cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
A new universal ratio in Random Matrix Theory and chaotic to integrable transition in Type-I and Type-II hybrid Sachdev-Ye-Kitaev models
Creators: name: Sun, Fadi
name: Yi-Xiang, Yu
name: Ye, Jinwu
name: Liu, W. -M.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: High Energy Physics - Theory (hep-th)
subject: Chaotic Dynamics (nlin.CD)
subject: FOS: Physical sciences

description: We investigate chaotic to integrable transition in two types of hybrid SYK models which contain both $ q=4 $ SYK with interaction $ J $ and $ q=2 $ SYK with an interaction $ K $ in type-I or $(q=2)^2$ SYK with an interaction $ \sqrt{K} $ in type-II. These models include hybrid Majorana fermion, complex fermion and bosonic SYK. For the Majorana fermion case, we discuss both $ N $ even and $ N $ odd case. We make exact symmetry analysis on the possible symmetry class of both types of hybrid SYK in the 10 fold way by Random Matrix Theory (RMT) and also work out the degeneracy of each energy levels. We introduce a new universal ratio which is the ratio of the next nearest neighbour (NNN) energy level spacing to characterize the RMT. We perform exact diagonalization to evaluate both the known NN ratio and the new NNN ratio, then use both ratios to study Chaotic to Integrable transitions (CIT) in both types of hybrid SYK models. Some preliminary results on possible quantum analog of Kolmogorov-Arnold-Moser (KAM) theorem and its dual version in the quantum chaotic side are given. We explore some intrinsic connections between the two complementary approaches to quantum chaos: the RMT and the Lyapunov exponent by the $ 1/N $ expansion in the large $ N $ limit at a suitable temperature range. Comments on some previously related works are given. Some future perspectives, especially the failure of the Zamoloddchikov's c-theorem in 1d CFT RG flow are outlined.
description: 23 pages, 14 figures, REVTEX4
Supercritical Disk Accretion with Mass Loss
Creators: name: Lipunova, Galina V.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We consider supercritical accretion onto a compact object when the accretion rate exceeds its value derived from the Eddington limit: L_{Edd}/c^2. We use the scenario that was proposed by Shakura and Sunyaev (1973) for the supercritical regime, according to which matter flows out of the gas-disk surface under radiation pressure. An analytic solution of the accretion-disk structure is obtained for this scenario by using classical equations. An attempt is made to construct a model for nonconservative supercritical accretion with advection. To this end, we develop a numerical scheme for calculating the structure of an advective disk with mass outflow. The goal of solving the problem of a supercritical disk with mass loss is to explain accreting sources with outflowing envelopes, for example, SS 433 and galactic nuclei. The structure and observational manifestations of the envelope which forms around a supercritical disk are considered by taking into account bremsstrahlung absorption and Thomson scattering of photons.
description: 26 pages, 8 figures, Latex2e, will appear in Astronomy Letters
WWF: a generator for e+e- to 4 fermions + gamma
Creators: name: van Oldenborgh, Geert Jan
name: Franzini, Paula. J.
name: Borrelli, Arianna
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We present an efficient generator for the process e+e- to 4 fermions + gamma through off-shell W pairs. It is based on a massless matrix element with leading order(m^2) corrections. Only the resonant WW graphs are included. We have tested it against a matrix element without these approximations and found agreement to within ~1% at LEPII energies.
description: 13 pages incl 2 figures, latex+axodraw, full ps file available as ftp://pss058.psi.ch/pub/preprints/wwf.ps, PSI-PR-94-06
Ultraviolet and Multiwavelength Variability of the Blazar 3C 279: Evidence for Thermal Emission
Creators: name: Pian, E.
name: Urry, C. M.
name: Maraschi, L.
name: Madejski, G.
name: McHardy, I. M.
name: Koratkar, A.
name: Treves, A.
name: Chiappetti, L.
name: Grandi, P.
name: Hartman, R. C.
name: Kubo, H.
name: Leach, C. M.
name: Pesce, J. E.
name: Imhoff, C.
name: Thompson, R.
name: Wehrle, A. E.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The gamma-ray blazar 3C 279 was monitored on a nearly daily basis with IUE, ROSAT and EGRET for three weeks between December 1992 and January 1993. During this period, the blazar was at a historical minimum at all wavelengths. Here we present the UV data obtained during the above multiwavelength campaign. A maximum UV variation of ~50% is detected, while during the same period the X-ray flux varied by no more than 13%. At the lowest UV flux level the average spectrum in the 1230-2700 A interval is unusually flat for this object (~1). The flattening could represent the lowest energy tail of the inverse Compton component responsible for the X-ray emission, or could be due to the presence of a thermal component at ~20000 K possibly associated with an accretion disk. The presence of an accretion disk in this blazar object, likely observable only in very low states and otherwise hidden by the beamed, variable synchrotron component, would be consistent with the scenario in which the seed photons for the inverse Compton mechanism producing the gamma-rays are external to the relativistic jet. We further discuss the long term correlation of the UV flux with the X-ray and gamma-ray fluxes obtained at various epochs. All UV archival data are included in the analysis. Both the X- and gamma-ray fluxes are generally well correlated with the UV flux, approximately with square root and quadratic dependences, respectively.
description: 22 pages, Latex, 7 PostScript figures, to appear in The Astrophysical Journal
Additional file 4: of Radial probe endobronchial ultrasound using a guide sheath for peripheral lung lesions in beginners
Creators: name: Eom, Jung
name: Mok, Jeong
name: Insu Kim
name: Lee, Min
name: Geewon Lee
name: Hyemi Park
name: Lee, Ji
name: Jeong, Yeon
name: Kim, Won-Young
name: Jo, Eun
name: Kim, Mi
name: Kwangha Lee
name: Kim, Ki
name: Park, Hye-Kyung
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Developmental Biology

