cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Unification of gauge couplings in Kaluza-Klein theory with two internal manifolds
Creators: name: Arik, M.
name: Gabay, V.
Publisher: name: arXiv
Year: 1993
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We consider a Kaluza-Klein theory whose ground state is ${\bf R}^4 \times {\bf M } \times {\bf K}$ where ${\bf M}$ and ${\bf K}$ are compact, irreducible, homogenous internal mani folds. This is the simplest ground state compatible with the existence of the graviton, gauge fields, massless scalar fields and the absence of the cosmological constan t. The requirement for these conditions to be satisfied are the odd dimensionality of ${\bf M}$ and ${\bf K}$, and the choice of a dimensionally continued Euler form action whose dimension is the same as the dimension of ${\bf M} \times {\bf K}$. We show that in such a theory, which is not simple due to presence of two internal manifolds, the gauge couplings $g^2_M$ and $g^2_K$ are actually unified provided that the internal space sizes are constant. For ${\bf M} \times {\bf K} = S^{2m+ 1} \times S^{2k+1}$ this gauge coupling unification relation reads $g^2_M / g^2_K = m / k$.
description: 6,BUFB0993
Dynamical onset of superconductivity and retention of magnetic fields in cooling neutron stars
Creators: name: Ho, Wynn C. G.
name: Andersson, Nils
name: Graber, Vanessa
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Superconductivity (cond-mat.supr-con)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: A superconductor of paired protons is thought to form in the core of neutron stars soon after their birth. Minimum energy conditions suggest magnetic flux is expelled from the superconducting region due to the Meissner effect, such that the neutron star core is largely devoid of magnetic fields for some nuclear equation of state and proton pairing models. We show via neutron star cooling simulations that the superconducting region expands faster than flux is expected to be expelled because cooling timescales are much shorter than timescales of magnetic field diffusion. Thus magnetic fields remain in the bulk of the neutron star core for at least 10^6-10^7 yr. We estimate the size of flux free regions at 10^7 yr to be
description: 6 pages, 5 figures; accepted for publication in Physical Review C
Additional file 2: of A realist approach to eliciting the initial programme theory of the antiretroviral treatment adherence club intervention in the Western Cape Province, South Africa
Creators: name: Mukumbang, Ferdinand
name: Marchal, Bruno
name: Belle, Sara Van
name: Wyk, Brian Van
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Biotechnology
subject: Ecology
subject: FOS: Biological sciences
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Developmental Biology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: 60506 Virology
subject: Computational Biology

description: Nonparticipant observation guide. (DOCX 14 kb)
Colder Freeze-in Axinos Decaying into Photons
Creators: name: Bae, Kyu Jung
name: Kamada, Ayuki
name: Liew, Seng Pei
name: Yanagi, Keisuke
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We point out that 7 keV axino dark matter (DM) in the R-parity violating (RPV) supersymmetric (SUSY) Dine-Fischler-Srednicki-Zhitnitsky model can simultaneously reproduce the 3.5keV X-ray excess, and evade stringent constraints from the Ly-alpha forest data. Peccei-Quinn symmetry breaking naturally generates both axino interactions with minimal SUSY standard model particles and RPV interactions. The RPV interaction introduces an axino-neutrino mixing and provides axino DM as a variant of sterile neutrino DM, whose decay into a monochromatic photon can be detected by X-ray observations. Axinos, on the other hand, are produced by freeze-in processes of thermal particles in addition to the Dodelson-Widrow mechanism of sterile neutrinos. The resultant phase space distribution tends to be colder than the Fermi-Dirac distribution. The inherent entropy production from late-time saxion decay makes axinos even colder. The linear matter power spectrum satisfies even the latest and strongest constraints from the Ly-alpha forest data.
description: 5 pages, 4 figures
Structure of symmetric and asymmetric "ripple" phases in lipid bilayers
Creators: name: Lenz, Olaf
name: Schmid, Friederike
Publisher: name: arXiv
Year: 2006
Subjects: subject: Biological Physics (physics.bio-ph)
subject: Chemical Physics (physics.chem-ph)
subject: FOS: Physical sciences

description: We reproduce the symmetric and asymmetric ``rippled'' $P_{β'}$ states of lipid membranes by Monte Carlo simulations of a coarse-grained molecular model for lipid-solvent mixtures. The structure and properties compare favorably with experiments. The asymmetric ripple state is characterized by a periodic array of fully interdigitated ``defect'' lines. The symmetric ripple state maintains a bilayer structure, but is otherwise structurally similar. The formation of both ripple states is driven by the propensity of lipid molecules with large head groups to exhibit splay.
