cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Characterization of the frequency of extreme events by the Generalized Pareto Distribution
Creators: name: Pisarenko, V. F.
name: Sornette, D.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: Based on recent results in extreme value theory, we use a new technique for the statistical estimation of distribution tails. Specifically, we use the Gnedenko-Pickands-Balkema-de Haan theorem, which gives a natural limit law for peak-over-threshold values in the form of the Generalized Pareto Distribution (GPD). Useful in finance, insurance, hydrology, we investigate here the earthquake energy distribution described by the Gutenberg-Richter seismic moment-frequency law and analyze shallow earthquakes (depth h < 70 km) in the Harvard catalog over the period 1977-2000 in 18 seismic zones. The whole GPD is found to approximate the tails of the seismic moment distributions quite well above moment-magnitudes larger than mW=5.3 and no statistically significant regional difference is found for subduction and transform seismic zones. We confirm that the b-value is very different in mid-ocean ridges compared to other zones (b=1.50=B10.09 versus b=1.00=B10.05 corresponding to a power law exponent close to 1 versus 2/3) with a very high statistical confidence. We propose a physical mechanism for this, contrasting slow healing ruptures in mid-ocean ridges with fast healing ruptures in other zones. Deviations from the GPD at the very end of the tail are detected in the sample containing earthquakes from all major subduction zones (sample size of 4985 events). We propose a new statistical test of significance of such deviations based on the bootstrap method. The number of events deviating from the tails of GPD in the studied data sets (15-20 at most) is not sufficient for determining the functional form of those deviations. Thus, it is practically impossible to give preference to one of the previously suggested parametric families describing the ends of tails of seismic moment distributions.
description: pdf document of 21 pages + 2 tables + 20 figures (ps format) + one file giving the regionalization
Decaying Vacuum Energy and Deflationary Cosmology in Open and Closed Universes
Creators: name: Lima, J. A. S.
name: Trodden, M.
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We consider a nonsingular deflationary cosmological model with decaying vacuum energy density in universes of arbitrary spatial curvature. Irrespective of the value of $k$, the models are characterized by an arbitrary time scale $H_I^{-1}$ which determines the initial temperature of the universe and the largest value of the vacuum energy density, the slow decay of which generates all the presently observed matter-energy of the universe. If $H_I^{-1}$ is of the order of the Planck time, the models begin with the Planck temperature and the present day value of the cosmological constant satisfies $Λ_I/Λ_0 \simeq 10^{118}$ as theoretically suggested. It is also shown that all models allow a density parameter $Ω_0 <2/3$ and that the age of the universe is large enough to agree with observations even with the high value of $H_0$ suggested by recent measurements.
description: 20 pages, 2 figures (available from the authors), uses LaTeX
The origin of the mass scales for maximal star formation efficiency and quenching: the critical role of Supernovae
Creators: name: Henriques, Bruno
name: White, Simon
name: Lilly, Simon
name: Bell, Eric
name: Bluck, Asa
name: Terrazas, Bryan
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We use the Henriques et al. (2015) version of the Munich galaxy formation model (L-GALAXIES) to investigate why the halo and stellar mass scales above which galaxies are quenched are constant with redshift and coincide with the scale where baryons are most efficiently converted into stars. This model assumes that central galaxies are quenched by AGN feedback when hot halo gas accretes onto a supermassive black hole. Nevertheless, we find that supernova (SN) feedback sets both mass scales. As haloes grow above a threshold mass, SNe can no longer eject material so their hot gas content increases, enhancing the cooling rate onto the central galaxy, its cold gas content, its star formation rate and the growth rate of its central black hole. Strong AGN feedback terminates this short-lived phase by suppressing the fuel supply for star formation. Despite strong evolution of the halo mass - temperature relation, quenching occurs at a redshift-independent halo and stellar mass which coincides with the mass where baryons have been converted into stars with maximal efficiency. These regularities and coincidences are a result of the specific parameters selected by MCMC tuning of the model to fit the observed abundance and passive fraction of galaxies over the redshift range 0
description: 12 pages, 8 figures, submitted to MNRAS
Hydrogen oxidation on oxygen-rich IrO2(110)
Creators: name: Li, Tao
name: Kim, Minkyu
name: Liang, Zhu
name: Asthagiri, Aravind
name: Weaver, Jason F.
Publisher: name: Taylor & Francis
Year: 2019
Subjects: subject: Biophysics
subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Physiology
subject: Chemical Sciences not elsewhere classified
subject: Ecology
subject: Developmental Biology
subject: Cancer

description: We investigated the adsorption and oxidation of H2 on O-rich IrO2(110) using temperature programmed reaction spectroscopy (TPRS) and density functional theory (DFT) calculations. Our results show that H2 dissociation occurs efficiently on O-rich IrO2(110) at low temperature and initiates from an adsorbed H2 σ-complex on the coordinatively-unsaturated Ir atoms (Ircus). We find that on-top oxygen atoms (Oot), adsorbed on the Ircus sites, promote the desorption-limited evolution of H2O during subsequent oxidation of the adsorbed hydrogen on IrO2(110) while suppressing reaction-limited production of H2O via the recombination of bridging HO groups (HObr) (~500 to 750 K) during TPRS. The desorption-limited TPRS peak of H2O shifts from ~490 to 550 K with increasing Oot coverage, demonstrating that Oot atoms stabilize adsorbed OH and H2O species. DFT predicts that molecularly-adsorbed H2 dissociates on O-rich IrO2(110) at low temperature and that the resulting H-atoms redistribute to produce a mixture of HObr and HOot groups, with equilibrium favouring HOot groups. Our calculations further predict that subsequent H2O evolution occurs through the recombination of HObr/HOot and HOot/HOot pairs, and that these reactions represent desorption-limited pathways because the dissociative chemisorption of H2O is favoured over molecular adsorption on IrO2(110). The higher stability of HOot groups and their preferred formation causes the higher-barrier HOot/HOot recombination reaction to become the dominant pathway for H2O formation with increasing Oot coverage, consistent with the experimentally-observed upshift in the H2O TPRS peak temperature.
Sauropus androgynus Merr.
Creators: name: Jarvis, Charlie
Publisher: name: Linnaean Society of London in association with the Natural History Museum
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Malpighiales
Phyllanthaceae
Sauropus
Sauropus androgynus

