cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Fast Domain Growth through Density-Dependent Diffusion in a Driven Lattice Gas
Creators: name: Wickham, L. K.
name: Sethna, J. P.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: We study electromigration in a driven diffusive lattice gas (DDLG) whose continuous Monte Carlo dynamics generate higher particle mobility in areas with lower particle density. At low vacancy concentrations and low temperatures, vacancy domains tend to be faceted: the external driving force causes large domains to move much more quickly than small ones, producing exponential domain growth. At higher vacancy concentrations and temperatures, even small domains have rough boundaries: velocity differences between domains are smaller, and modest simulation times produce an average domain length scale which roughly follows $L \sim t^ζ$, where $ζ$ varies from near .55 at 50% filling to near .75 at 70% filling. This growth is faster than the $t^{1/3}$ behavior of a standard conserved order parameter Ising model. Some runs may be approaching a scaling regime. At low fields and early times, fast growth is delayed until the characteristic domain size reaches a crossover length which follows $L_{cross} \propto E^{-β}$. Rough numerical estimates give $β= >.37$ and simple theoretical arguments give $β= 1/3$. Our conclusion that small driving forces can significantly enhance coarsening may be relevant to the YB$_2$Cu$_3$O$_{7- δ}$ electromigration experiments of Moeckly {\it et al.}(Appl. Phys. Let., {\bf 64}, 1427 (1994)).
description: 18 pages, RevTex3.0
Effects of Redshift Uncertainty on Cross-Correlations of CMB Lensing and Galaxy Surveys
Creators: name: Cawthon, Ross
Publisher: name: arXiv
Year: 2018
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We explore the effects of incorporating redshift uncertainty into measurements of galaxy clustering and cross-correlations of galaxy positions and cosmic microwave background (CMB) lensing maps. We use a simple Gaussian model for a redshift distribution in a redshift bin with two parameters: the mean, $z_0$, and the width, $σ_z$. We vary these parameters, as well as a galaxy bias parameter, $b_{\text{g}}$, and a matter fluctuations parameter, $σ_8$, for each redshift bin, as well as the parameter $Ω_{\text{m}}$, in a Fisher analysis across 12 redshift bins from $z=0-7$. We find that incorporating redshift uncertainties degrades constraints on $σ_8(z)$ in the Large Synoptic Survey Telescope (LSST)/CMB-S4 era by about a factor of 10 compared to the case of perfect redshift knowledge. In our fiducial analysis of LSST/CMB-S4 including redshift uncertainties, we project constraints on $σ_8(z)$ for $z<3$ of less than $5 \%$. Galaxy imaging surveys are expected to have priors on redshift parameters from photometric redshift algorithms and other methods. When adding priors with the expected precision for LSST redshift algorithms, the constraints on $σ_8(z)$ can be improved by a factor of 2-3 compared to the case of no prior information. We also find that `self-calibrated' constraints on the redshift parameters from just the autocorrelation and cross-correlation measurements (with no prior information) are competitive with photometric redshift techniques. In the LSST/CMB-S4 era, we find uncertainty on the redshift parameters ($z_0,σ_z$) to be below 0.004(1+z) at $z<1$. For all parameters, constraints improve significantly if smaller scales can be used. We also project constraints for nearer term survey combinations, Dark Energy Survey (DES)/SPT-SZ, DES/SPT-3G, and LSST/SPT-3G, and analyze how our constraints depend on a variety of parameter and model choices.
description: 22 pages, 22 figures. Updated to match text published by PRD. Main conclusions unchanged, added Section IX and expanded Section VII D. Presented as a thesis to the Department of Astronomy and Astrophysics, The University of Chicago, in partial fulfillment of the requirements for the Ph.D. degree
title: Совершенствование алгоритма лечения острых полиморфных психотических заболеваний
Creators: name: Гапурова, Г.Ф.
name: Усманова, Ш.Ф.
name: Курбаниязова, Ш.Э.
Publisher: name: TASHKENT STATE DENTAL INSTITUTE
Year: 2021
Subjects: subject: FOS: Medical and health sciences
valueUri: http://www.oecd.org/science/inno/38235147.pdf

description: В данной научной статье описаны изменения иммунных параметров крови, вызванные острыми полиморфными психотическими расстройствами, и меры по оптимизации алгоритма лечения путем лечения иммуномодуляторами.
History of the NeoClassical Interpretation of Quantum and Relativistic Physics
Creators: name: Meucci, Shiva
Publisher: name: arXiv
Year: 2018
Subjects: subject: History and Philosophy of Physics (physics.hist-ph)
subject: FOS: Physical sciences

