole production may be larger than the string contribution at higher energies. We illustrate the observability of the string signal at the Auger Observatory and the IceCube neutrino telescope for a string scale about 1 TeV.
description: version to appear in PLB
Nanophotonic quantum storage at telecommunications wavelength
Creators: name: Craiciu, Ioana
name: Lei, Mi
name: Rochman, Jake
name: Kindem, Jonathan M.
name: Bartholomew, John G.
name: Miyazono, Evan
name: Zhong, Tian
name: Sinclair, Neil
name: Faraon, Andrei
Publisher: name: arXiv
Year: 2019
Subjects: subject: Quantum Physics (quant-ph)
subject: Applied Physics (physics.app-ph)
subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: Quantum memories for light are important components for future long distance quantum networks. We present on-chip quantum storage of telecommunications band light at the single photon level in an ensemble of erbium-167 ions in an yttrium orthosilicate photonic crystal nanobeam resonator. Storage times of up to 10 $μ$s are demonstrated using an all-optical atomic frequency comb protocol in a dilution refrigerator under a magnetic field of 380 mT. We show this quantum storage platform to have high bandwidth, high fidelity, and multimode capacity, and we outline a path towards an efficient erbium-167 quantum memory for light.
description: 12 pages, 4 figures
Continuum HFB calculations with finite range pairing interactions
Creators: name: Grasso, M.
name: Van Giai, N.
name: Sandulescu, N.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: A new method of calculating pairing correlations in coordinate space with finite range interactions is presented. In the Hartree-Fock-Bogoliubov (HFB) approach the mean field part is derived from a Skyrme-type force whereas the pairing field is constructed with a Gogny force. An iterative scheme is used for solving the integro-differential HFB equations via the introduction of a local equivalent potential. The method is illustrated on the case of the nucleus $^{18}$C. It is shown that the results are insensitive to the cut off value in the quasiparticle spectrum if this value is above 100 MeV.
description: 3 figures, in press, Phys. Lett. B
Hygropoda Thorell 1894
Creators: name: Cruz Da Silva, Estevam L.
Publisher: name: Zenodo
Year: 2013
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Arachnida
Araneae
Pisauridae
Hygropoda

description: Hygropoda Thorell, 1894
 Hygropoda Thorell 1894: 4; Simon 1898: 315; Pocock 1900: 245; Hu 1984: 260; Yaginuma 1986: 176; Zhang et al. 2004: 381; Dankittipakul et al. 2008: 312.
 Hypsithylla Simon 1903: 38; Silva, 2012: 60 (Syn. of Hypsithylla under Hygropoda).
 Type species. Tegenaria dolomedes Doleschall, 1859, by original designation.
 Diagnosis. This genus can be distinguished from the other members of the family by: long and slender legs I, II and IV; long and flexible tarsi (this character also occurs in Megadolomedes Davies & Raven, 1980, endemic to Australia) (Fig. 24); distal tegular apophysis membranous, conductor membranous (Figs 7, 26), large and sclerotized embolus (Figs 11, 30). The females present a short and rounded spermatheca (Fig. 16) and base of spermatheca and copulatory ducts are enlarged and curved (Fig. 16).
 Distribution. Oriental, Australiasian and Afrotropical.
