cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Systematic study of $\boldsymbol{\mathcalα}$ decay of nuclei around $\boldsymbol{Z=82}$, $\boldsymbol{N=126}$ shell closure within the cluster-formation model and proximity potential 1977 formalism
Creators: name: Deng, Jun-Gang
name: Zhao, Jie-Cheng
name: Chu, Peng-Cheng
name: Li, Xiao-Hua
Publisher: name: arXiv
Year: 2018
Subjects: subject: Nuclear Theory (nucl-th)
subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: In the present work, we systematically study the $\mathcalα$ decay preformation factors $P_α$ within the cluster-formation model and $\mathcalα$ decay half-lives by the proximity potential 1977 formalism for nuclei around $Z=82$, $N=126$ closed shells. The calculations show that the realistic $P_α$ is linearly dependent on the product of valance protons (holes) and valance neutrons (holes) $N_pN_n$. It is consistent with our previous works [X.-D. Sun \textit{et al.}, \href{https://journals.aps.org/prc/abstract/10.1103/PhysRevC.94.024338}{ Phys. Rev. C 94, 024338 (2016)}, J.-G. Deng \textit{et al.}, \href{https://journals.aps.org/prc/abstract/10.1103/PhysRevC.96.024318}{Phys. Rev. C 96, 024318 (2017)}], which $P_α$ are model-dependent and extracted from the ratios of calculated $\mathcalα$ half-lives to experimental data. Combining with our previous works, we confirm that the valance proton-neutron interaction plays a key role in the $\mathcalα$ preformation for nuclei around $Z=82$, $N=126$ shell closures whether the $P_α$ is model-dependent or microcosmic. In addition, our calculated $\mathcalα$ decay half-lives by using the proximity potential 1977 formalism taking $P_α$ evaluated by the cluster-formation model can well reproduce the experimental data and significantly reduce the errors.
description: 4 figures, 7 tables; Accepted by Physical Review C
Additional file 1 of Telerehabilitation program for older adults on a waiting list for physical therapy after hospital discharge: study protocol for a pragmatic randomized trial protocol
Creators: name: Borges, Pollyana Ruggio Tristão
name: Resende, Renan Alves
name: Dias, Jane Fonseca
name: Mancini, Marisa Cotta
name: Sampaio, Rosana Ferreira
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: Immunology
subject: FOS: Clinical medicine
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: 60506 Virology
subject: FOS: Biological sciences

description: Additional file 1. SPIRIT Checklist.
Modelling variability of solar activity cycles
Creators: name: Kitchatinov, L. L.
name: Mordvinov, A. V.
name: Nepomnyashchikh, A. A.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Context. Solar activity cycles vary in amplitude and duration. The variations can be at least partly explained by fluctuations in dynamo parameters. Aims. We want to restrict uncertainty in fluctuating dynamo parameters and find out which properties of the fluctuations control the amplitudes of the magnetic field and energy in variable dynamo cycles. Methods. A flux-transport model for the solar dynamo with fluctuations of the Babcock-Leighton type $α$-effect was applied to generate statistics of magnetic cycles for our purposes. The statistics were compared with data on solar cycle periods to restrict the correlation time of dynamo fluctuations. Results. A characteristic time of fluctuations in the $α$-effect is estimated to be close to the solar rotation period. The fluctuations produce asymmetry between the times of rise and descent of dynamo cycles, the rise time being on average shorter. The affect of the fluctuations on cycle amplitudes depends on the phase of the cycle in which the fluctuations occur. Negative fluctuations (decrease in $α$) in the rise phase delay decay of poloidal field and increase the cycle amplitude in toroidal field and magnetic energy. Negative fluctuation in the decline phase reduces the polar field at the end of a cycle and the amplitude of the next cycle. The low amplitude of the 24th solar cycle compared to the preceding 23rd cycle can be explained by this effect. Positive fluctuations in the descent phase enhance the magnetic energy of the next cycle by increasing the seed poloidal field for the next cycle. The statistics of the computed energies of the cycles suggest that superflares of $\ge 10^{34}$ erg are not possible on the Sun.
description: 8 pages, 11 figures, A&A (accepted)
Biased discrete symmetry and domain wall problem
Creators: name: Dvali, G.
name: Tavartkiladze, Z.
name: Nanobashvili, J.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We reconsider a cosmological evolution of domain walls produced by spontaneous breaking of an approxime discrete symmetry. We show, that domain walls may never collapse even if the standard bound on the vacuum energy asymmetry is satisfied. Instead of disappearing, these defects may form stable ``bound states'' - double wall systems. Possible stability of such a wall is a dynamical question and consequently restricts the allowed range of parameters. In particular, in the two Higgs doublet standard model with an anomalous Z(2) symmetry, the above restriction suggests the mass of the pseudoscalar Higgs (would be axion) being close to the mass of the scalar one.
description: 15 pages, latex, no figures
Non-circular Gas Kinematics and Star Formation in the Ringed Galaxy NGC 4736
Creators: name: Wong, Tony
name: Blitz, Leo
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We analyze the gas kinematics and star formation properties of the nearby RSab galaxy NGC 4736 using interferometric and single-dish CO(1-0) data and previously published Halpha and HI data. The CO morphology is dominated by a central molecular bar and tightly wound spiral arms associated with a bright ring of star formation. Strong HI emission is also found in the ring, but HI is absent from the central regions. Comparison of the HI and Halpha distributions suggests that HI in the ring is primarily dissociated H$_2$. Modeling of the CO kinematics reveals gas motion in elliptical orbits around the central bar, and we argue that the ring represents both the OLR of the bar and the ILR of a larger oval distortion. The HI kinematics show evidence for axisymmetric inflow towards the ring and are inconsistent with streaming in aligned elliptical orbits, but the highly supersonic (~40 km/s) inflow velocities required, corresponding to mass inflow rates of ~2 Msol/yr, suggest that more sophisticated models (e.g., gas orbiting in precessed elliptical orbits) should be considered. The radial CO and Halpha profiles are poorly correlated in the vicinity of the nuclear bar, but show a better correlation (in rough agreement with the Schmidt law) at the ring. Even along the ring, however, the azimuthal correspondence between CO and Halpha is poor, suggesting that massive stars form more efficiently at some (perhaps resonant) locations than at others. These results indicate that the star formation rate per unit gas mass exhibits strong spatial variations and is not solely a function of the available gas supply. The localization of star formation to the ring is broadly consistent with gravitational instability theory, although the instability parameter $Q \sim 3$ on average in the ring, only falling below 1 in localized regions.
description: Revised version accepted by ApJ, with new section on p-v diagrams. 24 pages with 24 figures (emulateapj5). Full resolution and color versions are available at http://astro.berkeley.edu/~twong/preprints
Entry Barrier Analysis in Signal-Jamming Predatory Pricing
Creators: name: Asmit Raj Pandey
Publisher: name: figshare
Year: 2018
Subjects: subject: 140206 Experimental Economics
subject: FOS: Economics and business

