cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Real-Time Quantum Dynamics of Long-Range Electronic Excitation Transfer in Plasmonic Nanoantennas
Creators: name: Ilawe, Niranjan V.
name: Oviedo, M. Belén
name: Wong, Bryan M.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Materials Science (cond-mat.mtrl-sci)
subject: Chemical Physics (physics.chem-ph)
subject: FOS: Physical sciences

description: Using large-scale, real-time quantum dynamics calculations, we present a detailed analysis of electronic excitation transfer (EET) mechanisms in a multi-particle plasmonic nanoantenna system. Specifically, we utilize real-time, time-dependent, density functional tight binding (RT-TDDFTB) to provide a quantum-mechanical description (at an electronic/atomistic level of detail) for characterizing and analyzing these systems, without recourse to classical approximations. We also demonstrate highly long-range electronic couplings in these complex systems and find that the range of these couplings is more than twice the conventional cutoff limit considered by FRET based approaches. Furthermore, we attribute these unusually long-ranged electronic couplings to the coherent oscillations of conduction electrons in plasmonic nanoparticles. This long-range nature of plasmonic interactions has important ramifications for EET - in particular, we show that the commonly used "nearest-neighbor" FRET model is inadequate for accurately characterizing EET even in simple plasmonic antenna systems. These findings provide a real-time, quantum-mechanical perspective for understanding EET mechanisms and provide guidance in enhancing plasmonic properties in artificial light-harvesting systems.
description: Accepted by the Journal of Chemical Theory and Computation
Many-body quantum dynamics by the reduced density matrix based on the time-dependent density functional theory
Creators: name: Nazarov, Vladimir U.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We evaluate the density matrix of an arbitrary quantum mechanical system in terms of the quantities pertinent to the solution of the time-dependent density functional theory (TDDFT) problem. Our theory utilizes the adiabatic connection perturbation method of Görling and Levy, from which the expansion of the many-body density matrix in powers of the coupling constant $λ$ naturally arises. We then find the reduced density matrix $ρ_λ({\bf r},{\bf r}',t)$, which, by construction, has the $λ$-independent diagonal elements $ρ_λ({\bf r},{\bf r},t)=n({\bf r},t)$, $n({\bf r},t)$ being the particle density. The off-diagonal elements of $ρ_λ({\bf r},{\bf r}',t)$ contribute importantly to the processes, which cannot be treated via the density, directly or by the use of the known TDDFT functionals. Of those, we consider the momentum-resolved photoemission, doing this to the first order in $λ$, i.e., on the level of the exact exchange theory. In illustrative calculations of photoemission from the quasi-2D electron gas and isolated atoms, we find quantitatively strong and conceptually far-reaching differences with the independent-particle Fermi's golden rule formula.
description: 13 pages, 4 figures
Phalaena holmiana Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Lepidoptera
Noctuidae
Phalaena
Phalaena holmiana

description: Phalaena holmiana [spec. nov.]
P. Tortrix alis superioribus luteo ferrugineis; macula marginali trigona argentea.
Fn. svec. 883.
Habitat in Pomonae arboribus.
Praecedentibus duabus paulo minor.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 532, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Mining Twitter Conversations around E-commerce Promotional Events
Creators: name: Mathew, Binny
name: A, Unnikrishnan T
name: Chakraborty, Tanmoy
name: Ganguly, Niloy
name: Datta, Samik
Publisher: name: arXiv
Year: 2018
Subjects: subject: Social and Information Networks (cs.SI)
subject: FOS: Computer and information sciences

description: With Social Media platforms establishing themselves as the de facto destinations for their customers views and opinions, brands around the World are investing heavily on invigorating their customer connects by utilizing such platforms to their fullest. In this paper, we develop a novel technique for mining conversations in Twitter by weaving together all conversations around an event into one unified graph (Conversation Graph, henceforth). The structure of the Conversation Graph emerges as a variant of the BOWTIE structure (dubbed ASKEWBOWTIE henceforth) as a result of the complex communication patterns amongst these players. Finally, we investigate the structural properties of the ASKEWBOWTIE structure to understand the configuration of the components and their temporal evolution.
description: 4 pages, 5 tables, 3 figures
DEFORMATION OF MORAL VALUES.
Creators: name: Yuldasheva, R.E.
Publisher: name: Zenodo
Year: 2024

description: Considering moral deviations as a holistic, dynamic formation (process), we identify from the variety of interrelations of this process with the moral life of society only four components that are most noticeable for our study: terrorism, drug addiction, corruption, irresponsibility. All of them have both theoretical and practical significance for the study of moral deviations.
Simplified landscapes for optimization of shaken lattice interferometry
Creators: name: Weidner, C. A.
name: Anderson, D. Z.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Quantum Physics (quant-ph)
subject: Atomic Physics (physics.atom-ph)
subject: FOS: Physical sciences

