cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Dynamical calculation of $d^*$ mass and NN decay width in the quark delocalization, color screening model
Creators: name: Ping, Jialun
name: Wang, Fan
name: Goldman, T.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: The mass estimate of the $d^* (IJ^P=03^+)$ dibaryon is improved by a dynamical calculation in the quark delocalization, color screening model. The partial decay width of $d^*$ into an $NN$ D-wave state is also obtained. The mass obtained is slightly larger than that obtained in adiabatic calculations, due to the anharmonicity of the effective potential between two $Δ$'s. The value of the width obtained due to tensor one-gluon-exchange is about 5 MeV, comparable in magnitude to earlier results found using pion exchange.
description: 11 pages, no figures, additional references
Hydrodynamic limit of boundary driven exclusion processes with nonreversible boundary dynamics
Creators: name: Erignoux, Clément
Publisher: name: arXiv
Year: 2017
Subjects: subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: Using duality techniques, we derive the hydrodynamic limit for one-dimensional, boundary-driven, symmetric exclusion processes with different types of non-reversible dynamics at the boundary, for which the classical entropy method fails.
WS_ Value Sensitive Design for Clinical Dashboard in the Medical Context
Creators: name: ACM TVX2018
name: Jinah Su
name: Jieun Han
name: Kwon, Gyu Hyun
Publisher: name: figshare
Year: 2018
Subjects: subject: 80602 Computer-Human Interaction
subject: FOS: Psychology

description: When you visualize medical information, which value would be important and how could we adopt these values to UI/UX design?We attempted to answer these questions by designing the clinical dashboard for general hospital use in South Korea. After conducting an evaluation via Focus Group Interview, user testing, and video analysis of the original demo version, we decided to implement a more systematic approach to identify weak points using a value-sensitive design. Using this method, we were able to minimize the potential exposure of sensitive information and avoid overloading the user with too much information. The potential achievement of such results suggests a practical way of optimizing the design of clinical dashboard while highlighting the value of a systematic approach to satisfying design requirements. This examination of the current version of clinical dashboards indicates the need to conduct further detailed research studies to verify their efficacy and establish more stringent design guidelines.
Additional file 5 of Multi-locus phylogeny and taxonomy of an unresolved, heterogeneous species complex within the genus Golovinomyces (Ascomycota, Erysiphales), including G. ambrosiae, G. circumfusus and G. spadiceus
Creators: name: Qiu, Peng-Lei
name: Liu, Shu-Yan
name: Bradshaw, Michael
name: Rooney-Latham, Suzanne
name: Takamatsu, Susumu
name: Bulgakov, Timur
name: Tang, Shu-Rong
name: Feng, Jing
name: Jin, Dan-Ni
name: Aroge, Temitope
name: Li, Yu
name: Wang, Li-Lan
name: Braun, Uwe
Publisher: name: figshare
Year: 2020
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Evolutionary Biology
subject: Environmental Sciences not elsewhere classified
subject: Ecology
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Plant Biology

description: Additional file 5: Figure S5. Phylogenetic analysis of the CHS1 region of the Golovinomyces ambrosiae complex and G. circumfusus. The tree was constructed based on 49 sequences from tribe Golovinomyceteae. Three sequences from NeoÃ«rysiphe galeopisidis (accession numbers: MK452438, MK452439, MK452440) was used as an outgroup. Bootstrap values based on 1000 replications are indicated above/below the branches.
D2.3 - Methodological guidelines
Creators: name: González-Martínez, Ana
name: Jongeneel, Roel
name: van Asseldonk, Marcel
name: Witzke, Peter
name: Salputra, Guna
name: Havlík, Petr
name: Arbelaez-Gaviria, Juliana
name: Donnellan, Trevor
name: Erjavec, Emil
Publisher: name: Zenodo
Year: 2024

description: Deliverable 2.3 aims at encouraging end users to apply modelling tools during the design and implementation of the CAP Strategic Plans (CSPs). More specifically, the concept ‘modelling tools’ refers to a set of mathematical/econometric models and methodologies for analysis to carry out ex-ante and ex-post evaluations of the CAP, generating quantitative evidence based on statistical data. Ex-ante analysis refers to those cases in which tools are employed before policy implementation and are instrumental in evaluating potential outcomes, benefits, and risks associated with various policy options. In contrast, ex-post analysis tools are used for evaluating and comparing past experiences or similar experiences from other contexts and assess outcomes under various policies and policy mixes. These methodological guidelines capture the general (and practical) aspects to keep in mind when considering their use for policy assessment
Extended Two--Particle Green's Functions and Optical Potentials for Two--Particle Scattering by Many--Body Targets
Creators: name: Brand, Joachim
name: Cederbaum, Lorenz S.
Publisher: name: arXiv
Year: 1996
Subjects: subject: Chemical Physics (physics.chem-ph)
subject: Atomic Physics (physics.atom-ph)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: An extension of the fermionic particle--particle propagator is presented, that possesses similar algebraic properties to the single--particle Green's function. In particular, this extended two--particle Green's function satisfies Dyson's equation and its self energy has the same analytic structure as the the self energy of the single--particle Green's function. For the case of a system interacting by one--particle potentials only, the two--particle self energy takes on a particularly simple form, just like the common self energy does. The new two--particle self energy also serves as a well behaved optical potential for the elastic scattering of a two--particle projectile by a many--body target. Due to its analytic structure, the two--particle self energy avoids divergences that appear with effective potentials derived by other means.
description: 17 pages of LaTeX, no figures, submitted to Annals of Physics (N. Y.)
Precise design of highly isoform-selective p21-activated kinase 4 inhibitors: computational insights into the selectivity mechanism through molecular dynamics simulation and binding free energy calculation
Creators: name: Su, Yuan
name: Song, Peilu
name: Wang, Hanxun
name: Hu, Baichun
name: Wang, Jian
name: Cheng, Mao-Sheng
Publisher: name: Taylor & Francis
Year: 2019
Subjects: subject: Biophysics
subject: Biochemistry
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Chemical Sciences not elsewhere classified
subject: Biological Sciences not elsewhere classified
subject: Information Systems not elsewhere classified
subject: Cancer
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Virology

description: Understanding the selectivity mechanisms of inhibitors towards highly similar protein kinases is the first step in discovering new selective candidate for satisfactory safety profile. P21-activated kinases (PAKs) are pertain to a family of serine/threonine (Ser/Thr) protein kinases, which are the first Rho family GTPase-regulated kinases identified and served as important downstream mediators of Ras-Rac and Cdc42 function. Among PAKs, PAK4 is emerging as a promising target for cancer treatment. Since the PAK2 inhibition correlates with increased acute cardiovascular toxicity, which may be enhanced by PAK1 inhibitor, selective inhibition of PAK4 over PAK1 is crucial in discovering safe anticancer candidates with optimal therapeutic efficacy. While the conserved ATP-binding pockets of both PAK1/4 make it challenging to discriminating selective inhibitors between PAK1 and PAK4, thus the selectivity mechanism of PAK1/4 inhibitors will be explored in this present study through, computational strategies which combine molecular docking, structural comparison, molecular dynamics simulation and molecular mechanics/generalized Born surface area calculation. The research would provide valuable insight into the selectivity mechanism of PAK4 inhibitors over PAK1 and thus be helpful for designing selective PAK4 inhibitors. Communicated by Ramaswamy H. Sarma
Characterizations of topological superconductors: Chern numbers, edge states and Majorana zero modes
Creators: name: Liu, Xiao-Ping
name: Zhou, Yuan
name: Wang, Yi-Fei
name: Gong, Chang-De
Publisher: name: arXiv
Year: 2017
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: The topological properties in topological superconductors are usually characterized by the bulk Chern numbers, edge-state spectra, and Majorana zero modes. Whether they are equivalent or inequivalent is not well understood. Here, we investigate this issue with focus on a checkerboard-lattice model combining the Chern insulator and chiral $p$-wave superconductivity. Multiple topologically superconducting phases with Chern numbers up to $\mathcal{N}=4$ are produced. We explicitly demonstrate the mismatch between the Chern numbers, edge states and Majorana zero modes in this two-dimensional topological-superconductor model. The intrinsic reason is that some edge states in the superconducting phases inherited from the Chern-insulator phase are not protected by the particle-hole symmetry. We further check the mismatches in vortex states. Our results therefore clarify these different but complementary topological features and suggest that further considerations are required to characterize various topological superconductors.
description: 14 pages, 5 figures
title: Universalist children’s services. From two-part to inclusive social infrastructure
Creators: name: Thalheim, Vinzenz
Publisher: name: Universität Kassel
Year: 2024
Subjects: subject: Stigma
subject: (Targeted) family support
subject: Social work
subject: Inclusion
subject: Goffman
subject: 300
subject: Sozialarbeit
subject: Soziale Infrastruktur
subject: Stigmatisierung
subject: Inklusion
subject: Kinderbetreuung

description: Gefördert im Rahmen des Projekts DEAL
Large Nuclear shape transition at finite temperature in a relativistic mean field approach
Creators: name: Agrawal, B. K.
name: Sil, Tapas
name: De, J. N.
name: Samaddar, S. K.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: The relativistic Hartree-BCS theory is applied to study the temperature dependence of nuclear shape and pairing gap for $^{166}Er$ and $^{170}Er$. For both the nuclei, we find that as temperature increases the pairing gap vanishes leading to phase transition from superfluid to normal phase as is observed in nonrelativistic calculation. The deformation evolves from prolate shapes to spherical shapes at $T\sim 2.7$ MeV. Comparison of our results for heat capacity with the ones obtained in the non-relativistic mean field framework indicates that in the relativistic mean field theory the shape transition occurs at a temperature about 0.9 MeV higher and is relatively weaker. The effect of thermal shape fluctuations on the temperature dependence of deformation is also studied. Relevant results for the level density parameter are further presented. PACS numbers: 21.10.Ma, 21.60.-n, 27.70.+q
description: ReVtex file of 17 pages, 11 ps files for figures, To be appear in Phys. ReV. C
title: ESLO1: interview de personnalité 427_A
Creators: name: Laboratoire Ligérien De Linguistique
name: Baude, Olivier
name: Dugua, Céline
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2015
Subjects: subject: Français
subject: fra
subject: text_and_corpus_linguistics