description: The main aim of this thesis paper is to establish a significant relation between Signal-Jamming predatory pricing and its entry barrier ability. An experiment was conducted with 26 participants. The experiment was conducted considering the parameters of signal-jamming predatory pricing. The result of the experiment gave an exit ratio of entry barrier ability. With this data, a binomial test was conducted to test the significance of the research. The result showed that there is a statistical significance between signal-jamming predatory pricing and entry barrier.This thesis paper also shows in detail the reasons and rationality behind predatory pricing, its result and probable impact on the market.
Classifying magnetic resonance image modalities with convolutional neural networks
Creators: name: Remedios, Samuel
name: Pham, Dzung L.
name: Butman, John A.
name: Roy, Snehashis
Publisher: name: arXiv
Year: 2018
Subjects: subject: Computer Vision and Pattern Recognition (cs.CV)
subject: FOS: Computer and information sciences

description: Magnetic Resonance (MR) imaging allows the acquisition of images with different contrast properties depending on the acquisition protocol and the magnetic properties of tissues. Many MR brain image processing techniques, such as tissue segmentation, require multiple MR contrasts as inputs, and each contrast is treated differently. Thus it is advantageous to automate the identification of image contrasts for various purposes, such as facilitating image processing pipelines, and managing and maintaining large databases via content-based image retrieval (CBIR). Most automated CBIR techniques focus on a two-step process: extracting features from data and classifying the image based on these features. We present a novel 3D deep convolutional neural network (CNN)-based method for MR image contrast classification. The proposed CNN automatically identifies the MR contrast of an input brain image volume. Specifically, we explored three classification problems: (1) identify T1-weighted (T1-w), T2-weighted (T2-w), and fluid-attenuated inversion recovery (FLAIR) contrasts, (2) identify pre vs post-contrast T1, (3) identify pre vs post-contrast FLAIR. A total of 3418 image volumes acquired from multiple sites and multiple scanners were used. To evaluate each task, the proposed model was trained on 2137 images and tested on the remaining 1281 images. Results showed that image volumes were correctly classified with 97.57% accuracy.
description: Github: https://github.com/sremedios/phinet
Near-infrared to visible upconversion imaging using a broadband pump laser
Creators: name: Demur, Romain
name: Garioud, Renaud
name: Grisard, Arnaud
name: Lallier, Eric
name: Leviandier, Luc
name: Morvan, LoÏc
name: Treps, Nicolas
name: Fabre, Claude
Publisher: name: arXiv
Year: 2018
Subjects: subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: We present an upconversion imaging experiment from the near-infrared to the visible spectrum. Using a dedicated broadband pump laser to increase the number of resolved elements converted in the image we obtain up to 56x64 spatial elements with a 2.7 nm wide pump spectrum, more than 10 times the number of elements accessible with a narrowband laser. Results in terms of field of view, resolution and conversion efficiency are in good agreement with simulations. The computed sensitivity of our experiment favorably compares with direct InGaAs camera detection.
Constraints on the electroweak universal parameters and the top and Higgs masses from updated LEP/SLC data
Creators: name: Matsumoto, Seiji
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: A global analysis is performed using the latest data from LEP and SLC. Constraints on the electroweak universal parameters ($S,T,U$) and on the masses of the top quark and Higgs boson within the Standard Model (SM) are investigated. The uncertainties due to the QCD and QED effective couplings, $α_s(\mz)$ and $\barα(\mmz)$, are examined in detail. Even though the mean value of $S$ is increased to be consistent with zero, the naive Technicolor models are still disfavored due to its reduced error. Within the SM, we find the 90\,\%CL constraints; $133\gev
description: 19 pages, uuencoded compressed tar file of LaTeX file and 7 EPS files (uses cite.sty and psfig.sty), PostScript version of complete paper available at ftp://ftp.kek.jp/kek/preprints/TH/TH-418/kekth418.ps.gz
Measurements of the NMR Knight shift tensor and nonlinear magnetization in URu$_2$Si$_2$
Creators: name: Lawson, M.
name: Bush, B. T.
name: Kissikov, T.
name: Brubaker, Z.
name: Shirer, K. R.
name: Jeffries, J. R.
name: Ran, S.
name: Jeon, I.
name: Maple, M. B.
name: Curro, N. J.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: URu$_2$Si$_2$ exhibits an anomalous peak in the nonlinear magnetic susceptibility at the hidden order transition. In order to investigate this anomaly, we conducted direct magnetization measurements and investigated the detailed angular dependence of the $^{29}$Si nuclear magnetic resonance Knight shift tensor. We find that the nonlinear magnetization is smaller than previously reported, and the analogous nonlinear Knight shift tensor is below the detection limit. Our results suggest that the magnitude of the anomalous peak is sample dependent.
description: 5 pages, 6 figures, to appear in Phys. Rev. B
Additional file 1 of Do perceived social neighborhood factors explain the association between neighborhood age composition and mental health among Dutch older adults?
Creators: name: Verspoor, Eline
name: Beenackers, Mariëlle A.
name: Oude Groeniger, Joost
name: van Lenthe, Frank J.
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Physiology
subject: FOS: Biological sciences
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Sociology
subject: FOS: Sociology
subject: Developmental Biology
subject: Science Policy
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Additional file 1: Table S1. Rotated factor loadings of individual perceptions of neighborhood social factors (N = 1092). Table S2. Linear regression analysis of the individual perceptions of social neighborhood factors with mental health in older adults (N = 1255). Table S3. Mediation analysis between the neighborhood age composition and mental health in older adults of individual perceptions of neighborhood social factors (N = 1255). Table S4. Sensitivity analysis: Mediation analysis between the neighborhood age composition and mental health in older adults of individual perceptions of neighborhood social factors without neighborhood income as a confounder (N = 1255).
Orbit Estimation Using a Horizon Detector in the Presence of Uncertain Celestial Body Rotation and Geometry
Creators: name: Shakouri, Amir
name: Azad, Mahdi Hazrati
name: Assadian, Nima
Publisher: name: arXiv
Year: 2018
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: Systems and Control (eess.SY)
subject: FOS: Physical sciences
subject: FOS: Electrical engineering, electronic engineering, information engineering