description: Published as part of Cruz Da Silva, Estevam L., 2013, The nursery-web spider Hygropoda tanganus (Roewer, 1955) comb. nov. (Araneae: Lycosoidea: Pisauridae); generic transfer, first description of the female and redescription of the male, pp. 289-296 in Zootaxa 3710 (3) on page 290, DOI: 10.11646/zootaxa.3710.3.7, http://zenodo.org/record/10099469
Cosmological Perturbation Theory Using the Schrödinger Equation
Creators: name: Szapudi, Istvan
name: Kaiser, Nick
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We introduce the theory of non-linear cosmological perturbations using the correspondence limit of the Schrödinger equation. The resulting formalism is equivalent to using the collisionless Boltzman (or Vlasov) equations which remain valid during the whole evolution, even after shell crossing. Other formulations of perturbation theory explicitly break down at shell crossing, e.g. Eulerean perturbation theory, which describes gravitational collapse in the fluid limit. This paper lays the groundwork by introducing the new formalism, calculating the perturbation theory kernels which form the basis of all subsequent calculations. We also establish the connection with conventional perturbation theories, by showing that third order tree level results, such as bispectrum, skewness, cumulant correlators, three-point function are exactly reproduced in the appropriate expansion of our results. We explicitly show that cumulants up to N=5 predicted by Eulerian perturbation theory for the dark matter field $δ$ are exactly recovered in the corresponding limit. A logarithmic mapping of the field naturally arises in the Schrödinger context, which means that tree level perturbation theory translates into (possibly incomplete) loop corrections for the conventional perturbation theory. We show that the first loop correction for the variance is $σ^2 = σ_L^2+ (-1.14+n)σ_L^4$ for a field with spectral index $n$. This yields 1.86 and 0.86 for $n=-3,-2$ respectively, and to be compared with the exact loop order corrections 1.82, and 0.88. Thus our tree-level theory recovers the dominant part of first order loop corrections of the conventional theory, while including (partial) loop corrections to infinite order in terms of $δ$.
description: 5 pages, submitted to ApJ Letters
Unified lensing and kinematic analysis for any elliptical mass profile
Creators: name: Shajib, Anowar J.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: We demonstrate an efficient method to compute the strong-gravitational-lensing deflection angle and magnification for any elliptical surface-density profile. This method solves a numerical hurdle in lens modelling that has lacked a general solution for nearly three decades. The hurdle emerges because it is prohibitive to derive analytic expressions of the lensing quantities for most elliptical mass profiles. In our method, we first decompose an elliptical mass profile into Gaussian components. We introduce an integral transform that provides us with a fast and accurate algorithm for the Gaussian decomposition. We derive analytic expressions of the lensing quantities for a Gaussian component. As a result, we can compute these quantities for the total mass profile by adding up the contributions from the individual components. This lensing analysis self-consistently completes the kinematic description in terms of Gaussian components presented by Cappellari (2008). Our method is general without extra computational burden unlike other methods currently in use.
description: 11 pages + appendices, 6 figures, submitted to MNRAS. An interactive jupyter notebook version of this paper is accessible on Google colab at https://colab.research.google.com/drive/10jw5T07mhvdP0hp60HqVqNqWK49Cfzby
MOESM2 of Investigation into limiting dilution and tick transmissibility phenotypes associated with attenuation of the S24 vaccine strain
Creators: name: Mans, Ben
name: Ronel Pienaar
name: P. Christo Troskie
name: Combrink, Michael
Publisher: name: figshare
Year: 2019
Subjects: subject: Space Science
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: Cancer
subject: Inorganic Chemistry
subject: FOS: Chemical sciences
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Additional file 2: Table S2. Mapping statistics for reads to their respective de novo assembled genomes. Indicated are the number of paired-end reads generated after quality trimming, the number mapped to their respective de novo assembled genomes, the number of reads mapped in pairs; and the percentage reads mapped and the percentage reads mapped in pairs.
OCC: A Smart Reply System for Efficient In-App Communications
Creators: name: Weng, Yue
name: Zheng, Huaixiu
name: Bell, Franziska
name: Tur, Gokhan
Publisher: name: arXiv
Year: 2019
Subjects: subject: Computation and Language (cs.CL)
subject: Machine Learning (stat.ML)
subject: FOS: Computer and information sciences

description: Smart reply systems have been developed for various messaging platforms. In this paper, we introduce Uber's smart reply system: one-click-chat (OCC), which is a key enhanced feature on top of the Uber in-app chat system. It enables driver-partners to quickly respond to rider messages using smart replies. The smart replies are dynamically selected according to conversation content using machine learning algorithms. Our system consists of two major components: intent detection and reply retrieval, which are very different from standard smart reply systems where the task is to directly predict a reply. It is designed specifically for mobile applications with short and non-canonical messages. Reply retrieval utilizes pairings between intent and reply based on their popularity in chat messages as derived from historical data. For intent detection, a set of embedding and classification techniques are experimented with, and we choose to deploy a solution using unsupervised distributed embedding and nearest-neighbor classifier. It has the advantage of only requiring a small amount of labeled training data, simplicity in developing and deploying to production, and fast inference during serving and hence highly scalable. At the same time, it performs comparably with deep learning architectures such as word-level convolutional neural network. Overall, the system achieves a high accuracy of 76% on intent detection. Currently, the system is deployed in production for English-speaking countries and 71% of in-app communications between riders and driver-partners adopted the smart replies to speedup the communication process.
