cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð±Ð¸Ð·Ð½ÐµÑ-Ð¿Ð»Ð°Ð½Ð° Ð¿Ð¾ Ð´Ð¸Ð²ÐµÑÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÑÐºÑÑÐºÐ¸Ð½, ÐÐ²Ð°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: 2016
Subjects: Ð´Ð¸Ð²ÐµÑÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¸Ñ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð°
Ð±Ð¸Ð·Ð½ÐµÑ Ð¿Ð»Ð°Ð½ Ð¿ÐµÑÐµÐ¿ÑÐ¾ÑÐ¸Ð»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ
Ð°Ð½ÑÐ¸ÐºÑÐ¸Ð·Ð¸ÑÐ½Ð¾Ðµ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ
diversification of production
business plan redevelopment
crisis management

description: Ð Ð¿ÐµÑÐ²Ð¾Ð¹ Ð³Ð»Ð°Ð²Ðµ Ð¾Ð¿Ð¸ÑÑÐ²Ð°ÐµÑÑÑ Ð¾ÑÐ½Ð¾Ð²Ð½Ð°Ñ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ ÐÐÐ Â«ÐÑÐ¾Ð½Ð°Ð¡ÑÑÐ¾Ð¹Ð¡ÐµÑÐ²Ð¸ÑÂ», Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÑÐµÑÑÑ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÑÑÑÐºÑÑÑÐ°. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐ¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸. ÐÑÐ¸Ð²ÐµÐ´ÐµÐ½Ð¾ Ð¾Ð¿Ð¸ÑÐ°Ð½Ð¸Ðµ ÑÑÑÐµÑÑÐ²ÑÑÑÐµÐ¹ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ. ÐÑÑÐ²Ð»ÐµÐ½Ñ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ, ÑÑÐ¾ÑÐ¼ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ñ ÑÐµÐ»Ð¸ Ð¸ Ð·Ð°Ð´Ð°ÑÐ¸ Ð´Ð°Ð»ÑÐ½ÐµÐ¹ÑÐµÐ³Ð¾ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ. ÐÐ¾ Ð²ÑÐ¾ÑÐ¾Ð¹ Ð³Ð»Ð°Ð²Ðµ ÑÐ°ÑÐºÑÑÐ²Ð°ÑÑÑÑ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð°ÑÐ¿ÐµÐºÑÑ Ð±Ð¸Ð·Ð½ÐµÑ Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸ÑÑ, ÑÑÐ¾ÑÐ¼ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð¿ÑÑÐ¸ ÑÐµÑÐµÐ½Ð¸Ñ Ð¿Ð¾ÑÑÐ°Ð²Ð»ÐµÐ½Ð½ÑÑ Ð·Ð°Ð´Ð°Ñ. Ð¢ÑÐµÑÑÑ Ð³Ð»Ð°Ð²Ð° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐµ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹ Ð¿Ð¾ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐµ Ð±Ð¸Ð·Ð½ÐµÑ-Ð¿Ð»Ð°Ð½Ð° Ð¿Ð¾ Ð´Ð¸Ð²ÐµÑÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ. ÐÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ñ Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ¸ ÑÐ¸Ð½Ð°Ð½ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ Ð´Ð°Ð½Ð½ÑÑ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹. Ð Ð°ÑÑÑÐ¸ÑÐ°Ð½Ð° ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ°Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ Ð¾Ñ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ Ð¿ÑÐµÐ´Ð»Ð°Ð³Ð°ÐµÐ¼ÑÑ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹.
description: The first Chapter describes the main activity of OOO "Constrainers", analyzes the organizational structure. Conducted financial analysis of economic activities. The description of the existing management system. Identified problems, defined objectives and tasks for further research. The second Chapter describes the main theoretical aspects of business planning at the enterprises, the basic ways of the decision of tasks in view. The third Chapter is devoted to the development of measures for the development of a business plan for diversification of the enterprise. Identified funding sources to implement these activities. Calculated economic efficiency from implementation of the proposed activities.
La storia turbolenta delle galassie, in un disco
Creators: Redazione Media Inaf
Publisher: name: Media Inaf
Year: 2016

Due studi guidati da astronomi italiani con osservazioni da terra e dallo spazio hanno permesso di misurare l'età delle stelle che compongono i dischi nucleari al centro delle galassie, da cui si può dedurre da quanto tempo una galassia sta evolvendo in tranquillità. I risultati saranno pubblicati sul prossimo numero di Monthly Notices of the Royal Astronomical Society
Unitarity bound for gluon shadowing
Creators: name: Kopeliovich, B. Z.
name: Levin, E.
name: Potashnikova, I. K.
name: Schmidt, Ivan
Publisher: name: arXiv
Year: 2008
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Although at small Bjorken x gluons originated from different nucleons in a nucleus overlap in the longitudinal direction, most of them are still well separated in the transverse plane, therefore cannot fuse. For this reason the gluon density in nuclei cannot drop at small x below a certain bottom bound, which we evaluated in a model independent manner assuming the maximal strength of gluon fusion. We also calculated gluon shadowing in the saturated regime using on the Balitsky-Kovchegov equation, and found the nuclear ratio to be well above the unitarity bound. The recently updated analysis of parton distributions in nuclei \cite{eps08} including RHIC data on high-pT hadron production at forward rapidities, led to astonishingly strong gluon shadowing, which is far beyond the unitarity bound. This indicates a misconception in the interpretation of the nuclear suppression observed at HRIC.
description: 7 pages, 4 figures
Spazio, cresce l’Italia ma rallenta ExoMars
Creators: Redazione Media Inaf
Publisher: name: Media Inaf
Year: 2016

Il nostro paese, terzo finanziatore fra i membri dell’Agenzia Spaziale Europea dopo Germania e Francia, rafforza il proprio impegno nello spazio, arrivando a 512 milioni di euro. Incertezze nei finanziamenti rischiano però di far slittare di due anni il lancio della seconda missione ExoMars
Высшее образование сегодня,Выпуск 9 (2018) 2018
Creators: name: Автономная некоммерческая организация высшего образования «Российский новый университет»
Publisher: name: Автономная некоммерческая организация высшего образования «Российский новый университет»
Year: 2018

description: Высшее образование сегодня,Выпуск 9 (2018) 2018
Vacuum energy density kicked by the electroweak crossover
Creators: name: Klinkhamer, F. R.
name: Volovik, G. E.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Using q-theory, we show that the electroweak crossover can generate a remnant vacuum energy density Λ\sim E_{ew}^8 / E_{planck}^4, with effective electroweak energy scale E_{ew} \sim 10^{3} GeV and reduced Planck-energy scale E_{planck} \sim 10^{18} GeV. The obtained expression for the effective cosmological constant Λmay be a crucial input for the suggested solution by Arkani-Hamed et al. of the triple cosmic coincidence puzzle (why the orders of magnitude of the energy densities of vacuum, matter, and radiation are approximately the same in the present Universe).
description: 16 pages; v6: published version
A theoretical study of magnetic self-pinching in a semiconductor
Creators: name: Strome, William Murray
Publisher: name: University of British Columbia
Year: 2011

description: The subject of this thesis is the theoretical investigation of the possibility of observing magnetic self-pinching of the hole-electron plasma present in a semiconductor. The steady-state pinch equations are derived for conditions which might be expected to prevail in such a plasma, both with and without the effects of generation and recombination. Recent reports of the observance of pinch effect in indium antimonide operated under avalanche breakdown conditions are discussed. All these reports based their claim of observing pinch on slight changes in overall resistance of the sample, a purely secondary effect of self- pinching. It is indicated that a plasma generated by avalanching is a poor medium from which to compare experimental results with available theory. Hence it is concluded that the above reports offer only circumstantial evidence of self-pinching. Finally, an experimental arrangement is suggested with which one should be able to determine unambiguously whether or not pinch can occur in semiconductors.
MOKA: a new tool for Strong Lensing Studies
Creators: name: Giocoli, Carlo
name: Meneghetti, Massimo
name: Bartelmann, Matthias
name: Moscardini, Lauro
name: Boldrin, Michele
Publisher: name: INFN Open Access Repository
Year: 2011