description: 4 pages, 4 figures
AdditionalÂ fileÂ 10:
Creators: name: Opatovsky, Itai
name: Santos-Garcia, Diego
name: Zhepu Ruan
name: Lahav, Tamar
name: Shany Ofaim
name: Mouton, Laurence
name: ValĂŠrie Barbe
name: Jiandong Jiang
name: Zchori-Fein, Einat
name: Shiri Freilich
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Biotechnology
subject: Ecology
subject: FOS: Biological sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Developmental Biology
subject: Marine Biology

description: Comparison of annotations retrieved for the four different Porteria genomes using the JGI platform. (DOCX 111 kb)
Magnetic swirls and associated fast magnetoacoustic kink waves in a solar chromospheric flux tube
Creators: name: Murawski, K.
name: Kayshap, P.
name: Srivastava, A. K.
name: Pascoe, D. J.
name: Jelínek, P.
name: Kuźma, B.
name: Fedun, V.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We perform numerical simulations of impulsively generated magnetic swirls in an isolated flux tube which is rooted in the solar photosphere. These swirls are triggered by an initial pulse in a horizontal component of the velocity. The initial pulse is launched either: (a) centrally, within the localized magnetic flux tube; or (b) off-central, in the ambient medium. The evolution and dynamics of the flux tube is described by three-dimensional, ideal magnetohydrodynamic equations. These equations are numerically solved to reveal that in case (a) dipole-like swirls associated with the fast magnetoacoustic kink and $m=1$ Alfvén waves are generated. In case (b), the fast magnetoacoustic kink and $m=0$ Alfvén modes are excited. In both these cases, the excited fast magnetoacoustic kink and Alfvén waves consist of similar flow pattern and magnetic shells are also generated with clockwise and counter-clockwise rotating plasma within them, which can be the proxy of dipole-shaped chromospheric swirls. The complex dynamics of vortices and wave perturbations reveals the channelling of sufficient amount of energy to fulfill energy losses in the chromosphere ($\sim$ 10$^{4}$ W m$^{-1}$) and in the corona ($\sim$ 10$^{2}$ W m$^{-1}$). Some of these numerical findings are reminiscent of signatures in recent observational data.
Manipulating exciton fine-structure in quantum dots with a lateral electric field
Creators: name: Gerardot, B. D.
name: Seidl, S.
name: Dalgarno, P. A.
name: Warburton, R. J.
name: Granados, D.
name: Garcia, J. M.
name: Kowalik, K.
name: Krebs, O.
name: Karrai, K.
name: Badolato, A.
name: Petroff, P. M.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: The fine structure of the neutral exciton in a single self assembled InGaAs quantum dot is investigated under the effect of a lateral electric field. Stark shifts up to 1.5 meV, an increase in linewidth, and a decrease in photoluminescence intensity were observed due to the electric field. We show that the lateral electric field strongly affects the exciton fine structure splitting due to active manipulation of the single particle wave-functions. Remarkably, the splitting can be tuned over large values and through zero.
description: 4 pages, 5 figures
Theory of Superselection Sectors for Generalized Ising models
Creators: name: Martínez, J. R. Reyes
Publisher: name: arXiv
Year: 1993
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We apply the theory of superselection sectors in the same way as done by G.Mack and V.Schomerus for the Ising model to generalizations of this model described by J.Fröhlich and T.Kerler.
description: Latex
An Imaging and Spectroscopic Study of the z=3.38639 Damped Lyman Alpha System in Q0201+1120: Clues to Star Formation Rate at High Redshift
Creators: name: Ellison, Sara L.
name: Pettini, Max
name: Steidel, Charles C.
name: Shapley, Alice E.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present the results of a series of imaging and spectroscopic observations aimed at identifying and studying the galaxy responsible for the z = 3.38639 damped lya system in the z = 3.61 QSO Q0201+1120. We find that the DLA is part of a concentration of matter which includes at least four galaxies (probably many more) over linear comoving dimensions, greater than 5h^-1Mpc. The absorber may be a 0.7 L* galaxy at an impact parameter of 15 h^-1 kpc, but follow-up spectroscopy is still required for positive identification. The gas is turbulent, with many absorption components distributed over approximately 270 km/s and a large spin temperature, T_s greater than 4000K. The metallicity is relatively high for this redshift, Z(DLA) approximately 1/20 Z(solar). From consideration of the relative ratios of elements which have different nucleosynthetic timescales, it would appear that the last major episode of star formation in this DLA occurred at z greater than 4.3, more than approximately 500 Myr prior to the time when we observe it.
description: Accepted for publication in ApJ
The effect of the junction model on the anomalous diffusion in the 3D comb structure
Creators: name: Dzhanoev, A. R.
