cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Damage Spreading During Domain Growth
Creators: name: Graham, I. S.
name: Hernandez-Garcia, E.
name: Grant, M.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: High Energy Physics - Lattice (hep-lat)
subject: FOS: Physical sciences

description: We study damage spreading in models of two-dimensional systems undergoing first order phase transitions. We consider several models from the same non-conserved order parameter universality class, and find unexpected differences between them. An exact solution of the Ohta-Jasnow-Kawasaki model yields the damage growth law $D \sim t^ϕ$, where $ϕ= t^{d/4}$ in $d$ dimensions. In contrast, time-dependent Ginzburg-Landau simulations and Ising simulations in $d= 2$ using heat-bath dynamics show power-law growth, but with an exponent of approximately $0.36$, independent of the system sizes studied. In marked contrast, Metropolis dynamics shows damage growing via $ϕ\sim 1$, although the damage difference grows as $t^{0.4}$. PACS: 64.60.-i, 05.50.+q
description: 4 pags of revtex3 + 3 postscript files appended as a compressed and uuencoded file. UIB9403200
Papilio lucina Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Lepidoptera
Papilionidae
Papilio
Papilio lucina

description: Papilio lucina [spec. nov.]
P. N. alis dentatis fuscis testaceo-maculatis, subtus fasciis duabus macularum albidarum.
Pet. gaz. t. 16. f. 10.
Raj. ins. 122. n. 12.
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 480, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Dispersive approach to non-Abelian axial anomaly
Creators: name: Khlebtsov, Sergey
name: Klopot, Yaroslav
name: Oganesian, Armen
name: Teryaev, Oleg
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Manifestations of strong and electromagnetic axial anomalies in two-photon decays of $η$ and $η'$ mesons are studied. Applying dispersive approach to axial anomaly in the singlet current, we obtain an anomaly sum rule containing strong and electromagnetic anomaly contributions. The relevant low energy theorem was generalized to the case of mixed states and used to evaluate the subtraction constant of the strong anomaly-related form factor $\langle 0 |G\tilde{G} |γγ\rangle$. We made a numerical estimation of the contributions of gluon and electromagnetic anomalies to the two-photon decays of $η$ and $η'$ mesons and found significant suppression of the gluon anomaly contribution.
description: 10 pages
Quantum heat engine operating between thermal and spin reservoirs
Creators: name: Wright, Jackson S. S. T.
name: Gould, Tim
name: Carvalho, André R. R.
name: Bedkihal, Salil
name: Vaccaro, Joan A.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Landauer's erasure principle is a cornerstone of thermodynamics and information theory. According to this principle, erasing information incurs a minimum energy cost. Recently, Vaccaro and Barnett [Proc. R. Soc {\bf 467}, 1770 (2011)] explored information erasure in the context of multiple conserved quantities and showed that the erasure cost can be solely in terms of spin angular momentum. As Landauer's erasure principle plays a fundamental role in heat engines, their result considerably widens the possible configurations that heat engines can have. Motivated by this, we propose here a novel optical heat engine that operates under a single thermal reservoir and a spin angular momentum reservoir coupled to a three level system with an energy-degenerate ground state. The proposed heat engine operates without producing waste heat and goes beyond the traditional Carnot engine where the working fluid is subjected to two thermal baths at different temperatures.
John Frederick Knott - Bibliography from John Frederick Knott. 9 December 1938 — 5 October 2017
Creators: name: Burdekin, Frederick Michael
name: Bowen, Paul
Publisher: name: The Royal Society
Year: 2018
Subjects: subject: 30199 Analytical Chemistry not elsewhere classified
subject: FOS: Chemical sciences

description: John Knott was a leading expert in materials, fracture and structural integrity applied particularly to the fields of nuclear power generation and aero-engine applications. He made significant contributions to the quantitative scientific understanding of fracture processes in metals and alloys and its applications in engineering. His early work elucidated the role of microstructure in the initiation and propagation of cracks and involved detailed analysis of the micro-mechanisms of cleavage, ductile and fatigue fracture modes in many types of steel and non-ferrous alloys. He developed innovative techniques of mechanical testing which allowed detailed monitoring of crack propagation. He was the author of a much-used text book on the principles of fracture mechanics.The wide range of his expertise meant that John Knott was in high demand to serve on advisory committees for both government and industry organizations, particularly in the civil nuclear power generation and aerospace industries. With his deep knowledge of materials behaviour, he was invited to give many prestigious lectures at conferences. He was a convivial character with a keen sense of humour and often entertained conference dinners with poems he had composed about the particular event and about other participants.
Prospects for Heavy Scalar Searches at the LHeC
Creators: name: Rose, Luigi Delle
name: Fischer, Oliver
name: Hammad, A.
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: In this article we study the prospects of the proposed Large Hadron electron Collider (LHeC) in the search for heavy neutral scalar particles. We consider a minimal model with one additional complex scalar singlet that interacts with the Standard Model (SM) via mixing with the Higgs doublet, giving rise to a SM-like Higgs boson $h_1$ and a heavy scalar particle $h_2$. Both scalar particles are produced via vector boson fusion and can be tested via their decays into pairs of SM particles, analogously to the SM Higgs boson. Using multivariate techniques we show that the LHeC is sensitive to $h_2$ with masses between 200 and 800 GeV down to scalar mixing of $\sin^2 α\sim 10^{-3}$.
Papilio maturna Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Lepidoptera
Papilionidae
Papilio
Papilio maturna