description: A detailed description of the cumulative sum analysis. (DOCX 14 kb)
Blood manganese level and gestational diabetes mellitus: a systematic review and meta-analysis
Creators: name: Sun, Yingmei
name: Zhang, Yu
Publisher: name: Taylor & Francis
Year: 2023
Subjects: subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Biotechnology
subject: Chemical Sciences not elsewhere classified
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Mathematical Sciences not elsewhere classified
subject: Science Policy

description: Previous studies evaluating the relationship between blood manganese (Mn) level and gestational diabetes mellitus (GDM) in pregnant women showed inconsistent results. A systematic review and meta-analysis was therefore performed to investigate the above association. Relevant observational studies were obtained by search of electronic databases including Medline, Embase, Cochrane Library and Web of Science from database inception to 10 March 2023. Two authors independently performed database search, literature identification and data extraction. A randomised-effects model was selected to pool the data by incorporating the influence of potential heterogeneity. Subgroup analysis was performed to evaluate the influence of study characteristics on the results of the meta-analysis. Six datasets from five observational studies, involving 91,249 pregnant women were included in the meta-analysis. Among the participants, 3597 (3.9%) were diagnosed as GDM. Overall, pooled results showed that a high blood level of Mn was associated with a higher risk of GDM (compared between women with highest versus lowest category blood Mn, odds ratio: 1.31, 95% confidence interval: 1.19–1.44, p < .001) with no significant heterogeneity (p for Cochrane Q-test = 0.93, I2 = 0%). Subgroup analyses according to study design, mean maternal age, matrix or methods for measuring blood Mn, and the incidence of GDM also showed consistent results (p for subgroup difference all >.05). Results of the meta-analysis suggest that a high blood Mn level may be a risk factor of GDM in pregnant women. Studies are needed to determine the underlying mechanisms, and to investigate if the relationship between blood Mn level and GDM is dose-dependent. Changes of blood manganese (Mn) have been suggested to be involved in the pathogenesis of diabetes. However, the relationship between blood Mn level and gestational diabetes mellitus (GDM) in pregnant women remains undetermined. Our study represents the first systematic review and meta-analysis to investigate the potential association between blood Mn concentration and the risk of GDM. In this meta-analysis, we pooled the results of six datasets from five observational and showed that compared to pregnant women with the lowest category of blood Mn level, those with the highest category of blood Mn level were associated with a higher risk of GDM. These results suggest that a high blood concentration of Mn in pregnant women may be a risk factor of GDM.
Phase transition and heat engine efficiency of phantom AdS black holes
Creators: name: Mo, Jie-Xiong
name: Lan, Shan-Quan
Publisher: name: arXiv
Year: 2018
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: Phase transition and heat engine efficiency of phantom AdS black holes are investigated with peculiar properties found. In the non-extended phase space, we probe the possibility of $T-S$ criticality in both the canonical ensemble and grand-canonical ensemble. It is shown that no $T-S$ criticality exists for the phantom AdS black hole in the canonical ensemble, which is different from the RN-AdS black hole. Contrary to the canonical ensemble, no critical point can be found for neither phantom AdS black holes nor RN-AdS black hole in the grand-canonical ensemble. Moreover, we study the specific heat at constant electric potential. When the electric potential satisfies $A_0>1$, only phantom AdS black holes undergo phase transition in the grand-canonical ensemble. In the extended phase space, we show that there is no $P-V$ criticality for phantom AdS black holes, contrary to the case of the RN-AdS black hole. Furthermore, we define a new kind of heat engine via phantom AdS black holes. Comparing to RN-AdS black holes, phantom AdS black holes have a lower heat engine efficiency. However, the ratio $η/η_C$ of phantom AdS black hole is higher, thus increasing the possibility of approaching the Carnot limit. This observation is obviously of interest. The interesting results obtained in this paper may be attributed to the existence of phantom field whose energy density is negative.
description: 9pages,4figures. Comments welcome
MOESM1 of Toll-like Receptor 4 (TLR4) Antagonist Eritoran Tetrasodium Attenuates Liver Ischemia and Reperfusion Injury through Inhibition of High-Mobility Group Box Protein B1 (HMGB1) Signaling
Creators: name: McDonald, Kerry-Ann
name: Huang, Hai
name: Tohme, Samer
name: Loughran, Patricia
name: Ferrero, Kimberly
name: Billiar, Timothy
name: Tsung, Allan
Publisher: name: figshare
Year: 2014
Subjects: subject: Biochemistry
subject: Physical Sciences not elsewhere classified
subject: Medicine
subject: Molecular Biology
subject: Neuroscience
subject: Physiology
subject: FOS: Biological sciences
subject: Chemical Sciences not elsewhere classified
subject: Immunology
subject: FOS: Clinical medicine
subject: Mental Health

description: Supplementary material, approximately 1.04 MB.
Donax trunculus Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Bivalvia
Veneroida
Donacidae
Donax
Donax trunculus

