cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Constraining alternative theories of gravity by gravitational waves from precessing eccentric compact binaries with LISA
Creators: name: Yagi, Kent
name: Tanaka, Takahiro
Publisher: name: arXiv
Year: 2009
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We calculate how strongly one can put constraints on alternative theories of gravity such as Brans-Dicke and massive graviton theories with LISA. We consider inspiral gravitational waves from a compact binary composed of a neutron star (NS) and an intermediate mass black hole (IMBH) in Brans-Dicke (BD) theory and that composed of 2 super massive black holes (SMBHs) in massive graviton theories. We use the restricted 2PN waveforms including the effects of spins. We also take both precession and eccentricity of the orbit into account. For simplicity, we set the fiducial value for the spin of one of the binary constituents to zero so that we can apply the approximation called \textit{simple precession}. We perform the Monte Carlo simulations of $10^4$ binaries, estimating the determination accuracy of binary parameters including the BD parameter $ω_{\mathrm{BD}}$ and the Compton wavelength of graviton $λ_g$ for each binary using the Fisher matrix method. We find that including both the spin-spin coupling $σ$ and the eccentricity $e$ into the binary parameters reduces the determination accuracy by an order of magnitude for the Brans-Dicke case, whilst it has less influence on massive graviton theories. On the other hand, including precession enhances the constraint on $ω_{\mathrm{BD}}$ only 20$%$ but it increases the constraint on $λ_g$ by an order of magnitude. Using a $(1.4+1000)M_{\odot}$ NS/BH binary of SNR=$\sqrt{200}$, one can put a constraint $ω_{\mathrm{BD}}>6944$, whilst using a $(10^7+10^6)M_{\odot}$ BH/BH binary at 3Gpc, one can put $λ_g>3.06\times10^{21}$cm, on average. The latter is 4 orders of magnitude stronger than the one obtained from the solar system experiment. These results indicate that the effects of precession and eccentricity must be taken carefully in the parameter estimation analysis.
description: 35 pages, 17 figures; some corrections have been made on the Monte Carlo simulations for the massive graviton case; corresponding tables and figures have been replaced, but the major result almost unchanged.
title: ÐÐ·ÑÑÐµÐ½Ð¸Ðµ ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ²Ð¾Ð¹ÑÑÐ² ÑÑÐ°Ð¼Ð¼Ð¾Ð² Ð´ÑÐ¾Ð¶Ð¶ÐµÐ¹ Saccharomyces cerevisiae, Ð¸ÑÐ¿Ð¾Ð»ÑÐ·ÑÐµÐ¼ÑÑ Ð² Ð¿Ð¸Ð²Ð¾Ð²Ð°ÑÐµÐ½Ð¸Ð¸
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÑÐ´ÑÑÑÐ¾Ð²Ð°, Ð¢Ð°ÑÑÑ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: 2016
Subjects: Ð¿Ð¸Ð²Ð¾Ð²Ð°ÑÐµÐ½Ð½ÑÐµ Ð´ÑÐ¾Ð¶Ð¶Ð¸
Ð´ÑÐ¾Ð¶Ð¶ÐµÐ²Ð¾Ðµ Ð³Ð°Ð·Ð¾Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ðµ
Ð¿Ð¸Ð²Ð¾
Ð¿Ð¸Ð²Ð¾Ð²Ð°ÑÐµÐ½Ð¸Ðµ

description: Ð ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ Ð¿Ð¾ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ²Ð¾Ð¹ÑÑÐ² Ð¿Ð¸Ð²Ð¾Ð²Ð°ÑÐµÐ½Ð½ÑÑ Ð´ÑÐ¾Ð¶Ð¶ÐµÐ¹ ÑÐ¾Ð´Ð° Saccharomyces cerevisiae. Ð ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð´ÑÐ¾Ð¶Ð¶ÐµÐ¹ Ð²ÐµÑÑÐ¾Ð²Ð¾Ð³Ð¾ Ð¸ Ð½Ð¸Ð·Ð¾Ð²Ð¾Ð³Ð¾ Ð±ÑÐ¾Ð¶ÐµÐ½Ð¸Ñ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¾ ÐºÐ¾Ð»Ð¸ÑÐµÑÑÐ²Ð¾ Ð¶Ð¸Ð²ÑÑ Ð¸ Ð¼ÐµÑÑÐ²ÑÑ ÐºÐ»ÐµÑÐ¾Ðº, Ð¶Ð¸Ð·Ð½ÐµÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÑ, Ð³Ð°Ð·Ð¾Ð¾Ð±ÑÐ°Ð·ÑÑÑÐ°Ñ Ð¸ ÑÐ»Ð¾ÐºÑÐ»ÑÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÐ¸.
Network synchronization landscape reveals compensatory structures, quantization, and the positive effect of negative interactions
Creators: name: Nishikawa, Takashi
name: Motter, Adilson E.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: Dynamical Systems (math.DS)
subject: Optimization and Control (math.OC)
subject: Adaptation and Self-Organizing Systems (nlin.AO)
subject: Computational Physics (physics.comp-ph)
subject: Physics and Society (physics.soc-ph)
subject: FOS: Physical sciences
subject: FOS: Mathematics

description: Synchronization, in which individual dynamical units keep in pace with each other in a decentralized fashion, depends both on the dynamical units and on the properties of the interaction network. Yet, the role played by the network has resisted comprehensive characterization within the prevailing paradigm that interactions facilitating pair-wise synchronization also facilitate collective synchronization. Here we challenge this paradigm and show that networks with best complete synchronization, least coupling cost, and maximum dynamical robustness, have arbitrary complexity but quantized total interaction strength that constrains the allowed number of connections. It stems from this characterization that negative interactions as well as link removals can be used to systematically improve and optimize synchronization properties in both directed and undirected networks. These results extend the recently discovered compensatory perturbations in metabolic networks to the realm of oscillator networks and demonstrate why "less can be more" in network synchronization.
description: 11 pages and 8 figures (including Supporting Information), Supporting video available at http://www.youtube.com/watch?v=3dMI1Yyxmbw
title: ÐÐ¿ÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¸ ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÐ²Ð¾Ð¹ÑÑÐ²Ð° ÑÑÑÑÐºÑÑÑ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð½Ð°Ð½Ð¾ÐºÐ¾Ð¼Ð¿Ð¾Ð·Ð¸ÑÐ¾Ð² ÐºÐ¾Ð»Ð»Ð¾Ð¸Ð´Ð½ÑÑ ÐºÐ²Ð°Ð½ÑÐ¾Ð²ÑÑ ÑÐ¾ÑÐµÐº PbS Ñ Ð¿ÑÐ¾Ð²Ð¾Ð´ÑÑÐ¸Ð¼ Ð¿Ð¾Ð»Ð¸Ð¼ÐµÑÐ¾Ð¼
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: Ð¨Ð°ÑÐ°Ð²Ð¿Ð¸Ð» ÐÐ°Ð½ÑÑÐ»Ð³Ð°
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: ÐÐ°Ð½Ð¾ÑÑÑÑÐºÑÑÑÐ½ÑÐµ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ñ
ÐÐ¾Ð¼Ð¿Ð¾Ð·Ð¸ÑÐ¸Ð¾Ð½Ð½ÑÐµ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ñ Ð¿Ð¾Ð»Ð¸Ð¼ÐµÑÐ½ÑÐµ