description: Clutia androgyna Linnaeus, Systema Naturae, ed. 12, 2: 663; Mantissa Plantarum: 128. 1767.
"Habitat in India." RCN: 7351.
 Lectotype (van Welzen in Blumea 48: 340. 2003): Herb. Linn. No. 1206.14 (LINN).
 Current name:  Sauropus androgynus  (L.) Merr. (Euphorbiaceae).
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part C), pp. 370-473 in Order out of Chaos. Linnaean Plant Types and their Types, London :Linnaean Society of London in association with the Natural History Museum on page 429, DOI: 10.5281/zenodo.291971
The Transition Temperature to the Superconducting Phase of QCD at High Baryon Density
Creators: name: Brown, William E.
name: Liu, James T.
name: Ren, Hai-cang
Publisher: name: arXiv
Year: 1999
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Superconductivity (cond-mat.supr-con)
subject: High Energy Physics - Theory (hep-th)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: Recent interest in the study of color superconductivity has focused on the regime of high baryon density where perturbative QCD may be employed. Based on the dominant one-gluon-exchange interaction, both the transition temperature and zero temperature gap have been determined to leading order in the coupling, g. While the leading non-BCS behavior, $T_C\simμg^{-5}e^{-κ/g}$, is easily obtained, the pre-exponential factor has proved more difficult to evaluate. Focusing on the transition temperature, we present a perturbative derivation of this factor, exact to leading order in g. This approach is first motivated by the study of a toy model and involves working to second order in the perturbative expansion. We compare this result to the zero temperature gap. Additionally, we extend the analysis to the case of higher angular momentum for longitudinal and transverse quark pairing.
description: 37 pages, 5 figures (revtex v3.1)
Large spin-orbit splitting of deep in-gap defect states of engineered sulfur vacancies in monolayer WS2
Creators: name: Schuler, Bruno
name: Qiu, Diana Y.
name: Refaely-Abramson, Sivan
name: Kastl, Christoph
name: Chen, Christopher T.
name: Barja, Sara
name: Koch, Roland J.
name: Ogletree, D. Frank
name: Aloni, Shaul
name: Schwartzberg, Adam M.
name: Neaton, Jeffrey B.
name: Louie, Steven G.
name: Weber-Bargioni, Alexander
Publisher: name: arXiv
Year: 2018
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Structural defects in 2D materials offer an effective way to engineer new material functionalities beyond conventional doping in semiconductors. Specifically, deep in-gap defect states of chalcogen vacancies have been associated with intriguing phenomena in monolayer transition metal dichalcogenides (TMDs). Here, we report the direct experimental correlation of the atomic and electronic structure of a sulfur vacancy in monolayer WS2 by a combination of CO-tip noncontact atomic force microscopy (nc-AFM) and scanning tunneling microscopy (STM). Sulfur vacancies, which are absent in as-grown samples, were deliberately created by annealing in vacuum. Two energetically narrow unoccupied defect states of the vacancy provide a unique fingerprint of this defect. Direct imaging of the defect orbitals by STM and state-of-the-art GW calculations reveal that the large splitting of 252 meV between these defect states is induced by spin-orbit coupling. The controllable incorporation and potential decoration of chalcogen vacancies provide a new route to tailor the optical, catalytic and magnetic properties of TMDs.
HIGH ACCURACY DIFFERENCE SCHEME FOR THE EQUATION  OF DYNAMICS OF COMPRESSIVE STRATIFIED  ROTATING FLUID
Creators: name: Utebaev, D.
name: Kazimbetova, M.M.
Publisher: name: Zenodo
Year: 2024

description: Difference schemes of the finite difference method of high-order accuracy for the sixth-order Sobolev-type equation are constructed and investigated. In particular, the first boundary value problem for the wave equation of a compressible stratified rotating fluid is considered. First, approximation is performed only in spatial variables by the finite difference method, and the resulting system of high-dimensional ordinary differential equations is also approximated by this method. Using the method of energy inequalities, a priori estimates were obtained and, on their basis, theorems on the stability and convergence of the constructed difference schemes were proven; accuracy estimates were obtained for sufficient smoothness of the solution to the original initial boundary value problem. An algorithm for implementing difference schemes is proposed.
On the exponential ultradistribution semigroups in Banach spaces
Creators: name: c, Marko Kosti\'
name: c, Stevan Pilipovi\'
name: Velinov, Daniel
Publisher: name: arXiv
Year: 2018
Subjects: subject: Functional Analysis (math.FA)
subject: FOS: Mathematics
subject: 47D06, 47D60, 47D99

description: In this paper, we continue our previous research studies of exponential ultradistribution semigroups in Banach spaces. The existence and uniqueness of analytical solutions of abstract fractional relaxation equations associated with the generators of exponential ultradistribution semigroups have been considered. Some other results are also proved.
Additional file 3: of HIV-1 molecular transmission clusters in nine European countries and Canada: association with demographic and clinical factors
Creators: name: Paraskevis, Dimitrios
name: Beloukas, Apostolos
name: Stasinos, Kostantinos
name: Pantazis, Nikos
name: Mendoza, Carmen
name: Bannert, Norbert
name: Meyer, Laurence
name: Zangerle, Robert
name: Gill, John
name: Prins, Maria
name: Montforte, Antonella DâArminio
name: Anne-Marte Kran
name: Kholoud Porter
name: Touloumi, Giota
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: CASCADE and EuroCoord acknowledgements, and list of ethics committees. (DOCX 20 kb)
Como a licença CC BY para Preprints impacta a publicação em periódicos Um guia para pesquisadores
Creators: name: Creative Commons
Publisher: name: Zenodo
Year: 2025
Subjects: Preprints
Licenciamento
Copyright
Direitos de autor
Acesso livre
Ciência Aberta
Investigação aberta
Investigação
Ciência

description: Um guia para publicar outras versões da sua investigação depois de licenciar o seu preprint com a licença CC BY.

