cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Additional file 7: of Complete genome of streamlined marine actinobacterium Pontimonas salivibrio strain CL-TW6T adapted to coastal planktonic lifestyle
Creators: name: Cho, Byung
name: Hardies, Stephen
name: Jang, Gwang
name: Hwang, Chung
Publisher: name: figshare
Year: 2018
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Genetics
subject: Molecular Biology
subject: Evolutionary Biology
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: Marine Biology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology

description: Figure S3. Phylogenomic tree. Encoded protein sequences catenated were selected from among large genes, with congruent single gene trees, and enriched with genes having BlastP results suggesting greater similarity of P. salivibrio with Yonghaparkia than to Microbacteria, Clavibacter, Rathayibacter, and Leifsonia. The computation is specifically designed to accept or reject a closer common ancestor with Yonghaparkia. Genes used were C3B54_11793, C3B54_11942, C3B54_11990, C3B54_111069, C3B54_111092, C3B54_111098, C3B54_111113, C3B54_111132, C3B54_111675. Time scale was determined as described in Fig. 2. (DOC 78 kb)
IN03020 Vessagiri Rock C Cave 8 Inscription
Creators: name: Wickremasinghe, Don Martino de Zilva
Publisher: name: Zenodo
Year: 2019
Subjects: IN03020
Epigraphia Zeylanica
Vessagiri

description: IN03020 Vessagiri Rock C Cave 8 Inscription - Transcript and Translation Source: Wickremasinghe, Don Martino de Zilva. (1904-12). ‘No. 2. Vessagiri Inscriptions,’ Epigraphia Zeylanica 1, pp. 10-39.
Spatial correlation function of quasars and power spectrum of cosmological matter density perturbations
Creators: name: Novosyadlyj, B.
name: Chornij, Yu.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We examine the dependence of the spatial two-point correlation function of quasars $ξ_{qq}(r,z)$ at different redshifts on the initial power spectrum in flat cosmological models. Quasars and other elements of the large-scale structure of the universe are supposed to form in the peaks of the scalar Gaussian field of density fluctuations of appropriate scales. Quasars are considered as a manifestation of short-term active processes at the centers of these fluctuations. We propose a method for calculating the correlation function $ξ_{qq}(r,z)$ and show its amplitude and slope to depend on the shape of the initial power spectrum and the scale R of the fluctuations in which quasars are formed. We demonstrate that in the CDM models with the initial power spectrum slope $n=0.7\div1$ it is possible to explain, by choosing appropriate values of R, how the amplitudes and correlation radii of $ξ_{qq}(r,z)$ may either increase or decrease with increasing redshift z. In particular, the correlation radii of $ξ_{qq}(r,z)$ grow from $6-10h^{-1}$ Mpc when R grows from $0.45 h^{-1}$ to $1.3h^{-1}$ Mpc. The H+CDM model at realistic values of R fails to account for the observational data according to which the $ξ_{qq}(r,z)$ amplitude decreases with increasing $z$.
description: 8 pages, 2 figures
Computing the quasipotential for highly dissipative and chaotic SDEs. An application to stochastic Lorenz'63
Creators: name: Cameron, Maria
name: Yang, Shuo
Publisher: name: arXiv
Year: 2018
Subjects: subject: Dynamical Systems (math.DS)
subject: FOS: Mathematics
subject: 65N99, 65P99, 58J65