description: link to demo: https://www.youtube.com/watch?v=nOffUT7rS0A&t=32s
Masses of the pseudo-Nambu-Goldstone bosons in two flavor color superconducting phase
Creators: name: Miransky, V. A.
name: Shovkovy, I. A.
name: Wijewardhana, L. C. R.
Publisher: name: arXiv
Year: 2001
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Theory (hep-th)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: The masses of the pseudo-Nambu-Goldstone bosons in the color superconducting phase of dense QCD with two light flavors are estimated by making use of the Cornwall-Jackiw-Tomboulis effective action. Parametrically, the masses of the doublet and antidoublet bosons are suppressed by a power of the coupling constant as compared to the value of the superconducting gap. This is qualitatively different from the mass expression for the singlet pseudo-Nambu-Goldstone boson, resulting from non-perturbative effects. It is argued that the (anti-) doublet pseudo-Nambu-Goldstone bosons form colorless [with respect to the unbroken SU(2)_{c}] charmonium-like bound states. The corresponding binding energy is also estimated.
description: 18 pages and 1 figure. REVTeX. New references and Appendix C with a discussion of the gauge invariance in color superconductivity are added. To appear in Phys. Rev. D
Formation of quasi-periodic slow magnetoacoustic wave trains by the heating/cooling misbalance
Creators: name: Zavershinskii, D. I.
name: Kolotkov, D. Y.
name: Nakariakov, V. M.
name: Molevich, N. E.
name: Ryashchikov, D. S.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Plasma Physics (physics.plasm-ph)
subject: FOS: Physical sciences

description: Slow magnetoacoustic waves are omnipresent in both natural and laboratory plasma systems. The wave-induced misbalance between plasma cooling and heating processes causes the amplification or attenuation, and also dispersion, of slow magnetoacoustic waves. The wave dispersion could be attributed to the presence of characteristic time scales in the system, connected with the plasma heating or cooling due to the competition of the heating and cooling processes in the vicinity of the thermal equilibrium. We analysed linear slow magnetoacoustic waves in a plasma in a thermal equilibrium formed by a balance of optically thin radiative losses, field-align thermal conduction, and an unspecified heating. The dispersion is manifested by the dependence of the effective adiabatic index of the wave on the wave frequency, making the phase and group speeds frequency-dependent. The mutual effect of the wave amplification and dispersion is shown to result into the occurrence of an oscillatory pattern in an initially broadband slow wave, with the characteristic period determined by the thermal misbalance time scales, i.e. by the derivatives of the combined radiation loss and heating function with respect to the density and temperature, evaluated at the equilibrium. This effect is illustrated by estimating the characteristic period of the oscillatory pattern, appearing because of thermal misbalance in the plasma of the solar corona. It is found that by an order of magnitude the period is about the typical periods of slow magnetoacoustic oscillations detected in the corona.
