cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Resistivity in the Vicinity of a Van Hove Singularity: Sr$_2$RuO$_4$ Under Uniaxial Pressure
Creators: name: Barber, Mark E.
name: Gibbs, Alexandra S.
name: Maeno, Yoshiteru
name: Mackenzie, Andrew P.
name: Hicks, Clifford W.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We report the results of a combined study of the normal state resistivity and superconducting transition temperature $T_c$ of the unconventional superconductor Sr$_2$RuO$_4$ under uniaxial pressure. There is strong evidence that as well as driving $T_c$ through a maximum at $\sim$3.5 K, compressive strains $\varepsilon$ of nearly 1 % along the crystallographic [100] axis drive the $γ$ Fermi surface sheet through a Van Hove singularity, changing the temperature dependence of the resistivity from $T^2$ above and below the transition region to $T^{1.5}$ within it. This occurs in extremely pure single crystals in which the impurity contribution to the resistivity is $
title: ADCO, Second cartulaire de Saint-Étienne de Dijon (XVe siècle), Cart. 22 (G 126), 110 folios, f. 0016
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2012
name: Petot, Frédéric
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire
subject: LaMOP

description: Second cartulaire de Saint-Étienne de Dijon (XVe siècle), Archives départementales de la Côte-d'Or, Cart. 22 (G 126), 110 folios, f. 0016, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Second cartulaire de Saint-Étienne de Dijon (XVe siècle), Archives départementales de la Côte-d'Or, Cart. 22 (G 126), 110 folios, f. 0016, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https://manuscrits.cbma-project.eu/
description: Provenance: abbaye Saint-Étienne de Dijon
description: Provenance: http://www.wikidata.org/entity/Q15945019
Snapshot Identification of Gamma Ray Burst Optical Afterglows
Creators: name: Rhoads, James E.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Gamma ray burst afterglows can be identified in single epoch observations using three or more optical filters. This method relies on color measurements to distinguish the power law spectrum of an afterglow from the curved spectra of stars. Observations in a fourth filter will further distinguish between afterglows and most galaxies up to redshifts z ~ 1. Many afterglows can also be identified with fewer filters using ultraviolet excess, infrared excess, or Lyman break techniques. By allowing faster identification of gamma ray burst afterglows, these color methods will increase the fraction of bursts for which optical spectroscopy and other narrow-field observations can be obtained. Because quasar colors can match those of afterglows, the maximum error box size where an unambiguous identification can be expected is set by the flux limit of the afterglow search and the quasar number-flux relation. For currently typical error boxes (10 -- 100 square arcminutes), little contamination is expected at magnitudes R < 21.5 +- 0.5. Archival data demonstrates that the afterglow of GRB 000301C could have been identified using this method. In addition to finding gamma ray burst counterparts, this method will have applications in ``orphan afterglow'' searches used to constrain gamma ray burst collimation.
description: 9 pages; LaTeX manuscript + 5 postscript files comprising 4 figures. Revised version accepted to The Astrophysical Journal. The most important change from submitted manuscript is an expanded discussion of single-color UV excess and IR excess afterglow identification techniques
On the "Matrix Approach" to interacting particle systems
Creators: name: De Sanctis, Luca
name: Isopi, Marco
Publisher: name: arXiv
Year: 2006
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: Derrida et al. and Schütz and Stinchcombe gave algebraic formulas for the correlation functions of the partially asymmetric simple exclusion process. Here we give a fairly general recipe of how to get these formulas and extend them to the whole time evolution (starting from the generator of the process), for a certain class of interacting systems. We then analyze the algebraic relations obtained to show that the matrix approach does not work with some models such as the voter and the contact processes.
description: 14 pages; written in 2000
Supplementary material from "Direct synthesis, characterization, in vitro and in silico studies of simple chalcones as potential antibacterial, antifungal, and antileishmanial agents"
Creators: name: Rashid, Haroon
name: Khan,, Sherwali
name: .., Irum
name: Khan, Asad
name: Ahmad, Nasir
name: Khan, Khalid
Publisher: name: figshare
Year: 2024
Subjects: classificationCode: 340503
subject: Organic chemical synthesis
classificationCode: 340701
subject: Computational chemistry
classificationCode: 340401
subject: Biologically active molecules

