cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
The spectrum of multi-flavor QCD_2 and the non-Abelian Schwinger equation
Creators: name: Armoni, A.
name: Frishman, Y.
name: Sonnenschein, J.
name: Trittmann, U.
Publisher: name: arXiv
Year: 1998
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Massless $QCD_2$ is dominated by classical configurations in the large $N_f$ limit. We use this observation to study the theory by finding solutions to equations of motion, which are the non-Abelian generalization of the Schwinger equation. We find that the spectrum consists of massive mesons with $M^2={e^2 N_f\over 2π}$ which correspond to Abelian solutions. We generalize previously discovered non-Abelian solutions and discuss their interpretation. We prove a no-go theorem ruling out the existence of soliton solutions. Thus the semi-classical approximation shows no baryons in the case of massless quarks, a result derived before in the strong-coupling limit only.
description: 17 pages, Latex. 1 figure
Genomrekonstruktion und Klassifizierung unkultivierter Chloroflexi aus Fumarolen von São Miguel (Azoren)-Anhang
Creators: name: Fuchs, Jannick
Publisher: name: Zenodo
Year: 2019

description: Anhang der Bachelorarbeit "Genomrekonstruktion und Klassifizierung unkultivierter Chloroflexi aus Fumarolen von São Miguel (Azoren)"
Balance functions of (un)identified hadrons in Pb--Pb, p--Pb, and pp collisions at the LHC
Creators: name: Pan, Jinjin
Publisher: name: arXiv
Year: 2018
Subjects: subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: In ultrarelativistic heavy-ion collisions, correlations of particles with opposite quantum numbers provide insight into quark production mechanisms and time scales, collective motion, and re-scattering in the hadronic phase. The longitudinal and azimuthal widths of balance functions for charged kaons and charged pions are used to examine the two-wave quark production model proposed to explain quark-antiquark production within the QGP, which predicts a large increase in up and down quark pairs relative to strange quark pairs around the time of hadronization. Balance functions are also analyzed in small collision systems such as p--Pb and pp to study fragmentation effects and possible collective effects in high-multiplicity events. A comprehensive set of balance functions has been measured using the ALICE detector, including results for unidentified hadrons in Pb--Pb and p--Pb collisions at $\sqrt{s_{\rm{NN}}}=5.02$ TeV, for charged pions in Pb--Pb collisions at $\sqrt{s_{\rm{NN}}}=2.76$ TeV, p--Pb collisions at $\sqrt{s_{\rm{NN}}}=5.02$ TeV and pp collisions at $\sqrt{s}=7$ TeV, and for charged kaons in Pb--Pb collisions at $\sqrt{s_{\rm{NN}}}=2.76$ TeV. The first balance function yield results are also presented.
Small Instantons and Weak Scale String Theory
Creators: name: Benakli, Karim
name: Oz, Yaron
Publisher: name: arXiv
Year: 1999
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We consider heterotic string compactifications to four dimensions when instantons shrink to zero size. If the standard model gauge group originates from the new gauge symmetry associated with the small instantons singularity, then the weakly or strongly coupled heterotic string scales can be taken to be arbitrarily low. The SO(32) and E_8\times E_8 gauge groups can then be very weakly coupled even at the string scale and behave as non-abelian global symmetries. We comment on a possible role of small instantons in supersymmetry breaking.
description: 9 pages, Latex
New variable stars in the Galactic Bulge: I. The bright regime
Creators: name: Kains, N.
name: Calamida, A.
name: Rejkuba, M.
name: Bhardwaj, A.
name: Inno, L.
name: Sahu, K. C.
name: Zoccali, M.
name: Bono, G.
name: Surot, F.
name: Anderson, J.
name: Casertano, S.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We report the detection of 1143 variable stars towards the Galactic bulge, including 320 previously uncatalogued variables, using time-series photometry extracted from data obtained with the VIMOS imager at the Very Large Telescope. Observations of the Sagittarius Window Eclipsing Extrasolar Planet Search (SWEEPS) field in the Galactic Bulge were taken over 2 years between March and October at a cadence of $\sim$ 4 days, enabling the detection of variables with periods up to $\sim$100 days. Many of these were already known, but we detected a significant number of new variables, including 26 Cepheids, a further 18 Cepheid candidates, and many contact binaries. Here we publish the catalog of the new variables, containing coordinates, mean magnitudes as well as periods and classification; full light curves for these variables are also made available electronically.
description: 14 pages, 9 figures; submitted to MNRAS
Koenderink filters and the Microwave Background
Creators: name: Schmalzing, Jens
Publisher: name: arXiv
Year: 1997
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We introduce Koenderink filters as novel tools for statistical cosmology. Amongst several promising applications, they provide a test for the Gaussianity of random fields. We focus on this application and present some preliminary results from an analysis of the Cosmic Microwave Background (CMB).