description: Accepted for publication in Physics of Plasmas
Directly testing gravity with Proxima Centauri
Creators: name: Banik, Indranil
name: Kroupa, Pavel
Publisher: name: arXiv
Year: 2019
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The wide binary orbit of Proxima Centauri around $α$ Centauri A and B differs significantly between Newtonian and Milgromian dynamics (MOND). By combining previous calculations of this effect with mock observations generated using a Monte Carlo procedure, we show that this prediction can be tested using high precision astrometry of Proxima Centauri. This requires ${\approx 10}$ years of observations at an individual epoch precision of $0.5 \, μ$as, within the design specifications of the proposed Theia mission. In general, the required duration should scale as the 2/5 power of the astrometric precision. A long-period planet could produce a MOND-like astrometric signal, but only if it has a particular ratio of mass to separation squared and a sky position close to the line segment connecting Proxima Centauri with $α$ Centauri. Uncertainties in perspective effects should be small enough for this test if the absolute radial velocity of Proxima Centauri can be measured to within ${\approx 10}$ m/s, better than the present accuracy of 32 m/s. We expect the required improvement to become feasible using radial velocity zero points estimated from larger samples of close binaries, with the Sun providing an anchor. We demonstrate that possible astrometric microlensing of Proxima Centauri is unlikely to affect the results. We also discuss why it should be possible to find sufficiently astrometrically stable reference stars. Adequately addressing these and other issues would enable a decisive test of gravity in the currently little explored low acceleration regime relevant to the dynamical discrepancies in galactic outskirts.
description: 10 pages, 2 figures. Published in the Monthly Notices of the Royal Astronomical Society in this form
Neutrinos as the messengers of CPT violation
Creators: name: Barenboim, G.
name: Borissov, L.
name: Lykken, J.
name: Smirnov, A. Yu
Publisher: name: arXiv
Year: 2001
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: CPT violation has the potential to explain all three existing neutrino anomalies without enlarging the neutrino sector. CPT violation in the Dirac mass terms of the three neutrino flavors preserves Lorentz invariance, but generates independent masses for neutrinos and antineutrinos. This specific signature is strongly motivated by braneworld scenarios with extra dimensions, where neutrinos are the natural messengers for Standard Model physics of CPT violation in the bulk. A simple model of maximal CPT violation is sufficient to explain the exisiting neutrino data quite neatly, while making dramatic predictions for the upcoming KamLAND and MiniBooNE experiments. Furthermore we obtain a promising new mechanism for baryogenesis.
description: 10 pages latex, 1 eps fig, footnote added, enhanced referencing
Next-to-leading order numerical calculations in Coulomb gauge
Creators: name: Kramer, Michael
name: Soper, Davison E.
Publisher: name: arXiv
Year: 2002
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Calculations of observables in quantum chromodynamics can be performed using a method in which all of the integrations, including integrations over virtual loop momenta, are performed numerically. We use the flexibility inherent in this method in order to perform next-to-leading order calculations for event shape variables in electron-positron annihilation in Coulomb gauge. The use of Coulomb gauge provides the potential to go beyond a purely order alpha_s^2 calculation by including, for instance, renormalon or parton showering effects. We expect that the approximations needed to include such effects at all orders in alpha_s will be simplest in a gauge in which unphysically polarized gluons do not propagate over long distances.
description: 36 pages with 7 figures
K+/pi+ probes of jet quenching in AA collisions
Creators: name: Levai, P.
name: Papp, G.
name: Fai, G.
name: Gyulassy, M.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: Non-abelian energy loss in quark gluon plasma is shown to lead to novel hadron ratio suppression patterns in ultrarelativistic nuclear collisions. We apply recent (GLV) estimates for the gluon radiative energy loss, which increases linearly with the jet energy up to E<20 GeV and depends quadratically on the nuclear radius, R. The K+/π+ ratio is found to be most sensitive to the initial density of the plasma.
description: Presented at 6th International Conference on Strange Quarks in Matter: 2001: A Flavourspace Odyssey (SQM2001), Frankfurt, Germany, 25-29 Sep 2001
Electro-weak production of pseudovector C-even heavy quarkonia in electron-positron collisions on Belle II and BES III
Creators: name: Achasov, Nikolay
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: It is shown that the molecular model for the X{3872) state contradicts the new experimental data as well as the old ones. It is suggested to study the χ_{c1} and χ_{b1} states in the e+e-\toχ_{c1}/χ_{b1} reactions.
description: 7 pages, 4 figures, Plenary Talk given at the 12th Workshop on e+e- Collisions from Phi to Psi, 25.02.2019 - 01.03.2019, Novosibirsk, Russia
MOESM1 of Investigation into limiting dilution and tick transmissibility phenotypes associated with attenuation of the S24 vaccine strain
Creators: name: Mans, Ben
name: Ronel Pienaar
name: P. Christo Troskie
name: Combrink, Michael
Publisher: name: figshare
Year: 2019
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Ecology
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Additional file 1: Table S1 Summary of the de novo assembly of the Babesia bovis genome compared to the reference genome size for the chromosomes and organelles. The size of the reference genome is indicated and the relative size of each de novo assembled genome in percentage. Highlighted chromosomes were used for the analysis of recombination and genome similarity.