description: The study of noise-driven transitions occurring rarely on the time-scale of systems modeled by SDEs is of crucial importance for understanding such phenomena as genetic switches in living organisms and magnetization switches of the Earth. For a gradient SDE, the predictions for transition times and paths between its metastable states are done using the potential function. For a nongradient SDE, one needs to decompose its forcing into a gradient of the so-called quasipotential and a rotational component, which cannot be done analytically in general. We propose a methodology for computing the quasipotential for highly dissipative and chaotic systems built on the example of Lorenz'63 with an added stochastic term. It is based on the ordered line integral method, a Dijkstra-like quasipotential solver, and combines 3D computations in whole regions, a dimensional reduction technique, and 2D computations on radial meshes on manifolds or their unions. Our collection of source codes is available on M. Cameron's web page and on GitHub.
description: 38 pages, 17 figures, 5 3D figures are linked to movies posted on youtube, software is available on GitHub
The state of the molecular gas in a luminous starburst/Seyfert 2 galaxy: NGC 1068 revisited
Creators: name: Papadopoulos, Padeli. P.
name: Seaquist, E. R.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present fully sampled ^{12}$CO, ^{13}CO J=2-1, 3-2 maps of the inner $\sim 1'\times 1'$ region of NGC 1068. We combine these measurements with an existing interferometric map of ^{12}CO J=1-0 that includes single dish data and thus contains all the flux present. This allows a reliable estimate of the ^{12}CO (J=3-2)/(J=1-0) ratio at the highest angular resolution currently possible and the use of this sensitive line ratio to probe the physical condition of the molecular gas. We also present two measurements of the faint C ^{18}O J=2--1 emission which confirm earlier measurements of a high $C ^{18}O/ ^{13}CO$ intensity ratio in this galaxy. A simple two-phase model for the gas can account for all the observed line ratios if C ^{18}O emission and part of the ^{13}CO emission arise in a dense spatially concentrated component. The ^{12}CO emission originates from a warmer, diffuse gas phase.The dense gas phase contains the bulk of the molecular gas mass while the diffuse phase may not be virialized leading to an overestimate of molecular gas mass when deduced from the luminosity of the ^{12}CO J=1--0 line and a standard galactic conversion factor.
description: 41 pages, 5 figures, to appear in Astrophysical Journal 1999, May 1
$η$-pairing as a mechanism of superconductivity in models of strongly correlated electrons
Creators: name: de Boer, Jan
name: Korepin, Vladimir E.
name: Schadschneider, Andreas
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We consider extended versions of the Hubbard model which contain additional interactions between nearest neighbours. In this letter we show that a large class of these models has a superconducting ground state in arbitrary dimensions. In some special cases we are able to find the complete phase diagram. The superconducting phase exist even for moderate repulsive values of the Hubbard interaction $U$.
description: 9 pages, RevTex, ITP-SB-94-18, 1 PS figure appended
ОПРЕДЕЛЕНИЕ ТЕСТА РАСТВОРЕНИЯ И КОЛИЧЕСТВЕННЫЙ АНАЛИЗ ТАБЛЕТОК ЛЕВОФЛОКСАЦИНА, ИЗГОТОВЛЕННЫХ ПО НОВОМУ  СОСТАВУ И ТЕХНОЛОГИИ
Creators: name: Хамидуллаев, Ш.А.
name: Хайдаров, В.Р.
name: Исматова, М.У.
Publisher: name: Zenodo
Year: 2024

description: Разработан тест на растворимость и количественный анализ таблеток левофлоксацина, полученных по новому составу и технологии. Для определения обоих показателей использовали метод высокоэффективной жидкостной хроматографии.
VLBI imaging of extremely high redshift quasars at 5 GHz
Creators: name: Paragi, Z.
name: Frey, S.
name: Gurvits, L. I.
name: Kellermann, K. I.
name: Schilizzi, R. T.
name: McMahon, R. G.
name: Hook, I. M.
name: Pauliny-Toth, I. I. K.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present very long baseline interferometry (VLBI) images of ten very high redshift (z>3) quasars at 5 GHz. The sources 0004+139, 0830+101, 0906+041, 0938+119 and 1500+045 were observed in September 1992 using a global VLBI array, while 0046+063, 0243+181, 1338+381, 1428+423 and 1557+032 were observed in October 1996 with the European VLBI Network and Hartebeesthoek, South Africa. Most of the sources are resolved and show asymmetric structure. The sample includes 1428+423, the most distant radio loud quasar known to date (z=4.72). It is barely resolved with an angular resolution of about 2.0*1.4 mas.
description: Astronomy and Astrophysics, in press, Latex2e, 10 pages, 3 figures (and lots of sub-figures)
Sphinx creusa Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Lepidoptera
Sphingidae
Sphinx
Sphinx creusa

description: Sphinx creusa [spec. nov.]
S. nigra, alis maculis fenestratis, abdominis basi viridi: segmentorum marginibus rubris. M. L. U.
Habitat in Calidis regionibus.
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 494, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Re-Structuring Method for the Negative Sign Problem in Quantum Spin Systems
Creators: name: Munehisa, Tomo
name: Munehisa, Yasuko
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: We present detailed discussions on a new approach we proposed in a previous paper to numerically study quantum spin systems. This method, which we will call re-structuring method hereafter, is based on rearrangement of intermediate states in the path integral formulation. We observed our approach brings remarkable improvement in the negative sign problem when applied to one-dimensional quantum spin $1/2$ system with next-to-nearest neighbor interactions. In this paper we add some descriptions on our method and show results from analyses by the exact diagonalization and by the transfer matrix method of the system on a small chain. These results also indicate that our method works quite effectively.
description: 14 pages, LaTeX, figures on request, YAMANASHI-94-01
Precursor of Superfluidity in a Strongly Interacting Fermi Gas with Negative Effective Range
Creators: name: Tajima, Hiroyuki
Publisher: name: arXiv
Year: 2018
Subjects: subject: Quantum Gases (cond-mat.quant-gas)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We theoretically investigate the effects of pairing fluctuations in an ultracold Fermi gas near a Feshbach resonance with a negative effective range. By employing a many-body T-matrix theory with a coupled boson-fermion model, we show that the single-particle density of states exhibits the so-called pseudogap phenomenon which is a precursor of superfluidity induced by strong pairing fluctuations. We clarify the region where strong pairing fluctuations play a crucial role in single-particle properties, from the broad-resonance region to the narrow-resonance limit at the divergent two-body scattering length. We also extrapolate the effects of pairing fluctuations to the positive-effective-range region from our results near the narrow Feshbach resonance. Results shown in this paper are relevant to the connection between ultracold Fermi gases and low-density neutron matter from the viewpoint of finite-effective-range corrections.
description: 21 pages, 8 figures
IN03021 Vessagiri Rock B Inscription 1
Creators: name: Wickremasinghe, Don Martino de Zilva
Publisher: name: Zenodo
Year: 2019
Subjects: IN03021
Epigraphia Zeylanica
Vessagiri