description: Papilio maturna [spec. nov.]
P. N. alis dentatis purpurascentibus nigro-maculatis: subtus fasciis tribus flavis.
Merian. eur. t. 88?
Wilk. pap. 58. t. 2. a. 9.
Habitat in Corylo, Erica.
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 480, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
The Horn Problem for Real Symmetric and Quaternionic Self-Dual Matrices
Creators: name: Coquereaux, Robert
name: Zuber, Jean-Bernard
Publisher: name: arXiv
Year: 2018
Subjects: subject: Representation Theory (math.RT)
subject: High Energy Physics - Theory (hep-th)
subject: Mathematical Physics (math-ph)
subject: Combinatorics (math.CO)
subject: FOS: Mathematics
subject: FOS: Physical sciences
subject: 17B08, 17B10, 22E46, 43A75, 52Bxx

description: Horn's problem, i.e., the study of the eigenvalues of the sum $C=A+B$ of two matrices, given the spectrum of $A$ and of $B$, is re-examined, comparing the case of real symmetric, complex Hermitian and self-dual quaternionic $3\times 3$ matrices. In particular, what can be said on the probability distribution function (PDF) of the eigenvalues of $C$ if $A$ and $B$ are independently and uniformly distributed on their orbit under the action of, respectively, the orthogonal, unitary and symplectic group? While the two latter cases (Hermitian and quaternionic) may be studied by use of explicit formulae for the relevant orbital integrals, the case of real symmetric matrices is much harder. It is also quite intriguing, since numerical experiments reveal the occurrence of singularities where the PDF of the eigenvalues diverges. Here we show that the computation of the PDF of the symmetric functions of the eigenvalues for traceless $3\times 3$ matrices may be carried out in terms of algebraic functions;- roots of quartic polynomials;- and their integrals. The computation is carried out in detail in a particular case, and reproduces the expected singular patterns. The divergences are of logarithmic or inverse power type. We also relate this PDF to the (rescaled) structure constants of zonal polynomials and introduce a zonal analogue of the Weyl ${\rm SU}(n)$ characters.
Excitation Spectrum of the Spin-1/2 Ferromagnetic-Antiferromagnetic Alternating Heisenberg Chain:
Creators: name: Hida, Kazuo
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: The natural explanation of the excitation spectrum of the spin-1 antiferromagnetic Heisenberg chain is given from the viewpoint of the spin-1/2 ferromagnetic-antiferromagnetic alternating Heisenberg chain. The energy spectrum of the latter is calculated with fixed momentum $k$ by numerical diagonalization of finite size systems. It consists of a branch of propagating triplet pair (triplet wave) and the continuum of multiple triplet waves for weak ferromagnetic coupling. As the ferromagnetic coupling increases, the triplet wave branch is absorbed in the continuum for small $k$, reproducing the characteristics of the spin-1 antiferromagnetic Heisenberg chain.
description: 12 Pages REVTEX, Postscript file for the figures included. SKPH-94-C001
Copper and Barium Abundances in the Ursa Major Moving Group
Creators: name: Castro, S.
name: de Mello, G. F. Porto
name: da Silva, L.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present Cu and Ba abundances for 7 G-K dwarf stars, members of the solar-metallicity, 0.3 Gyr old Ursa Major Moving Group. All analyzed member stars show [Ba/Fe] excesses of +0.3-plus, associated with [Cu/Fe] deficiencies of up to -0.23 dex. The present results suggest that there is an anti-correlation between the abundances of Cu and the heavy elements produced by the main component of the neutron capture s-process. Other possible anomalies are Na and C deficiencies with respect to normal solar-metallicity stars. The new data do not confirm the recent claim that the group member HR6094 is a Ba dwarf star.
description: 8 pages, 6 figures, accepted to MNRAS
Full- & Reduced-Order State-Space Modeling of Wind Turbine Systems with Permanent-Magnet Synchronous Generator
Creators: name: Hackl, Christoph M.
name: Pfeifer, Martin
name: Schechner, Korbinian
name: Jané-Soneira, Pol
name: Hohmann, Sören
Publisher: name: arXiv
Year: 2018
Subjects: subject: Systems and Control (eess.SY)
subject: FOS: Electrical engineering, electronic engineering, information engineering

