cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Echinostelium brooksii K. D. Whitney
Creators: name: Kluša, Julita
Publisher: name: Zenodo
Year: 2023
Subjects: Biodiversity
Taxonomy
Protozoa
Mycetozoa
Myxomycetes
Echinosteliales
Echinosteliaceae
Echinostelium
Echinostelium brooksii

description: ^ Echinostelium brooksii K.D. Whitney,
Brūksa adatīte
- leg. G. Adamonytė, 2005, det. G. Adamonytė, 2006.
description: Published as part of Kluša, Julita, 2023, Complete Checklist Of Myxomycetes In Latvia, pp. 127-151 in Acta Biologica Universitatis Daugavpiliensis 23 (2) on pages 127-151, DOI: 10.59893/abud.23(2).002, http://zenodo.org/record/12650118
Diamagnetic Length-Scales of Condon Domain Phase in Lifschitz-Kosevich-Shoenberg Approximation
Creators: name: Logoboy, Nathan
name: Joss, Walter
Publisher: name: arXiv
Year: 2009
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: Equilibrium properties of non-uniform diamagnetic phase in normal metals (Condon domains) are studied theoretically in the framework of Lifschitz-Kosevich-Shoenberg (LKS) approximation. It is found that characteristic diamagnetic lengths of the phase, e. g. a period of domain structure and width of interface boundary between domains, as well as specific surface energy of domain wall, are strongly affected by electron correlations and depend on temperature, magnetic field and purity of the sample. The developed theory is in a good agreement with existent experiment data.
description: 7 pages, 6 figures
On the phenomenology of a two-Higgs-doublet model with maximal CP symmetry at the LHC, II: radiative effects
Creators: name: Maniatis, M.
name: Nachtmann, O.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The processes proton + antiproton -> gamma + heavy-flavour jet(s) + X and proton + proton -> gamma + heavy-flavour jet(s) + X are studied in the framework of a special two-Higgs-doublet model, the MCPM. As distinguishing feature of this model we find that radiative Higgs-boson production and decay lead to heavy flavour c jets but no b jets in the above processes. Thus, the prediction is that b jets should be given by the normal QCD processes whereas for c jets an excess over the QCD expectation should occur. We present results both for Tevatron and LHC energies.
description: 13 pages, 9 figures
Nonequilibrium Dynamics of Scalar Fields in a Thermal Bath
Creators: name: Anisimov, A.
name: Buchmueller, W.
name: Drewes, M.
name: Mendizabal, S.
Publisher: name: arXiv
Year: 2008
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We study the approach to equilibrium for a scalar field which is coupled to a large thermal bath. Our analysis of the initial value problem is based on Kadanoff-Baym equations which are shown to be equivalent to a stochastic Langevin equation. The interaction with the thermal bath generates a temperature-dependent spectral density, either through decay and inverse decay processes or via Landau damping. In equilibrium, energy density and pressure are determined by the Bose-Einstein distribution function evaluated at a complex quasi-particle pole. The time evolution of the statistical propagator is compared with solutions of the Boltzmann equations for particles as well as quasi-particles. The dependence on initial conditions and the range of validity of the Boltzmann approximation are determined.
description: 37 pages, 14 figures; references added
VEÍCULO 100% ELÉTRICO BRASILEIRO PARA TRANSIÇÃO ENERGÉTICA – OUTUBRO/2021
Creators: name: Junior, Milton Francisco dos Santos
name: Jr, Eloy Fassy Casagrande
Publisher: name: figshare
Year: 2022
Subjects: Environmental Science

description: The world is experiencing a moment of transition, moving from the use of internal combustion vehicles for all-electric ones. However, there are several issues that affect car manufacturers, electric power companies, consumers, and users of all-electric vehicles, impacting their popularization, such as: a) will there be electricity to power all electric vehicles? b) how to ensure that electric vehicles will be recharged only with renewable energies? (c) can electric vehicles, considering their capacity to store electricity, encourage the acceleration of the energy transition to maximize the use of renewable sources of electricity? The article seeks to clarify all these points and to record the understanding that electric vehicles are an important tool for the promotion of renewable and intermittent sources of electricity. It concludes that there are already business models involving the commercial exploitation of electric vehicles understood as appropriate in all aspects analyzed, presenting an example.
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð´Ð¸Ð·Ð°Ð¹Ð½-Ð¿ÑÐ¾ÐµÐºÑÐ° Ð¸Ð½ÑÐµÑÑÐµÑÐ° Ð·Ð°Ð³Ð¾ÑÐ¾Ð´Ð½Ð¾Ð³Ð¾ Ð´Ð¾Ð¼Ð°
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐµÐ³ÐµÐ½ÑÐºÐ°Ñ, 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: 2017
Subjects: Ð¸Ð½ÑÐµÑÑÐµÑ
Ð´Ð¸Ð·Ð°Ð¹Ð½-Ð¿ÑÐ¾ÐµÐºÑ
ÐºÐ¾ÑÑÐµÐ´Ð¶

description: Ð¦ÐµÐ»ÑÑ Ð´Ð°Ð½Ð½Ð¾Ð¹ Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ ÑÐ¾ÑÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð´Ð¸Ð·Ð°Ð¹Ð½-Ð¿ÑÐ¾ÐµÐºÑÐ° Ð·Ð°Ð³Ð¾ÑÐ¾Ð´Ð½Ð¾Ð³Ð¾ Ð´Ð¾Ð¼Ð° Ð¾Ð±ÑÐµÐ¹ Ð¿Ð»Ð¾ÑÐ°Ð´ÑÑ 325 Ð¼2, Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ñ Ð¾Ð±ÑÐµÐ¼Ð½Ð¾-Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð¾ÑÐ½ÑÑ Ð¸ ÑÐ²ÐµÑÐ¾Ð²ÑÑ ÑÐµÑÐµÐ½Ð¸Ð¹ Ð´Ð¾Ð¼Ð°, Ð¿Ð¾Ð´Ð±Ð¾Ñ Ð¸ ÑÑÐ³Ð¾Ð½Ð¾Ð¼Ð¸ÑÐ½Ð°Ñ ÑÐ°ÑÑÑÐ°Ð½Ð¾Ð²ÐºÐ° ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ¾Ð² Ð¼ÐµÐ±ÐµÐ»Ð¸, Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð´Ð»Ñ Ð¿Ð¾Ð»ÑÑÐµÐ½Ð¸Ñ ÑÑÐ¸Ð»ÑÐ½Ð¾Ð³Ð¾, Ð³Ð°ÑÐ¼Ð¾Ð½Ð¸ÑÐ½Ð¾Ð³Ð¾ Ð¸ ÐºÐ¾Ð¼ÑÐ¾ÑÑÐ½Ð¾Ð³Ð¾ Ð´Ð»Ñ Ð¶Ð¸Ð·Ð½Ð¸ Ð¸Ð½ÑÐµÑÑÐµÑÐ°. Ð ÑÐ¾Ð´Ðµ ÑÐ°Ð±Ð¾ÑÑ Ð½Ð°Ð´ Ð¿ÑÐ¾ÐµÐºÑÐ¾Ð¼ Ð±ÑÐ» Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½ Ð²Ð°ÑÐ¸Ð°Ð½Ñ Ð¿ÐµÑÐµÐ¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²ÐºÐ¸ Ð·Ð°Ð³Ð¾ÑÐ¾Ð´Ð½Ð¾Ð³Ð¾ Ð´Ð¾Ð¼Ð° Ð² ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²Ð¸Ð¸ Ñ Ð¢ÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¼ Ð·Ð°Ð´Ð°Ð½Ð¸ÐµÐ¼. Ð ÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¾Ð¼ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ ÑÑÐ°Ð»Ð¾ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ðµ Ð¿Ð¾Ð»Ð½Ð¾ÑÐµÐ½Ð½Ð¾Ð³Ð¾ Ð´Ð¸Ð·Ð°Ð¹Ð½-Ð¿ÑÐ¾ÐµÐºÑÐ°, Ð²ÐºÐ»ÑÑÐ°ÑÑÐµÐ³Ð¾ Ð² ÑÐµÐ±Ñ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÑ Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð¾ÑÐ½ÑÑ ÑÐµÑÐµÐ½Ð¸Ð¹ Ð¸ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ Ð¿ÑÐ¾ÐµÐºÑÐ° Ð¸Ð½ÑÐµÑÑÐµÑÐ°, Ð¾ÑÐ²ÐµÑÐ°ÑÑÐµÐ³Ð¾ Ð·Ð°Ð¿ÑÐ¾ÑÐ°Ð¼ Ð·Ð°ÐºÐ°Ð·ÑÐ¸ÐºÐ°. ÐÑÐ¾ÐµÐºÑ Ð²ÐºÐ»ÑÑÐ°ÐµÑ Ð² ÑÐµÐ±Ñ: Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²Ð»ÐµÐ½Ð½ÑÐ¹ Ð¿Ð°ÐºÐµÑ Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼ÑÑ ÑÐµÑÑÐµÐ¶ÐµÐ¹, Ð¾ÑÐ¾ÑÐ¼Ð»ÐµÐ½Ð½ÑÐ¹ Ð² ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²Ð¸Ð¸ ÐÐ¡ÐÐ Ð¸ Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ð¼Ð¸ ÑÐºÐ°Ð·Ð°Ð½Ð¸ÑÐ¼Ð¸; 3d Ð¼Ð¾Ð´ÐµÐ»Ñ ÐºÐ¾Ð¼Ð½Ð°Ñ Ð·Ð°Ð³Ð¾ÑÐ¾Ð´Ð½Ð¾Ð³Ð¾ Ð´Ð¾Ð¼Ð°; Ð²Ð¸Ð·ÑÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ ÑÑÐ´Ð° Ð¿Ð¾Ð¼ÐµÑÐµÐ½Ð¸Ð¹, Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼Ð°Ñ Ð´Ð»Ñ Ð¿Ð¾Ð»Ð½Ð¾Ð³Ð¾ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÐºÐ¾Ð½ÑÐµÐ¿ÑÐ¸Ð¸ Ð´Ð°Ð½Ð½Ð¾Ð³Ð¾ Ð´Ð¸Ð·Ð°Ð¹Ð½-ÑÐµÑÐµÐ½Ð¸Ñ.
Stinging the Predators: A collection of papers that should never have been published
Creators: name: Faulkes, Zen
Publisher: name: figshare
Year: 2020
Subjects: Science Policy