description: IN03021 Vessagiri Rock B Inscription 1 - Transcript and Translation Source: Wickremasinghe, Don Martino de Zilva. (1904-12). ‘No. 2. Vessagiri Inscriptions,’ Epigraphia Zeylanica 1, pp. 10-39.
Additional file 1: of Advanced modes of mechanical ventilation and optimal targeting schemes
Creators: name: Staay, Matthias Van Der
name: Chatburn, Robert
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Medicine
subject: Molecular Biology
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Developmental Biology

description: Supplementary material. (DOCX 1009 kb)
Doppler tomography of intermediate polar spin cycles
Creators: name: Hellier, Coel
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: I collect emission line profiles for seven intermediate polars, phase-resolved over the spin cycles. I then present the first systematic application of Doppler tomography to the spin cycles, with the aim of investigating whether spin-cycle tomography is a useful diagnostic tool. Four stars show line emission from material falling onto both magnetic poles of the white dwarf, but three others show line emission from only the upper pole. Tomography can map the extent and shape of the line-emitting accretion curtains, but it can also give misleading results if the line flux changes significantly over the spin cycle.
description: To appear in ApJ Supp, 1999, LaTeX, 7 figures also at http://www.astro.keele.ac.uk/~ch/publist.html
A continuum model of multi-phase reactive transport in igneous systems
Creators: name: Keller, Tobias
name: Suckale, Jenny
Publisher: name: arXiv
Year: 2018
Subjects: subject: Geophysics (physics.geo-ph)
subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: Multi-phase reactive transport processes are ubiquitous in igneous systems. A challenging aspect of modelling igneous phenomena is that they range from solid-dominated porous to liquid-dominated suspension flows and therefore entail a wide spectrum of rheological conditions, flow speeds, and length scales. Most previous models have been restricted to the two-phase limits of porous melt transport in deforming, partially molten rock and crystal settling in convecting magma bodies. The goal of this paper is to develop a framework that can capture igneous system from source to surface at all phase proportions including not only rock and melt but also an exsolved volatile phase. Here, we derive an n-phase reactive transport model building on the concepts of Mixture Theory, along with principles of Rational Thermodynamics and procedures of Non-equilibrium Thermodynamics. Our model operates at the macroscopic system scale and requires constitutive relations for fluxes within and transfers between phases, which are the processes that together give rise to reactive transport phenomena. We introduce a phase- and process-wise symmetrical formulation for fluxes and transfers of entropy, mass, momentum, and volume, and propose phenomenological coefficient closures that determine how fluxes and transfers respond to mechanical and thermodynamic forces. Finally, we demonstrate that the known limits of two-phase porous and suspension flow emerge as special cases of our general model and discuss some ramifications for modelling pertinent two- and three-phase flow problems in igneous systems.
description: Revised preprint submitted for peer-reviewed publication: main text with 8 figures, 1 table; appendix with 3 figures and 2 tables
Parallel plate capacitor analogy of equatorial plasma bubble and associated fringe fields with implications to equatorial valley region irregularities
Creators: name: Mukherjee, Sampath
name: Patra, A. K.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Space Physics (physics.space-ph)
subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: VHF radar echoes from the valley region plasma irregularities, displaying ascending pattern, are often observed during the active phase of equatorial plasma bubble in the close vicinity of the geomagnetic equator and have been attributed to bubble-related fringe field effect. These irregularities however are not observed at a few degrees away from the equator. In this paper, we attempt to understand this contrasting observational result by comparing fringe field at the geomagnetic equator and low latitudes. We use parallel plate capacitor analogy of equatorial plasma bubble and choose a few capacitor configurations, consistent with commonly observed dimension and magnetic field-aligned property of plasma bubble, for computing fringe field. Results show that fringe field decreases significantly with decreasing altitude as expected. Further, fringe field decreases remarkably with latitude, which clearly indicates the role of magnetic field-aligned property of plasma bubble in reducing the magnitude of fringe field at low latitudes compared to that at the geomagnetic equator. The results are presented and discussed in the light of current understanding of plasma bubble-associated fringe field-induced plasma irregularities in the valley region.
description: Publised in JGR: Space Physics
A Prescription for Star Formation Feedback: The Importance of Multiple Shell Interactions
Creators: name: Scalo, John
name: Chappell, David
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The relation between the star formation rate and the kinetic energy increase in a region containing a large number of stellar sources is investigated as a possible prescription for star formation feedback in larger scale galaxy evolution simulations, and in connection with observed scaling relations for molecular clouds, extragalactic giant H II regions, and starburst galaxies. The kinetic energy increase is not simply proportional to the source input rate, but depends on the competition between stellar power input and dissipation due to interactions between structures formed and driven by the star formation. A simple one-zone model is used to show that, in a steady-state, the energy increase should be proportional to the two-thirds power of the stellar energy injection rate, with additional factors depending on the mean density of the region and mean column density of fragments. The scaling relation is tested using two-dimensional pressureless hydrodynamic simulations of wind-driven star formation, in which star formation occurs according to a threshold condition on the column density through a shell, and a large number of shells are present at any one time. The morphology of the simulations resembles an irregular network or web of dynamically-interacting filaments. A set of 16 simulations in which different parameters were varied agree remarkably with the simple analytical prescription for the scaling relation. Converting from wind power of massive stars to Lyman continuum luminosity shows that the cluster wind model for giant H II regions may still be viable.
description: 8 pp, LaTeX, 2 ps figs, mnras.sty, submitted to MNRAS, Revisions and clarifications made in response to referee's comments
Open Spin Chains from Determinant Like Operators in ABJM Theory
Creators: name: Chen, Hui-Huang
name: Ouyang, Hao
name: Wu, Jun-Bao
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We study the mixing problem of the determinant like operators in ABJM theory to two loop order in the scalar sector. The gravity duals of these operators are open strings attached to the maximal giant graviton, which is a D4-brane wrapping a $\mathbb{CP}^2$ inside $\mathbb{CP}^3$ in our case. The anomalous dimension matrix of these operators can be regarded as an open spin chain Hamiltonian. We provide strong evidence of its integrability based on coordinate Bethe ansatz method and boundary Yang-Baxter equation.
description: 11 pages, no figures; v2, typos corrected, references added, 11 pages, no figures; v3 typos fixed, 11 pages, no figures
Additional file 4: of Dynamic changes in ORC localization and replication fork progression during tissue differentiation
Creators: name: Hua, Brian
name: Bell, George
name: Kashevsky, Helena
name: Stetina, Jessica Von
name: Orr-Weaver, Terry
Publisher: name: figshare
Year: 2018
Subjects: subject: Biophysics
subject: 29999 Physical Sciences not elsewhere classified
subject: FOS: Physical sciences
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Neuroscience
subject: Physiology
subject: Pharmacology
subject: Ecology
subject: Immunology
subject: FOS: Clinical medicine
subject: Developmental Biology
subject: Inorganic Chemistry
subject: FOS: Chemical sciences
subject: Computational Biology

