cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: ÐÐµÑÐ¾Ð´Ð¸ÐºÐ° Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ ÑÑÐ¾Ð¸Ð¼Ð¾ÑÑÐ¸ Ð¾Ð±ÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð·Ð´Ð°Ð½Ð¸Ð¹ Ð¸ ÑÐ¾Ð¾ÑÑÐ¶ÐµÐ½Ð¸Ð¹ Ð¿Ð¾ ÑÑÑÐ´Ð¾Ð·Ð°ÑÑÐ°ÑÐ°Ð¼
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´Ð°Ñ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: 2016
Subjects: ÐÐ´Ð°Ð½Ð¸Ñ Ð¸ Ð¿Ð¾ÑÑÑÐ¾Ð¹ÐºÐ¸
Ð¡ÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð¾
Ð¡ÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½ÑÐµ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸
ÑÐ¼ÐµÑÐ½Ð°Ñ ÑÑÐ¾Ð¸Ð¼Ð¾ÑÑÑ
estimated cost

description: Ð Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ð¸ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ ÑÑÑÐµÑÑÐ²ÑÑÑÐ¸Ðµ Ð¿Ð¾Ð´ÑÐ¾Ð´Ñ Ðº Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ ÑÑÐ¾Ð¸Ð¼Ð¾ÑÑÐ¸ ÑÐ°Ð±Ð¾Ñ Ð¿Ð¾ Ð¾Ð±ÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ. ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ð¸ Ð¾Ð±Ð·Ð¾ÑÐ° Ð»Ð¸ÑÐµÑÐ°ÑÑÑÐ½ÑÑ Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ¾Ð², Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð¸ ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ñ Ð½Ð¾ÑÐ¼Ð°ÑÐ¸Ð²Ð¾Ð² Ð¿Ð¾ ÑÐµÐ½Ð¾Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð² Ð¾Ð±Ð»Ð°ÑÑÐ¸ ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¾Ð±ÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð²ÑÑÐ²Ð»ÐµÐ½Ð¾, ÑÑÐ¾ Ð¾ÑÑÑÑÑÑÐ²ÑÐµÑ ÐµÐ´Ð¸Ð½ÑÐ¹ Ð¿Ð¾Ð´ÑÐ¾Ð´ Ðº Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ ÑÑÐ¾Ð¸Ð¼Ð¾ÑÑÐ¸ ÑÐ°Ð±Ð¾Ñ. ÐÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½ Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½ Ð¿Ð¾Ð´ÑÐ¾Ð´ Ðº Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ ÑÑÐ¾Ð¸Ð¼Ð¾ÑÑÐ¸ Ð¾Ð±ÑÐ»ÐµÐ´Ð¾Ð²Ð°ÑÐµÐ»ÑÑÐºÐ¸Ñ ÑÐ°Ð±Ð¾Ñ Ð¿Ð¾ ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ð¼ ÑÑÑÐ´Ð¾Ð·Ð°ÑÑÐ°ÑÐ°Ð¼. ÐÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð° ÑÑÐ¾Ð¸Ð¼Ð¾ÑÑÑ ÑÐ°Ð±Ð¾Ñ Ð¿Ð¾ Ð²Ð¸Ð·ÑÐ°Ð»ÑÐ½Ð¾Ð¼Ñ Ð¾Ð±ÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÐ¼Ð¸ ÑÐ¿Ð¾ÑÐ¾Ð±Ð°Ð¼Ð¸: Ð¿Ð¾ ÑÑÑÐ´Ð¾Ð·Ð°ÑÑÐ°ÑÐ°Ð¼ Ð¸ ÑÐ±Ð¾ÑÐ½Ð¸ÐºÐ°Ð¼ Ð±Ð°Ð·Ð¾Ð²ÑÑ ÑÐµÐ½. Ð¡Ð´ÐµÐ»Ð°Ð½Ñ Ð²ÑÐ²Ð¾Ð´Ñ Ð¾ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ð¸ Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ¸ ÑÐ°ÑÑÑÑÐ° ÑÑÐ¾Ð¸Ð¼Ð¾ÑÑÐ¸ Ð¿Ð¾ Ð·Ð°ÑÑÐ°ÑÐ°Ð¼ ÑÑÑÐ´Ð° Ð¸ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½ÑÑ Ð¿ÑÑÑÑ ÐµÑ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ.
description: In the thesis the existing approaches to determination of cost of works on inspection are considered. On the basis of the review of references, the analysis and comparison of standards for pricing in the field of technical inspection it is revealed that there is no uniform approach to determination of cost of works. Approach to determination the cost of inspection on the actual labor costs is offered and developed. The cost of works on visual inspection is determined in various ways: on engineering man-hours and collections of the base prices. Conclusions are drawn on application of a method of calculation of cost on expenses of work and possible ways of its application.
title: ÐÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¸Ð½ÑÐµÑÐ°ÐºÑÐ¸Ð²Ð½ÑÑ Ð²ÐµÐ±-Ð¸Ð½ÑÐµÑÑÐµÐ¹ÑÐ¾Ð² Ð´Ð»Ñ Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ Ð½Ð¾ÑÐ½Ð¾Ð¹ Ð³ÑÐ°Ð¼Ð¾ÑÐµ
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¼Ð°Ð³Ð¸ÑÑÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¾ÑÐµÐ½Ð¾, Ð Ð°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Ð½ÑÐµÑÑÐµÐ¹ÑÑ
ÐÐ½ÑÐµÑÐ½ÐµÑ
Ð²ÐµÐ±-ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ°
ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ðµ Ð²ÐµÐ±-ÑÐ°Ð¹ÑÐ°
Ð¾Ð½Ð»Ð°Ð¹Ð½-Ð¾Ð±ÑÑÐµÐ½Ð¸Ðµ
ÑÐµÐ¾ÑÐ¸Ñ Ð¼ÑÐ·ÑÐºÐ¸

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ° Ð´Ð»Ñ Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ Ð½Ð¾ÑÐ½Ð¾Ð¹ Ð³ÑÐ°Ð¼Ð¾ÑÐµ Ð¸ ÑÐµÐ¾ÑÐ¸Ð¸ Ð¼ÑÐ·ÑÐºÐ¸. Ð ÑÐ¾Ð´Ðµ ÑÐ°Ð±Ð¾ÑÑ Ð½Ð°Ð´ Ð¿ÑÐ¾ÐµÐºÑÐ¾Ð¼ Ð±ÑÐ»Ð¾ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¾ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¿Ð¾Ð´ÑÐ¾Ð´Ð¾Ð² Ðº Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ ÑÐµÐ¾ÑÐ¸Ð¸ Ð¼ÑÐ·ÑÐºÐ¸. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° ÑÑÐµÐ¼Ð° Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ, Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ ÐºÐ¾ÑÐ¾ÑÐ¾Ð¹ Ð±ÑÐ»Ð¸ ÑÐ¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÑÑÑÑÐºÑÑÑÐ½ÑÐµ ÑÐ»ÐµÐ¼ÐµÐ½ÑÑ Ð²ÐµÐ±-ÑÐµÑÑÑÑÐ° Ð¸ Ð½Ð°Ð²Ð¸Ð³Ð°ÑÐ¸Ñ. Ð¡Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½ Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½ Ð¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°ÑÐµÐ»ÑÑÐºÐ¸Ð¹ Ð¸Ð½ÑÐµÑÑÐµÐ¹Ñ Ð¸ Ð²ÐµÐ±-ÑÐ°Ð¹Ñ Ñ Ð°Ð´Ð¼Ð¸Ð½Ð¸ÑÑÑÐ°ÑÐ¸Ð²Ð½Ð¾Ð¹ Ð¿Ð°Ð½ÐµÐ»ÑÑ Ð´Ð»Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¸ Ð¼Ð¾Ð´ÐµÑÐ°ÑÐ¸Ð¸ ÑÐ°Ð¹ÑÐ°. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð¾Ð¿ÑÐ¾Ñ ÑÑÐµÐ´Ð¸ ÑÐµÑÑÐ¾Ð²ÑÑ Ð¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°ÑÐµÐ»ÐµÐ¹, Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ ÐºÐ¾ÑÐ¾ÑÐ¾Ð³Ð¾ ÑÐ´ÐµÐ»Ð°Ð½Ñ Ð²ÑÐ²Ð¾Ð´Ñ Ð¾Ð± ÑÑÐ¿ÐµÑÐ½Ð¾ÑÑÐ¸ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð²ÑÐ²Ð¾Ð´Ð¾Ð².
Approximation of elements in henselizations
Creators: name: Kuhlmann, Franz-Viktor
Publisher: name: arXiv
Year: 2010
Subjects: subject: Commutative Algebra (math.AC)
subject: FOS: Mathematics
subject: 12J20 (Primary), 12J10 (Secondary)

description: For valued fields $K$ of rank higher than 1, we describe how elements in the henselization $K^h$ of $K$ can be approximated from within $K$; our result is a handy generalization of the well-known fact that in rank 1, all of these elements lie in the completion of $K$. We apply the result to show that if an element $z$ algebraic over $K$ can be approximated from within $K$ in the same way as an element in $K^h$, then $K(z)$ is not linearly disjoint from $K^h$ over $K$.
description: 13 pages
title: ÐÑÐ½Ð¾Ð²Ð½ÑÐµ Ð¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ ÑÐµÐ¾ÑÐ¸Ð¸ Ð»Ð¸Ð½Ð³Ð²Ð¾-ÐºÐ¾Ð¼Ð±Ð¸Ð½Ð°ÑÐ¾ÑÐ½Ð¾Ð³Ð¾ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð. Ð. ÐÐ³Ð½Ð°ÑÑÐµÐ²Ð°
title: Basic provisions of M. B. Ignatievâs linguo-combinatory modeling theory
Creators: name: ÐÐ°ÑÐµÑÐ¼Ð¸Ð½Ð°, Ð¢Ð°ÑÑÑÐ½Ð°
name: "Ð¡Ð¸ÑÑÐµÐ¼Ð½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· Ð² Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ð¸ Ð¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ð¸", Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½Ð°Ñ Ð½Ð°ÑÑÐ½Ð°Ñ Ð¸ ÑÑÐµÐ±Ð½Ð¾-Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ°Ñ ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ñ (24; 2020; Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³)
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2020
Subjects: Ð¡Ð»Ð¾Ð¶Ð½ÑÐµ ÑÐ¸ÑÑÐµÐ¼Ñ
Ð»Ð¸Ð½Ð³Ð²Ð¾-ÐºÐ¾Ð¼Ð±Ð¸Ð½Ð°ÑÐ¾ÑÐ½Ð¾Ðµ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
Ð¸Ð·Ð±ÑÑÐ¾ÑÐ½Ð¾ÑÑÑ

description: Ð¡ÑÐ°ÑÑÑ Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° Ð¾ÑÐ½Ð¾Ð²Ð°Ð¼ ÑÐµÐ¾ÑÐ¸Ð¸ Ð»Ð¸Ð½Ð³Ð²Ð¾-ÐºÐ¾Ð¼Ð±Ð¸Ð½Ð°ÑÐ¾ÑÐ½Ð¾Ð³Ð¾ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ, Ð¼ÐµÑÐ¾Ð´Ð° Ð¸Ð·Ð±ÑÑÐ¾ÑÐ½ÑÑ Ð¿ÐµÑÐµÐ¼ÐµÐ½Ð½ÑÑ Ð¿ÑÐ¾ÑÐµÑÑÐ¾ÑÐ° ÐÐ¸ÑÐ°Ð¸Ð»Ð° ÐÐ¾ÑÐ¸ÑÐ¾Ð²Ð¸ÑÐ° ÐÐ³Ð½Ð°ÑÑÐµÐ²Ð°, ÑÑÐµÐ´ÑÐµÐ³Ð¾ Ð¸Ð· Ð¶Ð¸Ð·Ð½Ð¸ Ð² 2019 Ð³Ð¾Ð´Ñ.
description: The article is devoted to the basics of the theory of linguo-combinatorial modeling, the method of redundant variables of the professor Michail B. Ignatiev.
Towards Data Redaction in Bitcoin
Creators: name: Botta, Vincenzo
name: Iovino, Vincenzo
name: Visconti, Ivan
Publisher: name: arXiv
Year: 2023
Subjects: subject: Cryptography and Security (cs.CR)
subject: FOS: Computer and information sciences

description: A major issue for many applications of blockchain technology is the tension between immutability and compliance to regulations. For instance, the GDPR in the EU requires to guarantee, under some circumstances, the right to be forgotten. This could imply that at some point one might be forced to delete some data from a locally stored blockchain, therefore irreparably hurting the security and transparency of such decentralized platforms. Motivated by such data protection and consistency issues, in this work we design and implement a mechanism for securely deleting data from Bitcoin blockchain. We use zero-knowledge proofs to allow any node to delete some data from Bitcoin transactions, still preserving the public verifiability of the correctness of the spent and spendable coins. Moreover, we specifically use STARK proofs to exploit the transparency that they provide. Our solution, unlike previous approaches, avoids the complications of asking nodes to reach consensus on the content to delete. In particular, our design allows every node to delete some specific data without coordinating this decision with others. In our implementation, data removal can be performed (resp., verified) in minutes (resp., seconds) on a standard laptop rather than in days as required in previous designs based on consensus.
Spectral sum rules for the quark-gluon plasma
Creators: name: Romatschke, Paul
name: Son, Dam Thanh
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Theory (hep-th)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We derive sum rules involving the spectral density of the stress-energy tensor in N=4 super-Yang-Mills theory and pure Yang-Mills theory. The sum rules come from the hydrodynamic behavior at small momenta and the conformal (in the case of N=4 SYM theory) or asymptotically free (as for the pure Yang-Mills theory) behavior at large momenta. These sum rules may help constrain QGP transport coefficients obtained from lattice QCD.
description: 21 pages, 3 figures
On the velocity field of sunspot penumbrae - I. A global view
Creators: name: Franz, Morten
name: Schlichenmaier, Rolf
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We investigated the vertical penumbral plasma flow on small spatial scales using data recorded by the spectropolarimeter of the solar optical telescope onboard Hinode. To this end we computed maps of apparent Doppler velocities by comparing the spectral position of the Fe I 630.15 nm & Fe I 630.25 nm lines with the averaged line profiles of the quiet Sun. To visualize the flow pattern in the low photosphere, we used a bisector of the wing of the absorption lines. Due to the small heliocentric angle (3 < Theta < 9) of our data sets, the horizontal component of the Evershed flow (EF) does not contribute significantly to the line shift. We found that in the quiet Sun (QS), the area showing up-flows is always larger than the one exhibiting down-flows. In the penumbra, up-flows dominate only at low velocities |v_dop| < 0.4 km/s while at larger velocities |v_dop| > 0.6 km/s down-flows prevail. Additionally, the maximal up-flow velocity in penumbrae is smaller, while the maximal down-flow velocity is larger with respect to the QS velocities. Furthermore, on a spatial average, the penumbra shows a red-shift, corresponding to a down-flow of more than 0.1 km/s. Up-flows are elongated and appear predominately in the inner penumbra. Strong down-flows with velocities of up to 9 km/s are concentrated at the penumbra-QS boundary. They are magnetized and are rather round in shape. The inner penumbra shows an average up-flow, which turns into a mean down-flow in the outer penumbra. The up-flow patches in the inner penumbra and the down-flow locations in the outer penumbra could be interpreted as the sources and the sinks of the EF. We did not find any indication of roll-type convection within penumbral filaments.
description: 9 pages, 8 figures
A Europa em que estamos
Creators: name: Revista, Direção
Publisher: name: AD ASTRA
Year: 2025

description:  Neste primeiro número da revista AD ASTRA o dossier temático debruça-se sobre o tema “A Europa em que estamos”, composto por vários olhares, cujo enfoque passa por contextos políticos, culturais, sociais, históricos … sobre o nosso transitivo presente. A par desta múltipla abordagem, os ensaios que corporizam a secção Varia propõem várias viagens, desde as oferecidas por novas formações educativas e por vozes literárias aos percursos de antigas diásporas. Nas secções recensões e testemunhos convidamos à leitura, à fruição musical e a uma memória que nos acompanha.
description: AD ASTRA, v. 1 n. 1 (2025): A Europa em que estamos
title: ÐÑÑÐ¾ÐºÐ¾Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´Ð¸ÑÐµÐ»ÑÐ½Ð°Ñ Ð²Ð¸ÑÑÑÐ°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð°Ñ ÑÐ¸ÑÑÐµÐ¼Ð° Ð¿Ð°ÑÐ°Ð»Ð»ÐµÐ»ÑÐ½Ð¾Ð³Ð¾ ÑÐ¸ÑÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÑÐ°ÑÐ¸ÐºÐ°
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð ÑÐ±Ð¸Ð½, 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: 2016
Subjects: Ð²Ð¸ÑÑÑÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ
ÑÐ¸ÑÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ÑÑÐ°ÑÐ¸ÐºÐ°
Ð¿ÑÐ¾ÑÐ¾ÐºÐ¾Ð»Ñ SSL/TLS
Ð±Ð°Ð»Ð°Ð½ÑÐ¸ÑÐ¾Ð²ÐºÐ° Ð½Ð°Ð³ÑÑÐ·ÐºÐ¸
Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
virtualization
traffic encryption
SSL / TLS protocols
load balancing
simulation

description: ÐÐ°ÑÑÐ¾ÑÑÐ°Ñ Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° ÑÐ¾Ð´ÐµÑÐ¶Ð¸Ñ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¿Ð¾Ð´ÑÐ¾Ð´Ð° Ðº Ð¿Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ñ Ð²ÑÑÐ¾ÐºÐ¾Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð¹ Ð²Ð¸ÑÑÑÐ°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¿Ð°ÑÐ°Ð»Ð»ÐµÐ»ÑÐ½Ð¾Ð³Ð¾ ÑÐ¸ÑÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÑÐ°ÑÐ¸ÐºÐ° Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð½ÑÑ Ð¸Ð¼Ð¸ÑÐ°ÑÐ¸Ð¾Ð½Ð½ÑÑ Ð¼Ð¾Ð´ÐµÐ»Ñ. ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ð¹ Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ Ð¿Ð¾ÑÐ¾ÑÐ½Ð¾Ðµ ÑÐ¸ÑÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ÑÐµÑÐµÐ²Ð¾Ð³Ð¾ ÑÑÐ°ÑÐ¸ÐºÐ°. ÐÑÐµÐ´Ð¼ÐµÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÑÑÑÑ Ð¼ÐµÑÐ¾Ð´Ñ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´Ð¸ÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿Ð¾ÑÐ¾ÑÐ½Ð¾Ð³Ð¾ ÑÐ¸ÑÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÑÐ°ÑÐ¸ÐºÐ°. Ð¦ÐµÐ»Ñ ÑÐ°Ð±Ð¾ÑÑ - Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ðµ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´Ð¸ÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÑÑÐµÐ´ÑÑÐ² Ð·Ð°ÑÐ¸ÑÑ Ð¿ÐµÑÐµÐ´Ð°Ð²Ð°ÐµÐ¼ÑÑ Ð´Ð°Ð½Ð½ÑÑ Ð² Ð¼ÑÐ»ÑÑÐ¸Ð¼ÐµÐ´Ð¸Ð¹Ð½ÑÑ ÑÐ¸ÑÑÐµÐ¼Ð°Ñ Ð¿ÑÐµÐ´Ð¾ÑÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÑÑÐ»ÑÐ³ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð²Ð¸ÑÑÑÐ°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð¹ Ð²ÑÑÐ¸ÑÐ»Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð¹ ÑÑÐµÐ´Ñ.
description: The graduate work contains the results of the research approach to the construction of high-performance virtualized system parallel traffic encryption and developed a simulation model. The object of this research is in-line encryption of network traffic. The subject of this research are methods of improving performance in-line traffic encryption. The purpose of this work is to increase productivity protection of data transmitted in the multimedia systems on the basis of a virtualized computing environment services.
Theory of charge transport in ferromagnetic semiconductor/s-wave superconductor junction
Creators: name: Mizuno, Yoshihiro
name: Yokoyama, Takehito
name: Tanaka, Yukio
Publisher: name: arXiv
Year: 2009
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: We study tunneling conductance in ferromagnetic semiconductor/insulator/s-wave superconductor junction where Rashba spin-orbit interaction (RSOI) and exchange field are taken into account in the ferromagnetic semiconductor. We show that normalized conductance at zero voltage has a maximum as a function of RSOI for high transparent interface and finite exchange field. This is because Andreev reflection probability shows a nonmonotonic dependence on RSOI in the presence of the exchange field. On the other hand, for intermediate transparent interface, normalized conductance at zero voltage has a reentrant shape at zero or small exchange field with increasing RSOI but is monotonically increasing by RSOI at large exchange field.
description: 6 pages, 6 figures
Additional file 1 of Biomechanical and clinical relationships between lower back pain and knee osteoarthritis: a systematic review
Creators: name: Amarasinghe, Piyumi
name: Wadugodapitiya, Surangika
name: Weerasekara, Ishanka
Publisher: name: figshare
Year: 2023
Subjects: subject: Medicine
subject: Biotechnology
subject: Ecology
subject: FOS: Biological sciences
subject: Cancer
subject: Mental Health

description: Additional file 1. PRISMA_2020_checklist.
title: ÐÐµÐ¿ÑÐµÑÑÐ²Ð½Ð¾Ðµ Ð´Ð·ÑÐ´Ð¾ Ð´Ð»Ñ Ð´ÐµÑÐµÐ¹ Ð´Ð¾ÑÐºÐ¾Ð»ÑÐ½Ð¾Ð³Ð¾ Ð¸ Ð¼Ð»Ð°Ð´ÑÐµÐ³Ð¾ ÑÐºÐ¾Ð»ÑÐ½Ð¾Ð³Ð¾ Ð²Ð¾Ð·ÑÐ°ÑÑÐ° ÐºÐ°Ðº Ð°Ð²ÑÐ¾ÑÑÐºÐ°Ñ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð°Ñ ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ñ
title: The continuous judo for kids of preschool and primary school age as an authorâs educational technology
Creators: name: ÐÐ¸ÑÐ°Ð¹Ð»Ð¾Ð²Ð°, Ð.
name: "Ð¡Ð¿Ð¾ÑÑ, ÑÐµÐ»Ð¾Ð²ÐµÐº, Ð·Ð´Ð¾ÑÐ¾Ð²ÑÐµ", Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÐ¹ Ð½Ð°ÑÑÐ½ÑÐ¹ ÐºÐ¾Ð½Ð³ÑÐµÑÑ
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2021
Subjects: Ð´Ð·ÑÐ´Ð¾
Ð´Ð¾ÑÐºÐ¾Ð»ÑÐ½ÑÐ¹ Ð²Ð¾Ð·ÑÐ°ÑÑ
Ð¼Ð»Ð°Ð´ÑÐ¸Ð¹ ÑÐºÐ¾Ð»ÑÐ½ÑÐ¹ Ð²Ð¾Ð·ÑÐ°ÑÑ
Ð½ÐµÐ¿ÑÐµÑÑÐ²Ð½Ð¾Ðµ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ðµ
Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð°Ñ ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ñ
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description: ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð·Ð°ÑÑÐ°Ð³Ð¸Ð²Ð°ÐµÑ Ð½Ð°ÑÑÐ½ÑÑ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ Ð²ÑÑÐ²Ð»ÐµÐ½Ð¸Ñ, Ð°Ð´Ð°Ð¿ÑÐ°ÑÐ¸Ð¸, ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸, Ð°Ð¿ÑÐ¾Ð±Ð°ÑÐ¸Ð¸ Ð¸ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¹ Ð½ÐµÐ¿ÑÐµÑÑÐ²Ð½Ð¾Ð³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð´Ð·ÑÐ´Ð¾Ð¸ÑÑÐ¾Ð². ÐÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½ Ð°Ð²ÑÐ¾ÑÑÐºÐ¸Ð¹ Ð¿Ð¾Ð´ÑÐ¾Ð´ Ð² ÑÐ¾ÑÐ¼Ð°ÑÐµ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¿ÑÐ¸Ð½ÑÐ¸Ð¿Ð° Ð¼Ð½Ð¾Ð³Ð¾ÑÐ¸ÐºÐ»Ð¾Ð²Ð¾Ð³Ð¾ ÑÐµÑÐµÐ½Ð¸Ñ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½ÑÑ Ð·Ð°Ð´Ð°Ñ Ð² ÑÐ¼ÐµÑÐ°Ð½Ð½ÑÑ Ð³ÑÑÐ¿Ð¿Ð°Ñ ÑÐ¾ÑÑÐ¸Ð¹ÑÐºÐ¸Ñ Ð´Ð·ÑÐ´Ð¾Ð¸ÑÑÐ¾Ð² Ð´Ð¾ÑÐºÐ¾Ð»ÑÐ½Ð¾Ð³Ð¾ Ð¸ Ð¼Ð»Ð°Ð´ÑÐµÐ³Ð¾ ÑÐºÐ¾Ð»ÑÐ½Ð¾Ð³Ð¾ Ð²Ð¾Ð·ÑÐ°ÑÑÐ°. Ð ÐµÐ·ÑÐ»ÑÑÐ°ÑÑ Ð¿ÑÑÐ¸Ð»ÐµÑÐ½ÐµÐ³Ð¾ Ð¿ÐµÐ´Ð°Ð³Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐºÑÐ¿ÐµÑÐ¸Ð¼ÐµÐ½ÑÐ° Ð¿Ð¾Ð´ÑÐ²ÐµÑÐ¶Ð´Ð°ÑÑ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ Ð°Ð²ÑÐ¾ÑÑÐºÐ¾Ð³Ð¾ Ð¿Ð¾Ð´ÑÐ¾Ð´Ð°.
description: The research touches upon the scientific problem of identification, adaptation, development, testing and implementation of continuous educationâs technologies for judokas. The authorâs approach is presented in the format of the implementation of the
principle of multi-cycle solution of educational tasks in mixed groups of Russian judokas of preschool and primary school age. The results of a five-year pedagogical experiment confirm the effectiveness of the authorâs approach.
The beaming effect for Fermi-LAT-detected FR-I radio galaxies
Creators: name: Ye, Xu-Hong
name: Zeng, Xiang-Tao
name: Huang, Dan-Yi
name: Zhang, Zhuang
name: Pei, Zhi-Yuan
name: Fan, Jun-Hui
Publisher: name: arXiv
Year: 2023
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Our knowledge of Giga-electron volt (GeV) radio galaxies has been revolutionized by the Fermi-LAT Telescope, which provides an excellent opportunity to study the physical properties of GeV radio galaxies. According to the radio power and morphology, radio galaxies can be separated into Fanaroff-Riley Type I radio galaxies (FR-Is) and Type II radio galaxies (FR-IIs). In this paper, we consider the unification of FR-Is and BL Lacertae objects (BL Lacs), and assume FR-Is to be a standard candle to discuss the beaming effect for Fermi-LAT-detected FR-Is. Our main conclusions are as follows: (1) The estimated Doppler factors for 30 Fermi-LAT-detected FR-Is are in a range of $δ_{\rm{I}}=0.88-7.49$. The average Doppler factor ($<δ_{\rm{I}}>=2.56\pm0.30$) of the 30 FR-Is is smaller than that ($<δ_{\rm{BL}}>=10.28\pm2.03$) of the 126 Fermi-LAT-detected BL Lacs, supporting the unification model that FR-Is are regarded as the misaligned BL Lacs with smaller Doppler factors; (2) We propose that different regions of FR-Is in the plot of the $γ$-ray luminosity against the photon spectral index $(\log L_γ-α_{\rm{ph}})$ may indicate the different beaming effects; (3) The average Doppler factor of the 6 TeV FR-Is is similar to that of the 24 non-TeV FR-Is, which implies that the difference between the TeV and GeV emissions is not driven by the beaming effect in the Fermi-LAT-detected FR-I samples.
description: 15 pages, 6 figures, 2 tables. publication in PASP
title: ÐÐ°ÑÑÑÐ°Ð±Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ¸Ñ ÐºÐ°ÑÑ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð¾ÑÑÐ»ÐµÐ¶Ð¸Ð²Ð°Ð½Ð¸Ñ Ð²Ð·Ð³Ð»ÑÐ´Ð° Ð´Ð»Ñ ÑÐµÑÐµÐ½Ð¸Ñ Ð¿Ð¾Ð¸ÑÐºÐ¾Ð²ÑÑ Ð·Ð°Ð´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Ð¾Ð»Ð¾Ð»Ð¾Ð±Ð¾Ð², ÐÐ»Ð°Ð´Ð¸Ð¼Ð¸Ñ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: ÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÐºÐ°ÑÑÑ
Ð¼Ð°ÑÑÑÐ°Ð±Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
ÑÐµÐ³Ð¸ÑÑÑÐ°ÑÐ¸Ñ Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ñ Ð³Ð»Ð°Ð·
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description: Ð Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ¾Ð¹ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ð¸ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ Ð¸Ð·ÑÑÐµÐ½Ð¸Ñ Ð²Ð·Ð°Ð¸Ð¼Ð¾ÑÐ²ÑÐ·Ð¸ Ð³ÐµÐ½ÐµÑÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¸ Ð¼Ð°ÑÑÑÐ°Ð±Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð½Ð° ÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ¸Ñ ÐºÐ°ÑÑÐ°Ñ Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ Ð³ÐµÐ¾Ð³ÑÐ°ÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½ÑÑ ÑÐ¸ÑÑÐµÐ¼, ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð¾ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð¾Ðµ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ðµ, ÐºÐ¾ÑÐ¾ÑÐ¾Ðµ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·ÑÐµÑ Ð½ÐµÑÐºÐ¾Ð»ÑÐºÐ¾ ÑÑÐ¾Ð²Ð½ÐµÐ¹ Ð¼Ð°ÑÑÑÐ°Ð±Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¾Ð´Ð½Ð¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾, Ð¸ Ñ ÐºÐ¾ÑÐ¾ÑÑÐ¼ Ð¼Ð¾Ð¶Ð½Ð¾ Ð²Ð·Ð°Ð¸Ð¼Ð¾Ð´ÐµÐ¹ÑÑÐ²Ð¾Ð²Ð°ÑÑ ÑÑÐµÐ¼Ñ ÑÐ¿Ð¾ÑÐ¾Ð±Ð°Ð¼Ð¸, Ð² ÑÐ¾Ð¼ ÑÐ¸ÑÐ»Ðµ Ð²Ð·Ð³Ð»ÑÐ´Ð¾Ð¼, Ð²ÑÑÐ¸ÑÐ»ÐµÐ½Ð° ÑÐºÐ¾ÑÐ¾ÑÑÑ ÑÐµÑÐµÐ½Ð¸Ñ Ð¿Ð¾Ð¸ÑÐºÐ¾Ð²ÑÑ Ð·Ð°Ð´Ð°Ñ Ð´Ð»Ñ ÐºÐ°Ð¶Ð´Ð¾Ð³Ð¾ ÑÐ¿Ð¾ÑÐ¾Ð±Ð°. Ð ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐµ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ ÑÐºÑÐ¿ÐµÑÐ¸Ð¼ÐµÐ½ÑÐ° Ð´Ð¾ÐºÐ°Ð·Ð°Ð½Ð° Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð²Ð·Ð¾Ñ-ÑÐ¾Ð´ÐµÑÐ¶Ð°ÑÐµÐ³Ð¾ Ð¼Ð°ÑÑÑÐ°Ð±Ð¸ÑÑÐµÐ¼Ð¾Ð³Ð¾ Ð¸Ð½ÑÐµÑÑÐµÐ¹ÑÐ° Ð´Ð»Ñ ÑÐµÑÐµÐ½Ð¸Ñ Ð¿Ð¾Ð¸ÑÐºÐ¾Ð²ÑÑ Ð·Ð°Ð´Ð°Ñ.
Model-independent analysis of Tau -> lll' decays
Creators: name: Turczyk, Sascha
Publisher: name: arXiv
Year: 2008
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Many models for physics beyond the Standard Model predict lepton-flavour violating decays of charged leptons at a level which may become observable very soon. We investigate the decays of a Tau-lepton into three charged leptons (Tau -> lll', l(') = e,μin a generic way. Using effective-field-theory methods, the relevant operators are classified according to their chirality structure. For each case, we work out the Dalitz plots for the decay distributions, including interference terms which arise from four-lepton operators and radiatively induced processes. We discuss phenomenological implications, in particular the potential to distinguish different new physics models.
description: 6 pages, 6 figures. To be published in the Proceedings of the Tau08 Conference, Novosibirsk, Russia (September 2008)
The Radio Detector of the Pierre Auger Observatory -- status and expected performance
Creators: name: Huege, Tim
Publisher: name: arXiv
Year: 2023
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: As part of the ongoing AugerPrime upgrade of the Pierre Auger Observatory, we are deploying short aperiodic loaded loop antennas measuring radio signals from extensive air showers in the 30-80 MHz band on each of the 1,660 surface detector stations. This new Radio Detector of the Observatory allows us to measure the energy in the electromagnetic cascade of inclined air showers with zenith angles larger than $\sim 65^\circ$. The water-Cherenkov detectors, in turn, perform a virtually pure measurement of the muon component of inclined air showers. The combination of both thus extends the mass-composition sensitivity of the upgraded Observatory to high zenith angles and therefore enlarges the sky coverage of mass-sensitive measurements at the highest energies while at the same time allowing us to cross-check the performance of the established detectors with an additional measurement technique. In this contribution, we outline the concept and design of the Radio Detector, report on its current status and initial results from the first deployed stations, and illustrate its expected performance with a detailed, end-to-end simulation study.
description: Contribution to the proceedings of the UHECR2022 conference, L'Aquila, Italy
Climate Crisis, Libraries, and Evidence-Based Decision Making
Creators: name: Brown, Helen L.
Publisher: name: Journal of the Canadian Health Libraries Association
Year: 2021

description: Introduction: In October 2018, the United Nations Intergovernmental Panel on Climate Change stated that 'transformative change' is needed to limit catastrophic impacts of global heating. In 2019, the UN's Emissions Gap Report described their findings as 'bleak' as emissions continued to rise, increasing risks to ecosystems, communities, and health. The level of change necessary is stark and involves steep reductions in emissions, especially in high emitting countries like Canada. One of the most significant contributors is air travel. Methods: This study applies climate science evidence to library professional activities by analyzing the emissions produced by air travel to past CHLA conferences. It uses conference attendance data from CHLA's three most recent conferences. Emissions calculations assume attendees used air travel for trips of more than 500km, or for the 2018 conference, travel from outside of Newfoundland. Results: As in similar studies, emissions resulting from air travel to CHLA conferences comprise a substantial portion of a sustainable per capita annual carbon budget. Significantly reducing air travel is necessary to meet climate targets. Discussion: This assessment addresses only one part of the carbon footprint of the three CHLA conferences studied and offers no baseline for other emissions sources, such as food and accommodations, that could be used in future measurements and decarbonization efforts. However, air travel is the most significant source of emissions from professional development activities. Thus, this poster also explores low carbon meeting options, professional roles in advocating for policy change, and implications for COVID-19 recovery efforts.
Intrusion-aware Alert Validation Algorithm for Cooperative Distributed Intrusion Detection Schemes of Wireless Sensor Networks
Creators: name: Shaikh, Riaz Ahmed
name: Jameel, Hassan
name: Auriol, Brian J. d
name: Lee, Heejo
name: Lee, Sungyoung
name: Song, Young-Jae
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cryptography and Security (cs.CR)
subject: FOS: Computer and information sciences

description: Existing anomaly and intrusion detection schemes of wireless sensor networks have mainly focused on the detection of intrusions. Once the intrusion is detected, an alerts or claims will be generated. However, any unidentified malicious nodes in the network could send faulty anomaly and intrusion claims about the legitimate nodes to the other nodes. Verifying the validity of such claims is a critical and challenging issue that is not considered in the existing cooperative-based distributed anomaly and intrusion detection schemes of wireless sensor networks. In this paper, we propose a validation algorithm that addresses this problem. This algorithm utilizes the concept of intrusion-aware reliability that helps to provide adequate reliability at a modest communication cost. In this paper, we also provide a security resiliency analysis of the proposed intrusion-aware alert validation algorithm.
description: 19 pages, 7 figures
A Population of Metal-Poor Galaxies with ~L* Luminosities at Intermediate Redshifts
Creators: name: Salzer, John J.
name: Williams, Anna L.
name: Gronwall, Caryl
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We present new spectroscopy and metallicity estimates for a sample of 15 star-forming galaxies with redshifts in the range 0.29 - 0.42. These objects were selected in the KPNO International Spectroscopic Survey via their strong emission lines seen in red objective-prism spectra. Originally thought to be intermediate-redshift Seyfert 2 galaxies, our new spectroscopy in the far red has revealed these objects to be metal-poor star-forming galaxies. These galaxies follow a luminosity-metallicity (L-Z) relation that parallels the one defined by low-redshift galaxies, but is offset by a factor of more than ten to lower abundances. The amount of chemical and/or luminosity evolution required to place these galaxies on the local L-Z relation is extreme, suggesting that these galaxies are in a very special stage of their evolution. They may be late-forming massive systems, which would challenge the current paradigm of galaxy formation. Alternatively, they may represent intense starbursts in dwarf-dwarf mergers or a major infall episode of pristine gas into a pre-existing galaxy. In any case, these objects represent an extreme stage of galaxy evolution taking place at relatively low redshift.
description: 6 pages, 3 figures; to appear in 10 April 2009 ApJL
Material Parameters for Faster Ballistic Switching of an In-plane Magnetized Nanomagnet
Creators: name: Yamaji, Toshiki
name: Imamura, Hiroshi
Publisher: name: arXiv
Year: 2023
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Applied Physics (physics.app-ph)
subject: FOS: Physical sciences

description: High-speed magnetization switching of a nanomagnet is necessary for faster information processing. The ballistic switching by a pulsed magnetic filed is a promising candidate for the high-speed switching. It is known that the switching speed of the ballistic switching can be increased by increasing the magnitude of the pulsed magnetic field. However it is difficult to generate a strong and short magnetic field pulse in a small device. Here we explore another direction to achieve the high-speed ballistic switching by designing material parameters such as anisotropy constant, saturation magnetization, and the Gilbert damping constant. We perform the macrospin simulations for the ballistic switching of in-plane magnetized nano magnets with varying material parameters. The results are analyzed based on the switching dynamics on the energy density contour. We show that the pulse width required for the ballistic switching can be reduced by increasing the magnetic anisotropy constant or by decreasing the saturation magnetization. We also show that there exists an optimal value of the Gilbert damping constant that minimizes the pulse width required for the ballistic switching.
title: ÐÐ»Ð¸ÑÐ½Ð¸Ðµ ÑÐ¸ÑÐºÐ¾Ð² Ð½Ð° ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ¾ÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÑ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð² ÑÑÐµÑÐµ Ð¶Ð¸Ð»Ð¸ÑÐ½Ð¾Ð³Ð¾ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð°
Creators: name: ÐÐ¾Ð»Ð¾Ð²Ð½Ð¸ÐºÐ¾Ð²Ð°, Ð.
name: ÐÐ¸ÐºÐ¾Ð»Ð¸ÑÐ¸Ð½Ð°, Ð¡.
name: ÐÑÑÐ´Ð°Ð½Ð¾Ð²Ð°, Ð.
name: "Ð£Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ ÑÐ¸ÑÐºÐ°Ð¼Ð¸ Ð² ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐµ: Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ Ð¸ ÑÐµÑÐµÐ½Ð¸Ñ", Ð½Ð°ÑÑÐ½Ð¾-Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ°Ñ ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ñ Ñ Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÐ¼ ÑÑÐ°ÑÑÐ¸ÐµÐ¼ (Ð ÐÐ¡ÐâÐ­â2018) (2018; Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³)
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2018

description: Ð­ÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ð¹ ÐºÑÐ¸Ð·Ð¸Ñ Ð¾ÐºÐ°Ð·Ð°Ð» ÑÑÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ðµ Ð²Ð»Ð¸ÑÐ½Ð¸Ðµ Ð½Ð° ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½ÑÑ ÑÑÐµÑÑ, Ð¾ÐºÐ°Ð·Ð°Ð² Ð²Ð»Ð¸ÑÐ½Ð¸Ðµ Ð½Ð° ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ¾ÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÑ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¹. Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÑÐ°ÑÑÐµ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ ÑÐ¸ÑÐºÐ¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¹, ÑÑÐ½ÐºÑÐ¸Ð¾Ð½Ð¸ÑÑÑÑÐ¸Ñ Ð½Ð° ÑÑÐ½ÐºÐµ Ð¶Ð¸Ð»ÑÑ Ð¸ Ð¸Ñ Ð²Ð»Ð¸ÑÐ½Ð¸Ðµ Ð½Ð°
ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ¾ÑÐ¿Ð¾ÑÐ¾Ð±Ð½Ð¾ÑÑÑ.
title: ÐÐ½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐµ Ð¼ÐµÑÐ¾Ð´Ñ Ð³ÐµÐ¾Ð»Ð¾Ð³Ð¾ÑÐ°Ð·Ð²ÐµÐ´Ð¾ÑÐ½ÑÑ ÑÐ°Ð±Ð¾Ñ Ð½Ð° Ð½ÐµÑÑÑ Ð¸ Ð³Ð°Ð·. Ð§. 1
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐµÑÐºÐ¸Ð½, ÐÐ¼Ð¸ÑÑÐ¸Ð¹
name: ÐÐ»ÑÐ¸Ð½ÑÐºÐ¸Ð¹, ÐÐ»ÐµÐºÑÐ°Ð½Ð´Ñ
name: ÐÑÐ°Ð½Ð°ÑÑÐµÐ², ÐÐ¸ÑÐ°Ð¸Ð»
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2023
Subjects: ÐÐµÑÑÑÐ½ÑÐµ Ð¸ Ð³Ð°Ð·Ð¾Ð²ÑÐµ Ð¼ÐµÑÑÐ¾ÑÐ¾Ð¶Ð´ÐµÐ½Ð¸Ñ
ÐÐµÐ¾Ð»Ð¾Ð³Ð¾-ÑÐ°Ð·Ð²ÐµÐ´Ð¾ÑÐ½Ð¾Ðµ Ð´ÐµÐ»Ð¾

description: Ð Ð¿Ð¾ÑÐ¾Ð±Ð¸Ð¸ Ð¸Ð·Ð»Ð¾Ð¶ÐµÐ½Ñ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÐµ Ð¼ÐµÑÐ¾Ð´Ñ Ð¸ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ Ð³ÐµÐ¾Ð»Ð¾Ð³Ð¾ÑÐ°Ð·Ð²ÐµÐ´Ð¾ÑÐ½ÑÑ ÑÐ°Ð±Ð¾Ñ (ÐÐ Ð ) Ð½Ð° Ð½ÐµÑÑÑ Ð¸ Ð³Ð°Ð·. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ðµ Ð²Ð¾Ð¿ÑÐ¾ÑÑ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð³ÐµÐ¾Ð»Ð¾Ð³Ð¾ÑÐ°Ð·Ð²ÐµÐ´Ð¾ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÑÐµÑÑÐ°, Ð²ÐºÐ»ÑÑÐ°ÑÑÐ¸Ðµ: Ð¼ÐµÑÐ¾Ð´Ñ ÐºÐ¾Ð»Ð¸ÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð¾ÑÐµÐ½ÐºÐ¸ Ð¿ÑÐ¾Ð³Ð½Ð¾Ð·Ð½Ð¾Ð³Ð¾ ÑÐ³Ð»ÐµÐ²Ð¾Ð´Ð¾ÑÐ¾Ð´Ð½Ð¾Ð³Ð¾ Ð¿Ð¾ÑÐµÐ½ÑÐ¸Ð°Ð»Ð°, Ð¼ÐµÑÐ¾Ð´Ñ Ð¾ÑÐµÐ½ÐºÐ¸ Ð³ÐµÐ¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð¸ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¹ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÐÐ Ð , Ð¼ÐµÑÐ¾Ð´Ñ Ð°Ð½Ð°Ð»Ð¸Ð·Ð°
ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¾Ð² Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð½ÑÑ ÐÐ Ð  Ð¸ Ð¼ÐµÑÐ¾Ð´Ñ Ð¿ÑÐ¸Ð½ÑÑÐ¸Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½ÑÐµÑÐºÐ¸Ñ ÑÐµÑÐµÐ½Ð¸Ð¹ Ð¿ÑÐ¸ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ ÐÐ Ð . ÐÐ°Ð¶Ð´Ð°Ñ Ð³Ð»Ð°Ð²Ð° Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Ð´Ð¾Ð¿Ð¾Ð»Ð½ÐµÐ½Ð° ÐºÐ¾Ð½ÑÑÐ¾Ð»ÑÐ½ÑÐ¼Ð¸ Ð²Ð¾Ð¿ÑÐ¾ÑÐ°Ð¼Ð¸ Ð´Ð»Ñ ÑÐ°Ð¼Ð¾Ð¿ÑÐ¾Ð²ÐµÑÐºÐ¸ Ð¸ Ð²Ð°ÑÐ¸Ð°Ð½ÑÐ°Ð¼Ð¸ Ð´Ð»Ñ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ ÑÐ°ÑÑÐµÑÐ½Ð¾-Ð³ÑÐ°ÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð·Ð°Ð´Ð°Ð½Ð¸Ð¹. Ð£ÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð¿Ð¾ ÐºÑÑÑÑ Â«ÐÐ½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐµ Ð¼ÐµÑÐ¾Ð´Ñ Ð³ÐµÐ¾Ð»Ð¾Ð³Ð¾ÑÐ°Ð·Ð²ÐµÐ´ÐºÐ¸ Ð½ÐµÑÑÐ¸ Ð¸ Ð³Ð°Ð·Ð°Â» Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ Ð¼Ð°Ð³Ð¸ÑÑÑÐ°Ð½ÑÐ¾Ð² Ð¾ÑÐ½Ð¾Ð¹ Ð¸ Ð·Ð°Ð¾ÑÐ½Ð¾Ð¹ ÑÐ¾ÑÐ¼ Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ Ð¿Ð¾ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐ¸ 38.04.02_15 Â«ÐÐµÐ½ÐµÐ´Ð¶Ð¼ÐµÐ½Ñ Ð² Ð½ÐµÑÑÐµÐ³Ð°Ð·Ð¾Ð²Ð¾Ð¼ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐµÂ».
Anisotropy of the space orientation of radio sources. II: The axis distribution function
Creators: name: Amirkhanyan, V. R.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: An analysis of the position angles distribution of 10461 extended radio sources shows that the spatial orientation of the axes of these objects is anisotropic: they avoid the direction towards the Celestial Pole and are mostly oriented in the equatorial direction. The ratio of the probability densities of the orientation in these two directions is 0.68. The probability that the sky distribution of axes is isotropic is less then 0.00004. This conclusion is consistent with the results of the analyses of the spatial distribution of galactic normals orientation in the galaxies from UGC, ESO and FGC catalogs
description: 7 pages, 6 figures
Relativistic Equations for Spin Particles: What Can We Learn From Noncommutativity?
Creators: name: Dvoeglazov, Valeri V.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: We derive relativistic equations for charged and neutral spin particles. The approach for higher-spin particles is based on generalizations of the Bargmann-Wigner formalism. Next, we study, what new physical information can the introduction of non-commutativity give us. Additional non-commutative parameters can provide a suitable basis for explanation of the origin of mass.
description: 5 pages, aipproc.cls, no figures, presented at the XXVIII WGMP09, Bialowieza, Poland, June 28-July 4, 2009. The extended version is contributed to the 12th International Workshop "What Comes Beyond the Standard Models?", July 14- 24, 2009, Bled, Slovenia
Automatic Hyperparameter Tuning in Sparse Matrix Factorization
Creators: name: Kawasumi, Ryota
name: Takeda, Koujin
Publisher: name: arXiv
Year: 2023
Subjects: subject: Machine Learning (stat.ML)
subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: Information Theory (cs.IT)
subject: Machine Learning (cs.LG)
subject: FOS: Computer and information sciences
subject: FOS: Physical sciences

description: We study the problem of hyperparameter tuning in sparse matrix factorization under Bayesian framework. In the prior work, an analytical solution of sparse matrix factorization with Laplace prior was obtained by variational Bayes method under several approximations. Based on this solution, we propose a novel numerical method of hyperparameter tuning by evaluating the zero point of normalization factor in sparse matrix prior. We also verify that our method shows excellent performance for ground-truth sparse matrix reconstruction by comparing it with the widely-used algorithm of sparse principal component analysis.
description: 13 pages, 5 figures
title: ÐÑÐ¸Ñ Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ Ð°ÑÐ¿ÐµÐºÑÑ ÑÐ¿Ð¾ÑÑÐ¸Ð²Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð² Ð¾ÑÐµÐ½ÐºÐµ Ð¾Ð»Ð¸Ð¼Ð¿Ð¸Ð¹ÑÐºÐ¸Ñ ÑÐµÐ¼Ð¿Ð¸Ð¾Ð½Ð¾Ð²
title: Psychological aspects of sports activity in the assessment of olympic champions
Creators: name: ÐÐ°ÑÑÑÐ°, Ð.
name: ÐÑÐ¾ÑÐºÐ¸Ð½, Ð.
name: ÐÐ¾ÑÑÐºÐ¾Ð², Ð.
name: "Ð¡Ð¿Ð¾ÑÑ, ÑÐµÐ»Ð¾Ð²ÐµÐº, Ð·Ð´Ð¾ÑÐ¾Ð²ÑÐµ", Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÐ¹ Ð½Ð°ÑÑÐ½ÑÐ¹ ÐºÐ¾Ð½Ð³ÑÐµÑÑ
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2021
Subjects: Ð¿ÑÐ¸Ñ Ð¾Ð»Ð¾Ð³Ð¸Ñ
ÑÐ¿Ð¾ÑÑ
ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¾Ð±ÑÑÐµÐ½Ð¸Ðµ
ÑÐ¾ÑÐµÐ²Ð½Ð¾Ð²Ð°Ð½Ð¸Ñ
ÑÐ¿Ð¾ÑÑÑÐ¼ÐµÐ½
ÑÐµÐ¼Ð¿Ð¸Ð¾Ð½
Ð²Ð¾ÑÐ¿Ð¾Ð¼Ð¸Ð½Ð°Ð½Ð¸Ñ
ÐÐ»Ð¸Ð¼Ð¿Ð¸Ð¹ÑÐºÐ¸Ðµ Ð¸Ð³ÑÑ

description: Ð ÑÑÐ°ÑÑÐµ Ð¸ÑÑÐ»ÐµÐ´ÑÑÑÑÑ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÐµ Ð°ÑÐ¿ÐµÐºÑÑ Ð¿ÑÐ¸ÑÐ¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ Ð¸ ÑÐ¾Ð¿ÑÐ¾Ð²Ð¾Ð¶Ð´ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð¸ ÑÑÐ°ÑÑÐ¸Ñ Ð² ÐÐ»Ð¸Ð¼Ð¿Ð¸Ð¹ÑÐºÐ¸Ñ Ð¸Ð³ÑÐ°Ñ Ð³Ð»Ð°Ð·Ð°Ð¼Ð¸ ÑÐ¿Ð¾ÑÑÑÐ¼ÐµÐ½Ð¾Ð², ÑÑÐ°Ð²ÑÐ¸Ñ ÐÐ»Ð¸Ð¼Ð¿Ð¸Ð¹ÑÐºÐ¸Ð¼Ð¸ ÑÐµÐ¼Ð¿Ð¸Ð¾Ð½Ð°Ð¼Ð¸ Ð² ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÐµ Ð³Ð¾Ð´Ñ, ÑÑÐ¾ Ð¼Ð¾Ð³Ð»Ð¾ Ð±Ñ Ð¿Ð¾Ð¼Ð¾ÑÑ Ð¿Ð¾Ð½Ð¸Ð¼Ð°Ð½Ð¸Ñ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð³Ð¾ ÐÐ»Ð¸Ð¼Ð¿Ð¸Ð¹ÑÐºÐ¾Ð³Ð¾ Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ñ. Ð¡ÑÐ°ÑÑÑ Ð¾Ð¿Ð¸ÑÐ°ÐµÑÑÑ Ð½Ð° ÑÐ¿Ð¾ÑÑÐ¸Ð²Ð½ÑÑ Ð»Ð¸ÑÐµÑÐ°ÑÑÑÑ, Ð²Ð¾ÑÐ¿Ð¾Ð¼Ð¸Ð½Ð°Ð½Ð¸Ñ Ð¸ ÐºÐ½Ð¸Ð³Ð¸, Ð°Ð²ÑÐ¾ÑÐ°Ð¼Ð¸ ÐºÐ¾ÑÐ¾ÑÑÑ Ð±ÑÐ»Ð¸ Ð¾Ð»Ð¸Ð¼Ð¿Ð¸Ð¹ÑÐºÐ¸Ðµ ÑÐµÐ¼Ð¿Ð¸Ð¾Ð½Ñ, Ð¿ÐµÑÐ¸Ð¾Ð´Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¸Ð·Ð´Ð°Ð½Ð¸Ñ, Ð¾ÑÐ²ÐµÑÐ°ÑÑÐ¸Ðµ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ Ð² ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð¼ ÑÐ¿Ð¾ÑÑÐµ Ð²ÑÑÑÐ¸Ñ Ð´Ð¾ÑÑÐ¸Ð¶ÐµÐ½Ð¸Ð¹.
description: The article examines various aspects of psychological support and support for the preparation and participation in the Olympic Games of athletes, who have become Olympic champions in different years. It could help to understand the problems of the modern Olympic movement. The article is based on sports literature, memories and books, authored by Olympic champions, periodicals, highlighting the problems in modern sports of the highest achievements.
title: ÐÐ»Ð³Ð¾ÑÐ¸ÑÐ¼ Ð¸ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð°Ñ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ Ð¼ÐµÑÐ¾Ð´Ð°, Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð½Ð¾Ð³Ð¾ Ð½Ð° Ð¿Ð¾Ð¸ÑÐºÐµ ÐºÑÐ°ÑÑÐ°Ð¹ÑÐµÐ³Ð¾ Ð¿ÑÑÐ¸ Ð² Ð³ÑÐ°ÑÐµ, Ð´Ð»Ñ Ð¸Ð½ÑÐµÑÐ°ÐºÑÐ¸Ð²Ð½Ð¾Ð¹ ÑÐµÐ³Ð¼ÐµÐ½ÑÐ°ÑÐ¸Ð¸ Ð¼ÐµÐ´Ð¸ÑÐ¸Ð½ÑÐºÐ¸Ñ Ð¸Ð·Ð¾Ð±ÑÐ°Ð¶ÐµÐ½Ð¸Ð¹
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Ð¾Ð²Ð¾ÑÐ¾Ð², ÐÐµÑÑ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: ÑÐµÐ³Ð¼ÐµÐ½ÑÐ°ÑÐ¸Ñ Ð¼ÐµÐ´Ð¸ÑÐ¸Ð½ÑÐºÐ¸Ñ Ð¸Ð·Ð¾Ð±ÑÐ°Ð¶ÐµÐ½Ð¸Ð¹
ÑÐ¼Ð½ÑÐµ Ð½Ð¾Ð¶Ð½Ð¸ÑÑ
Ð³ÑÐ°Ñ
ÐºÑÐ°ÑÑÐ°Ð¹ÑÐ¸Ð¹ Ð¿ÑÑÑ Ð² Ð³ÑÐ°ÑÐµ

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼ Ð¸ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð°Ñ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ Ð¼ÐµÑÐ¾Ð´Ð°, Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð½Ð¾Ð³Ð¾ Ð½Ð° Ð¿Ð¾Ð¸ÑÐºÐµ ÐºÑÐ°ÑÑÐ°Ð¹ÑÐµÐ³Ð¾ Ð¿ÑÑÐ¸ Ð² Ð³ÑÐ°ÑÐµ, Ð¸ÑÐ¿Ð¾Ð»ÑÐ·ÑÑÑÐµÐ³Ð¾ÑÑ Ð´Ð»Ñ Ð¿Ð¾Ð»ÑÐ°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÑÐµÐ³Ð¼ÐµÐ½ÑÐ°ÑÐ¸Ð¸ Ð¼ÐµÐ´Ð¸ÑÐ¸Ð½ÑÐºÐ¸Ñ Ð¸Ð·Ð¾Ð±ÑÐ°Ð¶ÐµÐ½Ð¸Ð¹. ÐÑÐ½Ð¾Ð²Ð½Ð°Ñ Ð¸Ð´ÐµÑ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ð° Ð·Ð°ÐºÐ»ÑÑÐ°ÐµÑÑÑ Ð² Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð¸Ð·Ð¾Ð±ÑÐ°Ð¶ÐµÐ½Ð¸Ñ Ð² Ð²Ð¸Ð´Ðµ Ð²Ð·Ð²ÐµÑÐµÐ½Ð½Ð¾Ð³Ð¾ Ð³ÑÐ°ÑÐ° ÑÐ°ÐºÐ¸Ð¼ Ð¾Ð±ÑÐ°Ð·Ð¾Ð¼, ÑÑÐ¾ Ð³ÑÐ°Ð½Ð¸ÑÑ Ð¾Ð±Ð»Ð°ÑÑÐµÐ¹ Ð±ÑÐ´ÑÑ Ð¸Ð¼ÐµÑÑ Ð¼Ð¸Ð½Ð¸Ð¼Ð°Ð»ÑÐ½ÑÐ¹ Ð²ÐµÑ. ÐÐ¾ÑÐ»Ðµ ÑÑÐ¾Ð³Ð¾ Ð¿Ð¸ÐºÑÐµÐ»Ð¸ Ð¿ÑÐ¸Ð½Ð°Ð´Ð»ÐµÐ¶Ð°ÑÐ¸Ðµ Ð³ÑÐ°Ð½Ð¸ÑÐµ Ð¼Ð¾Ð¶Ð½Ð¾ Ð½Ð°Ð¹ÑÐ¸ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ð¾Ð¼ Ð¿Ð¾Ð¸ÑÐºÐ° ÐºÑÐ°ÑÑÐ°Ð¹ÑÐµÐ³Ð¾ Ð¿ÑÑÐ¸ Ð² Ð³ÑÐ°ÑÐµ. Ð ÑÐ¾Ð´Ðµ ÑÐ°Ð±Ð¾ÑÑ Ð±ÑÐ»Ð¸ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ñ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÐµ Ð²ÐµÑÐ¾Ð²ÑÐµ ÑÑÐ½ÐºÑÐ¸Ð¸ Ð´Ð»Ñ Ð¿Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ñ Ð³ÑÐ°ÑÐ°, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ðµ ÑÐ¸Ð»ÑÑÑÐ°ÑÐ¸Ð¸ Ð² ÐºÐ°ÑÐµÑÑÐ²Ðµ Ð¿ÑÐµÐ´Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð¸Ð·Ð¾Ð±ÑÐ°Ð¶ÐµÐ½Ð¸Ñ.
A Comparison of Six Photometric Redshift Methods Applied to 1.5 Million Luminous Red Galaxies
Creators: name: Abdalla, Filipe B.
name: Banerji, Manda
name: Lahav, Ofer
name: Rashkov, Valery
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present an updated version of MegaZ-LRG (Collister et al.,(2007)) with photometric redshifts derived with the neural network method, ANNz as well as five other publicly available photo-z codes (HyperZ, SDSS, Le PHARE, BPZ and ZEBRA) for ~1.5 million Luminous Red Galaxies (LRGs) in SDSS DR6. This allows us to identify how reliable codes are relative to each other if used as described in their public release. We compare and contrast the relative merits of each code using ~13000 spectroscopic redshifts from the 2SLAQ sample. We find that the performance of each code depends on the figure of merit used to assess it. As expected, the availability of a complete training set means that the training method performs best in the intermediate redshift bins where there are plenty of training objects. Codes such as Le PHARE, which use new observed templates perform best in the lower redshift bins. All codes produce reasonable photometric redshifts, the 1-sigma scatters ranging from 0.057 to 0.097 if averaged over the entire redshift range. We also perform tests to check whether a training set from a small region of the sky such as 2SLAQ produces biases if used to train over a larger area of the sky. We conclude that this is not likely to be a problem for future wide-field surveys. The complete photometric redshift catalogue including redshift estimates and errors on these from all six methods can be found at www.star.ucl.ac.uk/~mbanerji/MegaZLRGDR6/megaz.html
description: 14 pages, 8 figures, submitted to MNRAS
Maps on ultrametric spaces, Hensel's Lemma, and differential equations over valued fields
Creators: name: Kuhlmann, Franz-Viktor
Publisher: name: arXiv
Year: 2010
Subjects: subject: Commutative Algebra (math.AC)
subject: FOS: Mathematics
subject: 12J10, 12J20

description: We give a criterion for maps on ultrametric spaces to be surjective and to preserve spherical completeness. We show how Hensel's Lemma and the multi-dimensional Hensel's Lemma follow from our result. We give an easy proof that the latter holds in every henselian field. We also prove a basic infinite-dimensional Implicit Function Theorem. Further, we apply the criterion to deduce various versions of Hensel's Lemma for polynomials in several additive operators, and to give a criterion for the existence of integration and solutions of certain differential equations on spherically complete valued differential fields, for both valued D-fields in the sense of Scanlon, and differentially valued fields in the sense of Rosenlicht. We modify the approach so that it also covers logarithmic-exponential power series fields. Finally, we give a criterion for a sum of spherically complete subgroups of a valued abelian group to be spherically complete. This in turn can be used to determine elementary properties of power series fields in positive characteristic.
description: 47 pages
A refinement of sharply F-pure and strongly F-regular pairs
Creators: name: Schwede, Karl
Publisher: name: arXiv
Year: 2009
Subjects: subject: Commutative Algebra (math.AC)
subject: Algebraic Geometry (math.AG)
subject: FOS: Mathematics
subject: 13A35, 14B05

description: We point out that the usual argument used to prove that $R$ is strongly $F$-regular if and only if $R_{Q}$ is strongly $F$-regular for every prime ideal $Q \in \Spec R$, does not generalize to the case of pairs $(R, \ba^t)$. The author's definition of sharp $F$-purity for pairs $(R, \ba^t)$ suffers from the same defect. We therefore propose different definitions of sharply $F$-pure and strongly $F$-regular pairs. Our new definitions agree with the old definitions in several common contexts, including the case that $R$ is a local ring.
description: 13 pages, to appear in the Journal of Commutative Algebra
Concurrent Gaussian elimination
Creators: name: Berger, Ulrich
name: Seisenberger, Monika
name: Spreen, Dieter
name: Tsuiki, Hideki
Publisher: name: arXiv
Year: 2023
Subjects: subject: Logic in Computer Science (cs.LO)
subject: FOS: Computer and information sciences
subject: F.4.1; F.3.1; F.3.2
subject: 03B70, 03Dxx, 03Fxx

description: Working in a semi-constructive logical system that supports the extraction of concurrent programs, we extract a program inverting non-singular real valued matrices from a constructive proof based on Gaussian elimination. Concurrency is used for efficient pivoting, that is, for finding an entry that is apart from zero in a non-null vector of real numbers.
description: To be published as a chapter of the book 'Mathematics for Computation - M4C', Marco Benini, Olaf beyersdorf, Michael Rathjen, Peter Schuster (eds.), World Scientific (publ.), 25 pages
The Small Scatter in BH-Host Correlations & The Case for Self-Regulated BH Growth
Creators: name: Hopkins, Philip F.
name: Murray, Norman
name: Thompson, Todd
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Supermassive black holes (BHs) obey tight scaling relations between their mass and their host galaxy properties such as total stellar mass, velocity dispersion, and potential well depth. This has led to the development of self-regulated models for BH growth, in which feedback from the central BH halts its own growth upon reaching a critical threshold. However, models have also been proposed in which feedback plays no role: so long as a fixed fraction of the host gas supply is accreted, relations like those observed can be reproduced. Here, we argue that the scatter in the observed BH-host correlations, and its run with scale, presents a demanding constraint on any model for these correlations, and that it favors self-regulated models of BH growth. We show that the scatter in the stellar mass fraction within a radius R in observed ellipticals and spheroids increases strongly at small R. At fixed total stellar mass (or host velocity dispersion), on very small scales near the BH radius of influence, there is an order-of-magnitude scatter in the amount of gas that must have entered and formed stars. In short, the BH appears to 'know more' about the global host galaxy potential on large scales than the stars and gas supply on small scales. This is predicted in self-regulated models; however, models where there is no feedback would generically predict order-of-magnitude scatter in the BH-host correlations. Likewise, models in which the BH feedback in the 'bright' mode does not regulate the growth of the BH itself, but sets the stellar mass of the galaxy by inducing star formation or blowing out a mass in gas much larger than the galaxy stellar mass, are difficult to reconcile with the scatter on small scales.
description: 9 pages, 3 figures, accepted to MNRAS (revised to match published version)