cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
ГЛОБАЛИЗАЦИЯ И ЭКОНОМИЧЕСКОЕ РАЗВИТИЕ
Creators: name: Успаева Милана Гумкиевна
name: Гачаев Ахмед Магомедович
Publisher: name: Международный журнал прикладных наук и технологий «Integral»
Year: 2020
Subjects: ГЛОБАЛИЗАЦИЯ
ВЛИЯНИЕ
ЭКОНОМИЧЕСКОЕ РАЗВИТИЕ
GLOBALIZATION
INFLUENCE
ECONOMIC DEVELOPMENT

description: Доктринальный подход к сущности и оценке такого феномена как глобализация является неоднозначным с точки зрения ее позитивного или негативного влияния на развитие человечества. С одной стороны, осуществляют толкование глобализации как объективного, закономерного процесса, который охватывает экономику, культуру и другие сферы жизни общества. С другой она рассматривается как искусственное, насильственное явление, формируется под давлением развитых стран и особенно ТНК с целью удовлетворения собственных потребностей и интересов. Первая теория отталкивается от закономерностей развития внутренних и международных экономических систем и рассматривает глобализацию как необходимый, ярко выраженный, неизбежный процесс, вызванный экономическими и политическими факторами. Согласно конъюнктурной концепции главные черты глобализации определяются отдельной политикой и обстоятельствами, которые зависят от изменения условий внутреннего и внешнего окружений, их взаимодействия в пространстве и времени из-за уникальной конфигурации социальных сил и исторических предпосылок. Такая глобализация может иметь дискретный, прерывчастый характер, из-за которой могут развиваться и обратные процессы так называемая деглобализация. Это и показывает отдельные эпизоды человеческой истории, когда некоторые страны и регионы были долгое время отгорожены от экономического общения с остальным миром. Конструктивистская теория базируется на идеях, которые характеризуют глобализацию как случайный, стохастический, непредсказуемый процесс, что обусловлено коммуникативным дискурсом политических агентов, содержанием которого является мотивации, интересы, идеи.
Covariance and gauge invariance in relativistic theories of gravity
Creators: name: Papini, Giorgio
Publisher: name: arXiv
Year: 2014
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: Any metric theory of gravity whose interaction with quantum particles is described by a covariant wave equation is equivalent to a vector theory that satisfies Maxwell-type equations identically. This result does not depend on any particular set of field equations for the metric tensor, but only on covariance. It is derived in the linear case, but can be extended to any order of approximation in the metric deviation. In this formulation of the interaction of gravity with matter, angular momentum and momentum are conserved locally.
description: 8 pages, to appear in Modern Physics Letters A
Evaluation Of New Towns In The Context Of A National Human Settlements Strategy For Algeria Arising From A Critical Study Of New Town Developments In Britain, France And Egypt
Creators: name: Hamaizia, Mohamed
Publisher: name: London South Bank University
Year: 1989

description: This thesis evaluates new towns in the context of a National Human Settlements Strategy for Algeria, with special reference to the new provincial capital, Oum El Bouaghi as a case study. It arises from a critical study of new town developments in Britain, France and Egypt. The concepts of ‘social balance’ and ‘’self-containment’ used in British New Towns as Terms of Reference have been adopted as basic criteria for evaluating new towns. The study is made up of two parts, each consisting of three and four Chapters respectively. The first part is made up of the three following Chapters. Chapter I presents the objectives of the study. Chapter II reviews the British, French and Egyptian new towns, and concludes with a comparative review by presenting their similarities and their differences. Chapter III focuses upon national and regional development and considers the new towns idea in Algeria since the French occupation in 1830. In the second part, Chapter IV introduces’ the research methods used for gathering both primary and secondary data. A questionnaire survey was designed to evaluate Oum El Bouaghi new provincial capital in terms of ‘social balance’ and ‘’self-containment’. The development of Oum El Bouaghi has in many cases been based on an existing town like those of the third generation of British new towns (1966 onwards) which were designated to create a focal point for economic growth. This Chapter also reviews the questionnaire, proposes a sample for further research, describes the problems encountered in carrying out a survey in a developing country such as Algeria. Chapter V provides a detailed description of the case study town, Oum El Bouaghi with some criticisms and suggestions based on the lessons learnt from British, French and Egyptian new towns. Chapter VI illustrates the different stages involved in the analysis of both primary and secondary data gathered through the pilot study in the light of the two selected concepts of ‘social balance’ and ‘'self-containment’ with reference to the theoretical writings on British, French and Egyptian new towns. Chapter VII concludes that a literature review has been restricted to areas of comparative studies. It also concludes that the concepts of ‘social balance’ and ‘'self containment’ go hand-in-hand and can be applied in a developing country such as Algeria. However, this study develops a research methodology for a later Ph.D.
A Small Step, a Big Jump: GoTriple and Linked Open Data
Creators: name: Bertozzi, Alessandro
Publisher: name: Zenodo
Year: 2023
Subjects: Open Science
Linked Open Data
TRIPLE
FAIR
Open Data

description: Data today are everywhere. Despite this large amount of data, the use of good data publication practices, such as Linked Open Data, is only just beginning. This research has the goal of connecting GoTriple to the Web of Data through the use of Linked Data. Two macro steps are required: defining an ontology, based on GoTriple's existing data model and extending its APIs to expose serialized data in JSON-LD, a W3C recommended format. Achieving this goal would bring several benefits to GoTriple: matching the best practices of the leading European platforms for digital cultural heritage management; achieving the highest level in the scale of Tim Berners-Lee's 5-star scheme on Linked Open Data; reducing duplication of information by connecting with external resources; facilitating users and researchers in content discovery; connecting with authoritative metadata sources (e.g. Confederation of Open Access Repositories, Library of Congress); reuse of GoTriple's data in other external projects, resulting in an expansion of users; increased quality of content, resulting in improved user experience; more efficient use of resources, due to the ability of users to add or reuse GoTriple's metadata; and achievement of most FAIR principles, including interoperability, reusability, and findability. This research sets itself the fundamental task of adapting GoTriple to the standards, trusted and supported by the Linked Open Data community at the European level. It is not only a theoretical work: as part of the development team of Net7, I'll present the actual implementation of these ideas that I was able to apply on the GoTriple platform.
description: The TRIPLE project has received funding from the European Union's Horizon 2020 research and innovation programme under grant agreement No 863420 Disclaimer. The content of this publication is the sole responsibility of the author and can in no way be taken to reflect the views of the European Commission. The European Commission is not responsible for any use that may be made of the information it contains.
Synthetic photometry for carbon-rich giants. IV. An extensive grid of dynamic atmosphere and wind models
Creators: name: Eriksson, Kjell
name: Nowotny, Walter
name: Höfner, Susanne
name: Aringer, Bernhard
name: Wachter, Astrid
Publisher: name: arXiv
Year: 2014
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: The evolution and spectral properties of stars on the AGB are significantly affected by mass loss through dusty stellar winds. Dynamic atmosphere and wind models are an essential tool for studying these evolved stars, both individually and as members of stellar populations, to understand their contribution to the integrated light and chemical evolution of galaxies. This paper is part of a series testing state-of-the-art atmosphere and wind models of carbon stars against observations, and making them available for use in various theoretical and observational studies. We have computed low-resolution spectra and photometry (in the wavelength range 0.35-25 mu) for a grid of 540 dynamic models with stellar parameters typical of solar-metallicity C-rich AGB stars and with a range of pulsation amplitudes. The models cover the dynamic atmosphere and dusty outflow (if present), assuming spherical symmetry, and taking opacities of gas-phase species and dust grains consistently into account. To characterize the time-dependent dynamic and photometric behaviour of the models in a concise way we defined a number of classes for models with and without winds. Comparisons with observed data in general show a quite good agreement for example regarding mass-loss rates vs. (J-K) colours or K magnitudes vs. (J-K) colours. Some exceptions from the good overall agreement, however, are found and attributed to the range of input parameters (e.g. relatively high carbon excesses) or intrinsic model assumptions (e.g. small particle limit for grain opacities). While current results indicate that some changes in model assumptions and parameter ranges should be made in the future to bring certain synthetic observables into better agreement with observations, it seems unlikely that these pending improvements will significantly affect the mass-loss rates of the models.
description: 28 pages, 15 figures. Table B.1, an 11-page table, is only available at CDS
Impact of climate on Odonata traits
Creators: name: Haque, Md Tangigul
Publisher: name: Macquarie University
Year: 2022
Subjects: Other education not elsewhere classified

description: Insects exhibit diverse colours between and within species that may function in thermoregulation, mate signalling, and predator-prey interactions. Variation in climate along latitudinal gradients may impact insects’ traits such as body size and colour. We quantified several phenotypic traits and asked whether variation in these traits can be explained by latitude and local climatic factors (temperature, precipitation, and humidity). We collected Australian odonate photographs from online databases, and measured colour and sexual dichromatism. Furthermore, we measured odonate body size and sexual size dimorphism. Bioclimatic variables were extracted from WorldClim and the Australian Government Bureau of Meteorology databases. Body size of odonates followed Bergmann’s (body size increases with latitude) and Rensch’s rule (sexual size dimorphism increases with body size when males are larger and decreases with body size when females are larger). We also found a significant correlation between precipitation and male body size. Moreover, body colour of odonates had no relationship with any of our predictors whereas precipitation, humidity, and body size were strongly correlated with sexual dichromatism. Overall, our study provides insight into how climatic factors relate to insect traits and will highlight the consequences of such variations under the changing climate.
Simultaneous NuSTAR and XMM-Newton 0.5-80 keV spectroscopy of the Narrow Line Seyfert 1 galaxy SWIFT J2127.4+5654
Creators: name: Marinucci, A.
name: Matt, G.
name: Kara, E.
name: Miniutti, G.
name: Elvis, M.
name: Arevalo, P.
name: Ballantyne, D. R.
name: Balokovic, M.
name: Bauer, F.
name: Brenneman, L.
name: Boggs, S. E.
name: Cappi, M.
name: Christensen, F. E.
name: Craig, W. W.
name: Fabian, A. C.
name: Fuerst, F.
name: Hailey, C. J.
name: Harrison, F. A.
name: Risaliti, G.
name: Reynolds, C. S.
name: Stern, D. K.
name: Walton, D. J.
name: Zhang, W.
Publisher: name: arXiv
Year: 2014
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present a broad band spectral analysis of the joint XMM-Newton and NuSTAR observational campaign of the Narrow Line Seyfert 1 SWIFT J2127.4+5654, consisting of 300 ks performed during three XMM-Newton orbits. We detect a relativistic broadened iron K$α$ line originating from the innermost regions of the accretion disc surrounding the central black hole, from which we infer an intermediate spin of $a$=$0.58^{+0.11}_{-0.17}$. The intrinsic spectrum is steep ($Γ=2.08\pm0.01$) as commonly found in Narrow Line Seyfert 1 galaxies, while the cutoff energy (E$_{\rm c}=108^{+11}_{-10}$ keV) falls within the range observed in Broad Line Seyfert 1 Galaxies. We measure a low-frequency lag that increases steadily with energy, while at high frequencies, there is a clear lag following the shape of the broad Fe K emission line. Interestingly, the observed Fe K lag in SWIFT J2127.4+5654 is not as broad as in other sources that have maximally spinning black holes. The lag amplitude suggests a continuum-to-reprocessor distance of about $ 10-20\ r_{\mathrm{g}}$. These timing results independently support an intermediate black hole spin and a compact corona.
description: 11 pages, 10 figures, accepted for publication on MNRAS
Tettigettalna acoustic diversity
Creators: name: Mendes, Raquel
name: L. Nunes, Vera
name: Marabuto, Eduardo
name: J. Costa, Gonçalo
name: E. Silva, Sara
name: S. Paulo, Octávio
name: Simões, Paula
Publisher: name: Zenodo
Year: 2022