Nothotragopus tuberosus
Creators: name: Setliff, Gregory P.
Publisher: name: Zenodo
Year: 2008
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Curculionidae
Nothotragopus
Nothotragopus tuberosus

description: Nothotragopus tuberosus (Boheman)
(Fig. 2–3, 10, 14–17)
 Tragopus tuberosus Boheman, in Schönherr 1844: 428 [description]; Lea, 1913: 466 [notes]. Nothotragopus tuberosus (Boheman), Zimmerman 1992: 282 Plate 445.1 and 445.2. [transferred and illustrated]; Zimmerman 1994: 657 [redescription].
 Diagnosis. This species is distinguished from its congeners by the combination of its smaller size (length 7.9 mm, width 3.3 mm) and pronotum uniformly covered in dense squamae. The unmodified ventral apex of the female rostrum separates this species from N. tragopoides (Fig. 10). The truncate and smooth apex of the female tergite VIII is evenly set with numerous short stout setae (Fig. 16) and further separates it from N. zimmermani. See Zimmerman (1994: 657) for redescription.
 Type material examined. Holotype: 1 ♀. ‘‘N.H./Hope 184 N. Holl./19, NG [on underside]/ Tragopus tuberous /Specimen figured, ECZ.’’ [UMO].
 Other material examined. 1 ♀. [formerly a syntype of Cyamobolus tragopoides Heller]: ‘‘ Java /ex. coll. Felsche. / Paratypus [sic], Cyamobolus tragopoides Hellr. ’’ [NHML].
 210 Dubious material. Male provisionally determined to species: 1 Oi. [formerly a syntype of Cyamobolus tragopoides Heller]: ‘‘ P.F. Sijthoff., Preanger, Java /1912, 44/ Paratypus [sic], Cyamobolus tragopoides Hellr. 39/ Syntypus / Cyamobolus, tragopoides m.i.l, Heller det. 1939’’ [DEI]. I tentatively assign this male to N. tuberosus based on similarity of the dorsal vestiture and smaller, less robust facies.
description: Published as part of Setliff, Gregory P., 2008, Review of the Indonesian GenusNothotragopusZimmerman (Coleoptera: Curculionidae: Cryptorhynchinae), pp. 203-214 in The Coleopterists Bulletin (Basel, Switzerland) (Basel, Switzerland) 62 (2) on pages 203-214, DOI: 10.1649/1057.1, http://zenodo.org/record/5369831
The Phoenix Deep Survey: The 1.4 GHz microJansky catalogue
Creators: name: Hopkins, A. M.
name: Afonso, J.
name: Chan, B.
name: Cram, L. E.
name: Georgakakis, A.
name: Mobasher, B.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The initial Phoenix Deep Survey (PDS) observations with the Australia Telescope Compact Array have been supplemented by additional 1.4 GHz observations over the past few years. Here we present details of the construction of a new mosaic image covering an area of 4.56 square degrees, an investigation of the reliability of the source measurements, and the 1.4 GHz source counts for the compiled radio catalogue. The mosaic achieves a 1-sigma rms noise of 12 microJy at its most sensitive, and a homogeneous radio-selected catalogue of over 2000 sources reaching flux densities as faint as 60 microJy has been compiled. The source parameter measurements are found to be consistent with the expected uncertainties from the image noise levels and the Gaussian source fitting procedure. A radio-selected sample avoids the complications of obscuration associated with optically-selected samples, and by utilising complementary PDS observations including multicolour optical, near-infrared and spectroscopic data, this radio catalogue will be used in a detailed investigation of the evolution in star-formation spanning the redshift range 0 < z < 1. The homogeneity of the catalogue ensures a consistent picture of galaxy evolution can be developed over the full cosmologically significant redshift range of interest. The 1.4 GHz mosaic image and the source catalogue are available on the web at http://www.atnf.csiro.au/~ahopkins/phoenix/ or from the authors by request.
description: 16 pages, 11 figures, 4 tables. Accepted for publication by AJ
Nothotragopus tragopoides Setliff 2008, new combination
Creators: name: Setliff, Gregory P.
