cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Cold Dark Matter Substructure and Galactic Disks II: Dynamical Effects of Hierarchical Satellite Accretion
Creators: name: Kazantzidis, Stelios
name: Zentner, Andrew R.
name: Kravtsov, Andrey V.
name: Bullock, James S.
name: Debattista, V. P.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: (Abridged) We perform dissipationless N-body simulations to elucidate the dynamical response of thin disks to bombardment by cold dark matter (CDM) substructure. Our method combines (1) cosmological simulations of the formation of Milky Way (MW)-sized CDM halos to derive the properties of substructure and (2) controlled numerical experiments of consecutive subhalo impacts onto an initially-thin, fully-formed MW type disk galaxy. The present study is the first to account for the evolution of satellite populations over cosmic time in such an investigation of disk structure. We find that accretions of massive subhalos onto the central regions of host halos, where the galactic disks reside, since z~1 should be common. One host halo accretion history is used to initialize the controlled simulations of satellite-disk encounters. We show that these accretion events severely perturb the thin galactic disk and produce a wealth of distinctive dynamical signatures on its structure and kinematics. These include (1) considerable thickening and heating at all radii, with the disk thickness and velocity ellipsoid nearly doubling at the solar radius; (2) prominent flaring associated with an increase in disk thickness greater than a factor of 4 in the disk outskirts; (3) surface density excesses at large radii, beyond ~5 disk scale lengths, resembling those of observed antitruncated disks; (4) lopsidedness at levels similar to those measured in observational samples of disk galaxies; and (5) substantial tilting. The interaction with the most massive subhalo drives the disk response while subsequent bombardment is much less efficient at disturbing the disk. We conclude that substructure-disk encounters of the kind expected in the LCDM paradigm play a significant role in setting the structure of disk galaxies and driving galaxy evolution.
description: Accepted for publication in ApJ, 28 pages, 13 figures, LaTeX (uses emulateapj.cls)
title: ÐÐµÑÑÐ¿ÐµÐºÑÐ¸Ð²Ñ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ Ð¿ÑÐ¾ÑÐµÐ´ÑÑÑ Ð¾ÑÐµÐ½ÐºÐ¸ Ð¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿ÑÐ¾ÑÐµÑÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½ÑÐ¼ ÑÐ¸ÑÐºÐ¾Ð¼ Ð² ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¾Ñ ÑÐ°Ð½Ð¾Ð¹ ÑÑÑÐ´Ð°
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: Ð§ÐµÐ¿ÐµÐ»ÐµÐ², ÐÐ¼Ð¸Ñ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: 2017
Subjects: ÐÑ ÑÐ°Ð½Ð° ÑÑÑÐ´Ð°
ÐÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÑ Ð¶Ð¸Ð·Ð½ÐµÐ´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÑÐµÐ»Ð¾Ð²ÐµÐºÐ°
ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ ÑÐ¸ÑÐºÐ¾Ð¼
Ð¿ÑÐ¾ÑÐµÑÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½ÑÐµ ÑÐ¸ÑÐºÐ¸
ÑÑÐ»Ð¾Ð²Ð¸Ñ ÑÑÑÐ´Ð°

description: Ð Ð°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° Ð°Ð½Ð°Ð»Ð¸Ð·Ñ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼ Ð¸ Ð¿ÐµÑÑÐ¿ÐµÐºÑÐ¸Ð² Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ Ð¿ÑÐ¾ÑÐµÐ´ÑÑÑ Ð¾ÑÐµÐ½ÐºÐ¸ Ð¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿ÑÐ¾ÑÐµÑÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½ÑÐ¼ ÑÐ¸ÑÐºÐ¾Ð¼ Ð² ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¾ÑÑÐ°Ð½Ð¾Ð¹ ÑÑÑÐ´Ð°. Ð ÑÐ¾Ð´Ðµ ÑÐ°Ð±Ð¾ÑÑ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ñ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð²Ð¾Ð¿ÑÐ¾ÑÐ¾Ð² Ð² Ð¾Ð±Ð»Ð°ÑÑÐ¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÑÐ¸ÑÐºÐ°Ð¼Ð¸, Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ñ Ð¸ Ð¸Ð·ÑÑÐµÐ½Ñ ÑÐ¾ÑÑÐ°Ð²Ð»ÑÑÑÐ¸Ðµ Ð¿ÑÐ¾ÑÐµÑÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ ÑÐ¸ÑÐºÐ°, Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ ÑÑÐ°Ð²Ð½Ð¸ÑÐµÐ»ÑÐ½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÑÑÐµÑÑÐ²ÑÑÑÐ¸Ñ Ð¼ÐµÑÐ¾Ð´Ð¸Ðº Ð¾ÑÐµÐ½ÐºÐ¸ Ð¿ÑÐ¾ÑÐµÑÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ ÑÐ¸ÑÐºÐ° ÑÐ°Ð±Ð¾ÑÐ½Ð¸ÐºÐ¾Ð², Ð²ÑÑÐ²Ð»ÐµÐ½ ÑÑÐ´ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼ Ð¸ Ð¿ÐµÑÑÐ¿ÐµÐºÑÐ¸Ð², ÐºÐ¾ÑÐ¾ÑÑÐµ Ð²Ð¾Ð·Ð½Ð¸ÐºÐ½ÑÑ Ð² Ð¿ÑÐ¾ÑÐµÑÑÐµ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ Ð¾ÑÐµÐ½ÐºÐ¸ Ð¿ÑÐ¾ÑÐµÑÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½ÑÑ ÑÐ¸ÑÐºÐ¾Ð².
Self-force with (3+1) codes: a primer for numerical relativists
Creators: name: Vega, Ian
name: Diener, Peter
name: Tichy, Wolfgang
name: Detweiler, Steven
Publisher: name: arXiv
Year: 2009
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: Prescriptions for numerical self-force calculations have traditionally been designed for frequency-domain or (1+1) time-domain codes which employ a mode decomposition to facilitate in carrying out a delicate regularization scheme. This has prevented self-force analyses from benefiting from the powerful suite of tools developed and used by numerical relativists for simulations of the evolution of comparable-mass black hole binaries. In this work, we revisit a previously-introduced (3+1) method for self-force calculations, and demonstrate its viability by applying it to the test case of a scalar charge moving in a circular orbit around a Schwarzschild black hole. Two (3+1) codes originally developed for numerical relativity applications were independently employed, and in each we were able to compute the two independent components of the self-force and the energy flux correctly to within $< 1%$. We also demonstrate consistency between $t$-component of the self-force and the scalar energy flux. Our results constitute the first successful calculation of a self-force in a (3+1) framework, and thus open opportunities for the numerical relativity community in self-force analyses and the perturbative modeling of extreme-mass-ratio inspirals.
description: 23 pages, 13 figures
title: Ð¡Ð¸ÑÑÐµÐ¼Ð½ÑÐµ ÑÐµÑÑÑÑÑ ÐºÐ°ÑÐµÑÑÐ²Ð° Ð²ÑÑÑÐµÐ³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð Ð¾ÑÑÐ¸Ð¸ Ð¸ ÐÐ²ÑÐ¾Ð¿Ñ
Creators: name: ÐÑÐ»Ð°ÐµÐ², ÐÐ¸ÐºÐ¾Ð»Ð°Ð¹
name: ÐÐ¾Ð·Ð»Ð¾Ð², ÐÐ»Ð°Ð´Ð¸Ð¼Ð¸Ñ
name: ÐÐ¾Ð·Ð»Ð¾Ð², ÐÐ»Ð°Ð´Ð¸Ð¼Ð¸Ñ
name: Ð ÑÐ´ÑÐºÐ¾Ð¹, ÐÐ½Ð´ÑÐµÐ¹
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2009
Subjects: Ð²ÑÑÑÐµÐµ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ðµ
ÐºÐ°ÑÐµÑÑÐ²Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ
ÑÐ¸ÑÑÐµÐ¼Ð½ÑÐµ ÑÐµÑÑÑÑÑ
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Cross sections for neutron capture from surrogate measurements: An examination of Weisskopf-Ewing and ratio approximations
Creators: name: Escher, Jutta E.
name: Dietrich, Frank S.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: Motivated by the renewed interest in the surrogate nuclear reactions approach, an indirect method for determining compound-nuclear reaction cross sections, the prospects for determining (n, gamma) cross sections for deformed rare-earth and actinide nuclei are investigated. A nuclear-reaction model is employed to simulate physical quantities that are typically measured in surrogate experiments and used to assess the validity of the Weisskopf-Ewing and ratio approximations, which are typically employed in the analysis of surrogate reactions. The expected accuracy of (n,gamma) cross sections extracted from typical surrogate measurements is discussed and limitations of the approximate methods are illustrated. Suggestions for moving beyond presently-employed approximations are made.
description: 18 pages, 15 figures
Community detection in networks with positive and negative links
Creators: name: Traag, V. A.
name: Bruggeman, Jeroen
Publisher: name: arXiv
Year: 2008
Subjects: subject: Physics and Society (physics.soc-ph)
subject: FOS: Physical sciences