description: Divergence in acoustic signals may have a crucial role in the speciation process of animals that rely on sound for intra-specific recognition and mate attraction. The acoustic adaptation hypothesis (AAH) postulates that signals should diverge according to the physical properties of the signaling environment. To be efficient, signals should maximize transmission and decrease degradation. To test which drivers of divergence, exert the most influence in a speciose group of insects, we used a phylogenetic approach to the evolution of acoustic signals in the cicada genus Tettigettalna, investigating the relationship between acoustic traits (and their mode of evolution) and body size, climate, and micro/ macro-habitat usage. Different traits showed different evolutionary paths. While acoustic divergence was generally independent of phylogenetic history, some temporal variables' divergence was associated with genetic drift. We found support for ecological adaptation at the temporal but not the spectral level. Temporal patterns are correlated with micro- and macro-habitat usage and temperature stochasticity in ways that run against the AAH predictions, degrading signals more easily. These traits are likely to have evolved as an anti-predator strategy in conspicuous environments and low-density populations. Our results support a role of ecological selection, not excluding a likely role of sexual selection in the evolution of Tettigettalna calling songs, which should be further investigated in an integrative approach.
description: Funding provided by: Foundation for Science and Technology
Crossref Funder Registry ID: http://dx.doi.org/10.13039/501100019370
Award Number: PTDC/BIA-BIC/115511/2009Funding provided by: Foundation for Science and Technology
Crossref Funder Registry ID: http://dx.doi.org/10.13039/501100019370
Award Number: PD/BD/106040/2015Funding provided by: Centre for Ecology, Evolution and Environmental Changes*
Crossref Funder Registry ID:
Award Number: UID/BIA/00329/2013
Relics of Galaxy Merging: Observational Predictions for a Wandering Massive Black Hole and Accompanying Star Cluster in the Halo of M31
Creators: name: Kawaguchi, Toshihiro
name: Saito, Yuriko
name: Miki, Yohei
name: Mori, Masao
Publisher: name: arXiv
Year: 2014
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Galaxies and massive black holes (BHs) presumably grow via galactic merging events and subsequent BH coalescence. As a case study, we investigate the merging event between the Andromeda galaxy (M31) and a satellite galaxy. We compute the expected observational appearance of the massive BH that was at the center of the satellite galaxy prior to the merger, and is currently wandering in the M31 halo. We demonstrate that a radiatively inefficient accretion flow with a bolometric luminosity of a few tens of solar luminosities develops when Hoyle-Lyttleton accretion onto the BH is assumed. We compute the associated broadband spectrum and show that the radio band (observable with EVLA, ALMA and SKA) is the best frequency range to detect the emission. We also evaluate the mass and the luminosity of the stars bound by the wandering BH and find that such a star cluster is sufficiently luminous that it could correspond to one of the star clusters found by the PAndAS survey. The discovery of a relic massive BH wandering in a galactic halo will provide a direct means to investigate in detail the coevolution of galaxies and BHs. It also means a new population of BHs (off-center massive BHs), and offers targets for clean BH imaging that avoids strong interstellar scattering in the center of galaxies.
description: 5 pages, 3 figures, Accepted for publication in ApJL
Erste Frühjahrs-Schule der Sektion Biologiedidaktik im Verband Deutscher Biologen (vdbiol)
Creators: name: Schröer, Thomas
name: Vogt, Helmut
Publisher: name: Zeitschrift für Didaktik der Biologie (ZDB) - Biologie Lehren und Lernen
Year: 2003

description: Vom 19. bis 21. März 1999 fand in Münster mit großem Erfolg die erste nationale Frühjahrs-Schule zur Förderung des Nachwuchses in der Biologiedidaktik statt. Diese Veranstaltung wurde initiiert von Dr. Thomas Schröer und Dr. Helmut Vogt in Zusammenarbeit mit der Sektion Biologiedidaktik im Verband Deutscher Biologen. Das Ministerium für Schule und Weiterbildung, Wissenschaft und Forschung des Landes Nordrhein-Westfalen hat die Durchführung finanziell unterstützt und den Teilnehmern einen Reisekostenzuschuss gezahlt. Neben einem Gastvortrag von Herrn Prof. Dr. Ulrich Kattmann mit dem Thema „Didaktische Rekonstruktion“ berichtete ein Teil der Teilnehmer in Kurzvorträgen über ihre Forschungsvorhaben und stellte diese zur Diskussion. Nachfolgend werden die Kurzfassungen der Beiträge dieses Nachwuchses abgedruckt. Dabei muss berücksichtigt werden, dass ein Teil der Vorhaben erst am Anfang der Bearbeitung bzw. Entwicklung steht und durch die Diskussion bei der Frühjahrs-Schule eine Unterstützung erfahren sollte und auch erhielt. (Die Beiträge von Barbara Wieder und Astrid Kleine sind als Artikel im vorderen Teil dieser Ausgabe von IDB abgedruckt.) Neben der Erfahrung durch die Diskussionen wurden auch etliche wertvolle Kontakte geknüpft. Einhellige Meinung unter den Teilnehmern war, dass diese Veranstaltung unbedingt im jährlichen Rhythmus fortgeführt werden sollte. Im Jahr 2000 findet noch einmal die Frühjahrs-Schule in Münster statt, bevor sie dann in darauffolgenden Jahren in anderen Orten durchgeführt werden soll.
description: Zeitschrift für Didaktik der Biologie (ZDB) - Biologie Lehren und Lernen, Vol 8 (1999)
Dobischat, Rolf, Elias, Arne & Rosendahl, Anna (Hrsg.). (2018). Das Personal in der Weiterbildung. Im Spannungsfeld von Professionsanspruch und Beschäftigungsrealität. Wiesbaden: Springer VS.
Creators: name: Meyer, Kirsten
Publisher: name: Zeitschrift Hochschule und Weiterbildung (ZHWB)
Year: 2019

description: Zeitschrift Hochschule und Weiterbildung (ZHWB), 2019/2: Steuerung in der wissenschaftlichen Weiterbildung
The Kepler map in the three-body problem
Creators: name: Shevchenko, Ivan I.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Chaotic Dynamics (nlin.CD)
subject: FOS: Physical sciences

description: The Kepler map was derived by Petrosky (1986) and Chirikov and Vecheslavov (1986) as a tool for description of the long-term chaotic orbital behaviour of the comets in nearly parabolic motion. It is a two-dimensional area-preserving map, describing the motion of a comet in terms of energy and time. Its second equation is based on Kepler's third law, hence the title of the map. Since 1980s the Kepler map has become paradigmatic in a number of applications in celestial mechanics and atomic physics. It represents an important kind of general separatrix maps. Petrosky and Broucke (1988) used refined methods of mathematical physics to derive analytical expressions for its single parameter. These methods became available only in the second half of the 20th century, and it may seem that the map is inherently a very modern mathematical tool. With the help of the Jacobi integral I show that the Kepler map, including analytical formulae for its parameter, can be derived by quite elementary methods. The prehistory and applications of the Kepler map are considered and discussed.
description: 18 pages
Collapse and fragmentation of molecular clouds under pressure
Creators: name: Zubovas, Kastytis
name: Sabulis, Kostas
name: Naujalis, Rokas
Publisher: name: arXiv
Year: 2014
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Recent analytical and numerical models show that AGN outflows and jets create ISM pressure in the host galaxy that is several orders of magnitude larger than in quiescent systems. This pressure increase can confine and compress molecular gas, thus accelerating star formation. In this paper, we model the effects of increased ambient ISM pressure on spherically symmetric turbulent molecular clouds. We find that large external pressure confines the cloud and drives a shockwave into it, which, together with instabilities behind the shock front, significantly accelerates the fragmentation rate. The compressed clouds therefore convert a larger fraction of their mass into stars over the cloud lifetime, and produce clusters that are initially more compact. Neither cloud rotation nor shear against the ISM affect this result significantly, unless the shear velocity is higher than the sound speed in the confining ISM. We conclude that external pressure is an important element in the star formation process, provided that it dominates over the internal pressure of the cloud.
description: 20 pages, 9 figures. Accepted for publication in MNRAS
Safer Transits or Legal Oblivion for Syrian Refugees?
Creators: name: Javed, Hassan
name: Yordanova, Maria
name: Stoyanova, Maria
Publisher: name: Zenodo
Year: 2022
Subjects: perceptions
narratives
migration
safer transit
legal oblivion

description: The 2016 EU-Turkey Statement and the succeeding 2021 Greek Joint Ministerial Decision have affected refugee ambitions to seek better lives in Europe. The former outlines procedures for returning irregular migrant arrivals from Greece to Turkey to stop the flow of irregular migration from Turkey to Europe and prevent in-transit deaths in the Aegean Sea; meanwhile, the latter has declared Turkey a safe third country, restricting European asylum eligibility for refugees from Syria, Afghanistan, Somalia, Pakistan and Bangladesh. As a result, the number of irregular refugees reaching the EU from the Aegean Sea and the Balkan Route has dropped significantly. Yet, on the other hand, the impact of these legal instruments on refugee safety has been criticized. Turkey has begun to renege on its responsibilities per the EU-Turkey Statement, leaving some refugees in limbo, while the EU has struggled to resettle enough refugees and provide them with safe, legal ways of entry. Meanwhile, the Joint Ministerial Decision does not consider how Syrian refugees face refoulement and xenophobic violence in Turkey, overlooking the threat to their lives and livelihoods. As such, this policy brief discusses what impacts the EU-Turkey Statement and the Joint Ministerial Decision have had since their implementation and how their negative consequences can be lessened through five policy recommendations, including placing Turkey under a European sanctions and monitoring mechanism, repealing the Joint Ministerial Decision to acknowledge the threats refugees face in Turkey, and activating the Voluntary Humanitarian Admissions Scheme to increase the number of resettled Syrian refugees.
The Gemini Planet Imager: First Light
Creators: name: Macintosh, Bruce
name: Graham, James R.
name: Ingraham, Patrick
name: Konopacky, Quinn
name: Marois, Christian
name: Perrin, Marshall
name: Poyneer, Lisa
name: Bauman, Brian
name: Barman, Travis
name: Burrows, Adam
name: Cardwell, Andrew
name: Chilcote, Jeffrey
name: De Rosa, Robert J.
name: Dillon, Daren
name: Doyon, Rene
name: Dunn, Jennifer
name: Erikson, Darren
name: Fitzgerald, Michael
name: Gavel, Donald
name: Goodsell, Stephen
name: Hartung, Markus
name: Hibon, Pascale
name: Kalas, Paul G.
name: Larkin, James
name: Maire, Jerome
name: Marchis, Franck
name: Marley, Mark
name: McBride, James
name: Millar-Blanchaer, Max
name: Morzinski, Katie
name: Norton, Andew
name: Oppenheimer, B. R.
name: Palmer, Dave
name: Patience, Jennifer
name: Pueyo, Laurent
name: Rantakyro, Fredrik
name: Sadakuni, Naru
name: Saddlemyer, Leslie
name: Savransky, Dmitry
name: Serio, Andrew
name: Soummer, Remi
name: Sivaramakrishnan, Anand
name: Song, Inseok
name: Thomas, Sandrine
name: Wallace, J. Kent
name: Wiktorowicz, Sloane
name: Wolff, Schuyler
Publisher: name: arXiv
Year: 2014
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: The Gemini Planet Imager (GPI) is a dedicated facility for directly imaging and spectroscopically characterizing extrasolar planets. It combines a very high-order adaptive optics system, a diffraction-suppressing coronagraph, and an integral field spectrograph with low spectral resolution but high spatial resolution. Every aspect of GPI has been tuned for maximum sensitivity to faint planets near bright stars. During first light observations, we achieved an estimated H band Strehl ratio of 0.89 and a 5-sigma contrast of $10^6$ at 0.75 arcseconds and $10^5$ at 0.35 arcseconds. Observations of Beta Pictoris clearly detect the planet, Beta Pictoris b, in a single 60-second exposure with minimal post-processing. Beta Pictoris b is observed at a separation of $434 \pm 6$ milli-arcseconds and position angle $211.8 \pm 0.5$ deg. Fitting the Keplerian orbit of Beta Pic b using the new position together with previous astrometry gives a factor of three improvement in most parameters over previous solutions. The planet orbits at a semi-major axis of $9.0^{+0.8}_{-0.4}$ AU near the 3:2 resonance with the previously-known 6 AU asteroidal belt and is aligned with the inner warped disk. The observations give a 4% posterior probability of a transit of the planet in late 2017.
description: 9 pages, 5 figures, accepted for publication Proc. Natl. Acad. Sci
Liability of Internet Service Providers for Hate Speech in Migration Contexts
Creators: name: Mora Gonzalez, Jesus Ivan
Publisher: name: Zenodo
Year: 2022
Subjects: perceptions
narratives
migration
hate speech

description: The purpose of this policy brief is to analyse the liability of internet service providers in cases of hate speech directed towards the migrant population, with the aim of protecting all parties on the internet. In the European Union, liability of internet service providers is regulated by the E-Commerce Directive and covers several services, such as transmission, catching, or data hosting, which are key for platforms such as Facebook, Twitter, Youtube, Amazon, or Ebay. Internet users rely on these services, but such services can also be used to commit crimes. This situation requires a deep study on liability to develop clear normative criteria for cases where platforms are used by third parties. However, liability must be established in a balanced way, taking into account the fundamental rights assessment of the different parties involved.
European Literary Bibliography: Aggregation and Harmonization of Literary Bibliographical Data
Creators: name: Hubar, Patryk
name: Giersz, Marcin
Publisher: name: Zenodo
Year: 2023
Subjects: open science
semantic web
linked open data
bibliography

