cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Ground-State Magnetization in Mixtures of a Few Ultra-Cold Fermions in One-Dimensional Traps
Creators: name: Sowiński, Tomasz
Publisher: name: arXiv
Year: 2018
Subjects: subject: Quantum Gases (cond-mat.quant-gas)
subject: FOS: Physical sciences

description: Ground-state properties of a few spin-$1/2$ ultra-cold fermions confined in a one-dimensional trap are studied by the exact diagonalization method. In contrast to previous studies, it is not assumed that the projection of a spin of individual particles is fixed. Therefore, the spin is treated as an additional degree of freedom and the global magnetization of the system is established spontaneously. Depending on the shape of the trap, inter-particle interactions, and an external magnetic field, the phase diagram of the system is determined. It is shown that, for particular confinements, some values of the magnetization cannot be reached by the ground-state of the system.
description: This article belongs to the Special Issue "New Trends in Quantum Complex Matter"
title: ADCO, Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Cart. 32 (G 136), 745 folios, f. 0887
Creators: name: de la Côte d'Or, Archives départementales
name: Petot, Frédéric
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2012
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: Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Archives départementales de la Côte-d'Or, Cart. 32 (G 136), 745 folios, f. 0887, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Archives départementales de la Côte-d'Or, Cart. 32 (G 136), 745 folios, f. 0887, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: abbaye Saint-Étienne de Dijon
description: Provenance: http://www.wikidata.org/entity/Q15945019
Phase transitions of the Kane-Mele-Hubbard model with a long-range hopping
Creators: name: Du, Tao
name: Li, Yue-Xun
name: Lu, He-Lin
name: Zhang, Hui
Publisher: name: arXiv
Year: 2018
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: The interacting Kane-Mele model with a long-range hopping is studied using analytical method. The original Kane-Mele model is defined on a honeycomb lattice. In the work, we introduce a four-lattice-constant range hopping and the on-site Hubbard interaction into the model and keep its lattice structure unchanged. From the single-particle energy spectrum, we obtain the critical strength of the long-range hopping $t_L$ at which the topological transition occurs in the non-interacting limit of the model and our results show that it is independent of the spin-orbit coupling. After introducing the Hubbard interaction, we investigate the Mott transition and the magnetic transition of the generalized strongly correlated Kane-Mele model using the slave-rotor mean field theory and Hartree-Fock mean field theory respectively. In the small long-range hopping region, it is a correlated quantum spin Hall state below the Mott transition, while a topological Mott insulator above the Mott transition. By comparing the energy band of spin degree of freedom with the one of electrons in non-interacting limit, we find a condition for the $t_L$-driven topological transition. Under the condition, critical values of $t_L$ at which the topological transition occurs are obtain numerically from seven self-consistency equations in both regions below and above the Mott transition. Influences of the interaction and the spin-orbit coupling on the topological transition are discussed in this work. Finally, we show complete phase diagrams of the generalized interacting topological model at some strength of spin-orbital coupling.
description: 20 pages,10 figures
Polarized deep inelastic scattering at high energies and parity violating structure functions
Creators: name: Anselmino, M.
name: Gambino, P.
name: Kalinowski, J.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: A comprehensive analysis of deep inelastic scattering of polarized charged leptons on polarized nucleons is presented; weak interaction contributions, both in neutral and charged current processes, are taken into account and the parity violating polarized nucleon structure functions are studied. Possible ways of their measurements and their interpretations in the parton model are discussed.
description: (slightly modified version, includes a few new references and corrects few misprints for publication), 14 pages in TeX (needs harvmac) no figure, DFTT 80/93
Electromagnetically driven convection suitable for mass transfer enhancement in liquid metal batteries
Creators: name: Weber, Norbert
name: Nimtz, Michael
name: Personnettaz, Paolo
name: Salas, Alejandro
name: Weier, Tom
Publisher: name: arXiv
Year: 2018
Subjects: subject: Applied Physics (physics.app-ph)
subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: Liquid metal batteries (LMBs) were recently proposed as cheap large scale energy storage. Such devices are urgently required for balancing highly fluctuating renewable energy sources. During discharge, intermetallic phases tend to form in the cathode of LMBs. These do not only limit the up-scalability, but also the efficiency of the cells. Generating a mild fluid flow in the fully liquid cell will smoothen concentration gradients and minimise the formation of intermetallics. In this context we study electro-vortex flow numerically. We simulate a recent LMB related experiment and discuss how the feeding lines to the cell can be optimised to enhance mass transfer. The Lorentz forces have to overcome the stable thermal stratification in the cathode of the cell; we show that thermal effects may reduce electro-vortex flow velocities considerable. Finally, we study the influence of the Earth magnetic field on the flow.
Development of the Medication adherence Estimation and Differentiation Scale (MEDS)
Creators: name: Amod S. Athavale
name: Bentley, John P.
name: Banahan, Benjamin F.
name: McCaffrey, David J.
name: Pace, Patrick F.
name: Vorhies, Douglas W.