description: Detecting communities in complex networks accurately is a prime challenge, preceding further analyses of network characteristics and dynamics. Until now, community detection took into account only positively valued links, while many actual networks also feature negative links. We extend an existing Potts model to incorporate negative links as well, resulting in a method similar to the clustering of signed graphs, as dealt with in social balance theory, but more general. To illustrate our method, we applied it to a network of international alliances and disputes. Using data from 1993--2001, it turns out that the world can be divided into six power blocs similar to Huntington's civilizations, with some notable exceptions.
description: 7 pages, 2 figures. Revised version
Analysis of a mathematical model for multi-phase motion and local non-equilibrium heat transfer in a blast furnace
Creators: name: Vynnycky, Michael
name: V. Rangavittal, B.
name: Glaser, B.
Publisher: name: University of Limerick
Year: 2025
Subjects: classificationCode: 49
subject: Mathematical sciences

description: In this paper, we extend a recent asymptotic axisymmetric model for isothermal gas–solid flow in a countercurrent moving-bed reactor to a non-isothermal model for the heat transfer in an ironmaking blast furnace. The appended heat transfer model accounts for conduction, convection, thermal non-equilibrium between the gas and solid phases and the dominant endothermic chemical reaction in the bulk of the furnace, the Boudouard reaction. Asymptotic analysis is used to determine the leading-order heat balances and to interpret numerically obtained solutions for the phase tempera?tures. Although the model is considerably simpler than the many numerical models that already exist for blast-furnace operation, its future extension would form the basis of a computationally efficient approach for modelling the transient state of a blast furnace.
On a conjecture of Vorst
Creators: name: Geisser, Thomas
name: Hesselholt, Lars
Publisher: name: arXiv
Year: 2009
Subjects: subject: K-Theory and Homology (math.KT)
subject: Algebraic Geometry (math.AG)
subject: FOS: Mathematics
subject: 19D35, 14F20

description: We prove the following result. Let k be an infinite perfect field of positive characteristic and assume that strong resolution of singularities holds over k. Let R be a localization of a commutative d-dimensional k-algebra of finite type and suppose that R is K_{d+1}-regular. Then R is a regular ring.
title: ÐÐ½Ð°Ð»Ð¸Ð· Ð¿ÐµÑcÐ¿ÐµÐºÑÐ¸Ð² Ð¸Ð½ÑÐµÑÐ½Ð°ÑÐ¸Ð¾Ð½Ð°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ ÐºÐ¸ÑÐ°Ð¹cÐºÐ¾Ð³Ð¾ ÑÐ°Ð½Ñ
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¶Ð¾Ñ Ð®Ð¹Ñ ÑÐ½
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: ÑÐ°Ð½Ñ
Ð¸Ð½ÑeÑÐ½Ð°ÑÐ¸oÐ½Ð°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ Ð²Ð°Ð»ÑÑ
Ð¿ÑÐ¾ÑÐµÑÑ Ð¸Ð½ÑeÑÐ½Ð°ÑÐ¸oÐ½Ð°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÐ°Ð½Ñ

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Additional file 1 of Horizontal transfer of a plasmid possessing mcr-1 marked with a single nucleotide mutation between Escherichia coli isolates from community residents
Creators: name: Yamamoto, Yoshimasa
name: Higashi, Ayano
name: Ikawa, Kanoko
name: Hoang, Hoa Thi Thanh
name: Yamaguchi, Takahiro
name: Kawahara, Ryuji
name: Noguchi, Hideki
name: Nguyen, Thang Nam
name: Khong, Diep Thi
name: Tran, Hoa Thi
Publisher: name: figshare
Year: 2022
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 1. Details of an example of sequence assembly using Unicycler in this study.
Blazars in hard X-rays
Creators: name: Ghisellini, Gabriele
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Although blazars are thought to emit most of their luminosity in the gamma-ray band, there are subclasses of them very prominent in hard X-rays. These are the best candidates to be studied by Simbol-X. They are at the extremes of the blazar sequence, having very small or very high jet powers. The former are the class of TeV emitting BL Lacs, whose synchrotron emission often peaks at tens of keV or more. The latter are the blazars with the most powerful jets and have high black hole masses accreting at high (i.e. close to Eddington) rates. These sources are predicted to have their high energy peak even below the MeV band, and therefore are very promising candidates to be studied with Simbol-X.
description: Invited talk at the Simbol-X symposium held in Paris, 2-5 December, 2008. 6 pages, 6 figures
title: ÐÐ¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð°Ñ Ð¸ Ð¼ÑÐ½Ð¸ÑÐ¸Ð¿Ð°Ð»ÑÐ½Ð°Ñ ÑÐ»ÑÐ¶Ð±Ð°
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐ²Ð°Ð½Ð¾Ð²Ð°, ÐÐ°ÑÐ¸Ð½Ð°
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2019
Subjects: Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð°Ñ ÑÐ»ÑÐ¶Ð±Ð°
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description: ÐÐ°ÑÑÐ½Ð°Ñ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÑ â 08.00.05 Â«Ð­ÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ° Ð¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð½Ð°ÑÐ¾Ð´Ð½ÑÐ¼
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Género y territorio: condiciones de reproducción de la vida, política pública y participación de las mujeres indígenas, campesinas y agricultoras en Ecuador
Creators: name: Mejía, Silvia Viviana
Publisher: name: Knowledge Commons
Year: 2025

