cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
The sharp ALMA view of infall and outflow in the massive protocluster G31.41+0.31
Creators: name: Beltrán, M. T.
name: Rivilla, V. M.
name: Cesaroni, R.
name: Galli, D.
name: Moscadelli, L.
name: Ahmadi, A.
name: Beuther, H.
name: Etoka, S.
name: Goddi, C.
name: Klaassen, P. D.
name: Kuiper, R.
name: Kumar, M. S. N.
name: Lorenzani, A.
name: Peters, T.
name: Sánchez-Monge, Á.
name: Schilke, P.
name: van der Tak, F.
name: Vig, S.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Context. To better understand the formation of high-mass stars, it is fundamental to investigate how matter accretes onto young massive stars, how it is ejected, and how all this differs from the low-mass case. The massive protocluster G31.41+0.31 is the ideal target to study all these processes because observations at millimeter and centimeter wavelengths have resolved the emission of the Main core into at least four massive dust continuum sources, named A, B, C, and D, within 1" or 0.018 pc, and have identified signatures of infall and several outflows associated with the core. Aims. We study the interplay between infall and outflow in G31.41+0.31 by investigating at a spatial resolution of a few 100 au their properties and their possible impact on the core. Methods. We carried out molecular line observations of typical high-density tracers, such as CH3CN or H2CO, and shock and outflow tracers, such as SiO, with ALMA at 1.4 mm that achieved an angular resolution of 0.09" (340 au). Results. The observations have revealed inverse P-Cygni profiles in CH3CN and H2CO toward the four sources embedded in the Main core, suggesting that all of them are undergoing collapse. The infall rates, estimated from the red-shifted absorption are on the order of 1E-2 Msun/yr. The individual infall rates imply that the accretion timescale of the Main core is an order of magnitude smaller than its rotation timescale. This confirms that rotating toroids such as the G31 Main core are non-equilibrium, transient collapsing structures that need to be constantly replenished with fresh material from a large-scale reservoir. For sources B, C, and D, the infall could be accelerating inside the sources, while for source A, the presence of a second emission component complicates the interpretation. The SiO observations have revealed the presence of at least six outflows in the G31.41+0.31 star-forming region, ...
description: 17 pages, 9 figures, 2 tables. Accepted by A&A
Common Frame of reference in collaborative virtual environments and their impact on presence
Creators: name: Chellali, Amine
name: Dumas, Cédric
name: Milleville-Pennel, Isabelle
name: Nouri, Eric
Publisher: name: arXiv
Year: 2010
Subjects: subject: Human-Computer Interaction (cs.HC)
subject: FOS: Computer and information sciences

description: Virtual collaborative environment are 3D shared spaces in which people can work together. To collaborate through these systems, users must have a shared comprehension of the environment. The objective of this experimental study was to determine if visual stable landmarks improve the construction of a common representation of the virtual environment and thus facilitate collaboration. This seems to increase the awareness of the partner's presence.
title: ÐÐ¾Ð´ÐµÐ»Ñ Ð¸ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð°Ñ Ð´Ð¸Ð°Ð»Ð¾Ð³Ð¾Ð²Ð°Ñ Ð¿ÑÐ¾ÑÐµÐ´ÑÑÐ° Ð´Ð»Ñ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° ÑÐ¸ÑÑÐ°ÑÐ¸Ð¹ Ñ ÑÑÐµÑÐ¾Ð¼ Ð²Ð·Ð°Ð¸Ð¼Ð½Ð¾Ð³Ð¾ Ð²Ð»Ð¸ÑÐ½Ð¸Ñ ÐºÐ¾Ð¼Ð¿Ð¾Ð½ÐµÐ½Ñ
title: Model and automated dialogue procedure for analysis of situations taking into account mutual influence of components
Creators: name: ÐÐ½Ð¸ÑÐ¸Ð¼Ð¾Ð², ÐÐ½Ð´ÑÐµÐ¹
name: "Ð¡Ð¸ÑÑÐµÐ¼Ð½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· Ð² Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ð¸ Ð¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ð¸", Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½Ð°Ñ Ð½Ð°ÑÑÐ½Ð°Ñ Ð¸ ÑÑÐµÐ±Ð½Ð¾-Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ°Ñ ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ñ (24; 2020; Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³)
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2020
Subjects: Ð¡Ð¸ÑÑÐµÐ¼Ð½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð·
Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐµ ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¸
Ð¼Ð¾Ð´ÐµÐ»Ñ
Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð°Ñ Ð´Ð¸Ð°Ð»Ð¾Ð³Ð¾Ð²Ð°Ñ Ð¿ÑÐ¾ÑÐµÐ´ÑÑÐ°

description: Ð¦ÐµÐ»ÑÑ Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÑÐ°ÑÑÐ¸ ÑÐ²Ð»ÑÐµÑÑÑ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¼Ð¾Ð´ÐµÐ»Ð¸ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð¹ Ð´Ð¸Ð°Ð»Ð¾Ð³Ð¾Ð²Ð¾Ð¹ Ð¿ÑÐ¾ÑÐµÐ´ÑÑÑ Ð´Ð»Ñ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð²Ð·Ð°Ð¸Ð¼Ð½Ð¾Ð³Ð¾ Ð²Ð»Ð¸ÑÐ½Ð¸Ñ ÐºÐ¾Ð¼Ð¿Ð¾Ð½ÐµÐ½Ñ Ð¿ÑÐ¸ Ð¸Ñ Ð²Ð·Ð°Ð¸Ð¼Ð¾Ð´ÐµÐ¹ÑÑÐ²Ð¸Ð¸ Ð² ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÑ ÑÐ¸ÑÑÐ°ÑÐ¸ÑÑ.
description: The purpose of this article is to develop a the model and an automated dialogue procedure for analyzing the mutual influence of components during their interaction in various situations.
Large ion Coulomb crystals: a near-ideal medium for coupling optical cavity modes to matter
Creators: name: Dantan, A.
name: Albert, M.
name: Marler, J. P.
name: Herskind, P. F.
name: Drewsen, M.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We present an investigation of the coherent coupling of various transverse field modes of an optical cavity to ion Coulomb crystals. The obtained experimental results, which include the demonstration of identical collective coupling rates for different transverse modes of a cavity field to ions in the same large Coulomb crystal, are in excellent agreement with theoretical predictions. The results furthermore suggest that Coulomb crystals in the future may serve as near-ideal media for highfidelity multi-mode quantum information processing and communication purposes, including the generation and storage of single photon qubits encoded in different transverse modes.
description: 4 pages, 5 figures
title:  Il giudice amministrativo e le decisioni della Corte di giustizia dell’Unione europea (CGUE) nell’applicazione della direttiva ricorsi n. 665/1989: effettività della tutela giurisdizionale e interesse strumentale nel rapporto tra ricorso principale e ricorso incidentale escludente
Creators: name: Lipari  ,  Marco
Publisher: name: Roma TrE-Press
Year: 2021

description: Premessa una disamina del quadro legislativo e giurisprudenziale in cui il tema si colloca, l’Autore – Consigliere di Stato – analizza criticamente la questione, dibattuta nella giurisprudenza italiana, connessa alla fattispecie del ricorso incidentale c.d. escludente: l’ipotesi, cioè, in cui il giudice deve pronunciarsi sia sul ricorso principale, volto a contestare l’aggiudicazione della gara di appalto, sia sul ricorso incidentale, volto a contestare la legittimità dell’ammissione del ricorrente principale alla gare di appalto. In tal caso è dubbio se e quando, in base al diritto UE, ai fini del riconoscimento del diritto al ricorso in via principale, rilevi la verifica sulla legittimità della partecipazione del ricorrente principale alla procedura di gara. Sul punto la CGUE, più volte interpellata dai giudici italiani (v., in particolare, le sentenze Fastweb and Puligienica), non ha dato risposte risolutive. Nell’ultimo parte del contributo, l’Autore esprime una valutazione sui imiti – ma anche sui meriti – dell’intervento dell’Unione europea in questa materia.
description: National Judges and the Case Law of the Court of Justice of the European Union
Filtering of complex systems using overlapping tree networks
Creators: name: Garas, Antonios
name: Argyrakis, Panos
Publisher: name: arXiv
Year: 2008
Subjects: subject: Physics and Society (physics.soc-ph)
subject: FOS: Physical sciences