Publisher: name: Taylor & Francis
Year: 2018
Subjects: subject: Medicine
subject: Pharmacology
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Science Policy

description: Objectives: To develop a self-reported measure for medication adherence and compare its ability to predict proportion of days covered (PDC) with contemporary scales. Methods: Retrospective prescription fill data from three community pharmacies in the Southeastern US were assessed to identify patients that are 18 years of age or older, and have received at least one medication for diabetes, hypertension, or dyslipidemia. A cross-sectional survey containing the Medication adherence Estimation and Differentiation Scale (MEDS), was administered among these pharmacy patrons. The MEDS assessed the extent and reasons for non-adherence. Survey responses were anonymously linked with retrospective prescription fill data. A total of 685 patients were sampled. Proportion of days covered (PDC) was used as the criterion measure. The Morisky, Green and Levine Adherence Scale (1986 Morisky scale) and the Medication Adherence Reasons Scale (MAR-Scale) were used as comparators. Results: The MEDS presented a five-factor solution – worries about side-effects, worries about addiction, worries about cost, lack of perceived need, and unintentional non-adherence (CFI = 0.97; RMSEA = 0.06; SRMR = 0.03; standardized factor loadings greater than 0.5, and statistically significant). The relationship between MEDS scores and PDC was statistically significant (unstandardized regression coefficient = -0.50, p<0.01). The MEDS performed better than the 1986 Morisky scale (R2  = 0.02 vs. 0.05, standardized regression coefficient = -0.13 vs. -0.21) and the MAR-Scale (R2 = 0.02 vs. 0.05, standardized regression coefficient = -0.12 vs. -0.21) in predicting PDC. Conclusions: The MEDS demonstrated good psychometric properties and performed better than the comparator scales in the prediction of PDC.
Electroweak Baryogenesis in the Adiabatic Limit
Creators: name: Dine, Michael
name: Thomas, Scott
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Electroweak baryogenesis can occur in the ``adiabatic limit,'' in which expanding bubbles of true vacuum are assumed to have rather thick walls and be slowly moving. Here the problem of calculating the baryon asymmetry in this limit is reconsidered. A simple prescription for obtaining the relevant kinetic equations is given. An additional suppression beyond that usually assumed is found. This arises because the generation of an asymmetry requires violation of approximately conserved currents by Higgs expectation values, which are small near the front of the walls. As applications, the asymmetries in multi-Higgs models and the minimal supersymmetric standard model are estimated to be proportional to $α_w^8$ and $α_w^6$ respectively. Also, in this limit the baryon asymmetry in the Minimal Standard Model is extraordinarily small.
description: Tex file, requires phyzzx, 14 pages, 2 figures (not included), SCIPP preprint 94/01
การพัฒนาหลักสูตรฝึกอบรมเพศศึกษาด้วยเทคนิคการเรียนรู้แบบร่วมมือของนักศึกษาสถาบันการพลศึกษา
Creators: name: ชบา ขี่ทอง
Publisher: name: สถาบันวิจัย จัดการความรู้ และมาตรฐานการควบคุมโรค
Year: 2559
Subjects: การเรียนรู้แบบร่วมมือ
หลักสูตรฝึกอบรม
เพศศึกษา
นักศึกษาสถาบันการพลศึกษา

description: วารสารควบคุมโรค, 42, 3, 243-254
Methods for separation of deuterons produced in the medium and in jets in high energy collisions
Creators: name: Sharma, Natasha
name: Perez, Tony
name: Castro, Andy
name: Kumar, Lokesh
name: Nattrass, Christine
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: Coalescence has long been used to describe the production of light (anti-)nuclei in heavy ion collisions. The same underlying mechanism may also exist in jets when a proton and a neutron are close enough in phase space to form a deuteron. We model deuteron production in jets by applying an afterburner to protons and neutrons produced in PYTHIA for $p$+$p$ collisions at a center of mass energy $\sqrt{s} =$ 7 TeV. PYTHIA provides a reasonable description of the proton spectra and the shape of the deuteron spectrum predicted by the afterburner is in agreement with the data. We show that the rise in the coalescence parameter $B_2$ with momentum observed in data is consistent with coalescence in jets. We show that di-hadron correlations can be used to separate the contributions from the jet and the underlying event. This model predicts that the conditional coalescence parameter in the jet-like correlation should be independent of the trigger momentum.
description: 6 pages, 7 figures
Development of the medication adherence estimation and differentiation scale (MEDS)
Creators: name: Amod S. Athavale
name: Bentley, John P.
name: Banahan, Benjamin F.
name: McCaffrey, David J.
name: Pace, Patrick F.
name: Vorhies, Douglas W.