Publisher: name: Zenodo
Year: 2008
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Curculionidae
Nothotragopus
Nothotragopus tragopoides

description: Nothotragopus tragopoides (Heller), new combination
(Figs. 4–5, 11, 18–21)
description: Published as part of Setliff, Gregory P., 2008, Review of the Indonesian GenusNothotragopusZimmerman (Coleoptera: Curculionidae: Cryptorhynchinae), pp. 203-214 in The Coleopterists Bulletin (Basel, Switzerland) (Basel, Switzerland) 62 (2) on pages 203-214, DOI: 10.1649/1057.1, http://zenodo.org/record/5369831
An X-ray reverberation mass measurement of Cygnus X-1
Creators: name: Mastroserio, Guglielmo
name: Ingram, Adam
name: van der Klis, Michiel
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We present the first X-ray reverberation mass measurement of a stellar-mass black hole. Accreting stellar-mass and supermassive black holes display characteristic spectral features resulting from reprocessing of hard X-rays by the accretion disc, such as an Fe K$α$ line and a Compton hump. This emission probes of the innermost region of the accretion disc through general relativistic distortions to the line profile. However, these spectral distortions are insensitive to black hole mass, since they depend on disc geometry in units of gravitational radii. Measuring the reverberation lag resulting from the difference in path length between direct and reflected emission calibrates the absolute length of the gravitational radius. We use a relativistic model able to reproduce the behaviour of the lags as a function of energy for a wide range of variability timescales, addressing both the reverberation lags on short timescales and the intrinsic hard lags on longer timescales. We jointly fit the time-averaged spectrum and the real and imaginary parts of the cross-spectrum as a function of energy for a range of Fourier frequencies to Rossi X-ray Timing Exporer data from the X-ray binary Cygnus X-1. We also show that introducing a self-consistently calculated radial ionisation profile in the disc improves the fit, but requires us to impose an upper limit on ionisation profile peak to allow a plausible value of the accretion disc density. This limit leads to a mass value more consistent with the existing dynamical measurement.
description: 14 pages, accepted for publication in MNRAS
Additional file 6: of Temporal and partial inhibition of GLI1 in neural stem cells (NSCs) results in the early maturation of NSC derived oligodendrocytes in vitro
Creators: name: Poommaree Namchaiw
name: Wen, Han
name: Mayrhofer, Florian
name: Chechneva, Olga
name: Biswas, Sangita
name: Wenbin Deng
Publisher: name: figshare
Year: 2019
Subjects: subject: Biochemistry
subject: Space Science
subject: Pharmacology
subject: Biotechnology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Developmental Biology
subject: Cancer

description: Table S1. List of primers used in this study. (DOCX 15 kb)
A note on brane cosmology
Creators: name: Kehagias, A.
name: Tamvakis, K.
Publisher: name: arXiv
Year: 2001
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We derive a new class of time-dependent solutions for the Randall-Sundrum model by patching together isometries broken by the brane. Solutions generated by generalized boosts along the fifth dimension are associated with localized gravity and lead to an effective Friedman equation on the brane with a scale factor exhibiting power law or exponential behaviour. The effective energy-density on the brane depends linearly on the brane tension.
description: 10 pages, references added
Electric charge quantization and the muon anomalous magnetic moment
Creators: name: Pires, C. A. de S.