description: The need for revolution in modern physics is a well known and often broached subject, however, the precision and success of current models narrows the possible changes to such a great degree that there appears to be no major change possible. We provide herein, the first step toward a possible solution to this paradox via reinterpretation of the conceptual-theoretical framework while still preserving the modern art and tools in an unaltered form. This redivision of concepts and redistribution of the data can revolutionize expectations of new experimental outcomes. This major change within finely tuned constraints is made possible by the fact that numerous mathematically equivalent theories were direct precursors to, and contemporaneous with, the modern interpretations. In this first of a series of papers, historical investigation of the conceptual lineage of modern theory reveals points of exacting overlap in physical theories which, while now considered cross discipline, originally split from a common source and can be reintegrated as a singular science again. This revival of an older associative hierarchy, combined with modern insights, can open new avenues for investigation. This reintegration of cross-disciplinary theories and tools is defined as the Neoclassical Interpretation.
description: Preprint/Draft. Submission Pending
A Second Bright Source Detected Near SN1987A
Creators: name: Nisenson, Peter
name: Papaliolios, Costas
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Speckle interferometry observations, made just 30 and 38 days after the explosion of supernova SN1987A (SN) (which was first seen on February 23, 1987), showed evidence for a bright source, separated from the SN by only 60 mas. Reprocessing of that data using new image reconstruction algorithms has resulted in much cleaner images which not only clearly show the bright spot reported in 1987, but also a 2nd spot on the opposite side of the SN with a larger spatial separation. If the spots were ejected from the SN then the velocities of the spots are relativistic and the 2nd spot appears to be superluminal and must be blue-shifted. We explore the consequences of these results on the geometry of the SN1987A system, and we conclude that our observations may well be evidence for a relativistic jet emanating from the supernova.
description: 7 pages Latex, 1 figure, accepted for publication in ApJ Letters
Knight Shift Anomalies in Heavy Electron Materials
Creators: name: Kim, Eunsik
name: Makivik, M. S.
name: Cox, D. L.
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: We calculate non-linear Knight Shift $K$ vs. susceptibility $χ$ anomalies for Ce ions possessing local moments in metals. The ions are modeled with the Anderson Hamiltonian and studied within the non-crossing approximation (NCA). The $K-vs.- χ$ non-linearity diminishes with decreasing Kondo temperature $T_0$ and nuclear spin- local moment separation. Treating the Ce ions as an incoherent array in CeSn$_3$, we find excellent agreement with the observed Sn $K(T)$ data.
description: 4 pages, Revtex, 3 figures available upon request from eunsik@pacific.mps.ohio-state.edu
Asilus tipuloides Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Asilidae
Asilus
Asilus tipuloides

description: Asilus tipuloides [spec. nov.]
A. lividus nudus, thoracis lineis dorsalibus tribus nigris.
Fn. svec. 1033.
Habitat in Europa.
description: Published as part of Linnaeus, Carolus, 1758, Systema Naturae per regna tria naturae: secundum classes, ordines, genera, species, cum characteribus, differentiis, synonymis, locis, Stockholm :Laurentius Salvius on page 606, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Magnetically Driven Warping, Precession and Resonances in Accretion Disks
Creators: name: Lai, Dong
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The inner region of the accretion disk onto a rotating magnetized central star (neutron star, white dwarf or T Tauri star) is subjected to magnetic torques which induce warping and precession of the disk. The origin of these torques lies in the interaction between the (induced) surface current on the disk and the horizontal magnetic field (parallel to the disk) produced by the inclined magnetic dipole. Under quite general conditions, there exists a magnetic warping instability in which the magnetic torque drives the disk plane away from the equatorial plane of the star toward a state where the disk normal vector is perpendicular to the spin axis. Viscous stress tends to suppress the warping instability at large radii, but the magnetic torque always dominates as the disk approaches the magnetosphere boundary. The magnetic torque also drives the tilted inner disk into retrograde precession around the stellar spin axis. Moreover, resonant magnetic forcing on the disk can occur which may affect the dynamics of the disk. The magnetically driven warping instability and precession may be related to a number observational puzzles, including: (1) Spin evolution (torque reversal) of accreting X-ray pulsars; (2) Quasi-periodic oscillations in low-mass X-ray binaries; (3) Super-orbital periods in X-ray binaries; (4) Photometric period variations of T Tauri stars.
description: 39 pages including 1 ps figure; Published version; ApJ, 524, 1030-1047 (1999)
Guimaraesiella (Guimaraesiella) aedon Gustafsson & Bush, 2025, sp. nov.
Creators: name: Gustafsson, Daniel R.
name: Bush, Sarah E.
Publisher: name: Zenodo
Year: 2025
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Psocodea
Philopteridae
Guimaraesiella
Guimaraesiella aedon