description: Figure S3. Comparison of ORC binding in the larval salivary gland (SG) with underreplication. A) aCGH profile of late-3rd-instar larval salivary gland. UR regions in the late-3rd-instar larval salivary gland are denoted as black boxes and are highlighted by green shading. Regions that are underreplicated in other larval tissues but are fully replicated in late-3rd-instar larval salivary gland are denoted as red boxes. The peak summit locations of ORC2 from the salivary gland relative to dm3 genome coordinates are shown (the aCGH and ORC ChIP data are from [8]). B) Comparison of the number of salivary gland ORC2 binding sites per 100 kb within the late-3rd-instar larval salivary gland UR regions relative to fully replicated regions. *p
New Family of Solvable 1D Heisenberg Models
Creators: name: Frahm, Holger
name: Inozemtsev, Vladimir I.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: Starting from a Calogero--Sutherland model with hyperbolic interaction confined by an external field with Morse potential we construct a Heisenberg spin chain with exchange interaction $\propto 1/\sinh^2 x$ on a lattice given in terms of the zeroes of Laguerre polynomials. Varying the strength of the Morse potential the Haldane--Shastry and harmonic spin chains are reproduced. The spectrum of the models in this class is found to be that of a classical one-dimensional Ising chain with nonuniform nearest neighbour coupling in a nonuniform magnetic field which allows to study the thermodynamics in the limit of infinite chains.
description: 8 pp, LaTeX, ITP-UH-07/94
Geometry and Statistics of Cosmic Microwave Polarization
Creators: name: Dolgov, A.
name: Doroshkevich, A.
name: Novikov, D.
name: Novikov, I.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Geometrical and statistical properties of polarization of CMB are analyzed. Singular points of the vector field which describes CMB polarization are found and classified. Statistical distribution of the singularities is studied. A possible signature of tensor perturbations in CMB polarization is discussed. For a further analysis of CMB statistics Minkowski functionals are used, which present a technically simple method to search for deviations from a Gaussian distribution.
description: 37 pages, 5 figures, submitted in Int.J.Mod.Phys. D
Associated Press-NORC Center for Public Affairs Research Poll: Is the Public Willing to Pay to Help Fix Climate Change?
Creators: name: The Energy Policy Institute At The University Of Chicago (EPIC)
Publisher: name: Roper Center for Public Opinion Research
Year: 2019

