cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Estimation « in situ » de l'efficacité de capteurs solaires sous vide pour la production d'eau chaude
Creators: name: Gambade, Julien
name: Noël, Hervé
name: Glouannec, Patrick
Publisher: name: Société Française de Thermique
Year: 2021
Subjects: Solaire Thermique
Mesures sur site
Bilan énergétique
Tubes sous vides

description: L'Union Européenne s'est engagée à augmenter de 17 à 27\% la part d'énergie renouvelable produite en Europe pour 2030 afin de diminuer les émissions de gaz à effet de serre. C'est dans ce contexte que le laboratoire est impliqué dans le projet Interreg NWE ICaRE4Farms dont l'objectif est de réduire l'usage des procédés de chauffage traditionnels à énergies fossiles par la production d'eau chaude solaire. Nos travaux concernent la mise en œuvre d'une instrumentation adaptée à des suivis in situ pour poser des bilans thermiques et développer des modèles numériques. Le site étudié dans le cadre de cette étude est situé dans les Cotes d'Armor, il est destiné à produire de l'eau chaude pour un élevage. L'installation solaire thermique utilise 24 Capteurs solaires à tubes sous vide non pressurisés avec circulation directe du fluide caloporteur dans les tubes par thermosiphon et ballon de stockage (CSSV). Cette installation est constituée de CSSV disposés tout d'abord en série pour la montée en température de l'eau puis en parallèle pour le stockage et le chauffage complémentaire. En fonctionnement standard, deux soutirages sont effectués quotidiennement. L'installation est non pressurisée, son soutirage est effectué par pompage et son remplissage par le réseau d'adduction en eau potable. L'objet de la communication est de présenter la métrologie mise en œuvre à l'échelle d'un CSSV et de montrer la démarche mise en œuvre afin de bien appréhender son fonctionnement et ses performances énergétiques. L'instrumentation mise en place, outre la station météorologique implantée sur le site, comprend des capteurs de température en entrée et sortie ainsi qu'à plusieurs niveaux dans le réservoir de stockage afin d'en étudier la stratification. Un débitmètre en entrée de l'installation nous donne le débit de circulation dans la rangée de CSSV. L'étude a pour objectif de quantifier, pour un CSSV en série, l'énergie fournie par la circulation, l'énergie stockée dans le ballon de stockage ainsi que ses déperditions et ainsi déterminer son efficacité en usage. Deux séquences expérimentales sont présentées et analysées dans cette communication.
The Vela Pulsar's Radio Nebula
Creators: name: Dodson, R.
name: Lewis, D.
name: McConnell, D.
name: Deshpande, A. A.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have discovered that the radio nebula surrounding the Vela pulsar covers a much wider extent than previously reported, with two lobes to the North and South of the pulsar. Indications of this object have been reported previously, but its symmetric morphology around the pulsar and other details had not been identified as they were hidden due to poor sensitivity to low spatial frequencies. The structure is highly polarised and the polarisation vectors, once corrected for Faraday rotation, reveal symmetry with respect to the spin axis of the pulsar. The X-ray emission found by Chandra lies at the centre of this structure, in a region which has no detectable excess of radio emission. We estimate total fluxes and regional fluxes from the Northern and Southern lobes, plus the X-ray region at four radio frequencies; 1.4, 2.4, 5 and 8.5 GHz. We present the corresponding images in both the total and polarised intensities, as well as those showing the derotated linear polarisation vectors.
description: 17 pages, to appear in MNRAS
A View through Faraday's Fog 2: Parsec Scale Rotation Measures in 40 AGN
Creators: name: Zavala, R. T.
name: Taylor, G. B.
Publisher: name: arXiv
Year: 2004
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Results from a survey of the parsec scale Faraday rotation measure properties for 40 quasars, radio galaxies and BL Lac objects are presented. Core rotation measures for quasars vary from approximately 500 to several thousand radians per meter squared. Quasar jets have rotation measures which are typically 500 radians per meter squared or less. The cores and jets of the BL Lac objects have rotation measures similar to those found in quasar jets. The jets of radio galaxies exhibit a range of rotation measures from a few hundred radians per meter squared to almost 10,000 radians per meter squared for the jet of M87. Radio galaxy cores are generally depolarized, and only one of four radio galaxies (3C-120) has a detectable rotation measure in the core. Several potential identities for the foreground Faraday screen are considered and we believe the most promising candidate for all the AGN types considered is a screen in close proximity to the jet. This constrains the path length to approximately 10 parsecs, and magnetic field strengths of approximately 1 microGauss can account for the observed rotation measures. For 27 out of 34 quasars and BL Lacs their optically thick cores have good agreement to a lambda squared law. This requires the different tau = 1 surfaces to have the same intrinsic polarization angle independent of frequency and distance from the black hole.
description: Accepted to the Astrophysical Journal: 71 pages, 40 figures
SWift -- A SignWriting improved fast transcriber
Creators: name: Bianchini, Claudia S.
name: Borgia, Fabrizio
name: Bottoni, Paolo
name: de Marsico, Maria
Publisher: name: arXiv
Year: 2019
Subjects: subject: Computation and Language (cs.CL)
subject: Human-Computer Interaction (cs.HC)
subject: FOS: Computer and information sciences

description: We present SWift (SignWriting improved fast transcriber), an advanced editor for computer-aided writing and transcribing using SignWriting (SW). SW is devised to allow deaf people and linguists alike to exploit an easy-to-grasp written form of (any) sign language. Similarly, SWift has been developed for everyone who masters SW, and is not exclusively deaf-oriented. Using SWift, it is possible to compose and save any sign, using elementary components called glyphs. A guided procedure facilitates the composition process. SWift is aimed at helping to break down the "electronic" barriers that keep the deaf community away from Information and Communication Technology (ICT). The editor has been developed modularly and can be integrated everywhere the use of SW, as an alternative to written vocal language, may be advisable.
