cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Unveiling the dynamical state of massive clusters through the ICL fraction
Creators: name: Jiménez-Teja, Y.
name: Dupke, R.
name: Benítez, N.
name: Koekemoer, A. M.
name: Zitrin, A.
name: Umetsu, K.
name: Ziegler, B. L.
name: Frye, B. L.
name: Ford, H.
name: Bouwens, R. J.
name: Bradley, L. D.
name: Broadhurst, T.
name: Coe, D.
name: Donahue, M.
name: Graves, G. J.
name: Grillo, C.
name: Infante, L.
name: Jouvel, S.
name: Kelson, D. D.
name: Lahav, O.
name: Lazkoz, R.
name: Lemze, D.
name: Maoz, D.
name: Medezinski, E.
name: Melchior, P.
name: Meneghetti, M.
name: Mercurio, A.
name: Merten, J.
name: Molino, A.
name: Moustakas, L. A.
name: Nonino, M.
name: Ogaz, S.
name: Riess, A. G.
name: Rosati, P.
name: Sayers, J.
name: Seitz, S.
name: Zheng, W.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We have selected a sample of eleven massive clusters of galaxies observed by the Hubble Space Telescope in order to study the impact of the dynamical state on the IntraCluster Light (ICL) fraction, the ratio of total integrated ICL to the total galaxy member light. With the exception of the Bullet cluster, the sample is drawn from the Cluster Lensing and Supernova Survey and the Frontier Fields program, containing five relaxed and six merging clusters. The ICL fraction is calculated in three optical filters using the CHEFs IntraCluster Light Estimator, a robust and accurate algorithm free of a priori assumptions. We find that the ICL fraction in the three bands is, on average, higher for the merging clusters, ranging between $\sim7-23\%$, compared with the $\sim 2-11\%$ found for the relaxed systems. We observe a nearly constant value (within the error bars) in the ICL fraction of the regular clusters at the three wavelengths considered, which would indicate that the colors of the ICL and the cluster galaxies are, on average, coincident and, thus, their stellar populations. However, we find a higher ICL fraction in the F606W filter for the merging clusters, consistent with an excess of lower-metallicity/younger stars in the ICL, which could have migrated violently from the outskirts of the infalling galaxies during the merger event.
description: 25 pages, 13 figures, 2 tables. Accepted for publication in ApJ
Second-Order Scaling in the Two-Flavor QCD Chiral Transition
Creators: name: Berera, Arjun
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Lattice (hep-lat)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Scaling behavior is analyzed for the two-flavor QCD lattice gauge theory chiral transition. Leading scaling behavior and correction to leading scaling from lattice spacing effects are examined for the quark condensate. Scaling predictions under the assumption of quark mass dominance are tested for the longitudinal correlation length. Second order scaling behavior is consistent with present data.
description: 8 pages, 1 figure , Phys. Rev D, in press 1994
Organizations Interested in Open OnDemand
Creators: name: OH-TECH Consortium
Publisher: name: figshare
Year: 2019
Subjects: subject: 80110 Simulation and Modelling
subject: FOS: Computer and information sciences

description: This is a list of organizations that have expressed interest in, are deploying, or have deployed Open OnDemand.
Tuning the electronic properties of gated multilayer phosphorene: A self-consistent tight-binding study
Creators: name: Li, L. L.
name: Partoens, B.
name: Peeters, F. M.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: By taking account of the electric-field-induced charge screening, a self-consistent calculation within the framework of the tight-binding approach is employed to obtain the electronic band structure of gated multilayer phosphorene and the charge densities on the different phosphorene layers. We find charge density and screening anomalies in single-gated multilayer phosphorene and electron-hole bilayers in dual-gated multilayer phosphorene. Due to the unique puckered lattice structure, both intralayer and interlayer charge screenings are important in gated multilayer phosphorene. We find that the electric-field tuning of the band structure of multilayer phosphorene is distinctively different in the presence and absence of charge screening. For instance, it is shown that the unscreened band gap of multilayer phosphorene decreases dramatically with increasing electric-field strength. However, in the presence of charge screening, the magnitude of this band-gap decrease is significantly reduced and the reduction depends strongly on the number of phosphorene layers. Our theoretical results of the band-gap tuning are in good agreement with recent experiments.
description: 11 pages, 10 figures, To appear in Phys. Rev. B
Discovery of circularly polarised radio emission from SS 433
Creators: name: Fender, Robert
name: Rayner, David
name: Norris, Ray
name: Sault, R. J.
name: Pooley, Guy
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report the discovery of circularly polarised radio emission from the radio-jet X-ray binary SS 433 with the Australia Telescope Compact Array. The flux density spectrum of the circular polarization, clearly detected at four frequencies between 1 - 9 GHz, has a spectral index of (-0.9 +/- 0.1). Multiple components in the source and a lack of very high spatial resolution do not allow a unique determination of the origin of the circular polarization, nor of the spectrum of fractional polarization. However, we argue that the emission is likely to arise in the inner regions of the binary, possibly via propagation-induced conversion of linear to circular polarization, and the fractional circular polarization of these regions may be as high as 10%. Observations such as these have the potential to investigate the composition, whether pairs or baryonic, of the ejecta from X-ray binaries.
description: Accepted for publication in ApJ Letters
Additional file 1 of Transcriptome analysis reveals the defense mechanism of cotton against Verticillium dahliae in the presence of the biocontrol fungus Chaetomium globosum CEF-082
Creators: name: Zhang, Yun
name: Yang, Na
name: Zhao, Lihong
name: Zhu, Heqin
name: Tang, Canming
Publisher: name: figshare
Year: 2020
Subjects: subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Ecology
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Computational Biology