description: This paper presents an orbit estimation using non-simultaneous horizon detector measurements in the presence of uncertainties in the celestial body rotational velocity and its geometrical characteristics. The celestial body is modelled as a tri-axial ellipsoid with a three-dimensional force field. The non-simultaneous modelling provides the possibility to consider the time gap between horizon measurements. An unscented Kalman filter is used to estimate the spacecraft motion states and estimate the geometric characteristics as well as the rotational velocity of the celestial body. A Monte-Carlo simulation is implemented to verify the results. Simulations showed that using non-simultaneous horizon vector measurements, the spacecraft state errors converge to zero even in the presence of an uncertain geometry and rotational velocity of the celestial body.
description: 17 pages, 7 figures, accepted for publication in Acta Astronautica
Additional file 1 of Impact on 6-month outcomes of hospital trajectory in critically ill older patients: analysis of the ICE-CUB2 clinical trial
Creators: name: Thietart, Sara
name: Boumendil, Ariane
name: Pateron, Dominique
name: Guidet, Bertrand
name: Vallet, Hélène
Publisher: name: figshare
Year: 2022
Subjects: subject: Medicine
subject: Biotechnology
subject: Immunology
subject: FOS: Clinical medicine
subject: Cancer
subject: Science Policy

description: Additional file 1: Table S1. Factors associated with 6-month overall survival according to hospital destination—multivariate analysis. Table S2. Multivariate analysis of factors associated with 6-month mortality or loss of one-point ADL at 6 months according to hospital destination. Table S3. Multivariate analysis of factors associated with 6-month overall survival using multiple imputation for missing values. Table S4. Comparison of 6-month overall survival according to orientation after propensity score matching. Table S5. Comparison of mortality or loss of one-point ADL at 6 months according to orientation after propensity score matching.
Lensing effect on polarization in microwave background: extracting convergence power spectrum
Creators: name: Guzik, Jacek
name: Seljak, Uros
name: Zaldarriaga, Matias
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Matter inhomogeneities along the line of sight deflect the cosmic microwave background (CMB) photons originating at the last scattering surface at redshift $z \sim 1100$. These distortions modify the pattern of CMB polarization. We identify specific combinations of Stokes $Q$ and $U$ parameters that correspond to spin 0,$\pm 2$ variables and can be used to reconstruct the projected matter density. We compute the expected signal to noise as a function of detector sensitivity and angular resolution. With Planck satellite the detection would be at a few $σ$ level. Several times better detector sensitivity would be needed to measure the projected dark matter power spectrum over a wider range of scales, which could provide an independent confirmation of the projected matter power spectrum as measured from other methods.
description: 17 pages, 5 figures, accepted for publication in PRD
Characterizing the velocity of a wandering black hole and properties of the surrounding medium using convolutional neural networks
Creators: name: Gonzalez, J. A.
name: Guzman, F. S.
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We present a method for estimating the velocity of a wandering black hole and the equation of state for the gas around, based on a catalog of numerical simulations. The method uses machine learning methods based on convolutional neural networks applied to the classification of images resulting from numerical simulations. Specifically we focus on the supersonic velocity regime and choose the direction of the black hole to be parallel to its spin. We build a catalog of 900 simulations by numerically solving Euler's equations onto the fixed space-time background of a black hole, for two parameters: the adiabatic index $Γ$ with values in the range [1.1, 5/3], and the asymptotic relative velocity of the black hole with respect to the surroundings $v_{\infty}$, with values within $[0.2, 0.8]c$. For each simulation we produce a 2D image of the gas density once the process of accretion has approached a stationary regime. The results obtained show that the implemented Convolutional Neural Networks are capable to classify correctly the adiabatic index $87.78\%$ of the time within an uncertainty of $\pm 0.0284$ while the prediction of the velocity is correct $96.67\%$ of the times within an uncertainty of $\pm 0.03c$. We expect that this combination of a massive number of numerical simulations and machine learning methods will help analyze more complicated scenarios related to future high resolution observations of black holes, like those from the Event Horizon Telescope.