Underthrusting of continental lithospheric mantle controls architecture of crustal deformation: Numerical modeling of the northern margin of the Tibetan plateau
Creators: name: Chen, Qizhi
name: Hu, Caibo
name: Zuza, Andrew V.
name: Zhang, Kai-jun
name: Zhang, Huai
name: Shi, Yaolin
Publisher: name: Geological Society of London
Year: 2025
Subjects: classificationCode: 3705
subject: Geology
subject: FOS: Earth and related environmental sciences

description: Supplementary material.
MOESM1 of BOMET-QoL-10 questionnaire for breast cancer patients with bone metastasis: the prospective MABOMET GEICAM study
Creators: name: A. Barnadas
name: M. Muñoz
name: M. Margelí
name: J. Chacón
name: J. Cassinello
name: S. Antolin
name: E. Adrover
name: M. Ramos
name: E. Carrasco
name: M. Jimeno
name: B. Ojeda
name: X. González
name: S. González
name: M. Constenla
name: J. Florián
name: A. Miguel
name: A. Llombart
name: A. Lluch
name: M. Ruiz-Borrego
name: R. Colomer
name: S. Barco
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Cancer
subject: Science Policy

description: Additional file 1. BOMET-QoL 10 points items
Stellar pollution and [Fe/H] in the Hyades
Creators: name: Dotter, Aaron
name: Chaboyer, Brian
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The Hyades open cluster presents a unique laboratory for planet formation and stellar pollution studies because all of the stars have essentially the same age and were born from the same cloud of gas. Furthermore, with an age of roughly 650 Myr most of the intermediate and low mass stars are on the main sequence. Given these assumptions, the accretion of metal rich material onto the surface of a star during and shortly after the formation of planetary systems should be evident via the enhanced metallicity of the star. Building on previous work, stellar evolution models which include the effects of stellar pollution are applied to the Hyades. The results of several Monte Carlo simulations, in which the amount of accreted material is drawn at random from a Gaussian distribution with standard deviation equal to half the mean, are presented. An effective temperature-[Fe/H] relation is produced and compared to recent observations. The theoretical predictions presented in this letter will be useful in future searches for evidence of stellar pollution due to planet formation. It is concluded that stellar pollution effects at the mean level of >=2 Earth masses of iron are ruled out by current observational data.
description: 10 pages, 3 figures, AASTeX, accepted to the ApJL
Additional file 1 of Analyses and interpretation of whole-genome gene expression from formalin-fixed paraffin-embedded tissue: an illustration with breast cancer tissues
Creators: name: Kibriya, Muhammad G
name: Jasmine, Farzana
name: Shantanu Roy
name: Paul-Brutus, Rachelle M
name: Argos, Maria
name: Habibul Ahsan
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Authors’ original file for figure 1
Thermodynamic Instabilities of Generalized Exotic BTZ Black Holes
Creators: name: Cong, Wan
name: Mann, Robert B.
Publisher: name: arXiv
Year: 2019
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We examine the conjecture that black holes violating the reverse isoperimetric inequality have negative specific heat at constant volume $C_V$. We test this conjecture on the family of generalized exotic Bañados, Teitelbiom and Zanelli (BTZ) black holes and find that $C_V$ can be positive even when the reverse isoperimetric inequality is violated, providing a counter example to the conjecture. However in all cases where $C_V$ is positive, the specific heat at constant pressure $C_P$ is negative, indicating that generalized exotic black holes are thermodynamically unstable, suggesting that a broader version of the conjecture might hold.
description: 4 pages, 2 figures
Neutrino Masses and Mixing Matrix from SU(1,1) Horizontal Symmetry
Creators: name: Inoue, Kenzo
name: Yamashita, Nao-aki
Publisher: name: arXiv
Year: 2003
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: A new mechanism is proposed to explain neutrino masses and their mixing via SU(1,1) horizontal symmetry breaking. Based on this mechanism smallness of neutrino masses is naturally realized and inverted hierarchical spectrum with large mixing is given.