description: We introduce a technique that is capable to filter out information from complex systems, by mapping them to networks, and extracting a subgraph with the strongest links. This idea is based on the Minimum Spanning Tree, and it can be applied to sets of graphs that have as links different sets of interactions among the system's elements, which are described as network nodes. It can also be applied to correlation-based graphs, where the links are weighted and represent the correlation strength between all pairs of nodes. We applied this method to the European scientific collaboration network, which is composed of all the projects supported by the European Framework Program FP6, and also to the correlation-based network of the 100 highest capitalized stocks traded in the NYSE. For both cases we identified meaningful structures, such as a strongly interconnected community of countries that play important role in the collaboration network, and clusters of stocks belonging to different sectors of economic activity, which gives significant information about the investigated systems.
description: 6 pages, 4 figures
Track-Hold System (THS): sperimentazione e validazione delle soluzioni tecnologiche derivanti dal progetto Track-Hold
Creators: name: Dolciotti Cristina
name: Massimo, Magrini
name: Davide, Moroni
name: Marco, Righi
Publisher: name: Zenodo
Year: 2021
Subjects: computer graphics
motion analysis
prognostics and health rehabilitation
robotics
rehabilitation robotics

description: Il progetto Track-Hold System (THS), realizzato in struttura sanitaria e quindi in un ambito sanitario controllato e protetto, si inserisce nel più generale e ampio contesto della Robotic Assisted Therapy (RAT). La RAT rappresenta una metodica di riabilitazione, sia motoria che cognitiva, più avanzata e innovativa e si avvale di dispositivi robotici attivi, passivi e facilitanti, spesso dotati di sensori di rilevazione e tracciamento di movimenti sia volontari che involontari, e di protocolli multimediali appositamente elaborati per raggiungere il massimo livello possibile di rieducazione funzionale. La RAT, al pari delle metodiche convenzionali di riabilitazione (ad es Metodo Perfetti, Mirror Therapy, Biofeedback, etc.) richiede la stretta collaborazione tra i componenti del Team Multidisciplinare, che nella RAT, oltre al Medico e al Terapista, prevede la presenza del Fisiologo e dell’Ingegnere Biomedico ed Informatico.
title: ÐÑÐµÐ½ÐºÐ° ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ñ Ð¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ð¸ Ð¸ Ð¿ÐµÑÑÐ¿ÐµÐºÑÐ¸Ð²Ð° ÐµÐ³Ð¾ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐÐ Â«ÐÐµÐ½ÑÐ°Â»)
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¾Ð»ÐºÐ¾Ð²Ð°, ÐÐ¸Ð°Ð½Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: Ñ Ð¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½Ð°Ñ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ
ÑÐ¾Ð²Ð°ÑÐ¾Ð¾Ð±Ð¾ÑÐ¾Ñ
Ð²Ð°Ð»Ð¾Ð²Ð¾Ð¹ Ð´Ð¾Ñ Ð¾Ð´
Ð¸Ð·Ð´ÐµÑÐ¶ÐºÐ¸ Ð¾Ð±ÑÐ°ÑÐµÐ½Ð¸Ñ

description: Ð¦ÐµÐ»ÑÑ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»ÐµÐ¹ ÑÐ¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ñ ÑÐµÐ»ÑÑ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÐµÐ³Ð¾ ÑÐ°Ð±Ð¾ÑÑ. ÐÑÐ»Ð¸ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ñ Ð²Ð½ÐµÑÐ½ÑÑ Ð¸ Ð²Ð½ÑÑÑÐµÐ½Ð½ÑÑ ÑÑÐµÐ´Ñ ÐÐÐ Â«ÐÐµÐ½ÑÐ°Â» Ð¸ Ð²ÑÑÐ²Ð»ÐµÐ½Ñ ÑÐ¸Ð»ÑÐ½ÑÐµ Ð¸ ÑÐ»Ð°Ð±ÑÐµ ÑÑÐ¾ÑÐ¾Ð½Ñ, Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÐ¸ Ð¸ ÑÐ³ÑÐ¾Ð·Ñ. ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ñ ÑÐ°ÐºÑÐ¾ÑÑ, Ð²Ð»Ð¸ÑÑÑÐ¸Ðµ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸ ÑÐ¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ. Ð¡Ð´ÐµÐ»Ð°Ð½ Ð¿ÑÐ¾Ð³Ð½Ð¾Ð· ÑÐ¾Ð²Ð°ÑÐ¾Ð¾Ð±Ð¾ÑÐ¾ÑÐ° ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÐ¼Ð¸ Ð¼ÐµÑÐ¾Ð´Ð°Ð¼Ð¸ Ð¸ Ð¾ÑÑÐ°Ð»ÑÐ½ÑÑ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»ÐµÐ¹. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¸ Ð´Ð¾ÐºÐ°Ð·Ð°Ð½Ð° Ð¸Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ Ñ ÑÐµÐ»ÑÑ ÑÐ²ÐµÐ»Ð¸ÑÐµÐ½Ð¸Ñ ÑÐ¾Ð²Ð°ÑÐ¾Ð¾Ð±Ð¾ÑÐ¾ÑÐ° Ð¸ ÑÐ¸ÑÑÐ¾Ð¹ Ð¿ÑÐ¸Ð±ÑÐ»Ð¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ.
The density field of the 10k zCOSMOS galaxies
Creators: name: Kovac, K.
name: Lilly, S. J.
name: Cucciati, O.
name: Porciani, C.
name: Iovino, A.
name: Zamorani, G.
name: Oesch, P.
name: Bolzonella, M.
name: Knobel, C.
name: Finoguenov, A.
name: Peng, Y.
name: Carollo, C. M.
name: Pozzetti, L.
name: Caputi, K.
name: Silverman, J. D.
name: Tasca, L.
name: Scodeggio, M.
name: Vergani, D.
name: Zucca, E.
name: Contini, T.
name: Kneib, J. -P.
name: Fevre, O. Le
name: Mainieri, V.
name: Renzini, A.
name: Scoville, N. Z.
name: Capak, P.
name: Bardelli, S.
name: Bongiorno, A.
name: Coppa, G.
name: de la Torre, S.
name: de Ravel, L.
name: Franzetti, P.
name: Garilli, B.
name: Guzzo, L.
name: Kampczyk, P.
name: Lamareille, F.
name: Borgne, J. -F. Le
name: Brun, V. Le
name: Maier, C.
name: Mignoli, M.
name: Pello, R.
name: Montero, E. Perez
name: Ricciardelli, E.
name: Tanaka, M.
name: Tresse, L.
name: Abbas, U.
name: Bottini, D.
name: Cappi, A.
name: Cassata, P.
name: Cimatti, A.
name: Fumana, M.
name: Maccagni, D.
name: Marinoni, C.
name: McCracken, H. J.
name: Memeo, P.
name: Meneux, B.
name: Scaramella, R.
name: Koekemoer, A. M.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We use the current sample of ~10,000 zCOSMOS spectra of sources selected with I(AB) < 22.5 to define the density field out to z~1, with much greater resolution in the radial dimension than has been possible with either photometric redshifts or weak lensing. We apply new algorithms that we have developed (ZADE) to incorporate objects not yet observed spectroscopically by modifying their photometric redshift probability distributions using the spectroscopic redshifts of nearby galaxies. This strategy allows us to probe a broader range of galaxy environments and reduce the Poisson noise in the density field. The reconstructed overdensity field of the 10k zCOSMOS galaxies consists of cluster-like patterns surrounded by void-like regions, extending up to z~1. Some of these structures are very large, spanning the ~50 Mpc/h transverse direction of the COSMOS field and extending up to Delta z~0.05 in redshift. We present the three dimensional overdensity maps and compare the reconstructed overdensity field to the independently identified virialised groups of galaxies and clusters detected in the visible and in X-rays. The distribution of the overdense structures is in general well traced by these virialised structures. A comparison of the large scale structures in the zCOSMOS data and in the mock catalogues reveals an excellent agreement between the fractions of the volume enclosed in structures of all sizes above a given overdensity between the data and the mocks in 0.2
description: 35 pages, 20 figures; submitted to ApJ; the high resolution pdf available at http://www.exp-astro.phys.ethz.ch/kovac/public/zCOSMOS
title: ÐÐ²ÑÐ¾Ð¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ðµ ÑÐ°ÑÐ¿Ð¾Ð·Ð½Ð°Ð²Ð°Ð½Ð¸Ðµ Ð°Ð½Ð¾Ð¼Ð°Ð»ÑÐ½ÑÑ ÑÑÑÑÐºÑÑÑ Ð²Ð½ÑÑÑÐ¸ Ð»ÐµÐ³ÐºÐ¸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ÑÑÐµÐ¹ ÐÐ±Ð°Ð¹
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: ÐÐ½Ð°Ð»Ð¸Ð·Ð°ÑÐ¾ÑÑ Ð¸Ð·Ð¾Ð±ÑÐ°Ð¶ÐµÐ½Ð¸Ð¹
ÐÐµÐ¹ÑÐ¾Ð½Ð½ÑÐµ ÑÐµÑÐ¸
ÐºÐ¾Ð¼Ð¿ÑÑÑÐµÑÐ½Ð°Ñ ÑÐ¾Ð¼Ð¾Ð³ÑÐ°ÑÐ¸Ñ
Ð·Ð»Ð¾ÐºÐ°ÑÐµÑÑÐ²ÐµÐ½Ð½ÑÐµ Ð¾Ð¿ÑÑ Ð¾Ð»Ð¸
Ð¾Ð½ÐºÐ¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ Ð·Ð°Ð±Ð¾Ð»ÐµÐ²Ð°Ð½Ð¸Ñ