description: Additional file 1: Figure S1. Correlation thermograms of the 18 samples.
Additional file 3 of Transcriptome analysis reveals the defense mechanism of cotton against Verticillium dahliae in the presence of the biocontrol fungus Chaetomium globosum CEF-082
Creators: name: Zhang, Yun
name: Yang, Na
name: Zhao, Lihong
name: Zhu, Heqin
name: Tang, Canming
Publisher: name: figshare
Year: 2020
Subjects: subject: Biophysics
subject: Cell Biology
subject: Molecular Biology
subject: Ecology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Computational Biology

description: Additional file 3: Figure S3. Clustering thermogram of 1209 DEGs.
Additional file 5 of Transcriptome analysis reveals the defense mechanism of cotton against Verticillium dahliae in the presence of the biocontrol fungus Chaetomium globosum CEF-082
Creators: name: Zhang, Yun
name: Yang, Na
name: Zhao, Lihong
name: Zhu, Heqin
name: Tang, Canming
Publisher: name: figshare
Year: 2020
Subjects: subject: Biophysics
subject: Cell Biology
subject: Molecular Biology
subject: Ecology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Computational Biology

description: Additional file 5: Figure S5. Venn diagram of DEGs.
Snow Cover Reconstruction in the Brunswick Peninsula, Patagonia, Derived from a Combination of the Spectral Fusion, Mixture Analysis, and Temporal Interpolation of MODIS Data
Creators: name: Aguirre, Francisco
name: Bozkurt, Deniz
name: Sauter, Tobias
name: Carrasco, Jorge
name: Schneider, Christoph
name: Jaña, Ricardo
name: Casassa, Gino
Publisher: name: Humboldt-Universität zu Berlin
Year: 2023
Subjects: subject: snow cover
subject: remote sensing
subject: spectral downscaling
subject: Patagonia
subject: 550 Geowissenschaften

description: Several methods based on satellite data products are available to estimate snow cover properties, each one with its pros and cons. This work proposes and implements a novel methodology that integrates three main processes applied to MODIS satellite data for snow cover property reconstruction: (1) the increase in the spatial resolution of MODIS (MOD09) data to 250 m using a spectral fusion technique; (2) a new proposal of snow-cloud discrimination; (3) the daily spatio-temporal reconstruction of snow extent and its albedo signature using the endmembers extraction and spectral mixture analyses. The snow cover reconstruction method was applied to the Brunswick Peninsula, Chilean Patagonia, a low-elevation (<1500 m a.s.l.) mid-latitude area. The results show a 98% agreement between MODIS snow detection and ground-based snow measurements at the automatic weather station, Tres Morros (53.3174°S, 71.2790°W), with fractional snow cover values between 20% and 50%, showing a close relationship between snow and vegetation type. The number of snow days compiled from the MODIS data indicates a good performance (Pearson’s correlation of 0.9) compared with the number of skiing days at the Cerro Mirador ski center, Punta Arenas. Although the number of seasonal snow days showed a significant increasing trend of 0.54 days/year in the Brunswick Peninsula during the 2000–2020 period, a significant decrease of −4.64 days/year was detected in 2010–2020.
Additional file 1 of Self-supervised deep learning model for COVID-19 lung CT image segmentation highlighting putative causal relationship among age, underlying disease and COVID-19
Creators: name: Fung, Daryl L. X.
name: Liu, Qian
name: Zammit, Judah
name: Leung, Carson Kai-Sang
name: Hu, Pingzhao
Publisher: name: figshare
Year: 2021
Subjects: subject: Artificial Intelligence and Image Processing
subject: FOS: Computer and information sciences