 

A guide to publishing further versions of your research after licensing your preprint CC BY.

 

This text was translated to European Portuguese by Gracielle Higino.
N=4 supersymmetric integrable systems
Creators: name: Ivanov, E.
Publisher: name: arXiv
Year: 1997
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: I give an overview of recent progress in constructing the KdV, mKdV and NLS type hierarchies with extended N=4 supersymmetry.
description: 12 pages, LaTeX, Talk given at International Seminar "Supersymmetry And Quantum Field Theory", dedicated to the memory of Dmitrij Volkov (Kharkov, Ukraine) January 5-7, 1997 (to be published in Proceedings)
Intra-cell dynamics and cyclotron motion without magnetic field
Creators: name: Hasdeo, Eddwi H.
name: Frenzel, Alex J.
name: Song, Justin C. W.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: Intra-cell motion endows rich non-trivial phenomena to a wide variety of quantum materials. The most prominent example is a transverse current in the absence of a magnetic field (i.e. the anomalous Hall effect). Here we show that, in addition to a dc Hall effect, anomalous Hall materials possess circulating currents and cyclotron motion without magnetic field. These are generated from the intricate wavefunction dynamics within the unit cell, and correspond to interband transitions (coherences) in much the same way that cyclotron resonances arise from inter-Landau level transitions in magneto-optics. Curiously, anomalous cyclotron motion exhibits an intrinsic decay in time (even in pristine materials) displaying a characteristic power law decay. This reveals an intrinsic dephasing similar to that of inhomogeneous broadening of spinors. Circulating currents can manifest as the emission of circularly polarized light pulses in response to incident linearly polarized (pulsed) electric field, and provide a direct means of interrogating the intra-unit-cell dynamics of quantum materials.
Additional file 3: of Cortisol levels in different tissue samples in posttraumatic stress disorder patients versus controls: a systematic review and meta-analysis protocol
Creators: name: Heuvel, Leigh Van Den
name: Wright, Simonne
name: Sharain Suliman
name: Stalder, Tobias
name: Kirschbaum, Clemens
name: Seedat, Soraya
Publisher: name: figshare
Year: 2019
Subjects: subject: Molecular Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Figure S1. PRISMA flow diagram. (DOC 29 kb)
Additional file 2: of Cortisol levels in different tissue samples in posttraumatic stress disorder patients versus controls: a systematic review and meta-analysis protocol
Creators: name: Heuvel, Leigh Van Den
name: Wright, Simonne
name: Sharain Suliman
name: Stalder, Tobias
name: Kirschbaum, Clemens
name: Seedat, Soraya
Publisher: name: figshare
Year: 2019
Subjects: subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Search terms. (DOCX 14 kb)
Choosing to Grow a Graph: Modeling Network Formation as Discrete Choice
Creators: name: Overgoor, Jan
name: Benson, Austin R.
name: Ugander, Johan
Publisher: name: arXiv
Year: 2018
Subjects: subject: Social and Information Networks (cs.SI)
subject: Physics and Society (physics.soc-ph)
subject: FOS: Computer and information sciences
subject: FOS: Physical sciences

description: We provide a framework for modeling social network formation through conditional multinomial logit models from discrete choice and random utility theory, in which each new edge is viewed as a "choice" made by a node to connect to another node, based on (generic) features of the other nodes available to make a connection. This perspective on network formation unifies existing models such as preferential attachment, triadic closure, and node fitness, which are all special cases, and thereby provides a flexible means for conceptualizing, estimating, and comparing models. The lens of discrete choice theory also provides several new tools for analyzing social network formation; for example, the significance of node features can be evaluated in a statistically rigorous manner, and mixtures of existing models can be estimated by adapting known expectation-maximization algorithms. We demonstrate the flexibility of our framework through examples that analyze a number of synthetic and real-world datasets. For example, we provide rigorous methods for estimating preferential attachment models and show how to separate the effects of preferential attachment and triadic closure. Non-parametric estimates of the importance of degree show a highly linear trend, and we expose the importance of looking carefully at nodes with degree zero. Examining the formation of a large citation graph, we find evidence for an increased role of degree when accounting for age.
description: 12 pages, 5 figures, 4 tables
Croton cascarilla Linnaeus 1763
Creators: name: Jarvis, Charlie
Publisher: name: Linnaean Society of London in association with the Natural History Museum
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Malpighiales
Euphorbiaceae
Croton
Croton cascarilla

description: Clutia cascarilla Linnaeus, Species Plantarum 2: 1042. 1753.
"Habitat in Carolina." RCN: 7267.
 Basionym of: Croton cascarilla (L.) L. (1763).
 Lectotype (Dandy, Sloane Herbarium: 112. 1958): [icon] " An Ricinoides Aeleagni folio? " in Catesby, Nat. Hist. Carolina 2: 46, t. 46. 1736. - Voucher: Herb. Sloane 232: 24 (BM-SL).
 Current name:  Croton cascarilla  (L.) L. (Euphorbiaceae).
 Note: See discussion by Howard & Staples (in J. Arnold Arbor. 64: 524. 1983).
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part C), pp. 370-473 in Order out of Chaos. Linnaean Plant Types and their Types, London :Linnaean Society of London in association with the Natural History Museum on page 429, DOI: 10.5281/zenodo.291971
Additional file 1 of scSensitiveGeneDefine: sensitive gene detection in single-cell RNA sequencing data by Shannon entropy
Creators: name: Chen, Zechuan
name: Yang, Zeruo
name: Yuan, Xiaojun
name: Zhang, Xiaoming
name: Hao, Pei
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 1. Misidentification ratio and tools application in other data sets.
The structure functions of longitudinal virtual photon at low virtualities
Creators: name: Ioffe, B. L.
name: Shushpanov, I. A.
Publisher: name: arXiv
Year: 1996
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The structure functions of longitudinal virtual photon at low virtualities are calculated in the framework of chiral pertubation theory(ChPT) in the zero and first order of ChPT. It is assumed that the virtuality of target longitudinal photon is much less than the virtuality of the hard projectile photon and both are less than the characteristic ChPT scale.
description: 16 pages, 8 figures
THE DIFFERENCES BETWEEN THE MOVIE AND THE NOVEL 'THE JOY LUCK CLUB'
Creators: name: Dong, Lina
Publisher: name: Zenodo
Year: 2024