Publisher: name: Taylor & Francis
Year: 2018
Subjects: subject: Medicine
subject: Pharmacology
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Science Policy

description: Objectives: To develop a self-reported measure for medication adherence and compare its ability to predict the proportion of days covered (PDC) with contemporary scales. Methods: Retrospective prescription fill data from three community pharmacies in the Southeastern US were assessed to identify patients that were 18 years of age or older, and had received at least one medication for diabetes, hypertension, or dyslipidemia. A cross-sectional survey containing the Medication adherence Estimation and Differentiation Scale (MEDS) was administered among these pharmacy patrons. The MEDS assessed the extent and reasons for non-adherence. Survey responses were anonymously linked with retrospective prescription fill data. A total of 685 patients were sampled. The proportion of days covered (PDC) was used as the criterion measure. The Morisky, Green, and Levine Adherence Scale (1986 Morisky scale) and the Medication Adherence Reasons Scale (MAR-Scale) were used as comparators. Results: The MEDS presented a five-factor solution—worries about side-effects, worries about addiction, worries about cost, lack of perceived need, and unintentional non-adherence (CFI = 0.97; RMSEA = 0.06; SRMR = 0.03; standardized factor loadings greater than 0.5, and statistically significant). The relationship between MEDS scores and PDC was statistically significant (unstandardized regression coefficient = –0.50, p R2 = 0.02 vs 0.05, standardized regression coefficient = –0.13 vs –0.21) and the MAR-Scale (R2 = 0.02 vs 0.05, standardized regression coefficient = –0.12 vs –0.21) in predicting PDC. Conclusions: The MEDS demonstrated good psychometric properties and performed better than the comparator scales in the prediction of PDC.
Lieb polariton topological insulators
Creators: name: Li, Chunyan
name: Ye, Fangwei
name: Chen, Xianfeng
name: Kartashov, Yaroslav V.
name: Ferrando, Albert
name: Torner, Lluis
name: Skryabin, Dmitry V.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Pattern Formation and Solitons (nlin.PS)
subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: We predict that the interplay between the spin-orbit coupling, stemming from the TE-TM energy splitting, and the Zeeman effect in semiconductor microcavities supporting exci- ton-polariton quasi-particles results in the appearance of unidirectional linear topological edge states when the top microcavity mirror is patterned to form a truncated dislocated Lieb lattice of cylindrical pillars. Periodic nonlinear edge states are found to emerge from the linear ones. They are strongly localized across the interface and they are remarkably robust in comparison to their counterparts in hexagonal lattices. Such robustness makes possible the existence of nested unidirectional dark solitons that move steadily along the lattice edge.
description: 27 pages, 7 figures, to appear in Phys. Rev. B as a Rapid Communications
Mass loss and magnetospheres of massive stars
Creators: name: Küker, Manfred
Publisher: name: arXiv
Year: 2018
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: About ten percent of all OB stars show strong, large-scale surface magnetic fields. The interaction of the magnetic field and the wind is believed to be the cause for the X-ray emission shown by these objects. We therefore run numerical simulations in two dimensions for a number the O-type stars and Wolf Rayet stars to study the interaction of the stellar magnetic fields of these stars with their winds. While weak, dipolar magnetic fields leave the wind largely unmodified and the field opens up and becomes a split monopole, the interaction between magnetic field and outflowing gas is more complex as the magnetic field remains closed in some regions and outflowing gas can be trapped. We use the Nirvana MHD code with adaptive mesh refinement to study this interaction with high numerical resolution to model cases with confinement parameters up to $10^4$.
A Robust Age Indicator for Old Stellar Populations
Creators: name: Vazdekis, A.
name: Arimoto, N.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We derive new spectral H_gamma index definitions which are robust age indicators for old and relatively old stellar populations and thus have great potential for solving the age-metallicity degeneracy of galaxy spectra. To study H_gamma as a function of age, metallicity and resolution, we used a new spectral synthesis model which predicts SEDs of single-age, single-metallicity stellar populations at resolution FWHM=1.8A (which can be smoothed to different resolutions), allowing direct measurements of the equivalent widths of particular absorption features. We find that the H_gamma strong age disentangling power strongly depends strongly on the adopted resolution and galaxy velocity dispersion. We propose a system of indices which are completely insensitive to metallicity and stable against resolution, allowing the study of galaxies up to ~300 km/s. Observational spectra of very high S/N and relatively high dispersion, are required to gain this unprecedented age discriminating power. Once such spectra are obtained, accurate and reliable estimates for the luminosity-weighted average stellar ages of these galaxies will become possible for the first time, without assessing their metallicities. We measured this index for two globular clusters, a number of low-luminosity elliptical galaxies and a standard S0 galaxy. We find a large spread in the average stellar ages of a sample of low-luminosity ellipticals. In particular these indices yield 4 Gyr for M32, in agreement with the age provided by an extraordinary fit to the full spectrum of this galaxy that we achieve here.
description: 22 pages, 4 figures. ApJ, in press. Models and details can be found at http://www.ioa.s.u-tokyo.ac.jp/~vazdekis/
Precision Light Curves from TESS Full-Frame Images: A Difference Imaging Approach
Creators: name: Oelkers, Ryan J.