description: Not applicable
Chasing the peak: optimal statistics for weak shear analyses
Creators: name: Smit, Merijn
name: Kuijken, Konrad
Publisher: name: arXiv
Year: 2017
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Weak gravitational lensing analyses are fundamentally limited by the intrinsic, non-Gaussian distribution of galaxy shapes. We explore alternative statistics for samples of ellipticity measurements that are unbiased, efficient, and robust. We take the non-linear mapping of gravitational shear and the effect of noise into account. We then discuss how the distribution of individual galaxy shapes in the observed field of view can be modeled by fitting Fourier modes to the shear pattern directly. We simulated samples of galaxy ellipticities, using both theoretical distributions and real data for ellipticities and noise. We determined the possible bias $Δe$, the efficiency $η$ and the robustness of the least absolute deviations, the biweight, and the convex hull peeling estimators, compared to the canonical weighted mean. Using these statistics for regression, we have shown the applicability of direct Fourier mode fitting. These estimators can be unbiased in the absence of noise, and decrease noise bias by more than $\sim 30\%$. The convex hull peeling estimator distribution is centered around the underlying shear, and its bias least affected by noise. The least absolute deviations estimator to be the most efficient estimator in almost all cases, except in the Gaussian case, where it's still competitive ($0.83
description: 22 pages, 16 figures, accepted for publication in A&A
Additional file 1: of Quantitative background parenchymal uptake on molecular breast imaging and breast cancer risk: a case-control study
Creators: name: Hruska, Carrie
name: Geske, Jennifer
name: Tiffinee Swanson
name: Mammel, Alyssa
name: Lake, David
name: Manduca, Armando
name: Conners, Amy
name: Whaley, Dana
name: Scott, Christopher
name: Carter, Rickey
name: Rhodes, Deborah
name: OâConnor, Michael
name: Celine Vachon
Publisher: name: figshare
Year: 2018
Subjects: subject: Biophysics
subject: Space Science
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Cancer
subject: Plant Biology
subject: Computational Biology

description: Table S1. Association of quantitative BPU with breast cancer for each MBI view and combinations of views. (DOCX 18 kb)
Supplementary materials
Creators: name: Rashid, Haroon
name: Khan,, Sherwali
name: .., Irum
name: Khan, Asad
name: Ahmad, Nasir
name: Khan, Khalid
Publisher: name: figshare
Year: 2024
Subjects: classificationCode: 340503
subject: Organic chemical synthesis
classificationCode: 340502
subject: Natural products and bioactive compounds
classificationCode: 340701
subject: Computational chemistry

description: Not applicable
Supplementary materials from "Direct synthesis, characterization, in vitro and in silico studies of simple chalcones as potential antibacterial, antifungal, and antileishmanial agents".
Creators: name: Rashid, Haroon
name: Khan,, Sherwali
name: .., Irum
name: Khan, Asad
name: Ahmad, Nasir
name: Khan, Khalid
Publisher: name: figshare
Year: 2024
Subjects: classificationCode: 340503
subject: Organic chemical synthesis
classificationCode: 340502
subject: Natural products and bioactive compounds
classificationCode: 340701
subject: Computational chemistry

description: Not applicable
Dosimetry characterization of $^{32}$P intravascular brachytherapy source wires using Monte Carlo codes PENELOPE and GEANT4
Creators: name: Torres, Javier
name: Buades, Manuel J.
name: Almansa, Julio F.
name: Guerrero, Rafael
name: Lallena, Antonio M.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Medical Physics (physics.med-ph)
subject: FOS: Physical sciences

description: Monte Carlo calculations using the codes PENELOPE and GEANT4 have been performed to characterize the dosimetric parameters of the new 20 mm long catheter based $^{32}$P beta source manufactured by Guidant Corporation. The dose distribution along the transverse axis and the two dimensional dose rate table have been calculated. Also, the dose rate at the reference point, the radial dose function and the anisotropy function were evaluated according to the adapted TG-60 formalism for cylindrical sources. PENELOPE and GEANT4 codes were first verified against previous results corresponding to the old 27 mm Guidant $^{32}$P beta source. The dose rate at the reference point for the unsheathed 27 mm source in water was calculated to be $0.215 \pm 0.001$ cGy s$^{-1}$ mCi$^{-1}$, for PENELOPE, and $0.2312 \pm 0.0008$ cGy s$^{-1}$ mCi$^{-1}$, for GEANT4. For the unsheathed 20 mm source these values were $0.2908 \pm 0.0009$ cGy s$^{-1}$ mCi$^{-1}$ and $0.311 \pm 0.001$ cGy s$^{-1}$ mCi$^{-1}$, respectively. Also, a comparison with the limited data available on this new source is shown. We found non negligible differences between the results obtained with PENELOPE and GEANT4.
description: 13 pages, 7 figures, 7 tables (accepted for publication in Medical Physics)
Memoria de actividades 2000
Creators: name: CSIC-Instituto De Investigaciones Marinas (IIM)
Publisher: name: CSIC - Delegación Institucional de Galicia
Year: 2001