description: 9 pages, 5 figures with 14 eps-files; uses AMSTeX, a4wide.sty, epsf.sty, mncite.sty
Formation and maintenance of subsiding shells around non‐precipitating and precipitating cumulus clouds
Creators: name: Savre, Julien
Publisher: name: John Wiley & Sons, Ltd
Year: 2020

description: A shell of subsiding air is generally known to develop around cumulus clouds and shield them from their environment. We seek here to improve our understanding of such shells by (a) revealing the detailed vertical and horizontal structure of shells surrounding both shallow and deeper clouds, and (b) identifying the mechanisms responsible for in‐shell subsidence generation and maintenance. To that end, a high‐resolution Cloud Resolving Model simulation of the shallow‐to‐deep convection transition over a tropical land surface is analysed with an emphasis on the cloud's near environment. Shells surrounding shallow and deep clouds are found to possess surprisingly similar characteristics. However important differences are observed near cloud top where the deepest clouds are associated with stronger subsidence and broader shells. In the convective outflow region, stronger in‐shell subsidence coincides with strong buoyancy reversal, but also with strong pressure gradients naturally generated by cloud‐top vortex dynamics. A more delicate balance between various processes takes place below, and in‐shell subsidence is only barely sustained as buoyancy reversal is largely compensated by pressure gradients. Finally, while evaporation is clearly the main source of buoyancy reversal everywhere around cloud edges, it is also shown that the downward transport of warmer air from aloft through the subsiding shells may compensate for evaporative cooling to slowly bring in‐shell buoyancy to a near‐neutral state. Overall, while it cannot be denied that evaporative cooling and buoyancy reversal play important roles in generating and sustaining in‐shell subsidence, the present results also emphasise that mechanical forcing at cloud top and downward transport within the shells should not be overlooked.
description: Narrow “shells” of subsiding air generally form around cumulus clouds, but the mechanisms responsible for their formation and maintenance are still debated. In this study, the dynamics of these shells is investigated using a high‐resolution simulation of idealized tropical convection. It is shown that in‐shell subsiding motions are generally driven by buoyancy reversal. However, mechanical forcing contributes at least equally at the top of all convective clouds. In addition, it is found that buoyancy reversal due to evaporative cooling may be offset by the downward transport of warmer air from aloft through the subsiding shells.
Drivers of COVID-19 protest across localities in Israel: a machine-learning approach
Creators: name: Schlager, Nina
name: Donnay, Karsten
name: Kim, Hyunjung
name: Bhavnani, Ravi
Publisher: name: Taylor & Francis
Year: 2023
Subjects: subject: Medicine
subject: Cell Biology
subject: Sociology
subject: FOS: Sociology
subject: Cancer

description: Anti-government protests emerged globally in response to COVID-19 countermeasures. What are the key drivers of these pandemic-related protests, and to what extent do they differ from the drivers of non-COVID protests? We examine these questions in the context of Israel, which faced a growing political crisis at the start of the pandemic, effectively blurring the distinction between different causes of protest. Our data features 1,922 protests across 189 Israeli localities for the period between March and July 2022. Using a machine learning approach, we find that all protests, regardless of whether they were directly related to the pandemic or not, were motivated by the same set of key indicators – albeit with the ranking of drivers for COVID-related protests inverted for non-COVID protests. Local infection rates and government responses were more pronounced for the former, whereas differences in residential and commercial property taxes, access to affordable housing, quality of education and demography were among the most important drivers for the latter. Our analysis underscores the role that local governments played in managing the pandemic, and demonstrates that variation in socioeconomic conditions had an important effect on the incidence of protests across Israel.
Additional file 2: of Implementation study of an interprofessional medication adherence program for HIV patients in Switzerland: quantitative and qualitative implementation results
Creators: name: MĂŠlanie Lelubre
name: Clerc, Olivier
name: Grosjean, Marielle
name: Amighi, Karim
name: Vriese, Carine De
name: Bugnon, Olivier
name: Marie-Paule Schneider
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Molecular Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Content of organised meetings and focus groups during the operation phase. Description of data: Description of topics covered during meetings and focus groups with health care professionals. (DOCX 20 kb)
Coupling Constant Dependence in the Thermodynamics of N=4 Supersymmetric Yang-Mills Theory
Creators: name: Gubser, Steven S.
name: Klebanov, Igor R.
name: Tseytlin, Arkady A.
Publisher: name: arXiv
Year: 1998
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: The free energy of the maximally supersymmetric SU(N) gauge theory at temperature T is expected to scale, in the large N limit, as N^2 T^4 times a function of the 't Hooft coupling, f(g_{YM}^2 N). In the strong coupling limit the free energy has been deduced from the near-extremal 3-brane geometry, and its normalization has turned out to be 3/4 times that found in the weak coupling limit. In this paper we calculate the leading correction to this result in inverse powers of the coupling, which originates from the R^4 terms in the tree level effective action of type IIB string theory. The correction to 3/4 is positive and of order (g_{YM}^2 N)^{-3/2}. Thus, f(g_{YM}^2 N) increases as the 't Hooft coupling is decreased, in accordance with the expectation that it should be approaching 1 in the weak coupling limit. We also discuss similar corrections for other conformal theories describing coincident branes. In particular, we suggest that the coupling-independence of the near extremal entropy for D1-branes bound to D5-branes is related to the vanishing of the Weyl tensor of AdS_3\times S^3.
description: 24 pages; a paragraph about the 5-form background added in section 3; in the Note Added we clarify the meaning of the metric found in section 3; sign in eq. (34) corrected
Platythyrea lamellosa subsp. suturalis Forel, 1909, n. subsp.
