cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: On monotonic estimates of the norm of the minimizers of regularized quadratic functions in Krylov spaces
Creators: name: Cartis, C
name: Gould, N I M
name: Lange, M
Publisher: name: STFC
Year: 2019

description: We show that the minimizers of regularized quadratic functions restricted to their natural Krylov spaces increase in Euclidean norm as the spaces expand.
title: Stand-Alone Hemisphere-Tank Rupture in Tunnel Fire: Effect of Hydrogen Inventory on Blast Wave Strength in Far Field
Creators: name: Shentsov, V.
name: Makarov, D.
name: Dery, W.
name: International Seminar On Fire And Explosion Hazards (9; 2019; Saint Petersburg, Russia)
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: 2019

description: High-pressure hydrogen onboard storage rupture in a fire generates blast wave and fireball. These hazards
are not yet investigated enough, especially in a tunnel. Consequences of such event, e.g. a blast wave,
could be devastating depending on amount of stored hydrogen and tunnel dimensions. This raises the
question about the dependence of blast wave overpressure on hydrogen inventory in the tank. The
problem is studied here numerically. Large eddy simulation (LES) turbulence model with the eddy
dissipation concept (EDC) for combustion were employed in series of numerical simulations in three
different tunnel cross-sections with four hemispherical tank volumes at pressures of 94.5 MPa. The
dependence of blast wave overpressure on hydrogen inventory is defined. The results are conservative
and require experimental validation in tunnel tests.
Barium Stars: Theoretical Interpretation
Creators: name: Husti, L.
name: Gallino, R.
name: Bisterzo, S.
name: Straniero, O.
name: Cristallo, S.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Barium stars are extrinsic Asymptotic Giant Branch (AGB) stars. They present the s-enhancement characteristic for AGB and post-AGB stars, but are in an earlier evolutionary stage (main sequence dwarfs, subgiants, red giants). They are believed to form in binary systems, where a more massive companion evolved faster, produced the s-elements during its AGB phase, polluted the present barium star through stellar winds and became a white dwarf. The samples of barium stars of Allen & Barbuy (2006) and of Smiljanic et al. (2007) are analysed here. Spectra of both samples were obtained at high-resolution and high S/N. We compare these observations with AGB nucleosynthesis models using different initial masses and a spread of 13C-pocket efficiencies. Once a consistent solution is found for the whole elemental distribution of abundances, a proper dilution factor is applied. This dilution is explained by the fact that the s-rich material transferred from the AGB to the nowadays observed stars is mixed with the envelope of the accretor. We also analyse the mass transfer process, and obtain the wind velocity for giants and subgiants with known orbital period. We find evidence that thermohaline mixing is acting inside main sequence dwarfs and we present a method for estimating its depth.
description: 8 pages, 11 figures, 6 tables
Mining User Profiles to Support Structure and Explanation in Open Social Networking
Creators: name: Stewart, Avare
name: Diaz-Aviles, Ernesto
name: Nejdl, Wolfgang
Publisher: name: arXiv
Year: 2008
Subjects: subject: Information Retrieval (cs.IR)
subject: FOS: Computer and information sciences
subject: H.3.3; H.3.5

description: The proliferation of media sharing and social networking websites has brought with it vast collections of site-specific user generated content. The result is a Social Networking Divide in which the concepts and structure common across different sites are hidden. The knowledge and structures from one social site are not adequately exploited to provide new information and resources to the same or different users in comparable social sites. For music bloggers, this latent structure, forces bloggers to select sub-optimal blogrolls. However, by integrating the social activities of music bloggers and listeners, we are able to overcome this limitation: improving the quality of the blogroll neighborhoods, in terms of similarity, by 85 percent when using tracks and by 120 percent when integrating tags from another site.
description: International Workshop on Interacting with Multimedia Content in the Social Semantic Web (IMC-SSW 2008). Collocated with the 3rd International Conference on Semantic and Digital Media Technologies (SAMT 2008), Koblenz, Germany, Dec. 03 2008
Neutron star tidal disruption in mixed binaries: the imprint of the equation of state
Creators: name: Ferrari, V.
name: Gualtieri, L.
name: Pannarale, F.
Publisher: name: arXiv
Year: 2009
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We study the tidal disruption of neutron stars in black hole-neutron star coalescing binaries. We calculate the critical orbital separation at which the star is disrupted by the black hole tidal field for several equations of state describing the matter inside the neutron star, and for a large set of the binary parameters. When the disruption occurs before the star reaches the innermost stable circular orbit, the gravitational wave (GW) signal emitted by the system is expected to exhibit a cutoff frequency nu_GWtide, which is a distinctive feature of the waveform. We evaluate nu_GWtide and show that, if this frequency will be found in a detected gravitational wave, it will allow to determine the neutron star radius with an error of a few percent, providing valuable information on the behaviour of matter in the stellar core.
description: 11 pages, 9 figures, 3 tables; references added
title: ÐÑÐ¾ÐµÐºÑ Ð¢Ð­Ð¡ Ð¼Ð¾ÑÐ½Ð¾ÑÑÑÑ 500 ÐÐÑ Ð³. ÐÑÐ¾Ð·Ð½ÑÐ¹ Ð§ÐµÑÐµÐ½ÑÐºÐ°Ñ Ð ÐµÑÐ¿ÑÐ±Ð»Ð¸ÐºÐ°
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¾Ð»ÐµÑÑÐº, ÐÐ»ÐµÐºÑÐ°Ð½Ð´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: Ð¢Ð­Ð¡
ÑÐµÐ¿Ð»Ð¾Ð²Ð°Ñ ÑÑ ÐµÐ¼Ð°
Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ
ÐºÐ¾ÑÑÐ»-ÑÑÐ¸Ð»Ð¸Ð·Ð°ÑÐ¾Ñ
Ð¿Ð°ÑÐ¾Ð²Ð°Ñ ÑÑÑÐ±Ð¸Ð½Ð°

description: Ð ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½ Ð²Ð°ÑÐ¸Ð°Ð½Ñ Ð¿ÑÐ¾ÐµÐºÑÐ° Ð¢Ð­Ð¡ Ð´Ð»Ñ Ð³. ÐÑÐ¾Ð·Ð½Ð¾Ð³Ð¾ Ð§ÐµÑÐµÐ½ÑÐºÐ¾Ð¹ Ð ÐµÑÐ¿ÑÐ±Ð»Ð¸ÐºÐ¸, Ð¸ÑÐ¿Ð¾Ð»ÑÐ·ÑÑÑÐµÐ¹ Ð¿Ð°ÑÐ¾Ð³Ð°Ð·Ð¾Ð²ÑÑ ÑÑÑÐ°Ð½Ð¾Ð²ÐºÑ Ð´Ð»Ñ Ð³ÐµÐ½ÐµÑÐ°ÑÐ¸Ð¸ ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÑÐ½ÐµÑÐ³Ð¸Ð¸. ÐÐ¾Ð´Ð¾Ð±ÑÐ°Ð½Ð¾ Ð²ÑÐ¿Ð¾Ð¼Ð¾Ð³Ð°ÑÐµÐ»ÑÐ½Ð¾Ðµ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ, Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½ ÑÐ°ÑÑÐµÑ ÐÐÐ£-Ð¢Ð­Ð¡, ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ ÑÑÐ°Ð½ÑÐ¸Ð¸. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½ Ð³ÐµÐ½ÐµÑÐ°Ð»ÑÐ½ÑÐ¹ Ð¿Ð»Ð°Ð½ Ð¢Ð­Ð¡, Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð° ÐºÐ¾Ð¼Ð¿Ð¾Ð½Ð¾Ð²ÐºÐ° Ð³Ð»Ð°Ð²Ð½Ð¾Ð³Ð¾ Ð¸ Ð²ÑÐ¿Ð¾Ð¼Ð¾Ð³Ð°ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð² Ð³Ð»Ð°Ð²Ð½Ð¾Ð¼ Ð·Ð´Ð°Ð½Ð¸Ð¸ ÑÑÐ°Ð½ÑÐ¸Ð¸.
High Fidelity Analyses of Wind Turbines Exposed to Atmospheric Turbulence
Creators: name: Th. Lutz
Publisher: name: Zenodo
Year: 2021
Subjects: wind
wind power
wind turbines
floating wind
offshore wind