description: 5 RevTex pages. Published in Physical Review D
Precise Interplanetary Network Localization of the Bursting Pulsar GRO J1744-28
Creators: name: Hurley, K.
name: Kouveliotou, C.
name: Cline, T.
name: Cole, D.
name: Miller, M. C.
name: Harmon, A.
name: Fishman, G.
name: Briggs, M.
name: van Paradijs, J.
name: Kommers, J.
name: Lewin, W.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We analyze 426 observations of the bursting pulsar GRO J1744-28 by Ulysses and BATSE. Triangulating each burst, and statistically combining the triangulation annuli, we obtain a 3 sigma error ellipse whose area is 532 sq. arcsec. The accuracy of this statistical method has been independently verified with observations of the soft gamma repeater SGR1900+14. The ellipse is fully contained within the 1 ' radius ASCA error circle of the soft X-ray counterpart, and partially overlaps the 10 " radius ROSAT error circle of a source which may also be the soft X-ray counterpart. A variable source which has been proposed as a possible IR counterpart lies at the edge of the 3 sigma error ellipse, making it unlikely from a purely statistical point of view to be associated with the bursting pulsar.
description: Submitted to the Astrophysical Journal
Synthesis, characterization, and electrochemical properties of new water-soluble Mn12O12(O2CR)16(H2O)4 clusters
Creators: name: Gluz, Naama
name: Maayan, Galia
Publisher: name: Taylor & Francis
Year: 2018
Subjects: subject: Biophysics
subject: Biochemistry
subject: Medicine
subject: Pharmacology
subject: Biotechnology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Ecology
subject: FOS: Biological sciences

description: We report our attempts to produce water-soluble Mn clusters of the type [Mn12O12(O2CR)16(H2O)4] and the synthesis, spectroscopic, structural, and electrochemical characterization of the three new compounds that were obtained. Clusters 2, 3, and 4 were prepared via substitution of the acetate ligands in [Mn12O12(O2CMe)16(H2O)4] (1) with either 3,4-diaminobenzoic acid, L-proline or L-ascorbic acid, respectively, which are all inexpensive and readily available. Clusters 2, 3, and 4 were characterized by elemental analysis, UV-Vis, and FTIR spectroscopies, XPS, MS, and XRD analysis, suggesting that the clusters retain their structure during the substitution reaction, albeit 4 was obtained partially substituted and reduced. Electrochemical measurements in acetate buffer at pH 6, including continuous cyclic voltammetry scans of the free ligands and of the clusters, imply that 4 is stable to the oxidation process, while in 2 the primary amine ligands are oxidized rapidly, leading to precipitation of the cluster. Overall, the voltammetric measurements support the spectroscopic-based proposed structures.
title: AN, Registre des écrous du Châtelet, Y5266, f. p1000641
Creators: name: Claustre, Julie
name: Nationales, Archives
name: Archives Nationales
name: Claustre, Julie
name: ArchivesNationales/J.CLAUSTRE/H.REGAZZI/2020
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: Laboratoire de Médiévistique Occidentale de Paris
subject: Châtelet
subject: registre
subject: LaMOP

description: Registre des écrous du Châtelet, Archives Nationales, Y5266. Numérisation en mode image.
description: Bibliographic citation: Archives Nationales, Registre des écrous du Châtelet, Y5266, f. p1000641
Coordinated referral and scheduling decisions for specialized healthcare services
Creators: name: Dehkordi, Amin Mahmoudian
name: Pavlin, Michael
Publisher: name: Taylor & Francis
Year: 2024
Subjects: subject: Medicine
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Science Policy
subject: Mental Health