description: Donax trunculus [spec. nov.]
D. testa antice laevi, intus violacea marginibus crenatis
List. angl. 190. t. 5. f. 35.
Bonan. recr. 2. t. 47.
Gualt. test. t. 88. f. 0.
Argenv. conch. t. 25. f. L.
Habitat in Oceano Europaeo.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on pages 682-683, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Additional file 1 of Physiological characterization of chitin synthase A responsible for the biosynthesis of cuticle chitin in Culex pipiens pallens (Diptera: Culicidae)
Creators: name: Yang, Xiaoshan
name: Xu, Yang
name: Yin, Qi
name: Zhang, Hongbo
name: Yin, Haitao
name: Sun, Yan
name: Ma, Lei
name: Zhou, Dan
name: Shen, Bo
Publisher: name: figshare
Year: 2021
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Zoology

description: Additional file 1: Table S1. Gene-specific primers for the amplification of the CHSA cDNA from Culex pipiens pallens. Table S2. Gene-specific primers for qPCR. qPCR, quantitative real-time PCR. Table S3. Gene-specific primers for RNAi. RNAi, RNA interference; siRNA, small interfering RNA. Table S4. CpCHSA sequences used for polyclonal antibody preparation.
Status of the superworld: from theory to experiment
Creators: name: Lopez, J.
name: Nanopoulos, D.
name: Zichichi, A.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Review to appear in Progress in Particle and Nuclear Physics. Contents: {1}Introduction}{1} {2}High precision LEP data and convergence of couplings: physics is not Euclidean geometry}{2} {3}Interconnections between the measured quantities due to Unification}{7} {4}The origin of $M_{SUSY}$ and why it should be abandoned: masses and spectra are needed}{13} {5}The new step forward: Supergravity}{21} {6}The SU(5) Supergravity Model}{22} {7}SU(5)xU(1) Supergravity}{32} {8}Detailed calculations for the Tevatron}{47} {9}Detailed calculations for LEP}{48} {10}Detailed calculations for HERA}{53} {11}Detailed calculations for Underground Labs and Underwater facilities}{55} {12}Detailed calculations for indirect experimental detection}{65} {13}The problem of mass and $m_t$}{73} {14}Conclusions}{77}
description: 90 pages, 41 figures (not included), latex. Send requests for hard copies to "engsterj@cernvm.bitnet". CERN-TH.7136/94, CTP-TAMU-80/93
Donax pubescens Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Bivalvia
Veneroida
Donacidae
Donax
Donax pubescens

description: Donax pubescens [spec. nov.]
D. testa antice spinis ciliata. M. L. U.
Habitat in O. Indico.
Testa argute decussatim striata: antice plana laterum angulo carinato, versus apicem spinis e striis enatis membranaceis ciliato. Rima hians ovata: nymphis nudis. Anus ovato-oblongus.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 682, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
The fragmentation properties of massive protocluster gas clumps: an ALMA study
Creators: name: Fontani, F.
name: Commerçon, B.
name: Giannetti, A.
name: Beltrán, M. T.
name: Sánchez-Monge, Á.
name: Testi, L.
name: Brand, J.
name: Tan, J. C.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Fragmentation of massive dense molecular clouds is the starting point in the formation of rich clusters and massive stars. Theory and numerical simulations indicate that the population of the fragments (number, mass, diameter, separation) resulting from the gravitational collapse of such clumps is probably regulated by the balance between the magnetic field and the other competitors of self-gravity, in particular turbulence and protostellar feedback. We have observed 11 massive, dense and young star-forming clumps with the Atacama Large Millimeter Array (ALMA) in the thermal dust continuum emission at $\sim 1$~mm with an angular resolution of 0.25 arcseconds with the aim of determining their population of fragments. We find fragments on sub-arcsecond scales in 8 out of the 11 sources. The ALMA images indicate two different fragmentation modes: a dominant fragment surrounded by companions with much smaller mass and size, and many ($\geq 8$) fragments with a gradual change in masses and sizes. On average, the largest number of fragments is found towards the warmer and more massive clumps. Also, the warmer clumps tend to form fragments with larger mass and size. To understand the role of the different physical parameters to regulate the final population of the fragments, we have simulated the collapse of a massive clump of $100$ and $300$ M$_{\odot}$ having different magnetic support. The simulations indicate that: (1) fragmentation is inhibited when the initial turbulence is low, independent of the other physical parameters. (2) a filamentary distribution of the fragments is favoured in a highly magnetised clump. We conclude that the clumps that show many fragments distributed in a filamentary-like structure are likely characterised by a strong magnetic field, while the others are possible also in a weaker magnetic field.
description: 20 pages, 11 figures, 2 Appendices, accepted for publication in A/&A
Chemically Consistent Evolutionary Models with Dust
Creators: name: Möller, C. S.
name: Alvensleben, U. Fritze-v.
name: Fricke, K. J.
name: Calzetti, D.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: As a tool to interpret nearby and high redshift galaxy data from optical to K-band we present our chemically consistent spectrophotometric evolutionary synthesis models. These models take into account the increasing initial metallicity of successive stellar generations using recently published metallicity dependent stellar evolutionary tracks, stellar yields and model atmosphere spectra. The influence of the metallicity is analysed. Dust absorption is included on the basis of gas content and abundance as it varies with time and galaxy type. We compare our models with IUE template spectra and are able to predict UV fluxes for different spectral types. Combined with a cosmological model we obtain evolutionary and k-corrections for various galaxy types and show the differences to models using only solar metallicity input physics as a function of redshift, wavelength band and galaxy type.
description: 8 pages, 2 figures, to appear in the proceedings of the conference "The Evolution of Galaxies on Cosmological Timescales", Tenerife, Spain, December 1998
The exceptional X-ray properties of the NLSy1 galaxy RXJ 0134.3-4258
Creators: name: Komossa, Stefanie
name: Breitschwerdt, Dieter
name: Greiner, Jochen
name: Meerschweinchen, Janek
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The Narrow-line Seyfert 1 galaxy RXJ0134.3-4258 was detected during the ROSAT all-sky survey with an ultrasoft spectrum (Greiner 1996). Our later pointed observation led to the discovery of drastic spectral variability. Here, we present the first detailed analysis of the soft X-ray properties of this peculiar source.
description: 4 pages incl. 2 figures (needs crckapb.sty); contribution to the proc. of `Astrophysical Dynamics' (Evora, April 14-16, 1999), to appear in Ap&SS; Preprint and related papers on RXJ0134.3-4258 are available at http://www.xray.mpe.mpg.de/~skomossa/
Inconsistency of QED in the Presence of Dirac Monopoles II
Creators: name: He, Hong-Jian
name: Qiu, Zhaoming
name: Tze, Chia-Hsiung
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We enlarge the local gauge invariance of QED from $~U(1)_A~$ to $~U(1)_A \times U(1)_Θ~$ by introducing another unphysical pure gauge field $~Θ~$ with an independent, unphysical gauge coupling $~\tilde{e}~$. This pure gauge field can be gauge-transformed away and the resulting theory is {\it identical to} standard QED. We then re-examine the Dirac quantization condition (DQC) for point monopoles and find that two essentially different DQCs can be derived. One DQC involves a gauge coupling $~e~$ in the $~U(1)_A~$ group and the other only the unphysical gauge coupling $~\tilde{e}~$ in the $~U(1)_Θ~$ group. The unique physically consistent solution of these two DQCs is a vanishing magnetic charge, which implies that no Dirac monopole exists in nature.
description: Pages: 8; Report#: VPI-IHEP-93-13
Geschlechtergerechte frühkindliche Betreuung: Eine Forschungsarbeit zur Förderung von Geschlechtergerechtigkeit in Kitas durch die Soziale Arbeit
Creators: name: Giger, Sarah
Publisher: name: Hochschule Luzern – Soziale Arbeit
Year: 2024