description: Guimaraesiella (Guimaraesiella) aedon sp. nov.
(Figs 2–3, 5, 9–12)
Type host: Nesospiza questi Lowe, 1923 — Nightingale Island finch.
Type locality: Nightingale Island, Tristan da Cunha Archipelago, South Atlantic.
Diagnosis. See under G. inaccessibilis, above.
Description
Both sexes. Head flat-dome shaped (Fig. 5), frons slightly flattened, lateral margins of preantennal area convex. Dorsal preantennal suture reaches dsms but does not reach ads or lateral margins of head. Head chaetotaxy as in Fig. 5. Thoracic and abdominal segments as in Figs 2–3.
Male. Thoracic and abdominal chaetotaxy as in Fig. 2. Male genitalia as in Figs 9–11. Basal apodeme widening slightly anteriorly (Fig. 9). Proximal mesosome shorter than wide (Fig. 10). Mesosomal lobes with near-parallel lateral margins in proximal end, converging distally; small ridge near lateral margins; 2 ames sensilla on each side near ridge; 1 pmes sensillum and 2 pmes microsetae on each side lateral to gonopore. Gonopore wide proximally, narrowly open distally; wide rugose area follows proximal margin of gonopore, reaching lateral margins of mesosome. Parameral heads large, irregular (Fig. 11). Parameral blades short, slender; pst1 sensilla, near median margin; pst2 microseta, central. Measurements (n = 2): TL = 1.22–1.25; HL = 0.34; HW = 0.31–0.32; PRW = 0.19; PTW = 0.27–0.29; AW = 0.36–0.37.
Female. Thoracic and abdominal chaetotaxy as in Fig. 3. Subgenital plate broadly connected to partial cross-piece (Fig. 12). Vulval margin gently rounded (Fig. 12), with 2–3 long, slender vms on each side, and 3–5 short, thorn-like vss on each side; 5 long, slender vos on each side; distal 1 vos median to vss. Measurements (n = 2, except PTW, where n = 1): TL = 1.59–1.62; HL = 0.37; HW = 0.35–0.36; PRW = 0.22–0.24; PTW = 0.32; AW = 0.42–0.47.
Etymology: The specific name is derived from Greek “ aëdon ” for “nightingale”, referring to the type locality as well as the common name of the type host.
Type material. Ex Nesospiza questi: Holotype ♂, Nightingale Island, Tristan da Cunha Archipelago, South Atlantic, Oct./ Nov. 1988, Peter G. Ryan, N2/3 (NHML). Paratypes: 1♂, 2♀, same data as holotype (NHML).
description: Published as part of Gustafsson, Daniel R. & Bush, Sarah E., 2025, Two new species of Guimaraesiella Eichler, 1949 (Phthiraptera: Ischnocera: Philopteridae) from Tristan da Cunha finches, pp. 363-372 in Zootaxa 5588 (2) on pages 366-370, DOI: 10.11646/zootaxa.5588.2.10, http://zenodo.org/record/14896237
MOESM1 of Prepulse inhibition in patients with bipolar disorder: a systematic review and meta-analysis
Creators: name: Mao, Zhen
name: Bo, Qijing
name: Li, Weidi
name: Wang, Zhimin
name: Ma, Xin
name: Wang, Chuanyue
Publisher: name: figshare
Year: 2019
Subjects: Chemical Sciences not elsewhere classified
Developmental Biology

description: Additional file 1: The search strategy. (DOCX 14 kb)
Local Electronic Structure Changes in Polycrystalline CdTe with CdCl$_2$ Treatment and Air Exposure
Creators: name: Berg, Morgann
name: Kephart, Jason M.
name: Munshi, Amit
name: Sampath, Walajabad S.
name: Ohta, Taisuke
name: Chan, Calvin
Publisher: name: arXiv
Year: 2018
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Applied Physics (physics.app-ph)
subject: Chemical Physics (physics.chem-ph)
subject: Instrumentation and Detectors (physics.ins-det)
subject: FOS: Physical sciences

description: Post-deposition CdCl$_2$ treatment of polycrystalline CdTe is known to increase photovoltaic efficiency. However, the precise chemical, structural, and electronic changes that underpin this improvement are still debated. In this study, spectroscopic photoemission electron microscopy was used to spatially map the vacuum level and ionization energy of CdTe films, enabling the identification of electronic structure variations between grains and grain boundaries. In vacuo preparation and inert transfer of oxide-free CdTe surfaces isolated the separate effects of CdCl$_2$ treatment and ambient oxygen exposure. Qualitatively, grain boundaries displayed lower work function and downward band bending relative to grain interiors, but only after air exposure of CdCl$_2$-treated CdTe. Analysis of numerous space charge regions at grain boundaries (GBs) showed an average depletion width of 290 nm and an average band bending magnitude of 70 meV, corresponding to a GB trap density of 10$^{11}$ cm$^{-2}$ and a net carrier density of 10$^{15}$ cm$^{-3}$. These results suggest that both CdCl$_2$ treatment and oxygen exposure may be independently tuned to enhance CdTe photovoltaic performance by engineering the interface and bulk electronic structure.
Fig. S3: Biotite Mg/Mg+Fe+Mn vs Al diagram of P2 ash layers. Chemical and petrographic fingerprinting of volcanic ashes as a tool for high-resolution stratigraphy of the upper Miocene Pisco Formation (Peru)
Creators: name: Bosio, Giulia
name: Gioncada, Anna
name: Malinverno, Elisa
name: Celma, Claudio Di
name: Villa, Igor M.
name: Cataldi, Giuseppe
name: Gariboldi, Karen
name: Collareta, Alberto
name: Urbina, Mario
name: Bianucci, Giovanni
Publisher: name: Geological Society of London
Year: 2018
Subjects: subject: Geology
subject: FOS: Earth and related environmental sciences