description: This presentation was part of the EERA JP Wind & SETWind Annual Event 2021, in collaboration with ETIPWind (September 20 - 24, Amsterdam & online).
Cavities and shocks in the galaxy group HCG 62 as revealed by Chandra, XMM and GMRT data
Creators: name: Gitti, Myriam
name: O'Sullivan, Ewan
name: Giacintucci, Simona
name: David, Laurence P.
name: Vrtilek, Jan
name: Raychaudhury, Somak
name: Nulsen, Paul E. J.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We report on the results of an analysis of Chandra, XMM-Newton and new GMRT data of the X-ray bright compact group of galaxies HCG 62, which is one of the few groups known to possess clear, small X-ray cavities in the inner regions. This is part of an ongoing X-ray/low-frequency radio study of 18 groups, initially chosen for the availability of good-quality X-ray data and evidence for AGN/hot gas interaction. At higher frequency (1.4 GHz), the HCG 62 cavity system shows minimal if any radio emission, but the new GMRT observations at 235 MHz and 610 MHz clearly detect extended low-frequency emission from radio lobes corresponding to the cavities. By means of the synergy of X-ray and low-frequency radio observations, we compare and discuss the morphology, luminosity and pressure of the gas and of the radio source. We find that the radio source is radiatively inefficient, with a ratio of radio luminosity to mechanical cavity power of $\sim 10^{-4}$, and that the radio pressure of the lobes is about one order of magnitude lower than the X-ray pressure of the surrounding thermal gas. Thanks to the high spatial resolution of the Chandra surface brightness and temperature profiles, we also identify a shock front located at 36 kpc to the south-west of the group center, close to the southern radio lobe, with a Mach number $\sim 1.5$ and a total power which is about one order of magnitude higher than the cavity power. Such a shock may have heated the gas in the southern region, as indicated by the temperature map. The shock may also explain the arc-like region of enriched gas seen in the iron abundance map, as this may be produced by a non-Maxwellian electron distribution near its front.
description: 14 pages, 8 figures, accepted for publication in ApJ. Revised version including minor comments and expanded discussion (version with full resolution figures available at http://hea-www.harvard.edu/~mgitti/hcg62-gitti.pdf)
title: ÐÑÐµÐ½ÐºÐ° ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐÐ Â«ÐÑÑÐ³ÐµÑ Ð Ð£Ð¡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Ð¾Ð¿ÐµÐ»Ñ, ÐÐ»ÐµÐºÑÐ°Ð½Ð´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: 2018
Subjects: ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ½ÑÐµ Ð¿ÑÐµÐ¸Ð¼ÑÑÐµÑÑÐ²Ð°
ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð°Ñ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÑ
ÑÐµÐ½ÑÐ°Ð±ÐµÐ»ÑÐ½Ð¾ÑÑÑ
Ð´ÐµÐ»Ð¾Ð²Ð°Ñ Ð°ÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ
Ð±ÑÑ Ð³Ð°Ð»ÑÐµÑÑÐºÐ¸Ð¹ Ð±Ð°Ð»Ð°Ð½Ñ

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÐÐÐ Â«ÐÑÑÐ³ÐµÑ Ð ÑÑÂ».
Ð¦ÐµÐ»Ñ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°Ð½Ð°Ð»Ð¸Ð· Ð¸ Ð¾ÑÐµÐ½ÐºÐ° ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐÐ Â«ÐÑÑÐ³ÐµÑ Ð ÑÑÂ».
ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° ÑÑÐ½ÐºÐ° Ð¸ Ð¿Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ñ ÐºÐ°ÑÑÑ ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ¾Ð² Ð±ÑÐ»Ð¸ Ð²ÑÐ´ÐµÐ»ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð¸Ð³ÑÐ¾ÐºÐ¸.
ÐÑÐ»Ð° Ð¿ÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð° ÑÐ°Ð±Ð¾ÑÐ° ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ ÑÐ¾ ÑÑÐ¾ÑÐ¾Ð½Ñ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð¹ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÐ¸, Ð»Ð¸ÐºÐ²Ð¸Ð´Ð½Ð¾ÑÑÐ¸ Ð¸ Ð¿Ð»Ð°ÑÐµÐ¶ÐµÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÐ¸, Ð´ÐµÐ»Ð¾Ð²Ð¾Ð¹ Ð°ÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸, ÑÐµÐ½ÑÐ°Ð±ÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¸ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð° Ð´Ð¸Ð½Ð°Ð¼Ð¸ÐºÐ° Ð¿Ð¾ ÐºÐ°Ð¶Ð´Ð¾Ð¼Ñ Ð¸Ð· Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»ÐµÐ¹.
Ð¡Ð´ÐµÐ»Ð°Ð½ Ð¿ÑÐ¾Ð³Ð½Ð¾Ð· Ð²ÑÑÑÑÐºÐ¸ Ð¸ Ð·Ð°ÑÑÐ°Ñ Ð¾Ñ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð² Ð·Ð°Ð²Ð¸ÑÐ¸Ð¼Ð¾ÑÑÐ¸ Ð¾Ñ Ð·Ð°Ð¿ÑÑÐºÐ° Ð½Ð¾Ð²Ð¾Ð³Ð¾ Ð¿ÑÐ¾Ð´ÑÐºÑÐ°, Ð° ÑÐ°ÐºÐ¶Ðµ Ð·Ð° ÑÑÐµÑ ÑÐ¾ÐºÑÐ°ÑÐµÐ½Ð¸Ñ ÑÐ¿Ð¸ÑÐ°Ð½Ð¸Ð¹ Ð±ÑÐ°ÐºÐ°.
Predicting Fuel Consumption in Power Generation Plants using Machine Learning and Neural Networks
Creators: name: Nguegnang, Gabin Maxime
name: Atemkeng, Marcellin
name: Ansah-Narh, Theophilus
name: Rockefeller, Rockefeller
name: Nguegnang, Gabin Maxime
name: Garuti, Marco Andrea
Publisher: name: arXiv
Year: 2022
Subjects: subject: Machine Learning (cs.LG)
subject: FOS: Computer and information sciences

description: The instability of power generation from national grids has led industries (e.g., telecommunication) to rely on plant generators to run their businesses. However, these secondary generators create additional challenges such as fuel leakages in and out of the system and perturbations in the fuel level gauges. Consequently, telecommunication operators have been involved in a constant need for fuel to supply diesel generators. With the increase in fuel prices due to socio-economic factors, excessive fuel consumption and fuel pilferage become a problem, and this affects the smooth run of the network companies. In this work, we compared four machine learning algorithms (i.e. Gradient Boosting, Random Forest, Neural Network, and Lasso) to predict the amount of fuel consumed by a power generation plant. After evaluating the predictive accuracy of these models, the Gradient Boosting model out-perform the other three regressor models with the highest Nash efficiency value of 99.1%.
title: Ð¢ÐµÑÐ°Ð³ÐµÑÑÐµÐ²Ð°Ñ ÑÐºÑÐ¿ÑÐµÑÑ-Ð´Ð¸Ð°Ð³Ð½Ð¾ÑÑÐ¸ÐºÐ° ÑÐ°ÐºÐ° Ð¼Ð¾Ð»Ð¾ÑÐ½Ð¾Ð¹ Ð¶ÐµÐ»ÐµÐ·Ñ
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¼Ð°Ð³Ð¸ÑÑÑÐ°
titleType: Subtitle
Creators: name: Ð¢Ð°ÑÐ°Ð½ÐµÑ, ÐÐ¾Ð½ÑÑÐ°Ð½ÑÐ¸Ð½
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: ÐÑÐµÐ¼Ð½Ð¸Ð¹
ÐÐ°Ð½Ð¾ÑÑÑÑÐºÑÑÑÐ½ÑÐµ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ñ
Ð­Ð»ÐµÐºÑÑÐ¾Ð¼Ð°Ð³Ð½Ð¸ÑÐ½ÑÐµ Ð²Ð¾Ð»Ð½Ñ
ÐÐµÐ´Ð¸ÑÐ¸Ð½ÑÐºÐ¸Ðµ Ð¿ÑÐ¸Ð±Ð¾ÑÑ, Ð°Ð¿Ð¿Ð°ÑÐ°ÑÑ Ð¸ Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÑ
Ð¾Ð½ÐºÐ¾Ð»Ð¾Ð³Ð¸Ñ

description: ÐÐ¾Ð»ÑÑ-Ð°Ð¼Ð¿ÐµÑÐ½ÑÐµ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ¸ ÐºÑÐµÐ¼Ð½Ð¸ÐµÐ²Ð¾Ð³Ð¾ Ð½Ð°Ð½Ð¾ÑÐ°Ð½Ð´Ð²Ð¸ÑÐ°, ÐºÐ¾ÑÐ¾ÑÑÐ¹ Ð¾Ð´Ð½Ð¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾ ÑÐ²Ð»ÑÐµÑÑÑ Ð¸Ð·Ð»ÑÑÐ°ÑÐµÐ»ÐµÐ¼ Ð¸ Ð¿ÑÐ¸ÐµÐ¼Ð½Ð¸ÐºÐ¾Ð¼ Ð¢ÐÑ Ð¸Ð·Ð»ÑÑÐµÐ½Ð¸Ñ, Ð¾ÑÑÐ°Ð¶ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¾Ñ Ð±Ð¸Ð¾ÑÐºÐ°Ð½Ð¸, Ð½ÐµÑÑÑ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ñ Ð¾ ÑÑÐµÐ¿ÐµÐ½Ð¸ Ð¾Ð½ÐºÐ¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð·Ð°Ð±Ð¾Ð»ÐµÐ²Ð°Ð½Ñ Ð½Ð° ÑÐ°Ð½Ð½ÐµÐ¹ ÑÑÐ°Ð´Ð¸Ð¸.
SUMMARY OF DISSEMINATION AND COMMUNICATION ACTIVITIES N.2
Creators: name: Rivas, Freddy
name: Zamora, Eduardo
name: Mihailescu, Elena
name: Sanderson, Michael
name: Garrett, Natalie
name: Terrado, Marta
name: Calmanti, Sandro
Publisher: name: Zenodo
Year: 2019