name: da Silva, P. S. Rodrigues
Publisher: name: arXiv
Year: 2001
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We investigate some proposals to solve the electric charge quantization puzzle, which simultaneously explain the recent measured deviation on the muon anomalous magnetic moment. For this we assess extensions of the Electro-Weak Standard Model spanning modifications on the scalar sector only. It is interesting to verify that one can have modest extensions which easily account for the solution for both problems.
description: 20 pages, 1 figures, needs macro axodraw.sty
Cosmological Simulations of Satellites around Isolated Dwarf Galaxies
Creators: name: Chun, Kyungwon
name: Shin, Jihye
name: Smith, Rory
name: Kim, Sungsoo S.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We trace the cosmological origin of satellites around a dwarf galaxy using a very high resolution (12~pc/h) cosmological hydrodynamic zoom simulation. To realistically describe the formation and evolution of small-mass stellar satellites, our model includes a full baryonic physics treatment including a recipe for UV self-shielding. We find that the mini-halos form objects resembling dwarf galaxies. Despite our high resolution, none of our 'mini-halos' form objects that might be considered globular cluster-like. Instead such objects are formed in the host galaxy's gaseous disk. We investigate why some form stars more efficiently than others. We find that the majority of their star forming gas is accreted after reionisation, thus the survival of a mini-halo's gas to reionisation is not an important factor. Instead, the key factor seems to be the ability for a mini-halo to cool its recently accreted gas, which is more efficient in more massive halos. We find halos in denser environments suffer more mergers, enabling them to grow their mass such that cooling of accreted gas can occur efficiently. Although the host galaxy is only a dwarf galaxy itself, we find that ram pressure is an efficient means by which accreted mini-halos lose their gas content, both by interacting with hot halo gas but also in direct collisions with the gas disk of the host. The satellites are also disrupted by the tidal forces near the center of the host galaxy. Compared to the disrupted satellites, surviving satellites are relatively more massive, but tend to infall later into the host galaxy, thus reducing the time they are subjected to destructive environmental mechanisms and dynamical friction. In summary, our results suggest that the characteristics of satellites are mainly determined by their ability to efficiently cool gas that is accreted in the redshift range z=3-5, prior to their infall into the host galaxy.
description: 15 pages, 11 figures, 1 table. Accepted for publication in The Astrophysical Journal, June 14th, 2019
BALIQLARNING OZUQALARDAN ZAHARLANISHLARINI DIAGNOSTIKASI VA OLDINI OLISH CHORA-TADBIRLARI
Creators: name: Kurbanov F.E. - v.f.f.d. (PhD) Yuldoshev X.T. – b.f.f.d. (PhD) Saparov O.J. - assistent Fayzullayev I.A. – assistent Mamasharifov S.J. – talaba Xurramova S.G'. – talaba Samarqand davlat veterinariya medisinasi, chorvachilik va biotexnologiyalar universiteti
Publisher: name: Zenodo
Year: 2025

description: Суточные корма, даваемые рыбам, богаты различнымипитательными веществами, витаминами и минералами, должны удовлетворятьпотребности организма рыб и не должны отрицательно сказываться на ихздоровье, росте и развитии, качестве продукции
The Cosmic Lens All-Sky Survey:II. Gravitational lens candidate selection and follow-up
Creators: name: Browne, I. W. A.
name: Wilkinson, P. N.
name: Jackson, N. J. F.
name: Myers, S. T.
name: Fassnacht, C. D.
name: Koopmans, L. V. E.
name: Marlow, D. R.
name: Norbury, M.
name: Rusin, D.
name: Sykes, C. M.
name: Biggs, A. D.
name: Blandford, R. D.
name: de Bruyn, A. G.
name: Chae, K-H.
name: Helbig, P.
name: King, L. J.
name: McKean, J. P.
name: Pearson, T. J.
name: Phillips, P. M.
name: Readhead, A. C. S.
name: Xanthopoulos, E.