description: Fig. S3: Biotite Mg/Mg+Fe+Mn vs Al diagram of P2 ash layers.
Asilus morio Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Asilidae
Asilus
Asilus morio

description: Asilus morio [spec. nov.]
A. hirtus niger, alis albo nigroque variis.
Habitat in Europa.
Simillimus Muscae Morioni.
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 606, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Fluctuations and Instabilities of Ferromagnetic Domain Wall pairs in an External Magnetic Field
Creators: name: Braun, Hans-Benjamin
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: Soliton excitations and their stability in anisotropic quasi-1D ferromagnets are analyzed analytically. In the presence of an external magnetic field, the lowest lying topological excitations are shown to be either soliton-soliton or soliton-antisoliton pairs. In ferromagnetic samples of macro- or mesoscopic size, these configurations correspond to twisted or untwisted pairs of Bloch walls. It is shown that the fluctuations around these configurations are governed by the same set of operators. The soliton-antisoliton pair has exactly one unstable mode and thus represents a critical nucleus for thermally activated magnetization reversal in effectively one-dimensional systems. The soliton-soliton pair is stable for small external fields but becomes unstable for large magnetic fields. From the detailed expression of this instability threshold and an analysis of nonlocal demagnetizing effects it is shown that the relative chirality of domain walls can be detected experimentally in thin ferromagnetic films. The static properties of the present model are equivalent to those of a nonlinear sigma-model with anisotropies. In the limit of large hard-axis anisotropy the model reduces to a double sine-Gordon model.
description: 15 pages RevTex 3.0 (twocolumn), 9 figures available on request, to appear in Phys Rev B, Dec (1994)
Characterisation and extraction of a Rayleigh-wave mode in vertically-heterogeneous media using Quaternion SVD
Creators: name: Sajeva, Angelo
name: Menanno, Giovanni
Publisher: name: arXiv
Year: 2018
Subjects: subject: Geophysics (physics.geo-ph)
subject: FOS: Physical sciences

description: We propose a method that identifies a mode of Rayleigh waves and separates it from body waves and from other modes, using quaternions to represent multi-component data. Being well known the abilities of quaternions to handle rotations in space, we use previous results derived from Le Bihan and Mars (2004) to prove that a Rayleigh-wave mode recorded by an array of vector-sensors can be approximated by a sum of trace-by-trace rotating time signals. Our method decomposes the signal into narrow-frequency bands, which undergo both a velocity correction and a polarisation correction. The aim of these corrections is to reduce the mode of interest to a quasi-monochromatic wave packet with infinite apparent velocity and quasi-circular polarisation. Once written in quaternion notation, we refer to this wave packet as "quaternion brick". Based on theoretical considerations, we prove that this quaternion brick maps into the first quaternion eigenimage of the Quaternion Singular Value Decomposition. We apply this method to synthetic datasets derived from two vertically-heterogeneous models to extract the fundamental mode and we prove that it is correctly separated from either a higher mode of propagation or body waves with negligible residual. Results are presented in both time-offset and frequency-phase slowness domains.
description: 16 pages, 14 figures
Additional file 1 of Etiology and clinical characteristics of SARS-CoV-2 and other human coronaviruses among children in Zhejiang Province, China 2017–2019
Creators: name: Zhang, Yanjun
name: Su, Lingxuan
name: Chen, Yin
name: Yu, Sicong
name: Zhang, Dan
name: Mao, Haiyan
name: Fang, Lei
Publisher: name: figshare
Year: 2021
Subjects: subject: Biophysics
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Molecular Biology
subject: Biotechnology
subject: Environmental Sciences not elsewhere classified
subject: Biological Sciences not elsewhere classified
subject: Cancer
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Virology

description: Additional file 1. Supplementary table 1. Sequences of oligonucleotides used for molecular analysis.
Studying the morphology of HI isodensity surfaces during reionization using Shapefinders and percolation analysis
Creators: name: Bag, Satadru
name: Mondal, Rajesh
name: Sarkar, Prakash
name: Bharadwaj, Somnath
name: Choudhury, Tirthankar Roy
name: Sahni, Varun
Publisher: name: arXiv
Year: 2018
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Minkowski functionals and Shapefinders shed light on the connectedness of large-scale structure by determining its topology and morphology. We use a sophisticated code, SURFGEN2, to measure the Minkowski functionals and Shapefinders of individual clusters by modelling cluster surfaces using the 'Marching Cube 33' triangulation algorithm. In this paper, we study the morphology of simulated neutral hydrogen (HI) density fields using Shapefinders at various stages of reionization from the excursion set approach. Accompanying the Shapefinders, we also employ the 'largest cluster statistic' (LCS) to understand the percolation process. Percolation curves demonstrate that the non-Gaussianity in the HI field increases as reionization progresses. The large clusters in both the HI overdense and underdense excursion sets possess similar values of "thickness" ($T$), as well as "breadth" ($B$), but their third Shapefinder - "length" ($L$) - becomes almost proportional to their volume. The large clusters in both HI overdense and underdense segments are overwhelmingly filamentary. The 'cross-section' of a filamentary cluster can be estimated using the product of the first two Shapefinders, $T \times B$. Hence the cross sections of the large clusters at the onset of percolation do not vary much with volume and their sizes only differ in terms of their lengths. This feature appears more vividly in HI overdense regions than in underdense regions and is more pronounced at lower redshifts which correspond to an advanced stage of reionization.
description: 19 pages, 15 figures, 1 table, accepted for publication in MNRAS
LUNZ Programme Overview
Creators: name: Sutherland, Lee-Ann
Publisher: name: Zenodo
Year: 2025

description: Presentation to the RIDE (Research and Innovation for our Dynamic Environment) Forum on the genesis and activities of the Land Use for Net Zero Hub

