cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: ÐÑÐ±Ð¾Ñ Ð¾Ð¿ÑÐµÑÐ½Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð¹ ÑÐ°ÑÑÐ¸ Ð¼Ð½Ð¾Ð³Ð¾ÑÐµÐ»ÐµÐ²ÑÑ Ð°ÑÐ¾Ð¼Ð½ÑÑ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ¾Ð² Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÑÑÑÐ°Ð½ ÐÐ»Ð¸Ð¶Ð½ÐµÐ³Ð¾ ÐÐ¾ÑÑÐ¾ÐºÐ° Ð¸ Ð¡ÐµÐ²ÐµÑÐ½Ð¾Ð¹ ÐÑÑÐ¸ÐºÐ¸
title: ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÑ 2.4.6. Ð¢ÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ°Ñ Ð¸ Ð¿ÑÐ¸ÐºÐ»Ð°Ð´Ð½Ð°Ñ ÑÐµÐ¿Ð»Ð¾ÑÐµÑ Ð½Ð¸ÐºÐ°
titleType: Subtitle
Creators: name: Ð¡Ð¾ÐºÐ¾Ð»Ð¾Ð²Ð°, 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: 2023
Subjects: ÐÐ¾Ð´Ð°
Ð¯Ð´ÐµÑÐ½ÑÐµ ÑÐµÐ°ÐºÑÐ¾ÑÑ
Ð¡ÐµÐ²ÐµÑÐ½Ð°Ñ ÐÑÑÐ¸ÐºÐ°
ÐÐ»Ð¸Ð¶Ð½Ð¸Ð¹ ÐÐ¾ÑÑÐ¾Ðº
Ð¾Ð¿ÑÐµÑÐ½Ð¸ÑÐµÐ»ÑÐ½Ð°Ñ ÑÑÑÐ°Ð½Ð¾Ð²ÐºÐ°
Ð°ÑÐ¾Ð¼Ð½Ð¾Ðµ Ð¾Ð¿ÑÐµÑÐ½ÐµÐ½Ð¸Ðµ
ÑÐµÑ Ð½Ð¸ÐºÐ¾-ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð°Ð½Ð°Ð»Ð¸Ð·

description: ÐÑÐ±Ð¾Ñ Ð¾Ð¿ÑÐµÑÐ½Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð¹ ÑÐ°ÑÑÐ¸ Ð¼Ð½Ð¾Ð³Ð¾ÑÐµÐ»ÐµÐ²ÑÑ Ð°ÑÐ¾Ð¼Ð½ÑÑ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ¾Ð² Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÑÑÑÐ°Ð½ ÐÐ»Ð¸Ð¶Ð½ÐµÐ³Ð¾ ÐÐ¾ÑÑÐ¾ÐºÐ° Ð¸ Ð¡ÐµÐ²ÐµÑÐ½Ð¾Ð¹ ÐÑÑÐ¸ÐºÐ¸. ÐÐ°Ð½Ð½Ð°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ ÑÐµÑÐ½Ð¸ÐºÐ¾-ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¿Ð¾ Ð²ÑÐ±Ð¾ÑÑ Ð½Ð°Ð¸Ð±Ð¾Ð»ÐµÐµ Ð¿Ð¾Ð´ÑÐ¾Ð´ÑÑÐ¸Ñ Ð¼Ð¾ÑÐ½Ð¾ÑÑÐµÐ¹, ÑÑÑÑÐºÑÑÑ Ð¸ ÑÐ¾ÑÑÐ°Ð²Ð° Ð¾Ð¿ÑÐµÑÐ½Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð¹ ÑÐ°ÑÑÐ¸ Ð¼Ð½Ð¾Ð³Ð¾ÑÐµÐ»ÐµÐ²Ð¾Ð³Ð¾ Ð°ÑÐ¾Ð¼Ð½Ð¾Ð³Ð¾ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ° Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð¿Ð¾ÑÑÐµÐ±Ð½Ð¾ÑÑÐµÐ¹ Ð¸ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÐµÐ¹ ÑÐ¸Ð¿Ð¸ÑÐ½Ð¾Ð³Ð¾ ÑÑÐ´Ð° ÑÑÑÐ°Ð½ Ð¸ Ñ Ð¿Ð¾Ð¼Ð¾ÑÑÑ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð½Ð¾Ð¹ Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ¸.
Cacciatori di Blazar
Creators: Marco Galliani
Publisher: name: Media Inaf
Year: 2016

Due ricercatori italiani, Raffaele D’Abrusco e Francesco Massaro, insieme ad un team internazionale di astronomi di cui fanno parte anche Nicola Masetti e Marco Landoni dell’INAF, hanno sviluppato un nuovo metodo per selezionare tra le sorgenti infrarosse quei ‘candidati blazar’ che potenzialmente corrispondessero a emissioni gamma non identificate. Individuando e confermando così l'esistenza di oltre 200 oggetti di questo tipo
Criticality and entanglement in random quantum systems
Creators: name: Refael, Gil
name: Moore, Joel E.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We review studies of entanglement entropy in systems with quenched randomness, concentrating on universal behavior at strongly random quantum critical points. The disorder-averaged entanglement entropy provides insight into the quantum criticality of these systems and an understanding of their relationship to non-random ("pure") quantum criticality. The entanglement near many such critical points in one dimension shows a logarithmic divergence in subsystem size, similar to that in the pure case but with a different universal coefficient. Such universal coefficients are examples of universal critical amplitudes in a random system. Possible measurements are reviewed along with the one-particle entanglement scaling at certain Anderson localization transitions. We also comment briefly on higher dimensions and challenges for the future.
description: Review article for the special issue "Entanglement entropy in extended systems" in J. Phys. A
Towards Parameterized Regular Type Inference Using Set Constraints
Creators: name: Bueno, F.
name: Navas, J.
name: Hermenegildo, M.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Logic in Computer Science (cs.LO)
subject: Programming Languages (cs.PL)
subject: FOS: Computer and information sciences

description: We propose a method for inferring \emph{parameterized regular types} for logic programs as solutions for systems of constraints over sets of finite ground Herbrand terms (set constraint systems). Such parameterized regular types generalize \emph{parametric} regular types by extending the scope of the parameters in the type definitions so that such parameters can relate the types of different predicates. We propose a number of enhancements to the procedure for solving the constraint systems that improve the precision of the type descriptions inferred. The resulting algorithm, together with a procedure to establish a set constraint system from a logic program, yields a program analysis that infers tighter safe approximations of the success types of the program than previous comparable work, offering a new and useful efficiency vs. precision trade-off. This is supported by experimental results, which show the feasibility of our analysis.
title: ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð´Ð¾Ð·Ñ ÑÐ¾ÑÐ¾Ð½Ð¾Ð² Ð²ÑÑÐ¾ÐºÐ¸Ñ ÑÐ½ÐµÑÐ³Ð¸Ð¹ Ð² ÑÐºÐ°Ð½ÐµÑÐºÐ²Ð¸Ð²Ð°Ð»ÐµÐ½ÑÐ½Ð¾Ð¹ ÑÑÐµÐ´Ðµ
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¼Ð°Ð³Ð¸ÑÑÑÐ°
titleType: Subtitle
Creators: name: Ð¡Ð¸Ð»Ð¸Ð½, ÐÐ°Ð²ÐµÐ»
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Ð½Ð°Ñ ÑÐ¸Ð·Ð¸ÐºÐ°
Ð¤Ð¾ÑÐ¾Ð½Ñ
ÐÐ¾Ð½ÑÐµ-ÐÐ°ÑÐ»Ð¾ Ð¼ÐµÑÐ¾Ð´
ÐÑÑÐ¸ÑÐ»Ð¸ÑÐµÐ»ÑÐ½ÑÐµ Ð¼Ð°ÑÐ¸Ð½Ñ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½ÑÐµ
ÐÐ¾Ð½Ð¸Ð·Ð¸ÑÑÑÑÐ¸Ðµ Ð¸Ð·Ð»ÑÑÐµÐ½Ð¸Ñ

