cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: ÐÑÐ°Ð²Ð¾Ð²Ð¾Ðµ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ðµ Ð¿ÑÐ¾Ð´Ð¾Ð²Ð¾Ð»ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸ Ð² Ð Ð¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð¹ Ð¤ÐµÐ´ÐµÑÐ°ÑÐ¸Ð¸
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
Creators: name: ÐÑÑÐµÐ½ÐºÐ¾, ÐÐµÐ½Ð¸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¿ÑÐ¾Ð´Ð¾Ð²Ð¾Ð»ÑÑÑÐ²Ð¸Ðµ
Ð¿ÑÐ¾Ð´Ð¾Ð²Ð¾Ð»ÑÑÑÐ²ÐµÐ½Ð½Ð°Ñ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÑ
Ð¿ÑÐ¾Ð´Ð¾Ð²Ð¾Ð»ÑÑÑÐ²ÐµÐ½Ð½Ð°Ñ Ð½ÐµÐ·Ð°Ð²Ð¸ÑÐ¸Ð¼Ð¾ÑÑÑ
Ð¿ÑÐ¾Ð´ÑÐºÑÑ Ð¿Ð¸ÑÐ°Ð½Ð¸Ñ
ÐºÐ°ÑÐµÑÑÐ²Ð¾ Ð¸ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÑ Ð¿Ð¸ÑÐµÐ²ÑÑ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¾Ð².

description: Ð Ð½Ð°ÑÑÐ¾ÑÑÐµÐ¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¸ÑÑÐ»ÐµÐ´ÑÐµÑÑÑ Ð¿ÑÐ°Ð²Ð¾Ð²Ð¾Ðµ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ðµ Ð¿ÑÐ¾Ð´Ð¾Ð²Ð¾Ð»ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð»Ð¸ÑÐ½ÑÑ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸ Ð Ð¾ÑÑÐ¸Ð¸. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¿Ð¾Ð½ÑÑÐ¸Ðµ Ð¸ ÑÐ°ÐºÑÐ¾ÑÑ Ð¿ÑÐ¾Ð´Ð¾Ð²Ð¾Ð»ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸. ÐÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð¾ Ð½Ð¾ÑÐ¼Ð°ÑÐ¸Ð²Ð½Ð¾Ðµ Ð¿ÑÐ°Ð²Ð¾Ð²Ð¾Ðµ Ð·Ð°Ð¿ÑÐµÑ ÑÐµÐ³ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¿ÑÐ¾Ð´Ð¾Ð²Ð¾Ð»ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð·Ð°ÑÐ¸ÑÐ° Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸ Ð Ð¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð¹ Ð¤ÐµÐ´ÐµÑÐ°ÑÐ¸Ð¸. Ð ÑÐ¾Ð´Ðµ Ð·Ð°ÑÐ¸ÑÐµ ÑÐ°Ð±Ð¾ÑÑ Ð±ÑÐ»Ð¸ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¾ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ðµ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ðµ Ð¿ÑÐ¾Ð´Ð¾Ð²Ð¾Ð»ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð·ÐµÐ¼ÐµÐ»Ñ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸ Ð Ð¾ÑÑÐ¸Ð¸, ÑÐ³ÑÐ¾Ð·Ñ Ð¸ ÑÐ¸ÑÐºÐ¸ Ð¿ÑÐ¾Ð´Ð¾Ð²Ð¾Ð»ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸, Ð¸Ð¼Ð¿Ð¾ÑÑ Ð° ÑÐ°ÐºÐ¶Ðµ Ð¸Ð½Ð´ÐµÐºÑ Ð²ÑÑÐ²Ð»ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð¸ÑÐ¾Ð³Ð°Ð¼ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð Ð¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð¹ Ð¤ÐµÐ´ÐµÑÐ°ÑÐ¸Ð¸ Ð¿Ð¾ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ Ð¿ÑÐ¾Ð´Ð¾Ð²Ð¾Ð»ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸ Ð¸ Ð¿ÑÐµÐ¾Ð´Ð¾Ð»ÐµÐ½Ð¸Ñ Ð²Ð¾Ð·Ð½Ð¸ÐºÐ°ÑÑÐ¸Ñ Ð² ÑÐ²ÑÐ·Ð¸ Ñ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸ÐµÐ¼ Ð¿ÑÐ¾Ð´Ð¾Ð²Ð¾Ð»ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼.
Solution of Peter Winkler's Pizza Problem
Creators: name: Cibulka, Josef
name: Kynčl, Jan
name: Mészáros, Viola
name: Stolař, Rudolf
name: Valtr, Pavel
Publisher: name: arXiv
Year: 2008
Subjects: subject: Discrete Mathematics (cs.DM)
subject: FOS: Computer and information sciences
subject: G.2.1

description: Bob cuts a pizza into slices of not necessarily equal size and shares it with Alice by alternately taking turns. One slice is taken in each turn. The first turn is Alice's. She may choose any of the slices. In all other turns only those slices can be chosen that have a neighbor slice already eaten. We prove a conjecture of Peter Winkler by showing that Alice has a strategy for obtaining 4/9 of the pizza. This is best possible, that is, there is a cutting and a strategy for Bob to get 5/9 of the pizza. We also give a characterization of Alice's best possible gain depending on the number of slices. For a given cutting of the pizza, we describe a linear time algorithm that computes Alice's strategy gaining at least 4/9 of the pizza and another algorithm that computes the optimal strategy for both players in any possible position of the game in quadratic time. We distinguish two types of turns, shifts and jumps. We prove that Alice can gain 4/9, 7/16 and 1/3 of the pizza if she is allowed to make at most two jumps, at most one jump and no jump, respectively, and the three constants are the best possible.
description: 29 pages, 14 figures
title: ÐÐ¾ÐºÐ°Ð»ÑÐ½Ð°Ñ Ð½Ð°Ð²Ð¸Ð³Ð°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ¸ÑÑÐµÐ¼Ð°, Ð²ÐºÐ»ÑÑÐ°ÑÑÐ°Ñ Ð¼Ð¾Ð±Ð¸Ð»ÑÐ½ÑÑ Ð±Ð°Ð·Ð¾Ð²ÑÑ ÑÑÐ°Ð½ÑÐ¸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¢ÑÐ¸ÑÐ¾Ð½Ð¾Ð², ÐÐ»ÐµÐºÑÐ°Ð½Ð´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¡Ð¿ÑÑÐ½Ð¸ÐºÐ¾Ð²Ð°Ñ Ð½Ð°Ð²Ð¸Ð³Ð°ÑÐ¸Ñ
Ð Ð°Ð´Ð¸Ð¾Ð½Ð°Ð²Ð¸Ð³Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐµ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¸ ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð°
ÐÐ°ÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ðµ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
ÐÑÑÐ¸ÑÐ»Ð¸ÑÐµÐ»ÑÐ½ÑÐµ Ð¼Ð°ÑÐ¸Ð½Ñ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½ÑÐµ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»ÑÐ½ÑÐµ
Ð½Ð°Ð²Ð¸Ð³Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐ¹ Ð¾Ð±ÑÐµÐºÑ
Ð¼Ð¾Ð±Ð¸Ð»ÑÐ½Ð°Ñ Ð±Ð°Ð·Ð¾Ð²Ð°Ñ ÑÑÐ°Ð½ÑÐ¸Ñ
the navigation object
mobile base station

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ð¸ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÐµÑÑÑ Ð»Ð¾ÐºÐ°Ð»ÑÐ½Ð°Ñ Ð½Ð°Ð²Ð¸Ð³Ð°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ¸ÑÑÐµÐ¼Ð° (ÐÐÐ¡), Ð²ÐºÐ»ÑÑÐ°ÑÑÐ°Ñ Ð¼Ð¾Ð±Ð¸Ð»ÑÐ½ÑÑ Ð±Ð°Ð·Ð¾Ð²ÑÑ ÑÑÐ°Ð½ÑÐ¸Ñ (ÐÐÐ¡). ÐÐ¾ÑÐºÐ¾Ð»ÑÐºÑ ÐºÐ¾Ð¾ÑÐ´Ð¸Ð½Ð°ÑÑ ÐÐÐ¡ Ð¿Ð¾ÑÑÐ¾ÑÐ½Ð½Ð¾ Ð¸Ð·Ð¼ÐµÐ½ÑÑÑÑÑ, Ð²Ð¾Ð·Ð½Ð¸ÐºÐ°ÐµÑ Â«Ð´Ð²Ð¾Ð¹Ð½Ð°ÑÂ» Ð½Ð°Ð²Ð¸Ð³Ð°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ Ð·Ð°Ð´Ð°ÑÐ°: Ð¿ÑÐµÐ¶Ð´Ðµ, ÑÐµÐ¼ Ð¾Ð¿ÑÐµÐ´ÐµÐ»Ð¸ÑÑ Ð¼ÐµÑÑÐ¾Ð¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ðµ Ð½Ð°Ð²Ð¸Ð³Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð¾Ð±ÑÐµÐºÑÐ°, Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼Ð¾ ÑÐ°ÑÑÑÐ¸ÑÐ°ÑÑ ÐºÐ¾Ð¾ÑÐ´Ð¸Ð½Ð°ÑÑ ÐÐÐ¡. Ð ÑÑÐµÐ´Ðµ Matlab ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° Ð¼Ð¾Ð´ÐµÐ»Ñ, Ð¿Ð¾Ð·Ð²Ð¾Ð»ÑÑÑÐ°Ñ Ð¾ÑÐµÐ½Ð¸ÑÑ ÑÐ¾ÑÐ½Ð¾ÑÑÑ ÑÐµÑÐµÐ½Ð¸Ñ Ð½Ð°Ð²Ð¸Ð³Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ Ð·Ð°Ð´Ð°ÑÐ¸, ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¼ÐµÑÐ¾Ð´Ñ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÑÐ¾ÑÐ½Ð¾ÑÑÐ¸ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ ÐºÐ¾Ð¾ÑÐ´Ð¸Ð½Ð°Ñ Ð½Ð°Ð²Ð¸Ð³Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð¾Ð±ÑÐµÐºÑÐ°.
description: The subject of this research is the local navigation system (LNS) with mobile base station (MBS). The mobile base station changes its location permanently, so there is a âdualâ navigation problem: it is necessary to find coordinates of MBS before find location of navigation object. The model of LNS is developed in Matlab environment. The model allows to find precision of navigation object positioning. The methods of increasing of navigation object positioning have been researched.
Democracy & Distrust: The Election Integrity Movement, 2020–2023
Creators: name: Garai, Zachary
Publisher: name: University of Chicago
Year: 2023

description: I aim in this thesis to explain why Republican politicians have pursued restrictive election laws, while Democrats have promoted permissive ones, after the 2020 election. During the 2020–2023 period, following Donald Trump’s disinformation campaign alleging that the 2020 presidential results were illegitimate, American politics increasingly polarized around election integrity concerns. Republicans fearful of widespread fraud wanted to enhance security measures while Democrats generally sought to expand ballot access. Previous research focused on the differentiation of conservative and liberal media spheres, the asymmetrical radicalization of those in the conservative network, and different conceptions of democracy. The scholarship also addresses how rising polarization has reduced politics to a zero-sum game, and how American federalism has led policymaking processes in Republican and Democratic-controlled states to diverge. My argument synthesizes these strands and contributes by identifying the mechanism that produced these diverging approaches to election administration. I then present and test a series of hypotheses designed to evaluate the theory I elaborate and its implications by using survey data, self-made datasets, and several regression models.
title: Ð¢Ð¾Ð²Ð°ÑÐ¾Ð²ÐµÐ´Ð½Ð°Ñ Ñ Ð°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ°, ÑÐºÑÐ¿ÐµÑÑÐ¸Ð·Ð° ÐºÐ°ÑÐµÑÑÐ²Ð° Ð¿Ð¾Ð»ÑÑÐ°Ð±ÑÐ¸ÐºÐ°ÑÐ¾Ð² Ð¸Ð· Ð¼ÑÑÐ° Ð¿ÑÐ¸ÑÑ Ð¸ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ñ ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ð¸ Ð¼ÑÑÐ½ÑÐ¼Ð¸ ÑÐ¾Ð²Ð°ÑÐ°Ð¼Ð¸ Ð² ÑÐ¾Ð·Ð½Ð¸ÑÐ½Ð¾Ð¼ ÑÐ¾ÑÐ³Ð¾Ð²Ð¾Ð¼ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸
title: Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¾Ð·ÑÑÐµÐ², Ð¯ÑÐ¾Ñ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: 2016
Subjects: Ð¼ÑÑÐ¾ Ð¿ÑÐ¸ÑÑ
Ð¾ÑÐµÐ½ÐºÐ° ÐºÐ°ÑÐµÑÑÐ²Ð°
ÑÐºÑÐ¿ÐµÑÑÐ¸Ð·Ð° ÐºÐ°ÑÐµÑÑÐ²Ð°
poultry meat
quality control
expert's quality report

description: Ð Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ "Ð¢Ð¾Ð²Ð°ÑÐ¾Ð²ÐµÐ´Ð½Ð°Ñ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ°, ÑÐºÑÐ¿ÐµÑÑÐ¸Ð·Ð° ÐºÐ°ÑÐµÑÑÐ²Ð° Ð¿Ð¾Ð»ÑÑÐ°Ð±ÑÐ¸ÐºÐ°ÑÐ¾Ð² Ð¸Ð· Ð¼ÑÑÐ° Ð¿ÑÐ¸ÑÑ Ð¸ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ñ ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ð¸ Ð¼ÑÑÐ½ÑÐ¼Ð¸ ÑÐ¾Ð²Ð°ÑÐ°Ð¼Ð¸ Ð² ÑÐ¾Ð·Ð½Ð¸ÑÐ½Ð¾Ð¼ ÑÐ¾ÑÐ³Ð¾Ð²Ð¾Ð¼ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸" ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð²Ð¾Ð¿ÑÐ¾ÑÑ ÑÑÐ½ÐºÐ°, ÐºÐ»Ð°ÑÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¸ Ð¸ Ð°ÑÑÐ¾ÑÑÐ¸Ð¼ÐµÐ½ÑÐ° Ð¿Ð¾Ð»ÑÑÐ°Ð±ÑÐ¸ÐºÐ°ÑÐ¾Ð² Ð¸Ð· Ð¼ÑÑÐ° Ð¿ÑÐ¸ÑÑ. ÐÑÐ¸Ð²ÐµÐ´ÐµÐ½Ñ ÑÐµÐ»Ñ, Ð·Ð°Ð´Ð°ÑÐ¸ Ð¸ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ ÑÐºÑÐ¿ÐµÑÑÐ¸Ð·Ñ ÐºÐ°ÑÐµÑÑÐ²Ð° ÑÑÐ±Ð»ÐµÐ½ÑÑ Ð¿Ð¾Ð»ÑÑÐ°Ð±ÑÐ¸ÐºÐ°ÑÐ¾Ð² Ð¸Ð· Ð¼ÑÑÐ° Ð¿ÑÐ¸ÑÑ Ð¿Ð¾ Ð¾ÑÐ³Ð°Ð½Ð¾Ð»ÐµÐ¿ÑÐ¸ÑÐµÑÐºÐ¸Ð¼, ÑÐ¸Ð·Ð¸ÐºÐ¾-ÑÐ¸Ð¼Ð¸ÑÐµÑÐºÐ¸Ð¼ Ð¸ Ð¼Ð¸ÐºÑÐ¾Ð±Ð¸Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ð¼ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»ÑÐ¼. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð° ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ¾-Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÑÑÑÐºÑÑÑÐ° ÑÐ¾Ð·Ð½Ð¸ÑÐ½Ð¾Ð³Ð¾ ÑÐ¾ÑÐ³Ð¾Ð²Ð¾Ð³Ð¾ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Â«ÐÐµÐ»ÐµÑÂ» Ð¸ Ð¾ÑÐµÐ½ÐµÐ½Ð° ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¼ÑÑÐ½Ð¾Ð¹ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¸Ð¸ Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸.
description: In the final qualifying work "Commodity research characteristics, examination of the quality of semi-finished products from poultry and the trade in meat products retail trade enterprise" examines the issues of market, classification and assortment of semi-finished products from poultry meat. Given the purpose, objectives and results of quality evaluation of minced semi-finished products of poultry meat by organoleptic, physico-chemical and microbiological indicators. Reviewed economic and organizational structure of the retail trade enterprise "Veles" and evaluated the effectiveness of the implementation of meat products at the plant.
title: Ð¡Ð¿Ð¾ÑÑÐ¸Ð²Ð½Ð°Ñ Ð¼ÐµÐ´Ð¸ÑÐ¸Ð½Ð° Ð² ÐºÐ¾Ð½ÑÐµÐºÑÑÐµ Ð¸Ð½Ð´Ð¸Ð²Ð¸Ð´ÑÐ°Ð»ÑÐ½Ð¾Ð¹ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾Ð¹ ÑÑÐ°ÐµÐºÑÐ¾ÑÐ¸Ð¸ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ñ Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð²-Ð¼ÐµÐ´Ð¸ÐºÐ¾Ð²
title: Sports medicine in the context of an individual educational training program for medical students
Creators: name: ÐÑÑÐ°ÑÑÐ¸Ðº, ÐÐ°Ð»Ð¸Ð½Ð°
name: ÐÐ°ÑÐ¼Ð¾Ð½, ÐÐ»ÐµÐ½Ð°
name: "Ð¡Ð¿Ð¾ÑÑ, ÑÐµÐ»Ð¾Ð²ÐµÐº, Ð·Ð´Ð¾ÑÐ¾Ð²ÑÐµ", Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÐ¹ Ð½Ð°ÑÑÐ½ÑÐ¹ ÐºÐ¾Ð½Ð³ÑÐµÑÑ
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2023
Subjects: ÑÐ¿Ð¾ÑÑÐ¸Ð²Ð½Ð°Ñ Ð¼ÐµÐ´Ð¸ÑÐ¸Ð½Ð°
Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ðµ
Ð¸Ð½Ð´Ð¸Ð²Ð¸Ð´ÑÐ°Ð»ÑÐ½Ð°Ñ ÑÑÐ°ÐµÐºÑÐ¾ÑÐ¸Ñ
sports medicine
education
individual trajectory

description: ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð·Ð°ÑÑÐ±ÐµÐ¶Ð½Ð¾Ð³Ð¾ Ð¸ Ð¾ÑÐµÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¾Ð¿ÑÑÐ°, ÑÑÐµÐ±Ð½ÑÑ Ð¿Ð»Ð°Ð½Ð¾Ð² Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð²-Ð¼ÐµÐ´Ð¸ÐºÐ¾Ð² Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Â«Ð¡Ð¿Ð¾ÑÑÐ¸Ð²Ð½Ð°Ñ Ð¼ÐµÐ´Ð¸ÑÐ¸Ð½Ð°Â». ÐÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ñ Ð¾Ð³ÑÐ°Ð½Ð¸ÑÐµÐ½Ð¸Ñ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Â«Ð¡Ð¿Ð¾ÑÑÐ¸Ð²Ð½Ð°Ñ Ð¼ÐµÐ´Ð¸ÑÐ¸Ð½Ð°Â» Ð² ÑÑÐµÐ±Ð½ÑÐµ Ð¿Ð»Ð°Ð½Ñ Ð¸ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð²ÑÐ°ÑÐµÐ¹ Ð½Ð° Ð´Ð¾Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½Ð¾Ð¼ ÑÑÐ¾Ð²Ð½Ðµ. ÐÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½ Ð¾Ð¿ÑÑ Ð¿Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ñ Ð¸Ð½Ð´Ð¸Ð²Ð¸Ð´ÑÐ°Ð»ÑÐ½Ð¾Ð¹ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾Ð¹ ÑÑÐ°ÐµÐºÑÐ¾ÑÐ¸Ð¸ Â«Ð¡Ð¿Ð¾ÑÑÐ¸Ð²Ð½Ð°Ñ Ð¼ÐµÐ´Ð¸ÑÐ¸Ð½Ð°Â» Ð¿ÑÐ¸ Ð¾Ð±ÑÑÐµÐ½Ð¸Ð¸ Ð¿Ð¾ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ðµ ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸ÑÐµÑÐ° Â«ÐÐµÑÐµÐ±Ð½Ð¾Ðµ Ð´ÐµÐ»Ð¾Â» Ð² Ð¦ÐµÐ½ÑÑÐµ ÐÐ»Ð¼Ð°Ð·Ð¾Ð²Ð°.
description: The analysis of foreign and domestic experience, curricula for the training of medical students in the direction of âSports Medicineâ was carried out. The limitations of introducing the disciplines of the direction âSports medicineâ into curricula and programs at the undergraduate level were revealed. The experience of building an individual educational trajectory âSports Medicineâ under the program of the specialty âGeneral Medicineâ at the Almazov Center is presented.
Comment on "A 'local observables' method for wave mechanics applied to atomic hydrogen," by Peter Bowman [Am. J. Phys. 76, 1120-1129 (2008)]
Creators: name: Ohanian, Hans C.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: This comment identifies a mistake in a paper by P. Bowman that claims that the total angular momentum of the ground state of atomic hydrogen is 1.
description: 2 pp. To be published in Am. J. Phys
Ефективне використання наукометричних баз даних платформи EbscoHOST в університеті
Creators: name: Vasyliev, Oleksii
Publisher: name: Zenodo
Year: 2019
Subjects: EBSCOhost
Academic Search Premier
SCOPUS
Web of Science
Information Retrieval

description: План презентації: а) Колекція баз даних (пакет eIFL) компанії EbscoHOST та їх використання у наукових та наукометричних дослідженнях. б) Фактори ефективного використання Колекції в інформаційному забезпеченні наукових дослідженнях університету. Проблеми доступу до повних текстів публікацій. г) Організація моніторинга та менеджменту інформації про наукові публікації на платформі EbscoHOST
title: Ð¤Ð¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð·Ð°ÑÑÐ°Ñ Ð½Ð°ÑÐµÐ»ÐµÐ½Ð¸Ñ Ð½Ð° ÑÑÐ»ÑÐ³Ð¸ Ð¶Ð¸Ð»Ð¸ÑÐ½Ð¾-ÐºÐ¾Ð¼Ð¼ÑÐ½Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ Ñ Ð¾Ð·ÑÐ¹ÑÑÐ²Ð°
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð¢Ð°Ð³Ð¸Ð»ÑÑÐµÐ²Ð°, ÐÐ½Ð½Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2016
Subjects: Ð¶Ð¸Ð»Ð¸ÑÐ½Ð¾-ÐºÐ¾Ð¼Ð¼ÑÐ½Ð°Ð»ÑÐ½Ð¾Ðµ Ñ Ð¾Ð·ÑÐ¹ÑÑÐ²Ð¾
Ð¶Ð¸Ð»Ð¸ÑÐ½Ð¾-ÐºÐ¾Ð¼Ð¼ÑÐ½Ð°Ð»ÑÐ½ÑÐµ ÑÑÐ»ÑÐ³Ð¸
ÑÐ°ÑÐ¸ÑÑ
housing services
rates

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ Ð¿ÑÐ¾ÑÐµÑÑ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¶Ð¸Ð»Ð¸ÑÐ½Ð¾-ÐºÐ¾Ð¼Ð¼ÑÐ½Ð°Ð»ÑÐ½ÑÐ¼ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ¾Ð¼ Ð¼ÑÐ½Ð¸ÑÐ¸Ð¿Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ. ÐÑÐµÐ´Ð¼ÐµÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð²ÑÑÑÑÐ¿Ð°ÑÑ Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸Ñ Ð¸ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¶Ð¸Ð»Ð¸ÑÐ½Ð¾-ÐºÐ¾Ð¼Ð¼ÑÐ½Ð°Ð»ÑÐ½ÑÐ¼ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ¾Ð¼ Ð³Ð¾ÑÐ¾Ð´Ð° ÐÐµÐ»Ð³Ð¾ÑÐ¾Ð´Ð°. Ð¦ÐµÐ»Ñ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ - Ð°Ð½Ð°Ð»Ð¸Ð· Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¹ Ð¿Ð¾ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¶Ð¸Ð»Ð¸ÑÐ½Ð¾-ÐºÐ¾Ð¼Ð¼ÑÐ½Ð°Ð»ÑÐ½ÑÐ¼ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ¾Ð¼. Ð ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÑÑÐ°Ð½Ð¾Ð²Ð»ÐµÐ½Ð° ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð½Ð¾Ð²ÑÑ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² Ð¾Ð¿Ð»Ð°ÑÑ Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ Ð¿ÑÐ¸Ð±Ð¾ÑÐ¾Ð² ÑÑÐµÑÐ°, Ð¿ÐµÑÐµÐ´ ÑÐ¸ÑÑÐµÐ¼Ð¾Ð¹ Ð¾Ð¿Ð»Ð°ÑÑ Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ Ð½Ð¾ÑÐ¼Ð°ÑÐ¸Ð²Ð¾Ð². ÐÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ñ ÐºÐ¾Ð½ÐºÑÐµÑÐ½ÑÐµ Ð¼ÐµÑÑ Ð¿Ð¾ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ ÐÐÐ Ð³Ð¾ÑÐ¾Ð´Ð° ÐÐµÐ»Ð³Ð¾ÑÐ¾Ð´Ð°, Ð° ÑÐ°ÐºÐ¶Ðµ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¿Ð¾ ÑÐ¿Ð¾ÑÑÐ´Ð¾ÑÐµÐ½Ð¸Ñ ÑÐ°ÑÐ¸ÑÐ½Ð¾Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ¸.
description: The object of this work is the management of housing and communal services of the municipality. The subject of research are the relationships and management indicators of housing and communal complex of the city of Belgorod. The purpose of the final work - the analysis and development of recommendations to improve the management of housing and communal complex. The study established the effectiveness of the use of new payment methods using meters, before payment system using standards. Proposed specific measures to improve the FCC city of Belgorod, as well as recommendations to streamline the tariff policy.
Spitzer 24 um Images of Planetary Nebulae
Creators: name: Chu, Y. -H.
name: Gruendl, R. A.
name: Guerrero, M. A.
name: Su, K. Y. L.
name: Bilikova, J.
name: Cohen, M.
name: Parker, Q. A.
name: Volk, K.
name: Caulet, A.
name: Chen, W. -P.
name: Hora, J. L.
name: Rauch, T.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Spitzer MIPS 24 um images were obtained for 36 Galactic planetary nebulae (PNe) whose central stars are hot white dwarfs (WDs) or pre-WDs with effective temperatures of ~100,000 K or higher. Diffuse 24 um emission is detected in 28 of these PNe. The eight non-detections are angularly large PNe with very low H-alpha surface brightnesses. We find three types of correspondence between the 24 um emission and H-alpha line emission of these PNe: six show 24 um emission more extended than H-alpha emission, nine have a similar extent at 24 um and H-alpha, and 13 show diffuse 24 um emission near the center of the H-alpha shell. The sizes and surface brightnesses of these three groups of PNe and the non-detections suggest an evolutionary sequence, with the youngest ones being brightest and the most evolved ones undetected. The 24 um band emission from these PNe is attributed to [O IV] 25.9 um and [Ne V] 24.3 um line emission and dust continuum emission, but the relative contributions of these three components depend on the temperature of the central star and the distribution of gas and dust in the nebula.
description: 24 pages, 8 figures, to appear in the Astronomical Journal, September issue. Relace previous file; two references are added and typos are corrected
title: ÐÑÐ¾ÐµÐºÑ ÐºÐ¾ÑÐµÐ»ÑÐ½Ð¾Ð¹ Ð´Ð»Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐµÐ¿Ð»Ð° Ð¸ Ð³Ð¾ÑÑÑÐ¸Ñ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¾Ð² Ð¿ÐµÑÐµÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð¾ÑÑ Ð¾Ð´Ð¾Ð²
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
Creators: name: Ð¨Ð°ÑÐ¾Ð², Ð¡ÐµÑÐ³ÐµÐ¹
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¿ÑÐ¾ÐµÐºÑ ÐºÐ¾ÑÐµÐ»ÑÐ½Ð¾Ð¹
Ð±Ð¸Ð¾ÑÐ¾Ð¿Ð»Ð¸Ð²Ð¾
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description: ÐÑÐ»Ð° Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð° Ð¸ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð° Ð·Ð°Ð¼ÐµÐ½Ð° Ð¾Ð´Ð½Ð¾Ð³Ð¾ Ð¸Ð· Ð¾ÑÐ½Ð¾Ð²Ð½ÑÑ ÐºÐ¾ÑÐ»Ð¾Ð² Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸, ÑÐºÑÐ¿Ð»ÑÐ°ÑÐ¸ÑÑÑÑÐ¸ÑÑÑ Ð½Ð° Ð³Ð°Ð·Ðµ, Ð½Ð° ÐºÐ¾ÑÐµÐ» Ð-12-1,4Ð , ÑÐ°Ð±Ð¾ÑÐ°ÑÑÐµÐ³Ð¾ Ð½Ð° Ð±Ð¸Ð¾ÑÐ¾Ð¿Ð»Ð¸Ð²Ðµ(Ð¿Ð¾Ð´ÑÑÐ¸Ð»Ð¾ÑÐ½Ð¾-Ð¿Ð¾Ð¼ÐµÑÐ½Ð¾Ð¹ Ð¼Ð°ÑÑÐµ). ÐÑÐ¿Ð¾Ð»Ð½ÐµÐ½ ÑÐ°ÑÑÐµÑ ÑÐµÐ¿Ð»Ð¾Ð²ÑÑ Ð½Ð°Ð³ÑÑÐ·Ð¾Ðº, ÑÐµÐ¿Ð»Ð¾Ð²Ð¾Ð¹ ÑÑÐµÐ¼Ñ ÐºÐ¾ÑÐµÐ»ÑÐ½Ð¾Ð¹ Ð¸ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð¾ Ð¾Ð¿Ð¸ÑÐ°Ð½Ð¸Ðµ ÑÐµÐ¿Ð»Ð¾Ð²Ð¾Ð³Ð¾ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ. ÐÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½Ð° Ð¾ÑÐµÐ½ÐºÐ° ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¹ ÑÐµÐ»ÐµÑÐ¾Ð¾Ð±ÑÐ°Ð·Ð½Ð¾ÑÑÐ¸ ÑÑÑÐ°Ð½Ð¾Ð²ÐºÐ¸.
The Matter Bispectrum in N-body Simulations with non-Gaussian Initial Conditions
Creators: name: Sefusatti, Emiliano
name: Crocce, Martin
name: Desjacques, Vincent
Publisher: name: arXiv
Year: 2010
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We present measurements of the dark matter bispectrum in N-body simulations with non-Gaussian initial conditions of the local kind for a large variety of triangular configurations and compare them with predictions from Eulerian Perturbation Theory up to one-loop corrections. We find that the effects of primordial non-Gaussianity at large scales, when compared to Perturbation Theory, are well described by the initial component of the matter bispectrum, linearly extrapolated at the redshift of interest. In addition, we find that, for f_NL=100, the nonlinear corrections due to non-Gaussian initial conditions are of the order of ~3, 4% for generic triangles up to ~20% for squeezed configurations, at any redshift. We show that the predictions of Perturbation Theory at tree-level fail to describe the simulation results at redshift z=0 already at scales corresponding to k ~ 0.02 - 0.08 h/Mpc, depending on the triangle, while one-loop corrections can significantly extend their validity to smaller scales. At higher redshift, one-loop Perturbation Theory provides indeed quite accurate predictions, particularly with respect to the relative correction due to primordial non-Gaussianity.
description: 17 pages, 7 figures. Revised to match journal version with updated references. Accepted for publication in MNRAS.
Calculation of two-loop beta-function for general N=1 supersymmetric Yang--Mills theory with the higher covariant derivative regularization
Creators: name: Pimenov, A. B.
name: Shevtsova, E. S.
name: Stepanyantz, K. V.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: For the general renormalizable N=1 supersymmetric Yang--Mills theory, regularized by higher covariant derivatives, a two-loop beta-function is calculated. It is shown that all integrals, needed for obtaining this function, can be easily calculated, because they are integrals of total derivatives.
description: 9 pages, no figures, some references added
Measuring the Spin of GRS 1915+105 with Relativistic Disk Reflection
Creators: name: Blum, J. L.
name: Miller, J. M.
name: Fabian, A. C.
name: Miller, M. C.
name: Homan, J.
name: van der Klis, M.
name: Cackett, E. M.
name: Reis, R. C.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: GRS 1915+105 harbors one of the most massive known stellar black holes in the Galaxy. In May 2007, we observed GRS 1915+105 for 117 ksec in the low/hard state using Suzaku. We collected and analyzed the data with the HXD/PIN and XIS cameras spanning the energy range from 2.3-55 keV. Fits to the spectra with simple models reveal strong disk reflection through an Fe K emission line and a Compton back-scattering hump. We report constraints on the spin parameter of the black hole in GRS 1915+105 using relativistic disk reflection models. The model for the soft X-ray spectrum (i.e. < 10 keV) suggests a/M = 0.56(2) and excludes zero spin at the 4 sigma level of confidence. The model for the full broadband spectrum suggests that the spin may be higher, a/M = 0.98(1) (1 sigma confidence), and again excludes zero spin at the 2 sigma level of confidence. We discuss these results in the context of other spin constraints and inner disk studies in GRS 1915+105.
description: Accepted for publication in ApJ
Additional file 10 of Identification of biomarkers and therapeutic targets related to Sepsis-associated encephalopathy in rats by quantitative proteomics
Creators: name: Yang, Miaoxian
name: He, Yu
name: Xin, Yuewen
name: Jiang, Junliang
name: Tian, Mi
name: Tan, Jiaying
name: Deng, Shuixiang
name: Gong, Ye
Publisher: name: figshare
Year: 2023
Subjects: subject: Biophysics
subject: Biochemistry
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Neuroscience
subject: Physiology
subject: Pharmacology
subject: Chemical Sciences not elsewhere classified
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified

description: Additional file 10. Full-length blots of ApoA1.
title: Ð£Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð´ÐµÐ±Ð¸ÑÐ¾ÑÑÐºÐ¾Ð¹ Ð·Ð°Ð´Ð¾Ð»Ð¶ÐµÐ½Ð½Ð¾ÑÑÑÑ Ð² ÑÐ¸ÑÑÐµÐ¼Ðµ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð³Ð¾ Ð¼ÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½ÑÐ° 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Ð²Ð°Ð½Ð¾Ð²Ð°, ÐÐ½Ð°ÑÑÐ°ÑÐ¸Ñ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: Ð°Ð½Ð°Ð»Ð¸Ð· Ð´ÐµÐ±Ð¸ÑÐ¾ÑÑÐºÐ¾Ð¹ Ð·Ð°Ð´Ð¾Ð»Ð¶ÐµÐ½Ð½Ð¾ÑÑÐ¸
ÑÑÑÐ½Ð¾ÑÑÑ Ð´ÐµÐ±Ð¸ÑÐ¾ÑÑÐºÐ¾Ð¹ Ð·Ð°Ð´Ð¾Ð»Ð¶ÐµÐ½Ð½Ð¾ÑÑÐ¸
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description: Ð¦ÐµÐ»ÑÑ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ðµ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð´ÐµÐ±Ð¸ÑÐ¾ÑÑÐºÐ¾Ð¹ Ð·Ð°Ð´Ð¾Ð»Ð¶ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐ Â«Ð§ÑÐ²Ð°ÑÑÐºÐ°Ñ Ð°Ð²ÑÐ¾ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ½Ð°Ñ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸ÑÂ»).
ÐÐ»Ñ Ð´Ð¾ÑÑÐ¸Ð¶ÐµÐ½Ð¸Ñ ÑÐµÐ»ÐµÐ¹ Ð¸Ð·ÑÑÐµÐ½Ñ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¾ÑÐ½Ð¾Ð²Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð´ÐµÐ±Ð¸ÑÐ¾ÑÑÐºÐ¾Ð¹ Ð·Ð°Ð´Ð¾Ð»Ð¶ÐµÐ½Ð½Ð¾ÑÑÐ¸, ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð° Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾-ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ°Ñ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ° ÐÐ Â«Ð§ÑÐ²Ð°ÑÑÐºÐ°Ñ Ð°Ð²ÑÐ¾ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ½Ð°Ñ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸ÑÂ», Ð¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð´ÐµÐ±Ð¸ÑÐ¾ÑÑÐºÐ¾Ð¹ Ð·Ð°Ð´Ð¾Ð»Ð¶ÐµÐ½Ð½Ð¾ÑÑÐ¸ ÐÐ Â«Ð§ÐÐÂ» Ð¸ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ñ Ð¼ÐµÑÐ¾Ð´Ñ Ð¿Ð¾ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð´ÐµÐ±Ð¸ÑÐ¾ÑÑÐºÐ¾Ð¹ Ð·Ð°Ð´Ð¾Ð»Ð¶ÐµÐ½Ð½Ð¾ÑÑÑÑ. Ð ÐºÐ°ÑÐµÑÑÐ²Ðµ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¾ÑÐ½Ð¾Ð² ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð´ÐµÐ±Ð¸ÑÐ¾ÑÑÐºÐ¾Ð¹ Ð·Ð°Ð´Ð¾Ð»Ð¶ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð±ÑÐ»Ð¸ ÑÐ°ÑÐºÑÑÑÑ Ð¿Ð¾Ð½ÑÑÐ¸Ðµ, ÑÑÑÐ½Ð¾ÑÑÑ Ð´ÐµÐ±Ð¸ÑÐ¾ÑÑÐºÐ¾Ð¹ Ð·Ð°Ð´Ð¾Ð»Ð¶ÐµÐ½Ð½Ð¾ÑÑÐ¸, Ð° ÑÐ°ÐºÐ¶Ðµ ÑÑÐ±ÑÐµÐºÑÑ Ð¸ Ð¼ÐµÑÐ¾Ð´Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð´ÐµÐ±Ð¸ÑÐ¾ÑÑÐºÐ¾Ð¹ Ð·Ð°Ð´Ð¾Ð»Ð¶ÐµÐ½Ð½Ð¾ÑÑÑÑ Ð² ÑÐ¸ÑÑÐµÐ¼Ðµ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð³Ð¾ Ð¼ÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½ÑÐ° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ.
ÐÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð½ÑÐµ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð½Ð° ÑÐ»ÑÑÑÐµÐ½Ð¸Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð´ÐµÐ±Ð¸ÑÐ¾ÑÑÐºÐ¾Ð¹ Ð·Ð°Ð´Ð¾Ð»Ð¶ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ñ Ð½Ð° ÑÐ¼ÐµÐ½ÑÑÐµÐ½Ð¸Ðµ Ð¿ÑÐ¾ÑÑÐ¾ÑÐµÐ½Ð½Ð¾Ð¹ Ð·Ð°Ð´Ð¾Ð»Ð¶ÐµÐ½Ð½Ð¾ÑÑÐ¸.
Milky Way vs Andromeda: a tale of two disks
Creators: name: Yin, J.
name: Hou, J. L.
name: Prantzos, N.
name: Boissier, S.
name: Chang, R. X.
name: Shen, S. Y.
name: Zhangh, B.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We study the chemical evolution of the disks of the Milky Way (MW) and of Andromeda (M31), in order to reveal common points and differences between the two major galaxies of the Local group. We use a large set of observational data for M31, including recent observations of the Star Formation Rate (SFR) and gas profiles, as well as stellar metallicity distributions along its disk. We show that, when expressed in terms of the corresponding disk scale lengths, the observed radial profiles of MW and M31 exhibit interesting similarities, suggesting the possibility of a description within a common framework. We find that the profiles of stars, gas fraction and metallicity of the two galaxies, as well as most of their global properties, are well described by our model, provided the star formation efficiency in M31 disk is twice as large as in the MW. We show that the star formation rate profile of M31 cannot be fitted with any form of the Kennicutt-Schmidt law (KS Law) for star formation. We attribute those discrepancies to the fact that M31 has undergone a more active star formation history, even in the recent past, as suggested by observations of a "head-on" collision with the neighboring M32 galaxy about 200 Myr ago. The MW has most probably undergone a quiescent secular evolution, making possible a fairly successful description with a simple model. If M31 is more typical of spiral galaxies, as recently suggested by Hammer et al. (2007), more complex models, involving galaxy interactions, will be required for the description of spirals.
description: 13 Pages, 7 figures, 2 tables, accepted for publication in Astronomy and Astrophysics
The Hot and Cold Spots in Five-Year WMAP Data
Creators: name: Hou, Zhen
name: Banday, A. J.
name: Gorski, K. M.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We present an extensive frequentist analysis of the one-point statistics (number, mean, variance, skewness and kurtosis) and two-point correlation functions determined for the local extrema of the cosmic microwave background temperature field observed in five-years of Wilkinson Microwave Anisotropy Probe (WMAP) data. Application of a hypothesis test on the one-point statistics indicates a low-variance of hot and cold spots in all frequency bands of the WMAP data. The consistency of the observations with Gaussian simulations of the the best-fitting cosmological model is rejected at the 95% C.L. outside the WMAP KQ75 mask and the northern hemispheres in the Galactic and ecliptic coordinate frames. We demonstrate that it is unlikely that residual Galactic foreground emission contributes to the observed non-Gaussianities. However, the application of a high-pass filter that removes large angular scale power does improve the consistency with the best-fitting cosmological model. Two-point correlation functions of the local extrema are calculated for both the temperature pair product (T-T) and spatial pair-counting (P-P). The T-T observations demonstrate weak correlation on scales below 20 degree and lie completely below the lower 3-sigma confidence region once various temperature thresholds are applied to the extrema determined for the KQ75 mask and northern sky partitions. The P-P correlation structure corresponds to the clustering properties of the temperature extrema, and provides evidence that it is the large angular-scale structures, and some unusual properties thereof, that are intimately connected to the properties of the hot and cold-spots observed in the WMAP five-year data.
description: 15 pages, 6 figures, 8 tables, accepted for publication in MNRAS
Born-Oppenheimer approximation for open quantum systems within the quantum trajectory approach
Creators: name: Huang, X. L.
name: Wu, S. L.
name: Wang, L. C.
name: Yi, X. X.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Based on the quantum trajectory approach, we extend the Born-Oppenheimer (BO) approximation from closed quantum system to open quantum system, where the open quantum system is described by a master equation in Lindblad form. The BO approximation is defined and the validity condition is derived. We find that the dissipation in fast variables benefits the BO approximation that is different from the dissipation in slow variables. A detailed comparison between this extension and our previous approximation (that is based on the effective Hamiltonian approach, see X. L. Huang and X. X. Yi, Phys. Rev. A 80, 032108 (2009)) is presented. Several new features and advantages are analyzed, which show that the two approximations are complementary to each other. Two examples are taken to illustrate our method.
description: 7 pages, 5 figures. Accepted by Phys. Rev. A
title: ÐÐ°Ð·Ð¾Ð¿ÐµÑÐµÐºÐ°ÑÐ¸Ð²Ð°ÑÑÐ¸Ð¹ Ð°Ð³ÑÐµÐ³Ð°Ñ âÐÐ°Ð´Ð¾Ð³Ð° - 32â
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ÐµÑ, ÐÐ°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: 2018
Subjects: Ð³Ð°Ð·Ð¾Ð²Ð°Ñ ÑÑÑÐ±Ð¸Ð½Ð°
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description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½ ÑÐ°ÑÑÐµÑ Ð³Ð°Ð·Ð¾ÑÑÑÐ±Ð¸Ð½Ð½Ð¾Ð¹ ÑÑÑÐ°Ð½Ð¾Ð²ÐºÐ¸ Ð¼Ð¾ÑÐ½Ð¾ÑÑÑÑ 32 ÐÐÑ, Ð²ÑÐ¾Ð´ÑÑÐµÐ¹ Ð² ÑÐ¾ÑÑÐ°Ð² Ð³Ð°Ð·Ð¾Ð¿ÐµÑÐµÐºÐ°ÑÐ¸Ð²Ð°ÑÑÐµÐ³Ð¾ Ð°Ð³ÑÐµÐ³Ð°ÑÐ° "ÐÐ°Ð´Ð¾Ð³Ð° - 32". ÐÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ Ð²ÑÑÐ¸ÑÐ»ÐµÐ½Ð¸Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÑ ÑÐ°ÑÑÐµÐ¹ Ð³Ð°Ð·Ð¾ÑÑÑÐ±Ð¸Ð½Ð½Ð¾Ð¹ ÑÑÑÐ°Ð½Ð¾Ð²ÐºÐ¸: ÑÑÑÐ±Ð¸Ð½Ñ Ð¸ ÐºÐ¾Ð¼Ð¿ÑÐµÑÑÐ¾ÑÐ°. ÐÐ¾Ð»ÐµÐµ Ð¿Ð¾Ð´ÑÐ¾Ð±Ð½Ð¾ Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÐ½Ñ ÑÐ°ÑÑÐµÑÑ: ÑÐµÐ¿Ð»Ð¾Ð²Ð¾Ð¹ ÑÑÐµÐ¼Ñ ÐÐ¢Ð£, Ð¿ÑÐ¸Ð±Ð»Ð¸Ð¶ÐµÐ½Ð½ÑÐ¹ ÑÐ°ÑÑÐµÑ Ð¾ÑÐµÐ²Ð¾Ð³Ð¾ ÐºÐ¾Ð¼Ð¿ÑÐµÑÑÐ¾ÑÐ°, Ð³Ð°Ð·Ð¾Ð´Ð¸Ð½Ð°Ð¼Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ°ÑÑÐµÑ Ð³Ð°Ð·Ð¾Ð²Ð¾Ð¹ ÑÑÑÐ±Ð¸Ð½Ñ, ÑÐ°ÑÑÐµÑ Ð·Ð°ÐºÑÑÑÐºÐ¸ Ð¿Ð¾ÑÐ¾ÐºÐ° Ð¿Ð¾ÑÐ»ÐµÐ´Ð½ÐµÐ¹ ÑÑÑÐ¿ÐµÐ½Ð¸ ÑÐ¸Ð»Ð¾Ð²Ð¾Ð¹ ÑÑÑÐ±Ð¸Ð½Ñ Ð¸ Ð¿ÑÐ¸Ð±Ð»Ð¸Ð¶ÐµÐ½Ð½ÑÐ¹ ÑÐ°ÑÑÐµÑ Ð´Ð¸ÑÑÑÐ·Ð¾ÑÐ°. ÐÑÐ¾Ð²Ð¾Ð´Ð¸ÑÑÑ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ðµ Ð¿ÑÐ¾ÑÐ½Ð¾ÑÑÐ½ÑÑ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸Ðº Ð¾ÑÐ½Ð¾Ð²Ð½ÑÑ ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ¾Ð² ÑÐ²Ð¾Ð±Ð¾Ð´Ð½Ð¾Ð¹ ÑÑÑÐ±Ð¸Ð½Ñ, ÑÐµÐ¼Ñ ÑÐ´ÐµÐ»ÑÐµÑÑÑ Ð¾ÑÐ¾Ð±Ð¾Ðµ Ð²Ð½Ð¸Ð¼Ð°Ð½Ð¸Ðµ. Ð¡Ð¾ÑÑÐ°Ð²Ð»ÐµÐ½Ð¾ Ð¿Ð¾Ð»Ð½Ð¾Ðµ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð²Ð½Ð¾Ðµ Ð¾Ð¿Ð¸ÑÐ°Ð½Ð¸Ðµ ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ¾Ð² Ð³Ð°Ð·Ð¾ÑÑÑÐ±Ð¸Ð½Ð½Ð¾Ð¹ ÑÑÑÐ°Ð½Ð¾Ð²ÐºÐ¸, Ð¿ÑÐ¸Ð½ÑÐ¸Ð¿Ð° Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¸Ñ. ÐÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½ Ð¿ÑÐ¾Ð´Ð¾Ð»ÑÐ½ÑÐ¹ ÑÐ°Ð·ÑÐµÐ· ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÐµÐ¼Ð¾Ð¹ ÑÑÑÐ°Ð½Ð¾Ð²ÐºÐ¸.
Holographic description of quantum field theory
Creators: name: Lee, Sung-Sik
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We propose that general D-dimensional quantum field theories are dual to (D+1)-dimensional local quantum theories which in general include objects with spin two or higher. Using a general prescription, we construct a (D+1)-dimensional theory which is holographically dual to the D-dimensional O(N) vector model. From the holographic theory, the phase transition and critical properties of the model in dimensions D>2 are described.
description: 23 pages, 1 figure; v2) references added; appendix expanded
Cardiovascular risk profles clusters among children and adolescents with disabilities
Creators: name: Bar Yehuda, Maayan
name: Barak, Sharon
name: Hutzler, Yeshayahu
name: NG, KWOK
name: Giladi, Ariela
name: Bar Meir, Lilach
name: Marques, Adilson
name: Zigdon, Avi
name: Zwilling, Moti
name: Reges, Orna
name: Harel-Fisch, Yossi
name: Tesler, Riki
Publisher: name: University of Limerick
Year: 2023
Subjects: subject: Physical sciences
subject: FOS: Physical sciences
subject: Health sciences
subject: FOS: Health sciences

description: Background Cardiovascular diseases (CVD) are a precursor for disabilities and death worldwide. Being overweight or obese in combination with physical inactivity and smoking habits may increase the risk for CVD and other health problems such as lower limb osteoarthritis, diabetes, stroke, and various cancer types among children and adolescents. The literature emphasizes the need to follow such groups and evaluate the risk of individuals developing CVD diseases. Therefore, the current study explores the variety of cardiovascular risks in children and adolescents’ profles clusters with and without disabilities. Methods Data from 42 countries including Israel, was collected with the support of the world health organization (WHO, Europe) through a questionnaire from 11–19 years old school-aged. Results The study fnding shows that children and adolescents with disabilities demonstrated a higher prevalence of overweight than those who completed the HBSC youth behavior survey. Moreover, the prevalence of tobacco smoking and alcohol use was statisticaly signifcantly higher among the disabled group than the non-disabled group. In addition, socioeconomic status of responders who presented a very high CVD risk was found as signifcantly lower than those from the frst and second low risk groups. Conclusion This led to the conclusion that children and adolescents with disability were at a higher risk of developing CVDs than their non-disabled peers. In addition, intervention programs tailored to the needs of adolescents with disability should consider lifestyle habit change and promoting healthy living thus improving their quality of life as well as reducing their risk of being exposed to severe CVD diseases.
title: Ð ÐµÐºÑÐµÐ°ÑÐ¸Ð¾Ð½Ð½ÑÐµ Ð·Ð¾Ð½Ñ Ð½Ð° ÑÐµÑÑÐ¸ÑÐ¾ÑÐ¸ÑÑ ÑÑÐ°ÑÐ¾Ð¹ Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½Ð¾Ð¹ Ð·Ð°ÑÑÑÐ¾Ð¹ÐºÐ¸
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±Ð»Ð¾Ð½ÑÐºÐ°Ñ, ÐÐ»ÑÐ³Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: ÐÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½ÑÐµ ÑÐµÑÑÐ¸ÑÐ¾ÑÐ¸Ð¸
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description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÐµÑÑÑ Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ° ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ Ð½Ð° Ð¼ÐµÑÑÐµ Ð¿Ð¾Ð»Ð½Ð¾ÑÑÑÑ Ð¸Ð»Ð¸ ÑÐ°ÑÑÐ¸ÑÐ½Ð¾ Ð·Ð°Ð±ÑÐ¾ÑÐµÐ½Ð½ÑÑ Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½ÑÑ ÑÐµÑÑÐ¸ÑÐ¾ÑÐ¸Ð¹ Ð¿ÑÐ¾ÑÐ²ÐµÑÐ¸ÑÐµÐ»ÑÐ½Ð¾-ÑÐµÐºÑÐµÐ°ÑÐ¸Ð¾Ð½Ð½ÑÑ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ¾Ð², Ð¸Ð·ÑÑÐ°ÐµÑÑÑ ÑÐ¾ÑÑÐ¸Ð¹ÑÐºÐ¸Ð¹ Ð¸ Ð·Ð°ÑÑÐ±ÐµÐ¶Ð½ÑÐ¹ Ð¾Ð¿ÑÑ ÑÐµÐ¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¿ÑÐ¾Ð¼ÑÑÐ»ÐµÐ½Ð½ÑÑ ÑÐµÑÑÐ¸ÑÐ¾ÑÐ¸Ð¹. ÐÐ¾ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ°Ð¼ ÑÐ°Ð±Ð¾ÑÑ Ð±ÑÐ»Ð° Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð° Ð°Ð¿ÑÐ¾Ð±Ð°ÑÐ¸Ñ Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ¸ Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ Ð¾ÑÐ°Ð½Ð¶ÐµÑÐµÐ¸ Ð´Ð»Ñ ÑÑÐ¾Ð¿Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ°ÑÑÐµÐ½Ð¸Ð¹ Ð½Ð° ÑÐµÑÑÐ¸ÑÐ¾ÑÐ¸Ð¸ Ð·Ð°Ð²Ð¾Ð´Ð° ÐÑÐ°ÑÐ½ÑÐ¹ Ð¢ÑÐµÑÐ³Ð¾Ð»ÑÐ½Ð¸Ðº Ð² Ð³Ð¾ÑÐ¾Ð´Ðµ Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³Ðµ.
Close supermassive binary black holes
Creators: name: Gaskell, C. Martin
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: It has been proposed that when the peaks of the broad emission lines in active galactic nuclei (AGNs) are significantly blueshifted or redshifted from the systemic velocity of the host galaxy, this could be a consequence of orbital motion of a supermassive blackhole binary (SMB) (Gaskell 1983). The AGN J1536+0441 (=SDSS J153636.22+044127.0) has recently been proposed as an example of this phenomenon (Boroson & Lauer 2009). It is proposed here instead that 1536+044 is an example of line emission from a disc. If this is correct, the lack of clear optical spectral evidence for close SMBs is significant and argues either that the merging of close SMBs is much faster than has generally been hitherto thought, or if the approach is slow, that when the separation of the binary is comparable to the size of the torus and broad-line region, the feeding of the black holes is disrupted.
description: Nature in press. 4 pages, 1 figure [Title, abstract, text, and references shortened to conform to journal requirements]
Electric Dipole Moments of Charged Leptons from Their Majorana-type Yukawa Couplings
Creators: name: Liao, Yi
Publisher: name: arXiv
Year: 2008
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The electric dipole moments (EDMs) of charged leptons are significantly suppressed in standard model. It has been found previously that they are even more severely suppressed in seesaw type models by powers of tiny neutrino masses as far as a leptonic CP source is concerned. We investigate whether a Majorana-type Yukawa coupling between charged leptons and a doubly charged scalar can contribute significantly to their EDMs. An observable EDM would then help unravel the Majorana nature of neutrinos by a lepton number conserving quantity. We find that the EDMs are indeed parametrically large, of the form d_α\propto em_α(m^2_β-m^2_γ)/m^4 up to logarithms, where m_αand m are respectively the masses of charged leptons and the scalar. And they satisfy a sum rule to good precision, d_e/m_e+d_μ/m_μ+d_τ/m_τ=0. With the most stringent constraints from lepton flavor violating transitions taken into account, their values are still much larger than the mentioned previous results. Unfortunately, even in the most optimistic case the electron EDM is about three orders of magnitude below the foreseeable experimental sensitivity.
description: 13 pages, 1 figure, 1 table; v2: corrected typos in eqs. (9,15), no other changes, to appear in PLB
title: ÐÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð°Ñ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ Ð¸Ð½ÑÐµÐ³ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð¹ ÑÑÐµÐ´Ñ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð² Ð±ÑÐ°ÑÐ·ÐµÑÐµ
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ°Ð¿ÐºÐ¾Ð²ÑÐºÐ¸Ð¹, ÐÐ²Ð³ÐµÐ½Ð¸Ð¹
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: Ð¸Ð½ÑÐµÐ³ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½Ð°Ñ ÑÑÐµÐ´Ð°
web-ÑÐ°Ð¹ÑÐ°
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description: ÐÐ¸Ð¿Ð»Ð¾Ð¼Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° ÑÐ¾Ð´ÐµÑÐ¶Ð¸Ñ: 67 ÑÑÑÐ°Ð½Ð¸Ñ, 16 Ð¸Ð»Ð»ÑÑÑÑÐ°ÑÐ¸Ð¹. ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ° ÑÐ²Ð»ÑÐµÑÑÑ Ð¸Ð½ÑÐµÐ³ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½Ð°Ñ ÑÑÐµÐ´Ð° ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð² Ð±ÑÐ°ÑÐ·ÐµÑÐµ. Ð ÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¾Ð¼ Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²ÐºÐ° Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° web-ÑÐ°Ð¹ÑÐ°, Ð¿Ð¾Ð·Ð²Ð¾Ð»ÑÑÑÐµÐ³Ð¾ ÑÐ¾Ð·Ð´Ð°Ð²Ð°ÑÑ Ð¸ Ð·Ð°Ð¿ÑÑÐºÐ°ÑÑ Ð¿ÑÐ¾ÐµÐºÑÑ, Ð½Ð°Ð¿Ð¸ÑÐ°Ð½Ð½ÑÐµ Ð½Ð° ÑÐ·ÑÐºÐ°Ñ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ: HTML, CSS Ð¸ JavaScript. ÐÑÐ¸ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ð¸ web-Ð¿ÑÐ¸Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ð±ÑÐ»Ð¸ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ: WebStorm - Ð¸Ð½ÑÐµÐ³ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½Ð°Ñ ÑÑÐµÐ´Ð° ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð¾Ñ JetBrains; Node.js - Ð¿Ð»Ð°ÑÑÐ¾ÑÐ¼Ð°, ÐºÐ¾ÑÐ¾ÑÐ°Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·ÑÐµÑÑÑ Ð² ÐºÐ°ÑÐµÑÑÐ²Ðµ web-ÑÐµÑÐ²ÐµÑÐ°; NPM - Ð¼ÐµÐ½ÐµÐ´Ð¶ÐµÑ Ð¿Ð°ÐºÐµÑÐ¾Ð²; ÑÐ·ÑÐº Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ JavaScript 2015; ÑÑÐµÐ¹Ð¼Ð²Ð¾ÑÐº React; Ð¿Ð¾Ð´ÑÐ¾Ð´ Redux; Ð¿Ð°ÑÑÐµÑÐ½ MVC; Ð±Ð°Ð·Ð° Ð´Ð°Ð½Ð½ÑÑ MongoDB; ÑÐ·ÑÐºÐ¸ ÑÐ°Ð·Ð¼ÐµÑÐºÐ¸ HTML5 Ð¸ CSS3.
Chiral Supergravity
Creators: name: Becker, Melanie
name: Bruillard, Paul
name: Downes, Sean
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We study the linearized approximation of N=1 topologically massive supergravity around AdS3. Linearized gravitino fields are explicitly constructed. For appropriate boundary conditions, the conserved charges demonstrate chiral behavior, so that chiral gravity can be consistently extended to chiral supergravity.
description: 30 pages
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¼ÐµÑÐ¾Ð´Ð¸Ðº ÑÐ°ÑÑÐµÑÐ° Ð¸ Ð¾Ð¿ÑÐ¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ñ ÑÑÐ°Ð½ÑÑÐ¾ÑÐ¼Ð°ÑÐ¾ÑÐ¾Ð² Ð¸Ð½Ð²ÐµÑÑÐ¾ÑÐ½ÑÑ Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ¾Ð² Ð¿Ð¸ÑÐ°Ð½Ð¸Ñ Ð¼Ð°ÑÐ¸Ð½ ÐºÐ¾Ð½ÑÐ°ÐºÑÐ½Ð¾Ð¹ ÑÐ²Ð°ÑÐºÐ¸
title: Ð°Ð²ÑÐ¾ÑÐµÑ. Ð´Ð¸Ñ. â¦ ÐºÐ°Ð½Ð´. ÑÐµÑ Ð½. Ð½Ð°ÑÐº: 05.09.05
titleType: Subtitle
Creators: name: ÐÐ¸ÑÐ°ÑÐµÐ², ÐÐµÐ½Ð¸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¢ÑÐ°Ð½ÑÑÐ¾ÑÐ¼Ð°ÑÐ¾ÑÑ
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A Massive swelling of Neck mimicking parotid tumor
Creators: name: Chaurasia, Akhilanand
Publisher: name: EURORAD
Year: 2014
Subjects: subject: Head and neck
subject: CT
subject: Diagnostic procedure
subject: Lymphoma

description: Clinical History Image Findings Discussion Find Diagnosis Differential Diagnosis
description: male, 48 years
description: Clinical History: A 48-year-old male patient complaint of a swelling on the left side of the face since 3 years. It was progressively increasing in size. The swelling was approximately 20x20 cm in size, firm to hard, non tender and non fluctuant extending from the left par... Final Diagnosis: Hodgkin's Lymphoma
title: ÐÑÐ»ÑÑÐ¸Ð¿Ð»ÐµÐºÑÐ½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· Ð°Ð»ÑÑÐ°-2-Ð¼Ð°ÐºÑÐ¾Ð³Ð»Ð¾Ð±ÑÐ»Ð¸Ð½Ð°, ÑÐµÑÑÐ¸Ð½Ð° Ð Ð¸ ÑÑÐ²Ð¾ÑÐ¾ÑÐ¾ÑÐ½Ð¾Ð³Ð¾ Ð°Ð¼Ð¸Ð»Ð¾Ð¸Ð´Ð° Ð1 ÐºÐ°Ðº ÑÐ°ÐºÑÐ¾ÑÐ¾Ð² Ð²Ð¾ÑÐ¿Ð°Ð»ÐµÐ½Ð¸Ñ Ð² ÑÑÐ²Ð¾ÑÐ¾ÑÐºÐµ ÐºÑÐ¾Ð²Ð¸ Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ Ð½Ð¾Ð²ÑÑ Ð¼Ð°ÑÑ-ÑÐ¿ÐµÐºÑÑÐ¾Ð¼ÐµÑÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¿Ð¾Ð´Ñ Ð¾Ð´Ð¾Ð²
title: ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÑ 03.01.03 "ÐÐ¾Ð»ÐµÐºÑÐ»ÑÑÐ½Ð°Ñ Ð±Ð¸Ð¾Ð»Ð¾Ð³Ð¸Ñ"
titleType: Subtitle
Creators: name: Ð¢Ð°ÑÐ°ÑÐºÐ¸Ð½, ÐÐ»ÐµÐºÑÐ°Ð½Ð´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: 2021
Subjects: ÐÐ¾Ð»ÐµÐºÑÐ»ÑÑÐ½Ð°Ñ Ð±Ð¸Ð¾Ð»Ð¾Ð³Ð¸Ñ
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Evidence for intermediate-age stellar populations in early-type galaxies from K-band spectroscopy
Creators: name: Mármol-Queraltó, E.
name: Cardiel, N.
name: Sánchez-Blázquez, P.
name: Trager, S. C.
name: Peletier, R. F.
name: Kuntschner, H.
name: Silva, D. R.
name: Cenarro, A. J.
name: Vazdekis, A.
name: Gorgas, J.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: The study of stellar populations in early-type galaxies in different environments is a powerful tool for constraining their star formation histories. This study has been traditionally restricted to the optical range, where dwarfs around the turn-off and stars at the base of the RGB dominate the integrated light at all ages. The near-infrared spectral range is especially interesting since in the presence of an intermediate-age population, AGB stars are the main contributors. In this letter, we measure the near-infrared indices NaI and D$_{\rm CO}$ for a sample of 12 early-type galaxies in low density environments and compare them with the Fornax galaxy sample presented by Silva et al. (2008). The analysis of these indices in combination with Lick/IDS indices in the optical range reveals i) the NaI index is a metallicity indicator as good as C4668 in the optical range, and ii) D$_{\rm CO}$ is a tracer of intermediate-age stellar populations. We find that low-mass galaxies in low density environments show higher NaI and D$_{\rm CO}$ than those located in Fornax cluster, which points towards a late stage of star formation for the galaxies in less dense environments, in agreement with results from other studies using independent methods.
description: 7 pages, 3 figures, accepted for publication in ApJL