cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Electrohydrodynamic & surface acoustic wave-driven microfluidic actuation
Creators: name: Raghavan, Rohan Veera.
Publisher: name: Monash University
Year: 2022

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.
Swarm Intelligence for Multiobjective Optimization of Extraction Process
Creators: name: Ganesan, T.
name: Elamvazuthi, I.
name: Vasant, P.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Neural and Evolutionary Computing (cs.NE)
subject: Artificial Intelligence (cs.AI)
subject: FOS: Computer and information sciences

description: Multi objective (MO) optimization is an emerging field which is increasingly being implemented in many industries globally. In this work, the MO optimization of the extraction process of bioactive compounds from the Gardenia Jasminoides Ellis fruit was solved. Three swarm-based algorithms have been applied in conjunction with normal-boundary intersection (NBI) method to solve this MO problem. The gravitational search algorithm (GSA) and the particle swarm optimization (PSO) technique were implemented in this work. In addition, a novel Hopfield-enhanced particle swarm optimization was developed and applied to the extraction problem. By measuring the levels of dominance, the optimality of the approximate Pareto frontiers produced by all the algorithms were gauged and compared. Besides, by measuring the levels of convergence of the frontier, some understanding regarding the structure of the objective space in terms of its relation to the level of frontier dominance is uncovered. Detail comparative studies were conducted on all the algorithms employed and developed in this work.
Orbital eccentricities in primordial black holes binaries
Creators: name: Cholis, Ilias
name: Kovetz, Ely D.
name: Ali-Haïmoud, Yacine
name: Bird, Simeon
name: Kamionkowski, Marc
name: Muñoz, Julian B.
name: Raccanelli, Alvise
Publisher: name: arXiv
Year: 2016
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: It was recently suggested that the merger of $\sim30\,M_\odot$ primordial black holes (PBHs) may provide a significant number of events in gravitational-wave observatories over the next decade, if they make up an appreciable fraction of the dark matter. Here we show that measurement of the eccentricities of the inspiralling binary black holes can be used to distinguish these binaries from those produced by more traditional astrophysical mechanisms. These PBH binaries are formed on highly eccentric orbits and can then merge on timescales that in some cases are years or less, retaining some eccentricity in the last seconds before the merger. This is to be contrasted with massive-stellar-binary, globular-cluster, or other astrophysical origins for binary black holes (BBHs) in which the orbits have very effectively circularized by the time the BBH enters the observable LIGO window. Here we discuss the features of the gravitational-wave signals that indicate this eccentricity and forecast the sensitivity of LIGO and the Einstein Telescope to such effects. We show that if PBHs make up the dark matter, then roughly one event should have a detectable eccentricity given LIGO's expected sensitivity and observing time of six years. The Einstein Telescope should see $O(10)$ such events after ten years.
description: 13 pages, 8 figures, 3 tables and 1 appendix
The 6 $μ$m Feature as A Tracer of Aliphatic Components of Interstellar Carbonaceous Grains
Creators: name: Hsia, Chih-Hao
name: Sadjadi, Seyedabdolreza
name: Zhang, Yong
name: Kwok, Sun
Publisher: name: arXiv
Year: 2016
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: An unidentified infrared emission (UIE) feature at 6.0 $μ$m is detected in a number of astronomical sources showing the UIE bands. In contrast to the previous suggestion that this band is due to C=O vibrational modes, we suggest that the 6.0 $μ$m feature arises from olefinic double-bond functional groups. These groups are likely to be attached to aromatic rings which are responsible for the major UIE bands. The possibility that the formation of these functional groups is related to the hydrogenation process is discussed.
description: 43 pages, 15 figures, accepted for publication in the Astrophysical Journal
The Government of the Sangha According to the Sappurisdharn Principle of the Abbot In Prachantakham District, Prachanburi Province
Creators: name: Phra Adirek Ushujaro (Na Nakornpanom)
Publisher: name: DR.KET INSTITUTE OF ACADEMIC DEVELOPMENT AND PROMOTION
Year: 2023
Subjects: Sangha Administration
Sappurisadhamma
Abbot

description: Journal of Interdisciplinary Social Development, 1, 4, 15-28
Sonnenfleckenzeichnung Nr. 157.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 02.07.1981, 14:00, erstellt von Sergio Cortesi, Sonnenobservatorium Specola Solare Ticinese in Locarno
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1981

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf dem Vordruck der Eidgenössischen Sternwarte Zürich. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 4.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)
Sonnenfleckenzeichnung Nr. 120.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 21.05.1981, 07:30, erstellt von Sergio Cortesi, Sonnenobservatorium Specola Solare Ticinese in Locarno
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1981

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf dem Vordruck der Eidgenössischen Sternwarte Zürich. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 3.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)
Microencapsulation of water-soluble bioactive particles
Creators: name: Abubakr, Nada.
Publisher: name: Monash University
Year: 2022