name: Stassun, Keivan G.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: The Transiting Exoplanet Survey Satellite (TESS) will observe $\sim$150~million stars brighter than $T_{\rm mag} \approx 16$, with photometric precision from 60~ppm to 3~percent, enabling an array of exoplanet and stellar astrophysics investigations.While light curves will be provided for $\sim$400,000 targets observed at 2-min cadence, observations of most stars will only be provided as full-frame images (FFIs) at 30~min cadence. The TESS image scale of $\sim21$''/pix is highly susceptible to crowding, blending, and source confusion, and the highly spatially variable point spread function (PSF) will challenge traditional techniques, such as aperture and Gaussian-kernel PSF photometry. We use official "End-to-End~6" TESS simulated FFIs to demonstrate a difference image analysis pipeline, using a $δ$-function kernel,that achieves the mission specification noise floor of 60~ppm~hr$^{-1/2}$. We show that the pipeline performance does not depend on position across the field, and only $\sim$2\% of stars appear to exhibit residual systematics at the level of $\sim$5~ppt. We also demonstrate recoverability of planet transits, eclipsing binaries, and other variables. We provide the pipeline as an open-source tool at https://github.com/ryanoelkers/DIA in both IDL and PYTHON. We intend to extract light curves for all point sources in the \textit{TESS} FFIs as soon as they become publicly available, and will provide the light curves through the Filtergraph data visualization service. An example data portal based on the simulated FFIs is available for inspection at https://filtergraph.com/tess_ffi.
description: 11 pages, 4 figures, submitted to AAS journals, comments and suggestions are welcome! Release version 0 of the pipeline can be found at the URL: https://github.com/ryanoelkers/DIA. All data products from this letter, and future data products produced by the pipeline, can be found at the URL: https://filtergraph.com/tess_ffi
Production of Jet Pairs at Large Relative Rapidity in Hadron-Hadron Collisions as a Probe of the Perturbative Pomeron
Creators: name: Stirling, W. J.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The production of jet pairs with small transverse momentum and large relative rapidity in high energy hadron-hadron collisions is studied. The rise of the parton-level cross section with increasing rapidity gap is a fundamental prediction of the BFKL `perturbative pomeron' equation of Quantum Chromodynamics. However, at fixed collider energy it is difficult to disentangle this effect from variations in the cross section due to the parton distributions. It is proposed to study instead the distribution in the azimuthal angle difference of the jets as a function of the rapidity gap. The flattening of this distribution with increasing dijet rapidity gap is shown to be a characteristic feature of the BFKL behaviour. Predictions for the Fermilab proton-antiproton collider are presented.
description: 17 pages, 11 figures, preprint DTP/94/04
Future millimeter, submillimeter and far-infrared surveys and their successful follow up
Creators: name: Blain, Andrew W.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The first unbiased surveys for high-redshift galaxies in the submillimeter (submm) and far-infrared (FIR) wavebands have been made over the last two years. When combined with the intensity of extragalactic background radiation in the same wavebands, we have a reasonable first view of the dust enshrouded Universe. Limited spatial resolution hampers the identification of the submm galaxies, and follow-up observations currently consume much larger amounts of telescope time than the initial submm-wave detections. Here the prospects for future submm/FIR surveys are discussed, highlighting the importance of planning careful multiwaveband radio/submm/FIR observations. These can be used to yield photometric redshift information. Radio observations are vital to give accurate positions for the detected sources.
description: 11 pages, 5 figures, to appear in ASP proceedings `Photometric Redshifts and the detection of high-redshift galaxies' OCIW, April 1999. Revised version is updated and includes minor corrections to Table 1
ESM 1 - Supplementary manuscript from Tasting the unexpected: disconfirmation of expectations leads to lower perceived food value in an invertebrate
Creators: name: F. B. Oberhauser
name: T. J. Czaczkes
Publisher: name: The Royal Society
Year: 2018
Subjects: subject: Ecology
subject: FOS: Biological sciences
subject: 170299 Cognitive Science not elsewhere classified
subject: FOS: Psychology
subject: 60801 Animal Behaviour

description: Detailed description of methods and results and supplementary figures and tables
Can Deflagration-Detonation-Transitions occur in Type Ia Supernovae?
Creators: name: Niemeyer, J. C.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The mechanism for deflagration-detonation-transition (DDT) by turbulent preconditioning, suggested to explain the possible occurrence of delayed detonations in Type Ia supernova explosions, is argued to be conceptually inconsistent. It relies crucially on diffusive heat losses of the burned material on macroscopic scales. Regardless of the amplitude of turbulent velocity fluctuations, the typical gradient scale for temperature fluctuations is shown to be the laminar flame width or smaller, rather than the factor of thousand more required for a DDT. Furthermore, thermonuclear flames cannot be fully quenched in regions much larger than the laminar flame width as a consequence of their simple ``chemistry''. Possible alternative explosion scenarios are briefly discussed.
description: 8 pages, uses aastex; added references. Accepted by ApJ Letters
Accretion in the Early Outer Solar System
Creators: name: Kenyon, Scott J.
name: Luu, Jane X.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We describe calculations of the evolution of an ensemble of small planetesimals in the outer solar system. In a solar nebula with a mass of several times the Minimum Mass Solar Nebula, objects with radii of 100-1000 km can form on timescales of 10-100 Myr. Model luminosity functions derived from these calculations agree with current observations of bodies beyond the orbit of Neptune (Kuiper Belt objects). New surveys with current and planned instruments can place better constraints on the mass and dynamics of the solar nebula by measuring the luminosity function at red magnitudes of 28 or larger.
description: 12 pages of text, 3 tables, 2 figures; accepted for publication in the Astrophysical Journal
Characterization of the regimes of hydrodynamic escape from low-mass exoplanets
Creators: name: Guo, J. H.