description: Ð Ð½Ð°ÑÑÐ¾ÑÑÐµÐ¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ Ð¸Ð·Ð¼ÐµÐ½ÐµÐ½Ð¸Ð¸ ÑÐ¾ÑÐ¾ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÐ²Ð¾Ð¹ÑÑÐ² Ð¿Ð»ÐµÐ½Ð¾Ðº ÑÐ°ÑÑÐ²Ð¾ÑÐ¸Ð¼Ð¾Ð³Ð¾ ÑÐ¾Ð¿ÑÑÐ¶ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿Ð¾Ð»Ð¸Ð¼ÐµÑÐ° MEH-PPV Ð¸ ÐºÐ¾Ð¼Ð¿Ð¾Ð·Ð¸ÑÐ¾Ð² Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð¿Ð¾Ð»Ð¸Ð¼ÐµÑÐ° MEH-PPV Ñ Ð½Ð°Ð½Ð¾ÑÐ°ÑÑÐ¸ÑÐ°Ð¼Ð¸ PbS (Ñ Ð´Ð¸Ð°Ð¼ÐµÑÑÐ¾Ð¼ Ð¾ÐºÐ¾Ð»Ð¾ 5 Ð½Ð¼) Ð½Ð° Ð¿ÑÐ¾Ð²Ð¾Ð´ÑÑÐµÐ¹ Ð¿Ð¾Ð´Ð»Ð¾Ð¶ÐºÐµ ÑÐ¾ ÑÐ»Ð¾ÐµÐ¼ ITO Ð´Ð¾ Ð¸ Ð¿Ð¾ÑÐ»Ðµ Ð¾Ð±Ð»ÑÑÐµÐ½Ð¸Ñ Ð³Ð°Ð¼Ð¼Ð°-ÐºÐ²Ð°Ð½ÑÐ°Ð¼Ð¸. Ð¡ÑÑÑÐºÑÑÑÐ° Ð¾Ð±ÑÐ°Ð·ÑÐ¾Ð² Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÑÐµÑ ÑÐ¾Ð±Ð¾Ð¹, ÐºÐ°Ðº ÑÐµÐ½Ð´Ð²Ð¸ÑÐ° Ð¼ÐµÐ¶Ð´Ñ Ð´Ð²ÑÐ¼Ñ ÐºÐ¾Ð½ÑÐ°ÐºÑÐ°Ð¼Ð¸ ITO Ð¸ Al. ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ñ ÑÐ¿ÐµÐºÑÑÑ ÑÐ¾ÑÐ¾Ð»ÑÐ¼Ð¸Ð½Ð¸ÑÑÐµÐ½ÑÐ¸Ð¸ (Ð¤Ð), ÑÐ¿ÐµÐºÑÑÑ Ð¿ÑÐ¾Ð¿ÑÑÐºÐ°Ð½Ð¸Ð¸, Ð¸ ÑÐµÐ¼Ð½Ð¾Ð²ÑÐµ Ð¸ ÑÐ²ÐµÑÐ¾Ð²ÑÐµ Ð²Ð¾Ð»ÑÑ-Ð°Ð¼Ð¿ÐµÑÐ½ÑÐµ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ¸ Ð´Ð¾ Ð¸ Ð¿Ð¾ÑÐ»Ðµ Ð¾Ð±Ð»ÑÑÐµÐ½Ð¸Ñ Ð³Ð°Ð¼Ð¼Ð°-ÐºÐ²Ð°Ð½ÑÐ°Ð¼Ð¸. Ð¢Ð°ÐºÐ¶Ðµ Ð¿Ð¾Ð»ÑÑÐµÐ½Ñ ÑÐ¾ÑÐ¾Ð­ÐÐ¡ Ð² Ð¾Ð±Ð¾Ð¸Ñ ÑÑÑÑÐºÑÑÑÐ°Ñ Ð´Ð¾ Ð¸ Ð¿Ð¾ÑÐ»Ðµ Ð¾Ð±Ð»ÑÑÐµÐ½Ð¸Ð¸ Ð³Ð°Ð¼Ð¼Ð°-ÐºÐ²Ð°Ð½ÑÐ°Ð¼Ð¸.
description: This work presents the results of changing the photoelectrical properties of the thin films of the soluble conjugated polymer MEH-PPV and composites based on polymer MEH-PPV nanoparticles PbS (with a diameter of about 5 nm) on the conductive substrate with the ITO layer before and after irradiation with gamma rays. The structure of the sample is as a sandwich between two contacts ITO and Al. The spectra of photoluminescence (PL), spectra of the transmission and dark and light current-voltage characteristics are investigated before and after irradiation with gamma rays. Also, the photo voltage obtained in both structures before and after irradiation with gamma rays.
Mitocondri, tallone d’Achille degli astronauti
Creators: Valentina Guglielmo
Publisher: name: Media Inaf
Year: 2020

Uno studio pubblicato ieri nella rivista Cell utilizza e combina diverse analisi “omiche” raccolte in decenni di esplorazione spaziale per comprendere gli effetti di microgravità e raggi cosmici sulla salute degli astronauti. Per la prima volta gli scienziati hanno individuato una causa sistemica che spiegherebbe diverse disfunzioni dell’organismo - dalla perdita di tessuto osseo e muscolare ai danni cardiovascolari: l’alterazione nella funzionalità mitocondriale. Questa nuova consapevolezza potrà guidare nuovi interventi nutrizionali e farmaceutici volti a migliorare le condizioni di salute e i rischi connessi alla permanenza nello spazio, soprattutto in vista di future missioni di lunga durata sulla Luna o su Marte
Unstable Planetary Systems Emerging Out Of Gas Disks
Creators: name: Matsumura, Soko
name: Thommes, Edward W.
name: Chatterjee, Sourav
name: Rasio, Frederic A.
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: The discovery of over 400 extrasolar planets allows us to statistically test our understanding of formation and dynamics of planetary systems via numerical simulations. Traditional N-body simulations of multiple-planet systems without gas disks have successfully reproduced the eccentricity (e) distribution of the observed systems, by assuming that the planetary systems are relatively closely packed when the gas disk dissipates, so that they become dynamically unstable within the stellar lifetime. However, such studies cannot explain the small semi-major axes (a) of extrasolar planetary systems, if planets are formed, as the standard planet formation theory suggests, beyond the ice line. In this paper, we numerically study the evolution of three-planet systems in dissipating gas disks, and constrain the initial conditions that reproduce the observed semi-major axis and eccentricity distributions simultaneously. We adopt the initial conditions that are motivated by the standard planet formation theory, and self-consistently simulate the disk evolution, and planet migration by using a hybrid N-body and 1D gas disk code. We also take account of eccentricity damping, and investigate the effect of saturation of corotation resonances on the evolution of planetary systems. We find that the semi-major axis distribution is largely determined in a gas disk, while the eccentricity distribution is determined after the disk dissipation. We also find that there may be an optimum disk mass which leads to the observed a-e distribution. Our simulations generate a larger fraction of planetary systems trapped in mean-motion resonances (MMRs) than the observations, indicating that the disk's perturbation to the planetary orbits may be important to explain the observed rate of MMRs. We also find much lower occurrence of planets on retrograde orbits than the current observations of close-in planets suggest.
description: 12 pages, 9 figures, accepted for publication in ApJ
Disfunzioni mitocondriali e patologie nello spazio
Creators: Valentina Guglielmo
Publisher: name: Media Inaf
Year: 2020