description: Ð ÑÐ°Ð±Ð¾ÑÐµ Ð¸Ð·ÑÑÐµÐ½ Ð¿Ð¾Ð´ÑÐ¾Ð´ Ðº Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð³Ð»Ð¾ÑÐµÐ½Ð½Ð¾Ð¹ Ð´Ð¾Ð·Ñ ÑÐ¾ÑÐ¾Ð½Ð¾Ð² Ð²ÑÑÐ¾ÐºÐ¸Ñ ÑÐ½ÐµÑÐ³Ð¸Ð¹ Ð² ÑÐºÐ°Ð½ÐµÑÐºÐ²Ð¸Ð²Ð°Ð»ÐµÐ½ÑÐ½Ð¾Ð¼ ÑÐ°Ð½ÑÐ¾Ð¼Ðµ ÑÑÐµÐ´ÑÑÐ²Ð°Ð¼Ð¸ ÑÑÐµÐ¹Ð¼Ð²Ð¾ÑÐºÐ° GEANT4. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÐ¸ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð¾Ð³Ð¾ ÐºÐ¾Ð´Ð° Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ GEANT4. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð° ÑÐ°ÑÑÐµÑÐ° ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð³Ð»Ð¾ÑÐµÐ½Ð½Ð¾Ð¹ Ð´Ð¾Ð·Ñ Ð² Ð²Ð¾ÐºÑÐµÐ»ÑÐ½Ð¾Ð¼ ÑÐºÐ°Ð½ÐµÑÐºÐ²Ð¸Ð²Ð°Ð»ÐµÐ½ÑÐ½Ð¾Ð¼ ÑÐ°Ð½ÑÐ¾Ð¼Ðµ Ð´Ð»Ñ ÑÐ°Ð·Ð½ÑÑ ÑÐ¸Ð¿Ð¾Ð² Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ¾Ð² ÑÐ¾ÑÐ¾Ð½Ð¾Ð² Ð²ÑÑÐ¾ÐºÐ¸Ñ ÑÐ½ÐµÑÐ³Ð¸Ð¹. ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¾ ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ðµ Ð¿ÑÐ¾ÑÐµÐ½ÑÐ½Ð¾Ð¹ Ð³Ð»ÑÐ±Ð¸Ð½Ð½Ð¾Ð¹ Ð´Ð¾Ð·Ñ Ð²Ð±Ð»Ð¸Ð·Ð¸ Ð¿Ð¾Ð²ÐµÑÑÐ½Ð¾ÑÑÐ¸ ÑÐµÐ»Ð° Ð¿Ð°ÑÐ¸ÐµÐ½ÑÐ° Ð¿ÑÐ¸ Ð¾Ð±Ð»ÑÑÐµÐ½Ð¸Ð¸ ÑÐ¾ÑÐ¾Ð½Ð°Ð¼Ð¸ Ð²ÑÑÐ¾ÐºÐ¸Ñ ÑÐ½ÐµÑÐ³Ð¸Ð¹ ÑÐµÑÐµÐ· ÑÐµÑÐ°Ð¿ÐµÐ²ÑÐ¸ÑÐµÑÐºÐ¸Ð¹ ÑÑÐ¾Ð».
Quasi-linear regime and rare-event tails of decaying Burgers turbulence
Creators: name: Valageas, P.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: We study the decaying Burgers dynamics in $d$ dimensions for random Gaussian initial conditions. We focus on power-law initial energy spectra, such that the system shows a self-similar evolution. This is the case of interest for the "adhesion model" in cosmology and a standard framework for "decaying Burgers turbulence". We briefly describe how the system can be studied through perturbative expansions at early time or large scale (quasi-linear regime). Next, we develop a saddle-point method, based on spherical instantons, that allows to obtain the asymptotic probability distributions $\cP(η_r)$ and $\cP(\ctheta_r)$, of the density and velocity increment over spherical cells, reached in the quasi-linear regime. Finally, we show how this approach can be extended to take into account the formation of shocks and we derive the rare-event tails of these probability distributions, at any finite time and scale. This also gives the high-mass tail of the mass function of point-like singularities (shocks in the one dimensional case).
description: 32 pages
title: ÐÑ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°: ÑÑÑÑÐºÑÑÑÐ°, Ð¾ÑÐ¾ÑÐ¼Ð»ÐµÐ½Ð¸Ðµ, Ð·Ð°ÑÐ¸ÑÐ°
title: ÑÑÐµÐ±Ð½Ð¾-Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐ²Ð°Ð½ÑÐµÐ½ÐºÐ¾, ÐÐ»Ñ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: 2021
Subjects: Ð²ÑÐ¿ÑÑÐºÐ½ÑÐµ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½ÑÐµ ÑÐ°Ð±Ð¾ÑÑ
Ð½Ð°ÑÑÐ½ÑÐµ ÑÐ°Ð±Ð¾ÑÑ
Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ¸Ð°Ñ

description: Ð£ÑÐµÐ±Ð½Ð¾-Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð², Ð¾Ð±ÑÑÐ°ÑÑÐ¸ÑÑÑ Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ¸Ð°ÑÐ° 19.03.01 Â«ÐÐ¸Ð¾ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÂ» Ð²ÑÐµÑ ÑÐ¾ÑÐ¼ Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ, Ð²ÑÐ¿Ð¾Ð»Ð½ÑÑÑÐ¸Ñ Ð²ÑÐ¿ÑÑÐºÐ½ÑÐµ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½ÑÐµ ÑÐ°Ð±Ð¾ÑÑ. Ð Ð¿Ð¾ÑÐ¾Ð±Ð¸Ð¸ Ð¸Ð·Ð»Ð¾Ð¶ÐµÐ½Ñ Ð¿ÑÐ°Ð²Ð¸Ð»Ð° Ð¾ÑÐ¾ÑÐ¼Ð»ÐµÐ½Ð¸Ñ Ð²ÑÐ¿ÑÑÐºÐ½ÑÑ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½ÑÑ ÑÐ°Ð±Ð¾Ñ Ð² ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²Ð¸Ð¸ Ñ ÑÑÐµÐ±Ð¾Ð²Ð°Ð½Ð¸ÑÐ¼Ð¸ ÑÑÐ°Ð½Ð´Ð°ÑÑÐ¾Ð², Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÐ½Ñ ÑÐ²ÐµÐ´ÐµÐ½Ð¸Ñ Ð¾ ÑÑÑÑÐºÑÑÑÐµ Ð¸ ÑÐ¾Ð´ÐµÑÐ¶Ð°Ð½Ð¸Ð¸ ÑÐ°Ð±Ð¾ÑÑ. ÐÐ¾Ð´ÑÐ¾Ð±Ð½Ð¾ Ð¾Ð¿Ð¸ÑÐ°Ð½Ñ Ð¿ÑÐ°Ð²Ð¸Ð»Ð° Ð¾ÑÐ¾ÑÐ¼Ð»ÐµÐ½Ð¸Ñ ÑÐ¸ÑÑÐ½ÐºÐ¾Ð², ÑÐ°Ð±Ð»Ð¸Ñ. ÐÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ Ð¿ÑÐ¸Ð¼ÐµÑÑ Ð¾ÑÐ¾ÑÐ¼Ð»ÐµÐ½Ð¸Ñ ÑÐ¸ÑÑÐ»ÑÐ½Ð¾Ð³Ð¾ Ð»Ð¸ÑÑÐ°, Ð·Ð°Ð´Ð°Ð½Ð¸Ñ, ÑÐ¿Ð¸ÑÐºÐ° Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð½ÑÑ Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ¾Ð², Ð¾ÑÐ·ÑÐ²Ð° ÑÑÐºÐ¾Ð²Ð¾Ð´Ð¸ÑÐµÐ»Ñ Ð¸ ÑÐµÑÐµÐ½Ð·Ð¸Ð¸, ÑÐµÑÑÐµÐ¶ÐµÐ¹.
Single-angle to multi-angle transition in the collective flavor dynamics
  of neutrinos in supernovae
Creators: name: Baldo, Marcello
name: Palmisano, Vincenzo
Publisher: name: INFN Open Access Repository
Year: 2012

description: In this paper we study in detail the dynamics of flavor transformation for
neutrinos propagating in the very dense environment of astrophysical compact
objects as Type II supernova in post collapse phase and proto-neutron stars.
The analysis is based on the formalism by Strack and Burrows, who introduced
the generalized Boltzmann equation for Wigner phase space density. In
appropriate limits the formalism reduces to the usual evolution equations for
the wave functions or for density matrix elements of Liouville equation. We
incorporate the most important aspects of neutrino propagation physics: the
phenomenology of standard oscillations with MSW resonance induced by ordinary
matter, collective behavior due to self-interaction, which can produce bipolar
and synchronized flavor oscillations, whose relevance is recognized by recent
literature, the combination of these effects with collisions including
scattering, emission and absorption of neutrinos.
title: ÐÐ»Ð³Ð¾ÑÐ¸ÑÐ¼Ñ Ð¿Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ñ ÐºÐ¾Ð»Ð¾ÑÐ¸ÑÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð³Ð°Ð¼Ð¼ Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ ÑÐ¸ÑÑÐ¾Ð²ÑÑ ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¹
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°Ð¹Ð½ÑÐ»Ð¸Ð½Ð°, 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: 2017
Subjects: Ð¦Ð²ÐµÑ
ÐÐ¾Ð¼Ð¿ÑÑÑÐµÑÐ½Ð¾Ðµ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
ÐÐµÐ»ÑÐ¸ (Delphi)
ÐºÐ¾Ð»Ð¾ÑÐ¸ÑÑÐ¸ÑÐµÑÐºÐ°Ñ Ð³Ð°Ð¼Ð¼Ð°
ÑÐ²ÐµÑÐ¾Ð²Ð°Ñ Ð¼Ð¾Ð´ÐµÐ»Ñ
Ð²ÐµÐºÑÐ¾ÑÐ½Ð¾Ðµ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ ÑÐ²ÐµÑÐ°
ÐºÐ¾Ð¼Ð¿Ð¾Ð½ÐµÐ½ÑÑ ÑÐ²ÐµÑÐ°
Ð¼Ð°ÑÑÐ¸ÑÐ½ÑÐµ Ð²ÑÑÐ¸ÑÐ»ÐµÐ½Ð¸Ñ

description: Ð Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ¾Ð¹ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ð¸ Ð¸Ð·Ð»Ð¾Ð¶ÐµÐ½ Ð¿ÑÐ¾ÑÐµÑÑ ÑÐ¾ÑÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÐºÐ¾Ð»Ð¾ÑÐ¸ÑÑÐ¸ÑÐµÑÐºÐ¾Ð¹ Ð³Ð°Ð¼Ð¼Ñ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð²ÐµÐºÑÐ¾ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ RGB ÐºÐ¾Ð¼Ð¿Ð¾Ð½ÐµÐ½ÑÐ¾Ð² Ð¸Ð·Ð¾Ð±ÑÐ°Ð¶ÐµÐ½Ð¸Ñ. ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¾ Ð²Ð¾ÑÐ¿ÑÐ¸ÑÑÐ¸Ðµ Ð³ÑÐ°ÑÐ¸ÑÐµÑÐºÐ¾Ð¹ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¸, Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð´Ð°Ð½Ð½ÑÑ, ÑÐ¾ÑÑÐ°Ð²Ð»ÐµÐ½Ñ Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½ Ð¿ÑÐ¾ÑÐ¾ÑÐ¸Ð¿ ÑÐ°Ð±Ð¾ÑÐµÐ¹ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ñ.
Luna e Terra shakerate ad arte
Creators: Marco Malaspina
Publisher: name: Media Inaf
Year: 2016