description: ÐÐ°Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° Ð·Ð°Ð´Ð°ÑÐµ Ð½Ð°ÑÐ¾Ð¶Ð´ÐµÐ½Ð¸Ñ ÑÐ°ÐºÐ¾Ð²ÑÑ ÑÐ·Ð»Ð¾Ð² (Ð¾Ð¿ÑÑÐ¾Ð»ÐµÐ¹) Ð½Ð° Ð¾Ð±ÑÐµÐ¼Ð°Ñ Ð»ÐµÐ³ÐºÐ¸Ñ, Ð¿Ð¾Ð»ÑÑÐµÐ½Ð½ÑÑ Ñ Ð¿Ð¾Ð¼Ð¾ÑÑÑ ÐºÐ¾Ð¼Ð¿ÑÑÑÐµÑÐ½Ð¾Ð¹ ÑÐ¾Ð¼Ð¾Ð³ÑÐ°ÑÐ¸Ð¸, Ð° ÑÐ°Ðº Ð¶Ðµ Ð°ÐºÑÑÐ°Ð»ÑÐ½Ð¾Ð¹ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ðµ Ð»Ð¾Ð¶Ð½Ð¾Ð³Ð¾ Ð´ÐµÑÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐ°ÐºÐ¾Ð²ÑÑ ÑÐ·Ð»Ð¾Ð² Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸ÑÐµÑÐºÐ¸Ð¼Ð¸ ÑÐ¸ÑÑÐµÐ¼Ð°Ð¼Ð¸.
Ð ÑÐ°Ð±Ð¾ÑÐµ Ð¾Ð¿Ð¸ÑÑÐ²Ð°ÐµÑÑÑ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼ ÑÐ°ÑÐ¿Ð¾Ð·Ð½Ð°Ð²Ð°Ð½Ð¸Ñ ÑÐ°ÐºÐ¾Ð²ÑÑ ÑÐ·Ð»Ð¾Ð², ÐºÐ¾ÑÐ¾ÑÑÐ¹ Ð¾ÑÐ½Ð¾Ð²Ð°Ð½ Ð½Ð° ÑÐµÐ³Ð¼ÐµÐ½ÑÐ°ÑÐ¸Ð¸ Ð¾Ð±ÑÐµÐ¼Ð° Ð»ÐµÐ³ÐºÐ¸Ñ Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð¸Ð·Ð¾Ð±ÑÐ°Ð¶ÐµÐ½Ð¸Ð¹ Ð¸ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ð¸ ÑÐ²ÐµÑÑÐ¾ÑÐ½ÑÑ Ð½ÐµÐ¹ÑÐ¾Ð½Ð½ÑÑ ÑÐµÑÐµÐ¹ Ð² ÐºÐ°ÑÐµÑÑÐ²Ðµ ÐºÐ»Ð°ÑÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¾ÑÐ°. ÐÐ¿Ð¸ÑÐ°Ð½ Ð¿ÑÐ¾ÑÐµÑÑ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð¼ÐµÐ´Ð¸ÑÐ¸Ð½ÑÐºÐ¸Ñ Ð´Ð°Ð½Ð½ÑÑ Ð´Ð»Ñ Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ ÑÐ²ÐµÑÑÐ¾ÑÐ½ÑÑ Ð½ÐµÐ¹ÑÐ¾Ð½Ð½ÑÑ ÑÐµÑÐµÐ¹. Ð ÑÐ°Ð±Ð¾ÑÐµ Ð¾Ð¿Ð¸ÑÐ°Ð½Ð° Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð°Ñ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ð° Ð¿Ð¾Ð¸ÑÐºÐ° Ð¾Ð¿ÑÑÐ¾Ð»ÐµÐ¹, Ð° ÑÐ°Ðº Ð¶Ðµ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¿Ð¾Ð»ÑÑÐµÐ½Ð½ÑÑ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¾Ð² ÑÐµÑÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð½Ð° Ð¼Ð¾Ð´ÐµÐ»ÑÐ½ÑÑ (Ð¸ÑÐºÑÑÑÑÐ²ÐµÐ½Ð½Ð¾ ÑÐ³ÐµÐ½ÐµÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÑ) Ð¸ ÑÐµÐ°Ð»ÑÐ½ÑÑ Ð´Ð°Ð½Ð½ÑÑ. ÐÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½Ð¾ ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ðµ ÐºÐ°ÑÐµÑÑÐ²Ð° ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ° ÑÐ°Ð±Ð¾ÑÑ Ñ Ð´ÑÑÐ³Ð¸Ð¼Ð¸ ÑÐµÑÐµÐ½Ð¸ÑÐ¼Ð¸ Ð´Ð°Ð½Ð½Ð¾Ð¹ Ð·Ð°Ð´Ð°ÑÐ¸.
title: ÐÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ½Ð¾Ðµ Ð¸Ð½Ð¶ÐµÐ½ÐµÑÐ½Ð¾Ðµ Ð±Ð»Ð°Ð³Ð¾ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð¾ Ð½Ð°ÑÐµÐ»ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ½ÐºÑÐ° Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ ÑÐ½ÐµÑÐ³Ð¾ÑÐ±ÐµÑÐµÐ³Ð°ÑÑÐ¸Ñ ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¹ Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ Ð¼Ð°Ð»Ð¾ÑÑÐ°Ð¶Ð½Ð¾Ð³Ð¾ Ð¶Ð¸Ð»Ð¾Ð³Ð¾ Ð´Ð¾Ð¼Ð° Ð² ÐÐµÐ½Ð¸Ð½Ð³ÑÐ°Ð´ÑÐºÐ¾Ð¹ Ð¾Ð±Ð»Ð°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Ð¾Ð±Ð¾Ð²Ð°, 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: 2018
Subjects: ÐºÐ¾ÑÑÐµÐ´Ð¶Ð½ÑÐ¹ Ð¿Ð¾ÑÐµÐ»Ð¾Ðº
Ð¸Ð½Ð¶ÐµÐ½ÐµÑÐ½Ð°Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ°
Ð²Ð¾Ð´Ð¾Ð¾ÑÐ²ÐµÐ´ÐµÐ½Ð¸Ðµ
ÑÐµÐ¿Ð»Ð¾Ð²Ð¾Ð¹ Ð±Ð°Ð»Ð°Ð½Ñ
Ð´Ð¾Ð¶Ð´ÐµÐ²Ð°Ñ ÐºÐ°Ð½Ð°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑÑÑ Ð²Ð¾Ð¿ÑÐ¾ÑÑ Ð±Ð»Ð°Ð³Ð¾ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð° Ð¸ Ð¸Ð½Ð¶ÐµÐ½ÐµÑÐ½Ð¾Ð¹ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ ÑÐµÑÑÐ¸ÑÐ¾ÑÐ¸Ð¸ Ð½Ð°ÑÐµÐ»ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ½ÐºÑÐ° Ð² ÐÐµÐ½Ð¸Ð½Ð³ÑÐ°Ð´ÑÐºÐ¾Ð¹ Ð¾Ð±Ð»Ð°ÑÑÐ¸, Ð° ÑÐ°ÐºÐ¶Ðµ ÑÐ½ÐµÑÐ³Ð¾ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾Ð¹ ÑÐºÑÐ¿Ð»ÑÐ°ÑÐ°ÑÐ¸Ð¸ ÐºÐ¾ÑÑÐµÐ´Ð¶Ð° Ð² Ð·Ð¾Ð½Ðµ ÐÐÐ¡. Ð ÑÐ¾Ð´Ðµ ÑÐ°Ð±Ð¾ÑÑ Ð±ÑÐ»Ð° Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð° Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð¾ÑÐ½Ð°Ñ ÑÑÑÑÐºÑÑÑÐ° Ð¿Ð¾ÑÐµÐ»ÐºÐ°, Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½ Ð¿ÑÐ¾ÐµÐºÑ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÐµÐ»ÑÐµÑÐ° ÑÐµÑÑÐ¸ÑÐ¾ÑÐ¸Ð¸, ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½ Ð¿ÑÐ¾ÐµÐºÑ Ð»Ð¸Ð²Ð½ÐµÐ²Ð¾Ð¹ ÐºÐ°Ð½Ð°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸, Ð° ÑÐ°ÐºÐ¶Ðµ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½ Ð¿Ð¾Ð´Ð±Ð¾Ñ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½ÑÑ ÑÐ½ÐµÑÐ³Ð¾ÑÑÑÐµÐºÑÐ¸Ð²Ð½ÑÑ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¹ Ð´Ð»Ñ ÑÐºÑÐ¿Ð»ÑÐ°ÑÐ°ÑÐ¸Ð¸ Ð¼Ð°Ð»Ð¾ÑÑÐ°Ð¶Ð½Ð¾Ð³Ð¾ Ð¶Ð¸Ð»Ð¾Ð³Ð¾ Ð¾Ð´Ð½Ð¾ÐºÐ²Ð°ÑÑÐ¸ÑÐ½Ð¾Ð³Ð¾ Ð´Ð¾Ð¼Ð°.
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð¸Ð½Ð´ÑÐºÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ Ð·Ð°ÐºÐ°Ð»ÐºÐ¸ ÑÑÐ°Ð»ÑÐ½ÑÑ ÑÐµÐµÐº ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð²Ð°Ð»Ð° Ð´Ð¸Ð°Ð¼ÐµÑÑÐ¾Ð¼ 64 Ð¼Ð¼
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ÐºÐ¾Ð², ÐÐ°Ð½Ð¸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: Ð²ÑÐ±Ð¾Ñ ÑÐ°ÑÑÐ¾ÑÑ
ÑÐµÐ¿Ð»Ð¾Ð²Ð¾Ð¹ ÑÐ°ÑÑÐµÑ
ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ°ÑÑÐµÑ Ð¸Ð½Ð´ÑÐºÑÐ¾ÑÐ°
ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ðµ Ð¼Ð¾Ð´ÐµÐ»Ð¸ Ð² Comsol Multiphysics