description: The Joy Luck Club is a novel published in 1989, written in by Amy Tan, a Chinese American writer. In 1993, it was adapted into a movie directed by Wayne Wang and achieved a great success. The study aims at analyzing the differences between the novel and the movie in content and narrative strategy. Though the movie is basically faithful to the novel---the main characters and stories are the same and both in flashback narrative order, it made some changes in story endings, narrative order and other expressive techniques, some omissions and some supplements. Consequently, the themes expressed in the movie, in addition to the commonalities of love, communication, and cultural identity with those in the novel, showing less feminist spirit but more ethnic community culture, less conflicts but more reconciliation.
Pair Production of Heavy-Exotic-Fermions
Creators: name: Montalvo, Jorge Eduardo Cieza
Publisher: name: arXiv
Year: 1998
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We study the production and signatures of heavy exotic fermion pairs in the framework of the vector singlet model (VSM), vector doublet model (VDM) and fermion-mirror-fermion (FMF) model. We show that the pair production cross sections are competitive with the ones for the single production of exotic fermions due to the exchange of a photon in the $s$ channel and to the vector component of the $Z$ - boson coupling to exotic fermions. We also exhibit some kinematical distributions.
description: 13 pages, 10 figures
Topology optimization in the framework of the linear Boltzmann equation -- a method for designing optimal nuclear equipment and particle optics
Creators: name: Chabod, Sébastien
Publisher: name: arXiv
Year: 2018
Subjects: subject: Instrumentation and Detectors (physics.ins-det)
subject: Nuclear Experiment (nucl-ex)
subject: Applied Physics (physics.app-ph)
subject: FOS: Physical sciences

description: In this study, we describe a procedure of topology optimization in the framework of the linear Boltzmann equation, implemented using a reference Monte-Carlo particle transport code. This procedure can design complex structures that optimize the transport of particles, according to preset objectives and constraints. Although simple and perfectible, this procedure was successfully tested on a series of difficult problems, with results outperforming human capabilities. Improved, it could be used to assist or automate the design of particle optics or nuclear devices.
description: Paper (46 pages), followed by its Supplemental Material section (58 pages), published in Nucl. Instr. Meth. A
A thermally driven spin-transfer-torque system far from equilibrium: enhancement of the thermoelectric current via pumping current
Creators: name: Ludwig, Tim
name: Burmistrov, Igor S.
name: Gefen, Yuval
name: Shnirman, Alexander
Publisher: name: arXiv
Year: 2018
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We consider a small itinerant ferromagnet exposed to an external magnetic field and strongly driven by a thermally induced spin current. For this model, we derive the quasi-classical equations of motion for the magnetization where the effects of a dynamical non-equilibrium distribution function are taken into account self-consistently. We obtain the Landau-Lifshitz-Gilbert equation supplemented by a spin-transfer torque term of Slonczewski form. We identify a regime of persistent precessions in which we find an enhancement of the thermoelectric current by the pumping current.
description: 17 pages, 3 figures
Effects of non-Kozai mutual inclinations on two-planet system stability through all phases of stellar evolution
Creators: name: Veras, Dimitri
name: Georgakarakos, Nikolaos
name: Gänsicke, Boris T.
name: Dobbs-Dixon, Ian
Publisher: name: arXiv
Year: 2018
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Previous full-lifetime simulations of single-star multi-planet systems across all phases of stellar evolution have predominately assumed coplanar or nearly-coplanar orbits. Here we assess the consequences of this assumption by removing it and exploring the effect of giant branch mass loss on the stability of two-planet systems with small to moderate non-Kozai (<40 degrees) relative inclinations. We run nearly 10^4 simulations over 14 Gyr for F-star, A-star and B-star planet hosts, incorporating main sequence stellar masses of 1.5, 2.0, 2.5, 3.0 and 5.0 solar masses, and initial planetary semimajor axis ratios that straddle their three-dimensional Hill stability limits. We find that the near-coplanar assumption can approximate well the stability frequencies and critical separations found for higher inclinations, except around strong mean-motion commensurabilities. Late instabilities -- after the star has become a white dwarf -- occur throughout the explored mutual inclination range. Consequently, non-Kozai mutual inclination should not be used as a predictive orbital proxy for determining which white dwarf multi-planet systems discovered by Gaia should represent high-priority follow-up targets for the detection of metal pollution and planetary debris discs.
description: Accepted for publication in MNRAS
title: ADCO, Premier cartulaire de Saint-Étienne de Dijon (XIIe siècle), Cart. 21 (G 125), 71 folios, f. 00118
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/2015
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire

description: Premier cartulaire de Saint-Étienne de Dijon (XIIe siècle), Archives départementales de la Côte-d'Or, Cart. 21 (G 125), 71 folios, f. 00118, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Premier cartulaire de Saint-Étienne de Dijon (XIIe siècle), Archives départementales de la Côte-d'Or, Cart. 21 (G 125), 71 folios, f. 00118, 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
Spatially Resoved 12CO(2-1)/12CO(1-0) in the Starburst Galaxy NGC 253: Assessing Optical Depth to Constrain the Molecular Mass Outflow Rate
Creators: name: Zschaechner, Laura K.
name: Bolatto, Alberto D.
name: Walter, Fabian
name: Leroy, Adam K.
name: Herrera, Cinthya
name: Krieger, Nico
name: Kruijssen, J. M. Diederik
name: Meier, David S.
name: Mills, Elisabeth A. C.
name: Ott, Juergen
name: Veilleux, Sylvain
name: Weiss, Axel
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present Atacama Large Millimeter/submillimeter Array (ALMA) observations of 12CO(1-0) and 12CO(2-1) in the central 40" (680 pc) of the nuclear starburst galaxy NGC 253, including its molecular outflow. We measure the ratio of brightness temperature for CO(2-1)/CO(1-0), r_21, in the central starburst and outflow-related features. We discuss how r_21 can be used to constrain the optical depth of the CO emission, which impacts the inferred mass of the outflow and consequently the molecular mass outflow rate. We find r_21 less than or equal to 1 throughout, consistent with a majority of the CO emission being optically-thick in the outflow, as it is in the starburst. This suggests that the molecular outflow mass is 3-6 times larger than the lower limit reported for optically thin CO emission from warm molecular gas. The implied molecular mass outflow rate is 25-50 solar masses per year, assuming that conversion factor for the outflowing gas is similar to our best estimates for the bulk of the starburst. This is a factor of 9-19 times larger than the star formation rate in NGC 253. We see tentative evidence for an extended, diffuse CO(2-1) component.
description: Accepted to ApJ on 31 August 2018, 14 pages, 8 figures
MOESM3 of Prognostic implications of Aquaporin 9 expression in clear cell renal cell carcinoma
Creators: name: Xu, Wen-Hao
name: Shi, Shen-Nan
name: Xu, Yue
name: Wang, Jun
name: Wang, Hong-Kai
name: Cao, Da-Long
name: Shi, Guo-Hai
name: Qu, Yuan-Yuan
name: Zhang, Hai-Liang
name: Ye, Ding-Wei
Publisher: name: figshare
Year: 2019
Subjects: subject: Space Science
subject: Genetics
subject: FOS: Biological sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Mathematical Sciences not elsewhere classified
subject: Marine Biology
subject: Cancer
subject: Science Policy

description: Additional file 3: Table S1. Clinicopathological characteristics baseline in relation to AQP9 expression status in TCGA cohort. Table S2. Univariate Cox logistic regression analysis of PFS in TCGA and FUSCC cohort (PFS: progression-free survival; TCGA: the Cancer Genome Atlas; FUSCC: Fudan university shanghai cancer center). Table S3. Univariate Cox logistic regression analysis of OS in TCGA and FUSCC cohort (OS: overall survival; TCGA: the Cancer Genome Atlas; FUSCC: Fudan university shanghai cancer center). Table S4. Correlation analysis between AQP9 and immune cell infiltrations in ccRCC samples using TIMER.
Additional file 2: of HIV-1 molecular transmission clusters in nine European countries and Canada: association with demographic and clinical factors
Creators: name: Paraskevis, Dimitrios
name: Beloukas, Apostolos
name: Stasinos, Kostantinos
name: Pantazis, Nikos
name: Mendoza, Carmen
name: Bannert, Norbert
name: Meyer, Laurence
name: Zangerle, Robert
name: Gill, John
name: Prins, Maria
name: Montforte, Antonella DâArminio
name: Anne-Marte Kran
name: Kholoud Porter
name: Touloumi, Giota
Publisher: name: figshare
Year: 2019
Subjects: subject: Space Science
subject: Medicine
subject: Molecular Biology
subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: Computational Biology

description: Table S2. Bootstrap support values of MTCs identified with ML phylogenies. (DOCX 22 kb)
Reconstructing the Inflaton Potential --- an Overview
Creators: name: Lidsey, James E
name: Liddle, Andrew R
name: Kolb, Edward W
name: Copeland, Edmund J
name: Barreiro, Tiago
name: Abney, Mark
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We review the relation between the inflationary potential and the spectra of density (scalar) perturbations and gravitational waves (tensor perturbations) produced, with particular emphasis on the possibility of reconstructing the inflaton potential from observations. The spectra provide a potentially powerful test of the inflationary hypothesis; they are not independent but instead are linked by consistency relations reflecting their origin from a single inflationary potential. To lowest-order in a perturbation expansion there is a single, now familiar, relation between the tensor spectral index and the relative amplitude of the spectra. We demonstrate that there is an infinite hierarchy of such consistency equations, though observational difficulties suggest only the first is ever likely to be useful. We also note that since observations are expected to yield much better information on the scalars than on the tensors, it is likely to be the next-order version of this consistency equation which will be appropriate, not the lowest-order one. If inflation passes the consistency test, one can then confidently use the remaining observational information to constrain the inflationary potential, and we survey the general perturbative scheme for carrying out this procedure. Explicit expressions valid to next-lowest order in the expansion are presented. We then briefly assess the prospects for future observations reaching the quality required, and consider a simulated data set that is motivated by this outlook.
description: 69 pages standard LaTeX plus 4 postscript figures. Postscript version of text in landscape format (35 pages) available at http://star-www.maps.susx.ac.uk/papers/infcos_papers.html Modifications are a variety of updates to discussion and references
AN INVESTIGATION INTO SOCIOECONOMIC AND CULTURAL FACTORS LIMITING ACCESS TO QUALITY BASIC EDUCATION IN JIMETA OUTSKIRT, YOLA NORTH LGA OF ADAMAWA STATE IN NIGERIA
Creators: name: Aisha, Kadiri Mohammed
name: Yahaya, Abdulrasheed
name: Dr Ibrahim, Umar Jongur
name: Mrs Basira, Bisi  Salawu
name: Fatima, A. Umar
name: Esther, Daniel  Mshelbila
Publisher: name: top journals
Year: 2024
Subjects: Socioeconomic, Cultural, Income level, Quality Basic Education,