Non c’è differenza apprezzabile fra le abbondanze d’isotopi d’ossigeno presenti nelle rocce terrestri e in quelle lunari. Lo studio, uscito oggi su Science, conferma e rafforza uno scenario già ipotizzato. Media INAF ha intervistato uno degli autori, Alessandro Morbidelli, dell’Osservatorio di Nizza
Deuteron magnetic resonance properties in deuterated modifications of methane
Creators: name: De Wit, Gerald Aloysius
Publisher: name: University of British Columbia
Year: 2011

description: Relaxation properties of the deuteron spin system in CD₄ and CD₃H were studied in the temperature range from 105°K - 57°K. These results show that the intra-molecular quadrupole interactions dominate and the relaxation occurs through the molecular reorientations of the molecule. The deuteron spin-lattice relaxation times are approximately temperature independent, except for a small contribution from the magnetic dipolar interactions near the melting point in CD₃H. From this data it is concluded that the reorientatlonal correlation time is temperature independent. The deuteron T₂ shows the same temperature dependence as the proton T₂; the deuteron T₂ can be accounted for on the basis of magnetic dipolar interactions alone.
La geometria dei Babilonesi per inseguire Giove
Creators: Stefano Parisini
Publisher: name: Media Inaf
Year: 2016

Le fondamenta del calcolo integrale potrebbero essere state gettate dagli astronomi e sacerdoti babilonesi, almeno 14 secoli prima di quanto conosciuto finora. È la novità più eclatante riportata nell’articolo sul metodo di calcolo geometrico del movimento di Giove rintracciato in antiche tavolette cuneiformi, in copertina sull’ultimo numero di Science. Media INAF ha intervistato l’autore, Mathieu Ossendrijver della Università Humboldt di Berlino
Models for TMDs and numerical methods
Creators: name: B. Pasquini
name: C. Lorce'
Publisher: name: INFN Open Access Repository
Year: 2012

description: We study the connection between the quark orbital angular momentum and the
pretzelosity transverse-momentum dependent parton distribution function. We
discuss the origin of this relation in quark models, identifying as key
ingredient for its validity the assumption of spherical symmetry for the
nucleon in its rest frame. Finally we show that the individual quark
contributions to the orbital angular momentum obtained from this relation can
not be interpreted as the intrinsic contributions, but include the contribution
from the transverse centre of momentum which cancels out only in the total
orbital angular momentum.
UDT Position Paper December 2022
Creators: name: Meyers, Natalie
name: Agostini, Caterina
name: Hawkins, Michael
name: Johnson, Daniel
name: Ralley, Robert
name: Jefferies, Neil
name: Zimmern, Arnaud
name: Goulding, Robert
name: Van Hulle, Dirk
name: Gooch, Megan
Publisher: name: Open Science Framework
Year: 2023

description: Position paper issued as a precursor to workshops, December 2022
Suppression of high-pT heavy-flavour particles in Pb-Pb collisions at
  the LHC, measured with the ALICE detector
Creators: name: Dainese, Andrea
name: For The ALICE Collaboration
Publisher: name: INFN Open Access Repository
Year: 2012

description: The ALICE experiment studies nucleus-nucleus collisions at the LHC in order
to investigate the properties of QCD matter at extreme energy densities. The
measurement of open charm and open beauty production allows one to probe the
mechanisms of heavy-quark propagation, energy loss and hadronization in the hot
and dense medium formed in high-energy nucleus-nucleus collisions. In
particular, in-medium energy loss is predicted to be different for massless
partons (light quarks and gluons) and heavy quarks at moderate momentum. The
ALICE apparatus allows us to measure open heavy-flavour particles in several
decay channels and with a wide phase-space coverage.
  We present the results on the nuclear modification factors for heavy-flavour
particle production in Pb-Pb collisions at sqrtsNN=2.76 TeV. Using
proton-proton and lead-lead collision samples at sqrts=2.76 and 7 TeV and at
sqrtsNN=2.76 TeV, respectively, nuclear modification factors R_AA(pT) were
measured for D mesons at central rapidity (via displaced decay vertex
reconstruction), and for electrons and muons from heavy-flavour decays, at
central and forward rapidity, respectively. A large suppression is observed, by
a factor 2.5-4 in central Pb--Pb collisions with respect to the pp reference,
in the high-pT region, indicating a strong in-medium energy loss of heavy
quarks.
Convective motions and net circular polarization in sunspot penumbrae
Creators: name: Borrero, J. M.
name: Solanki, S. K.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We have employed a penumbral model, that includes the Evershed flow and convective motions inside penumbral filaments, to reproduce the azimuthal variation of the net circular polarization (NCP) in sunspot penumbrae at different heliocentric angles for two different spectral lines. The theoretical net circular polarization fits the observations as satisfactorily as penumbral models based on flux-tubes. The reason for this is that the effect of convective motions on the NCP is very small compared to the effect of the Evershed flow. In addition, the NCP generated by convective upflows cancels out the NCP generated by the downflows. We have also found that, in order to fit the observed NCP, the strength of the magnetic field inside penumbral filaments must be very close to 1000 G. In particular, field-free or weak-field filaments fail to reproduce both the correct sign of the net circular polarization, as well as its dependence on the azimuthal and heliocentric angles.
description: Accepted for publication in the Astrophysical Journal. 10 pages, 7 figures (3 in color). Uses emulatedapj
title: ÐÐ¾ÑÐ¿ÑÐ¸ÑÑÐ¸Ðµ ÑÐµÐºÐ»Ð°Ð¼Ñ Ð²ÑÐ·Ð¾Ð² ÑÑÐ°ÑÐ¸Ð¼Ð¸ÑÑ ÑÑÐ°ÑÑÐ¸Ñ ÐºÐ»Ð°ÑÑÐ¾Ð²
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¼Ð°Ð³Ð¸ÑÑÑÐ°
titleType: Subtitle
Creators: name: Ð¡Ð°Ð²ÑÐµÐ½ÐºÐ¾, Ð£Ð»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: 2018
Subjects: Ð²Ð¾ÑÐ¿ÑÐ¸ÑÑÐ¸Ðµ
Ð¾Ð±ÑÐ°Ð·
ÑÐµÐºÐ»Ð°Ð¼Ð°
Ð²ÑÐ·Ñ