description: Die vorliegende Bachelorarbeit von Sarah Giger untersucht Geschlechtergerechtigkeit in der
frühkindlichen Betreuung. Trotz gesetzlich verankerter Gleichstellung der Geschlechter, sind
Frauen und Menschen anderer Geschlechter gegenüber Männern in der Schweiz
benachteiligt. Die frühkindliche Phase ist eine sehr prägende Zeit für die Entwicklung der
Geschlechtsidentität. Eine Erziehung, die sich an stereotypen Rollenvorstellungen der
Geschlechter orientiert, birgt Nachteile für Kinder aller Geschlechter. Eine
geschlechtersensible Pädagogik ist deshalb ein wichtiger Teil der frühkindlichen Bildung und
Betreuung. Die qualitative Untersuchung der Kitas in der Stadt Bern hat ergeben, dass
Konzepte zu Geschlechtergerechtigkeit an vielen Orten bereits vorhanden sind, die Umsetzung
aber nicht überall gewährleistet ist. Um Verbesserungen in diesem Bereich zu erreichen,
müssen die Rahmenbedingungen in der Schweiz untersucht werden. Es wird aufgezeigt, dass
die Arbeitsbedingungen der Kitas kritisierbar sind und im internationalen Vergleich die Schweiz
bei der frühkindlichen Betreuung auf den hintersten Plätzen steht. In der Sozialen Arbeit der
Schweiz fehlt der Diskurs zu Kitas im Gegensatz zu Deutschland, wo ein Diskurs zu Kita-
Sozialarbeit geführt wird und aufgrund dessen Projekte etabliert wurden. Zur Förderung der
Geschlechtergerechtigkeit in Kitas besteht die Aufgabe der Sozialen Arbeit darin,
niederschwellige Schulungsangebote zu erstellen und sich auf sozialpolitischer Ebene für die
Verbesserungen der Rahmenbedingungen von Kitas einzusetzen. Die Soziale Arbeit in der
Schweiz muss das Potential des Arbeitsfelds Kita als Handlungsfeld erkennen.
description: + Code Diss LU: hslusa bask + Fussnote: Bachelor-Arbeit, Hochschule Luzern – Soziale Arbeit, Studienrichtung Soziokultur, 2024 + NL-Code: NLLUHSA202401
Additional file 9: of Implementing advance care planning in nursing homes â study protocol of a cluster-randomized clinical trial
Creators: name: SĂŚvareid, Trygve
name: Lillemoen, Lillian
name: Thoresen, Lisbeth
name: FĂ¸Rde, Reidun
name: Gjerberg, Elisabeth
name: Pedersen, Reidar
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Developmental Biology
subject: Cancer
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Changes to the project. (DOCX 13 kb)
Mass estimation in the outer regions of galaxy clusters
Creators: name: Diaferio, Antonaldo
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a technique for estimating the mass in the outskirts of galaxy clusters where the usual assumption of dynamical equilibrium is not valid. The method assumes that clusters form through hierarchical clustering and requires only galaxy redshifts and positions on the sky. We apply the method to dissipationless cosmological N-body simulations where galaxies form and evolve according to semi-analytic modelling. The method recovers the actual cluster mass profile within a factor of two to several megaparsecs from the cluster centre. This error originates from projection effects, sparse sampling, and contamination by foreground and background galaxies. In the absence of velocity biases, this method can provide an estimate of the mass-to-light ratio on scales ~1-10 Mpc/h where this quantity is still poorly known.
description: 14 pages, 7 figures, MN LaTeX style, MNRAS, in press
$γγ$ Production of Non--Strongly Interacting SUSY Particles at Hadron Colliders
Creators: name: Ohnemus, J.
name: Walsh, T. F.
name: Zerwas, P. M.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Non--strongly interacting supersymmetric particles -- sleptons, charginos, neutral\-inos, and charged Higgs bosons -- are difficult to detect at the Large Hadron Collider. We therefore examine the possibility of producing particles of this type in virtual $γγ$ collisions at the LHC. Since photons can be emitted from protons which do not break up in the radiation process, very clean events can be generated, compensating to some extent for the small event numbers. Higher rates are expected, at the expense of stray hadrons, for events in which one or two protons break up.
description: 6 pages plus 2 postscript figures appended as uuencoded compressed tar file, DESY 93--173, UCD--93--39
title: ADCO, Ordre cistercien : comptes (1403-1423) (11 H 1161), f. 00239
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: comptes
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge

description: Ordre cistercien : comptes (1403-1423), Archives départementales de la Côte-d'Or, (11 H 1161). Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Ordre cistercien : comptes (1403-1423), Archives départementales de la Côte-d'Or, (11 H 1161), f. 00239, in Projet CBMA - Corpus Burgundiae Medii Aevi \[Ressource en ligne\], https:// manuscrits.cbma-project.eu/
Klinische Sozialarbeit mit suchtbetroffenen Personen: «So könnte die Planung der Nachsorge gelingen»
Creators: name: Tankoy, Manuel
Publisher: name: Hochschule Luzern – Soziale Arbeit
Year: 2024

description: Die Organisation der Nachsorge für suchtbetroffene Personen gehört zu den Kernaufgaben der Klinischen Sozialarbeit. Dieser Auftrag wird von verschiedenen Faktoren beeinflusst. Ein Hauptaugenmerk dieser Bachelorarbeit liegt in der gründlichen Analyse dieser Fakoren.
Ein weiterer Schwerpunkt dieser Bachelorarbeit liegt in der Verdeutlichung der Relevanz einer systemischen Ausrichtung in der Nachsorgeplanung mit suchtbetroffenen Personen. Die Betonung liegt hierbei zum einen in der Einbindung von Modellen und Abklärungsprozessen, die ein ganzheitliches Bild der Betroffenen vermitteln. Zum anderen in der Errichtung von Kolloborationen, die essenziel in der Entwicklung von langfristigen Lösungen sind.
Abschliessend werden klare Handlungsempfehlungen für die Klinische Sozialarbeit präsentiert, die darauf abzielen, die Zusammenarbeit mit suchtbetroffenen Personen im klinischen Kontext zu verbessern. Trotz klinischen, politischen und gesellschaftlichen Vorgaben sollen diese Empfehlungen dazu beitragen, eine effektive Unterstützung und Nachsorge für suchterkrankte Personen zu ermöglichen.
Diese Bachelorarbeit trägt somit zur Entwicklung effektiverer Lösungsansätze in der Unterstützung von suchterkrankten Personen bei und verdeutlicht, wie die Klinische Sozialarbeit einen wertvollen Beitrag zur Verbesserung der Lebensqualität von suchtbetroffenen leisten kann.
description: + Code Diss LU: hslusa basa + Fussnote: Bachelor-Arbeit, Hochschule Luzern – Soziale Arbeit, Studienrichtung Sozialarbeit, 2024 + NL-Code: NLLUHSA202401
Numerical hydrodynamics in special relativity
Creators: name: Marti, Jose M.
name: Mueller, Ewald
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: This review is concerned with a discussion of numerical methods for the solution of the equations of special relativistic hydrodynamics (SRHD). Particular emphasis is put on a comprehensive review of the application of high-resolution shock-capturing methods in SRHD. Results obtained with different numerical SRHD methods are compared, and two astrophysical applications of SRHD flows are discussed. An evaluation of the various numerical methods is given and future developments are analyzed.
description: submitted to the electronic journal Living Reviews in Relativity, at http://www.livingreviews.org 72 pages, 14 postscript figures included
Additional file 1 of A biodegradable PVA coating constructed on the surface of the implant for preventing bacterial colonization and biofilm formation
Creators: name: Lei, Zhonghua
name: Liang, Haifeng
name: Sun, Wei
name: Chen, Yan
name: Huang, Zhi
name: Yu, Bo
Publisher: name: figshare
Year: 2024
Subjects: subject: Biophysics
subject: Space Science
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Biotechnology
subject: Chemical Sciences not elsewhere classified
subject: Ecology
subject: Biological Sciences not elsewhere classified
subject: Cancer
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Virology