description: Wind energy is an integral part of nowadays energy supply and one of the fastest growing sources of electricity in the world today. Accurate models for wind energy conversion systems (WECSs) are of key interest for the analysis and control design of present and future energy systems. Existing control-oriented WECSs models are subject to unstructured simplifications, which have not been discussed in literature so far. Thus, this technical note presents are thorough derivation of a physical state-space model for permanent magnet synchronous generator WECSs. The physical model considers all dynamic effects that significantly influence the system's power output, including the switching of the power electronics. Alternatively, the model is formulated in the $(a,b,c)$- and $(d,q)$-reference frame. Secondly, a complete control and operation management system for the wind regimes II and III and the transition between the regimes is presented. The control takes practical effects such as input saturation and integral windup into account. Thirdly, by a structured model reduction procedure, two state-space models of WECS with reduced complexity are derived: a non-switching model and a non-switching reduced-order model. The validity of the models is illustrated and compared through a numerical simulation study.
description: 23 pages, 11 figures
A Morphological and Multicolor Survey for Faint QSOs in the Groth-Westphal Strip
Creators: name: Beck-Winchatz, Bernhard
name: Anderson, Scott F.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Quasars representative of the populous faint end of the luminosity function are frustratingly dim with m~24 at intermediate redshift; moreover groundbased surveys for such faint QSOs suffer substantial morphological contamination by compact galaxies having similar colors. In order to establish a more reliable ultrafaint QSO sample, we used the APO 3.5-m telescope to take deep groundbased U-band CCD images in fields previously imaged in V,I with WFPC2/HST. Our approach hence combines multicolor photometry with the 0.1" spatial resolution of HST, to establish a morphological and multicolor survey for QSOs extending about 2 magnitudes fainter than most extant groundbased surveys. We present results for the "Groth-Westphal Strip", in which we identify 10 high likelihood UV-excess candidates having stellar or stellar-nucleus+galaxy morphology in WFPC2. For m(606)<24.0 (roughly B<24.5) the surface density of such QSO candidates is 420 (+180,-130) per square degree, or a surface density of 290 (+160,-110) per square degree with an additional V-I cut that may further exclude compact emission line galaxies. Even pending confirming spectroscopy, the observed surface density of QSO candidates is already low enough to yield interesting comparisons: our measures agree extremely well with the predictions of several recent luminosity function models.
description: 29 pages including 6 tables and 7 figures. As accepted for publication in The Astronomical Journal (minor revisions)
Better figures for natural sciences
Creators: name: Jambor, Helena
Publisher: name: figshare
Year: 2018
Subjects: subject: Uncategorized
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences

description: For every research finding, scientists find a figure that supports their claims. Visual communication and data visualization strategies are however rarely taught. Here are a couple of tipps and tricks for producing visualizations that communicate research results.
Spin Susceptibility and Gap Structure of the Fractional-Statistics Gas
Creators: name: Levy, J. L.
name: Laughlin, R. B.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: This paper establishes and tests procedures which can determine the electron energy gap of the high-temperature superconductors using the $t\!-\!J$ model with spinon and holon quasiparticles obeying fractional statistics. A simpler problem with similar physics, the spin susceptibility spectrum of the spin 1/2 fractional-statistics gas, is studied. Interactions with the density oscillations of the system substantially decrease the spin gap to a value of $(0.2 \pm 0.2)$ $\hbar ω_c$, much less than the mean-field value of $\hbarω_c$. The lower few Landau levels remain visible, though broadened and shifted, in the spin susceptibility. As a check of the methods, the single-particle Green's function of the non-interacting Bose gas viewed in the fermionic representation, as computed by the same approximation scheme, agrees well with the exact results. The same mechanism would reduce the gap of the $t\!-\!J$ model without eliminating it.
description: 35 pages, written in REVTeX, 16 figures available upon request from jared@large.stanford.edu
BioFuse Embedding Cache for MedMNIST+ 2D Datasets
Creators: name: Hossain, Mirza Nasir
name: Harris-Birtill, David
Publisher: name: Zenodo
Year: 2025

description: # BioFuse Embedding Cache for MedMNIST+

This dataset contains comprehensive embedding vectors extracted from 10 foundation models (9 biomedical and CLIP) across all 12 MedMNIST+ datasets, as described in our paper "BioFuse: An embedding fusion framework for biomedical foundation models."

## Contents- Embedding vectors stored as pickle (.pkl) files for each foundation model and dataset combination- Files are organized using the naming convention: `{dataset}_{model}_{resolution}_{split}.pkl`- All embeddings are generated from 224x224 resolution images- Each dataset includes separate files for train, validation, and test splits

## File Structure Example

organamnist_CheXagent_224_train.pklorganamnist_CheXagent_224_val.pklorganamnist_CheXagent_224_test.pkl

## Models IncludedEmbeddings from the following foundation models are included:- BioMedCLIP- PubMedCLIP- CONCH- rad-dino- UNI- UNI2- Hibou-B- Prov-GigaPath- CheXagent- CLIP

## Datasets IncludedEmbeddings for all 12 MedMNIST+ datasets:- PathMNIST- ChestMNIST- DermaMNIST- OCTMNIST- PneumoniaMNIST- RetinaMNIST- BreastMNIST- BloodMNIST- TissueMNIST- OrganAMNIST- OrganCMNIST- OrganSMNIST## UsageThese embeddings can be used to:1. Reproduce the results reported in our paper2. Explore alternative fusion strategies beyond those investigated in our work3. Analyze cross-modal capabilities of biomedical foundation models4. Benchmark new fusion approaches without re-extracting embeddings5. Investigate feature representations across different medical imaging modalities6. Compare performance between general-purpose and biomedical foundation models

## CitationIf you use these embeddings in your research, please cite our paper "BioFuse: An embedding fusion framework for biomedical foundation models" (citation details will be added upon publication).
Interplaying mechanisms behind single inclusive jet suppression in heavy-ion collisions
Creators: name: He, Yayun
name: Cao, Shanshan
name: Chen, Wei
name: Luo, Tan
name: Pang, Long-Gang
name: Wang, Xin-Nian
Publisher: name: arXiv
Year: 2018
Subjects: subject: Nuclear Theory (nucl-th)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The suppression factor for single inclusive jets in Pb+Pb collisions at the Large Hadron Collider (LHC) has a weak dependence on the transverse momentum $p_T$ and remains almost the same at two colliding energies, $\sqrt{s}=2.76$ and 5.02 TeV, though the central rapidity density of bulk hadrons increases by about 20\%. This phenomenon is investigated within the Linear Boltzmann Transport (LBT) model, which includes elastic and inelastic processes based on perturbative QCD for both jet shower and recoil medium partons as they propagate through a quark-gluon plasma (QGP). With the dynamic evolution of the QGP given by the 3+1D CLVisc hydrodynamic model with event-by-event fully fluctuating initial conditions, single inclusive jet suppression in Pb+Pb collisions from LBT agrees well with experimental data. The weak $\sqrt{s}$ and $p_T$-dependence of the jet suppression factor at LHC are found to result directly from the $\sqrt{s}$-dependence of the initial jet $p_T$ spectra and slow $p_T$-dependence of the jet energy loss. Contributions from jet-induced medium response, influence of radial expansion, both of which depend on jet-cone size, and jet flavor composition all conjoin to give a slow $p_T$-dependence of jet energy loss and the single jet suppression factor $R_{\rm AA}$, their dependence on $\sqrt{s}$ and jet-cone size. Single inclusive jet suppression at $\sqrt{s}=200$ GeV is also predicted that actually decreases slightly with $p_T$ in the $p_T<50$ GeV/$c$ range because of the steeper initial jet spectra though the $p_T$-dependence of the jet energy loss is weaker than that at LHC.
description: 22 pages in ReVTeX with 29 figures, final version to appear in PRC
Selection and processing of calibration samples to measure the particle identification performance of the LHCb experiment in Run 2
Creators: name: Aaij, Roel
name: Anderlini, Lucio
name: Benson, Sean
name: Cattaneo, Marco
name: Charpentier, Philippe
name: Clemencic, Marco
name: Falabella, Antonio
name: Ferrari, Fabio
name: Fontana, Marianna
name: Gligorov, Vladimir
name: Hill, Donal
name: Humair, Thibaud
name: Jones, Christopher Robert
name: Lupton, Oliver
name: Malde, Sneha
name: Benito, Carla Marin
name: Matev, Rosen
name: Pearce, Alex
name: Poluektov, Anton
name: Sciascia, Barbara
name: Stagni, Federico
name: Gomez, Ricardo Vazquez
name: Zhang, Yanxi
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: Since 2015, with the restart of the LHC for its second run of data taking, the LHCb experiment has been empowered with a dedicated computing model to select and analyse calibration samples to measure the performance of the particle identification (PID) detectors and algorithms. The novel technique was developed within the framework of the innovative trigger model of the LHCb experiment, which relies on online event reconstruction for most of the datasets, reserving offline reconstruction to special physics cases. The strategy to select and process the calibration samples, which includes a dedicated data-processing scheme combining online and offline reconstruction, is discussed. The use of the calibration samples to measure the detector PID performance, and the efficiency of PID requirements across a large range of decay channels, is described. Applications of the calibration samples in data-quality monitoring and validation procedures are also detailed.
Backreaction effects of dissipation in neutrino decoupling
Creators: name: Maartens, Roy
name: Triginer, Josep
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Dissipative effects during neutrino decoupling in the early universe create a small backreaction on the Hubble rate, and lead to a small rise in temperature and entropy. We use a simplified thermo-hydrodynamic model, which provides a causal approximation to kinetic theory, in order to estimate the backreaction effects and the entropy production.
description: Version accepted by Gen. Rel. Grav
title: ADCO, Grènetier de Cîteaux : comptes (1497-1504) (11 H 1172), f. 00563
Creators: name: de la Côte-d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CBMA/CG21/F.PETOT/2019
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: comptes

description: Grènetier de Cîteaux : comptes (1497-1504), Archives départementales de la Côte-d'Or, (11 H 1172). Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Grènetier de Cîteaux : comptes (1497-1504), Archives départementales de la Côte-d'Or, (11 H 1172), f. 00563, 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
The Electron-Phonon Interaction in the Presence of Strong Correlations
Creators: name: Grilli, M.
name: Castellani, C.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: We investigate the effect of strong electron-electron repulsion on the electron-phonon interaction from a Fermi-liquid point of view: the strong interaction is responsible for vertex corrections, which are strongly dependent on the $v_Fq/ω$ ratio. These corrections generically lead to a strong suppression of the effective coupling between quasiparticles mediated by a single phonon exchange in the $v_Fq/ω\gg 1$ limit. However, such effect is not present when $v_Fq/ω\ll 1$. Analyzing the Landau stability criterion, we show that a sizable electron-phonon interaction can push the system towards a phase-separation instability. A detailed analysis is then carried out using a slave-boson approach for the infinite-U three-band Hubbard model. In the presence of a coupling between the local hole density and a dispersionless optical phonon, we explicitly confirm the strong dependence of the hole-phonon coupling on the transferred momentum versus frequency ratio. We also find that the exchange of phonons leads to an unstable phase with negative compressibility already at small values of the bare hole-phonon coupling. Close to the unstable region, we detect Cooper instabilities both in s- and d-wave channels supporting a possible connection between phase separation and superconductivity in strongly correlated systems.
description: LateX 3.14, 04.11.1994 Preprint no.1012
Analytical Modeling of the Weak Lensing of Standard Candles I. Empirical Fitting of Numerical Simulation Results
Creators: name: Wang, Yun
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Weak lensing leads to the non-Gaussian magnification distribution of standard candles at given redshift $z$, $p(μ|z)$. In this paper, we give accurate and simple empirical fitting formulae of the weak lensing numerical simulation results with the generalized Dyer-Roeder prescription. The smoothness parameter $\tildeα$ essentially represents the amount of matter that can cause magnification of a given source. Since matter distribution in our universe is inhomogeneous, we can think of our universe as a mosaic of cones centered on the observer, each with a different value of $\tildeα$. We define the {\it direction dependent} smoothness parameter $\tildeα$ via the Dyer-Roeder equation; there is a unique mapping between $\tildeα$ and the magnification of a source. We find that the distribution of $\tildeα$ at given $z$, $p(\tildeα|z)$, is well described by a modified Gaussian distribution. For the same matter distribution, i.e., the same $p(\tildeα|z)$, different values of $Ω_m$ and $Ω_Λ$ can lead to very different magnification distributions. Our formulae can be conveniently used to calculate the weak lensing effects for observed Type Ia supernovae at arbitrary redshifts.
description: 24 pages including 12 figures. Extensive wording changes for clarification, main results unchanged. To apper in ApJ, November 10, 1999, issue, Volume 525 #2
Stress effects in structure formation
Creators: name: Maartens, Roy
name: Triginer, Josep
name: Matravers, David
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Residual velocity dispersion in cold dark matter induces stresses which lead to effects that are absent in the idealized dust model. A previous Newtonian analysis showed how this approach can provide a theoretical foundation for the phenomenological adhesion model. We develop a relativistic kinetic theory generalization which also incorporates the anisotropic velocity dispersion that will typically be present. In addition to density perturbations, we consider the rotational and shape distortion properties of clustering. These quantities together characterize the linear development of density inhomogeneity, and we find exact solutions for their evolution. As expected, the corrections are small and arise only in the decaying modes, but their effect is interesting. One of the modes for density perturbations decays less rapidly than the standard decaying mode. The new rotational mode generates precession of the axis of rotation. The new shape modes produce additional distortion that remains frozen in during the subsequent (linear) evolution, despite the rapid decay of the terms that caused it.
description: significantly improved discussion of kinetic theory of CDM velocity dispersion; to appear Phys. Rev. D
Static chaos and scaling behaviour in the spin-glass phase
Creators: name: Ritort, Felix
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: We discuss the problem of static chaos in spin glasses. In the case of magnetic field perturbations, we propose a scaling theory for the spin-glass phase. Using the mean-field approach we argue that some pure states are suppressed by the magnetic field and their free energy cost is determined by the finite-temperature fixed point exponents. In this framework, numerical results suggest that mean-field chaos exponents are probably exact in finite dimensions. If we use the droplet approach, numerical results suggest that the zero-temperature fixed point exponent $θ$ is very close to $\frac{d-3}{2}$. In both approaches $d=3$ is the lower critical dimension in agreement with recent numerical simulations.
description: 28 pages + 6 figures, LateX, figures uuencoded at the end of file
The Relative Orientation of Nuclear Accretion and Galaxy Stellar Disks in Seyfert Galaxies
Creators: name: Nagar, Neil M.
name: Wilson, Andrew S.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We use the difference (delta) between the position angles of the nuclear radio emission and the host galaxy major axis to investigate the distribution of the angle (beta) between the axes of the nuclear accretion disk and the host galaxy disk in Seyfert galaxies. We provide a critical appraisal of the quality of all measurements, and find that the data are limited by observational uncertainties and biases, such as the well known deficiency of Seyfert galaxies of high inclination. There is weak evidence that the distribution of delta for Seyfert 2 galaxies may be different (at the 90% confidence level) from a uniform distribution, while the Seyfert 1 delta distribution is not significantly different from a uniform distribution or from the Seyfert 2 delta distribution. The cause of the possible non-uniformity in the distribution of delta for Seyfert 2 galaxies is discussed. Seyfert nuclei in late-type spiral galaxies may favor large values of delta (at the ~96% confidence level), while those in early-type galaxies show a more or less random distribution of delta. This may imply that the nuclear accretion disk in non-interacting late-type spirals tends to align with the stellar disk, while that in early-type galaxies is more randomly oriented, perhaps as a result of accretion following a galaxy merger. We point out that biases in the distribution of inclination translate to biased estimates of beta in the context of the unified scheme. When this effect is taken into account, the distributions of beta for all Seyferts together, and of Seyfert 1's and 2's separately, agree with the hypothesis that the radio jets are randomly oriented with respect to the galaxy disk. The data are consistent with the expectations of the unified scheme, but do not demand it.
description: To appear in the Astrophysical Journal, Vol 516 #1, May 1, 1999. Corrected figure placement within paper
Better figures for life sciences
Creators: name: Jambor, Helena
Publisher: name: figshare
Year: 2018
Subjects: subject: Uncategorized
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences

description: For every research finding, scientists find a figure that supports their claims. Visual communication and data visualization strategies are however rarely taught. Here are a couple of tipps and tricks for producing visualizations that communicate research results.
Phase-Locking in Strongly Coupled Squid Cells
Creators: name: Basler, M.
name: Krech, W.
name: Platov, K. Yu.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: Within the RSJ model we performed an analytical and numerical investigation of SQUID cells consisting of two Josephson junctions shunted by an extremely small inductance leading to strong coupling of the elements. Contrary to the well-known behavior of cells shunted by a high inductance voltage phases of the junctions are locked with very small phase difference for almost all values of external flux. Only for external flux in the vicinity of half a flux quantum phase difference rises rapidly to $π$.
description: 11 pages, LaTeX, report JENA-FKS-94-2
Ultra High Energy Neutrinos from Supernova Remnants
Creators: name: Roy, Mou
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: In this paper we discuss possible ultra high energy ($\ge$ TeV) neutrino emission from Supernova Remnants (SNRs), specifically the hadronic gamma ray production models. Recent very high energy (VHE) $γ$ ray observation from SNRs is the main motivation behind this study.
description: 6 pages, 3 figures, uses revtex
Additional file 1 of Clinicopathological heterogeneity between primary and metastatic sites of gastroenteropancreatic neuroendocrine neoplasm
Creators: name: Shi, Huiying
name: Jiang, Chen
name: Zhang, Qin
name: Qi, Cuihua
name: Yao, Hailing
name: Lin, Rong
Publisher: name: figshare
Year: 2020
Subjects: Cell Biology
Biotechnology
Biological Sciences not elsewhere classified
Cancer

description: Additional file 1: Supplementary Table 1. CgA, Syn and grading in patients between primary and metastatic sites.
Papilio cinxia Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Lepidoptera
Papilionidae
Papilio
Papilio cinxia