description: El artículo examina la situación de las mujeres indígenas y campesinas ecuatorianas en relación
con sus condiciones de vida, el impacto de la política pública, su inclusión en normativas y su
participación territorial. Las mujeres rurales ecuatorianas tuvieron un papel protagónico entre
2011 y 2015, destacándose en el debate político sobre sus derechos, el territorio y la defensa
de los recursos naturales. Durante este periodo, las políticas públicas tuvieron un impacto
favorable en la reproducción social de la vida, pero persistieron índices de precariedad que
evidenciaron la exclusión social y económica.
El artículo busca evidenciar la doble dinámica que enfrentan las mujeres indígenas, campesinas
y agricultoras en Ecuador: la reproducción de la vida en condiciones precarias y su
participación en el territorio rural. Se investiga cómo se autodefinen las mujeres rurales de
Ecuador y si lograron inclusión en las políticas públicas y mejorar sus condiciones de vida y
participación política. Se utilizan metodologías cualitativas y cuantitativas, incluyendo
entrevistas a lideresas del Encuentro Político de las Mujeres Rurales Diversas unidas por el
Buen Vivir y la Soberanía Alimentaria
Strong field gravitational lensing in the deformed Hǒrava-Lifshitz black hole
Creators: name: Chen, Songbai
name: Jing, Jiliang
Publisher: name: arXiv
Year: 2009
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: Adopting the strong field limit approach, we studied the properties of strong field gravitational lensing in the deformed Hǒrava-Lifshitz black hole and obtained the angular position and magnification of the relativistic images. Supposing that the gravitational field of the supermassive central object of the galaxy described by this metric, we estimated the numerical values of the coefficients and observables for gravitational lensing in the strong field limit. Comparing with the Reissner-Norstr\"{om} black hole, we find that with the increase of parameter $α$, the angular position $θ_{\infty}$ decreases more slowly and $r_m$ more quickly, but angular separation $s$ increases more rapidly. This may offer a way to detect the effects of to distinguish a deformed Hǒrava-Lifshitz black hole from a Reissner-Norstr\"{om} black hole by the astronomical instruments in the future.
description: 12 pages, 2 figures,some references added, Accepted by PRD
Optical conductivity of a metal-insulator transition for the Anderson-Hubbard model in 3 dimensions away from 1/2 filling
Creators: name: Chen, X.
name: Gooding, R. J.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: FOS: Physical sciences

description: We have completed a numerical investigation of the Anderson-Hubbard model for three-dimensional simple cubic lattices using a real-space self-consistent Hartree-Fock decoupling approximation for the Hubbard interaction. In this formulation we treat the spatial disorder exactly, and therefore we account for effects arising from localization physics. We have examined the model for electronic densities well away 1/2 filling, thereby avoiding the physics of a Mott insulator. Several recent studies have made clear that the combined effects of electronic interactions and spatial disorder can give rise to a suppression of the electronic density of states, and a subsequent metal-insulator transition can occur. We augment such studies by calculating the ac conductivity for such systems. Our numerical results show that weak interactions enhance the density of states at the Fermi level and the low-frequency conductivity, there are no local magnetic moments, and the ac conductivity is Drude-like. However, with a large enough disorder strength and larger interactions the density of states at the Fermi level and the low-frequency conductivity are both suppressed, the conductivity becomes non-Drude-like, and these phenomena are accompanied by the presence of local magnetic moments. The low-frequency conductivity changes from a sigma-sigma_dc omega^{1/2} behaviour in the metallic phase, to a sigma omega^2 behaviour in the nonmetallic regime. Our numerical results show that the formation of magnetic moments is essential to the suppression of the density of states at the Fermi level, and therefore essential to the metal-insulator transition.
Analytical Treatment of Particle-Core Interaction
Creators: name: Batygin, Yuri K.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Accelerator Physics (physics.acc-ph)
subject: FOS: Physical sciences

description: Particle-core interaction is the well-developed model of halo formation in high-intensity beams. In present paper an analytical solution for averaged single particle dynamics around uniformly charged beam core is obtained. The problem is analyzed through sequence of canonical transformations of Hamiltonian describing nonlinear particle oscillations. An analytical expression for maximum particle deviation from the axis is obtained. Results of the study are in good agreement with numerical simulations and with previously achieved data.
description: 11 pages, 7 figures
Citizen participation in neighbourhood rehabilitation: a pilot study of a sample area (Lower Mount Pleasant) Vancouver, British Columbia, 1962
Creators: name: Hicks, Helga Maria
Publisher: name: University of British Columbia
Year: 2011

description: For a long time, the section of the city in which social welfare, city planning and housing reformers have had common ground, has been that of "the slums". Just as the more comprehensive approach of "urban renewal" has taken over from "slum clearance", so also has interest in the modern city, in the throes of growth and decay, shifted to districts where rehabilitation rather than large-scale demolition may be appropriate. The present study is a pilot project for this kind of area. A small neighbourhood from the "limited redevelopment" section of Vancouver (Lower Mount Pleasant, to the south of False Creek) has been selected for detailed study, with special reference to (a) its physical and environmental features, (b) its resident population, and (c) the prospects of local community action, as well as the forms of aid and encouragement from appropriate agencies of government or citizen action needed to bring about effective rehabilitation. There are implications here for individual social workers, for social agencies, and for the social work profession which can only be concretely drawn on the basis of a "grass roots" survey. Ways and means of co-operation between social workers and planners is also one of the issues in this kind of study. The method of the project was twofold: (a) A review of the rapidly growing literature on neighbourhood rehabilitation, largely American, was undertaken to abstract the broad principles for gaining and maintaining citizen participation which are emerging. (b) The pilot area was surveyed in detail. (i) All appropriate voluntary and public agencies and government departments were approached for information about the physical and social features of the area. (Maps help to define the district.) (ii) Leaders of representative community groups operating in the larger neighbourhood were interviewed to appraise needs and attitudes. (iii) A questionnaire was devised to assess the identification of the residents with the area, and the possibility of involving residents in the rehabilitation of the neighbourhood. Perhaps the main finding of this pioneer survey is that both assets and liabilities must be realistically assessed for a successful community organization undertaking. (a) Neighbourhood rehabilitation requires (i) abroad national legislative and administrative framework, (ii) a partnership between city officials, city-wide citizen groups and residential groups at the neighbourhood level, (iii) at least a minimum staff trained in community organization to assist local neighbourhood action, (b) This particular area is not likely to initiate action by itself, (c) Current public utilities (including school, parks, streets, etc.) are of strategic importance in neighbourhood development; financing, both from new and existing sources, must be given proper consideration in the total program.
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¹ Ð¿Ð¾ ÑÐ»ÑÑÑÐµÐ½Ð¸Ñ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¾Ð±ÑÐ·Ð°ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð°Ð²ÑÐ¾ÑÑÑÐ°Ñ Ð¾Ð²Ð°Ð½Ð¸Ñ Ð³ÑÐ°Ð¶Ð´Ð°Ð½ÑÐºÐ¾Ð¹ Ð¾ÑÐ²ÐµÑÑÑÐ²ÐµÐ½Ð½Ð¾ÑÑÐ¸
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: ÐÐ¸ÑÐ¾Ð½Ð¾Ð², ÐÐ¸ÑÐ°Ð¸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: 2017
Subjects: ÑÑÑÐ°Ñ Ð¾Ð²Ð°Ð½Ð¸Ðµ
Ð³ÑÐ°Ð¶Ð´Ð°Ð½ÑÐºÐ°Ñ Ð¾ÑÐ²ÐµÑÑÑÐ²ÐµÐ½Ð½Ð¾ÑÑÑ
Ð¼Ð¾ÑÐµÐ½Ð½Ð¸ÑÐµÑÑÐ²Ð¾

