cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
A second update on double parton distributions
Creators: name: Ceccopieri, Federico Alberto
Publisher: name: arXiv
Year: 2014
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: We present two equivalent consistency checks of the momentum sum rule for double parton distributions and show the importance of the inclusion of the so-called inhomogeneous term in order to preserve correct longitudinal momentum correlations. We further discuss in some detail the kinematics of the splitting at the basis of the inhomogeneous term and update the double parton distributions evolution equations at different virtualities.
description: Two reference added. Additional appendix. Minor changes on the text
ГЕНЕЗИС РОССИЙСКОГО ЗАКОНОДАТЕЛЬСТВА О БАНКРОТСТВЕ ФИЗИЧЕСКОГО ЛИЦА
Creators: name: НУСС Н.В.
Publisher: name: Международный журнал гуманитарных и естественных наук
Year: 2020
Subjects: ИСТОРИЯ
ЗАКОН
ПРОЦЕДУРА
ИСТОЧНИК ПРАВА
ДОЛГ
РАССРОЧКА
КРЕДИТОР
БАНКРОТСТВО
HISTORY
LAW
PROCEDURE
SOURCE OF LAW
DEBT
INSTALLMENTS
CREDITOR
BANKRUPTCY

description: История возникновения и развития процедуры несостоятельности (банкротства) зародилась довольно давно, когда основным источником права была Русская Правда. Необходимость в признании человека несостоятельным всегда была и сохраняется по настоящее время. Несовершенство ранее принятых законов привело к изданию, действующего Федерального закона «О несостоятельности (банкротстве)» от 26.10.2002 №127-ФЗ. В законе предусмотрены процедуры, которые необходимы для восстановления платежеспособности, а так же назначается арбитражный управляющий, который регулирует проведение данной процедуры.
Charge density wave fluctuations in La2-xSrxCuO4 and their competition with superconductivity
Creators: name: Croft, T. P.
name: Lester, C.
name: Senn, M. S.
name: Bombardi, A.
name: Hayden, S. M.
Publisher: name: arXiv
Year: 2014
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We report hard (14 keV) x-ray diffraction measurements on three compositions (x=0.11,0.12,0.13) of the high-temperature superconductor La2-xSrxCuO4. All samples show charge-density-wave (CDW) order with onset temperatures in the range 51-80 K and ordering wavevectors close to (0.23,0,0.5). The CDW is strongest with the longest in-plane correlation length near 1/8 doping. On entering the superconducting state the CDW is suppressed, demonstrating the strong competition between the charge order and superconductivity. CDW order coexists with incommensurate magnetic order and wavevectors of the two modulations have the simple relationship $δ_{charge}= 2δ_{spin}$. The intensity of the CDW Bragg peak tracks the intensity of the low-energy (quasi-elastic) spin fluctuations. We present a phase diagram of La2-xSrxCuO4 including the pseudogap phase, CDW and magnetic order.
description: Correct Fig. 7 included
Natural antioxidant potential by the ethanolic extract of Rhodomyrtus tomentosa (Aiton) Hassk.
Creators: name: Saat Egra
name: Arung, Enos Tangke
name: Irawan Wijaya Kusuma
name: Yong-Ung Kim
Publisher: name: F1000 Research Limited
Year: 2019

description: Indonesia is one of the countries in tropical area having high diversity of medicinal plants. Our preliminary study showed that Rhodomyrtus tomentosa possess some biological activities. Rhodomyrtus tomentosa (Aiton) Hassk., commonly known as masisin in Indonesia, is a small shrubby tree with pink flowers and pink edible fruit. It has been reported that the plant species is native to southern and southeastern Asia (Winotai et al. 2005). The plant has been used as traditional medicine for diarrhea and woud treatments (Ho, 1999). In relation with cosmeceutical purposes, R. tomentosa has also been used as skin-whitening, antiaging, and skin beautifying agents (Miyake et al. 2006). Potential of the R. tomentosa extract was reported to exhibit strong antimicrobial activity against gram-positive bacteria (Saising et al. 2008; Limsuwan et al. 2009). In our course into the search for Indonesian plants having potential biological activities and isolation of their active compounds, the antioxidant property of leaves, wood and root extracts of R. tomentosa was reported here.
Nonlinear evolution of streaming instabilities in accreting protoplanetary disks
Creators: name: Hsu, Chun-Yen
name: Lin, Min-Kai
Publisher: name: arXiv
Year: 2022
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: The streaming instability (SI) is one of the most promising candidates for triggering planetesimal formation by producing dense dust clumps that undergo gravitational collapse. Understanding how the SI operates in realistic protoplanetary disks (PPDs) is therefore crucial to assess the efficiency of planetesimal formation. Modern models of PPDs show that large-scale magnetic torques or winds can drive laminar gas accretion near the disk midplane. In a previous study, we identified a new linear dust-gas instability, the azimuthal drift SI (AdSI), applicable to such accreting disks and is powered by the relative azimuthal motion between dust and gas that results from the gas being torqued. In this work, we present the first nonlinear simulations of the AdSI. We show that it can destabilize an accreting, dusty disk even in the absence of a global radial pressure gradient, which is unlike the classic SI. We find the AdSI drives turbulence and the formation of vertically-extended dust filaments that undergo merging. In dust-rich disks, merged AdSI filaments reach maximum dust-to-gas ratios exceeding 100. Moreover, we find that even in dust-poor disks the AdSI can increase local dust densities by two orders of magnitude. We discuss the possible role of the AdSI in planetesimal formation, especially in regions of an accreting PPD with vanishing radial pressure gradients.
description: Accepted by ApJ
Metaphorical perceptions of nursing students about nursing care, a phenomenological study
Creators: name: Oznur, Kavakli
name: Nefise, Karagoz
Publisher: name: Zenodo
Year: 2024