Uno studio pubblicato oggi nella rivista Cell mostra come, alla base di molte patologie spaziali – dalle atrofie fisiche alle malattie neurologiche, a disfunzioni dei singoli organi o del sistema cardivascolare – ci sia una alterazione nei processi fisiologici dei mitocondri. Lo studio si avvale di diversi tessuti e cellule raccolte da esperimenti dedicati nello spazio, di dati sul sangue e sulle urine degli astronauti e si appoggia all’enorme database GeneLab della Nasa. Media Inaf ha intervistato il primo autore dello studio, Willian Abraham da Silveira, ricercatore della Queen's University Belfast
MPEC 2023-X278 : 2023 XX12
Creators: name: Minor Planet Center Staff
Publisher: name: The Minor Planet Center
Year: 2023
Subjects: subject: Small Solar System bodies
valueUri: http://astrothesaurus.org/uat/1469
subject: 2023 XX12

description: The Minor Planet Electronic Circulars contain information on unusual minor planets, routine data on comets and natural satellites, and occasional editorial announcements.  They are published on behalf of Division F of the International Astronomical Union by the Minor Planet Center, Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A.
Hyperfine splittings in the $b\bar{b}$ system
Creators: name: Radford, Stanley F.
name: Repko, Wayne W.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Recent measurements of the $η_b(1S)$, the ground state of the $b\bar{b}$ system, show the splitting between it and the $\Up(1S)$ to be 69.5$\pm$3.2 MeV, considerably larger than lattice QCD and potential model predictions, including recent calculations published by us. The models are unable to incorporate such a large hyperfine splitting within the context of a consistent description of the energy spectrum and decays. We demonstrate that in our model, which incorporates a relativistic kinetic energy term, a linear confining term including its scalar-exchange relativistic corrections, and the complete one-loop QCD short distance potential, such a consistent description, including the measured hyperfine splitting, can be obtained by not softening the delta function terms in the hyperfine potential. We calculate the hyperfine splitting to be 67.5 MeV.
description: 5 pages, 3 tables, text revisions
Ottimizzazione del punto di lavoro per Afrodite "empty-foto" a 6 periodi (AF11c)
Creators: name: Biagini, M. E.
name: Guiducci, S.
Publisher: name: INFN Open Access Repository
Year: 1986
Subjects: ADONE
Afrodite
AF11c

description: Ottimizzazione del punto di lavoro per Afrodite "empty-foto2 a 6 periodi (AF11c)
Il Sole trema? Macchie solari in arrivo
Creators: Marco Malaspina
Publisher: name: Media Inaf
Year: 2020

Grazie all’eliosismologia, una tecnica sviluppata dagli scienziati del National Solar Observatory statunitense negli anni Novanta, è possibile rilevare come le onde sonore interagiscano con la struttura interna del Sole, in particolare con i campi magnetici, e prevedere con qualche giorno di anticipo la comparsa di macchie solari
title: Ð­ÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ°Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ ÑÐµÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¸ ÐºÐ¾ÑÐµÐ»ÑÐ½Ð¾Ð¹ Ð² Ð¢Ð­Ð¦ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐºÐ¾ÑÐµÐ»ÑÐ½Ð¾Ð¹ â 11 Ð³. ÐÐ°ÑÑÐ¸Ð½Ð°)
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð¡Ð¸ÑÐµÐ½ÐºÐ¾, ÐÐ¸ÐºÐ¾Ð»Ð°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: 2016
Subjects: ÑÑÑÑÐºÑÑÑÐ° Ð³ÐµÐ½ÐµÑÐ°ÑÐ¸Ð¸ Ð Ð¾ÑÑÐ¸Ð¸
Ð¼Ð°Ð»Ð°Ñ ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð½Ð°Ñ ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÐºÐ°
ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð½Ð°Ñ Ð³ÐµÐ½ÐµÑÐ°ÑÐ¸Ñ
Ð¼Ð¸Ð½Ð¸-Ð¢Ð­Ð¦

description: ÐÑÐ» Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÐ½ Ð¾Ð±Ð·Ð¾Ñ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ñ Ð¾ÑÑÐ°ÑÐ»ÐµÐ¹ ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÐºÐ¸ Ð Ð¾ÑÑÐ¸Ð¸, Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³Ð° Ð¸ ÐÐµÐ½Ð¸Ð½Ð³ÑÐ°Ð´ÑÐºÐ¾Ð¹ Ð¾Ð±Ð»Ð°ÑÑÐ¸. ÐÑÐ»Ð¸ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÐºÐ¸, ÑÑÑÐµÑÑÐ²ÑÑÑÐ¸Ðµ Ð½Ð° Ð´Ð°Ð½Ð½ÑÐ¹ Ð¼Ð¾Ð¼ÐµÐ½Ñ Ð² Ð½Ð°ÑÐµÐ¹ ÑÑÑÐ°Ð½Ðµ, Ð¸ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½ÑÐµ Ð¿ÑÑÐ¸ Ð¸Ñ ÑÐµÑÐµÐ½Ð¸Ñ. ÐÐ¾Ð¼Ð¸Ð¼Ð¾ ÑÑÐ¾Ð³Ð¾, Ð±ÑÐ»Ð¾ ÑÐ°ÑÐºÑÑÑÐ¾ Ð¿Ð¾Ð½ÑÑÐ¸Ðµ Â«ÐºÐ¾Ð³ÐµÐ½ÐµÑÐ°ÑÐ¸ÑÂ». ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¸ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð¾ ÑÐµÑÐ½Ð¸ÐºÐ¾ - ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ðµ Ñ ÑÑÑÑÐ¾Ð¼ ÑÐ¸ÑÑÐµÐ¼Ð½Ð¾Ð³Ð¾ ÑÑÑÐµÐºÑÐ° ÑÐµÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¸ ÐºÐ¾ÑÐµÐ»ÑÐ½Ð¾Ð¹ Ð² Ð¼Ð¸Ð½Ð¸-Ð¢Ð­Ð¦.
Borexino: così brillano le stelle massive
Creators: Ufficio Comunicazione Infn
Publisher: name: Media Inaf
Year: 2020

Pubblicato oggi su Nature l’annuncio della prima rivelazione dei neutrini prodotti nel Sole dal ciclo CNO (carbonio-azoto-ossigeno). Lo studio è firmato dalla collaborazione scientifica Borexino, esperimento ai Laboratori nazionali del Gran Sasso dell’Istituto nazionale di fisica nucleare
title: Ð¤Ð¸Ð·Ð¸ÐºÐ°-1. ÐÐ°Ð·ÐµÑÐ½ÑÐµ Ð¿ÑÐ¸Ð±Ð¾ÑÑ ÑÐ°Ð´Ð¸Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ ÐºÐ¾Ð½ÑÑÐ¾Ð»Ñ
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð´Ð»Ñ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÑ Ð¿ÑÐ¾ÑÐµÑÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½ÑÑ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼ Ð²ÑÑÑÐµÐ³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ¾Ð² 16.03.01 Â«Ð¢ÐµÑ Ð½Ð¸ÑÐµÑÐºÐ°Ñ ÑÐ¸Ð·Ð¸ÐºÐ°Â» Ð¸ Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð¼Ð°Ð³Ð¸ÑÑÑÐ¾Ð² 16.04.01 Â«Ð¢ÐµÑ Ð½Ð¸ÑÐµÑÐºÐ°Ñ ÑÐ¸Ð·Ð¸ÐºÐ°Â»
titleType: Subtitle
Creators: name: ÐÑÐ¸Ð²Ð°Ð»Ð¾Ð², ÐÐ°Ð´Ð¸Ð¼
name: Ð¤Ð¾ÑÐ¸Ð°Ð´Ð¸, ÐÐ»ÐµÐºÑÐ°Ð½Ð´Ñ
name: Ð¨ÐµÐ¼Ð°Ð½Ð¸Ð½, ÐÐ°Ð»ÐµÑÐ¸Ð¹
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2016
Subjects: ÐÐ¾Ð½ÑÑÐ¾Ð»ÑÐ½Ð¾-Ð¸Ð·Ð¼ÐµÑÐ¸ÑÐµÐ»ÑÐ½ÑÐµ Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÑ Ð¸ Ð¿ÑÐ¸Ð±Ð¾ÑÑ Ð»Ð°Ð·ÐµÑÐ½ÑÐµ
ÐÐ¸Ð´Ð°ÑÑ