name: Sokolov, I. M.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: The diffusion in the comb structures is a popular model of geometrically induced anomalous diffusion. In the present work we concentrate on the diffusion along the backbone in a system where sidebranches are planes, and the diffusion thereon is anomalous and described by continuous time random walks (CTRW). We show that the mean squared displacement (MSD) in the backbone of the comb behaves differently depending on whether the waiting time periods in the sidebranches are reset after the step in the backbone is done (a rejuvenating junction model), or not (a non-rejuvenating junction model). In the rejuvenating case the subdiffusion in the sidebranches only changes the prefactor in the ultra-slow (logarithmic) diffusion along the backbone, while in the non-rejuvenating case the ultraslow, logarithmic subdiffusion is changed to a much faster power-law subdiffusion (with a logarithmic correction) as it was found earlier by Iomin and Mendez [Chaos Solitons and Fractals 2016; 82:142]. Moreover, in the first case the result does not change if the diffusion in the backbone is itself anomalous, while in the second case it does. Two of the special cases of the considered models (the non-rejuvenating junction under normal diffusion in the backbone, and rejuvenating junction for the same waiting time distribution in the sidebranches and in junction points) were also investigated within the approach based on the corresponding generalized Fokker-Planck equations.
description: 12 pages, 4 figures
Affine Lie Algebras in Massive Field Theory and Form-Factors from Vertex Operators
Creators: name: LeClair, Andre
Publisher: name: arXiv
Year: 1993
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We present a new application of affine Lie algebras to massive quantum field theory in 2 dimensions, by investigating the $q\to 1$ limit of the q-deformed affine $\hat{sl(2)}$ symmetry of the sine-Gordon theory, this limit occurring at the free fermion point. Working in radial quantization leads to a quasi-chiral factorization of the space of fields. The conserved charges which generate the affine Lie algebra split into two independent affine algebras on this factorized space, each with level 1 in the anti-periodic sector, and level $0$ in the periodic sector. The space of fields in the anti-periodic sector can be organized using level-$1$ highest weight representations, if one supplements the $\slh$ algebra with the usual local integrals of motion. Introducing a particle-field duality leads to a new way of computing form-factors in radial quantization. Using the integrals of motion, a momentum space bosonization involving vertex operators is formulated. Form-factors are computed as vacuum expectation values in momentum space. (Based on talks given at the Berkeley Strings 93 conference, May 1993, and the III International Conference on Mathematical Physics, String Theory, and Quantum Gravity, Alushta, Ukraine, June 1993.)
description: 13 pages, CLNS 93/1255
title: ADCO, Septième cartulaire de Saint-Étienne de Dijon (1661-1665), Cart. 29 (G 134), 996 folios, f. 0058
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2012
name: Petot, Frédéric
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Septième cartulaire de Saint-Étienne de Dijon (1661-1665), Archives départementales de la Côte-d'Or, Cart. 29 (G 134), 996 folios, f. 0058, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Septième cartulaire de Saint-Étienne de Dijon (1661-1665), Archives départementales de la Côte-d'Or, Cart. 29 (G 134), 996 folios, f. 0058, 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
Additional file 1: of Pneumonia mortality and healthcare utilization in young children in rural Bangladesh: a prospective verbal autopsy study
Creators: name: Ferdous, Farzana
name: Shahnawaz Ahmed
name: Sumon Das
name: Mohammod Chisti
name: Nasrin, Dilruba
name: Kotloff, Karen
name: Levine, Myron
name: Nataro, James
name: Enbo Ma
name: Khitam Muhsen
name: Wagatsuma, Yukiko
name: Tahmeed Ahmed
name: Faruque, Abu
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Biotechnology
subject: 69999 Biological Sciences not elsewhere classified
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Developmental Biology
subject: Cancer
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Table S1. Correlation between pneumonia and co-variates. (DOC 42Â kb)
POD-based reduced-order model of an eddy-current levitation problem
Creators: name: Hasan, MD Rokibul
name: Montier, Laurent
name: Henneron, Thomas
name: Sabariego, Ruth V.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Computational Engineering, Finance, and Science (cs.CE)
subject: FOS: Computer and information sciences

description: The accurate and efficient treatment of eddy-current problems with movement is still a challenge. Very few works applying reduced-order models are available in the literature. In this paper, we propose a proper-orthogonal-decomposition reduced-order model to handle these kind of motional problems. A classical magnetodynamic finite element formulation based on the magnetic vector potential is used as reference and to build up the reduced models. Two approaches are proposed. The TEAM workshop problem 28 is chosen as a test case for validation. Results are compared in terms of accuracy and computational cost.
description: Accepted
Semi-empirical seismic relations of A-F stars from CoRoT and Kepler legacy data
Creators: name: Moya, A.
name: Suárez, J. C.