description: Aim: This study aims to analyze metaphorical perceptions of nursing students about the concept of care.  Materials and Methods: The study had a phenomenological research design. The study was conducted at the Gulhane Faculty of Nursing in University of Health Sciences between May 2021 and January 2022.  Undergraduate nursing students, who enrolled to nursing faculty of a university during the fall semester of 2021-2022 academic year, constituted the population of the study.  Qualitative data were collected with 78 students selected from all classes. Data were collected using a semi-structured interview form that included questions on sociodemographic characteristics and statements with blanks about the concept of care. Results: Being allowed to create multiple metaphors, the participants expressed 51 metaphors. These metaphors are based on five themes: commitment to professional values and ethical principles of nursing, evaluating and meeting patient needs from a holistic perspective, being a virtuous person and giving confidence, communicating and having the ability to show empathy, satisfying needs and basing on health. Conclusions: The findings of this study may be used to prepare and evaluate the content of nursing courses. These findings are valuable to improve professional values and the awareness of nursing students on the meaning and importance of the concept of care.

Key words: Nursing, care, metaphor, student, phenomenology.
ПРЕЗУМПЦИИ, ПРЕЮДИЦИИ И ФИКЦИИ КАК РАЗНОВИДНОСТЬ ЮРИДИЧЕСКИХ ФАКТОВ
Creators: name: ПЕТЕНЕВА Д.А.
Publisher: name: Международный журнал гуманитарных и естественных наук
Year: 2020
Subjects: ЮРИДИЧЕСКИЕ ФАКТЫ
ПРЕЗУМПЦИИ
ПРЕЮДИЦИИ
ФИКЦИИ
ПРАВООТНОШЕНИЯ
ПРАВОВОЕ РЕГУЛИРОВАНИЕ
LEGAL FACTS
PRESUMPTIONS
ASSUMPTIONS
FICTIONS
LEGAL RELATIONS
LEGAL REGULATION

description: В работе рассматриваются особенности презумпции, преюдиции и фикции как разновидности юридических фактов, которые прямо не предусмотрены гипотезами правовых норм, но с которыми закон связывает наступление юридических последствий. Также презумпции, преюдиции и фикции нуждаются в дополнительном комплексе изучении нестандартных способов, для изучения нестандартных ситуаций.
Sonnenfleckenzeichnung Nr. 63.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 27.03.1996, 15:30, erstellt von Sergio Cortesi
Creators: name: Observatorium Specola Solare Ticinese Locarno (1957 bis 1980 Teil der Eidgenössischen Sternwarte der ETH Zürich)
Publisher: name: [s.n.]
Year: 1996

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf einem eigenen Vordruck. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 3.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)
Sonnenfleckenzeichnung Nr. 207.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 01.09.1996, 09:30, erstellt von Andrea Manna
Creators: name: Observatorium Specola Solare Ticinese Locarno (1957 bis 1980 Teil der Eidgenössischen Sternwarte der ETH Zürich)
Publisher: name: [s.n.]
Year: 1996

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf einem eigenen Vordruck. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 3.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)
Higher-order scalar interactions and SM vacuum stability
Creators: name: Lalak, Zygmunt
name: Lewicki, Marek
name: Olszewski, Pawel
Publisher: name: arXiv
Year: 2014
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Investigation of the structure of the Standard Model effective potential at very large field strengths opens a window towards new phenomena and can reveal properties of the UV completion of the SM. The map of the lifetimes of the vacua of the SM enhanced by nonrenormalizable scalar couplings has been compiled to show how new interactions modify stability of the electroweak vacuum. Whereas it is possible to stabilize the SM by adding Planck scale suppressed interactions and taking into account running of the new couplings, the generic effect is shortening the lifetime and hence further destabilisation of the SM electroweak vacuum. These findings have been illustrated with phase diagrams of modified SM-like models. It has been demonstrated that stabilisation can be achieved by lowering the suppression scale of higher order operators while picking up such combinations of new couplings, which do not deepen the new minima of the potential. Our results show the dependence of the lifetime of the electroweak minimum on the magnitude of the new couplings, including cases with very small couplings (which means very large effective suppression scale) and couplings vastly different in magnitude (which corresponds to two different suppression scales).
description: plain Latex, 9 figures
Sonnenfleckenzeichnung Nr. 242.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 13.10.1996, 09:15, erstellt von Andrea Manna
Creators: name: Observatorium Specola Solare Ticinese Locarno (1957 bis 1980 Teil der Eidgenössischen Sternwarte der ETH Zürich)
Publisher: name: [s.n.]
Year: 1996

