cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: ÐÐ¾Ð¼Ð¿ÐµÑÐµÐ½ÑÐ½Ð¾ÑÑÐ½ÑÐ¹ Ð¿Ð¾Ð´Ñ Ð¾Ð´ Ðº ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÐºÐ¾Ð¼Ð°Ð½Ð´Ñ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ°
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¼Ð°Ð³Ð¸ÑÑÑÐ°
titleType: Subtitle
title: Competence approach for forming an innovation project team
Creators: name: ÐÐ¾ÑÐ¾Ð¶Ð¸ÑÐµÐ²Ð°, ÐÐ¸ÐºÑÐ¾ÑÐ¸Ñ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2020
Subjects: IT Ð¿ÑÐ¾ÐµÐºÑ
ÐºÐ¾Ð¼Ð°Ð½Ð´Ð° Ð¿ÑÐ¾ÐµÐºÑÐ°
ÐºÐ¾Ð¼Ð¿ÐµÑÐµÐ½ÑÐ½Ð¾ÑÑÐ½ÑÐ¹ Ð¿Ð¾Ð´Ñ Ð¾Ð´
Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ° ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÐºÐ¾Ð¼Ð°Ð½Ð´Ñ Ð¿ÑÐ¾ÐµÐºÑÐ°
Ð¼Ð¾Ð´ÐµÐ»Ñ ÐºÐ¾Ð¼Ð¿ÐµÑÐµÐ½ÑÐ¸Ð¹
IT project
project team
competence approach
methodology of project team building
competency model

description: Ð ÑÐ°Ð±Ð¾ÑÐµ Ð¸Ð·ÑÑÐµÐ½Ñ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ IT Ð¿ÑÐ¾ÐµÐºÑÐ° Ñ ÑÐ¾ÑÐºÐ¸ Ð·ÑÐµÐ½Ð¸Ñ Ð¿ÑÐ¾ÑÐµÑÑÐ° ÑÐ¾Ñ-Ð¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÐºÐ¾Ð¼Ð°Ð½Ð´Ñ, Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ñ ÑÑÑÐµÑÑÐ²ÑÑÑÐ¸Ðµ Ð¿Ð¾Ð´ÑÐ¾Ð´Ñ Ðº Ð¿ÑÐ¾ÑÐµÑÑÑ ÑÐ¾ÑÐ¼Ð¸-ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÐºÐ¾Ð¼Ð°Ð½Ð´Ñ Ð¿ÑÐ¾ÐµÐºÑÐ°. ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ñ Ð¸ Ð¿ÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ñ Ð¿ÑÐ¾ÐµÐºÑÐ½ÑÐµ ÑÐ¾Ð»Ð¸, ÑÑÐ°ÑÑÐ²ÑÑÑÐ¸Ðµ Ð² ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¿ÑÐ¾ÐµÐºÑÐ°. ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ñ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð½ÑÑÐ¸Ð¹ ÐºÐ¾Ð¼Ð¿Ðµ-ÑÐµÐ½ÑÐ¸Ñ Ð¸ ÐºÐ¾Ð¼Ð¿ÐµÑÐµÐ½ÑÐ½Ð¾ÑÑÑ. ÐÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ñ Ð¸ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ñ Ð²Ð¸Ð´Ñ ÐºÐ¾Ð¼Ð¿ÐµÑÐµÐ½ÑÐ¸Ð¹.
Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° Ð¼Ð¾Ð´ÐµÐ»Ñ ÐºÐ¾Ð¼Ð¿ÐµÑÐµÐ½ÑÐ¸Ð¹ ÑÑÐ°ÑÑÐ½Ð¸ÐºÐ¾Ð² ÐºÐ¾Ð¼Ð°Ð½Ð´Ñ Ð¸ Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ° ÑÐ¾Ñ-Ð¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÐºÐ¾Ð¼Ð°Ð½Ð´Ñ, Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð½Ð°Ñ Ð½Ð° ÐºÐ¾Ð¼Ð¿ÐµÑÐµÐ½ÑÐ½Ð¾ÑÑÐ½Ð¾Ð¼ Ð¿Ð¾Ð´ÑÐ¾Ð´Ðµ. ÐÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½ Ð¿ÑÐ¸Ð¼ÐµÑ ÑÐµÑÑÐ° Ð½Ð° ÐÐ¾ÑÐ¿Ð¾ÑÐ°ÑÐ¸Ð²Ð½ÑÐµ ÐºÐ¾Ð¼Ð¿ÐµÑÐµÐ½ÑÐ¸Ð¸. Ð¡Ð¿ÑÐ¾ÐµÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð° Ð±Ð°Ð·Ð° Ð·Ð½Ð°Ð½Ð¸Ð¹ ÑÐºÑ-Ð¿ÐµÑÑÐ½Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ.
ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð° Ð°Ð¿ÑÐ¾Ð±Ð°ÑÐ¸Ñ Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ¸. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¿Ð¾ Ð¿ÑÐ¸Ð¼Ðµ-Ð½ÐµÐ½Ð¸Ñ Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ¸ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÐºÐ¾Ð¼Ð°Ð½Ð´ IT Ð¿ÑÐ¾ÐµÐºÑÐ° Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° ÐºÐ¾Ð¼Ð¿Ðµ-ÑÐµÐ½ÑÐ¸Ð¹.
description: In the work the peculiarities of the IT project in terms of team building process are studied, the existing approaches to the project team building process are in-vestigated. Project roles involved in the project implementation have been studied and analyzed. Definitions of competence and competence concepts were studied. Competence types were analyzed and studied.
Competence model of team members and methodology of team formation based on competence approach are developed. An example of Corporate Competence Test is presented. The knowledge base of the expert system is projected.
The method was tested. Recommendations on the application of IT project team building methodology based on competence analysis were developed.
Patterns of population structure and genetic diversity among Western Rattlesnakes (Crotalus oreganus) in the Pacific Northwest
Creators: name: Schmidt, Danielle Aimery
Publisher: name: University of British Columbia
Year: 2019

description: Advances in DNA sequencing technologies have enabled the collection of genome-wide data, facilitating a shift from population genetics to population genomics. This transition has greatly augmented the amount of data that can be collected from DNA samples as well as increased the scope of ecological and conservation studies. Historically, non-invasive or minimally-invasive sampling (MIS) has been widespread in wildlife studies, especially for those species of elevated conservation concern. Despite the benefits of MIS, the utility of these samples for collecting genomic information is limited. Low DNA quantity, degradation, and contamination by exogenous DNA make MIS challenging to use with modern genotyping-by-sequencing approaches, which have traditionally been developed for high quality DNA sources. Here, we demonstrate the utility of Genotyping-in-Thousands by sequencing (GT-seq), a targeted, multiplex amplicon approach, for genotyping minimally-invasive DNA samples from the Western Rattlesnake (Crotalus oreganus), a species-at-risk in British Columbia, Canada. Using a panel of 362 single nucleotide polymorphisms (SNPs) generated from high quality blood samples identified via restriction site-associated DNA sequencing (RADseq), we genotyped a total of 96 blood (n=68), minimally-invasive cloacal swab (n=9), and opportunistically collected roadkill tissue samples (n=19) across the distribution of Western Rattlesnakes in BC and Washington (USA). The targeted GT-seq panel yielded comparable estimates of within- and among-population variation to that of the larger RADseq dataset (n=9568 SNPs). We then applied this approach to a set of blood (n=68) and minimally-invasive samples (n =690) collected from across species the distribution. Hierarchical STRUCTURE analyses found evidence for population structure within and among all five geographic regions of C. oreganus occurrence in BC and Washington, as well as low levels of migration among groups of den sites across the distribution, with no evidence for a pattern of isolation-by-distance. These results provide evidence for population discreteness, as well as barriers to gene flow across the distribution suggesting that the single, recognized designatable unit for conservation for Western Rattlesnakes in BC should be re-assessed. More broadly, this thesis demonstrates the efficacy of combining genomic tools with MIS to investigate ecological and evolutionary processes impacting wild populations and better inform conservation management.
Supplementary material for The best defense is a good defense
Creators: name: Matsubara, Patrícia
name: Steinmacher, Igor
name: Gadelha, Bruno
name: Conte, Tayana
Publisher: name: figshare
Year: 2022
Subjects: subject: 80309 Software Engineering
subject: FOS: Computer and information sciences

description: Supplementary material containing the script for the focus group described in The best defense is a good defense. Larger version of Figure 1.
A Model of EUV Emission from Clusters of Galaxies
Creators: name: Lieu, Richard
name: Shi, Chun-Hui
Publisher: name: arXiv
Year: 2023
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: With tantalizing evidence of the recent e-Rosita mission, re-discovering very soft X-rays and EUV radiation from a cluster of galaxies or its environment, the question of the origin of cluster EUV excess is revisited in this work. It will be shown that the gas temperature, density, and frozen-in magnetic field of the intracluster medium, collectively support the emission and propagation of coherent uCerenkov radiation, which is low frequency and large amplitude radiation capable of accelerating charged particles to relativistic speeds. Owing to the spectrum of uCerenkov radiation, most of the incipient relativistic electrons undergo inverse-Compton scattering with the cosmic microwave background. It turns out the scattered radiation has observable ramifications only in the EUV band, of photon energy $70 -- 100$~eV, having a luminosity $\approx 10^{44}$~ergs~s$^{-1}$. This luminosity is on par with the EUV excess level detected from Abell 1795 and the Coma cluster. It should be stressed, as {\it caveat emptor}, that although the main subject is the putative large amplitude coherent uCerenkov modes which are highly nonlinear, the results presented were derived using a quasi-linear approach to highlight the observable features of the phenomenon, namely the EUV emission.
description: MNRAS in press
title: Ð Ð°ÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½ÑÐµ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÑ ÑÑÑÑÐºÑÑÑÐ½Ð¾Ð¹ ÑÐµÐ³ÑÐ»ÑÑÐ½Ð¾Ð¹ Ð¿Ð»Ð¸ÑÑ
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
title: Rational parameters of double-layer grid structure
Creators: name: Ð¤Ð°ÑÑ, Ð Ð¾Ð¼Ð°Ð½
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: 2019
Subjects: Ð¡ÑÐµÑÐ¶Ð½ÐµÐ²ÑÐµ ÑÐ¸ÑÑÐµÐ¼Ñ
ÐÑÐ¾ÑÑÑÐ°Ð½ÑÑÐ²ÐµÐ½Ð½ÑÐµ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¸
ÐÐ»Ð¸ÑÑ
Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÐ¸ÑÐµÑÐºÐ°Ñ Ð¾Ð¿ÑÐ¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ñ
ÑÑÑÑÐºÑÑÑÐ½Ð°Ñ ÑÐµÐ³ÑÐ»ÑÑÐ½Ð°Ñ Ð¿Ð»Ð¸ÑÐ°
ÑÐ°ÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½ÑÐµ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÑ
Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð°ÑÐ¸Ñ ÑÐ°ÑÑÐµÑÐ°

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½ ÑÐ¿Ð¾ÑÐ¾Ð± Ð¿Ð¾Ð¸ÑÐºÐ° ÑÐ°ÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½ÑÑ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÐ¾Ð² ÑÑÑÑÐºÑÑÑÐ½Ð¾Ð¹ ÑÐµÐ³ÑÐ»ÑÑÐ½Ð¾Ð¹ Ð¿Ð»Ð¸ÑÑ Ñ Ð¿Ð¾Ð¼Ð¾ÑÑÑ Ð¼ÐµÑÐ¾Ð´Ð° Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÐ¸ÑÐµÑÐºÐ¾Ð¹ Ð¾Ð¿ÑÐ¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¸ Ð¾ÑÐµÐ½ÐºÐ¸ ÑÑÐ¾Ð¸Ð¼Ð¾ÑÑÐ¸ Ð¿Ð¾Ð»ÑÑÐµÐ½Ð½ÑÑ Ð²Ð°ÑÐ¸Ð°Ð½ÑÐ¾Ð² ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¸. Ð Ð°Ð±Ð¾ÑÐ° Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð° Ñ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸ÐµÐ¼ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð¹ ÑÑÐ½ÐºÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ð¹ Ð¼Ð¾Ð´ÐµÐ»Ð¸ Ð² ÑÑÐµÐ´Ðµ Dynamo. ÐÐ¿ÑÐ¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ñ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¸ Ð²ÑÐ¿Ð¾Ð»Ð½ÑÐµÑÑÑ Ð¿Ð¾ ÐºÑÐ¸ÑÐµÑÐ¸Ñ Ð¼Ð¸Ð½Ð¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¼Ð°ÑÑÑ. ÐÐ»Ñ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¸ Ð¿Ð»Ð¸ÑÑ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÐµ Ð²Ð°ÑÐ¸Ð°Ð½ÑÑ ÑÑÐµÑÐ¶Ð½ÐµÐ²ÑÑ ÑÐ¸ÑÑÐµÐ¼: ÑÑÐµÑÐ¶Ð½Ð¸ Ð¸Ð· Ð¿Ð°ÑÐ½ÑÑ ÑÐ³Ð¾Ð»ÐºÐ¾Ð², Ð¿Ð°ÑÐ½ÑÑ ÑÐ²ÐµÐ»Ð»ÐµÑÐ¾Ð², ÐºÑÑÐ³Ð»Ð¾Ð¹ Ð¿Ð¾Ð»Ð¾Ð¹ ÑÑÑÐ±Ñ, ÐºÐ²Ð°Ð´ÑÐ°ÑÐ½Ð¾Ð¹ Ð¿ÑÐ¾ÑÐ¸Ð»ÑÐ½Ð¾Ð¹ ÑÑÑÐ±Ñ. ÐÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½ Ð²ÑÐ±Ð¾Ñ ÐºÐ²Ð°Ð´ÑÐ°ÑÐ½Ð¾Ð¹ Ð² Ð¿Ð»Ð°Ð½Ðµ ÑÐ°ÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ð¹ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¸ ÑÑÑÑÐºÑÑÑÐ½Ð¾Ð¹ Ð¿Ð»Ð¸ÑÑ Ð¿Ð¾ÑÐ»Ðµ ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ñ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÑ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð²Ð½ÑÑ ÑÐµÑÐµÐ½Ð¸Ð¹ Ð¸ Ð¾ÑÐµÐ½ÐºÐ¸ Ð¸Ñ ÑÑÐ¾Ð¸Ð¼Ð¾ÑÑÐ¸.
description: In this thesis, considered a method for finding rational parameters of double-layer grid structure using the parametric optimization method and estimating the cost of the obtained design options. The work was performed using an automated functional model in the Dynamo environment. The design optimization is performed by the criterion of mass minimization. For the analysis of the construction of the grid structure, various variants of rod systems are considered: rods from double angles, twin channels, round hollow tube, and square shaped tube. The choice was made of a rational design of the square double-layer grid structure after comparing various design solutions and estimating their cost.
Unified BCS-like model of pairing and alpha-correlations
Creators: name: Sen'kov, R. A.
name: Zelevinsky, V. G.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Nuclear Theory (nucl-th)
subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: We construct a BCS-like model that combines nucleonic pairing correlations and possible quartic correlations of alpha-type in a single variational wave function and derive corresponding gap equations. In the approximation of large logarithms typical for the BCS approach, we show that the system reveals two possible types of a condensate which cannot coexist. If the alpha-type condensate prevails at N=Z, the growth of the neutron excess will naturally lead to the first order phase transition to the nucleon condensates.
description: 18 pages
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¿ÑÐ¾ÐµÐºÑÐ° ÑÑÐ°ÑÑÐºÐ° Ð°Ð²ÑÐ¾Ð¼Ð¾Ð±Ð¸Ð»ÑÐ½Ð¾Ð¹ Ð´Ð¾ÑÐ¾Ð³Ð¸ III ÐºÐ°ÑÐµÐ³Ð¾ÑÐ¸Ð¸ Ð² Ð¡Ð°Ð¼Ð°ÑÑÐºÐ¾Ð¹ Ð¾Ð±Ð»Ð°ÑÑ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
title: Development of a project for a section of a III category highway in the Samara region
Creators: name: Ð ÑÐ´Ð°ÐºÐ¾Ð²Ð°, ÐÐ»ÐµÐ½Ð°
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¿ÑÐ¾ÐµÐºÑÐ¸ÑÑÐµÐ¼Ð°Ñ Ð°Ð²ÑÐ¾Ð¼Ð¾Ð±Ð¸Ð»ÑÐ½Ð°Ñ Ð´Ð¾ÑÐ¾Ð³Ð°
ÑÐ°Ð´Ð¸ÑÑ
ÑÐ°ÑÑÐµÑÐ½Ð°Ñ ÑÐºÐ¾ÑÐ¾ÑÑÑ
Ð¿ÑÐ¾Ð´Ð¾Ð»ÑÐ½ÑÐ¹ Ð¿ÑÐ¾ÑÐ¸Ð»Ñ
Ð´Ð¾ÑÐ¾Ð¶Ð½Ð°Ñ Ð¾Ð´ÐµÐ¶Ð´Ð°
projected road
radius
design speed
longitudinal profile
pavement

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½ Ð¿ÑÐ¾ÐµÐºÑ ÑÑÐ°ÑÑÐºÐ° Ð°Ð²ÑÐ¾Ð¼Ð¾Ð±Ð¸Ð»ÑÐ½Ð¾Ð¹ Ð´Ð¾ÑÐ¾Ð³Ð¸ III ÐºÐ°ÑÐµÐ³Ð¾ÑÐ¸Ð¸ Ð² ÑÐ°Ð¼Ð°ÑÑÐºÐ¾Ð¹ Ð¾Ð±Ð»Ð°ÑÑÐ¸. Ð Ð°ÑÑÑÐ¸ÑÐ°Ð½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ðµ Ð½Ð¾ÑÐ¼Ð°ÑÐ¸Ð²Ñ Ð°Ð²ÑÐ¾Ð¼Ð¾Ð±Ð¸Ð»ÑÐ½Ð¾Ð¹ Ð´Ð¾ÑÐ¾Ð³Ð¸, ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑ ÑÐµÑÑÐµÐ¶ÐµÐ¹. ÐÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½Ð¾ ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ðµ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¹ Ð´Ð¾ÑÐ¾Ð¶Ð½ÑÐ¹ Ð¾Ð´ÐµÐ¶Ð´, Ð° ÑÐ°ÐºÐ¶Ðµ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½ ÑÐ¼ÐµÑÐ½ÑÐ¹ ÑÐ°ÑÑÐµÑ Ð²ÑÐ±ÑÐ°Ð½Ð½Ð¾Ð¹ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¸ Ð´Ð¾ÑÐ¾Ð¶Ð½Ð¾Ð¹ Ð¾Ð´ÐµÐ¶Ð´Ñ
description: In this work, a project has been developed for a section of a category III highway in the Samara region. The main technical standards of the road have been calculated, a set of drawings has been developed. Comparison of pavement designs was made, as well as an estimate of the selected pavement design
Trombectomia da Artéria Basilar Através do Acesso Transbraquial num Paciente com Dissecção da Aorta
Creators: name: Proença, Filipa
name: Raposo, Francisco
name: Madureira, João
name: Campos, Catarina
name: Teotónio, Pedro
name: Neto, Lia
Publisher: name: Acta Radiológica Portuguesa
Year: 2020

description: Assunto: Submissão de um caso clínico intitulado “Trombectomia da artéria basilar através do acesso transbraquial num paciente com dissecção da aorta”. Editor da Ata Radiológica Portuguesa, Vimos por este meio submeter um caso clínico “Trombectomia da artéria basilar através do acesso transbraquial num paciente com dissecção da aorta” para colocar à consideração relativamente à publicação na vossa revista, Ata Radiológica Portuguesa. Nos últimos anos, o tratamento endovascular do acidente vascular cerebral tem emergido como um dos mais eficazes tratamentos médicos existentes. Através deste caso clínico, esperamos demonstrar a nossa experiência no que diz respeito ao uso de técnicas alternativas de acesso na trombectomia endovascular, para além da via femoral e relembrar todos os radiologistas da importância de realizar um estudo angio-TC dos vasos do pescoço eficaz, para o correto planeamento do tratamento. Descrevemos o caso de um paciente com dissecção da aorta e acidente vascular cerebral da artéria basilar que foi tratado, com sucesso, através de trombectomia endovascular pela via transbraquial. Revemos e interpretamos as alternativas de tratamento disponíveis atualmente e as suas vantagens relativamente ao acesso femoral clássico. A cardiologia de intervenção já demonstrou os benefícios e segurança de técnicas transradiais ou braquiais e, pese embora com cuidado e de forma gradual, os neurorradiologistas de intervenção começam a usar e a explorar estas alternativas. “O tempo é cérebro” e, quando ocorrem acidentes vasculares cerebrais agudos em pacientes nos quais o método clássico poderá não estar indicado, é fundamental conhecer e rapidamente adotar as técnicas alternativas disponíveis e realizá-las de forma segura para obtenção dos melhores outcomes possíveis. Antecipadamente grata, Filipa Maria Borges Costa de Brandão Proença
description: Acta Radiológica Portuguesa, Vol. 32 No. 3 (2020)
Photometry and spectroscopy of the Type Icn supernova 2021ckj: The diverse properties of the ejecta and circumstellar matter of Type Icn SNe
Creators: name: Nagao, T.
name: Kuncarayakti, H.
name: Maeda, K.
name: Moore, T.
name: Pastorello, A.
name: Mattila, S.
name: Uno, K.
name: Smartt, S. J.
name: Sim, S. A.
name: Ferrari, L.
name: Tomasella, L.
name: Anderson, J. P.
name: Chen, T. -W.
name: Galbany, L.
name: Gao, H.
name: Gromadzki, M.
name: Gutiérrez, C. P.
name: Inserra, C.
name: Kankare, E.
name: Magnier, E. A.
name: Müller-Bravo, T. E.
name: Reguitti, A.
name: Young, D. R.
Publisher: name: arXiv
Year: 2023
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We present photometric and spectroscopic observations of the Type Icn supernova (SN) 2021ckj. Spectral modeling of SN 2021ckj reveals that its composition is dominated by oxygen, carbon and iron group elements, and the photospheric velocity at peak is ~10000 km/s. From the light curve (LC) modeling applied to SNe 2021ckj, 2019hgp, and 2021csp, we find that the ejecta and CSM properties of Type Icn SNe are diverse. SNe 2021ckj and 2021csp likely have two ejecta components (an aspherical high-energy component and a spherical standard-energy component) with a roughly spherical CSM, while SN 2019hgp can be explained by a spherical ejecta-CSM interaction alone. The ejecta of SNe 2021ckj and 2021csp have larger energy per ejecta mass than the ejecta of SN 2019hgp. The density distribution of the CSM is similar in these three SNe, and is comparable to those of Type Ibn SNe. This may imply that the mass-loss mechanism is common between Type Icn (and also Type Ibn) SNe. The CSM masses of SN 2021ckj and SN 2021csp are higher than that of SN 2019hgp, although all these values are within the diversity seen in Type Ibn SNe. The early spectrum of SN 2021ckj shows narrow emission lines from C II and C III, without a clear absorption component, in contrast with that observed in SN 2021csp. The similarity of the emission components of these lines implies that the emitting regions of SNe 2021ckj and 2021csp have similar ionization states, and thus suggests that they have similar properties of the ejecta and CSM, which is inferred also from the LC modeling. Taking into account the difference in the strength of the absorption features, this heterogeneity may be attributed to viewing angle effects in otherwise common aspherical ejecta.
description: 13 pages, 5 figures, accepted for publication in A&A
Continual Reassessment and Related Dose-Finding Designs
Creators: name: O'Quigley, John
name: Conaway, Mark
Publisher: name: arXiv
Year: 2010
Subjects: subject: Methodology (stat.ME)
subject: FOS: Computer and information sciences

description: During the last twenty years there have been considerable methodological developments in the design and analysis of Phase 1, Phase 2 and Phase 1/2 dose-finding studies. Many of these developments are related to the continual reassessment method (CRM), first introduced by O'Quigley, Pepe and Fisher (\citeyearQPF1990). CRM models have proven themselves to be of practical use and, in this discussion, we investigate the basic approach, some connections to other methods, some generalizations, as well as further applications of the model. We obtain some new results which can provide guidance in practice.
description: Published in at http://dx.doi.org/10.1214/10-STS332 the Statistical Science (http://www.imstat.org/sts/) by the Institute of Mathematical Statistics (http://www.imstat.org)
The unusual distribution of spin-triplet supercurrents in disk-shaped Josephson junctions
Creators: name: Fermin, Remko
name: Yao, Junxiang
name: Lahabi, Kaveh
name: Aarts, Jan
Publisher: name: arXiv
Year: 2023
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: The phenomenon of s-wave spin triplet Cooper pairs induced in ferromagnetic metals has been researched now for more than a decade, and its main aspects are well understood. Crucial in converting s-wave singlet pairs in the superconductor to s-wave triplets in the ferromagnet is the engineering of well-defined magnetic inhomogeneity (the 'generator') at the interface with the superconductor. Vertical layer stacks are typically used as such, where two separate thin ferromagnetic layers with homogeneous but non-collinear magnetizations, provide the inhomogeneity. Alternatively, magnetic textures, like ferromagnetic domain walls and vortices, are possible triplet generators, although they are far less studied. In this paper we review our experiments on lateral disk-shaped Josephson junctions where a ferromagnetic bottom layer provides a weak link with a vortex magnetization imposed by the shape of the disk. We present three different junction configurations, exhibiting their own generator mechanism. In the first, we utilize the non-collinearity with a second ferromagnetic layer to produce the triplet correlations. The second configuration consists of only the bottom ferromagnet and the superconducting contacts; it relies on the vortex magnetization itself to generate the spin-polarized supercurrents. In the third case we exploit an intrinsic generator by combining a conventional superconductor (NbTi) and a half-metallic ferromagnetic oxide (La$_{0.7}$Sr$_{0.3}$MnO$_3$). We find strong supercurrents in all cases. A particularly interesting finding is that the supercurrents are strongly confined at the rims of the device, independent of the generating mechanism, but directly related to their triplet nature. What causes these rim currents remains an open question.
The IAG spectral atlas of the spatially resolved Sun: Centre-to-limb observations
Creators: name: Ellwarth, M.
name: Schäfer, S.
name: Reiners, A.
name: Zechmeister, M.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Solar surface magneto-convection appears as granulation pattern that impacts spectral lines in terms of both shape and wavelength. Such induced effects also tend to vary over the observed solar disc because of the changing observation angle and, thus, the changing observation height as well. Centre-to-limb observations of the resolved Sun offer an insight into the variable spectral behaviour across different heliocentric observing positions, providing crucial information about limb darkening, convective velocities, and line profile variability relevant to radial velocity (RV) calculations. Thus, RV measurements and exoplanet transit spectroscopy depend on precise reference templates. We want to provide a spectroscopic centre-to-limb solar atlas at high spectral resolution and high-frequency accuracy. The atlas shall help improve the understanding of the solar atmosphere and convection processes. We performed high-resolution observations of the resolved quiet Sun with a Fourier transform spectrograph at the Institut für Astrophysik und Geophysik in Göttingen. Our dataset contains a wavelength range from 4200Å to 8000Å. We obtained 165 spectra in total, with a spectral resolution of $Δν$ = 0.024cm$^{-1}$, corresponding to a resolving power $R$ of 700,000 at $\sim$6000Å. We present a centre-to-limb solar atlas containing 14 heliocentric positions. To check for consistency, we investigated the FeI ~6175Å absorption line and compared our line profiles with previous centre-to-limb observations and also with simulations. The line profile and also the bisector profiles are generally consistent with previous observations, but we have identified differences to model line profiles, especially close to the solar limb.
Large-scale Perturbations from the Waterfall Field in Hybrid Inflation
Creators: name: Fonseca, José
name: Sasaki, Misao
name: Wands, David
Publisher: name: arXiv
Year: 2010
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We estimate large-scale curvature perturbations from isocurvature fluctuations in the waterfall field during hybrid inflation, in addition to the usual inflaton field perturbations. The tachyonic instability at the end of inflation leads to an explosive growth of super-Hubble scale perturbations, but they retain the steep blue spectrum characteristic of vacuum fluctuations in a massive field during inflation. The power spectrum thus peaks around the Hubble-horizon scale at the end of inflation. We extend the usual delta-N formalism to include the essential role of these small fluctuations when estimating the large-scale curvature perturbation. The resulting curvature perturbation due to fluctuations in the waterfall field is second-order and the spectrum is expected to be of order 10^{-54} on cosmological scales.
description: 10 pages, 4 figures; v2 comments added on application of delta-N formalism including Hubble scale fluctuations
Additional file 1 of Computed tomographic assessment of lung aeration at different positive end-expiratory pressures in a porcine model of intra-abdominal hypertension and lung injury
Creators: name: Regli, Adrian
name: Ahmadi-Noorbakhsh, Siavash
name: Musk, Gabrielle Christine
name: Reese, David Joseph
name: Herrmann, Peter
name: Firth, Martin Joseph
name: Pillow, J. Jane
Publisher: name: figshare
Year: 2021
Subjects: subject: Biophysics
subject: Medicine
subject: Cell Biology
subject: Physiology
subject: FOS: Biological sciences
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Cancer

description: Additional file 1. Online Supplement.
Atmospheric parameters and kinematic information for the M giants stars from LAMOST DR9
Creators: name: Qiu, Dan
name: Tian, Hao
name: Li, Jing
name: Liu, Chao
name: Long, Lin
name: Shi, Jian-Rong
name: Yang, Ming
name: Zhang, Bo
Publisher: name: arXiv
Year: 2023
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: A catalog of more than 43,000 M giant stars has been selected by Li et al. from the ninth data release of LAMOST. Using the data-driven method SLAM, we obtain the stellar parameters (Teff, logg, [M/H], [$α$/M]) for all the M giant stars with uncertainties of 57 K, 0.25 dex, 0.16 dex and 0.06 dex at SNR > 100, respectively. With those stellar parameters, we constrain the absolute magnitude in K-band, which brings distance with relative uncertainties around 25% statistically. Radial velocities are also calculated by applying cross correlation on the spectra between 8000 A $Å$ and 8950 A $Å$ with synthetic spectra from ATLAS9, which covers the Ca II triplet. Comparison between our radial velocities and those from APOGEE DR17 and Gaia DR3 shows that our radial velocities have a system offset and dispersion around 1 and 4.6 km s$^{-1}$, respectively. With the distances and radial velocities combining with the astrometric data from Gaia DR3, we calculate the full 6D position and velocity information, which are able to be used for further chemo-dynamic studies on the disk and substructures in the halo, especially the Sagittarius Stream.
description: 21 pages, 11 figures, accepted by RAA
Two-fold anisotropic superconducting state in topological superconductor Sn$_4$Au
Creators: name: Sharma, M. M.
name: Gurjar, Ganesh
name: Patnaik, S.
name: Awana, V. P. S.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: Materials Science (cond-mat.mtrl-sci)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: Here we report the anisotropic magnetotransport properties in the superconducting state of Sn$_4$Au single crystal. Sn$_4$Au single crystal is synthesized through an easy melt growth method. Superconducting properties are evidenced by resistivity vs. temperature and DC magnetization measurements. Isothermal magnetization measurements hint toward type-II superconductivity in Sn$_4$Au. In-plane and out-of-plane resistivity measurements show anisotropic behavior of the upper critical field at temperatures below superconducting transition (T$_c$ = 2.3 K). The observed anisotropy is more elucidated in resistivity measurements performed below Tc at different tilt angles. The anisotropy parameter is found to be 1.26. The observed results show the presence two-fold anisotropic superconducting state in Sn$_4$Au single crystal, which may be induced due to the layered structure of synthesized Sn$_4$Au single crystal.
description: 10 Pages Text + Figs: Revised Submitted: Euro. Phys. Lett
Star formation trends in high-redshift galaxy surveys: the elephant or the tail?
Creators: name: Stringer, Martin
name: Cole, Shaun
name: Frenk, Carlos S.
name: Stark, Daniel P.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Star formation rate and accummulated stellar mass are two fundamental physical quantities that describe the evolutionary state of a forming galaxy. Two recent attempts to determine the relationship between these quantities, by interpreting a sample of star-forming galaxies at redshift of z~4, have led to opposite conclusions. We use a model galaxy population to investigate possible causes for this discrepancy and conclude that minor errors in the conversion from observables to physical quantities can lead to major misrepresentation when applied without awareness of sample selection. We also investigate, in a general way, the physical origin of the correlation between star formation rate and stellar mass within hierarchical galaxy formation theory.
description: 10 pages, 7 figures. Revised version: Fig. B2 removed after the discovery of an error, and Fig. 6 modified. Text and conclusions unchanged
Mapping Backsliding in the European Union
Creators: name: Sitter, Nick
name: Batory, Agnes
name: Kostka, Joanna
name: Krizsan, Andrea
name: Zentai, Violetta
Publisher: name: Zenodo
Year: 2016
Subjects: EU studies, democratic backsliding, Political systems and institutions, governance, Public administration, political leadership, crisis management, transboundary crisis, multi-level governance

description: When the European Union took on ten new member states in 2004, it went through an unprecedented enlargement that raised a number of questions about the future of the EU. The previous enlargements, from the original six member states to nine, then ten, twelve and fifteen states never admitted more than three new members at a time and the new member states had long track records of liberal democracy and market economies – or, in the case of the new Mediterranean member states in the 1980s, at least the latter. The debate about enlargement to formerly communist regimes began as soon as the Berlin Wall fell, and even in its earliest version it centred on the potential effects of a big round of enlargement on the EU’s capacity for governance and further integration.1 This coincided with a debate on the prospects for liberal democracy in terms of both party politics and public policy in the Europe’s new democracies.2 Apart from the questions about whether a wider Europe might mean more or less deepening in terms of supranational governance and increasing the scope of the EU’s competence, this debate also touched on the administrative capacity of the formerly communist states and their political will. The team put together by Paul Taggart and Alexs Szczerbiak focused on the latter question in particular, by examining the sources and consequences of popular and party-based Euroscepticism in both the old and new member states. The present policy brief takes the question debated by the Taggart and Szczerbiak team as a staring point: a dozen yeas after the first round of eastern enlargement, as Eurosceptic parties have come to power in some of the new member sates, has there been "backsliding” in the EU in terms of the states’ commitments to liberal democracy?
Additional file 1 of A rare familial rearrangement of chromosomes 9 and 15 associated with intellectual disability: a clinical and molecular study
Creators: name: Lemskaya, Natalya A.
name: Romanenko, Svetlana A.
name: Rezakova, Mariia A.
name: Filimonova, Elena A.
name: Prokopov, Dmitry Yu.
name: Dolskiy, Alexander A.
name: Perelman, Polina L.
name: Maksimova, Yulia V.
name: Shorina, Asia R.
name: Yudkin, Dmitry V.
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Neuroscience
subject: Science Policy
subject: 111714 Mental Health
subject: FOS: Health sciences
subject: Computational Biology

description: Additional file 1.
Pulsations in Hydrogen Burning Low Mass Helium White Dwarfs
Creators: name: Steinfadt, Justin D. R.
name: Bildsten, Lars
name: Arras, Phil
Publisher: name: arXiv
Year: 2010
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Helium core white dwarfs (WDs) with mass M
description: 6 pages, 3 figures. Published ApJ version
Mach Cones in Viscous Matter
Creators: name: Bouras, I.
name: El, A.
name: Fochler, O.
name: Lauciello, F.
name: Reining, F.
name: Uphoff, J.
name: Wesp, C.
name: Molnár, E.
name: Niemi, H.
name: Xu, Z.
name: Greiner, C.
Publisher: name: arXiv
Year: 2010
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Employing a microscopic transport model we investigate the evolution of high energetic jets moving through a viscous medium. For the scenario of an unstoppable jet we observe a clearly strong collective behavior for a low dissipative system $η/s \approx 0.005$, leading to the observation of cone-like structures. Increasing the dissipation of the system to $η/s \approx 0.32$ the Mach Cone structure vanishes. Furthermore, we investigate jet-associated particle correlations. A double-peak structure, as observed in experimental data, is even for low-dissipative systems not supported, because of the large influence of the head shock.
description: 4 pages, 3 figures, to appear in the conference proceedings of Hot Quarks 2010
Probing the structure of $χ_{c1}(3872)$ with photon transition form factors
Creators: name: Babiarz, Izabela
name: Pasechnik, Roman
name: Schäfer, Wolfgang
name: Szczurek, Antoni
Publisher: name: arXiv
Year: 2023
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We propose to study the structure of the enigmatic $χ_{c1}(3872)$ axial vector meson through its $γ^*_L γ\to χ_{c1}(3872)$ transition form factor. We derive a light-front wave function representation of the form factor for the lowest $c \bar c$ Fock-state. We found that the reduced width of the state is well within the current experimental bound recently published by the Belle collaboration. This strongly suggests a crucial role of the $c \bar c$ Fock-state in the photon-induced production. Our results for the $Q^2$ dependence can be tested by future single tagged $e^+ e^-$ experiments, giving further insights into the short-distance structure of this meson.
description: 5 pages, 2 figures
title: ÐÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ðµ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÑ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½ÑÑ ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¹ Ð¿ÑÐ¸ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÐ´Ð°Ð»ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð½Ð° Ð²ÑÐµÑ ÑÑÐ°Ð´Ð¸ÑÑ Ð¶Ð¸Ð·Ð½ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÐ¸ÐºÐ»Ð° Ð½Ð°ÑÐºÐ¾ÐµÐ¼ÐºÐ¾Ð¹ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¸Ð¸
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¼Ð°Ð³Ð¸ÑÑÑÐ° Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ 27.04.06 - ÐÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ñ Ð¸ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð½Ð°ÑÐºÐ¾ÐµÐ¼ÐºÐ¸Ð¼Ð¸ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð°Ð¼Ð¸ ; 27.04.06_02 - ÐÑÐ¾ÑÐµÑÑÑ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð½Ð°ÑÐºÐ¾ÐµÐ¼ÐºÐ¸Ð¼Ð¸ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð°Ð¼Ð¸
titleType: Subtitle
Creators: name: Ð¢Ð¸ÑÐ°Ð½Ð¾Ð², ÐÐ¸ÑÐ¸Ð»Ð»
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2019
Subjects: ÐÐ²ÑÐ¾Ð¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ðµ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ
ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ°Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ° Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð°
ÑÐ¾Ð¿ÑÐ¾Ð²Ð¾Ð¶Ð´ÐµÐ½Ð¸Ðµ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð°
plm-ÑÐ¸ÑÑÐµÐ¼Ñ
ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¾ÑÑÐºÐ¾-ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ¿ÑÐ°Ð²Ð¾ÑÐ½Ð¸Ðº
Ð¾ÑÐµÐ½ÐºÐ° ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð¾ Ð¿Ð¾Ð½ÑÑÐ¸Ðµ Ð¸ Ð¿ÑÐ¾ÑÐµÑÑ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð°, Ð¿Ð¾ÐºÐ°Ð·Ð°Ð½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð°ÑÐ¿ÐµÐºÑÑ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð°, ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð¾ Ð¿Ð¾Ð½ÑÑÐ¸Ðµ PLM-ÑÐ¸ÑÑÐµÐ¼Ñ. ÐÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð° Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ° Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½ÑÑ ÑÐ¸ÑÑÐµÐ¼ Ð´Ð»Ñ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ PLM-ÑÐ¸ÑÑÐµÐ¼Ñ, ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ Ð¾ÑÑÐµÑÑ Ð´Ð»Ñ ÐºÐ¾Ð½ÑÑÐ¾Ð»Ñ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸, Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð° Ð°Ð¿ÑÐ¾Ð±Ð°ÑÐ¸Ñ ÑÐ¸ÑÑÐµÐ¼Ñ Ð½Ð° ÐºÐ¾Ð½ÑÑÐ¾Ð»ÑÐ½Ð¾Ð¼ Ð¸Ð·Ð´ÐµÐ»Ð¸Ð¸ Ð¸ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð° ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ ÑÐ¸ÑÑÐµÐ¼Ñ Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸.
description: In this paper, the concept and process of technological preparation of production is analyzed, the main aspects of technological preparation of production are shown, the concept of a PLM system is considered. The production systems were prepared for the implementation of the PLM-system, reports were prepared for the control of technological preparation, the system was tested on the control product and the effectiveness of the system implementation at the enterprise was determined.
Amplified optomechanics in a unidirectional ring cavity
Creators: name: Xuereb, André
name: Horak, Peter
name: Freegarde, Tim
Publisher: name: arXiv
Year: 2011
Subjects: subject: Optics (physics.optics)
subject: Atomic Physics (physics.atom-ph)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We investigate optomechanical forces on a nearly lossless scatterer, such as an atom pumped far off-resonance or amicromirror, inside an optical ring cavity. Our model introduces two additional features to the cavity: an isolator is used to prevent circulation and resonant enhancement of the pump laser field and thus to avoid saturation of or damage to the scatterer, and an optical amplifier is used to enhance the effective $Q$-factor of the counterpropagating mode and thus to increase the velocity-dependent forces by amplifying the back-scattered light. We calculate friction forces, momentum diffusion, and steady-state temperatures to demonstrate the advantages of the proposed setup.
description: 9 pages, 3 figures
What inhibits male allyship? examining the influence of (mis)perceptions of other men's beliefs
Creators: name: De Souza, Lucille (Lucy)
Publisher: name: University of British Columbia
Year: 2020

description: Allyship is acting to support a marginalized individual or group. Although it is impactful, allyship is often avoided. Considering what inhibits male allyship towards women in male- dominated fields, I argue that pluralistic ignorance (Prentice & Miller, 1993; Miller & McFarland, 1991; Prentice, 2007) is a key factor. In this paper, I test hypotheses derived from the following model: men rarely enact allyship in male-dominated fields (e.g., STEM), leading to a general underestimation of men’s beliefs that sexism is problematic. I theorize that these misperceptions predict men’s own inaction, even if men do privately perceive gender bias as a problem. This inaction perpetuates a social norm that men do not enact allyship and the misperception that men are unconcerned about bias. Additionally, I suggest that sensitivity to other men’s judgements moderates the relationship between perceptions of other men’s beliefs and allyship intentions. In Study 1, I test if pluralistic ignorance occurs among men (and women) in STEM, examining relationships between beliefs about sexism and anticipated allyship behavior. In Study 2, I manipulate men’s perceptions of other men’s beliefs to assess if changing these perceptions causally influences men’s willingness to enact allyship behaviors. In Study 3, I test if men are less likely to enacting public reactive allyship among other men (compared to other women) and examine if backlash concerns mediate the relationship between perceptions of other men’s beliefs and allyship. In Study 4, I take this paradigm to an in-person context and observe if manipulating perceptions of other men’s beliefs about gender bias and social norms to confront sexism influences men’s (and women’s) actual likelihood of confronting sexist comments in real-time. My findings suggest that (mis)perceptions of men’s average beliefs inhibit individuals’ allyship intentions and behaviors, demonstrating the impact of pluralistic ignorance on addressing sexism.
The Origin of the Large Magellanic Cloud Globular Cluster NGC 2005
Creators: name: Piatti, Andrés E.
name: Hirai, Yutaka
Publisher: name: arXiv
Year: 2023
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The ancient Large Magellanic Cloud (LMC) globular cluster NGC 2005 has recently been reported to have an ex-situ origin, thus, setting precedents that the LMC could have partially formed from smaller merged dwarf galaxies. We here provide additional arguments from which we conclude that is also fairly plausible an in-situ origin of NGC 2005, based on the abundance spread of a variety of chemical elements measured in dwarf galaxies, their minimum mass in order to form globular clusters, the globular cluster formation imprints kept in their kinematics, and the recent modeling showing that explosions of supernovae are responsible for the observed chemical abundance spread in dwarf galaxies. The present analysis points to the need for further development of numerical simulations and observational indices that can help us to differentiate between two mechanisms of galaxy formation for the LMC, namely, a primordial dwarf or an initial merging event of smaller dwarfs.
description: 11 pages, 2 figures. Accepted for publication in The Astronomical Journal
Fold-Saddle Bifurcation in Non-Smooth Vector Fields on the Plane
Creators: name: Buzzi, Claudio A.
name: de Carvalho, Tiago
name: Teixeira, Marco A.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Dynamical Systems (math.DS)
subject: General Mathematics (math.GM)
subject: FOS: Mathematics
subject: 34A36, 37G10, 37G05

description: This paper presents results concerning bifurcations of 2D piecewise-smooth dynamical systems governed by vector fields. Generic three parameter families of a class of Non-Smooth Vector Fields are studied and its bifurcation diagrams are exhibited. Our main result describes the unfolding of the so called Fold-Saddle singularity.
On the origin of the non-detection of metastable HeI in the upper atmosphere of the hot Jupiter WASP-80b
Creators: name: Fossati, L.
name: Pillitteri, I.
name: Shaikhislamov, I. F.
name: Bonfanti, A.
name: Borsa, F.
name: Carleo, I.
name: Guilluy, G.
name: Rumenskikh, M. S.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: We aim to narrow down the origin of the non-detection of the metastable HeI triplet at about 10830 A obtained for the hot Jupiter WASP-80b. We measure the X-ray flux of WASP-80 from archival observations and use it as input to scaling relations accounting for the coronal [Fe/O] abundance ratio to infer the extreme-ultraviolet (EUV) flux in the 200-504 A range, which controls the formation of metastable HeI. We run three dimensional (magneto) hydrodynamic simulations of the expanding planetary upper atmosphere interacting with the stellar wind to study the impact on the HeI absorption of the stellar high-energy emission, the He/H abundance ratio, the stellar wind, and the possible presence of a planetary magnetic field up to 1 G. For a low stellar EUV emission, which is favoured by the measured logR'HK value, the HeI non-detection can be explained by a solar He/H abundance ratio in combination with a strong stellar wind, or by a sub-solar He/H abundance ratio, or by a combination of the two. For a high stellar EUV emission, the non-detection implies a sub-solar He/H abundance ratio. A planetary magnetic field is unlikely to be the cause of the non-detection. The low EUV stellar flux, driven by the low [Fe/O] coronal abundance, is the likely primary cause of the HeI non-detection. High-quality EUV spectra of nearby stars are urgently needed to improve the accuracy of high-energy emission estimates, which would then enable one to employ the observations to constrain the planetary He/H abundance ratio and the stellar wind strength. This would greatly enhance the information that can be extracted from HeI atmospheric characterisation observations.
description: Accepted for publication on A&A, 20 pages
How to Falsify the GR+LambdaCDM Model with Galaxy Redshift Surveys
Creators: name: Acquaviva, Viviana
name: Gawiser, Eric
Publisher: name: arXiv
Year: 2010
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: A wide range of models describing modifications to General Relativity have been proposed, but no fundamental parameter set exists to describe them. Similarly, no fundamental theory exists for dark energy to parameterize its potential deviation from a cosmological constant. This motivates a model-independent search for deviations from the concordance GR+LambdaCDM cosmological model in large galaxy redshift surveys. We describe two model-independent tests of the growth of cosmological structure, in the form of quantities that must equal one if GR+LambdaCDM is correct. The first, epsilon, was introduced previously as a scale-independent consistency check between the expansion history and structure growth. The second, upsilon, is introduced here as a test of scale-dependence in the linear evolution of matter density perturbations. We show that the ongoing and near-future galaxy redshift surveys WiggleZ, BOSS, and HETDEX will constrain these quantities at the 5-10% level, representing a stringent test of concordance cosmology at different redshifts. When redshift space distortions are used to probe the growth of cosmological structure, galaxies at higher redshift with lower bias are found to be most powerful in detecting deviations from the GR+LambdaCDM model.
description: 6 pages, 1 figure. Expanded discussion, matching version accepted for publication in Phys. Rev. D
Adverse association between ketosis and ovarian activity in Canadian dairy cows: Supplementary data
Creators: name: Alemu, Teshome
name: Duggavathi, Raj
Publisher: name: figshare
Year: 2025
Subjects: classificationCode: 300305
subject: Animal reproduction and breeding

description: Ketosis is a major metabolic disease characterized by high concentration of ketone bodies including β-hydroxy butyrate (BHB) in dairy cows. Although we and others have demonstrated the negative relationship between ketosis and reproductive performance of lactating cows, the mechanisms are not clear. We investigated the association between ketosis, determined by milk BHB concentrations during 3-14 days in milk (DIM), and ovarian activity, measured by milk progesterone (P4) profiles within 150 DIM in Holstein cows.