description: This ebook collects academic papers and conference abstracts that were meant to be so terrible that nobody in their right mind would publish them. All were submitted to journals and conferences to expose weak or non-existent peer review and other exploitative practices. Each paper has a brief introduction. Short essays round out the collection.

330 pages (version 16.0).

Version 1.0 released 26 July 2017.
Version 2.0 released 28 July 2017 (two new entries).
Version 3.0 released 31 July 2017 (two new entries).
Version 3.1 released 7 August 2017 (error corrected).
Version 4.0 released 16 February 2018 (one new entry).
Version 4.1 released 16 February 2018 (journal PDF replaced copied text).Version 5.0 released 4 July 2018 (one new entry).Version 6.0 released 26 July 2018 (one new entry).Version 6.1 released 28 July 2018 (journal PDF replaced copied text).Version 7.0 released 29 September 2018 (one new entry).Version 8.0 released 3 October 2018 (one new entry with featuring three new papers).Version 8.1 released 4 October 2018 (one new paper added associated with v 8.0 entry; PDF bookmarks fixed).Version 8.2 released 7 October 2018 (expanded introduction associated with v 8.0 entry).Version 8.3 released 30 October 2018 (expanded introduction associated with v 8.0 entry; minor addition to earlier entries).Version 9.0 released 16 March 2019 (new entry).Version 10.0 released 7 April 2019 (new entry; minor update to previous entry).Version 11.0 released 31 March 2020 (two new entries; minor update to previous entry).Version 12.0 released 4 April 2020 (new entry; various minor updates to earlier entries, including updated link, corrected date, corrected name, etc.)Version 12.1 released 5 April 2020 (excerpts from hoaxed paper replaced with full PDF)Version 13.0 released 1 June 2020 (two new entries)Version 14.0 released 15 August 2020 (one new entry)Version 14.1 released 15 August 2020 (expanded newest entry)Version 15.0 released 16 August 2020 (one new entry)Version 16.0 released 26 December 2020 (one new entry)
Austenite grain growth studies in line pipe steels
Creators: name: Swan, Joshua
Publisher: name: University of British Columbia
Year: 2024

description: The oil and natural gas industry, as well as newly developing technologies such as carbon sequestration and hydrogen transport rely on pipelines for transportation of their products. As the demand for safety and efficiency of pipelines increase, the properties of the line pipe steel from which they are made must improve. To do this, line pipe steel is manufactured using a thermomechanically controlled process (TMCP) which combines specific alloying elements with processing conditions to produce an engineered microstructure. Within the TMCP, the austenite grain size and structure are important factors in determining the final microstructure and thus mechanical properties. The purpose of this work is to investigate the austenite grain growth evolution during the thermal treatment in the reheat furnace and compare austenite grain growth characteristics in as-cast slab and hot-rolled material. Two different line pipe steels with varying amounts of manganese and niobium were studied. Thermal conditions were simulated with a Gleeble 3500 thermomechanical simulator while the austenite grain size was measured in-situ with a laser ultrasonics for metallurgy (LUMet) system. The reheat furnace treatment was simulated with a slow heating rate of 5°C/min to 1200°C followed by a 2hr hold. Grain growth comparison experiments consisted of a high heating rate of 50°C/s to one of three holding temperatures of 1100°C, 1200°C and 1300°C. Results of the LUMet measurements were validated by reconstructions of prior-austenite microstructures using electron backscatter diffraction (EBSD) data. LUMet measurements and reconstructions of austenite grain structures for the as-cast slab material undergoing the reheat furnace simulation show a bimodal grain size distribution with a few extremely large grains and many small grains clustered together. A similar but less extreme version of this microstructure was found in slab material undergoing grain growth comparison experiments. This bimodal microstructure was not observed in the hot rolled material. Current hypothesis is that solute segregation of Niobium and Titanium into the inter-dendritic zones is occurring during solidification. These alloying elements promote the formation of (Ti,Nb)(C,N) precipitates that inhibit grain growth and when concentrated into specific areas, allow for a bimodal microstructure to occur.
A Flexible Quasioptical Input System for a Submillimeter Muliobject Spectrometer
Creators: name: Goldsmith, Paul F.
name: Seiffert, Michael
Publisher: name: arXiv
Year: 2009
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: We present a conceptual design for the input optical system for a multi-object spectrometer operating at submillimeter wavelengths. The Mirror MOS is based on a sequence of mirrors that enables low-loss propagation of beams from selected positions distributed throughout the focal plane to the spectroscopic receiver inputs. This approach should be useful for observations of sources which have a relatively low density on the sky, for which it is inefficient to use a traditional array receiver with uniformly spaced, relatively closely packed beams. Our concept is based on assigning a patrol region to each of the receivers, which have inputs distributed over the focal plane of the telescope. The input to each receiver can be positioned at any point within this patrol region. This approach, with only 4 reflections, offers very low loss. The Gaussian beam optical system can be designed to produce frequency-independent illumination of the telescope, which is an important advantage for broadband systems such those required for determination of redshifts of submillimeter galaxies.
title: Ð¡Ð¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² ÑÐ°ÑÑÐµÑÐ° ÑÐ»ÐµÐºÑÑÐ¾ÑÑÐ°ÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¿Ð¾Ð»ÐµÐ¹ Ð² Ð·Ð°Ð´Ð°ÑÐ°Ñ Ð¾ÑÐ¸ÐµÐ½ÑÐ¸ÑÐ¾Ð²ÐºÐ¸ Ð¼Ð¾Ð»Ð½Ð¸Ð¸
title: Ð°Ð²ÑÐ¾ÑÐµÑ. Ð´Ð¸Ñ. â¦ ÐºÐ°Ð½Ð´. ÑÐµÑ Ð½. Ð½Ð°ÑÐº: 05.09.05
titleType: Subtitle
Creators: name: ÐÐµÑÐµÑÑÐºÐ¾Ð², ÐÐ¸Ñ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: 2017
Subjects: Ð­Ð»ÐµÐºÑÑÐ¾ÑÑÐ°ÑÐ¸ÑÐµÑÐºÐ¾Ðµ Ð¿Ð¾Ð»Ðµ
ÐÑÐ¾Ð·Ð¾Ð·Ð°ÑÐ¸ÑÐ°

