cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Multiple scattering effects on inclusive particle production in the large-x regime
Creators: name: Kang, Zhong-Bo
name: Vitev, Ivan
name: Xing, Hongxi
Publisher: name: arXiv
Year: 2013
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: Nuclear Experiment (nucl-ex)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We study the multiple scattering effects on inclusive particle production in p+A and $γ$+A collisions. Specifically, we concentrate on the region where the parton momentum fraction in the nucleus $x\sim {\cal O}(1)$ and incoherent multiple interactions are relevant. By taking into account both initial-state and final-state double scattering, we derive the nuclear size-enhanced power corrections to the differential cross section for single inclusive hadron production in p+A and $γ$+A reactions, and for prompt photon production in p+A reactions. We find that the final result can be written in a simple compact form in terms of four-parton correlation functions, in which the second-derivative, first-derivative and non-derivative terms of the correlation distributions share the same hard-scattering functions. We expect our result to be especially relevant for understanding the nuclear modification of particle production in the backward rapidity regions in p+A and e+A collisions.
description: 12 pages, 3 figures
Dense gas and star formation in the Outer Milky Way
Creators: name: Braine, Jonathan
name: Sun, Yan
name: Shimajiri, Yoshito
name: van der Tak, Floris F. S.
name: Fang, Min
name: André, Philippe
name: Chen, Hao
name: Gao, Yu
Publisher: name: arXiv
Year: 2023
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present maps and spectra of the HCN(1-0) and HCO$^+$(1-0) lines in the extreme outer Galaxy, at galactocentric radii between 14 and 22 kpc, with the 13.7 meter Delingha telescope. The 9 molecular clouds were selected from a CO/$^{13}$CO survey of the outer quadrants. The goal is to better understand the structure of molecular clouds in these poorly studied subsolar metallicity regions and the relation with star formation. The lines are all narrow, less than 2km/s at half power, enabling detection of the HCN hyperfine structure in the stronger sources and allowing us to observationally test hyperfine collision rates. The hyperfine line ratios show that the HCN emission is optically thin with column densities estimated at N(HCN)~$3x10^{12}$\scm. The HCO$^+$ emission is approximately twice as strong as the HCN (taken as the sum of all components), in contrast with the inner Galaxy and nearby galaxies where they are similarly strong. For an abundance ratio $χ_{HCN}/χ_{HCO^+} = 3$, this requires a relatively low density solution for the dense gas, with n(H2) $\sim 10^3 - 10^4$\ccm. The $^{12}$CO/$^{13}$CO line ratios are similar to solar neighborhood values, roughly 7.5, despite the low $^{13}$CO abundance expected at such large radii. The HCO$^+$/CO and HCO$^+$/$^{13}$CO integrated intensity ratios are also standard at about 1/35 and 1/5 respectively. HCN is weak compared to the CO emission, with HCN/CO $\sim 1/70$ even after summing all hyperfine components. At the parsec scales observed here, the correlation between star formation, as traced by 24~$μ$m emission as is standard in extragalactic work, and dense gas via the HCN or HCO$^+$ emission, is poor, perhaps due to the lack of dynamic range. We find that the lowest dense gas fractions are in the sources at high galactic latitude (b>2, h>300pc above the plane), possibly due to lower pressure.
description: 17 pages, 14 figures
Additional file 2 of AI-assisted evidence screening method for systematic reviews in environmental research: integrating ChatGPT with domain knowledge
Creators: name: Zuo, Chen
name: Yang, Xiaohao
name: Errickson, Josh
name: Li, Jiayang
name: Hong, Yi
name: Wang, Runzi
Publisher: name: figshare
Year: 2025
Subjects: subject: Artificial Intelligence and Image Processing
subject: FOS: Computer and information sciences

description: Supplementary Material 2
Probing holography in $p$-adic CFT
Creators: name: Ebert, Stephen
name: Sun, Hao-Yu
name: Zhang, Meng-Yang
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: We holographically calculate the partition functions of certain types of isotropic sectors of the CFTs dual to Bruhat-Tits trees and $p$-adic BTZ black holes. Along the way, we propose new spectral decompositions of the Laplacian operator other than the plane-wave basis on these two types of background, with both analytical and numerical evidence. We extract the density of states and hence entropy from the BTZ partition function via the inverse Laplace transform. Then the one-loop Witten diagram is computed in the $p$-adic BTZ black hole background, yielding constraints on the heavy-heavy-light averaged three-point coefficient of its boundary $p$-adic CFT. Finally, for general $p$-adic CFTs (not necessarily holographic), we analyze the representation theory of their global conformal group $PGL\left(2,\mathbb{Q}_p\right)$, and discuss the suitability of different representations as Hilbert spaces of $p$-adic CFT.
description: v3: 59 pages; published version
Psychological Resilience after Hurricane Sandy: The Influence of Individual- and Community-Level Factors on Mental Health after a Large-Scale Natural Disaster
Creators: name: Lowe, Sarah R.
name: Sampson, Laura
name: Gruebner, Oliver
name: Galea, Sandro
Publisher: name: Columbia University
Year: 2015
Subjects: Organizational resilience
Natural disasters--Economic aspects
Natural disasters--Psychological aspects
Hurricane Sandy (2012)
Mental health
Economics
Epidemiology