description: Ð¦ÐµÐ»Ñ ÑÐ°Ð±Ð¾ÑÑ â ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð¸Ð½Ð´ÑÐºÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ Ð¿Ð¾Ð²ÐµÑÑÐ½Ð¾ÑÑÐ½Ð¾Ð¹ Ð·Ð°ÐºÐ°Ð»ÐºÐ¸ ÑÑÐ°Ð»ÑÐ½ÑÑ ÑÐµÐµÐº ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð²Ð°Ð»Ð° Ð´Ð¸Ð°Ð¼ÐµÑÑÐ¾Ð¼ 64 Ð¼Ð¼ Ð¿ÑÑÐµÐ¼ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ ÑÐ°ÑÑÐµÑÐ¾Ð² Ð¿Ð¾ Ð°Ð½Ð°Ð»Ð¸ÑÐ¸ÑÐµÑÐºÐ¾Ð¼Ñ Ð¸ ÑÐ¸ÑÐ»ÐµÐ½Ð½Ð¾Ð¼Ñ Ð¼ÐµÑÐ¾Ð´Ñ.
Two atoms in dissipative cavities in dispersive limit: entanglement sudden death and long-lived entanglement
Creators: name: Zhang, Jian-Song
name: Chen, Ai-Xi
name: Abdel-Aty, M.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We investigate the entanglement dynamics and coherence of two two-level atoms interacting with two coherent fields of two spatially separated and dissipative cavities. It is in particular shown that entanglement sudden death is obtained within a short interacting time. However, after a long interaction time a long-lived entanglement is shown, that is, the initial entanglement of two atoms could be partially preserved. In addition, the coherence of the two atoms will not be lost during the evolution.
description: 18 pages, 7 figures
title: Switching to English medium instruction in academic disciplinesâ teaching in non-English speaking higher education
Creators: name: Shramko, Ludmila
name: Gorbaneva, Viktoriia
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2022
Subjects: Ð°Ð½Ð³Ð»Ð¸Ð¹ÑÐºÐ¸Ð¹ ÑÐ·ÑÐº
Ð¾Ð±ÑÑÐµÐ½Ð¸Ðµ

description: It has been widely acknowledged that internationalization of education and research is a crucial factor for improvements in any national educational system worldwide. Scientists argue that internationalisation is onnected with the process of integrating intercultural and international components into research and teaching levels. It is worth mentioning that internationalisation can be external and internal. In the framework of the current paper the authors focus on the external internationalisation that deals with international academic mobility and is connected with intercultural programs, world educational standards, and internationalization of educational programs or / and courses. The main reasons for higher education internationalisation are to promote the international profile of a university, attract foreign students, foster and widen partnership in education and research, build and develop intercultural communicative competence among domestic students and teaching staff. As a result, more and more countries, including the Russian Federation, keep promoting new initiatives to internationalise higher education. In response to this fact, there has been a significant upsurge in English medium instruction in tertiary education in non-native English-speaking environment.
The HI properties of galaxies in the Coma I cloud revisited
Creators: name: Boselli, A.
name: Gavazzi, G.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Pre-processing within small groups has been proposed to explain several of the properties of galaxies inhabiting rich clusters. The aim of the present work is to see whether pre-processing is acting in the nearby universe, where the structures that are merging to form rich clusters are rather large and massive. We study the HI gas properties of a large sample of late-type galaxies belonging to the Coma I cloud, an association of objects close to the Virgo cluster. Contrary to what previously claimed, late-type galaxies in the Coma I cloud are not deficient in HI gas (HI-def=0.06+-0.44). If the Coma I cloud is representative of infalling groups in nearby clusters, this result suggests that, in the local universe, the evolution of late-type galaxies belonging to loose structures with high velocity dispersions (>= 300 km/s)associated to rich clusters such as Virgo is not significantly perturbed by pre-processing.
description: Accepted for publication on A&A
Additional file 1 of Nicotinamide drives T cell activation in the mammary tumor microenvironment
Creators: name: Hu, Yang
name: Bloy, Norma
name: Elemento, Olivier
name: Buqué, Aitziber
Publisher: name: figshare
Year: 2022
Subjects: subject: Biochemistry
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Neuroscience
subject: Pharmacology
subject: Immunology
subject: FOS: Clinical medicine
subject: Developmental Biology
subject: Cancer
subject: Computational Biology

description: Additional file 1. Genes of interest differentially expressed in T cells from NAM-treated vs control TS/A tumors.
Comparing Monogamous and Polyamorous Sexual and Relationship Quality During COVID-19 Pandemic
Creators: name: Rodrigues, David L.
name: Slatcher, Richard B.
name: Zoppolat, Giulia
name: Balzarini, Rhonda Nicole
name: Himes, Taylor
Publisher: name: Open Science Framework
Year: 2023
Subjects: subject: Social and Behavioral Sciences
subject: Psychology
subject: FOS: Psychology

description: We seek to assess whether sexual and relationship quality among people in monogamous and polyamorous relationships differed during the early months of the COVID-19 pandemic. Hypotheses are outlined in the pre-registration document (see attachment).
General Electric Quarterly Survey 80-01, Versions I, II & II and College Student
Creators: name: Electric, General
Publisher: name: Roper Center for Public Opinion Research
Year: 2022

description: Adult sample: Most interesting concerns (3); local community interests (1); solving community problems (2); life satisfaction (1); interest in national issues (1); national issues discussions (10); price controls (1); wage controls (1); race relations (1); future race relations (1); companies helping race relations (1); product values (21); electricity fuels (3); future fuels (2); need for additional plants (1); power plant approvals (3); government activity changes (28); defense spending (7); company effects (1); magazine readership (1); television viewing habits (2); courses taken (7); financial situation (2); income change (1); future plans (2); inflation (5); unemployment (1); recession (2). College student sample: Most interesting concerns (3); life satisfaction (1); interest in national issues (1); national issues discussions (10); price controls (1); wage controls (1); race relations (1); future race relations (1); companies helping race relations (1); electricity fuels (3); future fuels (2); need for additional plants (1); power plant approvals (3); government activity changes (14); defense spending (7); company effects (1); magazine readership (1); television viewing habits (2); college attended (2); class year (1); major (1); degree (1); preferred career (2); important career aspects (9); academic standing (1).
OK-Net EcoFeed Knowledge synthesis of feed production
Creators: name: Díaz-Gaona, Cipriano
name: Kongsted, Anne Grete
name: Nørgaard, Jan Værum
name: Papi, Eugenio
name: Perez, Angela Morell
name: Reyes-Palomo, Carolina
name: Estévez, Vicente Rodríguez-
name: Roinsard, Antoine
name: Steenfeldt, Sanna
name: Studnitz, Merete
name: Stødkilde-Jørgensen, Lene
name: Theil, Peter Kappel
name: Åkerfeldt, Magdalena
name: Studnitz, Merete
Publisher: name: Zenodo
Year: 2021
Subjects: novel feed ingredient; sustainability; pig; poultry; protein; amino acid; digestibility; growth performance