description: Importance of various issues (6); climate change is/is not happening (1); cause of climate change (1); levels of government responsible for addressing climate change (3); science on climate change (1); influences on views about climate change science (7); electricity bill fee to combat climate change (6); support/oppose taxing use of carbon based fuels (7); support/oppose government freezing mile-per-gallon fuel standards at 2020 levels (2).
Sphinx polymena Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Lepidoptera
Sphingidae
Sphinx
Sphinx polymena

description: Sphinx polymena [spec. nov.]
S. nigra, alis maculis luteis: superiorum tribus, inferiorum duobus, abdomine cingulis binis coccineis.
Habitat in Asia.
Caput nigrum (Antennae deficiebant). Frons alba. Alae nigrae: superiores maculis 3 luteis: intermedia didyma; inferiores maculis 2 luteis. Abdomen atro-caeruleum: Segmento 1 coccineo; 2, 3 caeruleis; 4, 5, 6 coccineis; 7 atro.
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 494, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
title: ADCO, Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome V, Cart. 189 (11 H 74), 316 folios, f. 0144r
Creators: name: de la Côte d'Or, Archives départementales
name: CG21/F.PETOT/2012
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
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: 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. 0144r, 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. 0144r, 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
Additional file 6: of Complete genome of streamlined marine actinobacterium Pontimonas salivibrio strain CL-TW6T adapted to coastal planktonic lifestyle
Creators: name: Cho, Byung
name: Hardies, Stephen
name: Jang, Gwang
name: Hwang, Chung
Publisher: name: figshare
Year: 2018
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Evolutionary Biology
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: Marine Biology
subject: Inorganic Chemistry
subject: FOS: Chemical sciences
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: 60506 Virology

description: Table S4. Distribution of best BlastP matches, %GC, genome size, and numbers of tRNA and rRNA genes in representative Actinobacteria genomes. (DOC 40 kb)
Complete Additivity and Modal Incompleteness
Creators: name: Holliday, Wesley H.
name: Litak, Tadeusz
Publisher: name: arXiv
Year: 2018
Subjects: subject: Logic in Computer Science (cs.LO)
subject: FOS: Computer and information sciences

description: In this paper, we tell a story about incompleteness in modal logic. The story weaves together a paper of van Benthem, `Syntactic aspects of modal incompleteness theorems,' and a longstanding open question: whether every normal modal logic can be characterized by a class of completely additive modal algebras, or as we call them, V-BAOs. Using a first-order reformulation of the property of complete additivity, we prove that the modal logic that starred in van Benthem's paper resolves the open question in the negative. In addition, for the case of bimodal logic, we show that there is a naturally occurring logic that is incomplete with respect to V-BAOs, namely the provability logic GLB. We also show that even logics that are unsound with respect to such algebras do not have to be more complex than the classical propositional calculus. On the other hand, we observe that it is undecidable whether a syntactically defined logic is V-complete. After these results, we generalize the Blok Dichotomy to degrees of V-incompleteness. In the end, we return to van Benthem's theme of syntactic aspects of modal incompleteness.
Quantum Phase Transitions and Localization in Semigroup Fredkin Spin Chain
Creators: name: Padmanabhan, Pramod
name: Sugino, Fumihiko
name: Korepin, Vladimir
Publisher: name: arXiv
Year: 2018
Subjects: subject: Quantum Physics (quant-ph)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: High Energy Physics - Theory (hep-th)
subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: We construct an extended quantum spin chain model by introducing new degrees of freedom to the Fredkin spin chain. The new degrees of freedom called arrow indices are partly associated to the symmetric inverse semigroup $\cS^3_1$. Ground states of the model fall into three different phases, and quantum phase transition takes place at each phase boundary. One of the phases exhibits logarithmic violation of the area law of entanglement entropy and quantum criticality, whereas the other two obey the area law. As an interesting feature arising by the extension, there are excited states due to disconnections with respect to the arrow indices. We show that these states are localized without disorder.
description: 31 pages, 15 figures. arXiv admin note: text overlap with arXiv:1710.10426
Infrared activation of the Higgs mode by supercurrent injection in superconducting NbN
Creators: name: Nakamura, Sachiko
name: Iida, Yudai
name: Murotani, Yuta
name: Matsunaga, Ryusuke
name: Terai, Hirotaka
name: Shimano, Ryo
Publisher: name: arXiv
Year: 2018
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: Higgs mode in superconductors, i.e. the collective amplitude mode of the order parameter does not associate with charge nor spin fluctuations, therefore it does not couple to the electromagnetic field in the linear response regime. On the contrary to this common understanding, here, we demonstrate that, if the dc supercurrent is introduced into the superconductor, the Higgs mode becomes infrared active and is directly observed in the linear optical conductivity measurement. We observed a sharp resonant peak at $ω=2Δ$ in the optical conductivity spectrum of a thin-film NbN in the presence of dc supercurrent, showing a reasonable agreement with the recent theoretical prediction. The method as proven by this work opens a new pathway to study the Higgs mode in a wide variety of superconductors.
description: 5 pages, 4 figures
MOESM1 of Machine learning for the prediction of molecular dipole moments obtained by density functional theory
Creators: name: Pereira, Florbela
name: Aires-De-Sousa, João
Publisher: name: figshare
Year: 2018
Subjects: subject: Biophysics
subject: Biochemistry
subject: Molecular Biology
subject: Physiology
subject: FOS: Biological sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Developmental Biology
subject: Cancer