description: This document outlines the communication and dissemination activities that were performed during the second year of the project following the communication, dissemination and exploitation management plan (D7.1)
title: A new fast algorithm for micro-satellite attitude determination based on panoramic annular lens
Creators: name: Lu, Chen
name: Hao, Wang
name: Bendong, Wang
name: Joint International Conference On Astrophysics For Young Scientists (JICA) (1; 2017; Byurakan, Armenia)
Publisher: name: Peter the Great St. Petersburg Polytechnic University
Year: 2017
Subjects: ÐÑÑÑÐ¾ÑÐ¸Ð·Ð¸ÐºÐ°
ÐÑÐºÑÑÑÑÐ²ÐµÐ½Ð½ÑÐµ ÑÐ¿ÑÑÐ½Ð¸ÐºÐ¸ ÐÐµÐ¼Ð»Ð¸
micro-satellite
attitude determination algorithm
static infrared earth sensor

description: A new fast attitude determination algorithm based on panoramic annular lens has been developed. The panoramic annular lens is used as the static infrared sensor, which forms a large field of view to get the infrared image of the Earth. The algorithm of PAL projects the image points onto the virtual earth formatting a space circular loop. The points on this loop are used to construct the spatial vectors. Through the cross product of these spatial vectors, the micro-satellite direction vector can be estimated. This algorithm abandons the iterative process, which reduces the calculation time to meet the demand of rapid maneuver of micro-satellite.
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð¸Ð¹ Ð¿Ð¾ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÐµÐ³ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð² ÑÑÐµÑÐµ ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½Ð¾Ð¹ ÑÐµÐºÐ»Ð°Ð¼Ñ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐ¾Ð¼Ð¸ÑÐµÑÐ° Ð¿Ð¾ Ð¿ÐµÑÐ°ÑÐ¸ Ð¸ Ð²Ð·Ð°Ð¸Ð¼Ð¾Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ ÑÐ¾ ÑÑÐµÐ´ÑÑÐ²Ð°Ð¼Ð¸ Ð¼Ð°ÑÑÐ¾Ð²Ð¾Ð¹ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¸ Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³Ð°)
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ½Ð´ÑÐµÐµÐ²Ð°, 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: 2016
Subjects: ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½Ð°Ñ ÑÐµÐºÐ»Ð°Ð¼Ð°
ÑÐµÐºÐ»Ð°Ð¼Ð¾Ð´Ð°ÑÐµÐ»Ð¸
Ð·Ð°ÐºÐ°Ð·ÑÐ¸ÐºÐ¸
Ð¿ÐµÑÐ°ÑÑ
Ð¡ÐÐ
social adverting
advertisers
customers
press
mass media

description: Ð¢ÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¾Ðµ Ð·Ð½Ð°ÑÐµÐ½Ð¸Ðµ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð·Ð°ÐºÐ»ÑÑÐ°ÐµÑÑÑ Ð² ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¾Ð¼ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð¸Ð¸, Ð°Ð½Ð°Ð»Ð¸Ð·Ðµ Ð¸ Ð²ÑÑÐ²Ð»ÐµÐ½Ð¸Ð¸ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÑ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼ Ð² ÑÑÐµÑÐµ ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½Ð¾Ð¹ ÑÐµÐºÐ»Ð°Ð¼Ñ. ÐÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ°Ñ Ð·Ð½Ð°ÑÐ¸Ð¼Ð¾ÑÑÑ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²ÑÐ·Ð°Ð½Ð° Ñ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¾Ð¹ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð¸Ð¹ Ð¿Ð¾ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ ÑÐµÐ³ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð² ÑÑÐµÑÐµ ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½Ð¾Ð¹ ÑÐµÐºÐ»Ð°Ð¼Ñ.
description: The theoretical value of the research is theoretical analysis, analysis and identification of the main problems in the sphere of social advertising. The practical significance of the work associated with the development of proposals on improvement of state regulation in the sphere of social advertising.
Aharonov-Bohm effect and plasma oscillations in superconducting tubes and rings
Creators: name: Bogachek, E. N.
name: Romanovsky, I. A.
name: Landman, Uzi
Publisher: name: arXiv
Year: 2008
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: Low frequency plasma oscillations in superconducting tubes are considered. The emergence of two different dimensionality regimes of plasma oscillations in tubes, exhibiting a crossover from one-dimensional to two-dimensional behavior, depending on whether $k R\ll 1$ or $k R\gg 1$, where $k$ is the plasmon wave vector and $R$ is the radius of the tube, is discussed. The Aharonov-Bohm effect pertaining to plasma oscillations in superconducting tubes and rings, resulting in an oscillatory behavior of the plasmon frequency as a function of the magnetic flux, with a flux quantum period $hc/2e$ (analog of the Little-Parks effect), is studied. The amplitude of the oscillations is proportional to $(ξ/R)^2$, where $ξ$ is the superconducting coherence length.
description: 18 pages, 4 figures
title: Ð ÑÑÑÐºÐ¸Ð¹ ÑÐ·ÑÐº ÐºÐ°Ðº Ð¸Ð½Ð¾ÑÑÑÐ°Ð½Ð½ÑÐ¹. ÐÐ°ÑÐºÐ° Ð¸ ÑÑÑÐ½ÑÐµ Ð Ð¾ÑÑÐ¸Ð¸
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐ°ÑÐ°Ð½Ð¾Ð²Ð°, ÐÑÐ¸Ð½Ð°
name: ÐÐ¸Ð½Ð¾Ð³ÑÐ°Ð´Ð¾Ð²Ð°, ÐÐ°ÑÐ¸Ñ
name: ÐÐ¾ÑÐµÐ½ÐºÐ¾, ÐÐ°ÑÐ¸Ñ
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2021
Subjects: ÐÐ¾Ð¼Ð¾Ð½Ð¾ÑÐ¾Ð², ÐÐ¸Ñ Ð°Ð¸Ð» ÐÐ°ÑÐ¸Ð»ÑÐµÐ²Ð¸Ñ, 1711-1765
ÐÐ¾Ð²Ð°Ð»ÐµÐ²ÑÐºÐ°Ñ, Ð¡Ð¾ÑÑÑ ÐÐ°ÑÐ¸Ð»ÑÐµÐ²Ð½Ð°, 1850-1891
ÐÐ»ÑÑÑÐ¾Ð², ÐÐ¾ÑÐµÑ ÐÐ²Ð°Ð½Ð¾Ð²Ð¸Ñ, 1930-2019
ÐÐµÑÐ½Ð°Ð´ÑÐºÐ¸Ð¹, ÐÐ»Ð°Ð´Ð¸Ð¼Ð¸Ñ ÐÐ²Ð°Ð½Ð¾Ð²Ð¸Ñ, 1863-1945
ÐÐµÐ»Ð¸Ð½ÑÐºÐ¸Ð¹, ÐÐ¸ÐºÐ¾Ð»Ð°Ð¹ ÐÐ¼Ð¸ÑÑÐ¸ÐµÐ²Ð¸Ñ, 1861 - 1953
ÐÐ¾ÑÑÐµ, ÐÐ±ÑÐ°Ð¼ Ð¤ÐµÐ´Ð¾ÑÐ¾Ð²Ð¸Ñ, 1880-1960
ÐÐ°Ð¿Ð¸ÑÐ°, ÐÐµÑÑ ÐÐµÐ¾Ð½Ð¸Ð´Ð¾Ð²Ð¸Ñ, 1894-1984
ÐÑÑÑÐ°ÑÐ¾Ð², ÐÐ³Ð¾ÑÑ ÐÐ°ÑÐ¸Ð»ÑÐµÐ²Ð¸Ñ, 1902-1960
ÐÐ°Ð½Ð´Ð°Ñ, ÐÐµÐ² ÐÐ°Ð²Ð¸Ð´Ð¾Ð²Ð¸Ñ, 1908-1968
Ð¡ÐµÐ¼ÐµÐ½Ð¾Ð², ÐÐ¸ÐºÐ¾Ð»Ð°Ð¹ ÐÐ¸ÐºÐ¾Ð»Ð°ÐµÐ²Ð¸Ñ, 1896-1986
Ð¤ÑÐµÐ½ÐºÐµÐ»Ñ, Ð¯ÐºÐ¾Ð² ÐÐ»ÑÐ¸Ñ, 1894-1952
Ð¥Ð°ÑÐ¸ÑÐ¾Ð½, Ð®Ð»Ð¸Ð¹ ÐÐ¾ÑÐ¸ÑÐ¾Ð²Ð¸Ñ, 1904-1996
ÐÐ°Ð²Ð»Ð¾Ð², ÐÐ²Ð°Ð½ ÐÐµÑÑÐ¾Ð²Ð¸Ñ, 1849 - 1936
ÐÐ°Ð½ÑÐ¾ÑÐ¾Ð²Ð¸Ñ, ÐÐµÐ¾Ð½Ð¸Ð´ ÐÐ¸ÑÐ°Ð»ÑÐµÐ²Ð¸Ñ, 1912-1986
ÐÐ¸Ð½Ð¾Ð³ÑÐ°Ð´Ð¾Ð², ÐÐ¸ÐºÑÐ¾Ñ ÐÐ»Ð°Ð´Ð¸Ð¼Ð¸ÑÐ¾Ð²Ð¸Ñ, 1894-1969
ÐÐµÑÐ±Ð¸ÑÐºÐ°Ñ, ÐÑÐ´Ð¼Ð¸Ð»Ð° ÐÐ»ÐµÐºÑÐµÐµÐ²Ð½Ð°, 1936-2019
ÑÑÑÑÐºÐ¸Ð¹ ÑÐ·ÑÐº
ÑÐµÐºÑÑÑ
Ð¸ÑÑÐ¾ÑÐ¸Ñ Ð½Ð°ÑÐºÐ¸
Ð½Ð°ÑÑÐ½ÑÐµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ
ÑÑÐµÐ±Ð½Ð¸ÐºÐ¸ Ð¸ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Ð´Ð»Ñ Ð¸Ð½Ð¾ÑÑÑÐ°Ð½ÑÐµÐ²
ÑÑÐµÐ±Ð½Ð¸ÐºÐ¸ Ð¸ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Ð´Ð»Ñ Ð²ÑÐ·Ð¾Ð²