description: Motivated by recent results using shaken optical lattices to perform atom interferometry, we explore splitting of an atom cloud trapped in a phase-modulated ("shaken") optical lattice. Using a simple analytic model we are able to show that we can obtain the simplest case of $\pm2\hbar k_\mathrm{L}$ splitting via single-frequency shaking. This is confirmed both via simulation and experiment. Furthermore, we are able to split with a relative phase $θ$ between the two split arms of $0$ or $π$ depending on our shaking frequency. Addressing higher-order splitting, we determine that $\pm6\hbar k_\mathrm{L}$ splitting is sufficient to be able to accelerate the atoms in counter-propagating lattices. Finally, we show that we can use a genetic algorithm to optimize $\pm4\hbar k_\mathrm{L}$ and $\pm6\hbar k_\mathrm{L}$ splitting to within $\approx0.1\%$ by restricting our optimization to the resonance frequencies corresponding to single- and two-photon transitions between Bloch bands.
Hard X-ray emitting black hole fed by accretion of low angular momentum matter
Creators: name: Igumenshchev, Igor V.
name: Illarionov, Andrei F.
name: Abramowicz, Marek A.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Observed spectra of Active Galactic Nuclei (AGN) and luminous X-ray binaries in our Galaxy suggest that both hot (~10^9 K) and cold (~10^6 K) plasma components exist close to the central accreting black hole. Hard X-ray component of the spectra is usually explained by Compton upscattering of optical/UV photons from optically thick cold plasma by hot electrons. Observations also indicate that some of these objects are quite efficient in converting gravitational energy of accretion matter into radiation. Existing theoretical models have difficulties in explaining the two plasma components and high intensity of hard X-rays. Most of the models assume that the hot component emerges from the cold one due to some kind of instability, but no one offers a satisfactory physical explanation for this. Here we propose a solution to these difficulties that reverses what was imagined previously: in our model the hot component forms first and afterward it cools down to form the cold component. In our model, accretion flow has initially a small angular momentum, and thus it has a quasi-spherical geometry at large radii. Close to the black hole, the accreting matter is heated up in shocks that form due to the action of the centrifugal force. The hot post-shock matter is very efficiently cooled down by Comptonization of low energy photons and condensates into a thin and cold accretion disk. The thin disk emits the low energy photons which cool the hot component.
description: 15 pages, 2 figures, submitted to ApJ Lett
Dynamics of measurement induced nonlocality under decoherence
Creators: name: Muthuganesan, R.
name: Sankaranarayanan, R.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Measurement Induced Nonlocality (MIN) captures nonlocal effects of a quantum state due to local von Neumann projective measurements, is a bonafide measure of quantum correlation between constituents of a composite system. In this paper, we study the dynamical behavior of entanglement (measured by concurrence), Hilber-Schmidt MIN and fidelity based MIN (FMIN) under local noisy channels such as hybrid (consists of bit, phase, bit and phase flip), generalized amplitude damping (GAD) and depolarizing channels for the initial Bell diagonal state. We observed that while sudden death of entanglement occur in hybrid and GAD channels, MIN and FMIN are more robust against such noise. Finally, we demonstrate the revival of MIN and FMIN after a dark point of time against depolarizing noise.
title: ADCO, Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome V, Cart. 189 (11 H 74), 316 folios, f. 0059v
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
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 général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome V, Archives départementales de la Côte-d'Or, Cart. 189 (11 H 74), 316 folios, f. 0059v, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome V, Archives départementales de la Côte-d'Or, Cart. 189 (11 H 74), 316 folios, f. 0059v, 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
Ab initio molecular dynamics via density based energy functionals
Creators: name: Shah, Vaishali
name: Nehete, Dinesh
name: Kanhere, D. G.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: The use of energy functionals based on density as the basic variable is advocated for ab initio molecular dynamics. It is demonstrated that the constraint of positivity of density can be incorporated easily by using square root density for minimization of the energy functional. An ad hoc prescription for including nonlocal pseudopotentials for plane wave based calculations is proposed and is shown to yield improved results. Applications are reported for equilibrium geometries of small finite systems, viz. dimers and trimers of simple metal atoms like Na and Mg, which represent a rather stringent test for approximate kinetic energy functionals involved in such calculations.
description: 15 pages, RevTeX 3.0, 3 PS Figures at the end
NPA_ref1417
Creators: name: Santen, Jeffrey A Van
Publisher: name: Zenodo
Year: 2019

description: Citation for NP Atlas reference previously without DOI Citation:  Reusch, R N; Sadoff, H L 5-n-Alkylresorcinols from encysting Azotobacter vinelandii: isolation and characterization Journal of Bacteriology, 1979, 139(2), 448-453 PubMed ID: 457611 Publisher Access: https://jb.asm.org/content/139/2/448.long
Phalaena rolandriana Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Lepidoptera
Noctuidae
Phalaena
Phalaena rolandriana

description: Phalaena rolandriana [spec. nov.]
P. Tortrix alis superioribus pallide testaceis, strigis ferrugineis inferne antrorsum versis.
Habitat in Europa.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 532, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
A Puzzle about Further Facts
Creators: name: Conitzer, Vincent
Publisher: name: arXiv
Year: 2018
Subjects: subject: History and Philosophy of Physics (physics.hist-ph)
subject: FOS: Physical sciences

description: In metaphysics, there are a number of distinct but related questions about the existence of "further facts" -- facts that are contingent relative to the physical structure of the universe. These include further facts about qualia, personal identity, and time. In this article I provide a sequence of examples involving computer simulations, ranging from one in which the protagonist can clearly conclude such further facts exist to one that describes our own condition. This raises the question of where along the sequence (if at all) the protagonist stops being able to soundly conclude that further facts exist.
description: To appear in Erkenntnis: An International Journal of Scientific Philosophy
Interstellar communication. X. The colors of optical SETI
Creators: name: Hippke, Michael
Publisher: name: arXiv
Year: 2018
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: It has recently been argued from a laser engineering point of view that there are only a few magic colors for optical SETI. These are primarily the Nd:YAG line at 1064 nm and its second harmonic 532.1 nm. Next best choices would be the sum frequency and/or second harmonic generation of Nd:YAG and Nd:YLF laser lines, 393.8 nm (near Fraunhofer CaK), 656.5 nm (H$α$) and 589.1 nm (NaD2). In this paper, we examine the interstellar extinction, atmospheric transparency and scintillation, as well as noise conditions for these laser lines. For strong signals, we find that optical wavelengths are optimal for distances $d\lesssim\,$kpc. Nd:YAG at $λ=1{,}064\,$nm is a similarly good choice, within a factor of two, under most conditions and out to $d\lesssim3\,$kpc. For weaker transmitters, where the signal-to-noise ratio with respect to the blended host star is relevant, the optimal wavelength depends on the background source, such as the stellar type. Fraunhofer spectral lines, while providing lower stellar background noise, are irrelevant in most use cases, as they are overpowered by other factors. Laser-pushed spaceflight concepts, such as "Breakthrough Starshot", would produce brighter and tighter beams than ever assumed for OSETI. Such beamers would appear as naked eye stars out to kpc distances. If laser physics has already matured and converged on the most efficient technology, the laser line of choice for a given scenario (e.g., Nd:YAG for strong signals) can be observed with a narrow filter to dramatically reduce background noise, allowing for large field-of-view observations in fast surveys.
description: 17 pages, 12 Figures. Comments welcome
On the transfer of momentum from stellar jets to molecular outflows
Creators: name: Downes, T. P.
name: Ray, T. P.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: While it is generally thought that molecular outflows from young stellar objects (YSOs) are accelerated by underlying stellar winds or highly collimated jets, the actual mechanism of acceleration remains uncertain. The most favoured model, at least for low and intermediate mass stars, is that the molecules are accelerated at jet-driven bow shocks. Here we investigate, through high resolution numerical simulations, the efficiency of this mechanism in accelerating ambient molecular gas without causing dissociation. The efficiency of the mechanism is found to be surprisingly low suggesting that more momentum may be present in the underlying jet than previously thought. We also compare the momentum transferring efficiencies of pulsed versus steady jets. We find that pulsed jets, and the corresponding steady jet with the same average velocity, transfer virtually the same momentum to the ambient gas. The additional momentum ejected sideways from the jet beam in the case of the pulsed jet only serves to accelerate post-shock jet gas which forms a, largely atomic, sheath around the jet beam. For both the steady and pulsing jets, we find a power law relationship between mass and velocity ($m(v) \propto v^{-γ}$) which is similar to what is observed. We also find that increasing the molecular fraction in the jet decreases $γ$ as one might expect. We reproduce the so-called Hubble law for molecular outflows and show that it is almost certainly a local effect in the presence of a bow shock.
description: 9 pages, 6 figures in LaTeX2e, accepted by Astronomy and Astrophysics
On The Violation Of Marshall-Peierls Sign Rule In The Frustrated $J_{1}-J_{2}$ Heisenberg Antiferromagnet
Creators: name: Richter, J.
name: Ivanov, N. B.
name: Retzlaff, K.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: We present a number of arguments in favor of the suggestion that the Marshall-Peierls sign rule survives the frustration in the square-lattice Heisenberg antiferromagnet with frustrating next-nearest-neighbor (diagonal) bonds ($J_{1}-J_{2}$ model) for relatively large values of the parameter $J_{2}/J_{1}$. Both the spin-wave analysis and the exact-diagonalization data concerning the weight of Marshall states support the above suggestion.
description: 8 pages, LaTex, 2 figurs on request
title: #44 Feminist Resistance in Armed Conflicts: Beyond Victimhood, Toward Justice
Creators: name: Rau, Daniela
name: Chausse, Céline
Publisher: name: Fachinformationsdienst für internationale und interdisziplinäre Rechtsforschung
Year: 2025
Subjects: subject: 341

description: Women play diverse and complex roles in armed conflicts – whether as combatants, peacebuilders, community organizers, or as those directly impacted by war, including through gender-based violence. Yet, international law has long struggled to fully acknowledge their agency and provide meaningful protections. In this episode, Polina Kulish and Rishiti Choudaha sit down with Kateryna Demerza and Vladyslava Vorobiova from Vitsche e.V., a Berlin-based NGO that amplifies Ukrainian voices in Europe. Together, they discuss the realities of women’s resistance in wartime contexts, feminist activism’s role in challenging silences of international law, and the broader struggles against disinformation. Before the interview, Céline Chausse introduces the discussion by reflecting on the ‘Women in International Law’ symposium and the importance of centering women’s voices in conversations about conflict and justice. Sissy Katsoni then provides a legal overview, setting the stage with key facts and frameworks on how international humanitarian and human rights law seek to protect women in conflict – and where these frameworks continue to fall short. With armed conflicts around the world continuing to impact millions of women, this discussion provides a timely reflection on solidarity, activism, and the future of feminist engagement in international law. This special episode is part of the ‘Women in International Law’ symposium and was therefore produced in English. Have thoughts to share? We’re all ears! Whether it’s applause, reflections, or a dash of helpful critique, reach us anytime at podcast@voelkerrechtsblog.org. Be sure to subscribe via RSS, Spotify, or wherever your favorite podcasts live. And hey, if you love what you hear, a five-star rating goes a long way! Background information (all Open Access): Völkerrechtsblog, Women in International Law Vol. 4 (2025) Ruta Association for Central, South-Eastern, and Eastern European, Baltic, Caucasus, Central and Northern Asian Studies in Global Conversation Bohachevsky-Chomiak M, Feminists Despite Themselves: Women in Ukrainian Community Life, 1884-1939 (Canadian institute of Ukrainian studies, University of Alberta 1988) Yuliia Mieriemova, How Ukrainian servicewomen’s stories of war matter (2025). Maryna Shevtsova (ed.), Feminist Perspective on Russia’s War in Ukraine: Hear Our Voices (2024) UN Women, Gender alert: Scarcity and fear: A gender analysis of the impact of the war in Gaza on vital services essential to women’s and girls’ health, safety, and dignity – Water, sanitation, and hygiene (2024). Moderation: Céline Chausse Interview: Polina Kulish, Rishiti Choudaha, and Sissy Katsoni Background information: Sissy Katsoni Cut: Daniela Rau Credits: Georgetown Institute for Women, Peace & Security, “A Message from Oleksandra Matviichuk“ on YouTube (1:00-1:36)
description: Völkerrechtsblog
NPA_ref1549
Creators: name: Santen, Jeffrey A Van
Publisher: name: Zenodo
Year: 2019

description: Citation for NP Atlas reference previously without DOI Citation:  Gauze, G f; Preobrazhenskaia, T p; Ivanitskaia, L p; Sveshnikova, M a [Production of the antibiotic sibiromycin by the Streptosporangium sibiricum sp. nov. culture] Antibiotiki, 1969, 14(11), 963-969 PubMed ID: 4907802 Publisher Access: NONE
Phalaena solandriana Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Lepidoptera
Noctuidae
Phalaena
Phalaena solandriana

description: Phalaena solandriana [spec. nov.]
P. Tortrix alis superioribus pallidis: macula communi dorsali ferruginea.
De Geer ins. 1. t. 28. f. 29, 30.
Habitat in Betula.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 532, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
title: Kohaliku piiriliikluse rakendamise eripära Eestis ja lähiriikides (Soome, Läti, Leedu ja Poola)
Creators: name: Lindsaar, Inge
Publisher: name: Tallinn: Sisekaitseakadeemia
Year: 2021
Subjects: classificationCode: 5
subject: FOS: Social sciences

description: See mõttepaber annab ülevaate kohaliku piiriliikluse eri tahkudest ja nende tekkepõhjustest, samuti EL-i määrusest 1931/2006, mida tuntakse kohaliku piiriliikluse määruse nime all. See määrus kujutab endast Schengeni piirieeskirjade erisust, millega nähakse ette võimalus kohaldada välispiiri ääres elavatele kolmandate riikide kodanikele lihtsamat, vähemate piirikontrolli protseduuride rakendamisega seotud EL-i välise maismaapiiri ületamise korda läbi piiripunktide või nendevahelise ala.

 Võtmesõnad/Keywords: piirid (territooriumid); Eesti; Soome; Läti; Leedu; POola, Norra, Hispaania; Maroko; borders

description: Sissejuhatus ; 1. Kohaliku piiriliikluse õigusliku raamistiku põhipunktid ; 1.1. Kohaliku elaniku mõiste ; 1.2. Piiriäärsete alade elanikele kohalduvad eritingimused ; 1.3. Kohaliku piiriliikluse mõiste ; 1.4. Piiriala mõiste ; 1.5. Sissesõidu- ja piirialas viibimise nõuded ; 1.6. Kohaliku piiriliikluse load ; 2. Kohaliku piiriliikluse lepingud ; 3. Teiste riikide praktika ; 3.1. Norra ; 3.2. Soome ; 3.3. Läti ; 3.4. Leedu ; 3.5. Poola ; 3.6. Hispaania ja Maroko vaheline kohalik piiriliiklus ; 3.7. Eesti ja Venemaa vahelise kohaliku piiriliikluse problemaatika – igavesti lahendamata olukord ; Kokkuvõte
Dark Energy Survey Year 1 Results: The effect of intracluster light on photometric redshifts for weak gravitational lensing
Creators: name: Gruen, D.
name: Zhang, Y.
name: Palmese, A.
name: Yanny, B.
name: Busti, V.
name: Hoyle, B.
name: Melchior, P.
name: Miller, C. J.
name: Rozo, E.
name: Rykoff, E. S.
name: Varga, T. N.
name: Abdalla, F. B.
name: Allam, S.
name: Annis, J.
name: Avila, S.
name: Brooks, D.
name: Burke, D. L.
name: Rosell, A. Carnero
name: Kind, M. Carrasco
name: Carretero, J.
name: Cawthon, R.
name: Crocce, M.
name: Cunha, C. E.
name: da Costa, L. N.
name: Davis, C.
name: De Vicente, J.
name: Desai, S.
name: Diehl, H. T.
name: Dietrich, J. P.
name: Drlica-Wagner, A.
name: Flaugher, B.
name: Fosalba, P.
name: Frieman, J.
name: García-Bellido, J.
name: Gaztanaga, E.
name: Gerdes, D. W.
name: Gruendl, R. A.
name: Gschwend, J.
name: Hollowood, D. L.
name: Honscheid, K.
name: James, D. J.
name: Jeltema, T.
name: Krause, E.
name: Kron, R.
name: Kuehn, K.
name: Kuropatkin, N.
name: Lahav, O.
name: Lima, M.
name: Lin, H.
name: Maia, M. A. G.
name: Marshall, J. L.
name: Menanteau, F.
name: Miquel, R.
name: Ogando, R. L. C.
name: Plazas, A. A.
name: Romer, A. K.
name: Scarpine, V.
name: Sevilla-Noarbe, I.
name: Smith, M.
name: Soares-Santos, M.
name: Sobreira, F.
name: Suchyta, E.
name: Swanson, M. E. C.
name: Tarle, G.
name: Thomas, D.
name: Vikram, V.
name: Walker, A. R.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We study the effect of diffuse intracluster light on the critical surface mass density estimated from photometric redshifts of lensing source galaxies, and the resulting bias in a weak lensing measurement of galaxy cluster mass. Under conservative assumptions, we find the bias to be negligible for imaging surveys like the Dark Energy Survey (DES) with a recommended scale cut of >=200 kpc distance from cluster centers. For significantly deeper source catalogs from present and future surveys like the Large Synoptic Survey Telescope (LSST) program, more conservative scale and source magnitude cuts or a correction of the effect may be necessary to achieve per-cent level lensing measurement accuracy, especially at the massive end of the cluster population.
description: 11 pages, 4 figures, matches version published in MNRAS
Galaxy Cluster Abundance Evolution and Cosmological Parameters
Creators: name: Viana, Pedro T. P.
name: Liddle, Andrew R.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We use the observed evolution of the galaxy cluster X-ray integral temperature distribution function between z=0.05 and z=0.32 in an attempt to constrain the value of the density parameter, Omega_0, for both open and spatially-flat universes. We conclude that when all the most important sources of possible error, both in the observational data and in the theoretical modelling, are taken into account, an unambiguous determination of Omega_0 is not feasible at present. Nevertheless, we find that values of Omega_0 around 0.75 are most favoured, with Omega_0<0.3 excluded with at least 90 per cent confidence. In particular, the Omega_0=1 hypothesis is found to be still viable.
description: 7 pages, LaTex using emulateapj.sty, to appear in the electronic proceedings of the conference Cosmological Constraints from X-ray Clusters, Strasbourg, France, Dec. 9-11, 1998
Vocal effort modulates the motor planning of short speech structures
Creators: name: Taitz, Alan
name: Shalom, Diego E
name: Trevisan, Marcos A
Publisher: name: arXiv
Year: 2018
Subjects: subject: Neurons and Cognition (q-bio.NC)
subject: Biological Physics (physics.bio-ph)
subject: FOS: Biological sciences
subject: FOS: Physical sciences

description: Speech requires programming the sequence of vocal gestures that produce the sounds of words. Here we explored the timing of this program by asking our participants to pronounce, as quickly as possible, a sequence of consonant-consonant-vowel (CCV) structures appearing on screen. We measured the delay between visual presentation and voice onset. In the case of plosive consonants, produced by sharp and well defined movements of the vocal tract, we found that delays are positively correlated with the duration of the transition between consonants. We then used a battery of statistical tests and mathematical vocal models to show that delays reflect the motor planning of CCVs and transitions are proxy indicators of the vocal effort needed to produce them. These results support that the effort required to produce the sequence of movements of a vocal gesture modulates the onset of the motor plan.
description: 17 pages, 3 figures
$J_1-J_2$ Quantum Heisenberg Antiferromagnet: Improved Spin-Wave Theories Versus Exact-Diagonalization Data
Creators: name: Ivanov, N. B.
name: Richter, J.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: We reconsider the results cocerning the extreme-quantum $S=1/2$ square-lattice Heisenberg antiferromagnet with frustrating diagonal couplings ($J_1-J_2$ model) drawn from a comparison with exact-diagonalization data. A combined approach using also some intrinsic features of the self-consistent spin-wave theory leads to the conclusion that the theory strongly overestimates the stabilizing role of quantum flutcuations in respect to the Néel phase in the extreme-quantum case $S=1/2$. On the other hand, the analysis implies that the Néel phase remains stable at least up to the limit $J_{2}/J_{1} = 0.49$ which is pretty larger than some previous estimates. In addition, it is argued that the spin-wave ansatz predicts the existence of a finite range ($J_{2}/J_{1}<0.323$ in the linear spin-wave theory) where the Marshall-Peierls sigh rule survives the frustrations.
description: 13 pages, LaTex, 7 figures on request
The lattice of varieties of implication semigroups
Creators: name: Gusev, S. V.
name: Sankappanavar, H. P.
name: Vernikov, B. M.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Group Theory (math.GR)
subject: FOS: Mathematics
subject: Primary 06E75, secondary 08B15

description: In 2012, the second author introduced and examined a new type of algebras as a generalization of De Morgan algebras. These algebras are of type (2,0) with one binary and one nullary operation satisfying two certain specific identities. Such algebras are called implication zroupoids. They invesigated in a number of articles by the second author and J.M.Cornejo. In these articles several varieties of implication zroupoids satisfying the associative law appeared. Implication zroupoids satisfying the associative law are called implication semigroups. Here we completely describe the lattice of all varieties of implication semigroups. It turns out that this lattice is non-modular and consists of 16 elements.
description: Compared with the previous version, we rewrite Section 3 and add Appendixes A and B
Upper Critical Field in a Spin-Charge Separated Superconductor
Creators: name: Dias, R. G.
name: Wheatley, J. M.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: It is demonstrated that the spatial decay of the pair propagator in a Luttinger liquid with spin charge separation contains a logarithmic correction relative to the free fermi gas result in a finite interval between the spin and charge thermal lengths. It is argued that similar effects can be expected in higher dimensional systems with spin charge separation and that the temperature dependence of the upper critical field $H_{c2}$ curve is a probe of this effect.
description: 3 pages, postscript file (compressed and uuencoded)
title: ADCO, Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome IV, Cart. 188 (11 H 73), f. 0201v
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
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: cartulaire
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome IV, Archives départementales de la Côte-d'Or, Cart. 188 (11 H 73), f. 0201v, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome IV, Archives départementales de la Côte-d'Or, Cart. 188 (11 H 73), f. 0201v, 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
Implications of H-alpha Observations for Studies of the Cosmic Microwave Background
Creators: name: McCullough, P. R.
name: Gaustad, J. E.
name: Rosing, W.
name: Van Buren, D.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We summarize the relationship between the free-free emission foreground and Galactic H-alpha emission. H-alpha observations covering nearly the entire celestial sphere are described. These data provide a template to isolate and/or remove the effect of Galactic free-free emission from observations of the cosmic microwave background. Spectroscopy and imaging provide two complementary methods for measuring the H-alpha emission. Spectroscopy is favored for its velocity resolution and imaging is favored for its angular resolution. With templates of the three dominant foregrounds, namely synchrotron, thermal dust, and free-free emissions, it may be possible to quantify the location and the brightness of another foreground such as that from rotating dust grains.
description: 20 pages, 7 figures, Submitted to proceeding of Sloan Summit on Microwave Foregrounds, edited by Angelica de Oliveira-Costa & Max Tegmark (ASP, San Francisco, 1999)
NPA_ref1694
Creators: name: Santen, Jeffrey A Van
Publisher: name: Zenodo
Year: 2019

description: Citation for NP Atlas reference previously without DOI Citation:  Wollenweber, H W; Rietschel, E T; Hofstad, T; Weintraub, A; Lindberg, A A Nature, type of linkage, quantity, and absolute configuration of (3-hydroxy) fatty acids in lipopolysaccharides from Bacteroides fragilis NCTC 9343 and related strains Journal of Bacteriology, 1980, 144(3), 898 PubMed ID: 7440508 Publisher Access: https://jb.asm.org/content/144/3/898/article-info
Characteristic Potentials for Mesoscopic Rings Threaded by an Aharonov-Bohm Flux
Creators: name: Buttiker, M.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: Electro-static potentials for samples with the topology of a ring and penetrated by an Aharonov-Bohm flux are discussed. The sensitivity of the electron-density distribution to small variations in the flux generates an effective electro-static potential which is itself a periodic function of flux. We investigate a simple model in which the flux sensitive potential leads to a persistent current which is enhanced compared to that of a loop of non-interacting electrons. For sample geometries with contacts the sensitivity of the electro-static potential to flux leads to a flux-induced capacitance. This capacitance gives the variation in charge due to an increment in flux. The flux-induced capacitance is contrasted with the electro-chemical capacitance which gives the variation in charge due to an increment in an electro-chemical potential. The discussion is formulated in terms of characteristic functions which give the variation of the electro-static potential in the interior of the conductor due to an increment in the external control parameters (flux, electro-chemical potentials). Paper submitted to the 16th Nordic Semiconductor Meeting, Laugarvatan, Iceland, June 12-15, 1994. The proceedings will be published in Physica Scripta.
description: 23 pages + 4 figures, revtex, IBM-RC19557
Phalaena hastiana Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Lepidoptera
Noctuidae
Phalaena
Phalaena hastiana

description: Phalaena hastiana [spec. nov.]
P. Tortrix alis superioribus fuscis: fascia antrorsum obliqua alba.
Habitat in Salice. Reinh. Hast.
Fascia non tangit marginem interiorem alae & a summo descendit antrorsum.
Hast (Reinh.) fenno, natus ad Insectorum Historiam, at in flore aetatis periit egregius discipulus.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 532, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
The CNOC2 Field Galaxy Luminosity Function I: A Description of Luminosity Function Evolution
Creators: name: Lin, H.
name: Yee, H. K. C.
name: Carlberg, R. G.
name: Morris, S. L.
name: Sawicki, M.
name: Patton, D. R.
name: Wirth, G.
name: Shepherd, C. W.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We examine the evolution of the galaxy luminosity function (LF) using a sample of over 2000 galaxies, with 0.12 < z < 0.55 and 17.0 < Rc < 21.5, drawn from the Canadian Network for Observational Cosmology Field Galaxy Redshift Survey (CNOC2), at present the largest such sample at intermediate redshifts. We use UBVRcIc photometry to classify our galaxies into early, intermediate, and late types, for which we compute luminosity functions in the rest-frame B, Rc, and U bandpasses. In particular, we adopt a parameterization of LF evolution including luminosity and number density evolution, and take care to quantify correlations among our LF evolution parameters. Our principal result is a clear quantitative separation of luminosity and density evolution for different galaxy populations, and the finding that the character of the LF evolution is strongly dependent on galaxy type. Specifically, the early- and intermediate-type LF's show primarily brightening at higher redshifts and only modest density evolution, while the late-type LF is best fit by strong number density increases at higher z, with little luminosity evolution. We also carefully measure and account for sample selection effects as functions of galaxy magnitude and color, and show that our results are not significantly affected by potential systematic effects, such as surface brightness selection, photometric errors, or redshift incompleteness. (abstract abridged)
description: 57 pages, including 21 figures; ApJ, in press. Also available at http://manaslu.astro.utoronto.ca/~carlberg/cnoc/index.html
NPA_ref2298
Creators: name: Santen, Jeffrey A Van
Publisher: name: Zenodo
Year: 2019

description: Citation for NP Atlas reference previously without DOI Citation:  Kamiński, E; Libbey, L m; Stawicki, S; Wasowicz, E Identification of the predominant volatile compounds produced by Aspergillus flavus Applied Microbiology, 1972, 24(5), 721-726 PubMed ID: 4629700 Publisher Access: https://aem.asm.org/content/24/5/721
Interstellar communication. XI. Short pulse duration limits of optical SETI
Creators: name: Hippke, Michael
Publisher: name: arXiv
Year: 2018
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: Previous and ongoing searches for extraterrestrial optical and infrared nanosecond laser pulses and narrow line-width continuous emissions have so far returned null results. At the commonly used observation cadence of $\sim 10^{-9}\,$s, sky-integrated starlight is a relevant noise source for large field-of-view surveys. This can be reduced with narrow bandwidth filters, multipixel detectors, or a shorter observation cadence. We examine the limits of short pulses set by the uncertainty principle, interstellar scattering, atmospheric scintillation, refraction, dispersion and receiver technology. We find that optimal laser pulses are time-bandwidth limited Gaussians with a duration of $Δt \approx\,10^{-12}\,$s at a wavelength $λ_{0}\approx1\,μ$m, and a spectral width of $Δλ\approx 1.5\,$nm. Shorter pulses are too strongly affected through Earth's atmosphere. Given certain technological advances, survey speed can be increased by three orders of magnitude when moving from ns to ps pulses. Faster (and/or parallel) signal processing would allow for an all-sky-at-once survey of lasers targeted at Earth.
description: 17 pages, 9 Figures. Comments welcome
title: ADCO, Huitième cartulaire de Saint-Étienne de Dijon (1661-1667), Cart. 31 (G 135), 549 folios, f. 0691
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
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire
subject: Corpus Burgundiae Medii Aevi