description: Ð ÑÐ°Ð¼ÐºÐ°Ñ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¸Ð·ÑÑÐµÐ½Ñ: Ð½Ð¾ÑÐ¼Ð°ÑÐ¸Ð²Ð½Ð¾-Ð¿ÑÐ°Ð²Ð¾Ð²Ð°Ñ Ð±Ð°Ð·Ð° Ð² ÑÑÐµÑÐµ ÑÑÑÐ°ÑÐ¾Ð²Ð°Ð½Ð¸Ñ, Ð·Ð°ÑÑÐ±ÐµÐ¶Ð½ÑÐ¹ Ð¾Ð¿ÑÑ ÐÐ¡ÐÐÐ, Ð°Ð½Ð°Ð»Ð¸Ð· ÑÑÐ½ÐºÐ° ÑÑÑÐ°ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð² Ð Ð¤, Ð¿Ð¾ÑÑÐ´Ð¾Ðº Ð·Ð°ÐºÐ»ÑÑÐµÐ½Ð¸Ñ Ð´Ð¾Ð³Ð¾Ð²Ð¾ÑÐ°. ÐÑÐ»Ð¸ Ð²ÑÑÐ²Ð»ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð°ÐºÑÑÐ°Ð»ÑÐ½ÑÐµ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ Ð² ÑÑÐµÑÐµ ÑÑÑÐ°ÑÐ¾Ð²Ð°Ð½Ð¸Ñ. ÐÑÐ¾Ð±Ð¾Ðµ Ð¼ÐµÑÑÐ¾ ÑÐ´ÐµÐ»ÑÐµÑÑÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ, ÐºÐ°ÑÐ°ÑÑÐµÐ³Ð¾ÑÑ Ð¿Ð¾ÑÑÐ´ÐºÑ Ð·Ð°ÐºÐ»ÑÑÐµÐ½Ð¸Ñ Ð´Ð¾Ð³Ð¾Ð²Ð¾ÑÐ° ÐÐ¡ÐÐÐ. Ð ÐºÐ°ÑÐµÑÑÐ²Ðµ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¾Ð² Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÑÑÑÑÑ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ð¿Ð¾ ÑÐ»ÑÑÑÐµÐ½Ð¸Ñ ÑÐ¸ÑÑÐµÐ¼Ñ ÐÐ¡ÐÐÐ Ð¸ ÑÐ¼ÐµÐ½ÑÑÐµÐ½Ð¸Ñ Ð½ÐµÐ³Ð°ÑÐ¸Ð²Ð°, ÐºÐ°Ðº ÑÐ¾ ÑÑÐ¾ÑÐ¾Ð½Ñ ÑÑÑÐ°ÑÐ¾Ð²ÑÑ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¹, ÑÐ°Ðº Ð¸ ÑÑÑÐ°ÑÐ¾Ð²Ð°ÑÐµÐ»ÐµÐ¹.
Composite Gauge Fields in Renormalizable Models
Creators: name: F. Palumbo
Publisher: name: INFN Open Access Repository
Year: 1993

description: We construct models of gauge theories renormalizable by power counting in four dimensions, with gauge fields composite of bosonic or fermionic constituents. They are obtained by a regularization of CP^n-1 models where the constraint on constituent fields is replaced by a constraint on expectation values.
A Dose Comparison Between Gas Bremsstrahlung and Single Beam???Beam Bremsstrahlung at High Luminosity e+ e??? Storage Rings
Creators: name: D. Babusci
name: M. Pelliccioni
Publisher: name: INFN Open Access Repository
Year: 1994

description: It is well known that the gas bremsstrahlung produced by the electron and positron beams circulating in a storage ring is one of the main photon radiation source for this kind of machines. However, at high luminosity e+e- storage rings, another considerable photon source should be taken into account: the so called radiative Bhabha scattering or single beam-beam bremsstrahlung. According to the luminosity, to the residual gas pressure and to the length of the straight sections where e+e- beams are made to collide, the latter process can become as important as gas bremsstrahlung. The dose-rates due to the radiative Bhabha scattering have been evaluated in the case of the Main Rings of the DAPHNE Project, the e+e- PHI-factory presenctly under construction at the Frascati National Laboratories (Italy). A comparison is made with the espected dose-rates due to gas bremsstrahlung.
DIAPHDIAPH1DIAPH11 Regulates the Wnt/β-catenin Pathway Resulting in Microcephaly and Visual Impairment
Creators: name: Wang, Dayan
Publisher: name: figshare
Year: 2025
Subjects: classificationCode: 320601
subject: Gene and molecular therapy

description: Background: This study was designed to elucidate the pathogenesis of microcephaly syndrome caused by the mutation in double allele mutation of DIAPH1.Methods: We conducted high throughput whole exome sequencing on patient's peripheral blood. Due to Zebrafish lacking human DIAPH1 homolog, we used it to establish the microcephaly model by introducing the human DIAPH1 gene.Results: Exome sequencing found compound heterozygous DIAPH1 mutations causing clinical symptoms. Mutated DIAPH1 zebrafish displayed abnormal eye shape, short body length, axis defects, aberrant neuronal motor axon growth, and reduced behavioral activities. WNT8A, WNT9A, LRP5, and LRP6 genes were upregulated, while AXIN1, AXIN2, and Β-CATENIN were downregulatedConclusions: DIAPH1 mutation (c.1051C>T, p.R351X,922; c.609delA, p.E203E fs*19) might causes microcephaly and visual impairment via activated Wnt/β-catenin pathway.
Study of the High Energy Cosmic Ray Cascades using the Dual Parton Model
Creators: name: G. Battistoni
name: C. Forti
name: J. Ranft
Publisher: name: INFN Open Access Repository
Year: 1995