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf einem eigenen Vordruck. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 4.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)
Feedback Loops in Opinion Dynamics of Agent-Based Models with Multiplicative Noise
Creators: name: Conrad, Natasa Djurdjevac
name: Köppl, Jonas
name: Djurdjevac, Ana
Publisher: name: arXiv
Year: 2022
Subjects: subject: Dynamical Systems (math.DS)
subject: Social and Information Networks (cs.SI)
subject: FOS: Mathematics
subject: FOS: Computer and information sciences

description: We introduce an agent-based model for co-evolving opinion and social dynamics, under the influence of multiplicative noise. In this model, every agent is characterized by a position in a social space and a continuous opinion state variable. Agents' movements are governed by positions and opinions of other agents and similarly, the opinion dynamics is influenced by agents' spatial proximity and their opinion similarity. Using numerical simulations and formal analysis, we study this feedback loop between opinion dynamics and mobility of agents in a social space. We investigate the behavior of this ABM in different regimes and explore the influence of various factors on appearance of emerging phenomena such as group formation and opinion consensus. We study the empirical distribution and in the limit of infinite number of agents we derive a corresponding reduced model given by a partial differential equation (PDE). Finally, using numerical examples we show that a resulting PDE model is a good approximation of the original ABM.
ПРОБЛЕМНЫЕ ВОПРОСЫ РЕГУЛИРОВАНИЯ КОСВЕННЫХ ВЗАИМООТНОШЕНИЙ ГОСУДАРСТВЕННЫХ И КОММЕРЧЕСКИХ ЭКСПЕРТОВ ПРИ ОЦЕНКЕ ЗАКЛЮЧЕНИЙ ЭКСПЕРТА В СУДЕБНЫХ ЗАСЕДАНИЯХ
Creators: name: ПРОТАСОВ К.В.
name: ПОЖАРИЦКАЯ П.С.
Publisher: name: Международный журнал гуманитарных и естественных наук
Year: 2020
Subjects: ЭКСПЕРТ
СПЕЦИАЛИСТ
СУДЕБНАЯ ЭКСПЕРТИЗА
ЗАКЛЮЧЕНИЕ ЭКСПЕРТА
ЗАКЛЮЧЕНИЕ СПЕЦИАЛИСТА
РЕЦЕНЗИЯ
РЕЦЕНЗЕНТ
ОЦЕНКА ЗАКЛЮЧЕНИЯ ЭКСПЕРТА
СУДЕБНОЕ ЗАСЕДАНИЕ
РУКОВОДИТЕЛЬ ГОСУДАРСТВЕННОГО СУДЕБНО-ЭКСПЕРТНОГО УЧРЕЖДЕНИЯ
EXPERT
SPECIALIST
FORENSIC EXAMINATION
EXPERT OPINION
REVIEW
REVIEWER
EXPERT OPINION ASSESSMENT
COURT SESSION
HEAD OF THE STATE FORENSIC INSTITUTION

description: Статья посвящена современному критическому взгляду на заключение эксперта при оценке доказательств в суде. В частности, говорится о биполярной структуре заключения (юридической и специальной) с преобладанием последней. В связи с чем, необходимым становится опыт и компетенция, которыми обладают как рецензент (негосударственный эксперт, производящий оценку на коммерческой основе), так и руководитель государственного судебно-экспертного учреждения. В качестве решения проблемы, авторы статьи предлагают заранее знакомить эксперта с рецензией, а также привлекать в ходе допроса руководителя экспертного учреждения как своеобразного поручителя и гаранта.
ПЕРСПЕКТИВЫ РАЗВИТИЯ ПРАВОВОГО РЕГУЛИРОВАНИ ЦИФРОВОЙ ЭКОНОМИКИ В СФЕРЕ ФИНАНСОВЫХ ОТНОШЕНИЙ
Creators: name: ЛОШКАРЁВ А.В.
name: ПРИХОДЬКО С.О.
Publisher: name: Международный журнал гуманитарных и естественных наук
Year: 2020
Subjects: ЦИФРОВАЯ ЭКОНОМИКА
ФИНАНСОВЫЕ ОТНОШЕНИЯ
ЦИФРОВЫЕ ТЕХНОЛОГИИ
ПРАВОВОЕ РЕГУЛИРОВАНИЕ
СУДЕБНАЯ ПРАКТИКА
DIGITAL ECONOMY
FINANCIAL RELATIONS
DIGITAL TECHNOLOGIES
LEGAL REGULATION
JUDICIAL PRACTICE

