cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
A Performance Analysis for UMTS Packet Switched Network Based on Multivariate KPIS
Creators: name: Ouyang, Ye
name: Fallah, M. Hosein
Publisher: name: arXiv
Year: 2010
Subjects: subject: Networking and Internet Architecture (cs.NI)
subject: FOS: Computer and information sciences

description: Mobile data services are penetrating mobile markets rapidly. The mobile industry relies heavily on data service to replace the traditional voice services with the evolution of the wireless technology and market. A reliable packet service network is critical to the mobile operators to maintain their core competence in data service market. Furthermore, mobile operators need to develop effective operational models to manage the varying mix of voice, data and video traffic on a single network. Application of statistical models could prove to be an effective approach. This paper first introduces the architecture of Universal Mobile Telecommunications System (UMTS) packet switched (PS) network and then applies multivariate statistical analysis to Key Performance Indicators (KPI) monitored from network entities in UMTS PS network to guide the long term capacity planning for the network. The approach proposed in this paper could be helpful to mobile operators in operating and maintaining their 3G packet switched networks for the long run.
description: 15 Pages, IJNGN Journal
The magnetic field structure in NGC 253 in presence of a galactic wind
Creators: name: Heesen, V.
name: Krause, M.
name: Beck, R.
name: Dettmar, R. -J.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present radio continuum polarimetry observations of the nearby edge-on galaxy NGC 253 which possesses a very bright radio halo. Using the vertical synchrotron emission profiles and the lifetimes of cosmic-ray electrons, we determined the cosmic-ray bulk speed as (300+/-30) km/s, indicating the presence of a galactic wind in this galaxy. The large-scale magnetic field was decomposed into a toroidal axisymmetric component in the disk and a poloidal component in the halo. The poloidal component shows a prominent X-shaped magnetic field structure centered on the nucleus, similar to the magnetic field observed in other edge-on galaxies. Faraday rotation measures indicate that the poloidal field has an odd parity (antisymmetric). NGC 253 offers the possibility to compare the magnetic field structure with models of galactic dynamos and/or galactic wind flows.
description: 6 pages, 5 figures, in the proceedings of the IAU Symposium 259: "Cosmic magnetic fields: from planets, to stars and galaxies", Teneriffe, November 2008, in press
Additional file 1 of Study of microencapsulated fatty acid antimicrobial activity in vitro and its prevention ability of Clostridium perfringens induced necrotic enteritis in broiler chicken
Creators: name: Qi, Nanshan
name: Liu, Shaobing
name: Yan, Fangquan
name: Chen, Bing
name: Wu, Shilin
name: Lin, Xuhui
name: Yan, Zhuanqiang
name: Zhou, Qingfeng
name: Liao, Shenquan
name: Li, Juan
name: Lv, Minna
name: Cai, Haiming
name: Hu, Junjing
name: Zhang, Jianfei
name: Gu, Youfang
name: Sun, Mingfei
Publisher: name: figshare
Year: 2023
Subjects: subject: Biochemistry
subject: Space Science
subject: Microbiology
subject: FOS: Biological sciences
subject: Pharmacology
subject: Chemical Sciences not elsewhere classified
subject: Immunology
subject: FOS: Clinical medicine
subject: Cancer
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Virology

description: Additional file 1: Table S1. Ingredients and composition of wheat-based diet
Thomas-Fermi scaling in the energy spectra of atomic ions
Creators: name: Carcasses, Robert
name: Gonzalez, Augusto
Publisher: name: arXiv
Year: 2009
Subjects: subject: Atomic Physics (physics.atom-ph)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Other Condensed Matter (cond-mat.other)
subject: FOS: Physical sciences

description: The energy spectra of atomic ions are re-examined from the point of view of Thomas-Fermi scaling relations. For the first ionization potential, which sets the energy scale for the true discrete spectrum, Thomas-Fermi theory predicts the following relation: E_{ioniz}=Z^2 N^{-2/3} g(N/Z), where Z is the nuclear charge, N is the number of electrons, and g is a function of N/Z. This relation does not hold for neutral atoms, but works extremely well in the cationic domain, Z>N. We provide an analytic expression for g, with two adjustable parameters, which fits the available experimental data for more than 380 ions. In addition, we show that a rough fit to the integrated density of states with a single exponential: N_{states}=exp (Delta E/Theta), where Delta E is the excitation energy, leads to a parameter, Theta, exhibiting a universal scaling a la Thomas-Fermi: Theta=Z^2 N^{-4/3} h(N/Z), where h is approximately linear near N/Z=1.
description: published version
Topological Mott insulator in the odd-integer filled Anderson lattice model with Hatsugai-Kohmoto interactions
Creators: name: Jabłonowski, Krystian
name: Skolimowski, Jan
name: Brzezicki, Wojciech
name: Byczuk, Krzysztof
name: Wysokiński, Marcin M.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: Recently, a quantum anomalous Hall state at odd integer filling in moiré stacked MoTe$_2$/WSe$_2$ was convincingly interpreted as a topological Mott insulator state appearing due to strong interactions in {\it band} basis [P. Mai, J. Zhao, B. E. Feldman, and P. W. Phillips, Nat. Commun. {\bf 14}, 5999 (2023)]. In this work, we aim to analyze the formation of a topological Mott insulator due to interactions in {\it orbital} basis instead, being more natural for systems where interactions originate from the character of $f$ or $d$ orbitals rather than band flatness. For that reason, we study an odd-integer filled Anderson lattice model incorporating odd-parity hybridization between orbitals with different degrees of correlations introduced in the Hatsugai-Kohmoto spirit. We demonstrate that a topological Mott insulating state can be realized in a considered model only when weak intra- and inter-orbital correlations involving dispersive states are taken into account. Interestingly, we find that all topological transitions between trivial and topological Mott insulating phases are not accompanied by a spectral gap closing, consistent with a phenomenon called {\it first-order topological transition}. Instead, they are signaled by a kink developed in spectral function at one of the time reversal invariant momenta. We believe that our approach can provide insightful phenomenology of topological Mott insulators in spin-orbit coupled $f$ or $d$ electron systems.
description: 7 pages, 4 figs
Revisiting small-world network models: Exploring technical realizations and the equivalence of the Newman-Watts and Harary models
Creators: name: Son, Seora
name: Choi, Eun Ji
name: Lee, Sang Hoon
Publisher: name: arXiv
Year: 2023
Subjects: subject: Physics and Society (physics.soc-ph)
subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: Discrete Mathematics (cs.DM)
subject: Computation (stat.CO)
subject: FOS: Physical sciences
subject: FOS: Computer and information sciences

description: We address the relatively less known facts on the equivalence and technical realizations surrounding two network models showing the "small-world" property, namely the Newman-Watts and the Harary models. We provide the most accurate (in terms of faithfulness to the original literature) versions of these models to clarify the deviation from them existing in their variants adopted in one of the most popular network analysis packages. The difference in technical realizations of those models could be conceived as minor details, but we discover significantly notable changes caused by the possibly inadvertent modification. For the Harary model, the stochasticity in the original formulation allows a much wider range of the clustering coefficient and the average shortest path length. For the Newman-Watts model, due to the drastically different degree distributions, the clustering coefficient can also be affected, which is verified by our higher-order analytic derivation. During the process, we discover the equivalence of the Newman-Watts (better known in the network science or physics community) and the Harary (better known in the graph theory or mathematics community) models under a specific condition of restricted parity in variables, which would bridge the two relatively independently developed models in different fields. Our result highlights the importance of each detailed step in constructing network models and the possibility of deeply related models, even if they might initially appear distinct in terms of the time period or the academic disciplines from which they emerged.
description: 11 pages, 5 figures, 1 table
title: ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¸ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼ ÑÐ¸ÑÑÐ¾Ð²Ð¾Ð¹ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ¸ Ð² Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐµ Ð² Ð Ð¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð¹ Ð¤ÐµÐ´ÐµÑÐ°ÑÐ¸Ð¸
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¸ÐºÐ¾Ð»Ð°ÐµÐ²Ð°, Ð®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: 2018
Subjects: ÑÐ¸ÑÑÐ¾Ð²Ð°Ñ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ°
Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ°
Ð°Ð½Ð°Ð»Ð¸Ð· Ð´Ð¸Ð½Ð°Ð¼Ð¸ÐºÐ¸
Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ¸ ÑÐ¸Ð½Ð°Ð½ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½ÑÑ ÑÐ¸ÑÑÐµÐ¼

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÑÐ¸ÑÑÐ¾Ð²Ð°Ñ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ° Ð² Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐµ Ð² Ð Ð¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð¹ Ð¤ÐµÐ´ÐµÑÐ°ÑÐ¸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Ð¸ÑÑÐ¾Ð²Ð¾Ð¹ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ¸ Ð² ÑÑÐµÑÐµ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¹, ÑÐ°ÑÑÐµÑÐ° Ð´Ð»Ñ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ñ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½ÑÑ ÑÐ¸ÑÑÐµÐ¼, Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÑÐ½ÐºÐ° Ð±ÐµÑÐ¿Ð¸Ð»Ð¾ÑÐ½Ð¾Ð³Ð¾ ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ°.
Ð ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð° ÐºÑÐ°ÑÐºÐ°Ñ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ° ÑÐ¸ÑÑÐ¾Ð²Ð¾Ð¹ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ¸ Ð² Ð¾Ð±Ð»Ð°ÑÑÐ¸ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¹, Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½ÑÑ ÑÐ¸ÑÑÐµÐ¼ Â«Ð¦Ð¸ÑÑÐ¾Ð²Ð°Ñ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ°Â» Ð¸ Â«Ð­Ð»ÐµÐºÑÑÐ¾Ð½Ð½Ð¾Ðµ Ð¿ÑÐ°Ð²Ð¸ÑÐµÐ»ÑÑÑÐ²Ð¾Â».
ÐÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ñ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»ÐµÐ¹, Ð²Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²Ð° Ð¸ ÑÐ´ÐµÐ»Ð°Ð½Ñ Ð²ÑÐ²Ð¾Ð´Ñ Ð¿Ð¾ Ð½Ð¸Ð¼.
Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð½Ð¾ÑÐ¼Ð°ÑÐ¸Ð²Ð½Ð¾-Ð¿ÑÐ°Ð²Ð¾Ð²ÑÐµ Ð°ÐºÑÑ, ÑÐµÐ³ÑÐ»Ð¸ÑÑÑÑÐ¸Ðµ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½ÑÑ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ Ð² Ð Ð¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð¹ Ð¤ÐµÐ´ÐµÑÐ°ÑÐ¸Ð¸.
title: ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÑÐ½ÐºÐ° Ð¾Ð±Ð»Ð°ÑÐ½ÑÑ ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¹ Ð¸ Ð½ÐµÐ¾Ð±Ñ Ð¾Ð´Ð¸Ð¼Ð¾ÑÑÐ¸ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ Ð² Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¢Ð¡Ð 271
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÑÐ±ÑÐ¾, ÐÐ»ÐµÐºÑÐ°Ð½Ð´ÑÐ°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: ÑÐ¾Ð²Ð°ÑÐ¸ÑÐµÑÑÐ²Ð¾ ÑÐ¾Ð±ÑÑÐ²ÐµÐ½Ð½Ð¸ÐºÐ¾Ð² Ð¶Ð¸Ð»ÑÑ
Ð¶Ð¸Ð»Ð¸ÑÐ½Ð¾-ÐºÐ¾Ð¼Ð¼ÑÐ½Ð°Ð»ÑÐ½Ð¾Ðµ Ñ Ð¾Ð·ÑÐ¹ÑÑÐ²Ð¾
Ð¾Ð±Ð»Ð°ÑÐ½ÑÐµ ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¸
ÑÑÐ°Ð¿Ñ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ

description: Ð¦ÐµÐ»ÑÑ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÑÐ½ÐºÐ° Ð¾Ð±Ð»Ð°ÑÐ½ÑÑ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¹ Ð¸ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼Ð¾ÑÑÐ¸ Ð¸Ñ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ Ð² Ð¢Ð¡Ð 271. ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° ÑÑÐ½ÐºÐ° Ð¾Ð±Ð»Ð°ÑÐ½ÑÑ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¹, Ð±ÑÐ»Ð¸ Ð²ÑÐ±ÑÐ°Ð½Ñ Ð½Ð°Ð¸Ð±Ð¾Ð»ÐµÐµ Ð¿Ð¾Ð´ÑÐ¾Ð´ÑÑÐ¸Ðµ Ð´Ð»Ñ ÑÐ¾Ð²Ð°ÑÐ¸ÑÐµÑÑÐ²Ð° ÑÐ¸ÑÑÐµÐ¼Ñ. Ð Ð°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°Ñ Ð¿Ð¾Ð´ÑÐ¾Ð±Ð½Ð¾ ÐºÐ°Ð¶Ð´ÑÑ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¸ ÑÐ¾Ð¿Ð¾ÑÑÐ°Ð²Ð»ÑÑ Ñ Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼ÑÐ¼ ÑÑÐ½ÐºÑÐ¸Ð¾Ð½Ð°Ð»Ð¾Ð¼ Ð´Ð»Ñ ÑÐ¾Ð²Ð°ÑÐ¸ÑÐµÑÑÐ²Ð°, Ð±ÑÐ»Ð° Ð²ÑÐ±ÑÐ°Ð½Ð° Ð½Ð°Ð¸Ð±Ð¾Ð»ÐµÐµ Ð¿Ð¾Ð´ÑÐ¾Ð´ÑÑÐ°Ñ ÑÐ¸ÑÑÐµÐ¼Ð°, ÐºÐ¾ÑÐ¾ÑÐ°Ñ ÑÐ»ÑÑÑÐ¸Ñ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½ÑÑ ÑÐ²ÑÐ·Ñ Ñ Ð¶Ð¸Ð»ÑÑÐ°Ð¼Ð¸, ÑÐ¾ÐºÑÐ°ÑÐ¸Ñ ÑÐ°Ð±Ð¾ÑÐµÐµ Ð²ÑÐµÐ¼Ñ Ð±ÑÑÐ³Ð°Ð»ÑÐµÑÐ°, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¿ÑÐµÐ´ÑÐµÐ´Ð°ÑÐµÐ»Ñ.
title: Ð£ÑÐµÑ ÑÐ°ÑÑÐµÑÐ¾Ð² Ð¿Ð¾ ÑÐ¾Ð²Ð°ÑÐ½ÑÐ¼ Ð¾Ð¿ÐµÑÐ°ÑÐ¸ÑÐ¼ Ð² ÑÐ¸ÑÑÐµÐ¼Ðµ ÑÐ°ÑÑÐµÑÐ½ÑÑ Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸Ð¹ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÐ¾Ð·Ð½Ð¸ÑÐ½Ð¾Ð¹ ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ð¸
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð¤Ð°Ð¹Ð·ÑÐ»Ð»Ð¸Ð½Ð° , ÐÐ°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: 2016
Subjects: ÑÑÐµÑ ÑÐ°ÑÑÐµÑÐ¾Ð² Ð¿Ð¾ ÑÐ¾Ð²Ð°ÑÐ½ÑÐ¼ Ð¾Ð¿ÐµÑÐ°ÑÐ¸ÑÐ¼

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Ð¾Ð¼ÑÑ - ÐÐµÑÐµÑÐ±ÑÑÐ³Â». ÐÑÐµÐ´Ð¼ÐµÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ - ÑÐµÐ¾ÑÐµÑÐ¸ÐºÐ¾ - Ð¼ÐµÑÐ¾Ð´Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¸ Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð±ÑÑÐ³Ð°Ð»ÑÐµÑÑÐºÐ¾Ð³Ð¾ ÑÑÐµÑÐ° ÑÐ¾Ð²Ð°ÑÐ½ÑÑ Ð¾Ð¿ÐµÑÐ°ÑÐ¸Ð¹ Ð² Ð¾Ð±Ð¾ÑÐ¾Ð±Ð»ÐµÐ½Ð½ÑÑ Ð¿Ð¾Ð´ÑÐ°Ð·Ð´ÐµÐ»ÐµÐ½Ð¸ÑÑ. Ð¦ÐµÐ»Ñ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ: ÑÐ¾ÑÑÐ¾Ð¸Ñ Ð² Ð¸Ð·ÑÑÐµÐ½Ð¸Ð¸ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¸ Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ¸ Ð²ÐµÐ´ÐµÐ½Ð¸Ñ ÑÑÐµÑÐ° ÑÐ°ÑÑÐµÑÐ¾Ð² Ð¿Ð¾ ÑÐ¾Ð²Ð°ÑÐ½ÑÐ¼ Ð¾Ð¿ÐµÑÐ°ÑÐ¸ÑÐ¼ Ð¸ Ð²Ð½ÐµÑÐµÐ½Ð¸Ð¸ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð¸Ð¹ Ð¿Ð¾ Ð¸Ñ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ Ð² ÑÑÐ½Ð¾ÑÐ½ÑÑ ÑÑÐ»Ð¾Ð²Ð¸ÑÑ ÑÐ¾Ð·ÑÐ¹ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ.
Artificial molecular quantum rings under magnetic field influence
Creators: name: Castelano, L. K.
name: Hai, G. -Q.
name: Partoens, B.
name: Peeters, F. M.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: The ground states of few electrons confined in two vertically coupled quantum rings in the presence of an external magnetic field are studied systematically within the current spin-density functional theory. Electron-electron interactions combined with inter-ring tunneling affects the electronic structure and the persistent current. For small values of the external magnetic field, we recover the zero magnetic field molecular quantum ring ground state configurations. Increasing the magnetic field many angular momentum, spin, and iso-spin transitions are predicted to occur in the ground state. We show that these transitions follow certain rules, which are governed by the parity of the number of electrons, the single particle picture, the Hund's rules and many-body effects.
description: accepted for publication in Journal of Applied Physics (in press)
Ferromagnetism and insulating behavior with a logarithmic temperature dependence of resistivity in $Pb_{10-x}Cu_x\left( PO_4 \right) _6O$
Creators: name: Zhang, Yuhang
name: Liu, Cong
name: Zhu, Xiyu
name: Wen, Hai-Hu
Publisher: name: arXiv
Year: 2023
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: Recent claim of discovering above-room-temperature superconductivity (Tc about 400 K) at ambient pressure in copper doped apatite $Pb_{10}\left( PO_4 \right) _6O$ has stimulated world-wide enthusiasm and impulse of motion. A lot of follow-up works have been carried out with controversial conclusions. To check whether superconductivity is really present or absent in the material, we need samples which should have a rather pure phase of $Pb_{10-x}Cu_x\left( PO_4 \right) _6O$. Here we report the characterization results from the $Pb_{10-x}Cu_x\left( PO_4 \right) _6O$ with a fraction of about 97 wt.% inferred from the fitting to the x-ray diffraction pattern. The resistivity measurements show that it is a semiconductor characterized roughly by a ln(1/T) temperature dependence in wide temperature region without trace of superconductivity. Magnetization measurements show that it has a general ferromagnetic signal with a weak superparamagnetic background. Many grains of the sample show clear interactions with a NbFeB magnet. The detected Cu concentration is much lower than the expected nominal one and the conduction may be improved if more Cu atoms are successfully doped into the system. Our results show the absence of metallicity and superconductivity in $Pb_{10-x}Cu_x\left( PO_4 \right) _6O$ at ambient pressure, and suggest the presence of strong correlation effect.
description: 6 Pages,5 figures
title: Ð¡Ð¸ÑÑÐµÐ¼Ð° Ð³Ð¾ÑÑÑÐµÐ³Ð¾ Ð²Ð¾Ð´Ð¾ÑÐ½Ð°Ð±Ð¶ÐµÐ½Ð¸Ñ ÑÑÐµÐ´Ð½ÐµÐ¹ Ð¾Ð±ÑÐµÐ¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾Ð¹ ÑÐºÐ¾Ð»Ñ Ñ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸ÐµÐ¼ ÑÐ¾Ð»Ð½ÐµÑÐ½Ð¾Ð³Ð¾ ÐºÐ¾Ð»Ð»ÐµÐºÑÐ¾ÑÐ° Ð¸ ÑÐµÐ·Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð½Ð°ÐºÐ¾Ð¿Ð¸ÑÐµÐ»Ñ ÑÐµÐ¿Ð»Ð¾ÑÑ
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Ð¸Ð»Ð»Ð¾Ð²Ð°, ÐÐºÐ°ÑÐµÑÐ¸Ð½Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: ÐÐ¾Ð´Ð¾ÑÐ½Ð°Ð±Ð¶ÐµÐ½Ð¸Ðµ Ð³Ð¾ÑÑÑÐµÐµ
Ð¤Ð°Ð·Ð¾Ð²ÑÐµ Ð¿ÐµÑÐµÑ Ð¾Ð´Ñ
ÐÐ°ÐºÐ¾Ð¿Ð¸ÑÐµÐ»Ð¸ ÑÐ½ÐµÑÐ³Ð¸Ð¸
Ð¢ÐµÐ¿Ð»Ð¾ÑÐ½Ð°Ð±Ð¶ÐµÐ½Ð¸Ðµ
Ð¡Ð¾Ð»Ð½ÐµÑÐ½Ð°Ñ ÑÐ½ÐµÑÐ³Ð¸Ñ
ÑÐ¾Ð»Ð½ÐµÑÐ½ÑÐµ ÐºÐ¾Ð»Ð»ÐµÐºÑÐ¾ÑÑ

description: ÐÐ¾ÑÑÑÐ¾ÐµÐ½Ð° Ð¾Ð±ÑÐ°Ñ Ð¼Ð¾Ð´ÐµÐ»Ñ Ð´Ð»Ñ ÑÐ°ÑÑÐµÑÐ° ÑÐ¸ÑÑÐµÐ¼ Ð³Ð¾ÑÑÑÐµÐ³Ð¾ Ð²Ð¾Ð´Ð¾ÑÐ½Ð°Ð±Ð¶ÐµÐ½Ð¸Ñ, Ð²ÐºÐ»ÑÑÐ°ÑÑÐ¸Ñ ÑÐµÐ¿Ð»Ð¾Ð°ÐºÐºÑÐ¼ÑÐ»Ð¸ÑÑÑÑÑÑ ÑÑÑÐ°Ð½Ð¾Ð²ÐºÑ Ð¸ ÑÐ¾Ð»Ð½ÐµÑÐ½ÑÐµ ÐºÐ¾Ð»Ð»ÐµÐºÑÐ¾ÑÑ. ÐÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð¾ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐµÐ¿Ð»Ð¾Ð²Ð¾Ð³Ð¾ Ð½Ð°ÐºÐ¾Ð¿Ð¸ÑÐµÐ»Ñ ÑÐ°Ð·Ð¾Ð²Ð¾Ð³Ð¾ Ð¿ÐµÑÐµÑÐ¾Ð´Ð°. ÐÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð° ÑÐµÐ¼Ð¿ÐµÑÐ°ÑÑÑÐ° ÑÐµÐ¿Ð»Ð¾Ð½Ð¾ÑÐ¸ÑÐµÐ»Ñ Ð´Ð»Ñ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ Ð¿ÑÐ¾ÑÐµÑÑÐ° Ð¿Ð»Ð°Ð²Ð»ÐµÐ½Ð¸Ñ ÑÐµÐ¿Ð»Ð¾Ð°ÐºÐºÑÐ¼ÑÐ»Ð¸ÑÑÑÑÐµÐ³Ð¾ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð°. ÐÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð° ÑÐµÐ¼Ð¿ÐµÑÐ°ÑÑÑÐ° Ð² ÐºÐ¾Ð½ÑÑÑÐµ ÑÑÐµÐ¼Ñ Ð¾ÑÐºÑÑÑÐ¾Ð³Ð¾ ÑÐ¸Ð¿Ð°, Ð²ÐºÐ»ÑÑÐ°ÑÑÐµÐ¼ Ð±ÑÑÐµÑÐ½ÑÑ ÐµÐ¼ÐºÐ¾ÑÑÑ, Ð´Ð»Ñ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ Ð½Ð¾ÑÐ¼Ð°ÑÐ¸Ð²Ð½Ð¾Ð¹ ÑÐµÐ¼Ð¿ÐµÑÐ°ÑÑÑÑ Ð² ÑÐ¸ÑÑÐµÐ¼Ðµ Ð³Ð¾ÑÑÑÐµÐ³Ð¾ Ð²Ð¾Ð´Ð¾ÑÐ½Ð°Ð±Ð¶ÐµÐ½Ð¸Ñ.
The Milky Way's dark matter halo appears to be lopsided
Creators: name: Saha, Kanak
name: Levine, Evan S.
name: Jog, Chanda J.
name: Blitz, Leo
Publisher: name: arXiv
Year: 2009
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: The atomic hydrogen gas (HI) disk in the outer region (beyond ~10 kpc from the centre) of Milky Way can provide valuable information about the structure of the dark matter halo. The recent 3-D thickness map of the outer HI disk from the all sky 21-cm line LAB survey, gives us a unique opportunity to investigate the structure of the dark matter halo of Milky Way in great detail. A striking feature of this new survey is the North-South asymmetry in the thickness map of the atomic hydrogen gas. Assuming vertical hydrostatic equilibrium under the total potential of the Galaxy, we derive the model thickness map of the HI gas. We show that simple axisymmetric halo models, such as softened isothermal halo (producing a flat rotation curve with V_c ~ 220 km/s) or any halo with density falling faster than the isothermal one, are not able to explain the observed radial variation of the gas thickness. We also show that such axisymmetric halos along with different HI velocity dispersion in the two halves, cannot explain the observed asymmetry in the thickness map. Amongst the non-axisymmetric models, it is shown that a purely lopsided (m=1, first harmonic) dark matter halo with reasonable HI velocity dispersion fails to explain the North-South asymmetry satisfactorily. However, we show that by superposing a second harmonic (m=2) out of phase onto a purely lopsided halo e.g. our best fit and more acceptable model A (with parameters ε_{h}^{1}=0.2, ε_{h}^{2}=0.18 and σ_{HI}=8.5 km/s) can provide an excellent fit to the observation and reproduce the North-South asymmetry naturally. The emerging picture of the asymmetric dark matter halo is supported by the ΛCDM halos formed in the cosmological N-body simulation.
description: 37 pages, 8 figures, accepted for publication in ApJ
title: ÐÐ¾Ð¿ÑÐ¾ÑÑ Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ¸ Ð¿ÑÐµÐ¿Ð¾Ð´Ð°Ð²Ð°Ð½Ð¸Ñ Ð² Ð²ÑÐ·Ðµ
Creators: name: ÐÐºÐ¾Ð¿Ð¾Ð²Ð°, ÐÐ°ÑÐ¸Ñ
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2010
Subjects: Ð²ÑÑÑÐµÐµ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ðµ
Ð¿ÑÐµÐ¿Ð¾Ð´Ð°Ð²Ð°Ð½Ð¸Ðµ
Ð¼ÐµÑÐ¾Ð´Ñ Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ
Ð¸Ð½Ð¾ÑÑÑÐ°Ð½Ð½ÑÐµ ÑÐ·ÑÐºÐ¸

description: Ð 13-Ð¼ ÑÐ±Ð¾ÑÐ½Ð¸ÐºÐµ "ÐÐ¾Ð¿ÑÐ¾ÑÑ Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ¸ Ð¿ÑÐµÐ¿Ð¾Ð´Ð°Ð²Ð°Ð½Ð¸Ñ Ð² Ð²ÑÐ·Ðµ" Ð²ÐºÐ»ÑÑÐµÐ½Ñ ÑÑÐ°ÑÑÐ¸, Ð·Ð°ÑÑÐ°Ð³Ð¸Ð²Ð°ÑÑÐ¸Ðµ ÑÐ¸ÑÐ¾ÐºÐ¸Ð¹ ÑÐ¿ÐµÐºÑÑ Ð°ÐºÑÑÐ°Ð»ÑÐ½ÑÑ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼, ÑÐ²ÑÐ·Ð°Ð½Ð½ÑÑ Ñ ÑÐµÐ¾ÑÐ¸ÐµÐ¹ Ð¸ Ð¿ÑÐ°ÐºÑÐ¸ÐºÐ¾Ð¹ Ð²ÑÑÑÐµÐ³Ð¾ Ð¿ÑÐ¾ÑÐµÑÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð»Ð¸Ð½Ð³Ð²Ð¸ÑÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ. Ð¡Ð±Ð¾ÑÐ½Ð¸Ðº Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐ°ÐµÑÑÑ ÑÑÐµÐ½ÑÐ¼-Ð»Ð¸Ð½Ð³Ð²Ð¸ÑÑÐ°Ð¼, Ð°ÑÐ¿Ð¸ÑÐ°Ð½ÑÐ°Ð¼, ÑÐ¾Ð¸ÑÐºÐ°ÑÐµÐ»ÑÐ¼, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¿ÑÐµÐ¿Ð¾Ð´Ð°Ð²Ð°ÑÐµÐ»ÑÐ¼ Ð¸Ð½Ð¾ÑÑÑÐ°Ð½Ð½Ð¾Ð³Ð¾ ÑÐ·ÑÐºÐ°.
description: ÐÐµÑÐ°ÑÐ°ÐµÑÑÑ Ð¿Ð¾ ÑÐµÑÐµÐ½Ð¸Ñ ÑÐµÐ´Ð°ÐºÑÐ¸Ð¾Ð½Ð½Ð¾-Ð¸Ð·Ð´Ð°ÑÐµÐ»ÑÑÐºÐ¾Ð³Ð¾ ÑÐ¾Ð²ÐµÑÐ° Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¾Ð³Ð¾ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ°.
Dependence of AGN Activity on Halo Mass and Redshift in the SPT Cluster Surveys
Creators: name: Floyd, Benjamin
Publisher: name: Zenodo
Year: 2021

description: The number of active galactic nuclei (AGN) in galaxy clusters has been observed to grow by nearly two orders of magnitude from the local universe to z ~ 1.5. Star formation rates in clusters have also been observed to rise rapidly over this redshift interval. These trends, along with several other recent observations of high-redshift clusters, have led to the idea that this enhanced star formation and AGN activity may be driven by galaxy mergers within the clusters. Since mergers are more efficient in lower mass clusters with smaller galaxy velocity dispersions, the expectation is that AGN incidence should scale inversely with cluster mass. A recent study using X-ray selected AGN has offered some support for this model in low-redshift clusters, though with large uncertainties. We select infrared-bright AGN from a large, uniform, essentially mass-selected galaxy cluster sample from the South Pole Telescope spanning a redshift range of 0.15 < z < 1.7 for which we have acquired follow-up Spitzer Space Telescope observations. With these data we explore the incidence of IR-bright AGN in clusters as a function of cluster mass and redshift.
ebook - Menulis Ilmiah itu Menyenangkan
Creators: name: Irawan, Dasapta Erwin
Publisher: name: Open Science Framework
Year: 2021

description: ebook - Menulis Ilmiah itu Menyenangkan. Authors: Dasapta Erwin Irawan (myself) and Cut Novianti Rachmi (my wife). Published as OA book by ITB Press.
Design of A Low Power Low Voltage CMOS Opamp
Creators: name: Baruah, Ratul Kr.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Other Computer Science (cs.OH)
subject: FOS: Computer and information sciences

description: In this paper a CMOS operational amplifier is presented which operates at 2V power supply and 1microA input bias current at 0.8 micron technology using non conventional mode of operation of MOS transistors and whose input is depended on bias current. The unique behaviour of the MOS transistors in subthreshold region not only allows a designer to work at low input bias current but also at low voltage. While operating the device at weak inversion results low power dissipation but dynamic range is degraded. Optimum balance between power dissipation and dynamic range results when the MOS transistors are operated at moderate inversion. Power is again minimised by the application of input dependant bias current using feedback loops in the input transistors of the differential pair with two current substractors. In comparison with the reported low power low voltage opamps at 0.8 micron technology, this opamp has very low standby power consumption with a high driving capability and operates at low voltage. The opamp is fairly small (0.0084 mm 2) and slew rate is more than other low power low voltage opamps reported at 0.8 um technology [1,2]. Vittoz at al [3] reported that slew rate can be improved by adaptive biasing technique and power dissipation can be reduced by operating the device in weak inversion. Though lower power dissipation is achieved the area required by the circuit is very large and speed is too small. So, operating the device in moderate inversion is a good solution. Also operating the device in subthreshold region not only allows lower power dissipation but also a lower voltage operation is achieved.
description: 8 Pages, VLSICS Journal
Space-Efficient Simulation of Quantum Computers
Creators: name: Frank, Michael P.
name: Meyer-Baese, Uwe H.
name: Chiorescu, Irinel
name: Oniciuc, Liviu
name: van Engelen, Robert A.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Traditional algorithms for simulating quantum computers on classical ones require an exponentially large amount of memory, and so typically cannot simulate general quantum circuits with more than about 30 or so qubits on a typical PC-scale platform with only a few gigabytes of main memory. However, more memory-efficient simulations are possible, requiring only polynomial or even linear space in the size of the quantum circuit being simulated. In this paper, we describe one such technique, which was recently implemented at FSU in the form of a C++ program called SEQCSim, which we releasing publicly. We also discuss the potential benefits of this simulation in quantum computing research and education, and outline some possible directions for further progress.
description: 6 pages, 3 figures, author reprint of final submitted manuscript
Infrared spectra of TiO2 clusters for hot Jupiter atmospheres
Creators: name: Sindel, J. P.
name: Helling, Ch.
name: Gobrecht, D.
name: Chubb, K. L.
name: Decin, L.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Context. Clouds seem unavoidable in cool and dense environments, and hence, are necessary to explain observations of exoplanet atmospheres, most recently of WASP 96b with JWST. Understanding the formation of cloud condensation nuclei in non-terrestrial environments is therefore crucial to develop accurate models to interpret present and future observations. Aims. The goal of the paper is to support observations with infrared spectra for (TiO2)N clusters in order to study cloud formation in exoplanet atmospheres. Methods. Vibrational frequencies are derived from quantum-chemical calculations for 123 (TiO2)-clusters and their isomers, and line-broadening mechanisms are evaluated. Cluster spectra are calculated for several atmospheric levels for two example exoplanet atmospheres (WASP 121b-like and WASP 96b-like) to identify possible spectral fingerprints for cloud formation. Results. Rotational motion of and transitions in the clusters cause significant line broadening, so that individual vibrational lines are broadened beyond the spectral resolution of the medium resolution mode of the JWST mid-infrared instrument MIRI at R = 3000. However, each individual cluster isomer exhibits a "fingerprint" IR spectrum. In particular, larger (TiO2)-clusters have distinctly different spectra from smaller clusters. Morning and evening terminator for the same planet can exhibit different total absorbances due to different cluster sizes being more abundant. Conclusions. The largest (TiO2)-clusters are not necessarily the most abundant (TiO2)-clusters in the high-altitude regions of ultra-hot Jupiters, and the different cluster isomers will contribute to the local absorbance. Planets with a considerable day-night asymmetry will be most suitable to search for (TiO2)-cluster isomers in order to improve cloud formation modelling.
description: 8 pages, 8 figures, 1 table, accepted for publication in A&A
A site-controlled quantum dot system offering both high uniformity and spectral purity
Creators: name: Mereni, L. O.
name: Dimastrodonato, V.
name: Young, R. J.
name: Pelucchi, E.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: In this paper we report on the optical properties of site controlled InGaAs dots with GaAs barriers grown in pyramidal recesses by metalorganic vapour phase epitaxy. The inhomogeneous broadening of excitonic emission from an ensemble of quantum dots is found to be unusually narrow, with a standard deviation of 1.19 meV, and spectral purity of emission lines from individual dots is found to be very high (18-30 ueV), in contrast with other site-controlled systems.
description: 12 pages, 3 figures
title: ÐÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ñ Ð¸ Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ÑÐµÑ Ð½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¾Ð±ÑÐ»ÑÐ¶Ð¸Ð²Ð°Ð½Ð¸Ñ Ð¸ ÑÐµÐ¼Ð¾Ð½ÑÐ¾Ð² ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð½Ð° Ð¢Ð­Ð¡ Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ Ð¢Ð­Ð¦-22
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð¤Ð°Ð»Ð°Ð»ÐµÐµÐ²Ð°, ÐÐ¸ÐºÑÐ¾Ñ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: ÑÐµÐ¿Ð»Ð¾ÑÐ»ÐµÐºÑÑÐ¾ÑÑÐ°Ð½ÑÐ¸Ð¸
ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ¾Ðµ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ
ÑÐµÐ¼Ð¾Ð½Ñ ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ
Ð½Ð°Ð´ÐµÐ¶Ð½Ð¾ÑÑÑ ÑÐ»ÐµÐºÑÑÐ¾ÑÑÐ°Ð½ÑÐ¸Ð¹

description: ÐÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¿ÑÑÐµÐ¹ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐµÐ¼Ð¾Ð½ÑÐ½ÑÑ ÑÐ°Ð±Ð¾Ñ. ÐÐ·ÑÑÐµÐ½Ñ Ð¼ÐµÑÐ¾Ð´Ñ Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ, ÑÐ¿ÐµÑÐ¸ÑÐ¸ÐºÐ° Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ Ð¢ÐÐ¸Ð  Ð½Ð° ÑÐ»ÐµÐºÑÑÐ¾ÑÑÐ°Ð½ÑÐ¸Ð¸, ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¾Ð±ÑÐ¸Ðµ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸ Ð½Ð°Ð´ÐµÐ¶Ð½Ð¾ÑÑÐ¸ Ð¸ Ð¿ÑÐ¾ÑÐµÑÑ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¸ Ð²Ð»Ð¸ÑÐ½Ð¸Ðµ Ð²ÐµÐ»Ð¸ÑÐ¸Ð½Ñ ÑÐµÐ¼Ð¾Ð½ÑÐ½Ð¾Ð³Ð¾ ÑÐ¾Ð½Ð´Ð° Ð½Ð° Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ñ Ð¢ÐÐ¸Ð , Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ ÑÐµÐ³Ð¾ Ð±ÑÐ»Ð¸ ÑÐ°ÑÑÑÐ¸ÑÐ°Ð½Ñ ÐºÐ¾ÑÑÑÐ¸ÑÐ¸ÐµÐ½ÑÑ Ð³Ð¾ÑÐ¾Ð²Ð½Ð¾ÑÑÐ¸ Ð¸ Ð·Ð°Ð³ÑÑÐ·ÐºÐ¸ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¸ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÑÐ¸Ñ Ð²ÐµÐ»Ð¸ÑÐ¸Ð½. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ ÑÐ¿Ð¾ÑÐ¾Ð±Ñ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÑÐµÐ¼Ð¾Ð½ÑÐ½ÑÑ ÑÐ°Ð±Ð¾Ñ, ÑÑÑÑÐºÑÑÑÐ° Ð·Ð°ÑÑÐ°Ñ Ð½Ð° ÑÐµÐ¼Ð¾Ð½Ñ Ð¸ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð´Ð»Ñ 2015-2017 Ð³Ð¾Ð´Ð¾Ð².
Seminal Vesicle Cyst with Ipsilateral Renal Agenesis
Creators: name: Maschio, Vittorio
Publisher: name: EURORAD
Year: 2014
Subjects: subject: Urinary Tract / Bladder
subject: CT
subject: MR
subject: Diagnostic procedure
subject: Congenital
subject: Cysts

description: Clinical History Image Findings Discussion Find Diagnosis Differential Diagnosis
description: male, 42 years
description: Clinical History: A 42 year-old man presented  with progressive perineal pain, pain on ejaculation, dysuria and infertility. Final Diagnosis: Seminal Vesicle Cyst with Ipsilateral Renal Agenesis
Detecting active latitudes of Sun-like stars using asteroseismic a-coefficients
Creators: name: Benomar, Othman
name: Takata, Masao
name: Bazot, Michael
name: Sekii, Takashi
name: Gizon, Laurent
name: Lu, Yuting
Publisher: name: arXiv
Year: 2023
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We introduce a framework to measure the asphericity of Sun-like stars using $a_1$, $a_2$ and $a_4$ coefficients, and constrain their latitudes of magnetic activity. Systematic errors on the inferred coefficients are evaluated in function of key physical and seismic parameters (inclination of rotation axis, average rotation, height-to-noise ratio of peaks in power spectrum). The measured a-coefficients account for rotational oblateness and the effect of surface magnetic activity. We use a simple model that assumes a single latitudinal band of activity. Using solar SOHO/VIRGO/SPM data, we demonstrate the capability of the method to detect the mean active latitude and its intensity changes between 1999-2002 (maximum of activity) and 2006-2009 (minimum of activity). We further apply the method to study the solar-analogue stars 16 Cyg A and B using Kepler observations. An equatorial band of activity, exhibiting intensity that could be comparable to that of the Sun, is detected in 16 Cyg A. However, 16 Cyg B exhibits a bi-modality in $a_4$ that is challenging to explain. We suggest that this could be a manifestation of the transition between a quiet and an active phase of activity. Validating or invalidating this hypothesis may require new observations.
description: Accepted to A&A
ACRL’s Scholarly Communications Roadshow : [Bellwether for a changing profession]
Creators: name: Kirchner, Joy
name: Malenfant, Kara J.
Publisher: name: The University of British Columbia
Year: 2013

description: “This work originally appeared in “Common Ground at the Nexus of Information Literacy and Scholarly Communication” edited by Stephanie Davis-Kahl and Merinda Kaye Hensley. Chicago, IL: Association of College & Research Libraries, 2013. Any use of this work must be accompanied by this notification.”
title: Ð Ð¾Ð»Ñ Â«ÐÐ¢ÐÂ» Ð² ÑÐ¸ÑÑÐµÐ¼Ðµ ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð²Ð¾ÑÐ¿Ð¸ÑÐ°Ð½Ð¸Ñ ÑÐºÐ¾Ð»ÑÐ½Ð¸ÐºÐ¾Ð² XXI Ð²ÐµÐºÐ°
title: The role of the Â«Ready for labour and defenceÂ» in the system of physical education of schoolchildren of the XXI century
Creators: name: ÐÐ¾Ð¿Ð°ÑÐ¸Ð½, ÐÐµÐ½Ð¸Ñ
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: 2023
Subjects: Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð° Â«ÐÐ¾ÑÐ¾Ð² Ðº ÑÑÑÐ´Ñ Ð¸ Ð¾Ð±Ð¾ÑÐ¾Ð½ÐµÂ»
Ð¼Ð¾ÑÐ¸Ð²Ð°ÑÐ¸Ñ
Ð¿ÑÐ¸Ñ Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð´ÐµÑÐµÐ¹ ÑÑÐ°ÑÑÐµÐ³Ð¾ ÑÐºÐ¾Ð»ÑÐ½Ð¾Ð³Ð¾ Ð²Ð¾Ð·ÑÐ°ÑÑÐ°
Ð½Ð¾ÑÐ¼Ð°ÑÐ¸Ð²Ñ
ÑÐ¿Ð¾ÑÑ
ÑÐ¸Ð·ÐºÑÐ»ÑÑÑÑÐ°
Ð·Ð´Ð¾ÑÐ¾Ð²ÑÐµ
program Â«Ready for labour and defenceÂ»
motivation
psychological characteristics of children of senior school age
standards
sports
physical education
health

description: Ð ÑÑÐ°ÑÑÐµ Ð¾ÑÐ²ÐµÑÐµÐ½Ñ Ð²Ð¾Ð¿ÑÐ¾ÑÑ Ð¸ÑÑÐ¾ÑÐ¸Ð¸ ÐÐ¢Ð, Ð°ÐºÑÑÐ°Ð»ÑÐ½Ð¾ÑÑÐ¸ Ð¸ Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼Ð¾ÑÑÐ¸ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ñ ÐÐ¢Ð Ð² XXI Ð²ÐµÐºÐµ, ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¼Ð¾ÑÐ¸Ð²Ð°ÑÐ¸Ð¸ Ðº Ð·Ð°Ð½ÑÑÐ¸ÑÐ¼ ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¾Ð¹ ÐºÑÐ»ÑÑÑÑÐ¾Ð¹ Ñ Ð´ÐµÑÐµÐ¹ ÑÑÐ°ÑÑÐµÐ³Ð¾ ÑÐºÐ¾Ð»ÑÐ½Ð¾Ð³Ð¾ Ð²Ð¾Ð·ÑÐ°ÑÑÐ° ÐºÐ°Ðº ÑÐ»ÐµÐ´ÑÑÐ²Ð¸Ðµ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ Ð½Ð¾ÑÐ¼Ð°ÑÐ¸Ð²Ð¾Ð² ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ° ÐÐ¢Ð Ð½Ð° Ð·Ð¾Ð»Ð¾ÑÐ¾Ð¹ Ð·Ð½Ð°Ðº Ð¾ÑÐ»Ð¸ÑÐ¸Ñ. Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÑÐ°ÑÑÐµ Ð¸ÑÑÐ»ÐµÐ´ÑÐµÑÑÑ Ð²Ð»Ð¸ÑÐ½Ð¸Ðµ ÐÐ¢Ð Ð½Ð° ÑÐ¸Ð·Ð¸ÑÐµÑÐºÑÑ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÑ ÑÐ¾ÑÑÐ¸Ð¹ÑÐºÐ¸Ñ Ð¶Ð¸ÑÐµÐ»ÐµÐ¹. ÐÑÐ¸Ð¼ÐµÐ½ÑÐµÑÑÑ Ð´ÐµÑÐºÑÐ¸Ð¿ÑÐ¸Ð²Ð½ÑÐ¹ Ð½Ð°ÑÑÐ½ÑÐ¹ Ð¼ÐµÑÐ¾Ð´ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ. Ð Ð°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÐµÑÑÑ ÑÐ²ÐµÐ»Ð¸ÑÐµÐ½Ð¸Ðµ Ð·Ð½Ð°ÑÐ¸Ð¼Ð¾ÑÑÐ¸ ÐÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ° ÐÐ¢Ð Ð² ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¾Ð¼ Ð²Ð¾ÑÐ¿Ð¸ÑÐ°Ð½Ð¸Ð¸ Ð¼Ð¾Ð»Ð¾Ð´ÐµÐ¶Ð¸. ÐÐ¾ÐºÐ°Ð·Ð°Ð½Ð° Ð°ÐºÑÑÐ°Ð»ÑÐ½Ð¾ÑÑÑ Ð²Ð¾Ð²Ð»ÐµÑÐµÐ½Ð¸Ñ Ð³ÑÐ°Ð¶Ð´Ð°Ð½ Ð² ÑÐ¿Ð¾ÑÑÐ¸Ð²Ð½ÑÐµ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ñ.
description: The article highlights the issues of the history of the Â«Ready for Labour and DefenceÂ», the relevance and necessity of implementing the Â«RLDÂ» program in the 21st century, the formation of motivation for physical education in children of senior school age as a result of fulfilling the standards of the Â«RLDÂ» complex for a golden badge of distinction. This article examines the impact of the Â«RLDÂ» on the physical fitness of Russian residents. A descriptive scientific method of research is applied. The increase in the importance of the Â«RLDÂ» complex in the physical education of young people is considered. The relevance of involving citizens in sports events is shown.
On Sum--Connectivity Index of Bicyclic Graphs
Creators: name: Du, Zhibin
name: Zhou, Bo
Publisher: name: arXiv
Year: 2009
Subjects: subject: Combinatorics (math.CO)
subject: FOS: Mathematics
subject: 05C90, 05C35, 05C07

description: We determine the minimum sum--connectivity index of bicyclic graphs with $n$ vertices and matching number $m$, where $2\le m\le \lfloor\frac{n}{2}\rfloor$, the minimum and the second minimum, as well as the maximum and the second maximum sum--connectivity indices of bicyclic graphs with $n\ge 5$ vertices. The extremal graphs are characterized.
title: ÐÐ½Ð°Ð»Ð¸Ð· ÑÑÑÐ°Ð½Ð¾Ð²Ð¸Ð²ÑÐ¸Ñ ÑÑ Ð¸ Ð¿ÐµÑÐµÑ Ð¾Ð´Ð½ÑÑ ÑÐµÐ¶Ð¸Ð¼Ð¾Ð² Ð² ÑÐ»ÐµÐºÑÑÐ¾ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ðµ 220/110 ÐºÐ
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¾Ð·Ð°, ÐÑÑÐµÐ¼
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2016
Subjects: ÑÐµÐ¶Ð¸Ð¼
ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÑ
ÑÐ¸ÑÑÐµÐ¼Ð°
mode
stability
system

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð° ÑÐ»ÐµÐºÑÑÐ¾ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ°Ñ ÑÐ¸ÑÑÐµÐ¼Ð° ÑÐ¾Ð´ÐµÑÐ¶Ð°ÑÐ°Ñ 2 ÐºÐ»Ð°ÑÑÐ° Ð½Ð°Ð¿ÑÑÐ¶ÐµÐ½Ð¸Ñ 220 Ð¸ 110 ÐºÐ. ÐÑÐ¸Ð²ÐµÐ´ÐµÐ½Ñ ÑÐ°ÑÑÐµÑÑ, Ð¸ÑÐ¿Ð¾Ð»ÑÐ·ÑÐµÐ¼ÑÐµ Ð´Ð»Ñ Ð²ÑÐ±Ð¾ÑÐ° ÑÐ¸Ð»Ð¾Ð²Ð¾Ð³Ð¾ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÐµÑÐµÐ¹. ÐÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½ ÑÐ°ÑÑÐµÑ ÑÑÑÐ°Ð½Ð¾Ð²Ð¸Ð²ÑÐµÐ³Ð¾ÑÑ ÑÐµÐ¶Ð¸Ð¼Ð° ÑÐ°Ð±Ð¾ÑÑ ÑÐ»ÐµÐºÑÑÐ¾ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ ÑÐ¾ÑÐ¼ÑÐ» Ð´Ð»Ñ ÑÑÐ°ÑÑÐºÐ° ÑÐµÑÐ¸ (Ñ.Ðµ. Ð²ÑÑÑÐ½ÑÑ) Ð¸ Ñ Ð¿Ð¾Ð¼Ð¾ÑÑÑ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð¾Ð³Ð¾ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ RastrWin. ÐÑÐ¿Ð¾Ð»Ð½ÐµÐ½ ÑÐ°ÑÑÐµÑ ÑÐ¾ÐºÐ¾Ð² Ð´Ð²ÑÑÑÐ°Ð·Ð½Ð¾Ð³Ð¾ ÐºÐ¾ÑÐ¾ÑÐºÐ¾Ð³Ð¾ Ð·Ð°Ð¼ÑÐºÐ°Ð½Ð¸Ñ Ð² Ð¾Ð´Ð½Ð¾Ð¼ Ð¸Ð· ÑÐ·Ð»Ð¾Ð² Ð¸ÑÑÐ»ÐµÐ´ÑÐµÐ¼Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ. ÐÐ¾ÑÑÑÐ¾ÐµÐ½Ñ Ð²ÐµÐºÑÐ¾ÑÐ½ÑÐµ Ð´Ð¸Ð°Ð³ÑÐ°Ð¼Ð¼Ñ. ÐÑÐ¾Ð¼Ðµ ÑÐ¾Ð³Ð¾, Ð¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½Ð° Ð¾ÑÐµÐ½ÐºÐ° Ð´Ð¸Ð½Ð°Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¹ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÐ¸ Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¿ÑÐ¸ Ð²Ð¾Ð·Ð½Ð¸ÐºÐ½Ð¾Ð²ÐµÐ½Ð¸Ð¸ Ð´Ð²ÑÑÑÐ°Ð·Ð½Ð¾Ð³Ð¾ ÐºÐ¾ÑÐ¾ÑÐºÐ¾Ð³Ð¾ Ð·Ð°Ð¼ÑÐºÐ°Ð½Ð¸Ñ Ð½Ð° ÑÐ¸Ð½Ð°Ñ Ð¾Ð´Ð½Ð¾Ð¹ Ð¸Ð· ÑÑÐ°Ð½ÑÐ¸Ð¹.
description: This paper considers the power system comprising two voltage class 220 and 110 kV. The work presents the calculations used to select the power of electric grids equipment. The calculation of steady state mode of power system using the formula for the grid segment (i.e. by hand) and using special softwareRastrWin. The calculation of the current two-phase short circuit in one of the nodes of the system under study. Constructed vector diagrams. In addition, the dynamic stability of the system was evaluated in the event of a two-phase short circuit at one of the stations tire.
АПРОБАЦИЯ МЕТОДИКИ РАЗВИТИЯ ИКТ-КОМПЕТЕНТНОСТИ ПОСРЕДСТВОМ РАСПРЕДЕЛЕННЫХ МЕДИАОБРАЗОВАТЕЛЬНЫХ ПРОЕКТОВ
Creators: name: Касьянова Елена Васильевна
name: Сафонов Константин Владимирович
Publisher: name: Вестник Пермского государственного гуманитарно-педагогического университета. Серия № 1. Психологические и педагогические науки
Year: 2021
Subjects: ИТ-инженер
ИКТ-компетентность
медиаобрзовательный проект
распределенные технологии
цифровая дидактика.
IT engineer
ICT competence
media education project
distributed technologies
digital didactics

description: В статье раскрывается необходимость формирования информационно-коммуникационной компетенции будущих ИТ-инженеров. Обоснована актуальность подготовки студентов по направлениям, связанным с информационными технологиями. Задачей исследования было создание и апробация методики, позволяющей формировать ИКТ-компетентность, составляющую основу профессиональной подготовки будущих ИТ-инженеров, с применением распределенных медиаобразовательных проектов. Ориентация на распределенные технологии соответствует требованиям цифрового общества и отражает актуальность применяемых технологий. Основное внимание авторы концентрируют на облачных технологиях, применяемых при реализации медиаобразовательных проектов. В процессе апробации методики в СибГУ науки и технологий были получены результаты, представленные медиапродуктами, результатами опросов студентов и оценками освоения компонентов ИКТ-компетентности. Планируется продолжение исследования с уточнением критериев и показателей уровня сформированности ИКТкомпетентности.
description: The article reveals the need for the formation of information and communication competence of future IT engineers. The urgency of training students in areas related to information technology has been substantiated. The objective of the study was to create and test a methodology that allows the formation of ICT competence, which is the basis for the professional training of future IT engineers, using distributed media education projects. The focus on distributed technologies meets the requirements of the digital society and reflects the relevance of the technologies used. The authors focus on cloud technologies used in the implementation of media education projects. In the process of approbation of the methodology at the Siberian State University of Science and Technology, the results were obtained, presented by media products, the results of surveys of students and assessments of the development of components of ICT competence. It is planned to continue the study with the specification of the criteria and indicators of the level of formation of ICT competence.
title: Ð¤Ð¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¸ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ²Ð¾Ð¹ÑÑÐ² ÑÐ»ÐµÐºÑÑÐ¾Ð¿ÑÐ¾Ð²Ð¾Ð´ÑÑÐ¸Ñ Ð²Ð¾Ð»Ð¾ÐºÐ½Ð¸ÑÑÑÑ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð¾Ð² Ð´Ð»Ñ ÐºÐ»ÐµÑÐ¾ÑÐ½ÑÑ ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¹
title: ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÑ 03.01.02 Â«ÐÐ¸Ð¾ÑÐ¸Ð·Ð¸ÐºÐ°Â»
titleType: Subtitle
Creators: name: ÐÐ°ÑÑÐµÐ½Ð¸ÑÐµÐ², ÐÑÐµÐ²Ð¾Ð»Ð¾Ð´
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2021
Subjects: ÐÐ¾Ð¼Ð¿Ð¾Ð·Ð¸ÑÐ¸Ð¾Ð½Ð½ÑÐµ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ñ Ð²Ð¾Ð»Ð¾ÐºÐ½Ð¸ÑÑÑÐµ
ÐÐ°Ð½Ð¾ÑÑÑÑÐºÑÑÑÐ½ÑÐµ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ñ
ÐÐ»ÐµÐ½ÐºÐ¸ Ð¿Ð¾Ð»Ð¸Ð¼ÐµÑÐ½ÑÐµ
ÐÐ¾Ð»Ð¸Ð¼ÐµÑÑ ÑÐ»ÐµÐºÑÑÐ¾Ð¿ÑÐ¾Ð²Ð¾Ð´ÑÑÐ¸Ðµ
ÐÐ¾Ð»Ð¸Ð¼ÐµÑÑ
ÑÐºÐ°Ð½ÐµÐ²Ð°Ñ Ð¸Ð½Ð¶ÐµÐ½ÐµÑÐ¸Ñ
ÑÐ»ÐµÐºÑÑÐ¾ÑÐ¿Ð¸Ð½Ð½Ð¸Ð½Ð³
ÑÐ»ÐµÐºÑÑÐ¾ÑÐ¾ÑÐ¼Ð¾Ð²Ð°Ð½Ð¸Ðµ
ÑÐ»ÐµÐºÑÑÐ¾Ð¿ÑÑÐ´ÐµÐ½Ð¸Ðµ

description: ÐÐ¸ÑÑÐµÑÑÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° Ð¿Ð¾Ð»ÑÑÐµÐ½Ð¸Ñ Ð¼ÐµÑÐ¾Ð´Ð¾Ð¼ ÑÐ»ÐµÐºÑÑÐ¾ÑÐ¾ÑÐ¼Ð¾Ð²Ð°Ð½Ð¸Ñ Ð½ÐµÑÐºÐ°Ð½ÑÑ Ð²Ð¾Ð»Ð¾ÐºÐ½Ð¸ÑÑÑÑ ÑÐ»ÐµÐºÑÑÐ¾Ð¿ÑÐ¾Ð²Ð¾Ð´ÑÑÐ¸Ñ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð¾Ð² Ð´Ð»Ñ Ð±Ð¸Ð¾Ð¼ÐµÐ´Ð¸ÑÐ¸Ð½ÑÐºÐ¾Ð³Ð¾ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¸Ñ ÑÑÑÑÐºÑÑÑÑ Ð¸ ÑÐ¸Ð·Ð¸ÐºÐ¾-Ð¼ÐµÑÐ°Ð½Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ²Ð¾Ð¹ÑÑÐ² Ð¸ Ð±Ð¸Ð¾ÑÐ¾Ð²Ð¼ÐµÑÑÐ¸Ð¼Ð¾ÑÑÐ¸, ÐºÐ°Ðº in vitro, ÑÐ°Ðº Ð¸ in vivo. ÐÐ¿Ð¸ÑÐ°Ð½Ð¾ ÑÑÐ¸ Ð¼ÐµÑÐ¾Ð´Ð° Ð¿Ð¾Ð»ÑÑÐµÐ½Ð¸Ñ ÑÐ»ÐµÐºÑÑÐ¾Ð¿ÑÐ¾Ð²Ð¾Ð´ÑÑÐµÐ³Ð¾ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð°: Ð²Ð²ÐµÐ´ÐµÐ½Ð¸Ðµ ÑÐ³Ð»ÐµÑÐ¾Ð´Ð½ÑÑ Ð½Ð°Ð½Ð¾ÑÑÑÐ±Ð¾Ðº, Ð¿Ð¾ÐºÑÑÑÐ¸Ðµ Ð²Ð¾Ð»Ð¾ÐºÐ¾Ð½ ÑÐ»ÐµÐºÑÑÐ¾Ð¿ÑÐ¾Ð²Ð¾Ð´ÑÑÐ¸Ð¼ Ð¿Ð¾Ð»Ð¸Ð¼ÐµÑÐ¾Ð¼ Ð¿Ð¾Ð»Ð¸Ð¿Ð¸ÑÑÐ¾Ð»Ð¾Ð¼ Ð¸ ÑÐµÑÐ¼Ð¾Ð»Ð¸Ð· Ð²Ð¾Ð»Ð¾ÐºÐ¾Ð½ Ð°ÑÐ¾Ð¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿Ð¾Ð»Ð¸Ð¸Ð¼Ð¸Ð´Ð°.
Anisotropic scale invariant cosmology
Creators: name: Nakayama, Yu
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We study a possibility of anisotropic scale invariant cosmology. It is shown that within the conventional Einstein gravity, the violation of the null energy condition is necessary. We construct an example based on a ghost condensation model that violates the null energy condition. The cosmological solution necessarily contains at least one contracting spatial direction as in the Kasner solution. Our cosmology is conjectured to be dual to, if any, a non-unitary anisotropic scale invariant Euclidean field theory. We investigate simple correlation functions of the dual theory by using the holographic computation. After compactification of the contracting direction, our setup may yield a dual field theory description of the winding tachyon condensation that might solve the singularity of big bang/crunch of the universe.
description: 12 pages, v2: reference added
title: ÐÐ¸Ð´ÑÐ¾Ð¼ÐµÑ Ð°Ð½Ð¸ÑÐµÑÐºÐ°Ñ ÑÑÐ°Ð½ÑÐ¼Ð¸ÑÑÐ¸Ñ Ð¿ÐµÑÐµÐ´Ð½ÐµÐ¿ÑÐ¸Ð²Ð¾Ð´Ð½Ð¾Ð³Ð¾ Ð»ÐµÐ³ÐºÐ¾Ð²Ð¾Ð³Ð¾ Ð°Ð²ÑÐ¾Ð¼Ð¾Ð±Ð¸Ð»Ñ ÐºÐ»Ð°ÑÑÐ° Ð
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
Creators: name: ÐÑÑÐ¾Ð², ÐÐ°Ð½Ð¸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: 2018
Subjects: Ð³Ð¸Ð´ÑÐ¾Ð¼ÐµÑ Ð°Ð½Ð¸ÑÐµÑÐºÐ°Ñ ÑÑÐ°Ð½ÑÐ¼Ð¸ÑÑÐ¸Ñ Ð°Ð²ÑÐ¾Ð¼Ð¾Ð±Ð¸Ð»Ñ
Ð¿Ð»Ð°Ð½ÐµÑÐ°ÑÐ½Ð°Ñ ÐºÐ¾ÑÐ¾Ð±ÐºÐ° Ð¿ÐµÑÐµÐ´Ð°Ñ
ÑÑÐ³Ð¾Ð²ÑÐ¹ ÑÐ°ÑÑÐµÑ
ÑÐ¸Ð½ÑÐµÐ· ÑÑ ÐµÐ¼Ñ
Ð¿ÑÐ¾ÑÐ½Ð¾ÑÑÐ½ÑÐµ ÑÐ°ÑÑÐµÑÑ

description: Ð¡Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð° Ð³Ð¸Ð´ÑÐ¾Ð¼ÐµÑÐ°Ð½Ð¸ÑÐµÑÐºÐ°Ñ ÑÑÐ°Ð½ÑÐ¼Ð¸ÑÑÐ¸Ñ Ð´Ð»Ñ Ð¿ÐµÑÐµÐ´Ð½ÐµÐ¿ÑÐ¸Ð²Ð¾Ð´Ð½Ð¾Ð³Ð¾ Ð°Ð²ÑÐ¾Ð¼Ð¾Ð±Ð¸Ð»Ñ. Ð Ð°ÑÑÐµÑÐ½Ð°Ñ Ð¼Ð¾ÑÐ½Ð¾ÑÑÑ Ð´Ð²Ð¸Ð³Ð°ÑÐµÐ»Ñ â55 ÐºÐÑ. Ð¢ÑÐ°Ð½ÑÐ¼Ð¸ÑÑÐ¸Ñ Ð²ÐºÐ»ÑÑÐ°ÐµÑ Ð² ÑÐµÐ±Ñ Ð³Ð¸Ð´ÑÐ¾ÑÑÐ°Ð½ÑÑÐ¾ÑÐ¼Ð°ÑÐ¾Ñ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ½ÑÐ¹ (ÐÐ¢Ð), Ð¿Ð»Ð°Ð½ÐµÑÐ°ÑÐ½ÑÑ ÐºÐ¾ÑÐ¾Ð±ÐºÑ Ð¿ÐµÑÐµÐ´Ð°Ñ, Ð¾Ð±ÐµÑÐ¿ÐµÑÐ¸Ð²Ð°ÑÑÑÑ Ð¿ÑÑÑ Ð¿ÐµÑÐµÐ´Ð°Ñ Ð¿ÑÐ¸ Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ð¸ Ð²Ð¿ÐµÑÐµÐ´ Ð¸ Ð¾Ð´Ð½Ñ Ð¿ÑÐ¸ Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ð¸ Ð½Ð°Ð·Ð°Ð´, Ð³Ð»Ð°Ð²Ð½ÑÑ Ð¿ÐµÑÐµÐ´Ð°ÑÑ, Ð¼ÐµÐ¶ÐºÐ¾Ð»ÐµÑÐ½ÑÐ¹ Ð´Ð¸ÑÑÐµÑÐµÐ½ÑÐ¸Ð°Ð» Ð¸ Ð²ÐµÐ´ÑÑÐ¸Ðµ Ð²Ð°Ð»Ñ Ð½Ð° Ð¿ÑÐ¸Ð²Ð¾Ð´ Ð¿ÐµÑÐµÐ´Ð½Ð¸Ñ ÐºÐ¾Ð»ÐµÑ. ÐÐ¾ÑÐ¾Ð±ÐºÐ° Ð¿ÐµÑÐµÐ´Ð°Ñ, ÑÐºÐ¾Ð¼Ð¿Ð¾Ð½Ð¾Ð²Ð°Ð½Ð½Ð°Ñ Ð² Ð¾Ð´Ð½Ð¾Ð¼ ÐºÐ°ÑÑÐµÑÐµ Ñ Ð³Ð¸Ð´ÑÐ¾ÑÑÐ°Ð½ÑÑÐ¾ÑÐ¼Ð°ÑÐ¾ÑÐ¾Ð¼, Ð³Ð»Ð°Ð²Ð½Ð¾Ð¹ Ð¿ÐµÑÐµÐ´Ð°ÑÐµÐ¹ Ð¸ Ð´Ð¸ÑÑÐµÑÐµÐ½ÑÐ¸Ð°Ð»Ð¾Ð¼ Ð¸Ð¼ÐµÐµÑ ÑÐ»Ð°Ð½ÑÐµÐ²Ð¾Ðµ ÑÐ¾ÐµÐ´Ð¸Ð½ÐµÐ½Ð¸Ðµ Ñ Ð´Ð²Ð¸Ð³Ð°ÑÐµÐ»ÐµÐ¼ Ð¸ ÑÐ°ÑÐ¿Ð¾Ð»Ð°Ð³Ð°ÐµÑÑÑ Ð² Ð¿Ð¾Ð´ÐºÐ°Ð¿Ð¾ÑÐ½Ð¾Ð¼ Ð¿ÑÐ¾ÑÑÑÐ°Ð½ÑÑÐ²Ðµ Ð°Ð²ÑÐ¾Ð¼Ð¾Ð±Ð¸Ð»Ñ. Ð¢ÑÐ°Ð½ÑÐ¼Ð¸ÑÑÐ¸Ñ Ð¸Ð¼ÐµÐµÑ Ð³Ð¸Ð´ÑÐ°Ð²Ð»Ð¸ÑÐµÑÐºÐ¾Ðµ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ, Ð¿ÑÐµÐ´ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð° Ð±Ð»Ð¾ÐºÐ¸ÑÐ¾Ð²ÐºÐ° Ð³Ð¸Ð´ÑÐ¾ÑÑÐ°Ð½ÑÑÐ¾ÑÐ¼Ð°ÑÐ¾ÑÐ°.
פסיכולוגיה ניסויית- קבוצה 4- רמות מחירים והנחה
Creators: name: Bar Zwilich
name: Engel, Naama
name: Eilon, Evyatar
Publisher: name: Open Science Framework
Year: 2023
Subjects: subject: Social and Behavioral Sciences
subject: Psychology
subject: FOS: Psychology

description: ההרשמה מראש למחקר שלנו, במסגרת קורס פסיכולוגיה ניסויית
Probing Early Modification of Gravity with Planck, ACT and SPT
Creators: name: Abellán, Guillermo Franco
name: Braglia, Matteo
name: Ballardini, Mario
name: Finelli, Fabio
name: Poulin, Vivian
Publisher: name: arXiv
Year: 2023
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We consider a model of early modified gravity (EMG) that was recently proposed as a candidate to resolve the Hubble tension. The model consists in a scalar field $σ$ with a non-minimal coupling (NMC) to the Ricci curvature of the form $F(σ) = M_{\mathrm{pl}}^2+ξσ^2$ and an effective mass induced by a quartic potential $V(σ) = λσ^4/4$. We present the first analyses of the EMG model in light of the latest ACT DR4 and SPT-3G data in combination with full Planck data, and find a $\gtrsim 2σ$ preference for a non-zero EMG contribution from a combination of primary CMB data alone, mostly driven by ACT DR4 data. This is different from popular 'Early Dark Energy' models, which are detected only when the high-$\ell$ information from Planck temperature is removed. We find that the NMC plays a key role in controlling the evolution of density perturbations that is favored by the data over the minimally coupled case. Including measurements of supernovae luminosity distance from Pantheon+, baryonic acoustic oscillations and growth factor from BOSS, and CMB lensing of Planck leaves the preference unaffected. In the EMG model, the tension with S$H_0$ES is alleviated from $\sim 6σ$ to $\sim 3σ$. Further adding S$H_0$ES data rise the detection of the EMG model above $5σ$.
description: 25 pages, 9 figures, 5 tables. Added minor corrections. v2 matches the published JCAP version. Comments welcome!