cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Dynamics and potential origins of decimeter-sized particles around comet 67P/Churyumov-Gerasimenko
Creators: name: Pfeifer, Marius
name: Agarwal, Jessica
name: Marschall, Raphael
name: Grieger, Björn
name: Lemos, Pablo
Publisher: name: arXiv
Year: 2024
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Methods. We algorithmically tracked thousands of individual particles through four OSIRIS/NAC image sequences of 67P's near-nucleus coma. We then traced concentrated particle groups back to the nucleus surface, and estimated their potential source regions, size distributions, and projected dynamical parameters. Finally, we compared the observed activity to dust coma simulations. Results. We traced back 409 decimeter-sized particles to four suspected source regions. The regions strongly overlap and are mostly confined to the Khonsu-Atum-Anubis area. The activity may be linked to rugged terrain, and the erosion of fine dust and the ejection of large boulders may be mutually exclusive. Power-law indices fitted to the particle size--frequency distributions range from $3.4 \pm 0.3$ to $3.8 \pm 0.4$. Gas drag fits to the radial particle accelerations provide an estimate for the local gas production rates ($Q_\text{g} = 3.6 \cdot 10^{-5}$ kg s$^{-1}$ m$^{-2}$), which is several times higher than our model predictions based on purely insolation-driven water ice sublimation. Our observational results and our modeling results both reveal that our particles were likely ejected with substantial nonzero initial velocities of around 0.5$-$0.6 m s$^{-1}$. Conclusions. Our findings strongly suggest that the observed ejection of decimeter-sized particles cannot be explained by water ice sublimation and favorable illumination conditions alone. Instead, the local structures and compositions of the source regions likely play a major role. In line with current ejection models of decimeter-sized particles, we deem an overabundance of CO$_2$ ice and its sublimation to be the most probable driver. In addition, because of the significant initial velocities, we suspect the ejection events to be considerably more energetic than gradual liftoffs.
description: 31 pages, 29 figures
ความชุกและปัจจัยที่มีความสัมพันธ์กับความเครียด ภาวะหมดไฟในการทำงานและประสิทธิภาพในการทำงานของผู้ปฏิบัติงานในอุตสาหกรรมเฟอร์นิเจอร์ภายใต้สถานการณ์การแพร่ระบาดของโรคโควิด 19
Creators: name: โยธิน พลประถม
Publisher: name: สถาบันวิจัยและพัฒนา มหาวิทยาลัยกาฬสินธุ์
Year: 2024
Subjects: ความเครียด
ภาวะหมดไฟในการทำงาน
ประสิทธิภาพในการทำงาน
อุตสาหกรรมเฟอร์นิเจอร์

description: วารสารวิทยาศาสตร์ เทคโนโลยี และนวัตกรรม มหาวิทยาลัยกาฬสินธุ์, 3, 1, 76-90
Aspects of four-jet production in polarized proton-proton collisions
Creators: name: Fraser, S. P.
name: Fraser, S. T.
name: Robinett, R. W.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We examine the intrinsic spin-dependence of the dominant $gg \rightarrow gggg$ subprocess contribution to four-jet production in polarized proton-proton collisions using helicity amplitude techniques. We find that the partonic level, longitudinal spin-spin asymmetry, $\hat{a}_{LL}$, is intrinsically large in the kinematic regions probed in experiments detecting four isolated jets. Such events may provide another qualitative or semi-quantitative test of the spin-structure of QCD in planned polarized $pp$ collisions at RHIC.
description: 9 pages, LaTeX, 2 uuencoded postscript files attached
Additional file 1 of Meta-analysis of AKI to CKD transition in perioperative patients
Creators: name: Abdala, Pedro M.
name: Swanson, Elizabeth A.
name: Hutchens, Michael P.
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Developmental Biology
subject: Marine Biology
subject: Science Policy