name: York, T.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report the final results of the search for gravitationally lensed flat-spectrum radio sources found in the combination of CLASS (Cosmic Lens All Sky Survey) and JVAS (Jodrell-Bank VLA Astrometric Survey). VLA observations of 16,503 sources have been made, resulting in the largest sample of arcsec-scale lens systems available. Contained within the 16,503 sources is a complete sample of 11,685 sources having two-point spectral indices between 1.4 and 5 GHz flatter than -0.5 and 5 GHz flux densities $\geq$30 mJy. A subset of 8,958 sources form a well-defined statistical sample suitable for analysis of the lens statistics. We describe the systematic process by which 149 candidate lensed sources were picked from the statistical sample on the basis of possessing multiple compact components in the 0.2 arcsec-resolution VLA maps. Candidates were followed up with 0.05 arcsec resolution MERLIN and 0.003 arcsec VLBA observations at 5 GHz and rejected as lens systems if they failed well-defined surface brightness and/or morphological tests. Maps for all the candidates can be found on the World Wide Web at http://www.jb.man.ac.uk/research/gravlens/index.html We summarize the properties of each of the 22 gravitational lens systems in JVAS/CLASS. Twelve are double-image systems, nine are four-image systems and one is a six-image system. Thirteen constitute a statistically well-defined sample giving a point-source lensing rate of 1:690$\pm$190. The interpretation of the results in terms of the properties of the lensing galaxy population and cosmological parameters will be published elsewhere. (Abridged)
description: v2: web link in the abstract fixed; some corrections made in section 6.1
Additional file 1 of LinDA: linear models for differential abundance analysis of microbiome compositional data
Creators: name: Zhou, Huijuan
name: He, Kejun
name: Chen, Jun
name: Zhang, Xianyang
Publisher: name: figshare
Year: 2022
Subjects: subject: Statistics
subject: FOS: Mathematics

description: Additional file 1 Supplementary notes. Table S1 lists some robust normalization methods [11–14]. Lemmas S1 – S4 present intermediate results for proving Theorem 1. The proof depends on some useful results from [50–53].
Querying Knowledge via Multi-Hop English Questions
Creators: name: Gao, Tiantian
name: Fodor, Paul
name: Kifer, Michael
Publisher: name: arXiv
Year: 2019
Subjects: subject: Computation and Language (cs.CL)
subject: Artificial Intelligence (cs.AI)
subject: FOS: Computer and information sciences

description: The inherent difficulty of knowledge specification and the lack of trained specialists are some of the key obstacles on the way to making intelligent systems based on the knowledge representation and reasoning (KRR) paradigm commonplace. Knowledge and query authoring using natural language, especially controlled natural language (CNL), is one of the promising approaches that could enable domain experts, who are not trained logicians, to both create formal knowledge and query it. In previous work, we introduced the KALM system (Knowledge Authoring Logic Machine) that supports knowledge authoring (and simple querying) with very high accuracy that at present is unachievable via machine learning approaches. The present paper expands on the question answering aspect of KALM and introduces KALM-QA (KALM for Question Answering) that is capable of answering much more complex English questions. We show that KALM-QA achieves 100% accuracy on an extensive suite of movie-related questions, called MetaQA, which contains almost 29,000 test questions and over 260,000 training questions. We contrast this with a published machine learning approach, which falls far short of this high mark.
description: Paper presented at the 35th International Conference on Logic Programming (ICLP 2019), Las Cruces, New Mexico, USA, 20-25 September 2019, 16 pages
ХИРУРГИЧЕСКОЕ ЛЕЧЕНИЕ ФАРМАКОРЕЗИСТЕНТНЫХ ФОРМ ЭПИЛЕПСИИ
Creators: name: Хаккулов, Эзоз
name: Уралова, Севинч
name: Курбонов, Н.З.
Publisher: name: Zenodo
Year: 2025

description: Уточнить показаний к хирургическому лечению эпилепсии и определить наиболее оптимальный способ хирургического леченияфармакорезистентных форм эпилепсии. Оценить эффективности хирургического лечения у больных с фармакорезистентной формой эпилепсии.
Diffraction at HERA
Creators: name: Marage, P.
Publisher: name: arXiv
Year: 2001
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Talk given at the First Workshop on Forward Physics and Luminosity Determination at the LHC, Helsinki, Finland, November 2000. 12 pages, 9 figures