name: Hernández, A. García
name: Mendoza, M. A.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Asteroseismology is witnessing a revolution thanks to high-precise asteroseismic space data (MOST, CoRoT, Kepler, BRITE), and their large ground-based follow-up programs. Those instruments have provided an unprecedented large amount of information, which allows us to scrutinize its statistical properties in the quest for hidden relations among pulsational and/or physical observables. This approach might be particularly useful for stars whose pulsation content is difficult to interpret. This is the case of intermediate-mass classical pulsating stars (i.e. gamma Dor, delta Scuti, hybrids) for which current theories do not properly predict the observed oscillation spectra. Here we establish a first step in finding such hidden relations from Data Mining techniques for these stars. We searched for those hidden relations in a sample of delta Scuti and hybrid stars observed by CoRoT and Kepler (74 and 153, respectively). No significant correlations between pairs of observables were found. However, two statistically significant correlations emerged from multivariable correlations in the observed seismic data, which describe the total number of observed frequencies and the largest one, respectively. Moreover, three different sets of stars were found to cluster according to their frequency density distribution. Such sets are in apparent agreement with the asteroseismic properties commonly accepted for A-F pulsating stars.
description: 14 pages, 7 figures. Accepted for publication in MNRAS
Governance, Sustainability and HRD at the Regional Level: The Case of the University Training Programme for Local Government Executives in the Region of Crete
Creators: name: Papadakis, Nikos
name: Drakaki, Maria
name: Tzagkarakis, Stylianos Ioannis
name: Kamekis, Apostolos
name: Kotroyannos, Dimitrios
name: Calogiannakis, Pella
name: Lavdas, Kostas A.
Publisher: name: Academia
Year: 2019
Subjects: Regional Governance; Sustainability; Needs Assessment; Training; Human Resource Development; Region of Crete.

description: The paper deals with the Training Programme for Local Government Executives in the Region of Crete, which was designed and implemented based on the findings of the qualitative research-needs assessment, carried out within the framework of the Research Project entitled “Governance, Sustainability and Regional Innovation” (KA 4289) in the Region of Crete. The project was carried out by the Centre of Political Research Documentation (KEPET) and the Centre for Human Rights (KEADIK) of the Department of Political Science of the University of Crete, while it was entirely funded by the Region of Crete. In particular, the first part provides a brief analysis of the theoretical dimensions concerning the relation between governance, sustainability and regional development, with particular regard to the role of training-reskilling in the development of Local Government Human Resources. This is followed by a focus on the methodological strategy used for implementing the field study conducted as part of the Project, emphasizing on the primary qualitative research-needs assessment and its key research findings, based on which the Project’s Training Programme was designed and implemented. Then, the framework, the methodology and the teaching modules of the Training Programme are presented and analyzed, as they were designed and implemented based on the Project’s qualitative-research findings.
description: Academia, No 18 (2020): Higher Education and Lifelong Learning
Reflections on Modern Macroeconomics: Can We Travel Along a Safer Road?
Creators: name: Gaffeo, E.
name: Catalano, M.
name: Clementi, F.
name: Gatti, D. Delli
name: Gallegati, M.
name: Russo, A.
Publisher: name: arXiv
Year: 2006
Subjects: subject: Physics and Society (physics.soc-ph)
subject: General Finance (q-fin.GN)
subject: FOS: Physical sciences
subject: FOS: Economics and business

description: In this paper we sketch some reflections on the pitfalls and inconsistencies of the research program - currently dominant among the profession - aimed at providing microfoundations to macroeconomics along a Walrasian perspective. We argue that such a methodological approach constitutes an unsatisfactory answer to a well-posed research question, and that alternative promising routes have been long mapped out but only recently explored. In particular, we discuss a recent agent-based, truly non-Walrasian macroeconomic model, and we use it to envisage new challenges for future research.
description: Latex2e v1.6; 17 pages with 4 figures; for inclusion in the APFA5 Proceedings
Additional file 14: of Prevalence and antimicrobial resistance of coagulase negative staphylococci clinical isolates from Ethiopia: a meta-analysis
Creators: name: Serawit Deyno
name: Sintayehu Fekadu
name: Sisay Seyfe
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Biotechnology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Hematology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: 60506 Virology

description: Figure S14. Forest plot of the proportion of CoNS resistance to clinidamycin. (DOCX 17 kb)
Quasi-biennial oscillations in the cross-correlation of properties of macrospicules
Creators: name: Kiss, T. S.
name: Gyenge, N.
name: Erdelyi, R.
Publisher: name: arXiv
Year: 2017
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Jets, whatever small (e.g. spicules) or large (e.g. macrospicules) their size, may play a key role in momentum and energy transport from photosphere to chromosphere and at least to the low corona. Here, we investigate the properties of abundant, large-scale dynamic jets observable in the solar atmosphere: the macrospicules (MS). These jets are observationally more distinct phenomena than their little, and perhaps more ubiquitous, cousins, the spicules. Investigation of long-term variation of the properties of macrospicules may help to a better understanding of their underlying physics of generation and role in coronal heating. Taking advantage of the high temporal and spatial resolution of the Solar Dynamics Observatory, a new dataset, with several hundreds of macrospicules, was constructed encompassing a period of observations over six years. Here, we analyse the measured properties and relations between these properties of macrospicules as function of time during the observed time interval. We found that cross-correlations of several of these macrospicule properties display a strong oscillatory pattern. Next, wavelet analysis is used to provide more detailed information about the temporal behaviour of the various properties of MS. For coronal hole macrospicules, a significant peak is found at around 2-year period. This peak also exists partially or is shifted to longer period, in the case of quiet Sun macrospicules. These observed findings may be rooted in the underlying mechanism generating the solar magnetic field, i.e. the global solar dynamo.