description: The transition to 100% organic feed ingredients for organic livestock is expected to take effect from January
 1st 2020 in Europe. In order to contribute to the goal of 100% use of organic and regional feed for
 monogastrics, this knowledge synthesis “Feeding monogastrics 100% organic and regionally produced feed“
 aims to describe:
 • the protein need for organic monogastric animals (pigs, layers and broilers), including different
 breeds and rearing conditions
 • different protein feed resources, mostly new or not commonly used protein sources, their nutrient
 content, production prerequisites, and their potential feeding value
 • small-scale, on-farm equipment for feed processing
 • different feeding strategies.
 The knowledge synthesis should enable participants in Innovation groups (IG) and Thematic groups (TG) to
 choose feed materials, feeding strategies, breeds and perhaps even small-scale on-farm equipment for
 testing when aiming at 100% organic and regionally produced feed for monogastrics.
 In the knowledge synthesis it is concluded: When feeding pigs and poultry 100% organic and regionally
 produced feed, getting enough protein and specific amino acids is a challenge. There are two ways to go and
 they can be combined. One is to utilize by-products, for example waste from various productions, and explore
 new protein sources e.g. marine products or to refine already known products such as grass. The other way
 is to feed the animals less intensively and for this feeding strategy slow-growing breeds fit better. Some slowgrowing
 breeds are already known, some are rediscovered old breeds. The challenge with the slow-growing
 and less-yielding breeds is that the production is getting smaller and either the farmer will earn less or the
 prices of eggs and meat will increase.
 However, the possibilities for combinations of regionally grown feed, low-yielding breeds with different
 feeding strategies are many and they need to be explored.
 Finally, the knowledge synthesis identify needs for new knowledge on:
 • nutritional requirements of alternative breeds. Precise nutrient recommendations for organically
 produced pigs and poultry do not exist.
 • nutritional value of new protein sources for monogastric animals
 • various combinations of breeds, grazing and supplemental feed.
 Small-scale on-farm equipment to refine locally produced raw materials needs to be developed.
title: ÐÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ ÐºÐ°Ð»ÑÐ¿Ð°Ð¸Ð½Ð¾Ð² Ð² Ð¼Ð¸Ð¾ÑÐ¸ÑÐ°Ñ Ð¸ ÐºÐ»ÐµÑÐºÐ°Ñ Ð¦ÐÐ¡ ÐºÑÑÑ Ñ Ð¼ÑÑÐµÑÐ½Ð¾Ð¹ Ð´Ð¸ÑÑÐ¾Ð½Ð¸ÐµÐ¹
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: ÐÑÑÐ·Ð¸Ð½Ð°, ÐÐ½Ð°ÑÑÐ°ÑÐ¸Ñ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2016
Subjects: Ð¼ÑÑÐµÑÐ½Ð°Ñ Ð´Ð¸ÑÑÐ¾Ð½Ð¸Ñ
Ð´Ð¾ÑÐ°Ð¼Ð¸Ð½
Ð¼Ð¾ÑÐ¾ÑÐ½ÑÐµ Ð½Ð°ÑÑÑÐµÐ½Ð¸Ñ
muscular dystonia
dopamine
motor disturbances

description: Ð¦ÐµÐ»ÑÑ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐ»Ð¾ÑÑ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¼ÑÑÐµÑÐ½Ð¾Ð¹ Ð´Ð¸ÑÑÐ¾Ð½Ð¸Ð¸ Ð½Ð° ÐºÑÑÑÐ°Ñ ÐÐ¸ÑÑÐ°Ñ Ð´Ð»Ñ Ð²ÑÑÐ²Ð»ÐµÐ½Ð¸Ñ Ð½Ð¾Ð²ÑÑ Ð¼Ð¸ÑÐµÐ½ÐµÐ¹ Ð´Ð»Ñ ÑÐ°ÑÐ¼Ð°ÐºÐ¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð²Ð¾Ð·Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ. Ð¢Ð°ÐºÐ¶Ðµ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°Ð»Ð°ÑÑ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÑ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ Ð¸Ð½Ð³Ð¸Ð±Ð¸ÑÐ¾ÑÐ¾Ð² m-ÐºÐ°Ð»ÑÐ¿Ð°Ð¸Ð½Ð° Ð´Ð»Ñ ÐºÑÐ¿Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¸Ð¼Ð¿ÑÐ¾Ð¼Ð¾Ð² Ð´Ð°Ð½Ð½Ð¾Ð³Ð¾ Ð·Ð°Ð±Ð¾Ð»ÐµÐ²Ð°Ð½Ð¸Ñ. Ð Ð°Ð±Ð¾ÑÐ° Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð° Ð½Ð° ÐºÑÑÑÐ°Ñ ÑÐ°Ð¼ÑÐ°Ñ Ð»Ð¸Ð½Ð¸Ð¸ ÐÐ¸ÑÑÐ°Ñ Ñ Ð¿Ð¾Ð¼Ð¾ÑÑÑ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² Ð¾ÑÐµÐ½ÐºÐ¸ Ð¿Ð¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ ("ÐÑÐºÑÑÑÐ¾Ðµ Ð¿Ð¾Ð»Ðµ", "Gait analysis system"), Ð¼ÐµÑÐ¾Ð´Ð° ÐÐ­ÐÐ¥ Ð¸ ÐºÐ°Ð·ÐµÐ¸Ð½Ð¾Ð²Ð¾Ð¹ Ð·Ð¸Ð¼Ð¾Ð³ÑÐ°ÑÐ¸Ð¸. ÐÐ¾ÐºÐ°Ð·Ð°Ð½Ð¾ ÑÐ½Ð¸Ð¶ÐµÐ½Ð¸Ðµ ÑÑÐ¾Ð²Ð½Ñ Ð´Ð¾ÑÐ°Ð¼Ð¸Ð½Ð° Ð² ÑÑÑÐ¸Ð°ÑÑÐ¼Ðµ Ð¶Ð¸Ð²Ð¾ÑÐ½ÑÑ, Ð¿Ð¾Ð»ÑÑÐ°Ð²ÑÐ¸Ñ 3-Ð½Ð¸ÑÑÐ¾Ð¿ÑÐ¾Ð¿Ð¸Ð¾Ð½Ð¾Ð²ÑÑ ÐºÐ¸ÑÐ»Ð¾ÑÑ Ð¸Ð½ÑÑÐ°Ð¿ÐµÑÐ¸ÑÐ¾Ð½ÐµÐ°Ð»ÑÐ½Ð¾ Ð² ÑÐµÑÐµÐ½Ð¸Ðµ 5-8 Ð´Ð½ÐµÐ¹. ÐÑÐ¼ÐµÑÐµÐ½Ð¾ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ðµ Ð°ÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ m-ÐºÐ°Ð»ÑÐ¿Ð°Ð¸Ð½Ð° Ð² ÐºÐ»ÐµÑÐºÐ°Ñ ÑÑÑÐ¸Ð°ÑÑÐ¼Ð° Ð¸ Ð¼Ð¸Ð¾ÑÐ¸ÑÐ°Ñ Ð² 1.7-2.0 ÑÐ°Ð·Ð° Ð¿Ð¾ ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ñ Ñ ÐºÐ¾Ð½ÑÑÐ¾Ð»ÐµÐ¼. Ð­ÑÐ¸ Ð¸Ð·Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ ÑÐ¾Ð¿ÑÐ¾Ð²Ð¾Ð¶Ð´Ð°Ð»Ð¸ÑÑ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²ÑÐ¼Ð¸ Ð¼Ð¾ÑÐ¾ÑÐ½ÑÐ¼Ð¸ Ð½Ð°ÑÑÑÐµÐ½Ð¸ÑÐ¼Ð¸. ÐÐ¾ÐºÐ°Ð·Ð°Ð½Ð° Ð½Ð¾ÑÐ¼Ð°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ Ð°ÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ m-ÐºÐ°Ð»ÑÐ¿Ð°Ð¸Ð½Ð° Ð² Ð¼Ð¸Ð¾ÑÐ¸ÑÐ°Ñ ÑÐºÑÐ¿ÐµÑÐ¸Ð¼ÐµÐ½ÑÐ°Ð»ÑÐ½ÑÑ Ð¶Ð¸Ð²Ð¾ÑÐ½ÑÑ Ð¿ÑÐ¸ Ð¸Ð½ÑÑÐ°Ð½Ð°Ð·Ð°Ð»ÑÐ½Ð¾Ð¼ Ð²Ð²ÐµÐ´ÐµÐ½Ð¸Ð¸ Ð¸Ð½Ð³Ð¸Ð±Ð¸ÑÐ¾ÑÐ¾Ð² m-ÐºÐ°Ð»ÑÐ¿Ð°Ð¸Ð½Ð°.
description: The aim of the work was modeling muscular dystonia on Wistar rats to identify new targets for pharmacological influence. Also consider the use of inhibitors of m-calpain for the relief of symptoms of the disease. Work carried out on male Wistar rats by using valuation techniques of behavior ("Open field","Gait analysis system"), HPLC method and casein zymography. Displaying decrease levels of dopamine in the striatum of animals receiving 3-nitropropionic acid intraperitoneally for 5-8 days. Noted increase activity of m-calpain in the striatum cells and myocytes in 1.7-2.0-fold compared to the control. These changes were accompanied by persistent motor impairments. It is shown the normalization of the activity of m-calpain in myocytes in experimental animals by intranasal administration of inhibitors of m-calpain.
Cross-sections of large-angle hadron production in proton- and pion-nucleus interactions IV: Copper nuclei and beam momenta from +/-3 GeV/c to +/-15 GeV/c
Creators: name: CDP Group
name: Bolshakova, A.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: We report on double-differential inclusive cross-sections of the production of secondary protons, charged pions, and deuterons, in the interactions with a 5% nuclear interaction length thick stationary copper target, of proton and pion beams with momentum from +/-3 GeV/c to +/-15 GeV/c. Results are given for secondary particles with production angles between 20 and 125 degrees.
description: 66 pages, 12 figures corrected typo in author name
P.Oxy. XXXII 2628. Lyrical Verses; Euripides, Andromeda (see T. F. Brunner, ZPE 88 (1991) 165-166)
Creators: name: Oxyrhynchus Papyri
Publisher: name: University of Oxford
Year: 2022
Subjects: Latin and classical Greek languages