description: Ð£ÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ ÑÐ¾Ð´ÐµÑÐ¶Ð¸Ñ ÑÐµÐºÑÑÑ Ð¾Ð± Ð¸ÑÑÐ¾ÑÐ¸Ð¸ Ð½Ð°ÑÐºÐ¸, Ð¾ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÑ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸ÑÑ Ð½Ð°ÑÑÐ½ÑÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ð¹, Ð¾ Ð²ÑÐ´Ð°ÑÑÐ¸ÑÑÑ ÑÑÑÐ½ÑÑ Ð¸ ÑÐ¸ÑÑÐµÐ¼Ñ Ð·Ð°Ð´Ð°Ð½Ð¸Ð¹ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ ÑÐµÐºÑÑÐ¾Ð², Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð½ÑÑ Ð½Ð° Ð¾Ð±ÑÑÐµÐ½Ð¸Ðµ Ð¸Ð½Ð¾ÑÑÑÐ°Ð½Ð½ÑÑ ÑÑÐ°ÑÐ¸ÑÑÑ ÑÑÐµÐ½Ð¸Ñ, Ð¼Ð¾Ð½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð¸ Ð´Ð¸Ð°Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð¹ ÑÐµÑÐ¸. Ð¦ÐµÐ»Ñ Ð´Ð°Ð½Ð½Ð¾Ð³Ð¾ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ â Ð¿Ð¾Ð·Ð½Ð°ÐºÐ¾Ð¼Ð¸ÑÑ Ð¸Ð½Ð¾ÑÑÑÐ°Ð½Ð½ÑÑ ÑÑÐ°ÑÐ¸ÑÑÑ Ñ Ð´Ð¾ÑÑÐ¸Ð¶ÐµÐ½Ð¸ÑÐ¼Ð¸ Ð¸Ð·Ð²ÐµÑÑÐ½ÑÑ ÑÐ¾ÑÑÐ¸Ð¹ÑÐºÐ¸Ñ
ÑÑÑÐ½ÑÑ, ÐºÐ¾ÑÐ¾ÑÑÐµ Ð²Ð½ÐµÑÐ»Ð¸ Ð±Ð¾Ð»ÑÑÐ¾Ð¹ Ð²ÐºÐ»Ð°Ð´ Ð² ÑÐ°Ð·Ð½ÑÐµ Ð¾Ð±Ð»Ð°ÑÑÐ¸ Ð½Ð°ÑÐºÐ¸ â ÑÐ¸Ð·Ð¸ÐºÑ, ÑÐ¸Ð¼Ð¸Ñ, ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÑ, ÑÐ¸Ð·Ð¸Ð¾Ð»Ð¾Ð³Ð¸Ñ, Ð»Ð¸Ð½Ð³Ð²Ð¸ÑÑÐ¸ÐºÑ. Ð£ÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð°Ð´ÑÐµÑÐ¾Ð²Ð°Ð½Ð¾ Ð¸Ð½Ð¾ÑÑÑÐ°Ð½Ð½ÑÐ¼ ÑÑÐ°ÑÐ¸Ð¼ÑÑ, Ð²Ð»Ð°Ð´ÐµÑÑÐ¸Ð¼ ÑÑÑÑÐºÐ¸Ð¼ ÑÐ·ÑÐºÐ¾Ð¼ Ð² Ð¾Ð±ÑÑÐ¼Ðµ Ð±Ð°Ð·Ð¾Ð²Ð¾Ð³Ð¾ ÑÑÐ¾Ð²Ð½Ñ (Ð2).
The transverse spin structure of the pion at short distances
Creators: name: Diehl, Markus
name: Szymanowski, Lech
Publisher: name: arXiv
Year: 2010
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We study the form factors of the quark tensor currents in the pion at large squared momentum transfer Q^2. It turns out that certain form factors can be evaluated using collinear factorization, whereas others receive important contributions from the end-point regions of the longitudinal quark momenta in the pion. We derive simple analytic expressions for the dominant terms at high Q^2 and illustrate them numerically.
description: 13 pages, 3 figures. v2: added discussion of chiral limit, changed references
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ° Ð¿Ð¾ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½ÑÑ ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¹ Ð² Ð¼ÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½Ñ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ ÑÑÐµÑÑ Ð³Ð¾ÑÑÐµÐ¿ÑÐ¸Ð¸Ð¼ÑÑÐ²Ð°.
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¸Ð½ÑÐºÐ¸Ð½Ð°, ÐÐºÐ°ÑÐµÑ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: 2017
Subjects: Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¸
Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½ÑÐ¹ Ð¿ÑÐ¾ÐµÐºÑ
Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐµ ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¸
Ð¼ÐµÑÐ¾Ð´Ñ Ð¾ÑÐµÐ½ÐºÐ¸ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¸
Ð¼ÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½Ñ

description: Ð¦ÐµÐ»Ñ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 ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ° Ð¿Ð¾ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½ÑÑ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¹ Ð² Ð¼ÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½Ñ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ ÑÑÐµÑÑ Ð³Ð¾ÑÑÐµÐ¿ÑÐ¸Ð¸Ð¼ÑÑÐ²Ð°. ÐÐ»Ñ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¿ÑÐ¾ÐµÐºÑÐ° Ð¸Ð·ÑÑÐµÐ½Ñ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð°ÑÐ¿ÐµÐºÑÑ Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¸ Ð¼ÐµÑÐ°Ð½Ð¸Ð·Ð¼ Ð¸Ñ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÐµ Ð¼ÐµÑÐ¾Ð´Ñ Ð¾ÑÐµÐ½ÐºÐ¸ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½ÑÑ Ð¿ÑÐ¾ÐµÐºÑÐ¾Ð². ÐÐ°Ð½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ ÐºÐ»Ð¸Ð¼Ð°ÑÐ° Ð¸ Ð¿Ð¾ÑÐµÐ½ÑÐ¸Ð°Ð»Ð° Ð ÐµÑÐ¿ÑÐ±Ð»Ð¸ÐºÐ¸ ÐÐ¾ÑÐ´Ð¾Ð²Ð¸Ñ, Ð° ÑÐ°ÐºÐ¶Ðµ Ð´Ð°Ð½Ð° Ð¾ÑÐµÐ½ÐºÐ° Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ Ð¿ÑÐ¸Ð²Ð»ÐµÐºÐ°ÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¸ Ð¼ÐµÑÐ¾Ð´Ñ ÐµÐµ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ Ð´Ð»Ñ Ð´Ð°Ð½Ð½Ð¾Ð³Ð¾ ÑÐµÐ³Ð¸Ð¾Ð½Ð°. Ð¡ÑÐ¾ÑÐ¼ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ñ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ð¿Ð¾ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐµ Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ° Ð¸Ð½ÑÐµÑÐ°ÐºÑÐ¸Ð²Ð½Ð¾Ð³Ð¾ ÑÐ°Ð¹ÑÐ° Ð´Ð»Ñ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ ÐÐÐ Â«ÐÐ¾Ð¼ ÐÑÑÐ°Â». Ð ÑÐ°Ð¼ÐºÐ°Ñ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ ÑÐ°Ð¹ÑÐ° Ð¿Ð¾ÑÑÐ¸ÑÐ°Ð½ ÑÐµÐ·ÑÐ»ÑÑÐ°Ñ Ð¾Ñ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸, ÐºÐ¾ÑÐ¾ÑÑÐ¹ Ð½Ð°ÑÐµÐ» ÑÐ²Ð¾Ðµ Ð¾ÑÑÐ°Ð¶ÐµÐ½Ð¸Ðµ Ð² Ð²ÑÑÑÑÐºÐµ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ.
Importance Truncation for Large-Scale Configuration Interaction Approaches
Creators: name: Roth, Robert
Publisher: name: arXiv
Year: 2009
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We introduce an iterative importance truncation scheme which aims at reducing the dimension of the model space of configuration interaction approaches by an a priori selection of the physically most relevant basis states. Using an importance measure derived from multiconfigurational perturbation theory in combination with an importance threshold, we construct a model space optimized for the description of individual eigenstates of a given Hamiltonian. We discuss in detail various technical aspects and refinements of the importance truncation, such as perturbative corrections for excluded basis states, threshold extrapolation techniques, and different iterative model-space update schemes. We apply the idea of the importance truncation in the context of the no-core shell model (NCSM) for the ab initio description of nuclear ground states. In a series of benchmark calculations for closed- and open-shell nuclei up to O-16 we compare the ground-state energies obtained in the importance truncated NCSM to the full NCSM. All calculations show an excellent agreement of importance truncated and full NCSM for all cases where the latter is feasible. The results demonstrate that the importance truncated NCSM, while preserving most of the advantages of the full NCSM, gives access to much larger N_max*hbar*Omega spaces and heavier nuclei. In this way we are able to perform importance truncated NCSM calculations for nuclei like C-12 and O-16 up to N_max=22.
description: 19 pages, 13 figures, 1 table
Relaxation Mechanism for Ordered Magnetic Materials
Creators: name: Vittoria, C.
name: Yoon, S. D.
name: Widom, A.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: We have formulated a relaxation mechanism for ferrites and ferromagnetic metals whereby the coupling between the magnetic motion and lattice is based purely on continuum arguments concerning magnetostriction. This theoretical approach contrasts with previous mechanisms based on microscopic formulations of spin-phonon interactions employing a discrete lattice. Our model explains for the first time the scaling of the intrinsic FMR linewidth with frequency, and 1/M temperature dependence and the anisotropic nature of magnetic relaxation in ordered magnetic materials, where M is the magnetization. Without introducing adjustable parameters our model is in reasonable quantitative agreement with experimental measurements of the intrinsic magnetic resonance linewidths of important class of ordered magnetic materials, insulator or metals.
Uma coleção de dados estratificados em Acesso Aberto para análises bibliométricas
Creators: name: Dias, Patrícia Mascarenhas
name: Dias, Thiago Magela Rodrigues
Publisher: name: Zenodo
Year: 2021

