cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
GEMINGA'S SOFT X-RAY EMISSION AND THE STRUCTURE OF ITS SURFACE
Creators: name: Page, Dany
name: Shibanov, Yu. A.
name: Zavlin, V. E.
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a model to explain the decrease in the amplitude of the pulse profile with increasing energy observed in Geminga's soft X-ray surface thermal emission. We assume the presence of plates surrounded by a surface with very distinct physical properties: these two regions emit spectra of very distinct shapes which present a crossover, the warm plates emitting a softer spectrum than the colder surrounding surface. The strongly pulsed emission from the plates dominates at low energy while the surroundings emission dominates at high energy, producing naturally a strong decrease in the pulsed fraction. In our illustrative example the plates are assumed to be magnetized while the rest of the surface is field free. This plate structure may be seen as a schematic representation of a continuous but very nonuniform distribution of the surface magnetic field or as a quasi realistic structure induced by past tectonic activity on Geminga.
description: 10 pages, AASTeX latex, + 3 figures (compressed 7 uuencoded). Submitted to Ap. J. Lett
Graphene oxide & reduced graphene oxide polysulfone nanocomposite pellets: An alternative adsorbent of antibiotic pollutant-ciprofloxacin
Creators: name: S. Indherjith
name: S. Karthikeyan
name: J. Helen Ratna Monica
name: Kumar, Karthik Krishna
Publisher: name: Taylor & Francis
Year: 2018
Subjects: subject: Space Science
subject: 29999 Physical Sciences not elsewhere classified
subject: FOS: Physical sciences
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Physiology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Marine Biology
subject: 60506 Virology

description: Efficient nanocomposites, GO-Psf and RGO-Psf has been synthesised from polysulfone and graphene oxide. The synthesised nanomaterials were characterised using contact angle measurements, SEM, TEM, XRD, TGA, DSC, Raman and FT-IR analytical techniques. The reported polymeric nanomaterials are attractive due to their high surface area and thermal stability. The maximum adsorption capacity for ciprofloxacin is 82.781 mg/g and 21.486 mg/g on GO-Psf and RGO-Psf, respectively. The kinetic and adsorption analysis identifies the nanomaterials as attractive adsorbents for removal of antibiotic pollutant, ciprofloxacin from aqueous solution.
Starburst-driven Starbursts in the Heart of Ultraluminous Infrared Galaxies
Creators: name: Taniguchi, Yoshiaki
name: Trentham, Neil
name: Shioya, Yasuhiro
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: There is increasing evidence for the presence of blue super star clusters in the central regions of ultraluminous infrared galaxies like Arp 220. Ultraluminous galaxies are thought to be triggered by galaxy mergers, and it has often been argued that these super star clusters may form during violent collisions between gas clouds in the final phase of the mergers. We now investigate another set of models which differ from previous ones in that the formation of the super star clusters is linked directly to the very intense starburst occurring at the very center of the galaxy. Firstly we show that a scenario in which the super star clusters form in material compressed by shock waves originating from the central starburst is implausible because the objects so produced are much smaller than the observed star clusters in Arp 220. We then investigate a scenario (based on the Shlosman-Noguchi model) in which the infalling dense gas disk is unstable gravitationally and collapses to form massive gaseous clumps. Since these clumps are exposed to the external high pressure driven by the superwind (a blast wave driven by a collective effect of a large number of supernovae in the very core of the galaxy), they can collapse and then massive star formation may be induced in them. The objects produced in this kind of collapse have properties consistent with those of the observed super star clusters in the center of Arp 220.
description: 13 pages, 1 figure, ApJ (Letters) in press
The rapid growth phase of supermassive black holes
Creators: name: McAlpine, Stuart
name: Bower, Richard G.
name: Rosario, David J.
name: Crain, Robert A.
name: Schaye, Joop
name: Theuns, Tom
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We investigate the rapid growth phase of supermassive black holes (BHs) within the hydrodynamical cosmological \eagle simulation. This non-linear phase of BH growth occurs within $\sim$$L_{*}$ galaxies, embedded between two regulatory states of the galaxy host: in sub $L_{*}$ galaxies efficient stellar feedback regulates the gas inflow onto the galaxy and significantly reduces the growth of the central BH, while in galaxies more massive than $L_{*}$ efficient AGN feedback regulates the gas inflow onto the galaxy and curbs further non-linear BH growth. We find evolving critical galaxy and halo mass scales at which rapid BH growth begins. Galaxies in the low-redshift Universe transition into the rapid BH growth phase in haloes that are approximately an order of magnitude more massive than their high-redshift counterparts (\M{200} $\approx 10^{12.4}$~\Msol at $z \approx 0$ decreasing to \M{200} $\approx 10^{11.2}$~\Msol at $z \approx 6$). Instead, BHs enter the rapid growth phase at a fixed critical halo virial temperature ($T_{\mathrm{vir}} \approx 10^{5.6}$~K). We additionally show that major galaxy--galaxy interactions ($μ\geq \frac{1}{4}$, where $μ$ is the stellar mass ratio) play a substantial role in triggering the rapid growth phase of BHs in the low-redshift Universe, whilst potentially having a lower influence at high redshift. Approximately 40\% of BHs that initiate the rapid BH growth phase at $z \approx 0$ do so within $\pm 0.5$ dynamical times of a major galaxy--galaxy merger, a fourfold increase above what is expected from the background merger rate. We find that minor mergers ($\frac{1}{10} \leq μ< \frac{1}{4}$) have a substantially lower influence in triggering the rapid growth phase at all epochs.
description: 12 pages, 8 figures, accepted to MNRAS
LYMAN-ALPHA FOREST CORRELATIONS USING NEIGHBOR COUNTS
Creators: name: Meiksin, Avery
name: Bouchet, Francois R.
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a novel technique for calculating the two-point autocorrelation function of the Lyman-alpha forest based on the relation between the two-point correlation function and the Neighbor Probability Distribution Functions. The technique appears to reduce the scatter in estimates of the correlation function by a factor of about two from the traditional pair-counting method. We apply the technique to the Lyman-alpha forest line lists determined from the spectra of seven z > 2 QSOs observed at high resolution ( < 25 km/s ). Of these, only two spectra, those of Q0055-259 and Q0014+813, appear to be sufficiently free of systematics to obtain meaningful estimates of the correlation function. We find positive correlations, with a maximum amplitude of 0.5 - 1, on the scale of 0.5 - 3 h^{-1} Mpc (comoving), or 100 - 600 km/s, in the forests of both QSOs. The technique also finds strong evidence for anticorrelation on the scale of 3 - 6 h^{-1} Mpc. The strength of the positive correlations is comparable to that predicted from the primordial power spectrum inferred from optically-selected galaxy redshift surveys. If the anticorrelations are physical, it becomes unclear whether the detected clustering is consistent with current models of structure formation with a homogeneous photoionizing UV metagalactic background. Instead, the anti-clustering may require inhomogeneity in the UV background, and possibly in the process of reionization itself.
description: 18 pages, uuencoded, compressed, postscript, figures included. To appear in the Astrophysical Journal Letters
Microlensing of Extended Stellar Sources
Creators: name: Hendry, M. A.
name: Coleman, I. J.
name: Gray, N.
name: Newsam, A. M.
name: Simmons, J. F. L.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We investigate the feasibility of reconstructing the radial intensity profile of extended stellar sources by inverting their microlensed light curves. Using a simple, linear, limb darkening law as an illustration, we show that the intensity profile can be accurately determined, at least over the outer part of the stellar disc, with realistic light curve sampling and photometric errors. The principal requirement is that the impact parameter of the lens be less than or equal to the stellar radius. Thus, the analysis of microlensing events provides a powerful method for testing stellar atmosphere models.
description: 4 pages LaTeX, to appear in New Astronomy Reviews - proceedings of the Oxford Workshop `Gravitational Lensing: Nature's Own Weighing Scales'. Uses elsart.cls. Paper also available at ftp://info.astro.gla.ac.uk/pub/martin/extended.ps
The structure of near stoichiometric Ge-Ga-Sb-S glasses: a reverse Monte Carlo study
Creators: name: Pethes, Ildikó
name: Nazabal, Virginie
name: Chahal, Radwan
name: Bureau, Bruno
name: Kaban, Ivan
name: Beuneu, Brigitte
name: Bednarcik, Jozef
name: Jóvári, Pál
Publisher: name: arXiv
Year: 2018
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: Chemical Physics (physics.chem-ph)
subject: FOS: Physical sciences