description: Ð Ð¿Ð¾ÑÐ¾Ð±Ð¸Ð¸ Ð¸Ð·Ð»Ð¾Ð¶ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð¿ÑÐ¸Ð·Ð½Ð°ÐºÐ¸ ÑÐ°Ð´Ð¸Ð¾Ð°ÐºÑÐ¸Ð²Ð½Ð¾Ð³Ð¾ Ð·Ð°Ð³ÑÑÐ·Ð½ÐµÐ½Ð¸Ñ Ð²Ð¾Ð·Ð´ÑÑÐ°, Ð¼ÐµÑÐ¾Ð´Ñ ÐºÐ¾Ð½ÑÑÐ¾Ð»Ñ, ÑÐ²Ð¾Ð¹ÑÑÐ²Ð° Ð¸Ð·Ð¾ÑÐ¾Ð¿Ð¾Ð² Ð¹Ð¾Ð´Ð°, Ð¿ÑÐ¸Ð½ÑÐ¸Ð¿Ñ Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ Ð»Ð¸Ð´Ð°ÑÐ¾Ð² Ð¸ Ð¿ÑÐ¸Ð¼ÐµÑÑ ÑÐ°ÑÑÐµÑÐ¾Ð² Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÐ¾Ð² Ð·Ð°Ð³ÑÑÐ·Ð½ÐµÐ½Ð¸Ñ, ÐºÐ¾ÑÐ¾ÑÑÐµ Ð¼Ð¾Ð³ÑÑ Ð±ÑÑÑ Ð¸Ð·Ð¼ÐµÑÐµÐ½Ñ Ñ Ð¿Ð¾Ð¼Ð¾ÑÑÑ ÑÐ°ÐºÐ¸Ñ Ð»Ð¸Ð´Ð°ÑÐ¾Ð². ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ ÑÐ¾Ð´ÐµÑÐ¶Ð¸Ñ Ð±Ð¾Ð»ÑÑÐ¾Ð¹ ÑÐ¿ÑÐ°Ð²Ð¾ÑÐ½ÑÐ¹ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð» Ð´Ð»Ñ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ ÑÐ°ÑÑÐµÑÐ½ÑÑ ÑÐ°Ð±Ð¾Ñ. ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð¸ Ð°ÑÐ¿Ð¸ÑÐ°Ð½ÑÐ¾Ð², Ð¾Ð±ÑÑÐ°ÑÑÐ¸ÑÑÑ Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸ÑÐ¼ 223200 Â«Ð¢ÐµÑÐ½Ð¸ÑÐµÑÐºÐ°Ñ ÑÐ¸Ð·Ð¸ÐºÐ°Â» Ð¸ 280200 Â«ÐÐ°ÑÐ¸ÑÐ° Ð¾ÐºÑÑÐ¶Ð°ÑÑÐµÐ¹ ÑÑÐµÐ´ÑÂ», Ð° ÑÐ°ÐºÐ¶Ðµ Ð´Ð»Ñ ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸ÑÑÐ¾Ð², ÑÐ°Ð±Ð¾ÑÐ°ÑÑÐ¸Ñ Ð² Ð¾Ð±Ð»Ð°ÑÑÐ¸ ÑÐµÑÐ½Ð¾ÑÑÐµÑÐ½Ð¾Ð¹ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸ Ð¸ ÑÐºÐ¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¼Ð¾Ð½Ð¸ÑÐ¾ÑÐ¸Ð½Ð³Ð°.
description: ÐÐµÑÐ°ÑÐ°ÐµÑÑÑ Ð¿Ð¾ ÑÐµÑÐµÐ½Ð¸Ñ Ð¡Ð¾Ð²ÐµÑÐ° Ð¿Ð¾ Ð¸Ð·Ð´Ð°ÑÐµÐ»ÑÑÐºÐ¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð£ÑÐµÐ½Ð¾Ð³Ð¾ ÑÐ¾Ð²ÐµÑÐ° Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¾Ð³Ð¾ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ° ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾.
Structure and deformations of strongly magnetized neutron stars with twisted torus configurations
Creators: name: Ciolfi, R.
name: Ferrari, V.
name: Gualtieri, L.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We construct general relativistic models of stationary, strongly magnetized neutron stars. The magnetic field configuration, obtained by solving the relativistic Grad-Shafranov equation, is a generalization of the twisted torus model recently proposed in the literature; the stellar deformations induced by the magnetic field are computed by solving the perturbed Einstein's equations; stellar matter is modeled using realistic equations of state. We find that in these configurations the poloidal field dominates over the toroidal field and that, if the magnetic field is sufficiently strong during the first phases of the stellar life, it can produce large deformations.
description: 10 pages, 5 figures. Minor changes to match the version published on MNRAS
Nature Intervention in Behavior Modification Therapy
Creators: name: Osei, Albert
Publisher: name: figshare
Year: 2023
Subjects: Educational psychology

description: This study investigated the treatment of four developmental deficits associated with autism spectrum disorder using bird-assisted activities. Using the principles of Applied Behavior Analysis, a reward gave the participant the opportunity to interact with the bird in the study and the absence of the bird was to punish a negative behavior. Tally marks were used to measure the number of times a behavior occurred within an observation period. The longitudinal study of a child with autism’s interest in birds was followed with therapeutic activities that brought about remarkable improvements in social, cognitive and communication skills. The study hypothesizes that nature intervention can improve pathological patterns in behavior such as self-stimulation, echolalia, lack of play skills and poor motor behavior.
Application of Graphics Processing Units to Search Pipeline for Gravitational Waves from Coalescing Binaries of Compact Objects
Creators: name: Chung, Shin Kee
name: Wen, Linqing
name: Blair, David
name: Cannon, Kipp
name: Datta, Amitava
Publisher: name: arXiv
Year: 2009
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We report a novel application of graphics processing units (GPUs) for the purpose of accelerating the search pipelines for gravitational waves from coalescing binaries of compact objects. A speed-up of 16 fold has been achieved compared with a single central processing unit (CPU). We show that substantial improvements are possible and discuss the reduction in CPU count required for the detection of inspiral sources afforded by the use of GPUs.
description: 15 pages, 7 figures
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÐºÐ¾Ð½ÑÐµÐ¿ÑÐ¸Ð¸ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½Ð¾Ð³Ð¾ Ð¼Ð°Ð³Ð°Ð·Ð¸Ð½Ð°
title: Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð¥ÑÑÐºÐ°, ÐÐ½Ð°ÑÑÐ°Ñ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Ð»ÐµÐºÑÑÐ¾Ð½Ð½ÑÐ¹ Ð¼Ð°Ð³Ð°Ð·Ð¸Ð½
Ð¸Ð½ÑÐµÑÐ½ÐµÑ-Ð¿ÑÐ¾Ð´Ð°Ð¶Ð¸
Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð¾Ð²Ð°Ñ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ
electronic shop
Internet sales
marketing activity

description: Ð ÑÐ¾Ð´Ðµ ÑÐ°Ð±Ð¾ÑÑ Ð¸Ð·ÑÑÐµÐ½Ñ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð°ÑÐ¿ÐµÐºÑÑ Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð¾Ð²Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð² ÑÐ¸ÑÑÐµÐ¼Ðµ Ð¸Ð½ÑÐµÑÐ½ÐµÑ-Ð¿ÑÐ¾Ð´Ð°Ð¶ Ð¼Ð°Ð³Ð°Ð·Ð¸Ð½Ð°, Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÑÐ»ÐµÐ¼ÐµÐ½ÑÑ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¸Ð½ÑÐµÑÐ½ÐµÑ-Ð¿ÑÐ¾Ð´Ð°Ð¶ Ð¼Ð°Ð³Ð°Ð·Ð¸Ð½Ð°, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð¾Ð²ÑÐµ ÑÐµÑÐµÐ½Ð¸Ñ Ð² ÑÐ¸ÑÑÐµÐ¼Ðµ Ð¸Ð½ÑÐµÑÐ½ÐµÑ-Ð¿ÑÐ¾Ð´Ð°Ð¶ Ð² ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ðµ. ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ðµ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ð¹ Ð±ÑÐ»Ð° Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð° Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾-ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ°Ñ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ° ÑÐ¾ÑÐ³Ð¾Ð²Ð¾Ð³Ð¾ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ ÐÐÐ Â«Ð¢ÐµÐºÑÑÐ¸Ð»ÑÐ¢Ð¾ÑÐ³ ÐÐ¡ÐÂ». Ð ÑÑÐµÑÑÐµÐ¹ Ð³Ð»Ð°Ð²Ðµ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ Ð¿ÑÐ¾Ð²Ð¾Ð´Ð¸ÑÑÑ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÐºÐ¾Ð½ÑÐµÐ¿ÑÐ¸Ð¸ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½Ð¾Ð³Ð¾ Ð¼Ð°Ð³Ð°Ð·Ð¸Ð½Ð° Ð´Ð»Ñ ÐÐÐ Â«Ð¢ÐµÐºÑÑÐ¸Ð»ÑÐ¢Ð¾ÑÐ³ ÐÐ¡ÐÂ».
description: During the studied theoretical aspects of marketing activity in the store online sales system, the main elements of the store online sales system and marketing solutions in the online sales system to trade. On the basis of theoretical research was carried out organizational and economic characteristics of commercial enterprise LLC "Tekstiltorg MSK".In the third chapter of final qualifying work carried out e-shop concept development for Â«Tekstiltorg MSK".
Role of GABAB Receptor and L-Arg in GABA-Induced Vasorelaxation in Non-diabetic and Streptozotocin-Induced Diabetic Rat Vessels
Creators: name: Fatemah Kharazmi
name: Nepton Soltani
name: Rezaei, Sana
name: Keshavarz, Mansoor
name: Farsi, Leila
Publisher: name: the Pasteur Institute of Iran
Year: 1996
Subjects: subject: Basic Sciences

description: Iranian Biomedical Journal (IBJ); ISSN 1028-852X
Grandi inondazioni nel passato di Marte
Creators: Valentina Guglielmo
Publisher: name: Media Inaf
Year: 2020

Non solo acqua liquida, ma vere e proprie mega alluvioni hanno segnato il passato di Marte. Le prove sono state individuate nel cratere Gale, il sito di esplorazione del rover Curiosity, e a causarle sarebbe stato un impatto meteoritico in grado di cambiare radicalmente – e per un breve periodo – le condizioni climatiche sul Pianeta rosso. Tutti i dettagli su Scientific Reports
Le prime foto “spaziali” di un altro pianeta: Marte
Creators: Roberto Della Ceca
Publisher: name: Media Inaf
Year: 2020

Ricorre sabato prossimo il 56esimo anniversario del lancio della sonda spaziale statunitense Mariner 4, avvenuto il 28 novembre 1964 da Cape Canaveral. Sue le prime immagini ravvicinate – 22 fotografie, una delle quali incompleta – del suolo marziano, ricorda oggi su Media Inaf Roberto Della Ceca, responsabile dell’Unità per la gestione dei progetti spaziali dell’Inaf
Incontri violenti al confine della Via Lattea
Creators: Maura Sandri
Publisher: name: Media Inaf
Year: 2020

Circa 700 milioni di anni fa, la Grande Nube di Magellano ha sfiorato il confine della Via Lattea, provocando violente perturbazioni sulla nostra galassia. Adesso si sta allontanando, ma il nostro disco di stelle, gas e polveri ne porta ancora il segno. Dallo studio del moto delle stelle, i ricercatori possono inferire le caratteristiche degli aloni di materia oscura che circondano le due galassie
Induced cosmology on a codimension-2 brane in a conical bulk
Creators: name: De Risi, G.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We study the cosmology of a 5-dimensional brane, which represents a regularization of a 4-dimensional codimension-2 brane, embedded in a conical bulk. The brane is assumed to be tensional, and to contain a curvature term. Cosmology is obtained by letting the brane move trough the bulk, and implementing dynamical junction conditions. Our results shows that, with suitable choices of the parameters, the resulting cosmological dynamics mimics fairly well standard 4-dimensional cosmology.
description: 14 pages, 1 figure. Corrections and clarifications troughout the text. Match the published version on NPB
title: Ð­Ð»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ°Ñ ÑÐ°ÑÑÑ Ð¿Ð¾Ð´ÑÑÐ°Ð½ÑÐ¸Ð¸ 220/110/35/10 ÐºÐ
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ³ÐµÐµÐ²Ð°, 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: 2016
Subjects: Ð¿Ð¾Ð´ÑÑÐ°Ð½ÑÐ¸Ñ
Ð°Ð²ÑÐ¾ÑÑÐ°Ð½ÑÑÐ¾ÑÐ¼Ð°ÑÐ¾Ñ
ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»Ð¸ÑÐµÐ»ÑÐ½Ð¾Ðµ ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð¾
substation
autotransformer
switchgear

description: Ð ÑÐ°Ð±Ð¾ÑÐµ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÑÐ°ÑÑÐ¸ Ð¿Ð¾Ð´ÑÑÐ°Ð½ÑÐ¸Ð¸. ÐÑÐ±ÑÐ°Ð½Ð° Ð¾Ð¿ÑÐ¸Ð¼Ð°Ð»ÑÐ½Ð°Ñ ÑÑÑÑÐºÑÑÑÐ½Ð°Ñ ÑÑÐµÐ¼Ð° Ð¸ Ð¾ÑÐ½Ð¾Ð²Ð½Ð¾Ðµ ÑÐ»ÐµÐºÑÑÐ¾Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ. Ð Ð°ÑÑÑÐ¸ÑÐ°Ð½Ñ ÑÐ¾ÐºÐ¸ ÐºÐ¾ÑÐ¾ÑÐºÐ¾Ð³Ð¾ Ð·Ð°Ð¼ÑÐºÐ°Ð½Ð¸Ñ. ÐÑÐ±ÑÐ°Ð½Ñ ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð°Ð¿Ð¿Ð°ÑÐ°ÑÑ Ð¸ Ð¿ÑÐ¾Ð²Ð¾Ð´Ð½Ð¸ÐºÐ¸. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° Ð³Ð»Ð°Ð²Ð½Ð°Ñ ÑÑÐµÐ¼Ð° ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÐ¾ÐµÐ´Ð¸Ð½ÐµÐ½Ð¸Ð¹ Ð¸ ÑÑÐµÐ¼Ð° ÑÐ¾Ð±ÑÑÐ²ÐµÐ½Ð½ÑÑ Ð½ÑÐ¶Ð´.
description: This paper focuses on designing the electrical system of a substation. The appropriate block diagram and the basic electrical equipment are presented; short circuit currents are calculated; electrical appliances and conductors are covered in this study. The main scheme of electrical connections, as well as auxiliaries schemes elaborated in the course of the work are presented.
Recent Star Formation in Low Metallicities. The Star-Forming Region NGC 346/N66 in the Small Magellanic Cloud from Near-Infrared VLT/ISAAC Observations
Creators: name: Gouliermis, Dimitrios A.
name: Bestenlehner, Joachim M.
name: Brandner, Wolfgang
name: Henning, Thomas
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We perform a photometric analysis on deep, seeing-limited near-IR VLT images of the region NGC 346/N66 and a nearby control field of the SMC in order to locate the centres of active high- and intermediate-mass star formation through the identification of near-IR bright objects as candidate stellar sources under formation.We use archived imaging data obtained with the high-resolution camera ISAAC at VLT of NGC 346/N66 and we construct the near-IR colour-magnitude (CMD) and colour-colour diagrams (C-CD) of all detected sources. We investigate the nature of all stellar populations in the observed CMDs, and we identify all stellar sources that show significant near-IR excess emission in the observed C-CD. We select, thus, the best candidates for being young stellar sources. Based on their near-IR colours we select 263 candidate young stellar sources. This sample comprises a variety of objects such as intermediate-mass PMS and Herbig Ae/Be stars and possibly massive YSOs, providing original near-IR colours for them. The spatial distribution of the selected candidate sources shows that they are located along the dusty filamentary structures of N66 seen in mid- and far-IR dust emission and agrees very well with that of previously detected candidate YSOs and PMS stars. Our study provides an original accurate set of near-IR colours for candidate young stellar sources. While this adds significant information on the star formation process in NGC 346/N66, it is still necessary to reveal the exact nature of these objects, a process that requires the combination of multi-wavelength data, so that complete Spectral Energy Distributions can be constructed for individual sources. This would be a quite important follow-up study to that presented here.
description: A&A in press. Low-resolution gray-scale figures. Full photometric catalog in JHKs of 2,506 sources in NGC 346, available in CDS
Secure Multi-Party Computation with a Dishonest Majority via Quantum Means
Creators: name: Loukopoulos, Klearchos
name: Browne, Daniel E.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We introduce a scheme for secure multi-party computation utilising the quantum correlations of entangled states. First we present a scheme for two-party computation, exploiting the correlations of a Greenberger-Horne-Zeilinger state to provide, with the help of a third party, a near-private computation scheme. We then present a variation of this scheme which is passively secure with threshold t=2, in other words, remaining secure when pairs of players conspire together provided they faithfully follow the protocol. We show that this can be generalised to computations of n-party polynomials of degree 2 with a threshold of n-1. The threshold achieved is significantly higher than the best known classical threshold, which satisfies the bound t
description: 8 pages, 1 figure, Revised to address referee comments, includes a clearer definition of security model, more secure protocols and improved analysis
Marte a Torino
Creators: Marco Malaspina
Publisher: name: Media Inaf
Year: 2020

Utilizzando una replica del rover Rosalind Franklin, i tecnici della missione ExoMars stanno simulando, nei locali del Rover Operations Control Center di Torino, tutte le attività previste durante il viaggio verso Marte e nei primi giorni sul suolo del Pianeta rosso. Nelle scorse settimane sono state provate tutte le fasi in programma fino alla discesa sul terreno
A study of a laboratory animal colony
Creators: name: McLeod, Melville Coburn-Emma
Publisher: name: University of British Columbia
Year: 2012

description: This thesis is a study of the small animal colonies operated by the animal nutrition laboratory in the Department of Animal Husbandry. The four animal units studied are the albino rat, albino mouse, guinea pig and rabbit. The management practices used for each species are described fully. They include the housing, feeding, breeding and control of disease methods utilized. The factors discussed in the housing of the animals are the space utilization per animal and the type of cages. In addition, scale drawings and illustrations of the cages and cage racks are included. The method of feeding and the formula of each ration for each species is reported. The system of breeding used in each of the colonies is described. Control of disease is discussed with reference to the sanitation procedures practised. Growth and production data are reported for each species and a comparison made with the data published in the literature for other colonies. The number of animals involved in the study are 1,700 rats, 258 mice, 73 guinea pigs and 85 rabbits. The growth data includes size of litter, birth weights and weekly weights there after until weaning age. The production data comprises the percentage fertility and percentage weaned. In addition the results of a cost survey is reported. The cost per animal for each species includes the cost of housing, feeding and labour. The results reported here are comparable to those reported elsewhere.
Chang’e-5: un pezzo di Luna sulla Via della seta
Creators: Luca Nardi
Publisher: name: Media Inaf
Year: 2020

Il lanciatore Lunga Marcia 5 è decollato alle 21:31 ora italiana di oggi, lunedì 23 novembre, con a bordo la sonda Chang’e-5. È il più recente e complesso passo del programma lunare cinese. Obiettivo della missione: prelevare e riportare a casa alcuni frammenti di roccia lunare, andando a riempire il vuoto lasciato dalle missioni Apollo
The von Neumann entropy of networks
Creators: name: Passerini, Filippo
name: Severini, Simone
Publisher: name: arXiv
Year: 2008
Subjects: subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: Molecular Networks (q-bio.MN)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences
subject: FOS: Biological sciences

description: We normalize the combinatorial Laplacian of a graph by the degree sum, look at its eigenvalues as a probability distribution and then study its Shannon entropy. Equivalently, we represent a graph with a quantum mechanical state and study its von Neumann entropy. At the graph-theoretic level, this quantity may be interpreted as a measure of regularity; it tends to be larger in relation to the number of connected components, long paths and nontrivial symmetries. When the set of vertices is asymptotically large, we prove that regular graphs and the complete graph have equal entropy, and specifically it turns out to be maximum. On the other hand, when the number of edges is fixed, graphs with large cliques appear to minimize the entropy.
description: 6 pages, 3 figures
Aperte le iscrizioni alle Olimpiadi di astronomia
Creators: Daria Guidetti
Publisher: name: Media Inaf
Year: 2020

Le scuole possono iscriversi a partire da oggi, lunedì 23 novembre, dalle ore 17:00, ed entro il prossimo 7 dicembre. Se permanessero le attuali restrizioni legate al Covid-19, la gara si svolgerà in modalità online e ogni scuola potrà usare la propria piattaforma per la Dad. Nell’autunno 2021 a Matera la finale internazionale
Sulle tracce di un “nuovo tipo” di elettroni
Creators: Marco Malaspina
Publisher: name: Media Inaf
Year: 2020

Perché alcuni materiali emettono elettroni con un’energia molto specifica? Come quelli a 3.7 elettronvolt osservati fuoriuscire dalla grafite? Un team di fisici del Politecnico di Vienna ha ora trovato una risposta. Media Inaf ha intervistato una delle scienziate che hanno firmato il risultato, Alessandra Bellissimo
Costante di Hubble sotto la lente gravitazionale
Creators: Valentina Guglielmo
Publisher: name: Media Inaf
Year: 2020

Un nuovo metodo per stimare la costante di Hubble chiamato “time-delay cosmography” e basato sul fenomeno fisico delle lenti gravitazionali forti è stato messo a punto dal team internazionale TdCosmo. La nuova tecnica di misura ha dimostrato la sua potenzialità nello stimare la costante con un’accuratezza e una precisione senza precedenti. Ne parliamo con Chiara Spiniello, coautrice dell’articolo pubblicato oggi su A&A
MyHealthMyData (MHMD): Deliverable 10.6 - Second dissemination event
Creators: name: Rizzo, Anna
Publisher: name: Zenodo
Year: 2019
Subjects: Dissemination
communication
event
demo
public
presentation

description: The present deliverable is meant to report about the second of the two major dissemination events organised by the consortium to present the project and demo its prototype system to general public and peers in the research, clinical and industry sectors. Besides the EU Digital Assembly (Sofia, 25-26 June 2018), reported in D10.3 - First dissemination event as ‘first dissemination event’ for being the first public demo of the MHMD system, another major opportunity for project dissemination was offered by ICT 2018 (Vienna, 4-6 December 2018), the research and innovation participatory event organised by the European Commission and the Austrian Presidency of the Council of the European Union, which attracted about 4,800 visitors among science community members, policymakers and citizens. The report will thus detail the event and Consortium participation, including a project booth – including posters, brochures and a live system demo - and the three networking sessions organised within the event, along with other dissemination and outreach activities.

Along with that, the report will also give an account of the other minor dissemination events organised/attended by the whole consortium or its partners (individually) in the second reporting period (M19-M36), as well as planned for the next months until the end of the project. These include research conferences and public networking events in the field of health IT, personal data, AI, blockchain and ICT for health, organised at institutional or industry level. There, Project Coordinator and other Consortium partners have presented the project or its emerging innovations (e.g., synthetic data, homomorphic encryption, etc.) with relevant academic communities, industry stakeholders, policy makers and mass media representatives, chaired and animated sessions on relevant themes (e.g., personal data, health data, blockchain in health, ICT for health), and posed the base for further cross-fertilisation, feedback gathering from peers in the clinical and IT community and possible exploitation routes for the future project sustainability.
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¾Ñ ÑÐ°Ð½Ñ ÑÑÑÐ´Ð° Ð² ÐÐÐ Â«ÐÐÐ¢ÐÐ ÐÐÐ ÐÐÐ¢Â»
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¾Ð»ÑÐ±ÐµÐ², 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: 2016
Subjects: ÑÐ¸ÑÑÐµÐ¼Ð° ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¾Ñ ÑÐ°Ð½Ð¾Ð¹ ÑÑÑÐ´Ð°
Ð¡Ð£ÐÐ¢
Ð¿ÑÐ¾ÑÐµÑÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½ÑÐµ ÑÐ¸ÑÐºÐ¸
occupational risks
OSH management system

description: Ð¦ÐµÐ»Ñ ÑÐ°Ð±Ð¾ÑÑ - Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ ÑÑÐµÐ±Ð¾Ð²Ð°Ð½Ð¸Ð¹ Ð½Ð¾ÑÐ¼Ð°ÑÐ¸Ð²Ð½Ð¾-Ð¿ÑÐ°Ð²Ð¾Ð²ÑÑ Ð°ÐºÑÐ¾Ð², ÑÐ¾Ð´ÐµÑÐ¶Ð°ÑÐ¸Ñ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½ÑÐµ Ð½Ð¾ÑÐ¼Ð°ÑÐ¸Ð²Ð½ÑÐµ ÑÑÐµÐ±Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¾ÑÑÐ°Ð½Ñ ÑÑÑÐ´Ð°, ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° ÑÐ¸ÑÑÐµÐ¼Ð° ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¾ÑÑÐ°Ð½Ð¾Ð¹ ÑÑÑÐ´Ð° Ð´Ð»Ñ Ð¿Ð°ÑÐºÐµÑÐ½Ð¾Ð¹ ÑÐ¸ÑÐ¼Ñ ÐÐÐÂ«ÐÐÐ¢ÐÐ ÐÐÐ ÐÐÐ¢Â».
Ion-beam driven dust ion-acoustic solitary waves in dusty plasmas
Creators: name: Adhikary, N. C.
name: Misra, A. P.
name: Bailung, H.
name: Chutia, J.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Plasma Physics (physics.plasm-ph)
subject: FOS: Physical sciences

description: The nonlinear propagation of small but finite amplitude dust ion-acoustic waves (DIAWs) in an ion-beam driven plasma with Boltzmannian electrons, positive ions and stationary charged dust grains, is studied by using the standard reductive perturbation technique (RPT). It is shown that there exist two critical values $(γ_{c1}$ and $γ_{c2})$ of ion-beam to ion phase speed ratio $(γ)$, beyond which the beam generated solitons are not possible. The effects of the parameters, namely $γ$, the ratio of the ion-beam to plasma ion density $(μ_{i})$, the dust to ion density ratio $(μ_{d})$ as well as the ion-beam to plasma ion mass ratio $(μ)$ on both the amplitude and width of the stationary DIAWs are analyzed numerically, and applications of the results to laboratory ion-beam as well as space plasmas (e.g., auroral plasmas) are explained.
description: 4 pages, 6 figures
Instanton Corrections to the Universal Hypermultiplet and Automorphic Forms on SU(2,1)
Creators: name: Bao, Ling
name: Kleinschmidt, Axel
name: Nilsson, Bengt E. W.
name: Persson, Daniel
name: Pioline, Boris
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Number Theory (math.NT)
subject: FOS: Physical sciences
subject: FOS: Mathematics

description: The hypermultiplet moduli space in Type IIA string theory compactified on a rigid Calabi-Yau threefold X, corresponding to the "universal hypermultiplet", is described at tree-level by the symmetric space SU(2,1)/(SU(2) x U(1)). To determine the quantum corrections to this metric, we posit that a discrete subgroup of the continuous tree-level isometry group SU(2,1), namely the Picard modular group SU(2,1;Z[i]), must remain unbroken in the exact metric -- including all perturbative and non perturbative quantum corrections. This assumption is expected to be valid when X admits complex multiplication by Z[i]. Based on this hypothesis, we construct an SU(2,1;Z[i])-invariant, non-holomorphic Eisenstein series, and tentatively propose that this Eisenstein series provides the exact contact potential on the twistor space over the universal hypermultiplet moduli space. We analyze its non-Abelian Fourier expansion, and show that the Abelian and non-Abelian Fourier coefficients take the required form for instanton corrections due to Euclidean D2-branes wrapping special Lagrangian submanifolds, and to Euclidean NS5-branes wrapping the entire Calabi-Yau threefold, respectively. While this tentative proposal fails to reproduce the correct one-loop correction, the consistency of the Fourier expansion with physics expectations provides strong support for the utility of the Picard modular group in constraining the quantum moduli space.
description: 61 pages, (v2) typos corrected, references added, clarification regarding the fact that our analysis applies to rigid Calabi-Yau 3-folds that admit complex multiplication by the Gaussian integers Z[i], (v3) references added, one-loop discrepancy revised (but still discrepant), other cosmetic changes, (v4) final version, published in CNTP
title: ÐÐ°ÐºÐ¾Ð½Ð¾Ð´Ð°ÑÐµÐ»ÑÐ½ÑÐ¹ Ð¿ÑÐ¾ÑÐµÑÑ Ð² Ð Ð¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð¹ Ð¤ÐµÐ´ÐµÑÐ°ÑÐ¸Ð¸
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð¡Ð¾ÐºÐ¾Ð»Ð¾Ð²Ð°, ÐÐ°ÑÑ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: Ð·Ð°ÐºÐ¾Ð½Ð¾Ð´Ð°ÑÐµÐ»ÑÐ½ÑÐ¹ Ð¿ÑÐ¾ÑÐµÑÑ
ÑÐµÐ¾ÑÐµÑÐ¸ÐºÐ¾-Ð¿ÑÐ°Ð²Ð¾Ð²ÑÐµ Ð¾ÑÐ½Ð¾Ð²Ñ
Ð·Ð°ÐºÐ¾Ð½Ð¾Ð´Ð°ÑÐµÐ»ÑÐ½Ð°Ñ Ð¸Ð½Ð¸ÑÐ¸Ð°ÑÐ¸Ð²Ð°
legislative process
teoretiko-legal bases
legislative initiative

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑÑÑ ÑÐµÐ¾ÑÐµÑÐ¸ÐºÐ¾-Ð¿ÑÐ°Ð²Ð¾Ð²ÑÐµ Ð¾ÑÐ½Ð¾Ð²Ñ Ð·Ð°ÐºÐ¾Ð½Ð¾Ð´Ð°ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÑÐµÑÑÐ°, ÑÑÐ±ÑÐµÐºÑÑ Ð·Ð°ÐºÐ¾Ð½Ð¾Ð´Ð°ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÑÐµÑÑÐ°. Ð ÑÐ°Ð±Ð¾ÑÐµ Ð¸ÑÑÐ»ÐµÐ´ÑÑÑÑÑ ÐºÐ¾Ð½ÑÑÐ¸ÑÑÑÐ¸Ð¾Ð½Ð½Ð¾-Ð¿ÑÐ°Ð²Ð¾Ð²ÑÐµ Ð¾ÑÐ½Ð¾Ð²Ñ ÑÐµÐ´ÐµÑÐ°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð·Ð°ÐºÐ¾Ð½Ð¾Ð´Ð°ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÑÐµÑÑÐ°. Ð Ð°ÑÐºÑÑÐ²Ð°ÐµÑÑÑ ÑÐ¿ÐµÑÐ¸ÑÐ¸ÐºÐ° ÑÑÐ°Ð´Ð¸Ð¹ Ð·Ð°ÐºÐ¾Ð½Ð¾Ð´Ð°ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÑÐµÑÑÐ° Ð² Ð Ð¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð¹ Ð¤ÐµÐ´ÐµÑÐ°ÑÐ¸Ð¸. Ð¦ÐµÐ»Ñ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ - Ð¸Ð·ÑÑÐµÐ½Ð¸Ðµ Ð¸ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ñ, Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ñ Ð¾ÑÐ½Ð¾Ð² Ð¸ Ð¿ÑÐ°ÐºÑÐ¸ÐºÐ¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð¸ Ð¿ÑÐ¸Ð½ÑÑÐ¸Ñ ÑÐµÐ´ÐµÑÐ°Ð»ÑÐ½ÑÑ Ð·Ð°ÐºÐ¾Ð½Ð¾Ð².ÐÐ±ÑÐµÐºÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ - Ð¿ÑÐ°Ð²Ð¾Ð²Ð°Ñ Ð¿ÑÐ¸ÑÐ¾Ð´Ð° Ð·Ð°ÐºÐ¾Ð½Ð¾Ð´Ð°ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÑÐµÑÑÐ° Ð¸ Ð²Ð¾Ð·Ð½Ð¸ÐºÐ°ÑÑÐ¸Ñ Ð² ÑÐ¾Ð´Ðµ ÐµÐ³Ð¾ Ð¾ÑÑÑÐµÑÑÐ²Ð»ÐµÐ½Ð¸Ñ Ð¾Ð±ÑÐµÑÑÐ²ÐµÐ½Ð½ÑÑ Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸Ð¹. ÐÑÐµÐ´Ð¼ÐµÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ - Ð·Ð°ÐºÐ¾Ð½Ð¾Ð´Ð°ÑÐµÐ»ÑÐ½ÑÐ¹ Ð¿ÑÐ¾ÑÐµÑÑ Ð² Ð Ð¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð¹ Ð¤ÐµÐ´ÐµÑÐ°ÑÐ¸Ð¸.
description: In this final thesis teoretiko-legal basics of legislative process, subjects of legislative process are covered. In work constitutional and legal bases of federal legislative process are investigated. Specifics of stages of legislative process in the Russian Federation reveal. Research objective - study and improvement of theoretical and methodological bases and practice of development and adoption of federal laws. Object of research - the legal nature of the legislative process and arising in the course of its implementation of public relations.
Dalla supernova al suo resto: lo studio di Palermo
Creators: Mario Guarcello
Publisher: name: Media Inaf
Year: 2020

I risultati di simulazioni magneto-idrodinamiche tridimensionali recentemente sviluppate da un team di astrofisici guidato da Antonio Tutone dell’Università di Palermo, associato all’Istituto nazionale di astrofisica, hanno permesso di ricostruire i legami tra i resti di supernove e i loro eventi progenitori
title: ÐÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð¾-Ð°Ð¿Ð¿Ð°ÑÐ°ÑÐ½ÑÐµ Ð¸Ð½ÑÐµÑÑÐµÐ¹ÑÑ ÑÐ°Ð´Ð¸Ð¾Ð¼Ð¾Ð´ÐµÐ¼Ð¾Ð²Ð´Ð»Ñ Ð²ÑÑÑÐ°Ð¸Ð²Ð°ÐµÐ¼ÑÑ ÑÐ°Ð´Ð¸Ð¾Ð¼Ð¾Ð´ÑÐ»ÐµÐ¹
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ°Ð±ÑÐ¸ÐµÐ»Ð¾Ð², 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: 2016
Subjects: ÑÐ¸Ð¿ÑÐµÑ Atheros AR5213
Ð¿ÑÐµÑÑÐ²Ð°Ð½Ð¸Ðµ

description: Ð Ð°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐµ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½ÑÑ Ð¸Ð½ÑÐµÑÑÐµÐ¹ÑÐ¾Ð² Ð´Ð»Ñ ÑÐ°Ð´Ð¸Ð¾Ð¼Ð¾Ð´ÑÐ»ÐµÐ¹ Ð²ÑÑÑÐ°Ð¸Ð²Ð°ÐµÐ¼ÑÑ Ð¿Ð¾Ð´ÑÐ¸ÑÑÐµÐ¼. Ð ÑÐ¸Ð»Ñ Ð½ÐµÐ´Ð¾ÑÑÐ°ÑÐ¾ÑÐ½Ð¾Ð¹ Ð´Ð¾ÐºÑÐ¼ÐµÐ½ÑÐ°ÑÐ¸Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð°ÑÑÐ²Ð°ÑÑ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð¾Ðµ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ðµ Ð´Ð»Ñ ÐºÐ¾Ð½ÐºÑÐµÑÐ½Ð¾Ð³Ð¾ ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð° Ð´Ð¾Ð²Ð¾Ð»ÑÐ½Ð¾ ÑÑÐ¶ÐµÐ»Ð¾ Ð¸ ÑÑÐµÐ±ÑÐµÑ ÑÑÐ°ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð¸Ð·ÑÑÐµÐ½Ð¸Ñ Ð¸Ð¼ÐµÑÑÐ¸ÑÑÑ Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ¾Ð². ÐÑÐ½Ð¾Ð²Ð½Ð°Ñ Ð·Ð°Ð´Ð°ÑÐ° - Ð¸Ð·ÑÑÐ¸ÑÑ Ð¸Ð¼ÐµÑÑÑÑÑÑ Ð´Ð¾ÐºÑÐ¼ÐµÐ½ÑÐ°ÑÐ¸Ñ Ð´Ð»Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·ÑÐµÐ¼Ð¾Ð³Ð¾ ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð°, Ð²ÑÑÑÐ½Ð¸ÑÑ, ÐºÐ°ÐºÐ¾Ð¹ ÑÑÐ½ÐºÑÐ¸Ð¾Ð½Ð°Ð» Ð´Ð°Ð½Ð½Ð¾Ðµ ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð¾ Ð¿Ð¾Ð´Ð´ÐµÑÐ¶Ð¸Ð²Ð°ÐµÑ Ð¸ Ð¿Ð¾ÑÑÑÐ¾Ð¸ÑÑ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½ÑÐµ Ð¸Ð½ÑÐµÑÑÐµÐ¹ÑÑ, ÐºÐ¾ÑÐ¾ÑÑÐµ Ð¼Ð¾Ð³Ð»Ð¸ Ð±Ñ Ð±ÑÑÑ Ð¿Ð¾Ð»ÐµÐ·Ð½Ñ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÑÐ¸ÐºÐ°Ð¼. Ð ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½ Ð¼Ð¾Ð´ÑÐ»Ñ Ð°Ð¿Ð¿Ð°ÑÐ°ÑÑÑÑ AR5213.
Polycyclic aromatic hydrocarbon processing in a hot gas
Creators: name: Micelotta, E. R.
name: Jones, A. P.
name: Tielens, A. G. G. M.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Context: PAHs are thought to be a ubiquitous and important dust component of the interstellar medium. However, the effects of their immersion in a hot (post-shock) gas have never before been fully investigated. Aims: We study the effects of energetic ion and electron collisions on PAHs in the hot post-shock gas behind interstellar shock waves. Methods: We calculate the ion-PAH and electron-PAH nuclear and electronic interactions, above the carbon atom loss threshold, in H II regions and in the hot post-shock gas, for temperatures ranging from 10^3 to 10^8 K. Results: PAH destruction is dominated by He collisions at low temperatures (T < 3x10^4 K), and by electron collisions at higher temperatures. Smaller PAHs are destroyed faster for T < 10^6 K, but the destruction rates are roughly the same for all PAHs at higher temperatures. The PAH lifetime in a tenuous hot gas (n_H ~ 0.01 cm^-3, T ~ 10^7 K), typical of the coronal gas in galactic outflows, is found to be about thousand years, orders of magnitude shorter than the typical lifetime of such objects. Conclusions: In a hot gas, PAHs are principally destroyed by electron collisions and not by the absorption of X-ray photons from the hot gas. The resulting erosion of PAHs occurs via C_2 loss from the periphery of the molecule, thus preserving the aromatic structure. The observation of PAH emission from a million degree, or more, gas is only possible if the emitting PAHs are ablated from dense, entrained clumps that have not yet been exposed to the full effect of the hot gas.
description: 16 pages, 11 figures, 3 tables, typos corrected and PAH acronym in the title substituted with full name to match version published in Astronomy and Astrophysics