Creators: name: Forel, A.
Publisher: name: Zenodo
Year: 1909
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Formicidae
Platythyrea
Platythyrea lamellosa
Platythyrea lamellosa rog. subsp. suturalis

description: Platythyrea lamellosa Rog. subsp. suturalis n. subsp.
— [[worker]]. — Long. 12 mill. — Un peu plus etroite et plus allongee que la subsp. longinoda Forel. Mandibules sans dents, sauf l'apicale. Tete carree, presque aussi large que longe. L'epistome est delimite par une suture bien visible, quoique tres faible. Le mesonotum est plat et enfonce, comme chez l'espece typique; les deux sutures sont distinctes (la mesoepinotale aussi distincte que la promesonotale, ce qui la distingue de l'espece typique), mais nullement enfoncees comme chez la subsp. longinoda Forel. L'epinotum n'a ni dents, ni elevations; sa face declive n'est pas concave et n'est que subbordee, ce qui la distingue encore de longinoda. Par contre le n oe ud est au moins aussi allonge que chez la subsp. longinoda Forel. Les yeux sont bien plus grands que chez cette sous espece, allonges, un peu plus longs que la distance de leur bord anterieur a celui de la tete. Second segment de l'abdomen a peine plus large que le premier (bien plus large chez la longinoda). Les gros points enfonces bien plus effaces et moins nombreux que chez la longinoda, tres peu apparents.
description: Published as part of Forel, A., 1909, Fourmis du Musée de Bruxelles. Fourmis de Benguela récoltées par M. Creighton Wellman, et fourmis du Congo récoltées par MM. Luja, Kohl et Laurent., pp. 51-73 in Annales de la Societe Entomologique de Belgique 53 on page 64
Microcanonical Treatment of Hadronizing the Quark-Gluon Plasma
Creators: name: WERNER, Klaus
name: AICHELIN, Joerg
Publisher: name: arXiv
Year: 1995
Subjects: subject: Nuclear Theory (nucl-th)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We recently introduced a completely new way to study ultrarelativistic nuclear scattering by providing a link between the string model approach and a statistical description. A key issue is the microcanonical treatment of hadronizing individual quark matter droplets. In this paper we describe in detail the hadronization of these droplets according to n-body phase space, by using methods of statistical physics, i.e. constructing Markov chains of hadron configurations.
description: Complete paper enclosed as postscript file (uuencoded)
Lepton non-universality in $B$ decays and fermion mass structure
Creators: name: Grinstein, B.
name: Pokorski, S.
name: Ross, G. G.
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We consider the possibility that the neutral-current $B$ anomalies are due to radiative corrections generated by Yukawa interactions of quarks and leptons with new vector-like quark and lepton electroweak doublets and new Standard Model singlet scalars. We show that the restricted interactions needed can result from an underlying Abelian family symmetry and that the same symmetry can give rise to an acceptable pattern of quark and charged lepton masses and mixings, providing a bridge between the non-universality observed in the B-sector and that of the fermion mass matrices. We construct two simple models, one with a single singlet scalar in which the flavour changing comes from quark and lepton mixing and one with an additional scalar in which the flavour changing can come from both fermion and scalar mixing. We show that for the case the new quarks are much heavier than the new leptons and scalars the $B$ anomalies can be due to box diagrams with couplings in the perturbative regime consistent with the bounds coming from $B_s- \bar B_s$, $K- \bar K$ and $D- \bar D$ mixing as well as other lepton family number violating processes. The new states can be dark matter candidates and, in the two scalar model with a light scalar of O(60) GeV and vector-like lepton of O(100) GeV, there can be a simultaneous explanation of the B-anomalies, the muon anomalous magnetic moment and the dark matter abundance.
description: Replacement contains few additional references
Entropy in cluster analysis of single events in heavy ion collisions
Creators: name: Fialkowski, K.
name: Wit, R.
Publisher: name: arXiv
Year: 1999
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We analyse the cluster structure of the final multihadron states resulting from heavy ion collisions using the concept of Jaynes - Shannon entropy. Further evidence for an interesting differentiation of events is provided.
description: 6 pages, 6 eps figures, 1 tex file
Power Spectra in Global Defect Theories of Cosmic Structure Formation
Creators: name: Pen, Ue-Li
name: Seljak, Uros
name: Turok, Neil
Publisher: name: arXiv
Year: 1997
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: An efficient technique for computing perturbation power spectra in field ordering theories of cosmic structure formation is introduced, enabling computations to be carried out with unprecedented precision. Large scale simulations are used to measure unequal time correlators of the source stress energy, taking advantage of scaling during matter and radiation domination, and causality, to make optimal use of the available dynamic range. The correlators are then re-expressed in terms of a sum of eigenvector products, a representation which we argue is optimal, enabling the computation of the final power spectra to be performed at high accuracy. Microwave anisotropy and matter perturbation power spectra for global strings, monopoles, textures and non-topological textures are presented and compared with recent observations.