description: Additional file 1: Figure S1. Architecture of the supervised InfNet. Figure S2. A is the original architecture of the SInfNet. B is the architecture of our self-supervised InfNet model. Highlighted purple block is the difference between the original single SInfNet and the single SSInfNet. Figure S3. A is the architecture of the original multi SInfNet model. B is the architecture of our self-supervised multi InfNet model. Highlighted green block is the difference between the original multi SInfNet and our self-supervised multi SSInfNet. Figure S4. ROC for single InfNet. Algorithm S1. SSInfNet. Table S1. Image phenotypes. Table S2. The three-fold cross-validation performance of single networks. It should be noted that the data were obtained by combining the training, testing, and validation set from the Med-Seg (medical segmentation) COVID-19 dataset, and then splitting the combined data into 3 folds. Table S3. The three-fold cross validation performance of multi networks. Table S4. Comparison with transfer learning based FCN8 network. Quantitative result of Ground-glass Opacities & Consolidation on the test data set of the Med-Seg (medical segmentation) COVID-19 dataset. Prior was obtained from the single segmentation InfNet. Table S5. Model performance on independent COVID-19 CT Dataset set 2. Table S6. Model performance on the independent COVID-19 CT Data set 3. Table S7. Results of ablation studies. The performance of the ablation of our proposed multi-SSInfNet. Multi-SSInfNet refers to the self-supervised SInfNet with Focal Loss and Lookahead optimizer. We tried a variety of the model with a subtraction of the different technologies to carry out the ablation. Table S8. Computational costs of processing one image
Parameters of the model analyzed in detail from From head to tail: a neuromechanical model of forward locomotion in Caenorhabditis elegans
Creators: name: Izquierdo, Eduardo J.
name: Beer, Randall D.
Publisher: name: The Royal Society
Year: 2018
Subjects: subject: Neuroscience
subject: 110601 Biomechanics
subject: FOS: Health sciences
subject: 60801 Animal Behaviour
subject: FOS: Biological sciences

description: With 302 neurons and a near-complete reconstruction of the neural and muscle anatomy at the cellular level, Caenorhabditis elegans is an ideal candidate organism to study the neuromechanical basis of behaviour. Yet, despite the breadth of knowledge about the neurobiology, anatomy and physics of C. elegans, there are still a number of unanswered questions about one of its most basic and fundamental behaviours: forward locomotion. How the rhythmic pattern is generated and propagated along the body is not yet well understood. We report on the development and analysis of a model of forward locomotion that integrates the neuroanatomy, neurophysiology and body mechanics of the worm. Our model is motivated by experimental analysis of the structure of the ventral cord circuitry and the effect of local body curvature on nearby motoneurons. We developed a neuroanatomically grounded model of the head motoneuron circuit and the ventral nerve cord circuit. We integrated the neural model with an existing biomechanical model of the worm's body, with updated musculature and stretch receptors. Unknown parameters were evolved using an evolutionary algorithm to match the speed of the worm on agar. We performed 100 evolutionary runs and consistently found electrophysiological configurations that reproduced realistic control of forward movement. The ensemble of successful solutions reproduced key experimental observations that they were not designed to fit, including the wavelength and frequency of the propagating wave. Analysis of the ensemble revealed that head motoneurons SMD and RMD are sufficient to drive dorsoventral undulations in the head and neck and that short-range posteriorly directed proprioceptive feedback is sufficient to propagate the wave along the rest of the body.This article is part of the theme issue ‘Understanding the mind of the worm: modelling C. elegans at cellular resolution’.
Anomalous quantum interference effects in graphene SNS junctions due to strain-induced gauge fields
Creators: name: Khanjani, Hadi
name: Moghaddam, Ali G.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: We investigate the influence of gauge fields induced by strain on the supercurrent passing through the graphene-based Josephson junctions. We show in the presence of a constant pseudomagnetic field ${\bf B}_S$ originated from an arc-shape elastic deformation, the Josephson current is monotonically enhanced. This is in contrast with the oscillatory behavior of supercurrent (known as Fraunhofer pattern) caused by real magnetic fields passing through the junction. The absence of oscillatory supercurrent originates from the fact that strain-induced gauge fields have opposite directions at the two valleys due to the time-reversal symmetry. Subsequently there is no net Aharonov-Bohm effect due to ${\bf B}_S$ in the current carried by the bound states composed of electrons and holes from different valleys. On the other hand, when both magnetic and pseudomagnetic fields are present, Fraunhofer-like oscillations as function of the real magnetic field flux are found. We find that the Fraunhofer pattern and in particular its period slightly change by varying the strain-induced gauge field as well as the geometric aspect ratio of the junction. Intriguingly, the combination of two kinds of gauge fields results in two special fingerprint in the local current density profile: (i) strong localization of the Josephson current density with more intense maximum amplitudes; (ii) appearance of the inflated vortex cores - finite regions with almost diminishing Josephson currents - which their sizes increases by increasing ${\bf B}_S$. These findings reveal unexpected interference signatures of strain-induced gauge fields in graphene SNS junctions and provide unique tools for sensitive probing of the pseudomagnetic fields.
description: 10 pages
title: ADCO, Privilèges de l'Ordre de Cîteaux en matière de succession (Fin XVe siècle), Cart. 176 (11 H 8), f. 0029
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2017
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi

description: Privilèges de l'Ordre de Cîteaux en matière de succession (Fin XVe siècle), Archives départementales de la Côte-d'Or, Cart. 176 (11 H 8), f. 0029, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Privilèges de l'Ordre de Cîteaux en matière de succession (Fin XVe siècle), Archives départementales de la Côte-d'Or, Cart. 176 (11 H 8), f. 0029, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
Model independent determination of |Vub| in heavy meson effective thoery
Creators: name: Kitazawa, Noriaki
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We propose a strategy of the model-independent determination of the Kobayashi-Maskawa matrix element $|V_{ub}|$ within the framework of the heavy meson effective theory. The effective theory is model-independent, since no assumption on the dynamics is introduced except for the symmetry of QCD. Although the effective theory can only be applied to the decay process with soft pions, high detection efficiency on the soft pions in the future B-factories makes this theory effective. The two exclusive processes, $B \rightarrow πl ν$ and $B \rightarrow ππl ν$, are used to determine the value of $|V_{ub}|$, under the condition that the values of the decay constants of $B$ and $B^*$ mesons are given.
description: KEK preprint TH-413, 14 pages
Isolated Neutron Stars: Accretors and Coolers
Creators: name: Treves, Aldo
name: Turolla, Roberto
name: Zane, Silvia
name: Colpi, Monica
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: As many as $10^9$ neutron stars populate the Galaxy, but only $\approx 10^3$ are directly observed as pulsars or as accreting sources in X-ray binaries. In principle also the accretion of the interstellar medium may make isolated neutron stars shine, and their weak luminosity could be detected in soft X-rays. Recent ROSAT observations have convincingly shown that neutron stars accreting from the interstellar medium are extremely rare, if observed at all, in contrast with earlier theoretical predictions. Until now two possible explanations for their elusiveness have been proposed: their velocity distribution may peak at $\sim 200-400 {\rm km s}^{-1}$, as inferred from pulsar statistics, and this would severely choke accretion; the magnetic field may decay on timescales $\sim 10^8-10^9$ yr, preventing a large fraction of neutron stars from entering the accretor stage. The search for accreting neutron stars has produced up to now a handful of promising candidates. While little doubt is left that these objects are indeed isolated neutron stars, the nature of their emission is still controversial. In particular accreting objects can be confused with much younger, cooling neutron stars. However, a combination of observations and theoretical modeling may help in discriminating between the two classes.
description: 22 pages Latex, 3 Figures, Invited Review to be published to PASP
Testing factorization in colour-suppressed beauty decays with the B -> η_c + K(K^*) modes
Creators: name: Gourdin, M.
name: Keum, Y. Y.
name: Pham, X. Y.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The large discrepancy recently observed between $B \ra J/Ψ+ K (K^*)$ data and commonly used hadronic form factor models might be due to a breakdown of the factorization assumption. By showing that the $B \ra η_c + K (K^*)$ rates can be calculated without relying on any form factor model, we propose a test of the factorization hypothesis. This test is free of possible uncertainties caused by final state interactions and $W$-exchange graph contributions. If factorization holds, the measurable ratio $Γ(B \ra η_c + K^*)/Γ(B \ra η_c + K )$ is predicted to be in the range from 0.18 to 0.95 when the CLEO II data on $B \ra J/Ψ+ K (K^*)$ are used.
description: Latex 17pages(excluded 2 figures),Preprint PAR/LPTHE/94-32
Additional file 2 of Transcriptome analysis reveals the defense mechanism of cotton against Verticillium dahliae in the presence of the biocontrol fungus Chaetomium globosum CEF-082
Creators: name: Zhang, Yun
name: Yang, Na
name: Zhao, Lihong
name: Zhu, Heqin
name: Tang, Canming
Publisher: name: figshare
Year: 2020
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Ecology
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Computational Biology

description: Additional file 2: Figure S2. PCA of the 18 samples.
On the orbital evolution and growth of protoplanets embedded in a gaseous disc
Creators: name: Papaloizou, J. C. B.
name: Larwood, J. D.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a new computation of the linear tidal interaction of a protoplanetary core with a thin gaseous disc in which it is fully embedded. For the first time a discussion of the orbital evolution of cores with eccentricity (e) significantly larger than the gas-disc scale height to radius ratio (H/r) is given. We find that the direction of orbital migration reverses for e>1.1H/r. This occurs as a result of the orbital crossing of resonances in the disc that do not overlap the orbit when the eccentricity is very small. Simple expressions giving approximate fits to the eccentricity damping rate and the orbital migration rate are presented. We go on to calculate the rate of increase of the mean eccentricity for a system of protoplanetary cores due to dynamical relaxation. By equating the eccentricity damping time-scale with the dynamical relaxation time-scale we deduce that an equilibrium between eccentricity damping and excitation through scattering is attained on a 10^3 to 10^4 yr time-scale, at 1au. The equilibrium thickness of the protoplanet distribution is such that it is generally well confined within the gas disc. By use of a three dimensional N-body code we simulate the evolution of a system of protoplanetary cores, incorporating our eccentricity damping and migration rates. Assuming that collisions lead to agglomeration, we find that the vertical confinement of the protoplanet distribution permits cores to build up from 0.1 to 1 earth mass in only ~10^4 yr, within 1au. The time-scale required to achieve this is comparable to the migration time-scale. We deduce that it is not possible to build up a massive enough core to form a gas giant planet before orbital migration ultimately results in the preferential delivery of all such bodies to the neighbourhood of the central star. [Abridged]
description: Latex in MNRAS style, 13 pages with 6 figures, also available from http://www.maths.qmw.ac.uk/~jdl/
title: Mail à Richard Cross, Aurèle Ricard, Hervé Deslandes, Laurent Hervieu, Jean-Sébastien Tisserand, Alessandro di Bergamo, copie à Valérie Laloux et réponse de Valérie Laloux
Creators: name: Laloux, Valérie
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020

description: En pièce jointe : Valérie Laloux, Cédric Tolley, "VIH SIDA : bientôt la fin de l'épidémie ?", extrait de Echos, no 87, décembre 2014. 2 exemplaires dont 1 retransféré par J. Leibowitch à Claude Capelier.
description: Source: http://www.calames.abes.fr/pub/ms/Calames-20193111134069941
description: created: start=2015-01-23;end=2015-01-29
title: V2_DU_LettreC
Creators: name: Basnage de Beauval, Henri
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020

description: Ceci est la V2 du Dictionnaire universel, revu et corrigé en 1701 par Basnage de Beauval. Cette version a été obtenue avec GROBID dictionaries, après adaptation du système et renentraînement en juillet 2020.
title: Mail à Pierre de Truchis, Jean-Claude Melchior, Christian Perronne, Roland Landman, Pierre-marie Girard, copie à Dominique Mathez, Philippe Poussier, John David - Pièce jointe
Creators: name: Leibowitch, Jacques
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020

description: Pièce jointe : Diapositives de présentation sur le traitement ICARRE.
description: Source: http://www.calames.abes.fr/pub/ms/Calames-20193111133912115
QCD corrections to inclusive $ΔS=1,2$ transitions
Creators: name: Jamin, Matthias
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The talk summarises a calculation of the two-point functions for $ΔS=1$ current-current and QCD-penguin operators, as well as for the $ΔS=2$ operator, at the next-to-leading order. The size of the gluonic corrections to current-current operators is large, providing a qualitative understanding of the observed enhancement in $ΔI=1/2$ transitions. In the $ΔS=2$ sector the QCD corrections are quite moderate ($\approx -20\%$). This work has been done in collaboration with Antonio Pich.
description: 3 pages, Invited talk presented at ``QCD'94'', Montpellier, France, July 7 - 13, 1994, hep-ph/yymmnnn
title: ADCO, Premier cartulaire de l'abbaye de Molesmes (XIIe siècle), Cart. 142 (7 H 6), 128 pages, f. 001
Creators: name: de la Côte d'Or, Archives départementales
name: Petot, Frédéric
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2009
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: cartulaire
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge

description: Premier cartulaire de l'abbaye de Molesmes (XIIe siècle), Archives départementales de la Côte-d'Or, Cart. 142 (7 H 6), 128 pages, f. 001, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Premier cartulaire de l'abbaye de Molesmes (XIIe siècle), Archives départementales de la Côte-d'Or, Cart. 142 (7 H 6), 128 pages, f. 001, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb137389344
description: Provenance: abbaye de Molesme
description: Provenance: http://www.wikidata.org/entity/Q334044
CP Violation in the Heavy Neutrinos Production Process $e^+e^-\rightarrow N_1N_2$
Creators: name: Gluza, J.
name: Zralek, M.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The problem of CP conservation and CP violation for two heavy neutrinos production in $e^+e^-$ interaction is considered. Very convenient way of parametrization of the neutrino mass matrix, from which necessary and sufficient condition for CP conservation easily follows, is presented. Contrary to the Kobayashi-Maskawa mechanism, the effects of CP violation in the lepton sector with Majorana neutrinos can be very large. Change of the total cross section caused by CP violation can be much larger then the cross section itself.
description: LATEX,12 pages
Commentary on Calculation of Dark Energy and Dark Matter, Journal of Physics and Astronomy, 25-May-2023, Vol.11, Issue 5, 346
Creators: name: Jöge, Friedhelm
Publisher: name: figshare
Year: 2024
Subjects: classificationCode: 510304
subject: Thermodynamics and statistical physics

description: A formula for calculating Dark Energy is established through derivation.. The conclusion is examined using the Max Planck Institute for Radio Astronomy's data. Additional formulas are subtracted. The universe's Dark Matter has been computed. there is a balance sheet created. Inferences are made.
title:  Investigating New Reporting Practices in Local Government: Is Integrating Reporting the Best Way?
Creators: name: Manes Rossi, Francesca
name: Levy Orelli, Rebecca
Publisher: name: RomaTrE-Press
Year: 2019

description: Nuove pratiche di reporting sono fiorite nelle pubbliche amministrazioni per comunicare agli stakeholder il valore creato per la comunità. Questo studio si propone di indagare l'evoluzione delle nuove pratiche di rendicontazione nelle amministrazioni locali, mettendo in discussione la capacità del reporting integrato di rappresentare il modo migliore per le amministrazioni locali per migliorare l’accountability e il coinvolgimento degli stakholders.
description: Qualitative Research in Intangibles, Intellectual Capital and Integrated Reporting Practices
Detection of Planetary Transits Across a Sun-like Star
Creators: name: Charbonneau, David
name: Brown, Timothy M.
name: Latham, David W.
name: Mayor, Michel
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report high precision, high cadence photometric measurements of the star HD 209458, which is known from radial velocity measurements to have a planetary mass companion in a close orbit. We detect two separate transit events at times that are consistent with the radial velocity measurements. In both cases, the detailed shape of the transit curve due to both the limb darkening of the star and the finite size of the planet is clearly evident. Assuming stellar parameters of 1.1 R_Sun and 1.1 M_Sun, we find that the data are best interpreted as a gas giant with a radius of 1.27 +/- 0.02 R_Jup in an orbit with an inclination of 87.1 +/- 0.2 degrees. We present values for the planetary surface gravity, escape velocity, and average density, and discuss the numerous observations that are warranted now that a planet is known to transit the disk of its parent star.
description: 10 pages, 3 figures, accepted by ApJ Letters
Supporting distributed, interactive Jupyter and RStudio in a scheduled HPC environment with Spark using Open OnDemand
Creators: name: OH-TECH Consortium
Publisher: name: figshare
Year: 2018
Subjects: subject: 80110 Simulation and Modelling
subject: FOS: Computer and information sciences

description: Paper presented at PEARC18 on Open OnDemand
Influence of dielectric layers on estimates of diffusion coefficients and concentrations of ions from impedance spectroscopy
Creators: name: Khazimullin, Maxim V.
name: Lebedev, Yuriy A.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: We present the analysis of the impedance spectra for a binary electrolyte confined between blocking electrodes with dielectric layers. An expression for the impedance is derived from Poisson-Nernst-Planck equations in the linear approximation taking into account the voltage drop on the dielectric layer. The analysis shows, that characteristic features of the frequency dependence of the impedance are determined by the ratio of the Debay length and the effective thickness of the dielectric layer. The impact of the dielectric layer is especially strong in the case of high concentrated electrolytes, where the Debay length is small and thus comparable to the effective thickness of the dielectric layer. To verify the model, measurements of the impedance spectra and transient currents in a liquid crystal 4-n-pentyl-4'-cyanobiphenyl (5CB) confined between polymer-coated electrodes in cells of different thicknesses are performed. The estimates for the diffusion coefficient and ion concentration in 5CB obtained from the analysis of the impedance spectra and the transient currents are consistent and agree with previously reported data. We demonstrate that calculations of the ion parameters from the impedance spectra without taking into account the dielectric layer contribution lead in most cases to incorrect results. Application of the model to analyze violations of the low-frequency impedance scaling and contradictions in the estimates of the ion parameters recently found in some ionic electrolytes are discussed.
description: 34 pages, 5 figures, 3 tables
Ground-State Wave Function with Interactions between Different Species in $M$-Component Miscible Bose-Einstein Condensates
Creators: name: Kohno, Wataru
name: Kirikoshi, Akimitsu
name: Kita, Takafumi
Publisher: name: arXiv
Year: 2018
Subjects: subject: Quantum Gases (cond-mat.quant-gas)
subject: FOS: Physical sciences

