cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
A pharmacological and enzymatic analysis of the venoms of two Australian ants, Myrmecia pilosula and Myrmecia pyriformis
Creators: name: Matuszek., Maria Anna
Publisher: name: Monash University
Year: 2021

description: This thesis was scanned from the print manuscript for digital preservation and is copyright the author.
 Researchers can access this thesis by asking their local university, institution or public library to
 make a request on their behalf. Monash staff and postgraduate students can use the link in the References field.
ФАКТИЧЕСКИЙ БРАК В СТРАНАХ ЕВРОПЫ
Creators: name: ВАРИВАНСКАЯ Ю.С.
Publisher: name: StudNet
Year: 2020
Subjects: ГРАЖДАНСКИЙ БРАК
СОЖИТЕЛЬСТВО
НЕЗАКОННЫЙ БРАК
НЕЗАРЕГИСТРИРОВАННЫЙ БРАК
ФАКТИЧЕСКИЕ СУПРУГИ
СОЖИТЕЛИ
ПРАВА СОЖИТЕЛЕЙ
COMMON-LAW MARRIAGE
COHABITATION
ILLEGAL MARRIAGE
UNREGISTERED MARRIAGE
ACTUAL SPOUSES
COHABITANTS
RIGHTS OF COHABITANTS

description: В статье рассматривается вопрос легитимации гражданского брака в ряде стран романо-германкой правовой семьи: права, обязанности сожителей, а также необходимость таких правовых норм в современном мире. Также в статье были проанализированные исследования, сообщающие, что институт брака и семьи теряет свою популярность. Рассмотрены современные тенденции и альтернативные формы семейной жизни, а также рассмотрены причины смен ценностей у молодого поколения.The article considers the issue of the legitimation of civil marriage in a number of countries by the Romano-German legal family: rights, obligations of cohabitants, as well as the need for such legal norms in the modern world. The article also analyzed studies reporting that the institution of marriage and the family was losing its popularity. The current trends and alternative forms of family life are considered, as well as the reasons for the change of values among the young generation are considered.
Additional file 2 of Clustering of the causes of death in Northeast Iran: a mixed growth modeling
Creators: name: Talkhi, Nasrin
name: Emamverdi, Zohreh
name: Jamali, Jamshid
name: Salari, Maryam
Publisher: name: figshare
Year: 2023
Subjects: subject: Medicine
classificationCode: 39999
subject: Chemical Sciences not elsewhere classified
subject: Ecology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
classificationCode: 69999
subject: Biological Sciences not elsewhere classified
classificationCode: 80699
subject: Information Systems not elsewhere classified
subject: Cancer
subject: Plant Biology

description: Additional file 2: Figure A1. Representation of membership to classes 1 and 2 using LGMM by sex. Figure A2. Representation of membership to classes 1 to 3 using LGMM by age.
Optimising the K dark filter for the Kunlun Infrared Sky Survey
Creators: name: Li, Yushan
name: Zheng, Jessica
name: Tuthill, Peter
name: Freeman, Matthew
name: Ashley, Michael
name: Burton, Michael
name: Lawrence, Jon
name: Mould, Jeremy
name: Wang, Lifan
Publisher: name: arXiv
Year: 2016
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: The Kunlun Infrared Sky Survey will be the first comprehensive exploration of the time varying Universe in the infrared. A key feature in optimizing the scientific yield of this ambitious research program is the choice of the survey passband. In particular the survey aims to maximally exploit the unique thermal and atmospheric conditions pertaining to the high Antarctic site. By simulating the expected signal-to-noise for varying filter properties within the so-called "K_DARK" 2.4um window, filter performance can be tuned and best-case designs are given covering a range of conditions.
description: to appear in PASA
Fragmentation with Discontinuous Galerkin schemes: Non-linear fragmentation
Creators: name: Lombart, Maxime
name: Hutchison, Mark
name: Lee, Yueh-Ning
Publisher: name: arXiv
Year: 2022
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Atmospheric and Oceanic Physics (physics.ao-ph)
subject: FOS: Physical sciences

description: Small grains play an essential role in astrophysical processes such as chemistry, radiative transfer, gas/dust dynamics. The population of small grains is mainly maintained by the fragmentation process due to colliding grains. An accurate treatment of dust fragmentation is required in numerical modelling. However, current algorithms for solving fragmentation equation suffer from an over-diffusion in the conditions of 3D simulations. To tackle this challenge, we developed a Discontinuous Galerkin scheme to solve efficiently the non-linear fragmentation equation with a limited number of dust bins.
description: 16 pages, Accepted for publication in MNRAS
ULX pulsar Swift J0243.6+6124 observations with NuSTAR -- dominance of reflected emission in the super-Eddington state
Creators: name: Bykov, S. D.
name: Gilfanov, M. R.
name: Tsygankov, S. S.
name: Filippova, E. V.
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We report the discovery of the bright reflected emission component in the super-Eddington state of the ULX pulsar Swift J0243.6+6124, based on the NuSTAR observations of the source during its 2017 outburst. The flux of the reflected emission is weakly variable over the pulsar phase while the direct emission shows significantly larger pulsation amplitude. We propose that in this system the neutron star finds itself in the centre of the well formed by the inner edge of the geometrically thick super-Eddington accretion disc truncated by the magnetic field of the pulsar. The aspect ratio of the well is H/R \sim 1. The inner edge of the truncated disc is continuously illuminated by the emission of the accretion column giving rise to the weakly variable reflected emission. As the neutron star rotates, its emission sweeps through the line of sight, giving rise to the pulsating direct emission. From Doppler broadening of the iron line, we measure the truncation radius of the accretion disc \sim 50 R_g. The inferred dipole component of the magnetic field is consistent with previous estimates favouring a not very strong field. The uniqueness of this system is determined by its moderately super-Eddington accretion rate and the moderate magnetic field so that the inner edge of the truncated geometrically thick accretion disc is seen from the neutron star at a large solid angle.
description: 12 pages, 9 figures, 2 tables. Monthly Notices of the Royal Astronomical Society Main Journal Accepted. Code available via this url: https://github.com/SergeiDBykov/nustar_sj0243
Salacia beddomei Gamble 1916
Creators: name: Jadhav, Durga C.
name: Prabhugaonkar, Ashish V.
name: Nandikar, Mayur D.
Publisher: name: Zenodo
Year: 2016
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Celastrales
Celastraceae
Salacia
Salacia beddomei

