cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Rate of convergence to self-similarity for Smoluchowski's coagulation equation with constant coefficients
Creators: name: Cañizo, José Alfredo
name: Mischler, Stéphane
name: Mouhot, Clément
Publisher: name: arXiv
Year: 2008
Subjects: subject: Analysis of PDEs (math.AP)
subject: FOS: Mathematics
subject: 82C21,45K05,82C05

description: We show that solutions to Smoluchowski's equation with a constant coagulation kernel and an initial datum with some regularity and exponentially decaying tail converge exponentially fast to a self-similar profile. This convergence holds in a weighted Sobolev norm which implies the L\^2 convergence of derivatives up to a certain order k depending on the regularity of the initial condition. We prove these results through the study of the linearized coagulation equation in self-similar variables, for which we show a spectral gap in a scale of weighted Sobolev spaces. We also take advantage of the fact that the Laplace or Fourier transforms of this equation can be explicitly solved in this case.
description: 41 pages
Qualcosa che non va negli anelli di Saturno
Creators: Eleonora Ferroni
Publisher: name: Media Inaf
Year: 2015

Un'estesa sezione all'esterno del più largo degli anelli (Anello A) è risultata essere più calda, con un picco soprattutto al centro. Le particelle ghiacciate sono più soffici all'esterno, ma nell'Anello A risultano più grandi e ghiacciate e con solo un sottile strato superficiale di regolite
A scuola di pensiero critico
Creators: Corrado Ruscica
Publisher: name: Media Inaf
Year: 2015

Alcuni fisici delle Università  di Stanford e della British Columbia hanno trovato un metodo in base al quale incoraggiare gli studenti a prendere ripetutamente delle decisioni sui dati raccolti durante i corsi di laboratorio migliora le loro capacità in termini del pensiero critico. I risultati sono pubblicati su Proceedings of the National Academy of Sciences
Lo Space System Award a Herschel e Planck
Creators: Marco Malaspina
Publisher: name: Media Inaf
Year: 2015

Va ai project team dei due telescopi spaziali ESA il riconoscimento annuale dell’American Institute of Aeronautics and Astronautics dedicato ai sistemi spaziali. La medaglia è stata consegnata durante la cerimonia di chiusura di Space2015. Il commento di Anna Maria Di Giorgio (INAF IAPS Roma)
L’autostoppista delle comete
Creators: Eleonora Ferroni
Publisher: name: Media Inaf
Year: 2015

Si tratta di un'idea innovativa per viaggiare nello spazio usando un arpione e una catena per agganciarsi ad asteroidi e comete in modo da utilizzare meno propellente possibile (bene molto prezioso nei viaggi spaziali)
Additional file 1 of The effects of developmental model of peer observation on the virtual teaching quality of basic medical sciences faculty
Creators: name: Doroh, Mohammad Habibi
name: Farajpour, Arezou
name: Amirmajdi, Elham Mokhtari
Publisher: name: figshare
Year: 2023
Subjects: subject: Medicine
subject: Neuroscience
subject: Physiology
subject: FOS: Biological sciences
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Science Policy
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Supplementary Material 1
Satelliti fuori uso? Eliminiamoli così
Creators: Marco Galliani
Publisher: name: Media Inaf
Year: 2015

Sviluppato da alcuni ricercatori dell'Università di La Rioja in Spagna un nuovo metodo per eliminare satelliti artificiali su orbite altamente ellittiche giunti alla fine della loro vita operativa, riducendo i costi e i rischi delle procedure di deorbitazione
Feedback and the Formation of Dwarf Galaxy Stellar Halos
Creators: name: Stinson, Greg
name: Dalcanton, Julianne
name: Quinn, Tom
name: Gogarten, Stephanie
name: Kaufmann, Tobias
name: Wadsley, James
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Stellar population studies show that low mass galaxies in all environments exhibit stellar halos that are older and more spherically distributed than the main body of the galaxy. In some cases, there is a significant intermediate age component that extends beyond the young disk. We examine a suite of Smoothed Particle Hydrodynamic (SPH) simulations and find that elevated early star formation activity combined with supernova feedback can produce an extended stellar distribution that resembles these halos for model galaxies ranging from $v_{200}$ = 15 km s$^{-1}$ to 35 km s$^{-1}$, without the need for accretion of subhalos.
description: 15 pages, 15 figures, accepted MNRAS
Esopianeti: è tutta un’altra chimica
Creators: Davide Coero Borga
Publisher: name: Media Inaf
Year: 2015

E se la chimica su cui si basa l’interno di pianeti rocciosi, nell’orbita di stelle lontane, fosse completamente diversa da quella cui siamo abituati a Terra? Secondo uno studio della Carnegie Institution potrebbe verificarsi abbondanza di composti di magnesio
title: ÐÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ðµ ÐºÑÐ¸ÑÐµÑÐ¸ÐµÐ² ÐºÐ°ÑÐµÑÑÐ²Ð° Ð² ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ð¸ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð¾Ð¼ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½Ð¾-ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð¹ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸
title: Determination of quality criteria in hr management of a production and technology company
Creators: name: ÐÐ¼Ð¸ÑÑÐ¸ÐµÐ²Ð°, ÐÐ½Ð°ÑÑÐ°ÑÐ¸Ñ
name: "Ð£Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸ÑÐ¼Ð¸ Ð² ÑÑÐ»Ð¾Ð²Ð¸ÑÑ  ÑÐ¸ÑÑÐ¾Ð²Ð¾Ð¹ ÑÑÐ°Ð½ÑÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¸", Ð²ÑÐµÑÐ¾ÑÑÐ¸Ð¹ÑÐºÐ°Ñ ÑÑÑÐ´ÐµÐ½ÑÐµÑÐºÐ°Ñ ÑÑÐµÐ±Ð½Ð¾-Ð½Ð°ÑÑÐ½Ð°Ñ ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ñ (2023; Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³)
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2023
Subjects: ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð¾Ð¼
ÑÐµÐ»Ð¾Ð²ÐµÑÐµÑÐºÐ¸Ðµ ÑÐµÑÑÑÑÑ
Ð¿ÑÐ¾ÑÐµÑÑ
Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸ ÐºÐ°ÑÐµÑÑÐ²Ð°
ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ñ
ÐºÐ»Ð°ÑÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¸Ñ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»ÐµÐ¹
personnel management
human resources
process
quality indicators
company
classification of indicators

description: Ð ÑÐ°Ð±Ð¾ÑÐµ Ð¸ÑÑÐ»ÐµÐ´ÑÑÑÑÑ ÐºÑÐ¸ÑÐµÑÐ¸Ð¸, Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼ÑÐµ Ð´Ð»Ñ Ð¾ÑÐµÐ½ÐºÐ¸ ÐºÐ°ÑÐµÑÑÐ²Ð° Ð¿ÑÐ¾ÑÐµÑÑÐ° ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð¾Ð¼ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½Ð¾-ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð¹ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸. ÐÐµÑÑÐ¾Ð½Ð°Ð» ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÐµÑÑÑ ÐºÐ°Ðº ÐºÐ»ÑÑÐµÐ²Ð¾Ð¹ ÑÐµÑÑÑÑ, Ð±Ð»Ð°Ð³Ð¾Ð´Ð°ÑÑ ÐºÐ¾ÑÐ¾ÑÐ¾Ð¼Ñ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¼Ð¾Ð³ÑÑ Ð¿Ð¾Ð²ÑÑÐ¸ÑÑ ÑÐ²Ð¾Ð¹ ÑÑÐ¾Ð²ÐµÐ½Ñ ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ¾ÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÐ¸ Ð¸ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸. ÐÐºÑÑÐ°Ð»ÑÐ½Ð¾ÑÑÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð·Ð°ÐºÐ»ÑÑÐ°ÐµÑÑÑ Ð² Ð²Ð°Ð¶Ð½Ð¾ÑÑÐ¸ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ½Ð¾Ð¹ Ð¾ÑÐµÐ½ÐºÐ¸ Ð¿ÑÐ¾ÑÐµÑÑÐ° ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð¾Ð¼ Ð¸ Ð¿ÑÐ¾ÑÐ°Ð±Ð¾ÑÐºÐµ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ð½ÑÑ Ð·Ð¾Ð½ Ñ Ð¾Ð¿Ð¾ÑÐ¾Ð¹ Ð½Ð° ÑÑÐ¸ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸. Ð ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐµ ÑÐ°Ð±Ð¾ÑÑ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ñ Ð³ÑÑÐ¿Ð¿Ñ ÐºÑÐ¸ÑÐµÑÐ¸ÐµÐ² Ð¾ÑÐµÐ½ÐºÐ¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð¾Ð¼ Ð¸ Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÐ½Ñ Ð¿ÑÐ¸Ð¼ÐµÑÑ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»ÐµÐ¹ ÐºÐ°ÑÐµÑÑÐ²Ð°. ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ð¸ ÑÑÐ¾Ð³Ð¾ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ñ ÑÐ°Ð³Ð¸ Ð´Ð»Ñ ÑÐµÑÐµÐ½Ð¸Ñ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸. Ð¡Ð´ÐµÐ»Ð°Ð½Ñ Ð²ÑÐ²Ð¾Ð´Ñ Ð¾ Ð¿ÐµÑÑÐ¿ÐµÐºÑÐ¸Ð²Ð½ÑÑ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÑÐ°Ð±Ð¾ÑÑ.
description: The paper examines the criteria necessary to assess the quality of the personnel management process of a production and technology company. Personnel is seen as a key resource through which organizations can increase their level of competitiveness and efficiency. The relevance of the study lies in the importance of a comprehensive assessment of the personnel management process and the development of problem areas based on these indicators. As a result of the work, groups of criteria for assessing personnel management were identified and examples of quality indicators were given. Based on this, steps are proposed to solve the company's problem. Conclusions are drawn about promising areas of work.
The Pulsar Planets: A Test Case of Terrestrial Planet Assembly
Creators: name: Hansen, Brad
name: Shih, Hsin-Yi
name: Currie, Thayne
Publisher: name: arXiv
Year: 2009
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We model the assembly of planets from planetary embryos under the conditions suggested by various scenarios for the formation of the planetary system around the millisecond pulsar B1257+12. We find that the most likely models fall at the low angular momentum end of the proposed range. Models that invoke supernova fallback produce such disks, although we find that a solar composition disk produces a more likely evolution than one composed primarily of heavy elements. Furthermore, we find that dust sedimentation must occur rapidly as the disk cools, in order that the solid material be confined to a sufficiently narrow range of radii. A quantitative comparison between the observations and the best-fit models shows that the simulations can reproduce the observed eccentricities and masses, but have difficulty reproducing the compactness of the pulsar planet system. Finally, we examine the results of similar studies of solar system terrestrial planet accumulation and discuss what can be learned from the comparison.
Le stelle si dedicano al riciclo
Creators: Redazione Media Inaf
Publisher: name: Media Inaf
Year: 2015

Si tratta della nebulosa Gum 56. Per milioni di anni le stelle sono state create a partire dal gas di questa nebulosa, materiale che viene più tardi restituito all'incubatrice stellare quando le stelle invecchiando lo rilasciano con calma nello spazio oppure più drammaticamente lo espellono con esplosioni di supernova
Error Correcting Coding for a Non-symmetric Ternary Channel
Creators: name: Bitouze, Nicolas
name: Amat, Alexandre Graell i
name: Rosnes, Eirik
Publisher: name: arXiv
Year: 2009
Subjects: subject: Information Theory (cs.IT)
subject: FOS: Computer and information sciences

description: Ternary channels can be used to model the behavior of some memory devices, where information is stored in three different levels. In this paper, error correcting coding for a ternary channel where some of the error transitions are not allowed, is considered. The resulting channel is non-symmetric, therefore classical linear codes are not optimal for this channel. We define the maximum-likelihood (ML) decoding rule for ternary codes over this channel and show that it is complex to compute, since it depends on the channel error probability. A simpler alternative decoding rule which depends only on code properties, called $\da$-decoding, is then proposed. It is shown that $\da$-decoding and ML decoding are equivalent, i.e., $\da$-decoding is optimal, under certain conditions. Assuming $\da$-decoding, we characterize the error correcting capabilities of ternary codes over the non-symmetric ternary channel. We also derive an upper bound and a constructive lower bound on the size of codes, given the code length and the minimum distance. The results arising from the constructive lower bound are then compared, for short sizes, to optimal codes (in terms of code size) found by a clique-based search. It is shown that the proposed construction method gives good codes, and that in some cases the codes are optimal.
description: Submitted to IEEE Transactions on Information Theory. Part of this work was presented at the Information Theory and Applications Workshop 2009
title: Improvisational Computational Storytelling in Open Worlds
Creators: name: Martin, Lara J.
name: Harrison, Brent
name: Riedl, Mark O.
Publisher: name: Springer Nature
Year: 2016
Subjects: subject: Intelligent narrative technologies
subject: Brave new ideas
subject: Interactive narrative
subject: Computational improvisation

description: International Conference on Interactive Digital Storytelling
description: Improvisational storytelling involves one or more people interacting in real-time to create a story without advanced notice of topic or theme. Human improvisation occurs in an open-world that can be in any state and characters can perform any behaviors expressible through natural language. We propose the grand challenge of computational improvisational storytelling in open-world domains. The goal is to develop an intelligent agent that can sensibly co-create a story with one or more humans through natural language. We lay out some of the research challenges and propose two agent architectures that can provide the basis for exploring the research issues surrounding open-world human-agent interactions.
Additional file 1 of Bronchoscopy in the post-acute phase of COVID-19: an observational study
Creators: name: Mondoni, Michele
name: Rinaldo, Rocco Francesco
name: Cefalo, Jacopo
name: Saderi, Laura
name: Vigo, Beatrice
name: Carlucci, Paolo
name: Tirelli, Claudio
name: Cariboni, Umberto
name: Santus, Pierachille
name: Centanni, Stefano
name: Sotgiu, Giovanni
Publisher: name: figshare
Year: 2023
Subjects: subject: Space Science
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: Cancer
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Supplementary Material 1
Comparative study on the thermoelectric effect of parent oxypnictides La$T$AsO ($T$ = Fe, Ni)
Creators: name: Tao, Qian
name: Zhu, Zengwei
name: Lin, Xiao
name: Cao, Guanghan
name: Xu, Zhu-an
name: Chen, Genfu
name: Luo, Jianlin
name: Wang, Nanlin
Publisher: name: arXiv
Year: 2010
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: The thermopower and Nernst effect were investigated for undoped parent compounds LaFeAsO and LaNiAsO. Both thermopower and Nernst signal in iron-based LaFeAsO are significantly larger than those in nickel-based LaNiAsO. Furthermore, abrupt changes in both thermopower and Nernst effect are observed below the structural phase transition temperature and spin-density wave (SDW) type antiferromagnetic (AFM) order temperature in Fe-based LaFeAsO. On the other hand, Nernst effect is very small in the Ni-based LaNiAsO and it is weakly temperature-dependent, reminiscent of the case in normal metals. We suggest that the effect of SDW order on the spin scattering rate should play an important role in the anomalous temperature dependence of Hall effect and Nernst effect in LaFeAsO. The contrast behavior between the LaFeAsO and LaNiAsO systems implies that the LaFeAsO system is fundamentally different from the LaNiAsO system and this may provide clues to the mechanism of high $T_c$ superconductivity in the Fe-based systems.
description: 6 pages, 6 figures
Measurements of Charmless Hadronic b->s Penguin Decays in the pi+pi-K+pi- Final State and First Observation of B0 -> rho0K+pi-
Creators: name: Belle Collaboration
name: Kyeong, S. -H.
name: Kwon, Y. -J.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: We report measurements of charmless hadronic B^0 decays into the pi+pi-K+pi+ final state. The analysis uses a sample of 657x10^6 BBbar pairs collected with the Belle detector at the KEKB asymmetric-energy e+e- collider at the Y(4S) resonance. The decay B^0 -> rho0 Kpi is observed for the first time; the significance is 5.0sigma and the corresponding partial branching fraction for M_Kpi in (0.75,1.20) GeV/c^2 is [2.8 +- 0.5(stat) +-0.5(syst)] x 10^{-6}. We also obtain the first evidence for B^0 -> f0Kpi with 3.5sigma significance and for B^0 -> pi+pi-K*0 with 4.5sigma significance. For the two-body decays B^0 -> rho0K*0 and B^0 -> f0K*0, the significances are 2.7sigma and 2.5sigma, respectively, and the upper limits on the branching fractions are 3.4x10^{-6} and 2.2x10^{-6} at 90% confidence level.
description: 6 pages, 3 figures. accepted by PRD(RC)
Direct characterization of and search for gas giant exoplanets with near-infrared long-baseline interferometry
Creators: name: Kammerer, Jens
name: Team, The ExoGRAVITY
Publisher: name: Zenodo
Year: 2022

description: Understanding the formation of gas giant planets is a major goal of contemporary exoplanet science since these planets are believed to dominate the architecture and evolution of planetary systems. A detailed characterization of an extrasolar planet requires the combination of multiple techniques exposing its physical and orbital parameters, its atmospheric composition, and its dynamical interaction with the circumstellar environment. Near-infrared long-baseline interferometry with VLTI/GRAVITY has proven its ability to directly image already known gas giant exoplanets and contribute micro-arcsecond astrometry and medium-resolution K-band spectra toward the comprehensive characterization of these objects. Furthermore, GRAVITY demonstrated the first direct detection of exoplanets whose existence was predicted from radial velocity and Gaia measurements, heralding a new era for direct imaging of exoplanets where planet searches are no longer blind, but target systems with radial velocity or astrometric trends to maximize the survey efficiency. We present our study of the HD 206893 debris disk system, a clone of the archetypical beta Pictoris system, hosting the reddest known sub-stellar companion HD 206893 B. Using GRAVITY spectra and astrometry, we derive a super-solar C/O ratio and a mass close to the boundary between exoplanets and brown dwarfs. By combining our data with spectra from the literature, we find that its unusually red color is likely caused by a layer of sub-micron sized dust particles in its upper atmosphere, and future JWST observations (PI Kammerer) are required to constrain the size distribution of these particles. Finally, we illustrate our search for an additional planet in the HD 206893 system whose existence has been predicted from indirect techniques and highlight how GRAVITY observations of multi-planet systems can yield unprecedented constraints on planet masses, ages, and therefore formation scenarios.
Deconfinement, Monopoles and New Phenomena in Heavy Ion Collisions
Creators: name: Shuryak, Edward
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We discuss various manifestations of the "magnetic scenario" for the quark-gluon plasma viewed as a mixture of two plasmas, of electrically (quark and gluons) as well as magnetically charged quasiparticles. Near the deconfinement phase transition, $T\approx T_c$ very small density of free quarks should lead to negligible screening of electric field while magnetic screening remains strong. The consequence of this should be existence of a "corona" of the QGP, in a way similar to that of the Sun, in which electric fields influence propagation of perturbations and even form metastable flux tubes. The natural tool for its description is (dual) magnetohydrodynamics: among observable consequences is splitting of sound into two modes, with larger and smaller velocity. The latter can be zero, hinting for formation of pressure-stabilized flux tubes. Remarkably, recent experimental discoveries at RHIC show effects similar to expected for "corona structures". In dihadron correlation function with large-$p_t$ trigger there are a "cone" and a "hard ridge",while the so called "soft ridge" is a similar structure seen without hard trigger. They seem to be remnants of flux tubes, which -- contrary to naive expectations -- seem to break less often in near-$T_c$ matter than do confining strings in vacuum.
description: Written version of talk given at "Shifmania" conference, June 2009, Minneapolis, related to 60-the birthday of Misha Shifman
Additional file 1 of Post-neoadjuvant treatment pancreatic cancer resectability and outcome prediction using CT, 18F-FDG PET/MRI and CA 19–9
Creators: name: Yoo, Jeongin
name: Lee, Jeong Min
name: Joo, Ijin
name: Lee, Dong Ho
name: Yoon, Jeong Hee
name: Yu, Mi Hye
name: Jang, Jin-Young
name: Lee, Sang Hyub
Publisher: name: figshare
Year: 2023
Subjects: subject: Medicine
subject: Cell Biology
subject: Neuroscience
subject: Immunology
subject: FOS: Clinical medicine
subject: Cancer

description: Additional file 1: Supplementary Material 1. Neoadjuvant chemoradiation therapy reference. Supplementary Material 2. CT scanners and imaging protocol. Supplementary Material 3. PET/MRI protocol. Supplementary Material 4. Post-NAT CT criteria for R0 resection. Supplementary Material 5. Interobserver agreement for resectability.
title: ÐÑÐ¸Ð½ÑÐ¸Ð¿ Ð¿Ð¾Ð´Ð¾Ð±Ð¸Ñ Ð² ÑÐ¸ÑÑÐµÐ¼Ð½Ð¾Ð¼ Ð°Ð½Ð°Ð»Ð¸Ð·Ðµ ÑÐ²Ð¾Ð»ÑÑÐ¸Ð¸ Ð±Ð¾Ð»ÑÑÐ¸Ñ ÑÐ¸ÑÑÐµÐ¼
title: He similarity principle in systems analysis evolution of large systems
Creators: name: ÐÐ¾Ð³Ð¾Ð¼Ð¾Ð»Ð¾Ð², ÐÐ»ÐµÐºÑÐ°Ð½Ð´Ñ
name: ÐÐµÐ²ÐµÐ¶Ð¸Ð½, ÐÐ¸ÐºÑÐ¾Ñ
name: "Ð¡Ð¸ÑÑÐµÐ¼Ð½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· Ð² Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ð¸ Ð¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ð¸", Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½Ð°Ñ Ð½Ð°ÑÑÐ½Ð°Ñ Ð¸ ÑÑÐµÐ±Ð½Ð¾-Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ°Ñ ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ñ (25; 2021; Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³)
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2021
Subjects: Ð¡Ð¸ÑÑÐµÐ¼Ð½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð·
ÐÐ¾Ð´Ð¾Ð±Ð¸Ñ ÑÐµÐ¾ÑÐ¸Ñ
ÐÑÐµÐ»ÐµÐ½Ð½Ð°Ñ
ÑÑÐ¼Ð½Ð°Ñ ÑÐ½ÐµÑÐ³Ð¸Ñ
Ð§ÐµÐ»Ð¾Ð²ÐµÐº
Ð½Ð¾Ð¾ÑÑÐµÑÐ°

description: ÐÑÐµÐ´Ð»Ð°Ð³Ð°ÐµÑÑÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°ÑÑ Ð¿ÑÐ¸Ð½ÑÐ¸Ð¿ Ð¿Ð¾Ð´Ð¾Ð±Ð¸Ñ Ð² ÑÐ¸ÑÑÐµÐ¼Ð½Ð¾Ð¼ Ð°Ð½Ð°Ð»Ð¸Ð·Ðµ Ð±Ð¾Ð»ÑÑÐ¸Ñ ÑÐ¸ÑÑÐµÐ¼ Ð´Ð»Ñ Ð²ÑÐ´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ñ Ð³Ð¸Ð¿Ð¾ÑÐµÐ· Ð¾Ð± Ð¸Ñ ÑÑÑÑÐºÑÑÑÐµ, ÑÐ²Ð¾Ð¹ÑÑÐ²Ð°Ñ Ð¸ ÑÐ²Ð¾Ð»ÑÑÐ¸Ñ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ Ð°Ð½Ð°Ð»Ð¾Ð³Ð¸Ð¸ Ñ Ð¿Ð¾ÑÐ¾Ð¶Ð¸Ð¼Ð¸ Ð½Ð° Ð½Ð¸Ñ, Ð½Ð¾ Ð±Ð¾Ð»ÐµÐµ Ð´Ð¾ÑÑÑÐ¿Ð½ÑÐ¼Ð¸ Ð´Ð»Ñ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð´ÑÑÐ³Ð¸Ð¼Ð¸ ÑÐ¸ÑÑÐµÐ¼Ð°Ð¼Ð¸. Ð ÐºÐ°ÑÐµÑÑÐ²Ðµ Ð¿ÑÐ¸Ð¼ÐµÑÐ° Ð±Ð¾Ð»ÑÑÐ¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÐµÑÑÑ Ð½Ð°ÑÐ° ÐÑÐµÐ»ÐµÐ½Ð½Ð°Ñ, Ð¿ÑÐ¾Ð¸ÑÑÐ¾Ð¶Ð´ÐµÐ½Ð¸Ðµ, ÑÐ²Ð¾Ð¹ÑÑÐ²Ð° Ð¸ ÑÐ²Ð¾Ð»ÑÑÐ¸Ñ ÐºÐ¾ÑÐ¾ÑÐ¾Ð¹, Ð½ÐµÑÐ¼Ð¾ÑÑÑ Ð½Ð° ÑÑÐ¿ÐµÑÐ¸ Ð² ÐµÑ Ð¸Ð·ÑÑÐµÐ½Ð¸Ð¸ Ð°ÑÑÑÐ¾Ð½Ð¾Ð¼Ð¸ÐµÐ¹ Ð¸ ÐºÐ¾ÑÐ¼Ð¾Ð»Ð¾Ð³Ð¸ÐµÐ¹, Ð¾ÑÑÐ°ÑÑÑÑ Ð½ÐµÑÑÐ½ÑÐ¼Ð¸. ÐÑÐ¾Ð²Ð¾Ð´Ð¸ÑÑÑ Ð°Ð½Ð°Ð»Ð¾Ð³Ð¸Ñ Ð¼ÐµÐ¶Ð´Ñ ÐÑÐµÐ»ÐµÐ½Ð½Ð¾Ð¹ Ð¸ Ð§ÐµÐ»Ð¾Ð²ÐµÐºÐ¾Ð¼, ÐºÐ¾ÑÐ¾ÑÐ¾Ð³Ð¾ Ð¼Ð¾Ð¶Ð½Ð¾ ÑÐ°ÐºÐ¶Ðµ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑ ÑÐ¾Ð¶Ðµ ÐºÐ°Ðº Ð±Ð¾Ð»ÑÑÑÑ ÑÐ¸ÑÑÐµÐ¼Ñ. ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ð¸ Ð¿ÑÐ¸Ð½ÑÐ¸Ð¿Ð° Ð¿Ð¾Ð´Ð¾Ð±Ð¸Ñ Ð²ÑÐ´Ð²Ð¸Ð³Ð°ÐµÑÑÑ ÑÑÐ´ Ð³Ð¸Ð¿Ð¾ÑÐµÐ· Ð¾ Ð¿ÑÐ¾Ð¸ÑÑÐ¾Ð¶Ð´ÐµÐ½Ð¸Ð¸ Ð¸ ÑÐ²Ð¾Ð»ÑÑÐ¸Ð¸ Ð½Ð°ÑÐµÐ¹ ÐÑÐµÐ»ÐµÐ½Ð½Ð¾Ð¹.
description: It is proposed to use the similarity principle in system analysis of large systems to hypothesize their structure, properties and evolution based on analogy with similar, but more accessible for study other systems. As an example of a large system, our universe is considered, the origin, properties and evolution of which, despite the successes in its study by astronomy and cosmology, remain unclear. An analogy is drawn between the universe and Man, which can also be considered as a large system. On the basis of the principle of similarity, a number of hypotheses are put forward about the origin and evolution of our Universe.
Chiral Magnetic Effect and Chiral Phase Transition
Creators: name: Fu, Wei-jie
name: Liu, Yu-xin
name: Wu, Yue-liang
Publisher: name: arXiv
Year: 2010
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We study the influence of the chiral phase transition on the chiral magnetic effect. The azimuthal charge-particle correlations as functions of the temperature are calculated. It is found that there is a pronounced cusp in the correlations as the temperature reaches its critical value for the QCD phase transition. It is predicted that there will be a drastic suppression of the charge-particle correlations as the collision energy in RHIC decreases to below a critical value. We show then the azimuthal charge-particle correlations can be the signal to identify the occurrence of the QCD phase transitions in RHIC energy scan experiments.
description: 4 pages, 1 figure
title: Ð¡Ð¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ±ÑÑÐ° ÑÐ¾Ð²Ð°ÑÐ°
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¾Ð³Ð¾ÑÑÐ½, ÐÐ°Ð¹Ðº
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: ÑÐ±ÑÑÐ¾Ð²Ð°Ñ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ°
Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ±ÑÑÐ°
ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾-Ñ Ð¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½Ð°Ñ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ
Ð¾ÑÐµÐ½ÐºÐ° Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÐµÐ¹

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ ÐÐÐ Â«ÐÐ²Ð¸Ðº Ð¿ÑÐ¾ÑÐµÑÑÂ». ÐÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ðµ Ð¾ÑÑÑÐµÑÑÐ²Ð»ÑÐµÑ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ Ð¿Ð¾ ÑÐ¾Ð·Ð½Ð¸ÑÐ½Ð¾Ð¹ ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ðµ ÐºÐ¾Ð¼Ð¿ÑÑÑÐµÑÐ°Ð¼Ð¸, Ð¿ÐµÑÐ¸ÑÐµÑÐ¸Ð¹Ð½ÑÐ¼Ð¸ ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð°Ð¼Ð¸ Ðº Ð½Ð¸Ð¼ Ð¸ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½ÑÐ¼ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸ÐµÐ¼ Ð² ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÑ Ð¼Ð°Ð³Ð°Ð·Ð¸Ð½Ð°Ñ. Ð¦ÐµÐ»ÑÑ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ±ÑÑÐ° Ð¿ÑÐ¾Ð´ÑÐºÑÐ¸Ð¸ Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¿ÑÑÐµÐ¹ ÐµÐµ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ. ÐÐ°Ð´Ð°ÑÐ°Ð¼Ð¸ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾-ÑÐ¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ, Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐ±ÑÑÐ¾Ð²Ð¾Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ¸, Ð¾ÑÐµÐ½ÐºÐ° Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÐµÐ¹ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¿ÑÑÐµÐ¹ ÑÐ»ÑÑÑÐµÐ½Ð¸Ñ ÑÐ±ÑÑÐ¾Ð²Ð¾Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ¸. Ð ÑÐ¾Ð´Ðµ ÑÐ°Ð±Ð¾ÑÑ Ð±ÑÐ»Ð¸ Ð²ÑÑÐ²Ð»ÐµÐ½Ñ ÑÑÑÐµÑÑÐ²ÐµÐ½Ð½ÑÐµ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ Ð² ÑÐ±ÑÑÐ¾Ð²Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸, ÐºÐ¾ÑÐ¾ÑÑÐµ Ð½ÐµÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ Ð²Ð»Ð¸ÑÐ»Ð¸ Ð½Ð° ÑÐ°Ð±Ð¾ÑÑ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ð¸. ÐÐ»Ð°Ð³Ð¾Ð´Ð°ÑÑ Ð´Ð°Ð½Ð½Ð¾Ð¼Ñ Ð°Ð½Ð°Ð»Ð¸Ð·Ñ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑ Ð¼ÐµÑ Ð¿Ð¾ ÑÐ»ÑÑÑÐµÐ½Ð¸Ñ ÑÐ±ÑÑÐ° ÑÐ¾Ð²Ð°ÑÐ°.
D6.1 Initial Planning for Testbeds
Creators: name: Tardo, Alexandr
name: Lattuca, Domenico
name: Politis, Christos
name: Bizon Franco de Almeida, Ivo
name: Nimr, Ahmad
name: Bonfim, Roberto
name: Bednarczyk, Marek
name: Puźniakowski, Tadeusz
name: Czapiewski, Paweł
name: Cárcel, José Luis
name: Meseguer, Joan
name: Alcaide Pastrana, Carlos
name: Poikonen, Jussi
name: Bernini, Giacomo
name: Piscione, Pietro
name: Seder, Erin Elizabeth
name: Cantero, Miguel
name: Fuentes, Manuel
name: Meini, Francesco
name: Renart Espi, Javier
name: Escribano Garcia-Machin, Cristina
name: Lorfida, Chiara
name: Saur, Clemens
name: Miemietz, Till
name: Costa-Requena, Jose
name: Falcitelli, Mariano
Publisher: name: Zenodo
Year: 2021
Subjects: NG-IoT
EU-H2020
5G-IoT
Testbed

description: This deliverable focuses on the implementation plan for the iNGENIOUS use cases deployment and validation. It includes a list of required resources to be used for a proper testbeds' setup as well as a list of development and integration activities to be carried out during the project lifetime. A common methodology to keep track of system requirements verification per use case is also provided. In this deliverable use cases' implementation risks are also considered.
title: ÐÐµÐ±-ÑÐµÑÐ²Ð¸Ñ Ð´Ð»Ñ Ð¿ÑÐ±Ð»Ð¸ÐºÐ°ÑÐ¸Ð¸ Ð¿ÑÐ¾ÑÑÑÐ°Ð½ÑÑÐ²ÐµÐ½Ð½ÑÑ Ð´Ð°Ð½Ð½ÑÑ Ð°Ð½Ð°Ð»Ð¸ÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¾Ð¿ÐµÑÐ°ÑÐ¸Ð¹
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð§ÐµÐ±ÑÐºÐ¸Ð½Ð°, ÐÐ¸ÐºÑÐ¾ÑÐ¸Ñ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: GeoDjango
ÑÐ·ÑÐº Python
PostGIS
PostegreSQL
ÐºÐ°ÑÑÐ¾Ð³ÑÐ°ÑÐ¸ÑÐµÑÐºÐ¸Ð¹ Ð²ÐµÐ±-ÑÐµÑÐ²Ð¸Ñ
Google Maps JavaScript API

description: ÐÐºÑÑÐ°Ð»ÑÐ½Ð¾ÑÑÑ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ Ð¾Ð±ÑÑÐ»Ð¾Ð²Ð»ÐµÐ½Ð° Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼Ð¾ÑÑÑÑ Ð¾ÑÐ¾Ð±ÑÐ°Ð¶ÐµÐ½Ð¸ÐµÐ¼ Ð¾Ð±ÑÐµÐºÑÐ¾Ð² Ð¸ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¾Ð¹ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¸ Ñ Ð½Ð¸Ñ Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ Ð°Ð½Ð°Ð»Ð¸ÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¾Ð¿ÐµÑÐ°ÑÐ¸Ð¹. ÐÑÐ¸Ð»Ð¾Ð¶ÐµÐ½Ð¸Ðµ Ð¿ÑÐµÐ´Ð¾ÑÑÐ°Ð²Ð»ÑÐµÑ ÑÐµÐ·ÑÐ»ÑÑÐ°Ñ Ð²ÑÑÐ¸ÑÐ»ÐµÐ½Ð¸Ð¹ Ð² Ð³ÑÐ°ÑÐ¸ÑÐµÑÐºÐ¾Ð¹ Ð¸ ÑÐ°Ð±Ð»Ð¸ÑÐ½Ð¾Ð¹ ÑÐ¾ÑÐ¼Ðµ Ñ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÑÑ Ð·Ð°Ð³ÑÑÐ·ÐºÐ¸ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¾Ð². ÐÐµÑÐ¾Ð´Ñ, Ð¸ÑÐ¿Ð¾Ð»ÑÐ·ÑÐµÐ¼ÑÐµ Ð² ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐµ: ÐºÐ»Ð¸ÐµÐ½Ñ-ÑÐµÑÐ²ÐµÑÐ½Ð¾Ðµ Ð¿ÑÐ¸Ð»Ð¾Ð¶ÐµÐ½Ð¸Ðµ, ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ñ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ Ð³ÐµÐ¾Ð³ÑÐ°ÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½ÑÑ ÑÐ¸ÑÑÐµÐ¼, Ð¾Ð±ÑÐµÐºÑÐ½Ð¾-ÑÐµÐ»ÑÑÐ¸Ð¾Ð½Ð½Ð¾Ðµ Ð¾ÑÐ¾Ð±ÑÐ°Ð¶ÐµÐ½Ð¸Ðµ, ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ñ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð²ÐµÐ±-Ð¿ÑÐ¸Ð»Ð¾Ð¶ÐµÐ½Ð¸Ð¹ Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ ÑÑÐµÐ¹Ð¼Ð²Ð¾ÑÐºÐ° Django. ÐÑÐ¸Ð»Ð¾Ð¶ÐµÐ½Ð¸Ðµ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÑÐµÑ ÑÐ¾Ð±Ð¾Ð¹ Ð³ÐµÐ¾Ð³ÑÐ°ÑÐ¸ÑÐµÑÐºÑÑ ÐºÐ°ÑÑÑ Ð¼Ð¸ÑÐ° Ñ Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÐ°Ð¼Ð¸ Ð´Ð»Ñ ÑÐµÐ´Ð°ÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ,ÑÐ¾ÑÑÐ°Ð½ÐµÐ½Ð¸Ñ, ÑÐºÐ°ÑÐ¸Ð²Ð°Ð½Ð¸Ñ Ð¸ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ Ð°Ð½Ð°Ð»Ð¸ÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¾Ð¿ÐµÑÐ°ÑÐ¸Ð¹.
Orion: a prova di avaria
Creators: Davide Coero Borga
Publisher: name: Media Inaf
Year: 2015

Primo test “truccato” per la capsula Orion Deep Space. La NASA, e Lockheed Martin prime contractor, vogliono evitare ogni genere di inconveniente per arrivare pronti al primo test di volo con Space Launch System (2018) e inscenano un'avaria al sistema di paracadute
Additional file 1 of Effect of an educational intervention on the knowledge, attitudes, and practices of healthcare workers at King Hussein Cancer Center towards predatory publishers
Creators: name: Al-Ani, Abdallah
name: Al-Huneidy, Leen
name: Sultan, Hala
name: Iqneibi, Shahad
name: Nazzal, Jamil
name: Mansour, Asem
name: Al-Hussaini, Maysa
Publisher: name: figshare
Year: 2023
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy

description: Additional file 1.
Viscoelastic Properties of Crystals
Creators: name: Williams, Stephen R.
name: Evans, Denis J.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: We examine the question of whether fluids and crystals are differentiated on the basis of their zero frequency shear moduli or their limiting zero frequency shear viscosity. We show that while fluids, in contrast with crystals, do have a zero value for their shear modulus, in contradiction to a widespread presumption, a crystal does not have an infinite or exceedingly large value for its limiting zero frequency shear viscosity. In fact, while the limiting shear viscosity of a crystal is much larger than that of the liquid from which it is formed, its viscosity is much less than that of the corresponding glass that may form assuming the liquid is a good enough glass former.
description: 13 pages, 3 figures
Occhio digitale da record: 3.2 miliardi di pixel
Creators: Marco Malaspina
Publisher: name: Media Inaf
Year: 2015

Approvato il progetto per la realizzazione della macchina fotografica con rivelatore a più alta definizione mai costruito: oltre tre miliardi di pixel. Dovrebbe entrare in funzione dal 2022 sul Large Synoptic Survey Telescope, in Cile, e permetterà agli astronomi di redigere in dieci anni un catalogo d'oggetti celesti senza precedenti
Early-type galaxies in the PEARS survey: Probing the stellar populations at moderate redshift
Creators: name: Ferreras, Ignacio
name: Pasquali, Anna
name: Malhotra, Sangeeta
name: Rhoads, James
name: Cohen, Seth
name: Windhorst, Rogier
name: Pirzkal, Nor
name: Grogin, Norman
name: Koekemoer, Anton M.
name: Lisker, Thorsten
name: Panagia, Nino
name: Daddi, Emanuele
name: Hathi, Nimish P.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Using HST/ACS slitless grism spectra from the PEARS program, we study the stellar populations of morphologically selected early-type galaxies in the GOODS North and South fields. The sample - extracted from a visual classification of the (v2.0) HST/ACS images and restricted to redshifts z>0.4 - comprises 228 galaxies (F775W<24 ABmag) out to z~1.3 over 320 arcmin2, with a median redshift zM=0.75. This work significantly increases our previous sample from the GRAPES survey in the HUDF (18 galaxies over ~11 arcmin2; Pasquali et al. 2006b). The grism data allow us to separate the sample into `red' and `blue' spectra, with the latter comprising 15% of the total. Three different grids of models parameterising the star formation history are used to fit the low-resolution spectra. Over the redshift range of the sample - corresponding to a cosmic age between 5 and 10 Gyr - we find a strong correlation between stellar mass and average age, whereas the **spread** of ages (defined by the RMS of the distribution) is roughly ~1 Gyr and independent of stellar mass. The best-fit parameters suggest it is formation epoch and not formation timescale, that best correlates with mass in early-type galaxies. This result - along with the recently observed lack of evolution of the number density of massive galaxies - motivates the need for a channel of (massive) galaxy formation bypassing any phase in the blue cloud, as suggested by the simulations of Dekel et al. (2009).
description: 12 pages, 12 figures, 3 tables. Submitted for publication in ApJ
Are the spin axes of stars randomly aligned within a cluster?
Creators: name: Jackson, R. J.
name: Jeffries, R. D.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We investigate to what extent the spin axes of stars in young open clusters are aligned. Assuming that the spin vectors lie uniformly within a conical section, with an opening half-angle between lambda=0 (perfectly aligned) and lambda=90 degrees(completely random), we describe a Monte-Carlo modelling technique that returns a probability density for this opening angle given a set of measured sin i values, where i is the unknown inclination angle between a stellar spin vector and the line of sight. Using simulations we demonstrate that although azimuthal information is lost, it is easily possible to discriminate between strongly aligned spin axes and a random distribution, providing that the mean spin-axis inclination lies outside the range 45--75 degrees. We apply the technique to G- and K-type stars in the young Pleiades and Alpha Per clusters. The sin i values are derived using rotation periods and projected equatorial velocities, combined with radii estimated from the cluster distances and a surface brightness/colour relationship. For both clusters we find no evidence for spin-axis alignment: lambda=90 degrees is the most probable model and lambda>40 degrees with 90 per cent confidence. Assuming a random spin-axis alignment, we re-determine the distances to both clusters, obtaining 133+/-7pc for the Pleiades and 182+/-11 pc for Alpha Per. If the assumption of random spin-axis alignment is discarded however, whilst the distance estimate remains unchanged, it has an additional +18/-32 percent uncertainty.
description: Accepted for publication in MNRAS
Il bosone di Higgs si assomiglia
Creators: Enrica Battifoglia
Publisher: name: Media Inaf
Year: 2015

Un nuovo e più preciso identikit del bosone di Higgs. Ad annunciarlo il CERN di Ginevra che sottolinea come il risultato indica nella particella che "ha dato vita" alla massa la forma (o almeno gli assomiglia tantissimo) prevista dalla teoria di riferimento della fisica contemporanea, il Modello Standard
Construction of totally reflexive modules from an exact pair of zero divisors
Creators: name: Holm, Henrik
Publisher: name: arXiv
Year: 2010
Subjects: subject: Commutative Algebra (math.AC)
subject: FOS: Mathematics
subject: 13C13; 13H99

description: Let A be a local ring which admits an exact pair x,y of zero divisors as defined by Henriques and Sega. Assuming that this pair is regular and that there exists a regular element on the A-module A/(x,y), we explicitly construct an infinite family of non-isomorphic indecomposable totally reflexive A-modules. In this setting, our construction provides an answer to a question raised by Christensen, Piepmeyer, Striuli, and Takahashi. Furthermore, we compute the module of homomorphisms between any two given modules from the infinite family mentioned above.
description: 15 pages
title: Ð¢ÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð¿ÑÐ¾ÑÐµÑÑ Ð¸Ð·Ð³Ð¾ÑÐ¾Ð²Ð»ÐµÐ½Ð¸Ñ Ð´ÐµÑÐ°Ð»Ð¸ Â«ÐÑÑÐ»ÐºÐ°Â»
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ°Ð»Ð¸ÑÑÐ½, ÐÑÑÐµÐ¼
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð¿ÑÐ¾ÑÐµÑÑ
ÑÑÐ°Ð½Ð¾Ðº
Ð¿ÐµÑÐµÑ Ð¾Ð´
ÑÐµÐ·ÐµÑ

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐ½Ð¾ÑÑÐ¸ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¸ Ð´ÐµÑÐ°Ð»Ð¸, Ð²ÑÐ±ÑÐ°Ð½ Ð¼ÐµÑÐ¾Ð´ Ð¿Ð¾Ð»ÑÑÐµÐ½Ð¸Ñ Ð¸ÑÑÐ¾Ð´Ð½Ð¾Ð¹ Ð·Ð°Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸, ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð¿ÑÐ¾ÑÐµÑÑ Ð¸Ð·Ð³Ð¾ÑÐ¾Ð²Ð»ÐµÐ½Ð¸Ñ Ð´ÐµÑÐ°Ð»Ð¸, Ð²ÑÐ±ÑÐ°Ð½Ñ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¸ Ð¾ÑÐ½Ð°ÑÑÐºÐ°, ÑÐ°ÑÑÑÐ¸ÑÐ°Ð½Ñ ÑÐµÐ¶Ð¸Ð¼Ñ ÑÐµÐ·Ð°Ð½Ð¸Ñ Ð¸ Ð½Ð¾ÑÐ¼Ñ Ð²ÑÐµÐ¼ÐµÐ½Ð¸ Ð½Ð° Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ðµ Ð¾Ð¿ÐµÑÐ°ÑÐ¸Ð¹ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿ÑÐ¾ÑÐµÑÑÐ°. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ Ð¿ÑÐ¸ÑÐ¿Ð¾ÑÐ¾Ð±Ð»ÐµÐ½Ð¸Ñ: ÑÑÐ°Ð½Ð¾ÑÐ½Ð¾Ðµ Ð¸ ÐºÐ¾Ð½ÑÑÐ¾Ð»ÑÐ½Ð¾-Ð¸Ð·Ð¼ÐµÑÐ¸ÑÐµÐ»ÑÐ½Ð¾Ðµ.
An algorithm to obtain global solutions of the double confluent Heun equation
Creators: name: Abad, J.
name: Gomez, F. J.
name: Sesma, J.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Classical Analysis and ODEs (math.CA)
subject: FOS: Mathematics
subject: 34B30; 33E20; 34M35

description: A procedure is proposed to construct solutions of the double confluent Heun equation with a determinate behaviour at the singular points. The connection factors are expressed as quotients of Wronskians of the involved solutions. Asymptotic expansions are used in the computation of those Wronskians. The feasibility of the method is shown in an example, namely, the Schroedinger equation with a quasi-exactly-solvable potential.
title: ÐÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐºÐ°Ð·Ð°Ð½Ð¸Ñ Ð¿Ð¾ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¸ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ Ð»Ð°Ð±Ð¾ÑÐ°ÑÐ¾ÑÐ½ÑÑ ÑÐ°Ð±Ð¾Ñ Ð¿Ð¾ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ðµ Â«Ð¥Ð¸Ð¼Ð¸Ñ Ð¿Ð¸ÑÐµÐ²ÑÑ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¾Ð²Â»
title: Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ 19.03.01 "ÐÐ¸Ð¾ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ñ"; ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ñ (ÑÑÐµÐ¿ÐµÐ½Ñ) Ð²ÑÐ¿ÑÑÐºÐ½Ð¸ÐºÐ° - Ð±Ð°ÐºÐ°Ð»Ð°Ð²Ñ; ÑÐ¾ÑÐ¼Ð° Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ - Ð¾ÑÐ½Ð°Ñ, Ð¾ÑÐ½Ð¾-Ð·Ð°Ð¾ÑÐ½Ð°Ñ, Ð·Ð°Ð¾ÑÐ½Ð°Ñ
titleType: Subtitle
Creators: name: ÐÐ°Ð¶ÐµÐ½Ð¾Ð²Ð°, ÐÑÐ¸Ð½Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2020
Subjects: Ð¥Ð¸Ð¼Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð°Ð½Ð°Ð»Ð¸Ð·
Ð¿Ð¸ÑÐµÐ²ÑÐµ Ð¿ÑÐ¾Ð´ÑÐºÑÑ
Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐºÐ°Ð·Ð°Ð½Ð¸Ñ
Ð»Ð°Ð±Ð¾ÑÐ°ÑÐ¾ÑÐ½ÑÐµ ÑÐ°Ð±Ð¾ÑÑ

description: ÐÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐºÐ°Ð·Ð°Ð½Ð¸Ñ Ð¿Ð¾ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¸ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ Ð»Ð°Ð±Ð¾ÑÐ°ÑÐ¾ÑÐ½ÑÑ ÑÐ°Ð±Ð¾Ñ Ð¿Ð¾ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ðµ Â«Ð¥Ð¸Ð¼Ð¸Ñ Ð¿Ð¸ÑÐµÐ²ÑÑ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¾Ð²Â» ÑÐ¾ÑÑÐ°Ð²Ð»ÐµÐ½Ñ Ð² ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²Ð¸Ð¸ Ñ ÑÑÐµÐ±Ð½ÑÐ¼ Ð¿Ð»Ð°Ð½Ð¾Ð¼ Ð¸ ÑÐ°Ð±Ð¾ÑÐµÐ¹ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð¾Ð¹ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ñ Â«Ð¥Ð¸Ð¼Ð¸Ñ Ð¿Ð¸ÑÐµÐ²ÑÑ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¾Ð²Â» Ð¸ Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ñ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð²ÑÐµÑ ÑÐ¾ÑÐ¼ Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸ÑÐ¼ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð£ÐÐ¡Ð 19.00.00 Â«ÐÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½Ð°Ñ ÑÐºÐ¾Ð»Ð¾Ð³Ð¸Ñ Ð¸ Ð±Ð¸Ð¾ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÂ».
ÐÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐºÐ°Ð·Ð°Ð½Ð¸Ñ ÑÐ¾Ð´ÐµÑÐ¶Ð°Ñ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ðº Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ Ð»Ð°Ð±Ð¾ÑÐ°ÑÐ¾ÑÐ½ÑÑ ÑÐ°Ð±Ð¾Ñ, ÑÐ¿ÑÐ°Ð²Ð¾ÑÐ½ÑÐµ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ñ, Ð²Ð¾Ð¿ÑÐ¾ÑÑ Ð´Ð»Ñ ÑÐ°Ð¼Ð¾ÐºÐ¾Ð½ÑÑÐ¾Ð»Ñ, ÑÐ¿Ð¸ÑÐ¾Ðº ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´ÑÐµÐ¼Ð¾Ð¹ Ð»Ð¸ÑÐµÑÐ°ÑÑÑÑ.
ÐÐ°ÑÑÐ¾ÑÑÐ¸Ðµ ÐÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐºÐ°Ð·Ð°Ð½Ð¸Ñ Ð¼Ð¾Ð³ÑÑ Ð±ÑÑÑ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð¾Ð²Ð°Ð½Ñ Ð¿ÑÐ¸ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ð¸ ÐºÑÑÑÐ¾Ð²ÑÑ, Ð½Ð°ÑÑÐ½ÑÑ Ð¸ Ð²ÑÐ¿ÑÑÐºÐ½ÑÑ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½ÑÑ ÑÐ°Ð±Ð¾Ñ.
Eclissi di superluna in arrivo
Creators: Marco Galliani
Publisher: name: Media Inaf
Year: 2015

Questo mese, occhi all’insù per seguire l’eclissi totale di Luna, che sarà visibile anche dall'Italia. L’appuntamento è fissato, nuvole permettendo, per le prime ore del 28, giorno in cui il nostro satellite naturale si troverà anche alla distanza minima dalla Terra, apparendoci anche un po' più grande del solito
Additional file 2 of Effect of an educational intervention on the knowledge, attitudes, and practices of healthcare workers at King Hussein Cancer Center towards predatory publishers
Creators: name: Al-Ani, Abdallah
name: Al-Huneidy, Leen
name: Sultan, Hala
name: Iqneibi, Shahad
name: Nazzal, Jamil
name: Mansour, Asem
name: Al-Hussaini, Maysa
Publisher: name: figshare
Year: 2023
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy

description: Additional file 2.
Housing conditions in relation to child protection : a descriptive examination of significant family cases from the Children's Aid Society and the City Social Service Department, Vancouver, 1956
Creators: name: Daggett, Jessie Catherine
Publisher: name: University of British Columbia
Year: 2012

description: There are many reasons for child neglect, and many variables in the family circumstances from which the need for child protection or removal arises; but in recent years bad housing has not been given the prominence it demands. Improvements in institutions, new treatment centres, modern school facilities, point up the contrast, when bad housing and demoralizing neighbourhoods place heavy burdens on marginal families, and handicap social services which attempt to be restorative. To gain some perspective on family conditions associated with protection cases, active or potential, a small group of examples were chosen for detailed study; four from the Children's Aid Society and four from the City Social Service Department, Vancouver. All live in a semi-industrialized slum area, where there is general deterioration, and the housing is inadequate. Each family has an average of five children, ranging in age from one to sixteen years. Three of the families live in rented suites, and five in rented houses. Both parents are in the home, in all but two of the families. The information for the study was obtained from personal interviews with the families, from agency case records, discussions with the social workers to whom the families are presently known. The resulting "word pictures" portray the home life and social environment, having special reference to child neglect and substandard family life. The various aspects of family life are described with special emphasis on the families' present housing conditions, their previous accommodation, economic status, the neighbourhood, the general health of the family, and their attitude in regard to present housing conditions. This is followed by an assessment of the strengths and weaknesses of the families, their interests and activities, the children's progress at school, and the use made of social services in the community. A major implication of the study is that more adequate low-rent housing is urgently needed, particularly for families with a large number of children. If the parents, and especially the children, are to benefit fully from the educational, health and welfare services of the community, a good home which is a basic need, must be provided or made available. It is hoped that this study will serve as an introduction for further research into family living conditions, of more thorough examination of the influences which bear on children in neglected homes and neighbourhoods, as part of the process of creating a sound base from which social services can operate.
Rotation in relativity and the propagation of light
Creators: name: Kajari, E.
name: Buser, M.
name: Feiler, C.
name: Schleich, W. P.
Publisher: name: arXiv
Year: 2009
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We compare and contrast the different points of view of rotation in general relativity, put forward by Mach, Thirring and Lense, and Goedel. Our analysis relies on two tools: (i) the Sagnac effect which allows us to measure rotations of a coordinate system or induced by the curvature of spacetime, and (ii) computer visualizations which bring out the alien features of the Goedel Universe. In order to keep the paper self-contained, we summarize in several appendices crucial ingredients of the mathematical tools used in general relativity. In this way, our lecture notes should be accessible to researchers familiar with the basic elements of tensor calculus and general relativity.
description: 102 pages, 35 figures, The original publication is available at http://www.sif.it/SIF/en/portal/journals.html, to appear in "Atom Optics and Space Physics", Proceedings of the International School of Physics "Enrico Fermi", Course CLXVIII, edited by E. Arimondo, W. Ertmer, E. M. Rasel and W. P. Schleich, (IOS Press, Amsterdam) 2009
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¿Ð»Ð°Ð½Ð° Ð³ÑÐ°Ð¶Ð´Ð°Ð½ÑÐºÐ¾Ð¹ Ð¾Ð±Ð¾ÑÐ¾Ð½Ñ Ð¸ Ð·Ð°ÑÐ¸ÑÑ ÑÑÐµÐ·Ð²ÑÑÐ°Ð¹Ð½ÑÑ ÑÐ¸ÑÑÐ°ÑÐ¸ÑÑ Ð½Ð° ÑÐµÐ»ÑÑÐºÐ¾Ð¼ Ð¿Ð¾ÑÐµÐ»ÐµÐ½Ð¸Ð¸
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð£Ð¼Ð°ÑÐ¾Ð², ÐÐ»Ð¸Ð¼Ð¿Ð°ÑÐ°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: ÑÐµÐ»ÑÑÐºÐ¾Ðµ Ð¿Ð¾ÑÐµÐ»ÐµÐ½Ð¸Ðµ
ÑÑÐµÐ·Ð²ÑÑÐ°Ð¹Ð½Ð°Ñ ÑÐ¸ÑÑÐ°ÑÐ¸Ñ
Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹ Ð³ÑÐ°Ð¶Ð´Ð°Ð½ÑÐºÐ¾Ð¹ Ð¾Ð±Ð¾ÑÐ¾Ð½Ñ

description: ÐÐ¾ Ð²Ð²ÐµÐ´ÐµÐ½Ð¸Ð¸ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð° Ð°ÐºÑÑÐ°Ð»ÑÐ½Ð¾ÑÑÑ ÑÐµÐ¼Ñ, Ð¿Ð¾ÑÑÐ°Ð²Ð»ÐµÐ½Ð° ÑÐµÐ»Ñ Ð¸ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½ Ð¾Ð±ÑÐµÐºÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ. Ð Ð¿ÐµÑÐ²Ð¾Ð¹ Ð³Ð»Ð°Ð²Ðµ Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ° ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ»Ð¸ Ð³ÑÐ°Ð¶Ð´Ð°Ð½ÑÐºÑÑ Ð¾Ð±Ð¾ÑÐ¾Ð½Ñ, Ð·Ð°ÑÐ¸ÑÐ° Ð² Ð§Ð¡ ÑÐµÐ»ÑÑÐºÐ¸Ñ Ð¿Ð¾ÑÐµÐ»ÐµÐ½Ð¸Ð¹. ÐÐ¾ Ð²ÑÐ¾ÑÐ¾Ð¹ Ð³Ð»Ð°Ð²Ðµ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ»Ð¸ Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹ Ð¿Ð¾ Ð³ÑÐ°Ð¶Ð´Ð°Ð½ÑÐºÐ¾Ð¹ Ð¾Ð±Ð¾ÑÐ¾Ð½Ðµ Ð² ÑÐµÐ»ÑÑÐºÐ¸Ñ Ð¿Ð¾ÑÐµÐ»ÐµÐ½Ð¸ÑÑ. ÐÐ°ÐºÐ»ÑÑÐµÐ½Ð¸Ðµ ÑÐ¾Ð´ÐµÑÐ¶Ð¸Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð²ÑÐ²Ð¾Ð´Ñ Ð¿Ð¾ ÑÐ°Ð±Ð¾ÑÐµ.
Saturno non lo sa che Dione passa va
Creators: Eleonora Ferroni
Publisher: name: Media Inaf
Year: 2015

La sonda della NASA ci regala un'altra immagine della luna ghiacciata di Saturno. A ottobre Cassini volerà ancora due volte attorno alla luna Encelado per studiarne i potenti getti di ghiaccio, avvicinandosi fino a 48 chilometri nel passaggio finale
Additional file 1 of Comparing the effectiveness of asynchronous e-modules and didactic lectures to teach electrocardiogram interpretation to first year US medical students
Creators: name: Olvet, Doreen M.
name: Sadigh, Kaveh
Publisher: name: figshare
Year: 2023
Subjects: subject: Biochemistry
subject: Medicine
subject: Cell Biology
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: Supplementary Material