description: Extrait du corpus d'Orléans, réalisé dans le cadre de l'Enquête SocioLinguistique à Orléans à la fin des années 1960.
description: Conforms to: doi:10.34847/cocoon.69c4fa74-f324-3ddb-9f1a-580867fd5826
Spectroscopic confirmation and velocity dispersions for twenty Planck galaxy clusters at 0.16
Creators: name: Amodeo, S.
name: Mei, S.
name: Stanford, S. A.
name: Lawrence, C. R.
name: Bartlett, J. G.
name: Stern, D.
name: Chary, R. -R.
name: Shim, H.
name: Marleau, F.
name: Melin, J. -B.
name: Rodríguez-Gonzálvez, C.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We present Gemini and Keck spectroscopic redshifts and velocity dispersions for twenty clusters detected via the Sunyaev-Zel'dovich (SZ) effect by the Planck space mission, with estimated masses in the range $2.3 \times 10^{14} M_{\odot} < M < 9.4 \times 10^{14} M_{\odot}$. Cluster members were selected for spectroscopic follow-up with Palomar, Gemini and Keck optical and (in some cases) infrared imaging. Seven cluster redshifts were measured for the first time with this observing campaign, including one of the most distant Planck clusters confirmed to date, at $z=0.782\pm0.010$, PSZ2 G085.95+25.23. The spectroscopic redshift catalogs of members of each confirmed cluster are included as on-line tables. We show the galaxy redshift distributions and measure the cluster velocity dispersions. The cluster velocity dispersions obtained in this paper were used in a companion paper to measure the Planck mass bias and to constrain the cluster velocity bias.
description: 17 pages including appendices, ApJ in press
title: ESLO1: interview de personnalité 431_A
Creators: name: Laboratoire Ligérien De Linguistique
name: Baude, Olivier
name: Dugua, Céline
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2015
Subjects: subject: Français
subject: fra
subject: text_and_corpus_linguistics

description: Extrait du corpus d'Orléans, réalisé dans le cadre de l'Enquête SocioLinguistique à Orléans à la fin des années 1960.
description: Conforms to: doi:10.34847/cocoon.69c4fa74-f324-3ddb-9f1a-580867fd5826
A local anharmonic treatment of vibrations of methane
Creators: name: Lemus, R.
name: Perez-Bernal, F.
name: Frank, A.
name: Bijker, R.
name: Arias, J. M.
Publisher: name: arXiv
Year: 1996
Subjects: subject: Chemical Physics (physics.chem-ph)
subject: FOS: Physical sciences

description: The stretching and bending vibrations of methane are studied in a local anharmonic model of molecular vibrations. The use of symmetry-adapted operators reduces the eigenvalue problem to block diagonal form. For the 44 observed energies we obtain a fit with a standard deviation of 0.81 cm$^{-1}$ (and a r.m.s. deviation of 1.16 cm$^{-1}$).
description: revised and updated version: 13 pages, 3 tables, Revista Mexicana de Fisica, in press
Study on mangrove associated estuarine waters of Northeastern Bay of Bengal reveals potential diatom indicators of dissolved inorganic compounds
Creators: name: Mukherjee, Dr. Abhishek
Publisher: name: figshare
Year: 2021
Subjects: subject: Ecology
subject: FOS: Biological sciences
subject: Environmental Science
subject: Limnology
subject: 40501 Biological Oceanography
subject: FOS: Earth and related environmental sciences

description: An extensive study (2011 and 2012) was performed to narrow down certain diatom species with bioindicator potentials of highly dynamic and well mixed tropical estuary. The Hooghly Estuary in the Northeastern coast of Bay of Bengal was chosen as the study sites. The comparison between mangrove impoverished and mangrove dominated estuarine rivers revealed intriguing variation in the phytoplankton species composition in response to the dissolved nitrate, phosphate and silicate concentrations, thus forming the kernel of the study by focusing on certain species with greater abundances pointing to their better adaptability and responsiveness to biotic/abiotic parameters in a well mixed estuary. Coscinodiscus hyalinus, Coscinodiscus radiatus, Lioloma elongata, Skeletonema costatum, Synedra crystallinum, Thalassionema frauenfeldtii and Thalassionema nitzschioides have expressed better as bioindicators.
Human Mobility: Models and Applications
Creators: name: Barbosa-Filho, Hugo
name: Barthelemy, Marc
name: Ghoshal, Gourab
name: James, Charlotte R.
name: Lenormand, Maxime
name: Louail, Thomas
name: Menezes, Ronaldo
name: Ramasco, José J.
name: Simini, Filippo
name: Tomasini, Marcello
Publisher: name: arXiv
Year: 2017
Subjects: subject: Physics and Society (physics.soc-ph)
subject: FOS: Physical sciences

description: Recent years have witnessed an explosion of extensive geolocated datasets related to human movement, enabling scientists to quantitatively study individual and collective mobility patterns, and to generate models that can capture and reproduce the spatiotemporal structures and regularities in human trajectories. The study of human mobility is especially important for applications such as estimating migratory flows, traffic forecasting, urban planning, and epidemic modeling. In this survey, we review the approaches developed to reproduce various mobility patterns, with the main focus on recent developments. This review can be used both as an introduction to the fundamental modeling principles of human mobility, and as a collection of technical methods applicable to specific mobility-related problems. The review organizes the subject by differentiating between individual and population mobility and also between short-range and long-range mobility. Throughout the text the description of the theory is intertwined with real-world applications.
description: 126 pages, 45+ figures
title: ESLO1: interview de personnalité 429_A
Creators: name: Laboratoire Ligérien De Linguistique
name: Baude, Olivier
name: Dugua, Céline
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2015
Subjects: subject: Français
subject: fra
subject: text_and_corpus_linguistics

description: Extrait du corpus d'Orléans, réalisé dans le cadre de l'Enquête SocioLinguistique à Orléans à la fin des années 1960.
description: Conforms to: doi:10.34847/cocoon.69c4fa74-f324-3ddb-9f1a-580867fd5826
Additional file 5 of Recombinant Klotho protein enhances cholesterol efflux of THP-1 macrophage-derived foam cells via suppressing Wnt/β-catenin signaling pathway
Creators: name: Liu, Wei
name: Chen, Xiujuan
name: Wu, Min
name: Li, Lin
name: Liu, Jiani
name: Shi, Jing
name: Hong, Tian
Publisher: name: figshare
Year: 2020
Subjects: subject: Biochemistry
subject: Medicine
subject: Cell Biology
subject: Molecular Biology
subject: Biological Sciences not elsewhere classified
subject: Information Systems not elsewhere classified
subject: Developmental Biology
subject: Cancer
subject: Infectious Diseases
subject: FOS: Health sciences

description: Additional file 5: Figure S5. Unprocessed original scans for the blots.
Application of rotating packed bed for in-line aroma stripping from cell slurry
Creators: name: Lukin, Ilya
name: Wingartz, Isabell
name: Schembecker, Gerhard
Publisher: name: TU Dortmund
Year: 2020
Subjects: subject: Rotating packed bed
subject: Natural aromas
subject: In-line stripping
subject: Downstream processing
subject: Cell viability
subject: 660
subject: Stoffübertragung
subject: Bioreaktor
subject: Aromatische Verbindungen
subject: Produktaufarbeitung
subject: Saccharomyces cerevisiae

description: BACKGROUND Nowadays, biotechnological production receives increasing interest as an alternative source of natural aromas. Unfortunately, especially for hydrophobic and semi-volatile aromas, the heterogeneous product partitioning between all phases present in fermentation makes recovery challenging. Additionally, when an aroma displays an inhibitory effect on the production microorganism, product removal during fermentation is recommendable. In-line aroma stripping offers an elegant way to deal with such challenges. This study reports the use of rotating packed bed (RPB) technology for the intensification of stripping of α-ionone, a key aroma of raspberry, from a model fermentation slurry containing Saccharomyces cerevisiae cells in a concentration of 250 g-CWW L−1. RESULTS Throughout all experimental investigations, yeast cells were robust towards both the chemical stress from aroma exposure at a concentration of up to 400 mg L−1 and the mechanical stress from peripheral equipment and rotation of up to 2750 rpm, as a maximum of 11.3 ± 0.5% disrupted cells were measured during continuous processing in an RPB. An increase in the rotation speed led to an enhanced transfer of α-ionone from the fermentation slurry to the gaseous phase. CONCLUSIONS RPB technology is found to be promising for the intensification of in-line stripping of biotechnologically produced aromas from crude fermentation broth without cell separation. The use of subsequent RPBs equipped with custom packings and flexibly adjustable rotation speed displays a holistic aroma recovery process supporting the way to commercial competitiveness of biotechnological aromas. © 2020 The Authors. Journal of Chemical Technology & Biotechnology published by John Wiley & Sons Ltd on behalf of Society of Chemical Industry.
description: Journal of chemical technology and biotechnology;Vol. 95. 2020, issue 11, pp 2834-2841
Partial wave contributions to the antikaon potential at finite momentum
Creators: name: Tolos, Laura
name: Ramos, Angels
name: Polls, Artur
name: Kuo, Thomas T. S.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: The momentum dependence of the antikaon optical potential in nuclear matter is obtained from a microscopic and self-consistent calculation using the meson-exchange Jülich $\bar{K}N$ interaction. Two self-consistent schemes are discussed, which would lead to substantially different predictions for the width of ${\bar K}$ nuclear bound states. The effect of higher partial waves of the $\bar{K}N$ interaction, beyond the L=0 component, is studied and found to have moderate but non-negligible effects on the ${\bar K}$ nuclear potential at zero momentum. At momenta as large as 500 MeV/c, relevant in the analysis of heavy-ion collisions, the higher partial partial waves modify the ${\bar K}$ optical potential by nearly a factor of two.
description: 20 pages, 7 figures
Dust Growth in ALMA Rings: II. Dusty Rossby Wave Instability
Creators: name: Cui, Can
name: Gerbig, Konstantin
name: Li, Ya-Ping
name: Xu, Ziyan
name: Li, Rixin
name: Yu, Cong
name: Lin, Min-Kai
name: Yuan, Feng
Publisher: name: arXiv
Year: 2025
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Annular substructures serve as ideal venues for planetesimal formation. In this series, we investigate the linear stage of dust growth within rings. The first paper examines the global streaming instability, while this study focuses on the dusty Rossby wave instability (DRWI). We perform a linear analysis of the two-fluid equations on a background pressure bump, representing annular substructures. The spectral code \textsc{Dedalus} is used to solve the linear eigenvalue problem. We identify two distinct DRWI modes: Type I, which originates from dust-modified gas RWI, and Type II, which results from dust-gas coupling. These modes never coexist for a given azimuthal wavenumber $\ky$, but transition between each other as $\ky$ varies. Type I modes are driven by the advection of background vorticity, whereas Type II modes involve two primary waves: Rossby waves, driven by advection, and thin waves, driven by dust-gas drag. Finally, we assess the relevance of DRWI in ALMA rings using DSHARP sources. Our findings suggest that Type I modes could explain the absence of azimuthal asymmetries in many ALMA disks, whereas Type II modes are entirely absent in all eight observed rings, implying that unresolved narrow rings or alternative mechanisms may play a role in dust growth within annular substructures.
description: 24 pages, 15 figures, accepted to ApJ, DOI: 10.3847/1538-4357/add146
title: Affiche Journée d'études "Carrières d’images. Ce qu’archives et albums font à la photographie"
Creators: name: Pôle Images Et Sons, Collège Post-Doctoral LabexMed, IDEMEC (UMR 7307), TELEMME (UMR 7303)
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020

description: Journée d'études proposée dans le cadre des activités scientifiques des Post-doctorants.
Additional file 6 of Recombinant Klotho protein enhances cholesterol efflux of THP-1 macrophage-derived foam cells via suppressing Wnt/β-catenin signaling pathway
Creators: name: Liu, Wei
name: Chen, Xiujuan
name: Wu, Min
name: Li, Lin
name: Liu, Jiani
name: Shi, Jing
name: Hong, Tian
Publisher: name: figshare
Year: 2020
Subjects: subject: Biochemistry
subject: Medicine
subject: Cell Biology
subject: Molecular Biology
subject: Biological Sciences not elsewhere classified
subject: Information Systems not elsewhere classified
subject: Developmental Biology
subject: Cancer
subject: Infectious Diseases
subject: FOS: Health sciences

description: Additional file 6: Figure S6. Unprocessed original scans for the blots.
The protoplanetary system HD 100546 in H$α$ polarized light from SPHERE/ZIMPOL. A bar-like structure across the disk gap?
Creators: name: Mendigutía, I.
name: Oudmaijer, R. D.
name: Garufi, A.
name: Lumsden, S. L.
name: Huélamo, N.
name: Cheetham, A.
name: de Wit, W. J.
name: Norris, B.
name: Olguin, F. A.
name: Tuthill, P.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: HD 100546 is one of the few known pre-main-sequence stars that may host a planetary system in its disk. We analyze new VLT/SPHERE/ZIMPOL polarimetric images of HD 100546 with filters in H$α$ and the adjacent continuum. We have probed the disk gap and the surface layers of the outer disk, covering a region < 500 mas (< 55 au at 109 pc) from the star, at an angular resolution of ~ 20 mas. Our data show an asymmetry: the SE and NW regions of the outer disk are more polarized than the SW and NE. This can be explained from a preferential scattering angle close to 90$^o$, consistent with previous polarization images. The outer disk extends from 13 $\pm$ 2 to 45 $\pm$ 9 au, with a position angle and inclination of 137 $\pm$ 5$^o$ and 44 $\pm$ 8$^o$. The comparison with previous estimates suggests that the disk inclination could increase with the stellocentric distance, although the different measurements are still consistent within the error bars. In addition, no direct signature of the innermost candidate companion is detected from polarimetry, confirming recent results based on intensity imagery. We set an upper limit to its mass accretion rate < 10$^{-8}$ M$_{\odot}$/yr for a sub-stellar mass of 15M$_{Jup}$. Finally, we report the first detection (> 3$σ$) of a ~ 20 au bar-like structure that crosses the gap through the central region of HD 100546. It is tentatively suggested that the bar could be dust dragged by infalling gas that radially flows from the outer disk. This could represent an exceptional case in which a small-scale radial inflow is observed in a single system. If this scenario is confirmed, it could explain the presence of atomic gas in the inner disk that would otherwise accrete on to the central star on a timescale of a few months/years, as previously indicated from spectro-interferometric data, and could be related with additional (undetected) planets.
description: 8 pages, 7 figures. Accepted in A&A
$ΔI=4$ and $ΔI=8$ bifurcations in rotational bands of diatomic molecules
Creators: name: Bonatsos, Dennis
name: Daskaloyannis, C.
name: Lalazissis, G. A.
name: Drenska, S. B.
name: Minkov, N.
name: Raychev, P. P.
name: Roussev, R. P.
Publisher: name: arXiv
Year: 1996
Subjects: subject: Chemical Physics (physics.chem-ph)
subject: FOS: Physical sciences

description: It is shown that the recently observed $ΔI=4$ bifurcation seen in superdeformed nuclear bands is also occurring in rotational bands of diatomic molecules. In addition, signs of a $ΔI=8$ bifurcation, of the same order of magnitude as the $ΔI=4$ one, are observed both in superdeformed nuclear bands and rotational bands of diatomic molecules.
description: LaTex twice, 10 pages and 5 PS figures provided upon demand by the Authors
title: ESLO1: interview de personnalité 437_A
Creators: name: Laboratoire Ligérien De Linguistique
name: Baude, Olivier
name: Dugua, Céline
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2015
Subjects: subject: Français
subject: fra
subject: text_and_corpus_linguistics

description: Extrait du corpus d'Orléans, réalisé dans le cadre de l'Enquête SocioLinguistique à Orléans à la fin des années 1960.
description: Conforms to: doi:10.34847/cocoon.69c4fa74-f324-3ddb-9f1a-580867fd5826
The exact parity symmetric model and big bang nucleosynthesis
Creators: name: Foot, R.
name: Volkas, R. R.
Publisher: name: arXiv
Year: 1996
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The assumption of exact, unbroken parity symmetry leads directly to a simple predictive resolution of the atmospheric and solar neutrino puzzles. This is because the existence of this symmetry implies the existence of a set of mirror neutrinos which must mix maximally with the known neutrinos if neutrinos have mass. The maximal mixing of the electron neutrino with the mirror electron neutrino with $3 \times 10^{-10} eV^2 < |δm^2| < 10^{-3} eV^2$ eads to a predicted reduction of the solar neutrino flux by a factor of 2, which is in quite good agreement with the experiments. The maximal mixing of the muon neutrino with the mirror muon neutrino with $|δm^2| \simeq 10^{-2} eV^2$ also solves the atmospheric neutrino puzzle. We show that there is a significant range of parameters where these solutions are not in conflict with standard Big Bang Nucleosynthesis when the creation of lepton asymmetry due to neutrino oscillations is taken into account.
description: 17 pages, 2 figures, plain LaTeX
title: ESLO1: interview de personnalité 438_A
Creators: name: Laboratoire Ligérien De Linguistique
name: Baude, Olivier
name: Dugua, Céline
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2015
Subjects: subject: Français
subject: fra
subject: text_and_corpus_linguistics

description: Extrait du corpus d'Orléans, réalisé dans le cadre de l'Enquête SocioLinguistique à Orléans à la fin des années 1960.
description: Conforms to: doi:10.34847/cocoon.69c4fa74-f324-3ddb-9f1a-580867fd5826
title: ESLO1: interview de personnalité 441_A
Creators: name: Laboratoire Ligérien De Linguistique
name: Baude, Olivier
name: Dugua, Céline
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2015
Subjects: subject: Français
subject: fra
subject: text_and_corpus_linguistics

description: Extrait du corpus d'Orléans, réalisé dans le cadre de l'Enquête SocioLinguistique à Orléans à la fin des années 1960.
description: Conforms to: doi:10.34847/cocoon.69c4fa74-f324-3ddb-9f1a-580867fd5826
Quantum information/entanglement transfer rates between subsystems
Creators: name: Giddings, Steven B.
name: Rota, Massimiliano
Publisher: name: arXiv
Year: 2017
Subjects: subject: Quantum Physics (quant-ph)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: The size of quantum information -- or entanglement -- transfer rates between subsystems is a generic question in problems ranging from decoherence in quantum computation and sensing, to quantum underpinnings of thermodynamics, to the behavior of quantum black holes. We investigate such rates for given couplings between subsystems, for sufficiently random subsystem evolution, and find evidence for a conjectured relation of these rates to the size of the couplings. This provides a direct connection between entanglement transfer and the microphysical couplings responsible for it.
description: 8 pages with 3 figures
Hv Jussy annotation (blast, pfam, panther)
Creators: name: Wenger, Yvan
Publisher: name: figshare
Year: 2019
Subjects: subject: Developmental Biology
subject: 60808 Invertebrate Biology
subject: FOS: Biological sciences
subject: Evolutionary Biology
subject: 60102 Bioinformatics
subject: FOS: Computer and information sciences

description: Described in the materials and methods.Annotation by blast, Pfam 31, and Panther 13
title: ESLO1: interaction dans un magasin 290_A
Creators: name: Laboratoire Ligérien De Linguistique
name: Baude, Olivier
name: Dugua, Céline
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2015
Subjects: subject: Français
subject: fra
subject: text_and_corpus_linguistics