description: Strong gravitational lensing is a powerful tool for probing the matter
distribution in the cores of massive dark matter haloes. Recent and ongoing
analyses of galaxy cluster surveys (MACS, CFHTLS, SDSS, SGAS, CLASH, LoCuSS)
have adressed the question of the nature of the dark matter distribution in
clusters. N-body simulations of cold dark-matter haloes consistently find that
haloes should be characterized by a concentration-mass relation that decreases
monotonically with halo mass, and populated by a large amount of substructures,
representing the cores of accreted progenitor halos. It is important for our
understanding of dark matter to test these predictions. We present MOKA, a new
algorithm for simulating the gravitational lensing signal from cluster-sized
haloes. It implements the most recent results from numerical simulations to
create realistic cluster-scale lenses with properties independent of numerical
resolution. We perform systematic studies of the strong lensing cross section
as a function of halo structures. We find that the strong lensing cross
sections depend most strongly on the concentration and on the inner slope of
the density profile of a halo, followed in order of importance by halo
triaxiality and the presence of a bright central galaxy.
Magnetohydrodynamic turbulence in a strongly magnetised plasma
Creators: name: Sridhar, S.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: I present a review of incompressible magnetohydrodynamic (MHD) turbulence in a strongly magnetised plasma. The approach is phenomenological even where a more rigorous theory is available, so that a reader armed with paper, pencil and some determination may be able to work through most of the physics. The focus is on the inertial-range spectra for very large (fluid and magnetic) Reynolds numbers. These theories of the inertial-range are built on two important facts: (i) Kraichnan's insight that the turbulent cascades are a result of nonlinear interactions between oppositely directed wavepackets of Elsasser fields; (ii) these oppositely directed wavepackets do not exchange energy, but contribute only to changing each other's spatial structures. I begin with a description and critique of the Iroshnikov-Kraichnan theory, and explore the fundamental departures necessitated by the anisotropic nature of the turbulence. Derivations of the inertial-range spectra of four regimes of MHD turbulence -- the balanced weak, balanced strong, imbalanced weak and the imbalanced strong cascades -- are then presented. The need for studying the spectra of imbalanced turbulence when the waves on the outer scale have a short correlation time is briefly discussed.
description: invited review, submitted to Astronomische Nachrichten
Phenomenology from SIDIS and $e^+e^-$ multiplicities
Creators: name: Bacchetta, Alessandro
name: Echevarria, Miguel G.
name: Radici, Marco
name: Signori, Andrea
Publisher: name: INFN Open Access Repository
Year: 2014

description: This study is part of a project to investigate the transverse momentum
dependence in parton distribution and fragmentation functions, analyzing
(semi-)inclusive high-energy processes within a proper QCD framework. We
calculate the transverse-momentum-dependent (TMD) multiplicities for $e^+e^-$
annihilation into two hadrons (considering different combinations of pions and
kaons) aiming to investigate the impact of intrinsic and radiative partonic
transverse momentum and their mixing with flavor. Different descriptions of the
non-perturbative evolution kernel are available on the market and there are 200
sets of flavor configurations for the unpolarized TMD fragmentation functions
(FFs) resulting from a Monte Carlo fit of Semi-Inclusive Deep-Inelastic
Scattering (SIDIS) data at Hermes. We build our predictions of $e^+e^-$
multiplicities relying on this rich phenomenology. The comparison of these
calculations with future experimental data (from Belle and Babar
collaborations) will shed light on non-perturbative aspects of hadron
structure, opening important insights into the physics of spin, flavor and
momentum structure of hadrons.
Transverse single-spin asymmetries in proton-proton collisions at the
  AFTER@LHC experiment in a TMD factorisation scheme
Creators: name: M. Anselmino
name: U. D'Alesio
name: S. Melis
Publisher: name: INFN Open Access Repository
Year: 2015

description: The inclusive large-$p_T$ production of a single pion, jet or direct photon,
together with Drell-Yan processes, are considered for proton-proton collisions
in the kinematical range expected for the fixed-target experiment AFTER,
proposed at LHC. For all these processes, predictions are given for the
transverse single-spin asymmetry, $A_N$, computed according to a Generalised
Parton Model previously discussed in the literature and based on TMD
factorisation. Comparisons with the results of a collinear twist-3 approach,
recently presented, are made and discussed.
Pianeti in fila per cinque
Creators: Francesca Aloisio
Publisher: name: Media Inaf
Year: 2016

Per i più mattinieri lo spettacolo offerto dall’allineamento di cinque pianeti definiti “brillanti”, perché visibili ad occhio nudo, sarà osservabile anche dal nostro emisfero fino verso la metà del mese prossimo. Circa un’ora prima dell’alba Mercurio, Venere, Marte, Giove e Saturno appariranno nel cielo dei prossimi giorni lungo una linea immaginaria che va da sud est ad ovest
Quark deconfinement and the duration of short Gamma Ray Bursts
Creators: name: Drago, Alessandro
name: Lavagno, Andrea
name: Metzger, Brian
name: Pagliara, Giuseppe
Publisher: name: INFN Open Access Repository
Year: 2015

description: We propose a model for short duration gamma-ray bursts (sGRBs) based on the
formation of a quark star after the merger of two neutron stars. We assume that
the sGRB central engine is a proto-magnetar, which has been previously invoked
to explain the plateau-like X-ray emission observed following both long and
short GRBs. Here, we show that: i) a few milliseconds after the merger it is
possible to form a stable and massive star made in part of quarks; ii) during
the early cooling phase of the incompletely formed quark star, the flux of
baryons ablated from the surface by neutrinos is large and it does not allow
the outflow to achieve a bulk Lorentz factor high enough to produce a GRB; iii)
after the quark burning front reaches the stellar surface, baryon ablation
ceases and the jet becomes too baryon poor to produce a GRB; iv) however,
between these two phases a GRB can be produced over the finite timescale
required for the baryon pollution to cease; a characteristic timescale of the
order of $\sim 0.1 $ s naturally results from the time the conversion front
needs to cover the distance between the rotational pole and the latitude of the
last closed magnetic field line; v) we predict a correlation between the
luminosity of the sGRB and its duration, consistent with the data; vi) our
model also predicts a delay of the order of ten seconds between the time of the
merger event and the sGRB, allowing for the possibility of precursor emission
and implying that the jet will encounter the dense cocoon formed immediately
after the merger.
title: ÐÐ½Ð¶ÐµÐ½ÐµÑÐ½Ð¾Ðµ Ð±Ð»Ð°Ð³Ð¾ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð¾ ÐºÐ¾ÑÑÐµÐ´Ð¶Ð½Ð¾Ð³Ð¾ Ð¿Ð¾ÑÐµÐ»ÐºÐ° Ñ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸ÐµÐ¹ Ð¿Ð°ÑÐºÐ°
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
Creators: name: Ð¨Ð°Ð´ÑÐ¸Ð½, ÐÐ»Ð°Ð´Ð¸Ð¼Ð¸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: Ð´ÑÐµÐ½Ð°Ð¶
ÑÐ°ÑÐ½Ñ Ð°ÑÑ
Ð»Ð¸Ð²Ð½ÐµÐ²Ð°Ñ ÐºÐ°Ð½Ð°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ
ÑÐµÐºÑÐµÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ Ð·Ð¾Ð½Ð°
Ð±Ð»Ð°Ð³Ð¾ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð¾

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½ Ð¿Ð¾ÑÐµÐ»Ð¾Ðº Â«ÐÐ»Ð°ÐºÑÑÐ°Ñ Ð¸Ð²Ð°Â», ÑÐ°ÑÐ¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð½ÑÐ¹ Ð² ÐÑÑÐºÐ¸Ð½ÑÐºÐ¾Ð¼ ÑÐ°Ð¹Ð¾Ð½Ðµ Ð³. Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³Ð°. ÐÐ° Ð¿ÑÐµÐ´Ð¾ÑÑÐ°Ð²Ð»ÐµÐ½Ð½Ð¾Ð¹ ÑÐµÑÑÐ¸ÑÐ¾ÑÐ¸Ð¸ Ð·Ð°Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ñ: 33 Ð¸Ð½Ð´Ð¸Ð²Ð¸Ð´ÑÐ°Ð»ÑÐ½ÑÑ Ð¶Ð¸Ð»ÑÑ ÑÑÐ°ÑÑÐºÐ°, 25 ÑÑÐ°ÑÑÐºÐ¾Ð² ÑÐ°ÑÐ½ÑÐ°ÑÑÐ¾Ð², Ð°Ð´Ð¼Ð¸Ð½Ð¸ÑÑÑÐ°ÑÐ¸Ð²Ð½Ð¾-Ð±ÑÑÐ¾Ð²Ð¾Ð¹ ÑÐµÐ½ÑÑ Ð¸ ÑÐµÐºÑÐµÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ Ð·Ð¾Ð½Ð°, Ð²ÐºÐ»ÑÑÐ°ÑÑÐ°Ñ Ð¾ÑÐºÑÑÑÑÐµ Ð¿Ð»Ð¾ÑÐºÐ¾ÑÑÐ½ÑÐµ ÑÐ¿Ð¾ÑÑÐ¸Ð²Ð½ÑÐµ ÑÐ¾Ð¾ÑÑÐ¶ÐµÐ½Ð¸Ñ, Ð¸ÑÐºÑÑÑÑÐ²ÐµÐ½Ð½ÑÐ¹ Ð²Ð¾Ð´Ð¾ÐµÐ¼ Ð¸ Ð¿Ð°ÑÐº. ÐÐ»Ñ Ð¿Ð¾ÑÐµÐ»ÐºÐ° Ð¾ÑÑÑÐµÑÑÐ²Ð»ÐµÐ½ ÑÐ»Ð¾Ð¶Ð½ÑÐ¹ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑ Ð¸Ð½Ð¶ÐµÐ½ÐµÑÐ½ÑÑ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹, Ð²ÐºÐ»ÑÑÐ°ÑÑÐ¸Ð¹ ÑÑÐµÐ¼Ñ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÐµÐ»ÑÐµÑÐ° ÑÐµÑÑÐ¸ÑÐ¾ÑÐ¸Ð¸ Ð´Ð»Ñ Ð¾ÑÐ²Ð¾Ð´Ð° Ð¿Ð¾Ð²ÐµÑÑÐ½Ð¾ÑÑÐ½ÑÑ Ð²Ð¾Ð´, Ð° ÑÐ°ÐºÐ¶Ðµ Ð²Ð¾Ð´Ð¾Ð¿Ð¾Ð½Ð¸Ð¶ÐµÐ½Ð¸Ðµ ÑÐµÑÑÐ¸ÑÐ¾ÑÐ¸Ð¸ Ð² Ð¼ÐµÑÑÐ°Ñ, Ð³Ð´Ðµ ÑÑÐ¾Ð²ÐµÐ½Ñ Ð³ÑÑÐ½ÑÐ¾Ð²ÑÑ Ð²Ð¾Ð´ Ð½Ð°ÑÐ¾Ð´Ð¸ÑÑÑ Ñ Ð¿Ð¾Ð²ÐµÑÑÐ½Ð¾ÑÑÐ¸ Ð·ÐµÐ¼Ð»Ð¸. ÐÑÐ¾ÐµÐºÑ Ð¿Ð¾ Ð¸Ð½Ð¶ÐµÐ½ÐµÑÐ½Ð¾Ð¹ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐµ ÑÐµÑÑÐ¸ÑÐ¾ÑÐ¸Ð¸ Ð¿Ð¾ÑÑÐ»ÐºÐ° Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½ Ð² ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²Ð¸Ð¸ Ñ Ð·Ð°Ð´Ð°Ð½Ð¸ÐµÐ¼ Ð½Ð° Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¸ ÑÑÐµÐ±Ð¾Ð²Ð°Ð½Ð¸ÑÐ¼Ð¸ Ð´ÐµÐ¹ÑÑÐ²ÑÑÑÐ¸Ñ Ð½Ð¾ÑÐ¼Ð°ÑÐ¸Ð²Ð½ÑÑ Ð´Ð¾ÐºÑÐ¼ÐµÐ½ÑÐ¾Ð² Ð² ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ðµ.
A High Current Proton Linac with 352 MHz SC Cavities
Creators: name: C. Pagani
name: G. Bellomo
name: P. Pierini
Publisher: name: Conf.Proc.C9608262:107-109,1996
Year: 1996

description: A proposal for a 10-120 mA proton linac employing superconducting
beta-graded, CERN type, four cell cavities at 352 MHz is presented. The high
energy part (100 MeV-1 GeV) of the machine is split in three beta-graded
sections, and transverse focusing is provided via a periodic doublet array. All
the parameters, like power in the couplers and accelerating fields in the
cavities, are within the state of the art, achieved in operating machines. A
first stage of operation at 30 mA beam current is proposed, while the upgrade
of the machine to 120 mA operation can be obtained increasing the number of
klystrons and couplers per cavity. The additional coupler ports, up to four,
will be integrated in the cavity design. Preliminary calculations indicate that
beam transport is feasible, given the wide aperture of the 352 MHz structures.
A capital cost of less than 100 M$ at 10 mA, reaching up to 280 M$ for the 120
mA extension, has been estimated for the superconducting high energy section
(100 MeV-1 GeV). The high efficiency of the proposed machine, reaching 50% at
15 mA, makes it a good candidate for proposed nuclear waste incineration
facilities and Energy Amplifier studies.
Vola Jason-3, esplode Falcon 9
Creators: Davide Coero Borga
Publisher: name: Media Inaf
Year: 2016

Il satellite di Thales Alenia Space (TAS) è in volo verso la sua orbita di posizionamento, da dove fornirà una copertura globale delle superfici degli oceani prive di ghiaccio. Buone nuove per l'oceanografia, pessime notizie per Elon Musk e la sua SpaceX: il vettore riutilizzabile Falcon 9 è caduto esplodendo sulla piattaforma a controllo remoto nel bel mezzo del Pacifico
title: ÐÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ðµ Ð½Ð°Ð¸Ð»ÑÑÑÐ¸Ñ Ð´Ð¾ÑÑÑÐ¿Ð½ÑÑ ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¹ Ð´Ð»Ñ ÑÐ¼ÐµÐ½ÑÑÐµÐ½Ð¸Ñ Ð½ÐµÐ³Ð°ÑÐ¸Ð²Ð½Ð¾Ð³Ð¾ Ð²Ð»Ð¸ÑÐ½Ð¸Ñ ÑÐµÐ¿Ð»Ð¾ÑÐ»ÐµÐºÑÑÐ¾ÑÐµÐ½ÑÑÐ°Ð»ÐµÐ¹ Ð½Ð° Ð¾ÐºÑÑÐ¶Ð°ÑÑÑÑ ÑÑ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Ð¾Ð´Ð±ÐµÑÐµÐ·Ð½Ð°Ñ, 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: 2018
Subjects: Ð¢ÐµÐ¿Ð»Ð¾ÑÐ»ÐµÐºÑÑÐ¾ÑÐµÐ½ÑÑÐ°Ð»Ð¸
ÐÐºÑÑÐ¶Ð°ÑÑÐ°Ñ ÑÑÐµÐ´Ð°
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description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð° ÑÐµÐ¼Ð° Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ Ð½Ð°Ð¸Ð»ÑÑÑÐ¸Ñ Ð´Ð¾ÑÑÑÐ¿Ð½ÑÑ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¹ Ð´Ð»Ñ ÑÐ¼ÐµÐ½ÑÑÐµÐ½Ð¸Ñ Ð½ÐµÐ³Ð°ÑÐ¸Ð²Ð½Ð¾Ð³Ð¾ Ð²Ð»Ð¸ÑÐ½Ð¸Ñ Ð¢Ð­Ð¦ Ð½Ð° Ð¾ÐºÑÑÐ¶Ð°ÑÑÑÑ ÑÑÐµÐ´Ñ. ÐÐ°Ð½Ð° ÐºÐ»Ð°ÑÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¸Ñ ÑÑÐµÑ Ð¾ÐºÑÑÐ¶Ð°ÑÑÐµÐ¹ ÑÑÐµÐ´Ñ, Ð¿Ð¾Ð¿Ð°Ð´Ð°ÑÑÐ¸Ñ Ð¿Ð¾Ð´ Ð²Ð»Ð¸ÑÐ½Ð¸Ðµ Ð¢Ð­Ð¦. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÑ Ð¿ÑÐ¸Ð¼ÐµÐ½ÑÐµÐ¼ÑÑ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² Ð¿Ð¾ ÑÐ¼ÐµÐ½ÑÑÐµÐ½Ð¸Ñ Ð½ÐµÐ³Ð°ÑÐ¸Ð²Ð½Ð¾Ð³Ð¾ Ð²Ð»Ð¸ÑÐ½Ð¸Ñ. ÐÐ·ÑÑÐµÐ½Ñ Ð¼ÐµÑÐ¾Ð´Ñ ÑÐ¼ÐµÐ½ÑÑÐµÐ½Ð¸Ñ Ð°ÐºÑÑÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð²Ð»Ð¸ÑÐ½Ð¸Ñ Ð¢Ð­Ð¦. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½Ñ Ð·Ð°Ð¼ÐµÑÑ ÑÑÐ¾Ð²Ð½ÐµÐ¹ ÑÑÐ¼Ð° Ð²Ð±Ð»Ð¸Ð·Ð¸ Ð¾Ð±ÑÐµÐºÑÐ° Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ. Ð Ð°ÑÑÑÐ¸ÑÐ°Ð½Ñ ÑÑÐ¾Ð²Ð½Ð¸ ÑÑÐ¼Ð¾Ð²Ð¾Ð³Ð¾ Ð²Ð¾Ð·Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ Ð¢Ð­Ð¦ Ð¿ÑÐ¸ ÑÐ°Ð±Ð¾ÑÐµ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¿ÑÐ¸ Ð½ÐµÑÑÐ°ÑÐ¸Ð¾Ð½Ð°ÑÐ½ÑÑ ÑÐµÐ¶Ð¸Ð¼Ð°Ñ. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð¾ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð¸Ðµ Ð¿Ð¾ ÑÐ¼ÐµÐ½ÑÑÐµÐ½Ð¸Ñ Ð°ÐºÑÑÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð²Ð¾Ð·Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ Ð¾Ð±ÑÐµÐºÑÐ° Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð½Ð° Ð¾ÐºÑÑÐ¶Ð°ÑÑÑÑ ÑÑÐµÐ´Ñ.
Consistent Batalin--Fradkin quantization of Reducible First Class Constraints
Creators: name: S. Bellucci
name: A. Galajinsly
Publisher: name: INFN Open Access Repository
Year: 2000

description: We reconsider the problem of BRST quantization of a mechanics with infinitely reducible first class constraints. Following an earlier recipe [Phys. Lett. 381 105 (1996)], the original phase space is extended by purely auxiliary variables, the constraint set in the enlarged space being first stage of reducibility. The BRST charge involving only a finite number of ghost variables is explicitly constructed.
Lie groups in nonequilibrium thermodynamics: Geometric structure behind viscoplasticity
Creators: name: Öttinger, Hans Christian
Publisher: name: arXiv
Year: 2010
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: Poisson brackets provide the mathematical structure required to identify the reversible contribution to dynamic phenomena in nonequilibrium thermodynamics. This mathematical structure is deeply linked to Lie groups and their Lie algebras. From the characterization of all the Lie groups associated with a given Lie algebra as quotients of a universal covering group, we obtain a natural classification of rheological models based on the concept of discrete reference states and, in particular, we find a clear-cut and deep distinction between viscoplasticity and viscoelasticity. The abstract ideas are illustrated by a naive toy model of crystal viscoplasticity, but similar kinetic models are also used for modeling the viscoplastic behavior of glasses. We discuss some implications for coarse graining and statistical mechanics.
description: 11 pages, 1 figure, accepted for publication in J. Non-Newtonian Fluid Mech. Keywords: Elastic-viscoplastic materials, Nonequilibrium thermodynamics, GENERIC, Lie groups, Reference states
σ_eeγγ^tot at e^+e^- Colliders
Creators: name: R.M. Godbole
name: G. Pancheri
Publisher: name: INFN Open Access Repository
Year: 2001

description: In this talk I briefly summarize different models for σ_eeγγ^tot(e^+ e^- → γγ → hadrons) and contrast model predictions with the data. I will then discuss the capability of the future e^+e^- and γγ colliders to distinguish between various models and end with an outlook for future work.
A Review of Coronagraphic Observations of Shocks Driven by Coronal Mass Ejections
Creators: name: Vourlidas, A.
name: Ontiveros, V.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: The existence of shocks driven by Coronal Mass Ejections (CMEs) has always been assumed based on the superalfvenic speeds for some of these events and on indirect evidence such as radio bursts and distant streamer deflections. However, the direct signature of the plasma enhancement at the shock front has escaped detection until recently. Since 2003, work on LASCO observations has shown that CME-driven shocks can be detected by white light coronagraph observations from a few solar radii to at least 20 Rsun. Shock properties, such as the density compression ratio and their direction can be extracted from the data. We review this work here and demonstrate how to recognize the various shock morphologies in the images.We also discuss how the two-viewpoint coronagraph observations from the STEREO mission allow the reconstruction of the 3D envelope of the shock revealing some interesting properties of the shocks (e.g., anisotropic expansion).
description: 8 pages, 5 figures, to appear in Shocks Waves in Astrophysical Environments, Proceedings of the 8th Annual International Astrophysics Conference (referred), AIP Conf. Proc
title: ÐÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ ÑÐ¸Ð½Ð°Ð½ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÑÑÐµÐ¶Ð´ÐµÐ½Ð¸Ð¹ Ð·Ð´ÑÐ°Ð²Ð¾Ð¾Ñ ÑÐ°Ð½ÐµÐ½Ð¸Ñ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ ÑÑÐ½ÐºÐ° Ð¿Ð»Ð°ÑÐ½ÑÑ Ð¼ÐµÐ´Ð¸ÑÐ¸Ð½ÑÐºÐ¸Ñ ÑÑÐ»ÑÐ³
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÑÐµÐ½ÐºÐ¾, 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·Ð´ÑÐ°Ð²Ð¾Ð¾Ñ ÑÐ°Ð½ÐµÐ½Ð¸Ðµ
ÑÐ¸Ð½Ð°Ð½ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð·Ð´ÑÐ°Ð²Ð¾Ð¾Ñ ÑÐ°Ð½ÐµÐ½Ð¸Ñ
Ð¼ÐµÐ´Ð¸ÑÐ¸Ð½ÑÐºÐ¸Ðµ ÑÑÑÐµÐ¶Ð´ÐµÐ½Ð¸Ñ
Ð¿Ð»Ð°ÑÐ½ÑÐµ Ð¼ÐµÐ´Ð¸ÑÐ¸Ð½ÑÐºÐ¸Ðµ ÑÑÐ»ÑÐ³Ð¸

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÑÐ¸ÑÑÐµÐ¼Ð° Ð·Ð´ÑÐ°Ð²Ð¾Ð¾ÑÑÐ°Ð½ÐµÐ½Ð¸Ñ Ð Ð¤. 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¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐµÐ¹ ÑÐ¸Ð½Ð°Ð½ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÑÑÐµÐ¶Ð´ÐµÐ½Ð¸Ð¹ Ð·Ð´ÑÐ°Ð²Ð¾Ð¾ÑÑÐ°Ð½ÐµÐ½Ð¸Ñ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð¿Ð»Ð°ÑÐ½ÑÑ Ð¼ÐµÐ´Ð¸ÑÐ¸Ð½ÑÐºÐ¸Ñ ÑÑÐ»ÑÐ³ Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¹ Ð¿Ð¾ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÐºÐ°ÑÐµÑÑÐ²Ð° Ð¸ ÑÐ°ÑÑÐ¸ÑÐµÐ½Ð¸Ñ ÑÐ¿ÐµÐºÑÑÐ° Ð¼ÐµÐ´Ð¸ÑÐ¸Ð½ÑÐºÐ¸Ñ ÑÑÐ»ÑÐ³. Ð ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð° ÑÐ¸ÑÑÐµÐ¼Ð° Ð·Ð´ÑÐ°Ð²Ð¾Ð¾ÑÑÐ°Ð½ÐµÐ½Ð¸Ñ Ð² Ð Ð¾ÑÑÐ¸Ð¸, Ð¿ÑÐ¾Ð²ÐµÐ´ÑÐ½ ÑÑÐ°Ð²Ð½Ð¸ÑÐµÐ»ÑÐ½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¼Ð¸ÑÐ¾Ð²ÑÑ ÑÐ¸ÑÑÐµÐ¼ Ð·Ð´ÑÐ°Ð²Ð¾Ð¾ÑÑÐ°Ð½ÐµÐ½Ð¸Ñ, Ð¸Ð·ÑÑÐµÐ½Ð° Ð½Ð¾ÑÐ¼Ð°ÑÐ¸Ð²Ð½Ð¾-Ð¿ÑÐ°Ð²Ð¾Ð²Ð°Ñ Ð±Ð°Ð·Ð° Ð¸ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ñ ÑÐ¸Ð½Ð°Ð½ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¼ÐµÐ´Ð¸ÑÐ¸Ð½ÑÐºÐ¾Ð³Ð¾ ÑÑÑÐµÐ¶Ð´ÐµÐ½Ð¸Ñ. Ð¢Ð°ÐºÐ¶Ðµ Ð² ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐ¾Ð²ÐµÐ´ÑÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÑÐ½ÐºÐ° Ð¼ÐµÐ´Ð¸ÑÐ¸Ð½ÑÐºÐ¸Ð¹ ÑÑÐ»ÑÐ³ Ð² Ð Ð¾ÑÑÐ¸Ð¸, Ð²ÑÑÐ²Ð»ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÑÐµÐ½Ð´ÐµÐ½ÑÐ¸Ð¸ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ ÑÐµÐºÑÐ¾ÑÐ¾Ð² Ð·Ð´ÑÐ°Ð²Ð¾Ð¾ÑÑÐ°Ð½ÐµÐ½Ð¸Ñ Ð¸ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¿Ð»Ð°ÑÐ½ÑÑ Ð¼ÐµÐ´Ð¸ÑÐ¸Ð½ÑÐºÐ¸Ñ ÑÑÐ»ÑÐ³. Ð Ð°Ð±Ð¾ÑÐ° Ð¿Ð¾Ð·Ð²Ð¾Ð»Ð¸Ñ Ð¼ÐµÐ´Ð¸ÑÐ¸Ð½ÑÐºÐ¸Ð¼ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸ÑÐ¼ ÑÑÐµÑÑÑ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ ÑÐ¸ÑÑÐµÐ¼Ñ Ð·Ð´ÑÐ°Ð²Ð¾Ð¾ÑÑÐ°Ð½ÐµÐ½Ð¸Ñ Ð² ÑÐ²Ð¾ÐµÐ¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸, Ð¾Ð¿ÑÐµÐ´ÐµÐ»Ð¸ÑÑ Ð´Ð»Ñ ÑÐµÐ±Ñ ÑÐµÐ»ÐµÐ²ÑÐµ Ð¾ÑÐ¸ÐµÐ½ÑÐ¸ÑÑ, Ð¾ÑÐµÐ½Ð¸ÑÑ ÑÐ²Ð¾Ñ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ Ð¸ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ¾Ð² Ð¿Ð¾ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ ÑÑÐ½ÐºÐ° Ð¿Ð»Ð°ÑÐ½ÑÑ Ð¼ÐµÐ´Ð¸ÑÐ¸Ð½ÑÐºÐ¸Ñ ÑÑÐ»ÑÐ³ Ð¸ ÑÑÐ¿ÐµÑÐ½Ð¾ ÑÐµÐ°Ð»Ð¸Ð·Ð¾Ð²Ð°ÑÑ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ñ Ð¾ÐºÐ°Ð·Ð°Ð½Ð¸Ñ Ð¿Ð»Ð°ÑÐ½ÑÑ Ð¼ÐµÐ´Ð¸ÑÐ¸Ð½ÑÐºÐ¸Ñ ÑÑÐ»ÑÐ³, Ð¸Ð·Ð±ÐµÐ³Ð°Ñ ÑÐ²ÐµÐ»Ð¸ÑÐµÐ½Ð¸Ñ ÑÐµÐ½ÐµÐ²Ð¾Ð³Ð¾ ÑÐµÐºÑÐ¾ÑÐ° Ð¸ ÐºÐ¾ÑÑÑÐ¿ÑÐ¸Ð¸ Ð¸ Ð¿Ð¾ÑÐµÑÐ¸ ÐºÐ»Ð¸ÐµÐ½ÑÐ¾Ð² Ð¸Ð·-Ð·Ð° Ð½Ð°Ð²ÑÐ·ÑÐ²Ð°Ð½Ð¸Ñ Ð´Ð¾ÑÐ¾Ð³Ð¸Ñ Ð¿ÑÐ¾ÑÐµÐ´ÑÑ.
title: ÐÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ Ð±Ð°Ð½ÐºÐ° Ð¿Ð¾ Ð¿ÑÐ¸Ð²Ð»ÐµÑÐµÐ½Ð¸Ñ ÑÑÐµÐ´ÑÑÐ² Ð½Ð°ÑÐµÐ»ÐµÐ½Ð¸Ñ Ð¸ Ð¿ÑÑÐ¸ ÐµÐµ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ (Ð¿Ð¾ Ð·Ð°ÐºÐ°Ð·Ñ ÐÐ "Ð®Ð½Ð¸ÐÑÐµÐ´Ð¸Ñ ÐÐ°Ð½Ðº")
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÑÐ±Ð¸Ð¼Ð¾Ð²Ð°, Ð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ÑÐµÐ´ÑÑÐ²Ð° Ð½Ð°ÑÐµÐ»ÐµÐ½Ð¸Ñ
Ð´ÐµÐ¿Ð¾Ð·Ð¸ÑÐ°ÑÐ½Ð°Ñ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ°
ÐºÐ¾Ð¼Ð¼ÐµÑÑÐµÑÐºÐ¸Ðµ Ð±Ð°Ð½ÐºÐ¸
ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ðµ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ðµ
funds from the public
deposit policy
commercial banks
financial position

description: Ð ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑÑÑ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¾ÑÐ½Ð¾Ð²Ñ Ð±Ð°Ð½ÐºÐ¾Ð²ÑÐºÐ¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿Ð¾ Ð¿ÑÐ¸Ð²Ð»ÐµÑÐµÐ½Ð¸Ñ ÑÑÐµÐ´ÑÑÐ² Ð½Ð°ÑÐµÐ»ÐµÐ½Ð¸Ñ, ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¸ Ð¾ÑÑÑÐµÑÑÐ²Ð»ÐµÐ½Ð¸Ðµ Ð´ÐµÐ¿Ð¾Ð·Ð¸ÑÐ½Ð¾Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ¸ Ð±Ð°Ð½ÐºÐ°, Ð´Ð¸Ð½Ð°Ð¼Ð¸ÐºÐ° ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ ÑÑÐ½ÐºÐ° Ð´ÐµÐ¿Ð¾Ð·Ð¸ÑÐ¾Ð² Ð Ð¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð¹ Ð¤ÐµÐ´ÐµÑÐ°ÑÐ¸Ð¸. ÐÑÐ¾Ð²Ð¾Ð´Ð¸ÑÑÑ Ð¾ÑÐµÐ½ÐºÐ° ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð³Ð¾ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ñ ÐÐ "Ð®Ð½Ð¸ÐÑÐµÐ´Ð¸Ñ ÐÐ°Ð½Ðº", ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑÑÑ Ð´ÐµÐ¿Ð¾Ð·Ð¸ÑÐ½Ð°Ñ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ° Ð¸ ÑÑÑÑÐºÑÑÑÐ° Ð´ÐµÐ¿Ð¾Ð·Ð¸ÑÐ½Ð¾Ð³Ð¾ Ð¿Ð¾ÑÑÑÐµÐ»Ñ ÐÐ "Ð®Ð½Ð¸ÐÑÐµÐ´Ð¸Ñ ÐÐ°Ð½Ðº", Ð° ÑÐ°ÐºÐ¶Ðµ ÑÐ°Ð·ÑÐ°Ð±Ð°ÑÑÐ²Ð°ÑÑÑÑ Ð¼ÐµÑÐ¾Ð´Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¿Ð¾ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ Ð´ÐµÐ¿Ð¾Ð·Ð¸ÑÐ½Ð¾Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ¸ Ð±Ð°Ð½ÐºÐ° Ð¸ Ð¿ÑÐµÐ´Ð»Ð°Ð³Ð°ÑÑÑÑ Ð½Ð¾Ð²ÑÐµ Ð´ÐµÐ¿Ð¾Ð·Ð¸ÑÐ½ÑÐµ Ð¿ÑÐ¾Ð´ÑÐºÑÑ.
description: The paper deals with the theoretical basis of banking activities to raise public funds. The formation and implementation of the bank's deposit policy, the dynamics of development of the market deposits. An evaluation of the financial condition of JSC "UniCredit Bank", discusses deposit policy and the structure of the deposit portfolio of "UniCredit Bank", as well as the developed methodological recommendations for improving the deposit policy of the bank and offered new deposit products.
title: ÐÐ°ÑÐºÐµÑÐ¸Ð½Ð³Ð¾Ð²ÑÐµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÑÐ½ÐºÐ° Ð¿Ð¾ÑÑÐµÐ±Ð¸ÑÐµÐ»ÑÑÐºÐ¸Ñ ÑÐ¾Ð²Ð°ÑÐ¾Ð² (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐÐ "Ð Ð¢Ð")
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ°ÑÐµÐºÐ¸Ð½Ð°, 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: 2017
Subjects: ÑÐ±Ð¾Ñ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¸
Ð°Ð½ÐºÐµÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
ÑÑÐ½Ð¾Ðº ÑÐ¾ÑÐ¾Ð²ÑÑ Ð¾Ð¿ÐµÑÐ°ÑÐ¾ÑÐ¾Ð²
ÑÐ¾ÑÐ¾Ð²ÑÐ¹ ÑÐ¸ÑÐµÐ¹Ð»
ÑÑÐ°ÑÐ¸Ðº

description: ÐÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð´Ð¸Ð½Ð°Ð¼Ð¸ÐºÐ¸ ÑÐµÐºÑÑÐµÐ³Ð¾ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ ÑÐ¾ÑÐ¾Ð²ÑÑ ÑÐµÑÐµÐ¹ Ð¾Ð¿ÐµÑÐ°ÑÐ¾ÑÐ°, Ð° ÑÐ°ÐºÐ¶Ðµ ÑÑÐ½ÐºÐ° ÑÐ¾ÑÐ¾Ð²ÑÑ ÑÐµÐ»ÐµÑÐ¾Ð½Ð¾Ð² Ð¸ ÑÐ¼Ð°ÑÑÑÐ¾Ð½Ð¾Ð². ÐÑÐ´ÐµÐ»ÐµÐ½Ð° ÑÐµÐ»ÐµÐ²Ð°Ñ Ð°ÑÐ´Ð¸ÑÐ¾ÑÐ¸Ñ ÑÐ¾Ð·Ð½Ð¸ÑÐ½Ð¾Ð¹ ÑÐµÑÐ¸ Ð³. ÐÐ¾Ð»Ð¿Ð¸Ð½Ð¾. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¾ Ð°Ð½ÐºÐµÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¿Ð¾ÑÑÐµÐ±Ð¸ÑÐµÐ»ÐµÐ¹. Ð¡Ð¾Ð³Ð»Ð°ÑÐ¾Ð²Ð°Ð½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð¿Ð¾ÑÑÐµÐ±Ð½Ð¾ÑÑÐ¸ Ð¿Ð¾ÐºÑÐ¿Ð°ÑÐµÐ»ÐµÐ¹ Ñ Ð¿ÑÐ¾Ð´Ð°Ð²Ð°ÐµÐ¼Ð¾Ð¹ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¸ÐµÐ¹. ÐÑÐ¿Ð¾Ð»Ð½ÐµÐ½ Ð¾Ð¿ÑÐ¾Ñ ÑÐ´Ð¾Ð²Ð»ÐµÑÐ²Ð¾ÑÐµÐ½Ð½Ð¾ÑÑÐ¸ ÐºÐ°ÑÐµÑÑÐ²Ð¾Ð¼ Ð¾Ð±ÑÐ»ÑÐ¶Ð¸Ð²Ð°Ð½Ð¸Ñ.
Zinnia, il primo fiore nato nello spazio
Creators: Eleonora Ferroni
Publisher: name: Media Inaf
Year: 2016

Dopo aver raccolto la lattuga romana, questo è il secondo esperimento di giardinaggio spaziale sull'ISS, sulla quale ha trovato posto un impianto di coltivazione dedicato, il Veggie. Le foto della pianta e del fiore spopolano sul web
Analyzing SN2003Z with PHOENIX
Creators: name: Knop, S.
name: Hauschildt, P. H.
name: Baron, E.
name: Dreizler, S.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We present synthetic spectra around maximum for the type II supernova SN 2003Z, which was first detected on January 29.7 2003. Comparison with observed spectra aim at the determination of physical parameters for SN 2003Z. Synthetic spectra are calculated with our stellar atmosphere code PHOENIX. It solves the special relativistic equation of radiative transfer, including large NLTE-calculations and line blanketing by design, in 1-dimensional spherical symmetry. The observed spectra were obtained at the 3.5 meter telescope at Calar Alto. The TWIN instrument was used so that a spectral range from about 3600 to 7500 Angstroem was covered. The spectra were taken on Feb. 4, 5, 9, and 11, 2003. The physical parameters of the models give the luminosities, a range of possible velocity profiles for the SN, an estimate of the colour excess, and the observed metalicity.
description: 8 figures
Stratification in the Preferential Attachment Network
Creators: name: Ben-Naim, E.
name: Krapivsky, P. L.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: FOS: Physical sciences

description: We study structural properties of trees grown by preferential attachment. In this mechanism, nodes are added sequentially and attached to existing nodes at a rate that is strictly proportional to the degree. We classify nodes by their depth n, defined as the distance from the root of the tree, and find that the network is strongly stratified. Most notably, the distribution f_k^(n) of nodes with degree k at depth n has a power-law tail, f_k^(n) ~ k^{-γ(n)}. The exponent grows linearly with depth, gamma(n)=2+(n-1)/, where the brackets denote an average over all nodes. Therefore, nodes that are closer to the root are better connected, and moreover, the degree distribution strongly varies with depth. Similarly, the in-component size distribution has a power-law tail and the characteristic exponent grows linearly with depth. Qualitatively, these behaviors extend to a class of networks that grow by a redirection mechanism.
description: 6 pages, 4 figures
Il secondo buco nero più massivo della Via Lattea
Creators: Corrado Ruscica
Publisher: name: Media Inaf
Year: 2016

Osservazioni in banda radio hanno fornito agli astronomi una serie di indizi correlati all’esistenza di un buco nero di massa intermedia localizzato in prossimità del centro galattico. L’oggetto potrebbe rappresentare una sorta di anello mancante per comprendere la formazione e l’evoluzione dei buchi neri supermassicci che risiedono nei nuclei delle galassie. I risultati sono riportati su ApJ Letters
CTF3 Design report
Creators: name: D.Alesini
name: C.Biscari
name: R.Boni
name: A.Clozza
name: G.Di Pirro
name: A.Drago
name: A.Gallo
name: A.Ghigo
name: F.Marcellini
name: C.Milardi
name: M.A.Preger
name: C.Sanelli
name: F.Sannibale
name: M.Serio
name: F.Sgamma
name: A.Stecchi
name: A.Stella
name: M.Zobov
name: R.Bossart
name: H.Braun
name: P.Brown
name: G.Carron
name: V.Chohan
name: R.Corsini
name: E.D'Amico
name: S.Deghaye
name: J.P.Delahaye
name: F.DiMaio
name: S.Doebert
name: B.Dupuy
name: G.Geschonke
name: L.GrÃ¶Ning
name: G.Guignard
name: H.Hellgren
name: S.Hutchins
name: J.H.Lewis
name: E.Jensen
name: G.McMonagle
name: A.Millich
name: J.Monteiro
name: J.P.Delahaye
name: T.Otto
name: P.Pearce
name: E.Peschardt
name: R.Pittin
name: M.Poehler
name: J.P.Potier
name: L.Rinolfi
name: T.Risselada
name: G.Rossat
name: P.Royer
name: D.Schulte
name: J.Sladen
name: G.Suberlucq
name: I.Syratchev
name: F.Tecker
name: H.Trautner
name: L.Thorndahl
name: I.Wilson
name: W.WÃ¼nsch
name: A.Yeremian
name: R.Miller
name: R.Ruth
name: R.Koontz
name: I.N.Ross
name: E. Bente
name: G. Valentine
name: G.Bienvenu
name: M.Bernard
name: M.Omeich
name: R.Roux
name: T.Garvey
Publisher: name: INFN Open Access Repository
Year: 2002

description: The design of CLIC is based on a two-beam scheme, where short pulses of high power 30 GHz RF are extracted from a drive beam running parallel to the main beam.  The 3rd generation CLIC Test Facility (CTF3) will demonstrate the generation of the drive beam with the appropriate time structure, the extraction of 30 GHz RF power from this beam, as well as acceleration of a probe beam with 30 GHz RF cavities  The project makes maximum use of existing equipment and infrastructure of the LPI complex, which became available after the closure of LEP.
A study of the spark spectra of selenium
Creators: name: George, Simon
Publisher: name: University of British Columbia
Year: 2011

description: The spark spectra of selenium have been photographed from the infra-red to the vacuum ultra-violet on a variety of spectrographs including a two meter vacuum grating spectrograph, a twenty-one foot concave grating, a Hilger Constant Deviation, a Hilger medium quartz and a Hilger large automatic glass-quartz prism spectrograph. Two light sources have been used: An electrodeless spark discharge and a spark in helium. About 2200 selenium lines have been measured in the region 10450 to 345 Angstroms. On the basis of these measurements, new levels have been found in Se III, Se IV, and Se V. The most important achievement was the discovery of the deepest excited terms 4s4p³ ⁵S⁰₂ in Se III and 4s4p² ⁴p in Se IV. The chief extension of the analysis has been in Se IV. A few interferometric measurements were made in Se II and Se III. Using an electrodeless discharge tube excited by a high frequency generator wavelengths of 38 lines in the arc spectrum of potassium have been determined interferometrically.
title: ÐÑÐµÐ½ÐºÐ° ÑÐ¸ÑÑÐ¾Ð²ÑÑ ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¹ Ð² ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ð¸ ÑÐµÐ»Ð¾Ð²ÐµÑÐµÑÐºÐ¸Ð¼Ð¸ ÑÐµÑÑÑÑÐ°Ð¼Ð¸ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ Apple)
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Ð¾Ð½ÑÐ¾ÑÐ¸Ð½Ð°, 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: ÐÑÐºÑÑÑÑÐ²ÐµÐ½Ð½ÑÐ¹ Ð¸Ð½ÑÐµÐ»Ð»ÐµÐºÑ
ÐÐ½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐµ ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¸
ÑÐ¸ÑÑÐ¾Ð²Ð¸Ð·Ð°ÑÐ¸Ñ
ÑÐµÐºÑÑÑÐ¸Ð½Ð³

description: ÐÐ±ÑÐµÐºÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ - Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÐ¹ Ð±Ð¸Ð·Ð½ÐµÑ Apple Inc. ÐÑÐµÐ´Ð¼ÐµÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ â Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ñ HR-Digital Ð² Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½Ð¾Ð¼ Ð±Ð¸Ð·Ð½ÐµÑÐµ Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ Apple. Ð ÐºÐ°ÑÐµÑÑÐ²Ðµ Ð½Ð°ÑÑÐ½Ð¾Ð¹ Ð½Ð¾Ð²Ð¸Ð·Ð½Ñ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð½Ð¾Ð¹ ÑÐµÐ¼Ñ Ð¼Ð¾Ð¶Ð½Ð¾ Ð²ÑÐ´ÐµÐ»Ð¸ÑÑ ÑÑÐ¾ÑÐ½ÐµÐ½Ð¸Ðµ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ HR-Digital, Ð¾ÑÐµÐ½ÐºÑ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¹ Ð² ÑÑÐµÑÐµ Human resources (HR) Ð² Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½Ð¾Ð¼ Ð±Ð¸Ð·Ð½ÐµÑÐµ Ð² ÑÑÐ»Ð¾Ð²Ð¸ÑÑ ÑÐ¸ÑÑÐ¾Ð²Ð¸Ð·Ð°ÑÐ¸Ð¸, Ð°Ð½Ð°Ð»Ð¸Ð· Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¹ Ð² HR ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ Apple, ÑÑÐ¾ ÑÐµÐ³Ð¾Ð´Ð½Ñ Ð½Ðµ Ð³Ð»ÑÐ±Ð¾ÐºÐ¾ Ð¸Ð·ÑÑÐµÐ½Ð¾ Ð² Ð½Ð°ÑÑÐ½ÑÑ Ð¿ÑÐ±Ð»Ð¸ÐºÐ°ÑÐ¸ÑÑ. Ð¦ÐµÐ»Ñ ÑÐ°Ð±Ð¾ÑÑ - Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ ÑÐ¸ÑÑÐ¾Ð²ÑÑ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¹ Ð² HR Ð² ÑÐ°Ð¼ÐºÐ°Ñ Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½Ð¾Ð³Ð¾ Ð±Ð¸Ð·Ð½ÐµÑÐ° Ð¸ Ð²Ð½ÐµÑÐµÐ½Ð¸Ðµ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð¸Ð¹ Ð¿Ð¾ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ HR-Digital Ð² ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ Apple. Ð ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐµ ÑÐ°Ð±Ð¾ÑÑ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ HR-Digital Ð² Ð¼Ð¸ÑÐµ, Ð¸Ð·ÑÑÐµÐ½Ñ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÐµ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐµ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð¾Ð¼. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· Apple Inc., ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÑÐµÐ»Ð¾Ð²ÐµÑÐµÑÐºÐ¸Ð¼Ð¸ ÑÐµÑÑÑÑÐ°Ð¼Ð¸ Ð¸ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ HR ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¹ Ð² ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½ Ð¿ÑÐ¾ÐµÐºÑ Ð¿Ð¾ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ ÑÐ¸ÑÑÐ¾Ð²ÑÑ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¹ Ð² ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ ÑÐµÐ»Ð¾Ð²ÐµÑÐµÑÐºÐ¸Ð¼Ð¸ ÑÐµÑÑÑÑÐ°Ð¼Ð¸ Ð² Apple, Ð²ÐºÐ»ÑÑÐ°ÑÑÐ¸Ð¹ ÑÐ°Ð±Ð¾ÑÑ Ñ Ð¸ÑÐºÑÑÑÑÐ²ÐµÐ½Ð½ÑÐ¼ Ð¸Ð½ÑÐµÐ»Ð»ÐµÐºÑÐ¾Ð¼ Ð² ÑÐµÐºÑÑÑÐ¸Ð½Ð³Ðµ, Ð³ÐµÐ¹Ð¼Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¸ Ð² Ð¾Ð±ÑÑÐµÐ½Ð¸Ð¸, Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ñ ÑÐ°ÐºÐ°ÑÐ¾Ð½Ð¾Ð² IT Ð¸ HR Ð¸ Ð´ÑÑÐ³Ð¾Ðµ. Ð¡Ð´ÐµÐ»Ð°Ð½ Ð²ÑÐ²Ð¾Ð´ Ð¿Ð¾ Ð¾ÑÐµÐ½ÐºÐµ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð½ÑÑ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹.
BEXUS 22 parla italiano
Creators: Francesca Aloisio
Publisher: name: Media Inaf
Year: 2016

L'esperimento STRATONAV, sviluppato da un team di studenti della Sapienza di Roma e dell’Alma Mater di Bologna, è fra quelli selezionati per essere installati all'interno del pallone stratosferico BEXUS 22. Servirà a verificare l’affidabilità del sistema di navigazione VOR
title: ÐÐµÐ¶Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½ÑÐµ Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸Ñ Ð Ð¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð¹ Ð¤ÐµÐ´ÐµÑÐ°ÑÐ¸Ð¸ Ð¸ ÐÐ¸ÑÐ°Ð¹ÑÐºÐ¾Ð¹ ÐÐ°ÑÐ¾Ð´Ð½Ð¾Ð¹ Ð ÐµÑÐ¿ÑÐ±Ð»Ð¸ÐºÐ¸
title: ÑÑÐµÐ±Ð½Ð¾-Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: Ð¡Ð¸Ð´Ð¾ÑÑÑÐº, ÐÐ»ÑÑ
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2021
Subjects: Ð²Ð½ÐµÑÐ½ÑÑ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ°
Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÐµ Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸Ñ
Ð Ð¾ÑÑÐ¸Ð¹ÑÐºÐ°Ñ Ð¤ÐµÐ´ÐµÑÐ°ÑÐ¸Ñ
ÐÐ¸ÑÐ°Ð¹ÑÐºÐ°Ñ ÐÐ°ÑÐ¾Ð´Ð½Ð°Ñ Ð ÐµÑÐ¿ÑÐ±Ð»Ð¸ÐºÐ°

description: ÐÑÐ½Ð¾Ð²Ð½Ð°Ñ ÑÐµÐ»Ñ ÑÑÐµÐ±Ð½Ð¾-Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ â Ð´Ð°ÑÑ ÑÑÑÐ´ÐµÐ½ÑÐ°Ð¼ Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼ÑÐ¹ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑ Ð·Ð½Ð°Ð½Ð¸Ð¹ Ð¿Ð¾ Ð²Ð¾Ð¿ÑÐ¾ÑÑ Ð¼ÐµÐ¶Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½ÑÑ Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸Ð¹ Ð Ð¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð¹ Ð¤ÐµÐ´ÐµÑÐ°ÑÐ¸Ð¸ Ð¸ ÐÐ¸ÑÐ°Ð¹ÑÐºÐ¾Ð¹ ÐÐ°ÑÐ¾Ð´Ð½Ð¾Ð¹ Ð ÐµÑÐ¿ÑÐ±Ð»Ð¸ÐºÐ¸, Ð° ÑÐ°ÐºÐ¶Ðµ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ², ÐºÐ¾ÑÐ¾ÑÑÐµ ÑÑÑÐµÑÑÐ²Ð¾Ð²Ð°Ð»Ð¸ Ð½Ð° Ð¸Ñ ÑÐµÑÑÐ¸ÑÐ¾ÑÐ¸ÑÑ. Ð ÑÐ°Ð¼ÐºÐ°Ñ ÐºÑÑÑÐ° ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑÑÑ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÑÑÐ°Ð¿Ñ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾, ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾, Ð²Ð¾ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¸ ÐºÑÐ»ÑÑÑÑÐ½Ð¾Ð³Ð¾ Ð²Ð·Ð°Ð¸Ð¼Ð¾Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ Ð´Ð²ÑÑ ÑÑÑÐ°Ð½. ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ Ð²ÐºÐ»ÑÑÐ°ÐµÑ Ð² ÑÐµÐ±Ñ Ð¿Ð»Ð°Ð½ Ð¸ ÑÐ¾Ð´ÐµÑÐ¶Ð°Ð½Ð¸Ðµ ÑÐ°Ð·Ð´ÐµÐ»Ð¾Ð² ÐºÑÑÑÐ°, Ð´Ð¾ÐºÑÐ¼ÐµÐ½ÑÑ, ÑÐ¿Ð¸ÑÐºÐ¸ Ð»Ð¸ÑÐµÑÐ°ÑÑÑÑ, Ð·Ð°Ð´Ð°Ð½Ð¸Ñ Ð¸ Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð´Ð»Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ðº Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ð¼ Ð·Ð°Ð½ÑÑÐ¸ÑÐ¼, ÐºÑÐ¸ÑÐµÑÐ¸Ð¸ Ð¾ÑÐµÐ½Ð¸Ð²Ð°Ð½Ð¸Ñ Ð¸ Ð¾ÑÐµÐ½Ð¾ÑÐ½ÑÐµ ÑÑÐµÐ´ÑÑÐ²Ð°. ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ Ð°Ð´ÑÐµÑÐ¾Ð²Ð°Ð½Ð¾ ÑÑÑÐ´ÐµÐ½ÑÐ°Ð¼, Ð¾Ð±ÑÑÐ°ÑÑÐ¸Ð¼ÑÑ Ð¿Ð¾ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ðµ Ð¼Ð°Ð³Ð¸ÑÑÑÐ°ÑÑÑÑ Ð¿Ð¾ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐ¸ 41.04.01 Â«ÐÐ°ÑÑÐ±ÐµÐ¶Ð½Ð¾Ðµ ÑÐµÐ³Ð¸Ð¾Ð½Ð¾Ð²ÐµÐ´ÐµÐ½Ð¸ÐµÂ».
The Nature of the Hyper-Runaway Candidate HIP 60350
Creators: name: Irrgang, Andreas
name: Przybilla, Norbert
name: Heber, Ulrich
name: Nieva, M. Fernanda
name: Schuh, Sonja
Publisher: name: arXiv
Year: 2010
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Young, massive stars in the Galactic halo are widely supposed to be the result of an ejection event from the Galactic disk forcing some stars to leave their place of birth as so-called runaway stars. Here, we present a detailed spectroscopic and kinematic analysis of the runaway B-star HIP 60350 to determine which runaway scenario - a supernova explosion disrupting a binary system or dynamical interaction in star clusters - may be responsible for HIP 60350's peculiar orbit. Based on a non-local thermodynamic equilibrium approach, a high-resolution optical echelle spectrum was examined to revise spectroscopic quantities and for the first time to perform a differential chemical abundance analysis with respect to the B-type star 18 Peg. The results together with proper motions from the Hipparcos Catalog further allowed the three-dimensional kinematics of the star to be studied numerically. The abundances derived for HIP 60350 are consistent with a slightly supersolar metallicity agreeing with the kinematically predicted place of birth ca. 6 kpc away from the Galactic center. However, they do not exclude the possibility of an alpha-enhanced abundance pattern expected in the case of the supernova scenario. Its outstanding high Galactic rest frame velocity of 530 plus-minus 35 km/s is a consequence of ejection in the direction of Galactic rotation and slightly exceeds the local Galactic escape velocity in a standard Galactic potential. Hence HIP 60350 may be unbound to the Galaxy.
description: 10 pages, 6 figures, 2 tables
title: Ð Ð¾Ð¶Ð´ÐµÐ½Ð¸Ðµ ÐºÑÐ¼ÑÐ»ÑÑÐ¸Ð²Ð½ÑÑ Ð¿ÑÐ¾ÑÐ¾Ð½Ð¾Ð² Ð² ÑÑÐ¾Ð»ÐºÐ½Ð¾Ð²ÐµÐ½Ð¸ÑÑ ÑÐ´ÐµÑ Â¹Â²C Ð¸ â¹Be
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¡Ð¾Ð»Ð¾Ð²ÑÑÐ², ÐÐ»Ð°Ð´Ð¸Ð¼Ð¸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: Ð¯Ð´ÐµÑÐ½ÑÐµ ÑÐµÐ°ÐºÑÐ¸Ð¸
ÐÑÐ¾ÑÐ¾Ð½Ñ
ÐÐ¾Ð½ÑÐµ-ÐÐ°ÑÐ»Ð¾ Ð¼ÐµÑÐ¾Ð´
ÐÐ¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
ÐºÑÐ¼ÑÐ»ÑÑÐ¸Ð²Ð½ÑÐ¹ ÑÑÑÐµÐºÑ

description: Ð¦ÐµÐ»Ñ ÑÐ°Ð±Ð¾ÑÑ â Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ¾Ð¶Ð´ÐµÐ½Ð¸Ñ ÐºÑÐ¼ÑÐ»ÑÑÐ¸Ð²Ð½ÑÑ Ð¿ÑÐ¾ÑÐ¾Ð½Ð¾Ð² Ð² ÑÑÐ¾Ð»ÐºÐ½Ð¾Ð²ÐµÐ½Ð¸ÑÑ ÑÐ´ÐµÑ Â¹Â²C Ð¸ â¹Be Ð² ÑÐ°Ð¼ÐºÐ°Ñ Ð¼Ð¾Ð´ÐµÐ»Ð¸ Ð²Ð½ÑÑÑÐ¸ÑÐ´ÐµÑÐ½Ð¾Ð³Ð¾ ÐºÐ°ÑÐºÐ°Ð´Ð° ÐÑÐµÐ¶ÑÐºÐ¾Ð¹ Ð³ÑÑÐ¿Ð¿Ñ. Ð ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½ Ð¼ÐµÑÐ°Ð½Ð¸Ð·Ð¼ ÑÐ¾Ð¶Ð´ÐµÐ½Ð¸Ñ ÐºÑÐ¼ÑÐ»ÑÑÐ¸Ð²Ð½ÑÑ Ð¿ÑÐ¾ÑÐ¾Ð½Ð¾Ð², Ð¿Ð¾ÑÑÑÐ¾ÐµÐ½Ð½ÑÐ¹ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ ÐÐ¾Ð½ÑÐµ-ÐÐ°ÑÐ»Ð¾ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐµÐ°ÐºÑÐ¸Ð¸ 12C+9Be. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¾ ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ðµ Ñ Ð´Ð°Ð½Ð½ÑÐ¼Ð¸ ÑÐºÑÐ¿ÐµÑÐ¸Ð¼ÐµÐ½ÑÐ° FRAGM Ð¸ Ð¿ÑÐµÐ´ÑÐºÐ°Ð·Ð°Ð½Ð¸ÑÐ¼Ð¸ Ð¼Ð¾Ð´ÐµÐ»Ð¸ ÐºÐ²Ð°ÑÐºÐ¾Ð²ÑÑ ÐºÐ»Ð°ÑÑÐµÑÐ¾Ð².
title: ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð·Ð°Ð²Ð¸ÑÐ¸Ð¼Ð¾ÑÑÐ¸ ÑÑÐ¾Ð¸Ð¼Ð¾ÑÑÐ¸ ÑÐ²Ð¾Ð±Ð¾Ð´Ð½Ð¾Ð³Ð¾ Ð·ÐµÐ¼ÐµÐ»ÑÐ½Ð¾Ð³Ð¾ ÑÑÐ°ÑÑÐºÐ° Ð¾Ñ Ð²ÑÑÐ¾ÑÑ ÑÑÑÐ¾ÐµÐ½Ð¸Ñ Ð¸ Ð¿Ð»Ð¾ÑÐ°Ð´Ð¸ Ð·Ð°ÑÑÑÐ¾Ð¹ÐºÐ¸
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÑÑÐ»Ð¾Ð²Ð°, ÐÐ½Ð½Ð°
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: Ð¾ÑÐµÐ½ÐºÐ° Ð½ÐµÐ´Ð²Ð¸Ð¶Ð¸Ð¼Ð¾ÑÑÐ¸
Ð¾Ð¿ÐµÑÐ°ÑÐ¸Ð¾Ð½Ð½Ñe ÑÐ°ÑÑ Ð¾Ð´Ñ
Ð¾ÑÐ¸ÑÐ½Ð°Ñ ÑÑÐ½ÐºÑÐ¸Ñ
ÑÑÐ¾Ð¸Ð¼Ð¾ÑÑÑ Ð·ÐµÐ¼Ð»Ð¸

description: ÐÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð° Ð¾ÑÐµÐ½ÐºÐ° Ð·ÐµÐ¼ÐµÐ»ÑÐ½Ð¾Ð³Ð¾ ÑÑÐ°ÑÑÐºÐ° Ð¸ Ð²ÑÐ±ÑÐ°Ð½Ð¾ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð¾ Ð·Ð´Ð°Ð½Ð¸Ñ Ð¾ÑÐ¸ÑÐ½Ð¾Ð¹ ÑÑÐ½ÐºÑÐ¸Ð¸. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÑÐ½ÐºÐ° Ð¾ÑÐ¸ÑÐ½Ð¾Ð¹ Ð½ÐµÐ´Ð²Ð¸Ð¶Ð¸Ð¼Ð¾ÑÑÐ¸. ÐÐ·ÑÑÐµÐ½Ð¾ Ð²Ð»Ð¸ÑÐ½Ð¸Ðµ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð° Ð·Ð´Ð°Ð½Ð¸Ñ ÑÐ°Ð·Ð½Ð¾Ð¹ ÑÑÐ°Ð¶Ð½Ð¾ÑÑÐ¸ Ð½Ð° ÑÑÐ¾Ð¸Ð¼Ð¾ÑÑÑ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÐµÐ¼Ð¾Ð³Ð¾ Ð¾Ð±ÑÐµÐºÑÐ°. Ð Ð°ÑÑÑÐ¸ÑÐ°Ð½ ÐºÐ¾ÑÑÑÐ¸ÑÐ¸ÐµÐ½Ñ Ð¾Ð¿ÐµÑÐ°ÑÐ¸Ð¾Ð½Ð½ÑÑ ÑÐ°ÑÑÐ¾Ð´Ð¾Ð². ÐÑÐ±ÑÐ°Ð½ Ð¾Ð¿ÑÐ¸Ð¼Ð°Ð»ÑÐ½ÑÐ¹ Ð²Ð°ÑÐ¸Ð°Ð½Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð·ÐµÐ¼ÐµÐ»ÑÐ½Ð¾Ð³Ð¾ ÑÑÐ°ÑÑÐºÐ° Ð¸ Ð´Ð»Ñ Ð½ÐµÐ³Ð¾ Ð¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐ¸ÑÐºÐ¾Ð².
L’inflazione cosmica raddoppia
Creators: Corrado Ruscica
Publisher: name: Media Inaf
Year: 2016

L'Universo avrebbe subìto non uno bensì due periodi di rapida espansione esponenziale immediatamente dopo il Big Bang. È quanto emerge da uno studio condotto da un gruppo di fisici del BNL, Fermilab e della Stony Brook University che propone un nuovo modello per spiegare l’abbondanza della misteriosa materia oscura presente nel nostro Universo. I risultati su Physical Review Letters
L’insostenibile leggerezza dell’intuizione
Creators: Caterina Boccato
Publisher: name: Media Inaf
Year: 2016

Selezionata oggi 15 gennaio, a Padova, la cinquina che andrà in finale: Umberto Bottazzini, Dario Bressanini con Beatrice Mautino, Paolo Gallina, Till Roenneberg e Lucia Votano. L'opera vincitrice, scelta da una giuria popolare, verrà annunciata il 6 maggio
Revolution analysis of three-dimensional arbitrary cloaks
Creators: name: Dupont, Guillaume
name: Guenneau, Sébastien
name: Enoch, Stefan
name: Demésy, Guillaume
name: Nicolet, Andre
name: Zolla, Frédéric
name: Diatta, Andre
Publisher: name: arXiv
Year: 2009
Subjects: subject: Optics (physics.optics)
subject: Mathematical Physics (math-ph)
subject: Computational Physics (physics.comp-ph)
subject: FOS: Physical sciences

description: We extend the design of radially symmetric three-dimensional invisibility cloaks through transformation optics to cloaks with a surface of revolution. We derive the expression of the transformation matrix and show that one of its eigenvalues vanishes on the inner boundary of the cloaks, while the other two remain strictly positive and bounded. The validity of our approach is confirmed by finite edge-elements computations for a non-convex cloak of varying thickness.
description: 6 pages, 4 figures
SRT pronto a nuove sfide
Creators: Silvia Casu
Publisher: name: Media Inaf
Year: 2016

Delegazione NASA e ASI in visita all'antenna. Grazie alla sua sensibilità, oltre ai suoi compiti scientifici potrebbe essere usata per monitorare oggetti potenzialmente pericolosi (asteroidi, meteore, comete e spazzatura spaziale) e per le attività di ricezione dei segnali delle sonde interplanetarie