description: 4 pages, compressed and uuencoded RevTex file and postscript figures
Additional file 1: of Associations of context-specific sitting time with markers of cardiometabolic risk in Australian adults
Creators: name: Dempsey, Paddy
name: Nyssa Hadgraft
name: Winkler, Elisabeth
name: Clark, Bronwyn
name: Buman, Matthew
name: Gardiner, Paul
name: Owen, Neville
name: Lynch, Brigid
name: Dunstan, David
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Cell Biology
subject: Molecular Biology
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Developmental Biology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Sitting time questions from AusDiab3. (PDF 112 kb)
Jean-Baptiste Marescaille de Caffort
Creators: name: Plouvain, Pierre-Antoine-Samuel-Joseph (1754-1832)
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2017
Subjects: Officier de justice d'Ancien Régime

description: Source: http://www.sudoc.fr/080675700
description: Coverage: Parlement de Flandre
The origin of the mid-infrared nuclear polarization of active galactic nuclei
Creators: name: Lopez-Rodriguez, E.
name: Alonso-Herrero, A.
name: Diaz-Santos, T.
name: Gonzalez-Martin, O.
name: Ichikawa, K.
name: Levenson, N. A.
name: Martinez-Paredes, M.
name: Nikutta, R.
name: Packham, C.
name: Perlman, E.
name: Almeida, C. Ramos
name: Rodriguez-Espinosa, J. M.
name: Telesco, C. M.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We combine new (NGC 1275, NGC 4151, and NGC 5506) and previously published (Cygnus A, Mrk 231, and NGC 1068) sub-arcsecond resolution mid-infrared (MIR; 8-13 $μ$m) imaging- and spectro-polarimetric observations of six Seyfert galaxies using CanariCam on the 10.4-m Gran Telescopio CANARIAS. These observations reveal a diverse set of physical processes responsible for the nuclear polarization, and permit characterization of the origin of the MIR nuclear polarimetric signature of active galactic nuclei (AGN). For all radio quiet objects, we found that the nuclear polarization is low (<1 per cent), and the degree of polarization is often a few per cent over extended regions of the host galaxy where we have sensitivity to detect such extended emission (i.e., NGC 1068 and NGC 4151). We suggest that the higher degree of polarization previously found in lower resolution data arises only on the larger-than-nuclear scales. Only the radio-loud Cygnus A exhibits significant nuclear polarization ($\sim$11 per cent), attributable to synchrotron emission from the pc-scale jet close to the core. We present polarization models that suggest that the MIR nuclear polarization for highly obscured objects arises from a self-absorbed MIR polarized clumpy torus and/or dichroism from the host galaxy, while for unabsorbed cores, MIR polarization arises from dust scattering in the torus and/or surrounding nuclear dust.
description: 9 pages, 4 figures. Accepted to MNRAS
Numerical impacts on tracer transport: A proposed intercomparison test of Atmospheric General Circulation Models
Creators: name: Gupta, Aman
name: Gerber, Edwin P.
name: Lauritzen, Peter H.
Publisher: name: John Wiley & Sons, Ltd
Year: 2020

description: The transport of trace gases by the atmospheric circulation plays an important role in the climate system and its response to external forcing. Transport presents a challenge for Atmospheric General Circulation Models (AGCMs), as errors in both the resolved circulation and the numerical representation of transport processes can bias their abundance. In this study, two tests are proposed to assess transport by the dynamical core of an AGCM. To separate transport from chemistry, the tests focus on the age‐of‐air, an estimate of the mean transport time by the circulation. The tests assess the coupled stratosphere–troposphere system, focusing on transport by the overturning circulation and isentropic mixing in the stratosphere, or Brewer–Dobson Circulation, where transport time‐scales on the order of months to years provide a challenging test of model numerics. Four dynamical cores employing different numerical schemes (finite‐volume, pseudo‐spectral, and spectral‐element) and discretizations (cubed sphere versus latitude–longitude) are compared across a range of resolutions. The subtle momentum balance of the tropical stratosphere is sensitive to model numerics, and the first intercomparison reveals stark differences in tropical stratospheric winds, particularly at high vertical resolution: some cores develop westerly jets and others easterly jets. This leads to substantial spread in transport, biasing the age‐of‐air by up to 25% relative to its climatological mean, making it difficult to assess the impact of the numerical representation of transport processes. This uncertainty is removed by constraining the tropical winds in the second intercomparison test, in a manner akin to specifying the Quasi‐Biennial Oscillation in an AGCM. The dynamical cores exhibit qualitative agreement on the structure of atmospheric transport in the second test, with evidence of convergence as the horizontal and vertical resolution is increased in a given model. Significant quantitative differences remain, however, particularly between models employing spectral versus finite‐volume numerics, even in state‐of‐the‐art cores.
description: The climatological and zonal mean zonal wind ū (m·s−1), as simulated by two different dynamical cores, (left) pseudospectral (GFDL‐PS) and (right) finite‐volume (CAM‐FV), with (top) 40 vertical levels and (bottom) 80 vertical levels. With higher vertical resolution, the pseudospectral core develops westerlies in the tropical stratosphere between 20 and 80 hPa, while the finite‐volume core consistently simulates easterlies at both vertical resolutions. Both cores have comparable horizontal resolution. The contour interval is 10 m·s−1.
description: US National Science Foundation
Megaloponera foetens Forel (Hagensia)
Creators: name: Forel, A.