description: The main objective of the speech is to present the European Literary Bibliography service (ELB, literarybibliography.eu) as an aggregator of various literary bibliographic data and to show the main assumptions when binding and unifying diverse data sets with different structures. The aim of the ELB service is to collect, merge and provide one interface to present multilingual bibliographical metadata for literary studies, created based on the principles of Linked Open Data and Semantic Web standards. We would like to present the results of work related to the creation of a common data model and data processing workflow for records acquired from different resources, such as the Czech Literary Bibliography, the Polish Literary Bibliography, and the literary content extracted from the National Library of Finland. It was primarily necessary to unify the bibliographic data on authors, source documents, and subject and genre description systems using interoperable external data sources, e.g. VIAF, Geonames and Wikidata. Due to the specificity of the service and plans to expand its content with further national data sources, the workflow for data aggregation is designed in such a way that it can accommodate more data sources. We will also present the future of ELB service, in particular, further work on data harmonization and enrichment, creation of a RDF-based data model and implementation of graph database.
description: The TRIPLE project has received funding from the European Union's Horizon 2020 research and innovation programme under grant agreement No 863420 Disclaimer. The content of this publication is the sole responsibility of the authors and can in no way be taken to reflect the views of the European Commission. The European Commission is not responsible for any use that may be made of the information it contains.
Mismatched: Migrant Housing
Creators: name: Riachi, Catherine
name: Javed, Hassan
name: Yordanova, Maria
Publisher: name: Zenodo
Year: 2022
Subjects: perceptions
narratives
migration
migrant housing

description: Migrants across the world arrive in Europe to seek better lives from civil wars and economic and political instabilities, often perceiving the continent as a beacon of prosperity, health, and safety. However, the realities of migrant housing mismatch with their optimistic ideals. In comparison to EU nationals, foreign migrants are disproportionately exposed to poor living conditions - such as mould, inadequate fire safety, and overcrowding - and face exploitation in the housing market with overburdening rent prices and abrupt evictions. Through a combination of government allocation policies and economic pressures, migrants are commonly forced to live in underserved neighbourhoods where lack of investment in public infrastructure, healthcare, and education, as well as high petty crimes rates, often take place. These neighbourhoods tend to be characterised by poor public transit connectivity, spatial segregation and ghettoization processes, which severely impact migrants’ access to social and economic opportunities as well as their right to vote. As such, this policy brief discusses how inadequate housing conditions result in a mismatch between migrants’ expectations of Europe and their lived experiences, and what can be done about it.
D1.2 FAIRCORE4EOSC Technical Specifications
Creators: name: Suominen, Tommi
name: Atzori, Claudio
name: Baglioni, Miriam
name: Tsapelas, Christos
name: Katsogiannis, George
name: Chatzopoulos, Serafeim
name: Vergoulis, Thanasis
name: Eleftherakis, Stavroula
name: Manghi, Paolo
name: Iatropoulou, Katerina
name: Galouni, Konstantina
name: Wimalaratne, Sarala
name: Kesäniemi, Joonas
name: Broeder, Daan
name: Bingert, Sven
name: Ariyo, Chris
name: Lienhop, Hans
name: Tolley, Shorn
name: Leney, Rob
name: Liffers, Matthias
name: MCCafferly, Siobhan
name: Barlow., Melanie
name: Simons, Natasha
name: Zamani, Themis
name: Holm Nielsen, Lars
name: Hugo, Wim
name: Steinhoff, Wilko
name: Wagner, Michael
name: Elbers, Willem
name: Ahmed, Ramy-Badr
name: Monteil, Alain
name: Medves, Maud
name: Azzouz, Maxence
name: Schubotz, Moritz
name: Snyder, Kyle
name: van de Sanden, Mark
name: Tatum, Clifford
name: Widmann, Heinrich
name: Gruenpeter, Morane
name: Märkälä, Anu
name: Kauranen, Pihla
Publisher: name: Zenodo
Year: 2023
Subjects: EOSC
Open Science
EOSC-Core

description: The FAIRCORE4EOSC project started in June 2022 and will deliver nine new EOSC-Core components in support of a FAIR research life cycle, bridging the gaps identified in the EOSC SRIA. More specifically, the components will enable an EOSC PID infrastructure, an EOSC research software infrastructure, support for sharing and access to metadata schemas and crosswalks and offer advanced research-intent driven discovery services over all EOSC repositories.
This deliverable summarises the overall technical specifications for the FAIRCORE4EOSC components. The deliverable is a snapshot of the input received from WP2, WP3, WP4, WP5, WP6 and WP7 via the milestones at M7. This deliverable will be further updated during the project duration on the project wiki to take into account new requirements and feedback received. The Wiki page that this deliverable is derived from automatically mirrors updates to the content provided by the work packages.
Reentrant quantum spin Hall effect in the presence of an exchange field
Creators: name: Cheng, Xiaoyu
name: Zheng, Xiaohong
name: Chen, Jun
name: Xiao, Liantuan
name: Jia, Suotang
name: Zhang, Lei
Publisher: name: arXiv
Year: 2023
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: Driven by various physical origins, the interesting reentrant phenomena in quantum Hall effect (QHE), quantum anomalous Hall effect (QAHE) and non-Hermitian systems have been discussed recently. Here, we present that the reentrant phenomena of quantum spin Hall effect (QSHE) can be achieved by introducing a uniform exchange field into a topological insulator with a four-band model Hamiltonian. Furthermore, it is found that both time-reversal (TR) symmetry broken QSHE and spin-polarized QAHE can simultaneously be generated in the system with proper exchange field strength by inspecting the corresponding edge states. Through analyzing the energy dependent spin-Chern number $ν_s$ and transmission in the presence of random disorders, we verify the topological protection and the robustness of induced QSHE and QAHE. Finally, the theoretical realization of reentrant QSHE in a topolectrical circuit is demonstrated. Our work not only extends the reentrant phenomena into the QSHE but also stimulates interest in their realization in different systems.
description: 4 figures
Analysis of potential energy and cost savings of replacing air-cooled chillers with water-cooled chillers: A case study in hotel building in tropical climate
Creators: name: Arka Dwinanda Soewono
name: Kusmanto, Ivan Agustinus
name: Darmawan, Marten
name: Tobing, Sheila
Publisher: name: Faculty of Engineering, Khon Kaen University
Year: 2023
Subjects: Chiller
Cooling load
Energy saving
Life-cycle cost
Carbon emission

description: Engineering and Applied Science Research, 50, 4, 372-381
Noether-Lefschetz locus and a special case of the variational Hodge conjecture
Creators: name: Dan, Ananyo
Publisher: name: arXiv
Year: 2014
Subjects: subject: Algebraic Geometry (math.AG)
subject: FOS: Mathematics
subject: 14C30, 14D07

description: For a fixed integer $d$, we study here the locus of degree $d$ hypersurfaces $X$ in $\mathbb{P}^{2n+1}$ such that $H^{2n}(X,\mathbb{Q}) \cap H^{n,n}(X,\mathbb{C}) \not= \mathbb{Q}$. We call this locus \textit{the Noether-Lefschetz locus}. Any irreducible component of this locus is locally a Hodge locus. So, we see that the study of this locus is very closely related to the variational Hodge conjecture. In this article we show that the Hodge locus corresponding to the cohomology class of a complete intersection subscheme in $\mathbb{P}^{2n+1}$ of codimension $n+1$ and degree less than $d$ satisfies the variational Hodge conjecture. The interesting part is that we use techniques from commutative algebra to prove this statement (after certain identifications coming from Hodge theory). In the case $n=1$, we use similar methods to characterize all non-reduced components of the Noether-Lefschetz locus of codimension less than or equal to $3d$.
description: 11 pages
Preparing for the AI Act
Creators: name: Lewis, Dave
Publisher: name: Zenodo
Year: 2023
Subjects: EU AI Act, AI risk management, harmonised standards, AI Act Compliance, AI standards conformance

description: A briefing for ML practitioners on the potential impact of the EU's proposed AI Act on AI developers, the risk management apporach taken, the status of the current legislative and associated technical standards development processes and some the the relevant research to support practitioners from the PROTECTm ADAPT and EMPOWER research programmes.
Modelling the 3D morphology and proper motions of the planetary nebula NGC 6302
Creators: name: Uscanga, L.
name: Velázquez, P. F.
name: Esquivel, A.
name: Raga, A. C.
name: Boumis, P.
name: Cantó, J.
Publisher: name: arXiv
Year: 2014
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We present 3D hydrodynamical simulations of an isotropic fast wind interacting with a previously ejected toroidally-shaped slow wind in order to model both the observed morphology and the kinematics of the planetary nebula (PN) NGC 6302. This source, also known as the Butterfly nebula, presents one of the most complex morphologies ever observed in PNe. From our numerical simulations, we have obtained an intensity map for the H$α$ emission to make a comparison with the Hubble Space Telescope (HST) observations of this object. We have also carried out a proper motion (PM) study from our numerical results, in order to compare with previous observational studies. We have found that the two interacting stellar wind model reproduces well the morphology of NGC 6302, and while the PM in the models are similar to the observations, our results suggest that an acceleration mechanism is needed to explain the Hubble-type expansion found in HST observations.
description: 5 pages, 3 figures. Accepted by MNRAS
The width of a chaotic layer
Creators: name: Shevchenko, Ivan I.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Chaotic Dynamics (nlin.CD)
subject: FOS: Physical sciences

description: A model of nonlinear resonance as a periodically perturbed pendulum is considered, and a new method of analytical estimating the width of a chaotic layer near the separatrices of the resonance is derived for the case of slow perturbation (the case of adiabatic chaos). The method turns out to be successful not only in the case of adiabatic chaos, but in the case of intermediate perturbation frequencies as well.
description: 27 pages, 8 figures
Comments as reviews: Predicting answer acceptance by measuring sentiment on stack exchange
Creators: name: IV, William Chase Ledbetter
Publisher: name: Purdue University Graduate School
Year: 2023
Subjects: Affective computing
Natural language processing

description: Online communication has increased the need to rapidly interpret complex emotions due to the volatility of the data involved; machine learning tasks that process text, such as sentiment analysis, can help address this challenge by automatically classifying text as positive, negative, or neutral. However, while much research has focused on detecting offensive or toxic language online, there is also a need to explore and understand the ways in which people express positive emotions and support for one another in online communities. This is where sentiment dictionaries and other computational methods can be useful, by analyzing the language used to express support and identifying common patterns or themes.
 This research was conducted by compiling data from social question and answering around machine learning on the site Stack Exchange. Then a classification model was constructed using binary logistic regression. The objective was to discover whether predictions of marked solutions are accurate by treating the comments as reviews. Measuring collaboration signals may help capture the nuances of language around support and assistance, which could have implications for how people understand and respond to expressions of help online. By exploring this topic further, researchers can gain a more complete understanding of the ways in which people communicate and connect online.
Canonical methods of constructing invariant tori by phase-space sampling
Creators: name: Laakso, Teemu
name: Kaasalainen, Mikko
Publisher: name: arXiv
Year: 2014
Subjects: subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences
subject: 70H07, 70H15, 70K43, 65P10, 85A05