description: Additional file 1: Fig. S1. The process of coating titanium plate with 5% PVA. Fig. S2. In vivo assessment of PVA coating on implants 2 h after operation. A Plate coating 2 weeks after the operation, bar = 10 mm. B Crystal violet staining of the implant. C and D Quantitative results of colony formation around the implant. E and F Quantitative results of crystal violet staining on the implant Data are represented as means ± SD. Significant differences are indicated as **(p < 0.05). Fig. S3. In vivo assessment of PVA coating on implants 24 h after operation. A Plate coating 2 weeks after the operation, bar = 10 mm. B Crystal violet staining of the implant. C and D Quantitative results of colony formation around the implant. E and F Quantitative results of crystal violet staining on the implant Data are represented as means ± SD. Significant differences are indicated as **(p < 0.05).
Donax denticulata Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Mollusca
Bivalvia
Veneroida
Donacidae
Donax
Donax denticulata

description: Donax denticulata [spec. nov.]
D. testa antice obtusissima, labiis transverse rugosis, margine denticulato, nymphis dentiformibus.
Habitat in M. Mediterraneo. F. Logie.
Testa cuneiformis, laevis, longitudinaliter punctato striata, albida, purpurascenti-subfasciata. Vulva subrotunda, minima; antice obtusissima, area media transverse rugosa, laterali recta; margo denticulatus. Intus albicans.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 683, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Additional file 3: of Radial probe endobronchial ultrasound using a guide sheath for peripheral lung lesions in beginners
Creators: name: Eom, Jung
name: Mok, Jeong
name: Insu Kim
name: Lee, Min
name: Geewon Lee
name: Hyemi Park
name: Lee, Ji
name: Jeong, Yeon
name: Kim, Won-Young
name: Jo, Eun
name: Kim, Mi
name: Kwangha Lee
name: Kim, Ki
name: Park, Hye-Kyung
Publisher: name: figshare
Year: 2018
Subjects: subject: Space Science
subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Developmental Biology

description: The definition of cumulative sum analysis. (DOCX 15 kb)
Beziehungsgestaltung im erwachsenenschutzrechtlichen Verfahren mit alkoholabhängigen Personen: Welche Herausforderungen bestehen bei einem erwachsenenschutzrechtlichen Verfahren im Rahmen von der Gesprächsführung und der Beziehungsgestaltung mit alkoholabhängigen Personen?
Creators: name: Messerschmidt, Serena
Publisher: name: Hochschule Luzern – Soziale Arbeit
Year: 2024

description: Die vorliegende Bachelorarbeit befasst sich mit der Beziehungsgestaltung im erwachsenenschutzrechtlichen Verfahren mit alkoholabhängigen Personen und untersucht die Frage: Welche Methoden werden während der Abklärung angewendet und mit welchen Herausforderungen sehen sich die Fachpersonen in der Abklärung konfrontiert?

Die Autorin widmet sich drei wesentlichen Themen: die verschiedenen Facetten der Alkoholabhängigkeit, das erwachsenenschutzrechtliche Verfahren sowie die Vielfalt von Methoden in der Förderung von Beziehungsgestaltung. Im praktischen Teil wird anhand von Leitfadeninterviews mit drei Expertinnen der KESB des Kantons Luzern der Umgang in der Abklärung mit alkoholabhängigen Personen ausgewertet.

Die Ergebnisse zeigen, dass die Beziehungsgestaltung mit vielen Herausforderungen verknüpft sind. Auf die Gesprächsführung wirken sich kognitive und krankheitsbedingte Einschränkungen der abzuklärenden Personen erschwerend aus. Zur Förderung der Beziehungsgestaltung nutzen die befragten Expert*innen im Berufsalltag einen nicht festgelegten Methodenpluralismus zur Motivation. Dabei zeigt sich, dass u.a. die systemisch und lösungsorientierte Gesprächsführung und auch die motivierende Gesprächsführung in der Abklärung eingesetzt wird. Erweiterte Massnahmen zur Alkohol-Prävention werden gewünscht. Im Weiteren lassen sich sozialdemographische Unterschiede feststellen, was die gesellschaftliche Akzeptanz von Alkoholkonsum betrifft.
description: + Code Diss LU: hslusa basa + Fussnote: Bachelor-Arbeit, Hochschule Luzern – Soziale Arbeit, Studienrichtung Sozialarbeit, 2024 + NL-Code: NLLUHSA202401
title: A Study of pulmonary function in asbestosis
Creators: name: Regan, GM
Publisher: name: London School of Hygiene & Tropical Medicine
Year: 1977