description: 1. Salacia beddomei Gamble (1916: 133)
 Type:— INDIA, Tamil Nadu, Coimbatore district, Anamalai hills, 1866, Beddome s.n. [lectotype, K (K000669921, image! Fig. 1); isolectotype, MH! (MH00001914), designated here].
 Salacia beddomei was described by Gamble from Anamalai hills Coimbatore, India based on the Beddome’s collection. In the protologue no type has been mentioned. Two specimens are placed at K and MH collected by R. A. Beddome in 1866, and annotated by Gamble (1916). The specimen placed at K (K 000669921) agrees with protologue and has illustration of the flower by Gamble therefore designated here as lectotype, while duplicate at MH (MH 00001914) as isolectotype.
description: Published as part of Jadhav, Durga C., Prabhugaonkar, Ashish V. & Nandikar, Mayur D., 2016, Nomenclature notes on the genus Salacia L. (Celastraceae) in India, pp. 121-130 in Phytotaxa 265 (2) on page 121, DOI: 10.11646/phytotaxa.265.2.3, http://zenodo.org/record/13662647
The soundproof model of an acoustic--internal waves system with low stratification
Creators: name: Bresch, Didier
name: Klein, Rupert
name: Liu, Xin
Publisher: name: arXiv
Year: 2022
Subjects: subject: Analysis of PDEs (math.AP)
subject: Mathematical Physics (math-ph)
subject: FOS: Mathematics
subject: FOS: Physical sciences
subject: 76B55, 76B70, 76N30, 86A99

description: This work is devoted to investigating a compressible fluid system with low stratification, which is driven by fast acoustic waves and internal waves. The approximation using a soundproof model is justified. More precisely, the soundproof model captures the dynamics of both the non-oscillating mean flows and the oscillating internal waves, while filters out the fast acoustic waves, of the compressible system with or without initial acoustic waves. Moreover, the fast-slow oscillation structure is investigated.
ПРАВОВАЯ КОНСТРУКЦИЯ ДИСТРИБЬЮТОРСКОГО ДОГОВОРА
Creators: name: ДАШКИНА А.З.
Publisher: name: StudNet
Year: 2020
Subjects: DISTRIBUTION CONTRACT FILM DISTRIBUTION
SUPPLY CONTRACT
CONCESSION CONTRACT
ДИСТРИБЬЮТОРСКИЙ ДОГОВОР
КИНОДИСТРИБЬЮТОР
ДОГОВОР ПОСТАВКИ
ДОГОВОР КОММЕРЧЕСКОЙ КОНЦЕССИИ

description: Как в мировой, так и в российской практике предпринимательских отношений получила широкое распространение конструкция дистрибьюторского договора. Однако вопрос правового регулирования гражданско-правовых отношений по поводу заключения, исполнения и прекращения дистрибьюторского договора не имеет однозначного решения в связи с отсутствием соответствующего законодательного регулирования. В статье рассматриваются правовая конструкция дистрибьюторского договора на примере кинодистрибьюторского договора, а также отличия дистрибьюторского договора от правовых конструкций других договоров.Both in the world and in the Russian practice of entrepreneurial relations, the design of a distribution agreement has become widespread. However, the issue of legal regulation of civil law relations regarding the conclusion, execution and termination of a distribution agreement does not have an unambiguous solution due to the lack of appropriate legislative regulation. The article discusses the legal structure of the distribution agreement using the example of a film distribution agreement, as well as the differences between the distribution agreement and the legal structures of other agreements.
Voltage-Controlled Low-Energy Switching of Nanomagnets through Ruderman-Kittel-Kasuya-Yosida Interactions for Magnetoelectric Device Applications
Creators: name: Ghosh, Bahniman
name: Dey, Rik
name: Register, Leonard F.
name: Banerjee, Sanjay K.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: In this letter, we consider through simulation Ruderman-Kittel-Kasuya-Yosida (RKKY) interactions between nanomagnets sitting on a conductive surface, and voltage-controlled gating thereof for low-energy switching of nanomagnets for possible memory and nonvolatile logic applications. For specificity, we consider nanomagnets with perpendicular anisotropy on a three-dimensional topological insulator. We model the possibility and dynamics of RKKY-based switching of one nanomagnet by coupling to one or more nanomagnets of set orientation. Applications for both memory and nonvolatile logic are considered, with follower, inverter and majority gate functionality shown. Sub-attojoule switching energies, far below conventional spin transfer torque (STT)-based memories and even below CMOS logic appear possible. Switching times on the order of a few nanoseconds, comparable to times for STT switching, are estimated for ferromagnetic nanomagnets.
description: 6 pages,4 figures
Additional file 1 of Happy people live longer because they are healthy people
Creators: name: Song, Cai Feng
name: Tay, Peter Kay Chai
name: Gwee, Xinyi
name: Wee, Shiou Liang
name: Ng, Tze Pin
Publisher: name: figshare
Year: 2023
Subjects: subject: Medicine
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
classificationCode: 69999
subject: Biological Sciences not elsewhere classified
subject: Science Policy