Publisher: name: arXiv
Year: 2024
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: The hydrodynamic escape driven by external or internal energy sources sculpts the population of low mass close-in planets. However, distinguishing between the driving mechanisms responsible for the hydrodynamic escape of hydrogen-rich atmospheres is a complex task due to the involvement of many physical factors. My simulations show that the hydrodynamic escape can be driven solely by thermal energy deposited in the lower layers of the atmosphere due to the heat flux originating from the planetary core or bolometric heating from the star even in the absence of other energy sources, as long as the planet's Jeans parameter is below 3. Otherwise, stellar extreme ultraviolet irradiation or tidal forces are necessary in driving the escape, which means that the Jeans parameter is incapable of distinguishing the driving mechanisms, as it is only related to the properties of planet. Here, an upgraded Jeans parameter that takes into account tidal forces is introduced, which allows us to accurately categorize the driving mechanisms. The results show that when the upgraded Jeans parameter falls below 3 or exceeds 6, the atmospheric escape is primarily driven by tidal forces or extreme ultraviolet radiation from the host star, respectively. In the range of 3 to 6, both factors can trigger the escape of the atmosphere. I find that planets with high gravitational potential and low stellar irradiation are more likely to undergo subsonic escape, although transonic escape is prevalent among most planets. Moreover, the ionization status is significantly dependent on the gravitational potential. The upgraded Jeans parameter, which is closely related to the underlying physics, provides a concise method to categorize the driving mechanisms of hydrodynamic escape. The results can be applied to planetary evolution calculations.
description: 44 pages, 10 figures
Additional file 1 of USP29 activation mediated by FUBP1 promotes AURKB stability and oncogenic functions in gastric cancer
Creators: name: Tu, Rongfu
name: Kang, Ye
name: Pan, Yiwen
name: Da, Yanyan
name: Ren, Doudou
name: Zhang, Ru
name: Cai, Zeqiong
name: Liu, Yijia
name: Xu, Jiao
name: Ma, Junpeng
name: Zhou, Zhiyong
name: Yin, Shupeng
name: Li, Xiaozhuang
name: Zhang, Peng
name: Zhang, Qi
name: Wang, Jingchao
name: Lu, Xinlan
name: Zhang, Chengsheng
Publisher: name: figshare
Year: 2024
Subjects: subject: Biophysics
subject: Biochemistry
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Biological Sciences not elsewhere classified
subject: Cancer
subject: Computational Biology

description: Supplementary Material 1
Mya pictorum Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Bivalvia
Myoida
Myidae
Mya
Mya pictorum

description: Mya pictorum [spec. nov.]
M. testa ovata, cardinis dente primario crenulato; laterali longitudinali: alterius duplicato.
Bonan. recr. 2. t. 41.
List. angl. app. t. 1. f. 4.
Habitat in Europae fluviis.
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 671, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
ปัจจัยคุกคามสุขภาพจากการทำงานและภาวะสุขภาพตามความเสี่ยงของคนงานในสถานประกอบการเคาะพ่นสีรถยนต์ อำเภอเมือง จังหวัดพิษณุโลก
Creators: name: ณัชชารี อนงค์รักษ์
Publisher: name: สถาบันวิจัย จัดการความรู้ และมาตรฐานการควบคุมโรค
Year: 2559
Subjects: ปัจจัยคุกคามสุขภาพ
ภาวะสุขภาพ
คนงานเคาะพ่นสีรถยนต์

description: วารสารควบคุมโรค, 42, 3, 255-268
Jets in photon-photon collisions: from TRISTAN to J/N-LC
Creators: name: Aurenche, P.
name: Guillet, J. -Ph.
name: Fontannaz, M.
name: Shimizu, Y.
name: Fujimoto, J.
name: Kato, K.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We study jet production in photon-photon reactions at the next-to-leading logarithm accuracy. Special emphasis is placed on the discussion of the theoretical uncertainties and on the role of the hadronic component of the photon structure function. We also discuss subtleties in the quasi-real photon spectrum when the photon is involved in a large transverse momentum reaction. The phenomenology at TRISTAN energies is discussed and predictions are made for LEP and a $1\ TeV$ \epem collider.