description: This paper studies the coordination of referral and scheduling policies where access to specialized medical services, such as surgical procedures, imaging or other consultations, is managed through a centralized intake system. In this increasingly common mode of operation, a central body makes decisions regarding the allocation of patients between a set of providers, followed by the provider taking control of the scheduling and delivery of the required service. To study the coordination of the allocation and scheduling policies we present a sequential optimization model where both referrer and provider attempt to maximize the proportion of a heterogeneous set of patients receiving treatment within a targeted wait time. Motivated by observations of performance thresholds in queueing systems, we introduce an achievable region model which permits study of providers who vary in ability to coordinate scheduling different patient streams. We characterize optimal referral and scheduling policies for a range of demand patterns and operational abilities. We find that the optimal referral policy can result in large discrepancies in outcomes for different patient types but that the discrepancy in outcomes is muted when operational abilities are higher. In situations where operational abilities are low, it is optimal for the providers to prioritize patients by stream. Low capacity for both providers results in an optimal referral and scheduling policy where certain patients streams are deprioritized and with certainty will not be seen within their wait time targets. We also study the cost of enforcing parity between patient classes and find that the cost is reduced when providers have higher operational abilities. This paper illustrates how operational constraints lead to incentives to prioritize different patient streams. In particular, we show that when operations are challenging, a more hands-on design is required to ensure clinical intake systems maintain equitable access to the service.
Weak Gravitational Lensing
Creators: name: Bartelmann, Matthias
name: Schneider, Peter
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We review theory and applications of weak gravitational lensing. After summarising Friedmann-Lemaitre cosmological models, we present the formalism of gravitational lensing and light propagation in arbitrary space-times. We discuss how weak-lensing effects can be measured. The formalism is then applied to reconstructions of galaxy-cluster mass distributions, gravitational lensing by large-scale matter distributions, QSO-galaxy correlations induced by weak lensing, lensing of galaxies by galaxies, and weak lensing of the cosmic microwave background. Contents: Introduction - Cosmological Background - Gravitational Light Deflection - Principles of Weak Gravitational Lensing - Weak Lensing by Galaxy Clusters - Weak Cosmological Lensing - QSO Magnification Bias and Large-Scale Structure - Galaxy-Galaxy Lensing - The Impact of Weak Gravitational Lensing on the Microwave Background Radiation - Summary and Outlook
description: Review; 223 pages; figures embedded; to be submitted to Physics Reports; constructive comments are invited
Additional file 10: of Population structure, demographic history and local adaptation of the grass carp
Creators: name: Shen, Yubang
name: Wang, Le
name: Fu, Jianjun
name: Xu, Xiaoyan
name: Yue, Gen
name: Li, Jiale
Publisher: name: figshare
Year: 2019
Subjects: subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: Ecology
subject: Biological Sciences not elsewhere classified
subject: Mathematical Sciences not elsewhere classified
subject: Inorganic Chemistry
subject: FOS: Chemical sciences
subject: Science Policy
subject: Computational Biology

description: Table S3. Parameters used for Diyabc modelling and its distribution for historical demographic parameters of the best competing scenario for two datasets. (DOCX 16 kb)
Characteristics of QCD Phase Transitions in an Extended Skyrme Model on $S^3$
Creators: name: Kim, Joon Ha
name: Yee, Sooman
name: Lee, Hyun Kyu
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We study the characteristics of the QCD phase transitions in dense hadronic matter using the Skyrme model constructed on S^3. We find numerically the localized solutions on $S^3$ using the extended Skyrme model which implements correctly the scale symmetry of QCD. The transition from the localized phase to the delocalized phase is found to be of first order at the critical radius of the hypersphere, $L_c$. The chiral restoration and the gluon decondensation also take place at the same critical size.
description: 8 text pages (Latex) and 5 figures included
Black Hole/Pulsar Binaries in the Galaxy
Creators: name: Shao, Yong
name: Li, Xiang-Dong
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We have performed population synthesis calculation on the formation of binaries containing a black hole (BH) and a neutron star (NS) in the Galactic disk. Some of important input parameters, especially for the treatment of common envelope evolution, are updated in the calculation. We have discussed the uncertainties from the star formation rate of the Galaxy and the velocity distribution of NS kicks on the birthrate ($ \sim 0.6-13 \rm\, Myr^{-1}$) of BH/NS binaries. From incident BH/NS binaries, by modelling the orbital evolution duo to gravitational wave radiation and the NS evolution as radio pulsars, we obtain the distributions of the observable parameters such as the orbital period, eccentricity and pulse period of the BH/pulsar binaries. We estimate that there may be $\sim 3-80 $ BH/pulsar binaries in the Galactic disk and around 10\% of them could be detected by the Five-hundred-meter Aperture Spherical radio Telescope.
description: 5 pages, 4 figures, 1 table, accepted for publication in MNRAS Letters
Study of Total Electron Content-TEC and electron density profile during geomagnetic storms
Creators: name: Bhattarai, Niraj
name: Chapagain, Narayan Prasad
name: Adhikari, Binod
Publisher: name: arXiv
Year: 2018
Subjects: subject: Space Physics (physics.space-ph)
subject: Atmospheric and Oceanic Physics (physics.ao-ph)
subject: FOS: Physical sciences