description: Several individual-level factors are known to promote psychological resilience in the aftermath of disasters. Far less is known about the role of community-level factors in shaping postdisaster mental health. The purpose of this study was to explore the influence of both individual- and community-level factors on resilience after Hurricane Sandy. A representative sample of household residents (N = 418) from 293 New York City census tracts that were most heavily affected by the storm completed telephone interviews approximately 13–16 months postdisaster. Multilevel multivariable models explored the independent and interactive contributions of individual- and community-level factors to posttraumatic stress and depression symptoms. At the individual-level, having experienced or witnessed any lifetime traumatic event was significantly associated with higher depression and posttraumatic stress, whereas demographic characteristics (e.g., older age, non-Hispanic Black race) and more disaster-related stressors were significantly associated with higher posttraumatic stress only. At the community-level, living in an area with higher social capital was significantly associated with higher posttraumatic stress. Additionally, higher community economic development was associated with lower risk of depression only among participants who did not experience any disaster-related stressors. These results provide evidence that individual- and community-level resources and exposure operate in tandem to shape postdisaster resilience.
Additional file 1 of Application of the electronic book to promote self-directed learning in medical technologist continuing education: a cross-sectional study
Creators: name: Wen, Chiao-Ni
name: Huang, Chung-Guei
name: Chang, Pi-Yueh
name: Yang, Tsung-Han
name: You, Huey-Ling
name: Ning, Hsiao-Chen
name: Tsao, Kuo-Chien
Publisher: name: figshare
Year: 2022
Subjects: subject: Science Policy
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences

description: Additional file 1: Table S1. Demographic characteristics and CE learning styles of participants.
UV-excess sources with a red/IR-counterpart: low-mass companions, debris disks and QSO selection
Creators: name: Verbeek, Kars
name: Groot, Paul J.
name: Scaringi, Simone
name: Casares, Jorge
name: Corral-Santana, Jesus M.
name: Deacon, Niall
name: Drew, Janet E.
name: Gänsicke, Boris T.
name: González-Solares, Eduardo
name: Greimel, Robert
name: Heber, Ulrich
name: Napiwotzki, Ralf
name: Østensen, Roy H.
name: Steeghs, Danny
name: Wright, Nicholas J.
name: Zijlstra, Albert
Publisher: name: arXiv
Year: 2013
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We present the result of the cross-matching between UV-excess sources selected from the UV-excess survey of the Northern Galactic Plane (UVEX) and several infrared surveys (2MASS, UKIDSS and WISE). From the position in the (J-H) vs. (H-K) colour-colour diagram we select UV-excess candidate white dwarfs with an M-dwarf type companion, candidates that might have a lower mass, brown-dwarf type companion, and candidates showing an infrared-excess only in the K-band, which might be due to a debris disk. Grids of reddened DA+dM and sdO+MS/sdB+MS model spectra are fitted to the U,g,r,i,z,J,H,K photometry in order to determine spectral types and estimate temperatures and reddening. From a sample of 964 hot candidate white dwarfs with (g-r)<0.2, the spectral energy distribution fitting shows that ~2-4% of the white dwarfs have an M-dwarf companion, ~2% have a lower-mass companion, and no clear candidates for having a debris disk are found. Additionally, from WISE 6 UV-excess sources are selected as candidate Quasi-Stellar Objects (QSOs). Two UV-excess sources have a WISE IR-excess showing up only in the mid-IR W3 band of WISE, making them candidate Luminous InfraRed Galaxies (LIRGs) or Sbc star-burst galaxies.
description: Accepted for publication in MNRAS
Partition functions of non-Lagrangian theories from the holomorphic anomaly
Creators: name: Fucito, Francesco
name: Grassi, Alba
name: Morales, Jose Francisco
name: Savelli, Raffaele
Publisher: name: arXiv
Year: 2023
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: The computation of the partition function in certain quantum field theories, such as those of the Argyres-Douglas or Minahan-Nemeschansky type, is problematic due to the lack of a Lagrangian description. In this paper, we use the holomorphic anomaly equation to derive the gravitational corrections to the prepotential of such theories at rank one by deforming them from the conformal point. In the conformal limit, we find a general formula for the partition function as a sum of hypergeometric functions. We show explicit results for the round sphere and the Nekrasov-Shatashvili phases of the $Ω$ background. The first case is relevant for the derivation of extremal correlators in flat space, whereas the second one has interesting applications for the study of anharmonic oscillators.
description: 37 pages, references added
Die katholische Homo-Paranoia und die Würde des schwulen Katholiken
Creators: name: Brinkschröder, Michael
Publisher: name: Werkstatt Schwule Theologie
Year: 1970

description: Werkstatt Schwule Theologie, Bd. 9 Nr. 4 (2002): Werkstatt Schwule Theologie, Band 9, Heft 4
Additional file 1 of AI-assisted evidence screening method for systematic reviews in environmental research: integrating ChatGPT with domain knowledge
Creators: name: Zuo, Chen
name: Yang, Xiaohao
name: Errickson, Josh
name: Li, Jiayang
name: Hong, Yi
name: Wang, Runzi
Publisher: name: figshare
Year: 2025
Subjects: subject: Artificial Intelligence and Image Processing
subject: FOS: Computer and information sciences