description: We construct a variational ground-state wave function of weakly interacting M-component Bose-Einstein condensates beyond the mean-field theory by incorporating the dynamical 3/2-body processes, where one of the two colliding particles drops into the condensate and vice versa. Our numerical results with various masses and particle numbers show that the 3/2-body processes between different particles make finite contributions to lowering the ground-state energy, implying that many-body correlation effects between different particles are essential even in the weak-coupling regime of the Bose--Einstein condensates. We also consider the stability condition for $2$-component miscible states using the new ground-state wave function. Through this calculation, we obtain the relation $U^{2}_{AB}/U_{AA}U_{BB}<1+α$, where $U_{ij}$ is the effective contact potential between particles $i$ and $j$ and $α$ is the correction, which originates from the $3/2$-body and $2$-body processes.
description: 9 pages, 3 figures
Supersymmetry and SU(2)xU(1) breaking with naturally vanishing vacuum energy
Creators: name: Brignole, A.
name: Zwirner, F.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We show how the spontaneous breaking of local N=1 supersymmetry and of the SU(2)xU(1) gauge symmetry can be simultaneously realized, with naturally vanishing tree-level vacuum energy, in superstring effective supergravities. Both the gravitino mass m_{3/2} and the electroweak scale m_Z are classically undetermined, and slide along moduli directions that include the Higgs flat direction |H_1^0| = |H_2^0|. There are important differences with conventional supergravity models: the goldstino has components along the higgsino direction; SU(2) x U(1) breaking occurs already at the classical level; the scales m_{3/2} and m_Z, the gauge couplings, the lightest Higgs mass and the cosmological constant are entirely determined by quantum corrections.
description: 11 pages, no figures, plain LATEX, preprint CERN-TH.7439/94, LBL-35117
A Survey of CH3CN and HC3N in Protoplanetary Disks
Creators: name: Bergner, Jennifer B.
name: Guzman, Viviana G.
name: Oberg, Karin I.
name: Loomis, Ryan A.
name: Pegues, Jamila
Publisher: name: arXiv
Year: 2018
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: The organic content of protoplanetary disks sets the initial compositions of planets and comets, thereby influencing subsequent chemistry that is possible in nascent planetary systems. We present observations of the complex nitrile-bearing species CH3CN and HC3N towards the disks around the T Tauri stars AS 209, IM Lup, LkCa 15, and V4046 Sgr as well as the Herbig Ae stars MWC 480 and HD 163296. HC3N is detected towards all disks except IM Lup, and CH3CN is detected towards V4046 Sgr, MWC 480, and HD 163296. Rotational temperatures derived for disks with multiple detected lines range from 29-73K, indicating emission from the temperate molecular layer of the disk. V4046 Sgr and MWC 480 radial abundance profiles are constrained using a parametric model; the gas-phase CH3CN and HC3N abundances with respect to HCN are a few to tens of percent in the inner 100 AU of the disk, signifying a rich nitrile chemistry at planet- and comet-forming disk radii. We find consistent relative abundances of CH3CN, HC3N, and HCN between our disk sample, protostellar envelopes, and solar system comets; this is suggestive of a robust nitrile chemistry with similar outcomes under a wide range of physical conditions.
Semileptonic $B_{(s)}\to a_1(K_1)\ell^+ \ell^-$ decays via the light-cone sum rules with $B$-meson distribution amplitudes
Creators: name: Momeni, S.
name: Khosravi, R.
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The form factors of semileptonic $B_{(s)}\to a_{1}(K_1)\, \ell^{+}\ell^{-}$, $ \ell=τ,μ,e$ transitions are investigated in the framework of the light-cone sum rules with $B$-meson distribution amplitudes, which play an important role in exclusive $B$ decays. The $B$-meson distribution amplitudes, $φ_{\pm}(ω)$ are a model-dependent form, so we consider four different parameterizations which can provide a reasonable description of $φ_{\pm}(ω)$ from QCD corrections. The branching fractions of these transitions are calculated. For a better analysis, a comparison of our results with the prediction of other models is provided.
description: 14 pages, 5 figures
Detecting Weak Spectral Lines in Interferometric Data through Matched Filtering
Creators: name: Loomis, Ryan A.
name: Öberg, Karin I.
name: Andrews, Sean M.
name: Walsh, Catherine
name: Czekala, Ian
name: Huang, Jane
name: Rosenfeld, Katherine
Publisher: name: arXiv
Year: 2018
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: Modern radio interferometers enable observations of spectral lines with unprecedented spatial resolution and sensitivity. In spite of these technical advances, many lines of interest are still at best weakly detected and therefore necessitate detection and analysis techniques specialized for the low signal-to-noise ratio (SNR) regime. Matched filters can leverage knowledge of the source structure and kinematics to increase sensitivity of spectral line observations. Application of the filter in the native Fourier domain improves SNR while simultaneously avoiding the computational cost and ambiguities associated with imaging, making matched filtering a fast and robust method for weak spectral line detection. We demonstrate how an approximate matched filter can be constructed from a previously observed line or from a model of the source, and we show how this filter can be used to robustly infer a detection significance for weak spectral lines. When applied to ALMA Cycle 2 observations of CH3OH in the protoplanetary disk around TW Hya, the technique yields a ~53% SNR boost over aperture-based spectral extraction methods, and we show that an even higher boost will be achieved for observations at higher spatial resolution. A Python-based open-source implementation of this technique is available under the MIT license at https://github.com/AstroChem/VISIBLE.
description: 20 pages, 8 figures, accepted for publication in The Astronomical Journal
Constraints on the Spatial Distribution and Luminosity function of GRBs
Creators: name: Bulik, Tomasz
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The distance scale to gamma ray bursts has been a subject of scientific debate for almost thirty years. Up to the discovery of afterglows only indirect methods could be used to constrain the distance scale to this objects. I review some of these results, and show the current limits on the spatial distribution and luminosity function of GRBs. The results obtained with different methods indicate that gamma-ray bursts lie at the typical redshifts $z_{ave}$ between 1 and 2, however there can exist a long tail of the distribution stretching to higher redshifts. The width of the GRB luminosity function (the ratio of the intrinsic brightness of the brightest to the dimmest observed burst) estimated from Beppo SAX bursts with redshifts is almost $10^3$.
description: 16 pages, uses paspconf.sty, Proceedings of the February 1999 Workshop "Gamma Ray Bursts: The First Three Minutes" in Graftavallen, Sweden
Higgs Boson Contributions to Neutrino Production in e-e+ Collisions in a Left-Right Symmetric Model
Creators: name: Gluza, J.
name: Zralek, M.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: In gauge models with bigger number of Higgs particles their couplings to fermions are more complicated then in the standard model (SM). The influence of the Higgs bosons exchange on the neutrino production cross section in $e^-e^+$ collision ($e^-e^+ \rightarrow νN$) is investigated. The study has been done in the framework of the left-right symmetric model with the rich Higgs sector containing bidoublet and two triplets. The couplings of the Higgs particles even to light leptons can be as large as the gauge bosons couplings. The total effect of the Higgs bosons is small as a result of the big Higgs mass in the propagators.
description: LATEX, 25 pages
BAXSHILAR VA QO'SHIQCHILARNING IJODI: O'ZBEK XALQ QO'SHIQLARI VA TERMALARINING TA'LIMDA QO'LLANILISHI
Creators: name: Niyatqulova, Nozima
Publisher: name: Zenodo
Year: 2025