description: 14 + 10 figures included uuencoded tar-compressed (GUILLET@FRCPN11.IN2P3.FR) , KEK-CP-11, LAPP-TH436/93
Quasi-Thermal Comptonization and GRBs
Creators: name: Ghisellini, Gabriele
name: Celotti, Annalisa
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Quasi-thermal Comptonization is an attractive alternative to the synchrotron process to explain the spectra of GRBs, even if we maintain other important properties of the internal shock scenario, implying a compact emitting region and an equipartition magnetic field. Photon-photon absorption and electron-positron pairs can play a crucial role: this process may lock the effective temperature in a narrow range and may be the reason why burst spectra have high energy cut-offs close to the rest mass-energy of the electron. If the progenitors of GRB are hypernovae, the circum-burst matter is dominated by the wind of the pre-hypernova star. The presence of this dense material has strong effects on the generation of the radiation of the burst and its afterglow.
description: 7 pages, contributed paper for the meeting: "Gamma-ray bursts: the first three minutes", Editors: J. Poutanen and R. Svensson
New Galaxies Discovered in the First Blind HI Survey of the Centaurus A Group
Creators: name: Banks, G. D.
name: Disney, M. J.
name: Knezek, P. M.
name: Jerjen, H.
name: Barnes, D.
name: Bhatal, R.
name: de Blok, W. J. G.
name: Boyce, P. J.
name: Ekers, R. D.
name: Freeman, K. C.
name: Gibson, B. K.
name: Henning, P.
name: Kilborn, V.
name: Koribalski, B.
name: Kraan-Korteweg, R. C.
name: Malin, D.
name: Minchin, R. F.
name: Mould, J.
name: Oosterloo, T.
name: Price, R. M.
name: Putman, M. E.
name: Ryder, S. D.
name: Sadler, E. M.
name: Staveley-Smith, L.
name: Stewart, I.
name: Stootman, F.
name: Vaile, R. A.
name: Webster, R.
name: Wright, A. E.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have commenced a 21-cm survey of the entire southern sky (δ< 0 degrees, -1200 km/s < v < 12700 km/s) which is ''blind'', i.e. unbiased by previous optical information. In the present paper we report on the results of a pilot project which is based on data from this all-sky survey. The project was carried out on an area of 600 square degrees centred on the nearby Centaurus A (Cen A) group of galaxies at a mean velocity of v ~ 500 km/s. This was recently the subject of a separate and thorough optical survey. We found 10 new group members to add to the 21 galaxies already known in the Cen A group: five of these are previously uncatalogued galaxies, while five were previously catalogued but not known to be associated with the group. We found optical counterparts for all the HI detections, most of them intrinsically very faint low surface brightness dwarfs. The new group members add approximately 6% to the HI mass of the group and 4% to its light. The HI mass function, derived from all the known group galaxies in the interval 10^7 \Msun of HI to 10^9 \Msun of HI, has a faint-end slope of 1.30 +/- 0.15, allowing us to rule out a slope of 1.7 at 95% confidence. Even if the number in the lowest mass bin is increased by 50%, the slope only increases to 1.45 +/- 0.15.
description: 19 pages Latex, 6 figures (Fig. 2 in four parts, Fig.5 in two parts). To appear in The Astrophysical Journal (Vol. 524, October 1999)
Soil properties, crop productivity and energetics under different tillage practices in fodder sorghum + cowpea – wheat cropping system
Creators: name: Anoop Kumar Dixit
name: Agrawal, Rajiv Kumar
name: Sanjoy Kumar Das
name: Sahay, Chandra Shekhar
name: Choudhary, Mukesh
name: Rai, Arvind Kumar
name: Kumar, Sunil
name: Kantwa, Sita Ram
name: Palsaniya, Dana Ram
Publisher: name: Taylor & Francis
Year: 2018
Subjects: 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: Ecology
subject: FOS: Biological sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: Plant Biology

description: Tillage is an important agricultural operation which influences soil properties, crop yield and environment. Nine combinations of three tillage practices including conventional tillage (CT), minimum tillage (MT) and zero tillage (ZT) were evaluated in fodder sorghum (Sorghum bicolor) + cowpea (Vigna unguiculata) – wheat (Triticum durum) cropping system for 5 years (2009–2014) on clay loam soil under limited irrigation. Continuous ZT practices significantly improved surface soil organic carbon, bulk density, infiltration rate and maximum water holding capacity. Carbon sequestration rate, soil organic carbon stock and soil enzymatic activities were relatively more under ZT than CT-CT practice. Higher fodder yield of sorghum + cowpea was recorded with CT (kharif) while wheat grain yield with ZT (rabi). However, the system productivity was statistically similar in all the tillage treatments on pooled data basis. The economic benefits were also maximum under ZT-ZT practice. The ZT-ZT practice recorded significantly lowest energy input (17.1 GJ ha−1) which resulted in highest energy use efficiency (13.6) and energy productivity (518 kg GJ−1). Thus, adoption of ZT significantly improved soil health, stabilized crop yield, increased profitability and energy use efficiency in the semi-arid agro-ecosystem.
Mya margaritifera Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Bivalvia
Myoida
Myidae
Mya
Mya margaritifera

description: Mya margaritifera [spec. nov.]
M. testa ovata antice coarctata, cardinis dente primario conico, natibus decorticatis.
Fn. svec. 1331.