Additional file 10 of DNA methylation abnormalities of imprinted genes in congenital heart disease: a pilot study
Creators: name: Chang, Shaoyan
name: Wang, Yubo
name: Xin, Yu
name: Wang, Shuangxing
name: Luo, Yi
name: Wang, Li
name: Zhang, Hui
name: Li, Jia
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 10: Table S1. gDMR sequence information of 18 imprinted genes.
BeppoSAX Observations of the Maser Sy2 Galaxy: ESO103-G35
Creators: name: Wilkes, Belinda J.
name: Mathur, Smita
name: Fiore, Fabrizio
name: Antonelli, Angelo
name: Nicastro, Fabrizio
Publisher: name: arXiv
Year: 2000
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have made BeppoSAX observations of the Seyfert 2/1.9 galaxy ESO103-G35, which contains a nuclear maser source and is known to be heavily absorbed in the X-rays. Analysis of the X-ray spectra observed by SAX in October 1996 and 1997 yields a spectral index 0.74+/-0.07, typical of Seyfert galaxies and consistent with earlier observations of this source. The strong, soft X-ray absorption has column density 1.79E(23)/cm^2, again consistent with earlier results. The best fitting spectrum is that of a power law with a high energy cutoff at 29+/-10 keV, a cold, marginally resolved Fe Kalpha line with EW 290 eV (1996) and a mildly ionized Fe K-edge at 7.37 keV. The Kalpha line and cold absorption are consistent with origin in a accretion disk/torus through which our line-of-sight passes at a radial distance of $\sim 50$ pc. The Fe K-edge is mildly ionized suggesting the presence of ionized gas probably in the inner accretion disk, close to the central source or in a separate warm absorber. The data quality is too low to distinguish between these possibilities but the edge-on geometry implied by the water maser emission favors the former. Comparison with earlier observations of ESO103-G35 shows little/no change in spectral parameters while the flux changes by factors of a few on timescales of a few months. The 2--10 keV flux decreased by a factor of 2.7 between Oct 1996 and Oct 1997 with no detectable change in the count rate >20 keV suggesting a constant or delayed response reflection component. The high energy cutoff is lower than the typical 300keV values seen in Seyfert galaxies. A significant subset of similar sources would affect current models of the AGN contribution to the cosmic X-ray background which generally assume a high energy cutoff of 300 keV.
description: 22 pages, postscript file, accepted for publication in ApJ
Modeling Repeated M-dwarf Flaring at an Earth-like Planet in the Habitable Zone: I. Atmospheric Effects for an Unmagnetized Planet
Creators: name: Tilley, Matt A.
name: Segura, Antigona
name: Meadows, Victoria S.
name: Hawley, Suzanne
name: Davenport, James
Publisher: name: arXiv
Year: 2017
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Understanding the impact of active M-dwarf stars on the atmospheric equilibrium and surface conditions of a habitable zone Earth-like planet is key to assessing M dwarf planet habitability. Previous modeling of the impact of electromagnetic (EM) radiation and protons from a single large flare on an Earth-like atmosphere indicated that significant and long-term reductions in ozone were possible, but the atmosphere recovered. These stars more realistically exhibit frequent flaring with a power-law distribution of energies. Here we use a coupled 1D photochemical and radiative-convective model to investigate the effects of repeated flaring on the photochemistry and surface UV of an Earth-like planet unprotected by an intrinsic magnetic field. We use time-resolved flare spectra obtained for the dM3 star AD Leo, combined with flare occurrence frequencies and total energies (typically 10$^{30.5}$ to 10$^{34}$ erg) from the 4-year Kepler light curve for the dM4 flare star GJ1243. Our model results show repeated EM-only flares have little effect on the ozone column depth, but that multiple proton events can rapidly destroy the ozone column. Combining the realistic flare and proton event frequencies with nominal CME & SEP geometries, we find the ozone column for an Earth-like planet can be depleted by 94% in 10 years, with a downward trend that makes recovery unlikely and suggests further destruction. For more extreme stellar inputs O3 depletion allows a constant 0.1-1 W m$^{-2}$ of UV-C at the planet's surface, which is likely detrimental to organic complexity. Our results suggest that active M dwarf hosts may comprehensively destroy ozone shields and subject the surface of magnetically-unprotected Earth-like planets to long-term radiation that can damage complex organic structures. However, this does not preclude habitability, as a safe haven for life could still exist below an ocean surface.