description: In this paper we describe an application of the two component dual parton model, for the simulation of high energy cosmic ray cascades. The dpmjet interaction model has been tuned to accelerator data for hadron-nucleus and nucleus-nucleus interactions, and its performance in the fragmentation region has been optimized. We make use of this generator inside the HEMAS shower code. Results are presented with particular emphasis on the electromagnetic component and on the high energy muon content of the showers.
Features of spin-charge separation in the equilibrium conductance through finite rings
Creators: name: Rincon, Julian
name: Aligia, A. A.
name: Hallberg, K.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We calculate the conductance through rings with few sites $L$ described by the $t-J$ model, threaded by a magnetic flux $Φ$ and weakly coupled to conducting leads at two arbitrary sites. The model can describe a circular array of quantum dots with large charging energy $U$ in comparison with the nearest-neighbor hopping $t$. We determine analytically the particular values of $Φ$ for which a depression of the transmittance is expected as a consequence of spin-charge separation. We show numerically that the equilibrium conductance at zero temperature is depressed at those particular values of $Φ$ for most systems, in particular at half filling, which might be easier to realize experimentally.
description: 8 pages, 7 figures
$(σ,τ)$-amenability of $C^*$-algebras
Creators: name: Mirzavaziri, M.
name: Moslehian, M. S.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Operator Algebras (math.OA)
subject: Functional Analysis (math.FA)
subject: FOS: Mathematics
subject: Primary 46H25, Secondary 47B47, 46L05

description: Suppose that ${\mathcal A}$ is an algebra, $σ,τ:{\mathcal A}\to{\mathcal A}$ are two linear mappings such that both $σ({\mathcal A})$ and $τ({\mathcal A})$ are subalgebras of ${\mathcal A}$ and ${\mathcal X}$ is a $\big(τ({\mathcal A}),σ({\mathcal A})\big)$-bimodule. A linear mapping $D:{\mathcal A}\to {\mathcal X}$ is called a $(σ,τ)$-derivation if $D(ab)=D(a)\cdotσ(b)+τ(a)\cdot D(b) (a,b\in {\mathcal A})$. A $(σ,τ)$-derivation $D$ is called a $(σ,τ)$-inner derivation if there exists an $x\in{\mathcal X}$ such that $D$ is of the form either $D_x^-(a)=x\cdot σ(a)-τ(a)\cdot x (a\in {\mathcal A})$ or $D_x^ +(a)=x\cdot σ(a)+τ(a)\cdot x (a\in {\mathcal A})$. A Banach algebra ${\mathcal A}$ is called $(σ,τ)$-amenable if every $(σ,τ)$-derivation from ${\mathcal A}$ into a dual Banach $\big(τ({\mathcal A}),σ({\mathcal A})\big)$-bimodule is $(σ,τ)$-inner. Studying some general algebraic aspects of $(σ,τ)$-derivations, we investigate the relation between amenability and $(σ,τ)$-amenability of Banach algebras in the case when $σ, τ$ are homomorphisms. We prove that if $\mathfrak A$ is a $C^*$-algebra and $σ, τ$ are *-homomorphisms with $\ker(σ)=\ker(τ)$, then ${\mathfrak A}$ is $(σ, τ)$-amenable if and only if $σ({\mathfrak A})$ is amenable
description: 9 pages; to appear in Georgian Math. J
Reproducible D/Pd Ratio > 1 and Excess Heat Correlation by 1-ms-Pulse, High-Current Electrolysis
Creators: name: F. Celani
name: A. Spallone
name: P. Tripodi
name: A. Petrocchi
name: D. Di Gioacchino
name: M. Boutet
name: P. Marini
name: V. Di Stefano
name: M. Diociaiuti
name: W. Collis
Publisher: name: INFN Open Access Repository
Year: 1996

description: A high-current (up to 100A), short-pulse (1-ms duration) electrolysis technique is presented that permits high loading (D/Pd up to 1.2) of deuterium in palladium cathodes. Several different cold-worked palladium plates were used as cathodes, and some underwent surface treatments (oxidation or addition of intermetallic compounds). The surface-treated plates showed atypical deuterium absorption dynamics, and the D/Pd loading ratio exceeded 1. Moreover, during initial loading, these cathodes showed anomalous excess heat (up to 80%) far greater than the absorption enthalpy. The pure palladium surface plates did not show this effect.
title: Ð£ÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð¿Ð¾ Ð¸Ð½ÑÐµÐ³ÑÐ°Ð»Ð°Ð¼
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐ°Ð»Ð°Ð½Ð´ÑÐº, ÐÐ½Ð½Ð°
name: ÐÑÐµÐ¾Ð±ÑÐ°Ð¶ÐµÐ½ÑÐºÐ¸Ð¹, Ð¡ÐµÑÐ³ÐµÐ¹
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: 2022
Subjects: ÐÐ½ÑÐµÐ³ÑÐ°Ð»Ñ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð½ÑÐµ
ÐÐ½ÑÐµÐ³ÑÐ°Ð»Ñ Ð½ÐµÑÐ¾Ð±ÑÑÐ²ÐµÐ½Ð½ÑÐµ
ÐÑÐµÐ´ÐµÐ»Ñ (Ð¼Ð°Ñ.)

