cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Quantum Current Algebra for the $AdS_5 \times S^5$ Superstring
Creators: name: Bedoya, Oscar A.
name: Marchioro, Dafni Z.
name: Nedel, Daniel L.
name: Vallilo, Brenno Carlini
Publisher: name: arXiv
Year: 2010
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: The sigma model describing the dynamics of the superstring in the $AdS_5 \times S^5$ background can be constructed using the coset $PSU(2,2|4)/SO(4,1)\times SO(5)$. A basic set of operators in this two dimensional conformal field theory is composed by the left invariant currents. Since these currents are not (anti) holomorphic, their OPE's is not determined by symmetry principles and its computation should be performed perturbatively. Using the pure spinor sigma model for this background, we compute the one-loop correction to these OPE's. We also compute the OPE's of the left invariant currents with the energy momentum tensor at tree level and one loop.
description: 28 pages, 12 figures, v2: typos corrected.
Scalar field mass in generalized gravity
Creators: name: Faraoni, Valerio
Publisher: name: arXiv
Year: 2009
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: The notions of mass and range of a Brans-Dicke-like scalar field in scalar-tensor and f(R) gravity are subject to an ambiguity that hides a potential trap. We spell out this ambiguity and identify a physically meaningful and practical definition for these quantities. This is relevant when giving a mass to this scalar in order to circumvent experimental limits on the PPN parameters coming from Solar System experiments.
description: 11 pages, no figures, to appear in Class. Quantum Grav. References added
Hadronic Form Factors: Combining QCD Calculations with Analyticity
Creators: name: Khodjamirian, A.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: I discuss recent applications of QCD light-cone sum rules to various form factors of pseudoscalar mesons. In this approach both soft and hard contributions to the form factors are taken into account. Combining QCD calculation with the analyticity of the form factors, one enlarges the region of accessible momentum transfers.
description: 12 pages, 3 figures, Talk at the Workshop "Shifmania, Crossing the boundaries: Gauge dynamics at strong coupling", May 14-17,2009, Minneapolis, USA; table entry and reference updated
Additional file 10 of LncRNA WEE2-AS1 is a diagnostic biomarker that predicts poor prognoses in patients with glioma
Creators: name: Zhu, Xuqiang
name: Chen, Di
name: Sun, Yiyu
name: Yang, Shuo
name: Wang, Weiguang
name: Liu, Bing
name: Gao, Peng
name: Li, Xueyuan
name: Wu, Lixin
name: Ma, Siqi
name: Lin, Wenyang
name: Ma, Jiwei
name: Yan, Dongming
Publisher: name: figshare
Year: 2023
Subjects: subject: Biochemistry
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Biotechnology
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Mathematical Sciences not elsewhere classified
subject: Cancer

description: Supplementary Material 10
Crowdsourcing at the British Library
Creators: name: Ridge, Mia
Publisher: name: Zenodo
Year: 2022
Subjects: crowdsourcing
British Library
research libraries
GLAMs
digital participation

description: A general overview of my work in crowdsourcing at the British Library including: My perspective on crowdsourcing in GLAMs Definitions / key concepts Why is the British Library interested in crowdsourcing? Crowdsourcing projects at the BL Opportunities and challenges around crowdsourcing in libraries / GLAMs Future work / ideas for crowdsourcing at the British Library
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð±Ð¸Ð·Ð½ÐµÑ-Ð¿Ð»Ð°Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð®ÑÐºÐ¸Ð½Ð°, Ð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: 2016
Subjects: Ð±Ð¸Ð·Ð½ÐµÑ-Ð¿Ð»Ð°Ð½
Ð¿Ð»Ð°Ð½ Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð°
Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐ¹ Ð¿Ð»Ð°Ð½
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description: Ð Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½ Ð±Ð¸Ð·Ð½ÐµÑ-Ð¿Ð»Ð°Ð½ Ð´Ð»Ñ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ Ð±ÑÐ´ÑÑÐµÐ³Ð¾ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ñ Ð¾ÑÐ½Ð¾Ð² Ð±Ð¸Ð·Ð½ÐµÑ-Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ. Ð Ð¿ÐµÑÐ²Ð¾Ð¹ Ð³Ð»Ð°Ð²Ðµ Ð¾ÑÐ²ÐµÑÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð°ÑÐ¿ÐµÐºÑÑ, ÐºÐ°ÑÐ°ÑÑÐ¸ÐµÑÑ Ð±Ð¸Ð·Ð½ÐµÑ-Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ. Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ Ð³Ð»Ð°Ð²Ðµ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑÑÑ Ð¿Ð¾Ð½ÑÑÐ¸Ñ, ÑÑÐ½ÐºÑÐ¸Ð¸, Ð²Ð¸Ð´Ñ Ð¸ ÑÑÐ°Ð´Ð¸Ð¸ Ð½Ð°Ð¿Ð¸ÑÐ°Ð½Ð¸Ñ Ð±Ð¸Ð·Ð½ÐµÑ-Ð¿Ð»Ð°Ð½Ð°. Ð Ð°Ð·Ð´ÐµÐ»Ñ Ð±Ð¸Ð·Ð½ÐµÑ-Ð¿Ð»Ð°Ð½Ð° Ð²ÐºÐ»ÑÑÐ°ÑÑ Ð² ÑÐµÐ±Ñ: ÑÐµÐ·ÑÐ¼Ðµ, Ð¾Ð¿Ð¸ÑÐ°Ð½Ð¸Ðµ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ, Ð¾Ð¿Ð¸ÑÐ°Ð½Ð¸Ðµ ÑÑÐ»ÑÐ³Ð¸, Ð°Ð½Ð°Ð»Ð¸Ð· ÑÑÐ½ÐºÐ°, Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½ÑÐ¹ Ð¿Ð»Ð°Ð½, Ð¿Ð»Ð°Ð½ ÑÐ±ÑÑÐ°, ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÐ¹ Ð¿Ð»Ð°Ð½ Ð¸ Ð¿ÑÐ¸Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ. ÐÑÐ¾ÑÐ°Ñ Ð³Ð»Ð°Ð²Ð° ÑÐ²Ð»ÑÐµÑÑÑ Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¾Ð¹, Ð² Ð½ÐµÐ¹ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ ÑÐ°ÐºÐ¸Ðµ ÑÐ°Ð·Ð´ÐµÐ»Ñ Ð±Ð¸Ð·Ð½ÐµÑ-Ð¿Ð»Ð°Ð½Ð° ÐºÐ°Ðº: ÑÐµÐ·ÑÐ¼Ðµ, Ð¾Ð¿Ð¸ÑÐ°Ð½Ð¸Ðµ Ð±Ð¸Ð·Ð½ÐµÑÐ° Ð¸ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÑÐ½ÐºÐ°, Ð¿Ð»Ð°Ð½ Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð°, Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐ¹ Ð¿Ð»Ð°Ð½ Ð¸ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½ÑÐ¹ Ð¿Ð»Ð°Ð½. Ð ÑÑÐµÑÑÐµÐ¹ Ð³Ð»Ð°Ð²Ðµ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½ÑÐ¹ Ð¸ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÐ¹ Ð¿Ð»Ð°Ð½Ñ, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð±ÑÐ´ÑÑÐ¸Ñ Ð·Ð°ÑÑÐ°Ñ. Ð ÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¾Ð¼ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ Ð±Ð¸Ð·Ð½ÐµÑ-Ð¿Ð»Ð°Ð½ Ð³Ð¾ÑÐ¾Ð²ÑÐ¹ Ðº Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¾Ð¼Ñ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ.
Lipase Supporting Information
Creators: name: Nguyen, Quoc-Thai
name: Vo, Cam-Van T.
name: Luu, Nhan V. H.
name: Nguyen, Thoai T. H.
name: Nguyen, Truc T.
name: Ho, Bach Q.
name: Nguyen, Thuong H.
name: Tran, Thanh-Dao
Publisher: name: figshare
Year: 2021
Subjects: Biochemistry

description: This supporting information provides the experimental details and the raw data that have been presented in the corresponding main text article.
Quantized spin waves in the metallic state of magnetoresistive manganites
Creators: name: Petit, S.
name: Hennion, M.
name: Moussa, F.
name: Lamago, D.
name: Ivanov, A.
name: Mukovskii, Y. M.
name: Shulyatev, D.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: High resolution spin waves measurements have been carried out in ferromagnetic (F) La(1-x)(Sr,Ca)xMnO3 with x(Sr)=0.15, 0.175, 0.2, 0.3 and x(Ca)=0.3. In all q-directions, close to the zone boundary, the spin wave spectra consist of several energy levels, with the same values in the metallic and the x\approx 1/8 ranges. Mainly the intensity varies, jumping from the lower energy levels determined in the x\approx 1/8 range to the higher energy ones observed in the metallic state. On the basis of a quantitative agreement found for x(Sr)=0.15 in a model of ordered 2D clusters, the spin wave anomalies of the metallic state can be interpreted in terms of quantized spin waves within the same 2D clusters, embedded in a 3D matrix.
description: 4 pages, 5 figures
Observation of enhanced transmission for s-polarized light through a subwavelength slit
Creators: name: Guillaumee, M.
name: Nikitin, A. Yu.
name: Klein, M. J. K.
name: Dunbar, L. A.
name: Spassov, V.
name: Eckert, R.
name: Martin-Moreno, L.
name: Garcia-Vidal, F. J.
name: Stanley, R. P.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Other Condensed Matter (cond-mat.other)
subject: FOS: Physical sciences

description: Enhanced optical transmission (EOT) through subwavelength apertures is usually obtained for p-polarized light. The present study experimentally investigates EOT for s-polarized light. A subwavelength slit surrounded on each side by periodic grooves has been fabricated in a gold film and covered by a thin dielectric layer. The excitation of s-polarized dielectric waveguide modes inside the dielectric film strongly increases the s-polarized transmission. Transmission measurements are compared with a coupled mode model and show good qualitative agreement. Adding a waveguide can improve light transmission through subwavelength apertures, as both s and p-polarization can be efficiently transmitted.
description: 11 pages, 3 figures, submitted to Applied Physics Letters
HAQIQATNI O'ZGARTIRISH MUMKINMI?
Creators: name: Toʻlqinova, Sevinch
Publisher: name: Zenodo
Year: 2025

description: Haqiqatni o‘zgartirish mumkinmi? Aslida haqiqat tashqi olamda emas, balki insonning ichki dunyosida shakllanadi. Qanday fikrlasak, o‘zimizni qanday his qilsak, ong ostimiz o‘sha holatga moslashadi va uni haqiqat deb qabul qiladi. Agar biz doimo siqilish, hafagarchilik va umidsizlik holatida bo‘lsak, ongimiz bu holatni normal deb qabul qilib, uni davom ettirishga moyil bo‘ladi. Shuning uchun, hatto ongli ravishda bu holatdan chiqishga urinib ko‘rsak ham, tanamiz bunga qarshilik qiladi. Ko‘pchilik hayotda "sinovlar kelsa, birdaniga keladi" degan iborani eshitgan. Buning sababi shundaki, qiyinchiliklar vaqtida bizning ongimiz o‘sha negativ vaziyatni qabul qilib, uni takror-takror ong ostiga yuboradi. Masalan, "Menda doim shunaqa bo‘ladi. Hech nima yaxshi emas", degan fikrlar haqiqatga aylanib boradi. Natijada, hayotimizda shunga o‘xshash vaziyatlar yana takrorlanaveradi.
Interface controlled electronic variations in correlated heterostructures
Creators: name: Gehrke, K.
name: Moshnyaga, V.
name: Lebedev, O. I.
name: Kirilenko, D.
name: Van Tendeloo, G.
name: Samwer, K.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: An interface modification of LCMO-BTO superlattices was found to massively influence magnetic and magnetotransport properties. Moreover it determines the crystal structure of the manganite layers, changing it from orthorhombic (Pnma) for the conventional superlattice (cSL), to rhombohedral (R-3c) for the modified one (mSL). While the cSL shows extremely nonlinear ac transport, the mSL is an electrically homogeneous material. The observations go beyond an oversimplified picture of dead interface layers and evidence the importance of electronic correlations at perovskite interfaces.
Inflation and Reheating in Induced Gravity
Creators: name: Cerioni, A.
name: Finelli, F.
name: Tronconi, A.
name: Venturi, G.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Inflation is studied in the context of induced gravity (IG) $γσ^2 R$, where $R$ is the Ricci scalar, $σ$ a scalar field and $γ$ a dimensionless constant. We study in detail cosmological perturbations in IG and examine both a Landau-Ginzburg (LG) and a Coleman-Weinberg (CW) potential toy models for small field and large field (chaotic) inflation and find that small field inflationary models in IG are constrained to $γ\lesssim 3 \times 10^{-3}$ by WMAP 5 yrs data. Finally we describe the regime of coherent oscillations in induced gravity by an analytic approximation, showing how the homogeneous inflaton can decay in its short-scale fluctuations when it oscillates around a non-zero value $σ_0$.
description: 5 pages, 2 figures
title: ÐÐ½ÑÑÑÑÐ¼ÐµÐ½ÑÑ Ð¸ Ð¼ÐµÑÐ¾Ð´Ñ Ð°Ð´Ð°Ð¿ÑÐ°ÑÐ¸Ð¸ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð¿Ð¾ÑÐµÐ½ÑÐ¸Ð°Ð»Ð° Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½ÑÑ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¹
title: Ð½Ð°ÑÑÐ½ÑÐ¹ Ð´Ð¾ÐºÐ»Ð°Ð´
titleType: Subtitle
Creators: name: ÐÐ²Ð°Ð½Ð¾Ð²Ð°, ÐÐ°ÑÐ°Ð»ÑÑ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: ÐÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½ÑÐµ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ
Ð¿Ð¾ÑÐµÐ½ÑÐ¸Ð°Ð» Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ
Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¸

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²ÑÐ²Ð°ÐµÑÑÑ Ð²Ð°Ð¶Ð½Ð¾ÑÑÑ Ð°Ð´Ð°Ð¿ÑÐ°ÑÐ¸Ð¸ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð¿Ð¾ÑÐµÐ½ÑÐ¸Ð°Ð»Ð° Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½ÑÑ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¹ Ð² ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÑ ÑÑÐ»Ð¾Ð²Ð¸ÑÑ Ð´Ð¸Ð½Ð°Ð¼Ð¸ÑÐ½Ð¾ ÑÐ°Ð·Ð²Ð¸Ð²Ð°ÑÑÐµÐ³Ð¾ÑÑ ÑÑÐ½ÐºÐ°. ÐÐ¾Ð´ÑÑÑÐºÐ¸Ð²Ð°ÐµÑÑÑ Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼Ð¾ÑÑÑ ÐµÐ³Ð¾ Ð°Ð´Ð°Ð¿ÑÐ°ÑÐ¸Ð¸ Ð² ÑÑÐ»Ð¾Ð²Ð¸ÑÑ Ð½ÐµÐ¾Ð¿ÑÐµÐ´ÐµÐ»ÑÐ½Ð½Ð¾ÑÑÐ¸ Ð²Ð½ÐµÑÐ½ÐµÐ¹ ÑÑÐµÐ´Ñ Ñ ÑÐµÐ»ÑÑ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÐºÐ°ÑÐµÑÑÐ²Ð° Ð¿ÑÐ¾Ð´ÑÐºÑÐ¸Ð¸, ÑÑÐ¾Ð²Ð½Ñ ÑÐ´Ð¾Ð²Ð»ÐµÑÐ²Ð¾ÑÑÐ½Ð½Ð¾ÑÑÐ¸ ÐºÐ»Ð¸ÐµÐ½ÑÐ¾Ð², ÑÐ»ÑÑÑÐµÐ½Ð¸Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÑÐ°Ð±Ð¾ÑÑ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ, ÑÐ¼ÐµÐ½ÑÑÐµÐ½Ð¸Ñ Ð¸Ð·Ð´ÐµÑÐ¶ÐµÐº Ð¸ Ð¿ÑÐµÐ´Ð¾ÑÐ²ÑÐ°ÑÐµÐ½Ð¸Ñ Ð´Ð¾Ð¿Ð¾Ð»Ð½Ð¸ÑÐµÐ»ÑÐ½ÑÑ Ð¸Ð·Ð´ÐµÑÐ¶ÐµÐº Ð¸ Ð¿Ñ. Ð¢Ð°ÐºÐ¶Ðµ ÑÐ´ÐµÐ»ÑÐµÑÑÑ Ð²Ð½Ð¸Ð¼Ð°Ð½Ð¸Ðµ Ð°Ð´Ð°Ð¿ÑÐ°ÑÐ¸Ð¸ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð¿Ð¾ÑÐµÐ½ÑÐ¸Ð°Ð»Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð² ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²Ð¸Ð¸ ÑÐ¾ ÑÑÑÐ°ÑÐµÐ³Ð¸ÑÐµÑÐºÐ¸Ð¼Ð¸ Ð·Ð°Ð´Ð°ÑÐ°Ð¼Ð¸ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾-Ð°ÐºÑÐ¸Ð²Ð½ÑÑ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¹ Ð¸ Ð¼ÐµÑÑÐ¾ Ð°Ð´Ð°Ð¿ÑÐ°ÑÐ¸Ð¸ Ð² Ð¿ÑÐ¾ÑÐµÑÑÐµ ÑÑÑÐ°ÑÐµÐ³Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ. ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ð¸ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ¾Ð² Ð»Ð¸ÑÐµÑÐ°ÑÑÑÑ, Ð² Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¾ÑÑÐ°Ð¶ÐµÐ½Ñ ÑÑÑÐµÑÑÐ²ÑÑÑÐ¸Ðµ Ð¼ÐµÑÐ¾Ð´Ñ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð°Ð´Ð°Ð¿ÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ. Ð ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ ÑÑÐµÐ¼Ñ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¿ÑÐ¾ÑÐµÑÑÐ° Ð°Ð´Ð°Ð¿ÑÐ°ÑÐ¸Ð¸ Ð¸ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½ Ð¾Ð´Ð¸Ð½ Ð¸Ð· Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½ÑÑ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² Ð°Ð´Ð°Ð¿ÑÐ°ÑÐ¸Ð¸ Ð¿Ð¾ÑÐµÐ½ÑÐ¸Ð°Ð»Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ Ð¼ÐµÑÐ¾Ð´Ð°, Ð·Ð°Ð¸Ð¼ÑÑÐ²Ð¾Ð²Ð°Ð½Ð½Ð¾Ð³Ð¾ Ð² Ð½ÐµÑÑÐµÐ³Ð°Ð·Ð¾Ð²Ð¾Ð¹ Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð¸ Ð¼ÐµÑÐ¾Ð´Ð° Ð¿Ð¾ÑÑÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð°Ð½Ð°Ð»Ð¸Ð·Ð°.
Beyond Kirillov-Reshetikhin modules
Creators: name: Chari, Vyjayanthi
name: Hernandez, David
Publisher: name: arXiv
Year: 2008
Subjects: subject: Quantum Algebra (math.QA)
subject: Representation Theory (math.RT)
subject: FOS: Mathematics

description: In this survey, we shall be concerned with the category of finite-dimensional representations of the untwisted quantum affine algebras when the quantum parameter q is not a root of unity. We review the foundational results of the subject, including the Drinfeld presentation, the classification of simple modules and q-characters. We then concentrate on particular families of irreducible representations whose structure has recently been understood: Kirillov-Reshetikhin modules, minimal affinizations and beyond.
description: 35 pages
Elucidating the mechanisms regulating unilateral cytokinesis in Caenorhabditis elegans zygotes
Creators: name: Hsu, Christina Rou
Publisher: name: University of British Columbia
Year: 2024

description: The cytokinetic contractile ring plays a crucial role in animal morphogenesis by spatially controlling its orientation and position along the body axis. Unilateral cytokinesis is one such event where the contractile ring closes asymmetrically to maintain tissue integrity in various developmental contexts. Previous research suggests that a concerted movement of the cell cortex, termed cortical flow, is also asymmetrically regulated during this process. However, the roles and regulations of cortical flow during cytokinesis remain unclear due to difficulties in imaging both the cell surface and the division plane. In this thesis, we addressed this question using Caenorhabditis elegans embryos as a model system. We developed computational and experimental methods to analyze both the cell surface and ring closure dynamics in an integrative manner. High-resolution 4D imaging of dividing cells revealed that mechanical suppression of ring-directed cortical flow is associated with asymmetric ring closure. Consistently, artificially suppressing ring-directed cortical flow in symmetrically dividing cells induces asymmetric ring closure. Overall, this study demonstrated that ring closure asymmetry is controlled by the mechanosensitive action of the contractile ring.
Circumstellar molecular line emission from S-type AGB stars: Mass-loss rates and SiO abundances
Creators: name: Ramstedt, S.
name: Schoeier, F. L.
name: Olofsson, H.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: The main aim is to derive reliable mass-loss rates and circumstellar SiO abundances for a sample of 40 S-type AGB stars based on new multi-transitional CO and SiO radio line observations. In addition, the results are compared to previous results for M-type AGB stars and carbon stars to look for trends with chemical type. The circumstellar envelopes are assumed to be spherically symmetric and formed by a constant mass-loss rate. The mass-loss rates are estimated from fitting the CO observations using a non-local, non-LTE radiative transfer code. Once the physical properties of the circumstellar envelopes are determined, the same radiative transfer code is used to model the observed SiO lines in order to derive circumstellar abundances and the sizes of the SiO line-emitting regions. We have estimated mass-loss rates of 40 S-type AGB stars and find that the derived mass-loss rates have a distribution that resembles those previously derived for similar samples of M-type AGB stars and carbon stars. The estimated mass-loss rates also correlate well with the corresponding expansion velocity. In all, this indicates that the mass loss is driven by the same mechanism in all three chemical types of AGB stars. In addition, we have estimated the circumstellar fractional abundance of SiO relative to H2 in 26 of the sample S-type AGB stars. The derived SiO abundances are, on average, about an order of magnitude higher than predicted by stellar atmosphere thermal equilibrium chemistry, indicating that non-equilibrium chemical processes determines the abundance of SiO in the circumstellar envelope. Moreover, a comparison with the results for M-type AGB stars and carbon stars show that for a certain mass-loss rate, the circumstellar SiO abundance seems independent (although with a large scatter) of the C/O-ratio.
description: 24 pages, 11 figures
title: ÐÑÑÐ°ÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½ÑÐµ ÑÑÑÐ°Ð½Ð¾Ð²ÐºÐ¸ ÑÐ¿Ð¾ÑÑÑÐ¼ÐµÐ½Ð¾Ð² Ð² Ð¿ÐµÑÐ¸Ð¾Ð´ Ð¾Ð³ÑÐ°Ð½Ð¸ÑÐµÐ½Ð¸Ð¹, Ð²ÑÐ·Ð²Ð°Ð½Ð½ÑÑ Ð¿Ð°Ð½Ð´ÐµÐ¼Ð¸ÐµÐ¹ ÐºÐ¾ÑÐ¾Ð½Ð°Ð²Ð¸ÑÑÑÐ° COVID-19
title: Irrational attitudes of athletes during the period of restrictions caused by the COVID-19 pandemic
Creators: name: ÐÐ»ÑÐ¸Ð½Ð°, Ð.
name: "Ð¡Ð¿Ð¾ÑÑ, ÑÐµÐ»Ð¾Ð²ÐµÐº, Ð·Ð´Ð¾ÑÐ¾Ð²ÑÐµ", Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÐ¹ Ð½Ð°ÑÑÐ½ÑÐ¹ ÐºÐ¾Ð½Ð³ÑÐµÑÑ
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2021
Subjects: ÑÐ¿Ð¾ÑÑ
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description: Ð ÑÑÐ°ÑÑ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 Ð¸ÑÑÐ°ÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½ÑÑ ÑÑÑÐ°Ð½Ð¾Ð²Ð¾Ðº Ñ ÑÐ¿Ð¾ÑÑÑÐ¼ÐµÐ½Ð¾Ð² Ð²Ð¾ Ð²Ð·Ð°Ð¸Ð¼Ð¾ÑÐ²ÑÐ·Ð¸ Ñ ÐºÐ¾Ð¿Ð¸Ð½Ð³-ÑÑÑÐ°ÑÐµÐ³Ð¸ÑÐ¼Ð¸, Ð¿Ð¾Ð¼Ð¾Ð³Ð°ÑÑÐ¸Ð¼Ð¸ ÑÐ¿Ð¾ÑÑÑÐ¼ÐµÐ½Ð°Ð¼ Ð¿ÑÐµÐ¾Ð´Ð¾Ð»ÐµÐ²Ð°ÑÑ ÑÐ¸ÑÑÐ°ÑÐ¸Ñ Ð¿Ð°Ð½Ð´ÐµÐ¼Ð¸Ð¸ Â«COVID-19Â». ÐÑÐ»Ð¸ Ð²ÑÑÐ²Ð»ÐµÐ½Ñ Â«ÑÐµÑÑÑÑÐ½ÑÐµÂ» Ð¸ Â«Ð¾Ð³ÑÐ°Ð½Ð¸ÑÐ¸Ð²Ð°ÑÑÐ¸ÐµÂ» ÑÑÑÐ°Ð½Ð¾Ð²ÐºÐ¸ ÑÐ¿Ð¾ÑÑÑÐ¼ÐµÐ½Ð¾Ð², ÑÑÑÐ°Ð½Ð¾Ð²Ð»ÐµÐ½Ð° Ð¸Ñ ÑÐ²ÑÐ·Ñ Ñ ÐºÐ¾Ð³Ð½Ð¸ÑÐ¸Ð²Ð½ÑÐ¼Ð¸ Ð¸ÑÐºÐ°Ð¶ÐµÐ½Ð¸ÑÐ¼Ð¸. ÐÐ¾ÐºÐ°Ð·Ð°Ð½Ñ Ð¿ÑÑÐ¸ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð°Ð´Ð°Ð¿ÑÐ¸Ð²Ð½ÑÑ ÐºÐ¾Ð¿Ð¸Ð½Ð³-ÑÑÑÐ°ÑÐµÐ³Ð¸Ð¹.
description: The article presents the results of a study of irrational attitudes in athletes in connection with coping strategies that help athletes overcome the situation of the COVID-19 pandemic. The âresourceâ and âlimitingâ attitudes of athletes were identified, their connection with cognitive distortions was established. The ways of formation of adaptive coping strategies are shown.
A Search for B+ -> tau+ nu Recoiling Against B- -> D0 l- nu X
Creators: name: The BABAR Collaboration
name: Aubert, B.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: We present a search for the decay $B^+ \to \ell^+ ν_{\ell}$ ($\ell = e,μτ$) in $(458.9 \pm 5.1) \times 10^6$ $B\bar{B}$ pairs recorded with the BABAR detector at the PEP-II B-Factory. We search for these B decays in a sample of $B^+B^-$ events where one $B$-meson is reconstructed as $B^- \to D^0 \ell^- νX$. Using the method of Feldman and Cousins, we obtain $\mathcal{B}(B^+ \to τ^+ ν) = (1.7 \pm 0.8 \pm 0.2) \times 10^{-4}$, which excludes zero at $2.3σ$. We interpret the central value in the context of the Standard Model and find the B meson decay constant to be $f^2_B = (62 \pm 31) \times 10^3 \mathrm{MeV}^2$. We find no evidence for $B^+ \to e^+ ν_{e}$ and $B^+ \to μ^+ ν_μ$ and set upper limits at the 90% C.L. $\mathcal{B}(B^+ \to e^+ ν_{e}) < 0.8 \times 10^{-5}$ and $\mathcal{B}(B^+ \to μ^+ ν_μ) < 1.1 \times 10^{-5}$.
description: 8 pages, 8 postscript figures, submitted to Physical Review D (Rapid Communications)
title: ÐÐ½ÐµÐ²Ð¼Ð°ÑÐ¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ´Ð°ÑÐ½ÑÐ¹ ÑÑÐµÐ½Ð´ Ð¡ÐÐ£800
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¼Ð°Ð³Ð¸ÑÑÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¾Ð¿Ð°ÑÐ¸Ð½Ð°, ÐÐºÐ°ÑÐµÑÐ¸Ð½Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: ÐÐ½ÐµÐ²Ð¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ðµ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ
ÐÐ½ÐµÐ²Ð¼Ð°ÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¿ÑÐ¸Ð²Ð¾Ð´Ñ
ÐÑÐ¿ÑÑÐ°ÑÐµÐ»ÑÐ½ÑÐµ ÑÑÐµÐ½Ð´Ñ
Ð£Ð´Ð°Ñ (Ð¼ÐµÑ .)

description: ÐÐ°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐµ Ð¿Ð½ÐµÐ²Ð¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ´Ð°ÑÐ½Ð¾Ð³Ð¾ ÑÑÐµÐ½Ð´Ð° Ð¡ÐÐ£800. ÐÑÐ¾Ð²ÐµÐ´ÑÐ½ Ð°Ð½Ð°Ð»Ð¸ÑÐ¸ÑÐµÑÐºÐ¸Ð¹ Ð¾Ð±Ð·Ð¾Ñ ÑÐ´Ð°ÑÐ½ÑÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°ÑÐµÐ»ÑÑÐºÐ¸Ñ ÑÑÐµÐ½Ð´Ð¾Ð². ÐÑÐ±ÑÐ°Ð½Ð° ÐºÐ¸Ð½ÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ°Ñ ÑÑÐµÐ¼Ð° ÑÐ´Ð°ÑÐ½Ð¾Ð¹ Ð¼Ð°ÑÐ¸Ð½Ñ. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½Ñ ÑÐ°ÑÑÐµÑÑ Ð¸ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¿Ð¾ ÑÐ¸Ð½ÑÐµÐ·Ñ Ð¸ Ð¾Ð¿ÑÐ¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÐ°Ð±Ð¾ÑÑ Ð¿Ð½ÐµÐ²Ð¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ. ÐÑÐ²ÐµÐ´ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð·Ð°Ð²Ð¸ÑÐ¸Ð¼Ð¾ÑÑÐ¸, ÑÐ²ÑÐ·ÑÐ²Ð°ÑÑÐ¸Ðµ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÑ Ð½Ð°ÑÑÑÐ¾Ð¹ÐºÐ¸ ÑÑÐµÐ½Ð´Ð° Ñ Ð·Ð°Ð´Ð°Ð½Ð½ÑÐ¼Ð¸ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÐ°Ð¼Ð¸ Ð¸Ð¼Ð¿ÑÐ»ÑÑÐ°.
Leptogenesis in a model with Friedberg-Lee symmetry
Creators: name: Araki, Takeshi
name: Geng, C. Q.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We study the matter-antimatter asymmetry through the leptogenesis mechanism in a specific model with the Friedberg-Lee (FL) symmetry.We relate the leptogenesis with the CP violating Dirac and Majorana phases in the Maki-Nakagawa-Sakata leptonic mixing matrix and illustrate the net baryon asymmetry of the universe in terms of these phases.
description: 14 pages, 8 figures. v2: typos corrected, minor changes, accepted version in PLB
title: ÐÐ½Ð°Ð»Ð¸Ð· ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹ Ð¿Ð¾ ÑÐ»ÑÑÑÐµÐ½Ð¸Ñ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð³Ð¾ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ñ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¾Ð±ÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿Ð¸ÑÐ°Ð½Ð¸Ñ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÑÐµÑÑÐ¾ÑÐ°Ð½Ð° Â«ÐÐ½ÐµÐ·Ð´Ð¾Â»)
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ²Ð°Ð½Ð¾Ð²Ð°, ÐÐºÐ°ÑÐµÑÐ¸Ð½Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2016
Subjects: ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ðµ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ðµ
Ð°Ð½Ð°Ð»Ð¸Ð·
Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÑÑÑÐºÑÑÑÐ°
ÑÐµÑÑÐ¾ÑÐ°Ð½
ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÐµ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸
financial state
analysis
organizational structure
restaurant
financial performance

description: Ð¦ÐµÐ»ÑÑ Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ðµ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÑ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¾Ð² Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð½Ð¾Ð²Ð¾Ð³Ð¾ ÑÐµÑÑÐ¾ÑÐ°Ð½Ð° Â«ÐÐ½ÐµÐ·Ð´Ð¾Â», Ð²ÑÑÐ²Ð»ÐµÐ½Ð¸Ðµ ÑÐ»Ð°Ð±ÑÑ ÑÑÐ¾ÑÐ¾Ð½ Ð´Ð°Ð½Ð½Ð¾Ð³Ð¾ Ð·Ð°Ð²ÐµÐ´ÐµÐ½Ð¸Ñ, Ð° ÑÐ°ÐºÐ¶Ðµ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¼ÐµÑ Ð¿Ð¾ Ð¸Ñ Ð»Ð¸ÐºÐ²Ð¸Ð´Ð°ÑÐ¸Ð¸. Ð Ð°Ð±Ð¾ÑÐ° ÑÐ¾ÑÑÐ¾Ð¸Ñ Ð¸Ð· ÑÑÐµÑ Ð³Ð»Ð°Ð². Ð Ð¿ÐµÑÐ²Ð¾Ð¹ Ð³Ð»Ð°Ð²Ðµ Ð¿ÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½ ÑÑÐ½Ð¾Ðº Ð¾Ð±ÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿Ð¸ÑÐ°Ð½Ð¸Ñ Ð² Ð Ð¾ÑÑÐ¸Ð¸, Ð° ÑÐ°ÐºÐ¶Ðµ Ð°ÑÐ³ÑÐ¼ÐµÐ½ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð° Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼Ð¾ÑÑÑ Ð¸ Ð²Ð°Ð¶Ð½Ð¾ÑÑÑ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð³Ð¾ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸.ÐÐ¾ Ð²ÑÐ¾ÑÐ¾Ð¹ Ð³Ð»Ð°Ð²Ðµ Ð´Ð°Ð½Ð° Ð¾Ð±ÑÐ°Ñ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ° Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÑÐµÐ¼Ð¾Ð³Ð¾ ÑÐµÑÑÐ¾ÑÐ°Ð½Ð°, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ ÐµÐ³Ð¾ Ð¿Ð¾Ð»Ð½ÑÐ¹ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð·. Ð¢ÑÐµÑÑÑ Ð³Ð»Ð°Ð²Ð° Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° ÑÑÐ°Ð²Ð½Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð¼Ñ Ð°Ð½Ð°Ð»Ð¸Ð·Ñ ÑÐµÑÑÐ¾ÑÐ°Ð½Ð° Â«ÐÐ½ÐµÐ·Ð´Ð¾Â» Ñ Ð°Ð½Ð°Ð»Ð¾Ð³Ð¸ÑÐ½ÑÐ¼ ÑÐµÑÑÐ¾ÑÐ°Ð½Ð¾Ð¼-ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ¾Ð¼, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¿Ð¾Ð´Ð²ÐµÐ´ÐµÐ½Ð¸Ñ Ð¸ÑÐ¾Ð³Ð¾Ð² Ð¾ÑÐ½Ð¾ÑÐ¸ÑÐµÐ»ÑÐ½Ð¾ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð³Ð¾ Ð¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ ÑÐµÑÑÐ¾ÑÐ°Ð½Ð° Â«ÐÐ½ÐµÐ·Ð´Ð¾Â» Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐµ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¹ Ð¿Ð¾ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÑ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»ÐµÐ¹.
description: The purpose of this work is carrying out the analysis of financial results of activity of new restaurant "Gnezdo", detection of weaknesses of this institution, and also development of measures for their elimination. Work consists of three heads. In chapter 1 the market of public catering in Russia is analysed, and also need and importance of carrying out the financial analysis at the enterprise is reasoned. In chapter 2 the general characteristic of the analyzed restaurant is given, and also the full financial analysis is carried out it. The chapter 3 of this work is devoted to the comparative analysis of Gnezdo restaurant with similar rival restaurant, and also to summing up rather financial position of Gnezdo restaurant and development of recommendations about increase of financial performance.
Comatricha pulchella Rostaf.
Creators: name: Kluša, Julita
Publisher: name: Zenodo
Year: 2023
Subjects: Biodiversity
Taxonomy
Protozoa
Mycetozoa
Myxomycetes
Stemonitidales
Stemonitidaceae
Comatricha
Comatricha pulchella

description: ● Comatricha pulchella (C. Bab.) Rostaf.,
glītā kocīte
- leg. J.Kluša, 19 Sep 2022, Zebrene p., on a log of Quercus robur in a deciduous forest, det. J.Kluša, conf. E.Johannesen, 2022; (NMKK), very rare.
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
Consistency criteria for generalized Cuddeford systems
Creators: name: Ciotti, Luca
name: Morganti, Lucia
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: General criteria to check the positivity of the distribution function (phase-space consistency) of stellar systems of assigned density and anisotropy profile are useful starting points in Jeans-based modeling. Here we substantially extend previous results, and we present the inversion formula and the analytical necessary and sufficient conditions for phase-space consistency of the family of multi-component Cuddeford spherical systems: the distribution function of each density component of these systems is defined as the sum of an arbitrary number of Cuddeford distribution functions with arbitrary values of the anisotropy radius, but identical angular momentum exponent. The radial trend of anisotropy that can be realized by these models is therefore very general. As a surprising by-product of our study, we found that the ``central cusp-anisotropy theorem'' (a necessary condition for consistency relating the values of the central density slope and of the anisotropy parameter) holds not only at the center, but at all radii in consistent multi-component generalized Cuddeford systems. This last result suggests that the so--called mass--anisotropy degeneracy could be less severe than what is sometimes feared.
description: Comments: 8 pages, 3 figures, accepted by MNRAS
title: ÐÑÐ¿ÐµÐºÑÑ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»ÐµÐ¹ ÐºÐ°ÑÐµÑÑÐ²Ð° Ð°Ð²ÑÐ¾Ð¼Ð¾Ð±Ð¸Ð»Ñ Tata Nano Ð¿ÑÐ¸ Ð¾Ð¿ÑÐ¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ð¸ ÐµÐ³Ð¾ ÑÑÐ¾Ð¸Ð¼Ð¾ÑÑÐ¸
Creators: name: ÐÐµÐ±ÐµÐ´ÐµÐ²Ð°, Ð¢Ð°ÑÑÑÐ½Ð°
name: ÐÐµÐ´Ð¾Ð²ÑÐºÐ°Ñ, Ð®Ð»Ð¸Ñ
name: Ð¤Ð¸Ð»Ð¸Ð¼Ð¾ÑÐ¸Ð½Ð°, ÐÐ»ÐµÐºÑÐ°Ð½Ð´ÑÐ°
name: "Ð£Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ ÐºÐ°ÑÐµÑÑÐ²Ð¾Ð¼ Ð² Ð¸Ð½ÑÐµÑÐµÑÐ°Ñ  ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾Ð³Ð¾ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ", Ð¼ÐµÐ¶Ð²ÑÐ·Ð¾Ð²ÑÐºÐ°Ñ Ð½Ð°ÑÑÐ½Ð¾-Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ°Ñ ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ñ (2019; Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³)
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2019

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÑÐ°ÑÑÐµ Ð¾ÑÐ²ÐµÑÐ°ÑÑÑÑ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐµÑÐµÐ½Ð¸Ñ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ Tata MOTORS, Ð²ÑÐ¿ÑÑÑÐ¸Ð²ÑÐµÐ¹ ÑÐ°Ð¼ÑÐ¹ Ð´ÐµÑÐµÐ²ÑÐ¹ Ð² Ð¼Ð¸ÑÐµ Ð°Ð²ÑÐ¾Ð¼Ð¾Ð±Ð¸Ð»Ñ Tata Nano. Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÑÐ°ÑÑÐµ ÑÐ°ÐºÐ¶Ðµ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐµÑÐµÐ½Ð¸Ñ, ÐºÐ¾ÑÐ¾ÑÑÐµ Ð¿Ð¾Ð·Ð²Ð¾Ð»Ð¸Ð»Ð¸ Ð´Ð¾Ð±Ð¸ÑÑÑÑ ÑÑÐ¾Ð»Ñ Ð½Ð¸Ð·ÐºÐ¾Ð¹ ÑÑÐ¾Ð¸Ð¼Ð¾ÑÑÐ¸ ÑÑÐ°Ð½ÐºÐ°. Ð¡ÑÐ°Ð²Ð½Ð¸ÑÐµÐ»ÑÐ½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ¸ ÐÐ½Ð´Ð¸Ð¸ (Ð´Ð¾ Ð¸ Ð¿Ð¾ÑÐ»Ðµ Ð²ÑÐ¿ÑÑÐºÐ° Ð°Ð²ÑÐ¾Ð¼Ð¾Ð±Ð¸Ð»Ñ Ð½Ð° ÑÑÐ½Ð¾Ðº). Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½ Ð²Ð¾Ð¿ÑÐ¾Ñ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ Tata Nano Ð½Ð° ÑÐ¾ÑÑÐ¸Ð¹ÑÐºÐ¸Ð¹ ÑÑÐ½Ð¾Ðº. Ð ÑÐ°ÐºÐ¶Ðµ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ñ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½ÑÐµ Ð¸Ð·Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ Ð½ÐµÐºÐ¾ÑÐ¾ÑÑÑ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ñ Ð¼ÐµÑÐ°Ð½Ð¸Ð·Ð¼Ð¾Ð² ÑÑÐ°Ð½ÐºÐ°, Ð² ÑÐ°Ð¼ÐºÐ°Ñ Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÐ½Ð½Ð¾Ð¹ Ð²ÑÑÐµ ÑÑÐ¾Ð¸Ð¼Ð¾ÑÑÐ¸.
Dissecting the region of 3EG J1837-0423 and HESS J1841-055 with INTEGRAL
Creators: name: Sguera, V.
name: Romero, G. E.
name: Bazzano, A.
name: Masetti, N.
name: Bird, A. J.
name: Bassani, L.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: 3EG J1837-0423 and HESS J1841-055 are two unidentified and peculiar high-energy sources located in the same region of the sky, separated by 1.4 deg. Specifically, 3EG J1837-0423 is a transient MeV object detected by EGRET only once during flaring activity that lasted a few days while HESS J1841-055 is a highly extended TeV source. We attempted to match the high-energy emission from the unidentified sources 3EG J1837-0423 and HESS J1841-055 with X-rays (4-20 keV) and soft gamma-rays (20-100 keV) candidate counterparts detected through deep INTEGRAL observations of the sky region. As a result we propose the SFXT AX J1841.0-0536 as a possible candidate counterpart of 3EG J1837-0423, based on spatial proximity and transient behavior. Alternatively, AX J1841.0-0536 could be responsible for at least a fraction of the entire TeV emission from the extended source HESS J1841-055, based on a striking spatial correlation. In either case, the proposed association is also supported from an energetic standpoint by a theoretical scenario where AX J1841.0-0536 is a low magnetized pulsar which, due to accretion of massive clumps from the supergiant companion donor star, undergoes sporadic changes to transient Atoll-states where a magnetic tower can produce transient jets and as a consequence high-energy emission. In either case (by association with 3EG J1837-0423 or alternatively with HESS J1841-055), AX J1841.0-0536 might be the prototype of a new class of Galactic transient MeV/TeV emitters.
description: Accepted for publication in ApJ, 30 pages, 5 figures
Some Remarks on the Model Theory of Epistemic Plausibility Models
Creators: name: Demey, Lorenz
Publisher: name: arXiv
Year: 2010
Subjects: subject: Logic in Computer Science (cs.LO)
subject: FOS: Computer and information sciences
subject: F.4.1
subject: 03B42

description: Classical logics of knowledge and belief are usually interpreted on Kripke models, for which a mathematically well-developed model theory is available. However, such models are inadequate to capture dynamic phenomena. Therefore, epistemic plausibility models have been introduced. Because these are much richer structures than Kripke models, they do not straightforwardly inherit the model-theoretical results of modal logic. Therefore, while epistemic plausibility structures are well-suited for modeling purposes, an extensive investigation of their model theory has been lacking so far. The aim of the present paper is to fill exactly this gap, by initiating a systematic exploration of the model theory of epistemic plausibility models. Like in 'ordinary' modal logic, the focus will be on the notion of bisimulation. We define various notions of bisimulations (parametrized by a language L) and show that L-bisimilarity implies L-equivalence. We prove a Hennesy-Milner type result, and also two undefinability results. However, our main point is a negative one, viz. that bisimulations cannot straightforwardly be generalized to epistemic plausibility models if conditional belief is taken into account. We present two ways of coping with this issue: (i) adding a modality to the language, and (ii) putting extra constraints on the models. Finally, we make some remarks about the interaction between bisimulation and dynamic model changes.
description: 19 pages, 3 figures
title: CÐ±Ð¾ÑÐ½Ð¸Ðº ÑÑÑÐ´Ð¾Ð² Ð½Ð°ÑÑÐ½Ð¾-Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ð¸ Â«ÐÐºÑÑÐ°Ð»ÑÐ½ÑÐµ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ Ð²ÐµÑÐµÑÐ¸Ð½Ð°ÑÐ½Ð¾Ð¹ Ð¼ÐµÐ´Ð¸ÑÐ¸Ð½Ñ, Ð·Ð¾Ð¾ÑÐµÑ Ð½Ð¸Ð¸, Ð±Ð¸Ð¾ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð¸ ÑÐºÑÐ¿ÐµÑÑÐ¸Ð·Ñ ÑÑÑÑÑ Ð¸ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¾Ð² Ð¶Ð¸Ð²Ð¾ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐ¾Ð¸ÑÑ Ð¾Ð¶Ð´ÐµÐ½Ð¸ÑÂ»
Creators: name: ÐÐºÑÑÐ°Ð»ÑÐ½ÑÐµ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ Ð²ÐµÑÐµÑÐ¸Ð½Ð°ÑÐ½Ð¾Ð¹ Ð¼ÐµÐ´Ð¸ÑÐ¸Ð½Ñ, Ð·Ð¾Ð¾ÑÐµÑ Ð½Ð¸Ð¸, Ð±Ð¸Ð¾ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð¸ ÑÐºÑÐ¿ÐµÑÑÐ¸Ð·Ñ ÑÑÑÑÑ Ð¸ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¾Ð² Ð¶Ð¸Ð²Ð¾ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐ¾Ð¸ÑÑ Ð¾Ð¶Ð´ÐµÐ½Ð¸Ñ, Ð½Ð°ÑÑÐ½Ð¾-Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ°Ñ ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ñ (2022; ÐÐ¾ÑÐºÐ²Ð°)
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Ð¸Ð¾ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ñ
Ð²ÐµÑÐµÑÐ¸Ð½Ð°ÑÐ½Ð°Ñ Ð¼ÐµÐ´Ð¸ÑÐ¸Ð½Ð°
Ð·Ð¾Ð¾ÑÐµÑ Ð½Ð¸Ñ
ÑÐºÑÐ¿ÐµÑÑÐ¸Ð·Ð° ÑÑÑÑÑ
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description: Ð ÑÐ±Ð¾ÑÐ½Ð¸ÐºÐµ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ Ð½Ð°ÑÑÐ½ÑÐµ ÑÑÐ°ÑÑÐ¸ ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ð¸ Â«ÐÐºÑÑÐ°Ð»ÑÐ½ÑÐµ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ Ð²ÐµÑÐµÑÐ¸Ð½Ð°ÑÐ½Ð¾Ð¹ Ð¼ÐµÐ´Ð¸ÑÐ¸Ð½Ñ, Ð·Ð¾Ð¾ÑÐµÑÐ½Ð¸Ð¸, Ð±Ð¸Ð¾ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð¸ ÑÐºÑÐ¿ÐµÑÑÐ¸Ð·Ñ ÑÑÑÑÑ Ð¸ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¾Ð² Ð¶Ð¸Ð²Ð¾ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐ¾Ð¸ÑÑÐ¾Ð¶Ð´ÐµÐ½Ð¸ÑÂ» (ÐÐ¾ÑÐºÐ²Ð°, 8 Ð½Ð¾ÑÐ±ÑÑ 2022 Ð³.). ÐÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð½ÑÐµ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ñ Ð¾ÑÑÐ°Ð¶Ð°ÑÑ Ð´Ð¾ÑÑÐ¸Ð¶ÐµÐ½Ð¸Ñ Ð² Ð¾Ð±Ð»Ð°ÑÑÐ¸ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¾Ð¹ Ð¸ Ð¿ÑÐ¸ÐºÐ»Ð°Ð´Ð½Ð¾Ð¹ Ð½Ð°ÑÐºÐ¸ Ð°Ð³ÑÐ¾Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½Ð¾Ð³Ð¾ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ°. Ð¡Ð±Ð¾ÑÐ½Ð¸Ðº ÑÑÑÐ´Ð¾Ð² ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð¾Ð²Ð°Ð½ Ð´Ð»Ñ Ð½Ð°ÑÑÐ½ÑÑ ÑÐ¾ÑÑÑÐ´Ð½Ð¸ÐºÐ¾Ð², Ð°ÑÐ¿Ð¸ÑÐ°Ð½ÑÐ¾Ð² Ð¸ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð²
Ð²ÑÑÑÐ¸Ñ ÑÑÐµÐ±Ð½ÑÑ ÑÑÑÐµÐ¶Ð´ÐµÐ½Ð¸Ð¹ Ð·Ð¾Ð¾Ð²ÐµÑÐµÑÐ¸Ð½Ð°ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÑÐ¸Ð»Ñ, ÑÐ¾ÑÑÑÐ´Ð½Ð¸ÐºÐ¾Ð² Ð½Ð°ÑÑÐ½Ð¾-Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°ÑÐµÐ»ÑÑÐºÐ¸Ñ Ð¸Ð½ÑÑÐ¸ÑÑÑÐ¾Ð² Ð¸ ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸ÑÑÐ¾Ð² ÐÐÐ.
Steps in marker assisted selection to develop new cultivars
Creators: name: Ferreira, Juan Jose
name: García-Fernández, Carmen
name: Campa, Ana
Publisher: name: Zenodo
Year: 2021
Subjects: snap bean, plant breeding, marker assisted selection, introgression,

description: This gif shows the steps in marker assisted selection to develop new cultivars. This task is developed for disease resistance introgression in elite snap bean cultivars. Resistant cultivars are better adapted to organic farming A dissemination task developed by the Plant Genetic Group (SERIDA) for the BRESOV project. This work is part of the BRESOV project funded by the EU (Grant agreement ID: 774244).
The VOISE Algorithm: a Versatile Tool for Automatic Segmentation of Astronomical Images
Creators: name: Guio, P.
name: Achilleos, N.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Computer Vision and Pattern Recognition (cs.CV)
subject: Data Analysis, Statistics and Probability (physics.data-an)
subject: Applications (stat.AP)
subject: FOS: Physical sciences
subject: FOS: Computer and information sciences

description: The auroras on Jupiter and Saturn can be studied with a high sensitivity and resolution by the Hubble Space Telescope (HST) ultraviolet (UV) and far-ultraviolet (FUV) Space Telescope spectrograph (STIS) and Advanced Camera for Surveys (ACS) instruments. We present results of automatic detection and segmentation of Jupiter's auroral emissions as observed by HST ACS instrument with VOronoi Image SEgmentation (VOISE). VOISE is a dynamic algorithm for partitioning the underlying pixel grid of an image into regions according to a prescribed homogeneity criterion. The algorithm consists of an iterative procedure that dynamically constructs a tessellation of the image plane based on a Voronoi Diagram, until the intensity of the underlying image within each region is classified as homogeneous. The computed tessellations allow the extraction of quantitative information about the auroral features such as mean intensity, latitudinal and longitudinal extents and length scales. These outputs thus represent a more automated and objective method of characterising auroral emissions than manual inspection.
description: 9 pages, 7 figures; accepted for publication in MNRAS
The Prospect of Marketing Strategies in the Survival of Private Business in Cross River State 08-May-2023 16-58-11.pdf
Creators: name: Obo, Ekpenyong  Bassey
Publisher: name: figshare
Year: 2023
Subjects: Marketing communications
Marketing management (incl. strategy and customer relations)
Service marketing

description: The study examined the importance and performance of marketing strategies in the survival of the private businesses, and to determine whether and to what extent marketing strategies were at work, with emphasize on consumer and industrial goods business organizations. The study employed independent t-test analysis method attached to it
The JCMT Nearby Galaxies Legacy Survey I. Star Forming Molecular Gas in Virgo Cluster Spiral Galaxies
Creators: name: Wilson, C. D.
name: Warren, B. E.
name: Israel, F. P.
name: Serjeant, S.
name: Bendo, G.
name: Brinks, E.
name: Clements, D.
name: Courteau, S.
name: Irwin, J.
name: Knapen, J. H.
name: Leech, J.
name: Matthews, H. E.
name: Muehle, S.
name: Mortier, A. M. J.
name: Petitpas, G.
name: Sinukoff, E.
name: Spekkens, K.
name: Tan, B. K.
name: Tilanus, R. P. J.
name: Usero, A.
name: van der Werf, P.
name: Wiegert, T.
name: Zhu, M.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present large-area maps of the CO J=3-2 emission obtained at the James Clerk Maxwell Telescope for four spiral galaxies in the Virgo Cluster. We combine these data with published CO J=1-0, 24 micron, and Halpha images to measure the CO line ratios, molecular gas masses, and instantaneous gas depletion times. For three galaxies in our sample (NGC 4254, NGC4321, and NGC 4569), we obtain molecular gas masses of 7E8-3E9 Msun and disk-averaged instantaneous gas depletion times of 1.1-1.7 Gyr. We argue that the CO J=3-2 line is a better tracer of the dense star forming molecular gas than the CO J=1-0 line, as it shows a better correlation with the star formation rate surface density both within and between galaxies. NGC 4254 appears to have a larger star formation efficiency(smaller gas depletion time), perhaps because it is on its first passage through the Virgo Cluster. NGC 4569 shows a large-scale gradient in the gas properties traced by the CO J=3-2/J=1-0 line ratio, which suggests that its interaction with the intracluster medium is affecting the dense star-forming portion of the interstellar medium directly. The fourth galaxy in our sample, NGC 4579, has weak CO J=3-2 emission despite having bright 24 micron emission; however, much of the central luminosity in this galaxy may be due to the presence of a central AGN.
description: Comments: 30 pages, 18 figures, aastex preprint formation; accepted to ApJ. Version of paper with full resolution figures available at http://www.physics.mcmaster.ca/~wilson/www_xfer/NGLS_public/wilson2008.pdf
title: ÐÐ°ÑÐµÑÐ¸Ð°Ð»Ñ 2-Ð¹ ÐÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½Ð¾Ð¹ Ð½Ð°ÑÑÐ½Ð¾-Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ð¸ Â«ÐÐ¾Ð»ÐµÐºÑÐ»ÑÑÐ½Ð¾-Ð³ÐµÐ½ÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð´Ð»Ñ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° ÑÐºÑÐ¿ÑÐµÑÑÐ¸Ð¸ Ð³ÐµÐ½Ð¾Ð² Ð¿ÑÐ¾Ð´ÑÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¸ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÐ¸ Ðº Ð·Ð°Ð±Ð¾Ð»ÐµÐ²Ð°Ð½Ð¸ÑÐ¼ Ð¶Ð¸Ð²Ð¾ÑÐ½ÑÑ Â»
title: 25 Ð´ÐµÐºÐ°Ð±ÑÑ 2020 Ð³.
titleType: Subtitle
Creators: name: "ÐÐ¾Ð»ÐµÐºÑÐ»ÑÑÐ½Ð¾-Ð³ÐµÐ½ÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð´Ð»Ñ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° ÑÐºÑÐ¿ÑÐµÑÑÐ¸Ð¸ Ð³ÐµÐ½Ð¾Ð² Ð¿ÑÐ¾Ð´ÑÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¸ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÐ¸ Ðº Ð·Ð°Ð±Ð¾Ð»ÐµÐ²Ð°Ð½Ð¸ÑÐ¼ Ð¶Ð¸Ð²Ð¾ÑÐ½ÑÑ ", Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½Ð°Ñ Ð½Ð°ÑÑÐ½Ð¾-Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ°Ñ ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ñ (2; 2020; ÐÐ¾ÑÐºÐ²Ð°)
Publisher: name: Ð¡ÐµÐ»ÑÑÐºÐ¾ÑÐ¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½ÑÐµ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸
Year: 2020
Subjects: Ð¿ÑÐ¸ÑÐµÐ²Ð¾Ð´ÑÑÐ²Ð¾
Ð±Ð¾Ð»ÐµÐ·Ð½Ð¸ Ð¿ÑÐ¸Ñ

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Ð¡Ð±Ð¾ÑÐ½Ð¸Ðº Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð¾Ð² ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð¾Ð²Ð°Ð½ Ð´Ð»Ñ Ð½Ð°ÑÑÐ½ÑÑ ÑÐ¾ÑÑÑÐ´Ð½Ð¸ÐºÐ¾Ð², Ð°ÑÐ¿Ð¸ÑÐ°Ð½ÑÐ¾Ð² Ð¸ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð²ÑÑÑÐ¸Ñ ÑÑÐµÐ±Ð½ÑÑ ÑÑÑÐµÐ¶Ð´ÐµÐ½Ð¸Ð¹ Ð·Ð¾Ð¾Ð²ÐµÑÐµÑÐ¸Ð½Ð°ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÑÐ¸Ð»Ñ, ÑÐ¾ÑÑÑÐ´Ð½Ð¸ÐºÐ¾Ð² Ð½Ð°ÑÑÐ½Ð¾-Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°ÑÐµÐ»ÑÑÐºÐ¸Ñ Ð¸Ð½ÑÑÐ¸ÑÑÑÐ¾Ð² Ð¸ ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸ÑÑÐ¾Ð² ÐÐÐ.
title: ÐÐ¿ÐµÑÐ°ÑÐ¸Ð²Ð½Ð¾Ðµ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð±Ð¸Ð·Ð½ÐµÑ-Ð¿ÑÐ¾ÑÐµÑÑÐ°Ð¼Ð¸
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐ°ÐºÐ°ÑÐ¾Ð², ÐÐ°ÑÐ¸Ð»Ð¸Ð¹
name: ÐÐµÐ²ÐµÐ½ÑÐ¾Ð², ÐÐ°Ð»ÐµÑÐ¸Ð¹
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2009
Subjects: ÐÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½ÑÐµ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ
Ð¼ÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½Ñ
Ð±Ð¸Ð·Ð½ÐµÑ-Ð¿ÑÐ¾ÑÐµÑÑÑ
ÑÑÐµÐ±Ð½Ð¸ÐºÐ¸ Ð¸ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Ð´Ð»Ñ Ð²ÑÐ·Ð¾Ð²

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title: ÐÐ°ÑÐµÐ¼Ð°ÑÐ¸ÐºÐ°. ÐÑÐ¿. 2, ÐÐ²ÐµÐ´ÐµÐ½Ð¸Ðµ Ð² Ð¼Ð°ÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ¸Ð¹ Ð°Ð½Ð°Ð»Ð¸Ð·. ÐÐ¸ÑÑÐµÑÐµÐ½ÑÐ¸Ð°Ð»ÑÐ½Ð¾Ðµ Ð¸ÑÑÐ¸ÑÐ»ÐµÐ½Ð¸Ðµ ÑÑÐ½ÐºÑÐ¸Ð¸ Ð¾Ð´Ð½Ð¾Ð¹ Ð¿ÐµÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð¹
title: Ð¾Ð¿Ð¾ÑÐ½ÑÐ¹ ÐºÐ¾Ð½ÑÐ¿ÐµÐºÑ
titleType: Subtitle
Creators: name: ÐÐ¾Ð±ÐºÐ¾Ð²Ð°, ÐÐ°ÑÐ°Ð»ÑÑ
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2009
Subjects: Ð¤ÑÐ½ÐºÑÐ¸Ð¸ (Ð¼Ð°Ñ.) Ð´ÐµÐ¹ÑÑÐ²Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð¿ÐµÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð³Ð¾
Ð¤ÑÐ½ÐºÑÐ¸Ð¸ (Ð¼Ð°Ñ.)
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