description: Submitted to Astrobiology
Additional file 1: of A realist approach to eliciting the initial programme theory of the antiretroviral treatment adherence club intervention in the Western Cape Province, South Africa
Creators: name: Mukumbang, Ferdinand
name: Marchal, Bruno
name: Belle, Sara Van
name: Wyk, Brian Van
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Pharmacology
subject: Biotechnology
subject: Ecology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: 60506 Virology
subject: Computational Biology

description: A table of documents included in the document review. (DOCX 15 kb)
Tachyon Hair for Two-Dimensional Black Holes
Creators: name: Kostelecky, Alan
name: Perry, Malcolm
Publisher: name: arXiv
Year: 1993
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Using a combination of analytical and numerical methods, we obtain a two-dimensional spacetime describing a black hole with tachyon hair. The physical ADM mass of the black hole is finite. The presence of tachyon hair increases the Hawking temperature.
description: 17 pages, 4 figures (not included), DAMTP-R93-16, IUHET 261 (Sept. 1993)
title: Article_Le Moniteur du bibliophile, du libraire et de l'amateur d'estampes
Creators: name: AmateurS
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2021

description: ID_ARTI_00207
title: ADCO, Grènetier de Cîteaux : comptes (1497-1504) (11 H 1172), f. 00262
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: comptes
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

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. 00262, 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
Minimum-domain impulse theory for unsteady aerodynamic force
Creators: name: Kang, Linlin
name: Liu, Luoqin
name: Su, Weidong
name: Wu, Jiezhi
Publisher: name: arXiv
Year: 2017
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: We extend the impulse theory for unsteady aerodynamics, from its classic global form to finite-domain formulation then to minimum-domain form, and from incompressible to compressible flows. For incompressible flow, the minimum-domain impulse theory raises the finding of Li and Lu (J. Fluid Mech., 712: 598-613, 2012) to a theorem: The entire force with discrete wake is completely determined by only the time rate of impulse of those vortical structures still connecting to the body, along with the Lamb-vector integral thereof that captures the contribution of all the rest disconnected vortical structures. For compressible flow, we find that the global form in terms of the curl of momentum, obtained by Huang (Unsteady Vortical Aerodynamics. Shanghai Jiaotong Univ. Press, 1994), can be generalized to having arbitrary finite domain, but the formula is cumbersome and in general the curl of momentum no longer has discrete structure and hence no minimum-domain theory exists. Nevertheless, as the measure of transverse process only, the unsteady field of vorticity may still have discrete wake. This leads to a minimum-domain compressible vorticity-moment theory in terms of density-weighted vorticity (but it is beyond the classic concept of impulse). These new findings and applications have been confirmed by our numerical experiments. The results not only open an avenue to combine the theory with computation-experiment in wide applications, but also reveals a physical truth that it is no longer necessary to account for all wake vortical structures in computing the force and moment.
title: Αποκατάσταση και επανάχρηση κατοικιών σε σειρά στον οικισμό Βατολάκκου Χανίων και ανάπτυξη εργαστηρίου παρασκευής προϊόντων με πρώτη ύλη τα εσπεριδοειδή του κάμπου
title: Restoration and reuse of houses in a row in the settlement of Vatolakkos Chania and development of a laboratory for manufacturing of citrus -based products
Creators: name: Γεωργιλα Μαρια
Publisher: name: Technical University of Crete
Year: 2024

description: Η παρούσα διπλωματική εργασία μελετά την αποκατάσταση 6+1 παραδοσιακών κατοικιών που αναπτύσσονται σε σειρά στον οικισμό Βατολάκκου Χανίων Κρήτης και την ανάπλαση του άμεσα συνδεδεμένου περιβάλλοντος χώρου για την ανάπτυξη ενός συνεταιρισμού με επίκεντρο τα προϊόντα εσπεριδοειδών. Ο Βατόλακκος βρίσκεται στην ενδοχώρα του Δήμου Πλατανιά,  χτισμένος σε υψόμετρο 100μ. με ένα κτιριακό απόθεμα που αποτελείται τόσο από παραδοσιακές κατοικίες ιστορικής σημασίας όσο και από νεότερα κτίσματα, συνθέτοντας έτσι ένα ενδιαφέροντα αστικό ιστό. Η μορφολογία του εδάφους του παρουσιάζει επίσης ενδιαφέρον καθώς βόρεια του χωριού εκτείνεται η εύφορη κοιλάδα του ποταμού Κερίτη, ο λεγόμενος «κάμπος», μια περιοχή κατάφυτη από εσπεριδοειδή, ενώ νότια του χωριού το ανάγλυφο γίνεται πιο έντονο και οι καλλιέργειες αφορούν κυρίως αμπέλια και ελαιόδεντρα. Βασικός στόχος της εργασίας είναι η αποκατάσταση των παραδοσιακών κατοικιών και η μετατροπή τους σε ξενώνες φιλοξενίας με σεβασμό στην ιστορική τους αξία, καθώς επίσης η ανάπτυξη όλων των απαραίτητων εγκαταστάσεων για την δημιουργία εργαστηρίων παραγωγής προϊόντων με πρώτη ύλη τα εσπεριδοειδή, πωλητήριου και αναψυκτήριου διαχειριζόμενων από την κοινότητα για την ανάδειξη του αγροτικού πλούτου της περιοχής και την προώθηση της βιώσιμης ανάπτυξης του.