Publisher: name: Zenodo
Year: 1909
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Formicidae
Megaloponera
Megaloponera foetens

description: Megaloponera foetens. F.
— [[worker]]. — Mayr a montre (1907) que la M. crassicornis, Gerst n'est pas une espece, mais ne represente que les [[worker]] minimae de la M. f oe tens. Or Emery avait appele M. Dohrni une forme intermediaire entre f oe tens et crassicornis, forme qui donc, selon Mayr, doit representer les [[worker]] moyennes de la meme espece. M. Creighton Wellman a recolte des exemplaires qui constituent tous les passages de la Dohrni a la crassicornis, ce qui vient confirmer l'opinion de Mayr.
M. Creighton Wellman assure que cette espece va en armees (Army Ant) nombreuses.
description: Published as part of Forel, A., 1909, Fourmis du Musée de Bruxelles. Fourmis de Benguela récoltées par M. Creighton Wellman, et fourmis du Congo récoltées par MM. Luja, Kohl et Laurent., pp. 51-73 in Annales de la Societe Entomologique de Belgique 53 on page 64
New Directions for New Dimensions: From Strings to Neutrinos to Axions to...
Creators: name: Dienes, Keith R.
Publisher: name: arXiv
Year: 2000
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: In this talk, I discuss recent developments concerning the possibility of large extra spacetime dimensions. After briefly reviewing how such dimensions can lower the fundamental GUT, Planck, and string scales, I then outline how these scenarios lead to a new higher-dimensional seesaw mechanism for generating neutrino oscillations --- perhaps even without neutrino masses. I also discuss how extra dimensions lead to new mechanisms contributing to the ``invisibility'' of the QCD axion. This talk reports on work done in collaboration with Emilian Dudas and Tony Gherghetta.
description: 12 pages, LaTeX, 4 figures. Invited plenary talk given at PASCOS '99 (held at Lake Tahoe, California, 10-16 December 1999). To appear in the Proceedings
Analysis of the exclusive semileptonic decay Lambda_b -> Lambda_c + l nu_l within a light-front constituent quark model
Creators: name: Cardarelli, F.
name: Simula, S.
Publisher: name: arXiv
Year: 1999
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The exclusive semileptonic decay Lambda_b -> Lambda_c + l nu_l is investigated including both radiative and first-order power corrections in the inverse heavy-quark mass, while the Isgur-Wise function is calculated within a light-front constituent quark model. It turns out that the dependence on the model parameters can be effectively constrained using recent lattice QCD results at low values of the recoil. Our final predictions for the exclusive semileptonic branching ratio, the longitudinal and transverse asymmetries, and the longitudinal to transverse decay ratio are: Br(Lambda_b -> Lambda_c + l nu_l) = (6.3 \pm 1.6) % |V_{bc} / 0.040|**2 τ(Λ_b) / (1.24 ps), a_L = -0.945 \pm 0.014, a_T = -0.62 \pm 0.09 and R_L/T = 1.57 \pm 0.15, respectively. Moreover, the theoretical uncertainties both on a_L and the (partially integrated) R_L/T are found to be quite small and, therefore, the experimental determination of these quantities is a very interesting tool for testing the Standard Model and for investigating possible New Physics. In this respect the sensitivity to extract unique information both on the strength and phase of possible hadronic right-handed currents is illustrated.
description: in Proceedings of the International Conference PANIC '99, Uppsala (Sweden), June 1999
The FIRST Classifier: Compact and Extended Radio Galaxy Classification using Deep Convolutional Neural Networks
Creators: name: Alhassan, Wathela
name: Taylor, A. R.
name: Vaccari, Mattia
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Upcoming surveys with new radio observatories such as the Square Kilometer Array will generate a wealth of imaging data containing large numbers of radio galaxies. Different classes of radio galaxies can be used as tracers of the cosmic environment, including the dark matter density field, to address key cosmological questions. Classifying these galaxies based on morphology is thus an important step toward achieving the science goals of next generation radio surveys. Radio galaxies have been traditionally been classified as Fanaroff-Riley (FR) I and II, although some exhibit more complex 'bent' morphologies arising from environmental factors or intrinsic properties. In this work we present the FIRST Classifier, an on-line system for automated classification of Compact and Extended radio sources. We developed the FIRST Classifier based on a trained Deep Convolutional Neural Network Model to automate the morphological classification of compact and extended radio sources observed in the FIRST radio survey. Our model achieved an overall accuracy of 97% and a recall of 98%, 100%, 98% and 93% for Compact, BENT, FRI and FRII galaxies respectively. The current version of the FIRST classifier is able to predict the morphological class for a single source or for a list of sources as Compact or Extended (FRI, FRII and BENT).