description: Reproduction requests: https://www.ees.ac.uk/reproduction-requests-and-fees
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹, Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð½ÑÑ Ð½Ð° ÑÐºÑÐµÐ¿Ð»ÐµÐ½Ð¸Ðµ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð³Ð¾ Ð¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¸Ð½Ð´ÑÑÑÑÐ¸Ð¸ Ð³Ð¾ÑÑÐµÐ¿ÑÐ¸Ð¸Ð¼ÑÑÐ²Ð° (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ Ð¾ÑÐµÐ»Ñ Â«ÐÑÑÐ¾ÑÐ¸Ñ Rocco ForteÂ»)
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ»Ð¾Ð±Ð°Ð¶, Ð®ÑÐ¸Ð¹
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2016
Subjects: Ð°Ð½Ð°Ð»Ð¸Ð·
Ð¾Ð±Ð¾ÑÐ°ÑÐ¸Ð²Ð°ÐµÐ¼Ð¾ÑÑÑ
Ð¿ÑÐ¾ÐµÐºÑ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹
ÑÐµÐ½ÑÐ°Ð±ÐµÐ»ÑÐ½Ð¾ÑÑÑ
ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÐ¹ ÑÐµÐ·ÑÐ»ÑÑÐ°Ñ
ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ðµ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ðµ
ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð°Ñ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÑ
analysis
turnover
the project activities
profitability
financial result
financial condition
financial stability

description: Ð ÑÐ°Ð¼ÐºÐ°Ñ Ð´Ð°Ð½Ð½Ð¾Ð³Ð¾ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ð¸ Ð¸Ð·ÑÑÐµÐ½Ð½ÑÑ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¸ Ð¼ÐµÑÐ¾Ð´Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ñ Ð¾ÑÐ½Ð¾Ð² ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÐ¼ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸ÐµÐ¼ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ, Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÐµÑÑÐ¾ÑÐ¿ÐµÐºÑÐ¸Ð²Ð½Ð¾Ð³Ð¾ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾ - ÑÐ¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð±Ð°Ð·Ð¾Ð²Ð¾Ð³Ð¾ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ - Ð¾ÑÐµÐ»Ñ Â«ÐÑÑÐ¾ÑÐ¸Ñ RoccoForteÂ», Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½ Ð¿ÑÐ¾ÐµÐºÑ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹, Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð½ÑÐ¹ Ð½Ð° ÑÐºÑÐµÐ¿Ð»ÐµÐ½Ð¸Ðµ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð³Ð¾ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ñ Ð¸ÑÑÐ»ÐµÐ´ÑÐµÐ¼Ð¾Ð¹ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸.
description: In this study, based on the study of theoretical and methodological bases of management of the financial condition of the company, conducted a retrospective analysis of financial - economic activity of the basic research enterprise - the hotel "Astoria Rocco ForteÂ», the draft measures proposed, aimed at strengthening the financial condition of the organization under study.
Evaluating a methodology for characterizing resilience of infrastructure systems
Creators: name: Procyk, Andrea
Publisher: name: The University of British Columbia
Year: 2016

description: Efforts to make urban areas more resilient to disasters are becoming increasingly important. One key facet of resilient urban areas is functioning infrastructure systems. This study represents an evaluation of a methodology used to characterize infrastructure vulnerabilities to disaster events. The intended clients for this project are those interested in the implementation of approaches for understanding what makes urban regions more resilient, such as municipal planners, infrastructure managers, researchers and consultants.
Ultimate synchrotron cutoff in gamma-ray spectra of blazars as a signature of the converter mechanism
Creators: name: Stern, Boris E.
name: Tikhomirov, Yana Y.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: There is a robust upper limit on the energy of synchrotron radiation in high-energy astrophysics: $ \sim m_{\rm e} c^2 /α$, where $α= 1/137$ is the fine structure constant and the value refers to the comoving frame of the fluid. This is the maximal energy of synchrotron photons which can be emitted by an electron having an arbitrarily high initial energy after it turns by angle $\sim π$ in the magnetic field. This upper limit can be naturally reached if the converter mechanism contributes to the jet radiation and can be imprinted in spectra of some blazars as a cutoff or a dip in the GeV range. We use numerical simulations to probe the range of parameters of a radiating jet where the ultimate synchrotron cutoff appears. We reproduce the variety of spectra depending on the source luminosity and on the scale of the emission site. We also compare our results with the EGRET blazar spectra in order to illustrate that agreement is possible but still not statistically significant. The predicted feature, if it exists, should be observed by {\it Fermi} in spectra of some blazars.
description: Accepted to MNRAS
title: ÐÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð°Ñ ÑÐ¸ÑÑÐµÐ¼Ð° Ð´Ð»Ñ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð»Ð¾Ð³Ð¾Ð² Ñ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸ÐµÐ¼ Ð¸Ð½ÑÐµÐ»Ð»ÐµÐºÑÑÐ°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð´Ð°Ð½Ð½Ñ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ÑÐ½Ð¸Ð½, ÐÐ½Ð´ÑÐµÐ¹
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: Ð¤Ð°Ð¹Ð»Ñ
ÐÐ²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÐµ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ð¼Ð¸ Ð¿ÑÐ¾ÑÐµÑÑÐ°Ð¼Ð¸
Ð¡ÑÐ°ÑÐ¸ÑÑÐ¸ÑÐµÑÐºÐ¸Ð¹ Ð°Ð½Ð°Ð»Ð¸Ð·