description: Invariant tori in phase space can be constructed via a nonperturbative canonical transformation applied to a known integrable Hamiltonian H. Hitherto, this process has been carried through with H corresponding to the isochrone potential and the harmonic oscillator. In this paper, we expand the applicability regime of the torus construction method by demonstrating that H can be based on a Stäckel potential, the most general known form of an integrable potential. Also, we present a simple scheme, based on phase space sampling, for recovering the angle variables on the constructed torus. Numerical examples involving axisymmetric galactic potentials are given.
Stellar rotation--planetary orbit period commensurability in the HAT-P-11 system
Creators: name: Béky, Bence
name: Holman, Matthew J.
name: Kipping, David M.
name: Noyes, Robert W.
Publisher: name: arXiv
Year: 2014
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: A number of planet-host stars have been observed to rotate with a period equal to an integer multiple of the orbital period of their close planet. We expand this list by analyzing Kepler data of HAT-P-11 and finding a period ratio of 6:1. In particular, we present evidence for a long-lived spot on the stellar surface that is eclipsed by the planet in the same position four times, every sixth transit. We also identify minima in the out-of-transit lightcurve and confirm that their phase with respect to the stellar rotation is mostly stationary for the 48-month timeframe of the observations, confirming the proposed rotation period. For comparison, we apply our methods to Kepler-17 and confirm the findings of Bonomo & Lanza (2012) that the period ratio is not exactly 8:1 in that system. Finally, we provide a hypothesis on how interactions between a star and its planet could possibly result in an observed commensurability for systems where the stellar differential rotation profile happens to include a period at some latitude which is commensurable to the planetary orbit.
description: Accepted for publication in ApJ. 10 pages, 7 figures
Quantum Measurement Complexity
Creators: name: Kak, Subhash
Publisher: name: arXiv
Year: 2014
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: This paper explores the problem of quantum measurement complexity. In computability theory, the complexity of a problem is determined by how long it takes an effective algorithm to solve it. This complexity may be compared to the difficulty for a hypothetical oracle machine, the output of which may be verified by a computable function but cannot be simulated on a physical machine. We define a quantum oracle machine for measurements as one that can determine the state by examining a single copy. The complexity of measurement for a realizable machine will then be respect to the number of copies of the state that needs to be examined. A quantum oracle cannot perform simultaneous exact measurement of conjugate variables, although approximate measurement may be performed as circumscribed by the Heisenberg uncertainty relations. When considering the measurement of a variable, there might be residual uncertainty if the number of copies of the variable is limited. Specifically, we examine the quantum measurement complexity of linear polarization of photons that is used in several quantum cryptography schemes and we present a relation using information theoretic arguments. The idea of quantum measurement complexity is likely to find uses in measurements in biological systems.
description: 12 pages, 3 figures
The impact of UK immigration policies on the anti-modern slavery agenda
Creators: name: Le Louvier, Kahina
name: Latricia Hough, Karen
Publisher: name: Zenodo
Year: 2022
Subjects: perceptions
narratives
migration
UK immigration policies
anti-modern slavery

description: With 69% of referrals to the UK’s modern slavery identification and support system coming from non-UK nationals,i modern slavery appears to be closely linked to international migration. Indeed, while historical slavery was abolished, systems of exploitation have remained that ‘reflect an industrialised and increasingly globalised world where the migration of labour – almost half of it female – to new, strange contexts makes it more vulnerable to enslavement’.ii Yet, if the two phenomena are connected, the UK approached them in contrary ways. With the Modern Slavery Act 2015, the UK sought to take an internationally leading role in the fight against modern slavery, putting it on the global policy agenda and enacting a landmark piece of legislation to address it. At the same time, the UK continued to intensify its criminalising approach to immigration. Yet, as we show in this policy brief, hostile immigration policies that restrict entry to the UK and limit the legal, economic and social rights on migrants, including asylum seekers and survivors of modern slavery, have created vulnerabilities for people to fall into or remain in exploitative situations that undermine the success of the Modern Slavery Act. To effectively address modern slavery, a victim-centred approach is needed that shifts the focus from rescue to prevention by implementing human rights based immigration policies that mitigate the vulnerabilities leading individuals to exploitation, and by placing more emphasis on the role of businesses and financial institutions. In 2022, Home Secretaries have framed survivors of modern slavery as ‘abusers’ and trafficking as a matter that should be dealt with through stronger immigration enforcement. Modern slavery was therefore moved away from the minister for safeguarding to the minister for immigration in the Home Office. As these criminalising approaches to immigration and modern slavery continue to grow to new levels in the UK as well as in other European countries, it is important to highlight their impact on the increase of exploitative and undermining of international efforts to combat modern slavery. This brief contributes to this effort for highlighting research-informed policy alternatives.
New general integral inequalities for Lipschitzian functions via Hadamard fractional integrals
Creators: name: Iscan, Imdat
Publisher: name: arXiv
Year: 2013
Subjects: subject: Classical Analysis and ODEs (math.CA)
subject: FOS: Mathematics
subject: 26A33, 26A51, 26D15

description: In this paper, the author obtains new estimates on generalization of Hadamard, Ostrowski and Simpson type inequalities for Lipschitzian functions via Hadamard fractional integrals. Some applications to special means of positive reals numbers are also given.
description: 12 pages