description: Total Electron Content (TEC) and electron density are the basic parameters, which determine the major properties of the Ionosphere. Detail study of the ionospheric TEC and electron density variations has been carried out during geomagnetic storms, with longitude and latitude, for four different locations: (24°W-14°W, 25°S-10°S); (53°W- 46°W, 04°N-14°N); (161°E-165°E, 42°S-34°S), and (135°W- 120°W, 39°S-35°S) using the COSMIC satellite data. In order to find the background conditions of the ionosphere, the solar wind parameters such as north-south component of inter planetary magnetic field (Bz), plasma velocity (Vsw), AE, Dst and Kp indices, have also been correlated with the TEC and electron density. The results illustrates that the observed TEC and electron density profile significantly vary with longitudes and latitudes as well. This study illustrates that the values of TEC and the vertical electron density profile are influenced by the solar wind parameters associated with solar activities. The peak value of electron density and TEC increase as the geomagnetic storms becomes stronger. Similarly, the electron density profile vary with altitudes which peaks around the altitude range of about 180-280 km, depending on the strength of geomagnetic storms. The results clearly show that the peak electron density shifted to higher altitude (from about 180 km to 300 km) as the geomagnetic disturbances becomes stronger.
Synthesis, characterization and electrochemical properties of new water-soluble Mn12O12(O2CR)16(H2O)4 clusters
Creators: name: Gluz, Naama
name: Maayan, Galia
Publisher: name: Taylor & Francis
Year: 2018
Subjects: subject: Biophysics
subject: Biochemistry
subject: Medicine
subject: Pharmacology
subject: Biotechnology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Ecology
subject: FOS: Biological sciences

description: We report our attempts to produce water-soluble Mn clusters of the type [Mn12O12(O2CR)16(H2O)4] and the synthesis, spectroscopic, structural and electrochemical characterization of the three new compounds that were obtained. Clusters 2, 3 and 4 were prepared via substitution of the acetate ligands in [Mn12O12(O2CMe)16(H2O)4] (1) with either 3,4-diaminobenzoic acid, L-proline or L-ascorbic acid, respectively, which are all inexpensive and readily available. Clusters 2, 3 and 4 were characterized by elemental analysis, UV-Vis and FTIR spectroscopies, XPS, MS and XRD analysis, suggesting that the clusters retain their structure during the substitution reaction, albeit 4 was obtained partially substituted and reduced. Electrochemical measurements in acetate buffer at pH 6, including continuous cyclic voltammetry scans of the free ligands and of the clusters, imply that 4 is stable to the oxidation process, while in 2 the primary amine ligands are oxidized rapidly, leading to precipitation of the cluster. Overall, the voltammetric measurements support the spectroscopic-based proposed structures.
ANTIHYPERTENSIVE DRUGS FOR HYPERTENSIVE CRISIS
Creators: name: Tojaliev, Davlatbek
Publisher: name: Zenodo
Year: 2024

description: A hypertensive crisis is a sudden and significant increase in blood pressure to critical levels, which may be accompanied by target organ damage, such as the heart, brain, and kidneys. In such situations, the timely use of antihypertensive agents is vital.
Additional file 1 of Association between milk and yogurt intake and mortality: a community-based cohort study (Yamagata study)
Creators: name: Nakanishi, Akiko
name: Homma, Erika
name: Osaki, Tsukasa
name: Sho, Ri
name: Souri, Masayoshi
name: Sato, Hidenori
name: Watanabe, Masafumi
name: Ishizawa, Kenichi
name: Ueno, Yoshiyuki
name: Kayama, Takamasa
name: Konta, Tsuneo
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Cell Biology
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Cancer
subject: Science Policy
subject: Computational Biology

description: Additional file 1: Supplementary Table 1. Number of cancer-related deaths.
Molecular Cloud Formation in Shock-Compressed Layers
Creators: name: Koyama, Hiroshi
name: Inutsuka, Shu-Ichiro
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We investigate the propagation of a shock wave into a warm neutral medium and cold neutral medium by one-dimensional hydrodynamic calculations with detailed treatment of thermal and chemical processes. Our main result shows that thermal instability inside the shock-compressed layer produces a geometrically thin, dense layer in which a large amount of hydrogen molecules is formed. Linear stability analysis suggests that this thermally-collapsed layer will fragment into small molecular cloudlets. We expect that frequent compression due to supernova explosions, stellar winds, spiral density waves, etc., in the galaxy make the interstellar medium occupied by these small molecular cloudlets.
description: 21 pages, 11 figures. Accepted by ApJ
Flexible Energy Management Protocol for Cooperative EV-to-EV Charging
Creators: name: Zhang, Rongqing
name: Cheng, Xiang
name: Yang, Liuqing
Publisher: name: arXiv
Year: 2018
Subjects: subject: Systems and Control (eess.SY)
subject: FOS: Electrical engineering, electronic engineering, information engineering