description: Additional file 1: Supplemental Table 1. Results of assessment for bias.
Long-term optical, UV, and X-ray continuum variations in the changing-look AGN HE 1136-2304
Creators: name: Zetzl, M.
name: Kollatschny, W.
name: Ochmann, M. W.
name: Grupe, D.
name: Haas, M.
name: Ramolla, M.
name: Chelouche, D.
name: Kaspi, S.
name: Schartel, N.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: A strong outburst in the X-ray continuum and a change of its Seyfert spectral type was detected in HE 1136-2304 in 2014. The spectral type changed from nearly Seyfert 2 type (1.95) to Seyfert 1.5 type in comparison to previous observations taken ten to twenty years before. In a subsequent variability campaign we wanted to investigate whether this outburst was a single event or whether the variability pattern following the outburst was similar to those seen in other variable Seyfert galaxies. In addition to a SALT spectral variability campaign, we carried out optical continuum as well as X-ray and UV (Swift) monitoring studies from 2014 to 2017. HE 1136-2304 strongly varied on timescales of days to months from 2014 to 2017. No systematic trends were found in the variability behavior following the outburst in 2014. A general decrease in flux would have been expected for a tidal disruption event. This could not be confirmed. More likely the flux variations are connected to irregular fluctuations in the accretion rate. The strongest variability amplitudes have been found in the X-ray regime: HE 1136-2304 varied by a factor of eight during 2015. The amplitudes of the continuum variability (from the UV to the optical) systematically decreased with wavelength following a power law F_var = a ${\times}$ λ^-c with c = 0.84. There is a trend that the B-band continuum shows a delay of three light days with respect to the variable X-ray flux. The Seyfert type 1.5 did not change despite the strong continuum variations for the period between 2014 and 2017.
description: 25 pages, 21 figures, Astronomy & Astrophysics in press
Revisiting log-periodic oscillations
Creators: name: Luck, Jean-Marc
Publisher: name: arXiv
Year: 2024
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: This work is inspired by a recent study of a two-dimensional stochastic fragmentation model. We show that the configurational entropy of this model exhibits log-periodic oscillations as a function of the sample size, by exploiting an exact recursion relation for the numbers of its jammed configurations. This is seemingly the first statistical-mechanical model where log-periodic oscillations affect the size dependence of an extensive quantity. We then propose and investigate in great depth a one-dimensional analogue of the fragmentation model. This one-dimensional model possesses a critical point, separating a strong-coupling phase where the free energy is super-extensive from a weak-coupling one where the free energy is extensive and exhibits log-periodic oscillations. This model is generalized to a family of one-dimensional models with two integer parameters, which exhibit essentially the same phenomenology.
description: 26 pages, 13 figures, 2 tables
Additional file 1 of Association between low-density cholesterol change and outcomes in acute ischemic stroke patients who underwent reperfusion therapy
Creators: name: Cui, Ting
name: Wang, Changyi
name: Zhu, Qiange
name: Wang, Anmo
name: Zhang, Xuening
name: Li, Shucheng
name: Yang, Yuan
name: Shang, Wenzuo
name: Peng, Rong
name: Wu, Bo
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Physiology
subject: FOS: Biological sciences
subject: Science Policy
subject: Computational Biology

description: Additional file 1: Table S1. Patient characteristics stratified by included patients and excluded patients
Additional file 1 of Analysis of global Aeromonas veronii genomes provides novel information on source of infection and virulence in human gastrointestinal diseases
Creators: name: Liu, Fang
name: Yuwono, Christopher
name: Tay, Alfred Chin Yen
name: Wehrhahn, Michael C.
name: Riordan, Stephen M.
name: Zhang, Li
Publisher: name: figshare
Year: 2022
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 1.
High-precision measurements of $n=2\to n=1$ transition energies and level widths in He- and Be-like Argon Ions
Creators: name: Machado, J.
name: Szabo, C. I.
name: Santos, J. P.
name: Amaro, P.
name: Guerra, M.
name: Gumberidze, A.
name: Bian, Guojie
name: Isac, J. M.
name: Indelicato, P.
name: Szabó, C.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Atomic Physics (physics.atom-ph)
subject: FOS: Physical sciences

description: We performed a reference-free measurement of the transition energies of the $1s 2p\,^1P\_1\to 1s^2 \,^1S\_0$ line in He-like argon, and of the $1s 2s^2 2p\,^1P\_1\to 1s^2 2s^2\,^1S\_0$ line in Be-like argon ions. The highly-charged ions were produced in the plasma of an Electron-Cyclotron Resonance Ion Source. Both energy measurements were performed with an accuracy better than 3 parts in $10^6$, using a double flat-crystal spectrometer, without reference to any theoretical or experimental energy. The $1s 2s^2 2p\,^1P\_1\to 1s^2 2s^2\,^1S\_0$ transition measurement is the first reference-free measurement for this core-excited transition. The $1s 2p\,^1P\_1\to 1s^2 \,^1S\_0$ transition measurement confirms recent measurement performed at the Heidelberg Electron-Beam Ion Trap (EBIT). The width measurement in the He-like transition provides test of a purely radiative decay calculations. In the case of the Be-like argon transition, the width results from the sum of a radiative channel and three main Auger channels. We also performed Multiconfiguration Dirac-Fock (MCDF) calculations of transition energies and rates and have done an extensive comparison with theory and other experimental data. For both measurements reported here, we find agreement with the most recent theoretical calculations within the combined theoretical and experimental uncertainties.
Milagrito: a TeV air-shower array
Creators: name: The Milagro Collaboration
name: Atkins, R.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Milagrito, a large, covered water-Cherenkov detector, was the world's first air-shower-particle detector sensitive to cosmic gamma rays below 1 TeV. It served as a prototype for the Milagro detector and operated from February 1997 to May 1998. This paper gives a description of Milagrito, a summary of the operating experience, and early results that demonstrate the capabilities of this technique.
description: 38 pages including 24 figures
Quantification of iodine in salt, foods
and determination of knowledge and pattern of consumption of iodine containing food materials in Sokoto State, Nigeria
Creators: name: Aminu Umar Imam
Publisher: name: สถาบันวิจัยและพัฒนา มหาวิทยาลัยกาฬสินธุ์
Year: 2024
Subjects: Iodine
salt
chicken
vegetables
thyroid
goiter