description: The structure of Ge$_{22}$Ga$_3$Sb$_{10}$S$_{65}$ and Ge$_{15}$Ga$_{10}$Sb$_{10}$S$_{65}$ glasses was investigated by neutron diffraction (ND), X-ray diffraction (XRD), and extended X-ray absorption fine structure (EXAFS) measurements at the Ge, Ga and Sb K-edges. Experimental data sets were fitted simultaneously in the framework of the reverse Monte Carlo (RMC) simulation technique. Short range order parameters were determined from the obtained large-scale configurations. It was found that the coordination numbers of Ge, Sb and S are around the values predicted by the Mott-rule (4, 3 and 2, respectively). The Ga atoms have on average 4 nearest neighbors. The structure of these stoichiometric glasses can be described by the chemically ordered network model: Ge-S, Ga-S and Sb-S bonds are the most important. Long Sb-S distances (0.3 - 0.4 Å higher than the usual covalent bond lengths) are observed, suggesting that Sb atoms can be found in various local environments.
description: 27 pages, 7 figures
Poly(ethylenimine) functionalized magnetic nanoparticles for sorption of Pb, Cu, and Ni: potential application in catalysis
Creators: name: Rathod, Prakash Baburao
name: Sankararao Chappa
name: K. S. Ajish Kumar
name: Pandey, Ashok K.
name: Athawale, Anjali Anand
Publisher: name: Taylor & Francis
Year: 2018
Subjects: subject: Biophysics
subject: Biochemistry
subject: Space Science
subject: 29999 Physical Sciences not elsewhere classified
subject: FOS: Physical sciences
subject: Biotechnology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Inorganic Chemistry
subject: 60506 Virology
subject: FOS: Biological sciences