description: Additional file 1.
Nature of helicity injection in non-erupting solar active regions
Creators: name: Vemareddy, P.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Using time-sequence vector magnetic field and coronal observations from \textit{Solar Dynamics Observatory}, we report the observations of the magnetic field evolution and coronal activity in four emerging active regions (ARs). The ARs emerge with leading polarity being the same as for the majority of ARs in a hemisphere of solar cycle 24. After emergence, the magnetic polarities separate each other without building a sheared polarity inversion line. In all four ARs, the magnetic fields are driven by foot point motions such that the sign of the helicity injection ($dH/dt$) in the first half of the evolution is changed to the opposite sign in the later part of the observation time. This successive injection of opposite helicity is also consistent with the sign of mean force-free twist parameter ($α_{av}$). Further, the EUV light curves of the ARs in 94Å~and GOES X-ray flux reveal flaring activity below C-class magnitude. Importantly, the white-light coronagraph images in conjunction with the AR images in AIA 94 Å~delineate the absence of associated CMEs with the studied ARs. These observations imply that the ARs with successive injection of opposite sign magnetic helicity are not favorable to twisted flux rope formation with excess coronal helicity, and therefore are unable to launch CMEs, according to recent reports. This study provides the characteristics of helicity flux evolution in the ARs referring to the conservative property of magnetic helicity and more such studies would help to quantify the eruptive capability of a given AR.
description: 9 pages, 6 Figures, accepted to publish in MNRAS
Why are flare ribbons associated with the spines of magnetic null points generically elongated?
Creators: name: Pontin, D. I.
name: Galsgaard, K.
name: Demoulin, P.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Coronal magnetic null points exist in abundance as demonstrated by extrapolations of the coronal field, and have been inferred to be important for a broad range of energetic events. These null points and their associated separatrix and spine field lines represent discontinuities of the field line mapping, making them preferential locations for reconnection. This field line mapping also exhibits strong gradients adjacent to the separatrix (fan) and spine field lines, that can be analysed using the `squashing factor', $Q$. In this paper we make a detailed analysis of the distribution of $Q$ in the presence of magnetic nulls. While $Q$ is formally infinite on both the spine and fan of the null, the decay of $Q$ away from these structures is shown in general to depend strongly on the null-point structure. For the generic case of a non-radially-symmetric null, $Q$ decays most slowly away from the spine/fan in the direction in which $|{\bf B}|$ increases most slowly. In particular, this demonstrates that the extended, elliptical high-$Q$ halo around the spine footpoints observed by Masson et al. (Astrophys. J., 700, 559, 2009) is a generic feature. This extension of the $Q$ halos around the spine/fan footpoints is important for diagnosing the regions of the photosphere that are magnetically connected to any current layer that forms at the null. In light of this, we discuss how our results can be used to interpret the geometry of observed flare ribbons in `circular ribbon flares', in which typically a coronal null is implicated. We conclude that both the physics in the vicinity of the null and how this is related to the extension of $Q$ away from the spine/fan can be used in tandem to understand observational signatures of reconnection at coronal null points.
description: Pre-print version of article accepted for publication in Solar Physics
АНАЛИЗ ФОРМ ВОВЛЕЧЕНИЯ НАСЕЛЕНИЯ В МЕСТНОЕ САМОУПРАВЛЕНИЕ В Г. ВЛАДИВОСТОКЕ И ЕГО АГЛОМЕРАЦИИ
Creators: name: ДМИТРОВ АЛЕКСАНДР ИГОРЕВИЧ
Publisher: name: StudNet
Year: 2020
Subjects: МЕСТНОЕ САМОУПРАВЛЕНИЕ
ПУБЛИЧНЫЕ СЛУШАНИЯ
ТЕРРИТОРИАЛЬНОЕ ОБЩЕСТВЕННОЕ САМОУПРАВЛЕНИЕ
АГЛОМЕРАЦИЯ
ГРАЖДАНСКАЯ ИНИЦИАТИВА
LOCAL GOVERNMENT
PUBLIC HEARINGS
TERRITORIAL PUBLIC SELF-GOVERNMENT
AGGLOMERATION
CIVIC INITIATIVE

description: На сегодняшний день, местное самоуправление является одним из значимых элементов в государстве, а в активности местного сообщества и его взаимодействии с муниципальной властью заложен перспективный потенциал для эффективного развития муниципальных образований. В статье проводится анализ таких форм вовлечения населения в местное самоуправления, как публичные слушания и территориальное общественное самоуправление, на примере г. Владивостока и его агломерации.Today, local self-government is one of the significant elements in the state, and the potential of the local community in the activity of the local community and its interaction with the municipal authorities lies in the effective development of municipalities. The article discusses such forms of involving the population in local self-government as public hearings and territorial public self-government, using the example of Vladivostok and its agglomeration.
Save the world with innovation? Open scholarship is the key!
Creators: name: Paglione, Laura
Publisher: name: Zenodo
Year: 2023