description: ÐÐ¸ÑÑÐµÑÑÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² ÑÐ°ÑÑÐµÑÐ° ÑÐ»ÐµÐºÑÑÐ¾ÑÑÐ°ÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¿Ð¾Ð»ÐµÐ¹ Ð² Ð·Ð°Ð´Ð°ÑÐ°Ñ Ð¾ÑÐ¸ÐµÐ½ÑÐ¸ÑÐ¾Ð²ÐºÐ¸ Ð»Ð¸Ð´ÐµÑÐ° Ð¼Ð¾Ð»Ð½Ð¸Ð¸. Ð Ð¿ÑÐµÐ´Ð¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ð¸, ÑÑÐ¾ ÑÑÑÐµÐ´Ð½ÐµÐ½Ð½ÑÐ¹ Ð»Ð¸Ð´ÐµÑ Ð¼Ð¾Ð»Ð½Ð¸Ð¸ Ð´Ð²Ð¸Ð¶ÐµÑÑÑ Ð¿Ð¾ ÑÐ¸Ð»Ð¾Ð²ÑÐ¼ Ð»Ð¸Ð½Ð¸ÑÐ¼, Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ° Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð·Ð°ÐºÐ»ÑÑÐ°ÐµÑÑÑ Ð² Ð°Ð½Ð°Ð»Ð¸Ð·Ðµ Ð¸ÑÐºÐ°Ð¶ÐµÐ½Ð¸Ñ ÑÐ¸Ð»Ð¾Ð²Ð¾Ð¹ Ð»Ð¸Ð½Ð¸Ð¸ ÑÐ»ÐµÐºÑÑÐ¾ÑÑÐ°ÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿Ð¾Ð»Ñ Ð·Ð°ÑÑÐ¶ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¾Ð±Ð»Ð°ÐºÐ°, Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð½Ð¾Ð¹ ÑÐµÑÐµÐ· ÐºÑÐ°Ð¹Ð½ÑÑ ÑÐ¾ÑÐºÑ Ð·Ð¾Ð½Ñ Ð·Ð°ÑÐ²Ð°ÑÐ°. ÐÐ¾ÐºÐ°Ð·Ð°Ð½Ð¾, ÑÑÐ¾ Ð½Ð°Ð²ÐµÐ´ÐµÐ½Ð½ÑÐ¹ Ð·Ð°ÑÑÐ´ Ð½ÐµÐ²ÑÑÐ¾ÐºÐ¸Ñ Ð¾Ð±ÑÐµÐºÑÐ¾Ð² ÐºÐ¾Ð¼Ð¿ÐµÐ½ÑÐ¸ÑÑÐµÑÑÑ ÐµÐ³Ð¾ Ð·ÐµÑÐºÐ°Ð»ÑÐ½ÑÐ¼ Ð·Ð°ÑÑÐ´Ð¾Ð¼ Ð¸ ÑÐ»ÐµÐºÑÑÐ¾ÑÑÐ°ÑÐ¸ÑÐµÑÐºÐ¾Ðµ ÑÑÑÐ³Ð¸Ð²Ð°Ð½Ð¸Ðµ Ð½ÐµÐ·Ð½Ð°ÑÐ¸ÑÐµÐ»ÑÐ½Ð¾. ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¾ Ð²Ð»Ð¸ÑÐ½Ð¸Ðµ Ð²ÑÑÐ¾ÑÑ Ð¸ Ð´Ð¸Ð°Ð¼ÐµÑÑÐ° ÑÑÐµÑÐ¶Ð½ÐµÐ²ÑÑ Ð¾Ð±ÑÐµÐºÑÐ¾Ð², ÑÐ¾ÐºÐ° Ð¼Ð¾Ð»Ð½Ð¸Ð¸ Ð¸ ÑÐµÐ»ÑÐµÑÐ° Ð¼ÐµÑÑÐ½Ð¾ÑÑÐ¸ Ð½Ð° Ð¿Ð»Ð¾ÑÐ°Ð´Ñ ÑÑÑÐ³Ð¸Ð²Ð°Ð½Ð¸Ñ.
Galaxy Evolution with Hubble (and Roman) IR Spectroscopy
Creators: name: Papovich, Casey
Publisher: name: Zenodo
Year: 2021
Subjects: Relating the dark matter density field to galaxy properties

description: Roman Surveys will provide Samples of Galaxies 100× larger, with Hubble-like data. Facilitate studies that require large samples and statistics: Physical properties that (co-)depend on mass, star-formation rate, surface density, gas-fraction, environment, formation history. Studies of Rare objects: Recently quenched galaxies; Mergers, in all their merger / star-formation / AGN stages. Motivation from Hubble Space Telescope Imaging and Grism Observations: When do galaxies quench? How does quenching proceed in galaxies? In different environments? How does Star-formation proceed in galaxies? What can we learn about metal production and feedback in high redshift galaxies?
Exploring Product Development of Cyber-Physical Systems in Startups: A Status Quo Study
Creators: name: Völk, Thomas Alexander
name: Klippert, Monika
name: Düser, Tobias
name: Albers, Albert
Publisher: name: Karlsruher Institut für Technologie (KIT)
Year: 2024
Subjects: cyber-physical systems in startups
product development methodology in startups
entrepreneurship with cyber-physical systems
problems of product development in CPS-startups
product development characteristics of CPS-startups

description: In the interconnected world of today, we experience the evolution of mechatronic systems into cyber-physical systems (CPS) through their connection to the Internet of Things (IoT). Despite their vast potential for groundbreaking applications already present, e. g. autonomous cars or smart production systems, startups face significant hurdles in developing CPS, primarily due to limited knowledge and resources. Currently, only few scientific contributions cover how hardware-containing products are developed in startups and what possible challenges can be expected. This gap highlights a pressing need for research into the specific challenges and methodologies of CPS development within the startup ecosystem. The research goal of this paper is to set an explorative foundation for understanding the product development of CPS in startups to enable further research and suiting support for future founders. This paper offers a first attempt to give a qualitative description of the status quo of the development of CPS in startups. It begins by establishing an understanding of the four main problem fields discussed in the literature on CPS development, entrepreneurship, and hardware development in startups: The impetus of entrepreneurs in CPS-developing startups (1), the ideation of the CPS in development (2), the prototyping of CPS in startups (3) and processes, methods, and tools used in CPS development in startups (4). They are discussed by semi-structured interviews. Due to the limited number of possible participants, the interviews are conducted with a sample of eight founders and employees from CPS-developing startups in Southern Germany. Their answers are used to deduce recurring patterns and contradicting positions in their subjective experience with CPS development. The result of this paper are twelve proposed characteristic aspects of current CPS development practice in startups based on the deduced patterns. With this first qualitative description of the status quo of CPS development, this paper identifies potentially relevant topics that occupy CPS founders, delivers connecting points to current research in established research disciplines and reveals current missing research activities.
title: Ð£ÑÑÑÐ¾Ð¹ÑÑÐ²Ð¾ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð»Ð°Ð·ÐµÑÐ½ÑÐ¼ Ð·Ð°ÑÐ²Ð¾ÑÐ¾Ð¼
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°ÑÐµÐ»Ð¸Ð½, ÐÐ»Ð°Ð´Ð¸ÑÐ»Ð°Ð²
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ÐµÐ½ÐµÑÐ°ÑÐ¾ÑÑ ÐºÐ²Ð°Ð½ÑÐ¾Ð²ÑÐµ
ÐÑÑÐ¸ÑÐ»Ð¸ÑÐµÐ»ÑÐ½ÑÐµ Ð¼Ð°ÑÐ¸Ð½Ñ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½ÑÐµ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»ÑÐ½ÑÐµ
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ÐÐ¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÑ ÐµÐ¼Ñ