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ñ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¾Ð± Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÑÑ ÑÐµÐºÐ»Ð°Ð¼Ð½Ð¾Ð³Ð¾ Ð²Ð¾Ð·Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ, Ð¿ÑÐ¸ÑÐ¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ñ Ð°ÑÐ¿ÐµÐºÑÐ°Ñ Ð¸Ð·ÑÑÐµÐ½Ð¸Ñ ÑÐµÐºÐ»Ð°Ð¼Ñ ÐÐ£ÐÐ¾Ð², Ð¿ÑÐ¾ÑÐµÑÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ð¼ ÑÐ°Ð¼Ð¾Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ð¸ Ð² Ð¾ÑÐµÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð¸ Ð·Ð°ÑÑÐ±ÐµÐ¶Ð½Ð¾Ð¹ Ð»Ð¸ÑÐµÑÐ°ÑÑÑÐµ. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ ÐºÐ¾Ð½ÑÐµÐ½Ñ â Ð°Ð½Ð°Ð»Ð¸Ð· Ð¸ Ð¾ÑÐ±Ð¾Ñ ÑÐµÐºÐ»Ð°Ð¼Ð½ÑÑ Ð¿Ð»Ð°ÐºÐ°ÑÐ¾Ð² ÐÐ£ÐÐ¾Ð², Ð¸ÑÐ¿Ð¾Ð»ÑÐ·ÑÑÑÐ¸Ñ ÑÐ¼Ð¾ÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½ÑÐ¹ Ð¸ ÑÐ°ÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½ÑÐ¹ ÑÐ¸Ð¿ Ð²Ð¾Ð·Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ. ÐÐ·ÑÑÐµÐ½Ñ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸Ñ Ðº ÑÐµÐºÐ»Ð°Ð¼Ðµ ÐÐ£ÐÐ¾Ð² ÑÑÐ°ÑÐ¸Ð¼Ð¸ÑÑ ÑÑÐ°ÑÑÐ¸Ñ ÐºÐ»Ð°ÑÑÐ¾Ð² Ð² Ð·Ð°Ð²Ð¸ÑÐ¸Ð¼Ð¾ÑÑÐ¸ Ð¾Ñ ÑÑÐµÐ¿ÐµÐ½Ð¸ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð¿ÑÐ¾ÑÐµÑÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð²ÑÐ±Ð¾ÑÐ°, Ð°ÐºÑÑÐ°Ð»ÑÐ½Ð¾ÑÑÐ¸ ÑÐ¸ÑÑÐ°ÑÐ¸Ð¸ Ð²ÑÐ±Ð¾ÑÐ° ÑÐ¾ÑÐ¼Ñ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ. ÐÑÑÐ²Ð»ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÐºÐ¾Ð½ÑÑÑÑÐºÑÑ, ÑÑÑÐµÑÑÐ²ÑÑÑÐ¸Ðµ Ñ ÑÑÐ°ÑÑÐµÐºÐ»Ð°ÑÑÐ½Ð¸ÐºÐ¾Ð² Ð² Ð¿ÑÐ¾ÑÐµÑÑÐµ Ð²Ð¾ÑÐ¿ÑÐ¸ÑÑÐ¸Ñ ÑÐµÐºÐ»Ð°Ð¼Ñ ÐÐ£ÐÐ¾Ð²: Ð°Ð²ÑÐ¾ÑÐ¸ÑÐµÑÐ½Ð¾ÑÑÑ, ÑÐ²Ð¾ÐµÐ¾Ð±ÑÐ°Ð·Ð¸Ðµ Ð²ÑÐ·Ð°, Ð´Ð¾ÑÑÑÐ¿Ð½Ð¾ÑÑÑ Ð¸ ÐºÐ¾Ð½ÑÐ°ÐºÑÐ½Ð¾ÑÑÑ Ð²ÑÐ·Ð°. ÐÐ·ÑÑÐµÐ½Ð° ÑÐ¿ÐµÑÐ¸ÑÐ¸ÐºÐ° Ð²Ð¾ÑÐ¿ÑÐ¸ÑÑÐ¸Ñ ÑÐµÐºÐ»Ð°Ð¼Ñ ÐÐ£ÐÐ¾Ð² ÑÑÐ°ÑÐ¸Ð¼Ð¸ÑÑ ÑÑÐ°ÑÑÐ¸Ñ ÐºÐ»Ð°ÑÑÐ¾Ð² Ð² Ð·Ð°Ð²Ð¸ÑÐ¸Ð¼Ð¾ÑÑÐ¸ Ð¾Ñ ÑÑÐµÐ¿ÐµÐ½Ð¸ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð¿ÑÐ¾ÑÐµÑÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð²ÑÐ±Ð¾ÑÐ°, Ð°ÐºÑÑÐ°Ð»ÑÐ½Ð¾ÑÑÐ¸ ÑÐ¸ÑÑÐ°ÑÐ¸Ð¸ Ð²ÑÐ±Ð¾ÑÐ° ÑÐ¾ÑÐ¼Ñ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ.
On the Observation of the Cosmic Ray Anisotropy below 10$^{15}$ eV
Creators: name: G. Di Sciascio
name: R. Iuppa
Publisher: name: INFN Open Access Repository
Year: 2014

description: The measurement of the anisotropy in the arrival direction of cosmic rays is
complementary to the study of their energy spectrum and chemical composition to
understand their origin and propagation. It is also a tool to probe the
structure of the magnetic fields through which cosmic rays travel. As cosmic
rays are mostly charged nuclei, their trajectories are deflected by the action
of galactic magnetic field they propagate through before reaching the Earth
atmosphere, so that their detection carries directional information only up to
distances as large as their gyro-radius. If cosmic rays below
$10^{15}{\rm\,eV}$ are considered and the local galactic magnetic field
($\sim3{\rm\,\mu G}$) is accounted for, gyro-radii are so short that isotropy
is expected. At most, a weak di-polar distribution may exist, reflecting the
contribution of the closest CR sources. However, a number of experiments
observed an energy-dependent \emph{"large scale"} anisotropy in the sidereal
time frame with an amplitude of about 10$^{-4}$ - 10$^{-3}$, revealing the
existence of two distinct broad regions: an excess distributed around
40$^{\circ}$ to 90$^{\circ}$ in Right Ascension (commonly referred to as
"tail.in" excess) and a deficit (the "loss cone") around 150$^{\circ}$ to
240$^{\circ}$ in Right Ascension. In recent years the Milagro and ARGO-YBJ
collaborations reported the of a "medium" scale anisotropy inside the tail-in
region. The observation of such small features has been recently claimed by the
IceCube experiment also in the Southern hemisphere. So far, no theory of cosmic
rays in the Galaxy exists which is able to explain the origin of these
different anisotropies leaving the standard model of cosmic rays and that of
the galactic magnetic field unchanged at the same time.
(Sr_3Sc_2O_5)Fe_2As_2 as a possible parent compound for FeAs-based superconductors
Creators: name: Zhu, Xiyu
name: Han, Fei
name: Mu, Gang
name: Zeng, Bin
name: Cheng, Peng
name: Shen, Bing
name: Wen, Hai-Hu
Publisher: name: arXiv
Year: 2008
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: A new compound with the FeAs-layers, namely (Sr_3Sc_2O_5)Fe_2As_2 (abbreviated as FeAs-32522), was successfully fabricated. It has a layered structure with the space group of I4/mmm, and with the lattice constants a = 4.069 $Å$ and c = 26.876 $Å$. The in-plane Fe ions construct a square lattice which is close to that of other FeAs-based superconductors, such as REFeAsO (RE = rare earth elements) and (Ba,Sr)Fe_2As_2. However the inter FeAs-layer spacing in the new compound is greatly enlarged. The temperature dependence of resistivity exhibits a weak upturn in the low temperature region, but a metallic behavior was observed above about 60 K. The magnetic susceptibility shows also a non-monotonic behavior. Interestingly, the well-known resistivity anomaly which was discovered in all other parent compounds, such as REFeAsO, (Ba,Sr)Fe_2As_2 and (Sr,Ca,Eu)FeAsF and associated with the Spin-Density-Wave (SDW)/structural transition has not been found in the new system either on the resistivity data or the magnetization data. This could be induced by the large spacing distance between the FeAs-planes, therefore the antiferromagnetic correlation between the moments of Fe ions in neighboring FeAs-layers cannot be established. Alternatively it can also be attributed to the self-doping effect between Fe and Sc ions. The Hall coefficient R_H is negative but strongly temperature dependent in wide temperature region, which indicates the dominance of electrical conduction by electron-like charge carriers and probably a multi-band effect or a spin related scattering effect. It is found that the magnetoresistance cannot be described by the Kohler's rule, which gives further support to above arguments.
description: 5 pages, 5 figures, some contents added, and one figure added
Are we really seeing dark matter signals from the Milky Way center?
Creators: name: Gomez-Vargas, German A.
Publisher: name: INFN Open Access Repository
Year: 2014

description: The center of the Milky Way is one of the most interesting regions of the
$\gamma$-ray sky because of the potential for indirect dark matter (DM)
detection. It is also complicated due to the many sources and uncertainties
associated with the diffuse $\gamma$-ray emission. Many independent groups have
claimed a DM detection in the data collected by the Large Area Telescope on
board the Fermi $\gamma$-ray Satellite from the inner Galaxy region at energies
below 10 GeV. However, an exotic signal needs to be disentangled from the data
using a model of known $\gamma$-ray emitters, i.e. a background model. We point
out that deep understanding of background ingredients and their main
uncertainties is of capital importance to disentangle a dark matter signal from
the Galaxy center.
On the multipole moments of a rigidly rotating fluid body
Creators: name: Filter, Robert
name: Kleinwächter, Andreas
Publisher: name: arXiv
Year: 2009
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: Based on numerical simulations and analytical calculations we formulate a new conjecture concerning the multipole moments of a rigidly rotating fluid body in equilibrium. The conjecture implies that the exterior region of such a fluid is not described by the Kerr metric.
description: 5 pages, 4 figures, to appear in Annalen der Physik
title: ÐÐµÑÑÐ¾Ð»Ð¾Ð³Ð¸Ñ, ÑÑÐ°Ð½Ð´Ð°ÑÑÐ¸Ð·Ð°ÑÐ¸Ñ Ð¸ ÑÐµÑÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¸Ñ. ÐÑÐ±Ð¾Ñ ÑÑÐµÐ´ÑÑÐ² Ð¸Ð·Ð¼ÐµÑÐµÐ½Ð¸Ñ
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÑÐ±Ð¾Ð¼ÑÐ´ÑÐ¾Ð², Ð¡ÐµÑÐ³ÐµÐ¹
name: Ð¢Ð°ÑÐ°ÑÐ¾Ð², Ð¡ÑÐ°Ð½Ð¸ÑÐ»Ð°Ð²
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2008
Subjects: ÐÐµÑÑÐ¾Ð»Ð¾Ð³Ð¸Ñ
Ð¡ÑÐ°Ð½Ð´Ð°ÑÑÐ¸Ð·Ð°ÑÐ¸Ñ