Additional file 1: of A Phase I clinical trial of EUS-guided intratumoral injection of the oncolytic virus, HF10 for unresectable locally advanced pancreatic cancer
Creators: name: Hirooka, Yoshiki
name: Kasuya, Hideki
name: Ishikawa, Takuya
name: Kawashima, Hiroki
name: Eizaburo Ohno
name: Villalobos, Itzel
name: Naoe, Yoshinori
name: Ichinose, Toru
name: Nobuto Koyama
name: Tanaka, Maki
name: Kodera, Yasuhiro
name: Goto, Hidemi
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Evolutionary Biology
subject: Sociology
subject: FOS: Sociology
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Cancer
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Table S1. Criteria Defining Resectability Status. (DOCX 18Â kb)
Near-field enhancement and sub-wavelength imaging in the optical region using a pair of two-dimensional arrays of metal nanospheres
Creators: name: Alitalo, Pekka
name: Simovski, Constantin
name: Viitanen, Ari
name: Tretyakov, Sergei
Publisher: name: arXiv
Year: 2006
Subjects: subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: Near-field enhancement and sub-wavelength imaging properties of a system comprising a coupled pair of two-dimensional arrays of resonant nanospheres are studied. The concept of using two coupled material sheets possessing surface mode resonances for evanescent field enhancement is already well established in the microwave region. This paper shows that the same principles can be applied also in the optical region, where the performance of the resonant sheets can be realized with the use of metallic nanoparticles. In this paper we present design of such structures and study the electric field distributions in the image plane of such superlens.
description: 15 pages, 9 figures
Additional file 11 of DNA methylation abnormalities of imprinted genes in congenital heart disease: a pilot study
Creators: name: Chang, Shaoyan
name: Wang, Yubo
name: Xin, Yu
name: Wang, Shuangxing
name: Luo, Yi
name: Wang, Li
name: Zhang, Hui
name: Li, Jia
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 11: Table S2. Primer sequence information of 18 imprinted genes.
Relativistic protons in the Coma galaxy cluster: first gamma-ray constraints ever on turbulent reacceleration
Creators: name: Brunetti, G.
name: Zimmer, S.
name: Zandanel, F.
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: The Fermi-LAT collaboration recently published deep upper limits to the gamma-ray emission of the Coma cluster, a cluster that hosts the prototype of giant radio halos. In this paper we extend previous studies and use a formalism that combines particle reacceleration by turbulence and the generation of secondary particles in the intracluster medium to constrain relativistic protons and their role for the origin of the radio halo. We conclude that a pure hadronic origin of the radio halo is clearly disfavoured as it would require magnetic fields that are too strong. For instance $B_0 > 21 μ$G is found in the cluster center assuming that the magnetic energy density scales with thermal density, to be compared with $B_0 \sim 4-5 μ$G as inferred from Rotation Measures (RM) under the same assumption. However secondary particles can still generate the observed radio emission if they are reaccelerated. For the first time the deep gamma-ray limits allow us to derive meaningful constraints if the halo is generated during phases of reacceleration of relativistic protons and their secondaries by cluster-scale turbulence. In this paper we explore a relevant range of parameter-space of reacceleration models. Within this parameter space a fraction of model configurations is already ruled out by current gamma-ray limits, including the cases that assume weak magnetic fields in the cluster core, $B \leq 2-3 μ$G. Interestingly, we also find that the flux predicted by a large fraction of model configurations that assume a magnetic field consistent with RM is not far from the limits. This suggests that a detection of gamma rays from the cluster might be possible in the near future, provided that the electrons generating the radio halo are secondaries reaccelerated and the magnetic field in the cluster is consistent with that inferred from RM.