description: Huitième cartulaire de Saint-Étienne de Dijon (1661-1667), Archives départementales de la Côte-d'Or, Cart. 31 (G 135), 549 folios, f. 0691, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Huitième cartulaire de Saint-Étienne de Dijon (1661-1667), Archives départementales de la Côte-d'Or, Cart. 31 (G 135), 549 folios, f. 0691, 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
E and S0 galaxies in the central part of the Coma cluster: Ages, metal abundances and dark matter
Creators: name: Jorgensen, Inger
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Mean ages and metal abundances are estimated for the stellar populations in a sample of 115 E and S0 galaxies in the central 64'x70' of the Coma cluster. The estimates are based on the line indices Mg2, and Hbeta, and the mass-to-light ratios (M/L). Stellar population models from Vazdekis et al. were used to transform from the measured parameters to mean ages, [Mg/H] and [Fe/H]. Comparison of the ages derived from the Mg2-Hbeta diagram to those derived from the Mg2-M/L diagram gives an estimate of the variation in the fraction of dark matter. The distributions of the derived mean ages and abundances show that there are real variations in both the mean ages and in the abundances. We find an intrinsic rms scatter of [Mg/H], [Fe/H] and [Mg/Fe] of 0.2 dex, and an intrinsic rms scatter of the derived ages of 0.17 dex. The slopes of the scaling relations between the global parameters for the galaxies (the Mg2-sigma relation, the -sigma relation, the Hbeta-sigma relation) are consistent with the relation we find between the ages, the abundances and the velocity dispersions. The slope of the Fundamental Plane is steeper than predicted from the variations in the ages and abundances. Because of the correlation between the mean ages and the mean abundances, substantial variations in the ages and the abundances are possible while maintaining a low scatter of all the scaling relations.
description: 33 pages, 14 figures. MN LaTeX. Accepted for publication in MNRAS
El cuarto Sector en Argentina
Creators: name: Caruana, María Eugenia Castelao
name: IE Center For The Governance Of Change
name: Secretaría General Iberoamericana
Publisher: name: Zenodo
Year: 2019
Subjects: Economy
Fourth Sector
Social aspects
Environmental aspects
Finance
Argentina
Latinamerica

description: El origen de las organizaciones de ayuda mutua y participación voluntaria en Argentina se remonta a los primeros años del siglo XIX, cuando más allá de toda diferencia económica, política o cultural, los miembros comenzaron a relacionarse como pares en la persecución de un fin común (Sábato, 2002). Desde entonces, diversos modelos de organización se han instalado para resolver problemas colectivos participando activamente en el mercado y modificando, en algunos casos, sus reglas. Más recientemente, en respuesta a desafíos de alcance global como la desigualdad, el cambio climático y la pobreza, han surgido nuevos modelos de organización y producción que cuestionan el modelo de negocio tradicional -centrado en el beneficio económico- y proponen contribuir a resolver estos problemas a través del mercado, generando beneficios sociales, ambientales y económicos. Estas organizaciones buscan ser agentes de cambio a través de la oferta de productos o servicios innovadores, la adopción de modelos de organización disruptivos y/o la construcción de cadenas de valor basadas en el respeto por el trabajo y el medioambiente. Todas estas organizaciones integran el Cuarto Sector y se presentan en una variedad de formas jurídicas: cooperativas, mutuales, asociaciones, fundaciones, empresas de triple impacto y empresas sociales. Algunas, además, adoptan los estándares del Comercio Justo y/o del Sistema B y se identifican con la Economía Circular, la Economía Colaborativa, la Economía Social y Solidaria, entre otras. A pesar de sus heterogeneidades, el Cuarto Sector en el país se encuentra en expansión, impulsado por una mayor presencia en la agenda política de los últimos 15 años, una creciente visibilidad social y compromiso ciudadano con la resolución de los problemas públicos, en el marco de una tendencia global que promueve un mayor esfuerzo del sector privado para lograr los Objetivos de Desarrollo Sostenible (ODS) hacia el año 2030.
On Joint Distributions, Counterfactual Values, and Hidden Variables in Relation to Contextuality
Creators: name: Dzhafarov, Ehtibar
Publisher: name: arXiv
Year: 2018
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences
subject: 81P13, 81Q99, 60A99

description: This paper deals with three traditional ways of defining contextuality: (C1) in terms of (non)existence of certain joint distributions involving measurements made in several mutually exclusive contexts; (C2) in terms of relationship between factual measurements in a given context and counterfactual measurements that could be made if one used other contexts; and (C3) in terms of (non)existence of ``hidden variables'' that determine the outcomes of all factually performed measurements. It is generally believed that the three meanings are equivalent, but the issues involved are not entirely transparent. Thus, arguments have been offered that C2 may have nothing to do with C1, and the traditional formulation of C1 itself encounters difficulties when measurement outcomes in a contextual system are treated as random variables. I show that if C1 is formulated within the framework of the Contextuality-by-Default (CbD) theory, the notion of a probabilistic coupling, the core mathematical tool of CbD, subsumes both counterfactual values and ``hidden variables''. In the latter case, a coupling itself can be viewed as a maximally parsimonious choice of a hidden variable.
description: To be published in Dzhafarov, E.N. (2019). Philosophical Transactions of the Royal Society A