description: 9 pages
Solar neutrinos as probes of neutrino-matter interactions
Creators: name: Friedland, Alexander
name: Lunardini, Cecilia
name: Pena-Garay, Carlos
Publisher: name: arXiv
Year: 2004
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Data from solar neutrino and KamLAND experiments have led to a discovery of nonzero neutrino masses. Here we investigate what these data can tell us about neutrino interactions with matter, including the poorly constrained flavor-changing nu_e-nu_tau interactions. We give examples of the interaction parameters that are excluded by the solar/KamLAND data and are beyond the reach of other experiments. We also demonstrate that flavor-changing interactions, at the allowed level, may profoundly modify the conversion probability for neutrinos of energy
description: 6 pages, 3 figures
Analyse du confort thermique dans une cavité ventilée selon la position de l'ouverture de sortie
Creators: name: Harnane, Yamina
name: Bouzid, Sihem
name: Berkane, Sonia
name: Brima, Abdelhafid
Publisher: name: Société Française de Thermique
Year: 2021
Subjects: simulation
convection mixte
confort thermique

description: La ventilation a une influence majeure sur le confort thermique et sur l'efficacité des installations thermiques. Ainsi, un bon système de ventilation peut fournir un environnement dont les conditions thermiques sont confortables avec une consommation d'énergie plus basse. La ventilation naturelle et mixte avec des ouvertures Entrée/Sortie choisit judicieusement est l'une des solutions qui s'avère intéressante. Dans cet article, nous présentons une étude numérique du transfert de chaleur par convection mixte dans une cavité carrée ventilée de hauteur 2,5~m et de largeur 2,5~m. L'écoulement est bidimensionnel en régime turbulent et stationnaire. Selon la disposition de l'ouverture de sortie de l'air, quatre configurations sont considérées, l'entrée étant fixe et disposée en bas de la paroi gauche. Toutes les parois sont considérées adiabatiques sauf la paroi gauche d'épaisseur l qui exposée à une densité de flux fixe donnant un nombre de Grashof égal $\unit{7\cdot 10^{13}}$. Le modèle de turbulence RNG k-$\varepsilon$ est adopté, les équations gouvernantes sont résolues numériquement en utilisant le code Fluent 14.0. L'algorithme SIMPLEC est choisi pour le couplage pression-vitesse sur un maillage structuré 140x150, raffiné près des parois, plus 90 cellules dans la paroi solide gauche. Pour évaluer les performances du confort thermique pour chaque cas d'étude, nous avons analysé la dynamique de l'écoulement qui est trouvée bicellulaire et sa thermique indique un bon rafraîchissement. L'objectif de cette étude est d'analyser l'influence de l'emplacement de l'ouverture de sortie sur le confort thermique à l'intérieur. Afin d'optimiser la meilleure configuration offrant le confort thermique, les résultats obtenus pour l'efficacité de la ventilation sont donnés en termes de température moyenne à l'intérieur de la cavité, de distribution de température $\varepsilon_T$. Afin de prévoir numériquement les zones de confort thermique, on a calculé température effective de tirage EDT. L'indice EDT montre une grande sensibilité de la température et de la vitesse de l'air sur la zone de confort thermique. L'indice EDT supérieur à +1,1 indique une zone d'inconfort chaud et lorsque EDT est inférieur à -1,7 on parle d'une zone d'inconfort froid. Lorsque cet indice est entre -1,7 et +1,1 ces zones sont en confort thermique.
The Vela Pulsar's proper motion and parallax derived from VLBI observations
Creators: name: Dodson, R.
name: Legge, D.
name: Reynolds, J. E.
name: McCulloch, P. M.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The Vela pulsar is the brightest pulsar at radio wavelengths. It was the object that told us (via its glitching) that pulsars were solid rotating bodies not oscillating ones. Along with the Crab pulsar is it the source of many of the models of pulsar behavior. Therefore it is of vital importance to know how far away it is, and its origin. The proper motion and parallax for the Vela pulsar have been derived from 2.3 and 8.4 GHz Very Long Baseline Interferometry (VLBI) observations. The data spans 6.8 years and consists of eleven epochs. We find a proper motion of $μ_{α{\rm cos}δ}= -49.61 \pm 0.06, μ_δ= 29.8 \pm 0.1$ \myr and a parallax of $3.4 \pm 0.2$ mas, which is equivalent to a distance of $293_{-17}^{+19}$ pc. When we subtract out the galactic rotation and solar peculiar velocity we find $μ_* = 45 \pm 1.3$ \myr with a position angle (PA) of $301^\circ\pm1.8$ which implies that the proper motion has a small but significant offset from the X-ray nebula's symmetry axis.
description: Corrected for some minor errors and referee's comments
Studies of Star-forming Complexes in the Galaxies NGC 628, NGC 2976, and NGC 3351
Creators: name: Smirnova, K. I.
name: Wiebe, D. S.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We analyze parameters of the interstellar matter emission in star-forming complexes in the high metallicity galaxies NGC~628, NGC~2976, and NGC~3351, which have different morphological types. The relation between H$α$ emission and emission in CO and HI lines is considered along with the relation between H$α$ emission and dust emission in the infrared range (IR). The fluxes and surface brightnesses in the UV and IR correlate well with H$α$ emission. The HI emission also correlates well with H$α$, while the correlation between the CO and H$α$ emission is much less prominent. The ratio of the fluxes at 8 and 24 $μ$m decreases with increasing H$α$ flux. This may be due to changes in the properties of the dust ensemble (a decrease in the mass fraction of polycyclic aromatic hydrocarbons) or to changes in excitation conditions. Analysis of the kinematics of the CO lines shows that the CO flux grows with increasing velocity scatter $ΔV$ when $ΔV\lesssim70$~km/s. Preliminary evidence for the existence of star-forming complexes with higher values of $ΔV$ is presented, and the increase in the velocity scatter is accompanied by a decrease in the CO line luminosity of the complex.
description: 24 pages, 9 figures, 1 table
MOESM2 of The effect of an educational program for pregnant women to prevent allergic diseases in infants: study protocol for a randomized controlled trial
Creators: name: Nakamura, Rie
name: Ishiguro, Nao
name: Naru, Eiji
name: Ishitsuka, Yukiko
name: Nakade, Masato
name: Nezu, Yoko
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Cell Biology
subject: Physiology
subject: FOS: Biological sciences
subject: Pharmacology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Developmental Biology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Additional file 2. Consent, enrolment/allocation, and assessment of subjects according to SPRIT format.
Olidiana egregia Nielson 2015, n. comb.
Creators: name: Nielson, M. W.
Publisher: name: Zenodo
Year: 2015
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Cicadellidae
Olidiana
Olidiana egregia

description: Olidiana egregia (Schumacher), n. comb.
(Plate 3 G, H, Fig. 183-188)
 Description. Length. Male 8.20 mm., female 9.40 mm.
 External morphology. Moderately large, robust species. General color black to dark brown with 2 broad, yellow transverse bands on forewings; mesonotum and pronotum black; crown light brown; eyes dark brown; face in male black, in female brown; head narrower than pronotum, broadly rounded anteriorly; crown short, narrower than width of eyes, slightly produced anteriorly, lateral margins convergent basally; eyes large, semiglobular; clypeus long, broad, lateral margins broadly convex; clypellus in male obscured by glue, short, narrow in female. (Female body slightly teneral.)
 Male genitalia. Pygofer in lateral view large, sub-triangulate, small digitate caudoventral lobe mesally, small lobe apically, few setae apically (Fig. 183); aedeagus with long bifurcate, subapical process, one with row of secondary setae, one glabrous (Fig. 184, 185); style in dorsal view elongate, curved near middle (Fig. 186); dorsal connective long, narrow (Fig. 184); connective large, anterior arms broad, medial ridge absent, stem small, sub-quadrate (Fig. 187); subgenital plate long, broad in basal 1/5, membranous stripe in apical 1/5 on inner lateral margin (Fig. 188).
 Female seventh sternal segment. Length about twice as long as penultimate segment, posterior margin truncate, slightly sinuate, slightly teneral.
 Material examined. Jassus egregius Schumacher. Lectotype male, here designated: Formosa (Taiwan), Kosempo, H. Sauter, 1911 / 7. IV / Eberswalde, Coll. EDI / Jassus egregius Schumacher, Typen (in Schumacher’s handwriting), P. Schumacher det. / Syntypus (Red label) / DE Hemimetabola, #100093 (White label) / DEI Müncheberg, Hemi - 0001 (Green label). Jassus egregius Schumacher, syntype female, Formosa (Taiwan), Kosempo, Formosa, H. Sauter 1911 / 7. V. / Schumacher, det. / Eberswalde Coll., DEI / Syntypus (Red Label) / DEI Hemimetabola #100094 / DEI Müncheberg, Hemi – 00002 (DEI).
 Remarks. The species is a member of the O. brevis (Walker) species complex. Distinguishing features which separate O. egregia from related species are found in Table 2 and illustrated in Figures 1-12. Two “ syntypes ” of Jassus egregia Schumacher were located in the Senckenberg Deutsches Entomologische Institute in Müncheberg, Germany. The handwritten “Typen” label attached to the male specimen by Schumacher may be considered an important issue which may or may not impact the lectotype designation.
description: Published as part of Nielson, M. W., 2015, A revision of the tribe Coelidiini of the Oriental, Palearctic and Australian biogeographical regions (Hemiptera: Cicadellidae: Coelidiinae), pp. 1-202 in Insecta Mundi 2015 (410) on pages 42-43, DOI: 10.5281/zenodo.5181587
Gap and embedded solitons in microwave-coupled binary condensates
Creators: name: Fan, Zhiwei
name: Chen, Zhaopin
name: Li, Yongyao
name: Malomed, Boris A.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Quantum Gases (cond-mat.quant-gas)
subject: Pattern Formation and Solitons (nlin.PS)
subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: It was recently found that, under the action of the spin-orbit coupling (SOC) and Zeeman splitting (ZS), binary BEC with intrinsic cubic nonlinearity supports families of gap solitons, provided that the kinetic energy is negligible in comparison with the SOC and ZS terms. We demonstrate that, also under the action of SOC and ZS, a similar setting may be introduced for BEC with two components representing different atomic states, resonantly coupled by microwave radiation, while the Poisson equation accounts for the feedback of the two-component atomic wave function onto the radiation. The microwave-mediated interaction induces an effective nonlinear trapping potential, which strongly affects the purport of the linear spectrum in this system. As a result, families of both gap and embedded solitons (those overlapping with the continuous spectrum) are found, being chiefly stable. The shape of the solitons features exact or broken skew symmetry. In addition to fundamental solitons (whose shape may or may not include a node), a family of dipole solitons is constructed too, which are even more stable than their fundamental counterparts. A nontrivial stability area is identified for moving solitons in the present system, which lacks Galilean invariance. Colliding solitons merge into a single one.
