cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐµÐ»ÐµÑÐ¾Ð¾Ð±ÑÐ°Ð·Ð½Ð¾ÑÑÐ¸ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ° Ð²ÑÐ²Ð¾Ð´Ð° Ð½Ð° ÑÑÐ½Ð¾Ðº Ð½Ð¾Ð²Ð¾Ð³Ð¾ Ð¿ÑÐ¾Ð´ÑÐºÑÐ° (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÑÐµÐ¿Ð»Ð¾Ð²Ð¾Ð·Ð°)
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: ÐÐ°ÑÑÑÐ½ÐµÐ½ÐºÐ¾, Ð¢Ð¸Ð¼Ñ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: Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³
Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¸
ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÑ
Ð½Ð¾Ð²ÑÐµ Ð¿ÑÐ¾Ð´ÑÐºÑÑ
marketing
investments
competitors
new products

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ Ð½Ð¾Ð²ÑÐ¹ ÑÐµÐ¿Ð»Ð¾Ð²Ð¾Ð· Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð° ÐÐÐ "ÐÐµÐ»Ð´Ð¾ÑÑÐµÐ¼Ð¼Ð°Ñ" ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð½ÑÐ¹ Ð² ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²Ð¸Ð¸ Ñ ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¼ Ð·Ð°Ð´Ð°Ð½Ð¸ÐµÐ¼ Ð¢Ð 3181-039-64822735-12, ÑÑÐ²ÐµÑÐ¶Ð´ÐµÐ½Ð½ÑÐ¼ ÐÐÐ "Ð ÐÐ" Ð² ÑÑÑÐ°Ð½Ð¾Ð²Ð»ÐµÐ½Ð½Ð¾Ð¼ Ð¿Ð¾ÑÑÐ´ÐºÐµ. 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 Ð²ÑÐ²Ð¾Ð´Ð° Ð½Ð° ÑÑÐ½Ð¾Ðº Ð½Ð¾Ð²Ð¾Ð³Ð¾ Ð¿ÑÐ¾Ð´ÑÐºÑÐ° (ÑÐµÐ¿Ð»Ð¾Ð²Ð¾Ð·Ð°) Ð¸ÑÐ¿Ð¾Ð»ÑÐ·ÑÐµÐ¼Ð¾Ð³Ð¾ Ð² Ð»ÐµÐ³ÐºÐ¾Ð¹ Ð¼Ð°Ð½ÐµÐ²ÑÐ¾Ð²Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð´Ð»Ñ Ð½ÑÐ¶Ð´ ÐÐÐ "Ð ÐÐ" Ð¸ Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½ÑÑ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¹. ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° ÑÑÐ½ÐºÐ° Ð¼Ð°Ð½ÐµÐ²ÑÐ¾Ð²ÑÑ ÑÐµÐ¿Ð»Ð¾Ð²Ð¾Ð·Ð¾Ð² Ð±ÑÐ»Ð¸ Ð²ÑÐ´ÐµÐ»ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ½ÑÐµ Ð¿ÑÐµÐ¸Ð¼ÑÑÐµÑÑÐ²Ð° Ð½Ð¾Ð²Ð¾Ð³Ð¾ Ð¼Ð°Ð½ÐµÐ²ÑÐ¾Ð²Ð¾Ð³Ð¾ ÑÐµÐ¿Ð»Ð¾Ð²Ð¾Ð·Ð°. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¸ ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ðµ ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ¾Ð² Ð½Ð° ÑÑÐ½ÐºÐµ. Ð Ð°ÑÑÑÐ¸ÑÐ°Ð½ Ð¿Ð¾Ð»ÐµÐ·Ð½ÑÐ¹ ÑÑÑÐµÐºÑ Ð¾Ñ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ Ð½Ð° Ð»ÐµÐ³ÐºÐ¾Ð¹ Ð¼Ð°Ð½ÐµÐ²ÑÐ¾Ð²Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð´Ð²ÑÑÐ¾ÑÐ½ÑÑ ÑÐµÐ¿Ð»Ð¾Ð²Ð¾Ð·Ð¾Ð² Ð¸ ÑÐ¸ÑÑÑÐ¹ Ð´Ð¸ÑÐºÐ¾Ð½ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÐ¹ Ð´Ð¾ÑÐ¾Ð´ Ð¸ ÑÑÐ¾Ðº Ð¾ÐºÑÐ¿Ð°ÐµÐ¼Ð¾ÑÑÐ¸ Ð¿Ð¾ÑÑÐµÐ±Ð½ÑÑ Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¹ Ð¾Ñ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ Ð½Ð° Ð¼Ð°Ð½ÐµÐ²ÑÐ¾Ð²Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð´Ð²ÑÑÐ¾ÑÐ½ÑÑ ÑÐµÐ¿Ð»Ð¾Ð²Ð¾Ð·Ð¾Ð².
description: The object of research is the new diesel production JSC "Zheldorremmash" developed in accordance with the technical specifications of TK 3181-039-64822735-12 approved by JSC "Russian Railways" in the prescribed manner. The purpose of final qualifying work is to study the output of a new product (locomotive) used in light shunting operations for the needs of JSC "Russian Railways" and industrial enterprises. On the basis of shunting locomotives market analysis identified the key competitive advantages of the new shunting locomotive. The analysis and comparison of competitors in the market. Designed beneficial effect of the use on the track and shunting locomotives and biaxial net present value and payback period of investment needs of the application on two-axle shunting locomotives.
VLT/NACO Deep imaging survey of young, nearby austral stars
Creators: name: Chauvin, G.
name: Lagrange, A. -M.
name: Bonavita, M.
name: Zuckerman, B.
name: Dumas, C.
name: Bessell, M. S.
name: Beuzit, J. -L.
name: Bonnefoy, M.
name: Desidera, S.
name: Farihi, J.
name: Lowrance, P.
name: Mouillet, D.
name: Song, I.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Since November 2002, we have conducted the largest deep imaging survey of the young, nearby associations of the southern hemisphere. Our goal is detection and characterization of substellar companions at intermediate (10--500 AU) physical separations. We have observed a sample of 88 stars, mostly G to M dwarfs, that we essentially identify as younger than 100 Myr and closer to Earth than 100 pc. The VLT/NACO adaptive optics instrument of the ESO Paranal Observatory was used to explore the faint circumstellar environment between typically 0.1 and 10''. We report the discovery of 17 new close (0.1-5.0'') multiple systems. HIP108195AB and C (F1III-M6), HIP84642AB (a~14 AU, K0-M5) and TWA22AB (a~1.8 AU; M6-M6) confirmed comoving systems. TWA22AB is likely to be a astrometric calibrator that can be used to test evolutionary predictions. Among our complete sample, a total of 65 targets observed with deep coronagraphic imaging. About 240 faint candidates were detected around 36 stars. Follow-up observations VLT or HST for 83% of these stars enabled us to identify a fraction of contaminants. The latest results about the substellar companions to GSC08047-00232, AB Pic and 2M1207, confirmed during this survey and published earlier, are reviewed. Finally, the statistical analysis of our complete set of coronagraphic limits enables us to place constraints on the physical and properties of giant planets between typically 20 and 150 AU.
description: 23 pages; 11 figures; accepted for publication in A&A
Seasonal forecasting of streamflow in a mountainous catchment in British Columbia
Creators: name: Swift-LaPointe, Taylor
Publisher: name: University of British Columbia
Year: 2024

description: Forecasting of streamflow entering dam reservoirs is important for management of hydroelectricity operations, with economic and environmental impacts. On seasonal timescales, some prediction skill of variables that influence streamflow is derived from climate modes of variability, like the El Niño Southern Oscillation (ENSO) and Pacific Decadal Oscillation (PDO), among other factors. In this study, it is investigated how the phases of these climate modes affect inflow into the Kinbasket Lake Reservoir and Mica Dam in southeast British Columbia, a snowmelt-dominated catchment. El Niño and PDO positive phases produce greater streamflow than La Niña and PDO negative phases from April to June, with the opposite true from June to September, although the differences are small. It is investigated whether a forecast using meteorological conditions, affected by ENSO and PDO modes, to predict streamflow in this catchment achieves skill on seasonal timescales. The hybrid statistical-dynamical forecast of cumulative January to September seasonal streamflow at nine months lead time uses dynamical ECMWF SEAS5 seasonal meteorological hindcasts (retrospective "forecasts") as input into a Long Short-Term Memory (LSTM) neural network. A monthly LSTM model using 12 months of meteorological forcings outperforms a daily LSTM model using 365 days of forcings at capturing the interannual variability in seasonal streamflow volumes when forced with reanalysis (ERA5) meteorological data. Skill in the meteorological inputs is required in at least the first three months of the forecast year, reflecting that the main source of streamflow prediction skill is derived from snowpack build up prior to and at the beginning of the forecast year, rather than ENSO and PDO indices. The hybrid streamflow forecast underestimates seasonal volumes in most years due to biases present in the SEAS5 hindcasts. Three bias correction methods are investigated, and linearly shifting the mean of the SEAS5 hindcasts to that of reanalysis gives the largest improvement in skill of the streamflow forecast. This study demonstrates that it is possible to use a hybrid statistical-dynamical forecast to predict seasonal volumes in a mountainous catchment, however the skill in predicting interannual variability is largely limited by the accuracy of prediction of meteorological forcings on seasonal timescales.
How selection and weighting of astrometric observations influence the impact probability. Asteroid (99942) Apophis case
Creators: name: Krolikowska, Malgorzata
name: Sitarski, Grzegorz
name: Soltan, Andrzej M.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: The aim is to show that in case of low probability of asteroid collision with Earth, the appropriate selection and weighing of the data are crucial for the impact investigation, and to analyze the impact possibilities using extensive numerical simulations. By means of the Monte Carlo special method a large number of ``clone'' orbits have been generated. A full range of orbital elements in the 6-dimensional parameter space, e.g. in the entire confidence region allowed by the observational material has been examined. On the basis of 1000 astrometric observations of (99942) Apophis, the best solution for the geocentric encounter distance of 6.065\pm 0.081 R_{Earth} were derived for the close encounter with the Earth on April 13, 2029. The present uncertainties allow for the special configurations (``keyholes'') during these encounter which may lead to the very close encounters in the future approaches of Apophis. Two groups of keyholes are connected with the close encounter with the Earth in 2036 (within the minimal distance of 5.7736-5.7763 R_{Earth} on April 13, 2029) and 2037 (within the minimal distance of 6.3359-6.3488 R_{Earth}). The nominal orbits for our most accurate models run almost exactly in the middle between these two impact keyhole groups. A very small keyhole for the impact in 2076 has been found between these groups at the minimal distance of 5.97347 R_{Earth} (close to the nominal orbit).
title: ÐÐ°Ð»Ð¾Ð³Ð¾Ð¾Ð±Ð»Ð¾Ð¶ÐµÐ½Ð¸Ðµ, ÑÑÐµÑ Ð¸ Ð°ÑÐ´Ð¸Ñ Ð²ÐºÐ»Ð°Ð´Ð¾Ð² Ð² ÑÑÑÐ°Ð²Ð½ÑÐ¹ ÐºÐ°Ð¿Ð¸ÑÐ°Ð» Ð¸Ð½Ð¾ÑÑÑÐ°Ð½Ð½ÑÑ ÑÑÐ°ÑÑÐ½Ð¸ÐºÐ¾Ð² Ð¸ ÑÐ°ÑÑÐµÑÐ¾Ð² Ñ Ð½Ð¸Ð¼Ð¸
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¸Ð½ÐºÐ¾Ð²ÑÐºÐ¸Ð¹, 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: 2017
Subjects: Ð¸Ð½Ð¾ÑÑÑÐ°Ð½Ð½ÑÐµ ÑÑÐ°ÑÑÐ½Ð¸ÐºÐ¸
Ð´Ð¸Ð²Ð¸Ð´ÐµÐ½Ð´Ñ
Ð½Ð°Ð»Ð¾Ð³ Ð½Ð° Ð¿ÑÐ¸Ð±ÑÐ»Ñ
ÑÐ°ÑÑÐµÑÑ Ð² Ð²Ð°Ð»ÑÑÐµ

description: Ð Ð°Ð±Ð¾ÑÐ° ÑÐ¾Ð´ÐµÑÐ¶Ð¸Ñ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð²ÑÐµÐ²Ð¾Ð·Ð¼Ð¾Ð¶Ð½ÑÑ ÑÐ°ÑÑÐµÑÐ¾Ð² ÑÐ¾ÑÑÐ¸Ð¹ÑÐºÐ¸Ñ ÐºÐ¾Ð¼Ð¼ÐµÑÑÐµÑÐºÐ¸Ñ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¹ Ñ Ð¸Ð½Ð¾ÑÑÑÐ°Ð½Ð½ÑÐ¼Ð¸ ÑÑÑÐµÐ´Ð¸ÑÐµÐ»ÑÐ¼Ð¸ Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐÐ Â«ÐÐµÑ ÐÐ°ÑÑÐ»ÐµÑÑÂ». Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½ Ð¿ÑÐ¾ÑÐµÑÑ ÑÑÐµÑÐ°, Ð²Ð¾Ð¿ÑÐ¾ÑÑ Ð½Ð°Ð»Ð¾Ð³Ð¾Ð¾Ð±Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ð¸ Ð°ÑÐ´Ð¸ÑÐ°. ÐÑÐ¸Ð²ÐµÐ´ÐµÐ½Ð° ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ° Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸, ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð° ÐµÐµ ÑÑÑÑÐºÑÑÑÐ°. ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð¸Ð¼ÐµÑÑÐµÐ¹ÑÑ Ð±ÑÑÐ³Ð°Ð»ÑÐµÑÑÐºÐ¾Ð¹ Ð¾ÑÑÐµÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸. ÐÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ñ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¿Ð¾ ÑÐ»ÑÑÑÐµÐ½Ð¸Ñ ÑÐ°Ð±Ð¾ÑÑ Ð¸ ÑÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¾ Ð¸Ñ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ðµ.
Equivariant Lie-Rinehart cohomology
Creators: name: Eriksen, Eivind
name: Gustavsen, Trond S.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Algebraic Geometry (math.AG)
subject: Commutative Algebra (math.AC)
subject: Rings and Algebras (math.RA)
subject: FOS: Mathematics

description: In this paper, we study Lie-Rinehart cohomology for quotients of singularities by finite groups, and interpret these cohomology groups in terms of integrable connection on modules.
description: 7 pages, LaTeX, based on a talk I gave at the AGMF Baltic-Nordic Workshop in Tartu, 9-11 October, 2008
title: Огневая подготовка из стрелкового оружия
Creators: name: ELS IPR BOOKS
Publisher: name: Профобразование
Year: 2024

description: В учебном пособии рассмотрены теоретические основы стрельбы, приемы стрельбы из стрелкового оружия и правила обращения с ним. Дана общая характеристика стрелкового оружия, принцип работы частей и механизмов АК-74 и ПМ, приведены сведения о ручных осколочных гранатах. Изложены меры безопасности при обращении с оружием и боеприпасами на учебных стрельбах, общий порядок проведения учебных стрельб, хранения и эксплуатации оружия. Учебное пособие предназначено для студентов, обучающихся по укрупненной группе специальностей среднего профессионального образования «Юриспруденция», изучающих дисциплину «Огневая подготовка».
The Intensity Profile of the Solar Supergranulation
Creators: name: Goldbaum, N. J.
name: Rast, M. P.
name: Ermolli, I.
name: Sands, J. S.
name: Berrilli, F.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We have measured the average radial (cell center to network boundary) profile of the continuum intensity contrast associated with supergranular flows using data from the Precision Solar Photometric Telescope (PSPT) at the Mauna Loa Solar Observatory (MLSO). After removing the contribution of the network flux elements by the application of masks based on Ca II K intensity and averaging over more than 10^5 supergranular cells, we find a ~ 0.1% decrease in red and blue continuum intensity from the supergranular cell centers outward, corresponding to a ~ 1.0 K decrease in brightness temperature across the cells. The radial intensity profile may be caused either by the thermal signal associated with the supergranular flows or a variation in the packing density of unresolved magnetic flux elements. These are not unambiguously distinguished by the observations, and we raise the possibility that the network magnetic fields play an active role in supergranular scale selection by enhancing the radiative cooling of the deep photosphere at the cell boundaries.
description: Accepted to ApJ
Coherent Quantum Ratchets Driven by Tunnel Oscillations
Creators: name: Stark, Michael
name: Kohler, Sigmund
Publisher: name: arXiv
Year: 2009
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We demonstrate that the tunnel oscillations of a biased double quantum dot can be employed as driving source for a quantum ratchet. As a model, we use two capacitively coupled double quantum dots. One double dot is voltage biased and provides the ac force, while the other experiences the ac force and acts as coherent quantum ratchet. The current is obtained from a Bloch-Redfield master equation which ensures a proper equilibrium limit. We find that the two-electron states of the coupled ratchet-drive Hamiltonian lead to unexpected steps in the ratchet current.
description: 4 pages, 4 figures
Hot Jupiters, cold kinematics: High phase space densities of host stars reflect an age bias
Creators: name: Mustill, Alexander J.
name: Lambrechts, Michiel
name: Davies, Melvyn B.
Publisher: name: arXiv
Year: 2021
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Context. The birth environments of planetary systems are thought to influence planet formation and orbital evolution, through external photoevaporation and stellar flybys. Recent work has claimed observational support for this, in the form of a correlation between the properties of planetary systems and the local Galactic phase space density of the host star. In particular, Hot Jupiters are found overwhelmingly around stars in regions of high phase space density, which may reflect a formation environment with high stellar density. Aims. We instead investigate whether the high phase space density may have a galactic kinematic origin: Hot Jupiter hosts may be biased towards being young and therefore kinematically cold, because tidal inspiral leads to the destruction of the planets on Gyr timescales, and the velocity dispersion of stars in the Galaxy increases on similar timescales. Methods. We use 6D positions and kinematics from Gaia for the Hot Jupiter hosts and their neighbours, and construct distributions of the phase space density. We investigate correlations between the stars' local phase space density and peculiar velocity. Results. We find a strong anticorrelation between the phase space density and the host star's peculiar velocity with respect to the Local Standard of Rest. Therefore, most stars in "high-density" regions are kinematically cold, which may be caused by the aforementioned bias towards detecting Hot Jupiters around young stars before the planets' tidal destruction. Conclusions. We do not find evidence in the data for Hot Jupiter hosts preferentially being in phase space overdensities compared to other stars of similar kinematics, nor therefore for their originating in birth environments of high stellar density.
description: Accepted to A&A. Code and ancillary files to reproduce these results can be found at https://github.com/AJMustill/HJGalaxy
title: ÐÐ·ÑÑÐµÐ½Ð¸Ðµ Ð² ÑÑÐµÐ´Ðµ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ OMNet++ Ð²Ð»Ð¸ÑÐ½Ð¸Ñ ÑÐ°Ð·Ð¼ÐµÑÐ° Ð¢Ð¡Ð -ÑÐµÐ³Ð¼ÐµÐ½ÑÐ¾Ð² Ð¸ ÑÐ¸ÑÐ»Ð° ÑÑÐ°Ð½Ð·Ð¸ÑÐ½ÑÑ ÑÐ·Ð»Ð¾Ð² Ð½Ð° Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´Ð¸ÑÐµÐ»ÑÐ½Ð¾ÑÑÑ Ð¢Ð¡Ð -ÑÐ¾ÐµÐ´Ð¸Ð½ÐµÐ½Ð¸Ð¹
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð¤Ð°Ð¼ Ð¢Ñ Ð¸ Ð¢Ñ Ð°Ð½Ñ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´Ð¸ÑÐµÐ»ÑÐ½Ð¾ÑÑÑ Ð¢Ð¡Ð -ÑÐ¾ÐµÐ´Ð¸Ð½ÐµÐ½Ð¸Ð¹
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description: Ð Ð°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° Ð¸Ð·ÑÑÐµÐ½Ð¸Ñ ÑÐ°ÑÑÐ½ÑÑ Ð°ÑÐ¿ÐµÐºÑÐ¾Ð², Ð²Ð»Ð¸ÑÑÑÐ¸Ñ Ð½Ð° ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ Ð¾Ð±Ð¼ÐµÐ½Ð° Ð´Ð°Ð½Ð½ÑÐ¼Ð¸ Ð² IP-ÑÐµÑÑÑ Ð¿Ð¾ Ð¿ÑÐ¾ÑÐ¾ÐºÐ¾Ð»Ñ Ð¢Ð¡Ð , Ñ ÑÐµÐ»ÑÑ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´Ð¸ÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÑÐ¾ÐµÐ´Ð¸Ð½ÐµÐ½Ð¸Ð¹ Ð² ÐºÐ¾Ð½ÐºÑÐµÑÐ½ÑÑ ÑÑÐ»Ð¾Ð²Ð¸ÑÑ. ÐÑÑÐ»ÐµÐ´ÑÑÑÑÑ ÑÐ°ÐºÑÐ¾ÑÑ, Ð²Ð»Ð¸ÑÑÑÐ¸Ðµ Ð½Ð° ÑÐ°Ð·Ð¼ÐµÑ Ð¢Ð¡Ð -ÑÐµÐ³Ð¼ÐµÐ½ÑÐ¾Ð², Ð³ÐµÐ½ÐµÑÐ¸ÑÑÐµÐ¼ÑÑ Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ¾Ð¼ Ð´Ð°Ð½Ð½ÑÑ, Ð¸, Ð² ÑÐ²Ð¾Ñ Ð¾ÑÐµÑÐµÐ´Ñ, Ð²Ð»Ð¸ÑÐ½Ð¸Ñ ÑÐ°Ð·Ð¼ÐµÑÐ° ÑÐµÐ³Ð¼ÐµÐ½ÑÐ¾Ð² Ð½Ð° Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´Ð¸ÑÐµÐ»ÑÐ½Ð¾ÑÑÑ Ð¢Ð¡Ð -ÑÐ¾ÐµÐ´Ð¸Ð½ÐµÐ½Ð¸Ð¹. ÐÐ· ÑÑÐ¾Ð³Ð¾ ÑÐ»ÐµÐ´ÑÐµÑ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÑ Ð¾Ð¿ÑÐ¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÐ°Ð·Ð¼ÐµÑÐ° TCP-ÑÐµÐ³Ð¼ÐµÐ½ÑÐ¾Ð² Ð² ÑÐµÑÐ¸. Ð¤Ð¾ÑÐ¼ÑÐ»Ð¸ÑÑÑÑÑÑ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ¸ Ð³ÐµÐ½ÐµÑÐ¸ÑÑÐµÐ¼Ð¾Ð³Ð¾ Ð¿ÑÐ¸ Ð¿ÐµÑÐµÑÑÐ»ÐºÐµ ÑÐ°Ð¹Ð»Ð¾Ð² ÑÑÐ°ÑÐ¸ÐºÐ° Ð¿Ð¾ ÐºÑÐ¸ÑÐµÑÐ¸ÑÐ¼ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¸ ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²Ð¸Ñ ÑÑÐµÐ±Ð¾Ð²Ð°Ð½Ð¸ÑÐ¼ Ð´Ð¾Ð±ÑÐ¾Ð¶ÐµÐ»Ð°ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ ÑÐµÐ³ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð½Ð°Ð³ÑÑÐ·ÐºÐ¸ TFRC. ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ðµ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð½Ð¾Ð¹ Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ¸ Ð¿Ð¾ÑÑÑÐ¾ÐµÐ½Ð° Ð¸Ð¼Ð¸ÑÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ Ð¼Ð¾Ð´ÐµÐ»Ñ ÑÐµÑÑÐ¾Ð²Ð¾Ð³Ð¾ Ð¿Ð¾Ð»Ð¸Ð³Ð¾Ð½Ð° Ð² ÑÑÐµÐ´Ðµ OMNet++ Ð¸ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð° ÑÐµÑÐ¸Ñ ÑÐºÑÐ¿ÐµÑÐ¸Ð¼ÐµÐ½ÑÐ¾Ð² Ð¿Ð¾ Ð¾ÑÐµÐ½ÐºÐµ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¢Ð¡P-ÑÐ¾ÐµÐ´Ð¸Ð½ÐµÐ½Ð¸Ð¹ Ð½Ð° Ð¼Ð°ÑÑÑÑÑÐ°Ñ ÑÐ°Ð·Ð»Ð¸ÑÐ½Ð¾Ð¹ Ð´Ð»Ð¸Ð½Ñ Ð¿ÑÐ¸ ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÑÑÐµÐ¼ Ð²Ð°ÑÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ð¸ ÑÐ°Ð·Ð¼ÐµÑÐ° Ð³ÐµÐ½ÐµÑÐ¸ÑÑÐµÐ¼ÑÑ Ð¿Ð°ÐºÐµÑÐ¾Ð² Ð´Ð°Ð½Ð½ÑÑ.
Bi-partite entanglement entropy in massive 1+1-dimensional quantum field theories
Creators: name: Castro-Alvaredo, Olalla A.
name: Doyon, Benjamin
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: This manuscript is a review of the main results obtained in a series of papers involving the present authors and their collaborator J.L. Cardy over the last two years. In our work we have developed and applied a new approach for the computation of the bi-partite entanglement entropy in massive 1+1-dimensional quantum field theories. In most of our work we have considered these theories to be also integrable. Our approach combines two main ingredients: the "replica trick" and form factors for integrable models and more generally for massive quantum field theory. Our basic idea for combining fruitfully these two ingredients is that of the branch-point twist field. By the replica trick we obtained an alternative way of expressing the entanglement entropy as a function of the correlation functions of branch-point twist fields. On the other hand, a generalisation of the form factor program has allowed us to study, and in integrable cases to obtain exact expressions for, form factors of such twist fields. By the usual decomposition of correlation functions in an infinite series involving form factors, we obtained exact results for the infrared behaviours of the bi-partite entanglement entropy, and studied both its infrared and ultraviolet behaviours for different kinds of models: with and without boundaries and backscattering, at and out of integrability.
description: 51 pages, 9 figures. Review article to appear in the special issue "Entanglement entropy in extended quantum systems" of J. Phys. A
Numerical simulation of high-speed turbulent water jets in air
Creators: name: Guha, Anirban
name: Barron, Ronald M.
name: Balachandar, Ram
Publisher: name: arXiv
Year: 2010
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: Numerical simulation of high-speed turbulent water jets in air and its validation with experimental data has not been reported in the literature. It is therefore aimed to simulate the physics of these high-speed water jets and compare the results with the existing experimental works. High-speed water jets diffuse in the surrounding atmosphere by the processes of mass and momentum transfer. Air is entrained into the jet stream and the entire process contributes to jet spreading and subsequent pressure decay. Hence the physical problem is in the category of multiphase flows, for which mass and momentum transfer is to be determined to simulate the problem. Using the Eulerian multiphase and the k-εturbulence models, plus a novel numerical model for mass and momentum transfer, the simulation was achieved. The results reasonably predict the flow physics of high-speed water jets in air.
description: Journal of Hydraulic Research, 48(1), pp. 119-124 (2010)
title: Ð¡Ð±Ð¾ÑÐ½Ð¸Ðº Ð·Ð°Ð´Ð°Ñ Ð¿Ð¾ Ð»Ð¸Ð½ÐµÐ¹Ð½Ð¾Ð¹ Ð°Ð»Ð³ÐµÐ±ÑÐµ. ÐÐ°Ð½Ðº Ð²Ð°ÑÐ¸Ð°Ð½ÑÐ¾Ð². Ð§. 1
Creators: name: Ð¢Ð¸ÑÐ¾Ð¼Ð¸ÑÐ¾Ð², Ð¡ÐµÑÐ³ÐµÐ¹
Publisher: name: [ÐÐ·Ð´-Ð²Ð¾ Ð¡ÐÐ±ÐÐ¢Ð£]
Year: 1994
Subjects: ÐÐ¸Ð½ÐµÐ¹Ð½Ð°Ñ Ð°Ð»Ð³ÐµÐ±ÑÐ°

description: ÐÐ°Ð½Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð½Ð°Ð¿Ð¸ÑÐ°Ð½Ð¾ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð¼Ð½Ð¾Ð³Ð¾Ð»ÐµÑÐ½ÐµÐ³Ð¾ Ð¾Ð¿ÑÑÐ° Ð¿ÑÐµÐ¿Ð¾Ð´Ð°Ð²Ð°Ð½Ð¸Ñ Ð»Ð¸Ð½ÐµÐ¹Ð½Ð¾Ð¹ Ð°Ð»Ð³ÐµÐ±ÑÑ Ð² Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¾Ð¼ ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð¼ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐµ ÑÑÑÐ´ÐµÐ½ÑÐ°Ð¼ Ð¸Ð½Ð¶ÐµÐ½ÐµÑÐ½Ð¾-ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¸Ñ Ð¸ Ð¸Ð½Ð¶ÐµÐ½ÐµÑÐ½Ð¾ -ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐµÐ¹ Ð¸ Ð¾ÑÐ²Ð°ÑÑÐ²Ð°ÐµÑ Ð²Ð°Ð¶Ð½ÐµÐ¹ÑÐ¸Ðµ ÑÐ°Ð·Ð´ÐµÐ»Ñ ÐºÑÑÑÐ°. ÐÐ¾ ÐºÐ°Ð¶Ð´Ð¾Ð¼Ñ ÑÐ°Ð·Ð´ÐµÐ»Ñ cÑÐ¾ÑÐ¼ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ñ Ð·Ð°Ð´Ð°ÑÐ¸ Ð¸ Ð´Ð»Ñ ÐºÐ°Ð¶Ð´Ð¾Ð¹ Ð¸Ð· Ð½Ð¸Ñ ÑÐ¾ÑÑÐ°Ð²Ð»ÐµÐ½Ñ Ð²Ð°ÑÐ¸Ð°Ð½ÑÑ Ð´Ð»Ñ ÑÐ°Ð¼Ð¾ÑÑÐ¾ÑÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ ÑÐµÑÐµÐ½Ð¸Ñ. ÐÐ°Ð´Ð°ÑÐ¸ ÑÐ¾Ð¿ÑÐ¾Ð²Ð¾Ð¶Ð´Ð°ÑÑÑÑ ÐºÐ¾Ð¼Ð¼ÐµÐ½ÑÐ°ÑÐ¸ÑÐ¼Ð¸ Ð¸ Ð¿ÑÐ¸Ð¼ÐµÑÐ°Ð¼Ð¸. Ð¡Ð±Ð¾ÑÐ½Ð¸Ðº ÑÐ¾Ð´ÐµÑÐ¶Ð¸Ñ Ð±Ð¾Ð»ÐµÐµ 1000 Ð·Ð°Ð´Ð°Ñ. ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐ°ÐµÑÑÑ ÑÑÑÐ´ÐµÐ½ÑÐ°Ð¼ Ð²ÑÐ·Ð¾Ð², Ð¿ÑÐµÐ¿Ð¾Ð´Ð°Ð²Ð°ÑÐµÐ»ÑÐ¼ Ð¼Ð°ÑÐµÐ¼Ð°ÑÐ¸ÐºÐ¸ Ð¸ Ð»Ð¸ÑÐ°Ð¼, ÑÐ°Ð¼Ð¾ÑÑÐ¾ÑÑÐµÐ»ÑÐ½Ð¾ Ð¸Ð·ÑÑÐ°ÑÑÐ¸Ð¼ Ð»Ð¸Ð½ÐµÐ¹Ð½ÑÑ Ð°Ð»Ð³ÐµÐ±ÑÑ.
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 ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ°.
One-particle properties of deformed N $\approx$ 28 odd-N nuclei with weakly-bound or resonant neutrons
Creators: name: Hamamoto, Ikuko
Publisher: name: arXiv
Year: 2008
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: Possible deformation of odd-N nuclei with N $\approx$ 28 towards the neutron drip line is investigated using the Nilsson diagram based on deformed Woods-Saxon potentials. Both weakly-bound and resonant one-particle levels are properly obtained by directly solving the Schrödinger equation in mesh of space coordinate with the correct boundary condition. If we use the same diffuseness of the potential as that of $β$-stable nuclei, the energy difference between the neutron 2p$_{3/2}$ and 1f$_{7/2}$ levels becomes very small or the N=28 energy gap almost disappears, as the binding energies of those levels approach zero. This suggests that the ground states of those neutron drip line nuclei are likely to be deformed. In particular, the spin-parity and the magnetic moment of the ground state of odd-N nuclei, $^{43}_{16}$S$_{27}$ and $^{45}_{16}$S$_{29}$, are examined. Moreover, it is suggested that in $^{39}_{12}$Mg$_{27}$ lying outside the drip line the lowest resonant state may have 5/2$^{-}$, if the N=28 energy gap almost vanishes.
description: 3 figures
title: ÐÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ðµ ÑÐ°Ð¼Ð¾Ð¾ÑÐ³Ð°Ð½Ð¸Ð·ÑÑÑÐ¸Ñ ÑÑ ÐºÐ°ÑÑ ÐÐ¾Ñ Ð¾Ð½ÐµÐ½Ð° Ð´Ð»Ñ Ð¾Ð±Ð½Ð°ÑÑÐ¶ÐµÐ½Ð¸Ñ ÑÐµÑÐµÐ²ÑÑ Ð°ÑÐ°Ðº
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: Ð¥ÑÑÐ°Ð¸Ð½Ð¾Ð², Ð Ð°Ð¼Ð¸Ð»Ñ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: ÐÑÑÐ¸ÑÐ»Ð¸ÑÐµÐ»ÑÐ½ÑÐµ Ð¼Ð°ÑÐ¸Ð½Ñ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½ÑÐµ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»ÑÐ½ÑÐµ
ÐÐ½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ñ
ÑÐµÑÐµÐ²ÑÐµ Ð°ÑÐ°ÐºÐ¸
ÑÐµÑÐµÐ²ÑÐµ Ð°Ð½Ð¾Ð¼Ð°Ð»Ð¸Ð¸
ÑÐ°Ð¼Ð¾Ð¾ÑÐ³Ð°Ð½Ð¸Ð·ÑÑÑÐ¸ÐµÑÑ ÐºÐ°ÑÑÑ
Ð·Ð½Ð°ÑÐ¸Ð¼ÑÐµ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÑ

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¾ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ ÑÐ°Ð¼Ð¾Ð¾ÑÐ³Ð°Ð½Ð¸Ð·ÑÑÑÐ¸ÑÑÑ ÐºÐ°ÑÑ ÐÐ¾ÑÐ¾Ð½ÐµÐ½Ð° Ð´Ð»Ñ Ð¾Ð±Ð½Ð°ÑÑÐ¶ÐµÐ½Ð¸Ñ ÑÐµÑÐµÐ²ÑÑ Ð°ÑÐ°Ðº. ÐÑÐ¸Ð²Ð¾Ð´ÑÑÑÑ Ð½Ð°Ð±Ð¾ÑÑ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÐ¾Ð² Ð´Ð»Ñ Ð¾Ð¿ÑÐ¸Ð¼Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð¾Ð±Ð½Ð°ÑÑÐ¶ÐµÐ½Ð¸Ñ ÑÐµÑÐµÐ²ÑÑ Ð°ÑÐ°Ðº Ð¸ ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ðµ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¾Ð² Ð¾Ð±Ð½Ð°ÑÑÐ¶ÐµÐ½Ð¸Ñ ÑÐ¾ ÑÑÐ¾Ð´Ð½ÑÐ¼Ð¸ Ð½Ð°ÑÑÐ½ÑÐ¼Ð¸ ÑÐ°Ð±Ð¾ÑÐ°Ð¼Ð¸.
Glass Formation and Crystallization of a Simple Monatomic Liquid
Creators: name: Mizuguchi, Tomoko
name: Odagaki, Takashi
Publisher: name: arXiv
Year: 2009
Subjects: subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: A simple monatomic system in two dimensions with a double-well interaction potential is investigated in a wide range of temperature by molecular dynamics simulation. The system is melted and equilibrated well above the melting temperature, and then it is quenched to a temperature 88% below the melting temperature Tm at several cooling rates to produce an amorphous state. Various thermodynamic quantities are measured as a function of temperature while the system is heated at a constant rate. The glass transiton is observed by a sudden increase of the energy and Tg is shown to be an increasing function of the cooling rate in the preparation process of the amorphous state. In a relatively-high temperature region, the system gradually transforms into crystals, and the time-temperature-transformation(TTT) curve shows a typical nose shape. It is found that the transformation time to a crystalline state is the shortest at a temperature 14~15% below the melting temperature Tm and that at sufficiently low temperatures the transformation time is much longer than the available CPU time. This indicates that a long-lived glassy state is realized.
description: 14pages, 16figures
Hadronic final states in deep-inelastic scattering with Sherpa
Creators: name: Carli, Tancredi
name: Gehrmann, Thomas
name: Höche, Stefan
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We extend the multi-purpose Monte-Carlo event generator Sherpa to include processes in deeply inelastic lepton-nucleon scattering. Hadronic final states in this kinematical setting are characterised by the presence of multiple kinematical scales, which were up to now accounted for only by specific resummations in individual kinematical regions. Using an extension of the recently introduced method for merging truncated parton showers with higher-order tree-level matrix elements, it is possible to obtain predictions which are reliable in all kinematical limits. Different hadronic final states, defined by jets or individual hadrons, in deep-inelastic scattering are analysed and the corresponding results are compared to HERA data. The various sources of theoretical uncertainties of the approach are discussed and quantified. The extension to deeply inelastic processes provides the opportunity to validate the merging of matrix elements and parton showers in multi-scale kinematics inaccessible in other collider environments. It also allows to use HERA data on hadronic final states in the tuning of hadronisation models.
description: 32 pages, 22 figures
Conjugate Degradability and the Quantum Capacity of Cloning Channels
Creators: name: Bradler, Kamil
name: Dutil, Nicolas
name: Hayden, Patrick
name: Muhammad, Abubakr
Publisher: name: arXiv
Year: 2009
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: A quantum channel is conjugate degradable if the channel's environment can be simulated up to complex conjugation using the channel's output. For all such channels, the quantum capacity can be evaluated using a single-letter formula. In this article we introduce conjugate degradability and establish a number of its basic properties. We then use it to calculate the quantum capacity of N to N+1 and 1 to M universal quantum cloning machines as well as the quantum capacity of a channel that arises naturally when data is being transmitted to an accelerating receiver. All the channels considered turn out to have strictly positive quantum capacity, meaning they could be used as part of a communication system to send quantum states reliably.
description: 18 pages
title: Операционные системы. Linux
Creators: name: ELS IPR BOOKS
Publisher: name: Профобразование
Year: 2024

description: В учебном пособии приведены теоретические сведения об операционной системе Linux, рассмотрены способы хранения информации, команды управления данными. Изложены вопросы изменения прав доступа к файлам, управления командой оболочкой, создания простейшего скрипта, обработки параметров командной строки, передаваемых в скрипт. Отдельное внимание уделено каналам ввода-вывода, перенаправлению каналов, понятию процесса, групп процессов, сеансов, фоновому и интерактивному выполнению задач. Учебное пособие предназначено для студентов, обучающихся по укрупненным группам специальностей среднего профессионального образования «Информатика и вычислительная техника», «Информационная безопасность», изучающих дисциплину «Операционные системы».
title: ÐÐµÐ¾Ð¿ÑÐµÐ´ÐµÐ»ÑÐ½Ð½ÑÐ¹ Ð¸Ð½ÑÐµÐ³ÑÐ°Ð». ÐÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð·Ð°Ð½ÑÑÐ¸Ñ. ÐÐ°Ð´Ð°ÑÐ¸ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð´Ð¾Ð¼Ð°ÑÐ½ÐµÐ³Ð¾ Ð·Ð°Ð´Ð°Ð½Ð¸Ñ
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐµÑÑÐ¾Ð²Ð°, ÐÐ°Ñ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: 2022
Subjects: ÐÐ½ÑÐµÐ³ÑÐ°Ð»Ñ Ð½ÐµÐ¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð½ÑÐµ
ÐÐ°ÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ¸Ð¹ Ð°Ð½Ð°Ð»Ð¸Ð·

description: ÐÐ°Ð½Ð½Ð¾Ðµ ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ 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 Ð½Ð° ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ñ Ð¸ ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¸Ñ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸ÑÑ, Ð¸Ð·ÑÑÐ°ÑÑÐ¸Ñ Ð¾Ð±ÑÐ¸Ð¹ Ð¸ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½ÑÐµ ÐºÑÑÑÑ Ð²ÑÑÑÐµÐ¹ Ð¼Ð°ÑÐµÐ¼Ð°ÑÐ¸ÐºÐ¸. ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ ÑÐ¾Ð´ÐµÑÐ¶Ð¸Ñ ÐºÑÐ°ÑÐºÐ¸Ðµ ÑÐ²ÐµÐ´ÐµÐ½Ð¸Ñ Ð¿Ð¾ ÑÐµÐ¾ÑÐ¸Ð¸ Ð¿Ð¾ ÑÐµÐ¼Ðµ Â«ÐÐµÐ¾Ð¿ÑÐµÐ´ÐµÐ»ÑÐ½Ð½ÑÐ¹ Ð¸Ð½ÑÐµÐ³ÑÐ°Ð»Â», ÑÐµÑÐµÐ½Ð¸Ñ ÑÐ¸Ð¿Ð¸ÑÐ½ÑÑ Ð·Ð°Ð´Ð°Ñ Ð¸ Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐºÐ°Ð·Ð°Ð½Ð¸Ñ Ðº Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð´Ð¾Ð¼Ð°ÑÐ½ÐµÐ³Ð¾ Ð·Ð°Ð´Ð°Ð½Ð¸Ñ (ÐÐ/Ð) Ð¿Ð¾ ÑÑÐ¾Ð¹ ÑÐµÐ¼Ðµ, Ð° ÑÐ°ÐºÐ¶Ðµ ÑÐ¿Ð¸ÑÐ¾Ðº Ð½Ð¾Ð¼ÐµÑÐ¾Ð² Ð·Ð°Ð´Ð°Ñ Ð¿Ð¾ ÑÐºÐ°Ð·Ð°Ð½Ð½Ð¾Ð¼Ñ Ð² Ð»Ð¸ÑÐµÑÐ°ÑÑÑÐµ ÑÑÐµÐ±Ð½Ð¸ÐºÑ Ð´Ð»Ñ Ð·Ð°ÐºÑÐµÐ¿Ð»ÐµÐ½Ð¸Ñ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð°. ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ Ð¿Ð¾Ð´Ð¾Ð¹Ð´ÑÑ Ð¸ Ð»Ð¸ÑÐ°Ð¼, ÑÐ°Ð¼Ð¾ÑÑÐ¾ÑÑÐµÐ»ÑÐ½Ð¾ Ð¸Ð·ÑÑÐ°ÑÑÐ¸Ð¼ Ð´Ð°Ð½Ð½ÑÑ ÑÐµÐ¼Ñ Ð²ÑÑÑÐµÐ¹ Ð¼Ð°ÑÐµÐ¼Ð°ÑÐ¸ÐºÐ¸.
Evidence for the Gompertz Curve in the Income Distribution of Brazil 1978-2005
Creators: name: Moura, Newton J.
name: Ribeiro, Marcelo B.
Publisher: name: arXiv
Year: 2008
Subjects: subject: General Finance (q-fin.GN)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Adaptation and Self-Organizing Systems (nlin.AO)
subject: Physics and Society (physics.soc-ph)
subject: Statistical Finance (q-fin.ST)
subject: FOS: Economics and business
subject: FOS: Physical sciences

description: This work presents an empirical study of the evolution of the personal income distribution in Brazil. Yearly samples available from 1978 to 2005 were studied and evidence was found that the complementary cumulative distribution of personal income for 99% of the economically less favorable population is well represented by a Gompertz curve of the form $G(x)=\exp [\exp (A-Bx)]$, where $x$ is the normalized individual income. The complementary cumulative distribution of the remaining 1% richest part of the population is well represented by a Pareto power law distribution $P(x)= βx^{-α}$. This result means that similarly to other countries, Brazil's income distribution is characterized by a well defined two class system. The parameters $A$, $B$, $α$, $β$ were determined by a mixture of boundary conditions, normalization and fitting methods for every year in the time span of this study. Since the Gompertz curve is characteristic of growth models, its presence here suggests that these patterns in income distribution could be a consequence of the growth dynamics of the underlying economic system. In addition, we found out that the percentage share of both the Gompertzian and Paretian components relative to the total income shows an approximate cycling pattern with periods of about 4 years and whose maximum and minimum peaks in each component alternate at about every 2 years. This finding suggests that the growth dynamics of Brazil's economic system might possibly follow a Goodwin-type class model dynamics based on the application of the Lotka-Volterra equation to economic growth and cycle.
description: 22 pages, 15 figures, 4 tables. LaTeX. Accepted for publication in "The European Physical Journal B"
The relation between 13CO(2-1) line width in molecular clouds and bolometric luminosity of associated IRAS sources
Creators: name: Wang, Ke
name: Wu, Yuefang
name: Ran, Liang
name: Yu, Wentao
name: Miller, Martin
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We search for evidence of a relation between properties of young stellar objects (YSOs) and their parent molecular clouds to understand the initial conditions of high-mass star formation. A sample of 135 sources was selected from the Infrared Astronomical Satellite (IRAS) Point Source Catalog, on the basis of their red color to enhance the possibility of discovering young sources. Using the Kolner Observatorium fur SubMillimeter Astronomie (KOSMA) 3-m telescope, a single-point survey in 13CO(2-1) was carried out for the entire sample, and 14 sources were mapped further. Archival mid-infrared (MIR) data were compared with the 13CO emissions to identify evolutionary stages of the sources. A 13CO observed sample was assembled to investigate the correlation between 13CO line width of the clouds and the luminosity of the associated YSOs. We identified 98 sources suitable for star formation analyses for which relevant parameters were calculated. We detected 18 cores from 14 mapped sources, which were identified with eight pre-UC HII regions and one UC HII region, two high-mass cores earlier than pre-UC HII phase, four possible star forming clusters, and three sourceless cores. By compiling a large (360 sources) 13CO observed sample, a good correlation was found between the 13CO line width of the clouds and the bolometric luminosity of the associated YSOs, which can be fitted as a power law: lg(dV13/km/s)=-0.023+0.135lg(Lbol/Lsolar). Results show that luminous (>10^3Lsolar) YSOs tend to be associated with both more massive and more turbulent (dV13>2km/s) molecular cloud structures.
description: Accepted by Astronomy and Astrophysics; this version: sent to publisher; 13 pages, 4 figures, 2 tables, 1 online appendix
Beauty, charm and $F_L$ at HERA: new data vs. early predictions
Creators: name: Nikolaev, N. N.
name: Zoller, V. R.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: One of the well known effects of the asymptotic freedom is splitting of the leading-$\log$ BFKL pomeron into a series of isolated poles in complex angular momentum plane. Following our earlier works we explore the phenomenological consequences of the emerging BFKL-Regge factorized expansion for the small-$x$ charm ($F_2^c$) and beauty ($F_{2}^{b}$) structure functions of the proton. As we found earlier,the color dipole approach to the BFKL dynamics predicts uniquely decoupling of subleading hard BFKL exchanges from $F_2^c$ at moderately large $Q^{2}$. We predicted precocious BFKL asymptotics of $F_2^c(x,Q^2)$ with intercept of the rightmost BFKL pole $α_{\Pom}(0)-1=Δ_{\Pom}\approx 0.4$. High-energy open beauty photo- and electro-production probes the vacuum exchange at much smaller distances and detects significant corrections to the BFKL asymptotics coming from the subleading vacuum poles. In view of the accumulation of the experimental data on small-$x$ $F_{2}^{c}$ and $F_{2}^{b}$ we extended our early predictions to the kinematical domain covered by new HERA measurements.Our structure functions obtained in 1999 agree well with the determination of both $F_2^c$ and $F_2^b$ by the H1 published in 2006 but contradict to very recent (2008, preliminary) H1 results on $F_2^b$. We present also comparison of our early predictions for the longitudinal structure function $F_L$ with recent H1 data (2008) taken at very low Bjorken $x$. We comment on the electromagnetic corrections to the Okun-Pomeranchuk theorem.
description: 16 pages, 4 figures. The contribution to the volume in honor of Lev Okun's 80 birthday
Additional file 1 of Relationship between the non-HDLc-to-HDLc ratio and carotid plaques in a high stroke risk population: a cross-sectional study in China
Creators: name: Liu, Yan
name: Zhang, Zhenwen
name: Xia, Binlan
name: Wang, Liping
name: Zhang, Hengzhong
name: Zhu, Yan
name: Liu, Chao
name: Song, Bin
Publisher: name: figshare
Year: 2020
Subjects: subject: Medicine
subject: Neuroscience
subject: Physiology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified

description: Additional file 1.
title: ÐÐ°Ð»ÑÐ¹ Ð½Ð°ÑÐµÐ»ÐµÐ½Ð½ÑÐ¹ Ð¿ÑÐ½ÐºÑ
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÑ ÑÐ½ Ð¡ÐµÑÐµÐ¹Ð¿Ð¾Ð½Ð»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: ÐÑÐµÐ½Ð°Ð¶
ÐÐ°Ð½Ð°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ
ÐÐ¾Ð´Ð¾ÑÑÐ¾ÐºÐ¸
Ð¢ÑÑÐ±Ñ
Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ñ
organization
drain
sewerage
effluent
pipes

description: ÐÐ°Ð½Ð½Ð°Ñ Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° Ð¸Ð½Ð¶ÐµÐ½ÐµÑÐ½Ð¾Ð¹ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð¸ Ð±Ð»Ð°Ð³Ð¾ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð°, Ð²Ð¾Ð´Ð¾Ð¾ÑÐ²ÐµÐ´ÐµÐ½Ð¸Ðµ Ð¸ Ð²Ð¾Ð´Ð¾Ð¿Ð¾Ð½Ð¸Ð¶ÐµÐ½Ð¸Ðµ Ð½Ð° ÑÐµÑÑÐ¸ÑÐ¾ÑÐ¸Ð¸ Ð½ÐµÐ±Ð¾Ð»ÑÑÐ¾Ð³Ð¾ Ð¿Ð¾ÑÐµÐ»ÐºÐ°. Ð¡ÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½ÑÑ Ð¿Ð»Ð¾ÑÐ°Ð´ÐºÑ Ð½ÐµÐ±Ð¾Ð»ÑÑÐ¾Ð¹ Ð¿Ð¾ÑÐµÐ»Ð¾Ðº, ÑÐ°ÑÐ¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð½ÑÐ¹ Ð² ÐÐµÐ½Ð¸Ð½Ð³ÑÐ°Ð´ÑÐºÐ¾Ð¹ Ð¾Ð±Ð»Ð°ÑÑÐ¸. Ð ÑÑÐ¾Ð¼ Ð´Ð¾ÐºÑÐ¼ÐµÐ½ÑÐµ ÑÐ¾Ð´ÐµÑÐ¶Ð¸ÑÑÑ Ð¿ÑÐ¾ÐµÐºÑ Ð¼Ð°Ð»Ð¾ÑÑÐ°Ð¶Ð½Ð¾Ð³Ð¾ Ð±Ð»Ð¾Ðº Ñ Ð´ÐµÑÐ°Ð»ÑÐ½Ð¾Ð¹ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¾Ð¹ Ð·Ð´Ð°Ð½Ð¸Ñ Ð°Ð´Ð¼Ð¸Ð½Ð¸ÑÑÑÐ°ÑÐ¸Ð²Ð½Ð¾-Ð±ÑÑÐ¾Ð²Ð¾Ð¹ ÑÐµÐ½ÑÑ Ð¸ Ð·Ð¾Ð½Ð° Ð¾ÑÐ´ÑÑÐ°, Ð° ÑÐ°ÐºÐ¶Ðµ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½ Ð¿ÑÐ¾ÐµÐºÑ Ð»Ð¸Ð²Ð½ÐµÐ²Ð¾Ð¹ Ð¸ Ð´ÑÐµÐ½Ð°Ð¶Ð½Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼ Ð´Ð»Ñ ÑÐ°Ð¹ÑÐ°. ÐÑÐµ ÑÐµÑÑÐµÐ¶Ð¸ Ð±ÑÐ»Ð¸ ÑÐ´ÐµÐ»Ð°Ð½Ñ Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ ÑÐ¸ÑÑÐµÐ¼Ñ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ (Ð¡ÐÐÐ ) AutoCAD 2015.
description: This final qualification work is devoted to engineering training and improvement, sanitation and dewatering in the territory of a small village. The construction site of a small settlement located in the Leningrad region. This paper contains the project of low-rise block with a detailed development of the building of administrative and household center and recreational area and also developed a draft storm water and drainage systems for the site. All drawings were made by using Computer Aided Design (CAD) AutoCAD 2015.
Elektromagnetische transiente Ausgleichsvorgänge in HGÜ-Systemen und deren Auswirkung auf die Isolationskoordination von Kabelanlagen
Creators: name: Görtz, Max Heinrich
Publisher: name: Karlsruher Institut für Technologie (KIT)
Year: 2021
Subjects: EMT
Energieübertragung
HGÜ
Isolationskoordination
Modularer Multilevelumrichter

description: Die Hochspannungs-Gleichstrom-Übertragung (HGÜ) auf Basis selbstgeführter Umrichter stellt einen Eckpfeiler für den Erfolg der Energiewende dar. Ausgelöst durch die prognostizierten Netzausbaumaßnahmen werden HGÜ-Kabelsysteme mittelfristig eine tragende Rolle in den europäischen Stromübertragungsnetzen einnehmen. Um für solche HGÜ-Kabelanlagen eine zuverlässige Auslegungsstrategie ermöglichen zu können, ist eine umfassende Kenntnis über die potentiell zu erwartenden elektrischen Beanspruchungen von entscheidender Bedeutung. Der Fokus dieser Forschungsarbeit liegt auf der Identifikation der mannigfaltigen Spannungsbeanspruchungen, die in HGÜ-Systemen basierend auf der Umrichtertechnologie von modularen Multilevelumrichtern während der Lebensdauer auftreten können. Hierzu zählen sowohl äußere Überspannungen infolge atmosphärischer Einwirkungen als auch innere Überspannungen aufgrund von diversen internen Fehlerereignissen. Diese Dissertation liefert eine umfassende Analyse der auftretenden elektromagnetischen transienten Ausgleichsvorgänge und leistet einen Beitrag zur Isolationskoordination von HGÜ-Kabelanlagen.
title: ÐÑÐµÐ½ÐºÐ° ÑÐµÐ»ÐµÑÐ¾Ð¾Ð±ÑÐ°Ð·Ð½Ð¾ÑÑÐ¸ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¿Ð¾ Ð³ÑÑÐ·Ð¾Ð¿ÐµÑÐµÐ²Ð¾Ð·ÐºÐ°Ð¼ Â«ÐÐ²ÑÐ¾Ð¢ÑÐ°Ð½ÑÐÐ½ÑÐ¾Â» Ð´Ð»Ñ ÐÐÐ Â«Ð¤Ð¾ÑÐ²Ð°ÑÐ´Â»
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
Creators: name: Ð¡ÐµÐ½Ð¸Ð½Ð°, ÐÐ°Ð»ÐµÑ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: Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐµ ÑÐ¸ÑÑÐµÐ¼Ñ
Ð³ÑÑÐ·Ð¾Ð²ÑÐµ Ð¿ÐµÑÐµÐ²Ð¾Ð·ÐºÐ¸
ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ½Ð°Ñ Ð»Ð¾Ð³Ð¸ÑÑÐ¸ÐºÐ°
Ð°Ð²ÑÐ¾Ð¼Ð¾Ð±Ð¸Ð»ÑÐ½ÑÐ¹ ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑ

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ñ ÐÐÐ Â«Ð¤Ð¾ÑÐ²Ð°ÑÐ´Â» ÑÐ²Ð»ÑÐµÑÑÑ Ð¾Ð±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ. Ð¦ÐµÐ»ÑÑ Ð½Ð°Ð¿Ð¸ÑÐ°Ð½Ð¸Ñ Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ ÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾Ð³Ð¾ ÑÐ»ÑÑÑÐ¸ÑÑ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ ÐÐÐ Â«Ð¤Ð¾ÑÐ²Ð°ÑÐ´Â». Ð ÑÐ°Ð±Ð¾ÑÐµ Ð½Ð°Ð¹Ð´ÐµÐ½ ÑÐ¿Ð¾ÑÐ¾Ð± ÑÐ»ÑÑÑÐµÐ½Ð¸Ñ Ð²Ð·Ð°Ð¸Ð¼Ð¾Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ Ñ ÐºÐ¾Ð½ÑÑÐ°Ð³ÐµÐ½ÑÐ°Ð¼Ð¸. Ð¡Ð´ÐµÐ»Ð°Ð½ Ð¿ÑÐ¾Ð³Ð½Ð¾Ð· Ð²ÑÑÑÑÐºÐ¸ Ð¸ Ð·Ð°ÑÑÐ°Ñ. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ ÑÐ°ÑÑÐµÑ ÐºÐ¾Ð¼Ð¼ÐµÑÑÐµÑÐºÐ¾Ð¹ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð½ÑÑ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹.
The column density towards LMC X-1
Creators: name: Hanke, Manfred
name: Wilms, Joern
name: Nowak, Michael A.
name: Barragan, Laura
name: Schulz, Norbert S.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We measure the neutral absorption towards the black hole X-ray binary system LMC X-1 from six archival soft X-ray spectra obtained with the gratings and/or CCD detectors on Chandra, XMM-Newton, and Swift. Four spectral models for the soft continuum have been investigated. While the powerlaw model may overestimate NH considerably, the others give consistent results. Taking the lower metalicity of the Large Magellanic Cloud into account, we find equivalent hydrogen column densities of N_H = (1.0-1.3)*10^22 cm^-2, with a systematic dependence on the orbital phase. This variation of the neutral absorption can nearly explain the orbital modulation of the soft X-ray flux recently detected with the All Sky Monitor (ASM) on the Rossi X-ray Timing Explorer (RXTE).
description: 4 pages, accepted for publication as a Letter in Astronomy and Astrophysics
Linguistically diverse assessment : a Canadian context
Creators: name: Jackart, Laine
Publisher: name: University of British Columbia
Year: 2024

description: In Canada, there are currently no standardized national guidelines for the psychoeducational assessment of linguistically diverse individuals. It is the role of Canadian psychologists and psychological associates to adopt psychoeducational assessment practices that mitigate the historic over-referral to special education programs of students who are linguistically diverse, the misdiagnosis of these students, and the mismatch of educational services and supports to these students. The potential over-referral of these students for special education programming may be derived from a lack of understanding of language acquisition factors, an over-reliance on standardized tests with norms that may not reflect the diverse populations that psychologists are working with as well as a lack of standardized national assessment guidelines for practitioners to follow. This over-referral is a human rights issue and is potentially made worse by the lack of standardized guidelines, as these students may benefit more from the support of their language acquisition rather than special education services. In this study, an online survey of 73 practitioners conducting psychoeducational assessments for the purpose of supporting Canadian students was conducted to better understand what practices practitioners are employing when working with linguistically diverse clients. Respondents to the survey reported using a variety of assessment methods. Of the various assessment methods reported by surveyed practitioners, some align with the literature on ensuring appropriate assessment of linguistically diverse clients, while other do not.
title: ÐÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ñ Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð¾Ð²ÑÑ ÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð¹ Ð² Ð±Ð»Ð°Ð³Ð¾ÑÐ²Ð¾ÑÐ¸ÑÐµÐ»ÑÐ½Ð¾Ð¹ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ Ð¡ÐÐÐÐÐÐÐÐ Â«Ð£Ð¼ÐºÐ°Â»)
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ°ÑÐ¼Ð°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: 2017
Subjects: Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð¾Ð²ÑÐµ ÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð¸
Ð±Ð»Ð°Ð³Ð¾ÑÐ²Ð¾ÑÐ¸ÑÐµÐ»ÑÐ½Ð°Ñ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ
ÐºÐ°Ð½Ð°Ð»Ñ ÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð¸

description: Ð ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑÑÑ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð±Ð»Ð°Ð³Ð¾ÑÐ²Ð¾ÑÐ¸ÑÐµÐ»ÑÐ½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸. ÐÐ½Ð°Ð»Ð¸Ð·Ð¸ÑÑÐµÐ¼ÑÑ ÑÑÐ½Ð¾Ðº Ð¸ ÑÑÐµÐ´Ð° Ð±Ð»Ð°Ð³Ð¾ÑÐ²Ð¾ÑÐ¸ÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸. Ð Ð°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑÑÑ ÑÑÑÐ´Ð½Ð¾ÑÑÐ¸ Ð¸ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ, Ñ ÐºÐ¾ÑÐ¾ÑÑÐ¼Ð¸ ÑÑÐ°Ð»ÐºÐ¸Ð²Ð°ÑÑÑÑ Ð±Ð»Ð°Ð³Ð¾ÑÐ²Ð¾ÑÐ¸ÑÐµÐ»Ð¸, Ð±Ð»Ð°Ð³Ð¾ÑÐ²Ð¾ÑÐ¸ÑÐµÐ»ÑÐ½ÑÐµ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸. Ð Ð·Ð°ÐºÐ»ÑÑÐ¸ÑÐµÐ»ÑÐ½Ð¾Ð¹ Ð³Ð»Ð°Ð²Ðµ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¿Ð¾ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð¾Ð²ÑÑ ÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð¹ Ð´Ð»Ñ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Â«Ð£Ð¼ÐºÐ°Â».