description: Extrait du corpus d'Orléans, réalisé dans le cadre de l'Enquête SocioLinguistique à Orléans à la fin des années 1960.
description: Conforms to: doi:10.34847/cocoon.69c4fa74-f324-3ddb-9f1a-580867fd5826
On the Observation of Phase Transitions in Collisions of Elementary Matter
Creators: name: Paech, K.
name: Reiter, M.
name: Dumitru, A.
name: Stoecker, H.
name: Greiner, W.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We investigate the excitation function of directed flow, which can provide a clear signature of the creation of the QGP and demonstrate that the minimum of the directed flow does not correspond to the softest point of the EoS for isentropic expansion. A novel technique measuring the compactness is introduced to determine the QGP transition in relativistic-heavy ion collisions: The QGP transition will lead to higher compression and therefore to higher compactness of the source in coordinate space. This effect can be observed by pion interferometry. We propose to measure the compactness of the source in the appropriate principal axis frame of the compactness tensor in coordinate space.
description: LaTeX, 8 pages, 6 figures, Conference proceedings to CRIS 2000, 3rd Catania Relativistic Ion Studies
Dust inflated accretion disc as the origin of the Broad Line Region in Active Galactic Nuclei
Creators: name: Baskin, Alexei
name: Laor, Ari
Publisher: name: arXiv
Year: 2017
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The Broad Line Region (BLR) in AGN is composed of dense gas ($\sim 10^{11}$ cm$^{-3}$) on sub-pc scale, which absorbs about 30 per cent of the ionising continuum. The outer size of the BLR is likely set by dust sublimation, and its density by the incident radiation pressure compression (RPC). But, what is the origin of this gas, and what sets its covering factor (CF)? Czerny & Hryniewicz (2011) suggested that the BLR is a failed dusty wind from the outer accretion disc. We explore the expected dust properties, and the implied BLR structure. We find that graphite grains sublimate only at $T\simeq 2000$ K at the predicted density of $\sim 10^{11}$ cm$^{-3}$, and therefore large graphite grains ($\ge 0.3$ $μ$m) survive down to the observed size of the BLR, $R_{\rm BLR}$. The dust opacity in the accretion disc atmosphere is $\sim 50$ times larger than previously assumed, and leads to an inflated torus-like structure, with a predicted peak height at $R_{\rm BLR}$. The illuminated surface of this torus-like structure is a natural place for the BLR. The BLR CF is mostly set by the gas metallicity, the radiative accretion efficiency, a dynamic configuration, and ablation by the incident optical-UV continuum. This model predicts that the BLR should extend inwards of $R_{\rm BLR}$ to the disc radius where the surface temperature is $\simeq 2000$ K, which occurs at $R_{\rm in}\simeq 0.18 R_{\rm BLR}$. The value of $R_{\rm in}$ can be tested by reverberation mapping of the higher ionisation lines, predicted by RPC to peak well inside $R_{\rm BLR}$. The dust inflated disc scenario can also be tested based on the predicted response of $R_{\rm BLR}$ and the CF to changes in the AGN luminosity and accretion rate.
description: 28 pages, 15 figures; accepted for publication in MNRAS
Effects of Multiple Anthropogenic Stressors on Lake Erie and Associated Streams’ Algal Assemblages
Creators: name: Whorley, Sarah
Publisher: name: figshare
Year: 2018
Subjects: subject: 60204 Freshwater Ecology
subject: FOS: Biological sciences

description: The Buffalo-Niagara metropolitan region contains over 1.1 million residents on an urban to rural gradient. These populations place a variety of anthropogenic stressors on the streams and rivers that flow into Lake Erie and the lake itself. Excess nutrients and sediments from urban, suburban, and rural communities, wintertime road salt deposition, and fuel-pollution from leisure activities affect aquatic life. Our objective was to analyze the effects these stressors have on the periphytic algae and macroinvertebrates of regional streams and eastern Lake Erie. There is an increasing need to consider how disturbances affect the biochemical composition, specifically essential fatty acids (EFA), of these organisms. Road salts decreased the omega-3 and omega-6 concentrations in both stream periphyton and macroinvertebrates. Broader geographic assessments indicated that periphyton in urban and agricultural streams had higher concentrations of total EFAs than suburban and rural streams. Within eastern Lake Erie, phytoplankton samples near popular fishing locations had greater concentrations of total EFAs than samples collected at locations with less fishing. These findings present a complex assessment of how anthropogenic disturbance is affecting the base of aquatic food webs in the eastern Lake Eire drainage system.
Additional file 1 of Multiplexed capture of spatial configuration and temporal dynamics of locus-specific 3D chromatin by biotinylated dCas9
Creators: name: Liu, Xin
name: Chen, Yong
name: Zhang, Yuannyu
name: Liu, Yuxuan
name: Liu, Nan
name: Botten, Giovanni
name: Cao, Hui
name: Orkin, Stuart
name: Zhang, Michael
name: Xu, Jian
Publisher: name: figshare
Year: 2020
Subjects: subject: Medicine
subject: Molecular Biology
subject: Ecology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Information Systems not elsewhere classified
subject: Developmental Biology
subject: Cancer