description: ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÐµÑ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð¼Ñ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾Ð¼Ñ ÑÑÐ°Ð½Ð´Ð°ÑÑÑ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ñ Â«ÐÐµÑÑÐ¾Ð»Ð¾Ð³Ð¸Ñ, ÑÑÐ°Ð½Ð´Ð°ÑÑÐ¸Ð·Ð°ÑÐ¸Ñ Ð¸ ÑÐµÑÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¸ÑÂ». Ð Ð¿Ð¾ÑÐ¾Ð±Ð¸Ð¸ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð²Ð¾Ð¿ÑÐ¾ÑÑ Ð²ÑÐ±Ð¾ÑÐ° ÑÑÐµÐ´ÑÑÐ² Ð¸Ð·Ð¼ÐµÑÐµÐ½Ð¸Ñ Ð»Ð¸Ð½ÐµÐ¹Ð½ÑÑ Ð¸ ÑÐ³Ð»Ð¾Ð²ÑÑ ÑÐ°Ð·Ð¼ÐµÑÐ¾Ð², Ð° ÑÐ°ÐºÐ¶Ðµ Ð´Ð°Ð½Ñ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¿Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¸Ð·Ð¼ÐµÑÐ¸ÑÐµÐ»ÑÐ½ÑÑ Ð¿ÑÐ¸ÑÐ¿Ð¾ÑÐ¾Ð±Ð»ÐµÐ½Ð¸Ð¹ Ð´Ð»Ñ ÐºÐ¾Ð½ÑÑÐ¾Ð»Ñ ÑÐ¾ÑÐ¼Ñ Ð¸ Ð²Ð·Ð°Ð¸Ð¼Ð½Ð¾Ð³Ð¾ ÑÐ°ÑÐ¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð²ÐµÑÑÐ½Ð¾ÑÑÐµÐ¹ Ð´ÐµÑÐ°Ð»ÐµÐ¹. ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð¼ÐµÑÐ°Ð½Ð¸ÐºÐ¾-Ð¼Ð°ÑÐ¸Ð½Ð¾ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ ÑÐ°ÐºÑÐ»ÑÑÐµÑÐ°, Ð²ÑÐ¿Ð¾Ð»Ð½ÑÑÑÐ¸Ñ ÐºÑÑÑÐ¾Ð²Ð¾Ð¹ Ð¿ÑÐ¾ÐµÐºÑ Ð¿Ð¾ Ð¼ÐµÑÑÐ¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð¼Ñ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð°.
description: ÐÐµÑÐ°ÑÐ°ÐµÑÑÑ Ð¿Ð¾ ÑÐµÑÐµÐ½Ð¸Ñ ÑÐµÐ´Ð°ÐºÑÐ¸Ð¾Ð½Ð½Ð¾-Ð¸Ð·Ð´Ð°ÑÐµÐ»ÑÑÐºÐ¾Ð³Ð¾ ÑÐ¾Ð²ÐµÑÐ° Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¾Ð³Ð¾ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ°.
#givemefiveplanets: 5 pianeti per uno scatto
Creators: Francesca Aloisio
Publisher: name: Media Inaf
Year: 2016

Avete già programmato un’uscita dedicata a osservare i 5 pianeti che in questi giorni si possono vedere in fila nel cielo del mattino? Ricordatevi di portare la macchina fotografica: gli scatti che ci invierete saranno pubblicati in un blog dedicato. E se non siete dei professionisti niente paura: vanno bene anche disegni o foto con il cellulare. Partecipate numerosi!
Future Extensive Air Shower arrays: from Gamma-Ray Astronomy to Cosmic
  Rays
Creators: name: Sciascio, Giuseppe Di
Publisher: name: INFN Open Access Repository
Year: 2015

description: Despite large progresses in building new detectors and in the analysis
techniques, the key questions concerning the origin, acceleration and
propagation of Galactic Cosmic Rays are still open. A number of new EAS arrays
is in progress. The most ambitious and sensitive project between them is
LHAASO, a new generation multi-component experiment to be installed at very
high altitude in China (Daocheng, Sichuan province, 4400 m a.s.l.). The
experiment will face the open problems through a combined study of photon- and
charged particle-induced extensive air showers in the wide energy range
10$^{11}$ - 10$^{18}$ eV. In this paper the status of the experiment will be
summarized, the science program presented and the outlook discussed in
comparison with leading new projects.
5 pianeti: come fotografarli
Creators: Davide Coero Borga
Publisher: name: Media Inaf
Year: 2016

Intervista a Matteo Dunchi, astrofotografo e astrofilo. Tutte le istruzioni necessarie per fare un ritratto mozzafiato al filotto planetario che nei prossimi giorni luccicherà sull’orizzonte italiano. Smartphone, action-cam, fotocamere professionali: ce n’è per tutti
SKA: sempre più vicini all’accordo
Creators: Eleonora Ferroni
Publisher: name: Media Inaf
Year: 2016

Presso l’Accademia dei Lincei, la seconda tornata dei negoziati preparatori per la trasformazione della SKA Organisation in un’organizzazione intergovernativa (IGO) regolata da un trattato. A guida della fase negoziale è ancora l’Italia che presiede tutto il procedimento
title: ÐÐ¸Ð½Ð³Ð²Ð¾ÐºÑÐ»ÑÑÑÑÐ½ÑÐµ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÑÐ°Ð½ÐºÐ¾ÑÐ¾Ð½Ð½Ð¾Ð³Ð¾ Ð¿ÐµÑÐµÐ½Ð½Ð¾Ð³Ð¾ Ð´Ð¸ÑÐºÑÑÑÐ°
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¾ÑÑÑÐµÐ², 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: 2018
Subjects: Ð»Ð¸Ð½Ð³Ð²Ð¾ÐºÑÐ»ÑÑÑÑÐ¾Ð»Ð¾Ð³Ð¸Ñ
Ð¿ÐµÑÐµÐ½Ð½ÑÐ¹ Ð´Ð¸ÑÐºÑÑÑ
ÑÑÐ°Ð½ÐºÐ¾ÑÐ¾Ð½Ð¸Ñ
ÑÐ°Ð½ÑÐ¾Ð½

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¸Ð·Ð»Ð¾Ð¶ÐµÐ½Ñ Ð±Ð°Ð·Ð¾Ð²ÑÐµ Ð¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ ÑÐµÐ¾ÑÐ¸Ð¸ Ð´Ð¸ÑÐºÑÑÑÐ°, Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ñ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð»Ð¸Ð½Ð³Ð²Ð¾ÐºÑÐ»ÑÑÑÑÐ¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿Ð¾Ð´ÑÐ¾Ð´Ð° Ðº Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ð°ÑÐ¸ÐºÐµ. ÐÑÑÐ²Ð»ÐµÐ½Ñ ÑÐ°ÑÐ°ÐºÑÐµÑÐ½ÑÐµ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð¿ÐµÑÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÐµÐºÑÑÐ°. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð´Ð¸ÑÐºÑÑÑÐ½ÑÐ¹ Ð¸ ÑÑÐ¸Ð»Ð¸ÑÑÐ¸ÑÐµÑÐºÐ¸Ð¹ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð° Ð¸ ÑÑÐ¾ÑÐ¼ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ ÑÑÐ°Ð½ÐºÐ¾ÑÐ¾Ð½Ð½Ð¾Ð³Ð¾ Ð¿ÐµÑÐµÐ½Ð½Ð¾Ð³Ð¾ Ð´Ð¸ÑÐºÑÑÑÐ°.
Sensitivity of spin-torque diodes for frequency-tunable resonant microwave detection
Creators: name: Wang, C.
name: Cui, Y. -T.
name: Sun, J. Z.
name: Katine, J. A.
name: Buhrman, R. A.
name: Ralph, D. C.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We calculate the efficiency with which magnetic tunnel junctions can be used as resonant detectors of incident microwave radiation via the spin-torque diode effect. The expression we derive is in good agreement with the sensitivities we measure for MgO-based magnetic tunnel junctions with an extended (unpatterned) magnetic pinned layer. However, the measured sensitivities are reduced below our estimate for a second set of devices in which the pinned layer is a patterned synthetic antiferromagnet (SAF). We suggest that this reduction may be due to an undesirable coupling between the magnetic free layer and one of the magnetic layers within the etched SAF. Our calculations suggest that optimized tunnel junctions should achieve sensitivities for resonant detection exceeding 10,000 mV/mW.
description: 17 pages, 2 figures
Breaking the symmetries of the bulb model in two-dimensional
  self-induced supernova neutrino flavor conversions
Creators: name: Mirizzi, Alessandro
Publisher: name: INFN Open Access Repository
Year: 2015

description: Self-induced flavor conversions of supernova (SN) neutrinos have been
characterized in the spherically symmetric "bulb model", reducing the neutrino
evolution to a one dimensional problem along a radial direction. We lift this
assumption, presenting a two-dimensional model where neutrinos are launched
from a spherical neutrino-sphere with many zenithal angles and two azimuthal
angles. We also assume that self-induced conversions are not suppressed by
large matter effects. In this situation we find that self-interacting neutrinos
spontaneously break axial and spherical symmetries. As a result the flavor
content and the lepton number of the neutrino gas would acquire seizable
direction-dependent variations, breaking the coherent behavior found in the
spherically symmetric case. This finding would suggest that the previous
results of the self-induced flavor evolution obtained in one-dimensional models
should be critically re-examined.
Adozioni stellari
Creators: Elisa Nichelli
Publisher: name: Media Inaf
Year: 2016