description: Throughout history, changes in how research is conducted and shared have resulted in significant increases in innovation that have benefited society. How we communicate research and scholarship has been functionally unchanged since the mid-1600s when scientific societies were first formed, and the scholarly journal was born. With the advent of electronic publishing, open scholarship, and formal research artifact sharing, we are just at the start of a scholarly communication evolution that could drive solutions to our most pressing global challenges, including climate change, new diseases, and uneven societal opportunity. But this impact is not a given. With history as our guide, we will consider the necessary characteristics that the next scholarly communication evolution must possess to facilitate explosive innovation to save the world. And, we will explore the role of open infrastructure as a foundation for this scholarship transformation.
An Incoercible E-Voting Scheme Based on Revised Simplified Verifiable Re-encryption Mix-nets
Creators: name: Tamura, Shinsuke
name: Haddad, Hazim A.
name: Islam, Nazmul
name: Alam, Kazi Md. Rokibul
Publisher: name: arXiv
Year: 2015
Subjects: subject: Cryptography and Security (cs.CR)
subject: FOS: Computer and information sciences

description: Simplified verifiable re-encryption mix-net (SVRM) is revised and a scheme for e-voting systems is developed based on it. The developed scheme enables e-voting systems to satisfy all essential requirements of elections. Namely, they satisfy requirements about privacy, verifiability, fairness and robustness. It also successfully protects voters from coercers except cases where the coercers force voters to abstain from elections. In detail, voters can conceal correspondences between them and their votes, anyone can verify the accuracy of election results, and interim election results are concealed from any entity. About incoercibility, provided that erasable-state voting booths which disable voters to memorize complete information exchanged between them and election authorities for constructing votes are available, coercer C cannot know candidates that voters coerced by C had chosen even if the candidates are unique to the voters. In addition, elections can be completed without reelections even when votes were handled illegitimately.
ОСОБЕННОСТИ РАЗВИТИЯ КОНТЕЙНЕРНЫХ ПЕРЕВОЗОК
Creators: name: СУЛТАНОВА Ш.М.
name: РОМАНОВ К.И.
name: КОРОТКИХ Н.В.
Publisher: name: StudNet
Year: 2020
Subjects: ПЕРЕВОЗКИ
ГРУЗОПОТОК
ОПЕРАТОРЫ КОНТЕЙНЕРНЫХ ПЕРЕВОЗОК
МОРСКИЕ ЛИНИИ
КОНТЕЙНЕРЫ
ЛОГИСТИЧЕСКИЕ ОПЕРАТОРЫ
SHIPMENTS
GOODS FLUE
FORWARDERS CONTAINERS
SHIPPING LINES

description: Статья посвящена анализу нынешнего состояния рынка контейнерных перевозок. Проанализированы тенденции развития таких перевозок. Рассмотрены особенности развития контейнерных перевозок на территории России на основе Стратегии транспортного развития Российской Федерации до 2030 года. Проанализирован современный этап развития контейнеризации, выявлены его особенности, а также отличительные признаки предприятий, функционирующих на рынке контейнерных перевозок в условиях новой экономики.The article is devoted to the analysis of the current state of the container transportation market. The development trends of such transportations are analyzed. The features of the development of container transportation in Russia on the basis of the Transport Development Strategy of the Russian Federation until 2030 are considered. The current stage of the development of containerization is analyzed, its features are revealed, as well as the distinguishing features of enterprises operating in the container transportation market in the new economy.
ГРАЖДАНСКАЯ ДЕЕСПОСОБНОСТЬ НЕСОВЕРШЕННОЛЕТНИХ
Creators: name: ШАГИВАЛИЕВА И.Д.
Publisher: name: StudNet
Year: 2020
Subjects: ДЕЕСПОСОБНОСТЬ
НЕСОВЕРШЕННОЛЕТНИЕ
ГРАЖДАНСКОЕ ЗАКОНОДАТЕЛЬСТВО
ОТВЕТСТВЕННОСТЬ
ЭМАНСИПАЦИЯ
LEGAL CAPACITY
MINORS
CIVIL LAW
RESPONSIBILITY
EMANCIPATION

description: Статья посвящена правовой регламентации дееспособности несовершеннолетних. Рассматриваются условия объявления несовершеннолетних полностью дееспособным, степень дееспособности, вопрос об объеме дееспособности данной категории физических лиц. Рассматриваются правоспособность и дееспособность. Раскрываются понятия правоспособности, дееспособности, ограниченной дееспособности и недееспособности. Также дается характеристика такого способа получения преждевременно дееспособности, как эмансипация.The article is devoted to the legal regulation of the legal capacity of minors. It considers the conditions for declaring minors fully capable, the degree of legal capacity, the issue of the legal capacity of this category of individuals. Legal capacity is considered. The concepts of legal capacity, legal capacity, limited legal capacity and incapacity are disclosed. Also, a characteristic of such a method of obtaining premature capacity, such as emancipation, is given.
The regulation of male fertility : studies of the mechanism of hormonal contraception
Creators: name: Matthiesson., Kati
Publisher: name: Monash University
Year: 2021