description: Additional file 1: Figure S1. Graphical representation of the DFT-DM vs. a) DMNBO and b) DMPEOE for the test set. Figure S2. Predicted vs. DFT-calculated DM for the 3368 molecular structures of the test set using the model MACCS_DMNBO_DMPEOE.
Multi-jet merged top-pair production including electroweak corrections
Creators: name: Gütschow, Christian
name: Lindert, Jonas M.
name: Schönherr, Marek
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: We present theoretical predictions for the production of top-quark pairs in association with jets at the LHC including electroweak (EW) corrections. First, we present and compare differential predictions at the fixed-order level for $t \bar t$ and $t \bar t+$jet production at the LHC considering the dominant NLO EW corrections of order $\mathcal{O}(α_S^2 α)$ and $\mathcal{O}(α_S^3 α)$ respectively together with all additional subleading Born and one-loop contributions. The NLO EW corrections are enhanced at large energies and in particular alter the shape of the top transverse momentum distribution, whose reliable modelling is crucial for many searches for new physics at the energy frontier. Based on the fixed-order results we motivate an approximation of the EW corrections valid at the percent level, that allows us to readily incorporate the EW corrections in the MEPS@NLO framework of Sherpa combined with OpenLoops. Subsequently, we present multi-jet merged parton-level predictions for inclusive top-pair production incorporating NLO QCD+EW corrections to $t \bar t$ and $t \bar t+$jet. Finally, we compare at the particle-level against a recent 8 TeV measurement of the top transverse momentum distribution performed by ATLAS in the lepton+jet channel. We find very good agreement between the Monte Carlo prediction and the data when the EW corrections are included.
description: 10 pages, 5 figures
Superconductivity in the Two-Dimensional $t$-$J$ Model at Low Hole Doping
Creators: name: Heeb, Elmar S.
name: Rice, T. Maurice
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: By combining a generalized Lanczos scheme with the variational Monte Carlo method we can optimize the short- and long-range properties of the groundstate separately. This allows us to measure the long-range order of the groundstate of the $t$-$J$ model as a function of the coupling constant $J/t$, and identify a region of finite d-wave superconducting long-range order. With a lattice size of 50 sites we can reliably examine hole densities down to 0.16.
description: 12 pages and 4 PostScript figures, ReVTeX 3.0, ETH-TH/94-15
IN03022 Vessagiri Rock B Inscription 2 - Wickremasinghe (1904-12)
Creators: name: Wickremasinghe, Don Martino de Zilva
Publisher: name: Zenodo
Year: 2019
Subjects: IN03022
Epigraphia Zeylanica
Vessagiri