description: В статье рассматриваются роль цифровых технологий в финансовом секторе и их влияние на формирование российского законодательства в указанной области общественных отношений. Выявляются подходы исследователей к уровню правового регулирования на современном этапе цифровизации российской экономики, а также условия, оказывающие на него влияние.
РОЛЬ ДИСТРИБЬЮТОРСКОГО ДОГОВОРА В СИСТЕМЕ ГРАЖДАНСКО-ПРАВОВЫХ ДОГОВОРОВ РОССИЙСКОЙ ФЕДЕРАЦИИ
Creators: name: РОДИОНОВА А.Ю.
Publisher: name: Международный журнал гуманитарных и естественных наук
Year: 2020
Subjects: ДИСТРИБЬЮТОР
ДИСТРИБЬЮТОРСКИЙ ДОГОВОР
ПРОИЗВОДИТЕЛЬ
ЛИЦЕНЗИЯ
РОСПАТЕНТ
DISTRIBUTOR
DISTRIBUTION AGREEMENT
MANUFACTURER
LICENSE
FEDERAL SERVICE FOR INTELLECTUAL PROPERTY

description: Цель выполненного исследования - проанализировать проблемные вопросы нормативно-правовой базы, связанные с отсутствием в российской правовой системе дистрибьюторского договора как отдельно взятого. Дистрибьюторский договор конкретизирует и определяет отношения между производителем или поставщиком и компанией, которая берет на себя реализацию продукции, включая продвижение. Тема является актуальной для множества сфер бизнеса: от энергетики и фармацевтики до косметики и бытовой химии - и неоднократно поднималась в диссертациях, статьях и иных научных работах. Методы исследования включают поиск, сбор, обработку, анализ, интерпретацию и систематизацию информации по теме статьи. В результате подчёркивается необходимость лицензирования в случае передачи прав на интеллектуальную собственность в рамках дистрибьюции, а также важность совершенствования норм текущего законодательства: закрепить за дистрибьюторским договором официальный статус в нормативно-правовой системе РФ.
Influence of fine structures on gyrosynchrotron emission of flare loops modulated by sausage modes
Creators: name: Shi, Mijie
name: Li, Bo
name: Guo, Mingzhe
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Sausage modes are one leading mechanism for interpreting short period quasi-periodic pulsations (QPPs) of solar flares. Forward modeling their radio emission is crucial for identifying sausage modes observationally and for understanding their connections with QPPs. Using the numerical output from three-dimensional magnetohydrodynamic (MHD) simulations, we forward model the gyrosynchrotron (GS) emission of flare loops modulated by sausage modes and examine the influence of loop fine structures. The temporal evolution of the emission intensity is analyzed for an oblique line of sight crossing the loop center. We find that the low- and high-frequency intensities oscillate in-phase at the period of sausage modes for models with or without fine structures. For low-frequency emissions where the optically thick regime arises, the modulation magnitude of the intensity is dramatically reduced by the fine structures at some viewing angles. On the contrary, for high-frequency emissions where the optically thin regime holds, the effect of fine structures or viewing angle is marginal. Our results show that the periodic intensity variations of sausage modes are not wiped out by the fine structures, and sausage modes remains a promising candidate mechanism for QPPs even when flare loops are fine-structured.
description: Accepted for publication in ApJ Letters
ПРАВОВОЕ РЕГУЛИРОВАНИЕ КРИПТОВАЛЮТЫ В РОССИИ
Creators: name: ЛОШКАРЕВ А.В.
name: РУСАНОВА П.А.
Publisher: name: Международный журнал гуманитарных и естественных наук
Year: 2020
Subjects: КРИПТОВАЛЮТА
ПРАВОВОЕ РЕГУЛИРОВАНИЕ
ЦИФРОВАЯ ВАЛЮТА
ЦИФРОВЫЕ ФИНАНСОВЫЕ АКТИВЫ
CRYPTOCURRENCY
LEGAL REGULATION
DIGITAL CURRENCY
DIGITAL FINANCIAL ASSETS

description: Статья посвящена анализу современного состояния правового регулирования криптовалюты в России, а также перспективы его развития. Рассмотрены принятые законодательные акты и их значение в правовом поле цифровой валюты. Показано, что единого мнения по поводу правого статуса криптовалюты в настоящее время нет, приведены примеры отнесения цифровой валюты к различным объектам гражданских прав.
The Boltzmann Equation in Classical Yang-Mills Theory
Creators: name: Mathieu, V.
name: Mueller, A. H.
name: Triantafyllopoulos, D. N.
Publisher: name: arXiv
Year: 2014
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We give a detailed derivation of the Boltzmann equation, and in particular its collision integral, in classical field theory. We first carry this out in a scalar theory with both cubic and quartic interactions and subsequently in a Yang-Mills theory. Our method is not relied on a doubling of the fields, rather it is based on a diagrammatic approach representing the classical solution to the problem.
description: 24 pages, 7 figures; v2: typos corrected, reference added, published in Eur. Phys. J. C
Galaxy mergers can rapidly shut down star formation
Creators: name: Ellison, Sara L.
name: Wilkinson, Scott
name: Woo, Joanna
name: Leung, Ho-Hin
name: Wild, Vivienne
name: Bickley, Robert W.
name: Patton, David R.
name: Quai, Salvatore
name: Gwyn, Stephen
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Galaxy mergers trigger both star formation and accretion onto the central supermassive black hole. As a result of subsequent energetic feedback processes, it has long been proposed that star formation may be promptly extinguished in galaxy merger remnants. However, this prediction of widespread, rapid quenching in late stage mergers has been recently called into question with modern simulations and has never been tested observationally. Here we perform the first empirical assessment of the long-predicted end phase in the merger sequence. Based on a sample of ~500 post-mergers identified from the Ultraviolet Near Infrared Optical Northern Survey (UNIONS), we show that the frequency of post-merger galaxies that have rapidly shutdown their star formation following a previous starburst is 30-60 times higher than expected from a control sample of non-merging galaxies. No such excess is found in a sample of close galaxy pairs, demonstrating that mergers can indeed lead to a rapid halt to star formation, but that this process only manifests after coalescence.
description: Accepted for publication in MNRAS Letters
title: Understanding teachers' approaches to assessment and restorative justice in education Newfoundland and Labrador
Creators: name: Ozoren Sener, Nevra
Publisher: name: Memorial University of Newfoundland
Year: 2023

description: This study explores the relationship between future and current educators’ approaches to classroom assessment and their restorative justice in education practices in Newfoundland and Labrador. A two-phase triangulation mixed method research design was used in this study to explore the educators’ (both teacher candidates and classroom teachers) approaches to classroom assessment and restorative justice in education. In Phase 1, a survey was distributed to educators (n= 83) to explore their approaches and, in Phase 2, in-depth semi-structured interviews were used (n=7) to deeply explore their approaches to classroom assessment and restorative justice in education. The results of this study showed that (a) teacher candidates’ and classroom teachers’ approaches to classroom assessment and restorative justice in education were not statistically significantly different between groups, (b) teacher candidates’ and classroom teachers’ understanding of the relationship between classroom assessment restorative justice in education were quite different, and (c) both teacher candidates and classroom teachers believed they lacked sufficient knowledge about restorative justice in education, but did not hold similar beliefs regarding classroom assessment. Findings of this study serve to inform the development of teacher education programs, professional development opportunities, and educational policies in Newfoundland and Labrador.
Sonnenfleckenzeichnung Nr. 238.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 07.10.1996, 07:30, erstellt von Sergio Cortesi
Creators: name: Observatorium Specola Solare Ticinese Locarno (1957 bis 1980 Teil der Eidgenössischen Sternwarte der ETH Zürich)
Publisher: name: [s.n.]
Year: 1996

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf einem eigenen Vordruck. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 4.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)
Strong interplay between electron-phonon interaction and disorder in low doped systems
Creators: name: Di Sante, Domenico
name: Ciuchi, Sergio
Publisher: name: arXiv
Year: 2014
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: The effects of doping on the spectral properties of low doped systems are investigated by means of Coherent Potential Approximation to describe the distributed disorder induced by the impurities and Phonon-Phonon Non-Crossing Approximation to characterize a wide class of electron-phonon interactions which dominate the low-energy spectral features. When disorder and electron-phonon interaction work on comparable energy scales, a strong interplay between them arises, the effect of disorder can no more be described as a mere broadening of the spectral features and the phonon signatures are still visible despite the presence of strong disorder. As a consequence, the disorder-induced metal-insulator transition, is strongly affected by a weak or moderate electron-phonon coupling which is found to stabilize the insulating phase.
description: New version with improved bibliography and discussion
Sonnenfleckenzeichnung Nr. 226.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 24.09.1996, 07:15, erstellt von Sergio Cortesi
Creators: name: Observatorium Specola Solare Ticinese Locarno (1957 bis 1980 Teil der Eidgenössischen Sternwarte der ETH Zürich)
Publisher: name: [s.n.]
Year: 1996

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf einem eigenen Vordruck. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 3.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)
Sonnenfleckenzeichnung Nr. 91.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 25.04.1996, 08:00, erstellt von Sergio Cortesi
Creators: name: Observatorium Specola Solare Ticinese Locarno (1957 bis 1980 Teil der Eidgenössischen Sternwarte der ETH Zürich)
Publisher: name: [s.n.]
Year: 1996