description: This thesis was scanned from the print manuscript for digital preservation and is copyright the author.
 Researchers can access this thesis by asking their local university, institution or public library to
 make a request on their behalf. Monash staff and postgraduate students can use the link in the References field.
Active Galactic Nuclei signatures in Red Geyser galaxies from Gemini GMOS-IFU observations
Creators: name: Ilha, G. S.
name: Riffel, R. A.
name: Ricci, T. V.
name: Rembold, S. B.
name: Storchi-Bergmann, T.
name: Riffel, R.
name: Roy, N.
name: Bundy, K.
name: Nemmen, R.
name: Schimoia, J. S.
name: da Costa, L. N.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Red Geysers are quiescent galaxies with galactic scale ionised outflows, likely due to low-luminosity Active Galactic Nuclei (AGN). We used Gemini GMOS-IFU observations of the inner $\sim 1.0-3.0$ kpc of nine Red Geysers selected from the MaNGA survey to study the gas ionisation and kinematics. The emission-line ratios suggest the presence of Seyfert/LINER (Low Ionisation Nuclear Emission Region) nuclei in all sources. Two galaxies show H$α$ equivalent width (H$α$ EW) larger than 3 Å(indicative of AGN ionisation) within an aperture 2.5 arcsec of diameter ($1.3-3.7$ kpc at the distance of galaxies) for MaNGA data, while with the higher resolution GMOS data, four galaxies present H$α$ EW$>3$ Åwithin an aperture equal to the angular resolution ($0.3-0.9$ kpc). For two objects with GMOS-IFU data, the H$α$ EW is lower than 3 Åbut larger than 1.5 Å, most probably due to a faint AGN. The spatially resolved electron density maps show values between $100-3000$ cm$^{-3}$ and are consistent with those determined in other studies. The large (MaNGA) and the nuclear scale (GMOS-IFU) gas velocity fields are misaligned, with a kinematic position angle difference between 12$^{\circ}$ and 60$^{\circ}$. The [NII]$λ$6583 emission-line profiles are asymmetrical, with blue wings on the redshifted side of the velocity field and red wings on the blueshifted side. Our results support previous indications that the gas in Red Geysers is ionised by an AGN, at least in their central region, with the presence of outflows, likely originating in a precessing accretion disc.
description: Accepted for publication in August 3, 2022
Electronic Structure, Phase Stability and Resistivity of Hybrid Hexagonal C$_x$(BN)$_{1-x}$ Two-dimensional Nanomaterial: A First-principles Study
Creators: name: D'Souza, Ransell
name: Mukherjee, Sugata
Publisher: name: arXiv
Year: 2016
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: We use density functional theory based first-principles method to investigate the bandstructure and phase stability in the laterally grown hexagonal C$_x$(BN)$_{1-x}$, two-dimensional Graphene and $h$-BN hybrid nanomaterials, which were synthesized by experimental groups recently (Liu $et al$, Nature Nanotech, 8, 119 (2013)). Our detail electronic structure calculations on such materials, with both armchair and zigzag interfaces between the Graphene and $ h$-BN domains, indicate that the band-gap decreases non-monotonically with the concentration of Carbon. The calculated bandstructure shows the onset of Dirac cone like features near the band-gap at high Carbon concentration ($x \sim 0.8$). From the calculated energy of formation, the phase stability of C$_x$(BN)$_{1-x}$ was studied using a regular solution model and the system was found to be in the ordered phase below a few thousand Kelvin. Furthermore, using the Boltzmann transport theory we calculate the electrical resistivity from the bandstrcture of C$_x$(BN)$_{1-x}$ at different temperature ($T$), which shows a linear behaviour when plotted in the logarithmic scale against $T^{-1}$, as observed experimentally
description: 10 pages, 5 figures
ОСОБЫЕ ЭКОНОМИЧЕСКИЕ ЗОНЫ КАК ПРИМЕР ПРИВЛЕЧЕНИЯ ИНВЕСТИЦИЙ И РЕГИОНАЛЬНОГО РАЗВИТИЯ МЕКСИКИ И РОССИИ
Creators: name: ГАРСИЯ МАНЧА Х
Publisher: name: StudNet
Year: 2020
Subjects: ОСОБЫЕ ЭКОНОМИЧЕСКИЕ ЗОНЫ
ИНВЕСТИЦИИ
НАЛОГООБЛОЖЕНИЕ
РЕГИОНАЛЬНОЕ РАЗВИТИЕ
УСТОЙЧИВОЕ РАЗВИТИЕ
ПИИ
SPECIAL ECONOMIC ZONES
INVESTMENTS
TAXATION
REGIONAL DEVELOPMENT
SUSTAINABLE DEVELOPMENT
FDI

description: В данной статье подчеркивается экономический потенциал Мексики и России в использовании особых экономических зон для развития большей открытости для иностранного капитала и, в свою очередь, повышения инвестиционной привлекательности обеих стран. Также в статье выделены основные проблемы функционирования особых экономических зон в России и Мексике, проведена оценка их влияния на инновационное развитие промышленности, а также на формирование уровня инвестиционной привлекательности.This article emphasizes the economic potential of Mexico and Russia in using special economic zones to develop greater openness to foreign capital and, in turn, increase the investment attractiveness of both countries. The article also highlights the main problems of the functioning of special economic zones in Russia and Mexico, assesses their impact on the innovative development of industry, as well as on the formation of the level of investment attractiveness.
Characterizing the Daytime Sextantids Meteor Shower and Unveiling the Nature of the Phaethon-Geminid Stream Complex
Creators: name: Kipreos, Y.
name: Campbell-Brown, Margaret
name: Brown, P.
name: Vida, D.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: The Daytime Sextantids meteor shower, part of the Phaethon-Geminid Stream Complex (PGC), is closely related to the Geminids, currently the strongest meteor shower visible at the Earth. The DSX share a similar orbit to asteroid 2005 UD, but the nature of the association remains unclear. From optical data we find that DSX meteors ablate similarly to Geminids, suggesting that they are also high density and consistent with a common origin. From radar data we have isolated 19,007 DSX orbits through application of a novel convex hull approach to determine stream membership. We find at the peak the mean semi-major axis is near 1 AU, eccentricity is 0.86 and that both decrease as a function of solar longitude. The inclination averages 25 degrees at the peak but increases over time. Noticeable DSX activity extends from solar longitude 173-196$^{\circ}$ with a flux plateau between 186 - 189$^{\circ}$. The peak flux is $2 \pm 0.05 \times 10^{-3}$ km$^{-2}$ hr$^{-1}$, equivalent to a ZHR of 20. We estimate a true differential mass index for the shower of $s = 1.64 \pm 0.06$ at the time of peak and an average of $1.70 \pm 0.07$ for days surrounding the peak. The mass of the DSX stream is estimated to be $10^{16}$ g, the same order as 2005 UD, suggesting the stream is too massive to have been created by recent meteoroid production from 2005 UD. We propose that the DSX and 2005 UD were created in the same break-up event that created 3200 Phaethon.
description: Accepted for publication at Monthly Notices of the Royal Astronomical Society (MNRAS)
Salacia brunoniana Wight & Arn. 1834
Creators: name: Jadhav, Durga C.
name: Prabhugaonkar, Ashish V.
name: Nandikar, Mayur D.
Publisher: name: Zenodo
Year: 2016
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Celastrales
Celastraceae
Salacia
Salacia brunoniana