description: Supplementary Material 1: Text appendix show the Title & screening prompt and Full-text screening prompt. Tables show a search queries for datasets; an articles identified results; the article screening results of Steps 1 and 2; the criteria’s different versions in Steps 1 and 2; the screening results of ChatGPT-3.5 Turbo in Steps 1 and 2; the review results of human reviewers in Steps 1 and 2; the human reviewer and ChatGPT’s screening result of test set articles in Steps 1 and 2; the Cohen’s Kappa score of ChatGPT-3.5 Turbo at Steps 1 and 2; the Cohen’s Kappa score of human reviewers at Steps 1 and 2.
Additional file 1 of Medical students’ experiences of working with simulated patients in challenging communication training
Creators: name: Isaksson, Johan
name: Krabbe, Julia
name: Ramklint, Mia
Publisher: name: figshare
Year: 2022
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy

description: Additional file 1: Supplementary Table 1. Summaries of the standardized patient cases, with main goal and suggested use of communication tools.
Stability boundaries and collisions of two-dimensional solitons in PT-symmetric couplers with the cubic-quintic nonlinearity
Creators: name: Burlak, Gennadiy
name: Malomed, Boris A.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Pattern Formation and Solitons (nlin.PS)
subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: We introduce one- and two-dimensional (1D and 2D) models of parity-time ($% \mathcal{PT}$) -symmetric couplers with the mutually balanced linear gain and loss applied to the two cores, and cubic-quintic (CQ) nonlinearity acting in each one. The 2D and 1D models may be realized in dual-core optical waveguides, in the spatiotemporal and spatial domains, respectively. Stationary solutions for $\mathcal{PT}$-symmetric solitons in these systems reduce to their counterparts in the usual coupler. The most essential problem is the stability of the solitons, which become unstable against symmetry breaking with the increase of the energy (norm), and retrieve the stability at still larger energies. The boundary value of the intercore-coupling constant, above which the solitons are completely stable, is found by means of an analytical approximation, based on the CW (zero-dimensional) counterpart of the system. The approximation demonstrates good agreement with numerical findings for the 1D and 2D solitons. Numerical results for the stability limits of the 2D solitons are obtained by means of the computation of eigenvalues for small perturbations, and verified in direct simulations. Although large parts of the solitons families are unstable, the instability is quite weak. Collisions between 2D solitons in the $\mathcal{PT}$-symmetric coupler are studied by means of simulations. Outcomes of the collisions are inelastic but not destructive, as they do not break the $\mathcal{PT}$ symmetry.
description: Physical Review E, in press
Circumgalactic Medium on the Largest Scales: Detecting X-ray Absorption Lines with Large-Area Microcalorimeters
Creators: name: Bogdan, Akos
name: Khabibullin, Ildar
name: Kovacs, Orsolya
name: Schellenberger, Gerrit
name: ZuHone, John
name: Burchett, Joseph
name: Dolag, Klaus
name: Churazov, Eugene
name: Forman, William
name: Jones, Christine
name: Kilbourne, Caroline
name: Kraft, Ralph
name: Lau, Erwin
name: Markevitch, Maxim
name: McCammon, Dan
name: Nagai, Daisuke
name: Nelson, Dylan
name: Ogorzalek, Anna
name: Oppenheimer, Benjamin
name: Sarkar, Arnab
name: Su, Yuanyuan
name: Truong, Nhut
name: Veilleux, Sylvain
name: Vladutescu-Zopp, Stephan
name: Zhuravleva, Irina
Publisher: name: arXiv
Year: 2023
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: The circumgalactic medium (CGM) plays a crucial role in galaxy evolution as it fuels star formation, retains metals ejected from the galaxies, and hosts gas flows in and out of galaxies. For Milky Way-type and more massive galaxies, the bulk of the CGM is in hot phases best accessible at X-ray wavelengths. However, our understanding of the CGM remains largely unconstrained due to its tenuous nature. A promising way to probe the CGM is via X-ray absorption studies. Traditional absorption studies utilize bright background quasars, but this method probes the CGM in a pencil beam, and, due to the rarity of bright quasars, the galaxy population available for study is limited. Large-area, high spectral resolution X-ray microcalorimeters offer a new approach to exploring the CGM in emission and absorption. Here, we demonstrate that the cumulative X-ray emission from cosmic X-ray background sources can probe the CGM in absorption. We construct column density maps of major X-ray ions from the Magneticum simulation and build realistic mock images of nine galaxies to explore the detectability of X-ray absorption lines arising from the large-scale CGM. We conclude that the OVII absorption line is detectable around individual massive galaxies at the $3σ-6σ$ confidence level. For Milky Way-type galaxies, the OVII and OVIII absorption lines are detectable at the $\sim\,6σ$ and $\sim\,3σ$ levels even beyond the virial radius when co-adding data from multiple galaxies. This approach complements emission studies, does not require additional exposures, and will allow probing of the baryon budget and the CGM at the largest scales.
description: 16 pages, 8 figures, accepted for publication in ApJ
Cosmic Topology : Twenty Years After
Creators: name: Luminet, Jean-Pierre
Publisher: name: arXiv
Year: 2013
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: What is the shape of the Universe? Is it finite or infinite ? Is space multi-connected to create ghost images of faraway cosmic sources? After a "dark age" period, the field of cosmic topology has now become one of the major concerns in astronomy and cosmology, not only from theorists but also from observational astronomers. Here I give a personal account of the spectacular progress in the field since the beginning of the 1990's, when I started to work in it.
description: 14 pages. Contribution to a special issue of the journal "Gravitation and Cosmology" devoted to the 75th birthday of Prof. Andrey Grib. Version 2 (some sentences have been rephrased to avoid text overlap with arXiv:1303.5086, arXiv:1303.4226, arXiv:1104.0015 by other authors). arXiv admin note: text overlap with arXiv:0802.2236
Additional file 3 of AI-assisted evidence screening method for systematic reviews in environmental research: integrating ChatGPT with domain knowledge
Creators: name: Zuo, Chen
name: Yang, Xiaohao
name: Errickson, Josh
name: Li, Jiayang
name: Hong, Yi
name: Wang, Runzi
Publisher: name: figshare
Year: 2025
Subjects: subject: Artificial Intelligence and Image Processing
subject: FOS: Computer and information sciences