description: This study examines the socioeconomic and cultural barriers to accessing quality basic education in Jimeta Outskirt, Yola North LGA, Adamawa State, Nigeria. The objectives of the research were to investigate the influence of cultural practices and beliefs on children's education and to assess the impact of family income levels and parental education on educational accessibility. A survey research design was used, employing structured questionnaires to collect data from 320 respondents. Findings revealed that cultural norms such as early marriage and gender biases significantly hinder children's access to education, particularly for girls. Additionally, higher family income and parental education levels were shown to enhance children's educational opportunities. The study concludes that cultural practices and socioeconomic factors remain substantial barriers to education in the community. Recommendations include initiating cultural reorientation programs to address harmful norms, engaging community leaders in advocating for education, and providing economic support to families through scholarships and adult literacy initiatives.
Sequential eruptions triggered by flux emergence - observations and modeling
Creators: name: Dacie, Sally
name: Torok, Tibor
name: Demoulin, Pascal
name: Linton, Mark
name: Downs, Cooper
name: van Driel-Gesztelyi, Lidia
name: Long, David
name: Leake, James
Publisher: name: arXiv
Year: 2018
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We describe and analyze observations by the Solar Dynamics Observatory of the emergence of a small, bipolar active region within an area of unipolar magnetic flux that was surrounded by a circular, quiescent filament. Within only eight hours of the start of the emergence, a partial splitting of the filament and two consecutive coronal mass ejections took place. We argue that all three dynamic events occurred as a result of particular magnetic-reconnection episodes between the emerging bipole and the pre-existing coronal magnetic field. In order to substantiate our interpretation, we consider three-dimensional magnetohydrodynamic simulations that model the emergence of magnetic flux in the vicinity of a large-scale coronal flux rope. The simulations qualitatively reproduce most of the reconnection episodes suggested by the observations; as well as the filament-splitting, the first eruption, and the formation of sheared/twisted fields that may have played a role in the second eruption. Our results suggest that the position of emerging flux with respect to the background magnetic configuration is a crucial factor for the resulting evolution, while previous results suggest that parameters such as the orientation or the amount of emerging flux are important as well. This poses a challenge for predicting the onset of eruptions that are triggered by flux emergence, and it calls for a detailed survey of the relevant parameter space by means of numerical simulations.
description: 17 pages, 8 figures, accepted for publication by the Astrophysical Journal
title: Ð­ÑÑÐµÐºÑÑ ÑÑÑÑÐºÑÑÑÐ½ÑÑ Ð°Ð½Ð°Ð»Ð¾Ð³Ð¾Ð² Ð¿ÐµÐ¿ÑÐ¸Ð´Ð¾Ð² Ð±Ð°ÐºÑÐµÐ½ÐµÑÐ¸Ð½Ð¾Ð² Ð½Ð° Ð±Ð°ÐºÑÐµÑÐ¸Ð°Ð»ÑÐ½ÑÐµ Ð¸ ÑÑÐºÐ°ÑÐ¸Ð¾ÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÐºÐ»ÐµÑÐºÐ¸
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
Creators: name: Ð¡Ð°ÑÐ¸ÑÐ»Ð»Ð¸Ð½Ð°, ÐÐ°ÑÐ¸Ð½Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: Ð¸Ð¼Ð¼ÑÐ½Ð¸ÑÐµÑ
Ð°Ð½ÑÐ¸Ð¼Ð¸ÐºÑÐ¾Ð±Ð½ÑÐµ Ð¿ÐµÐ¿ÑÐ¸Ð´Ñ
Ð¿ÑÐ¾Ð»Ð¸Ð½-Ð±Ð¾Ð³Ð°ÑÑÐµ Ð¿ÐµÐ¿ÑÐ¸Ð´Ñ Ð¼Ð»ÐµÐºÐ¾Ð¿Ð¸ÑÐ°ÑÑÐ¸Ñ
Ð±Ð°ÐºÑÐµÐ½ÐµÑÐ¸Ð½Ñ