Uno studio condotto da un team internazionale di astronomi, guidato da ricercatori del Kavli Institute for Astronomy and Astrophysics di Pechino, ha analizzato le immagini raccolte dal telescopio spaziale Hubble per tre ammassi globulari all’interno delle Nubi di Magellano. I dati mostrano che le generazioni più giovani di stelle sarebbero prodotte da gas “adottato” da regioni esterne agli ammassi
title: ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ ÐºÐ¾Ð¼Ð±Ð¸Ð½Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ ÑÐ¾ÑÐ¾Ð´Ð¸Ð½Ð°Ð¼Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð²Ð¾Ð·Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ Ð¸ ÑÐ¸ÑÐ¾ÑÑÐ°ÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð°Ð³ÐµÐ½ÑÐ° Ð½Ð° Ð¼Ð¾Ð´ÐµÐ»ÑÐ½ÑÑ Ð¾Ð¿ÑÑ Ð¾Ð»ÐµÐ²ÑÑ ÐºÐ»ÐµÑÐ¾ÑÐ½ÑÑ ÐºÑÐ»ÑÑÑÑÐ°Ñ
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ°ÑÐµÐ¿Ð¸Ð½, ÐÑÑÐµÐ¼
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: Ð¾Ð½ÐºÐ¾Ð»Ð¾Ð³Ð¸Ñ
ÑÐ¸ÑÐ¿Ð»Ð°ÑÐ¸Ð½
ÑÐ¾ÑÐ¾Ð´Ð¸Ð½Ð°Ð¼Ð¸ÑÐµÑÐºÐ¾Ðµ Ð²Ð¾Ð·Ð´ÐµÐ¹ÑÑÐ²Ð¸Ðµ
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ÐºÐ¾Ð¼Ð±Ð¸Ð½Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ðµ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ðµ

description: Ð¦ÐµÐ»Ñ: Ð²ÑÑÐ²Ð»ÐµÐ½Ð¸Ðµ Ð¿ÑÐµÐ¸Ð¼ÑÑÐµÑÑÐ² ÐºÐ¾Ð¼Ð±Ð¸Ð½Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ ÑÐ¸ÑÐ¿Ð»Ð°ÑÐ¸Ð½Ð° Ð¸ ÑÐ¾ÑÐ¾Ð´Ð¸Ð½Ð°Ð¼Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð²Ð¾Ð·Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ ÑÐ°Ð´Ð°ÑÐ»Ð¾ÑÐ¸Ð½Ð° Ð² ÐºÐ°ÑÐµÑÑÐ²Ðµ ÑÐ¾ÑÐ¾ÑÐµÐ½ÑÐ¸Ð±Ð¸Ð»Ð¸Ð·Ð°ÑÐ¾ÑÐ° Ð¿Ð¾ ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ñ Ñ Ð¸Ð½Ð´Ð¸Ð²Ð¸Ð´ÑÐ°Ð»ÑÐ½ÑÐ¼ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ Ð´Ð°Ð½Ð½ÑÑ Ð²Ð¾Ð·Ð´ÐµÐ¹ÑÑÐ²Ð¸Ð¹ in vitro. ÐÐ±ÑÐµÐºÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ: ÐºÐ»ÐµÑÐ¾ÑÐ½ÑÐµ Ð»Ð¸Ð½Ð¸Ð¸ HeLa Ð¸ K562. ÐÐ¾Ð»ÑÑÐµÐ½Ð½ÑÐ¹ ÑÐµÐ·ÑÐ»ÑÑÐ°Ñ: Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ðµ ÐºÐ¾Ð¼Ð±Ð¸Ð½Ð°ÑÐ¸Ð¸ ÑÐ¸ÑÐ¿Ð»Ð°ÑÐ¸Ð½Ð° Ð¸ ÑÐ¾ÑÐ¾Ð´Ð¸Ð½Ð°Ð¼Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð²Ð¾Ð·Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ Ð¿ÑÐ¸Ð²Ð¾Ð´Ð¸Ñ Ðº ÑÐ½Ð¸Ð¶ÐµÐ½Ð¸Ñ Ð²ÑÐ¶Ð¸Ð²Ð°ÐµÐ¼Ð¾ÑÑÐ¸ Ð¾Ð±ÐµÐ¸Ñ ÐºÐ»ÐµÑÐ¾ÑÐ½ÑÑ Ð»Ð¸Ð½Ð¸Ð¹ Ð¸ ÑÐ²ÐµÐ»Ð¸ÑÐµÐ½Ð¸Ñ Ð¿ÑÐ¾ÑÐµÐ½ÑÐ° Ð°Ð¿Ð¾Ð¿ÑÐ¾ÑÐ¸ÑÐµÑÐºÐ¸Ñ ÐºÐ»ÐµÑÐ¾Ðº Ð² Ð¿ÑÐ¾Ð±Ð°Ñ Ð¿Ð¾ ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ñ Ñ Ð¾ÑÐ´ÐµÐ»ÑÐ½ÑÐ¼ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸ÐµÐ¼ Ð´Ð°Ð½Ð½ÑÑ Ð²Ð¾Ð·Ð´ÐµÐ¹ÑÑÐ²Ð¸Ð¹. Ð­ÑÑÐµÐºÑ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð½ÑÑ ÐºÐ¾Ð¼Ð±Ð¸Ð½Ð°ÑÐ¸Ð¹ Ð² Ð·Ð°Ð²Ð¸ÑÐ¸Ð¼Ð¾ÑÑÐ¸ Ð¾Ñ ÑÐ¾Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸Ñ Ð´Ð¾Ð· Ð²Ð¾Ð·Ð´ÐµÐ¹ÑÑÐ²Ð¸Ð¹ Ð²Ð°ÑÑÐ¸ÑÑÐµÑÑÑ Ð¾Ñ Ð°Ð´Ð´Ð¸ÑÐ¸Ð²Ð½Ð¾Ð³Ð¾ Ð´Ð¾ ÑÐ¸Ð½ÐµÑÐ³Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾.
The decay of Sb 125, Sn 113 and Ba 133.
Creators: name: Chaturvedi, Ram Prakash
Publisher: name: University of British Columbia
Year: 2011

description: A modified thin lens spectrometer has been used with improved geometry. The focussing properties of the instrument have been investigated for various geometries. Using this instrument the conversion electron spectra of Sn¹¹³ and Sb¹²⁵ have been taken. The intensity of the 256 kev conversion line in Sn¹¹³ spectrum showed that this transition is predominantly M1 in character and therefore the spin and parity of 648-kev level in In¹¹³ should be 1/2¯ or 3/2¯. The low energy part of the conversion spectrum of Sb¹²⁵showed the presence of the K conversion lines of 76 kev and 143 kev transitions, not observed before. The presence of these conversion lines confirmed the existence of a weak beta group feeding a level at 540 kev in the excited state of Te¹²⁵. The energy levels of Cs¹³³ have been studied through the decay of Ba¹³³. Scintillation spectra (using NaI(T1 ) crystal) together with photoelectron, conversion and e-gamma coincidence spectra have been taken. An analysis of the results indicate that the ground state and 81, 161, 383 and 437 kev levels in Cs¹³³ have spins and parities of 7/2⁺, 5/2⁺,5/2⁺,3/2⁺, 1/2⁺ respectively. The multipolarities of the connecting transitions are 383 kev (E2 ), 356 (E2 ) 302 kev (M1 with E2 admixture)} 276 kev (E2 ), 161 kev (probably M1 ) Electron capture from Ba¹³³ is limited almost entirely to the 437 and 383 kev levels in Cs¹³³, The decay energy available for capture to the 437 level is approximately 50 kev.
title: ÐÑÐ½Ð¾Ð²Ñ ÑÐºÐ¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð¹ Ñ Ð¸Ð¼Ð¸Ð¸. Ð§. 1
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐ»Ð¸Ð½Ð¾Ð², ÐÐµÐ²
name: ÐÑÐºÐ¸Ð½Ð°, Ð¢Ð°ÑÑÑÐ½Ð°
name: Ð¢Ð°Ð½ÑÑÑÐ°, ÐÐ°Ð´ÐµÐ¶Ð´Ð°
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2009
Subjects: ÐÑ ÑÐ°Ð½Ð° Ð¾ÐºÑÑÐ¶Ð°ÑÑÐµÐ¹ ÑÑÐµÐ´Ñ
Ð­ÐºÐ¾Ð»Ð¾Ð³Ð¸Ñ
Ð¥Ð¸Ð¼Ð¸Ñ