description: Apresentação realizada na sessão O meu Póster num minuto da 12ª Conferência Luso-Brasileira de Ciência Aberta, formato híbrido, de 13 a 15 de outubro de 2021.
title: ÐÐ¾Ð½Ð²ÐµÐ¹ÐµÑÐ½ÑÐ¹ Ð°Ð²ÑÐ¾Ð¼Ð°Ñ ÑÐ±Ð¾ÑÐºÐ¸ ÐºÐ»Ð°Ð¿Ð°Ð½Ð°
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¾Ð½Ð¾Ð², ÐÐ»ÐµÐºÑÐµÐ¹
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: Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸ÑÐµÑÐºÐ°Ñ ÑÐ±Ð¾ÑÐºÐ° ÐºÐ»Ð°Ð¿Ð°Ð½Ð°
Ð»ÐµÐ½ÑÐ¾ÑÐ½ÑÐ¹ ÐºÐ¾Ð½Ð²ÐµÐ¹ÐµÑ
Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð°Ñ Ð»Ð¸Ð½Ð¸Ñ
Ð¼Ð¾Ð´ÑÐ»Ñ ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ¸ÑÐ¾Ð²ÐºÐ¸
ÑÐ°ÑÑÐµÑÑ
ÑÐµÑÑÐµÐ¶Ð¸

description: ÐÑÐ¿ÑÑÐºÐ½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐµ ÐºÐ¾Ð½Ð²ÐµÐ¹ÐµÑÐ½Ð¾Ð³Ð¾ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ° ÑÐ±Ð¾ÑÐºÐ¸ ÐºÐ»Ð°Ð¿Ð°Ð½Ð°. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð»Ð¸ÑÐµÑÐ°ÑÑÑÐ½ÑÐ¹ Ð¾Ð±Ð·Ð¾Ñ Ð±Ð°Ð·Ð¾Ð²ÑÑ ÑÑÑÑÐºÑÑÑ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð»Ð¸Ð½Ð¸Ð¹ Ð¸ ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ½ÑÑ Ð¼ÐµÑÐ°Ð½Ð¸Ð·Ð¼Ð¾Ð². Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð¿ÑÐ¾ÑÐµÑÑ, ÑÐ¾ÑÑÐ°Ð²Ð»ÐµÐ½Ð° ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ°Ñ ÑÑÐµÐ¼Ð° Ð¿ÑÐ¾ÑÐµÑÑÐ° ÑÐ±Ð¾ÑÐºÐ¸ Ð¸Ð·Ð´ÐµÐ»Ð¸Ñ. ÐÑÐ¸Ð²ÐµÐ´ÐµÐ½Ñ ÑÑÑÑÐºÑÑÑÐ½Ð¾-ÑÑÐ½ÐºÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð°Ñ Ð¸ ÐºÐ¾Ð¼Ð±Ð¸Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð°Ñ ÑÑÐµÐ¼Ñ ÐºÐ¾Ð½Ð²ÐµÐ¹ÐµÑÐ½Ð¾Ð³Ð¾ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ°. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ñ Ð»ÐµÐ½ÑÐ¾ÑÐ½Ð¾Ð³Ð¾ ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐµÑÐ° Ñ ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ð¼ Ð¿ÑÐ¸Ð²Ð¾Ð´Ð¾Ð¼. ÐÐ±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½ Ð²ÑÐ±Ð¾Ñ Ð¸ ÑÐ°ÑÐ¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ðµ Ð¾ÑÐ´ÐµÐ»ÑÐ½ÑÑ Ð¼Ð¾Ð´ÑÐ»ÐµÐ¹, ÐºÐ¸Ð½ÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÐ²ÑÐ·Ð¸ Ð²ÑÐ¾Ð´ÑÑÐ¸Ñ Ð² Ð½Ð¸Ñ ÐµÐ´Ð¸Ð½Ð¸Ñ. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ ÑÐµÑÑÐµÐ¶ Ð¾Ð±ÑÐµÐ³Ð¾ Ð²Ð¸Ð´Ð° Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ°, ÑÐ±Ð¾ÑÐ¾ÑÐ½ÑÐ¹ ÑÐµÑÑÐµÐ¶ Ð»ÐµÐ½ÑÐ¾ÑÐ½Ð¾Ð³Ð¾ ÐºÐ¾Ð½Ð²ÐµÐ¹ÐµÑÐ°, ÑÐ°Ð±Ð¾ÑÐ¸Ðµ ÑÐµÑÑÐµÐ¶Ð¸ Ð´Ð²ÑÑ Ð´ÐµÑÐ°Ð»ÐµÐ¹.
Thin films flowing down inverted substrates: two dimensional flow
Creators: name: Lin, Te-sheng
name: Kondic, Lou
Publisher: name: arXiv
Year: 2009
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: We consider free surface instabilities of films flowing on inverted substrates within the framework of lubrication approximation. We allow for the presence of fronts and related contact lines, and explore the role which they play in instability development. It is found that a contact line, modeled by a commonly used precursor film model, leads to free surface instabilities without any additional natural or excited perturbations. A single parameter D=(3Ca)^{1/3}\cotα$, where $Ca$ is the capillary number and $α$ is the inclination angle, is identified as a governing parameter in the problem. This parameter may be interpreted to reflect the combined effect of inclination angle, film thickness, Reynolds number and the fluid flux. Variation of $D$ leads to change of the wave-like properties of the instabilities, allowing us to observe traveling wave behavior, mixed waves, and the waves resembling solitary ones.
title: EU SINE2020 WP 10 : report on guidelines and standards for data treatment software
Creators: name: Markvardsen, A J
name: Holm Rod, T
name: Cottrell, S P
name: Lim, A
name: Wuttke, J
name: Potrzebowski, W
name: Kaestner, A
name: Willendrup, P
name: Draper, N
name: Gonzalez, M A
Publisher: name: STFC
Year: 2019

description: This report summarises outputs from task 10.2 of WP10. The purpose of this task is to provide guidelines and standards that should be used to exploit and interface to neutron data treatment software developed in this WP. New, and improvements to existing, neutron data treatment software are continuously needed. The reasons for this is that the field of neutron scattering is not static; there is a continuous development of new instruments, new detectors and detector electrons, improvements in computing networks and hardware, and most topical in relation to the building of ESS. This report, in addition to an introduction, has three main sections: (1) Based on answers from a questionnaire broad guidelines are derived for how to best develop software for neutron data treatment, where the questionnaire targets existing well established data treatment software and look for commonalities between these. (2) For the specific use case of writing data loaders for complex neutron data formats, what best advices, i.e. guidelines, can be given for documenting such loaders? (3) Many data treatment software depends critically on fitting. This report presents a new benchmarking library for comparing fit minimizers; a required step towards providing a standard for comparing the performance and stability of minimizers used for treating/analysing neutron data. The proposed guidelines derived from the questionnaire were discussed in detail in a presentation at the SINE2020 workshop at ILL April 2017, where many participants provided inputs. The guidelines presented take into accounts these comments and these had the broad agreement of the 58 participants of this meeting.
title: Ð¢ÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¾ÑÐ½Ð¾Ð²Ñ ÐºÐ¾Ð¼Ð¿ÑÑÑÐµÑÐ½Ð¾Ð¹ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸. ÐÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ðµ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² Ð¸ÑÐºÑÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¸Ð½ÑÐµÐ»Ð»ÐµÐºÑÐ°
title: Ð»Ð°Ð±Ð¾ÑÐ°ÑÐ¾ÑÐ½ÑÐ¹ Ð¿ÑÐ°ÐºÑÐ¸ÐºÑÐ¼
titleType: Subtitle
Creators: name: ÐÐ°Ð»Ð¸Ð½Ð¸Ð½, ÐÐ°ÐºÑÐ¸Ð¼
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2010
Subjects: ÐÑÐºÑÑÑÑÐ²ÐµÐ½Ð½ÑÐ¹ Ð¸Ð½ÑÐµÐ»Ð»ÐµÐºÑ
ÐÑÑÐ¸ÑÐ»Ð¸ÑÐµÐ»ÑÐ½ÑÐµ Ð¼Ð°ÑÐ¸Ð½Ñ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½ÑÐµ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»ÑÐ½ÑÐµ