description: ÐÐ±ÑÐµÐºÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ â ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð¾ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð»Ð°Ð·ÐµÑÐ½ÑÐ¼ Ð·Ð°ÑÐ²Ð¾ÑÐ¾Ð¼.
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EWSB from the soft portal into Dark Matter and prediction for direct detection
Creators: name: Kadastik, M.
name: Kannike, K.
name: Racioppi, A.
name: Raidal, M.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: Scalar Dark Matter (DM) can have dimensionful coupling to the Higgs boson - the "soft" portal into DM - which is predicted to be unsuppressed by underlying SO(10) GUT. The dimensionful coupling can be large, μ/v >> 1, without spoiling perturbativity of low energy theory up to the GUT scale. We show that the soft portal into DM naturally triggers radiative EWSB via large 1-loop DM corrections to the effective potential. In this scenario EWSB, DM thermal freeze-out cross section and DM scattering on nuclei are all dominated by the same coupling, predicting DM mass range to be 700 GeV< M_{DM} < 2 TeV. The spin-independent direct detection cross section is predicted to be just at the present experimental sensitivity and can explain the observed CDMS II recoil events.
description: CDMS II new results added and analyzed, Fig. 3 modified, 4 pages, 3 figures
Semantic learning in autonomously active recurrent neural networks
Creators: name: Gros, C.
name: Kaczor, G.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Neurons and Cognition (q-bio.NC)
subject: FOS: Biological sciences

description: The human brain is autonomously active, being characterized by a self-sustained neural activity which would be present even in the absence of external sensory stimuli. Here we study the interrelation between the self-sustained activity in autonomously active recurrent neural nets and external sensory stimuli. There is no a priori semantical relation between the influx of external stimuli and the patterns generated internally by the autonomous and ongoing brain dynamics. The question then arises when and how are semantic correlations between internal and external dynamical processes learned and built up? We study this problem within the paradigm of transient state dynamics for the neural activity in recurrent neural nets, i.e. for an autonomous neural activity characterized by an infinite time-series of transiently stable attractor states. We propose that external stimuli will be relevant during the sensitive periods, {\it viz} the transition period between one transient state and the subsequent semi-stable attractor. A diffusive learning signal is generated unsupervised whenever the stimulus influences the internal dynamics qualitatively. For testing we have presented to the model system stimuli corresponding to the bars and stripes problem. We found that the system performs a non-linear independent component analysis on its own, being continuously and autonomously active. This emergent cognitive capability results here from a general principle for the neural dynamics, the competition between neural ensembles.
description: Journal of Algorithms in Cognition, Informatics and Logic, special issue on `Perspectives and Challenges for Recurrent Neural Networks', in press
title: Ð¡Ð¸Ð½ÑÐµÐ· Ð¸ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ²Ð¾Ð¹ÑÑÐ² ÑÐ¾ÐµÐ´Ð¸Ð½ÐµÐ½Ð¸Ñ ÑÑÐ»Ð»ÐµÑÐµÐ½Ð° Ñ Ð±Ð°ÑÐ¸ÐµÐ¼
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: ÐÐ¾Ð³Ð´Ð°Ð½Ð¾Ð², Ð¤ÐµÐ´Ð¾Ñ
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Ð»Ð»ÐµÑÐµÐ½Ñ
ÐÐ°ÑÐ¸Ð¹
ÐÑÐ¸ÑÑÐ°Ð»Ð»Ñ Ð¼Ð¾Ð»ÐµÐºÑÐ»ÑÑÐ½ÑÐµ

description: Ð¦ÐµÐ»Ñ ÑÐ°Ð±Ð¾ÑÑ: Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¼ÐµÑÐ¾Ð´Ð° ÑÐ¸Ð½ÑÐµÐ·Ð° Ð½Ð¾Ð²Ð¾Ð³Ð¾ Ð²ÐµÑÐµÑÑÐ²Ð° â ÑÑÐ»Ð»ÐµÑÐ¸ÑÐ° Ð±Ð°ÑÐ¸Ñ. ÐÐ½Ð°Ð»Ð¸Ð· Ð½ÐµÐºÐ¾ÑÐ¾ÑÑÑ ÐµÐ³Ð¾ ÑÐ²Ð¾Ð¹ÑÑÐ². Ð ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐ¾Ð²Ð¾Ð´Ð¸ÑÑÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¼ÐµÑÐ¾Ð´Ð° ÑÐ¸Ð½ÑÐµÐ·Ð° ÑÑÐ»Ð»ÐµÑÐ¸ÑÐ° Ð±Ð°ÑÐ¸Ñ, Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐµÐ¹ ÑÐ¸Ð¼Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿ÑÐ¾ÑÐµÑÑÐ°, Ð¼ÐµÑÐ¾Ð´Ñ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¸ Ð´Ð°Ð½Ð½ÑÐµ Ð¿Ð¾ Ð½ÐµÐºÐ¾ÑÐ¾ÑÑÐ¼ ÑÐ²Ð¾Ð¹ÑÑÐ²Ð°Ð¼ ÑÑÐ»Ð»ÐµÑÐ¸ÑÐ° Ð±Ð°ÑÐ¸Ñ. ÐÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ñ ÑÐ¿Ð¾ÑÐ¾Ð±Ñ Ð¸Ð½ÑÐµÐ½ÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¸ ÑÐ¸Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¹ ÑÐµÐ°ÐºÑÐ¸Ð¸ Ð¿Ð¾Ð»ÑÑÐµÐ½Ð¸Ñ ÑÑÐ»Ð»ÐµÑÐ¸ÑÐ° Ð±Ð°ÑÐ¸Ñ. Ð¡Ð´ÐµÐ»Ð°Ð½Ñ Ð²ÑÐ²Ð¾Ð´Ñ Ð¿Ð¾ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÑÐ¼ Ð¸ Ð¾Ð³ÑÐ°Ð½Ð¸ÑÐµÐ½Ð¸ÑÐ¼ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ Ð½Ð¾Ð²Ð¾Ð³Ð¾ Ð²ÐµÑÐµÑÑÐ²Ð° Ð² Ð¾ÑÑÐ°ÑÐ»ÑÑ Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½Ð¾ÑÑÐ¸.
Wish you were gone
Creators: name: Leyton, Carolina
Publisher: name: University of British Columbia
Year: 2024

description: This excerpt from a young adult novel, Wish You Were Gone, deals with topics of grief and memory as they intertwine with immigrant experiences and movements towards the global north. The story follows eighteen-year-old, Colombian-American, Maria Molina Herrera, after the passing of her maternal grandmother, Abuelita Lucero. Not to worry, though, because María doesn’t have to grieve. She’ll see her Abuelita again. Not in an, “I’ll see you in my dreams” or supernatural signs kind of way. María’s family can tether the souls of the departed to the living world, essentially bonding her blood and family marriage for eternity. So, everything is great because Abuelita Lucero will return and life can go on as normal. Except not really. María’s connection to her grandmother has been severed by none other than Abuelita herself. For María to be able to talk to her grandmother’s soul, Abuelita had to leave an item in her will for María to use as a conduit. Out of petty resentment over an argument, Abuelita Lucero didn’t leave anything for María’s parents, little brother, or María herself. Confused and hurt by her grandmother’s decision, María decides to take matters into her own hands, not only wanting to fully understand Abuelita’s reasons for doing this, but ultimately fix the rift post-mortem. She enlists the help of both dead and living relatives to undertake the bureaucratic process of inserting her family into Abuelita’s will (yes, even the dead can’t escape legalities) and, in the process, discovers out family secrets that might have been better left alone and now threaten to irreversibly break her family.
Initial-Phase Spectroscopy as a Control of Entangled Systems
Creators: name: Horvath, Levente
name: Ficek, Zbigniew
Publisher: name: arXiv
Year: 2010
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We introduce the concept of initial-phase spectroscopy as a control of the dynamics of entangled states encoded into a two-atom system interacting with a broadband squeezed vacuum field. We illustrate our considerations by examining the transient spectrum of the field emitted by two systems, the small sample (Dicke) and the spatially extended (non-Dicke) models. It is found that the shape of the spectral components depends crucially on the relative phase between the initial entangled state and the squeezed field. We follow the temporal evolution of the spectrum and show that depending on the relative phase a hole burning can occur in one of the two spectral lines. We compare the transient behavior of the spectrum with the time evolution of the initial entanglement and find that the hole burning can be interpreted as a manifestation of the phenomenon of entanglement sudden death. In addition, we find that in the case of the non-Dicke model, the collective damping rate may act like an artificial tweezer that rotates the phase of the squeezed field.
description: 20 pages, 9 figures
title: Ф.М. Достоевский и О.Ф. Миллер: история взаимоотношений
title: Монография
titleType: Subtitle
Creators: name: Окишева К.А.
Publisher: name: Набережночелнинский государственный педагогический университет
Year: 2019