description: Additional file 1: Supplementary Figure S1-S10.
Eclipse studies of the dwarf-nova Ex Draconis
Creators: name: Baptista, R.
name: Catalan, M. S.
name: Costa, L.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report on high speed photometry of EX Dra in quiescence and in outburst. The analysis of the lightcurves indicates that the outbursts do not start in the outer disc regions. The disc expands during rise to maximum and shrinks during decline and along the quiescent period. At the end of two outbursts the system was seen to go through a phase of lower brightness, characterized by an out-of-eclipse level ~15 per cent lower than the typical quiescent level and by the fairly symmetric eclipse of a compact source at disc centre with little evidence of a bright spot at disc rim. New eclipse timings were measured and a revised ephemeris was derived. The residuals with respect to the linear ephemeris are well described by a sinusoid of amplitude 1.2 minutes and period \~4 years and are possibly related to a solar-like magnetic activity cycle in the secondary star. Eclipse phases of the compact central source and of the bright spot were used to derive the geometry of the binary. By constraining the gas stream trajectory to pass through the observed position of the bright spot we find q=0.72+/-0.06 and i= 85 +3/-2 degrees. The binary parameters were estimated by combining the measured mass ratio with the assumption that the secondary star obeys an empirical main sequence mass-radius relation. We find M_1= 0.75+/-0.15 M_sun and M_2= 0.54+/-0.10 M_sun. The white dwarf at disc centre is surrounded by an extended and variable atmosphere or boundary layer of at least 3 times its radius and a temperature of T ~28000 K. The fluxes at mid-eclipse yield an upper limit to the contribution of the secondary star and lead to a lower limit photometric parallax distance of D= 290+/-80 pc. The fluxes of the secondary star are well matched by those of a M0+/-2 main sequence star.
description: submitted to MNRAS, 12 pages, 9 figures; coded with MNRAS latex style
Planetesimal formation starts at the snow line
Creators: name: Drazkowska, Joanna
name: Alibert, Yann
Publisher: name: arXiv
Year: 2017
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Planetesimal formation stage represents a major gap in our understanding of the planet formation process. The late-stage planet accretion models typically make arbitrary assumptions about planetesimals and pebbles distribution while the dust evolution models predict that planetesimal formation is only possible at some orbital distances. We want to test the importance of water snow line for triggering formation of the first planetesimals during the gas-rich phase of protoplanetary disk, when cores of giant planets have to form. We connect prescriptions for gas disk evolution, dust growth and fragmentation, water ice evaporation and recondensation, as well as transport of both solids and water vapor, and planetesimal formation via streaming instability into a single, one-dimensional model for protoplanetary disk evolution. We find that processes taking place around the snow line facilitate planetesimal formation in two ways. First, due to the change of sticking properties between wet and dry aggregates, there is a "traffic jam" inside of the snow line that slows down the fall of solids onto the star. Second, ice evaporation and outward diffusion of water followed by its recondensation increases the abundance of icy pebbles that trigger planetesimal formation via streaming instability just outside of the snow line. Planetesimal formation is hindered by growth barriers and radial drift and thus requires particular conditions to take place. Snow line is a favorable location where planetesimal formation is possible for a wide range of conditions, but still not in every protoplanetary disk model. This process is particularly promoted in large, cool disks with low intrinsic turbulence and increased initial dust-to-gas ratio.
description: Accepted for publication in Astronomy & Astrophysics
Theoretical description of deformed proton emitters: nonadiabatic coupled-channel method
Creators: name: Barmore, B.
name: Kruppa, A. T.
name: Nazarewicz, W.
name: Vertse, T.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: The newly developed nonadiabatic method based on the coupled-channel Schroedinger equation with Gamow states is used to study the phenomenon of proton radioactivity. The new method, adopting the weak coupling regime of the particle-plus-rotor model, allows for the inclusion of excitations in the daughter nucleus. This can lead to rather different predictions for lifetimes and branching ratios as compared to the standard adiabatic approximation corresponding to the strong coupling scheme. Calculations are performed for several experimentally seen, non-spherical nuclei beyond the proton dripline. By comparing theory and experiment, we are able to characterize the angular momentum content of the observed narrow resonance.
description: 12 pages including 10 figures
title: ESLO1: interaction dans un magasin 630_A
Creators: name: Laboratoire Ligérien De Linguistique
name: Baude, Olivier
name: Dugua, Céline
Publisher: name: COCOON - https://cocoon.huma-num.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2015
Subjects: subject: Français
subject: fra
subject: text_and_corpus_linguistics

description: Extrait du corpus d'Orléans, réalisé dans le cadre de l'Enquête SocioLinguistique à Orléans à la fin des années 1960.
description: Conforms to: doi:10.34847/cocoon.69c4fa74-f324-3ddb-9f1a-580867fd5826
A Computational Study of Thirteen-atom Ar-Kr Cluster Heat Capacities
Creators: name: Frantz, Don D.
Publisher: name: arXiv
Year: 1996
Subjects: subject: Chemical Physics (physics.chem-ph)
subject: FOS: Physical sciences

description: Heat capacity curves as functions of temperature were calculated using Monte Carlo methods for the series of Ar_{13-n}Kr_n clusters (0 <= n <= 13). The clusters were modeled classically using pairwise additive Lennard-Jones potentials. J-walking (or jump-walking) was used to overcome convergence difficulties due to quasiergodicity present in the solid-liquid transition regions, as well as in the very low temperature regions where heat capacity anomalies arising from permutational isomers were observed. Substantial discrepancies between the J-walking results and the results obtained using standard Metropolis Monte Carlo methods were found. Results obtained using the atom-exchange method, another Monte Carlo variant designed for multi-component systems, were mostly similar to the J-walker results. Quench studies were also done to investigate the clusters' potential energy surfaces; in each case, the lowest energy isomer had an icosahedral-like symmetry typical of homogeneous thirteen-atom rare gas clusters, with an Ar atom being the central atom.
description: 46 pages, 13 Figures combined in 2 .gif files, Journal of Chemical Physics, AIP ID number 508646JCP
MPEC 2024-G127 : 2024 GF2
Creators: name: Minor Planet Center Staff
Publisher: name: The Minor Planet Center
Year: 2024
Subjects: subject: Small Solar System bodies
valueUri: http://astrothesaurus.org/uat/1469
subject: 2024 GF2

description: The Minor Planet Electronic Circulars contain information on unusual minor planets, routine data on comets and natural satellites, and occasional editorial announcements.  They are published on behalf of Division F of the International Astronomical Union by the Minor Planet Center, Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A.