description: In this paper, we investigate flexible power transfer among electric vehicles (EVs) from a cooperative perspective in an EV system. First, the concept of cooperative EV-to-EV (V2V) charging is introduced, which enables active cooperation via charging/discharging operations between EVs as energy consumers and EVs as energy providers. Then, based on the cooperative V2V charging concept, a flexible energy management protocol with different V2V matching algorithms is proposed, which can help the EVs achieve more flexible and smarter charging/discharging behaviors. In the proposed energy management protocol, we define the utilities of the EVs based on the cost and profit through cooperative V2V charging and employ the bipartite graph to model the charging/discharging cooperation between EVs as energy consumers and EVs as energy providers. Based on the constructed bipartite graph, a max-weight V2V matching algorithm is proposed in order to optimize the network social welfare. Moreover, taking individual rationality into consideration, we further introduce the stable matching concepts and propose two stable V2V matching algorithms, which can yield the EV-consumer-optimal and EV-provider-optimal stable V2V matchings, respectively. Simulation results verify the efficiency of our proposed cooperative V2V charging based energy management protocol in improving the EV utilities and the network social welfare as well as reducing the energy consumption of the EVs.
description: Accepted by IEEE Transactions on Intelligent Transportation Systems
Temporal 1/f^αFluctuations from Fractal Magnetic Fields in Black Hole Accretion Flow
Creators: name: Kawaguchi, T.
name: Mineshige, S.
name: Machida, M.
name: Matsumoto, R.
name: Shibata, K.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Rapid fluctuation with a frequency dependence of $1/f^α$ (with $α\simeq 1 - 2$) is characteristic of radiation from black-hole objects. Its origin remains poorly understood. We examine the three-dimensional magnetohydrodynamical (MHD) simulation data, finding that a magnetized accretion disk exhibits both $1/f^α$ fluctuation (with $α\simeq 2$) and a fractal magnetic structure (with the fractal dimension of $D \sim 1.9$). The fractal field configuration leads reconnection events with a variety of released energy and of duration, thereby producing $1/f^α$ fluctuations.
description: 5 pages, 4 figures. Accepted for publication in PASJ Letters, vol. 52 No.1 (Feb 2000)
Supplementary document for A strong electroluminescence from SnO2 nanocrystals and Er3+ co-doped silica thin film via introducing Ca2+ - 6575547.pdf
Creators: name: Zhao, Jingjie
name: Zhang, Yangyi
name: Wang, Lixiang
name: Chen, Jiaming
name: Li, Dongke
name: Qu, Enze
name: Xu, Jun
name: chen, kunji
Publisher: name: Optica Publishing Group
Year: 2023
Subjects: Uncategorized

description: Supplement 1
Aplikasi Nomogram Besi Cor Lamelar untuk Menentukan Kadar Karbon dan Silisium
Creators: name: Bandanadjaja, Beny
Publisher: name: figshare
Year: 2018
Subjects: subject: Mechanical Engineering
subject: FOS: Mechanical engineering
subject: 91207 Metals and Alloy Materials
subject: FOS: Materials engineering

description:
 Besi cor bergrafit lamelar atau yang dikenal dengan FC merupakan jenis bahan yang umum di produksi di industri pengecoran di Indonesia. Proses produksi besi cor lamelar relatif mudah, temperatur kerja yang tidak terlalu tinggi + 1300 oC, penggunaan paduan yang umum seperti FeMn, FeSi dan Carburiser cukup mudah ditemui di pasaran Indonesia. Kualitas atau grade dari FC sangat ditentukan oleh komposisi kimia dan juga kecepatan pendinginan. Kecepatan pendinginan dalam hal ini berhubungan dengan ketebalan benda. Untuk suatu kasus peramuan komposisi kimia FC dengan grade 25 pada ketebalan plat 15 akan menghasilkan grade yang berbeda apabila komposisi tersebut di cor ke benda dengan ketebalan yang lebih tipis atau lebih tebal. Metoda praktis untuk perhitungan komposisi kimia dapat dilakukan dengan mempergunakan aplikasi diagram yang disebut NOMOGRAM BESI COR LAMELAR. Dalam makalah ini akan di uraikan metoda peramuan FC dengan NOMOGRAM dan studi kasus untuk hasil pengecoran suatu komposisi FC tertentu dan di cor pada benda dengan ketebalan berbeda. 
АBU АLI IBN SINONING "HAYY IBN YAQZON" ASARIDA RUHIY POKLIK VA ILOHIY ISHQNING TASAVVUFIY TALQINI.
Creators: name: Nurova, Shoxida
Publisher: name: Zenodo
Year: 2025

description: Ushbu maqolida Abu Ali Ibn Sinoning «Hayy ibn Yaqzon (Uyg’oq o’g’li tirik)» — ramziy-majoziy uslubda yozilgan qissasining bosh qahramon — birinchi shaxs  Ibn Sino ekanligini, uning suhbatdoshi, hikoya qiluvchi — Hayy ibn Yaqzon – Uyg’oq o’g’li Tirik – Aql ekanligini ko’ramiz. Ibn Sinoning bu qissasi ko’p jihatdan majoziy, ramziy bitilgan, kishilar fe’li atvorini o’z ichiga qamrab ololgan va hayotiy gaplardan mulohaza yuritadigan adabiy asar ekanligini shu nuqtai nazardan qaraganda qissaning ikki sohada — ham falsafiy, ham adabiy sohada yozilganligi bayon qilingan.
Additional file 9: of Population structure, demographic history and local adaptation of the grass carp
Creators: name: Shen, Yubang
name: Wang, Le
name: Fu, Jianjun
name: Xu, Xiaoyan
name: Yue, Gen
name: Li, Jiale
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: Ecology
subject: Biological Sciences not elsewhere classified
subject: Marine Biology
subject: Inorganic Chemistry
subject: FOS: Chemical sciences
subject: Science Policy

description: Table S2. Pairwise FST values among each pair of locations of grass carp. Genetic differentiation that was non-significant after Bonferroni corrections (Pâ <â 0.001) is denoted in bold. (DOCX 14 kb)
Additional file 1 of The effectiveness of trauma care systems at different stages of development in reducing mortality: a systematic review and meta-analysis
Creators: name: Alharbi, Rayan Jafnan
name: Shrestha, Sumina
name: Lewis, Virginia
name: Miller, Charne
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy

description: Additional file 1: Supplemental file, Appendix 1.
A boundary-integral framework to simulate viscous erosion of a porous medium
Creators: name: Quaife, Bryan D.
name: Moore, M. Nicholas J.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Numerical Analysis (math.NA)
subject: FOS: Mathematics

description: We develop numerical methods to simulate the fluid-mechanical erosion of many bodies in two-dimensional Stokes flow. The broad aim is to simulate the erosion of a porous medium (e.g. groundwater flow) with grain-scale resolution. Our fluid solver is based on a second-kind boundary integral formulation of the Stokes equations that is discretized with a spectrally-accurate Nystrom method and solved with fast-multipole-accelerated GMRES. The fluid solver provides the surface shear stress which is used to advance solid boundaries. We regularize interface evolution via curvature penalization using the $θ$-$L$ formulation, which affords numerically stable treatment of stiff terms and therefore permits large time steps. The overall accuracy of our method is spectral in space and second-order in time. The method is computationally efficient, with the fluid solver requiring $\mathcal{O}(N)$ operations per GMRES iteration, a mesh-independent number of GMRES iterations, and a one-time $\mathcal{O}(N^2)$ computation to compute the shear stress. We benchmark single-body results against analytical predictions for the limiting morphology and vanishing rate. Multibody simulations reveal the spontaneous formation of channels between bodies of close initial proximity. The channelization is associated with a dramatic reduction in the resistance of the porous medium, much more than would be expected from the reduction in grain size alone.
description: 10 figures, 3 tables, 28 pages
Bounds on Scalar Leptoquarks from Z Physics
Creators: name: Mizukoshi, J. K.
name: Eboli, O. J. P.
name: Gonzalez-Garcia, M. C.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We analyse the constraints on scalar leptoquarks coming from radiative corrections to $Z$ physics. We perform a global fitting to the LEP data including the contributions of the most general effective Lagrangian for scalar leptoquarks, which exhibits the $SU(2)_L \times U(1)_Y$ gauge invariance. We show that the bounds on leptoquarks that couple to the top quark are much stronger than the ones obtained from low energy experiments.
description: RevTeX 3.0, 26 pages, 4 postscript figures included as uufile
Aplikasi Nomogram Besi Cor Lamelar untuk Menentukan Kadar Karbon dan Silisium.pdf
Creators: name: Bandanadjaja, Beny
Publisher: name: figshare
Year: 2018
Subjects: subject: Mechanical Engineering
subject: FOS: Mechanical engineering

description: p.p1 {margin: 0.0px 0.0px 0.0px 0.0px; font: 12.0px 'Times New Roman'; min-height: 15.0px} p.p2 {margin: 0.0px 0.0px 0.0px 0.0px; font: 10.0px 'Times New Roman'} span.s1 {font: 12.0px 'Times New Roman'} span.s2 {font: 6.5px 'Times New Roman'} table.t1 {border-collapse: collapse} td.td1 {padding: 0.0px 5.0px 0.0px 5.0px}
 Besi cor bergrafit lamelar atau yang dikenal dengan FC merupakan jenis bahan yang umum di produksi di industri pengecoran di Indonesia. Proses produksi besi cor lamelar relatif mudah, temperatur kerja yang tidak terlalu tinggi + 1300 oC, penggunaan paduan yang umum seperti FeMn, FeSi dan Carburiser cukup mudah ditemui di pasaran Indonesia. Kualitas atau grade dari FC sangat ditentukan oleh komposisi kimia dan juga kecepatan pendinginan. Kecepatan pendinginan dalam hal ini berhubungan dengan ketebalan benda. Untuk suatu kasus peramuan komposisi kimia FC dengan grade 25 pada ketebalan plat 15 akan menghasilkan grade yang berbeda apabila komposisi tersebut di cor ke benda dengan ketebalan yang lebih tipis atau lebih tebal. Metoda praktis untuk perhitungan komposisi kimia dapat dilakukan dengan mempergunakan aplikasi diagram yang disebut NOMOGRAM BESI COR LAMELAR. Dalam makalah ini akan di uraikan metoda peramuan FC dengan NOMOGRAM dan studi kasus untuk hasil pengecoran suatu komposisi FC tertentu dan di cor pada benda dengan ketebalan berbeda. 
Additional file 2 of The effectiveness of trauma care systems at different stages of development in reducing mortality: a systematic review and meta-analysis
Creators: name: Alharbi, Rayan Jafnan
name: Shrestha, Sumina
name: Lewis, Virginia
name: Miller, Charne
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy

description: Additional file 2: Supplemental file, Appendix 2.
Interaction of supernova blast waves with wind-driven shells: formation of "jets", "bullets", "ears", etc
Creators: name: Gvaramadze, V. V.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Most of middle-aged supernova remnants (SNRs) have a distorted and complicated appearance which cannot be explained in the framework of the Sedov-Taylor model. We consider three typical examples of such SNRs (Vela SNR, MSH 15-52, G 309.2-00.6) and show that their structure could be explained as a result of interaction of a supernova (SN) blast wave with the ambient medium preprocessed by the action of the SN progenitor's wind and ionized emission.
description: 4 pages, talk given at the Gamov Memorial International Conference "The Universe of Gamow: Original Ideas in Astrophysics and Cosmology", Odessa, August 16-22, 1999; to appear in Odessa Astronomical Publications, 1999, vol. 12