description: Maqolada O‘zbek xalqining og‘zaki ijodi, ayniqsa, xalq qo‘shiqlari va termalari, ularning xalqning ruhiy dunyosini, tarixiy xotirasini va turmush tarzini ifodalashdagi ahamiyati ta'kidlanadi. Baxshilar tomonidan kuylanadigan termalar ma'naviy va axloqiy mazmunlarga ega bo‘lib, adabiyot va musiqa san'ati o‘rtasidagi bog‘liqlikni ko‘rsatadi. Maqola, shuningdek, xalq qo‘shiqlari va termalarni o‘quvchilarga o‘rgatishdagi samarali metodlar va interaktiv yondashuvlarni ham ko‘rib chiqadi.
Axial Charge Fluctuation and Chiral Magnetic Effect from Stochastic Hydrodynamics
Creators: name: Lin, Shu
name: Yan, Li
name: Liang, Gui-Rong
Publisher: name: arXiv
Year: 2018
Subjects: subject: Nuclear Theory (nucl-th)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: The amount of axial charge produced in heavy ion collisions is one of the key quantities in understanding chiral magnetic effect. Current phenomenological studies assume large axial charge chemical potential $μ_5$ produced in Glasma phase and assume the conservation of axial charge throughout the evolution, which is valid in the long relaxation time limit. Based on the solution of stochastic hydrodynamics with phenomenological parameters, our study suggests that the situation of heavy ion collisions may be close to the opposite limit, in which axial charge fluctuation approaches thermodynamic limit. Using $μ_5$ set by the thermodynamic limit for chiral magnetic effect and a background from parity-even $v_1$, we obtain a reasonable description of the centrality dependence of charged particle correlation measured in experiment.
description: 20 pages, 1 figure
Microfabricated sensor platform with through-glass vias for bidirectional 3-omega thermal characterization of solid and liquid samples
Creators: name: Grosse, Corinna
name: Ras, Mohamad Abo
name: Varpula, Aapo
name: Grigoras, Kestutis
name: May, Daniel
name: Wunderle, Bernhard
name: Chapuis, Pierre-Olivier
name: Gomès, Séverine
name: Prunnila, Mika
Publisher: name: arXiv
Year: 2018
Subjects: subject: Instrumentation and Detectors (physics.ins-det)
subject: FOS: Physical sciences

description: A novel microfabricated, all-electrical measurement platform is presented for a direct, accurate and rapid determination of the thermal conductivity and diffusivity of liquid and solid materials. The measurement approach is based on the bidirectional 3-omega method. The platform is composed of glass substrates on which sensor structures and a very thin dielectric nanolaminate passivation layer are fabricated. Using through-glass vias for contacting the sensors from the chip back side leaves the top side of the platform free for deposition, manipulation and optical inspection of the sample during 3-omega measurements. The thin passivation layer, which is deposited by atomic layer deposition on the platform surface, provides superior chemical resistance and allows for the measurement of electrically conductive samples, while maintaining the conditions for a simple thermal analysis. We demonstrate the measurement of thermal conductivities of borosilicate glass, pure water, glycerol, 2-propanol, PDMS, cured epoxy, and heat-sink compounds. The results compare well with both literature values and values obtained with the steady-state divided bar method. Small sample volumes (~0.02 mm$^2$) suffice for accurate measurements using the platform, allowing rapid temperature-dependent measurements of thermal properties, which can be useful for the development, optimization and quality testing of many materials, such as liquids, gels, pastes and solids.
Topological terms, AdS_2n gravity and renormalized Entanglement Entropy of holographic CFTs
Creators: name: Anastasiou, Giorgos
name: Araya, Ignacio J.
name: Olea, Rodrigo
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We extend our topological renormalization scheme for Entanglement Entropy to holographic CFTs of arbitrary odd dimensions in the context of the AdS/CFT correspondence. The procedure consists in adding the Chern form as a boundary term to the area functional of the Ryu-Takayanagi minimal surface. The renormalized Entanglement Entropy thus obtained can be rewritten in terms of the Euler characteristic and the AdS curvature of the minimal surface. This prescription considers the use of the Replica Trick to express the renormalized Entanglement Entropy in terms of the renormalized gravitational action evaluated on the conically-singular replica manifold extended to the bulk. This renormalized action is obtained in turn by adding the Chern form as the counterterm at the boundary of the 2n-dimensional asymptotically AdS bulk manifold. We explicitly show that, up to next-to-leading order in the holographic radial coordinate, the addition of this boundary term cancels the divergent part of the Entanglement Entropy. We discuss possible applications of the method for studying CFT parameters like central charges.
description: 28 pages, 1 figure