description: ÐÐ°Ð½Ð½Ð¾Ðµ ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ ÑÐ¾Ð´ÐµÑÐ¶Ð¸Ñ ÑÐºÐ°Ð·Ð°Ð½Ð¸Ñ Ð¸ Ð¿ÑÐ¸Ð¼ÐµÑ Ðº Ð¸Ð½Ð´Ð¸Ð²Ð¸Ð´ÑÐ°Ð»ÑÐ½Ð¾Ð¼Ñ ÑÐ°ÑÑÐµÑÐ½Ð¾Ð¼Ñ Ð·Ð°Ð´Ð°Ð½Ð¸Ñ Ð¿Ð¾ Ð¼Ð°ÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ð¼Ñ Ð°Ð½Ð°Ð»Ð¸Ð·Ñ Ð¿Ð¾ ÑÐµÐ¼Ðµ Â«Ð¸Ð½ÑÐµÐ³ÑÐ°Ð»Â» Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð¿ÐµÑÐ²Ð¾Ð³Ð¾ ÐºÑÑÑÐ° Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ð¹ Â«Ð¿ÑÐ¸ÐºÐ»Ð°Ð´Ð½Ð°Ñ Ð¼Ð°ÑÐµÐ¼Ð°ÑÐ¸ÐºÐ° Ð¸ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸ÐºÐ°Â», Â«Ð¼ÐµÑÐ°Ð½Ð¸ÐºÐ° Ð¸ Ð¼Ð°ÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ðµ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸ÐµÂ», Â«ÑÐ¸Ð·Ð¸ÐºÐ°Â».
Ð£ÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÐµÑ Ð¤ÐÐÐ¡ ÐÐ Ð¿Ð¾ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ðµ Â«ÐÐ°ÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ¸Ð¹ Ð°Ð½Ð°Ð»Ð¸Ð·Â» Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸ÑÐ¼ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ 01.03.02 Â«ÐÑÐ¸ÐºÐ»Ð°Ð´Ð½Ð°Ñ Ð¼Ð°ÑÐµÐ¼Ð°ÑÐ¸ÐºÐ° Ð¸ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸ÐºÐ°Â», 01.03.03 Â«ÐÐµÑÐ°Ð½Ð¸ÐºÐ° Ð¸ Ð¼Ð°ÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ðµ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸ÐµÂ», 03.03.02 Â«Ð¤Ð¸Ð·Ð¸ÐºÐ°Â». Ð Ð°Ð±Ð¾ÑÐ° Ð¼Ð¾Ð¶ÐµÑ Ð±ÑÑÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð° Ð¿ÑÐ¸ Ð¸Ð·ÑÑÐµÐ½Ð¸Ð¸ ÑÐ»ÐµÐ´ÑÑÑÐ¸Ñ ÑÐ°Ð·Ð´ÐµÐ»Ð¾Ð² Ð²ÑÑÑÐµÐ¹ Ð¼Ð°ÑÐµÐ¼Ð°ÑÐ¸ÐºÐ¸: Ð½ÐµÐ¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð½ÑÐ¹ Ð¸Ð½ÑÐµÐ³ÑÐ°Ð», Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð½ÑÐ¹ Ð¸Ð½ÑÐµÐ³ÑÐ°Ð», Ð½ÐµÑÐ¾Ð±ÑÑÐ²ÐµÐ½Ð½ÑÐ¹ Ð¸Ð½ÑÐµÐ³ÑÐ°Ð». ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐ°ÐµÑÑÑ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð¤Ð¸Ð·Ð¸ÐºÐ¾-Ð¼ÐµÑÐ°Ð½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¸Ð½ÑÑÐ¸ÑÑÑÐ°.
title: Ð Ð°ÑÑÐµÑ Ð¸ Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¸Ðµ ÑÐµÑ Ð½Ð¸ÑÐµÑÐºÐ¸Ñ ÑÑÐµÐ±Ð¾Ð²Ð°Ð½Ð¸Ð¹ Ð½Ð° Ð´ÐµÑÐ°Ð»Ð¸ Ð¼Ð°ÑÐ¸Ð½. Ð§. 1
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐ½ÑÑÐ¸Ð½, ÐÐ¸ÐºÑÐ¾Ñ
Publisher: name: [Ð¡ÐÐ±ÐÐ¢Ð£]
Year: 1993
Subjects: ÐÐµÑÐ°Ð»Ð¸ Ð¼Ð°ÑÐ¸Ð½
ÐÐ¾Ð¿ÑÑÐºÐ¸ Ð¸ Ð¿Ð¾ÑÐ°Ð´ÐºÐ¸

description: ÐÐ·Ð»Ð¾Ð¶ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð¿Ð¾Ð´ÑÐ¾Ð´Ñ ÑÐ°ÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð²ÑÐ±Ð¾ÑÐ° Ð´Ð¾Ð¿ÑÑÐºÐ¾Ð² Ð¸ Ð¿Ð¾ÑÐ°Ð´Ð¾Ðº; ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð²Ð¾Ð¿ÑÐ¾ÑÑ Ð¿Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ñ Ð¸ ÑÐ°ÑÑÐµÑÐ° ÑÐ°Ð·Ð¼ÐµÑÐ½ÑÑ ÑÐµÐ¿ÐµÐ¹; Ð¸Ð¼ÐµÑÑÑÑ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¿Ð¾ Ð²ÑÐ±Ð¾ÑÑ ÑÐ¾ÑÐ½Ð¾ÑÑÐ½ÑÑ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÐ¾Ð² ÑÐµÑÐ²ÑÐºÐ¾Ð² Ð¸ ÑÐµÑÐ²ÑÑÐ½ÑÑ ÐºÐ¾Ð»ÐµÑ, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ, Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼ÑÐµ Ð´Ð»Ñ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ ÑÐµÑÑÐµÐ¶ÐµÐ¹ ÑÑÐ¸Ñ Ð´ÐµÑÐ°Ð»ÐµÐ¹. Ð¡Ð¾Ð´ÐµÑÐ¶Ð¸Ñ Ð¿ÑÐ¸Ð¼ÐµÑÑ Ð²ÑÐ±Ð¾ÑÐ° Ð¸ ÑÐ°ÑÑÐµÑÐ° Ð¿Ð¾ÑÐ°Ð´Ð¾Ðº, ÑÐ°ÑÑÐµÑÐ° ÑÐ°Ð·Ð¼ÐµÑÐ½ÑÑ ÑÐµÐ¿ÐµÐ¹, Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ ÑÐµÑÑÐµÐ¶ÐµÐ¹ ÑÐµÑÐ²ÑÐºÐ° Ð¸ ÑÐµÑÐ²ÑÑÐ½Ð¾Ð³Ð¾ ÐºÐ¾Ð»ÐµÑÐ°, Ð° ÑÐ°ÐºÐ¶Ðµ Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼ÑÐµ Ð½Ð¾ÑÐ¼Ð°ÑÐ¸Ð²Ð½ÑÐµ Ð´Ð°Ð½Ð½ÑÐµ.
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 ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ°.
Additional file 2 of Horizontal transfer of a plasmid possessing mcr-1 marked with a single nucleotide mutation between Escherichia coli isolates from community residents
Creators: name: Yamamoto, Yoshimasa
name: Higashi, Ayano
name: Ikawa, Kanoko
name: Hoang, Hoa Thi Thanh
name: Yamaguchi, Takahiro
name: Kawahara, Ryuji
name: Noguchi, Hideki
name: Nguyen, Thang Nam
name: Khong, Diep Thi
name: Tran, Hoa Thi
Publisher: name: figshare
Year: 2022
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 2. Additional data of the complete genome of colistin-resistant E. coli isolates.
title: Ð¡Ð¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¿ÑÐ¾Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ñ Ð±ÑÐµÐ½Ð´Ð° Ð² ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½ÑÑ ÑÐµÑÑÑ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ Ð¸Ð½ÑÐµÑÐ½ÐµÑ-Ð¼Ð°Ð³Ð°Ð·Ð¸Ð½Ð° "Wow!bikini")
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ÐµÐ¿Ð°Ð½Ð¾Ð²Ð°, ÐÐ½ÑÐ¾Ð½Ð¸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Ð½ÑÐµÑÐ½ÐµÑ
Ð±ÑÐµÐ½Ð´Ñ
ÑÐµÐºÐ»Ð°Ð¼Ð½ÑÐµ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ñ
Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð¾Ð²ÑÐµ ÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð¸
ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½ÑÐµ ÑÐµÑÐ¸