description: 58 páginas
description: Memoria anual de la actividad científico-técnica del Instituto de Investigaciones Marinas: información general, proyectos y convenios, producción científica, formación, cooperación y otras actividades
A Probabilistic Quantification of Galaxy Cluster Membership
Creators: name: Brunner, R. J.
name: Lubin, L. M.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Clusters of galaxies are important laboratories for understanding both galaxy evolution and constraining cosmological quantities. Any analysis of clusters, however, is best done when one can reliably determine which galaxies are members of the cluster. While this would ideally be done spectroscopically, the difficulty in acquiring a complete sample of spectroscopic redshifts becomes rather daunting, especially at high redshift where the background contamination becomes increasingly larger. Traditionally, an alternative approach of applying a statistical background correction has been utilized, which, while useful in a global sense, does not provide information for specific galaxies. In this paper, we develop a more robust technique which uses photometrically estimated redshifts to determine cluster membership. This technique can either be used as an improvement over the commonly used statistical correction method or it can be used to determine cluster candidates on an individual galaxy basis. By tuning the parameters of our algorithm, we can selectively maximize our completeness or, alternatively, minimize our contamination. Furthermore, our technique provides a statistical quantification of both our resulting completeness and contamination from foreground and background galaxies.
description: 21 Pages LaTex, 6 Figures, Accepted for publication in the November issue of A.J
Improvement of solar cycle prediction: Plateau of solar axial dipole moment
Creators: name: Iijima, H.
name: Hotta, H.
name: Imada, S.
name: Kusano, K.
name: Shiota, D.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Aims. We report the small temporal variation of the axial dipole moment near the solar minimum and its application to the solar cycle prediction by the surface flux transport (SFT) model. Methods. We measure the axial dipole moment using the photospheric synoptic magnetogram observed by the Wilcox Solar Observatory (WSO), the ESA/NASA Solar and Heliospheric Observatory Michelson Doppler Imager (MDI), and the NASA Solar Dynamics Observatory Helioseismic and Magnetic Imager (HMI). We also use the surface flux transport model for the interpretation and prediction of the observed axial dipole moment. Results. We find that the observed axial dipole moment becomes approximately constant during the period of several years before each cycle minimum, which we call the axial dipole moment plateau. The cross-equatorial magnetic flux transport is found to be small during the period, although the significant number of sunspots are still emerging. The results indicates that the newly emerged magnetic flux does not contributes to the build up of the axial dipole moment near the end of each cycle. This is confirmed by showing that the time variation of the observed axial dipole moment agrees well with that predicted by the SFT model without introducing new emergence of magnetic flux. These results allows us to predict the axial dipole moment in Cycle 24/25 minimum using the SFT model without introducing new flux emergence. The predicted axial dipole moment of Cycle 24/25 minimum is 60--80 percent of Cycle 23/24 minimum, which suggests the amplitude of Cycle 25 even weaker than the current Cycle 24. Conclusions. The plateau of the solar axial dipole moment is an important feature for the longer prediction of the solar cycle based on the SFT model.
description: 5 pages, 3 figures, accepted for publication in A&A Letter
Classical $W_3^{(2)}$ algebra and its Miura map
Creators: name: Chung, B. K.
name: Joo, K. G.
name: Nam, Soonkeon
Publisher: name: arXiv
Year: 1993
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We verify that the fractional KdV equation is a bi-hamiltonian system using the zero curvature equation in $SL(3)$ matrix valued Lax pair representation, and explicitly find the closed form for the hamiltonian operators of the system. The second hamiltonian operator is the classical version of the $W^{(2)}_3$ algebra. We also construct systematically the Miura map of $W^{(2)}_3$ algebra using a gauge transformation of the $SL(3)$ matrix valued Lax operator in a particular gauge, and construct the modified fractional KdV equaiotn as hamiltonian system.
description: 12pages, KHTP-93-02, SNUCTP-93-17
Additional file 1: of Impact of KCNQ1, CDKN2A/2B, CDKAL1, HHEX, MTNR1B, SLC30A8, TCF7L2, and UBE2E2 on risk of developing type 2 diabetes in Thai population
Creators: name: Nattachet Plengvidhya
name: Chutima Chanprasert
name: Nalinee Chongjaroen
name: Pa-Thai Yenchitsomanus
name: Mayuree Homsanit
name: Watip Tangjittipokin
Publisher: name: figshare
Year: 2018
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Biotechnology
subject: Evolutionary Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Developmental Biology
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Table S1 Summary of the single nucleotide polymorphisms (SNPs) investigated in this study. Table S2 Primer sequence, PCR product size, and annealing temperature for HRM assay of designated SNPs. Table S3 Primer sequences of SLC30A8 (rs13266634) used for PCR-RFLP method. (DOCX 27 kb)
title: Diapositive sur le protocole ICCARRE pour un exposé donné devant l'International Aids Society à Rome en juillet 2011
Creators: name: Leibowitch, Jacques
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: International AIDS Society