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¾ Ð´ÐµÐ¹ÑÑÐ²Ð¸Ðµ Ð¾Ð±Ð¾Ð³Ð°ÑÑÐ½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾Ð»Ð¸Ð½Ð¾Ð¼ Ð°Ð½ÑÐ¸Ð¼Ð¸ÐºÑÐ¾Ð±Ð½Ð¾Ð³Ð¾ Ð¿ÐµÐ¿ÑÐ¸Ð´Ð° Ð±Ð°ÐºÑÐµÐ½ÐµÑÐ¸Ð½Ð° 3.4 Ð»ÐµÐ¹ÐºÐ¾ÑÐ¸ÑÐ¾Ð² Ð´Ð¾Ð¼Ð°ÑÐ½ÐµÐ¹ ÐºÐ¾Ð·Ñ Ð¸ ÐµÐ³Ð¾ ÑÑÑÑÐºÑÑÑÐ½ÑÑ Ð¼Ð¾Ð´Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¹ Ð½Ð° Ð³ÑÐ°Ð¼Ð¿Ð¾Ð»Ð¾Ð¶Ð¸ÑÐµÐ»ÑÐ½ÑÐµ Ð¸ Ð³ÑÐ°Ð¼Ð¾ÑÑÐ¸ÑÐ°ÑÐµÐ»ÑÐ½ÑÐµ Ð±Ð°ÐºÑÐµÑÐ¸Ð¸, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¸Ð·ÑÑÐµÐ½Ñ Ð¸Ñ ÑÑÑÐµÐºÑÑ Ð² Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸Ð¸ ÑÑÐºÐ°ÑÐ¸Ð¾ÑÐ¸ÑÐµÑÐºÐ¸Ñ ÐºÐ»ÐµÑÐ¾Ðº. ÐÐµÑÐ¾Ð´Ð¾Ð¼ ÑÐµÑÐ¸Ð¹Ð½ÑÑ ÑÐ°Ð·Ð²ÐµÐ´ÐµÐ½Ð¸Ð¹ Ð² Ð¶Ð¸Ð´ÐºÐ¾Ð¹ Ð¿Ð¸ÑÐ°ÑÐµÐ»ÑÐ½Ð¾Ð¹ ÑÑÐµÐ´Ðµ, ÑÐ¾Ð´ÐµÑÐ¶Ð°ÑÐµÐ¹ Ð¼Ð¸ÐºÑÐ¾Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð¼Ñ, Ð½Ð°Ð¹Ð´ÐµÐ½Ñ Ð¼Ð¸Ð½Ð¸Ð¼Ð°Ð»ÑÐ½ÑÐµ Ð¸Ð½Ð³Ð¸Ð±Ð¸ÑÑÑÑÐ¸Ðµ ÑÐ¾ÑÑ Ð±Ð°ÐºÑÐµÑÐ¸Ð¹ ÐºÐ¾Ð½ÑÐµÐ½ÑÑÐ°ÑÐ¸Ð¸ Ð¿ÐµÐ¿ÑÐ¸Ð´Ð¾Ð². Ð¡ Ð¿Ð¾Ð¼Ð¾ÑÑÑ ÑÑÐ¾Ð¼Ð¾Ð³ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¼Ð°ÑÐºÐµÑÐ° Ð¿ÑÐ¾Ð²ÐµÐ´ÑÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ Ð¸ÑÑÐ»ÐµÐ´ÑÐµÐ¼ÑÑ ÑÑÑÑÐºÑÑÑÐ½ÑÑ Ð°Ð½Ð°Ð»Ð¾Ð³Ð¾Ð² Ð½Ð° Ð¿ÑÐ¾Ð½Ð¸ÑÐ°ÐµÐ¼Ð¾ÑÑÑ Ð¿Ð»Ð°Ð·Ð¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ð¹ Ð¼ÐµÐ¼Ð±ÑÐ°Ð½Ñ Ð±Ð°ÐºÑÐµÑÐ¸Ð¸ Escherichia coli ML-35Ñ Ð² ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ð¸ Ñ Ð´ÐµÐ¹ÑÑÐ²Ð¸ÐµÐ¼ Ð¼ÐµÐ¼Ð±ÑÐ°Ð½Ð¾Ð°ÐºÑÐ¸Ð²Ð½Ð¾Ð³Ð¾ Ð¿ÐµÐ¿ÑÐ¸Ð´Ð° ÑÐ´Ð° Ð¿ÑÐµÐ»Ñ - Ð¼ÐµÐ»Ð¸ÑÑÐ¸Ð½Ð°. ÐÐ¾Ð»ÑÑÐµÐ½Ñ Ð´Ð°Ð½Ð½ÑÐµ Ð¾ ÑÐ¸ÑÐ¾ÑÐ¾ÐºÑÐ¸ÑÐ½Ð¾ÑÑÐ¸ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÐµÐ¼ÑÑ Ð±Ð°ÐºÑÐµÐ½ÐµÑÐ¸Ð½Ð¾Ð² Ð´Ð»Ñ Ð¾Ð¿ÑÑÐ¾Ð»ÐµÐ²ÑÑ ÐºÐ»ÐµÑÐ¾Ðº Ð¸ Ð½ÐµÑÑÐ°Ð½ÑÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÑ Ð¼Ð¾Ð½Ð¾Ð½ÑÐºÐ»ÐµÐ°ÑÐ½ÑÑ Ð»ÐµÐ¹ÐºÐ¾ÑÐ¸ÑÐ¾Ð² Ð¿ÐµÑÐ¸ÑÐµÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÐºÑÐ¾Ð²Ð¸ ÑÐµÐ»Ð¾Ð²ÐµÐºÐ°. Ð¡ Ð¿Ð¾Ð¼Ð¾ÑÑÑ ÐºÑÐ°ÑÐ¸ÑÐµÐ»Ñ ÑÑÐ¸Ð¿Ð°Ð½Ð¾Ð²Ð¾Ð³Ð¾ ÑÐ¸Ð½ÐµÐ³Ð¾ Ð¸Ð·ÑÑÐµÐ½Ð° Ð´Ð¸Ð½Ð°Ð¼Ð¸ÐºÐ° ÑÐ¸ÑÐ¾ÑÐ¾ÐºÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ Ð¿ÐµÐ¿ÑÐ¸Ð´Ð¾Ð² Ð½Ð° ÑÐ°ÐºÐ¾Ð²ÑÐµ ÐºÐ»ÐµÑÐºÐ¸.
ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð±Ð¸Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð°ÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð´Ð°Ð½Ð½ÑÑ Ð¿ÐµÐ¿ÑÐ¸Ð´Ð¾Ð² Ð´Ð°Ð»Ð¾ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÑ Ð¿Ð¾Ð»ÑÑÐ¸ÑÑ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ñ Ð¾ Ð²Ð°Ð¶Ð½Ð¾ÑÑÐ¸ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð½ÑÑ ÑÐ¸Ð·Ð¸ÐºÐ¾-ÑÐ¸Ð¼Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ²Ð¾Ð¹ÑÑÐ² Ð¸Ñ Ð¼Ð¾Ð»ÐµÐºÑÐ» (Ð³Ð¸Ð´ÑÐ¾ÑÐ¾Ð±Ð½Ð¾ÑÑÐ¸ Ð¸ Ð²ÐµÐ»Ð¸ÑÐ¸Ð½Ñ Ð¿Ð¾Ð»Ð¾Ð¶Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð·Ð°ÑÑÐ´Ð°) Ð´Ð»Ñ Ð¿ÑÐ¾ÑÐ²Ð»ÐµÐ½Ð¸Ñ Ð¸Ñ Ð°Ð½ÑÐ¸Ð±Ð°ÐºÑÐµÑÐ¸Ð°Ð»ÑÐ½ÑÑ ÑÑÑÐµÐºÑÐ¾Ð² Ð¸ Ð´Ð»Ñ Ð¸Ñ ÑÐ¸ÑÐ¾ÑÐ¾ÐºÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ Ð½Ð° ÐºÐ»ÐµÑÐºÐ¸ Ð¼Ð°ÐºÑÐ¾Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð¼Ð°.
The Thermal Renormalization Group for Fermions, Universality, and the Chiral Phase-Transition
Creators: name: Bergerhoff, Bastian
name: Manus, Johannes
name: Reingruber, Juergen
Publisher: name: arXiv
Year: 1999
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Condensed Matter (cond-mat)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We formulate the thermal renormalization group, an implementation of the Wilsonian RG in the real-time (CTP) formulation of finite temperature field theory, for fermionic fields. Using a model with scalar and fermionic degrees of freedom which should describe the two-flavor chiral phase-transition, we discuss the mechanism behind fermion decoupling and universality at second order transitions. It turns out that an effective mass-like term in the fermion propagator which is due to thermal fluctuations and does not break chiral symmetry is necessary for fermion decoupling to work. This situation is in contrast to the high-temperature limit, where the dominance of scalar over fermionic degrees of freedom is due to the different behavior of the distribution functions. The mass-like contribution is the leading thermal effect in the fermionic sector and is missed if a derivative expansion of the fermionic propagator is performed. We also discuss results on the phase-transition of the model considered where we find good agreement with results from other methods.
description: References added, minor typos corrected
Additional file 1: of Cortisol levels in different tissue samples in posttraumatic stress disorder patients versus controls: a systematic review and meta-analysis protocol
Creators: name: Heuvel, Leigh Van Den
name: Wright, Simonne
name: Sharain Suliman
name: Stalder, Tobias
name: Kirschbaum, Clemens
name: Seedat, Soraya
Publisher: name: figshare
Year: 2019
Subjects: subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Table summarising published systematic reviews examining basal cortisol levels in posttraumatic stress disorder. (DOCX 17 kb)
Measurement of the Triple Higgs Coupling at a HE-LHC
Creators: name: Homiller, Samuel
name: Meade, Patrick