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf einem eigenen Vordruck. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 3.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)
Dipolar dark matter simulations on galaxy scales with the RAMSES code
Creators: name: Stahl, Clément
name: Famaey, Benoit
name: Thomas, Guillaume
name: Dubois, Yohan
name: Ibata, Rodrigo
Publisher: name: arXiv
Year: 2022
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We numerically explore on galaxy scales the Dipolar dark matter (DM) model based on the concept of gravitational polarization. This DM model has been proposed as a natural way to reproduce observed tight galactic scaling relations such as the baryonic Tully-Fisher relation and the Radial Acceleration Relation. We present a customized version of the \texttt{RAMSES} code including for the first time the dynamics of this Dipolar DM in $N$-body simulations. As a first application of this code, we check that we recover an equilibrium configuration that had been found analytically, where a low density Dipolar DM halo is at rest with respect to its central galaxy, recovering the aforementioned scaling relations. A characteristic signature of this equilibrium model is that it harbours a dynamical instability with a characteristic time depending on the Dipolar DM halo density, which we recover numerically. This represents a first step towards more involved simulations needed to test this framework, ranging from galaxy interactions to structure formation.
description: 9 pages, 5 figures, 1 table, MNRAS accepted
$R^2$ Gravity Effects on the Kinetic Axion Phase Space
Creators: name: Oikonomou, V. K.
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: In this work we consider the effect of an $R^2$ term on the kinetic misalignment axion theory. By using the slow-roll assumptions during inflation and the field equations, we construct an autonomous dynamical system for the kinetic axion, including the effects of the $R^2$ term and we solve numerically the dynamical system. As we demonstrate, the pure kinetic axion attractor is transposed to the right in the field phase space, and it is no longer $(ϕ,\dotϕ)=(\langle ϕ\rangle,0)$, but it is $(ϕ,\dotϕ)=(\langle ϕ'\rangle,0)$, with $\langle ϕ'\rangle\neq 0$ some non-zero value of the scalar field with $\langle ϕ'\rangle> \langle ϕ\rangle$. This feature indicates that the kinetic axion mechanism is enhanced, and the axion oscillations are further delayed, compared with the pure kinetic axion case. The phenomenological implications on the duration of the inflationary era, on the commencing of the reheating era and the reheating temperature, are also discussed.
description: EPL in press
Sonnenfleckenzeichnung Nr. 298.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 30.12.1996, 11:00, erstellt von Sergio Cortesi
Creators: name: Observatorium Specola Solare Ticinese Locarno (1957 bis 1980 Teil der Eidgenössischen Sternwarte der ETH Zürich)
Publisher: name: [s.n.]
Year: 1996

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf einem eigenen Vordruck. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 4.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)
ОСОБЕННОСТИ МЕТОДОВ РЕГУЛИРОВАНИЯ В КОММЕРЧЕСКОМ ПРАВЕ
Creators: name: МАЛИКОВА А.Х.
name: РУСАНОВА П.А.
Publisher: name: Международный журнал гуманитарных и естественных наук
Year: 2020
Subjects: МЕТОД
КОММЕРЧЕСКОЕ ПРАВО
ПРАВОВОЕ РЕГУЛИРОВАНИЕ
METHOD
COMMERCIAL LAW
LEGAL REGULATION

description: В работе рассматриваются основные методы регулирования в коммерческом праве, которые основаны на отраслевой принадлежности. Учитываются взгляды ученых-правоведов на методы регулирования в различных областях права и формы их применения. Обсуждаются специфические особенности коммерческой деятельности, определяющие ее правовое регулирование.
Collapsing rotating shells in Myers-Perry-AdS$_5$ spacetime: A perturbative approach
Creators: name: Rocha, Jorge V.
name: Santarelli, Raphael
name: Delsate, Térence
Publisher: name: arXiv
Year: 2014
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We study gravitational perturbations sourced by a rotating test shell collapsing into five-dimensional Myers-Perry black holes in anti-de Sitter (AdS). Our attention is restricted to the case in which the two possible angular momenta of the geometry are set equal. In this situation the background is cohomogeneity-1, which amounts to a crucial technical simplification. It is found that the linearized Einstein equations are consistent only when the test shell is corotating with the spacetime. However, it is argued that this is a consequence of the matter on the shell being described by dust or, more precisely, noninteracting test particles. We compute the mass and angular momenta of the perturbed spacetime using a counterterm subtraction method, for which we provide an explicit formula that has not appeared previously in the literature. The results are in agreement with the expected expressions for energy and angular momenta of geodesic particles in AdS$_5$.
description: 13 pages, 1 figure, uses revtex4; v2: typos corrected, minor addition regarding the one-point function of boundary stress-energy tensor, matches published version
Non-moraic schwa
Creators: name: Shih, Shu-Hao
Publisher: name: No Publisher Supplied
Year: 2018

description: This dissertation proposes that schwa can be non-moraic (Kager 1989, 1990, Féry 1995, 1996), analogous to high vowels.  In addition, such moraless schwas can head syllables (called ‘minor syllables’ after Matteson 1965, Lin 1993, 1997, 1998, Shaw 1994, Gafos 1998). Non-moraic, monomoraic, and bimoraic schwa can co-exist in the same phonological system. One of the major empirical consequences of this theory is that it accounts for stress systems in which stress avoids schwa.  I go further in claiming that non-moraic schwa is the only means by which stress systems are sensitive to vowel quality, contra Kenstowicz (1997), de Lacy (2002, 2004, 2006), and others. I argue that non-moraic, monomoraic, and bimoraic schwa co-exist in Piuma Paiwan, an Austronesian language that has been reported to have sonority-sensitive stress (Chen 2009a, b, Yeh 2011). My fieldwork and experimental results provide acoustic evidence that stress avoids landing on a schwa.  I argue that such avoidance is a side-effect of schwa’s prosodic status: schwa is usually non-moraic in Piuma Paiwan. However, schwa is required to be monomoraic when it appears in the non-head position of a foot, and bimoraic when it is forced to be in the head syllable of a foot. The different kinds of schwa have significantly distinct phonetic effects, particularly in duration and vowel quality variability.The theory proposed here predicts that stress should never avoid non-central vowels.  One of the major challenges to this prediction is found in sonority-driven stress systems that seem to make peripheral vowel distinctions.  However, I will present experimental evidence that the most discussed example of such a system – Gujarati – has been described incorrectly (cf. de Lacy 2004).   Of the five types of phonetic evidence examined, only F1 provides clear evidence for stress, revealing stress to be consistently penultimate, and not sonority-driven. I will also show that many descriptions of putative sonority-driven stress lack robust phonetic and phonological evidence. Finally, I present an Optimality Theory factorial typology of constraints relating to schwa moraicity, and identify important rankings for grammars with various effects.
2020-Ciaroshi-How_COVID-19_Spreads_MathModels
Creators: name: Ciarochei, Jennifer
Publisher: name: QUBES Educational Resources
Year: 2023