description: Supplementary Material 3
Global gyrokinetic simulations of the impact of magnetic island on ion temperature gradient driven turbulence
Creators: name: Li, J. C.
name: Xu, J. Q.
name: Qu, Y. R.
name: Lin, Z.
name: Dong, J. Q.
name: Peng, X. D.
name: Li, J. Q.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Plasma Physics (physics.plasm-ph)
subject: FOS: Physical sciences

description: The effect of island width on the multi-scale interactions between magnetic island (MI) and ion temperature gradient (ITG) turbulence has been investigated based on the global gyrokinetic approach. It is found that the coupling between the island and turbulence is enhanced when the MI width (w) becomes larger. A vortex flow that is highly sensitive to the width of the magnetic island can be triggered, ultimately resulting in a potent shear flow and a consequent reduction in turbulent transport. The shearing rate induced by the vortex flow is minimum at the O-point while it is maximum at both of the two reconnection points of the island, i.e., the X-points, regardless of the island width. There exists a nonmonotonic relationship between zonal flow (ZF) amplitude and island width, showing that the ZF is partially suppressed by medium-sized MIs whereas enhanced in the case of large island. A larger MI can tremendously damage the ITG mode structure, resulting in higher turbulent transport at the X-point whereas a lower one at the O-point, respectively. Such phenomenon will be less distinct at very small island widths below w/a =8% (a is the minor radius), where it shows that turbulence near the X-point is hardly affected although it is still suppressed inside the island. Furthermore, the influence of different island sizes on turbulence transport level is also discussed.
Ab initio calculation of the electron capture spectrum of 163Ho: Auger-Meitner decay into continuum states
Creators: name: Brass, M.
name: Haverkort, M. W.
Publisher: name: arXiv
Year: 2020
Subjects: subject: Nuclear Theory (nucl-th)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: Determining the electron neutrino mass by electron capture in $^{163}$Ho relies on an accurate understanding of the differential electron capture nuclear decay rate as a function of the distribution of the total decay energy between the neutrino and electronic excitations. The resulting spectrum is dominated by resonances due to local atomic multiplet states with core holes. Coulomb scattering between electrons couple the discrete atomic states, via Auger-Meitner decay, to final states with free electrons. The atomic multiplets are above the auto-ionisation energy, such that the delta functions representing these discrete levels turn into a superposition of Lorentzian, Mahan- and Fano-like line-shapes. We present an \textit{ab initio} method to calculate nuclear decay modifications due to such processes. It includes states with multiple correlated holes in local atomic orbitals interacting with unbound Auger-Meitner electrons. A strong energy-dependent, asymmetric broadening of the resonances in good agreement with recent experiments is found. We present a detailed analysis of the mechanisms determining the final spectral line-shape and discuss both the Fano interference between different resonances, as well as the energy dependence of the Auger-Meitner Coulomb matrix elements. The latter mechanism is shown to be the dominant channel responsible for the asymmetric line-shape of the resonances in the electron capture spectrum of $^{163}$Ho.
CARMA observations of protostellar outflows in NGC 1333
Creators: name: Plunkett, Adele L.
name: Arce, Hector G.
name: Corder, Stuartt A.
name: Mardones, Diego
name: Sargent, Anneila I.
name: Schnee, Scott L.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We present observations of outflows in the star-forming region NGC 1333 using the Combined Array for Research in Millimeter-Wave Astronomy (CARMA). We combined the 12CO and 13CO (1-0) CARMA mosaics with data from the 14-m Five College Radio Astronomy Observatory (FCRAO) to probe the central, most dense and active region of this protostellar cluster at scales from 5'' to 7' (or 1000 AU to 0.5 pc at a distance of 235 pc). We map and identify 12CO outflows, and along with 13CO data we estimate their mass, momentum and energy. Within the 7'x7' map, the 5'' resolution allows for a detailed study of morphology and kinematics of outflows and outflow candidates, some of which were previously confused with other outflow emission in the region. In total, we identify 22 outflow lobes, as well as 9 dense circumstellar envelopes marked by continuum emission, of which 6 drive outflows. We calculate a total outflow mass, momentum and energy within the mapped region of 6 Msun, 19 Msun km/s, and 7x10^44 erg, respectively. Within this same region, we compare outflow kinematics with turbulence and gravitational energy, and we suggest that outflows are likely important agents for the maintenance of turbulence in this region. In the earliest stages of star formation, outflows do not yet contribute enough energy to totally disrupt the clustered region where most star formation is happening, but have the potential to do so as the protostellar sources evolve. Our results can be used to constrain outflow properties, such as outflow strength, in numerical simulations of outflow-driven turbulence in clusters.
description: 24 pages, 9 figures, 5 tables, accepted for publication in ApJ
Gene-Wise Association of Variants in Four Lysosomal Storage Disorder Genes in Neuropathologically Confirmed Lewy Body Disease
Creators: name: Clark, Lorraine N.
name: Chan, Robin Barry
name: Cheng, Rong
name: Liu, Xinmin
name: Park, Naeun
name: Parmalee, Nancy
name: Kisselev, Sergey
name: Cortes, Etty Paola
name: Torres, Paola A.
name: Pastores, Gregory M.
name: Vonsattel, Jean Paul
name: Alcalay, Roy Nissim
name: Marder, Karen
name: Honig, Lawrence S.
name: Fahn, Stanley
name: Mayeux, Richard Paul
name: Shelanski, Michael L.
name: Di Paolo, Gilbert
name: Lee, Joseph H.
Publisher: name: Columbia University
Year: 2015
Subjects: subject: Nervous system--Diseases
subject: Bioinformatics
subject: FOS: Computer and information sciences
subject: Lysosomal storage diseases
subject: Neurology
subject: Pathology
subject: Biochemistry