description: 9 pages, 10 figures. Accepted for publication in MNRAS
title: ADCO, Cartulaire du prieuré de Saint-Vivant-sous-Vergy, dépendant de l’abbaye de Cluny (XIVe siècle), Cart. 231 (21 H), 40 folios, f. 0019v
Creators: name: de la Côte-d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CBMA/CG21/F.PETOT/2010
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Cartulaire du prieuré de Saint-Vivant-sous-Vergy, dépendant de l’abbaye de Cluny (XIVe siècle), Archives départementales de la Côte-d'Or, Cart. 231 (21 H), 40 folios. Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire du prieuré de Saint-Vivant-sous-Vergy, dépendant de l’abbaye de Cluny (XIVe siècle), Archives départementales de la Côte-d'Or, Cart. 231 (21 H), 40 folios, f. 0019v, in Projet CBMA - Corpus Burgundiae Medii Aevi \[Ressource en ligne\], https:// manuscrits.cbma-project.eu/
description: Provenance: abbaye Saint-Vivant de Vergy
description: Provenance: http://www.wikidata.org/entity/Q15945018
Supersymmetric Gauge Theories from Branes and Orientifold Six-planes
Creators: name: Landsteiner, Karl
name: Lopez, Esperanza
name: Lowe, David A.
Publisher: name: arXiv
Year: 1998
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We study brane configurations in the presence of orientifold six-planes. After deriving the curves for N=2 supersymmetric SU(Nc) gauge theories with one flavor in the symmetric or antisymmetric representation and Nf fundamental flavors, we rotate the brane configuration, reducing the supersymmetry to N=1. For the case of an antisymmetric flavor and less than two fundamental flavors, nonperturbative effects lead to a brane configuration that is topologically a torus. Using the description of the orientifold six-planes as Dn singularities we discuss the Higgs branches for N=2 brane configurations with Sp/SO gauge groups and the related N=1 theories with tensor representations.
description: 30 pages (harvmac b-mode), 5 figures, (v2 minor corrections), (v3 sign error corrected)
Additional file 1: of Implementation study of an interprofessional medication adherence program for HIV patients in Switzerland: quantitative and qualitative implementation results
Creators: name: MĂŠlanie Lelubre
name: Clerc, Olivier
name: Grosjean, Marielle
name: Amighi, Karim
name: Vriese, Carine De
name: Bugnon, Olivier
name: Marie-Paule Schneider
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Interview grids developed for focus groups with health care professionals and individual interviews with patients. Description of data: Interview grids (translated version) used during focus groups with health care professionals and individual interviews with patients. (DOCX 44 kb)
From ideological congruence to satisfaction with democracy: how leverage can mitigate the ill-effects of party polarization
Creators: name: Russo, Luana
name: Franklin, Mark
name: Beyens, Stefenie
Publisher: name: Taylor & Francis
Year: 2023
Subjects: subject: Medicine
subject: Neuroscience
subject: Science Policy
subject: Mental Health
subject: Plant Biology
subject: FOS: Biological sciences

description: The impact of party polarization on voter satisfaction is disputed. While a direct negative effect is expected, polarization has also been found to clarify party policies, with indirect positive impact. This Note proposes a more direct source of positive effects for polarization through an interaction with congruence. We use citizens’ satisfaction with democracy (SwD) as the evaluation of interest; we take ideological polarization among parties and citizen-government left-right congruence as independent variables; and we use data from the Comparative Study of Electoral Systems. We find that higher polarization, while indeed detrimental to satisfaction with democracy, gives rise to countervailing effects of congruence. We borrow the geometric concept of leverage to characterize the way this interaction enhances congruence’s positive effect on SwD.
Quark Matter 95: Concluding Remarks
Creators: name: Gyulassy, Miklos
Publisher: name: arXiv
Year: 1995
Subjects: subject: Nuclear Theory (nucl-th)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Highlights of Quark Matter 95 are discussed.
description: 14 pages, latex, 9 uuencoded figures, revised text
Non-Cartan Mordell-Weil lattices of rational elliptic surfaces and heterotic/F-theory compactifications
Creators: name: Mizoguchi, Shun'ya
name: Tani, Taro
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: The Mordell-Weil lattices (MW lattices) associated to rational elliptic surfaces are classified into 74 types. Among them, there are cases in which the MW lattice is none of the weight lattices of simple Lie algebras or direct sums thereof. We study how such "non-Cartan MW lattices" are realized in the six-dimensional heterotic/F-theory compactifications. In this paper, we focus on non-Cartan MW lattices that are torsion free and whose associated singularity lattices are sublattices of $A_7$. For the heterotic string compactification, a non-Cartan MW lattice yields an instanton gauge group $H$ with one or more $U(1)$ group(s). We give a method for computing massless spectra via the index theorem and show that the $U(1)$ instanton number is limited to be a multiple of some particular non-one integer. On the F-theory side, we examine whether we can construct the corresponding threefold geometries, i.e., rational elliptic surface fibrations over $P^1$. Except for some cases, we obtain such geometries for specific distributions of instantons. All the spectrum derived from those geometries completely match with the heterotic results.
description: 63 pages, 1 figure; v2: typos corrected, references added
Tephrochronology in Aotearoa New Zealand
Creators: name: Hopkins, Jenni L.
name: Lowe, David J.
name: Horrocks, Joanna L.