description: 22 pages, 12 figures, submitted
Phase behavior of weakly polydisperse sticky hard spheres: Perturbation theory for the Percus-Yevick solution
Creators: name: Fantoni, Riccardo
name: Gazzillo, Domenico
name: Giacometti, Achille
name: Sollich, Peter
Publisher: name: arXiv
Year: 2006
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: We study the effects of size polydispersity on the gas-liquid phase behaviour of mixtures of sticky hard spheres. To achieve this, the system of coupled quadratic equations for the contact values of the partial cavity functions of the Percus-Yevick solution is solved within a perturbation expansion in the polydispersity, i.e. the normalized width of the size distribution. This allows us to make predictions for various thermodynamic quantities which can be tested against numerical simulations and experiments. In particular, we determine the leading-order effects of size polydispersity on the cloud curve delimiting the region of two-phase coexistence and on the associated shadow curve; we also study the extent of size fractionation between the coexisting phases. Different choices for the size-dependence of the adhesion strengths are examined carefully; the Asakura-Oosawa model of a mixture of polydisperse colloids and small polymers is studied as a specific example.
description: 43 pages, 12 figures, and 1 table
Lepton flavor violating Higgs decay at $e^+ e^-$ colliders
Creators: name: Chakraborty, Indrani
name: Mondal, Subhadeep
name: Mukhopadhyaya, Biswarup
Publisher: name: arXiv
Year: 2017
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We estimate the smallest branching ratio for the Higgs decay channel $h \rightarrow μτ$, which can be probed at an $e^+e^-$ collider and compare it with the projected reach at the high-luminosity run of the LHC. Using a model-independent approach, Higgs production is considered in two separate cases. In the first case, $hWW$ and $hZZ$ couplings are allowed to be scaled by a factor allowed by the latest experimental limits on $hWW$ and $hZZ$ couplings. In the second case, we have introduced higher-dimensional effective operators for these interaction vertices. Keeping BR($h\toμτ$) as a purely phenomenological quantity, we find that this branching ratio can be probed down to $\approx 2.69\times 10^{-3}$ and $\approx 5.83\times 10^{-4}$ respectively, at the 250 GeV and 1000 GeV run of an $e^+e^-$ collider.
description: 37 pages, 13 figures, 13 tables
Super--Lax Operator Embedded in Self--Dual Supersymmetric Yang--Mills Theory
Creators: name: Nishino, H.
Publisher: name: arXiv
Year: 1993
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We show that the super-Lax operator for $~N=1$~ supersymmetric Kadomtsev-Petviashvili equation of Manin and Radul in three-dimensions can be embedded into recently developed self-dual supersymmetric Yang-Mills theory in $~2+2\-$dimensions, based on general features of its underlying super-Lax equation. The differential geometrical relationship in superspace between the embedding principle of the super-Lax operator and its associated super-Sato equation is clarified. This result provides a good guiding principle for the embedding of other integrable sub-systems in the super-Lax equation into the four-dimensional self-dual supersymmetric Yang-Mills theory, which is the consistent background for $~N=2$~ superstring theory, and potentially generates other unknown supersymmetric integrable models in lower-dimensions.
description: LATEX (with all macros), 11 pages, UMDEPP 94-47 (October 1993)
title: ADCO, Huitième cartulaire de Saint-Étienne de Dijon (1661-1667), Cart. 31 (G 135), 549 folios, f. 0597
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2012
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: cartulaire
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Huitième cartulaire de Saint-Étienne de Dijon (1661-1667), Archives départementales de la Côte-d'Or, Cart. 31 (G 135), 549 folios, f. 0597, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Huitième cartulaire de Saint-Étienne de Dijon (1661-1667), Archives départementales de la Côte-d'Or, Cart. 31 (G 135), 549 folios, f. 0597, 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
Additional file 12 of DNA methylation abnormalities of imprinted genes in congenital heart disease: a pilot study
Creators: name: Chang, Shaoyan
name: Wang, Yubo
name: Xin, Yu
name: Wang, Shuangxing
name: Luo, Yi
name: Wang, Li
name: Zhang, Hui
name: Li, Jia
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 12: Table S3. The average methylation levels of 18 imprinted genes detected in CHD patients and healthy individuals.
Additional file 13: of Prevalence and antimicrobial resistance of coagulase negative staphylococci clinical isolates from Ethiopia: a meta-analysis
Creators: name: Serawit Deyno
name: Sintayehu Fekadu
name: Sisay Seyfe
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Biotechnology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Hematology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: 60506 Virology

description: Figure S13. Forest plot of the proportion of CoNS resistance to chloramphenicol. (DOCX 18 kb)
Painting with bacteria: Smart templated self assembly using motile bacteria
Creators: name: Arlt, Jochen
name: Martinez, Vincent A
name: Dawson, Angela
name: Pilizota, Teuta
name: Poon, Wilson C K
Publisher: name: arXiv
Year: 2017
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: Biological Physics (physics.bio-ph)
subject: FOS: Physical sciences

description: External control of the swimming speed of `active particles' can be used to self assemble designer structures in situ on the micrometer to millimeter scale. We demonstrate such reconfigurable templated active self assembly in a fluid environment using light powered strains of Escherichia coli. The physics and biology controlling the sharpness and formation speed of patterns is investigated using a bespoke fast-responding strain.
description: 19 pages, 11 figures