description: 258 workers in three asbestos factories were examined, by clinical, radiological and pulmonary function tests. Rales was found in 35 workers (14%), approximately 2/3 of whom had radiological changes, most commonly both pleural and parenchymal, 63% had disturbed lung function and 38#, clubbing. Those with radiological abnormality 93 (37%) had lower values for TLco and VC than those without. Either pleural or parerchymal abnormality occurred in Isolation in 43 (46%). Clubbing occurred in 35% of those with both changes together who often had other abnormalities and the lowest mean values for TLco and VC. Airways obstruction was found in some individuals with asbestosis. Pulmonary function and pleural or parenchymal abnormality are probably the earliest signs of asbestosis, rales, clubbing and pleural and parenchymal changes together, appear later. No evidence for more asbestosis in smokers than non-smokers was found. Doubt was cast on the methods of certification as some certified workers had minimal grounds for certification, other uncertified workers had good evidence of the disease. An objective method for evaluating the results of any individual was obtained by using principal component analysis. TLco and VC were the best indicators of general lung disease, FEV/VC%, cough and phlegm of airways obstructive disease and radiological abnormality, rales and finger clubbing of asbestosis. A correlation between exposure and disease (as measured by component l) in factories B and U but not in factory M suggested that chrysotile, used at M, is less dangerous than amosite (at U) and amosite plus croeidolite (at B). Lack of comparable past dust figures in the three factories casts doubt on this conclusion.
An $α^{2}(Z α)^{5}m$ Contribution to the Hydrogen Lamb Shift from Virtual Light by Light Scattering
Creators: name: Eides, Michael I.
name: Grotch, Howard
name: Pebler, Peter
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The radiative correction to the Lamb shift of order $α^{2}(Zα)^5m$ induced by the light by light scattering insertion in external photons is obtained. The new contribution turns out to be equal to $-0.122(2)α^2(Zα)^5/(πn^3)(m_r/m)^3m$. Combining this contribution with our previous results we obtain the complete correction of order $α^{2}(Zα)^5m$ induced by all diagrams with closed electron loops. This correction is $37.3(1)$ kHz and $4.67(1)$ kHz for the $1S$- and $2S$-states in hydrogen, respectively.
description: pages, Penn State Preprint PSU/TH/142, February 1994
Quantum key distribution with phase-encoded coherent states: Asymptotic security analysis in thermal-loss channels
Creators: name: Papanastasiou, Panagiotis
name: Lupo, Cosmo
name: Weedbrook, Christian
name: Pirandola, Stefano
Publisher: name: arXiv
Year: 2018
Subjects: subject: Quantum Physics (quant-ph)
subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: We consider discrete-alphabet encoding schemes for coherent-state quantum key distribution. The sender encodes the letters of a finite-size alphabet into coherent states whose amplitudes are symmetrically distributed on a circle centered in the origin of the phase space. We study the asymptotic performance of this phase-encoded coherent-state protocol in direct and reverse reconciliation assuming both loss and thermal noise in the communication channel. In particular, we show that using just four phase-shifted coherent states is sufficient for generating secret key rates of the order of $4 \times 10^{-3}$ bits per channel use at about 15 dB loss in the presence of realistic excess noise.
description: REVTeX. 8 pages. 7 figures
Stability and Carrier Transport Properties of Phosphorene Based Polymorphic Nanoribbons
Creators: name: Kaur, Sumandeep
name: Kumar, Ashok
name: Srivastava, Sunita
name: Pandey, Ravindra
name: Tankeshwar, K.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: A few-layer black phosphorene has recently gained significant interest in the scientific community. In this paper, we consider several polymorphs of phosphorene nanoribbons (PNRs) and employ deformation potential theory within the effective mass approximation together with density functional theory to investigate their structural, mechanical and electronic properties. The results show that stability of PNRs strongly depends on the direction along which they can be cut from 2D counterpart. PNRs also exhibit a wide range of line stiffness ranging from 6x10^10 eV/m to 18x10^11 eV/m which has little dependence on the edge passivation. Likewise, the calculated electronic properties of PNRs display them to be either narrow-gap semiconductor (Eg < 1 eV) or wide-gap semiconductor (Eg > 1 eV). The carrier mobility of PNRs is found to be comparable to that of the black phosphorene. Some of the PNRs show n-type (p-type) semiconducting character owing to their higher electron (hole) mobility. Passivation of the edges leads to n-type p-type transition in many of the PNRs considered. The predicted novel characteristics of PNRs with a wide range of mechanical and electronic properties make PNRs to be potentially suitable for the use in nanoscale devices.
description: 20 pages, 5 figures, 1 table
Carnet nº 4, commencé à Novorossiïsk (p. 55)
Creators: name: Péraire, Lucien
name: CNRS
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2023

description: created: 8-5-1929
The Extended Blue Continuum and Line Emission around the Central Radio Galaxy in Abell 2597
Creators: name: Koekemoer, A. M.
name: O'Dea, C. P.
name: Sarazin, C. L.
name: McNamara, B. R.
name: Donahue, M.
name: Voit, G. M.
name: Baum, S. A.
name: Gallimore, J. F.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present results from detailed imaging of the centrally dominant radio elliptical galaxy in the cooling flow cluster Abell 2597, using data obtained with the Wide Field and Planetary Camera 2 (WFPC2) on the Hubble Space Telescope (HST). This object is one of the archetypal "blue-lobed" cooling flow radio elliptical galaxies, also displaying a luminous emission-line nebula, a compact radio source, and a significant dust lane and evidence of molecular gas in its center. We show that the radio source is surrounded by a complex network of emission-line filaments, some of which display a close spatial association with the outer boundary of the radio lobes. We present a detailed analysis of the physical properties of ionized and neutral gas associated with the radio lobes, and show that their properties are strongly suggestive of direct interactions between the radio plasma and ambient gas. We resolve the blue continuum emission into a series of knots and clumps, and present evidence that these are most likely due to regions of recent star formation. We investigate several possible triggering mechanisms for the star formation, including direct interactions with the radio source, filaments condensing from the cooling flow, or the result of an interaction with a gas-rich galaxy, which may also have been responsible for fueling the active nucleus. We propose that the properties of the source are plausibly explained in terms of accretion of gas by the cD during an interaction with a gas-rich galaxy, which combined with the fact that this object is located at the center of a dense, high-pressure ICM can account for the high rates of star formation and the strong confinement of the radio source.
description: Astrophysical Journal, in press, 34 pages, includes 6 PostScript figures. Latex format, uses aaspp4.sty and epsf.sty files
Multiple paths of deuterium fractionation in protoplanetary disks
Creators: name: Aikawa, Yuri
name: Furuya, Kenji
name: Hincelin, Ugo
name: Herbst, Eric
Publisher: name: arXiv
Year: 2018
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We investigate deuterium chemistry coupled with the nuclear spin-state chemistry of H$_2$ and H$_3^+$ in protoplanetary disks. Multiple paths of deuterium fractionation are found; exchange reactions with D atoms, such as HCO$^+$ + D, are effective in addition to those with HD. In a disk model with grain sizes appropriate for dark clouds, the freeze-out of molecules is severe in the outer midplane, while the disk surface is shielded from UV radiation. Gaseous molecules, including DCO$^+$, thus become abundant at the disk surface, which tends to make their column density distribution relatively flat. If the dust grains have grown to millimeter size, the freeze-out rate of neutral species is reduced, and the abundances of gaseous molecules, including DCO$^+$ and N$_2$D$^+$, are enhanced in the cold midplane. Turbulent diffusion transports D atoms and radicals at the disk surface to the midplane, and stable ice species in the midplane to the disk surface. The effects of turbulence on chemistry are thus multifold; while DCO$^+$ and N$_2$D$^+$ abundances increase or decrease depending on the regions, HCN and DCN in the gas and ice are much reduced at the innermost radii, compared with the model without turbulence. When cosmic rays penetrate the disk, the ortho-to-para ratio (OPR) of H$_2$ is found to be thermal in the disk, except in the cold ($\lesssim 10$ K) midplane. We also analyze the OPR of H$_3^+$ and H$_2$D$^+$, as well as the main reactions of H$_2$D$^+$, DCO$^+$, and N$_2$D$^+$ to analytically derive their abundances in the cold midplane.
description: accepted to ApJ
Ficus exasperata Vahl 1805
Creators: name: Rasplus, Jean-Yves
name: Harry, Myriam
name: Perrin, Hélène
name: Chassagnard, Marie-Thérèse
name: Lachaise, Daniel
Publisher: name: Zenodo
Year: 2003
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Rosales
Moraceae
Ficus
Ficus exasperata

description: Ficus exasperata Vahl, 1805
Savane niveau Cité-2 Base Technique 850 m, Forêt colline Gban 600 m, 580 m, 570 m, 560 m; Cité 1 près Zouguépo 500 m, Gbakoré 500 m, zone des bambous 500 m, savane de Bossou 550 m.
 Figuier dioïque abondant présentant dans la région du Nimba une importante variabilité intra-arbre (voire intrarameau) des feuilles qui rappelle celle de F. asperifolia.
description: Published as part of Rasplus, Jean-Yves, Harry, Myriam, Perrin, Hélène, Chassagnard, Marie-Thérèse & Lachaise, Daniel, 2003, Les Ficus (Moraceae) et l'entomofaune des figues (Hym. Agaonidae, Pteromalidae, Torymidae, Eurytomidae; Dipt. Drosophilidae; Col. Curculionidae) du mont Nimba en Guinée, pp. 107-182 in Mémoires du Muséum national d'Histoire naturelle 190 on page 114, DOI: 10.5281/zenodo.10683835
A Radio Polarimetric Study of the Galactic Center Threads
Creators: name: Lang, Cornelia C.
name: Morris, Mark
name: Echevarria, Luis
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Multi-frequency, polarimetric VLA observations of the non-thermal filaments (NTF's), G0.08+0.15, and G359.96+0.09, also known as the Northern and Southern Threads are presented at 20, 6, 3.6 and 2 cm, with high enough spatial resolution to be resolved for the first time at 6 and 3.6 cm. The 20 cm image reveals a wealth of new detail in the radio sources lying within the inner 60 pc of the Galaxy. The Southern Thread has a prominent split along its length, similar to splitting at the ends of previously studied NTF's. With resolutions as fine as 2'', the 3.6 and 6 cm images reveal a high degree of continuity and little substructure internal to the filament. The spectral index of the Northern Thread has been determined over a broad range of frequencies. Its flux density falls with frequency, alpha=-0.5 between 90 and 6 cm, and becomes much steeper (alpha=-2.0) between 6 and 2 cm. The spectral index does not vary significantly along the length of the Northern Thread, which implies either that the diffusion timescale for the emitting electrons is less than their synchrotron lifetime, or that the emitting electrons are reaccelerated continuously at multiple positions along the filament. Because of the lack of spectral index variation, we have not located the source of relativistic electrons. Polarization observations at 6 and 3.6 cm confirm the non-thermal nature of the emission from the Northern Thread. The fractional polarization in the Northern Thread reaches 70% in some regions, although the polarized emission is patchy. Large rotation measures (RM > 2000 rad/m2) have been observed with irregular variations across the filament.The intrinsic magnetic field in the Northern Thread is predominantly aligned along its long axis.
description: 19 pages, incl. 24 figs; to appear in the Astrophysical Journal