description: วารสารวิทยาศาสตร์ เทคโนโลยี และนวัตกรรม มหาวิทยาลัยกาฬสินธุ์, 3, 1, 92-104
Additional file 1: of Built and natural environment planning principles for promoting health: an umbrella review
Creators: name: E. Bird
name: J. Ige
name: P. Pilkington
name: A. Pinto
name: C. Petrokofsky
name: J. Burgess-Allen
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Developmental Biology
subject: Cancer
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: List of stakeholder organisation websites searched (alphabetical order). This file lists the stakeholder organisation websites searched for eligible review level documentation. (DOCX 14 kb)
Gamma rays from Dark Matter Annihilation in Three-loop Radiative Neutrino Mass Generation Models
Creators: name: Chowdhury, Talal Ahmed
name: Nasri, Salah
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We present the Sommerfeld enhanced Dark Matter (DM) annihilation into gamma ray for a class of three-loop radiative neutrino mass models with large electroweak multiplets where the DM mass is in O(TeV) range. We show that in this model, the DM annihilation rate becomes more prominent for larger multiplets and it is already within the reach of currently operating Imaging Atmospheric Cherenkov telescopes (IACTs), High Energy Stereoscopic System (H.E.S.S.). Furthermore, Cherenkov Telescope Array (CTA), which will begin operating in 2030, will improve this sensitivity by a factor of $\mathcal{O}{(10)}$ and may exclude a large portion of parameter space of this radiative neutrino mass model with larger electroweak multiplet. This implies that the only viable option is the model with lowest electroweak multiplets i.e. singlets of $SU(2)_{L}$ where the DM annihilation rate is not Sommerfeld enhanced and hence it is not yet constrained by the indirect detection limits from H.E.S.S. or future CTA.
description: 12 pages, 7 figures
title: Congenital stridor en route Swyer–James syndrome
Creators: name: Sourya Vengatesan, Jay
Publisher: name: EURORAD
Year: 2024
Subjects: subject: Chest imaging
subject: Lung
subject: Conventional radiography
subject: CT
subject: Clinical Case

description: Clinical History: An 11-year-old male child came with a 4-day history of fever, vomiting, abdominal pain, and a recent bout of cough with expectoration. A past history of congenital stridor, which was subsequently diagnosed as laryngomalacia, was managed conservatively. Since then, the child has had frequent hospitalisations due to recurrent lung infections.

description: 11 years, male
Additional file 1 of Midterm functional recovery of Total knee arthroplasty patients compared between the ATTUNE knee system and the press fit condylar (PFC) SIGMA knee system
Creators: name: Vanitcharoenkul, Ekasame
name: Unnanuntana, Aasis
Publisher: name: figshare
Year: 2021
Subjects: subject: Biophysics
subject: Medicine
subject: Neuroscience
subject: Physiology
subject: FOS: Biological sciences
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Additional file 1 Supplementary Table 1. Subgroup analysis of performance-based measures in the PFC Sigma and ATTUNE systems compared between those using and not using a gait aid. Supplementary Table 2. Subgroup analysis of performance-based measures in the PFC Sigma and ATTUNE systems compared between CCI score 0–3 and CCI score > 3
Coding culture at EEG
Creators: name: Philip Hackstock
Publisher: name: Zenodo
Year: 2022
Subjects: python
scientific software

description: These are the slides of a talk given on January 17th 2022, for the EEG at the TU Vienna.

The talk is subtitled 'Tools and best practices of scientific software development' and roughly covers the following three sections:

git

GitHub

General python best practices
High-Temperature Modifications of Charged Casimir Wormholes
Creators: name: Channuie, Phongpichit
Publisher: name: arXiv
Year: 2024
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: In this work, we extend the investigation of the consequences of thermal fluctuations on the Casimir effect within the context of a traversable wormhole, recently proposed by Garattini \& Faizal, arXiv:2403.15174 [gr-qc], subject to charge contributions. Specifically, we focus on scenarios where the plates exhibit both constant and radial variations. In our analysis, we initially concentrate on the high temperature approximation, considering solely the influence of charge on the thermal Casimir wormholes. Additionally, upon incorporating Generalized Uncertainty Principle (GUP) corrections to the Casimir energy, we obtain a new class of wormhole solutions. Notably, we establish that the flare-out condition remains consistently satisfied. Intriguingly, our findings reveal that both the charge and GUP contributions serve to further enlarge the throat's size in the radial variation.
description: v2: 11 pages, no figure, version accepted for publication by Nuclear Physics B
Additional file 2: of Built and natural environment planning principles for promoting health: an umbrella review
Creators: name: E. Bird
name: J. Ige
name: P. Pilkington
name: A. Pinto
name: C. Petrokofsky
name: J. Burgess-Allen
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Developmental Biology
subject: Science Policy