The RIDE forum is made up of 23 public sector member organisations who hold a stake in environmental change research, innovation, training and capabilities, whether that be as funders, providers or users.

The forum’s unique contribution lies in its breadth. It brings together:

the complementary resources of the many different disciplines and publicly funded sector stakeholders needed to increase our understanding of the natural, social, economic and technological systems interacting with environmental change

the translation of that knowledge into innovating policy and practice.

It focuses on the UK perspective and challenges, while placing this in the international context.

The forum aims to enhance the beneficial impact of the UK’s publicly funded research and innovation by informing:

policy and practice to support effective decision-making

the implementation of sustainable solutions that work with our dynamic natural environment.

The forum enables members to align, leverage their resources and avoid duplication through:

sharing and co-developing strategies

joint priority-setting

drawing out interdisciplinary partnership opportunities.

In doing so, members can be more efficient in their use of public funds to give decision-makers the knowledge they need to respond to the challenges and opportunities presented by environmental change.

RIDE is a mechanism that also enables the UK academic community to form independent beneficial and impactful links to the policy and practice community.
The Orion fingers: H$_2$ temperatures and excitation in an explosive outflow
Creators: name: Youngblood, Allison
name: France, Kevin
name: Ginsburg, Adam
name: Hoadley, Keri
name: Bally, John
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We measure H$_2$ temperatures and column densities across the Orion BN/KL explosive outflow from a set of thirteen near-IR H$_2$ rovibrational emission lines observed with the TripleSpec spectrograph on Apache Point Observatory's 3.5-meter telescope. We find that most of the region is well-characterized by a single temperature (~2000-2500 K), which may be influenced by the limited range of upper energy levels (6000-20,000 K) probed by our data set. The H$_2$ column density maps indicate that warm H$_2$ comprises 10$^{-5}$ - 10$^{-3}$ of the total H$_2$ column density near the center of the outflow. Combining column density measurements for co-spatial H$_2$ and CO at T = 2500 K, we measure a CO/H$_2$ fractional abundance of 2$\times$10$^{-3}$, and discuss possible reasons why this value is in excess of the canonical 10$^{-4}$ value, including dust attenuation, incorrect assumptions on co-spatiality of the H$_2$ and CO emission, and chemical processing in an extreme environment. We model the radiative transfer of H$_2$ in this region with UV pumping models to look for signatures of H$_2$ fluorescence from H I Ly$α$ pumping. Dissociative (J-type) shocks and nebular emission from the foreground Orion H II region are considered as possible Ly$α$ sources. From our radiative transfer models, we predict that signatures of Ly$α$ pumping should be detectable in near-IR line ratios given a sufficiently strong source, but such a source is not present in the BN/KL outflow. The data are consistent with shocks as the H$_2$ heating source.
description: 24 pages, 8 figures, 3 tables, accepted to ApJ
Aptera Linnaeus, 1758, ord. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Aptera

description: Aptera [ord. nov.]
VII. APTERA.
Alae nullae, in omni sexu.
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 608, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
MOESM2 of Prepulse inhibition in patients with bipolar disorder: a systematic review and meta-analysis
Creators: name: Mao, Zhen
name: Bo, Qijing
name: Li, Weidi
name: Wang, Zhimin
name: Ma, Xin
name: Wang, Chuanyue
Publisher: name: figshare
Year: 2019
Subjects: subject: Genetics
subject: FOS: Biological sciences
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Science Policy

description: Additional file 2: PRISMA Checklist. (DOC 64 kb)
title: The Digital Workplace : Antecedents and Consequences of Technostress
Creators: name: Becker, Julia
Publisher: name: University of Bayreuth
Year: 2021
Subjects: subject: Technostress
subject: Digital Workplace
subject: Digital Stress
subject: Antecedents of Technostress
subject: Consequences of Technostress
subject: Digital Technologies
subject: 330