description: 2. Salacia brunoniana Wight & Arn. (1834: 105)
 Type:— INDIA, Peninsular India, s.d., Herb Wight 347 [lectotype, E (E00174243, image! Fig. 2), designated here; syntype, K (K000669920, image!)].
 Wight and Arnott (1834) described Salacia brunoniana, based on collection of Robert Wight (Herb Wight 347). There are two herbarium specimens at E and K which bears no. 347 that are collected by Wight. From these specimens, the material deposited in E (E 00174243) has annotated by Wight and best matches with protologue and is designated here as lectotype and the duplicate at K (K 000669920) kept as syntype.
description: Published as part of Jadhav, Durga C., Prabhugaonkar, Ashish V. & Nandikar, Mayur D., 2016, Nomenclature notes on the genus Salacia L. (Celastraceae) in India, pp. 121-130 in Phytotaxa 265 (2) on page 122, DOI: 10.11646/phytotaxa.265.2.3, http://zenodo.org/record/13662647
Bubble nuclei: single-particle versus Coulomb interaction effects
Creators: name: Perera, U. C.
name: Afanasjev, A. V.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: The detailed investigation of microscopic mechanisms leading to the formation of bubble structures in the nuclei has been performed in the framework of covariant density functional theory. The main emphasis of this study is on the role of single-particle degrees of freedom and Coulomb interaction. In general, the formation of bubbles lowers the Coulomb energy. However, in nuclei this trend is counteracted by the quantum nature of the single-particle states: only specific single-particle states with specific density profiles can be occupied with increasing proton and neutron numbers. A significant role of central classically forbidden region at the bottom of the wine bottle potentials in the formation of nuclear bubbles (via primarily the reduction of the densities of the $s$ states at $r=0$) has been revealed for the first time. Their formation also depends on the availability of low-$l$ single-particle states for occupation since single-particle densities represent the basic building blocks of total densities. Nucleonic potentials disfavor the occupation of such states in hyperheavy nuclei and this contributes to the formation of bubbles in such nuclei. Additivity rule for densities has been proposed for the first time. It was shown that the differences in the densities of bubble and flat density nuclei follow this rule in the $A\approx 40$ mass region and in superheavy nuclei with comparable accuracy. This strongly suggests the same mechanism of the formation of central depression in bubble nuclei of these two mass regions. Nuclear saturation mechanisms and self-consistency effects also affect the formation of bubble structures. The detailed analysis of different aspects of bubble physics strongly suggests that the formation of bubble structures in superheavy nuclei is dominated by single-particle effects.
description: 25 pages, 23 figures, Physical Review C, in press
Computation Methods for combinatorial sums and Euler type numbers related to new families of numbers
Creators: name: Simsek, Yilmaz
Publisher: name: arXiv
Year: 2016
Subjects: subject: Number Theory (math.NT)
subject: FOS: Mathematics

description: The aim of this article is to define some new families of the special numbers. These numbers provide some further motivation for computation of combinatorial sums involving binomial coefficients and the Euler kind numbers of negative order. We can show that these numbers are related to the well-known numbers and polynomials such as the Stirling numbers of the second kind and the central factorial numbers, the array polynomials, the rook numbers and polynomials, the Bernstein basis functions and others. In order to derive our new identities and relations for these numbers, we use a technique including the generating functions and functional equations. Finally, we not only give a computational algorithm for these numbers, but also some numerical values of these numbers and the Euler numbers of negative order with tables. We also give some combinatorial interpretations of our new numbers.
description: arXiv admin note: text overlap with arXiv:1604.05601
Characterization of polymorphie 37 base pair insert within the alcohol dehydrogenase gene of Drosophila melanogaster
Creators: name: Matthew., Paul
Publisher: name: Monash University
Year: 2021

description: This thesis was scanned from the print manuscript for digital preservation and is copyright the author.
 Researchers can access this thesis by asking their local university, institution or public library to
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Additional file 1 of The impact of assisted reproductive technology treatment coverage on marriage, pregnancy, and childbirth in women of childbearing age: an interrupted time-series analysis
Creators: name: Yun, Il
name: Cha, Wontae
name: Nam, Chung-Mo
name: Nam, Jin Young
name: Park, Eun-Cheol
Publisher: name: figshare
Year: 2023
Subjects: Cell Biology
Biotechnology
Science Policy