List. conch. t. 149. f. 4.
angl. app. 15. t. 1. f. 1.
Klein. ostr. t. 10. f. 47.
Habitat in totius orbis arctici cataractis.
Testa ovali-oblonga, ponderosa, antice retuso compressa, extus rudis nigricans, latere angustiore s. superiore subvillosa, Natibus valde excorticatis, per siccitatem fragilis etiam per se. Intus Testa albida cicatricibus duabus pro insertione musculorum. Cardinis Dens conicus, obtusus, porrectus, lateralis nullus; sed in minoribus longitudinalis crenulatus; an vero minor specie diversa?
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 671, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Stability of the Broad Line Region Geometry and Dynamics in Arp 151 Over Seven Years
Creators: name: Pancoast, A.
name: Barth, A. J.
name: Horne, K.
name: Treu, T.
name: Brewer, B. J.
name: Bennert, V. N.
name: Canalizo, G.
name: Gates, E. L.
name: Li, W.
name: Malkan, M. A.
name: Sand, D.
name: Schmidt, T.
name: Valenti, S.
name: Woo, J. H.
name: Clubb, K. I.
name: Cooper, M. C.
name: Crawford, S. M.
name: Honig, S. F.
name: Joner, M. D.
name: Kandrashoff, M. T.
name: Lazarova, M.
name: Nierenberg, A. M.
name: Romero-Colmenero, E.
name: Son, D.
name: Tollerud, E.
name: Walsh, J. L.
name: Winkler, H.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The Seyfert 1 galaxy Arp 151 was monitored as part of three reverberation mapping campaigns spanning $2008-2015$. We present modeling of these velocity-resolved reverberation mapping datasets using a geometric and dynamical model for the broad line region (BLR). By modeling each of the three datasets independently, we infer the evolution of the BLR structure in Arp 151 over a total of seven years and constrain the systematic uncertainties in non-varying parameters such as the black hole mass. We find that the BLR geometry of a thick disk viewed close to face-on is stable over this time, although the size of the BLR grows by a factor of $\sim 2$. The dynamics of the BLR are dominated by inflow and the inferred black hole mass is consistent for the three datasets, despite the increase in BLR size. Combining the inference for the three datasets yields a black hole mass and statistical uncertainty of $\log_{10}($M$_{\rm BH}/\rm{M}_{\odot})=6.82^{+0.09}_{-0.09}$ with a standard deviation in individual measurements of 0.13 dex.
description: 21 pages, 8 figures, 2 tables. Accepted for publication in ApJ
Reaction pathways and overpotential in the cathode
Creators: name: Bhowmik, Arghya
name: Lastra, Juan María García
Publisher: name: Zenodo
Year: 2019
Subjects: Sulfur, Sulphur, Battery, Aluminium, reaction pathways

description: Report on the computation modelling of the formation of aluminum polysulfides during the charge and discharge of the battery, identifying the reaction pathways and the corresponding overpotentials
Bright single InAsP quantum dots at telecom wavelengths in position-controlled InP nanowires: the role of the photonic waveguide
Creators: name: Haffouz, Sofiane
name: Dalacu, Dan
name: Poole, Philip J.
name: Lapointe, Jean
name: Poitras, Daniel
name: Mnaymneh, Khaled
name: Wu, Xiaohua
name: Korkusinski, Marek
name: Williams, Robin L.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: We report on the site-selected growth of bright single InAsP quantum dots embedded within InP photonic nanowire waveguides emitting at telecom wavelengths. We demonstrate a dramatic dependence of the emission rate on both the emission wavelength and the nanowire diameter. With an appropriately designed waveguide, tailored to the emission wavelength of the dot, an increase in count rate by nearly two orders of magnitude (0.4kcps to 35kcps) is obtained for quantum dots emitting in the telecom O-band. Using emission-wavelength-optimised waveguides, we demonstrate bright, narrow linewidth emission from single InAsP quantum dots with an unprecedented tuning range from 880nm to 1550nm. These results pave the way towards efficient single photon sources at telecom wavelengths using deterministically grown InAsP/InP nanowire quantum dots.
Facile synthesis and fractal feature of pH-responsive poly(acrylic acid) hollow microspheres for ibuprofen delivery
Creators: name: Wang, Qian
name: Jin, Xiao Qi
name: Sun, Ji Hong
name: Bai, Shi Yang
name: Wu, Xia
name: Panezai, Hamida
Publisher: name: Taylor & Francis
Year: 2017
Subjects: subject: Biophysics
subject: Biochemistry
subject: Space Science
subject: Physical Sciences not elsewhere classified
subject: Medicine
subject: Pharmacology
subject: Biotechnology
subject: Chemical Sciences not elsewhere classified
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: The pH-responsive hollow poly(acrylic acid) (HPAA) microspheres with regulated cavity structure and various shell thicknesses were synthesized. Their structural parameters and textural properties were characterized by various techniques. The ibuprofen loading results indicate the good drug loading capabilities of HPAA microspheres from 13.81 to 17.18%. Their ibuprofen release properties demonstrated their good pH sensitivity and distance-controlled drug diffusion process. Specially, the small-angle X-ray scattering technique was used to suggest the surface roughness and structural irregularities of HPAA before and after drug loading and releasing. These findings clearly indicate the potential of HPAA microspheres to be used as promising candidates in drug delivery.