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The currently unmeasured triple Higgs coupling is one of the strong motivations for future physics programs at the LHC and beyond. A sufficiently precise measurement can lead to qualitative changes in our understanding of electroweak symmetry breaking and the cosmological history of the Higgs potential. As such, the quantitative measurement of this coupling is now one of the benchmark measurements for any proposed collider. We study the capability of a potential $27\,\mathrm{TeV}$ HE-LHC upgrade in measuring the Higgs trilinear coupling via the di-Higgs production process in the $b\bar{b}γγ$ channel. We emphasize that a key background from single Higgs production via gluon fusion has been underestimated and underappreciated in prior studies. We perform a detailed study taking into account two different potential detector scenarios, and validate against HL-LHC projections from ATLAS. We find that the di-Higgs production process can be observed at $\geq 4.5 σ$, corresponding to a $\sim 40\%$ measurement of the Higgs self-coupling, with $15\,\mathrm{ab}^{-1}$ of data at the HE-LHC.
description: 29 pages, 7 figures; matches version published in JHEP
Physics of a clumpy lensed galaxy at z=1.6
Creators: name: Girard, M.
name: Dessauges-Zavadsky, M.
name: Schaerer, D.
name: Richard, J.
name: Nakajima, K.
name: Cava, A.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Observations have shown that massive star-forming clumps are present in the internal structure of high-redshift galaxies. One way to study these clumps in detail with a higher spatial resolution is by exploiting the power of strong gravitational lensing which stretches images on the sky. In this work, we present an analysis of the clumpy galaxy A68-HLS115 at $z=1.5858$, located behind the cluster Abell 68, but strongly lensed by a cluster galaxy member. Resolved observations with SINFONI/VLT in the near-infrared show Ha, Hb, [NII], and [OIII] emission lines. Combined with images covering the B band to the far-infrared and CO(2-1) observations, this makes this galaxy one of the only sources for which such multi-band observations are available and for which it is possible to study the properties of resolved star-forming clumps and to perform a detailed analysis of the integrated properties, kinematics, and metallicity. We obtain a stability of $\upsilon_{rot}/σ_0 = 2.73$ by modeling the kinematics, which means that the galaxy is dominated by rotation, but this ratio also indicates that the disk is marginally stable. We find a high intrinsic velocity dispersion of $80\pm10$ km s$^{-1}$ that could be explained by the high gas fraction of $f_{gas}=0.75\pm0.15$ observed in this galaxy. This high $f_{gas}$ and the observed sSFR of $\rm 3.12 \, Gyr^{-1}$ suggest that the disk turbulence and instabilities are mostly regulated by incoming gas. The direct measure of the Toomre stability criterion of $Q_{crit}=0.70$ could also indicate the presence of a quasi-stable thick disk. Finally, we identify three clumps in the Ha map which have similar velocity dispersions, metallicities, and seem to be embedded in the rotating disk. These three clumps contribute together to $40\%$ on the SFR(Ha) of the galaxy and show a SFR density about $100$ times higher than HII regions in the local Universe.
description: Accepted for publication in A&A. 10 pages, 7 figures
Croton eluteria W. Wright 1787
Creators: name: Jarvis, Charlie
Publisher: name: Linnaean Society of London in association with the Natural History Museum
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Malpighiales
Euphorbiaceae
Croton
Croton eluteria

description: Clutia eluteria Linnaeus, Species Plantarum 2: 1042. 1753.
"Habitat in Indiis." RCN: 7534.
 Lectotype (designated here by Berry): Herb. Clifford: 486, Elutheria 1 (BM).
 Current name:  Croton eluteria  (L.) W. Wright (Euphorbiaceae).
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part C), pp. 370-473 in Order out of Chaos. Linnaean Plant Types and their Types, London :Linnaean Society of London in association with the Natural History Museum on page 429, DOI: 10.5281/zenodo.291971
Design work for the install of a vision system at Berry Plastics
Creators: name: Lasher, Chris
Publisher: name: Unknown
Year: 2014

description: This report documents the decision and design processes undertook to do all preimplementation
work for adding a vision system onto a thermoforming line at Berry Plastics.
Several defects can occur on the plastic that is used to make the plastic parts. Often these defects
are not detected until Quality Assurance completes their part studies. This project consisted of
finding a vision system that could detect the defects. Then mechanical and electrical designs
were completed in order to mount and power the vision system. Once implemented, the vision
system is expected to save the company just under $26,000 a year with a payback period of 21
months.