description: IN03022 Vessagiri Rock B Inscription 2 - Transcript and Translation Source: Wickremasinghe, Don Martino de Zilva. (1904-12). ‘No. 2. Vessagiri Inscriptions,’ Epigraphia Zeylanica 1, pp. 10-39.
Statistical characteristics of formation and evolution of structure in the universe
Creators: name: Demianski, M.
name: Doroshkevich, A.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: An approximate statistical description of the formation and evolution of structure of the universe based on the Zel'dovich theory of gravitational instability is proposed. It is found that the evolution of DM structure shows features of self-similarity and the main structure characteristics can be expressed through the parameters of initial power spectrum and cosmological model. For the CDM-like power spectrum and suitable parameters of the cosmological model the effective matter compression reaches the observed scales $R_{wall}\sim $20 -- 25$h^{-1}$Mpc with the typical mean separation of wall-like elements $D_{SLSS}\sim $50 -- 70$h^{-1}$Mpc. This description can be directly applied to the deep pencil beam galactic surveys and absorption spectra of quasars. For larger 3D catalogs and simulations it can be applied to results obtained with the core-sampling analysis. It is shown that the interaction of large and small scale perturbations modulates the creation rate of early Zel'dovich pancakes and generates bias on the SLSS scale. For suitable parameters of the cosmological model and reheating process this bias can essentially improve the characteristics of simulated structure of the universe. The models with $0.3\leq Ω_m \leq 0.5$ give the best description of the observed structure parameters. The influence of low mass "warm" dark matter particles, such as a massive neutrino, will extend the acceptable range of $Ω_m$ and $h$.
description: 20pages, 7 figures, MNRAS in press
Stellar Population of Ellipticals in Different Environments: Near-infrared Spectroscopic Observations
Creators: name: James, Philip
name: Mobasher, Bahram
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Near-infrared spectra of 50 elliptical galaxies in the Pisces, A2199 and A2634 clusters, and in the general field, have been obtained. The strength of the CO (2.3 micron) absorption feature in these galaxies is used to explore the presence of an intermediate-age population (e.g. Asymptotic Giant Branch stars) in ellipticals in different environments. We find the strongest evidence for such a population comes from ellipticals in groups of a few members, which we interpret as the result of recent minor merging of these galaxies with later type galaxies. Field galaxies from very isolated environments, on the other hand, show no evidence for young or intermediate-age stars as revealed by H beta and CO absorptions, and appear to form a very uniform, old population with very little scatter in metallicity and star formation history.
description: 13 pages, 6 figures, accepted for publication in the Monthly Notices of the Royal Astronomical Society
Flame propagation in random media
Creators: name: Provatas, N.
name: Ala-Nissila, T.
name: Grant, Martin
name: Elder, K. R.
name: Pich, Luc
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: We introduce a phase-field model to describe the dynamics of a self-sustaining propagating combustion front within a medium of randomly distributed reactants. Numerical simulations of this model show that a flame front exists for reactant concentration $c > c^* > 0$, while its vanishing at $c^*$ is consistent with mean-field percolation theory. For $c > c^*$, we find that the interface associated with the diffuse combustion zone exhibits kinetic roughening characteristic of the Kardar-Parisi-Zhang equation.
description: 4, LR5413
Additional file 3: of Dynamic changes in ORC localization and replication fork progression during tissue differentiation
Creators: name: Hua, Brian
name: Bell, George
name: Kashevsky, Helena
name: Stetina, Jessica Von
name: Orr-Weaver, Terry
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Developmental Biology
subject: Inorganic Chemistry
subject: FOS: Chemical sciences
subject: Computational Biology

description: Table S1. Genomic coordinates of underreplicated regions in endocycling larval and adult tissues. The sequence coordinates and cytological positions are shown for the regions called as underreplicated in the five tissues analyzed. A (+) indicates that the region was significantly underreplicated. The last column shows the size of the underreplicated domain. (PDF 312 kb)
Intensity Distribution of Waves Transmitted Through a Multiple Scattering Medium
Creators: name: Nieuwenhuizen, Th. M.
name: van Rossum, M. C. W.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: The distributions of the angular transmission coefficient and of the total transmission are calculated for multiple scattered waves. The calculation is based on a mapping to the distribution of eigenvalues of the transmission matrix. The distributions depend on the profile of the incoming beam. The distribution function of the angular transmission has a stretched exponential decay. The total-transmission distribution grows log-normally whereas it decays exponentially.
description: 8 pages, revtex3.0, 3 postscript figures, NvR01
Additional file 5: of Complete genome of streamlined marine actinobacterium Pontimonas salivibrio strain CL-TW6T adapted to coastal planktonic lifestyle
Creators: name: Cho, Byung
name: Hardies, Stephen
name: Jang, Gwang
name: Hwang, Chung
Publisher: name: figshare
Year: 2018
Subjects: subject: Biophysics
subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Evolutionary Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: Inorganic Chemistry
subject: FOS: Chemical sciences
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Table S3. A pair-wise comparison of selected genomes for (a) in silico DNA-DNA hybridization (DDH), (b) average amino acid identity (AAI), (c) Î´* differences (the average difference of dinucleotide relative abundance), and (d) the percentage of conserved proteins (POCP). 1, Pontimonas salivibrio CL-TW6T; 2, Rhodoluna lacicola MWH-Ta8T; 3, Yonghaparkia sp. Root332; 4, Microcella alkaliphila JAM AC0309; 5, acMicro-4. (PDF 60 kb)
Note on 3-Choosability of Planar Graphs with Maximum Degree 4
Creators: name: Dross, François
name: Lužar, Borut
name: Maceková, Mária
name: Soták, Roman
Publisher: name: arXiv
Year: 2018
Subjects: subject: Combinatorics (math.CO)
subject: FOS: Mathematics
subject: 05C15