description: to be published in Physical Review A
Additional file 2 of Analyses and interpretation of whole-genome gene expression from formalin-fixed paraffin-embedded tissue: an illustration with breast cancer tissues
Creators: name: Kibriya, Muhammad G
name: Jasmine, Farzana
name: Shantanu Roy
name: Paul-Brutus, Rachelle M
name: Argos, Maria
name: Habibul Ahsan
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Authors’ original file for figure 2
Boltzmann-Gibbs thermal equilibrium distribution for classical systems and Newton law: A computational discussion
Creators: name: Baldovin, Fulvio
name: Moyano, Luis G.
name: Tsallis, Constantino
Publisher: name: arXiv
Year: 2004
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: We implement a general numerical calculation that allows for a direct comparison between nonlinear Hamiltonian dynamics and the Boltzmann-Gibbs canonical distribution in Gibbs $Γ$-space. Using paradigmatic first-neighbor models, namely, the inertial XY ferromagnet and the Fermi-Pasta-Ulam $β$-model, we show that at intermediate energies the Boltzmann-Gibbs equilibrium distribution is a consequence of Newton second law (${\mathbf F}=m{\mathbf a}$). At higher energies we discuss partial agreement between time and ensemble averages.
description: New title, revision of the text. EPJ latex, 4 figures
Growth of Inflaton Perturbations and the Post-Inflation Era in Supersymmetric Hybrid Inflation Models
Creators: name: Broadhead, Matt
name: McDonald, John
Publisher: name: arXiv
Year: 2003
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: It has been shown that hybrid inflation may end with the formation of non-topological solitons of inflaton field. As a first step towards a fully realistic picture of the post-inflation era and reheating in supersymmetric hybrid inflation models, we study the classical scalar field equations of a supersymmetric hybrid inflation model using a semi-analytical ansatz for the spatial dependence of the fields. Using the minimal D-term inflation model as an example, the inflaton field is evolved using the full 1-loop effective potential from the slow-rolling era to the U(1)_{FI} symmetry-breaking phase transition. Spatial perturbations of the inflaton corresponding to quantum fluctuations are introduced for the case where there is spatially coherent U(1)_{FI} symmetry breaking. The maximal growth of the dominant perturbation is found to depend only on the ratio of superpotential coupling λto the gauge coupling g. The inflaton condensate fragments to non-topological solitons for λ/g > 0.09. Possible consequences of non-topological soliton formation in fully realistic SUSY hybrid inflation models are discussed.
description: 27 pages LaTeX, 8 figures. Additional references and discussion
Additional file 3 of Analyses and interpretation of whole-genome gene expression from formalin-fixed paraffin-embedded tissue: an illustration with breast cancer tissues
Creators: name: Kibriya, Muhammad G
name: Jasmine, Farzana
name: Shantanu Roy
name: Paul-Brutus, Rachelle M
name: Argos, Maria
name: Habibul Ahsan
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Authors’ original file for figure 3
Generalised thresholding of hidden variable network models with scale-free property
Creators: name: Balogh, Sámuel G.
name: Pollner, Péter
name: Palla, Gergely
Publisher: name: arXiv
Year: 2019
Subjects: subject: Physics and Society (physics.soc-ph)
subject: Data Analysis, Statistics and Probability (physics.data-an)
subject: FOS: Physical sciences

description: The hidden variable formalism (based on the assumption of some intrinsic node parameters) turned out to be a remarkably efficient and powerful approach in describing and analyzing the topology of complex networks. Owing to one of its most advantageous property - namely proven to be able to reproduce a wide range of different degree distribution forms - it has become a standard tool for generating networks having the scale-free property. One of the most intensively studied version of this model is based on a thresholding mechanism of the exponentially distributed hidden variables associated to the nodes (intrinsic vertex weights), which give rise to the emergence of a scale-free network where the degree distribution $p(k)\sim k^{-γ}$ is decaying with an exponent of $γ=2$. Here we propose a generalization and modification of this model by extending the set of connection probabilities and hidden variable distributions that lead to the aforementioned degree distribution, and analyze the conditions leading to the above behavior analytically. In addition, we propose a relaxation of the hard threshold in the connection probabilities, which opens up the possibility for obtaining sparse scale free networks with arbitrary scaling exponent.
Stylolidia Nielson 1986
Creators: name: Nielson, M. W.
Publisher: name: Zenodo
Year: 2015
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Cicadellidae
Stylolidia

description: Stylolidia Nielson 1986: 137
 Type species, Stylolidia pectinata, sp. nov.
 Description. The genus has features similar to Olidiana in general habitus and to Taharana in aedeagal characters. Absence of aedeagal processes and presence of spines distally on the style will readily distinguish the genus.
 Stylolidia was originally described from 2 species from Malaysia. One new species was recently described from Thailand with a key to 3 known species (Freytag 2010a).
description: Published as part of Nielson, M. W., 2015, A revision of the tribe Coelidiini of the Oriental, Palearctic and Australian biogeographical regions (Hemiptera: Cicadellidae: Coelidiinae), pp. 1-202 in Insecta Mundi 2015 (410) on page 55, DOI: 10.5281/zenodo.5181587
XMM-Newton observations of an absorbed z=0.67 QSO: no dusty torus?
Creators: name: Georgantopoulos, I.
name: Georgakakis, A.
name: Stewart, G. C.
name: Akylas, A.
name: Boyle, B. J.
name: Shanks, T.
name: Griffiths, R. E.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present XMM-Newton observations of AXJ0341.4-4453, a mildly reddened A_V<7 QSO at a redshift of z=0.672. The XMM-Newton spectrum shows a large obscuring column N_H~10^23 cm^{-2} corresponding to A_V~70, in agreement with previous results based on the lower limit of the ASCA hardness ratio. The X-ray spectrum is represented by a 'scattering' model with Gamma~2.0 with the scattered power-law normalization being a few per cent of the hard component. No FeK line is detected with a 90 per cent upper limit on its equivalent width of ~360eV. The large discrepancy between the column density observed in X-rays and that inferred from the Balmer decrement can be explained by dust sublimation near the nucleus. Then, the X-ray and the optical obscuration come from two different regions: the X-ray close to the accretion disk while the optical at much larger >0.25pc scales.
description: To appear in MNRAS
MOESM1 of The effect of an educational program for pregnant women to prevent allergic diseases in infants: study protocol for a randomized controlled trial
Creators: name: Nakamura, Rie
name: Ishiguro, Nao
name: Naru, Eiji
name: Ishitsuka, Yukiko
name: Nakade, Masato
name: Nezu, Yoko
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Additional file 1. Standard Protocol Items: Recommendations for Interventional Trial (SPIRIT) 2013 Checklist: recommended items to address in a clinical trial protocol and related documents.
A class of solitons in Maxwell-scalar and Einstein-Maxwell-scalar models
Creators: name: Herdeiro, Carlos A. R.
name: Oliveira, João M. S.
name: Radu, Eugen
Publisher: name: arXiv
Year: 2019
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Recently, no-go theorems for the existence of solitonic solutions in Einstein-Maxwell-scalar (EMS) models have been established in arXiv:1902.07721. Here we discuss how these theorems can be circumvented by a specific class of non-minimal coupling functions between a real, canonical scalar field and the electromagnetic field. When the non-minimal coupling function diverges in a specific way near the location of a point charge, it regularises all physical quantities yielding an everywhere regular, localised lump of energy. Such solutions are possible even in flat spacetime Maxwell-scalar models, wherein the model is fully integrable in the spherical sector, and exact solutions can be obtained, yielding an explicit mechanism to de-singularise the Coulomb field. Considering their gravitational backreaction, the corresponding (numerical) EMS solitons provide a simple example of self-gravitating, localised energy lumps.
description: 16 pages, 2 figures
Macroscopic Quantum Tunneling and Quasiparticle Dissipation in d-wave Superconductor Josephson Junctions
Creators: name: Kawabata, Shiro
name: Kashiwaya, Satoshi
name: Asano, Yasuhiro
name: Tanaka, Yukio
Publisher: name: arXiv
Year: 2004
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We examine the macroscopic quantum tunneling (MQT) in high-Tc superconductor Josephson junctions with a d-wave order parameter. Using microscopic Hamiltonian and the functional integral method, we analytically obtain the MQT rate (the inverse lifetime of the metastable state) for the c-axis twist Josephson junctions. In the case of the zero twist angle, the system shows the super-Ohmic dissipation due to the presence of the nodal quasiparticle tunneling. Therefore, the MQT rate is strongly suppressed in compared with the finite twist angle cases.
description: 4 pages, 1 figure, to appear in Phys. Rev. B 70 (2004) No.9
Hot Subdwarf All Southern Sky Fast Transit Survey with the Evryscope
Creators: name: Ratzloff, Jeffrey K.
name: Barlow, Brad N.
name: Nemeth, Peter
name: Corbett, Henry T.
name: Walser, Stephen
name: Galliher, Nathan W.
name: Glazier, Amy
name: Howard, Ward S.
name: Law, Nicholas M.
Publisher: name: arXiv
Year: 2019
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: We have conducted a survey of candidate hot subdwarf stars in the southern sky searching for fast transits, eclipses, and sinusoidal like variability in the Evryscope light curves. The survey aims to detect transit signals from Neptune size planets to gas-giants, and eclipses from M-dwarfs and brown dwarfs. The other variability signals are primarily expected to be from compact binaries and reflection effect binaries. Due to the small size of hot subdwarfs, transit and eclipse signals are expected to last only twenty minutes, but with large signal depths (up to completely eclipsing if the orientation is edge on). With its 2-minute cadence and continuous observing Evryscope is well placed to recover these fast transits and eclipses. The very large field of view (8150 sq. deg.) is critical to obtain enough hot subdwarf targets, despite their rarity. We identified 11,000 potential hot subdwarfs from the 9.3M Evryscope light curves for sources brighter than mg = 15. With our machine learning spectral classifier, we flagged high-confidence targets and estimate the total hot subdwarfs in the survey to be 1400. The light curve search detected three planet transit candidates, shown to have stellar companions from followup analysis. We discovered several new compact binaries (including two with unseen degenerate companions, and several others with potentially rare secondaries), two eclipsing binaries with M-dwarf companions, as well as new reflection effect binaries and others with sinusoidal like variability. The hot subdwarf discoveries identified here are spectroscopically confirmed and we verified the Evryscope discovery light curve with TESS light curves when available. Four of the discoveries are in the process of being published in separate followup papers, and we discuss the followup potential of several of the other discoveries.
description: Accepted to ApJ, December 2019
Laosolidia Nielson 2015, gen. nov.
Creators: name: Nielson, M. W.
Publisher: name: Zenodo
Year: 2015
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Cicadellidae
Laosolidia

description: Laosolidia, gen. nov.
 Type species, Laosolidia complexa, sp. nov.
 Description. Moderately large, slender species. Length male 8.20-8.50 mm., female 9.90 mm. General color dark brown to black with numerous small, yellow specks on forewings, veins marked with ivory dashes; head distinctly narrower than pronotum, obtusely angulate anteriorly; crown narrower than width of eyes, slightly produced anteriorly; eyes large, elongate ovoid; pronotum large, about ½ longer medially than crown, surface bullae yellow; mesonotum large, slightly longer medially than pronotum; forewings long, slender, venation typical; clypeus long, slender, nearly twice as long as clypellus; clypellus narrower than base of clypeus at juncture of clypeal suture, with medial longitudinal inflated ridge, flared laterally at apex; pygofer in lateral view with semi-oval, mesal subapical indentation on caudoventral margin, without typical long caudoventral or caudodorsal processes, apex slightly lobed; aedeagus asymmetrical, inflated in dorsal and lateral views, with processes on shaft; style short with apophysis about as long as base; dorsal connective long, narrow; connective nearly wholly membranous between arms, stem rectangular; subgenital plate very long, broad with subapical constriction or tapered toward apex.
 Etymology. The name is a combination of the root Laos after the country and the suffix -olidia, an arbitrary name derived from the genus Coelidia. The gender is feminine.
 Remarks. The genus has a unique combination of characters which consists of the following features: inflated, constricted aedeagus with an assortment of processes, broad subgenital plate and presence of a mesal ovate, subapical indentation on the caudoventral margin of the pygofer. It is most closely related to Jenolidia and is distinguished from it by the above combination of characters. Three new species are assigned to the genus, all from Laos.
description: Published as part of Nielson, M. W., 2015, A revision of the tribe Coelidiini of the Oriental, Palearctic and Australian biogeographical regions (Hemiptera: Cicadellidae: Coelidiinae), pp. 1-202 in Insecta Mundi 2015 (410) on pages 32-33, DOI: 10.5281/zenodo.5181587
Spectral Line Identification and Modelling (SLIM) in the MAdrid Data CUBe Analysis (MADCUBA) package: An interactive software for data cube analysis
Creators: name: Martín, S.
name: Martín-Pintado, J.
name: Blanco-Sánchez, C.
name: Rivilla, V. M.
name: Rodríguez-Franco, A.
name: Rico-Villas, F.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: In this paper we present the detailed formalism at the core of the Spectral Line Identification and Modelling (SLIM) within the MAdrid Data CUBe Analysis (MADCUBA) package and their main data handling functionalities. These tools have been developed to visualize, analyze and model large spectroscopic data cubes. We present the highly interactive on-the-fly visualization and modelling tools of MADCUBA and SLIM, which includes an stand-alone spectroscopic database. The parameters stored therein are used to solve the full radiative transfer equation under Local Thermodynamic Equilibrium (LTE). SLIM provides tools to generate synthetic LTE model spectra based on input physical parameters of column density, excitation temperature, velocity, line width and source size. SLIM also provides an automatic fitting algorithm to obtain the physical parameters (with their associated errors) better fitting the observations. Synthetic spectra can be overlayed in the data cubes/spectra to easy the task of multi-molecular line identification and modelling.We present the Java-based MADCUBA and its internal module SLIM packages which provide all the necessary tools for manipulation and analysis of spectroscopic data cubes. We describe in detail the spectroscopic fitting equations and make use of this tool to explore the breaking conditions and implicit errors of commonly used approximations in the literature. Easy-to-use tools like MADCUBA allow the users to derive the physical information from spectroscopic data without the need of resourcing to simple approximations. SLIM allows to use the full radiative transfer equation, and to interactively explore the space of physical parameters and associated uncertainties from observational data.
description: 18 pages, 7 Figures, Accepted for publication in A&A
The Economic Impact of the 2015 Avian Influenza outbreak on U.S. Egg Prices
Creators: name: Dobrowolska, Agnieszka
name: Brown, Scott
name: Dobrowolska, Agnieszka
name: Brown, Scott
Publisher: name: Unknown
Year: 2016
Subjects: Agricultural marketing

description: This study provides a partial equilibrium approach to quantifying the effect of the Highly Pathogenic Avian Influenza (HPAI) outbreak that occurred in the United States in late 2014 and early 2015. The quarterly model provides an estimate of egg prices that would have occurred over this period without the HPAI outbreak. This research also provides sensitivity analysis around the estimated retail demand elasticity based on a review of the literature surrounding the retail demand for eggs in the United States.
D-Branes in Topological Membranes
Creators: name: Ferreira, P. Castelo
name: Kogan, I. I.
name: Szabo, R. J.
Publisher: name: arXiv
Year: 2003
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: It is shown how two-dimensional states corresponding to D-branes arise in orbifolds of topologically massive gauge and gravity theories. Brane vertex operators naturally appear in induced worldsheet actions when the three-dimensional gauge theory is minimally coupled to external charged matter and the orbifold relations are carefully taken into account. Boundary states corresponding to D-branes are given by vacuum wavefunctionals of the gauge theory in the presence of the matter, and their various constraints, such as the Cardy condition, are shown to arise through compatibility relations between the orbifold charges and bulk gauge invariance. We show that with a further conformally-invariant coupling to a dynamical massless scalar field theory in three dimensions, the brane tension is naturally set by the bulk mass scales and arises through dynamical mechanisms. As an auxilliary result, we show how to describe string descendent states in the three-dimensional theory through the construction of gauge-invariant excited wavefunctionals.
description: 78 pages, 12 figures
Hamusolidia introrsa Nielson 2015, sp. nov.