description: The poly(ethylenimine) functionalized magnetite particles were studied for their preconcentration efficiencies toward Cu2+, Pb2+, and Ni2+ ions. The loading capacities were found to be 26 mg g−1, 46 mg g−1, and 13 mg g−1 of Cu2+, Pb2+, and Ni2+ ions, respectively. Cu2+ ions loaded on the magnetically retrievable nanoparticles were used for Henry reaction as a representative example of a heterogeneous catalyst. These particles were characterized for their chemical, physical, thermal and magnetic properties. The Henry reaction involved reaction between m-nitro benzaldehyde and nitromethane to afford the nitroaldol adducts 1-(3-nitrophenyl)-2-nitrosoethanol with 80% yield in ethanol at room temperature.
Maximal Subvacuum Effects: A Single Mode Example
Creators: name: Korolov, Anastasia
name: Ford, L. H.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Quantum Physics (quant-ph)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We discuss an example of a subvacuum effect, where a quantum expectation value is below the vacuum level, and is hence negative. The example is the time average of the mean squared electric field in a non-classical state where one mode is excited. We give some specific examples of such states, and discuss the lower bound on the squared field or its time average. We show when a lower bound can be obtained by diagonalization of the squared electric field operator, and calculate this bound. We also discuss the case of an instant time mean squared electric field, when the operator cannot be diagonalized. In this case, a lower bound still exists but is attained only by the limit of a sequence of quantum states. In general, the optimum lower bound on the mean squared electric field is minus one-half of the mean squared electric field in a one photon state. This provides a convenient estimate of the subvacuum effect, and may be useful for attempts to experimentally measure this effect.
description: 17 pages, 3 figures; expanded version, with more discussion and a new section on the physical interpretation of the results
A chemical alternative to phosphospecific antibodies
Creators: name: Murray, James Ian
Publisher: name: Imperial College London
Year: 2016

description: Signal transduction cascades in living systems are commonly controlled via posttranslational phosphorylation and dephosphorylation of proteins. These processes are catalyzed and controlled in vivo by the action of kinase and phosphatase enzymes, which consequently play an important role in many disease states, including cancer and immune system disorders. Current techniques for phosphoproteome analysis (using isotopic labelling, chromatographic purification and phosphospecific antibodies) are undoubtedly very powerful, however, these approaches have yet to provide a generally applicable tool for phosphoproteome analysis despite the widespread utility such a technique would have. The use of small molecule organic catalysts capable of promoting selective phosphate esterification would provide an extremely useful alternative to these current techniques for use in, e.g. the labelling and pull-down of phosphorylated proteins. This thesis describes the development of aryl-N-oxide catalysts capable of promoting site selective phosphorylation of polyol and peptide derivatives. Whilst, ultimately, it was shown that these catalysts are not optimal for achieving selective phosphate esterification in biological systems, an alternate synthetic tool for phosphoproteomic analysis was developed. Progress in the development of this pyrophosphorylate, eliminate, tag (pPET) strategy and its current applications are discussed.
Davis-Greenstein alignment of non-spherical grains
Creators: name: Lazarian, A.
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Paramagnetic alignment of non-spherical dust grains rotating at thermal velocities is studied. The analytical solution is found for the alignment measure of oblate grains. Perturbative approach is used for solving the problem. It is shown that even the first approximation of the suggested iteration procedure provides the accuracy well within one percent of the expected measure of alignment. The results obtained are applicable both to paramagnetic and to superferromagnetic grains.
description: 20 pages, uuencoded Postcript, accepted to ApJ
title: ADCO, Cartulaire de l'office de la Porte de l'abbaye de Cîteaux, Registrum possessionum porte Cistercii (début XVe siècle), Cart. 172 (11 H 69), 115 folios, f. 0181
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/2012
name: Petot, Frédéric
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Cartulaire de l'office de la Porte de l'abbaye de Cîteaux, Registrum possessionum porte Cistercii (début XVe siècle), Archives départementales de la Côte-d'Or, Cart. 172 (11 H 69), 115 folios, f. 0181, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire de l'office de la Porte de l'abbaye de Cîteaux, Registrum possessionum porte Cistercii (début XVe siècle), Archives départementales de la Côte-d'Or, Cart. 172 (11 H 69), 115 folios, f. 0181, 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
Rumex persicarioides Linnaeus, 1753, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1753
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Polygonales
Polygonaceae
Rumex
Rumex persicarioides

description: Rumex persicarioides, spec. nov.
7. Rumex floribus hermaphroditis: valvulis dentatis: omnibus graniferis, foliis lanceolatis.
 Habitat in Virginia . ☉
 Planta spithamaea, ramosissima. Folia lanceolata, petiolata, laevia, undata, integra: Floris valvulae dentibus utrinque tribus longis, omnes tectae granis pallidis magnis.
description: Published as part of Linnaeus, Carolus, 1753, Species plantarum: exhibentes plantas rite cognitas, ad genera relatas, cum differentiis specificis, nominibus trivialibus, synonymis selectis, locis natalibus, secundum systema sexuale digestas, Stockholm :Laurentius Salvius on page 335, DOI: 10.5281/zenodo.3931989
Rumex maritimus var. persicarioides Linnaeus 1753
Creators: name: Jarvis, Charlie
Publisher: name: Linnaean Society of London in association with the Natural History Museum
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Polygonales
Polygonaceae
Rumex
Rumex maritimus
Rumex maritimus l. var. persicarioides (l.) r.s. mitch.