description: Source: http://www.calames.abes.fr/pub/ms/Calames-20193111133762514
description: created: start=1975;end=2018
title: 01_2168
Creators: name: Wesley Baldwin, John
name: Baldwin, John W.
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2018
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: L'ensemble de ces notes ont été crée par John Baldwin lors d'une de ses premières périodes de résidence à Paris. Ces documents comprennent tous les magistri qu’il avait pu rencontrer dans ses sources. Aux XIIème et XIIIème siècles, les universités n'existant pas encore, le titre de magister s'il évoque certainement une compétence n'est pas rattaché de façon systématique au passage par les écoles. De surcroît, les magistris sont le plus souvent désignés par leur seul prénom. La lecture de ces données est donc difficile et suppose un long travail pour tenter d'identifier un individu auquel on pourrait rattacher plusieurs mentions. John Baldwin avait donc renoncé à utiliser ces données pour donner un prolongement à sa magnifique étude sur les gradués d'université et leur emploi par les Capétiens et les Plantagenêts. Néanmoins, il a conservé ces données et elles sont potentiellement très utile dans le cadre de Studium, comme le sont toutes les mentions dans les volumes des Fasti Ecclesiae Gallicanae de chanoines portant ce titre de magister sans autres précisions. L'ampleur des dépouillements rend ces données très utiles et nous devons une grande reconnaissance à John Baldwin pour avoir pris la peine de faire photocopier ses fiches et de nous les avoir transmises amicalement.
Les données ainsi que les images des fiches sont accessibles sur le site Internet à l'adresse suivante : http://studium-baldwin.lamop.fr/.
Les transcriptions des fiches ont été effectuées par des étudiants de Paris 1 Panthéon - Sorbonne mais elles n'ont pas été corrigées par la suite.
description: Relation: https://lamop.hypotheses.org/
Single-particle versus pair condensation of hard-core bosons with correlated hopping
Creators: name: Schmidt, K. P.
name: Dorier, J.
name: Laeuchli, A.
name: Mila, F.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Other Condensed Matter (cond-mat.other)
subject: FOS: Physical sciences

description: We investigate the consequences of correlated hopping on the ground state properties of hard-core bosons on a square lattice as revealed by extensive exact diagonalizations and quantum Monte Carlo simulations. While for non interacting hard-core bosons the effective attraction induced by the correlated hopping leads to phase separation at low density, we show that a modest nearest-neighbor repulsion suppresses phase separation, leading to a remarkable low-density pairing phase with no single particle Bose-Einstein condensation but long-range two-particle correlations, signaling a condensation of pairs. We also explain why the unusual properties of the pairing phase are a real challenge for standard one-worm quantum Monte Carlo simulations.
description: 8 pages, 7 figures
title: Advanced Oxidation of Drinking Water using Ultraviolet Light and Alternative Solid Forms of Hydrogen Peroxide
Creators: name: Monge, Zachary F.
Publisher: name: University of Massachusetts Amherst
Year: 2011
Subjects: subject: Environmental Engineering
subject: FOS: Environmental engineering

description: With the increasing focus on removing emerging, unregulated drinking water contaminants, the use of advanced oxidation processes (AOPs) has become more prevalent. A commonly used AOP is the ultraviolet light/hydrogen peroxide (UV/H2O2) AOP. This process utilizes the formation of hydroxyl radicals to oxidize contaminants to less harmful forms. In this analysis, two alternative solid forms of H2O2, sodium perborate (SPB) and sodium percarbonate (SPC) were used as sources of H2O2 in the UV/H2O2 AOP. The potential advantage of SPB and SPC is that they are solids in nature, and as a result, the shipping costs and shipping energy requirements can be reduced significantly compared to that of liquid H2O2. The yields of active H2O2 via SPB and SPC were investigated in deionized (DI) water and three natural water sources from the Northampton, MA Water Filtration Plant. In DI water, the active yields of H2O2 via SPB and SPC were much higher than in the vii natural water sources. The findings of this analysis indicate that both SPB and SPC are viable sources of H2O2, especially in waters that are treated to reduce the background carbonate concentration. In highly finished waters similar to DI water, it is expected that the use of SPB and SPC will result in reduced oxidation rates of drinking water contaminants. Therefore, the use of SPB and SPC as H2O2 sources in the UV/H2O2 AOP in highly finished waters is not encouraged. In natural water sources, SPB and SPC appear to be viable alternatives to liquid H2O2 for use in the UV/H2O2 AOP up to active H2O2 concentrations of 5mg/L. Using SPB and SPC has the potential for significant cost savings depending on the source of the water used in the drinking water treatment process. For facilities with surface waters as the source water, significant cost savings are possible. However water reclamation and reuse facilities have high purity source waters and SPB and SPC as sources of H2O2 are more costly alternatives. The reduction in treatment facilities carbon footprints‟ associated with shipping H2O2 is largely dependent on the location of the chemical production facilities of each reagent.
Decoupled molecules with binding polynomials of bidegree (n,2)
Creators: name: Ren, Yue
name: Martini, Johannes W. R.
name: Torres, Jacinta
Publisher: name: arXiv
Year: 2017
Subjects: subject: Biomolecules (q-bio.BM)
subject: Symbolic Computation (cs.SC)
subject: Algebraic Geometry (math.AG)
subject: Chemical Physics (physics.chem-ph)
subject: FOS: Biological sciences
subject: FOS: Computer and information sciences
subject: FOS: Mathematics
subject: FOS: Physical sciences
subject: 92C40, 65H10, 68W30