Creators: name: Nielson, M. W.
Publisher: name: Zenodo
Year: 2015
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Cicadellidae
Hamusolidia
Hamusolidia introrsa

description: Hamusolidia introrsa, sp. nov.
(Plate 2I, Fig. 134-140)
 Description. Length. Male 8.85 mm., female 9.40 mm.
 External morphology. Moderately large, slender species. General color dark brown to black with numerous, small yellow spots except on head, light to dark brown; face tannish with orange longitudinal stripe on inner lateral margins of clypeus; clypellus brown; head small, distinctly narrower than pronotum, anterior margin narrowly obtuse; crown short, narrow, narrower than width of eyes, produced about ¼ distance beyond anterior margin of eyes; eyes large, semiglobular; pronotum slightly longer medially than crown, surface bullated; mesonotum large, slightly longer medially than pronotum; forewings with typical venation; clypeus long, narrow, lateral margins broadly convex; clypellus short, about 1/3 as long as clypeus, narrow, slightly inflated longitudinally on middle, apex flared laterally.
 Male genitalia. Pygofer in lateral view broadly triangular, small lobe apically, with narrow, mesal caudoventral lobe, glabrous (Fig. 134); aedeagus with long, very narrow shaft, with very long subapical process, process with 2 short, curved accessory processes (Fig. 135, 136); style short, broad with short, narrow apophysis (Fig. 137, 138); dorsal connective short, narrow, with apex curved in lateral view, sub ovate in dorsal view (Fig. 135, 136); connective large, anterior arms broad, complete ridge medially, stem elongate horizontally (Fig. 139); subgenital plate long, broad, apex abruptly curved laterally, tapered, rounded apically (Fig. 140).
 Female seventh sternum. Long, broad, posterior margin sub truncate.
 Material examined. Holotype male. LAOS: Houa Phan prov., 20°13’09-19”N. 103°59’54- 104°00’03”E, 1480-1510 m., Phou Pane Mt., 1-16.vi.2009, Vit Kuban, leg. / Primary mountain forest, yellow plate trap, Laos 2009 expedition, NHMB, Basel, NMPC Prague. / Collection Moraviske Museum, Brno (MMBC). Paratype female, same data as holotype (MMBC).
 Etymology. The name of the species is descriptive for the apical 1/3 of the subgenital plate which is strongly curved inwardly.
 Remarks. The genus is presently monobasic.
description: Published as part of Nielson, M. W., 2015, A revision of the tribe Coelidiini of the Oriental, Palearctic and Australian biogeographical regions (Hemiptera: Cicadellidae: Coelidiinae), pp. 1-202 in Insecta Mundi 2015 (410) on pages 27-28, DOI: 10.5281/zenodo.5181587
Métrologie infrarouge haute précision pour la détermination des coefficients de transfert en condensation convective
Creators: name: Beaumale, Marion
name: Lavieille, Pascal
name: Miscevic, Marc
Publisher: name: Société Française de Thermique
Year: 2021
Subjects: condensation convective
métrologie infrarouge
coefficient d'échange
expérimental

description: Les systèmes diphasiques sont envisagés comme des solutions de refroidissement pour de multiples applications. La particularité de ce type de systèmes est le couplage fort entre performances thermiques et structuration des phases liquide et vapeur au sein de l'écoulement. La prédiction des transferts de chaleur demeure encore aujourd'hui l'une des problématiques principales dans le dimensionnement des systèmes mettant en œuvre la condensation en film à faible vitesse massique. L'originalité du dispositif expérimental proposé est sa capacité à mesurer localement et simultanément l'épaisseur du film liquide et le coefficient de transfert de chaleur. Pour la mesure des épaisseurs des films de condensats un capteur confocal chromatique et des mesures interférométriques en lumière blanche ont été utilisés. Les mesures de température de paroi quant à elles ont été obtenues par thermographie infrarouge. Le saphir a été choisi comme matériau du condenseur de par sa transparence dans le domaine visible permettant la visualisation de l'écoulement, et sa haute conductivité thermique améliorant les transferts de chaleur radiaux dans le tube. La section test, placée entre deux réservoirs à pression constante, est refroidie par de l'air conditionné. Ce choix est motivé par la transparence de l'air dans le domaine des longueurs d'ondes infrarouges détectées par la caméra thermique. En raison du mode de refroidissement utilisé (i.e. convection forcée d'air) la détermination du coefficient de transfert de chaleur nécessite une extrême précision de mesure de la température de paroi difficile à atteindre par les outils habituels. Le travail réalisé porte sur la mise en place d'une technique de mesure permettant la détermination avec une haute précision (à 0.05$^{\circ}$C) de la température de paroi d'un tube vertical en saphir par caméra infrarouge lors de la condensation convective du HFE 7000 en écoulement descendant. Le protocole développé, ainsi que sa calibration, seront présentés en détails dans la communication.