description: On December 31, 2019, the Chinese city of Wuhan reported an outbreak of a novel coronavirus (COVID-19) that has since killed over 4,200 people. As of March 11, 2020, over 118,000 infections—have been confirmed by the World Health Organization.
Non Minimal Terms in Composite Higgs Models and in QCD
Creators: name: De Curtis, Stefania
name: Redi, Michele
name: Vigiani, Elena
Publisher: name: arXiv
Year: 2014
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We introduce a general parametrisation for theories where the Higgs is a Goldstone boson that encompasses all existing models. Our construction deviates from extra-dimensional or deconstructed theories through the inclusion of "non-local" interactions in theory space. These terms are necessary to reproduce the most general 4D effective lagrangian compatible with the symmetries. After showing the relation of our formalism to the Callan-Coleman-Wess-Zumino effective lagrangian we apply our framework to SO(5)/SO(4) composite Higgs models studying the implications for the Higgs potential, coupling of resonances and S-parameter. We also outline the relevance of non-minimal terms in effective descriptions of QCD, studying the electro-magnetic splitting of pions and the correlation between L_9 and L_10 in the chiral lagrangian.
description: 29 pages, v2 minor changes
ОСОБЕННОСТИ МЕТОДОЛОГИИ СОВРЕМЕННОЙ ЮРИДИЧЕСКОЙ НАУКИ
Creators: name: РЯЗАНЦЕВА М.П.
Publisher: name: Международный журнал гуманитарных и естественных наук
Year: 2020
Subjects: ЮРИДИЧЕСКАЯ НАУКА
МЕТОДОЛОГИЯ
СИСТЕМА
ИЗУЧЕНИЕ
СОВРЕМЕННОЕ
РАЗВИТИЕ
ПРОБЛЕМАТИКА
SCIENCE
METHODOLOGY
SYSTEM
STUDY
MODERN
DEVELOPMENT
PROBLEMS

description: Данная статья обращает внимание на два основных метода, используемых в изучении юриспруденции в наше время. Актуальность выполненного исследования заключается в значимости достоверных результатов для проводимых юридических исследований. В ходе проведения сравнительного исследования был сделан вывод о возрастающем интересе к юридической методологии, что подтверждается множеством научных публикаций и конференций. Однако, при этом, рассматривая тему глубже, складывается мнение о том, что проводимые исследования скорее заполняют бреши возникшие в теории методологии в советское время, и исходят из теории единственно верной истины.
Sonnenfleckenzeichnung Nr. 46.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 06.03.1996, 08:15, erstellt von Sergio Cortesi
Creators: name: Observatorium Specola Solare Ticinese Locarno (1957 bis 1980 Teil der Eidgenössischen Sternwarte der ETH Zürich)
Publisher: name: [s.n.]
Year: 1996

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf einem eigenen Vordruck. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 4.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)
Ammonia in the interstellar medium of a starbursting disc at z=2.6
Creators: name: Doherty, M. J.
name: Geach, J. E.
name: Ivison, R. J.
name: Menten, K. M.
name: Jacob, A. M.
name: Forbrich, J.
name: Dye, S.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We report the detection of the ground state rotational emission of ammonia, ortho-NH$_3$ $(J_K=1_0\rightarrow0_0)$ in a gravitationally lensed, intrinsically hyperluminous, star-bursting galaxy at $z=2.6$. The integrated line profile is consistent with other molecular and atomic emission lines which have resolved kinematics well-modelled by a 5 kpc-diametre rotating disc. This implies that the gas responsible for NH$_3$ emission is broadly tracing the global molecular reservoir, but likely distributed in pockets of high density ($n\gtrsim5\times10^4$ cm$^{-3}$). With a luminosity of $2.8\times10^{6}$ $L_\odot$, the NH$_3$ emission represents $2.5\times10^{-7}$ of the total infrared luminosity of the galaxy, comparable to the ratio observed in the Kleinmann-Low nebula in Orion and consistent with sites of massive star formation in the Milky Way. If $L_{\rm NH_3}/L_{\rm IR}$ serves as a proxy for the 'mode' of star formation, this hints that the nature of star formation in extreme starbursts in the early Universe is similar to that of Galactic star-forming regions, with a large fraction of the cold interstellar medium in this state, plausibly driven by a storm of violent disc instabilities in the gas-dominated disc. This supports the 'full of Orions' picture of star formation in the most extreme galaxies seen close to the peak epoch of stellar mass assembly.
description: 5 pages, 3 figures, accepted for publication in MNRAS Letters
Sonnenfleckenzeichnung Nr. 49.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 11.03.1996, 08:30, erstellt von Sergio Cortesi
Creators: name: Observatorium Specola Solare Ticinese Locarno (1957 bis 1980 Teil der Eidgenössischen Sternwarte der ETH Zürich)
Publisher: name: [s.n.]
Year: 1996