description: Deciding whether a planar graph (even of maximum degree $4$) is $3$-colorable is NP-complete. Determining subclasses of planar graphs being $3$-colorable has a long history, but since Grötzsch's result that triangle-free planar graphs are such, most of the effort was focused to solving Havel's and Steinberg's conjectures. In this paper, we prove that every planar graph of maximum degree $4$ obtained as a subgraph of the medial graph of any bipartite plane graph is $3$-choosable. These graphs are allowed to have close triangles (even incident), and have no short cycles forbidden, hence representing an entirely different class than the graphs inferred by the above mentioned conjectures.
Sphinx cassandra Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Lepidoptera
Sphingidae
Sphinx
Sphinx cassandra

description: Sphinx cassandra [spec. nov.]
S. nigra, abdomine utrinque maculis quinque caeruleis, ano ore basique femorum abdominisque coccineis.
Habitat in America.
Statura priorum s. S. Filipendulae. Os sanguineum. Lingua spiralis. Alae nigrae. Puncta thoracis ad alas & basis omnium femorum coccinea. Abdomen atrum, utrinque maculis 5 caeruleis nitidis. Ano sanguineo.
Larvae Sphingum supra anum cornu gerunt, quemadmodum Phalaenae Mori.
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 494, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Spatial Variability in the Ratio of Interstellar Atomic Deuterium to Hydrogen. I. Observations toward delta Orionis by the Interstellar Medium Absorption Profile Spectrograph
Creators: name: Jenkins, Edward B.
name: Tripp, Todd M.
name: Wozniak, Przemyslaw R.
name: Sofia, Ulysses J.
name: Sonneborn, G.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Studies of the abundances of deuterium in different astrophysical sites are of fundamental importance to answering the question about how much deuterium was produced during big bang nucleosynthesis and what fraction of it was destroyed later. With this in mind, we used the Interstellar Medium Absorption Profile Spectrograph (IMAPS) on the ORFEUS-SPAS II mission to observe at a wavelength resolution of 4 km/s (FWHM) the L-delta and L-epsilon absorption features produced by interstellar atomic deuterium in the spectrum of delta Ori A. A chi-square analysis indicated that 0.96 < N(D I)< 1.45e15 cm^{-2} at a 90% level of confidence, and the gas is at a temperature of about 6000K. To obtain an accurate value of N(H I) needed for a determination of the atomic ratio of D to H, we measured the L-alpha absorption features in 57 spectra of delta Ori in the IUE archive. From our measurement of N(H I)= 1.56e20 cm^{-2}, we found that N(D I)/N(H I)= 7.4(+1.9,-1.3)e-6 (90% confidence). Our result for D/H contrasts with the more general finding along other lines of sight that D/H is approximately 1.5e-5. The underabundance of D toward delta Ori A is not accompanied by an overabundance of N or O relative to H, as one might expect if the gas were subjected to more stellar processing than usual.
description: 37 pages, 6 figures. Submitted to the Astrophysical Journal
RECONSTRUCTION OF CONCURRENT CREDITOR RIGHTS IN BANKRUPTCY LAW AND SUSPENSION OF DEBT PAYMENT OBLIGATIONS IN THE FRAMEWORK OF LEGAL DEVELOPMENT
Creators: name: TIMOTIUS TUMBUR SIMBOLON
name: M.S. TUMANGGOR
name: WIWIK SRI WIDIARTY
name: BERNARD NAINGGOLAN
Publisher: name: Zenodo
Year: 2024
Subjects: Reconstruction, Concurrent Creditor, Bankruptcy, and Determinor.

description: Abstract

Debt payment obligation is the principle of justice as stated by Aristoteles, and is one of the important aspects in business transactions. If a debtor fails to fulfill his obligations, legal problem will arise that must be resolved. This research aims to examine and reconstruct the rights of Concurrent Creditors in the Bankruptcy law for the purpose of legal development so as to provide justice to all parties.  This research used normative legal research methods. Data collection techniques used in this research are literature studies and law research. The data analysis technique used in this research is qualitative analysis. The results show that the rights of Concurrent Creditors in the Bankruptcy Law need to be reconstructed in the context of the purpose of legal development. The reconstruction of Concurrent Creditors rights can be made by increasing the understanding and awareness of Concurrent Creditors, improving adequate facilities and infrastructure, and strengthening law enforcement with a new paradigm.
title: ADCO, Cart. 186 (11 H 71), f. 0085r
Creators: name: de la Côte d'Or, Archives départementales
name: Petot, Frédéric
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CBMA/CG21/F.PETOT/2012
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: cartulaire
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge

description: Cartulaire général de Cîteaux, dit de Jean de Cirey, t. II (XVe siècle), tome II, Archives départementales de la Côte-d'Or, C
art. 186 (11 H 71). Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire général de Cîteaux, dit de Jean de Cirey, t. II (XVe siècle), tome II, Archives départementales de la
 Côte-d'Or, Cart. 186 (11 H 71), f. 0085r, 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