description: Supplementary Material 1
The cold gas and dust properties of red star-forming galaxies
Creators: name: Chown, Ryan
name: Parker, Laura C.
name: Wilson, Christine D.
name: Brown, Toby
name: Evans, Fraser A.
name: Gao, Yang
name: Hwang, Ho Seong
name: Lin, Lihwai
name: Saintonge, Amelie
name: Sargent, Mark
name: Smith, Matthew W. L.
name: Xiao, Ting
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We study the cold gas and dust properties for a sample of red star forming galaxies called "red misfits." We collect single-dish CO observations and HI observations from representative samples of low-redshift galaxies, as well as our own JCMT CO observations of red misfits. We also obtain SCUBA-2 850 um observations for a subset of these galaxies. With these data we compare the molecular gas, total cold gas, and dust properties of red misfits against those of their blue counterparts ("blue actives") taking non-detections into account using a survival analysis technique. We compare these properties at fixed position in the log SFR-log M* plane, as well as versus offset from the star-forming main sequence. Compared to blue actives, red misfits have slightly longer molecular gas depletion times, similar total gas depletion times, significantly lower molecular- and total-gas mass fractions, lower dust-to-stellar mass ratios, similar dust-to-gas ratios, and a significantly flatter slope in the $\log M_\mathrm{mol}$-$\log M_\star$ plane. Our results suggest that red misfits as a population are likely quenching due to a shortage in gas supply.
description: 16 pages, 7 Figures, accepted to MNRAS
Fast nodal precession of the disc around Pleione requires a broken disc
Creators: name: Martin, Rebecca G.
name: Lepp, Stephen
Publisher: name: arXiv
Year: 2022
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Pleione is a Be star that is in a 218 day orbit with a low-mass binary companion. Recent numerical simulations have shown that a Be star disc can be subject to breaking when material is actively being fed into the inner parts of the disc. After breaking, the disc is composed of two rings: an inner ring that is anchored to the stellar equator and an outer ring that is free to nodally precess. A double ring disc may explain some of the observed variability in Pleione. We model the nodal precession of the outer disc ring that is driven by the companion on an observed timescale of $80.5\,\rm yr$. We find that the outer ring of a broken disc in a binary with an eccentricity of $e_{\rm b}= 0.6$ can precess on the observed timescale and have an outer radius that is in rough agreement with the observed disc size. An unbroken disc model cannot fit both the observed precession rate and disc size. Suppression of Kozai-Lidov driven disc eccentricity is more likely for a high binary eccentricity if the disc extends to the tidal truncation radius.
description: Accepted for publication in MNRAS Letters
Salacia floribunda Wight 1838
Creators: name: Jadhav, Durga C.
name: Prabhugaonkar, Ashish V.
name: Nandikar, Mayur D.
Publisher: name: Zenodo
Year: 2016
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Celastrales
Celastraceae
Salacia
Salacia floribunda

description: 3. Salacia floribunda Wight (1838: 134)
 Type:— MYANMAR, Tanintharyi Region, Mergui, s.d., Griffith, s.n. [lectotype, K (K000687005, image! Fig. 3), designated here; other syntypes: K (K0007004, image!), E (E00179088, image!), CAL! (CAL0000007473), MH! (sh. no. 10323)].
 Salacia floribunda was described by Wight based on material collected from Mergui by William Griffith. In the protologue no type has been mentioned apart from ‘Mergui:- communicated by Griffith’. In total five collections by Griffith and annotated by Wight were found deposited at E, K, CAL and MH. Two collections from K matching with protologue and are presumably collected from the same locality by Griffith; one of these is agrees protologue and designated here as lectotype (K000687005), while the other is kept as syntype. Even though the specimens placed at CAL (CAL0000007473), MH (sh. no 10323) and E (E00179088) are collected by Griffith and annotated by Wight, they are ambiguous with protologue and kept as syntypes.
description: Published as part of Jadhav, Durga C., Prabhugaonkar, Ashish V. & Nandikar, Mayur D., 2016, Nomenclature notes on the genus Salacia L. (Celastraceae) in India, pp. 121-130 in Phytotaxa 265 (2) on page 124, DOI: 10.11646/phytotaxa.265.2.3, http://zenodo.org/record/13662647
Formation of the penumbra and start of the Evershed flow
Creators: name: Murabito, M.
name: Romano, P.
name: Guglielmino, S. L.
name: Zuccarello, F.
name: Solanki, S. K.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We studied the variations of line-of-sight photospheric plasma flows during the formation phase of the penumbra around a pore in Active Region NOAA 11490. We used a high spatial, spectral, and temporal resolution data set acquired by the Interferometric BIdimensional Spectrometer (IBIS) operating at the NSO/Dunn Solar Telescope as well as data taken by the Helioseismic and Magnetic Imager onboard the Solar Dynamics Observatory satellite (SDO/HMI). Before the penumbra formed we observed a redshift of the spectral line in the inner part of the annular zone surrounding the pore as well as a blueshift of material associated with opposite magnetic polarity further away from the pore. We found that the onset of the classical Evershed flow occurs in a very short time scale -- 1-3 hours -- while the penumbra is forming. During the same time interval we found changes in the magnetic field inclination in the penumbra, with the vertical field actually changing sign near the penumbral edge, while the total magnetic field showed a significant increase, about 400 G. To explain these and other observations related to the formation of the penumbra and the onset of the Evershed flow we propose a scenario in which the penumbra is formed by magnetic flux dragged down from the canopy surrounding the initial pore. The Evershed flow starts when the sinking magnetic field dips below the solar surface and magnetoconvection sets in.
description: Accepted for ApJ
БЕЗДОГОВОРНОЕ ИСПОЛЬЗОВАНИЕ АУДИОВИЗУАЛЬНЫХ ПРОИЗВЕДЕНИЙ В СФЕРЕ КИНЕМАТОГРАФИИ
Creators: name: ДАШКИНА АЛИЯ ЗАГИДУЛЛОВНА
Publisher: name: StudNet
Year: 2020
Subjects: КИНЕМАТОГРАФИЯ
АВТОРСКОЕ ПРАВО
АУДИОВИЗУАЛЬНЫЕ ПРОИЗВЕДЕНИЯ
ПРАВО НА ПЕРЕРАБОТКУ
АЛЛЮЗИЯ
ПЛАГИАТ
CINEMATOGRAPHY
COPYRIGHT
AUDIO-VISUAL WORKS
REWORKING
ALLUSION
PLAGIARISM

description: Аудиовизуальное произведение произведение, состоящее из зафиксированной серии связанных между собой изображений и предназначенное для зрительного и слухового восприятия с помощью соответствующих технических устройств. В статье рассматриваются допустимые пределы использования аудиовизуальных произведений, приемы, обладающие свободным бездоговорным режимом использования, и специфика разграничения этих приемов от плагиата как гражданско-правого деликта.Audiovisual work a work consisting of a fixed series of interconnected images and intended for visual and auditory perception using appropriate technical devices. The article deals with permitted limits of using the audio-visual works, methods possessing free non-contract usage mode and specificity in the distinctions between these methods and plagiarism deliction.
Core-collapse supernovae in dense environments -- particle acceleration and non-thermal emission
Creators: name: Brose, Robert
name: Sushch, Iurii
name: Mackey, Jonathan
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Supernova remnants are known to accelerate cosmic-rays from the detection of non-thermal emission in radio waves, X-rays, and gamma-rays. However, the ability to accelerate cosmic-rays up to PeV energies has yet to be demonstrated. The presence of cut-offs in the gamma-ray spectra of several young SNRs led to the idea that PeV energies might only be achieved during the first years of a remnant's evolution. We use our time-dependent acceleration-code RATPaC to study the acceleration of cosmic-rays in supernovae expanding into dense environments around massive stars. We performed spherically symmetric 1-D simulations in which we simultaneously solve the transport equations for cosmic-rays, magnetic turbulence, and the hydrodynamical flow of the thermal plasma in the test-particle limit. We investigated typical CSM parameters expected around RSG and LBV stars for freely expanding winds and accounted for the strong gamma-gamma-absorption in the first days after explosion. The maximum achievable particle energy is limited to below 600TeV even for largest considered values of the magnetic field and mass-loss rates. The maximum energy is not expected to surpass 200TeV and 70TeV for LBVs and RSGs that experience moderate mass-loss prior to the explosion. We find gamma-ray peak-luminosities consistent with current upper limits and evaluated that current-generation instruments are able to detect the gamma-rays from Type-IIP explosions at distances up to 60kpc and Type-IIn explosions up to 1.0Mpc. We also find a good agreement between the thermal X-ray and radio synchrotron emission predicted by our models with a range of observations.
description: 14 pages, 8 figures, accepted to MNRAS
Health Systems Barriers to Cancer Care in Sub-Saharan Africa: A scoping review
Creators: name: Karanja, Grace
Publisher: name: Open Science Framework
Year: 2023
Subjects: subject: Social and Behavioral Sciences
subject: Medicine and Health Sciences
subject: Health Policy and Systems
subject: Health Policy Planning and Fiinancing
subject: Cancer Care in sub-Saharan Africa
subject: Health Equity

description: This scoping review aimed to synthesise evidence on health system barriers and deficiencies that impact access to quality cancer care in sub-Saharan Africa. The author conducted a search of multiple databases for relevant studies published between 2000-2020. They included quantitative and qualitative studies that examined health system challenges related to cancer care delivery in sub-Saharan African countries. Key findings from the 19 included studies highlighted deficiencies across all six building blocks of the health system framework defined by WHO. Specifically, the review found limited health financing for cancer, shortages in health workforce and training, inadequate access to essential cancer medicines and technologies, poor information systems for cancer data collection, challenges with service delivery models and referral systems, and suboptimal governance and leadership regarding cancer care policies in the region. Overall, the scoping review synthesises evidence that sub-Saharan African health systems currently have critical gaps in their capacity, resources and infrastructure to equitably meet the rising burden of cancer. The author advocates that addressing these health system barriers will be essential to improve access, quality and outcomes of cancer care for patients across sub-Saharan Africa.
The effect of ionizing background fluctuations on the spatial correlations of high redshift Ly$α$-emitting galaxies
Creators: name: Meiksin, Avery
name: Suarez, Teresita
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We investigate the possible influence of fluctuations in the metagalactic photoionizing ultra-violet background (UVBG) on the clustering of Ly$α$-emitting galaxies through the modulation of the ionization level of the gas surrounding the systems. At redshifts $z > 5$, even when assuming the reionization of the intergalactic medium has completed, the fluctuations are sufficiently large that they may non-negligibly enhance, and possibly even dominate, the angular correlation function on scales up to a few hundred arcsecs. Whilst a comparison with observations at $z \sim 5.7$ is statistically consistent with no influence of UVBG fluctuations, allowing for the fluctuations opens up the range of acceptable models to include those with relatively low bias factors for the Ly$α$-emitting galaxies. In this case, the evolution in the bias factor of Ly$α$-emitters over the approximate redshift range $3 < z < 7$ corresponds to a nearly constant halo mass for Ly$α$-emitting galaxies of $\sim 10^{10.5}\,M_\odot$.
description: 11 pages, 8 figures; accepted for publication in MNRAS