description: Digital transformation has a large impact on organizations, affecting their ways of doing business. This development offers many opportunities, for example products and services can be offered in less time, and costs can be reduced. By enabling new forms of collaboration, new markets can be tapped with innovative digital products and solutions. Digital technologies are the major driver of digital transformation. As they found their way into organizations, it did not only influence business models, but the conditions of work have changed tremendously. Todays’ workplaces are digital workplaces that are no longer bound to a certain location or time. While smart workplace technologies facilitate business processes and increase the productivity of the workforce in the digital age, research has shown the potential of digital technologies to cause technostress, a specific form of stress that is perceived by end-users of information and communication technologies. Technostress is considered the dark side of digital transformation. The research papers included in this dissertation, investigate technostress to understand how organizations can enhance and retain the productivity/performance of their employees under the umbrella of digital transformation by avoiding technostress. It allows researchers and practitioners to design and analyze measures countering technostress. The articles contribute to the following current research streams on technostress: environment technology conditions, technology driven spillover effects of demands into the private domain, coping and the mitigation of technostress, and stress outcomes. After evaluation antecedents and consequences of technostress, the last article closes the bracket around the dissertation, proposing an extension of the concept of technostress as a new conceptualization of stress due to digital technology use that fits the new socio-technical context of digital work.
Fig. S5: Biotite Mg/Mg+Fe+Mn vs K+Na+Ca diagram of P2 ash layers. Chemical and petrographic fingerprinting of volcanic ashes as a tool for high-resolution stratigraphy of the upper Miocene Pisco Formation (Peru)
Creators: name: Bosio, Giulia
name: Gioncada, Anna
name: Malinverno, Elisa
name: Celma, Claudio Di
name: Villa, Igor M.
name: Cataldi, Giuseppe
name: Gariboldi, Karen
name: Collareta, Alberto
name: Urbina, Mario
name: Bianucci, Giovanni
Publisher: name: Geological Society of London
Year: 2018
Subjects: subject: Geology
subject: FOS: Earth and related environmental sciences

description: Fig. S5: Biotite Mg/Mg+Fe+Mn vs K+Na+Ca diagram of P2 ash layers.
Measuring the effect of node aggregation on community detection
Creators: name: Gandica, Yérali
name: Decuyper, Adeline
name: Cloquet, Christophe
name: Thomas, Isabelle
name: Delvenne, Jean-Charles
Publisher: name: arXiv
Year: 2018
Subjects: subject: Physics and Society (physics.soc-ph)
subject: Social and Information Networks (cs.SI)
subject: FOS: Physical sciences
subject: FOS: Computer and information sciences

description: Many times the nodes of a complex network, whether deliberately or not, are aggregated for technical, ethical, legal limitations or privacy reasons. A common example is the geographic position: one may uncover communities in a network of places, or of individuals identified with their typical geographical position, and then aggregate these places into larger entities, such as municipalities, thus obtaining another network. The communities found in the networks obtained at various levels of aggregation may exhibit various degrees of similarity, from full alignment to perfect independence. This is akin to the problem of ecological and atomic fallacies in statistics, or to the Modified Areal Unit Problem in geography. We identify the class of community detection algorithms most suitable to cope with node aggregation, and develop an index for aggregability, capturing to which extent the aggregation preserves the community structure. We illustrate its relevance on real-world examples (mobile phone and Twitter reply-to networks). Our main message is that any node-partitioning analysis performed on aggregated networks should be interpreted with caution, as the outcome may be strongly influenced by the level of the aggregation.
description: 12 pages, 5 figures
Continuous Production of Rovibronic Ground State RbCs Molecules via Short-Range Photoassociation to the $b^3Π_{1}-c^3Σ^+_{1}-B^1Π_1$ States
Creators: name: Shimasaki, Toshihiko
name: Kim, Jin-Tae
name: Zhu, Yuqi
name: DeMille, David
Publisher: name: arXiv
Year: 2018
Subjects: subject: Atomic Physics (physics.atom-ph)
subject: FOS: Physical sciences

description: We have investigated rovibronic levels of the strongly mixed $b^3Π_1-c^3Σ^+_1-B^1Π_1$ states [the 2(1), 3(1), and 4(1) states in Hund's case (c) notation] of $^{85}$Rb$^{133}$Cs in the energy range of 13950$-$14200 cm$^{-1}$ using short-range photoassociation (PA). For selected PA states, vibrational and rotational branching in the $X^1Σ^+$ state have been investigated using resonance-enhanced multiphoton ionization and depletion spectroscopy. Efficient production of $^{85}$Rb$^{133}$Cs molecules in the rovibronic ground state $X^1Σ^+ (v=0, J=0)$, at up to $\sim$1$\times 10^4$ molecules/s, has been achieved.
Fig. S1: 39Ar–40Ar step heating results. Chemical and petrographic fingerprinting of volcanic ashes as a tool for high-resolution stratigraphy of the upper Miocene Pisco Formation (Peru)
Creators: name: Bosio, Giulia
name: Gioncada, Anna
name: Malinverno, Elisa
name: Celma, Claudio Di
name: Villa, Igor M.
name: Cataldi, Giuseppe
name: Gariboldi, Karen
name: Collareta, Alberto
name: Urbina, Mario
name: Bianucci, Giovanni
Publisher: name: Geological Society of London
Year: 2018
Subjects: subject: Geology
subject: FOS: Earth and related environmental sciences