Publisher: name: Taylor & Francis
Year: 2021
Subjects: subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy

description: Tephra deposits in Aotearoa New Zealand (ANZ) have been studied for >180 years. The now-global discipline of tephrochronology, which has some developmental roots in ANZ, forms the basis of a powerful chronostratigraphic correlational tool and age-equivalent dating method for geological, volcanological, palaeoenvironmental, and archaeological research in ANZ. Its utility is founded on the key principle that tephras or cryptotephras provide widespread isochrons in many different environments. In the first part of this article, we summarise the history of tephra studies in ANZ and then describe how tephras have been mapped, characterised, and correlated using field and laboratory-based methods. We document advances in geochemical fingerprinting of glass; tephra/cryptotephra detection and correlation by sediment-core scanning methods (e.g. X-radiography, CT imaging, XRF elemental analysis, magnetic susceptibility); statistical correlation methods; and dating of tephras/cryptotephras. We discuss the advent of ANZ cryptotephra studies (from mid-1970s) and their more-recent growth. The second part comprises examples of applications of tephrochronology in ANZ: climate-event stratigraphy (NZ-INTIMATE project); eruptive-event stratigraphy in the Auckland Volcanic Field; developments in the marine tephra record; advances in identifying, correlating, and dating old (pre-50 ka) tephras and weathered-tephra deposits; forming soils/paleosols on tephras; tephras and archaeology; Kopouatai bog tephrostratigraphy and palaeoenvironments; and volcanic-hazard assessments.
Phase Space Structure and Transport in a Caldera Potential Energy Surface
Creators: name: Katsanikas, Matthaios
name: Wiggins, Stephen
Publisher: name: arXiv
Year: 2018
Subjects: subject: Chaotic Dynamics (nlin.CD)
subject: Mathematical Physics (math-ph)
subject: Dynamical Systems (math.DS)
subject: Chemical Physics (physics.chem-ph)
subject: FOS: Physical sciences
subject: FOS: Mathematics

description: We study phase space transport in a 2D caldera potential energy surface (PES) using techniques from nonlinear dynamics. The caldera PES is characterized by a flat region or shallow minimum at its center surrounded by potential walls and multiple symmetry related index one saddle points that allow entrance and exit from this intermediate region.We have discovered four qualitatively distinct cases of the structure of the phase space that govern phase space transport. These cases are categorized according to the total energy and the stability of the periodic orbits associated with the family of the central minimum, the bifurcations of the same family, and the energetic accessibility of the index one saddles. In each case we have computed the invariant manifolds of the unstable periodic orbits of the central region of the potential and the invariant manifolds of the unstable periodic orbits of the families of periodic orbits associated with the index one saddles. We have found that there are three distinct mechanisms determined by the invariant manifold structure of the unstable periodic orbits govern the phase space transport. The first mechanism explains the nature of the entrance of the trajectories from the region of the low energy saddles into the caldera and how they may become trapped in the central region of the potential. The second mechanism describes the trapping of the trajectories that begin from the central region of the caldera, their transport to the regions of the saddles, and the nature of their exit from the caldera. The third mechanism describes the phase space geometry responsible for the dynamical matching of trajectories originally proposed by Carpenter and described in Collins et al. (2014) for the two dimensional caldera PES that we consider.
description: 24 pages, International Journal of Bifurcation and Chaos (in press)
Absorption of High Energy Gamma Rays by Interactions With Starlight Photons in Extragalactic Space at High Redshifts and the High Energy Gamma-Ray Background
Creators: name: Salamon, M. H.
name: Stecker, F. W.
Publisher: name: arXiv
Year: 1997
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We calculate the absorption of 10-500 GeV gamma-rays at high redshifts. This calculation requires the determination of the high-redshift evolution of the intergalactic starlight photon field, including its IR-UV spectral energy distribution. To estimate this evolution, we have followed a recent analysis of Fall, Charlot and Pei which gives results consistent with recent data. We give our results for the gamma-ray opacity as a function of redshift out to a redshift of 3. We also give predicted gamma-ray spectra for selected blazars and give an extragalactic unresolved blazar background spectrum up to 500 GeV. Our results indicate that this background should steepen significantly above 20 GeV owing to intergalactic absorption. Future observations of this steepening would provide a test for the blazar background origin hypothesis. We have used our results to discuss upper limits on the redshifts of gamma-ray bursts. We note that the 17 Feb. 1994 burst observed by EGRET must have originated at a redshift less than 2. We also use our estimates of the background to determine the observability of multi-GeV gamma-ray lines from the annihilation of supersymmetric dark matter particles in the galactic halo.