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf einem eigenen Vordruck. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 4.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)
Vacuum refractive indices and helicity flip in strong-field QED
Creators: name: Dinu, Victor
name: Heinzl, Tom
name: Ilderton, Anton
name: Marklund, Mattias
name: Torgrimsson, Greger
Publisher: name: arXiv
Year: 2013
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Vacuum birefringence is governed by the amplitude for a photon to flip helicity or polarisation state in an external field. Here we calculate the flip and non-flip amplitudes in arbitrary plane wave backgrounds, along with the induced spacetime-dependent refractive indices of the vacuum. We compare the behaviour of the amplitudes in the low energy and high energy regimes, and analyse the impact of pulse shape and energy. We also provide the first lightfront-QED derivation of the coefficients in the Heisenberg-Euler effective action.
description: Version 2: additional results added, including discussion of vacuum refractive indices, analysis of flip and non-flip ampltidues at high-energy, additional plots, new title. Now 17 pages, 10 figures
Sonnenfleckenzeichnung Nr. 293.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 25.12.1996, 10:00, erstellt von Andrea Manna
Creators: name: Observatorium Specola Solare Ticinese Locarno (1957 bis 1980 Teil der Eidgenössischen Sternwarte der ETH Zürich)
Publisher: name: [s.n.]
Year: 1996

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf einem eigenen Vordruck. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 3.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)
Examination of future concerns of health management department students according to sociodemographic characteristics
Creators: name: Ali, Arslanoğlu
name: Fatmanur, Şener
name: Esma Nur, Sağlam
Publisher: name: Zenodo
Year: 2024

description: Aim: The aim of this study is to examine the future concerns of health management students studying at a state university according to their sociodemographic characteristics. The importance of the research is that no study has been conducted before on the future concerns of health management department students. It is important because it is the first study conducted in this field.

Material-Methods: The research is cross-sectional and descriptive type. In the study, Cronbach Alpha method was applied to the data to test the reliability of the future anxiety scale of university students. Difference tests, t tests and ANOVA tests were conducted for sociodemographic variables. The survey was administered face to face and was collected through convenience sampling among health management department students studying at a public university in Turkey who met the criteria.

Results: The Cronbach alpha value of the study was found to be.744. It is seen that 77.9% of the participants in the research are women and 22.1% are men. The average score of future anxiety was found to be 3.19, the average score of fear of the future was 3.07, and the despair about the future was 3.46.

Conclusion: In the study, a significant difference was found in the future anxiety average scores of health management department students in terms of gender and families' anxiety about the future. There was no significant difference in terms of department preference reason and KYK scholarship receipt. A significant difference was found between second and third grades according to the grades they attended.
ASymba: HI global profile asymmetries in the Simba simulation
Creators: name: Glowacki, M.
name: Deg, N.
name: Blyth, S. L.
name: Hank, N.
name: Davé, R.
name: Elson, E.
name: Spekkens, K.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Asymmetry in the spatially integrated, 1D HI global profiles of galaxies can inform us on both internal (e.g. outflows) and external (e.g. mergers, tidal interactions, ram pressure stripping) processes that shape galaxy evolution. Understanding which of these primarily drive HI profile asymmetry is of particular interest. In the lead-up to SKA pathfinder and SKA HI emission surveys, hydrodynamical simulations have proved to be a useful resource for such studies. Here we present the methodology behind, as well as first results, of ASymba: Asymmetries in HI of Simba galaxies, the first time this simulation suite has been used for this type of study. We generate mock observations of the HI content of these galaxies and calculate the profile asymmetries using three different methods. We find that $M_{\rm HI}$ has the strongest correlation with all asymmetry measures, with weaker correlations also found with the number of mergers a galaxy has undergone, and gas and galaxy rotation. We also find good agreement with the xGASS sample, in that galaxies with highly asymmetric profiles tend to have lower HI gas fractions than galaxies with symmetric profiles, and additionally find the same holds in sSFR parameter space. For low HI mass galaxies, it is difficult to distinguish between asymmetric and symmetric galaxies, but this becomes achievable in the high HI mass population. These results showcase the potential of ASymba and provide the groundwork for further studies, including comparison to upcoming large HI emission surveys.
description: 17 pages, 10 figures, 2 tables. Accepted in MNRAS