description: Fig. S1: 39Ar–40Ar age spectrum of the biotite separate of the tephra layer LB-T11.
High resolution optical and infrared spectroscopic observations of Cir X-1
Creators: name: Johnston, Helen
name: Fender, Rob
name: Wu, Kinwah
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present new optical and infrared (IR) observations of Cir X-1 taken near apastron. Both sets of spectra show asymmetric emission lines. Archival optical observations show that an asymmetric H-alpha emission line has been in evidence for the past twenty years, although the shape of the line has changed significantly. We present an eccentric (e ~ 0.7-0.9) low mass binary model, where the system consists of a neutron star orbiting around a (sub-)giant companion star of 3-5 solar masses. We suggest that the broad components of the emission lines arise in a high-velocity, optically thick flow near the neutron star; while the narrow components of the optical and the IR lines arise near the companion star and a heated ejecta-shell surrounding the binary respectively. In this model, the velocity of the narrow component reflects the space velocity of the binary; the implied radial velocity (+430 km/s after correcting for Galactic rotation) is the highest velocity known for an X-ray binary.
description: 9 pages including 9 figures; accepted for publication in MNRAS; references fixed
Lepisma saccharina Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Zygentoma
Lepismatidae
Lepisma
Lepisma saccharina

description: Lepisma saccharina [spec. nov.]
L. squamosa, cauda triplici.
Brown. jam. 425. Setoura subargentea, cauda setosa, setis hirsutis.
Adam. microgr. t. 28. f 147.
Habitat in America inter saccharum & utensilia domestica, inde per Europam vulgaris, hodie in S{?X} incepit.
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 608, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
Conformal scattering of the Maxwell-scalar field system on de Sitter space
Creators: name: Taujanskas, Grigalius
Publisher: name: arXiv
Year: 2018
Subjects: subject: Analysis of PDEs (math.AP)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Mathematics
subject: FOS: Physical sciences
subject: 83C30, 35Q75, 83C50

description: We prove small data energy estimates of all orders of differentiability between past null infinity and future null infinity of de Sitter space for the conformally invariant Maxwell-scalar field system. This allows us to construct bounded and invertible, but nonlinear, scattering operators taking past asymptotic data to future asymptotic data. We also deduce exponential decay rates for solutions with data having at least two derivatives, and for more regular solutions discover an asymptotic decoupling of the scalar field from the charge. The construction involves a carefully chosen complete gauge fixing condition which allows us to control all components of the Maxwell potential, and a nonlinear Grönwall inequality for higher order estimates.
description: updated to match published version
Lepisma terrestris Linnaeus, 1758, spec. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Zygentoma
Lepismatidae
Lepisma
Lepisma terrestris

description: Lepisma terrestris [spec. nov.]
L. nuda, cauda triplici.
Habitat in Europa.
Similis Podurae sed major, corpore toto albo cylindrico, Antennae corporis dimidii longitudine, obtusae ut in Podura.
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 608, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
MOESM1 of The efficacy and safety of core decompression for the treatment of femoral head necrosis: a systematic review and meta-analysis
Creators: name: Hua, Kun-chi
name: Yang, Xiong-gang
name: Feng, Jiang-tao
name: Wang, Feng
name: Yang, Li
name: Zhang, Hao
name: Hu, Yong-cheng
Publisher: name: figshare
Year: 2019
Subjects: Chemical Sciences not elsewhere classified
Biological Sciences not elsewhere classified
Information Systems not elsewhere classified
Developmental Biology
Science Policy

description: Additional file 1: The searching strategies used in platforms of PubMed and EMBASE. (12.9 KB)
Flux Rope Breaking and Formation of a Rotating Blowout Jet
Creators: name: Joshi, Navin Chandra
name: Nishizuka, Naoto
name: Filippov, Boris
name: Magara, Tetsuya
name: Tlatov, Andrey G.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We analyzed a small flux rope eruption converted into a helical blowout jet in a fan-spine configuration using multi-wavelength observations taken by SDO, which occurred near the limb on 2016 January 9. In our study, first, we estimated the fan-spine magnetic configuration with the potential field calculation and found a sinistral small filament inside it. The filament along with the flux rope erupted upward and interacted with the surrounding fan- spine magnetic configuration, where the flux rope breaks in the middle section. We observed compact brightening, flare ribbons and post-flare loops underneath the erupting filament. The northern section of the flux rope reconnected with the surrounding positive polarity, while the southern section straightened. Next, we observed the untwisting motion of the southern leg, which was transformed into a rotating helical blowout jet. The sign of the helicity of the mini-filament matches the one of the rotating jet. This is consistent with the jet models presented by Adams et al. (2014) and Sterling et al. (2015). We focused on the fine thread structure of the rotating jet and traced three blobs with the speed of 60-120 km/s, while the radial speed of the jet is approx 400 km/s. The untwisting motion of the jet accelerated plasma upward along the collimated outer spine field lines, and it finally evolved into a narrow coronal mass ejection at the height of approx 9 Rsun . On the basis of the detailed analysis, we discussed clear evidence of the scenario of the breaking of the flux rope and the formation of the helical blowout jet in the fan-spine magnetic configuration.
description: 18 pages, 12 figures, Accepted for publication in MNRAS Jouranl
Statistical Mechanics of Nonuniform Magnetization Reversal
Creators: name: Braun, Hans-Benjamin
Publisher: name: arXiv
Year: 1994
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: The magnetization reversal rate via thermal creation of soliton pairs in quasi-1D ferromagnetic systems is calculated. Such a model describes e.g. the time dependent coercivity of elongated particles as used in magnetic recording media. The energy barrier that has to be overcome by thermal fluctuations corresponds to a soliton-antisoliton pair whose size depends on the external field. In contrast to other models of first order phase transitions such as the phi^4 model, an analytical expression for this energy barrier is found for all values of the external field. The magnetization reversal rate is calculated using a functional Fokker-Planck description of the stochastic magnetization dynamics. Analytical results are obtained in the limits of small fields and fields close to the anisotropy field. In the former case the hard-axis anisotropy becomes effectively strong and the magnetization reversal rate is shown to reduce to the nucleation rate of soliton-antisoliton pairs in the overdamped double sine-Gordon model. The present theory therefore includes the nucleation rate of soliton-antisoliton pairs in the double sine-Gordon chain as a special case. These results demonstrate that for elongated particles, the experimentally observed coercivity is significantly lower than the value predicted by the standard theories of Néel and Brown.
description: 21 pages RevTex 3.0 (twocolumn), 6 figures available on request, to appear in Phys Rev B, Dec (1994)
Topology of the Universe: background and recent observational approaches
Creators: name: Roukema, Boudewijn F.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Is the Universe (a spatial section thereof) finite or infinite? Knowing the global geometry of a Friedmann-Lema\^ıtre (FL) universe requires knowing both its curvature and its topology. A flat or hyperbolic (``open'') FL universe is {\em not} necessarily infinite in volume. Multiply connected flat and hyperbolic models are, in general, as consistent with present observations on scales of 1-20{\hGpc} as are the corresponding simply connected flat and hyperbolic models. The methods of detecting multiply connected models (MCM's) are presently in their pioneering phase of development and the optimal observationally realistic strategy is probably yet to be calculated. Constraints against MCM's on ~1-4 h^{-1} Gpc scales have been claimed, but relate more to inconsistent assumptions on perturbation statistics rather than just to topology. Candidate 3-manifolds based on hypothesised multiply imaged objects are being offered for observational refutation. The theoretical and observational sides of this rapidly developing subject have yet to make any serious contact, but the prospects of a significant detection in the coming decade may well propel the two together.
description: 5 pages, proceedings of the Workshop ``Cosmology: Observations Confront Theories,'' 11-17 Jan 1999, IIT Kharagpur, West Bengal, to appear in Pramana - Journal of Physics
Colors and Shapes of the Irregular Planetary Satellites
Creators: name: Graykowski, Ariel
name: Jewitt, David
Publisher: name: arXiv
Year: 2018
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: It is widely recognized that the irregular satellites of the giant planets were captured from initially heliocentric orbits. However, the mechanism of capture and the source region from which they were captured both remain unknown. We present an optical color survey of 43 irregular satellites of the outer planets conducted using the LRIS camera on the 10-meter telescope at the Keck Observatory in Hawaii. The measured colors are compared to other planetary bodies in search for similarities and differences that may reflect upon the origin of the satellites. We find that ultrared matter (with color index B-R $\ge$ 1.6), while abundant in the Kuiper belt and Centaur populations, is depleted from the irregular satellites. We also use repeated determinations of the absolute magnitudes to make a statistical estimate of the average shape of the irregular satellites. The data provide no evidence that the satellites and the main-belt asteroids are differently shaped, consistent with collisions as the major agent shaping both.
description: 35 pages, 10 figures
Podura Linnaeus, 1758, gen. nov.
Creators: name: Linnaeus, Carolus
Publisher: name: Laurentius Salvius
Year: 1758
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Entognatha
Collembola
Poduridae
Podura

description: Podura [gen. nov.]
Pedes VI, cursorii.
Oculi II, compositi ex octonis.
Cauda bifurca, saltatrix, inflexa.
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 608, DOI: 10.5962/bhl.title.542, http://zenodo.org/record/3922206
title: ADCO, Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome VI, Cart. 190 (11 H 75), 316 folios, f. 0017r
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: cartulaire
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge

description: Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome VI, Archives départementales de la Côte-d'Or, Cart. 190 (11 H 75), 316 folios, f. 0017r, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Cartulaire général de Cîteaux, dit de Jean de Cirey, (XVe siècle), tome VI, Archives départementales de la Côte-d'Or, Cart. 190 (11 H 75), 316 folios, f. 0017r, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https:// manuscrits.cbma-project.eu/
description: Provenance: http://www.wikidata.org/entity/Q843261
description: Provenance: https://www.geonames.org/3024876
description: Provenance: http://www.idref.fr/030974844/id
description: Provenance: https://catalogue.bnf.fr/ark:/12148/cb12228351v
description: Provenance: abbaye de Cîteaux