description: We present a result on the number of decoupled molecules for systems binding two different types of ligands. In the case of $n$ and $2$ binding sites respectively, we show that, generically, there are $2(n!)^{2}$ decoupled molecules with the same binding polynomial. For molecules with more binding sites for the second ligand, we provide computational results.
description: 18 pages, 8 figures
Memoria bienal 2013-2014
Creators: name: CSIC-UIB-Instituto Mediterráneo De Estudios Avanzados (IMEDEA)
Publisher: name: CSIC-UIB - Instituto Mediterráneo de Estudios Avanzados (IMEDEA)
Year: 2014

description: Como Directora del IMEDEA (CSIC/UIB) les presento en esta memoria una síntesis del trabajo que, durante 2013-2014, hemos realizado los científicos, técnicos, personal en formación y administrativos que trabajamos en este Instituto mixto entre el Consejo Superior de Investigaciones Científicas (CSIC) y la Universitat de les Illes Balears (UIB).
title: 01_2418
Creators: name: Wesley Baldwin, John
name: Baldwin, John W.
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2018
Subjects: subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: L'ensemble de ces notes ont été crée par John Baldwin lors d'une de ses premières périodes de résidence à Paris. Ces documents comprennent tous les magistri qu’il avait pu rencontrer dans ses sources. Aux XIIème et XIIIème siècles, les universités n'existant pas encore, le titre de magister s'il évoque certainement une compétence n'est pas rattaché de façon systématique au passage par les écoles. De surcroît, les magistris sont le plus souvent désignés par leur seul prénom. La lecture de ces données est donc difficile et suppose un long travail pour tenter d'identifier un individu auquel on pourrait rattacher plusieurs mentions. John Baldwin avait donc renoncé à utiliser ces données pour donner un prolongement à sa magnifique étude sur les gradués d'université et leur emploi par les Capétiens et les Plantagenêts. Néanmoins, il a conservé ces données et elles sont potentiellement très utile dans le cadre de Studium, comme le sont toutes les mentions dans les volumes des Fasti Ecclesiae Gallicanae de chanoines portant ce titre de magister sans autres précisions. L'ampleur des dépouillements rend ces données très utiles et nous devons une grande reconnaissance à John Baldwin pour avoir pris la peine de faire photocopier ses fiches et de nous les avoir transmises amicalement.
Les données ainsi que les images des fiches sont accessibles sur le site Internet à l'adresse suivante : http://studium-baldwin.lamop.fr/.
Les transcriptions des fiches ont été effectuées par des étudiants de Paris 1 Panthéon - Sorbonne mais elles n'ont pas été corrigées par la suite.
description: Relation: https://lamop.hypotheses.org/
Lattice analogues of W-algebras and Classical Integrable Equations
Creators: name: Belov, Alexander A.
name: Chaltikian, Karen D.
Publisher: name: arXiv
Year: 1993
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We propose a regular way to construct lattice versions of $W$-algebras, both for quantum and classical cases. In the classical case we write the algebra explicitly and derive the lattice analogue of Boussinesq equation from the Hamiltonian equations of motion. Connection between the lattice Faddeev-Takhtadjan-Volkov algebra [1] and q-deformed Virasoro is also discussed.
description: LaTeX, ILG-TMP-93-01, (the problems caused by mailer are fixed)
Information-theoretic bound on the entropy production to maintain a classical nonequilibrium distribution using ancillary control
Creators: name: Horowitz, Jordan M.
name: England, Jeremy L.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: There are many functional contexts where it is desirable to maintain a mesoscopic system in a nonequilibrium state. However, such control requires an inherent energy dissipation. In this article, we unify and extend a number of works on the minimum energetic cost to maintain a mesoscopic system in a prescribed nonequilibrium distribution using ancillary control. For a variety of control mechanisms, we find that the minimum amount of energy dissipation necessary can be cast as an information-theoretic measure of distinguishability between the target nonequilibrium state and the underlying equilibrium distribution. This work offers quantitative insight into the intuitive idea that more energy is needed to maintain a system farther from equilibrium.
description: 6 pages, 2 figures
Bias in the temperature of helium nanodroplets measured by an embedded rotor
Creators: name: Lehmann, Kevin K.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Chemical Physics (physics.chem-ph)
subject: FOS: Physical sciences