description: Characteristics of eligible review-level evidence, according to domain of interest. This file details the characteristics of eligible review-level evidence included within the umbrella review, and includes study population characteristics and quality appraisal outcomes. (DOCX 47 kb)
Thermal and Dynamical Equilibrium in Two-Component Star Clusters
Creators: name: Watters, W. A.
name: Joshi, K. J.
name: Rasio, F. A.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present the results of Monte Carlo simulations for the dynamical evolution of star clusters containing two stellar populations with individual masses m1 and m2 > m1, and total masses M1 and M2 < M1. We use both King and Plummer model initial conditions and we perform simulations for a wide range of individual and total mass ratios, m2/m1 and M2/M1. We ignore the effects of binaries, stellar evolution, and the galactic tidal field. The simulations use N = 10^5 stars and follow the evolution of the clusters until core collapse. We find that the departure from energy equipartition in the core follows approximately the theoretical predictions of Spitzer (1969) and Lightman & Fall (1978), and we suggest a more exact condition that is based on our results. We find good agreement with previous results obtained by other methods regarding several important features of the evolution, including the pre-collapse distribution of heavier stars, the time scale on which equipartition is approached, and the extent to which core collapse is accelerated by a small subpopulation of heavier stars. We briefly discuss the possible implications of our results for the dynamical evolution of primordial black holes and neutron stars in globular clusters.
description: 31 pages, including 13 figures, to appear in ApJ
Supersymmetric Magnetic Moments Sum Rules and Spontaneous Supersymmetry Breaking
Creators: name: Khalil, S. S.
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: In supersymmetry the anomalous magnetic moment of particles belonging to the same supermultiplet is related by simple sum rules. We study the modification of these sum rules in the case of spontaneously broken N=1 global supersymmetry.
description: 10 pages, 3 figures ( not included )
Diffusion in mesoscopic lattice models of amorphous plasticity
Creators: name: Tyukodi, Botond
name: Maloney, Craig E
name: Vandembroucq, Damien
Publisher: name: arXiv
Year: 2018
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: We present results on tagged particle diffusion in a meso-scale lattice model for sheared amorphous material in athermal quasi-static conditions. We find a short time diffusive regime and a long time diffusive regime whose diffusion coefficients depend on system size in dramatically different ways. At short time, we find that the diffusion coefficient, $D$, scales roughly linearly with system length, $D\sim L^{1.05}$. This short time behavior is consistent with particle-based simulations. The long-time diffusion coefficient scales like $D\sim L^{1.6}$, close to previous studies which found $D\sim L^{1.5}$. Furthermore, we show that the near-field details of the interaction kernel do not affect the short time behavior, but qualitatively and dramatically affect the long time behavior, potentially causing a saturation of the mean-squared displacement at long times. Our finding of a $D\sim L^{1.05}$ short time scaling resolves a long standing puzzle about the disagreement between the diffusion coefficient measured in particle-based models and meso-scale lattice models of amorphous plasticity.
description: 5 pages, 5 figures, Supplementary Information
Coronal activity as a consequence of dynamos in astrophysical rotators
Creators: name: Blackman, Eric G.
name: Field, George B.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We show that the presence of a steady $\ao$ dynamo in astrophysical rotators likely leads to an outflow of relative magnetic helicity and thus magnetic energy available for particle acceleration in a corona. The connection between energy and magnetic helicity arises because the generation of large scale field is linked to a generation of large scale magnetic helicity. In a steady state, the relative magnetic helicity associated with the large scale field can escape, accompanied by an equal and opposite small scale contribution from the field, since the total magnetic helicity in large magnetic Reynolds number flows is conserved. From the helicity flow, a lower limit on the magnetic energy deposited in the corona can be estimated. Steady coronal activity and the dissipation of magnetic energy is therefore a signature of an internal dynamo. Our theoretical estimate of the power delivered by a mean field dynamo is consistent with that inferred from observations to be delivered to the solar corona, the Galactic corona, and Seyfert I AGN coronae.
description: 16 pages LaTeX, Submitted to MNRAS
Additional file 1 of Meta-analysis of AKI to CKD transition in perioperative patients
Creators: name: M. Abdala, Pedro
name: Swanson, Elizabeth A.
name: P. Hutchens, Michael
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Developmental Biology
subject: Marine Biology
subject: Science Policy

description: Additional file 1: Supplemental Table 1. Results of assessment for bias.
title: ADCO, Premier cartulaire de Saint-Étienne de Dijon (XIIe siècle), Cart. 21 (G 125), 71 folios, f. 00100
Creators: name: de la Côte d'Or, Archives départementales
name: CG21/F.PETOT/2015
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: cartulaire
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Premier cartulaire de Saint-Étienne de Dijon (XIIe siècle), Archives départementales de la Côte-d'Or, Cart. 21 (G 125), 71 folios, f. 00100, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Premier cartulaire de Saint-Étienne de Dijon (XIIe siècle), Archives départementales de la Côte-d'Or, Cart. 21 (G 125), 71 folios, f. 00100, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https://manuscrits.cbma-project.eu/
description: Provenance: abbaye Saint-Étienne de Dijon
description: Provenance: http://www.wikidata.org/entity/Q15945019
Constraints on the emission mechanisms of gamma-ray bursts
Creators: name: Ghisellini, Gabriele
name: Celotti, Annalisa
name: Lazzati, Davide
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: If the emission of gamma-ray bursts were due to the synchrotron process in the standard internal shock scenario, then the typical observed spectrum should have a slope F(nu) \propto nu^{-1/2}, which strongly conflicts with the much harder spectra observed. This directly follows from the cooling time being much shorter than the dynamical time. Particle re-acceleration, deviations from equipartition, fastly changing magnetic fields and adiabatic losses are found to be inadequate to account for this discrepancy. We also find that in the internal shock scenario the relativistic inverse Compton scattering is always as important as the synchrotron process, and faces the same problems. This indicates that the burst emission is not produced by relativistic electrons emitting synchrotron and inverse Compton radiation.
description: 5 pages, accepted for publications in MNRAS, pink pages
ออกแบบและพัฒนาบรรจุภัณฑ์สบู่น้ำผึ้งชันโรงของชุมชนตลาดน้ำสองคลองวัดตลิ่งชัน
Creators: name: พิเชฐ มีมะแม
Publisher: name: สถาบันวิจัยและพัฒนา มหาวิทยาลัยกาฬสินธุ์
Year: 2024
Subjects: การออกแบบและพัฒนา
บรรจุภัณฑ์
สบู่น้ำผึ้งชันโรง
ชุมชนตลาดน้ำสองคลองวัดตลิ่งชัน

description: วารสารวิทยาศาสตร์ เทคโนโลยี และนวัตกรรม มหาวิทยาลัยกาฬสินธุ์, 3, 1, 105-119
INVESTMENT ACCOUNTING AND ITS ROLE IN THE ECONOMY OF UZBEKISTAN
Creators: name: Berdaliyev, Xaydarqul
Publisher: name: Zenodo
Year: 2024

description: Investment accounting is a crucial foundation for economic development. The role of investments is particularly significant in ensuring the economic growth and stability of Uzbekistan. This article analyzes the key concepts of investment accounting and its place in the economy of Uzbekistan.
Nonequilibrium many-body quantum dynamics: from full random matrices to real systems
Creators: name: Santos, Lea F.
name: Torres-Herrera, E. J.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: We present an overview of our studies on the nonequilibrium dynamics of quantum systems that have many interacting particles. Our emphasis is on systems that show strong level repulsion, referred to as chaotic systems. We discuss how full random matrices can guide and support our studies of realistic systems. We show that features of the dynamics can be anticipated from a detailed analysis of the spectrum and the structure of the initial state projected onto the energy eigenbasis. On the other way round, if we only have access to the dynamics, we can use it to infer the properties of the spectrum of the system. Our focus is on the survival probability, but results for other observables, such as the spin density imbalance and Shannon entropy are also mentioned.
description: 14 pages, 7 figures, chapter for the book "Thermodynamics in the Quantum Regime - Recent Progress and Outlook"
Additional file 1: of The prevalence of psychiatric disorders among students aged 6~ 16 years old in central Hunan, China
Creators: name: Shen, Yan-Mei
name: Chan, Bella
name: Liu, Jian-Bo
name: Yuan-Yue Zhou
name: Cui, Xi-Long
name: He, Yu-Qiong
name: Fang, Yu-Min
name: Xiang, Yu-Tao
name: Luo, Xue-Rong
Publisher: name: figshare
Year: 2018
Subjects: subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Demarcation and total scores for subscales of behavior problem. The Additional file 1 provided information on the demarcation score for the various subscales of behavior problem and total score in adolescents aged 6–16 years old. The scores are presented in 4 separate tables that are divided by gender (boys and girls) and by age group (6–11, 12–16). (DOCX 16 kb)
นวัตกรรมตู้เตรียมตัวอย่างสำหรับงานเพาะเลี้ยงแบคทีเรีย
Creators: name: เจตนา วีระกุล
Publisher: name: สถาบันวิจัยและพัฒนา มหาวิทยาลัยกาฬสินธุ์
Year: 2024
Subjects: ตู้ปลอดเชื้อ
ตู้เขี่ยเชื้อ
ตู้ชีวนิรภัย
ตู้ไบโอฮาซาดร์ด

description: วารสารวิทยาศาสตร์ เทคโนโลยี และนวัตกรรม มหาวิทยาลัยกาฬสินธุ์, 3, 1, 120-131
title: Solar Fridge Vaccine Storage System
Creators: name: Elhagehassan, Hanin
name: O'Malley, Connor
name: Hamby, Ryan
name: Putti, Amanda
name: Xu, Eldon
name: Chen, Thomas
name: Gallagher, Carina
name: Lee, Aham
name: Lee, Allison
name: Chen, Nancy
name: Fang, Ryan
name: Gallagher, Cara
name: Govindswamy, Avani
name: Bueno Reis, Thiago
name: Richards, Zach
name: Shi, Alan
name: Ferriero, Gabriel
name: Zavala, Paola
name: Mendonca, Amol
name: Tappeta, Rishi
name: Desai, Sarina
name: Garzo Dominguez, Olivia
name: Hagan, Peter
name: Kondur, Amrita
name: Nazareno, Evan
name: Robbins, Maggie
name: Segal, Elise
name: Wadhawan, Aayushi
name: Alrazzi, Saad
name: Hansen, Anders Martin
name: Starzacher, Elaina
name: Tikekar, Ava
name: Vatakencherry, Aryan
Publisher: name: University of Michigan
Year: 2024
Subjects: subject: socially engaged design
subject: innovation
subject: medicine
subject: Engineering

description: Although vaccines are considered one of the most significant advancements in medicine, many areas around the world have limited access to power, which makes it difficult to keep vaccines viable. At Solar Fridge, my team and I aim to address this issue at our partner clinic in Rincon Claro in the Dominican Republic as they face frequent power outages. Rincon Claro faces constant excessive heat, so any time they have a power outage the temperature in their fridges and freezers go up at an alarming rate which contributes to spoiling vaccines in rural clinics. All they have to fight against these challenges is a small Styrofoam box with melting ice, which is not very effective. There is a need for a cost-effective vaccine storage system that maintains vaccine viability during these shutoffs. These clinics need to be able to maintain vaccine viability so that all patients in Rincon Claro can have a fair access to vaccines and boost their immunity to 9 different types of diseases and viruses. One part of the proposed prototype will be concerned with insulating the whole cooler as much as possible using materials which have low thermal resistivity. The other electrical component is focused on cooling the inside to the desired temperature range, which will run on solar power when solar energy is incorporated.
Properties of the two-temperature corona model for active galactic nuclei and galactic black holes
Creators: name: Janiuk, Agnieszka
name: Czerny, Bozena
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We study in detail the properties of the accreting corona model for active galactic nuclei and galactic black holes. In this model the fraction of the energy liberated in the corona at a given radius is calculated from the global parameters of the model (mass of the central object, accretion rate and viscosity parameter) and it appears to be a strong function of the radius. The model predicts the relative decrease of the coronal hard X-ray emission with an increase of the accretion rate. The presented description of disc/corona interaction forms a basis for further studies of disc disruption mechanism.
description: 31 pages, 18 figures, accepted for publication in New Astronomy
High-velocity collimated outflows in planetary nebulae: NGC 6337, He 2-186, and K 4-47
Creators: name: Corradi, Romano L. M.
name: Goncalves, Denise R.
name: Villaver, Eva
name: Mampaso, Antonio
name: Perinotto, Mario
name: Schwarz, Hugo E.
name: Zanin, Caterina
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have obtained narrow-band images and high-resolution spectra of the planetary nebulae NGC 6337, He 2-186, and K 4-47, with the aim of investigating the relation between their main morphological components and several low-ionization features present in these nebulae. The data suggest that NGC 6337 is a bipolar PN seen almost pole on, with polar velocities higher than 200 km/s. The bright inner ring of the nebula is interpreted to be the "equatorial" density enhancement. It contains a number of low-ionization knots and outward tails that we ascribe to dynamical instabilities leading to fragmentation of the ring or transient density enhancements due to the interaction of the ionization front with previous density fluctuations in the ISM. The lobes show a pronounced point-symmetric morphology and two peculiar low-ionization filaments whose nature remains unclear. The most notable characteristic of He 2-186 is the presence of two high-velocity (higher than 135 km/s) knots from which an S-shaped lane of emission departs toward the central star. K 4-47 is composed of a compact core and two high-velocity, low-ionization blobs. We interpret the substantial broadening of line emission from the blobs as a signature of bow shocks, and using the modeling of Hartigan, Raymond, & Hartman (1987), we derive a shock velocity of 150 km/s and a mild inclination of the outflow on the plane of the sky. We discuss possible scenarios for the formation of these nebulae and their low-ionization features. In particular, the morphology of K 4-47 hardly fits into any of the usually adopted mass-loss geometries for single AGB stars. Finally, we discuss the possibility that point-symmetric morphologies in the lobes of NGC 6337 and the knots of He 2-186 are the result of precessing outflows from the central stars.
description: 16 pages plus 7 figures, ApJ accepted. Also available at http://www.iac.es/publicaciones/preprints.html
Observation of different reactivities of para- and ortho-water towards cold diazenylium ions
Creators: name: Kilaj, Ardita
name: Gao, Hong
name: Rösch, Daniel
name: Rivero, Uxia
name: Küpper, Jochen
name: Willitsch, Stefan
Publisher: name: arXiv
Year: 2018
Subjects: subject: Chemical Physics (physics.chem-ph)
subject: FOS: Physical sciences

description: Water, H$_2$O, is one of the fundamental molecules in chemistry, biology and astrophysics. It exists as two distinct nuclear-spin isomers, para- and ortho-water, which do not interconvert in isolated molecules. The experimental challenges in preparing pure samples of the two isomers have thus far precluded a characterization of their individual chemical behaviour. Capitalizing on recent advances in the electrostatic deflection of polar molecules, we separated the ground states of para- and ortho-water in a molecular beam to show that the two isomers exhibit different reactivities in a prototypical reaction with cold diazenylium ions (N$_2$H$^+$). Based on ab initio calculations and a modelling of the reaction kinetics using rotationally adiabatic capture theory, we rationalize this finding in terms of different rotational averaging of ion-dipole interactions during the reaction. The present results highlight the subtle interplay between nuclear-spin and rotational symmetry and its ramifications on chemical reactivity.
description: 10 pages, 4 figures, supplementary information: 9 pages, 5 figures
Lattice Regularization of Gauge Theories Without Loss of Chiral Symmetry
Creators: name: Hooft, G. 't
Publisher: name: arXiv
Year: 1994
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: High Energy Physics - Lattice (hep-lat)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: A lattice regularization procedure for gauge theories is proposed in which fermions are given a special treatment such that all chiral flavor symmetries that are free of Adler-Bell-Jackiw anomalies are kept intact. There is no doubling of fermionic degrees of freedom. A price paid for this feature is that the number of fermionic degrees of freedom per unit cell is still infinite, although finiteness of the complete functional integrals can be proven (details are outlined in an Appendix). Therefore, although perhaps of limited usefulness for numerical simulations, our scheme can be applied for studying aspects such as analytic convergence questions, spontaneous symmetry breakdown and baryon number violation in non-Abelian gauge theories.
description: Correction of formula in Appendix, and extra references added
Lettre de Charles Martin Hurson à Jean-François Séguier, 1762-07-29
Creators: name: Hurson, Charles Martin
name: Hurson, Charles Martin
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2022
Subjects: Recommandation

description: Toulon 29 juillet 1762

Je ne sais pas, Monsieur, si vous voudrez bien vous souvenir de moi mais je sais bien que je n’ai point oublié. Les politesses dont vous m’avez comblé lorsque je passais à Nîmes en 1759 avec M. Marade. 
Oserais-je vous supplier de vouloir bien rendre un service qui dépend tout de vous à trois étrangers qui vont voir les curiosités de votre ville.
Cette lettre vous sera rendue par M. de Kauderbach, ministre plénipotentiaire de Pologne à la Haye qui accompagne dans ses voyages M. le chevalier de Bruhl fils du fameux M. le comte de Bruhl, Premier ministre du roi de Pologne, électeur de Saxe ; ce sont des gens de mérite et instruits, je les ai assurés qu’ils trouveraient chez vous tout ce qu’ils pourraient désirer et pour l’instruction sur les Antiquités de Nîmes et pour la politesse avec laquelle vous voulez bien recevoir les étrangers. Ils verront aussi votre cabinet dont ils seront surement contents.
Je profite avec grand plaisir de cette occasion pour vous assurer du sincère et inviolable attachement avec lequel j’ai l’honneur d’être, Monsieur,

 Votre très humble et très obéissant serviteur

 Hurson
 Intendant de Toulon

M. Séguier, correspondant de l’Académie
Des inscriptions et belles-lettres de Paris
À Nîmes

[fol. 68] cartes de visite imprimées au nom du chevalier de Brühl (annotée par Séguier : « fils du premier ministre du roi de Pologne le 7 août 1762 ») et au nom de Mr Kauderbach, « conseiller privé d’ambassade de Sa Majesté le Roi de Pologne, Electeur de Saxe etc. et son ministre près L.H.P. les seigneurs États généraux des Provinces Unies des Pays Bas ».

Personnes citées : Heinrich von Brühl (1700-1763), Hans Moritz von Brühl (1746-1811), comte Johann Heinrich de Kauderbach (1707-1785) ministre plénipotentiaire de Pologne à la Haye
description: Source: [établissement de conservation] Nîmes, Bibliothèque Carré d'Art [cote] ms. 249, fol. 59, 68
Tensor-based Nonlinear Classifier for High-Order Data Analysis
Creators: name: Makantasis, Konstantinos
name: Doulamis, Anastasios
name: Doulamis, Nikolaos
name: Nikitakis, Antonis
name: Voulodimos, Athanasios
Publisher: name: arXiv
Year: 2018
Subjects: subject: Machine Learning (cs.LG)
subject: Machine Learning (stat.ML)
subject: FOS: Computer and information sciences

description: In this paper we propose a tensor-based nonlinear model for high-order data classification. The advantages of the proposed scheme are that (i) it significantly reduces the number of weight parameters, and hence of required training samples, and (ii) it retains the spatial structure of the input samples. The proposed model, called \textit{Rank}-1 FNN, is based on a modification of a feedforward neural network (FNN), such that its weights satisfy the {\it rank}-1 canonical decomposition. We also introduce a new learning algorithm to train the model, and we evaluate the \textit{Rank}-1 FNN on third-order hyperspectral data. Experimental results and comparisons indicate that the proposed model outperforms state of the art classification methods, including deep learning based ones, especially in cases with small numbers of available training samples.
description: To appear in IEEE ICASSP 2018. arXiv admin note: text overlap with arXiv:1709.08164
Additional file 1 of Optimal SARS-CoV-2 vaccine allocation using real-time attack-rate estimates in Rhode Island and Massachusetts
Creators: name: Tran, Thu Nguyen-Anh
name: Wikle, Nathan B.
name: Albert, Emmy
name: Inam, Haider
name: Strong, Emily
name: Brinda, Karel
name: Leighow, Scott M.
name: Yang, Fuhan
name: Hossain, Sajid
name: Pritchard, Justin R.
name: Chan, Philip
name: Hanage, William P.
name: Hanks, Ephraim M.
name: Boni, Maciej F.
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Biotechnology
subject: Immunology
subject: FOS: Clinical medicine
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Additional file 1 Supplementary figures.
Additional file 2: of Advice-seeking during implementation: a network study of clinicians participating in a learning collaborative
Creators: name: Bunger, Alicia
name: Doogan, Nathan
name: Hanson, Rochelle
name: Birken, Sarah
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy

description: ERGM model-building details (DOCX 37Â kb)
Jets, knots and tails in planetary nebulae: NGC 3918, K 1-2 and Wray 17-1
Creators: name: Corradi, Romano L. M.
name: Perinotto, Mario
name: Villaver, Eva
name: Mampaso, Antonio
name: Goncalves, Denise R.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We analyze optical images and high-resolution, long-slit spectra of three planetary nebulae which possess collimated, low-ionization features. NGC 3918 is composed of an inner, spindle-shaped shell mildly inclined with respect to the plane of the sky. Departing from the polar regions of this shell, we find a two-sided jet expanding with velocities which increase linearly with distance from 50 to 100 km/s. The jet is probably coeval with the inner shell (with the age of approximately 1000 D yr, where D is the distance in kpc), suggesting that its formation should be ascribed to the same dynamical processes which also shaped the main nebula, and not to a more recent mass loss episode. We discuss the formation of the aspherical shell and jet in the light of current hydrodynamical and magnetohydrodynamical theories. K 1-2 is a planetary nebula with a close binary nucleus which shows a collimated string of knots embedded in a diffuse, elliptical shell. The knots expand with a velocity similar to that of the elliptical nebula (25 km/s), except for an extended tail located out of the main nebula, which linearly accelerates up to 45 km/s. We estimate an inclination on the line of the sight of 40 degres for the string of knots; once the orientation of the orbit is also determined, this information will allow us to test the prediction of current theories of the occurrence of polar jets from close binary systems. Wray 17-1 has a complex morphology, showing two pairs of low-ionization structures located in almost perpendicular directions from the central star, and embedded in a large, diffuse nebula. The two pairs show notable similarities and differences, and their origin is very puzzling.
description: 20 pages plus 10 figures. ApJ recently published (ApJ 523, 721 (1999))
title: ADCO, Huitième cartulaire de Saint-Étienne de Dijon (1661-1667), Cart. 31 (G 135), 549 folios, f. 0567
Creators: name: de la Côte d'Or, Archives départementales
name: Archives Départementales De La Côte-D'Or
name: Petot, Frédérique
name: Projet CBMA
name: CG21/F.PETOT/2012
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020
Subjects: subject: cartulaire
subject: Corpus Burgundiae Medii Aevi
subject: Chartes de la Bourgogne du Moyen Âge
subject: LaMOP
subject: Laboratoire de Médiévistique Occidentale de Paris

description: Huitième cartulaire de Saint-Étienne de Dijon (1661-1667), Archives départementales de la Côte-d'Or, Cart. 31 (G 135), 549 folios, f. 0567, Numérisation en mode image.
description: Relation: http://www.cbma-project.eu/
description: Bibliographic citation: Huitième cartulaire de Saint-Étienne de Dijon (1661-1667), Archives départementales de la Côte-d'Or, Cart. 31 (G 135), 549 folios, f. 0567, in Projet CBMA - Corpus Burgundiae Medii Aevi [Ressource en ligne], https://manuscrits.cbma-project.eu/
description: Provenance: abbaye Saint-Étienne de Dijon
description: Provenance: http://www.wikidata.org/entity/Q15945019
Additional file 1 of Residual malaria in Jazan region, southwestern Saudi Arabia: the situation, challenges and climatic drivers of autochthonous malaria
Creators: name: Al-Mekhlafi, Hesham M.
name: Madkhali, Aymen M.
name: Ghailan, Khalid Y.
name: Abdulhaq, Ahmed A.
name: Ghzwani, Ahmad Hassn
name: Zain, Khalid Ammash
name: Atroosh, Wahib M.
name: Alshabi, Alkhansa
name: Khadashi, Hussein A.
name: Darraj, Majid A.
name: Eisa, Zaki M.
Publisher: name: figshare
Year: 2021
Subjects: subject: 29999 Physical Sciences not elsewhere classified
subject: FOS: Physical sciences
subject: Medicine
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Sociology
subject: FOS: Sociology
subject: Cancer
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Additional file 1: Table S1. Pearson’s correlation coefficient matrix of unlagged monthly climatic variables and autochthonous malaria cases reported in Jazan region between 2010 and 2017
Optimal softening for force calculations in collisionless N-body simulations
Creators: name: Athanassoula, E.
name: Fady, E.
name: Lambert, J. -C.
name: Bosma, A.
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: In N-body simulations the force calculated between particles representing a given mass distribution is usually softened, to diminish the effect of graininess. In this paper we study the effect of such a smoothing, with the aim of finding an optimal value of the softening parameter. As already shown by Merritt (1996), for too small a softening the estimates of the forces will be too noisy, while for too large a softening the force estimates are systematically misrepresented. In between there is an optimal softening, for which the forces in the configuration approach best the true forces. The value of this optimal softening depends both on the mass distribution and on the number of particles used to represent it. For higher number of particles the optimal softening is smaller. More concentrated mass distributions necessitate smaller softening, but the softened forces are never as good an approximation of the true forces as for not centrally concentrated configurations. We give good estimates of the optimal softening for homogeneous spheres, Plummer spheres, and Dehnen spheres. We also give a rough estimate of this quantity for other mass distributions, based on the harmonic mean distance to the $k$th neighbour ($k$ = 1, .., 12), the mean being taken over all particles in the configuration. Comparing homogeneous Ferrers ellipsoids of different shapes we show that the axial ratios do not influence the value of the optimal softening. Finally we compare two different types of softening, a spline softening (Hernquist & Katz 1989) and a generalisation of the standard Plummer softening to higher values of the exponent. We find that the spline softening fares roughly as well as the higher powers of the power-law softening and both give a better representation of the forces than the standard Plummer softening.
description: 16 pages Latex, 19 figures, accepted for publication in MNRAS, corrected typos, minor changes mainly in sec. 5