cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
WEB SERVERLAR VA HOSTING TEXNALOGIYALARI
Creators: name: Qodirov, Farrux
name: Safarova, Mohinabonu
Publisher: name: Zenodo
Year: 2025

description: Ushbu maqolada web server va hosting texnologiyalari ning mohiyati, ularning rivojlanish bosqichlari va zamonaviy tendensiyalari tahlil qilinadi. Web serverlarning asosiy funksiyalari, hosting turlari, bulutli xizmatlarning afzalliklari va kelajak istiqbollari yoritiladi. Shuningdek, serverless hosting, edge computing, sun’iy intellekt va xavfsizlik texnologiyalarining web infratuzilmadagi roli ko‘rib chiqiladi. Tadqiqot natijalari asosida web serverlarni samarali boshqarish va hosting xizmatlarining sifatini oshirish bo‘yicha tavsiyalar beriladi.
Vortex Synchronization in Bose-Einstein Condensates: A Time-Dependent Gross-Pitaevskii Equation Approach
Creators: name: Barnett, Ryan
name: Chen, Edward
name: Refael, Gil
Publisher: name: arXiv
Year: 2009
Subjects: subject: Quantum Gases (cond-mat.quant-gas)
subject: FOS: Physical sciences

description: In this work we consider vortex lattices in rotating Bose-Einstein Condensates composed of two species of bosons having different masses. Previously [1] it was claimed that the vortices of the two species form bound pairs and the two vortex lattices lock. Remarkably, the two condensates and the external drive all rotate at different speeds due to the disparity of the masses of the constituent bosons. In this paper we study the system by solving the full two-component Gross-Pitaevskii equations numerically. Using this approach we verify the stability of the putative locked state which is found to exist within a disk centered on the axis of rotation and which depends on the mass ratio of the two bosons. We also show that an analytic estimate of this locking radius based on a two-body force calculation agrees well with the numerical results.
description: 6.1 pages, 3 figures
title: Особенности системы спортивного отбора и ориентации в циклических видах спорта на примере гребного спорта
Creators: name: ELS IPR BOOKS
Publisher: name: Донской государственный технический университет
Year: 2022

description: Представлена модель системы спортивного отбора и ориентации в циклических видах спорта на примере академической гребли, разработанная на основе анализа и обобщения опыта Федеральной экспериментальной площадки на базе Ростовского областного училища олимпийского резерва. Описаны цели, задачи, содержание процедур спортивного отбора гребцов на всех этапах спортивной подготовки в УОР. Предложены формы организации спортивного отбора, а также образцы документов, регламентирующих экспериментальную деятельность в области спортивного отбора и ориентации. В приложении представлены модельные характеристики показателей, характеризующих основные системы организма гребца-академиста, а также уровень его спортивной подготовленности. Даны предложения по дальнейшему совершенствованию системы спортивного отбора и ориентации в спорте. Представляет интерес для специалистов, занимающихся спортивной подготовкой в училищах олимпийского резерва, а также студентов вузов и ссузов, обучающихся по направлению подготовки 49.03.01 Физическая культура.
title: ÐÑÐ¾Ð±Ð»ÐµÐ¼Ñ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ Ð±ÑÐ¾Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÑ ÐºÐ°Ð±ÐµÐ»ÐµÐ¹ 6-110 ÐºÐ Ð¸ ÑÐ¿Ð¾ÑÐ¾Ð±Ñ Ð¸Ñ ÑÐµÑÐµÐ½Ð¸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¡Ð¾Ð»Ð¾Ð²ÑÐµÐ²Ð°, ÐÑÐ¸ÑÑ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Ð°Ð±ÐµÐ»Ð¸
Ð±ÑÐ¾Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÐµ ÐºÐ°Ð±ÐµÐ»Ð¸
ÑÑ ÐµÐ¼Ñ Ð·Ð°Ð·ÐµÐ¼Ð»ÐµÐ½Ð¸Ñ Ð¸ ÑÐ¾ÐµÐ´Ð¸Ð½ÐµÐ½Ð¸Ñ
Ð¿Ð¾ÑÐµÑÐ¸ Ð°ÐºÑÐ¸Ð²Ð½Ð¾Ð¹ Ð¼Ð¾ÑÐ½Ð¾ÑÑÐ¸

description: ÐÐ´Ð½Ð¾ÑÐ°Ð·Ð½ÑÐµ ÐºÐ°Ð±ÐµÐ»Ð¸ Ñ Ð¸Ð·Ð¾Ð»ÑÑÐ¸ÐµÐ¹ Ð¸Ð· ÑÑÐ¸ÑÐ¾Ð³Ð¾ Ð¿Ð¾Ð»Ð¸ÑÑÐ¸Ð»ÐµÐ½Ð° Ð¿Ð¾Ð»ÑÑÐ¸Ð»Ð¸ ÑÐ¸ÑÐ¾ÐºÐ¾Ðµ ÑÐ°ÑÐ¿ÑÐ¾ÑÑÑÐ°Ð½ÐµÐ½Ð¸Ðµ Ð¸ ÑÐ¶Ðµ Ð´Ð¾ÑÑÐ°ÑÐ¾ÑÐ½Ð¾ ÑÐ¾ÑÐ¾ÑÐ¾ Ð¸Ð·ÑÑÐµÐ½Ñ. ÐÐµÐºÐ¾ÑÐ¾ÑÐ¾Ðµ Ð²ÑÐµÐ¼Ñ Ð½Ð°Ð·Ð°Ð´ Ð½Ð° ÑÑÐ½ÐºÐµ Ð¿Ð¾ÑÐ²Ð¸Ð»Ð°ÑÑ Ð¼Ð¾Ð´Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ñ Ð¾Ð´Ð½Ð¾ÑÐ°Ð·Ð½ÑÑ ÐºÐ°Ð±ÐµÐ»ÐµÐ¹ ÐºÐ»Ð°ÑÑÐ¾Ð² 6-110 ÐºÐ, Ð³Ð´Ðµ Ð² Ð¸Ñ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ñ Ð´Ð¾Ð±Ð°Ð²Ð»ÐµÐ½Ð° Ð±ÑÐ¾Ð½Ñ Ð¸Ð· Ð¿ÑÐ¾Ð²Ð¾Ð»Ð¾Ðº Ð°Ð»ÑÐ¼Ð¸Ð½Ð¸Ñ Ð¸Ð»Ð¸ ÐµÐ³Ð¾ ÑÐ¿Ð»Ð°Ð²Ð°. ÐÐºÐ°Ð·Ð°Ð»Ð¾ÑÑ, ÑÑÐ¾ Ñ ÑÐ°ÐºÐ¾Ð³Ð¾ Ð±ÑÐ¾Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð³Ð¾ ÐºÐ°Ð±ÐµÐ»Ñ Ð¸Ð¼ÐµÐµÑÑÑ ÑÑÐ´ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐµÐ¹, ÐºÐ¾ÑÐ¾ÑÑÐµ Ð½ÐµÐ»ÑÐ·Ñ Ð¾ÑÑÐ°Ð²Ð»ÑÑÑ Ð±ÐµÐ· Ð²Ð½Ð¸Ð¼Ð°Ð½Ð¸Ñ. ÐÑÐ¾Ð²Ð¾Ð»Ð¾ÑÐ½Ð°Ñ Ð±ÑÐ¾Ð½Ñ, ÑÐ°ÐºÐ¶Ðµ, ÐºÐ°Ðº Ð¸ Ð¿ÑÐ¾Ð²Ð¾Ð»Ð¾ÑÐ½ÑÐ¹ ÑÐºÑÐ°Ð½, Ð¿Ð¾Ð´Ð²ÐµÑÐ³Ð°ÐµÑÑÑ Ð½Ð°Ð²Ð¾Ð´ÐºÐ°Ð¼ Ð¾Ñ Ð¼Ð°Ð³Ð½Ð¸ÑÐ½Ð¾Ð³Ð¾ Ð¿Ð¾Ð»Ñ Ð¶Ð¸Ð»Ñ. Ð Ð±ÑÐ¾Ð½Ðµ Ð½Ð°Ð²Ð¾Ð´ÑÑÑÑ Ð½Ð°Ð¿ÑÑÐ¶ÐµÐ½Ð¸Ñ Ð¸ ÑÐ¾ÐºÐ¸ Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½Ð¾Ð¹ ÑÐ°ÑÑÐ¾ÑÑ, Ð²Ð¾Ð·Ð½Ð¸ÐºÐ°ÑÑ Ð¿Ð¾ÑÐµÑÐ¸ Ð°ÐºÑÐ¸Ð²Ð½Ð¾Ð¹ Ð¼Ð¾ÑÐ½Ð¾ÑÑÐ¸. Ð Ð°ÑÑÐµÑÑ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´Ð¸Ð»Ð¸ÑÑ Ñ Ð¿Ð¾Ð¼Ð¾ÑÑÑ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð¾Ð³Ð¾ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ Mathcad Ð¸ ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð¾Ð³Ð¾ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ EMTP. ÐÐ°ÑÐ¸ÑÐ° Ð±ÑÐ¾Ð½Ð¸ Ð¸ ÑÐºÑÐ°Ð½Ð¾Ð² Ð¾Ñ Ð½Ð°Ð²ÐµÐ´ÐµÐ½Ð½ÑÑ Ð½Ð°Ð¿ÑÑÐ¶ÐµÐ½Ð¸Ð¹ Ð¸ ÑÐ¾ÐºÐ¾Ð² Ð´Ð¾ÑÑÐ¸Ð³Ð°ÐµÑÑÑ Ð¿ÑÑÐµÐ¼ Ð¾Ð¿ÑÐ¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÑÐµÐ¼ Ð¸Ñ ÑÐ¾ÐµÐ´Ð¸Ð½ÐµÐ½Ð¸Ñ Ð¸ Ð·Ð°Ð·ÐµÐ¼Ð»ÐµÐ½Ð¸Ñ. ÐÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ñ ÑÐ¿Ð¾ÑÐ¾Ð±Ñ Ð±Ð¾ÑÑÐ±Ñ Ñ Ð¿Ð¾ÑÐµÑÑÐ¼Ð¸ Ð¼Ð¾ÑÐ½Ð¾ÑÑÐ¸ Ð² Ð±ÑÐ¾Ð½Ðµ. Ð ÑÐ°ÑÑÐ½Ð¾ÑÑÐ¸, Ð¾ÑÐºÐ°Ð· Ð¾Ñ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ Ð±ÑÐ¾Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÑ ÐºÐ°Ð±ÐµÐ»ÐµÐ¹ Ð² Ð¿Ð¾Ð»ÑÐ·Ñ Ð¿ÑÐ¾ÐºÐ»Ð°Ð´ÐºÐ¸ ÐºÐ°Ð±ÐµÐ»ÐµÐ¹ Ð² Ð¿Ð¾Ð»Ð¸Ð¼ÐµÑÐ½ÑÑ ÑÑÑÐ±Ð°Ñ Ñ ÑÐ¾ÑÑÐ°Ð½ÐµÐ½Ð¸ÐµÐ¼ ÑÑÐµÐ±ÑÐµÐ¼Ð¾Ð¹ Ð¼ÐµÑÐ°Ð½Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð¿ÑÐ¾ÑÐ½Ð¾ÑÑÐ¸.
Additional file 3 of Transcriptomics and metabolomics reveal changes in the regulatory mechanisms of osteosarcoma under different culture methods in vitro
Creators: name: Yang, Sen
name: Tian, Zhi
name: Feng, Yi
name: Zhang, Kun
name: Pan, Yongchun
name: Li, Yuan
name: Wang, Zhichao
name: Wei, Wenhao
name: Qiao, Xiaochen
name: Zhou, Ruhao
name: Yan, Lei
name: Li, Qian
name: Guo, Hua
name: Yuan, Jie
name: Li, Pengcui
name: Lv, Zhi
Publisher: name: figshare
Year: 2023
Subjects: subject: Biochemistry
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Genetics
subject: Molecular Biology
subject: Physiology
subject: Chemical Sciences not elsewhere classified
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer
subject: Computational Biology

description: Additional file 3: Fig S3. Principal component analysis of ion quantification in each 3D OS tissue. QC samples are clustered, indicating that the experimental data is of high quality. A POS, B NEG.
Jet Precession Driven by Neutrino-Cooled Disc for Gamma-Ray Bursts
Creators: name: Liu, Tong
name: Liang, En-Wei
name: Gu, Wei-Min
name: Zhao, Xiao-Hong
name: Dai, Zi-Gao
name: Lu, Ju-Fu
Publisher: name: arXiv
Year: 2010
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: A model of jet precession driven by a neutrino-cooled disc around a spinning black hole is present in order to explain the temporal structure and spectral evolution of gamma-ray bursts (GRBs). The differential rotation of the outer part of a neutrino dominated accretion disc may result in precession of the inner part of the disc and the central black hole, hence drives a precessed jet via neutrino annihilation around the inner part of the disc. Both analytic and numeric results for our model are present. Our calculations show that a black hole-accretion disk system with black hole mass $M \simeq 3.66 M_\odot$, accretion rate $\dot{M} \simeq 0.54 M_\odot \rm s^{-1}$, spin parameter $a=0.9$ and viscosity parameter $α=0.01$ may drive a precessed jet with period P=1 s and luminosity $L=10^{51}$ erg s$^{-1}$, corresponding to the scenario for long GRBs. A precessed jet with $P=0.1$s and $L=10^{50}$ erg s$^{-1}$ may be powered by a system with $M \simeq 5.59 M_\odot$, $\dot{M} \simeq 0.74 M_\odot \rm s^{-1}$, $a=0.1$, and $α=0.01$, possibly being responsible for the short GRBs. Both the temporal and spectral evolution in GRB pulse may explained with our model. GRB central engines likely power a precessed jet driven by a neutrino-cooled disc. The global GRB lightcurves thus could be modulated by the jet precession during the accretion timescale of the GRB central engine. Both the temporal and spectral evolution in GRB pulse may be due to an viewing effect due to the jet precession.
description: 5 pages, 4 figures, accepted for publication in Astronomy and Astrophysics
Compartilhamento e uso de dados de pesquisa: um questionário para os pesquisadores da Universidade Federal do Estado do Rio de Janeiro (UNIRIO)
Creators: name: Jesus, Lyvia Araujo Rocha de
name: Pereira, Solange Campos
name: Menezes, Maria Simone Alencar
Publisher: name: Zenodo
Year: 2021

description: Apresentação realizada na sessão O meu Póster num minuto da 12ª Conferência Luso-Brasileira de Ciência Aberta, formato híbrido, de 13 a 15 de outubro de 2021.
First detection of a magnetic field in low-luminosity B[e] stars: New scenarios for the nature and evolutionary stages of FS CMa stars
Creators: name: Korcakova, D.
name: Sestito, F.
name: Manset, N.
name: Kroupa, P.
name: Votruba, V.
name: Slechta, M.
name: Danford, S.
name: Dvorakova, N.
name: Raj, A.
name: Chojnowski, S. D.
name: Singh, H. P.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We report the first detection of the magnetic field in a star of FS CMa type, a subgroup of objects characterized by the B[e] phenomenon. The split of magnetically sensitive lines in IRAS 17449+2320 determines the magnetic field modulus of 6.2+/-0.2 kG. Spectral lines and their variability reveal the presence of a B-type spectrum and a hot continuum source in the visible. The hot source confirms GALEX UV photometry. Because there is a lack of spectral lines for the hot source in the visible, the spectral fitting gives only the lower temperature limit of the hot source, which is 50 000 K, and the upper limit for the B-type star of 11 100 K. The V/R ratio of the H alpha line shows quasiperiodic behavior on timescale of 800 days. We detected a strong red-shifted absorption in the wings of Balmer and OI lines in some of the spectra. The absorption lines of helium and other metals show no, or very small, variations, indicating unusually stable photospheric regions for FS CMa stars. We detected two events of material infall, which were revealed to be discrete absorption components of resonance lines. The discovery of the strong magnetic field together with the Gaia measurements of the proper motion show that the most probable nature of this star is that of a post-merger object created after the leaving the binary of the birth cluster. Another possible scenario is a magnetic Ap star around Terminal-Age Main Sequence (TAMS). On the other hand, the strong magnetic field defies the hypothesis that IRAS 17449+2320 is an extreme classical Be star. Thus, IRAS 17449+2320 provides a pretext for exploring a new explanation of the nature of FS CMa stars or, at least, a group of stars with very similar spectral properties.
title: Not as Simple(x) as it seems: the importance of radiological follow-up in HSV encephalitis
Creators: name: Vara, Sarina
Publisher: name: EURORAD
Year: 2021
Subjects: subject: Neuroradiology
subject: CNS
subject: Head and neck
subject: CT
subject: MR
subject: Haemorrhage
subject: Inflammation
subject: Clinical Cases

description: Clinical History: An 18-year-old male, with no significant past medical history, presented to hospital with a frontal headache, pyrexia, and generalised tonic-clonic seizures. Examination revealed no focal neurological deficit. He was commenced on intravenous acyclovir for suspected Herpes Simplex Encephalitis (HSE), prior to confirmation of Herpes Simplex Virus (HSV) from positive cerebrospinal fluid analysis. 

description: 18 years, male
title: Fünf Schulen - Fünf MakerSpaces: Making als Schulentwicklungsprojekt
Creators: name: Maurer, Björn
name: Ingold, Selina
Publisher: name: Publikationsserver der Pädagogischen Hochschule Thurgau
Year: 2022
Subjects: FabLab
Schulentwicklung

description: Making & more: gemeinsam Lernen gestalten. Book of Abstracts., p. 14
RUBI e o Rubicão
Creators: name: Reis, Clea Mara Barradas dos
name: Pereira, Vitor Silveira
name: Medeiros, Ana Lígia
name: Lessa, Luziana
Publisher: name: Zenodo
Year: 2021

description: Apresentação realizada na sessão O meu Póster num minuto da 12ª Conferência Luso-Brasileira de Ciência Aberta, formato híbrido, de 13 a 15 de outubro de 2021.
All Aboard? Transit Oriented Development Opportunities Around Suburban Commuter Rail Stations
Creators: name: Enns, Darren A.
Publisher: name: The University of British Columbia
Year: 2008

description: This report provides suburban communities which are adopting commuter rail technology with recommendations on how to maximize the potential for station area benefit. These recommendations were developed from a rigorous assessment of case studies, which used metrics based on Transit Oriented Development (TOD) to gauge the potential for station area development. The project overview is as follows: 1. Start with providing an overview of Transit Oriented Development, its history and relevance to commuter rail; 2. Examine the existing body of research around suburban station area development, Transit Oriented Development and commuter rail; 3. Develop a methodology and a set of metrics to examine different case studies; 4. Analyze the selected case studies using a defined and replicable set of methods; 5. Determine the lessons learned from the case studies; 6. Compile a set of recommendations for communities adopting commuter rail. The project selected case studies were in Seattle and Vancouver, with a total of six station areas examined; two in industrial suburbs, two in residential suburbs, and two in exurban locations. This matched pair approach was used to determine if there were any similar lessons to be learned from like cities in different regions. The sampling methodology within each case study looked at station area land use, pedestrian environments, commercial activity, employment activity, and residential activity. The methodology also controlled for commuter rail technology and community type to ensure that similar communities served by similar rail systems were used as case studies.
On the theory of Bose-condensate fluctuations in finite size systems
Creators: name: Bugrij, A. I.
name: Loktev, V. M.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: An asymptotic expansions for the grand partition function of ideal Bose gas in the canonical ensemble with arbitrary number of particles is obtained. It is shown that the expressions found are valid in the whole temperature region, the critical temperature included. A comparison between the asymptotic formulas for Bose-condensate fluctuations and the exact ones is carried out and their quantitative agreement is established.
On the wavenumber-frequency spectra of the wall pressure fluctuations in turbulent channel flow
Creators: name: Yang, Bowen
name: Yang, Zixuan
Publisher: name: arXiv
Year: 2022
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: Direct numerical simulations (DNS) of turbulent channel flows up to $Re_τ \approx 1000$ are conducted to investigate the three-dimensional (consisting of streamwise wavenumber, spanwise wavenumber and frequency) spectrum of wall pressure fluctuations. To develop a predictive model of the wavenumber-frequency spectrum from the wavenumber spectrum, the time decorrelation mechanisms of wall pressure fluctuations are investigated. It is discovered that the energy-containing part of the wavenumber-frequency spectrum of wall pressure fluctuations can be well predicted using a similar random sweeping model for streamwise velocity fluctuations. To refine the investigation, we further decompose the spectrum of the total wall pressure fluctuations into the auto spectra of rapid and slow pressure fluctuations, and the cross spectrum between them. We focus on evaluating the assumption applied in many predictive models, that is, the magnitude of the cross spectrum is negligibly small. The present DNS shows that neglecting the cross spectrum causes a maximum error up to 4.7dB in the sub-convective region for all Reynolds numbers under test. Our analyses indicate that the assumption of neglecting the cross spectrum needs to be applied carefully in the investigations of acoustics at low Mach numbers, in which the sub-convective components of wall pressure fluctuations make important contributions to the radiated acoustic power.
description: 27 pages, 18 figures
title: ÐÐ·ÑÑÐµÐ½Ð¸Ðµ Ð¿ÑÐ¾ÑÐµÑÑÐ¾Ð² ÑÑÑÑÐºÑÑÑÐ¾Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¿ÑÐ¸ Ð¿Ð¾Ð»ÑÑÐµÐ½Ð¸Ð¸ Ð¸ Ð¿Ð»Ð°ÑÑÐ¸ÑÐµÑÐºÐ¾Ð¹ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐµ Ð¼ÐµÑ Ð°Ð½Ð¾Ð»ÐµÐ³Ð¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÑ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð¾Ð² ÑÐ¸ÑÑÐµÐ¼Ñ "Ð°Ð»ÑÐ¼Ð¸Ð½Ð¸Ð¹ - Ð±Ð¾Ñ"
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ÐµÑÑÐ¾Ð²Ð°, ÐÐ»ÑÐ³Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: ÐÐ¾Ð¼Ð¿Ð¾Ð·Ð¸ÑÐ¸Ð¾Ð½Ð½ÑÐµ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ñ
ÐÐ»ÑÐ¼Ð¸Ð½Ð¸Ð¹
ÐÐ¾Ñ
ÐÐµÐ»ÑÐ½Ð¸ÑÑ (Ð´ÑÐ¾Ð±Ð¸Ð».) ÑÐ°ÑÐ¾Ð²ÑÐµ
ÐÐµÑÐ°Ð»Ð»Ñ

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð±ÑÐ»Ð¸ Ð¿Ð¾Ð»ÑÑÐµÐ½Ñ ÐºÐ¾Ð¼Ð¿Ð¾Ð·Ð¸ÑÐ¸Ð¾Ð½Ð½ÑÐµ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ñ ÑÐ¸ÑÑÐµÐ¼Ñ Ð°Ð»ÑÐ¼Ð¸Ð½Ð¸Ð¹-Ð±Ð¾Ñ, Ñ Ð¿Ð¾ÑÐ»ÐµÐ´ÑÑÑÐ¸Ð¼ Ð¸Ð·ÑÑÐµÐ½Ð¸ÐµÐ¼ Ð²Ð»Ð¸ÑÐ½Ð¸Ñ ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ñ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÐ¾Ð² Ð¼ÐµÑÐ°Ð½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð»ÐµÐ³Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð½Ð° ÑÑÑÑÐºÑÑÑÑ. ÐÐ¾Ð¼Ð¿Ð¾Ð·Ð¸ÑÐ¸Ð¾Ð½Ð½ÑÐµ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ñ Ð¿Ð¾Ð»ÑÑÐµÐ½Ñ Ð¼ÐµÑÐ¾Ð´Ð¾Ð¼ Ð¼ÐµÑÐ°Ð½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð»ÐµÐ³Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð² ÑÐ°ÑÐ¾Ð²Ð¾Ð¹ Ð¼ÐµÐ»ÑÐ½Ð¸ÑÐµ. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¾ ÐºÐ¾Ð¼Ð¿Ð°ÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð¾Ð², Ð² ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐµ ÐºÐ¾ÑÐ¾ÑÐ¾Ð³Ð¾ Ð¿Ð¾Ð»ÑÑÐµÐ½ Ð¿Ð¾Ð»ÑÑÐ°Ð±ÑÐ¸ÐºÐ°Ñ, ÑÐ²Ð¾Ð¹ÑÑÐ²Ð° Ð¸ ÑÑÑÑÐºÑÑÑÑ ÐºÐ¾ÑÐ¾ÑÐ¾Ð³Ð¾ Ð¸Ð·ÑÑÐ°Ð»Ð°ÑÑ Ð´Ð°Ð»ÐµÐµ. ÐÐµÑÐ°Ð½Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¸ÑÐ¿ÑÑÐ°Ð½Ð¸Ñ Ð½Ð° ÑÐ°ÑÑÑÐ¶ÐµÐ½Ð¸Ðµ Ð¸ Ð¾ÑÐ°Ð´ÐºÑ Ð´Ð¾ÐºÐ°Ð·Ð°Ð»Ð¸, ÑÑÐ¾ Ð¿Ð¾Ð»ÑÑÐµÐ½Ð½ÑÐ¹ ÐºÐ¾Ð¼Ð¿Ð¾Ð·Ð¸ÑÐ¸Ð¾Ð½Ð½ÑÐ¹ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð» Ð¼Ð¾Ð¶ÐµÑ Ð¿Ð¾Ð´Ð²ÐµÑÐ³Ð°ÑÑÑÑ Ð´Ð¾Ð¿Ð¾Ð»Ð½Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð¹ Ð¿Ð»Ð°ÑÑÐ¸ÑÐµÑÐºÐ¾Ð¹ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐµ.
title: Ð Ð°Ð·Ð²Ð¸ÑÐ¸Ðµ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾-ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¼ÐµÑ Ð°Ð½Ð¸Ð·Ð¼Ð° Â«Ð·ÐµÐ»ÐµÐ½ÑÑ Â» Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¹ Ð² Ð½ÐµÑÑÐµÐ³Ð°Ð·Ð¾Ð²Ð¾Ð¼ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐµ
title: ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÑ 08.00.05 â Ð­ÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ° Ð¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð½Ð°ÑÐ¾Ð´Ð½ÑÐ¼ Ñ Ð¾Ð·ÑÐ¹ÑÑÐ²Ð¾Ð¼ (ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸ÑÐ¼Ð¸)
titleType: Subtitle
Creators: name: ÐÐ°Ð³ÑÑÐµÐ½ÐºÐ¾Ð², ÐÐ»ÐµÐºÑÐµÐ¹
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2022
Subjects: Â«Ð·ÐµÐ»ÐµÐ½ÑÐµÂ» Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¸
Ð½ÐµÑÑÐµÐ³Ð°Ð·Ð¾Ð²ÑÐ¹ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑ
Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾-ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð¼ÐµÑ Ð°Ð½Ð¸Ð·Ð¼ Ð¿Ð¾Ð´Ð´ÐµÑÐ¶ÐºÐ¸
ÑÑÐ°Ð½ÑÑÐµÑ ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¹

description: ÐÐµÑÐµÑÐ¾Ð´ Ð¼Ð¸ÑÐ¾Ð²Ð¾Ð¹ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ¸ Ð¾Ñ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ³Ð»ÐµÐ²Ð¾Ð´Ð¾ÑÐ¾Ð´Ð¾Ð² ÐºÐ¾ Ð²ÑÐµ Ð±Ð¾Ð»ÐµÐµ ÑÐ°ÑÑÐ¸ÑÑÑÑÐµÐ¼ÑÑÑ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ Ð²Ð¾Ð·Ð¾Ð±Ð½Ð¾Ð²Ð»ÑÐµÐ¼ÑÑ Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ¾Ð² ÑÐ½ÐµÑÐ³Ð¸Ð¸, Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÐµÑÑÑÑÐ¾Ð² Ñ Ð½Ð¸Ð·ÐºÐ¸Ð¼ ÑÐ³Ð»ÐµÑÐ¾Ð´Ð½ÑÐ¼ ÑÐ»ÐµÐ´Ð¾Ð¼ Ð¾Ð±ÑÑÐ»Ð¾Ð²Ð»Ð¸Ð²Ð°ÐµÑ Ð°ÐºÑÑÐ°Ð»ÑÐ½Ð¾ÑÑÑ ÐºÐ»Ð¸Ð¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ð¹ Ð¿Ð¾Ð²ÐµÑÑÐºÐ¸ Ð½Ð° Ð½Ð°ÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ð¼ ÑÑÐ¾Ð²Ð½Ðµ. ÐÐ°Ð½Ð½Ð°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐµ Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ñ Ð¿Ð¾Ð´ÑÐ¾Ð´Ð¾Ð² Ðº ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾-ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¼ÐµÑÐ°Ð½Ð¸Ð·Ð¼Ð° Ð¿Ð¾Ð´Ð´ÐµÑÐ¶ÐºÐ¸ Â«Ð·ÐµÐ»ÐµÐ½ÑÑÂ» Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¹ Ð² Ð½ÐµÑÑÐµÐ³Ð°Ð·Ð¾Ð²Ð¾Ð¼ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐµ Ð² ÑÑÐ»Ð¾Ð²Ð¸ÑÑ ÑÐ°Ð½ÐºÑÐ¸Ð¾Ð½Ð½ÑÑ Ð¾Ð³ÑÐ°Ð½Ð¸ÑÐµÐ½Ð¸Ð¹.
Lattice dynamics in magnetic superelastic Ni-Mn-In alloys. Neutron scattering and ultrasonic experiments
Creators: name: Moya, Xavier
name: Gonzalez-Alonso, David
name: Manosa, Lluis
name: Planes, Antoni
name: Garlea, V. O.
name: Lograsso, T. A.
name: Schlagel, D. L.
name: Zarestky, J. L.
name: Aksoy, Seda
name: Acet, Mehmet
Publisher: name: arXiv
Year: 2009
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Neutron scattering and ultrasonic methods have been used to study the lattice dynamics of two single crystals of Ni-Mn-In Heusler alloys close to Ni$_{50}$Mn$_{34}$In$_{16}$ magnetic superelastic composition. The paper reports the experimental determination of the low-lying phonon dispersion curves and the elastic constants for this alloy system. We found that the frequencies of the TA$_{2}$ branch are relatively low and it exhibits a small dip anomaly at a wave number $ξ_{0} \approx 1/3$, which softens with decreasing temperature. Associated with the softening of this phonon, we also observed the softening of the shear elastic constant $C'=(C_{11}-C_{12})/2$. Both temperature softenings are typical for bcc based solids which undergo martensitic transformations and reflect the dynamical instability of the cubic lattice against shearing of $\{110\}$ planes along $<1\bar{1}0>$ directions. Additionally, we measured low-lying phonon dispersion branches and elastic constants in applied magnetic fields aimed to characterize the magnetoelastic coupling.
description: 8 pages, 7 figures. Accepted for publication in the Physical Review B
title: ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¿Ð°ÑÐ°Ð»Ð»ÐµÐ»ÑÐ½ÑÑ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ð¾Ð² Ð¿Ð¾Ð¸ÑÐºÐ° Ñ Ð°ÑÐ°ÐºÑÐµÑÐ½ÑÑ Ð½Ð°Ð±Ð¾ÑÐ¾Ð² Ñ Ð¿Ð¾Ð¼Ð¾ÑÑÑ ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ GPU
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¸ÑÑÐ½, ÐÐ»Ð°Ð´Ð¸ÑÐ»Ð°Ð²
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: ÐÐ»Ð³Ð¾ÑÐ¸ÑÐ¼Ñ
ÐÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐ·ÑÐºÐ¸
Ñ Ð°ÑÐ°ÐºÑÐµÑÐ½ÑÐµ Ð½Ð°Ð±Ð¾ÑÑ
Ð¸Ð½ÑÐµÐ»Ð»ÐµÐºÑÑÐ°Ð»ÑÐ½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· Ð´Ð°Ð½Ð½ÑÑ
Ð°ÑÑÐ¾ÑÐ¸Ð°ÑÐ¸Ð²Ð½ÑÐµ Ð¿ÑÐ°Ð²Ð¸Ð»Ð°

description: Ð ÑÐ¾Ð´Ðµ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ ÑÐ°Ð±Ð¾ÑÑ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ Ð¿Ð°ÑÐ°Ð»Ð»ÐµÐ»ÑÐ½ÑÐµ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ñ Eclat Ð¸ FPG Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ ÐºÑÐ¾ÑÑÐ¿Ð»Ð°ÑÑÐ¾ÑÐ¼ÐµÐ½Ð½Ð¾Ð¹ Ð¸ Ð°Ð¿Ð¿Ð°ÑÐ°ÑÐ½Ð¾Ð¹ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ GPU OpenCL. ÐÑÑÑÐµÑÑÐ²Ð»ÐµÐ½Ð¾ ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ðµ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð´Ð°Ð½Ð½ÑÑ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ð¾Ð² Ð¸ Ð´Ð°Ð½Ñ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¸Ñ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ.
Small-World Networks in Geophysics
Creators: name: Yang, Xin-She
Publisher: name: arXiv
Year: 2010
Subjects: subject: Geophysics (physics.geo-ph)
subject: Physics and Society (physics.soc-ph)
subject: FOS: Physical sciences
subject: geophysics

description: Many geophysical processes can be modelled by using interconnected networks. The small-world network model has recently attracted much attention in physics and applied sciences. In this paper, we try to use and modify the small-world theory to model geophysical processes such as diffusion and transport in disordered porous rocks. We develop an analytical approach as well as numerical simulations to try to characterize the pollutant transport and percolation properties of small-world networks. The analytical expression of system saturation time and fractal dimension of small-world networks are given and thus compared with numerical simulations.
Insights into the genetic and host adaptability of emerging porcine circovirus 3
Creators: name: Li, Gairu
name: Wang, Huijuan
name: Wang, Shilei
name: Xing, Gang
name: Zhang, Cheng
name: Zhang, Wenyan
name: Liu, Jie
name: Zhang, Junyan
name: Su, Shuo
name: Zhou, Jiyong
Publisher: name: Taylor & Francis
Year: 2018
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Genetics
subject: Molecular Biology
subject: Biotechnology
subject: Evolutionary Biology
subject: Environmental Sciences not elsewhere classified
subject: Ecology

description: Porcine circovirus 3 (PCV3) was found to be associated with reproductive disease in pigs, and since its first identification in the United States, it subsequently spread worldwide, especially in China, where it might pose a potential threat to the porcine industry. However, no exhaustive analysis was performed to understand its evolution in the prospect of codon usage pattern. Here, we performed a deep codon usage analysis of PCV3. PCV3 sequences were classified into two clades: PCV3a and PCV3b, confirmed by principal component analysis. Additionally, the degree of codon usage bias of PCV3 was slightly low as inferred from the analysis of the effective number of codons. The codon usage pattern was mainly affected by natural selection, but there was a co-effect of mutation pressure and dinucleotide frequency. Moreover, based on similarity index analysis, codon adaptation index analysis and relative codon deoptimization index analysis, we found that PCV3 might pose a potential risk to public health though with unknow pathogenicity. In conclusion, this work reinforces the systematic understanding of the evolution of PCV3, which was reflected by the codon usage patterns and fitness of this novel emergent virus.
Strong [OIII]λ5007 emission line compact galaxies in LAMOST DR9: Blueberries, Green Peas and Purple Grapes
Creators: name: Liu, Siqi
name: Luo, A-Li
name: Yang, Huan
name: Shen, Shi-Yin
name: Wang, Jun-Xian
name: Zhang, Hao-Tong
name: Zheng, Zhenya
name: Song, Yi-Han
name: Kong, Xiao
name: Wang, Jian-Ling
name: Chen, Jian-Jun
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Green Pea and Blueberry galaxies are well-known for their compact size, low mass, strong emission lines and analogs to high-z Lyα emitting galaxies. In this study, 1547 strong [OIII]λ5007 emission line compact galaxies with 1694 spectra are selected from LAMOST DR9 at the redshift range from 0.0 to 0.59. According to the redshift distribution, these samples can be separated into three groups: Blueberries, Green Peas and Purple Grapes. Optical [MgII]λ2800 line feature, BPT diagram, multi-wavelength SED fitting, MIR color, and MIR variability are deployed to identify 23 AGN candidates from these samples, which are excluded for the following SFR discussions. We perform the multi-wavelength SED fitting with GALEX UV and WISE MIR data. Color excess from Balmer decrement shows these strong [OIII]λ5007 emission line compact galaxies are not highly reddened. The stellar mass of the galaxies is obtained by fitting LAMOST calibrated spectra with the emission lines masked. We find that the SFR is increasing with the increase of redshift, while for the sources within the same redshift bin, the SFR increases with mass with a similar slope as the SFMS. These samples have a median metallicity of 12+log(O/H) of 8.10. The metallicity increases with mass, and all the sources are below the mass-metallicity relation. The direct-derived Te-based metallicity from the [OIII]λ4363 line agrees with the empirical N2-based empirical gas-phase metallicity. Moreover, these compact strong [OIII]λ5007 are mostly in a less dense environment.
description: 13 pages, 20 figures, accepted by ApJ
Compact Q-balls and Q-shells in a scalar electrodynamics
Creators: name: Arodź, H.
name: Lis, J.
Publisher: name: arXiv
Year: 2008
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Pattern Formation and Solitons (nlin.PS)
subject: FOS: Physical sciences

description: We investigate spherically symmetric non topological solitons in electrodynamics with a scalar field self interaction U ~|ψ| taken from the complex signum-Gordon model. We find Q-balls for small absolute values of the total electric charge Q, and Q-shells when |Q| is large enough. In both cases the charge density exactly vanishes outside certain compact region in the three dimensional space. The dependence of the total energy E of small Q-balls on the total electric charge has the form E ~ |Q|^(5/6), while in the case of very large Q-shells E ~ |Q|^(7/6).
description: 21 pages, 7 figures
title: ÐÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½ÑÐ¹ Ð¼ÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½Ñ
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð²ÑÑÑÐ¸Ñ ÑÑÐµÐ±Ð½ÑÑ Ð·Ð°Ð²ÐµÐ´ÐµÐ½Ð¸Ð¹, Ð¾Ð±ÑÑÐ°ÑÑÐ¸Ñ ÑÑ Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ¾Ð² Â«Ð¢ÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¼Ð°ÑÐ¸Ð½Ñ Ð¸ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸ÐµÂ»
titleType: Subtitle
Creators: name: ÐÐ¾Ð¼ÑÐµÐ½ÐºÐ¾, Ð®ÑÐ¸Ð¹
name: ÐÐ¾ÑÐ¼Ð°ÑÐ¾Ð², Ð­Ð´ÑÐ°ÑÐ´
name: ÐÐ²ÑÐ°ÑÐ¾Ð²Ð°, ÐÐºÐ°ÑÐµÑÐ¸Ð½Ð°
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2013
Subjects: Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½ÑÐ¹ Ð¼ÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½Ñ
ÑÑÐµÐ±Ð½Ð¸ÐºÐ¸ Ð¸ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Ð´Ð»Ñ Ð²ÑÐ·Ð¾Ð²

description: Ð¡Ð¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÐµÑ ÑÐ¾Ð´ÐµÑÐ¶Ð°Ð½Ð¸Ñ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ñ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ ÑÑÐ°Ð½Ð´Ð°ÑÑÐ° Â«ÐÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½ÑÐ¹ Ð¼ÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½ÑÂ». ÐÐ·Ð»Ð¾Ð¶ÐµÐ½Ñ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¸ Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¾ÑÐ½Ð¾Ð²Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿ÑÐ¾ÑÐµÑÑÐ¾Ð¼ Ð¿ÑÐ¸Ð¾Ð±ÑÐµÑÐµÐ½Ð¸Ñ Ð¸ Ð¿ÑÐµÐ¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐµÑÑÑÑÐ¾Ð² Ð² Ð³Ð¾ÑÐ¾Ð²ÑÐ¹ Ð¿ÑÐ¾Ð´ÑÐºÑ. Ð ÑÐ°ÑÑÐ½Ð¾ÑÑÐ¸, ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ ÑÐ°ÐºÐ¸Ðµ Ð²Ð¾Ð¿ÑÐ¾ÑÑ, ÐºÐ°Ðº Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ñ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÑÐµÑÑÐ°, ÑÑÑÐ°ÑÐµÐ³Ð¸ÑÐµÑÐºÐ¾Ðµ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð¼Ð¾ÑÐ½Ð¾ÑÑÑÑ, Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð°, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½ÑÐµ Ð³ÑÐ°ÑÐ¸ÐºÐ¸ - ÑÐ°ÑÐ¿Ð¸ÑÐ°Ð½Ð¸Ñ Ð¸ ÐºÐ¾Ð½ÑÑÐ¾Ð»Ñ Ð¸Ñ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ, ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ°Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ° Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð°, Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ñ ÑÐ¾Ð²Ð¼ÐµÑÑÐ½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð², Ð¾Ð±ÑÑÐ°ÑÑÐ¸ÑÑÑ Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Â«ÐÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½ÑÂ».
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°.
O'ZBEKISTONDA TURIZIMNING BARQAROR RIVOJLANISH YO'NALISHLARI
Creators: name: Xudoyberdiyeva, Hilola
Publisher: name: Zenodo
Year: 2025

description: Mazkur maqolada O‘zbekistonda turizmning barqaror rivojlanish yo’nalishlari va holati va taraqqiyoti industriyasi,ichki turizmni rivojlantirishning dolzarbligi va mamlakatning turizm infratuzilmasi tarmoqlariga alohida e’tibor qaratilgan. Shuningdek, turizm sohasini rivojlantirish bo‘yicha davlat siyosati va strategiyasini amalga oshirish jarayonida muhim tarmoqlardan biriga aylanib ulgurgan soha hisoblanadi.
title: Оценка качества технологических процессов с помощью контрольных карт
Creators: name: ELS IPR BOOKS
Publisher: name: Донской государственный технический университет
Year: 2022

description: Описаны методы контроля и обеспечения качества продукции с помощью использования контрольных карт. Предназначено для обучающихся бакалавриата и магистратуры, изучающих дисциплину «Управление качеством»», а также для специалистов предприятий.
Subleading Jet Functions in Inclusive B Decays
Creators: name: Paz, Gil
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The contribution of subleading jet functions to inclusive decay distributions of $B$ mesons are derived from a systematic two-step matching of QCD current correlators onto soft collinear and heavy quark effective theory. Focusing on the tree level matching of QCD onto soft collinear effective theory, the subleading jet functions are defined to all orders in $α_s(μ_i)$ (with $μ_i^2\sim m_bΛ_{\rm QCD}$) and are calculated explicitly at first order in $α_s(μ_i)$. We present explicit expressions for the decay rates of $B\to X_u l \barν$ and the $Q_{7γ}-Q_{7γ}$ contribution to $B\to X_s γ$, where the subleading jet functions are multiplied by a tree level hard function and appear in a convolution with the leading order shape function. Together with the recent two loop calculation of the leading order hard function for $B\to X_u l \barν$, this paper will allow for a more precise description of inclusive B decays in the end point region.
description: Minor changes: reference added, typos corrected, journal version
title: Ð§Ð¸ÑÐ»ÐµÐ½Ð½ÑÐµ Ð¼ÐµÑÐ¾Ð´Ñ ÑÐµÑÐµÐ½Ð¸Ñ Ð»Ð¸Ð½ÐµÐ¹Ð½Ð¾Ð¹ Ð·Ð°Ð´Ð°ÑÐ¸ Ð´Ð¾Ð¿Ð¾Ð»Ð½Ð¸ÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¼Ð°Ð³Ð¸ÑÑÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¸Ð½ÐµÐ²Ð¸Ñ, ÐÐ»ÑÐ³Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: Ð§Ð¸ÑÐ»ÐµÐ½Ð½ÑÐµ Ð¼ÐµÑÐ¾Ð´Ñ
ÐÑÐ¿ÑÐºÐ»Ð¾Ðµ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
ÐÐ°ÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ðµ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ

description: ÐÐ°Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° Ð¸Ð·ÑÑÐµÐ½Ð¸Ñ ÑÐ¸ÑÐ»ÐµÐ½Ð½ÑÑ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² ÑÐµÑÐµÐ½Ð¸Ñ Ð»Ð¸Ð½ÐµÐ¹Ð½Ð¾Ð¹ Ð·Ð°Ð´Ð°ÑÐ¸ Ð´Ð¾Ð¿Ð¾Ð»Ð½Ð¸ÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸. Ð ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑÑÑ ÑÐ²Ð¾Ð¹ÑÑÐ²Ð° Ð»Ð¸Ð½ÐµÐ¹Ð½Ð¾Ð¹ Ð·Ð°Ð´Ð°ÑÐ¸ Ð´Ð¾Ð¿Ð¾Ð»Ð½Ð¸ÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð´Ð»Ñ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÑ ÐºÐ»Ð°ÑÑÐ¾Ð² Ð¼Ð°ÑÑÐ¸Ñ. Ð¢ÐµÐ¾ÑÐ¸Ñ Ð»Ð¸Ð½ÐµÐ¹Ð½Ð¾Ð¹ Ð´Ð¾Ð¿Ð¾Ð»Ð½Ð¸ÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐ¸Ð¼ÐµÐ½ÑÐµÑÑÑ Ðº Ð·Ð°Ð´Ð°ÑÐ°Ð¼ ÐºÐ²Ð°Ð´ÑÐ°ÑÐ¸ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ. Ð Ð°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑÑÑ Ð¿ÑÑÐ¼ÑÐµ Ð¸ Ð¸ÑÐµÑÐ°ÑÐ¸Ð¾Ð½Ð½ÑÐµ ÑÐ¸ÑÐ»ÐµÐ½Ð½ÑÐµ Ð¼ÐµÑÐ¾Ð´Ñ ÑÐµÑÐµÐ½Ð¸Ñ. ÐÐ»Ñ ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ñ ÑÐ¸ÑÐ»ÐµÐ½Ð½ÑÑ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² Ð¿ÑÐ¸Ð²Ð¾Ð´ÑÑÑÑ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ ÑÐµÑÐ¸Ð¸ Ð²ÑÑÐ¸ÑÐ»Ð¸ÑÐµÐ»ÑÐ½ÑÑ ÑÐºÑÐ¿ÐµÑÐ¸Ð¼ÐµÐ½ÑÐ¾Ð² Ð´Ð»Ñ Ð·Ð°Ð´Ð°ÑÐ¸ Ð¾ ÑÐ²ÐµÐ´ÐµÐ½Ð¸Ð¸ Ð·Ð°Ð·Ð¾ÑÐ° Ð¼ÐµÐ¶Ð´Ñ Ð´ÐµÑÐ°Ð»ÑÐ¼Ð¸.
Insights into the evolution of five isolated galaxies
Creators: name: Mazzei, Paola
name: Rampazzo, Roberto
name: Marino, Antonietta
name: Trinchieri, Ginevra
name: Uslenghi, Michela
name: Wolter, Anna
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The galaxy evolution is believed to be conditioned by the environment. Isolated galaxies or galaxies in poor groups are an excellent laboratory to study evolutionary mechanisms where effects of the environment are minimal. We present new {\it Swift}-{\tt UVOT} data in six filters, three in the ultraviolet (UV), of five isolated galaxies aiming at shedding light into their evolution. For all of our targets we present new UV integrated fluxes and for some of them also new UBV magnitudes. Our observations allow us to improve their multi-wavelength spectral energy distributions extending it over about 3 orders of magnitude in wavelength. We exploit our smooth-particle hydro-dynamical simulations with chemo-photometric implementation anchored, a posteriori, to the global multi-wavelength properties of our targets, to give insight into their evolution. Then we compare their evolutionary properties with those previously derived for several galaxies in groups. The evolution of our targets is driven by a merger occurred several Gyrs ago, in the redshift range $0.5\leq z \leq 4.5$, not unlike what we have already found for galaxies in groups. The merger shapes the potential well where the gas is accreting driving the star formation rate and the galaxy evolution. Isolated galaxies should not have suffered from interactions for at least 3\,Gyr. However, the initial merger is still leaving its signatures on the properties of our targets. Several rejuvenation episodes, triggered by {\it in situ} accretion, are highlighted. Moreover, jelly-fish morphologies appear as these galaxies achieve their maximum star formation rate, before their quenching phase.
description: 25 pages, 19 figures, 10 tables, Accepted for pubblication in ApJ
Asymptotic dimension, Property A, and Lipschitz maps
Creators: name: Cencelj, M.
name: Dydak, J.
name: Vavpetic, A.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Metric Geometry (math.MG)
subject: Geometric Topology (math.GT)
subject: FOS: Mathematics
subject: 54F45, 55M10

description: It is well-known that a paracompact space X is of covering dimension n if and only if any map f from X to a simplicial complex K can be pushed into its n-skeleton. We use the same idea to define dimension in the coarse category. It turns out the analog of maps f from X to K is related to asymptotically Lipschitz maps, the analog of paracompact spaces are spaces related to Yu's Property A, and the dimension coincides with Gromov's asymptotic dimension.
description: 10 pages
title: Ð Ð¾Ð±Ð°ÑÑÐ½Ð¾Ðµ Ð²ÑÑÐ¾ÐºÐ¾ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾Ðµ Ð¾ÑÐµÐ½Ð¸Ð²Ð°Ð½Ð¸Ðµ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÐ° Ð¼Ð°ÑÑÑÐ°Ð±Ð° ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ð¹ Ð¡ÑÑÑÐ´ÐµÐ½ÑÐ°
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¸ÑÐ²Ð¸Ð½Ð¾Ð²Ð°, ÐÐµÑÐ¾Ð½Ð¸ÐºÐ°
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Ð¾Ð±Ð°ÑÑÐ½Ð¾ÑÑÑ
Ð-Ð¾ÑÐµÐ½ÐºÐ¸
Ð¿Ð°ÑÐ°Ð¼ÐµÑÑ Ð¼Ð°ÑÑÑÐ°Ð±Ð°

description: ÐÐ·Ð²ÐµÑÑÐ½Ð°Ñ Ð²ÑÑÐ¾ÐºÐ¾ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð°Ñ ÑÐ¾Ð±Ð°ÑÑÐ½Ð°Ñ - Ð¾ÑÐµÐ½ÐºÐ° Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÐ° Ð¼Ð°ÑÑÑÐ°Ð±Ð°, Ð¿Ð¾Ð»ÑÑÐµÐ½Ð½Ð°Ñ Ð² ÑÐ°Ð±Ð¾ÑÐµ Ð ÑÑÑÐµÑ Ð¸ ÐÑÑÐºÑÐ° (1993), Ð°Ð¿Ð¿ÑÐ¾ÐºÑÐ¸Ð¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð° Ñ Ð¿Ð¾Ð¼Ð¾ÑÑÑ Ð±ÑÑÑÑÑÑ M-Ð¾ÑÐµÐ½Ð¾Ðº Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÐ° Ð¼Ð°ÑÑÑÐ°Ð±Ð°, Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð½ÑÑ Ð¥ÑÑÐ±ÐµÑÐ¾Ð¼. ÐÐ° ÑÑÐµÑ Ð²ÑÐ±Ð¾ÑÐ° Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÐ¾Ð² Ð°Ð¿Ð¿ÑÐ¾ÐºÑÐ¸Ð¼Ð°ÑÐ¸Ð¸ Ð¿Ð¾Ð»ÑÑÐµÐ½Ð½Ð°Ñ Ð¾ÑÐµÐ½ÐºÐ° ÑÐ²Ð»ÑÐµÑÑÑ Ð²ÑÑÐ¾ÐºÐ¾ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾Ð¹ Ð¸ ÑÐ¾Ð±Ð°ÑÑÐ½Ð¾Ð¹ Ð½Ð° ÑÐµÐ¼ÐµÐ¹ÑÑÐ²Ðµ ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ð¹ Ð¡ÑÑÑÐ´ÐµÐ½ÑÐ°, Ð²ÐºÐ»ÑÑÐ°Ñ ÑÐ°ÑÑÐ½ÑÐµ ÑÐ»ÑÑÐ°Ð¸ Ð½Ð¾ÑÐ¼Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ Ð¸ ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ ÐÐ¾ÑÐ¸. ÐÑÑÐ¸ÑÐ»ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ¸ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¸ ÑÐ¾Ð±Ð°ÑÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð½Ð¾Ð¹ Ð¾ÑÐµÐ½ÐºÐ¸: Ð°ÑÐ¸Ð¼Ð¿ÑÐ¾ÑÐ¸ÑÐµÑÐºÐ°Ñ Ð´Ð¸ÑÐ¿ÐµÑÑÐ¸Ñ Ð¸ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ, ÑÑÐ½ÐºÑÐ¸Ñ Ð²Ð»Ð¸ÑÐ½Ð¸Ñ, Ð¿Ð¾ÑÐ¾Ð³Ð¾Ð²ÑÐµ ÑÐ¾ÑÐºÐ¸. ÐÐ¾Ð»ÑÑÐµÐ½Ð½ÑÐµ Ð¾ÑÐµÐ½ÐºÐ¸ Ð¼Ð¾Ð³ÑÑ Ð±ÑÑÑ Ð¿Ð¾Ð»ÐµÐ·Ð½Ñ ÐºÐ°Ðº Ð¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ¼ ÑÑÐ°ÑÐ¸ÑÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¿Ð°ÐºÐµÑÐ¾Ð², ÑÐ°Ðº Ð¸ Ð¿ÑÐ¾ÑÐµÑÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½ÑÐ¼ ÑÑÐ°ÑÐ¸ÑÑÐ¸ÐºÐ°Ð¼ Ð¿ÑÐ¸ ÑÐ¸Ð½ÑÐµÐ·Ðµ Ð¸ Ð°Ð½Ð°Ð»Ð¸Ð·Ðµ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² ÑÐ¾Ð±Ð°ÑÑÐ½Ð¾Ð³Ð¾ Ð¾ÑÐµÐ½Ð¸Ð²Ð°Ð½Ð¸Ñ ÐºÐ¾ÑÑÑÐ¸ÑÐ¸ÐµÐ½ÑÐ° ÐºÐ¾ÑÑÐµÐ»ÑÑÐ¸Ð¸.
Towards a realistic evaluation of transport coefficients in non-equilibrium space plasmas
Creators: name: Husidic, Edin
name: Scherer, Klaus
name: Lazar, Marian
name: Fichtner, Horst
name: Poedts, Stefaan
Publisher: name: arXiv
Year: 2022
Subjects: subject: Plasma Physics (physics.plasm-ph)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Recent studies have outlined the interest for the evaluation of transport coefficients in space plasmas, where the observed velocity distributions of plasma particles are conditioned not only by the binary collisions, e.g., at low energies, but also by the energisation of particles from their interaction with wave turbulence and fluctuations, generating the suprathermal Kappa-distributed populations. This paper provides a first estimate of the main transport coefficients based on regularised Kappa distributions (RKDs), which, unlike standard Kappa distributions (SKDs), enable macroscopic parameterisation without mathematical divergences or physical inconsistencies. All transport coefficients derived here, i.e., the diffusion and mobility coefficients, electric conductivity, thermoelectric coefficient and thermal conductivity, are finite and well defined for all values of $κ> 0$. Moreover, for low values of $κ$ (i.e., below the SKD poles), the transport coefficients can be orders of magnitudes higher than the corresponding Maxwellian limits, meaning that significant underestimations can be made if suprathermal electrons are ignored.
description: 13 pages, 5 figures, 1 table
P.Oxy. XXX 2517. Homer Lexicon, Apollonius Sophista ? (see K. Alpers, Hermes 94 (1966) 430-4)
Creators: name: Oxyrhynchus Papyri
Publisher: name: University of Oxford
Year: 2022
Subjects: Latin and classical Greek languages

description: Reproduction requests: https://www.ees.ac.uk/reproduction-requests-and-fees
Sulfate radical oxidation of benzophenone: Kinetics, mechanisms and influence of water matrix anions
Creators: name: Ma, Jie
name: Feng, Yuan
name: Yang, Xin
name: Wu, Yongxin
name: Wang, Shuo
name: Zhang, Congchao
name: Shi, Quan
Publisher: name: Taylor & Francis
Year: 2020
Subjects: subject: Biophysics
subject: Biochemistry
subject: Space Science
subject: Physiology
subject: FOS: Biological sciences
subject: Environmental Sciences not elsewhere classified
subject: Chemical Sciences not elsewhere classified
subject: Ecology
subject: Biological Sciences not elsewhere classified
subject: Inorganic Chemistry
subject: FOS: Chemical sciences

description: Benzophenone (BP) is an emerging contaminant that is widely distributed in soil, groundwater, sediment and surface water. In this study, the degradation kinetics, mechanisms, and influence of anions on thermally activated persulfate (TAP) oxidation of BP were systematically investigated. BP degradation was promoted by elevated temperature. The BP degradation data fitted well to the Arrhenius equation with calculated activation energy of 122.8 kJ/mol. BP degradation was also promoted by alkaline pH and high persulfate concentrations. Radical scavenging experiments suggested that both SO4•− and HO• were involved in BP oxidation. Ultra-high-performance liquid chromatography coupled to Orbitrap mass spectrometry (UHPLC-Orbitrap-MS) identified six degradation intermediates. Based on these results, two possible reaction pathways were proposed. Water matrix anions had complex impacts on BP degradation by TAP. Cl− had dual effects on the reaction: low concentration promoted it while high concentration inhibited it. Br− strongly suppressed the reaction. SO42− and NO3− did not affect the reaction. Overall, this study shows that thermally activated persulfate can effectively remove BP and water matrix anions greatly influence the reaction.
Unsolved Problems about Supernovae
Creators: name: Panagia, Nino
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: A number of unsolved problems and open questions about the nature and the properties of supernovae are identified and briefly discussed. Some suggestions and directions toward possible solutions are also considered.
description: 7 pages, Proceedings of 'Probing Stellar Populations out to the Distant Universe', Cefalu, Italy, Sep 7-19, 2008, AIP Conf. Proc. Series
title: ÐÐ±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¹ Ð² ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ðµ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ
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Ð¼ÐµÐ»ÑÑÐ½Ð¾Ð², ÐÐ½ÑÐ¾Ð½
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¸
Ð¼ÐµÑÐ¾Ð´Ñ Ð¾ÑÐµÐ½ÐºÐ¸ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¹
Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½ÑÐ¹ Ð¿ÑÐ¾ÐµÐºÑ
ÑÑÐ¾Ðº Ð¾ÐºÑÐ¿Ð°ÐµÐ¼Ð¾ÑÑÐ¸
Ð´Ð¸ÑÐºÐ¾Ð½ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð´ÐµÐ½ÐµÐ¶Ð½ÑÑ Ð¿Ð¾ÑÐ¾ÐºÐ¾Ð²

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 Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¹ Ð² ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ðµ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ ÐÐÐ Â«Ð¥Ð¸Ð¼Ð¸ÐºÂ».
ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾-ÑÐ¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÑÐ¸Ð¼Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð·Ð°Ð²Ð¾Ð´Ð° Ð±ÑÐ»Ð¸ Ð²ÑÐ´ÐµÐ»ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ.
ÐÑÐ» ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½ Ð¿Ð»Ð°Ð½ Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¹ Ð² ÐºÐ°Ð¿Ð¸ÑÐ°Ð»ÑÐ½Ð¾Ðµ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð¾ Ð´Ð»Ñ ÐÐÐ Â«Ð¥Ð¸Ð¼Ð¸ÐºÂ», Ð° Ð¸Ð¼ÐµÐ½Ð½Ð¾ Ð¿Ð»Ð°Ð½ Ð¿Ð¾ ÑÐµÑÑÑÑÐºÑÑÑÐ¸Ð·Ð°ÑÐ¸Ð¸ Ð±Ð¸Ð·Ð½ÐµÑÐ°, Ð¿Ð¾Ð·Ð²Ð¾Ð»ÑÑÑÐ¸Ð¹ Ð¿ÐµÑÐµÐ¼ÐµÑÑÐ¸ÑÑ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½ÑÐµ Ð¼Ð¾ÑÐ½Ð¾ÑÑÐ¸ Ð½Ð° ÑÐ¾Ð±ÑÑÐ²ÐµÐ½Ð½ÑÐµ Ð¿Ð»Ð¾ÑÐ°Ð´Ð¸.
Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ñ Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¸ Ð² ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ðµ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ.
Ð Ð°ÑÑÑÐ¸ÑÐ°Ð½Ñ ÑÐ»ÐµÐ´ÑÑÑÐ¸Ðµ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸: ÑÐ¸ÑÑÐ°Ñ Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÐ½Ð½Ð°Ñ ÑÑÐ¾Ð¸Ð¼Ð¾ÑÑÑ, ÑÐµÐ½ÑÐ°Ð±ÐµÐ»ÑÐ½Ð¾ÑÑÑ Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¹, Ð²Ð½ÑÑÑÐµÐ½Ð½ÑÑ Ð½Ð¾ÑÐ¼Ð° Ð¿ÑÐ¸Ð±ÑÐ»Ð¸ Ð¸ ÑÑÐ¾Ðº Ð¾ÐºÑÐ¿Ð°ÐµÐ¼Ð¾ÑÑÐ¸.
ÐÑÑÑÐµÑÑÐ²Ð»ÐµÐ½Ð¸Ðµ Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ°, Ð° Ð¸Ð¼ÐµÐ½Ð½Ð¾ Ð¿ÐµÑÐµÑÐ¾Ð´ Ð½Ð° ÑÐ¾Ð±ÑÑÐ²ÐµÐ½Ð½ÑÐµ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½ÑÐµ Ð¿Ð»Ð¾ÑÐ°Ð´Ð¸, Ð¿Ð¾Ð·Ð²Ð¾Ð»Ð¸Ñ Ð¿ÑÐµÐ¾Ð´Ð¾Ð»ÐµÑÑ Ð½ÐµÐ´Ð¾ÑÑÐ°ÑÐ¾Ðº ÑÐ²Ð¾Ð±Ð¾Ð´Ð½ÑÑ Ð¿Ð»Ð¾ÑÐ°Ð´ÐµÐ¹ Ð¸ ÑÐ°ÑÑÐ¸ÑÐ¸ÑÑ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð¾, ÑÑÐ¾ Ð¿Ð¾Ð»Ð¾Ð¶Ð¸ÑÐµÐ»ÑÐ½Ð¾ Ð¿Ð¾Ð²Ð»Ð¸ÑÐµÑ Ð½Ð° ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ðµ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ.
Possible link of a structurally driven spin flip transition and the insulator-metal transition in the perovskite La$_{1-x}$Ba$_{x}$CoO$_{3}$
Creators: name: Tong, Peng
name: Yu, Juan
name: Huang, Qingzhen
name: Yamada, Kazuyoshi
name: Louca, Despina
Publisher: name: arXiv
Year: 2010
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: The complex nature of the magnetic ground state in La$_{1-x}$A$_{x}$CoO$_{3}$ (A = Ca, Sr, Ba) has been investigated via neutron scattering. It was previously observed that ferromagnetic (FM) as well as antiferromagnetic (AFM) correlations can coexist prior to the insulator-metal transition (IMT). We focused on a unique region in the Ba phase diagram, from x = 0.17 - 0.22, in which a commensurate AFM phase appears first with a propagation vector, k = (0, -0.5, 0.5), and the Co moment in the (001)$_{R}$ plane of the rhombohedral lattice. With increasing x, the AFM component weakens while an FM order appears with the FM Co moment directed along the (001)$_{R}$ (=(111)$_{C}$) axis. By x = 0.22, a spin flip to new FM component appears as the crystal fully transforms to an orthorhombic (Pnma) structure, with the Co moments pointing along a new direction, (001)$_{O}$ (=(110)$_{C}$). It is the emergence of the magnetic Pnma phase that leads to IMT.
description: 5 pages