description: Ð Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ¾Ð¹ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ð¸ Ð½Ð° ÑÐµÐ¼Ñ: Â«Ð¡Ð¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¿ÑÐ¾Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ñ Ð±ÑÐµÐ½Ð´Ð° Ð² ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½ÑÑ ÑÐµÑÑÑ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ Ð¸Ð½ÑÐµÑÐ½ÐµÑ-Ð¼Ð°Ð³Ð°Ð·Ð¸Ð½Ð° Â«Wow!bikiniÂ»)Â» Ð±ÑÐ»Ð¾ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¾ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð²ÑÑÐ²Ð»ÐµÐ½Ð¸Ñ Ð¿Ð¾ÑÑÐµÐ±Ð¸ÑÐµÐ»ÑÑÐºÐ¸Ñ Ð¿ÑÐµÐ´Ð¿Ð¾ÑÑÐµÐ½Ð¸Ð¹ Ð¿ÑÐ¸ Ð²ÑÐ±Ð¾ÑÐµ Ð±ÑÐµÐ½Ð´Ð° ÐºÑÐ¿Ð°Ð»ÑÐ½Ð¸ÐºÐ¾Ð² Ð¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ¼Ð¸ ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½ÑÑ ÑÐµÑÐµÐ¹. Ð ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÑÐ°ÑÑÐ¸ Ð±ÑÐ»Ð¸ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÑ Ð¿ÑÐ¾Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ñ Ð±ÑÐµÐ½Ð´Ð° Ð² ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½Ð¾Ð¹ ÐºÐ¾Ð¼Ð¼ÐµÑÑÐ¸Ð¸, Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÐ¹ Ð¾Ð¿ÑÑ Ð¿ÑÐ¾Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ñ Ð±ÑÐµÐ½Ð´Ð° Ð² ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½ÑÑ ÑÐµÑÑÑ, Ð¿ÑÐ°Ð²Ð¾Ð²Ð¾Ðµ ÑÐµÐ³ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¸Ð½ÑÐµÑÐ½ÐµÑ-ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ð¸. ÐÐ¾ Ð²ÑÐ¾ÑÐ¾Ð¹ Ð³Ð»Ð°Ð²Ðµ Ð±ÑÐ» Ð¿ÑÐ¾Ð²ÐµÐ´ÑÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð¾Ð²Ð¾Ð¹-ÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¼Ð°Ð³Ð°Ð·Ð¸Ð½Ð° Ð¸ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÑÐ½ÐºÐ° ÐºÑÐ¿Ð°Ð»ÑÐ½Ð¸ÐºÐ¾Ð². ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½Ñ SWOT Ð¸ PEST Ð°Ð½Ð°Ð»Ð¸Ð·Ñ. ÐÑÐ»Ð¸ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¿ÑÐ¾Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ñ Ð´ÑÑÐ³Ð¸Ñ Ð¼Ð°Ð³Ð°Ð·Ð¸Ð½Ð¾Ð². Ð ÑÐ¾Ð´Ðµ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ½Ð¾Ð¹ ÑÑÐµÐ´Ñ Ð±ÑÐ»Ð¾ Ð²ÑÑÐ²Ð»ÐµÐ½Ð¾, ÑÑÐ¾ Ñ Ð¸Ð½ÑÐµÑÐ½ÐµÑ-Ð¼Ð°Ð³Ð°Ð·Ð¸Ð½Ð° Ð¾ÑÑÑÑÑÑÐ²ÑÐµÑ SMM Ð¿ÑÐ¾Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ðµ. Ð ÑÑÐµÑÑÐµÐ¹ Ð³Ð»Ð°Ð²Ðµ Ð±ÑÐ»Ð° Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð° Ð¾ÑÐµÐ½ÐºÐ° ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÑÐµÐºÐ»Ð°Ð¼Ð½ÑÑ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹ Ð¸Ð½ÑÐµÑÐ½ÐµÑ-Ð¼Ð°Ð³Ð°Ð·Ð¸Ð½Ð° Â«Wow!bikiniÂ». ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ð¸ Ð¿Ð¾Ð»ÑÑÐµÐ½Ð½ÑÑ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¾Ð² Ð°Ð½ÐºÐµÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð±ÑÐ» ÑÐ¾Ð·Ð´Ð°Ð½ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼ Ð¿ÑÐ¾Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ñ Ð±ÑÐµÐ½Ð´Ð° Â«Wow!bikiniÂ» Ð² ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½ÑÑ ÑÐµÑÑÑ Â«ÐÐºÐ¾Ð½ÑÐ°ÐºÑÐµÂ» Ð¸ Â«InstagramÂ».
The metabolism of radioactive glutamic acid in normal and epileptic cat brain
Creators: name: Steiner, K. David
Publisher: name: University of British Columbia
Year: 2011

description: The indirect in vivo inhibition of the enzyme glutamic acid decarboxylase (GAD) by either vitamin B-6 deficiency or the administration of vitamin B-6 antimetabolites decreases the conversion of glutamic acid to gamma aminobutyric acid (GABA) in brain. This decrease is a concomitant to the occurrence of seizures resembling grand mal. The in vivo reactivation of GAD by vitamin B-6 administration and/or by the topical application of GABA to the brain surface reduces the intensity of the convulsions. Because of this, it has been suggested that a decrease in the conversion of glutamic acid to GABA in brain may be a factor in the precipitation and maintenance of epileptic seizures. In order to investigate this suggestion, the in vivo metabolism of C-14 labelled glutamic acid to GABA and other amino acids was quantitatively determined in various brain areas of several normal cats; a cat with a epileptogenic lesion in the left motor cortex produced by alumina cream; and one cat in status epilepticus. Throughout most non-epileptogenic brain areas there were similar rates of conversion of glutamic acid to GABA, aspartic acid and glutamine. Notable exceptions to this consistency were found repeatedly in the quadri-geminal plate, thalamus and putamen-globus pallidus where there was a higher conversion of glutamic acid to GABA. No apparent consistency in the degree of conversion of glutamic acid to the other amino acids could be discerned throughout the brain of the cat in status epilepticus. In the epileptogenic lesion there was a decrease in the conversion of glutamic acid to GABA, which is compatible with the suggestion that a reduction in GABA levels increases the degree of brain excitability.
Operation of the Gravitational Wave Detector NAUTILUS
Creators: name: P. Astone
name: M. Bassan P. Bonifazi
name: P. Carelli
name: E. Coccia
name: V. Fafone
name: S. Frasca
name: A. Marini
name: S.M. Merkowitz
name: Y. Minenkov
name: I. Modena
name: G. Modestino
name: A. Moleti
name: G.V. Pallottino
name: M.A. Papa
name: G. Pizzella
name: F. Ronga
name: R. Terenzi
name: M. Visco
name: L. Votano
Publisher: name: INFN Open Access Repository
Year: 1998

description: The ultracryogenic resonant-mass gravitational wave (GW) detector NAUTILUS of the Rome group is in continuos operation at the Frascati INFN National Laboratories since December 1995. The detector is cooled at about 0.1 K. The measured spectral amplitude sensitivity is h≅6*10^-22 Hz^-1/2, with a bandwidth of about 1 Hz, and the best pulse sensitivity is of the order of h≅4*10^-19. We describe the detector performances, the search for monochromatic wave and the first experiment of cross-correlation between the data obtained with NAUTILUS and Explorer, the detector of the Rome group located at CERN.
Disentangling the system geometry of the Supergiant Fast X-ray Transient IGR J11215-5952 with Swift
Creators: name: Romano, P.
name: Sidoli, L.
name: Cusumano, G.
name: Vercellone, S.
name: Mangano, V.
name: Krimm, H. A.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: IGR J11215-5952 is a hard X-ray transient discovered in 2005 April by INTEGRAL and a member of the new class of HMXB, the Supergiant Fast X-ray Transients (SFXTs). While INTEGRAL and RXTE observations have shown that the outbursts occur with a periodicity of ~330 days, Swift data have recently demonstrated that the true outburst period is ~165 days. IGR J11215-5952 is the first discovered SFXT displaying periodic outbursts, which are possibly related to the orbital period. We performed a Guest Investigator observation with Swift that lasted 20ks and several follow-up Target of Opportunity (ToO) observations, for a total of ~32ks, during the expected "apastron" passage (defined assuming an orbital period of ~330 days), between 2008 June 16 and July 4. The characteristics of this "apastron'' outburst are quite similar to those previously observed during the "periastron'' outburst of 2007 February 9. The mean spectrum of the bright peaks can be fit with an absorbed power law model with a photon index of 1 and an absorbing column of 1E22 cm^-2. This outburst reached luminosities of ~1E36 erg/s (1-10keV), comparable with the ones measured in 2007. The light curve can be modelled with the parameters obtained by Sidoli et al. (2007) for the 2007 February 9 outburst, although some differences can be observed in its shape. The properties of the rise to this new outburst and the comparison with the previous outbursts allow us to suggest that the true orbital period of IGR J11215-5952 is very likely 164.6 days, and that the orbit is eccentric, with the different outbursts produced at the periastron passage, when the neutron star crosses the inclined equatorial wind from the supergiant companion. Based on a ToO observation performed on 2008 March 25-27, we can exclude that the period is 165/2 days. [Abridged]
description: 7 pages, accepted for publication by the Astrophysical Journal. Abstract abridged
The Single Reflection Regime of X-Rays Travelling into a Monocapillary
Creators: name: S.B. Dabagov
name: A. Marcelli
Publisher: name: INFN Open Access Repository
Year: 1999

description: In this manuscript an analysis of the transmission of x-rays through a single monocapillary under the single reflection regime is presented and discussed. Because ray tracing does not allow to explain the experimental data, a first qualitative interpretation of the observed behavior is given in the framework of the wave theory.
title: ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ°ÐºÑÐ¾ÑÐ¾Ð², Ð²Ð»Ð¸ÑÑÑÐ¸Ñ Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ðµ Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð¾Ð²ÑÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ð¹ Ð½Ð° B2B ÑÑÐ½ÐºÐµ
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: Ð¡Ð¾Ð»ÑÐ°Ð½Ð°Ð±Ð°Ð´Ð¸ Ð¤Ð°ÑÑ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: 2017
Subjects: ÑÑÐ½Ð¾Ðº
Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð¾Ð²ÑÐµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ
ÐºÐ°ÑÐµÑÑÐ²ÐµÐ½Ð½ÑÐµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ

description: ÐÑÐ½Ð¾Ð²Ð½Ð¾Ð¹ ÑÐµÐ»ÑÑ Ð´Ð°Ð½Ð½Ð¾Ð³Ð¾ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð±ÑÐ»Ð¾ Ð²ÑÑÑÐ½Ð¸ÑÑ Ð¿ÑÐ¸ÑÐ¸Ð½Ñ, Ð¿Ð¾ ÐºÐ¾ÑÐ¾ÑÑÐ¼ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ Ð² Ð¿Ð¾ÑÑÑÐ¾Ð²ÐµÑÑÐºÐ¸Ñ ÑÑÑÐ°Ð½Ð°Ñ Ð½Ð° ÑÑÐ½ÐºÐµ Ð2Ð Ð½Ðµ Ð¿ÑÐ¾Ð²Ð¾Ð´ÑÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ, Ð¿ÐµÑÐµÐ´ Ð¿ÑÐ¸Ð½ÑÑÐ¸ÐµÐ¼ ÑÐµÑÐµÐ½Ð¸Ð¹. ÐÐ»Ñ ÑÑÐ¾Ð³Ð¾, ÐºÐ°Ðº Ð¿ÑÐ¸Ð¼ÐµÑ, Ð±ÑÐ»Ð¾ ÑÑÐ°ÑÐµÐ»ÑÐ½Ð¾ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¾ Ð¿Ð¾Ð´ÑÐ¾Ð±Ð½Ð¾Ðµ Ð¸Ð½ÑÐµÑÐ²ÑÑ. ÐÐ»Ñ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ ÑÑÐµÐ±Ð¾Ð²Ð°Ð½Ð¸Ð¹ ÑÑÐ¾Ð³Ð¾ ÐºÐ°ÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ, Ð¸Ð½ÑÐµÑÐ²ÑÑ Ð±ÑÐ»Ð¸ Ð¿ÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ñ, Ð¸ Ð¿ÑÐ¸ÑÐ¸Ð½Ñ, Ð½Ðµ Ð¿Ð¾Ð·Ð²Ð¾Ð»ÑÑÑÐ¸Ðµ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸ÑÐ¼ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ðµ Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð¾Ð²ÑÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ð¹ Ð½Ð° ÑÑÐ½ÐºÐµ Ð2Ð, Ð¾ÐºÐ°Ð·Ð°Ð»Ð¸ÑÑ Ð² ÑÐ»ÐµÐ´ÑÑÑÐµÐ¼: Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð¾Ð²ÑÐµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ - ÑÑÐ¾ Ð´Ð¾ÑÐ¾Ð³Ð¾, Ð¿ÑÐ¾ÑÐµ Ð¿Ð¾Ð»Ð¾Ð¶Ð¸ÑÑÑÑ Ð½Ð° ÑÐµÑÑ Ð¸Ð½ÑÐµÑÐ½ÐµÑ Ð¸ ÑÑÑÐ»ÐºÐ¸ Ð¿ÑÐ¾ÑÐµ, ÑÐµÐ¼ Ð¿ÑÐ¾Ð²Ð¾Ð´Ð¸ÑÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ; Ð¸Ð·ÑÑÐµÐ½Ð¸Ðµ ÑÑÐ½ÐºÐ° Ð²ÑÐµÐ¼ÑÐ·Ð°ÑÑÐ°ÑÐ½Ð¾; Ð½ÐµÑÑÐ°Ð±Ð¸Ð»ÑÐ½Ð¾ÑÑÑ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ¸, ÐºÑÐ°ÑÐºÐ¾ÑÑÐ¾ÑÐ½Ð°Ñ Ð¾ÑÐ¸ÐµÐ½ÑÐ°ÑÐ¸Ñ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¹; Ð½ÐµÐ²Ð¸Ð´Ð¸Ð¼Ð¾ÑÑÑ ÑÑÐ½ÐºÐ° Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°ÑÐµÐ»ÑÑÐºÐ¸Ñ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¹; Ð´ÐµÑÐ¸ÑÐ¸Ñ ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸ÑÑÐ¾Ð² Ð¿Ð¾ Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ñ Ð² Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð¾Ð²ÑÑ Ð¾ÑÐ´ÐµÐ»Ð°Ñ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¹; Ð½ÐµÑÑÐ°Ð±Ð¸Ð»ÑÐ½Ð¾ÑÑÑ Ð½Ð° ÑÑÐ½ÐºÐµ ÑÐµÐ»ÐµÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½ÑÑ ÑÑÐ»ÑÐ³.