description: Rumex persicarioides Linnaeus, Species Plantarum 1: 335. 1753.
"Habitat in Virginia." RCN: 2582.
Lectotype (St John in Rhodora 17: 74. 1915): Kalm, Herb. Linn. No. 464.9 (LINN).
Current name: Rumex maritimus L. var. persicarioides (L.) R.S. Mitch. (Polygonaceae).
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part R), pp. 785-805 in Order out of Chaos. Linnaean Plant Types and their Types, London :Linnaean Society of London in association with the Natural History Museum on page 804, DOI: 10.5281/zenodo.291971
The Reclassification of Asteroids from Planets to Non-Planets
Creators: name: Metzger, Philip T.
name: Sykes, Mark V.
name: Stern, Alan
name: Runyon, Kirby
Publisher: name: arXiv
Year: 2018
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: History and Philosophy of Physics (physics.hist-ph)
subject: Popular Physics (physics.pop-ph)
subject: FOS: Physical sciences

description: It is often claimed that asteroids' sharing of orbits is the reason they were re-classified from planets to non-planets. A critical review of the literature from the 19th Century to the present shows this is factually incorrect. The literature shows the term asteroid was broadly recognized as a subset of planet for 150 years. On-going discovery of asteroids resulted in a de facto stretching of the concept of planet to include the ever-smaller bodies. Scientists found utility in this taxonomic identification as it provided categories needed to argue for the leading hypothesis of planet formation, Laplace's nebular hypothesis. In the 1950s, developments in planet formation theory found it no longer useful to maintain taxonomic identification between asteroids and planets, Ceres being the primary exception. At approximately the same time, there was a flood of publications on the geophysical nature of asteroids showing them to be geophysically different than the large planets. This is when the terminology in asteroid publications calling them planets abruptly plunged from a high level of usage where it had hovered during the period 1801 - 1957 to a low level that held constant thereafter. This marks the point where the community effectively formed consensus that asteroids should be taxonomically distinct from planets. The evidence demonstrates this consensus formed on the basis of geophysical differences between asteroids and planets, not the sharing of orbits. We suggest attempts to build consensus around planetary taxonomy not rely on the non-scientific process of voting, but rather through precedent set in scientific literature and discourse, by which perspectives evolve with additional observations and information, just as they did in the case of asteroids.
description: 31 pages, 5 figures
Learning and Generalizing Motion Primitives from Driving Data for Path-Tracking Applications
Creators: name: Wang, Boyang
name: Li, Zirui
name: Gong, Jianwei
name: Liu, Yidi
name: Chen, Huiyan
name: Lu, Chao
Publisher: name: arXiv
Year: 2018
Subjects: subject: Machine Learning (cs.LG)
subject: Machine Learning (stat.ML)
subject: FOS: Computer and information sciences

description: Considering the driving habits which are learned from the naturalistic driving data in the path-tracking system can significantly improve the acceptance of intelligent vehicles. Therefore, the goal of this paper is to generate the prediction results of lateral commands with confidence regions according to the reference based on the learned motion primitives. We present a two-level structure for learning and generalizing motion primitives through demonstrations. The lower-level motion primitives are generated under the path segmentation and clustering layer in the upper-level. The Gaussian Mixture Model(GMM) is utilized to represent the primitives and Gaussian Mixture Regression (GMR) is selected to generalize the motion primitives. We show how the upper-level can help to improve the prediction accuracy and evaluate the influence of different time scales and the number of Gaussian components. The model is trained and validated by using the driving data collected from the Beijing Institute of Technology (BIT) intelligent vehicle platform. Experiment results show that the proposed method can extract the motion primitives from the driving data and predict the future lateral control commands with high accuracy.
description: 2018 IEEE Intelligent Vehicles Symposium (IV)
QUANTIFYING INDIGENOUS KNOWLEDGE: A RAPID METHOD FOR ASSESSING CROP PERFORMANCE WITHOUT FIELD TRIALS
Creators: name: Villiers, Anne
name: Villiers, Anne
Publisher: name: Unknown
Year: 1996
Subjects: Crop Production/Industries

description: This paper describes the development and use of a methodology for quantifying indigenous technical knowledge. Matrix ranking is adapted and used in systematic interviews with experienced farmers to generate numerical data on crop performance. Data sets compiled from a number of interviews are then subjected to statistical analysis. This enables hypotheses to be tested and agronomic parameters to be quantified without field trials. The methodology was developed to complement on-farm and station research. It may also have potential as an alternative to field trials because it provides information that is directly relevant to the farm situation at afar lower cost than field trials. This is particularly true for perennial crops, as conventional trials for these may take many years to yield data. Though the methodology has only been tested in the field of agronomy, the concept may have wider applications in a number of other disciplines in which indigenous technical knowledge is important in the research and development process. The paper therefore comments on both the risks and the potential of using the methodology.
Probability Distribution of the Hubble Constant and the Age of the Universe Inferred from the Local Observation
Creators: name: Nakamura, T.
name: Suto, Y.
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a method to compute the probability distribution function of the (true) Hubble constant and the age of the universe, given the estimate of the Hubble constant in our nearby galaxy samples. Our method takes into account both the observational errors and the cosmic variance, and enables to quantitatively compute the constraints on the cosmological models. Based on the present local observation $H_0=80\pm17$ km/s/Mpc, the probability of $H_0<50$ km/s/Mpc is about 6\% for the Einstein -- de Sitter universe ($Ω_0=1$) and 4\% for an open ($Ω_0=0.2$) universe. These probabilities are reduced to 0.8\% and 0.03\%, respectively, if the accuracy of the observational uncertainty is improved within 10\%. Similar probabilistic constraints on $t_0$ are also discussed.
description: 8 pages, 3 figures (uuencoded postscript)
Charm-strange meson production in ultra-relativistic heavy-ion collisions at the CERN-LHC energies
Creators: name: Li, Shuang
name: Wang, Chaowen
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The nuclear modification factor ${R}_{\rm AA}$ and the elliptic flow coefficient ${v}_{\rm 2}$ of charm-strange meson $D^{+}_{s}$ is systematically studied in Pb--Pb collisions at $\sqrt{s_{\rm NN}}=5.02~{\rm TeV}$ and $2.76~{\rm TeV}$. During the modeling, the coupling strength between the injected charm quark and the incident medium constituents, is extracted from the lattice QCD calculations: $2πTD_{s}=7$ (\textbf{Model-A}) and $2πTD_{s}=1.3 + (T/T_{c})^2$ (\textbf{Model-B}). We find that, comparing ${R}_{\rm AA}(D^{+}_{s})$ with ${R}_{\rm AA}(non-strange)$, the heavy-light coalescence effect is more pronounced for the former one, resulting in an enhancement behavior in the range $2\lesssim {p}_{\rm T}\lesssim5~{\rm GeV}$. The predictions of ${R}_{\rm AA}(D^{+}_{s})$ and ${R}_{\rm AA}(non-strange)$ favor Model-A to have a better description of the measured ${p}_{\rm T}$ dependence in both energies, while their ${v}_{\rm 2}$ prefer Model-B at moderate ${p}_{\rm T}$ ($2\lesssim {p}_{\rm T}\lesssim4~{\rm GeV}$). Therefore, it is necessary to consider the temperature- and/or momentum-dependence of $2πTD_{s}$ to describe simultaneously ${R}_{\rm AA}(D^{+}_{s})$ and ${v}_{\rm 2}(D^{+}_{s})$ in different centrality classes in Pb--Pb collisions.
description: 8 pages, 8 figures; Accepted by Phys. Rev. C
EQUILIBRIUM WITH INCOMPLETE MARKETS OVER AN INFINITE HORIZON
Creators: name: Magill, Michael
name: Quinaii, Martinc
name: Magill, Michael
name: Quinaii, Martinc
Publisher: name: Unknown
Year: 1993
Subjects: Research Methods/ Statistical Methods

description: This paper shows how the general equilibrium model with incomplete markets (GEI) can be extended to an open-ended future, thereby providing a natural setting for analyzing problems in macroeconomics. To obtain a concept of equilibrium which respects the incompleteness of markets and ensures that agents' plans are node consistent, a transversality condition must be imposed on ever3r subtree. Conditions for the existence of an equilibrium as well as certain properties of an equilibrium are derived. The prices of infinite-lived securities in zero net supply are shown to permit speculative bubbles which affect (do not affect) the equilibrium allocation if markets are incomplete (complete). The prices of securities in positive net supply (for example equity contracts) cannot have speculative bubbles, thus limiting the extent of speculation in the GET model.
Search for the Higgs boson produced in association with a vector boson and decaying into two spin-zero particles in the $H \rightarrow aa \rightarrow 4b$ channel in $pp$ collisions at $\sqrt{s} = 13$ TeV with the ATLAS detector
Creators: name: ATLAS Collaboration
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: A search for exotic decays of the Higgs boson into a pair of spin-zero particles, $H \rightarrow aa$, where the $a$-boson decays into $b$-quarks promptly or with a mean proper lifetime $cτ_a$ up to 6 mm and has a mass in the range of $20-60$ GeV, is presented. The search is performed in events where the Higgs boson is produced in association with a $W$ or $Z$ boson, giving rise to a signature of one or two charged leptons (electrons or muons) and multiple jets from $b$-quark decays. The analysis is based on the dataset of proton-proton collisions at $\sqrt{s} = 13$ TeV recorded in 2015 and 2016 by the ATLAS detector at the CERN Large Hadron Collider, corresponding to an integrated luminosity of 36.1 fb$^{-1}$. No significant excess of events above the Standard Model background prediction is observed, and 95% confidence-level upper limits are derived for the production cross-sections for $pp \rightarrow WH$, $ZH$ and their combination, times the branching ratio of the decay chain $H \rightarrow aa \rightarrow 4b$. For $a$-bosons which decay promptly, the upper limit on the combination of cross-sections for $WH$ and $ZH$ times the branching ratio of $H \rightarrow aa \rightarrow 4b$ ranges from 3.0 pb for $m_a= 20$ GeV to 1.3 pb for $m_a = 60$ GeV, assuming that the ratio of $WH$ to $ZH$ cross-sections follows the Standard Model prediction. For $a$-bosons with longer proper lifetimes, the most stringent limits are 1.8 pb and 0.6 pb, respectively, at $cτ_a \sim 0.4$ mm.
description: 48 pages in total, author list starting page 32, 10 figures, 5 tables, final version published in JHEP. All figures including auxiliary figures are available at https://atlas.web.cern.ch/Atlas/GROUPS/PHYSICS/PAPERS/HIGG-2017-05/
Rumex pulcher Linnaeus, 1753, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1753
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Polygonales
Polygonaceae
Rumex
Rumex pulcher

description: Rumex pulcher, spec. nov.
 12. Rumex floribus hermaphroditis, foliis lyratis. Guett. stamp. 1. p.7.
 Lapathum ramis procumbentibus, seminis involucro dentato, foliis inferioribus instar fidium. Moris. hist.2. p.580.
 Lapathum pulchrum bononiense sinuatum. Bauh. hist. 2. p. 988. Raj. hist.1. p.174.
 Habitat in Gallia , Italia , Veronae .
description: Published as part of Linnaeus, Carolus, 1753, Species plantarum: exhibentes plantas rite cognitas, ad genera relatas, cum differentiis specificis, nominibus trivialibus, synonymis selectis, locis natalibus, secundum systema sexuale digestas, Stockholm :Laurentius Salvius on page 336, DOI: 10.5281/zenodo.3931989
Rumex pulcher subsp. pulcher Linnaeus 1753
Creators: name: Jarvis, Charlie
Publisher: name: Linnaean Society of London in association with the Natural History Museum
Year: 2007
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Polygonales
Polygonaceae
Rumex
Rumex pulcher
Rumex pulcher l. subsp. pulcher

description: Rumex pulcher Linnaeus, Species Plantarum 1: 336. 1753.
"Habitat in Gallia, Italia, Veronae." RCN: 2589.
Lectotype (Siddiqi & El-Taife in Jafri & El-Gadi, Fl. Libya 106: 14. 1983): Herb. Linn. No. 464.19 (LINN).
Current name: Rumex pulcher L. subsp. pulcher (Polygonaceae).
description: Published as part of Jarvis, Charlie, 2007, Chapter 7: Linnaean Plant Names and their Types (part R), pp. 785-805 in Order out of Chaos. Linnaean Plant Types and their Types, London :Linnaean Society of London in association with the Natural History Museum on page 804, DOI: 10.5281/zenodo.291971
Asymptotics to all orders of the Euler--Darboux equation in a triangle
Creators: name: Mauersberger, Julian
Publisher: name: arXiv
Year: 2018
Subjects: subject: Mathematical Physics (math-ph)
subject: Analysis of PDEs (math.AP)
subject: FOS: Physical sciences
subject: FOS: Mathematics
subject: 35Q75, 41A60, 83C35

description: In Einstein's theory of relativity, the interaction of two collinearly polarized plane gravitational waves can be described by a Goursat problem for the Euler--Darboux equation in a triangular domain. In this paper, using a representation of the solution in terms of Abel integrals, we give a full asymptotic expansion of the solution near the diagonal of the triangle. The expansion is related to the formation of a curvature singularity of the spacetime. In particular, our framework allows for boundary data with derivatives which are singular at the corners. This level of generality is crucial for the application to gravitational waves.
description: 16 pages
Interpreting New Data on Large Scale Bulk Flows
Creators: name: Watkins, Richard
name: Feldman, Hume A.
Publisher: name: arXiv
Year: 1995
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We study the implications of a recent estimate of the bulk flow of a sample of galaxies containing supernovae type Ia by Riess, Press, and Kirshner. We find that their results are quite consistent with power spectra from several currently popular models of structure formation, but that the sample is as yet too sparse to put significant constraints on the power spectrum. We compare this new result with that of Lauer and Postman, with which there is apparent disagreement. We find that for the power spectra we consider, the difference in window functions between the two samples used for the measurements results in a low level of expected correlation between the estimated bulk flows. We calculate a $χ^2$ for the two measurements taken together and find that their lack of agreement tends to disfavor spectra with excessive power on large scales, but not at a level sufficient to rule them out. A sample consisting of other SN type Ia's found in the Asiago catalog is used to study how the sensitivity of the method used by RPK will improve with increasing sample size. We conclude that the local group motion should be able to be determined with a sample of $\sim 100$ SN Ia light curve shapes.
description: 13 pages, 2 figures included in a self-unpacking uudecoded gzipped postscript file. We changed some of the power spectra analyzed and expanded the discussion. The postscript file is available at http://pupgga.princeton.edu/disk20/anonymous/feldman/bflows.ps
Electrophysiological And Behavioural Correlates Of Motivation And Choice In A Simple Visually Guided Task
Creators: name: Berditchevskaia, Aleksandra
Publisher: name: Imperial College London
Year: 2015

description: Motivation is a fundamental driving force in animal behaviour. As such, it is vital that we are aware of its influence in shaping the behaviour examined in a laboratory setting. We set out to explore how changes in motivation affected the performance of a simple visual task using both behavioural analyses and multi-unit recordings in primary visual cortex (V1) of behaving mice. To address the question we trained water-restricted mice to selectively lick for a water reward during a ‘Go’ stimulus in a Go/NoGo version of a two-category discrimination. This simple paradigm is widely used across the neuroscience community due its relative ease of implementation. On the level of behavioural analysis we show that depending on motivation, performance of the task is reliant on a balance of different behavioural processes. Specifically, we demonstrate the novel result that in a state of overmotivation, goal-directed instrumental contingencies are ‘masked’ while Pavlovian processes dominate over action selection. Secondly, we investigated the multi-unit neural correlates of a simple visual discrimination task recorded in V1. We hypothesized that the typical changes to motivational state within a behavioural session would affect sensory processing, and that the neural signature of this effect could be found in V1. Our choice of time frame for the focus of our analysis brings valuable insights to an increasingly encountered behavioural paradigm. Furthermore, we show novel evidence of temporally specific correlates of motivation and choice behaviour in mouse V1. The recent shift to experiments using head-fixed, behaving rodents by many neurophysiologists makes a thorough understanding of underlying processes paramount. Exploring the boundary between intentional choices and overt interference by motivational states cannot be underestimated. Throughout this work we aim to incorporate existing behavioural psychology literature within the context of modern neuroscience approaches; thus providing a valuable resource for both of these communities.
title: Retrofitted building skins – Energetische Optimierung der Gebäudehülle im Bestand
title: Retrofitted building skins – energetic optimization of the building envelope of existing buildings
titleType: AlternativeTitle
Creators: name: Albus, Jutta
name: Rehnig, Lena
Publisher: name: TU Dortmund
Year: 2022
Subjects: subject: Klimaschutzziele der Bundesregierung
subject: Gebäudehülle von Bestandsgebäuden
subject: energetische Optimierungsstrategien
subject: Federal Government's Climate Action Programme
subject: building envelope of existing buildings
subject: energetic optimization strategies
subject: 690
subject: 720

description: Um das Klimaziel der Bundesregierung zu erreichen, gilt die energetische Optimierung im Gebäudesektor als eine übergeordnete Aufgabe, die nicht nur die Erstellung neuer Gebäude, sondern auch die Ertüchtigung des Gebäudebestands betrifft. Gegenstand der Forschungs- und Lehrtätigkeiten des Lehrgebiets bilden Entwurfsentwicklungen, die durch innovative Gebäudehüllen und Fassadentechnologien einen nachhaltigen und ressourcenschonenden Beitrag auch für den hohen Anteil von Bestandsgebäuden leisten. Sanierungs- und Instandhaltungsmaßnahmen werden vor dem Hintergrund energetischer Optimierungsstrategien, nachhaltiger Gebäudekonzeption und ressourcenschonendem Materialeinsatz entwickelt und fokussieren dabei aktive und passive Maßnahmen. Dabei soll insbesondere der Anteil von bestehenden Büro- und Verwaltungsbauten betrachtet werden, der neben dem Wohngebäudebestand ein erhebliches Potential zur Reduzierung von CO2-Emissionen aufzeigt.
description: In order to adapt to the Federal Government's Climate Action Programme, energy optimization in the building sector is considered an important task that not only affects the construction of new buildings, but also the renovation of existing building stock. The research and teaching activities of the junior professorship focus on architectural design developments that follow sustainable and resource-saving parameters by implementing innovative building skins and facade technologies to improve the energetic building performance. Renovation and maintenance methods are developed against the background of energy optimization strategies, sustainable building design and resource-efficient use of materials, focusing on the implementation of active and passive measures. This paper emphasizes the proportion of existing office and administrative buildings, which, in addition to the residential building stock, have considerable potential to reduce CO2 emissions.
description: ce/papers;5(1)
Non-Identical Neutron Star Twins
Creators: name: Glendenning, Norman K.
name: Kettner, Christiane
Publisher: name: arXiv
Year: 1998
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The work of J. A. Wheeler in the mid 1960's showed that for smooth equations of state no stable stellar configurations with central densities above that corresponding to the limiting mass of ``neutron stars'' (in the generic sense) were stable against acoustical vibrational modes. A perturbation would cause any such star to collapse to a black hole or explode. Accordingly, there has been no reason to expect that a stable degenerate family of stars with higher density than the known white dwarfs and neutron stars might exist. We have found a class of exceptions corresponding to certain equations of state that describe a first order phase transition. We discuss how such a higher density family of stars could be formed in nature, and how the promising new exploration of oscillations in the X-ray brightness of accreting neutron stars might provide a means of identifying them. Our proof of the possible existence of a third family of degenerate stars is one of principle and rests on general principles like causality, microstability of matter and General Relativity.
description: 4 pages, 3 figures, Revtex, (Revised to make clearer that in principle three families of compact stars, white dwarfs, neutron stars, and their `twins', are allowed by GR and general constraints on the equation of state, namely, causality and microstability.)
MPEC 2025-G101 : 2025 GD1
Creators: name: Minor Planet Center Staff
Publisher: name: The Minor Planet Center
Year: 2025
Subjects: subject: Small Solar System bodies
valueUri: http://astrothesaurus.org/uat/1469
subject: 2025 GD1

description: The Minor Planet Electronic Circulars contain information on unusual minor planets, routine data on comets and natural satellites, and occasional editorial announcements.  They are published on behalf of Division F of the International Astronomical Union by the Minor Planet Center, Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A.
Appendix 5 to "The Status of Biological Invasions and their Management in South Africa in 2022"—Pathways change tracker
Creators: name: SANBI
name: CIB
Publisher: name: Zenodo
Year: 2024

description: SANBI and CIB 2023. Appendix 5 to "The Status of Biological Invasions and their Management in South Africa in 2022"—Pathways change tracker. South African National Biodiversity Institute, Kirstenbosch and DSI-NRF Centre of Excellence for Invasion Biology, Stellenbosch. http://dx.doi.org/10.5281/zenodo.8217224

 

For more details see: http://iasreport.sanbi.org.za
For the report itself see: http://dx.doi.org/10.5281/zenodo.8217182
title: ADCO, Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Cart. 32 (G 136), 745 folios, f. 0292
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/2012
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: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire

description: Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Archives départementales de la Côte-d'Or, Cart. 32 (G 136), 745 folios, f. 0292, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Archives départementales de la Côte-d'Or, Cart. 32 (G 136), 745 folios, f. 0292, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: abbaye Saint-Étienne de Dijon
description: Provenance: http://www.wikidata.org/entity/Q15945019
ADMA metabolism and chronic hypoxia-induced pulmonary hypertenstion
Creators: name: Iannone, Lucio
Publisher: name: Imperial College London
Year: 2014

description: Rationale: Elevated asymmetric dimethylarginine (ADMA) levels contribute to the pathogenesis of hypoxia-induced pulmonary hypertension. Chronic hypoxia decreases the activity of the enzymes metabolising ADMA, dimethylarginine dimethylaminohydrolases (DDAH1 and DDAH2) but the mechanisms responsible are not understood. Objective: To elucidate the physiological significance and the mechanism of hypoxia-induced downregulation of ADMA metabolism. Methods and Results: Exposure of human pulmonary artery endothelial cells (HPAECs) to hypoxia inhibited both DDAH1 and DDAH2 gene and protein expression, reduced DDAH activity and increased ADMA levels. In contrast, in human pulmonary artery smooth muscle cells (HPASMCs) only DDAH2 was reduced while ADMA levels remained unchanged. This endothelium-specific regulation of DDAH1 and ADMA resulted from NFκB-dependent, microRNA-21 (miR-21)-mediated degradation of DDAH1 mRNA. Down regulation of DDAH1 activity contributed to hypoxia-induced endothelial barrier dysfunction and HPASMC proliferation and was prevented by overexpression of DDAH1 and miR-21 blockade. Conversely, overexpression of miR-21 mimicked the effects of hypoxia. DDAH1 overexpressing transgenic mice exposed to 2 weeks hypoxia, showed attenuated pulmonary hypertension and vascular remodelling, compared with wildtype controls. Importantly, inhibition of miR21 in vivo prevented the hypoxia-induced reduction in pulmonary DDAH1 expression and attenuated the development of pulmonary hypertension. Lung tissue samples from hypoxic mice and treatment-naïve IPAH patients also showed reduced DDAH1 expression and increased miR-21 levels, compared with controls. Conclusion: Down regulation of DDAH1 expression by miR-21 in the pulmonary vascular endothelium has a key role in the pathogenesis of hypoxia-induced pulmonary hypertension and may be of broader significance in pulmonary hypertension.
Appendix 5 to "The Status of Biological Invasions and their Management in South Africa in 2022 [FIRST DRAFT FOR PUBLIC COMMENT]"—Pathways change tracker
Creators: name: SANBI
name: CIB
Publisher: name: Zenodo
Year: 2022

description: For more details see: http://iasreport.sanbi.org.za SANBI and CIB 2020. Appendix 5 to "The Status of Biological Invasions and their Management in South Africa in 2022 [FIRST DRAFT FOR PUBLIC COMMENT]"—Pathways change tracker. South African National Biodiversity Institute, Kirstenbosch and DSI-NRF Centre of Excellence for Invasion Biology, Stellenbosch. http://dx.doi.org/10.5281/zenodo.7433141
Rumex roseus Linnaeus, 1753, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1753
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Polygonales
Polygonaceae
Rumex
Rumex roseus

description: Rumex roseus, spec. nov.
 17. Rumex floribus hermaphroditis distinctis: valvularum alis maximis membranaceis, foliis erosis. Roy. lugdb. 230.
 Acetosa aegyptia, roseo seminis involucro. Sauh. afr. 5. f. 5.
 Habitat in AEgypto . ☉
description: Published as part of Linnaeus, Carolus, 1753, Species plantarum: exhibentes plantas rite cognitas, ad genera relatas, cum differentiis specificis, nominibus trivialibus, synonymis selectis, locis natalibus, secundum systema sexuale digestas, Stockholm :Laurentius Salvius on page 337, DOI: 10.5281/zenodo.3931989
Appendix 5 to "The Status of Biological Invasions and their Management in South Africa in 2022 [SECOND DRAFT FOR PUBLIC COMMENT]"—Pathways change tracker
Creators: name: SANBI
name: CIB
Publisher: name: Zenodo
Year: 2023

description: For more details see: http://iasreport.sanbi.org.za SANBI and CIB 2023. Appendix 5 to "The Status of Biological Invasions and their Management in South Africa in 2022 [SECOND DRAFT FOR PUBLIC COMMENT]"—Pathways change tracker. South African National Biodiversity Institute, Kirstenbosch and DSI-NRF Centre of Excellence for Invasion Biology, Stellenbosch. http://dx.doi.org/10.5281/zenodo.8047687