description: Ð¦ÐµÐ½ÑÑÐ°Ð»ÑÐ½Ð¾Ð¹ ÑÐµÐ¼Ð¾Ð¹ Ð½Ð°ÑÑÐ¾ÑÑÐµÐ¹ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ð° Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð»Ð¾Ð³Ð¾Ð² Ð² ÐºÐ¾Ð½ÑÐµÐºÑÑÐµ Ð¿ÑÐ¾ÑÐµÑÑÐ° ÑÐ¾Ð¿ÑÐ¾Ð²Ð¾Ð¶Ð´ÐµÐ½Ð¸Ñ Ð¸ Ð¿Ð¾Ð´Ð´ÐµÑÐ¶ÐºÐ¸ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð¾Ð³Ð¾ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ. Ð ÑÐ°ÑÑÐ½Ð¾ÑÑÐ¸, ÑÑÐ¾ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ð° Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð°ÑÐ¸Ð¸ Ð¿ÑÐ¾ÑÐµÑÑÐ° Ñ Ð¿Ð¾Ð¼Ð¾ÑÑÑ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ð¾Ð² Ð¸ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² ÑÑÐ°ÑÐ¸ÑÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¸ Ð¸Ð½ÑÐµÐ»Ð»ÐµÐºÑÑÐ°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð°Ð½Ð°Ð»Ð¸Ð·Ð°.
Ð¦ÐµÐ»ÑÑ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐ»Ð¾ÑÑ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ðµ ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð¹ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ Ð´Ð»Ñ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð»Ð¾Ð³-Ð´Ð°Ð½Ð½ÑÑ. ÐÐ°Ð½Ð½Ð°Ñ ÑÐ¸ÑÑÐµÐ¼Ð° Ð½Ð°ÑÐµÐ»ÐµÐ½Ð° Ð½Ð° ÑÐ°Ð±Ð¾ÑÑ Ñ ÑÐ°Ð¹Ð»Ð°Ð¼Ð¸ ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð¾Ð³Ð¾ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ°, ÐºÐ¾ÑÐ¾ÑÑÐ¹ ÑÐ»ÑÐ¶Ð¸Ñ Ð´Ð»Ñ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ ÑÑÐ½ÐºÑÐ¸Ð¾Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐ°ÑÐ¾Ð² Ð²Ð½ÑÑÑÐ¸ ÐºÐ¾Ð½ÑÐ°ÐºÑ-ÑÐµÐ½ÑÑÐ°.
B-Decay Signatures of Warped Top-Condensation
Creators: name: Davoudiasl, Hooman
name: Ponton, Eduardo
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We point out that the light radion phi in a recently proposed Warped Top-Condensation Model, can provide distinct signatures in b -> s phi, where the on-shell phi can decay with displaced vertices. We find that some of the parameter space of these models is constrained by B-meson and astrophysical data. Future B-decay measurements can lead to the discovery of the WTCM.
description: 4 pages
title: ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ð¹ Ð¸ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² Ð±ÑÐµÐ½Ð´Ð¸Ð½Ð³Ð° ÑÐµÑÑÐ¸ÑÐ¾ÑÐ¸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°Ð½ÑÐ±Ð°, ÐÐ»ÐµÑÑ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: Ð±ÑÐµÐ½Ð´Ð¸Ð½Ð³ ÑÐµÑÑÐ¸ÑÐ¾ÑÐ¸Ð¹
Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³ ÑÐµÑÑÐ¸ÑÐ¾ÑÐ¸Ð¹

description: ÐÐ±ÑÐµÐºÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ - Ð³Ð¾ÑÐ¾Ð´ ÐÐµÐ³Ð¸Ð¾Ð½. ÐÑÐµÐ´Ð¼ÐµÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð±ÑÐµÐ½Ð´Ð° Ð³Ð¾ÑÐ¾Ð´Ð° ÐÐµÐ³Ð¸Ð¾Ð½Ð°. Ð¦ÐµÐ»Ñ - ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ð¹ Ð¸ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² Ð±ÑÐµÐ½Ð´Ð¸Ð½Ð³Ð° ÑÐµÑÑÐ¸ÑÐ¾ÑÐ¸Ð¹. ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð±ÑÐµÐ½Ð´Ð° Ð³Ð¾ÑÐ¾Ð´Ð° ÐÐµÐ³Ð¸Ð¾Ð½Ð° Ð¿ÑÐ¸Ð½ÑÑÐ¾ ÑÐµÑÐµÐ½Ð¸Ðµ Ð¾ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ð¸ Ð±ÑÐµÐ½Ð´Ð¸Ð½Ð³Ð° ÑÐµÑÑÐ¸ÑÐ¾ÑÐ¸Ð¸ Ð³Ð¾ÑÐ¾Ð´Ð°, Ð¿ÑÐµÐ´ÑÑÐ¼Ð¾ÑÑÐµÐ½ ÑÑÐ´ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹. Ð¡Ð¾Ð·Ð´Ð°Ð½Ð¸Ðµ ÑÐ¸ÑÐ¼ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÑÐ¸Ð»Ñ Ð³Ð¾ÑÐ¾Ð´Ð° (Ð»Ð¾Ð³Ð¾ÑÐ¸Ð¿, Ð¿Ð¾Ð»Ð¸Ð³ÑÐ°ÑÐ¸Ñ, ÑÐ°Ð¹Ñ, ÑÑÐ²ÐµÐ½Ð¸ÑÑ), Ð¾Ð±ÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ° (Ð²Ð¾ÐºÐ·Ð°Ð»Ñ Ð¸ Ð¾ÑÑÐ°Ð½Ð¾Ð²ÐºÐ¸), Ð½Ð°Ð²Ð¸Ð³Ð°ÑÐ¸Ð¸ (ÑÑÐµÐ¼Ñ, Ð²ÑÐ²ÐµÑÐºÐ¸), Ð¿ÑÐµÐ´Ð¾ÑÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ ÑÐ½Ð¸ÐºÐ°Ð»ÑÐ½Ð¾Ð³Ð¾ ÑÑÐ¸Ð»Ñ Ð³Ð¾ÑÐ¾Ð´ÑÐºÐ¸Ð¼ Ð¾Ð±ÑÐµÐºÑÐ°Ð¼ (Ð¼ÑÐ·ÐµÑÐ¼, Ð¿Ð°ÑÐºÐ°Ð¼, Ð´ÑÑÐ³Ð¸Ð¼ ÑÑÑÐµÐ¶Ð´ÐµÐ½Ð¸ÑÐ¼). ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ðµ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹, Ð¿ÑÐ°Ð·Ð´Ð½Ð¸ÐºÐ¾Ð², ÑÐµÑÑÐ¸Ð²Ð°Ð»ÐµÐ¹ Ð¸ Ð¸Ñ ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÑÑÐµÐµ Ð¾ÑÐ¾ÑÐ¼Ð»ÐµÐ½Ð¸Ðµ. Ð¡Ð¾Ð¾ÑÑÐ¶ÐµÐ½Ð¸Ðµ Ð¸Ð½ÑÐµÑÐµÑÐ½ÑÑ ÑÐ½Ð¸ÐºÐ°Ð»ÑÐ½ÑÑ Ð·Ð´Ð°Ð½Ð¸Ð¹. ÐÐ¾ÑÐ²Ð»ÐµÐ½Ð¸Ðµ Ð½Ð¾Ð²ÑÑ Ð³Ð¾ÑÐ¾Ð¶Ð°Ð½, Ð¶ÐµÐ»Ð°ÑÑÐ¸Ñ Ð¿ÑÐ¸Ð¾Ð±ÑÐµÑÑÐ¸ Ð¶Ð¸Ð»ÑÐµ Ð² Ð³Ð¾ÑÐ¾Ð´Ðµ, Ð²ÑÐ·Ð¾Ð²ÐµÑ Ð¿Ð¾ÑÑÐµÐ±Ð½Ð¾ÑÑÑ Ð² ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ðµ. Ð¡Ð¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÐµÐ½Ð½Ð¾ Ð¿Ð¾ÑÐ²ÑÑÑÑ Ð·Ð°ÑÑÑÐ¾Ð¹ÑÐ¸ÐºÐ¸ Ð¸ Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¸ Ð² Ð½ÐµÐ´Ð²Ð¸Ð¶Ð¸Ð¼Ð¾ÑÑÑ. Ð¡Ð´ÐµÐ»Ð°Ð½ Ð¿ÑÐ¾Ð³Ð½Ð¾Ð· Ð·Ð°ÑÑÐ°Ñ Ð¸ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¾Ð² Ð´Ð»Ñ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð¸ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ Ð¿ÑÐµÐ´Ð»Ð°Ð³Ð°ÐµÐ¼ÑÑ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ¾Ðº. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ ÑÐ°ÑÑÐµÑ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð½ÑÑ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹.
A tentative detection of He I in the atmosphere of GJ 1214b
Creators: name: Orell-Miquel, J.
name: Murgas, F.
name: Pallé, E.
name: Lampón, M.
name: López-Puertas, M.
name: Sanz-Forcada, J.
name: Nagel, E.
name: Kaminski, A.
name: Casasayas-Barris, N.
name: Nortmann, L.
name: Luque, R.
name: Molaverdikhani, K.
name: Sedaghati, E.
name: Caballero, J. A.
name: Amado, P. J.
name: Bergond, G.
name: Czesla, S.
name: Hatzes, A. P.
name: Henning, Th.
name: Khalafinejad, S.
name: Montes, D.
name: Morello, G.
name: Quirrenbach, A.
name: Reiners, A.
name: Ribas, I.
name: Sánchez-López, A.
name: Schweitzer, A.
name: Stangret, M.
name: Yan, F.
name: Osorio, M. R. Zapatero
Publisher: name: arXiv
Year: 2022
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: The $\ion{He}{I}$ 10833\,$Å$ triplet is a powerful tool for characterising the upper atmosphere of exoplanets and tracing possible mass loss. Here, we analysed one transit of GJ\,1214\,b observed with the CARMENES high-resolution spectrograph to study its atmosphere via transmission spectroscopy around the $\ion{He}{I}$ triplet. Although previous studies using lower resolution instruments have reported non-detections of $\ion{He}{I}$ in the atmosphere of GJ\,1214\,b, we report here the first potential detection. We reconcile the conflicting results arguing that previous transit observations did not present good opportunities for the detection of $\ion{He}{I}$, due to telluric H$_2$O absorption and OH emission contamination.We simulated those earlier observations, and show evidence that the planetary signal was contaminated. From our single non-telluric-contaminated transit, we determined an excess absorption of 2.10$^{+0.45}_{-0.50}$\,\% (4.6\,$σ$) with a full width at half maximum (FWHM) of 1.30$^{+0.30}_{-0.25}$\,Å. The detection of \ion{He}{I} is statistically significant at the 4.6\,$σ$ level, but repeatability of the detection could not be confirmed due to the availability of only one transit. By applying a hydrodynamical model and assuming an H/He composition of 98/2, we found that GJ\,1214\,b would undergo hydrodynamic escape in the photon-limited regime, losing its primary atmosphere with a mass-loss rate of (1.5--18)\,$\times$\,10$^{10}$\,g\,s$^{-1}$ and an outflow temperature in the range of 2900--4400\,K. Our $\ion{He}{I}$ excess absorption is the first tentative detection of a chemical species in the atmosphere of this benchmark sub-Neptune planet.
description: Accepted for publication in A&A. 12 pages, 7 figures
title: Ð£Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð¾Ð±Ð¾ÑÐ¾ÑÐ½ÑÐ¼ ÐºÐ°Ð¿Ð¸ÑÐ°Ð»Ð¾Ð¼ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ ÑÐ¾Ð·Ð½Ð¸ÑÐ½Ð¾Ð¹ ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ð¸
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð¨Ð¿Ð¸ÑÑÐºÐ¾, ÐÐºÑÐ°Ð½Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2016
Subjects: ÑÐ¾Ð·Ð½Ð¸ÑÐ½Ð°Ñ ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ñ
Ð¾Ð±Ð¾ÑÐ¾ÑÐ½ÑÐ¹ ÑÑÐµÐ´ÑÑÐ²Ð°
ÐºÐ°Ð¿Ð¸ÑÐ°Ð»