description: ÐÐ° Ð±Ð°Ð·Ðµ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð¸Ð¹ Ð¸ ÐºÐ¾Ð½ÑÐµÐ¿ÑÐ¸Ð¹, ÑÐ¾ÑÑÐ°Ð²Ð»ÑÑÑÐ¸Ñ Ð¾ÑÐ½Ð¾Ð²Ñ Ð¾Ð±ÑÐµÐ¹ Ð¸ Ð½ÐµÐ¾ÑÐ³Ð°Ð½Ð¸ÑÐµÑÐºÐ¾Ð¹ ÑÐ¸Ð¼Ð¸Ð¸; ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑÑÑ ÑÐ¸Ð¼Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ¾ÑÑÐ°Ð² Ð¾ÑÐ½Ð¾Ð²Ð½ÑÑ Ð¾Ð±Ð¾Ð»Ð¾ÑÐµÐº Ð¿Ð»Ð°Ð½ÐµÑÑ (Ð°ÑÐ¼Ð¾ÑÑÐµÑÑ, Ð³Ð¸Ð´ÑÐ¾ÑÑÐµÑÑ, Ð»Ð¸ÑÐ¾ÑÑÐµÑÑ, Ð±Ð¸Ð¾ÑÑÐµÑÑ) Ð¸ ÑÐ¸Ð·Ð¸ÐºÐ¾-ÑÐ¸Ð¼Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¿ÑÐ¾ÑÐµÑÑÑ, Ð¿ÑÐ¾ÑÐµÐºÐ°ÑÑÐ¸Ðµ Ð² Ð¾ÐºÑÑÐ¶Ð°ÑÑÐµÐ¹ ÑÑÐµÐ´Ðµ Ñ ÑÑÐ°ÑÑÐ¸ÐµÐ¼ Ð·Ð°Ð³ÑÑÐ·Ð½Ð¸ÑÐµÐ»ÐµÐ¹ Ð°Ð½ÑÑÐ¾Ð¿Ð¾Ð³ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾Ð¸ÑÑÐ¾Ð¶Ð´ÐµÐ½Ð¸Ñ. ÐÑÐ¸Ð²Ð¾Ð´ÑÑÑÑ Ð¿ÑÐ¸Ð¼ÐµÑÑ Ð²Ð¾Ð·Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ ÑÐ¸Ð¼Ð¸ÑÐµÑÐºÐ¸Ñ Ð·Ð°Ð³ÑÑÐ·Ð½Ð¸ÑÐµÐ»ÐµÐ¹ Ð½Ð° ÐºÐ¾Ð¼Ð¿Ð¾Ð½ÐµÐ½ÑÑ Ð¾Ð±Ð¾Ð»Ð¾ÑÐµÐº Ð¿Ð»Ð°Ð½ÐµÑÑ, ÑÐ°ÑÑÐ¸ÑÐµÐ»ÑÐ½ÑÐ¹ Ð¸ Ð¶Ð¸Ð²Ð¾ÑÐ½ÑÐ¹ Ð¼Ð¸Ñ, ÑÐµÑÐ½Ð¾ÑÑÐµÑÑ Ð¸ Ð±Ð¸Ð¾ÑÑÐµÑÑ. ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² 1-2-Ð³Ð¾ ÐºÑÑÑÐ¾Ð² ÑÐ°ÐºÑÐ»ÑÑÐµÑÐ¾Ð² ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð¸ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð¾Ð², ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð¹ ÐºÐ¸Ð±ÐµÑÐ½ÐµÑÐ¸ÐºÐ¸, ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ¸ Ð¸ Ð¼ÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½ÑÐ°, Ð¸Ð½Ð¶ÐµÐ½ÐµÑÐ½Ð¾-ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾, Ð²ÐµÑÐµÑÐ½ÐµÐ³Ð¾ ÑÐ°Ð´Ð¸Ð¾ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¸ ÐÐ½ÑÑÐ¸ÑÑÑÐ° Ð¸Ð½ÑÐµÐ»Ð»ÐµÐºÑÑÐ°Ð»ÑÐ½ÑÑ ÑÐ¸ÑÑÐµÐ¼ Ð¸ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¹, Ð¸Ð·ÑÑÐ°ÑÑÐ¸Ñ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ñ: "Ð¥Ð¸Ð¼Ð¸Ñ", "Ð­ÐºÐ¾Ð»Ð¾Ð³Ð¸Ñ", "Ð­ÐºÐ¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ°Ñ ÑÐ¸Ð¼Ð¸Ñ", "ÐÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÑ Ð¶Ð¸Ð·Ð½ÐµÐ´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸", "ÐÑÐ½Ð¾Ð²Ñ Ð¸Ð½Ð¶ÐµÐ½ÐµÑÐ½Ð¾Ð¹ Ð¾ÑÑÐ°Ð½Ñ Ð¾ÐºÑÑÐ¶Ð°ÑÑÐµÐ¹ ÑÑÐµÐ´Ñ".
description: ÐÐµÑÐ°ÑÐ°ÐµÑÑÑ Ð¿Ð¾ ÑÐµÑÐµÐ½Ð¸Ñ ÑÐµÐ´Ð°ÐºÑÐ¸Ð¾Ð½Ð½Ð¾-Ð¸Ð·Ð´Ð°ÑÐµÐ»ÑÑÐºÐ¾Ð³Ð¾ ÑÐ¾Ð²ÐµÑÐ° Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¾Ð³Ð¾ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ°.
Nota de Reorientação Epistemológica - As travessias (e travessuras) do senso de justiça
Creators: name: Dias Fortes, Pablo Dias Fortes
Publisher: name: Zenodo
Year: 2025
Subjects: Ontologia relacional
Comparação e reciprocidade
Filosofia do vínculo
Inteligência artificial generativa
ética
bioética
Antropoceno
Gongsheng
Cosmotécnica
Fenomenologia da presença
Ética do cuidado
Pacto pneumático

description: Esta nota de reorientação epistemológica apresenta os fundamentos conceituais e existenciais da reformulação da pesquisa As travessias (e travessuras) do senso de justiça, à luz de um processo reflexivo motivado pela confluência entre experiências vivenciais contemporâneas, transformações sociais e técnicas do Antropoceno, e a mediação de uma inteligência artificial generativa como ferramenta fenomenotécnica. Propõe-se uma chave hermenêutico-fenomenológica centrada nas categorias relacionais de comparação e reciprocidade, inspirada na ontologia do vínculo de Martin Buber e ampliada por diálogos com a crítica cultural de Sloterdijk, a mediação hermenêutica de Ricoeur, a filosofia do gongsheng de Bing Song, a fenomenologia sinocentrada de Xianglong Zhang e a cosmotécnica de Yuk Hui. A nota culmina na defesa de uma filosofia do vínculo como eixo ético e epistemológico para pensar o justo em tempos de colapso relacional, ampliando os horizontes da bioética e das práticas de cuidado diante das mediações técnicas contemporâneas.
Knowledge, attitude, perceived barriers, and practices among pharmacists regarding risk assessment of cardiovascular disease: a cross-sectional study in Yemen
Creators: name: Al-Ashwal, Fahmi Y.
name: Sulaiman, Syed Azhar Syed
name: Ghadzi, Siti Maisharah Sheikh
name: Kubas, Mohammed Abdullah
name: Halboup, Abdulsalam
Publisher: name: Taylor & Francis
Year: 2021
Subjects: subject: Medicine
subject: Pharmacology
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy

description: Risk evaluation of atherosclerotic cardiovascular diseases can guide the decision-making on various preventive measures, such as initiating or deferring statin therapy. Pharmacists can play an active part in the risk evaluation and primary prevention of atherosclerotic cardiovascular diseases. Thus, our study aimed to assess the pharmacists’ knowledge, attitude, perceived barriers, and practices regarding risk assessment of atherosclerotic cardiovascular disease. A cross-sectional study was conducted among 500 pharmacists using a structured validated questionnaire between November 2020 and February 2021. The Mann–Whitney and Kruskal–Wallis tests were used to analyze the data. A total of 456 pharmacists completed the questionnaire out of 500 distributed (91.2% response rate). Over 60% of participants responded with never or rarely for two out of five cardiovascular diseases (CVD) prevention practices. The lowest pharmacist-patient counseling practices were for side effects of statin medication (14.5%) and reviewing the patient’s medications to avoid potential statin-drug interactions (31.8%). Participants had a high positive attitude (median = 34 out of 40). The three major barriers for risk assessment were the lack of support (74.8%), the lack of resources (70.6%), and inadequate training (48.7%). Interestingly, having ≤75 customers a day, community pharmacies, PharmD degree, age ≥30 years, and experience ≥6 years were significantly associated (p < .05) with higher CVD prevention activities and counseling practices. Pharmacists have a high positive attitude toward CVD risk assessment. However, they had insufficient knowledge and only provided limited activities and counseling services for CVD prevention and statin therapy. Participants perceived several barriers to CVD risk assessment services in pharmacies. Therefore, it is necessary to remove these impediments for pharmacists to be more involved in CVD risk assessment and prevention. Also, continuing medical education and adequate training for pharmacists are required.
Il cielo di Anne
Creators: Marco Malaspina
Publisher: name: Media Inaf
Year: 2016