description: 26 pages, Latex, 10 ps figures, submitted to Ap.J
First evidence of diffuse ultra-steep-spectrum radio emission surrounding the cool core of a cluster
Creators: name: Savini, Federica
name: Bonafede, Annalisa
name: Brueggen, Marcus
name: van Weeren, Reinout
name: Brunetti, Gianfranco
name: Intema, Huib
name: Botteon, Andrea
name: Shimwell, Timothy
name: Wilber, Amanda
name: Rafferty, David
name: Giacintucci, Simona
name: Cassano, Rossella
name: Cuciti, Virginia
name: de Gasperin, Francesco
name: Roettgering, Huub
name: Hoeft, Matthias
name: White, Glenn
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Diffuse synchrotron radio emission from cosmic-ray electrons is observed at the center of a number of galaxy clusters. These sources can be classified either as giant radio halos, which occur in merging clusters, or as mini halos, which are found only in cool-core clusters. In this paper, we present the first discovery of a cool-core cluster with an associated mini halo that also shows ultra-steep-spectrum emission extending well beyond the core that resembles radio halo emission. The large-scale component is discovered thanks to LOFAR observations at 144 MHz. We also analyse GMRT observations at 610 MHz to characterise the spectrum of the radio emission. An X-ray analysis reveals that the cluster is slightly disturbed, and we suggest that the steep-spectrum radio emission outside the core could be produced by a minor merger that powers electron re-acceleration without disrupting the cool core. This discovery suggests that, under particular circumstances, both a mini and giant halo could co-exist in a single cluster, opening new perspectives for particle acceleration mechanisms in galaxy clusters.
Additional file 9 of HOME-BIO (sHOtgun MEtagenomic analysis of BIOlogical entities): a specific and comprehensive pipeline for metagenomic shotgun sequencing data analysis
Creators: name: Ferravante, Carlo
name: Memoli, Domenico
name: Palumbo, Domenico
name: Ciaramella, Paolo
name: Di Loria, Antonio
name: D’Agostino, Ylenia
name: Nassa, Giovanni
name: Rizzo, Francesca
name: Tarallo, Roberta
name: Weisz, Alessandro
name: Giurato, Giorgio
Publisher: name: figshare
Year: 2021
Subjects: subject: Artificial Intelligence and Image Processing
subject: FOS: Computer and information sciences
subject: Information Systems

description: Additional file 9. Tutorial and use examples of HOME-BIO.
Standard Sources of Particle Production in Heavy Ion Collisions
Creators: name: Capella, A.
Publisher: name: arXiv
Year: 1999
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We describe particle production in the framework of an independent string model: the dual parton model. We show that an improved version of this model, containing a diquark breaking component, allows to describe the bulk of particle production and, in particular, baryon stopping and most of the observed enhancement of strange baryons. Only for very rare processes, such as $Ω$ or $J/ψ$ production, the model has to be supplemented with final state interaction (comovers interaction). Recent data on event-by-event fluctuations in $p_{T}$ are also described by the model. Predictions for RHIC and LHC are presented and the effect of nuclear shadowing is discussed.
description: 24 pages, 9 postscript figures
Additional file 9: of CYP genetic variants and toxicity related to anti-tubercular agents: a systematic review and meta-analysis
Creators: name: Richardson, Marty
name: Kirkham, Jamie
name: Dwan, Kerry
name: Sloan, Derek
name: Davies, Geraint
name: Jorgensen, Andrea
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Genetics
subject: FOS: Biological sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: Science Policy

description: Table S4. Summary of results for other toxicity outcomes. (DOCX 16Â kb)
Graded Parafermions
Creators: name: Camino, J. M.
name: Ramallo, A. V.
name: de Santos, J. M. Sanchez
Publisher: name: arXiv
Year: 1998
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: A graded generalization of the Z_k parafermionic current osp(1|2)/U(1) coset conformal field theory. The structure of the parafermionic highest-weight modules is analyzed and the dimensions of the fields of the theory are determined. A free field realization of the graded parafermionic system is obtained and the structure constants of the current algebra are found. Although the theory is not unitary, it presents good reducibility properties.
description: 27 pages, LaTeX, 1 eps file. Typos corrected
Negative probabilities, II: What they are and what they are for
Creators: name: Blass, Andreas
name: Gurevich, Yuri
Publisher: name: arXiv
Year: 2018
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: A signed probability distribution may extend a given traditional probability from observable events to all events. We formalize and illustrate this approach. We also illustrate its limitation. We argue that the right question is not what negative probabilities are but what they are for.
Additional file 1 of Combined consideration of body mass index and waist circumference identifies obesity patterns associated with risk of stroke in a Chinese prospective cohort study
Creators: name: Cong, Xiangfeng
name: Liu, Shaobo
name: Wang, Wenjuan
name: Ma, Jixiang
name: Li, Jianhong
Publisher: name: figshare
Year: 2022
Subjects: subject: Medicine
subject: Physiology
subject: FOS: Biological sciences
subject: Biotechnology
subject: Biological Sciences not elsewhere classified
subject: Science Policy
subject: Mental Health

description: Additional file 1: Figure S1. Flowchart of participant inclusion. Figure S2. Prevalence (95%CI) of General Obesity by Sex in General Population and Sub-populations. Figure S3. Prevalence (95%CI) of Abdominal Obesity by Sex in General Population and Sub-populations. TableS1. Associations of Combining BMI and WC with Stroke in Males Subpopulation. TableS2. Associations of Combining BMI and WC with Stroke in Females Subpopulation. TableS3. Subgroup analysis and Sensitivity analysis for incident stroke in general and with CVD risk factor population in male and female (not included results of Overweight/High WC).