description: ÐÐ±ÑÐµÐºÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ - Ð¾Ð±ÑÐµÑÑÐ²Ð¾ Ñ Ð¾Ð³ÑÐ°Ð½Ð¸ÑÐµÐ½Ð½Ð¾Ð¹ Ð¾ÑÐ²ÐµÑÑÑÐ²ÐµÐ½Ð½Ð¾ÑÑÑÑ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ðµ ÑÐ¾Ð·Ð½Ð¸ÑÐ½Ð¾Ð¹ ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ð¸ Â«Ð®Ð½Ð¾ÑÑÑÂ». Ð¦ÐµÐ»Ñ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ - Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¾Ð±Ð¾ÑÐ¾ÑÐ½ÑÐ¼ ÐºÐ°Ð¿Ð¸ÑÐ°Ð»Ð¾Ð¼ Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ ÑÐ¾Ð·Ð½Ð¸ÑÐ½Ð¾Ð¹ ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ð¸ Ð¸ Ð²ÑÑÐ°Ð±Ð¾ÑÐºÐ° ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¹ Ð¿Ð¾ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¸Ð¼. Ð ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¾Ð±Ð¾ÑÐ¾ÑÐ½ÑÐ¼ ÐºÐ°Ð¿Ð¸ÑÐ°Ð»Ð¾Ð¼ Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ ÑÐ¾Ð·Ð½Ð¸ÑÐ½Ð¾Ð¹ ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ð¸ Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¿Ð¾ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¸Ð¼.
title: ÐÐµÑÐ¾Ð´Ð¸ÐºÐ° Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ðº Ð¿ÑÐµÐ¾Ð´Ð¾Ð»ÐµÐ½Ð¸Ñ ÑÑÐ½Ð¾ÐºÑÐ»ÑÑÑÑÐ½ÑÑ ÑÑÐµÑÐµÐ¾ÑÐ¸Ð¿Ð¾Ð² Ð² Ð¿ÑÐ¾ÑÐµÑÑÐµ Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ Ð¸Ð½Ð¾ÑÑÑÐ°Ð½Ð½ÑÐ¼ ÑÐ·ÑÐºÐ°Ð¼
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¸ÑÐ°Ð¹Ð»Ð¾Ð²Ð°, 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: ÑÑÐµÑÐµÐ¾ÑÐ¸Ð¿
ÑÐ¾ÑÐ¸Ð¾ÐºÑÐ»ÑÑÑÑÐ½Ð°Ñ ÐºÐ¾Ð¼Ð¿ÐµÑÐµÐ½ÑÐ¸Ñ
ÑÑÐ½Ð¾ÐºÑÐ»ÑÑÑÑÐ½ÑÐ¹ ÑÑÐµÑÐµÐ¾ÑÐ¸Ð¿
Ð°Ð²ÑÐ¾ÑÑÐµÑÐµÐ¾ÑÐ¸Ð¿
Ð³ÐµÑÐµÑÐ¾ÑÑÐµÑÐµÐ¾ÑÐ¸Ð¿

description: Ð Ð°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° Ð¾Ð´Ð½Ð¾Ð¹ Ð¸Ð· Ð½Ð°Ð¸Ð±Ð¾Ð»ÐµÐµ Ð·Ð½Ð°ÑÐ¸Ð¼ÑÑ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð¹ Ð¼ÐµÐ¶ÐºÑÐ»ÑÑÑÑÐ½Ð¾Ð¹ ÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð¸, Ð° Ð¸Ð¼ÐµÐ½Ð½Ð¾ ÑÑÐ½Ð¾ÐºÑÐ»ÑÑÑÑÐ½ÑÐ¼ ÑÑÐµÑÐµÐ¾ÑÐ¸Ð¿Ð°Ð¼ Ð¸ Ð¸Ñ Ð²Ð»Ð¸ÑÐ½Ð¸Ñ Ð½Ð° Ð²Ð·Ð°Ð¸Ð¼Ð¾Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ ÑÑÐ°ÑÑÐ½Ð¸ÐºÐ¾Ð² Ð¸Ð½ÑÐµÑÐ½Ð°ÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ð¹ Ð±ÐµÑÐµÐ´Ñ. ÐÐ¾ ÑÑÐ´Ñ Ð¿ÑÐ¸ÑÐ¸Ð½ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ÑÑÐ½Ð¾ÐºÑÐ»ÑÑÑÑÐ½ÑÑ ÑÑÐµÑÐµÐ¾ÑÐ¸Ð¿Ð¾Ð² Ð¿ÑÐ¾Ð´Ð¾Ð»Ð¶Ð°ÐµÑ ÑÐ²Ð¾Ðµ ÑÑÑÐµÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ðµ, Ð½ÐµÑÐ¼Ð¾ÑÑÑ Ð½Ð° Ð¿Ð¾ÑÐ²Ð»ÐµÐ½Ð¸Ðµ Ð¸ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ðµ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½ÑÑ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¹, Ð·Ð°Ð½Ð¸Ð¼Ð°ÑÑÐ¸Ñ Ð·Ð½Ð°ÑÐ¸ÑÐµÐ»ÑÐ½Ð¾Ðµ Ð¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ðµ Ð² Ð¶Ð¸Ð·Ð½Ð¸ ÐºÐ°Ð¶Ð´Ð¾Ð³Ð¾ ÑÐµÐ»Ð¾Ð²ÐµÐºÐ°. ÐÐ°Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° ÑÐ°ÑÐºÑÑÐ²Ð°ÐµÑ Ð¿Ð¾Ð½ÑÑÐ¸Ñ Ð¿ÑÐ¸ÑÐ°ÑÑÐ½ÑÐµ Ðº Ð´Ð°Ð½Ð½Ð¾Ð¹ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ðµ Ð¸ Ð´ÐµÐ¼Ð¾Ð½ÑÑÑÐ¸ÑÑÐµÑ Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÑ Ð¿Ð¾ Ð¿ÑÐµÐ¾Ð´Ð¾Ð»ÐµÐ½Ð¸Ñ ÑÐ°ÐºÐ¾Ð³Ð¾ ÑÐµÐ½Ð¾Ð¼ÐµÐ½Ð° ÐºÐ°Ðº Â«ÑÑÐ½Ð¾ÐºÑÐ»ÑÑÑÑÐ½ÑÐ¹ ÑÑÐµÑÐµÐ¾ÑÐ¸Ð¿Â» Ð² ÑÐ°Ð¼ÐºÐ°Ñ Ð´Ð²ÑÑ ÑÐ·ÑÐºÐ¾Ð²ÑÑ ÐºÑÐ»ÑÑÑÑ: Ð¸ÑÐ¿Ð°Ð½ÑÐºÐ¾Ð¹ Ð¸ ÑÑÑÑÐºÐ¾Ð¹.