description: Objective
Variants in GBA are associated with Lewy Body (LB) pathology. We investigated whether variants in other lysosomal storage disorder (LSD) genes also contribute to disease pathogenesis.

Methods
We performed a genetic analysis of four LSD genes including GBA, HEXA, SMPD1, and MCOLN1 in 231 brain autopsies. Brain autopsies included neuropathologically defined LBD without Alzheimer Disease (AD) changes (n = 59), AD without significant LB pathology (n = 71), Alzheimer disease and lewy body variant (ADLBV) (n = 68), and control brains without LB or AD neuropathology (n = 33). Sequencing of HEXA, SMPD1, MCOLN1 and GBA followed by ‘gene wise’ genetic association analysis was performed. To determine the functional effect, a biochemical analysis of GBA in a subset of brains was also performed. GCase activity was measured in a subset of brain samples (n = 64) that included LBD brains, with or without GBA mutations, and control brains. A lipidomic analysis was also performed in brain autopsies (n = 67) which included LBD (n = 34), ADLBV (n = 3), AD (n = 4), PD (n = 9) and control brains (n = 17), comparing GBA mutation carriers to non-carriers.

Results
In a ‘gene-wise’ analysis, variants in GBA, SMPD1 and MCOLN1 were significantly associated with LB pathology (p range: 0.03–4.14 x10-5). Overall, the mean levels of GCase activity were significantly lower in GBA mutation carriers compared to non-carriers (p<0.001). A significant increase and accumulation of several species for the lipid classes, ceramides and sphingolipids, was observed in LBD brains carrying GBA mutations compared to controls (p range: p<0.05-p<0.01).

Interpretation
Our study indicates that variants in GBA, SMPD1 and MCOLN1 are associated with LB pathology. Biochemical data comparing GBA mutation carrier to non-carriers support these findings, which have important implications for biomarker development and therapeutic strategies.
Additional file 4 of AI-assisted evidence screening method for systematic reviews in environmental research: integrating ChatGPT with domain knowledge
Creators: name: Zuo, Chen
name: Yang, Xiaohao
name: Errickson, Josh
name: Li, Jiayang
name: Hong, Yi
name: Wang, Runzi
Publisher: name: figshare
Year: 2025
Subjects: subject: Artificial Intelligence and Image Processing
subject: FOS: Computer and information sciences

description: Supplementary Material 4
Additional file 1 of Evaluation of baseline pediatric readiness of emergency departments in Manitoba, Canada
Creators: name: Aregbesola, Alex
name: Florescu, Oana
name: Tam, Clara
name: Coyle, Amanda
name: Knisley, Lisa
name: Hogue, Kaitlin
name: Beer, Darcy
name: Sawyer, Scott
name: Klassen, Terry P.
Publisher: name: figshare
Year: 2022
Subjects: subject: Medicine
subject: Biotechnology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy
subject: 111714 Mental Health
subject: FOS: Health sciences
subject: 110309 Infectious Diseases

description: Additional file 1: Supplementary material 1. Pediatric Readiness Initiative for Emergency Departments Survey.
title: Vorschläge zu einem allgemeinen deutschen Münz-, Maaß- und Gewicht-System; 1848
title: (Den Mitgliedern der Nationalversammlung zu Frankfurt übersandt)
titleType: Subtitle
Creators: name: Nördling, Wilhelm von
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2018

description: Kopftitel
The Fate of the Interstellar Medium in Early-type Galaxies. II. Observational Evidence for Morphological Quenching
Creators: name: Leśniewska, Aleksandra
name: Michałowski, Michał Jerzy
name: Gall, Christa
name: Hjorth, Jens
name: Nadolny, Jakub
name: Ryzhov, Oleh
name: Solar, Martin
Publisher: name: arXiv
Year: 2023
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The mechanism by which galaxies stop forming stars and get rid of their interstellar medium (ISM) remains elusive. Here, we study a sample of more than two thousand elliptical galaxies in which dust emission has been detected. This is the largest sample of such galaxies ever analysed. We infer the timescale for removal of dust in these galaxies and investigate its dependency on physical and environmental properties. We obtain a dust removal timescale in elliptical galaxies of $τ$ = 2.26 $\pm$ 0.18 Gyr, corresponding to a half-life time of 1.57 $\pm$ 0.12 Gyr. This timescale does not depend on environment, stellar mass or redshift. We observe a departure of dusty elliptical galaxies from the star formation rate vs. dust mass relation. This is caused by the star-formation rates declining faster than the dust masses and indicates that there exists an internal mechanism, which affects star formation, but leaves the ISM intact. Morphological quenching together with ionisation or outflows caused by older stellar populations (supernova type Ia or planetary nebulae) are consistent with these observations.
description: 10 pages, 3 figures, 2 tables, accepted for publication in ApJ
Measuring the Angular Momentum Distribution in Core-Collapse Supernova Progenitors with Gravitational Waves
Creators: name: Abdikamalov, Ernazar
name: Gossan, Sarah
name: DeMaio, Alexandra M.
name: Ott, Christian D.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: The late collapse, core bounce, and the early postbounce phase of rotating core collapse leads to a characteristic gravitational wave (GW) signal. The precise shape of the signal is governed by the interplay of gravity, rotation, nuclear equation of state (EOS), and electron capture during collapse. We explore the dependence of the signal on total angular momentum and its distribution in the progenitor core by means of a large set of axisymmetric general-relativistic core collapse simulations in which we vary the initial angular momentum distribution in the core. Our simulations include a microphysical finite-temperature EOS, an approximate electron capture treatment during collapse, and a neutrino leakage scheme for the postbounce evolution. We find that the precise distribution of angular momentum is relevant only for very rapidly rotating cores with T/|W|>~8% at bounce. We construct a numerical template bank from our baseline set of simulations, and carry out additional simulations to generate trial waveforms for injection into simulated advanced LIGO noise at a fiducial galactic distance of 10 kpc. Using matched filtering, we show that for an optimally-oriented source and Gaussian noise, advanced Advanced LIGO could measure the total angular momentum to within ~20%, for rapidly rotating cores. For most waveforms, the nearest known degree of precollapse differential rotation is correctly inferred by both our matched filtering analysis and an alternative Bayesian model selection approach. We test our results for robustness against systematic uncertainties by injecting waveforms from simulations using a different EOS and and variations in the electron fraction in the inner core. The results of these tests show that these uncertainties significantly reduce the accuracy with which the total angular momentum and its precollapse distribution can be inferred from observations.
description: 22 pages, 16 figures
title: Bericht der für den 9. Punkt des Programmes des Congresses deutscher Landwirthe niedergesetzten Commission; [1848]
title: erstattet von dem Hrn. Weinlig, Geh. Reg.-Rath aus Dresden, in der 6. Sitzung am 10. Nov. 1848
titleType: Subtitle
Creators: name: Weinlig, Christian Albert
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2018

description: Kopftitel
2021 occultations and transits of Linus orbiting (22) Kalliope: I. Polygonal and `cliptracing' algorithm
Creators: name: Brož, M.
name: Ďurech, J.
name: Ferrais, M.
name: Lee, H. -J.
name: Kim, M. -J.
name: Roh, D. -G.
name: Yim, H. -S.
name: Jehin, E.
name: Burdanov, A.
name: de Wit, J.
name: Fatka, P.
name: Hanuš, J.
name: Carry, B.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: The satellite Linus orbiting the main-belt asteroid (22) Kalliope exhibited occultation and transit events in late 2021. A photometric campaign was organized and observations were taken by the TRAPPIST-South, SPECULOOS-Artemis, OWL-Net, and BOAO telescopes, with the goal to constrain models of this system. Our dynamical model is complex, with multipoles (up to the order $\ell = 2$), internal tides, and external tides. The model was constrained by astrometry (spanning 2001--2021), occultations, adaptive-optics imaging, calibrated photometry, as well as relative photometry. Our photometric model was substantially improved. A new precise (${<}\,0.1\,{\rm mmag}$) light curve algorithm was implemented, based on polygon intersections, which are computed exactly -- by including partial eclipses and partial visibility of polygons. Moreover, we implemented a `cliptracing' algorithm, based again on polygon intersections, in which partial contributions to individual pixels are computed exactly. Both synthetic light curves and synthetic images are then very smooth. Based on our combined solution, we confirmed the size of Linus, $(28\pm 1)\,{\rm km}$. However, this solution exhibits some tension between the light curves and the PISCO speckle-interferometry dataset. In most solutions, Linus is darker than Kalliope, with the albedos $A_{\rm w} = 0.40$ vs. $0.44$. This is confirmed on deconvolved images. A~detailed revision of astrometric data allowed us to revise also the $J_2 \equiv -C_{20}$ value of Kalliope. Most importantly, a~homogeneous body is excluded. For a differentiated body, two solutions exist: low-oblateness ($C_{20} \simeq -0.12$), with a~spherical iron core, and alternatively, high-oblateness ($C_{20} \simeq -0.22$) with an elongated iron core. These correspond to the low- and high-energy collisions, respectively, studied by means of SPH simulations in our previous work.
description: Astronomy and Astrophysics, accepted
Garber, Marjorie: Die Vielfalt des Begehrens
Creators: name: Böse, Berta
Publisher: name: Werkstatt Schwule Theologie
Year: 1970

description: Werkstatt Schwule Theologie, Bd. 9 Nr. 3 (2002): Werkstatt Schwule Theologie, Band 9, Heft 3
Resolving The Moth at Millimeter Wavelengths
Creators: name: Ricarte, Angelo
name: Moldvai, Noel
name: Hughes, A. Meredith
name: Duchêne, Gaspard
name: Williams, Jonathan P.
name: Andrews, Sean M.
name: Wilner, David J.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: HD 61005, also known as "The Moth," is one of only a handful of debris disks that exhibit swept-back "wings" thought to be caused by interaction with the ambient interstellar medium (ISM). We present 1.3 mm Submillimeter Array (SMA) observations of the debris disk around HD 61005 at a spatial resolution of 1.9 arcsec that resolve the emission from large grains for the first time. The disk exhibits a double-peaked morphology at millimeter wavelengths, consistent with an optically thin ring viewed close to edge-on. To investigate the disk structure and the properties of the dust grains we simultaneously model the spatially resolved 1.3 mm visibilities and the unresolved spectral energy distribution. The temperatures indicated by the SED are consistent with expected temperatures for grains close to the blowout size located at radii commensurate with the millimeter and scattered light data. We also perform a visibility-domain analysis of the spatial distribution of millimeter-wavelength flux, incorporating constraints on the disk geometry from scattered light imaging, and find suggestive evidence of wavelength-dependent structure. The millimeter-wavelength emission apparently originates predominantly from the thin ring component rather than tracing the "wings" observed in scattered light. The implied segregation of large dust grains in the ring is consistent with an ISM-driven origin for the scattered light wings.
description: 10 pages, 6 figures
Predicting genes for orphan metabolic activities using phylogenetic profiles
Creators: name: Chen, Lifeng
name: Vitkup, Dennis
Publisher: name: Columbia University
Year: 2006
Subjects: subject: Biological systems--Mathematical models
subject: Phylogeny
subject: Metabolism--Regulation
subject: Bioinformatics
subject: FOS: Computer and information sciences
subject: Genetics
subject: FOS: Biological sciences
subject: Microbiology

description: Homology-based methods fail to assign genes to many metabolic activities present in sequenced organisms. To suggest genes for these orphan activities we developed a novel method that efficiently combines local structure of a metabolic network with phylogenetic profiles. We validated our method using known metabolic genes in Saccharomyces cerevisiae and Escherichia coli. We show that our method should be easily transferable to other organisms, and that it is robust to errors in incomplete metabolic networks.
Effects of quantum fluctuations on macroscopic quantum tunneling and self-trapping of BEC in a double well trap
Creators: name: Abdullaev, Fatkhulla Kh.
name: Galimzyanov, Ravil M.
name: Shermakhmatov, Akbar M.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Quantum Gases (cond-mat.quant-gas)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We study the influence of quantum fluctuations on the macroscopic quantum tunneling and self-trapping of a two-component Bose-Einstein condensate in a double-well trap. Quantum fluctuations are described by the Lee-Huang-Yang term in the modified Gross-Pitaevskii equation. Employing the modified Gross-Pitaevskii equation in scalar approximation, we derive the dimer model using a two-mode approximation. The frequencies of Josephson oscillations and self-trapping conditions under quantum fluctuations are found analytically and proven by numerical simulations of the modified Gross-Pitaevskii equation. The tunneling and localization phenomena are investigated also for the case of the Lee-Huang-Yang fluid loaded in the double-well potential.
description: 14 pages, 9 figures
Additional file 1 of Heat shock protein A4 ablation leads to skeletal muscle myopathy associated with dysregulated autophagy and induced apoptosis
Creators: name: Elkenani, Manar
name: Barakat, Amal Z.
name: Held, Torsten
name: Rodrigues, Daniel Marques
name: Mobarak, Sherok
name: Swarnka, Surabhi
name: Adham, Ibrahim M.
name: Mohamed, Belal A.
Publisher: name: figshare
Year: 2022
Subjects: subject: Biophysics
subject: Biochemistry
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Physiology
subject: 20199 Astronomical and Space Sciences not elsewhere classified
subject: FOS: Physical sciences
subject: Developmental Biology
subject: Computational Biology

description: Additional file 1: Fig. S1 HSPA4 protein is ubiquitously expressed in different types of skeletal muscles. Fig. S2 Maintained glucose and lipid metabolism in Hspa4-KO mice Fig. S3. Increased centrally nucleated myofibers in Hspa4-KO soleus muscle. Fig. S4 Myopathy in the paraspinal muscle in 18-month-old Hspa4-KO mice. Table S1. List of mouse primers used in this study.
Tunable magnon topology in monolayer CrI$_\mathbf{3}$ under external stimuli
Creators: name: Soenen, M.
name: Milosevic, M. V.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: Two-dimensional (2D) honeycomb ferromagnets, such as monolayer chromium-trihalides, are predicted to behave as topological magnon insulators - characterized by an insulating bulk and topologically protected edge states, giving rise to a thermal magnon Hall effect. Here we report the behavior of the topological magnons in monolayer CrI$_3$ under external stimuli, including biaxial and uniaxial strain, electric gating, as well as in-plane and out-of-plane magnetic field, revealing that one can thereby tailor the magnetic states as well as the size and the topology of the magnonic bandgap. These findings broaden the perspective of using 2D magnetic materials to design topological magnonic devices.
Hempelmann, Heinzpeter: Liebt Gott Schwule und Lesben?
Creators: name: Maurer, Frank
Publisher: name: Werkstatt Schwule Theologie
Year: 1970

description: Werkstatt Schwule Theologie, Bd. 9 Nr. 3 (2002): Werkstatt Schwule Theologie, Band 9, Heft 3
Curl-free positive definite form of time-harmonic Maxwells equations well-suitable for iterative numerical solving
Creators: name: Moiseenko, Vladimir E.
name: Agren, Olov
Publisher: name: arXiv
Year: 2020
Subjects: subject: Computational Physics (physics.comp-ph)
subject: FOS: Physical sciences
subject: J.2
subject: 78A25

description: A new form of time-harmonic Maxwells equations is developed and proposed for numerical modeling. It is written for the magnetic field strength, electric displacement, vector potential and the scalar potential. There are several attractive features of this form. The first one is that the differential operator acting on these quantities is positive. The second is absence of curl operators among the leading order differential operators. The Laplacian stands for the leading order operator in the equations for the magnetic field strength, vector potential and the scalar potential, while the gradient of divergence stands for the electric displacement. The third feature is absence of space varied coefficients in the leading order differential operators that provides diagonal domination of the resulting matrix of the discretized equations. A simple example is given to demonstrate the applicability of this new form of time-harmonic Maxwells equations.
description: Invited talk for 47th Annual EPS Plasma Conference
Magnetically tunable exciton valley coherence in monolayer WS$_2$ mediated by the electron-hole exchange and exciton-phonon interactions
Creators: name: Lan, Kang
name: Xie, Shijie
name: Fu, Jiyong
name: Qu, Fanyao
Publisher: name: arXiv
Year: 2023
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: We develop a model, which incorporates both intra- and intervalley scatterings to master equation, to explore exciton valley coherence in monolayer WS$_2$ subjected to magnetic field. For linearly polarized (LP) excitation accompanied with an initial coherence, our determined valley dynamics manifests the coherence decay being faster than the exciton population relaxation, and agrees with experimental data by Hao et al.[Nat. Phys. 12, 677 (2016)]. Further, we reveal that magnetic field may quench the electron-hole (e-h) exchange induced pure dephasing -- a crucial decoherence source -- as a result of lifting of valley degeneracy, allowing to magnetically regulate valley coherence. In particular, at low temperatures for which the exciton-phonon (ex-ph) interaction is weak, we find that the coherence time is expected to attain $τ_{\mathcal{C}}\sim 1$ ps, facilitating full control of qubits based on the valley pseudospin. For dark excitons, we demonstrate an emerging coherence even in the absence of initial coherent state, which has a long coherence time ($\sim 15$ ps) at low temperature. Our work provides an insight into tunable valley coherence and coherent valley control based on dark excitons.
description: 7 pages, 4 figures
Streiflichter auf die materiellen Zustände und Bestrebungen in Deutschland; [ca. 1848]
Creators: name: Glaser, Johann Karl
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2018

description: Enth.: Grundsätze für den künftigen Zolltarif Deutschlands (Fortsetzung). Eisenproduktion des preußischen Staates. Eiseneinfuhr in den deutschen Zollverein. Eine Aufgabe. Beschlüsse der Nationalversammlung
Additional file 5 of AI-assisted evidence screening method for systematic reviews in environmental research: integrating ChatGPT with domain knowledge
Creators: name: Zuo, Chen
name: Yang, Xiaohao
name: Errickson, Josh
name: Li, Jiayang
name: Hong, Yi
name: Wang, Runzi
Publisher: name: figshare
Year: 2025
Subjects: subject: Artificial Intelligence and Image Processing
subject: FOS: Computer and information sciences

description: Supplementary Material 5
Additional file 1 of Mechanical properties and moisture-related dimensional change of canvas paintings–canvas and glue sizing
Creators: name: Janas, Arkadiusz
name: Fuster-López, Laura
name: Andersen, Cecil Krarup
name: Escuder, Angel Vicente
name: Kozłowski, Roman
name: Poznańska, Katarzyna
name: Gajda, Aleksandra
name: Scharff, Mikkel
name: Bratasz, Łukasz
Publisher: name: figshare
Year: 2022
Subjects: subject: Biophysics
subject: 29999 Physical Sciences not elsewhere classified
subject: FOS: Physical sciences
subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Biotechnology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: Developmental Biology

description: Additional file 1. Nominal elasticity moduli of the materials investigated (in MPa).