description: The ro--vibrational spectra of molecules dissolved in liquid $^4$He nanodroplets display rotational structure. Where resolved, this structure has been used to determine a temperature that has been assumed to equal that of the intrinsic excitations of the helium droplets containing the molecules. Consideration of the density of states as a function of energy and total angular momentum demonstrates that there is a small but significant bias of the rotor populations that make the temperature extracted from a fit to its rotational level populations slightly higher than the temperature of the ripplons of the droplet. This bias grows with both the total angular momentum of the droplet and with the moment of inertia of the solute molecule.
description: 6 pages, 1 figure, to be published in Journal of Chemical Physics
Additional file 6: of Feasibility of sun and magnetic compass mechanisms in avian long-distance migration
Creators: name: Muheim, Rachel
name: Schmaljohann, Heiko
name: Alerstam, Thomas
Publisher: name: figshare
Year: 2018
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Molecular Biology
subject: Ecology
subject: Sociology
subject: FOS: Sociology
subject: Developmental Biology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Figure S6. Two examples of magnetoclinic compass routes during spring migration starting from the equator (0° latitude; left graph) or 20°S (right graph) with initial departure directions of 354°, 356°, 358°, 0°, 2°, 4° and 6°. Great circle routes (dark grey dashed) are given for comparison to indicate the shortest routes. The routes are presented in Mercator projection. (PDF 171 kb)
Spherically symmetric model atmospheres for low mass pre-Main Sequence stars with effective temperatures between 2000 and 6800 K
Creators: name: Allard, France
name: Hauschildt, Peter H.
name: Schweitzer, Andreas
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a grid of spherically symmetric model atmospheres for young pre-MS stars. This grid spans the parameter range $2000\K \leq \Teff \leq 6800\K$ and $2.0 \leq \logg \leq 3.5$ for $M=0.1\Msun$, appropriate for low mass stars and brown dwarfs. A major improvement is the replacement of TiO and \water line lists with the newer line list calculated by the NASA-AMES group, for TiO (about 175 million lines of 5 isotopes) and for \water (about 350 million lines in 2 isotopes). We provide the model structures, spectra and broad-band colors in standard filters in electronic form.
description: ApJ, in press. Also available at ftp://calvin.physast.uga.edu/pub/preprints
Segmentation of Glioma Tumors in Brain Using Deep Convolutional Neural Network
Creators: name: Hussain, Saddam
name: Anwar, Syed Muhammad
name: Majid, Muhammad
Publisher: name: arXiv
Year: 2017
Subjects: subject: Computer Vision and Pattern Recognition (cs.CV)
subject: FOS: Computer and information sciences

description: Detection of brain tumor using a segmentation based approach is critical in cases, where survival of a subject depends on an accurate and timely clinical diagnosis. Gliomas are the most commonly found tumors having irregular shape and ambiguous boundaries, making them one of the hardest tumors to detect. The automation of brain tumor segmentation remains a challenging problem mainly due to significant variations in its structure. An automated brain tumor segmentation algorithm using deep convolutional neural network (DCNN) is presented in this paper. A patch based approach along with an inception module is used for training the deep network by extracting two co-centric patches of different sizes from the input images. Recent developments in deep neural networks such as drop-out, batch normalization, non-linear activation and inception module are used to build a new ILinear nexus architecture. The module overcomes the over-fitting problem arising due to scarcity of data using drop-out regularizer. Images are normalized and bias field corrected in the pre-processing step and then extracted patches are passed through a DCNN, which assigns an output label to the central pixel of each patch. Morphological operators are used for post-processing to remove small false positives around the edges. A two-phase weighted training method is introduced and evaluated using BRATS 2013 and BRATS 2015 datasets, where it improves the performance parameters of state-of-the-art techniques under similar settings.
description: Submitted to Neurocomputing
title: ADCO, Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Cart. 32 (G 136), 745 folios, f. 0612
Creators: name: de la Côte d'Or, Archives départementales
name: Petot, Frédéric
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2012
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Archives départementales de la Côte-d'Or, Cart. 32 (G 136), 745 folios, f. 0612, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Neuvième cartulaire de Saint-Étienne de Dijon (1661 - 1684), Archives départementales de la Côte-d'Or, Cart. 32 (G 136), 745 folios, f. 0612, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: abbaye Saint-Étienne de Dijon
description: Provenance: http://www.wikidata.org/entity/Q15945019
Manipulating Bose-Einstein condensed atoms in toroidal traps
Creators: name: Jackson, A. D.
name: Kavoulakis, G. M.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Other Condensed Matter (cond-mat.other)
subject: FOS: Physical sciences

description: We consider Bose-Einstein condensed atoms confined in a toroidal trap. We demonstrate that under conditions of one-dimensional behavior, the density distribution of the atoms may be exponentially localized/delocalized, even for very small variations in the trapping potential along the torus. This observation allows one to control the atom density externally via slight modifications of the trapping potential. For similar reasons, small irregularities of the trap may also have a very pronounced effect on the density of the cloud.
description: 4 pages, RevTex, 2 figures
Fourier Analysis of Spectra of Solar-Type Stars
Creators: name: Sheminova, V. A.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We used Fourier transform techniques to determine macroturbulent velocity. The analysis is done with mictoturbulent velocity and rotation velocity as an unknown quantities. In order to distinguish the effects of rotation from macroturbulence effects in slowly rotating stars, primarily the main lobe of residual Fourier transforms of the observed lines, which were taken from the solar spectrum and the spectra of two other stars, was used. This case of Fourier analysis of spectral lines is the most complicated one. The end results were in a satisfactory agreement with the data obtained using different methods. We have obtained the average values of microturbulent, macroturbulent, and rotation velocities were 0.85, 2.22, and 1.75 km/s for the Sun as the star, 0.58, 1.73, and 0.78 km/s for HD 10700, and 1.16, 3.56, and 6.24 km/s for HD 1835. It was found that the macroturbulent velocity decreases with height in the atmosphere of the Sun and HD 1835. In the case of HD 10700, the macroturbulent velocity did not change with height, and the determined rotation velocity was two times lower than the one obtained using other methods. It was concluded that Fourier transform techniques are suitable for determining the velocities in atmospheres of solar-type stars with very slow rotation.
description: 16 pages, 5 figures, 2 tables, published in Kinematika i Fizika Nebesnykh Tel, 2017, Vol. 33, no. 5, P. 27-48 (in Russian), Kinematics and Physics of Celestial Bodies, 2017, Vol. 33, no. 5, P. 217-230 (in English)
Antisymmetric tensor gauge theory
Creators: name: Blasi, G. Bandelloni A.
Publisher: name: arXiv
Year: 1993
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We analyze to all perturbative orders the properties of two possible quantum extensions of classically on-shell equivalent antisymmetric tensor gauge models in four dimensions. The first case, related to the soft breaking of a topological theory wants a gauge field of canonical dimension one. The other possibility, which assigns canonical dimension two to the gauge field, leads to the $σ$ model interpretation of the theory. In both instances we find that the models are anomaly free.
description: 28 ,Latex,GEF-TH 10/93
Additional file 5: of Feasibility of sun and magnetic compass mechanisms in avian long-distance migration
Creators: name: Muheim, Rachel
name: Schmaljohann, Heiko
name: Alerstam, Thomas
Publisher: name: figshare
Year: 2018
Subjects: subject: 29999 Physical Sciences not elsewhere classified
subject: FOS: Physical sciences
subject: Medicine
subject: Cell Biology
subject: Neuroscience
subject: Physiology
subject: FOS: Biological sciences
subject: Evolutionary Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: 60506 Virology

description: Figure S5. Visualisation of the magnetoclinic compass. Magnetoclinic orientation refers to the case where migratory birds fly at a constant “apparent angle of inclination” (γ′ in blue). The apparent angle of inclination is the inclination of the geomagnetic field projected on a plane orthogonal to the bird’s heading or body axis. As inclination changes with latitude, a migrant must change its course in order to keep γ′ constant. In horizontal flight the apparent angle of inclination is a function of the geomagnetic inclination (γ in red) and the bird’s flight course (α in green), according to the relationship tan(γ′) = tan(γ)/ sin(α). The illustration shows the headings of a bird flying along a fixed γ’ in areas with different angles of inclination γ1 (left graph) and γ2 (right graph). The bird maintains a fixed γ′ by adjusting its heading from more westerly directions α1 to more southerly directions α2 with decreasing geomagnetic inclination from γ1 (left graph) and γ2 (right graph). Magnetoclinic orientation will be affected if birds do not fly horizontally and also by wind conditions depending on whether the birds perceive the apparent inclination magnetostatically in relation to their body axis or by a magnetic induction process in relation to their trajectory through the magnetic field, as evaluated by Alerstam (1987: J Exp Biol. 1987;130:63–86). These effects are not included in the simplified geometric explanation in the figure here. (PDF 173 kb)
Pushing the limits: detecting H2 emission from faint bipolar planetary nebulae in the IPHAS sample
Creators: name: Ramos-Larios, Gerardo
name: Guerrero, Martin A.
name: Sabin, Laurence
name: Santamaria, Edgar
Publisher: name: arXiv
Year: 2017
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We have obtained deep narrowband images in the near-infrared H2 (2.122 microns) emission line for a sample of 15 faint Isaac Newton Telescope Photometric Halpha Survey (IPHAS) bipolar planetary nebulae (PNe) to search for molecular material. H2 emission is found in most of them (14 out of 15), mostly associated with rings at their equatorial regions and with their bipolar lobes. These detections add to the high occurrence of H2 emission among bipolar PNe reported in previous works, resulting from the large reservoir of molecular material in these sources and the suitable excitation conditions for H2 emission. The correlation between detailed bipolar morphology and H2 luminosity is also confirmed: bipolar PNe with broad equatorial rings (R-BPNe) have almost no continuum emission, are H2 brighter and have larger H2/Brgamma line ratio than bipolar PNe with pinched equatorial waists (W-BPNe). The origin of this dichotomy is unclear. The larger size and age of R-BPNe are consistent with shock excitation of H2, whereas ultraviolet pumping is most likely the excitation mechanism in the smaller and younger W-BPNe, which would explain their lower H2 luminosity. Although both types of bipolar PNe seem to proceed from the same progenitor population, this does not imply that R-BPNe descend from W-BPNe. Otherwise, we note that some of the H2-weak bipolar PNe harbor post-common envelope binary systems and symbiotic stars. Finally, we suggest that the long-living H2 emission from R-BPNe arises from a discrete distribution of compact knots embedded within the ionized gas at the equatorial region.
description: 13 pages, 9 figures, Accepted for publication in MNRAS
Photon trajectories in incoherent atomic radiation trapping as Levy flights
Creators: name: Pereira, Eduardo
name: Martinho, Jose M. G.
name: Berberan-Santos, Mario N.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Atomic Physics (physics.atom-ph)
subject: FOS: Physical sciences

description: Photon trajectories in incoherent radiation trapping for Doppler, Lorentz and Voigt line shapes under complete frequency redistribution are shown to be Levy flights. The jump length (r) distributions display characteristic long tails. For the Lorentz line shape, the asymptotic form is a strict power-law r^{-3/2} while for Doppler the asymptotic is r^{-2} (ln r)^{-1/2}. For the Voigt profile, the asymptotic form has always a Lorentz character, but the trajectory is a self-affine fractal with two characteristic Hausdorff scaling exponents.
description: 3 figs
An exciton-coupled electron transfer process controlled by non-Markovian environments
Creators: name: Sakamoto, Souichi
name: Tanimura, Yoshitaka
Publisher: name: arXiv
Year: 2017
Subjects: subject: Quantum Physics (quant-ph)
subject: Other Condensed Matter (cond-mat.other)
subject: Biomolecules (q-bio.BM)
subject: FOS: Physical sciences
subject: FOS: Biological sciences

description: We theoretically investigate an exciton-coupled electron transfer (XCET) process that is conversion of an exciton into a charge transfer state. This conversion happens in an exciton transfer (XT) process, and the electron moves away in an electron transfer(ET) process in multiple environments (baths). This XCET process plays an essential role in the harvesting of solar energy in biological and photovoltaic materials. We develop a practical theoretical model to study the efficiency of XCET process that occurs either in consecutive or concerted processes under the influence of non-Markovian baths. The role of quantum coherence in the XT-ET system and the baths is investigated using reduced hierarchal equations of motion (HEOM). This model includes independent baths for each XT and ET state, in addition to a XCET bath for the conversion process. We found that, while quantum system-bath coherence is important in the XT and ET processes, coherence between the XT and ET processes must be suppressed in order to realize efficient irreversible XCET process through the weak off-diagonal interaction between the XT and ET bridge sites arises from a XCET bath.
description: J. Phys. Chem. Lett. accepted
TiO and H$_2$O absorption lines in cool stellar atmospheres
Creators: name: Allard, France
name: Hauschildt, Peter H.
name: Schwenke, David
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We compare the structures of model atmospheres and synthetic spectra calculated using different line lists for TiO and water vapor. We discuss the effects of different line list combinations on the model strutures and spectra for both dwarf and giant stars. It is shown that recent improvements result in significantly improved spectra, in particular in the optical where TiO bands are important. The water vapor dominated near-IR region remains problematic as the current water line lists do not yet completely reproduce the shapes of the observed spectra. We find that the AMES TiO list provides more opacity in most bands and that the new, smaller oscillator strengths lead to systematically cooler temperatures for early type M dwarfs than previous models. These effects combine and will help to siginificantly improve the fits of models to observations in the optical as well as result in improved synthetic photometry of M stars. We show that the Davis 1986 \fel-values for the $δ$ and $ϕ$ bands of TiO best reproduce the observed (V-I) color indices.
description: ApJ, in press. Also available at ftp://calvin.physast.uga.edu/pub/preprints
Kondo Quantum Dots and the Novel Kondo-doublet interaction
Creators: name: Simonin, J.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We analyze the interactions between two Kondo Quantum Dots connected to a Rashba-active Quantum Wire. We find that the Kondo-doublet interaction, at an inter-dot distance of the order of the wire Fermi length, is over an order of magnitude greater than the RKKY interaction. The effects induced on the Kondo-doublet interaction by the wire spin-orbit coupling can be used to control the Quantum Dots spin-spin correlation. These results imply that the widely used assumption that the RKKY is the dominant interaction between Anderson impurities must be revised.
description: 4 pages, 4 figs, accepted for publication in PRL. title changed and text polished