description: Монография посвящена исследованию личных и литературно-общественных взаимоотношений Ф.М. Достоевского и его будущего биографа О.Ф. Миллера. Анализ опубликованных и архивных материалов дает основание говорить: на духовное самоопределение О.Ф. Миллера значительное влияние оказал Ф.М. Достоевский, который, в свою очередь, увидел в О.Ф. Миллере нравственно и психологически близкого себе человека – «труженика во Христе», деятельного патриота России. Данное издание представляет интерес для студентов, исследователей русской литературы.
description: The monograph is devoted to investigation of the personal and the literary public of the relationship of F. M. Dostoevsky and his future biographer of O. F. Miller. Analysis of published and archival materials gives the basis to speak: the spiritual self-determination of O. F. Miller was strongly influenced by F. M. Dostoevsky, which in turn, saw in the O. F. Miller, morally and psychologically close to a person – "worker in Christ", an active patriot of Russia. This publication is of interest to students, scholars of Russian literature.
title: Ð£Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ ÑÑÑÐ´Ð¾Ð²ÑÐ¼Ð¸ ÐºÐ¾Ð½ÑÐ»Ð¸ÐºÑÐ°Ð¼Ð¸ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ âRadisson Hotels 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£ÑÑÐ¸Ð½Ð¾Ð²Ð°, 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: 2018
Subjects: ÐºÐ¾Ð½ÑÐ»Ð¸ÐºÑÐ½Ð°Ñ ÑÐ¸ÑÑÐ°ÑÐ¸Ñ
ÑÑÑÐ´Ð¾Ð²Ð¾Ð¹ ÐºÐ¾Ð½ÑÐ»Ð¸ÐºÑ
Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ñ
Ð¿ÑÑÐ¸ ÑÐ°Ð·ÑÐµÑÐµÐ½Ð¸Ñ
ÑÑÑÐµÑÑÐ¾ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÑ

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ñ Â«Radisson HotelsÂ». 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· ÑÑÑÐ´Ð¾Ð²ÑÑ ÐºÐ¾Ð½ÑÐ»Ð¸ÐºÑÐ¾Ð², Ð²Ð¾Ð·Ð½Ð¸ÐºÐ°ÑÑÐ¸Ñ Ð½Ð° Ð¿ÑÐ°ÐºÑÐ¸ÐºÐµ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ Â«Radisson HotelsÂ» Ð´Ð»Ñ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ ÑÑÑÐ°ÑÐµÐ³Ð¸Ð¸ ÑÑÐ¿ÐµÑÐ½Ð¾Ð³Ð¾ Ð²ÑÑÐ¾Ð´Ð° Ð¸Ð· ÐºÐ¾Ð½ÑÐ»Ð¸ÐºÑÐ½ÑÑ ÑÐ¸ÑÑÐ°ÑÐ¸Ð¹. ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° ÑÑÑÐ´Ð¾Ð²ÑÑ ÐºÐ¾Ð½ÑÐ»Ð¸ÐºÑÐ¾Ð² Ð±ÑÐ»Ð¸ Ð²ÑÐ´ÐµÐ»ÐµÐ½Ñ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½ÑÐµ ÑÑÑÐ´Ð¾Ð²ÑÐµ ÐºÐ¾Ð½ÑÐ»Ð¸ÐºÑÑ, ÐºÐ¾ÑÐ¾ÑÑÐµ Ð¼Ð¾Ð³ÑÑ Ð²Ð¾Ð·Ð½Ð¸ÐºÐ½ÑÑÑ Ð² ÑÑÐ»Ð¾Ð²Ð¸ÑÑ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð½Ð¾Ð³Ð¾ ÐºÐ»Ð¸ÐµÐ½ÑÐ¾Ð¿Ð¾ÑÐ¾ÐºÐ° Ð½Ð° Ð¿ÐµÑÐ¸Ð¾Ð´ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ Ð§ÐµÐ¼Ð¿Ð¸Ð¾Ð½Ð°ÑÐ° ÐÐ¸ÑÐ° Ð¿Ð¾ ÑÑÑÐ±Ð¾Ð»Ñ 2018 Ð½Ð° ÑÐµÑÑÐ¸ÑÐ¾ÑÐ¸Ð¸ Ð Ð¾ÑÑÐ¸Ð¸. ÐÑÐ»Ð° ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° ÑÑÑÐ°ÑÐµÐ³Ð¸Ñ Ð¿Ð¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ ÑÑÐºÐ¾Ð²Ð¾Ð´Ð¸ÑÐµÐ»Ñ Ð² ÑÐ¾Ð´Ðµ ÐºÐ¾Ð½ÐºÑÐµÑÐ½Ð¾Ð³Ð¾ ÑÑÑÐ´Ð¾Ð²Ð¾Ð³Ð¾ ÐºÐ¾Ð½ÑÐ»Ð¸ÐºÑÐ°. Ð ÑÐ°Ðº Ð¶Ðµ Ð±ÑÐ»Ð¸ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð¾Ð²Ð°Ð½Ñ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð´Ð»Ñ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÑÑÑÐµÑÑÐ¾ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÐ¸ ÑÐ¾ÑÑÑÐ´Ð½Ð¸ÐºÐ¾Ð² ÑÐ»ÑÐ¶Ð±Ñ Ð¿ÑÐ¸ÐµÐ¼Ð° Ð¸ ÑÐ°Ð·Ð¼ÐµÑÐµÐ½Ð¸Ñ Ð¾ÑÐµÐ»Ñ Ð¸ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ Ð¸Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¸, Ð¸ Ð²Ð²Ð¾Ð´ ÑÐ¸ÑÑÐµÐ¼Ñ Ð´ÐµÐ¿ÑÐµÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¾ÑÑÑÐ´Ð½Ð¸ÐºÐ¾Ð² Ð·Ð° ÐºÐ¾Ð½ÑÐ»Ð¸ÐºÑÐ½ÑÐµ ÑÐ¸ÑÑÐ°ÑÐ¸Ð¸. ÐÑÐ» Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð¾Ð²Ð°Ð½Ð½ÑÑ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹. Ð ÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹ Ð¿Ð¾ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÑÑÑÐµÑÑÐ¾ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÐ¸ Ð¸ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ðµ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¸ ÑÐ¾ÑÑÑÐ´Ð½Ð¸ÐºÐ¾Ð² Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÑ Ðº Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ Ð¸Ð½Ð´Ð¸Ð²Ð¸Ð´ÑÐ°Ð»ÑÐ½ÑÑ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»ÐµÐ¹ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸, ÑÑÐ¾ Ð¿Ð¾Ð·Ð²Ð¾Ð»Ð¸Ñ Ð¿ÑÐ¸Ð½Ð¸Ð¼Ð°ÑÑ Ð±Ð¾Ð»ÑÑÐµ Ð³Ð¾ÑÑÐµÐ¹ Ð¸ Ð¸Ð·Ð±ÐµÐ¶Ð°ÑÑ Ð½ÐµÐ³Ð°ÑÐ¸Ð²Ð½ÑÐµ Ð¾ÑÐ·ÑÐ²Ñ Ð¾Ð± Ð¾ÑÐµÐ»Ðµ Ð¸ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ Ð² ÑÐµÐ»Ð¾Ð¼.
The Spitzer view of FR-I radio galaxies: on the origin of the nuclear mid-infrared continuum
Creators: name: Leipski, C.
name: Antonucci, R.
name: Ogle, P.
name: Whysong, D.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We present Spitzer MIR spectra of 25 FR-I radio galaxies and investigate the nature of their MIR continuum emission. MIR spectra of star-forming galaxies and quiescent elliptical galaxies are used to identify host galaxy contributions while radio/optical core data are used to isolate the nuclear non-thermal emission. Out of the 15 sources with detected optical compact cores, four sources are dominated by emission related to the host galaxy. Another four sources show signs of warm, nuclear dust emission: 3C15, 3C84, 3C270, and NGC 6251. It is likley that these warm dust sources result from hidden AGN of optical spectral type 1. The MIR spectra of seven sources are dominated by synchrotron emission, with no significant component of nuclear dust emission. In parabolic SED fits of the non-thermal cores FR-Is tend to have lower peak frequencies and stronger curvature than blazars. This is roughly consistent with the common picture in which the core emission in FR-Is is less strongly beamed than in blazars.
description: 37 pages, 14 figures, accepted for publication in ApJ
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¸ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ðµ ÑÐ¸ÑÑÐµÐ¼Ñ pr-Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿Ð¾ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¿Ð¾Ð·Ð¸ÑÐ¸Ð²Ð½Ð¾Ð³Ð¾ Ð¸Ð¼Ð¸Ð´Ð¶Ð° Ð¾ÑÐ³Ð°Ð½Ð¾Ð² Ð¼ÐµÑÑÐ½Ð¾Ð³Ð¾ ÑÐ°Ð¼Ð¾ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐ Â«ÐÐ½ÑÐ¶ÐµÐ²Ð¾Â» Ð² ÑÐ¾ÑÑÐ°Ð²Ðµ ÐÐ¸ÑÐ¾Ð²ÑÐºÐ¾Ð³Ð¾ ÑÐ°Ð¹Ð¾Ð½Ð° Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³Ð°)
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð¡Ð°Ð²Ð²Ð°, 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: 2017
Subjects: Ð¼ÑÐ½Ð¸ÑÐ¸Ð¿Ð°Ð»ÑÐ½Ð°Ñ Ð²Ð»Ð°ÑÑÑ
ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¸Ð¼Ð¸Ð´Ð¶Ð°
PR-Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ

description: Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð° ÑÑÑÐ½Ð¾ÑÑÑ PR-Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿Ð¾ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¸Ð¼Ð¸Ð´Ð¶Ð° Ð² ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½Ð¾Ð¹ ÑÑÐµÑÐµ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ, ÑÐ¸ÑÑÐµÐ¼Ð½Ð¾ÑÑÑ, Ð½Ð¾ÑÐ¼Ñ Ð¸ Ð¿ÑÐ°Ð²Ð¾Ð²ÑÐµ Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ñ Ð´Ð»Ñ PR-Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð² Ð¼ÑÐ½Ð¸ÑÐ¸Ð¿Ð°Ð»ÑÐ½Ð¾Ð¼ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ð¸ Â«ÐÐ½ÑÐ¶ÐµÐ²Ð¾Â» Ð¸ ÑÐ»Ð¾Ð¶Ð¸Ð²ÑÐµÐ³Ð¾ÑÑ Ð¸Ð¼Ð¸Ð´Ð¶Ð°, Ñ ÑÐµÐ»ÑÑ Ð²ÑÑÐ²Ð»ÐµÐ½Ð¸Ñ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ð½ÑÑ ÑÑÐ°ÑÑÐºÐ¾Ð². Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° ÑÐ¸ÑÑÐµÐ¼Ð° ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÑ Ð´ÐµÐ¹ÑÑÐ²Ð¸Ð¹, Ñ ÑÐµÐ»ÑÑ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¿Ð¾Ð·Ð¸ÑÐ¸Ð²Ð½Ð¾Ð³Ð¾ Ð¸Ð¼Ð¸Ð´Ð¶Ð° Ð¼ÑÐ½Ð¸ÑÐ¸Ð¿Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ Â«ÐÐ½ÑÐ¶ÐµÐ²Ð¾Â» Ð² ÑÐ¾ÑÑÐ°Ð²Ðµ ÐÐ¸ÑÐ¾Ð²ÑÐºÐ¾Ð³Ð¾ ÑÐ°Ð¹Ð¾Ð½Ð° Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³Ð°.
The California Planet Survey II. A Saturn-Mass Planet Orbiting the M Dwarf Gl649
Creators: name: Johnson, John Asher
name: Howard, Andrew W.
name: Marcy, Geoffrey W.
name: Bowler, Brendan P.
name: Henry, Gregory W.
name: Fischer, Debra A.
name: Apps, Kevin
name: Isaacson, Howard
name: Wright, Jason T.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We report precise Doppler measurements of the nearby (d = 10.34 pc) M dwarf Gl649 that reveal the presence of a planet with a minimum mass Msini = 0.328 Mjup in an eccentric (e = 0.30), 598.3 day orbit. Our photometric monitoring reveals Gl649 to be a new variable star with brightness changes on both rotational and decadal timescales. However, neither of these timescales are consistent with the 600-day Doppler signal and so provide strong support for planetary reflex motion as the best interpretation of the observed radial velocity variations. Gl649b is only the seventh Doppler-detected giant planet around an M dwarf. The properties of the planet and host-star therefore contribute significant information to our knowledge of planet formation around low-mass stars. We revise and refine the occurrence rate of giant planets around M dwarfs based on the California Planet Survey sample of low-mass stars (M* < 0.6 Msun). We find that f = 3.4^{+2.2}_{-0.9}% of stars with M* < 0.6 Msun harbor planets with Msini > 0.3$ Mjup and a < 2.5 AU. When we restrict our analysis to metal-rich stars with [Fe/H] > +0.2 we find the occurrence rate is 10.7^{+5.9}_{-4.2}%.
description: 8 pages, 4 figures, 3 tables, PASP accepted
title: ÐÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ñ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½Ð¾-ÑÐ¾ÑÐ³Ð¾Ð²Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÐºÐ°ÑÐµ-ÐºÐ¾Ð½Ð´Ð¸ÑÐµÑÑÐºÐ¾Ð¹ Ð½Ð° 50 Ð¼ÐµÑÑ Ð² Ð³. ÐÑÑÐ¼Ð°Ð½ÑÐºÐµ
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¾ÑÐ´ÐµÐµÐ²Ð°, 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: 2016
Subjects: ÐºÐ°ÑÐµ-ÐºÐ¾Ð½Ð´Ð¸ÑÐµÑÑÐºÐ°Ñ
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description: ÐÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¾ Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð¾Ð²Ð¾Ðµ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼Ð¾ÑÑÐ¸ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÐºÐ°ÑÐµ-ÐºÐ¾Ð½Ð´Ð¸ÑÐµÑÑÐºÐ¾Ð¹, Ð¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½Ñ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐ°ÑÑÐµÑÑ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ, Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð° Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÑÑÑÐºÑÑÑÐ° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¿Ð¾ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÑÐµÐ¼Ð¾Ð³Ð¾ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ, ÐµÐ³Ð¾ Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð¾ÑÐ½Ð¾Ðµ ÑÐµÑÐµÐ½Ð¸Ðµ Ð¸ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸.
O'ZLASHTIRISHDA ORQADA QOLGAN O'QUVCHILAR PSIXOLOGIYASI VA ULAR BILAN KORREKSION ISHLAR
Creators: name: Xudoyberdiyeva, Komila
name: Berdaliyeva, Gulhayo
name: Shukurova, Matluba
Publisher: name: Zenodo
Year: 2025

description: O’zlashtirishda orqada qolgan o’quvchilar bilan ishlashda muvaffaqiyatga erishish uchun, eng avvalo, ularning oilasi, do’stlari to’g’risida ma’lumotga ega bo’lishimiz lozim. Barcha mamlakatlarda bo’lgani kabi yoshlarimiz orasida ham ta’lim olishda qiyinchilikga uchraydigan ammo qaysidir tamonlama iqtidorli farzandlar mavjud bo’lib, ularning ta’limiga alohida e’tibor qaratish lozim bo’ladi. “O’zlashtirishda orqada qolgan” bolalar bilan ishlash azaldan dolzarb vazifalardan biri hisoblanadi. Mazkur maqolada shu masalaga to’xtalib o’tamiz.
title: ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð²Ð»Ð¸ÑÐ½Ð¸Ñ Ð²ÑÑÐ¾ÐºÐ¾ÑÐµÐ¼Ð¿ÐµÑÐ°ÑÑÑÐ½Ð¾Ð¹ Ð²ÑÐ·ÐºÐ¾ÑÑÐ¸ Ð¼Ð¾ÑÐ¾ÑÐ½Ð¾Ð³Ð¾ Ð¼Ð°ÑÐ»Ð° Ð½Ð° ÑÐºÑÐ¿Ð»ÑÐ°ÑÐ°ÑÐ¸Ð¾Ð½Ð½ÑÐµ Ð¸ ÑÐµÑÑÑÑÐ½ÑÐµ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸ Ð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¡ÑÐ±Ð±Ð¾ÑÐ¸Ð½, ÐÐ²Ð³ÐµÐ½Ð¸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Ð¾ÑÐ¾ÑÐ½ÑÐµ Ð¼Ð°ÑÐ»Ð°
Ð¢ÑÐµÐ½Ð¸Ðµ
ÐÐ·Ð½Ð¾Ñ
ÐÑÐ·ÐºÐ¾ÑÑÑ
ÐÐ²Ð¸Ð³Ð°ÑÐµÐ»Ð¸ Ð²Ð½ÑÑÑÐµÐ½Ð½ÐµÐ³Ð¾ ÑÐ³Ð¾ÑÐ°Ð½Ð¸Ñ

description: Ð ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð²Ð»Ð¸ÑÐ½Ð¸Ñ Ð²ÑÑÐ¾ÐºÐ¾ÑÐµÐ¼Ð¿ÐµÑÐ°ÑÑÑÐ½Ð¾Ð¹ Ð²ÑÐ·ÐºÐ¾ÑÑÐ¸ Ð¼Ð¾ÑÐ¾ÑÐ½Ð¾Ð³Ð¾ Ð¼Ð°ÑÐ»Ð° Ð½Ð° ÑÐºÑÐ¿Ð»ÑÐ°ÑÐ°ÑÐ¸Ð¾Ð½Ð½ÑÐµ Ð¸ ÑÐµÑÑÑÑÐ½ÑÐµ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸ Ð¿Ð¾ÑÑÐ½ÐµÐ²Ð¾Ð³Ð¾ Ð´Ð²Ð¸Ð³Ð°ÑÐµÐ»Ñ. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð½Ð°ÑÑÑÐ½ÑÐ¹ ÑÐºÑÐ¿ÐµÑÐ¸Ð¼ÐµÐ½Ñ Ð¿Ð¾ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ Ð²ÑÑÐ¾ÐºÐ¾ÑÐµÐ¼Ð¿ÐµÑÐ°ÑÑÑÐ½Ð¾Ð¹ Ð´Ð¸Ð½Ð°Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð²ÑÐ·ÐºÐ¾ÑÑÐ¸ HTHS Ð¿ÑÐ¸ 150 Ð³ÑÐ°Ð´. Ð¡. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½Ñ Ð·Ð°Ð¼ÐµÑÑ Ð¼ÐµÑÐ°Ð½Ð¸ÑÐµÑÐºÐ¸Ñ Ð¿Ð¾ÑÐµÑÑ, ÑÐ°ÑÑÐ¾Ð´Ð° ÑÐ¾Ð¿Ð»Ð¸Ð²Ð°, Ð¼Ð¾ÑÐ½Ð¾ÑÑÐ¸ Ð´Ð²Ð¸Ð³Ð°ÑÐµÐ»Ñ Ð½Ð° Ð¼Ð¾ÑÐ¾ÑÐ½Ð¾Ð¼ ÑÑÐµÐ½Ð´Ðµ.
The Lyapunov spectrum is not always concave
Creators: name: Iommi, Godofredo
name: Kiwi, Jan
Publisher: name: arXiv
Year: 2008
Subjects: subject: Dynamical Systems (math.DS)
subject: FOS: Mathematics

description: We characterize one-dimensional compact repellers having nonconcave Lyapunov spectra. For linear maps with two branches we give an explicit condition that characterizes non-concave Lyapunov spectra.
Additional file 1 of Impact of rumination on sleep quality among patients with non‑alcoholic fatty liver disease: a moderated mediation model of anxiety symptoms and resilience
Creators: name: Chang, Xiaolin
name: Guo, Chenxi
name: Zhou, Heng
name: Liu, Li
Publisher: name: figshare
Year: 2023
Subjects: subject: Medicine
subject: Neuroscience
subject: Physiology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Science Policy

description: Additional file 1. Demographic and clinical characteristics in relation to anxiety symptoms and PSQI score.
Determining the forsterite abundance of the dust around Asymptotic Giant Branch stars
Creators: name: de Vries, B. L.
name: Min, M.
name: Waters, L. B. F. M.
name: Blommaert, J. A. D. L.
name: Kemper, F.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Aims. We present a diagnostic tool to determine the abundance of the crystalline silicate forsterite in AGB stars surrounded by a thick shell of silicate dust. Using six infrared spectra of high mass-loss oxygen rich AGB stars we obtain the forsterite abundance of their dust shells. Methods. We use a monte carlo radiative transfer code to calculate infrared spectra of dust enshrouded AGB stars. We vary the dust composition, mass-loss rate and outer radius. We focus on the strength of the 11.3 and the 33.6 μm forsterite bands, that probe the most recent (11.3 μm) and older (33.6 μm) mass-loss history of the star. Simple diagnostic diagrams are derived, allowing direct comparison to observed band strengths. Results. Our analysis shows that the 11.3 μm forsterite band is a robust indicator for the forsterite abundance of the current mass-loss period for AGB stars with an optically thick dust shell. The 33.6 μm band of forsterite is sensitive to changes in the density and the geometry of the emitting dust shell, and so a less robust indicator. Applying our method to six high mass-loss rate AGB stars shows that AGB stars can have forsterite abundances of 12% by mass and higher, which is more than the previously found maximum abundance of 5%.
description: Accepted for publication in A&A
title: ÐÑÐµÐ½ÐºÐ° ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ° Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ Ð³Ð¸Ð´ÑÐ¾ÑÐ°Ð·ÑÑÐ²Ð° Ð¿Ð»Ð°ÑÑÐ° Ð½Ð° ÐÐ¸Ð¼Ð½ÐµÐ¼ Ð½ÐµÑÑÑÐ½Ð¾Ð¼ Ð¼ÐµÑÑÐ¾ÑÐ¾Ð¶Ð´ÐµÐ½Ð¸Ð¸
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð§ÑÐ¼Ð°ÑÐ¸Ð½, ÐÐ»ÑÐ´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: 2017
Subjects: Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ðµ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð·Ð¸Ð¼Ð½ÐµÐ³Ð¾ Ð¼ÐµÑÑÐ¾ÑÐ¾Ð¶Ð´ÐµÐ½Ð¸Ñ
Ð³Ð¸Ð´ÑÐ¾ÑÐ°Ð·ÑÑÐ² Ð¿Ð»Ð°ÑÑÐ°
ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ°Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ Ð¿ÑÐ¾ÐµÐºÑÐ°

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÐÐÐ Â«ÐÐ°Ð·Ð¿ÑÐ¾Ð¼Ð½ÐµÑÑÑ-Ð¥Ð°Ð½ÑÐ¾ÑÂ» Ð½Ð° ÐÐ¸Ð¼Ð½ÐµÐ¼ Ð¼ÐµÑÑÐ¾ÑÐ¾Ð¶Ð´ÐµÐ½Ð¸Ð¸. Ð¦ÐµÐ»ÑÑ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ° Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ Ð³Ð¸Ð´ÑÐ¾ÑÐ°Ð·ÑÑÐ²Ð° Ð¿Ð»Ð°ÑÑÐ° Ð½Ð° ÐÐ¸Ð¼Ð½ÐµÐ¼ Ð½ÐµÑÑÑÐ½Ð¾Ð¼ Ð¼ÐµÑÑÐ¾ÑÐ¾Ð¶Ð´ÐµÐ½Ð¸Ð¸. Ð ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐµ ÑÐ°Ð±Ð¾ÑÑ Ð²ÑÐ±ÑÐ°Ð½Ð° ÑÐºÐ²Ð°Ð¶Ð¸Ð½Ð° Ñ Ð½Ð¸Ð·ÐºÐ¸Ð¼ Ð´ÐµÐ±Ð¸ÑÐ¾Ð¼Ð½ÐµÑÑÐ¸, Ð´Ð»Ñ Ð½ÐµÐµ ÑÐ°ÑÑÑÐ¸ÑÐ°Ð½Ñ Ð¾Ð¶Ð¸Ð´Ð°ÐµÐ¼ÑÐ¹ Ð´ÐµÐ±Ð¸Ñ Ð¿Ð¾ÑÐ»Ðµ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ ÐÐ Ð Ð¸ Ð¿ÑÐ¸Ð±ÑÐ»Ñ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð½Ð° Ð¿ÑÐ¾Ð³Ð½Ð¾Ð·Ð¸ÑÑÐµÐ¼ÑÐ¹ Ð¿ÐµÑÐ¸Ð¾Ð´ 3 Ð³Ð¾Ð´Ð°, Ð° ÑÐ°ÐºÐ¶Ðµ ÑÐ°ÑÑÑÐ¸ÑÐ°Ð½Ñ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸.
The Detection of Anomalous Dust Emission in the Nearby Galaxy NGC 6946
Creators: name: Murphy, E. J.
name: Helou, G.
name: Condon, J. J.
name: Schinnerer, E.
name: Turner, J. L.
name: Beck, R.
name: Mason, B. S.
name: Chary, R. -R.
name: Armus, L.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We report on the Ka-band (26-40 GHz) emission properties for 10 star-forming regions in the nearby galaxy NGC 6946. From a radio spectral decomposition, we find that the 33 GHz flux densities are typically dominated by thermal (free-free) radiation. However, we also detect excess Ka-band emission for an outer-disk star-forming region relative to what is expected given existing radio, submillimeter, and infrared data. Among the 10 targeted regions, measurable excess emission at 33 GHz is detected for half of them, but in only one region is the excess found to be statistically significant ($\approx7σ$). We interpret this as the first likely detection of so called `anomalous' dust emission outside of the Milky Way. We find that models explaining this feature as the result of dipole emission from rapidly rotating ultrasmall grains are able to reproduce the observations for reasonable interstellar medium conditions. While these results suggest that the use of Ka-band data as a measure of star formation activity in external galaxies may be complicated by the presence of anomalous dust, it is unclear how significant a factor this will be for globally integrated measurements as the excess emission accounts for $\la$10% of the total Ka-band flux density from all 10 regions.
description: 6 pages; Accepted to ApJ Letters
title: Ð­Ð»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ°Ñ ÑÐ°ÑÑÑ Ð¢Ð­Ð¦ Ñ 4 Ð±Ð»Ð¾ÐºÐ°Ð¼Ð¸ Ð¼Ð¾ÑÐ½Ð¾ÑÑÑÑ 32 ÐÐÑ
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¾Ð½Ð¸Ð½Ð°, ÐÐ¾Ð»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ÐµÐ¿Ð»Ð¾Ð²Ð°Ñ ÑÐ»ÐµÐºÑÑÐ¾ÑÐµÐ½ÑÑÐ°Ð»Ñ
ÑÑÑÑÐºÑÑÑÐ½Ð°Ñ ÑÑ ÐµÐ¼Ð°
ÑÐ»ÐµÐºÑÑÐ¾Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ

description: Ð ÑÐ°Ð±Ð¾ÑÐµ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÑÐ°ÑÑÐ¸ ÑÐµÐ¿Ð»Ð¾Ð²Ð¾Ð¹ ÑÐ»ÐµÐºÑÑÐ¾ÑÐµÐ½ÑÑÐ°Ð»Ð¸. ÐÑÐ±ÑÐ°Ð½Ð° Ð¾Ð¿ÑÐ¸Ð¼Ð°Ð»ÑÐ½Ð°Ñ ÑÑÑÑÐºÑÑÑÐ½Ð°Ñ ÑÑÐµÐ¼Ð° Ð¸ Ð¾ÑÐ½Ð¾Ð²Ð½Ð¾Ðµ ÑÐ»ÐµÐºÑÑÐ¾Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ. Ð Ð°ÑÑÑÐ¸ÑÐ°Ð½Ñ ÑÐ¾ÐºÐ¸ ÐºÐ¾ÑÐ¾ÑÐºÐ¾Ð³Ð¾ Ð·Ð°Ð¼ÑÐºÐ°Ð½Ð¸Ñ. ÐÑÐ±ÑÐ°Ð½Ñ ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð°Ð¿Ð¿Ð°ÑÐ°ÑÑ Ð¸ Ð¿ÑÐ¾Ð²Ð¾Ð´Ð½Ð¸ÐºÐ¸. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° Ð³Ð»Ð°Ð²Ð½Ð°Ñ ÑÑÐµÐ¼Ð° ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÐ¾ÐµÐ´Ð¸Ð½ÐµÐ½Ð¸Ð¹ Ð¸ ÑÑÐµÐ¼Ð° ÑÐ¾Ð±ÑÑÐ²ÐµÐ½Ð½ÑÑ Ð½ÑÐ¶Ð´.
O AIIB NA ORDEM FINANCEIRA INTERNACIONAL: ANÁLISE COMPARATIVA OS INSTRUMENTOS DE AVALIAÇÃO DE IMPACTO SOCIOAMBIENTAL DOS PROJETOS DO AIIB E DO BANCO MUNDIAL NA ÍNDIA (2017-2020)
Creators: name: Jukemura, Felipe
Publisher: name: figshare
Year: 2022
Subjects: Environmental Science

description: This expanded summary aims to analyze the performance of the Asian Infrastructure Investment Bank (AIIB) in a compared perspective to the World Bank (WB) in relation to the adoption of Environmental and Social Assessment (ESA) mechanisms in their projects. Thus, the objective is to understand how the emergence of the AIIB can be understood within the current international financial order, whether in overlap, complementarity, or divergence from other Multilateral Development Banks (MDBs). To this end, the projects carried out by the two banks in India in the period between 2017 and 2020 were analyzed, considering the social and environmental issues linked to their approval. This analysis is made up of two parts, the first is a general description and comparison of all twenty projects carried out in the proposed period, considering the amounts invested, risk classification and the ESA instruments adopted. The content of the ESA instruments of an AIIB project and a WB project is then compared, based on 10 parameters for comparison. It is concluded that the AIIB can be understood as a middle way bank, that is, with the internalization of some standards of the already established MDBs, but with innovative characteristics. Remarkably, the incorporation of the form of ESA instruments and some WB guides can be seen, but at the same time, the AIIB presents innovations in relation to the WB such as the focus on infrastructure, loans for projects of various sizes, greater respect and integration borrower's policies and programs or “reducing” the complexity of socio-environmental analysis instruments.