L’anno scorso, su queste pagine, abbiamo ricordato il Giorno della Memoria parlando di persone: di astronomi italiani costretti dalle leggi razziali ad abbandonare il proprio lavoro. Oggi proviamo invece a ricordarlo con un diario e con un luogo. Un luogo che comincia là dove finisce quel diario
D-modules on 1|1 Supercurves
Creators: name: Rothstein, Mitchell J.
name: Rabin, Jeffrey M.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Algebraic Geometry (math.AG)
subject: High Energy Physics - Theory (hep-th)
subject: Mathematical Physics (math-ph)
subject: FOS: Mathematics
subject: FOS: Physical sciences
subject: 14M30; 32C11

description: It is known that to every 1|1 dimensional supercurve X there is associated a dual supercurve \hat{X}, and a superdiagonal Δin their product. We establish that the categories of D-modules on X, \hat{X}, and Δare equivalent. This follows from a more general result about D-modules and purely odd submersions. The equivalences preserve tensor products, and take vector bundles to vector bundles. Line bundles with connection are studied, and examples are given where X is a superelliptic curve.
description: 18 pages
title: ÐÐ²ÐµÐ´ÐµÐ½Ð¸Ðµ Ð² Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÑ Ð¸Ð·Ð¾Ð±ÑÐ°Ð¶ÐµÐ½Ð¸Ð¹ Ð½Ð° ÑÐ·ÑÐºÐµ Python
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: Ð¡Ð°ÑÐ°Ð´Ð¶Ð¸ÑÐ²Ð¸Ð»Ð¸, Ð¡ÐµÑÐ³ÐµÐ¹
name: ÐÐµÐ¾Ð½ÑÑÐµÐ², ÐÐ»Ð°Ð´Ð¸Ð¼Ð¸Ñ
name: ÐÐ¾Ð¸Ð½Ð¾Ð², ÐÐ¸ÐºÐ¸ÑÐ°
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2020
Subjects: ÐÐ¸ÑÐ¾Ð½ (Python)
ÐÐ·Ð¾Ð±ÑÐ°Ð¶ÐµÐ½Ð¸Ñ

description: Ð£ÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ ÑÐ²Ð»ÑÐµÑÑÑ Ð´Ð¾Ð¿Ð¾Ð»Ð½Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð¹ Ð»Ð¸ÑÐµÑÐ°ÑÑÑÐ¾Ð¹ Ð¿Ð¾ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ðµ Â«Ð¦Ð¸ÑÑÐ¾Ð²Ð°Ñ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¼Ð½Ð¾Ð³Ð¾Ð¼ÐµÑÐ½ÑÑ ÑÐ¸Ð³Ð½Ð°Ð»Ð¾Ð²Â» Ð¸ Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ Ð¾ÑÐ²Ð¾ÐµÐ½Ð¸Ñ Ð»ÐµÐºÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð°, Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð·Ð°Ð½ÑÑÐ¸Ð¹, Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ ÑÐ°ÑÑÐµÑÐ½ÑÑ Ð·Ð°Ð´Ð°Ð½Ð¸Ð¹ Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾Ð³Ð¾ Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÐ° Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð¸Ð·Ð¾Ð±ÑÐ°Ð¶ÐµÐ½Ð¸Ð¹ Ð½Ð° ÑÐ·ÑÐºÐµ Python. ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð²ÑÑÑÐ¸Ñ ÑÑÐµÐ±Ð½ÑÑ Ð·Ð°Ð²ÐµÐ´ÐµÐ½Ð¸Ð¹, Ð¾Ð±ÑÑÐ°ÑÑÐ¸ÑÑÑ Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸ÑÐ¼ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð¼Ð°Ð³Ð¸ÑÑÑÐ¾Ð² Â«ÐÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð°Ñ Ð¸Ð½Ð¶ÐµÐ½ÐµÑÐ¸ÑÂ» Ð¸ Â«ÐÐ½ÑÐ¾ÑÐ¼Ð°ÑÐ¸ÐºÐ° Ð¸ Ð²ÑÑÐ¸ÑÐ»Ð¸ÑÐµÐ»ÑÐ½Ð°Ñ ÑÐµÑÐ½Ð¸ÐºÐ°Â». ÐÐ½Ð¾ Ð¼Ð¾Ð¶ÐµÑ Ð±ÑÑÑ ÑÐ°ÐºÐ¶Ðµ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¾ Ð² ÑÐ¸ÑÑÐµÐ¼Ð°Ñ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¸, Ð² ÑÑÑÐµÐ¶Ð´ÐµÐ½Ð¸ÑÑ Ð´Ð¾Ð¿Ð¾Ð»Ð½Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÑÐµÑÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ.
description: The training manual is additional literature on the course "Digital processing of multidimensional signals" and is intended for mastering the lecture material, practical exercises, performing calculation tasks using an effective image processing tool in the Python language. It is intended for students of higher education institutions, studying in the master's degree programs "Software Engineering" and "Computer Science and Computer Engineering". It can also be useful in advanced training systems, in institutions of supplementary vocational education.
‘Elettroshock’ per BepiColombo
Creators: Redazione ASI
Publisher: name: Media Inaf
Year: 2016

Eseguiti i test di compatibilità all’interno della ‘Camera di Maxwell’ dell’orbiter della missione ESA. Il lancio della missione ESA-JAXA dedicata allo studio del pianeta Mercurio è programmato per il 27 gennaio 2017
title: Ð£ÑÑÑ Ð¸ Ð°ÑÐ´Ð¸Ñ ÑÐ°ÑÑÑÑÐ¾Ð² Ð¿Ð¾ Ð¾Ð¿Ð»Ð°ÑÐµ ÑÑÑÐ´Ð°, ÐºÐ°Ðº ÑÐ»ÐµÐ¼ÐµÐ½Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð¾Ð¼
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð¤Ð°Ð·ÑÐ»Ð·ÑÐ½Ð¾Ð²Ð° , ÐÐ½Ð¶ÐµÐ»Ð¸ÐºÐ°
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ÐµÑ ÑÐ°ÑÑÐµÑÐ¾Ð²
Ð°ÑÐ´Ð¸Ñ ÑÐ°ÑÑÐµÑÐ¾Ð²
ÑÑÐµÑ ÑÐ°ÑÑÐµÑÐ¾Ð² Ñ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð¾Ð¼ Ð¿Ð¾ Ð¾Ð¿Ð»Ð°ÑÐµ ÑÑÑÐ´Ð°

description: Ð Ð¿ÐµÑÐ²Ð¾Ð¹ Ð³Ð»Ð°Ð²Ðµ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¾ÑÐ½Ð¾Ð²Ñ ÑÑÐµÑÐ° Ð¸ Ð°ÑÐ´Ð¸ÑÐ° ÑÑÑÐ´Ð° Ð¸ ÐµÐ³Ð¾ Ð¾Ð¿Ð»Ð°ÑÑ: ÑÐµÐ»Ñ, ÑÑÐ½ÐºÑÐ¸Ð¸ Ð¸ ÑÐ¾ÑÐ¼Ñ Ð¾Ð¿Ð»Ð°ÑÑ ÑÑÑÐ´Ð°, ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð¾ Ð½Ð¾ÑÐ¼Ð°ÑÐ¸Ð²Ð½Ð¾Ðµ ÑÐµÐ³ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¸ Ð¾ÑÑÐ°Ð¶ÐµÐ½Ð¸Ðµ Ð½Ð° ÑÑÐµÑÐ°Ñ Ð±ÑÑÐ³Ð°Ð»ÑÐµÑÑÐºÐ¾Ð³Ð¾ ÑÑÐµÑÐ° Ð·Ð°ÑÐ°Ð±Ð¾ÑÐ½Ð¾Ð¹ Ð¿Ð»Ð°ÑÑ, Ð° ÑÐ°ÐºÐ¶Ðµ ÑÐµÐ»Ñ, Ð·Ð°Ð´Ð°ÑÐ¸ Ð¸ Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ¸ Ð°ÑÐ´Ð¸ÑÐ° ÑÐ°ÑÑÐµÑÐ¾Ð² Ñ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð¾Ð¼ Ð¿Ð¾ Ð¾Ð¿Ð»Ð°ÑÐµ ÑÑÑÐ´Ð°. ÐÐ¾ Ð²ÑÐ¾ÑÐ¾Ð¹ Ð³Ð»Ð°Ð²Ðµ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð´ÐµÐ¹ÑÑÐ²ÑÑÑÐµÐ¹ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÑÐµÑÐ° Ð¸ Ð°ÑÐ´Ð¸ÑÐ° ÑÑÑÐ´Ð° Ð¸ Ð·Ð°ÑÐ°Ð±Ð¾ÑÐ½Ð¾Ð¹ Ð¿Ð»Ð°ÑÑ Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐÐ Â«ÐÐ°ÐºÑÑÐ¼Ð°Â»: Ð´Ð°Ð½Ð° ÐºÑÐ°ÑÐºÐ°Ñ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ° ÐÐÐ Â«ÐÐ°ÐºÑÑÐ¼Ð°Â», Ð¸Ð·ÑÑÐµÐ½ ÑÑÐµÑ ÑÐ°ÑÑÐµÑÐ¾Ð² Ñ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð¾Ð¼ Ð¿Ð¾ Ð¾Ð¿Ð»Ð°ÑÐµ ÑÑÑÐ´Ð°, Ð°ÑÐ´Ð¸ÑÐ¾ÑÑÐºÐ°Ñ Ð¿ÑÐ¾Ð²ÐµÑÐºÐ° ÑÑÐµÑÐ° ÑÐ°ÑÑÐµÑÐ¾Ð² Ñ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð¾Ð¼ Ð¿Ð¾ Ð¾Ð¿Ð»Ð°ÑÐµ ÑÑÑÐ´Ð°. Ð ÑÑÐµÑÑÐµÐ¹ Ð³Ð»Ð°Ð²Ðµ Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÐ½Ñ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¿Ð¾ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÑÐµÑÐ° ÑÐ°ÑÑÐµÑÐ¾Ð² Ð¿Ð¾ Ð¾Ð¿Ð»Ð°ÑÐµ ÑÑÑÐ´Ð° Ð² ÐÐÐ Â«ÐÐ°ÐºÑÑÐ¼Ð°Â» Ð¸ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ ÑÐ°ÑÑÐµÑ ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½Ð¾Ð¹ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð´Ð°Ð½Ð½ÑÑ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹. Ð Ð·Ð°ÐºÐ»ÑÑÐµÐ½Ð¸Ðµ ÑÐ´ÐµÐ»Ð°Ð½Ñ Ð²ÑÐ²Ð¾Ð´Ñ Ð¿Ð¾ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð½Ð¾Ð¼Ñ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ.