cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Associate Sneutrino-Neutralino/Chargino Production at LEPxLHC
Creators: name: Woehrmann, T.
name: Fraas, H.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We examine for representative gaugino-higgsino mixing scenarios sneutrino-neutralino and sneutrino-chargino production in deep inelastic ep-scattering at the cm-energy of 1.8 TeV. The cross sections for sneutrino-chargino production are more than one order of magnitude bigger than those for sneutrino-squark production. Also for zino-like neutralinos we find cross sections at least comparable to those for sneutrino-squark production.
description: 9 pages, report UWITP-94/1
Deep Radio Imaging of Globular Clusters and the Cluster Pulsar Population
Creators: name: Fruchter, A. S.
name: Goss, W. M.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have obtained deep multifrequency radio observations of seven globular clusters using the Very Large Array and the Australia Telescope Compact Array. Five of these, NGC 6440, NGC 6539, NGC 6544, NGC 6624 and Terzan 5 had previously been detected in a shallower survey for steep spectrum radio sources in globular clusters (Fruchter and Goss 1990). The sixth, the rich globular cluster, Liller 1, had heretofore been undetected in the radio, and the seventh, 47 Tucanae, was not included in our original survey. High resolution 6 and 20 cm images of three of the clusters, NGC 6440, NGC 6539, NGC 6624 reveal only point sources coincident with pulsars which have been discovered subsequent to our first imaging survey. 21 and 18 cm images reveal several point sources within a few core-radii of the center of 47 Tuc. Two of these are identified pulsars, and a third, which is both variable and has a steep spectrum, is also most likely a pulsar previously identified by a pulsed survey. However, the 6, 20 and 90 cm images of NGC 6544, Liller 1 and Terzan 5 display strong steep-spectrum emission which cannot be associated with known pulsars. The image of the rich cluster Terzan 5 displays numerous point sources within $30''$, or 4 core radii of the cluster center. The density of these objects rises rapidly toward the core, where an elongated region of emission is found. The brightest individual sources, as well as the extended emission, possess the steep spectra expected of pulsars. Furthermore, the flux distribution of the sources agrees well with the standard pulsar luminosity function. The total luminosity and number of objects observed suggest that Terzan 5 contains more pulsars than any other Galactic globular cluster.
description: 33 pages, 6 Postscript figures; Accepted for publication in the Astrophysical Journal; abstract abridged. PDF version also available at http://nemesis.stsci.edu/~fruchter/fg99/fg99.pdf
E2 Strength in the Radiative Charmed Baryon Decay
Creators: name: Savage, Martin J.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The radiative decay $Σ_Q^* \rightarrow Λ_Qγ$ can have both magnetic dipole (M1) and electric quadrupole (E2) components. In the heavy quark limit $M_Q\rightarrow\infty$ the transition arises from the spin of the light degrees of freedom changing from $s_l=1$ to $s_l=0$ and hence the E2 contribution vanishes. We compute the leading contribution to the E2 strength in chiral perturbation theory and find that the amplitude is enhanced by a small energy denominator in the chiral limit. This enhancement essentially compensates for the $1/M_c$ suppression that is present in the charm system. We find a mixing ratio of order a few percent dependent upon the $Σ_c^*--Σ_c$ spin symmetry breaking mass difference. The analogous quantity in the b-baryon sector is smaller by a factor of $\sim M_c/M_b$.
description: 10 pages, 2 uuencoded figures included, uses harvmac and epsf, CMU-HEP 94-25
Mass Models and Sunyaev-Zeldovich Effect Predictions for a Flux Limited Sample of 22 Nearby X-Ray Clusters
Creators: name: Mason, Brian S.
name: Myers, Steven T.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We define a 90% complete, volume-limited sample of 31 z<0.1 x-ray clusters and present a systematic analysis of public ROSAT PSPC data on 22 of these objects. Our efforts are undertaken in support of the Penn/OVRO SZE survey, and to this end we present predictions for the inverse Compton optical depth towards all 22 of these clusters. We have performed detailed Monte Carlo simulations to understand the effects of the cluster profile uncertainties on the SZE predictions given the OVRO 5.5-meter telescope beam and switching patterns; we find that the profile uncertainties are one of the least significant components of our error budget for SZE-based distance measurements. We also present baryonic masses and baryon mass fractions derived under the assumption of hydrostatic equilibrium for these 22 clusters. The mean baryonic mass fraction within R_500 \sim 500 h^-1 kpc is (7.02 \pm 0.28) x 10^-2 h^-3/2, or (19.8 \pm 0.8) x 10^-2 for h=0.5. We confirm the Allen et al. (1993) claim of an excess absorbing column density towards Abell 478, but do not find similar anomalies in the other 21 clusters in our sample. We also find some evidence for an excess of soft counts in the ROSAT PSPC data. A measurement of H_o using these models and OVRO SZE determinations will be presented in a second paper.
description: 51 pages, 6 figures included in text. Added comparison of different cosmologies; accepted for publication in ApJ
Cooling Flow Star Formation and the Apparent Stellar Ages of Elliptical Galaxies
Creators: name: Mathews, William G.
name: Brighenti, Fabrizio
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Observational constraints and theoretical arguments indicate that cooled interstellar gas in bright elliptical galaxies forms into a young stellar population throughout the region within the half-light radius. The young population has a bottom-heavy, but optically luminous IMF extending to 1 - 2 M_sun. When the colors and spectral features of this young population are combined with those of the underlying old stellar population, the apparent ages are significantly reduced, similar to the relatively young apparent ages observed in many ellipticals. Galactic mergers are not required to resupply young stars. The sensitivity of continuous star formation to L_B and L_x/L_B is likely to account for the observed spread in apparent ages among elliptical galaxies. Local star formation is accompanied by enhanced stellar H_beta equivalent widths, stronger optical emission lines, enhanced thermal X-ray emission and lower apparent temperatures in the hot gas. The young stars should cause M/L to vary with galactic radius, perturbing the fundamental plane occupied by the old stars.
description: 6 pages with 2 figures; accepted by Astrophysical Journal Letters
Art educators on Twitter and beyond: thinking with virtuality
Creators: name: KERRY FRANCES POWER
Publisher: name: Monash University
Year: 2018
Subjects: Digital Humanities
Education
Art

description: Art educator engagement with social media systems (SMS) oscillates practice in and out of virtual and physical planes and it is important to examine how and why this is done, including the potential connections and associated problems. In 2014, I established a research site on Twitter and spent six months studying the interactions of art educators. Together with my participation in the study, I found that thinking with virtuality encouraged diverse and experimental ways of conceptualising positions on artistic virtual communication. As virtuality is a constantly moving and changing concept, this thesis poses challenges for art education, art educators and art students.
QCD Corrections to $b \to s γ$ Decay in 2-Higgs Doublet Model
Creators: name: Lu, Cai-Dian
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We give a more complete calculation of $b \to sγ$ decay in 2-Higgs doublet model, including leading log QCD corrections from $m_{top}$ to $M_W$ in addition to corrections from $M_{W}$ to $m_b$. The inclusive decay rate in the first model is found to be suppressed 23\% comparing with the calculations without the QCD running from $m_{top}$ to $M_W$. And the enhancement up to 5\% is found in calculations of the second model. More strict restrictions to parameters of 2-Higgs doublet model II are found.
description: 23 pages, 8 figures(not included), Minor Changes
Reconstructing Horndeski theories from phenomenological modified gravity and dark energy models on cosmological scales
Creators: name: Kennedy, Joe
name: Lombriser, Lucas
name: Taylor, Andy
Publisher: name: arXiv
Year: 2018
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: Recently we have derived a set of mapping relations that enables the reconstruction of the family of Horndeski scalar-tensor theories which reproduce the background dynamics and linear perturbations of a given set of effective field theory of dark energy coefficients. In this paper we present a number of applications of this reconstruction. We examine the form of the underlying theories behind different phenomenological parameterizations of modified gravity and dark energy used in the literature, as well as examine theories that exhibit weak gravity, linear shielding, and minimal self-acceleration. Finally, we propose a new inherently stable parametrization basis for modified gravity and dark energy models.
description: 20 pages, 24 figures
Gravitational Lensing of Spherically Symmetric Black Holes in Dark Matter Halos
Creators: name: Liu, Yi-Gao
name: Qiao, Chen-Kai
name: Tao, Jun
Publisher: name: arXiv
Year: 2023
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The gravitational lensing of supermassive black holes surrounded by dark matter halo has attracted a great number of interests in recent years. However, many studies employed simplified dark matter density models, which makes it very hard to give a precise prediction on the dark matter effects in real astrophysical galaxies. In this work, to more accurately describe the distribution of dark matter in real astrophysical galaxies, we study the gravitational lensing of black holes in astrophysical dark matter halo models (Beta, Burkert, Brownstein, and Moore). The deflection angle is obtained using a generalized Gibbons-Werner approach. The visual angular positions and the Einstein rings are also calculated by adopting the gravitational lens equation. Specifically, we choose the supermassive black holes in Milky Way Galaxy, Andromeda galaxy (M31), Virgo galaxy (M87), and ESO138-G014 galaxy as examples, including the corresponding fitted value of dark matter halos. The results suggest that the dark matter halo described by the Beta model has non-negligible influences on the gravitational deflection angle and gravitational lensing observations. However, the Burkert, Brownstein, and Moore models have relatively small influences on angular position of images and the Einstein ring.
description: 30 pages, 9 figures, 3 appendices, V2: new references are included; V3 and V4: majar revision, two new appendices are added
D8.3: Dissemination & Communication Materials
Creators: name: Corongiu, Alessio
Publisher: name: Zenodo
Year: 2017
Subjects: EOSC
Dissemination
Communication

description: Dissemination activities are considered of primary importance for the EOSCpilot Consortium since only if the achieved results are widely communicated to the public, the impact of the project can be meaningful. The target groups for the dissemination activities are divided into several equally important categories, including experts and key stakeholders in different communities. The dissemination activities and all the material developed so far are evenly directed towards all these categories, implementing in every individual case various communication tools and channels.
title: ADCO, Boursier de Cîteaux : comptes (1489-1493) (11 H 1166), f. 00467
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: CBMA/CG21/F.PETOT/2019
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: comptes
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Boursier de Cîteaux : comptes (1489-1493), Archives départementales de la Côte-d'Or, (11 H 1166). Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Boursier de Cîteaux : comptes (1489-1493), Archives départementales de la Côte-d'Or, (11 H 1166), f. 00467, 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
Field Transformations and the Classical Equation of Motion in Chiral Perturbation Theory
Creators: name: Scherer, S.
name: Fearing, H. W.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: The construction of effective Lagrangians commonly involves the application of the `classical equation of motion' to eliminate redundant structures and thus generate the minimal number of independent terms. We investigate this procedure in the framework of chiral perturbation theory. The use of the 'classical equation of motion' is interpreted in terms of field transformations. Such an interpretation is crucial if one wants to bring a given Lagrangian into a canonical form with a minimal number of terms. We emphasize that the application of field transformations not only eliminates structures, or, what is equivalent, expresses certain structures in terms of already known different structures, but also leads to a modification of coefficients of higher--order terms. This will become relevant, once one considers effective interaction terms beyond next--to--leading order, i.e., beyond $O(p^4)$.
description: TRIUMF preprint TRI-PP-94-64, 10 pages in LaTex using RevTex macro
Off-Center Mergers of Clusters of Galaxies and Nonequipartition of Electrons and Ions in Intracluster Medium
Creators: name: Takizawa, Motokazu
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We investigate the dynamical evolution of clusters of galaxies and their observational consequences during off-center mergers, explicitly considering the relaxation process between ions and electrons in intracluster medium by N-body and hydrodynamical simulations. In the contracting phase a bow shock is formed between the two subclusters. The observed temperature between two peaks in this phase depends on the viewing angle even if the geometry of the system seems to be very simple like head-on collisions. Around the most contracting epoch, when we observe merging clusters nearly along the collision axis, they look like spherical relaxed clusters with large temperature gradients. In the expanding phase, spiral bow shocks occur. As in head-on mergers, the electron temperature is significantly lower than the plasma mean one especially in the post-shock regions in the expanding phase. When the systems have relatively large angular momentum, double-peak structures in the X-ray images can survive even after the most contracting epoch. Morphological features in both X-ray images and electron temperature distribution characteristic to off-center mergers are seriously affected by the viewing angle. When the clusters are observed nearly along the collision axis, the distribution of galaxies' line-of-sight (LOS) velocities is a good indicator of mergers. In the contracting phase, an negative kurtosis and a large skewness are expected for nearly equal mass collisions and rather different mass ones, respectively. To obtain statistically significant results, about 1000 galaxies' LOS velocities are required. For nearby clusters ($z<0.05$), large redshift surveys such as 2dF will enable us to study merger dynamics.
description: 21 pages, 7 figures. Accepted for publication in ApJ
Impulsively generated wave trains in coronal structures: II. Effects of transverse structuring on sausage waves in pressureless slabs
Creators: name: Li, Bo
name: Guo, Ming-Zhe
name: Yu, Hui
name: Chen, Shao-Xia
Publisher: name: arXiv
Year: 2018
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Impulsively generated sausage wave trains in coronal structures are important for interpreting a substantial number of observations of quasi-periodic signals with quasi-periods of order seconds. We have previously shown that the Morlet spectra of these wave trains in coronal tubes depend crucially on the dispersive properties of trapped sausage waves, the existence of cutoff axial wavenumbers and the monotonicity of the dependence of the axial group speed on the axial wavenumber in particular. This study examines the difference a slab geometry may introduce, for which purpose we conduct a comprehensive eigenmode analysis, both analytically and numerically, on trapped sausage modes in coronal slabs with a considerable number of density profiles. For the profile descriptions examined, coronal slabs can trap sausage waves with longer axial wavelengths, and the group speed approaches the internal Alfvén speed more rapidly at large wavenumbers in the cylindrical case. However, common to both geometries, cutoff wavenumbers exist only when the density profile falls sufficiently rapidly at distances far from coronal structures. Likewise, the monotonicity of the group speed curves depends critically on the profile steepness right at the structure axis. Furthermore, the Morlet spectra of the wave trains are shaped by the group speed curves for coronal slabs and tubes alike. Consequently, we conclude that these spectra have the potential for telling the sub-resolution density structuring inside coronal structures, although their detection requires an instrumental cadence of better than $\sim 1$ second.
description: 11 figures, accepted for publication in ApJ
Josephson current through the SYK model
Creators: name: Dell'Anna, Luca
Publisher: name: arXiv
Year: 2023
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Superconductivity (cond-mat.supr-con)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We calculate the equilibrium Josephson current through a disordered interacting quantum dot described by a Sachdev-Ye-Kitaev model fully contacted by two BCS superconductors, such that all modes of the dot contribute to the coupling, which encodes hopping and spin-flip processes. We show that, at zero temperature and at the conformal limit, i.e. in the strong interacting limit, the Josephson current is suppressed by $U$, the strength of the interaction, as $\ln(U)/U$ and becomes universal, namely it gets independent on the superconducting gap. At finite temperature, instead, it depends on the ratio between the gap and the temperature. A proximity effect exists but the self-energy corrections induced by the coupling with the superconducting leads seem subleading as compared to the interaction self-energy and the tunneling matrix for large number of particles. Finally we compare the results of the original four-fermion model with those obtained considering zero interaction, two-fermions and a generalized q-fermion model.
description: 23 pages, no figures
Production of magnetic GFP affinity beads
Creators: name: Nichanok Auevechanichkul
name: Lintermann, Ruth
name: Wirthmueller, Lennart
Publisher: name: figshare
Year: 2019
Subjects: subject: 60199 Biochemistry and Cell Biology not elsewhere classified
subject: FOS: Biological sciences
subject: Plant Biology
subject: Zoology
subject: 60802 Animal Cell and Molecular Biology
subject: Biological Techniques
subject: Cell Biology
subject: Molecular Biology

description: Our protocol for production of 'home-made' magnetic GFP affinity beads using a Camelid a-GFP nanobody. These can be used to immuno-purify GFP- or YFP-tagged proteins from cell extracts.
Principal Process Analysis of dynamic GlucoCEST MRI data
Creators: name: Casagranda, Stefano
name: Pizzolato, Marco
name: Torrealdea, Francisco
name: Golay, Xavier
name: Boutelier, Timothé
Publisher: name: arXiv
Year: 2018
Subjects: subject: Tissues and Organs (q-bio.TO)
subject: FOS: Biological sciences

description: GlucoCEST is an MRI contrast enhancement technique sensitive to the concentration of sugar in the tissue. Because of a differencein metabolism, it is thought that tumors consume more sugar than normal tissue. However, glucose metabolism is complex and depends onmany processes, which are all important to understand the origin of the measured signal. To achieve this goal we apply here a process analysismethod to a deterministic system describing the metabolism of glucose in the tissue.
How Disoriented Chiral Condensates Form: Quenching vs. Annealing
Creators: name: Asakawa, Masayuki
name: Huang, Zheng
name: Wang, Xin-Nian
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We demonstrate that semiclassical fluctuations, their relaxation, and the chiral phase transition are automatically incorporated in the numerical simulations of the classical equations of motion in the linear $σ$-model when longitudinal and transverse expansions are included. We find that domains of disoriented chiral condensate with 4--5 fm in size can form through a quench while an annealing leads to domains of smaller sizes. We also demonstrate that quenching cannot be achieved by relaxing a chirally symmetric system through expansion.
description: 10 pages, 3 uuencoded postscript figures included, REVTEX, LBL-35981. All figures can be printed with any postscript printer. However, Fig. 3 is actually in color and its hard copy is available in color upon request
title: ADCO, Cartulaire de Cîteaux pour les possessions d'Aloxe (XVe siècle), Cart. 182 (11 H 233), 105 folios, f. 0170
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/2017
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge

description: Cartulaire de Cîteaux pour les possessions d'Aloxe (XVe siècle), Archives départementales de la Côte-d'Or, Cart. 182 (11 H 233), 105 folios, f. 0170, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire de Cîteaux pour les possessions d'Aloxe (XVe siècle), Archives départementales de la Côte-d'Or, Cart. 182 (11 H 233), 105 folios, f. 0170, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
description: Provenance: https://www.geonames.org/3024876
Monopole acceleration in intergalactic magnetic fields
Creators: name: Perri, Daniele
name: Bondarenko, Kyrilo
name: Doro, Michele
name: Kobayashi, Takeshi
Publisher: name: arXiv
Year: 2024
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We provide a comprehensive analysis of the acceleration of magnetic monopoles in intergalactic magnetic fields. We demonstrate that monopoles with intermediate to low masses can be accelerated to relativistic velocities. This can significantly affect direct and indirect searches for magnetic monopoles. As an example, we show that the Parker bound is relaxed in the presence of intergalactic fields. We also find that a cosmic population of monopoles can produce significant backreaction on the intergalactic fields.
description: 23 pages, 5 figures
Hyperfine interaction and electronic spin fluctuation study on Sr$_{2-x}$La$_x$FeCoO$_6$ (x = 0, 1, 2) by high-resolution back-scattering neutron spectroscopy
Creators: name: Chatterji, T.
name: Frick, B.
name: Zamponi, M.
name: Appel, M.
name: Nair, H. S.
name: Pradheesh, R.
name: Hariprya, G. R.
name: Sankaranarayanan, V.
name: Sethupathi, K.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: The study of hyperfine interaction by high-resolution inelastic neutron scattering is not very well known compared to the other competing techniques viz. NMR, Mössbauer, PACS etc. Also the study is limited mostly to magnetically ordered systems. Here we report such study on Sr$_{2-x}$La$_x$FeCoO$_6$ (x = 0, 1, 2) of which first (Sr$_2$FeCoO$_6$ with x = 0) has a canonical spin spin glass, the second (SrLaFeCoO$_6$ with x = 1) has a so-called magnetic glass and the third (La$_2$FeCoO$_6$ with x = 2) has a magnetically ordered ground state. Our present study revealed clear inelastic signal for SrLaFeCoO$_6$, possibly also inelastic signal for Sr$_2$FeCoO$_6$ below the spin freezing temperatures $T_{sf}$ but no inelastic signal at all for for the magnetically ordered La$_2$FeCoO$_6$ in the neutron scattering spectra. The broadened inelastic signals observed suggest hyperfine field distribution in the two disordered magnetic glassy systems and no signal for the third compound suggests no or very small hyperfine field at the Co nucleus due to Co electronic moment. For the two magnetic glassy system apart from the hyperfine signal due only to Co, we also observed electronic spin fluctuations probably from both Fe and Co electronic moments. \end{abstract}
D8.1: EOSC Web Portal (initial version)
Creators: name: Hanahoe, Hilary
name: Panelli, Lorenza
Publisher: name: Zenodo
Year: 2017
Subjects: EOSC
Web portals
Websites

description: This document contains a description of the EOSCpilot website, which has been launched in M2, February 2017. The website is available at: www.eoscpilot.eu and it is maintained by the task leaders of subtask 8.2.1, Web portal & Branding, TRUST-IT. The document also outlines the internal web platform and mailing lists, used by the consortium members to communicate and manage project documentation.
Cumulants of QCD Multiplicity Distributions in Small Phase Space Bins
Creators: name: Dremin, I. M.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: It is shown that, as functions of their rank, cumulants of QCD multiplicity distributions in small phase space bins possess the quasi- oscillating behavior similar to that found for them in the total rapidity range. First minimum moves to lower ranks for smaller bins. For the total rapidity range, it moves to higher ranks with energy increase. The running property of the QCD coupling constant is in charge of these effects which can be verified in experiment.
description: 7 pages, no Figs, preprint IP-ASTP-19; FIAN-TD 94/7
Additional file 1 of Effectiveness comparisons of drug therapies for postoperative aneurysmal subarachnoid hemorrhage patients: network meta‑analysis and systematic review
Creators: name: Yu, Wanli
name: Huang, Yizhou
name: Zhang, Xiaolin
name: Luo, Huirong
name: Chen, Weifu
name: Jiang, Yongxiang
name: Cheng, Yuan
Publisher: name: figshare
Year: 2021
Subjects: Space Science
Medicine
Pharmacology
Biotechnology
Science Policy
Mental Health

description: Additional file 1: Figure 1.
Scale Invariant Scattering and Bernoulli Numbers
Creators: name: Curtright, Thomas L.
Publisher: name: arXiv
Year: 2024
Subjects: subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: Non-relativistic quantum mechanical scattering from an inverse square potential in two spatial dimensions leads to a novel representation of the Bernoulli numbers.
Data analysis techniques for stereo IACT systems
Creators: name: Hofmann, W.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Based on data and Monte-Carlo simulations of the HEGRA IACT system, improved analysis techniques were developed for the determination of the shower geometry and shower energy from the multiple Cherenkov images. These techniques allow, e.g., to select subsamples of events with better than 3' angular resolution, which are used to limit the rms radius of the VHE emission region of the Crab Nebula to less than 1.5'. For gamma-rays of the Mrk 501 data sample, the energy can be determined to typically 10% and the core location to 2-3 m.
description: 5 Pages, 3 Figures; Talk given at the TeV Gamma Ray Workshop, Snowbird, 1999
title: ADCO, Grènetier de Cîteaux : comptes (1499-1503) (11 H 1173), f. 00755
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: CBMA/CG21/F.PETOT/2019
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: comptes
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Grènetier de Cîteaux : comptes (1499-1503), Archives départementales de la Côte-d'Or, (11 H 1173). Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Grènetier de Cîteaux : comptes (1499-1503), Archives départementales de la Côte-d'Or, (11 H 1173), f. 00755, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https://manuscrits.cbma-project.eu/
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
description: Provenance: abbaye de Cîteaux
description: Provenance: http://www.wikidata.org/entity/Q843261
Вестник Российского нового университета серия «Человек в современном мире»,Выпуск 2 2021
Creators: name: Автономная некоммерческая организация высшего образования «Российский новый университет»
Publisher: name: Автономная некоммерческая организация высшего образования «Российский новый университет»
Year: 2021

description: Вестник Российского нового университета серия «Человек в современном мире»,Выпуск 2 2021
Current status and desired accuracy of the isotopic production cross sections relevant to astrophysics of cosmic rays I. Li, Be, B, C, N
Creators: name: Genolini, Yoann
name: Maurin, David
name: Moskalenko, Igor V.
name: Unger, Michael
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: High Energy Physics - Experiment (hep-ex)
subject: High Energy Physics - Theory (hep-th)
subject: Nuclear Experiment (nucl-ex)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: The accuracy of the current generation of cosmic-ray (CR) experiments, such as AMS-02, PAMELA, CALET, and ISS-CREAM, is now reaching $\sim$1--3\% in a wide range in energy per nucleon from GeV/n to multi-TeV/n. Their correct interpretation could potentially lead to discoveries of new physics and subtle effects that were unthinkable just a decade ago. However, a major obstacle in doing so is the current uncertainty in the isotopic production cross sections that can be as high as 20--50\% or even larger in some cases. While there is a recently reached consensus in the astrophysics community that new measurements of cross sections are desirable, no attempt to evaluate the importance of particular reaction channels and their required accuracy has been made yet. It is, however, clear that it is a huge work that requires an incremental approach. The goal of this study is to provide the ranking of the isotopic cross sections contributing to the production of the most astrophysically important CR Li, Be, B, C, and N species. In this paper, we (i) rank the reaction channels by their importance for a production of a particular isotope, (ii) provide comparisons plots between the models and data used, and (iii) evaluate a generic beam time necessary to reach a 3\% precision in the production cross-sections pertinent to the AMS-02 experiment. This first roadmap may become a starting point in the planning of new measurement campaigns that could be carried out in several nuclear and/or particle physics facilities around the world. A comprehensive evaluation of other isotopes $Z\leq30$ will be a subject of follow-up studies.
description: 37 pages, many figures and tables. Comments are welcome
Additional file 2 of Effectiveness comparisons of drug therapies for postoperative aneurysmal subarachnoid hemorrhage patients: network meta‑analysis and systematic review
Creators: name: Yu, Wanli
name: Huang, Yizhou
name: Zhang, Xiaolin
name: Luo, Huirong
name: Chen, Weifu
name: Jiang, Yongxiang
name: Cheng, Yuan
Publisher: name: figshare
Year: 2021
Subjects: Space Science
Medicine
Pharmacology
Biotechnology
Science Policy
Mental Health

description: Additional file 2: Figure 2.
Myrmococystus viaticus subsp. abyssinicus Forel, 1904, nov.
Creators: name: Forel, A.
Publisher: name: Zenodo
Year: 1904
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Formicidae
Myrmococystus
Myrmococystus viaticus
Myrmococystus viaticus f. r. abyssinicus

description: Myrmococystus viaticus F. r. abyssinicus nov.
2), [[worker]]. L. 7 a 9,5 mill. Peu dimorphe, a ce qu'il parait. Ressemble a la race megalocola Foerst. Mais il est plus petit, la tete, le thorax et l'ecaille un peu plus luisants, a sculpture plus faible et plus fine, et d'un rouge plus terne, tandis que l'abdomen est au contraire moins luisant, avec une sculpture plus forte, comme celle du reste du corps. Le noeud du pedicule est plus long, distinctement plus long que large. Du reste de la forme du megalocola, dont il a la tete carree, mais un peu plus convexe derriere et plutot plus longue que large, ainsi que les pattes etroites, avec une pubescence adjacente fine et line rangee soies ou piquants obliques et ecartes au bord interne. Pubescence du metanotum plutot faible. Stigmates du mesonotum tres proeminents.
[[queen]]. L. 7 a 8 mill. Etroite et remarquablement petite. La tete est plus etroite que chez la grande [[worker]] et le thorax tres etroit. Du reste comme l'ouvriere. Ailes manquent.
Abyssinie, Ingfal (Kachovskij!). J'ai recu la meme race, avec les deux seules [[worker]] de M. Alfred Ilg, conseiller de S. M. le roi Menelik d'Abyssinie, de Schoa et de l'Abyssinie occidentale.
description: Published as part of Forel, A., 1904, Note sur les fourmis du Musée Zoologique de l'Académie Impériale des Sciences à St. Pétersbourg., pp. 368-388 in Yezhegodnik Zoologicheskogo Muzeya Imperatorskoi Akademii Nauk 8 on page 15, DOI: 10.5281/zenodo.25586
IMPORTANCE OF VERB SUFFIX MAPPING IN DISCOURSE TRANSLATION SYSTEM
Creators: name: Suryakanthi Tangirala
Publisher: name: figshare
Year: 2018
Subjects: subject: 80107 Natural Language Processing
subject: FOS: Computer and information sciences

description: This paper discusses the importance of verb suffix mapping in Discourse translation system. In discourse translation, the crucial step is Anaphora resolution and generation. In Anaphora resolution, cohesion links like pronouns are identified between portions of text. These binders make the text cohesive by referring to nouns appearing in the previous sentences or nouns appearing in sentences after them. In Machine Translation systems, to convert the source language sentences into meaningful target language sentences the verb suffixes should be changed as per the cohesion links identified. This step of translation process is emphasized in the present paper. Specifically, the discussion is on how the verbs change according to the subjects and anaphors. To explain the concept, English is used as the source language (SL) and an Indian language Telugu is used as Target language (TL).
Multimodal Recurrent Neural Networks with Information Transfer Layers for Indoor Scene Labeling
Creators: name: Abdulnabi, Abrar H.
name: Shuai, Bing
name: Zuo, Zhen
name: Chau, Lap-Pui
name: Wang, Gang
Publisher: name: arXiv
Year: 2018
Subjects: subject: Computer Vision and Pattern Recognition (cs.CV)
subject: FOS: Computer and information sciences

description: This paper proposes a new method called Multimodal RNNs for RGB-D scene semantic segmentation. It is optimized to classify image pixels given two input sources: RGB color channels and Depth maps. It simultaneously performs training of two recurrent neural networks (RNNs) that are crossly connected through information transfer layers, which are learnt to adaptively extract relevant cross-modality features. Each RNN model learns its representations from its own previous hidden states and transferred patterns from the other RNNs previous hidden states; thus, both model-specific and crossmodality features are retained. We exploit the structure of quad-directional 2D-RNNs to model the short and long range contextual information in the 2D input image. We carefully designed various baselines to efficiently examine our proposed model structure. We test our Multimodal RNNs method on popular RGB-D benchmarks and show how it outperforms previous methods significantly and achieves competitive results with other state-of-the-art works.
description: 15 pages, 13 figures, IEEE TMM 2017
Fine Tuning in One-Higgs and Two-Higgs Standard Models
Creators: name: Andrianov, A. A.
name: Rodenberg, R.
name: Romanenko, N. V.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The fine-tuning principles are examined to predict the top-quark and Higgs-boson masses. The modification of the Veltman condition based on the compensation of vacuum energies is developed. It is implemented in the Standard Model and in its minimal extension with two Higgs doublets. The top-quark and Higgs-boson couplings are fitted in the SM for the lowest ultraviolet scale where the fine-tuning can be stable under rescaling. It yields the low-energy values $m_t \simeq 175 GeV; m_H \simeq 210 GeV$.
description: 13 pages, LaTeX, Preprint PITHA-94-23 (July 1993)
IN03035 Riṭigala Āṇḍiyā-kanda Cave Inscription 3
Creators: name: Wickremasinghe, Don Martino de Zilva
Publisher: name: Zenodo
Year: 2019
Subjects: IN03035
Epigraphia Zeylanica
Riṭigala
Āṇḍiyā-kanda

description: IN03035 Riṭigala Āṇḍiyā-kanda Cave Inscription 3 - Transcript and Translation Source: Wickremasinghe, Don Martino de Zilva. (1904-12). ‘No. 10. Riṭigala Inscriptions,’ Epigraphia Zeylanica 1, pp. 135-153.
EXACT SOLUTIONS OF A FAMILY OF HIGHER-DIMENSIONAL SPACE-TIME FRACTIONAL KDV-TYPE EQUATIONS
Creators: name: Al-Amr, Mohammed O.
Publisher: name: figshare
Year: 2018
Subjects: Applied Computer Science

description: In this paper, based on the definition of conformable fractional derivative, the functional variable method (FVM) is proposed to seek the exact traveling wave solutions of two higherdimensional space-time fractional KdV-type equations in mathematical physics, namely the (3+1)-dimensional space–time fractional Zakharov-Kuznetsov (ZK) equation and the (2+1)-dimensional space–time fractional Generalized Zakharov-Kuznetsov-Benjamin-Bona-Mahony (GZK-BBM) equation. Some new solutions are procured and depicted. These solutions, which contain kink-shaped, singular kink, bell-shaped soliton, singular soliton and periodic wave solutions, have many potential applications in mathematical physics and engineering. The simplicity and reliability of the proposed method is verified.
Mean-field optimal control as Gamma-limit of finite agent controls
Creators: name: Fornasier, Massimo
name: Lisini, Stefano
name: Orrieri, Carlo
name: Savaré, Giuseppe
Publisher: name: arXiv
Year: 2018
Subjects: subject: Analysis of PDEs (math.AP)
subject: Optimization and Control (math.OC)
subject: FOS: Mathematics

description: This paper focuses on the role of a government of a large population of interacting agents as a mean field optimal control problem derived from deterministic finite agent dynamics. The control problems are constrained by a PDE of continuity-type without diffusion, governing the dynamics of the probability distribution of the agent population. We derive existence of optimal controls in a measure-theoretical setting as natural limits of finite agent optimal controls without any assumption on the regularity of control competitors. In particular, we prove the consistency of mean-field optimal controls with corresponding underlying finite agent ones. The results follow from a $Γ$-convergence argument constructed over the mean-field limit, which stems from leveraging the superposition principle.
Reflection Measurement of the Scattering Mean Free Path at the Onset of Multiple Scattering
Creators: name: Goïcoechea, Antton
name: Brütt, Cécile
name: Ber, Arthur Le
name: Bureau, Flavien
name: Lambert, William
name: Prada, Claire
name: Derode, Arnaud
name: Aubry, Alexandre
Publisher: name: arXiv
Year: 2024
Subjects: subject: Medical Physics (physics.med-ph)
subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: Applied Physics (physics.app-ph)
subject: FOS: Physical sciences

description: Multiple scattering of waves presents challenges for imaging complex media but offers potential for their characterization. Its onset is actually governed by the scattering mean free path $\ell_s$ that provides crucial information on the medium micro-architecture. Here, we introduce a reflection matrix method designed to estimate this parameter from the time decay of the single scattering rate. Our method is first validated by an ultrasound experiment on a tissue-mimicking phantom before being applied in-vivo to a human liver. This study opens important perspectives for quantitative imaging of heterogeneous media with waves, whether it be for non-destructive testing, biomedical or geophysical applications.
description: 29 pages, 7 figures
Light Quark Dependence of the Isgur-Wise Function from QCD Sum rules
Creators: name: Huang, Tao
name: Luo, Chuan-Wang
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We study light quark dependence of the Isgur-Wise function for $B_a\rightarrow D_a$ and $B_a\rightarrow D^{*}_a$ in the framework of QCD sum rules. At zero recoil , all the Isgur-Wise functions equal as required by heavy quark symmetry and at non-zero recoil, the Isgur-Wise function for $B_s$ decay falls faster than that for $B_{u,d}$ decay , which is just contrary to the recent prediction of the heavy meson chiral perturbation theory. As by-products, we also estimate SU(3) breaking effects in the mass and the decay constant.
description: 13 Pages latex, 9 figures available upon request
Implanting germanium into graphene
Creators: name: Tripathi, Mukesh
name: Markevich, Alexander
name: Böttger, Roman
name: Facsko, Stefan
name: Besley, Elena
name: Kotakoski, Jani
name: Susi, Toma
Publisher: name: arXiv
Year: 2018
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Incorporating heteroatoms into the graphene lattice may be used to tailor its electronic, mechanical and chemical properties. Direct substitutions have thus far been limited to incidental Si impurities and P, N and B dopants introduced using low-energy ion implantation. We present here the heaviest impurity to date, namely $^{74}$Ge$^+$ ions implanted into monolayer graphene. Although sample contamination remains an issue, atomic resolution scanning transmission electron microscopy imaging and quantitative image simulations show that Ge can either directly substitute single atoms, bonding to three carbon neighbors in a buckled out-of-plane configuration, or occupy an in-plane position in a divacancy. First principles molecular dynamics provides further atomistic insight into the implantation process, revealing a strong chemical effect that enables implantation below the graphene displacement threshold energy. Our results show that heavy atoms can be implanted into the graphene lattice, pointing a way towards advanced applications such as single-atom catalysis with graphene as the template.
description: 20 pages, 5 figures
Additional file 3 of Effectiveness comparisons of drug therapies for postoperative aneurysmal subarachnoid hemorrhage patients: network meta‑analysis and systematic review
Creators: name: Yu, Wanli
name: Huang, Yizhou
name: Zhang, Xiaolin
name: Luo, Huirong
name: Chen, Weifu
name: Jiang, Yongxiang
name: Cheng, Yuan
Publisher: name: figshare
Year: 2021
Subjects: Space Science
Medicine
Pharmacology
Biotechnology
Science Policy
Mental Health

description: Additional file 3: Figure 3.