Sidorenko's conjecture for blow-ups
Creators: name: Conlon, David
name: Lee, Joonkyung
Publisher: name: arXiv
Year: 2018
Subjects: subject: Combinatorics (math.CO)
subject: FOS: Mathematics

description: A celebrated conjecture of Sidorenko and Erdős-Simonovits states that, for all bipartite graphs $H$, quasirandom graphs contain asymptotically the minimum number of copies of $H$ taken over all graphs with the same order and edge density. This conjecture has attracted considerable interest over the last decade and is now known to hold for a broad range of bipartite graphs, with the overall trend saying that a graph satisfies the conjecture if it can be built from simple building blocks such as trees in a certain recursive fashion. Our contribution here, which goes beyond this paradigm, is to show that the conjecture holds for any bipartite graph $H$ with bipartition $A \cup B$ where the number of vertices in $B$ of degree $k$ satisfies a certain divisibility condition for each $k$. As a corollary, we have that for every bipartite graph $H$ with bipartition $A \cup B$, there is a positive integer $p$ such that the blow-up $H_A^p$ formed by taking $p$ vertex-disjoint copies of $H$ and gluing all copies of $A$ along corresponding vertices satisfies the conjecture. Another way of viewing this latter result is that for every bipartite $H$ there is a positive integer $p$ such that an $L^p$-version of Sidorenko's conjecture holds for $H$.
description: Reformatted for Discrete Analysis
Regimes and quantum bounds of nanoscale thermoelectrics with peaked transmission function
Creators: name: Bevilacqua, Giuseppe
name: Cresti, Alessandro
name: Grosso, Giuseppe
name: Menichetti, Guido
name: Parravicini, Giuseppe Pastori
Publisher: name: arXiv
Year: 2018
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: Based on the Landauer-Büttiker theory, we explore the thermal regimes of two-terminal nanoscale systems with an energy-peaked transmission function. The device is in contact with two reservoirs held at different temperatures and chemical potentials. We identify the operation regions where the system acts as energy pump (thermal machine) or heat pump (refrigerator machine), or where it is working in dissipative modes. The corresponding thermoelectric parameters are obtained without numerical calculations. The recent literature, by focusing on systems with box-like or step-like shapes of the transmission functions, demonstrated that bounds of quantum origin exist for output power and heat currents of thermal machines and refrigerators. The simple model we adopt in this paper allows us to grasp easily and without numerical calculations the presence of quantum bounds for the above thermoelectric quantities, as function of the position of the transmission peak with respect to the chemical potentials of the left and right reservoirs. In spite of the simple model and treatment, our results are in qualitative agreement with analytic findings in previous researches obtained with more realistic description of the electronic transmission function.
description: 6 figures
title: ADCO, Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome VI, Cart. 190 (11 H 75), 316 folios, f. 0177v
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2012
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire

description: Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome VI, Archives départementales de la Côte-d'Or, Cart. 190 (11 H 75), 316 folios, f. 0177v, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome VI, Archives départementales de la Côte-d'Or, Cart. 190 (11 H 75), 316 folios, f. 0177v, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
High energy scattering in 2+1 QCD
Creators: name: Li, Miao
name: Tan, Chung-I
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: High energy scattering in 2+1 QCD is studied using the recent approach of Verlinde and Verlinde. We calculate the color singlet part of the quark-quark scattering exactly within this approach, and discuss some physical implication of this result. We also demonstrate, by two independent methods, that reggeization fails for the color singlet channel. We briefly comment on the problem in 3+1 QCD.
description: 20 pages, references added
Reducing the variance in the translocation times by pre-stretching the polymer
Creators: name: de Haan, Hendrick W.
name: Sean, David
name: Slater, Gary W.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: Langevin Dynamics simulations of polymer translocation are performed where the polymer is stretched via two opposing forces applied on the first and last monomer before and during translocation. In this setup, polymer translocation is achieved by imposing a bias between the two pulling forces such that there is net displacement towards the \textit{trans}-side. Under the influence of pre-stretching forces, the elongated polymer ensemble contains less variations in conformations compared to an unstretched ensemble. Simulations demonstrate that this reduced spread in initial conformations yields a reduced variation in translocations times relative to the mean translocation time. This effect is explored for different ratios of the amplitude of thermal fluctuations to driving forces to control for the relative influence of the thermal path sampled by the polymer. Since the variance in translocation times is due to contributions coming from sampling both thermal noise and initial conformations, our simulations offer independent control over the two main sources of noise, and allow us to shed light on how they both contribute to translocation dynamics. Experimentally relevant conditions are highlighted and shown to correspond to a significant decrease in the spread of translocation times, thus indicating that stretching DNA prior to translocation could assist in nanopore-based sequencing and sizing applications.