description: Ð¡Ð¾Ð´ÐµÑÐ¶Ð¸Ñ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¸ Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÐ²ÐµÐ´ÐµÐ½Ð¸Ñ Ð¾ ÑÐ¿Ð¾ÑÐ¾Ð±Ð°Ñ Ð¸ Ð¼ÐµÑÐ¾Ð´Ð°Ñ, ÑÐ¾ÑÑÐ°Ð²Ð»ÑÑÑÐ¸Ñ Ð¾ÑÐ½Ð¾Ð²Ñ Ð¿Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ñ ÑÐ¸ÑÑÐµÐ¼ Ð¸ÑÐºÑÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¸Ð½ÑÐµÐ»Ð»ÐµÐºÑÐ° Ð¿ÑÐ¸ ÑÐµÑÐµÐ½Ð¸Ð¸ Ð·Ð°Ð´Ð°Ñ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸. ÐÐ°Ð½Ñ ÑÐºÐ°Ð·Ð°Ð½Ð¸Ñ Ðº Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÐ°Ð±Ð¾Ñ Ð¿Ð¾ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¼ÐµÑÐ°Ð½Ð¸Ð·Ð¼Ð¾Ð² Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð·Ð½Ð°Ð½Ð¸Ð¹, ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ¾Ð² Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð·Ð°ÑÐ¸ÑÐµÐ½Ð½ÑÑ ÑÐ¸ÑÑÐµÐ¼; Ð¿Ð¾ Ð¸Ð·ÑÑÐµÐ½Ð¸Ñ Ð²Ð¾Ð¿ÑÐ¾ÑÐ¾Ð² Ð¿Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ñ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ½ÑÑ ÑÐ¸ÑÑÐµÐ¼ Ð¸ÑÐºÑÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¸Ð½ÑÐµÐ»Ð»ÐµÐºÑÐ°, ÑÐ¸ÑÑÐµÐ¼ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð·Ð½Ð°Ð½Ð¸Ð¹ Ð¸ Ð¿ÑÐ¸Ð½ÑÑÐ¸Ñ ÑÐµÑÐµÐ½Ð¸Ð¹, ÑÐºÑÐ¿ÐµÑÑÐ½ÑÑ ÑÐ¸ÑÑÐµÐ¼; Ð¿Ð¾ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ Ð½ÐµÐ¹ÑÐ¾ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¹, Ð³ÐµÐ½ÐµÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ð¾Ð² Ð¸ Ð½ÐµÑÐµÑÐºÐ¾Ð¹ Ð»Ð¾Ð³Ð¸ÐºÐ¸, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸ÑÐ¼ Ð¸Ñ ÑÐºÑÐ¿Ð»ÑÐ°ÑÐ°ÑÐ¸Ð¸ Ð² Ð¾Ð±Ð»Ð°ÑÑÐ¸ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸ Ð² ÑÐ°Ð¼ÐºÐ°Ñ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð·Ð°Ð½ÑÑÐ¸Ð¹ Ð½Ð° ÐºÐ°ÑÐµÐ´ÑÐµ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸ ÐºÐ¾Ð¼Ð¿ÑÑÑÐµÑÐ½ÑÑ ÑÐ¸ÑÑÐµÐ¼ Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¾Ð³Ð¾ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿Ð¾Ð»Ð¸ÑÐµÑÂ­Ð½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ°. ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐµÐ¹ 090102.65 Ð¸ 090105.65, Ð° ÑÐ°ÐºÐ¶Ðµ Ð´Ð»Ñ Ð¿ÑÐµÐ¿Ð¾Ð´Ð°Ð²Ð°ÑÐµÐ»ÐµÐ¹ Ð¸ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð², ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸Ð·Ð¸ÑÑÑÑÐ¸ÑÑÑ Ð² Ð¾Ð±Ð»Ð°ÑÑÐ¸ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¸Ð½ÑÐµÐ»Ð»ÐµÐºÑÑÐ°Ð»ÑÐ½ÑÑ ÑÐ¸ÑÑÐµÐ¼ Ð·Ð°ÑÐ¸ÑÑ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¸, Ð¸ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð², Ð¾Ð±ÑÑÐ°ÑÑÐ¸ÑÑÑ Ð¿Ð¾ Ð´ÑÑÐ³Ð¸Ð¼ ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¼ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÑÐ¼.
description: ÐÐµÑÐ°ÑÐ°ÐµÑÑÑ Ð¿Ð¾ ÑÐµÑÐµÐ½Ð¸Ñ ÑÐµÐ´Ð°ÐºÑÐ¸Ð¾Ð½Ð½Ð¾-Ð¸Ð·Ð´Ð°ÑÐµÐ»ÑÑÐºÐ¾Ð³Ð¾ ÑÐ¾Ð²ÐµÑÐ° Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¾Ð³Ð¾ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ°.
Reply to "Comment on 'Bell's Theorem Versus Local Realism in a Quaternionic Model of Physical Space'"
Creators: name: Christian, Joy
Publisher: name: arXiv
Year: 2022
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: In this paper, I respond to a critique of one of my papers previously published in this journal, entitled "Bell's Theorem Versus Local Realism in a Quaternionic Model of Physical Space." That paper presents a local-realistic model of quantum correlations based on a quaternionic 3-sphere, taken as a physical space in which we are confined to perform all our experiments. The critique, on the other hand, considers two entirely different models within a flat Euclidean space, neither related to my quaternionic 3-sphere model. It then criticizes its own flat space models and claims that it has thereby criticized the model presented in my paper. Along the way, without providing evidence or proof, it claims that the results in my paper are based on mistakes. I demonstrate that there are no mistakes of any kind in my paper. On the contrary, I bring out a number of elementary mathematical and conceptual mistakes from the critique and the critiques it relies on.
description: 12 pages, 4 figures. This paper is published in response to arXiv:2103.00225 [quant-ph]
title: ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¾Ð¿ÑÐ¸Ð¼Ð°Ð»ÑÐ½Ð¾Ð¹ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¸ Ð³Ð°Ð¼Ð¼Ð°-Ð¿ÐµÐ»ÐµÐ½Ð³Ð°ÑÐ¾ÑÐ° Ð¿Ð¾Ð»ÑÑÑÐµÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¾Ð±Ð·Ð¾ÑÐ°
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¾ÑÐ¸ÑÐ¾Ð², ÐÐ»Ð°Ð´Ð¸ÑÐ»Ð°Ð²
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: Ð³Ð°Ð¼Ð¼Ð°-Ð¸Ð·Ð»ÑÑÐµÐ½Ð¸Ðµ
Ð±Ð»Ð¾Ðº Ð´ÐµÑÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð³Ð°Ð¼Ð¼Ð°-Ð¸Ð·Ð»ÑÑÐµÐ½Ð¸Ñ
Ð²Ð¸Ð·ÑÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ¾Ð² Ð³Ð°Ð¼Ð¼Ð°-Ð¸Ð·Ð»ÑÑÐµÐ½Ð¸Ñ
Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ðµ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð½Ð° Ð¸ÑÑÐ¾ÑÐ½Ð¸Ðº
Ð¿Ð¾Ð¸ÑÐº Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ¾Ð²

description: ÐÐ°ÑÑÐ¾ÑÑÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¾ÑÐ½Ð¾ÑÐ¸ÑÑÑ Ðº Ð¾Ð±Ð»Ð°ÑÑÐ¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ ÑÑÐµÐ´ÑÑÐ² Ð¿Ð¾Ð¸ÑÐºÐ° Ð¸ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð½Ð° Ð¸ÑÑÐ¾ÑÐ½Ð¸Ðº Ð³Ð°Ð¼Ð¼Ð°-Ð¸Ð·Ð»ÑÑÐµÐ½Ð¸Ñ. Ð¦ÐµÐ»ÑÑ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐ»Ð¾ÑÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð·Ð°Ð²Ð¸ÑÐ¸Ð¼Ð¾ÑÑÐ¸ Ð·Ð¾Ð½Ñ Ð·ÑÐµÐ½Ð¸Ñ Ð±Ð»Ð¾ÐºÐ° Ð´ÐµÑÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¾Ñ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¸ Ð·Ð°ÑÐ¸ÑÐ½Ð¾Ð³Ð¾ ÑÐºÑÐ°Ð½Ð°. ÐÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¾, ÑÑÐ¾ ÑÐ²ÐµÐ»Ð¸ÑÐµÐ½Ð¸Ðµ Ð²ÑÑÐ¾ÑÑ ÑÑÐ¾Ð½ÑÐ°Ð»ÑÐ½Ð¾Ð¹ Ð¿Ð»Ð°ÑÑÐ¸Ð½Ñ Ð¿ÑÐ¸Ð²Ð¾Ð´Ð¸Ñ Ðº Ð±Ð¾Ð»ÐµÐµ ÑÐµÐ·ÐºÐ¾Ð¼Ñ Ð½Ð°ÐºÐ»Ð¾Ð½Ñ Ð´Ð¸Ð°Ð³ÑÐ°Ð¼Ð¼Ñ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð±Ð»Ð¾ÐºÐ° Ð´ÐµÑÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ. Ð£Ð¼ÐµÐ½ÑÑÐµÐ½Ð¸Ðµ Ð¿Ð»Ð¾ÑÐ½Ð¾ÑÑÐ¸ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð° Ð·Ð°ÑÐ¸ÑÐ½Ð¾Ð³Ð¾ ÑÐºÑÐ°Ð½Ð° Ð¿ÑÐ¸Ð²Ð¾Ð´Ð¸Ñ Ðº ÑÐ°ÑÑÐ¸ÑÐµÐ½Ð¸Ñ Ð·Ð¾Ð½Ñ Ð·ÑÐµÐ½Ð¸Ñ. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼ Ð²ÑÑÐ¸ÑÐ»ÐµÐ½Ð¸Ñ ÑÐ³Ð»Ð¾Ð²ÑÑ ÐºÐ¾Ð¾ÑÐ´Ð¸Ð½Ð°Ñ Ð³Ð°Ð¼Ð¼Ð°-Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ°.
title: ÐÑÐ°Ð²Ð¸ÑÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ðµ Ð²Ð·Ð°Ð¸Ð¼Ð¾Ð´ÐµÐ¹ÑÑÐ²Ð¸Ðµ Ð² ÑÑÐµÐ´Ðµ Ñ Ð½ÐµÐ½ÑÐ»ÐµÐ²Ð¾Ð¹ Ð¿Ð»Ð¾ÑÐ½Ð¾ÑÑÑÑ
Creators: name: ÐÐ¸ÑÑÑÐ½, ÐÐ¼Ð¸ÑÑÐ¸Ð¹
name: ÐÐ¸ÑÑÑÐ½, ÐÐµÐ¾ÑÐ³Ð¸Ð¹
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: 2019
Subjects: ÐÑÐµÐ¼Ð¸ÑÐ½Ð¾Ðµ ÑÑÐ³Ð¾ÑÐµÐ½Ð¸Ðµ
ÐÑÐ°Ð²Ð¸ÑÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ðµ Ð¿Ð¾Ð»Ðµ
ÐÑÐ°Ð²Ð¸Ð¼ÐµÑÑÐ¸Ñ

description: Ð ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÐ½Ñ Ð½Ð¾Ð²ÑÐµ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° ÑÐ¾ÑÐ¾ÑÐ¾ Ð¸Ð·Ð²ÐµÑÑÐ½ÑÑ Ð¸
Ð½Ð°Ð±Ð»ÑÐ´Ð°ÐµÐ¼ÑÑ ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¸Ñ Ð¿ÑÐ¾ÑÐµÑÑÐ¾Ð² ÑÐ²ÑÐ·Ð°Ð½Ð½ÑÑ Ñ Ð³ÑÐ°Ð²Ð¸ÑÐ°ÑÐ¸Ð¾Ð½Ð½ÑÐ¼ Ð²Ð·Ð°Ð¸Ð¼Ð¾Ð´ÐµÐ¹ÑÑÐ²Ð¸ÐµÐ¼ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»ÑÐ½ÑÑ ÑÐµÐ» Ð² ÑÑÐµÐ´Ðµ Ñ Ð½ÐµÐ½ÑÐ»ÐµÐ²Ð¾Ð¹ Ð¿Ð»Ð¾ÑÐ½Ð¾ÑÑÑÑ. Ð Ð¾ÑÐ½Ð¾Ð²Ñ ÑÐ°Ð±Ð¾ÑÑ Ð¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¾ ÑÑÐ²ÐµÑÐ¶Ð´ÐµÐ½Ð¸Ðµ Ð¾ ÑÐ¾Ð¼, ÑÑÐ¾ "Ð²ÑÑÐ°Ð»ÐºÐ¸Ð²Ð°ÑÑÐ°Ñ" ÑÐ¸Ð»Ð° ÐÑÑÐ¸Ð¼ÐµÐ´Ð°, Ð´ÐµÐ¹ÑÑÐ²ÑÑÑÐ°Ñ Ð½Ð° Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾Ðµ ÑÐµÐ»Ð¾, Ð½Ð°ÑÐ¾Ð´ÑÑÐµÐµÑÑ Ð² ÑÑÐµÐ´Ðµ Ñ Ð½ÐµÐ½ÑÐ»ÐµÐ²Ð¾Ð¹ Ð¿Ð»Ð¾ÑÐ½Ð¾ÑÑÑÑ Ð¸Ð¼ÐµÐµÑ Ð³ÑÐ°Ð²Ð¸ÑÐ°ÑÐ¸Ð¾Ð½Ð½ÑÑ Ð¿ÑÐ¸ÑÐ¾Ð´Ñ. ÐÐµ Ð²ÑÑÐ¾Ð´Ñ Ð·Ð° ÑÐ°Ð¼ÐºÐ¸ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ð¹ ÐºÐ»Ð°ÑÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÑÐ¸Ð·Ð¸ÐºÐ¸ Ð¸ Ð¼ÐµÑÐ°Ð½Ð¸ÐºÐ¸, ÑÑÐ¾Ñ Ð¿Ð¾Ð´ÑÐ¾Ð´ Ð¿Ð¾Ð·Ð²Ð¾Ð»Ð¸Ð» Ð²Ð²ÐµÑÑÐ¸ Ð¿Ð¾Ð½ÑÑÐ¸Ðµ Ð³ÑÐ°Ð²Ð¸ÑÐ¸ÑÑÑÑÐµÐ¹ Ð¼Ð°ÑÑÑ ÑÐµÐ»Ð°, ÐºÐ°Ðº Ð¼Ð°ÑÑÑ, ÐºÐ¾ÑÐ¾ÑÐ°Ñ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÑÐµÑ Ð²ÐµÐ»Ð¸ÑÐ¸Ð½Ñ Ð³ÑÐ°Ð²Ð¸ÑÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð²Ð·Ð°Ð¸Ð¼Ð¾Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ, Ð° ÑÐ°ÐºÐ¶Ðµ ÑÑÑÐ°Ð½Ð¾Ð²Ð¸ÑÑ Ð°Ð½Ð°Ð»Ð¸ÑÐ¸ÑÐµÑÐºÐ¾Ðµ ÑÐ¾Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸Ðµ Ð¼ÐµÐ¶Ð´Ñ Ð³ÑÐ°Ð²Ð¸ÑÐ¸ÑÑÑÑÐµÐ¹ Ð¸ Ð¸Ð½ÐµÑÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ Ð¼Ð°ÑÑÐ°Ð¼Ð¸ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ ÑÐµÐ»Ð°. ÐÐ±ÑÐµÐ´Ð¸Ð½ÐµÐ½Ð¸Ðµ Ð¿ÑÑÐ¼Ð¾Ð³Ð¾ Ð¸ Ð¾Ð¿Ð¾ÑÑÐµÐ´Ð¾Ð²Ð°Ð½Ð½Ð¾Ð³Ð¾ (ÑÐ¸Ð»Ð° ÐÑÑÐ¸Ð¼ÐµÐ´Ð°) Ð³ÑÐ°Ð²Ð¸ÑÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð²Ð¾Ð·Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ Ð½Ð° Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾Ðµ ÑÐµÐ»Ð¾, Ð½Ð°ÑÐ¾Ð´ÑÑÐµÐ³Ð¾ÑÑ Ð² ÑÑÐµÐ´Ðµ, Ð¿Ð¾Ð·Ð²Ð¾Ð»Ð¸Ð»Ð¾ Ð²ÑÐ´ÐµÐ»Ð¸ÑÑ Ð¸Ð· Ð¾Ð±ÑÐµÐ³Ð¾ Ð³ÑÐ°Ð²Ð¸ÑÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð¿Ð¾Ð»Ñ ÑÑÐ¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÑÑÑÐºÑÑÑÑ Ñ ÑÐ°ÑÐ°ÐºÑÐµÑÐ½ÑÐ¼ ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸ÐµÐ¼ ÑÐ¸Ð»Ð¾Ð²ÑÑ Ð»Ð¸Ð½Ð¸Ð¹, ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÑÑÑÑ Ð´Ð¸Ð¿Ð¾Ð»Ñ. Ð­ÑÐ¾Ñ ÑÐ°ÐºÑ Ð¿Ð¾Ð·Ð²Ð¾Ð»ÑÐµÑ ÑÑÐ²ÐµÑÐ¶Ð´Ð°ÑÑ, ÑÑÐ¾, Ð½Ð°ÑÑÐ´Ñ Ñ Ð³ÑÐ°Ð²Ð¸ÑÐ°ÑÐ¸Ð¾Ð½Ð½ÑÐ¼ Ð¿ÑÐ¸ÑÑÐ¶ÐµÐ½Ð¸ÐµÐ¼, ÑÑÑÐµÑÑÐ²ÑÐµÑ Ð¸ Ð³ÑÐ°Ð²Ð¸ÑÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ðµ Ð¾ÑÑÐ°Ð»ÐºÐ¸Ð²Ð°Ð½Ð¸Ðµ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»ÑÐ½ÑÑ ÑÐµÐ» Ð±ÐµÐ· ÑÐ¼ÑÑÐ»Ð¾Ð²Ð¾Ð³Ð¾ ÐºÐ¾Ð½ÑÐ»Ð¸ÐºÑÐ° Ñ ÑÑÑÐµÑÑÐ²ÑÑÑÐµÐ¹ ÑÐ¸ÑÑÐµÐ¼Ð¾Ð¹ Ð±Ð°Ð·Ð¾Ð²ÑÑ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ð¹ Ð¸ Ð¿Ð¾Ð½ÑÑÐ¸Ð¹ ÐºÐ»Ð°ÑÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÑÐ¸Ð·Ð¸ÐºÐ¸ Ð¸ Ð¼ÐµÑÐ°Ð½Ð¸ÐºÐ¸.
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð¸Ð¹ Ð¿Ð¾ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÑÐ°Ð±Ð¾ÑÑ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐÐ Â«ÐÐÐ-Ð¡Ð¿ÐµÑÑÑÐ°Ð»Ñ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Ð¾ÑÐ½Ð¸ÐµÐ½ÐºÐ¾, ÐÐ°Ð»ÐµÑ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: 2018
Subjects: ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸
Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸
ÑÐµÐ½ÑÐ°Ð±ÐµÐ»ÑÐ½Ð¾ÑÑÑ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸
Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½Ð¾ÑÑÑ

description: ÐÑÐ¿Ð¾Ð»Ð½ÐµÐ½ Ð¾Ð±Ð·Ð¾Ñ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¸ Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ñ Ð¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ð¹ Ð¿Ð¾ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾Ð¼Ñ Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑÑ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ. ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð° Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ Ð¾Ð±ÑÐµÐºÑÐ° ÑÐ°Ð±Ð¾ÑÑ â ÐÐÐ Â«ÐÐÐ-Ð¡Ð¿ÐµÑÑÑÐ°Ð»ÑÂ» Ð² Ð¿ÑÐµÐ´Ð¼ÐµÑÐ½Ð¾Ð¹ Ð¾Ð±Ð»Ð°ÑÑÐ¸, Ð²ÑÑÐ²Ð»ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ.
ÐÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¸ ÑÑÐ¾ÑÐ¼ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ñ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸. ÐÐ»Ñ Ð¾ÑÐµÐ½ÐºÐ¸ ÑÐµÐ»ÐµÑÐ¾Ð¾Ð±ÑÐ°Ð·Ð½Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð¸Ð¹ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ñ Ð¿ÑÐ¾Ð³Ð½Ð¾Ð·Ð½ÑÐµ ÑÐ°ÑÑÐµÑÑ, Ð¿Ð¾Ð´ÑÐ²ÐµÑÐ´Ð¸Ð²ÑÐ¸Ðµ ÑÐµÐ»ÐµÑÐ¾Ð¾Ð±ÑÐ°Ð·Ð½Ð¾ÑÑÑ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¹ Ð¿Ð¾ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¸ Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ.
title: ÐÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ñ ÑÐ¸ÑÑÐµÐ¼Ñ Ð´Ð¾ÐºÑÐ¼ÐµÐ½ÑÐ¾Ð¾Ð±Ð¾ÑÐ¾ÑÐ° Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð¡ÐµÑÐ¾Ð²Ð°, Ð¡Ð²ÐµÑÐ»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: 2017
Subjects: Ð´Ð¾ÐºÑÐ¼ÐµÐ½ÑÐ¾Ð¾Ð±Ð¾ÑÐ¾Ñ
ÐºÐ¾Ð½ÑÐ¸Ð´ÐµÐ½ÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÑ
ÑÑÐµÑ Ð´Ð¾ÐºÑÐ¼ÐµÐ½ÑÐ¾Ð²
ÑÑÐ°Ð½Ð´Ð°ÑÑÐ¸Ð·Ð°ÑÐ¸Ñ
Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð°ÑÐ¸Ñ
ÑÐ¸ÑÑÐµÐ¼Ð°ÑÐ¸Ð·Ð°ÑÐ¸Ñ

description: Ð¦ÐµÐ»Ñ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 ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ¸ÑÑÐµÐ¼Ñ Ð´Ð¾ÐºÑÐ¼ÐµÐ½ÑÐ¾Ð¾Ð±Ð¾ÑÐ¾ÑÐ° ÐÐÐ Â«ÐÐ°Ð»ÑÐÐ¾Ð¼Ð¿Â». ÐÐºÑÑÐ°Ð»ÑÐ½Ð¾ÑÑÑ Ð²ÑÐ±ÑÐ°Ð½Ð½Ð¾Ð¹ ÑÐµÐ¼Ñ Ð¾Ð±ÑÑÐ»Ð°Ð²Ð»Ð¸Ð²Ð°ÐµÑÑÑ Ð½ÐµÐ´Ð¾ÑÑÐ°ÑÐ¾ÑÐ½Ð¾Ð¹ Ð¿ÑÐ¾ÑÐ°Ð±Ð¾ÑÐºÐ¾Ð¹ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ Ð´Ð¾ÐºÑÐ¼ÐµÐ½ÑÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð² Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸ÑÑ. Ð ÐµÑÐµÐ½Ð¸Ðµ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð´Ð¾ÐºÑÐ¼ÐµÐ½ÑÐ°ÑÐ¸ÐµÐ¹ Ð² ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÑ ÑÑÐ»Ð¾Ð²Ð¸ÑÑ Ð¿Ð¾Ð·Ð²Ð¾Ð»Ð¸Ñ ÑÐµÐ»ÐµÐ½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð½Ð¾ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°ÑÑ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐµ ÑÐµÑÑÑÑÑ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¹, Ð¾Ð±ÐµÑÐ¿ÐµÑÐ¸Ð²Ð°ÑÑ Ð¸Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾Ðµ ÑÑÐ½ÐºÑÐ¸Ð¾Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¾ÑÐºÑÑÑÑ Ð´Ð¾ÑÑÑÐ¿ Ð¿Ð¾ÑÑÐµÐ±Ð¸ÑÐµÐ»ÑÐ¼ Ðº Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐ¼ ÑÐµÑÑÑÑÐ°Ð¼ Ñ Ð½Ð°Ð¸Ð¼ÐµÐ½ÑÑÐ¸Ð¼Ð¸ Ð·Ð°ÑÑÐ°ÑÐ°Ð¼Ð¸ Ð²ÑÐµÐ¼ÐµÐ½Ð¸, ÑÑÑÐ´Ð° Ð¸ ÑÑÐµÐ´ÑÑÐ², ÑÑÐ¾ Ð±ÐµÐ·ÑÑÐ»Ð¾Ð²Ð½Ð¾ Ð½Ðµ Ð¼Ð°Ð»Ð¾ Ð²Ð°Ð¶Ð½Ð¾ ÑÐµÐ¹ÑÐ°Ñ, Ð² ÑÑÐ»Ð¾Ð²Ð¸ÑÑ Ð¼Ð¸ÑÐ¾Ð²Ð¾Ð³Ð¾ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÐºÑÐ¸Ð·Ð¸ÑÐ°. ÐÑÐ» Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð°, Ð¸ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐ¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¸ Ð´ÐµÐ¹ÑÑÐ²ÑÑÑÐµÐ¹ ÑÐ¸ÑÑÐµÐ¼Ñ Ð´Ð¾ÐºÑÐ¼ÐµÐ½ÑÐ¾Ð¾Ð±Ð¾ÑÐ¾ÑÐ° ÐÐÐ Â«ÐÐ°Ð»ÑÐÐ¾Ð¼Ð¿Â». ÐÑÐ»Ð¸ Ð²ÑÑÐ²Ð»ÐµÐ½Ñ Ð½ÐµÐ´Ð¾ÑÑÐ°ÑÐºÐ¸. ÐÐ°Ð»ÐµÐµ Ð±ÑÐ»Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ Ð¼ÐµÑÑ Ð´Ð»Ñ ÑÑÑÑÐ°Ð½ÐµÐ½Ð¸Ñ Ð²ÑÑÐ²Ð»ÐµÐ½Ð½ÑÑ Ð½ÐµÐ´Ð¾ÑÑÐ°ÑÐºÐ¾Ð²: ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¿Ð¾ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¸ÑÑÐµÐ¼Ñ Ð´Ð¾ÐºÑÐ¼ÐµÐ½ÑÐ¾Ð¾Ð±Ð¾ÑÐ¾ÑÐ° ÐÐÐ Â«ÐÐ°Ð»ÑÐÐ¾Ð¼Ð¿Â».
Granular gas of viscoelastic particles in a homogeneous cooling state
Creators: name: Bodrova, A. S.
name: Brilliantov, N. V.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: Kinetic properties of a granular gas of viscoelastic particles in a homogeneous cooling state are studied analytically and numerically. We employ the most recent expression for the velocity-dependent restitution coefficient for colliding viscoelastic particles, which allows to describe systems with large inelasticity. In contrast to previous studies, the third coefficient a3 of the Sonine polynomials expansion of the velocity distribution function is taken into account. We observe a complicated evolution of this coefficient. Moreover, we find that a3 is always of the same order of magnitude as the leading second Sonine coefficient a2; this contradicts the existing hypothesis that the subsequent Sonine coefficients a2, a3 ..., are of an ascending order of a small parameter, characterizing particles inelasticity. We analyze evolution of the high-energy tail of the velocity distribution function. In particular, we study the time dependence of the tail amplitude and of the threshold velocity, which demarcates the main part of the velocity distribution and the high-energy part. We also study evolution of the self-diffusion coefficient D and explore the impact of the third Sonine coefficient on the self-diffusion. Our analytical predictions for the third Sonine coefficient, threshold velocity and the self-diffusion coefficient are in a good agreement with the numerical finding.
description: 10 pages, 8 figures