description: Papilio cinxia [spec. nov.]
P. N. alis dentatis fulvis nigro-maculatis: subtus fasciis tribus flavis.
Fn. svec. 783. Comes.
Wilk. pap. 58. t. 3. a. 8.
Habitat in Veronica, Plantagine, Trifolio, Gramine.
Mas elinguis; Femina vero lingua spirali. Rolander.
Fritillarii vulgo dicti 132 ad 144, qvum alae maculis fere tessellatae sint; sed 138 ad 144 ob maculas argenteas Nobiles communiter nominati sunt.
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 480, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
H0LiCOW - IX. Cosmographic analysis of the doubly imaged quasar SDSS 1206+4332 and a new measurement of the Hubble constant
Creators: name: Birrer, S.
name: Treu, T.
name: Rusu, C. E.
name: Bonvin, V.
name: Fassnacht, C. D.
name: Chan, J. H. H.
name: Agnello, A.
name: Shajib, A. J.
name: Chen, G. C. -F.
name: Auger, M.
name: Courbin, F.
name: Hilbert, S.
name: Sluse, D.
name: Suyu, S. H.
name: Wong, K. C.
name: Marshall, P.
name: Lemaux, B. C.
name: Meylan, G.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We present a blind time-delay strong lensing (TDSL) cosmographic analysis of the doubly imaged quasar SDSS 1206+4332. We combine the relative time delay between the quasar images, Hubble Space Telescope imaging, the Keck stellar velocity dispersion of the lensing galaxy, and wide-field photometric and spectroscopic data of the field to constrain two angular diameter distance relations. The combined analysis is performed by forward modelling the individual data sets through a Bayesian hierarchical framework, and it is kept blind until the very end to prevent experimenter bias. After unblinding, the inferred distances imply a Hubble constant $H_0 = 68.8^{+5.4}_{-5.1}$ kms$^{-1}$Mpc$^{-1}$, assuming a flat Lambda cold dark matter cosmology with uniform prior on $Ω_{\rm m}$ in [0.05, 0.5]. The precision of our cosmographic measurement with the doubly imaged quasar SDSS 1206+4332 is comparable with those of quadruply imaged quasars and opens the path to perform on selected doubles the same analysis as anticipated for quads. Our analysis is based on a completely independent lensing code than our previous three H0LiCOW systems and the new measurement is fully consistent with those. We provide the analysis scripts paired with the publicly available software to facilitate independent analysis. The consistency between blind measurements with independent codes provides an important sanity check on lens modelling systematics. By combining the likelihoods of the four systems under the same prior, we obtain $H_0 = 72.5^{+2.1}_{-2.3}$kms$^{-1}$Mpc$^{-1}$. This measurement is independent of the distance ladder and other cosmological probes.
description: 30 pages, 17 figures, MNRAS published likelihood available here: http://shsuyu.github.io/H0LiCOW/site/notebooks/H0_from_lenses.html, all modeling and analysis scripts available upon request
Accessing scrambling using matrix product operators
Creators: name: Xu, Shenglong
name: Swingle, Brian
Publisher: name: arXiv
Year: 2018
Subjects: subject: Quantum Physics (quant-ph)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Scrambling, a process in which quantum information spreads over a complex quantum system becoming inaccessible to simple probes, happens in generic chaotic quantum many-body systems, ranging from spin chains, to metals, even to black holes. Scrambling can be measured using out-of-time-ordered correlators (OTOCs), which are closely tied to the growth of Heisenberg operators. In this work, we present a general method to calculate OTOCs of local operators in local one-dimensional systems based on approximating Heisenberg operators as matrix-product operators (MPOs). Contrary to the common belief that such tensor network methods work only at early times, we show that the entire early growth region of the OTOC can be captured using an MPO approximation with modest bond dimension. We analytically establish the goodness of the approximation by showing that if an appropriate OTOC is close to its initial value, then the associated Heisenberg operator has low entanglement across a given cut. We use the method to study scrambling in a chaotic spin chain with $201$ sites. Based on this data and OTOC results for black holes, local random circuit models, and non-interacting systems, we conjecture a universal form for the dynamics of the OTOC near the wavefront. We show that this form collapses the chaotic spin chain data over more than fifteen orders of magnitude.
description: 14 pages, 9 figures
Towards the determination of heavy-quark transport coefficients in quark-gluon plasma
Creators: name: Cao, Shanshan
name: Coci, Gabriele
name: Das, Santosh Kumar
name: Ke, Weiyao
name: Liu, Shuai Y. F.
name: Plumari, Salvatore
name: Song, Taesoo
name: Xu, Yingru
name: Aichelin, Jörg
name: Bass, Steffen
name: Bratkovskaya, Elena
name: Dong, Xing
name: Gossiaux, Pol Bernard
name: Greco, Vincenzo
name: He, Min
name: Nahrgang, Marlene
name: Rapp, Ralf
name: Scardina, Francesco
name: Wang, Xin-Nian
Publisher: name: arXiv
Year: 2018
Subjects: subject: Nuclear Theory (nucl-th)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: Several transport models have been employed in recent years to analyze heavy-flavor meson spectra in high-energy heavy-ion collisions. Heavy-quark transport coefficients extracted from these models with their default parameters vary, however, by up to a factor of 5 at high momenta. To investigate the origin of this large theoretical uncertainty, a systematic comparison of heavy-quark transport coefficients is carried out between various transport models. Within a common scheme devised for the nuclear modification factor of charm quarks in a brick medium of a quark-gluon plasma, the systematic uncertainty of the extracted drag coefficient among these models is shown to be reduced to a factor of 2, which can be viewed as the smallest intrinsic systematical error band achievable at present time. This indicates the importance of a realistic hydrodynamic evolution constrained by bulk hadron spectra and of heavy-quark hadronization for understanding the final heavy-flavor hadron spectra and extracting heavy-quark drag coefficient. The transverse transport coefficient is less constrained due to the influence of the underlying mechanism for heavy-quark medium interaction. Additional constraints on transport models such as energy loss fluctuation and transverse-momentum broadening can further reduce theoretical uncertainties in the extracted transport coefficients.
description: 20 pages in ReVTex with 11 figures, final version to appear in PRC
title: ADCO, Cartulaire des Dominicains de Dijon (1286), Cart. 221 (H 53), 170 folios, f. 0174
Creators: name: de la Côte d'Or, Archives départementales
name: Petot, Frédéric
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2012
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: cartulaire
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge

description: Cartulaire des Dominicains de Dijon (1286), Archives départementales de la Côte-d'Or, Cart. 221 (H 53), 170 folios. Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire des Dominicains de Dijon (1286), Archives départementales de la Côte-d'Or, Cart. 221 (H 53), 170 folios, f. 0174, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb15250518p
description: Provenance: http://www.idref.fr/02643413X/id
description: Provenance: https://www.geonames.org/6453767
description: Provenance: Dijon
description: Provenance: http://www.wikidata.org/entity/Q7003
Inclusive electron-nucleus cross section within the Self Consistent Green's Function approach
Creators: name: Rocco, N.
name: Barbieri, C.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Nuclear Theory (nucl-th)
subject: High Energy Physics - Experiment (hep-ex)
subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: We compute inclusive electron-nucleus cross sections using ab initio spectral functions of $^4$He and $^{16}$O obtained within the Self Consistent Green's Function approach. The formalism adopted is based on the factorization of the spectral function and the nuclear transition matrix elements. This allows to provide an accurate description of nuclear dynamics and to account for relativistic effects in the interaction vertex. Our calculations use a saturating chiral Hamiltonian in order reproduce the correct nuclear sizes. When final state interactions for the struck particle are accounted for, we find nice agreement between the data and the theory for the inclusive electron-$^{16}$O cross section. The results lay the foundations for future applications of the Self Consistent Green's Function method, in both closed and open shell nuclei, to neutrino data analysis. This work also presents results for the point-proton, charge and single-nucleon momentum distribution of the same two nuclei. The center of mass can affect these quantities for light nuclei and cannot be separated cleanly in most ab initio post-Hartree-Fock methods. In order to address this, we developed a Metropolis Monte Carlo calculation in which the center of mass coordinate can be subtracted exactly from the trial wave function and the expectation values. We gauged this effect for $^4$He by removing the center of mass effect from the Optimal Reference State wave function that is generated during the Self Consistent Green's Function calculations. Our findings clearly indicate that the residual center of mass contribution strongly modifies calculated matter distributions with respect to those obtained in the intrinsic frame. Hence, its subtraction is crucial for a correct description of light nuclei.
description: 12 pages, 10 figures
Dust abundance and grain size in galaxy halos
Creators: name: Hirashita, Hiroyuki
name: Lin, Chih-Yu
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We investigate the abundance and properties (especially, grain size) of dust in galaxy halos using available observational data in the literature. There are two major sets of data. One is (i) the reddening curves at redshifts $z\sim 1$ and 2 derived for Mg II absorbers, which are assumed to trace the medium in galaxy halos. The other is (ii) the cosmic extinction up to $z\sim 2$ mainly traced by distant background quasars. For (i), the observed reddening curves favor a grain radius of $a\sim 0.03~μ$m for silicate, while graphite is not supported because of its strong 2175 Å bump. Using amorphous carbon improves the fit to the reddening curves compared with graphite if the grain radius is $a\lesssim 0.03~μ$m. For (ii), the cosmic extinction requires $η\gtrsim 10^{-2}$ ($η$ is the ratio of the halo dust mass to the stellar mass; the observationally suggested value is $η\sim 10^{-3}$) for silicate if $a\sim 0.03~μ$m as suggested by the reddening curve constraint. Thus, for silicate, we do not find any grain radius that satisfies both (i) and (ii) unless the halo dust abundance is much larger than suggested by the observations. For amorphous carbon, in contrast, a wide range of grain radius ($a\sim 0.01$--0.3~$μ$m) is accepted by the cosmic extinction; thus, we find that a grain radius range of $a\sim 0.01$--0.03 $μ$m is supported by combining (i) and (ii). We also discuss the origin of dust in galaxy halos, focusing on the importance of grain size in the physical mechanism of dust supply to galaxy halos.
description: 13 pages, 9 figures, accepted for publication in Planetary and Space Science (special issue for Cosmic Dust X)
Nonlinear Viscous Vortex Motion in Two-Dimensional Josephson-Junction Arrays
Creators: name: Hagenaars, T. J.
name: Tiesinga, P. H. E.
name: van Himbergen, J. E.
name: José, Jorge V.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: When a vortex in a two-dimensional Josephson junction array is driven by a constant external current it may move as a particle in a viscous medium. Here we study the nature of this viscous motion. We model the junctions in a square array as resistively and capacitively shunted Josephson junctions and carry out numerical calculations of the current-voltage characteristics. We find that the current-voltage characteristics in the damped regime are well described by a model with a {\bf nonlinear} viscous force of the form $F_D=η(\dot y)\dot y={{A}\over {1+B\dot y}}\dot y$, where $\dot y$ is the vortex velocity, $η(\dot y)$ is the velocity dependent viscosity and $A$ and $B$ are constants for a fixed value of the Stewart-McCumber parameter. This result is found to apply also for triangular lattices in the overdamped regime. Further qualitative understanding of the nature of the nonlinear friction on the vortex motion is obtained from a graphic analysis of the microscopic vortex dynamics in the array. The consequences of having this type of nonlinear friction law are discussed and compared to previous theoretical and experimental studies.
description: 14 pages RevTex, 9 Postscript figures