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.
The Repository Rodeo
Creators: name: Durand, Gustavo
name: Fyson, Will
name: Field, Dan
name: Greer Klein, Heather
name: Martínez García, Agustina
name: Stapelfeldt, Kirsta
name: Tarocco, Nicola
Publisher: name: Zenodo
Year: 2023
Subjects: OR2023
Dataverse
DSpace
EPrints
Fedora
Invenio
Islandora
Samvera

description: The Repository Rodeo returns for another round of questions and answers! This popular panel, featured since Open Repositories 2016 in Dublin, offers a broad overview of the main repository platforms at Open Repositories and provides an opportunity for spirited discussion amongst panelists and attendees. Join community representatives from Dataverse, DSpace, EPrints, Fedora, Invenio, Islandora, and Samvera as we briefly explain what each of our repositories actually does. We'll also talk about the directions of our respective technical and community developments and related to the conference theme of “Repositories Unlocked for Discovery and Interoperability”, we’ll discuss how our repository communities develop and implement the standards, frameworks, architectures, and methodologies for open repositories to serve as knowledge representation databases for the structured web of data. This panel will be a great opportunity for newcomers to Open Repositories to get a crash course on the major repository options and meet representatives from each of their communities. After a brief presentation from each representative, we'll open the session up for questions from the audience.
Sonnenfleckenzeichnung Nr. 123.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 28.05.1981, 06:45, erstellt von Sergio Cortesi, Sonnenobservatorium Specola Solare Ticinese in Locarno
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1981

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf dem Vordruck der Eidgenössischen Sternwarte Zürich. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 3.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)
Stellar evolutionary tracks for medium mass stars - effects of microphysics, core and envelope overshooting and mass loss
Creators: name: Smolec, Radoslaw
name: Ziolkowska, Oliwia
name: Rathour, Rajeev Singh
name: Hocde, Vincent
Publisher: name: Zenodo
Year: 2023

description: Reliable evolutionary tracks are a backbone of stellar astrophysics; they are an essential ingredient of asteroseismic inference. While some progress has been made towards advanced 3D modeling of stellar interiors, 1D evolutionary modeling will remain the only tool to efficiently model the large flow of data form new space telescopes and ground based surveys. Hence, it is critical to quantify the uncertainties inherent to 1D evolutionary modeling and to compute extensive grids of models that can later be used as a starting point for detailed stellar modeling. We present an extensive grid of stellar evolutionary tracks for medium mass stars computed with Modules for Experiments in Stellar Astrophysics (MESA). A grid covers stellar masses from 2 to 9 solar masses and a range of metallicties, from Z=0.0014 ([Fe/H]=-1) to Z=0.02 ([Fe/H]=+0.2), altogether 11 metallicity values. Models are computed form the Zero Age Main Sequence till the end of core Helium burning. For selected masses and metallicities models were computed assuming different microphysical setups, ie., models assume different scaled solar mixtures, different atmospheric boundary conditions, different variants of the Mixing Length Theory and different sets of nuclear reaction rates. This allows us to determine the uncertainties in the evolutionary tracks and in the parameters of the models (eg. luminosity, effective temperature, age, surface composition) at selected points in the evolution, due to uncertainties in the microphysics. These uncertainties are usually very low, provided mixing-length parameter is properly calibrated. The largest differences are observed for the highest metallicities and when considering different nuclear reaction rates. The effects of various macrophysical processes were investigated for the full model grid. The effects include convective core overshooting during the main sequence evolution, convective envelope overshooting and mass-loss. The latter two factors become important after the main sequence and influence the core helium burning phase, which is studied in detail. Mass-luminosity relations are computed and compared with observational constraints. The emergence of the blue loops, their properties, in particular dependence on the overshooting parameters and on the adopted nuclear reaction rates are studied. The loop properties (eg. minimum mass to enter the instability strip, temperature and luminosity extent) vary with mass and metallicity in a non-linear way and strongly depend on core and envelope overshooting parameters. While, in general, the larger the convective core overshooting, the shorter the loop, and the larger the envelope overshooting, the longer the loop, the details depend on metallicity. The adopted nuclear reaction rates also affect the extent of the blue loops, in particular for higher metallicities.
Quantum Hall Edges with Hard Confinement: Exact Solution beyond Luttinger Liquid
Creators: name: Fern, Richard
name: Simon, Steven H.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We consider a Laughlin droplet in a confining potential which is very steep but also weak compared to the ultra-short ranged inter-particle interactions. We find that the eigenstates have a Jack polynomial structure, and have an energy spectrum which is extremely different from the well-known Luttinger liquid edge.
description: 4 pages, 2 figures
AN INVESTIGATION OF CAPABILITY OF ARTIFICIAL INTELLIGENCE APPROACH IN DROUGHT FORECAST
Creators: name: Uruya Weesakul, Shekhar Mahat
Publisher: name: TuEngr Group
Year: 2020
Subjects: Deep neural network
Rainfall forecasting
Large-scale atmospheric variables
Drought forecasting modelling
Klong Yai river basin
Thailand.

description: International Transaction Journal of Engineering, Management, & Applied Sciences & Technologies, 11, 9, 11A9Q: 1-9
NEXUS AMONG SOCIAL SUSTAINABLE PERFORMANCE, SOCIAL SUSTAINABLE SUPPLY CHAIN PRACTICES AND OPERATION PERFORMANCE: DOES THE LONG-TERM ORIENTATION MATTER?
Creators: name: Abhishek Tripathi
Publisher: name: TuEngr Group
Year: 2020
Subjects: Operational performance (OP)
Supply Chain
Social sustainable
Sustainable service supply chain (SSSC)
Limited Time Offer (LTO)
Corporate sustainability
Business Sector Support Program (BSSP)
Social Sustainability Orientation (SSOR).

description: International Transaction Journal of Engineering, Management, & Applied Sciences & Technologies, 11, 9, 11A9R: 1-12
Fundamental effects of hydrophobic powders on nucleation and wet granulation
Creators: name: Nguyen, Thanh Huynh.
Publisher: name: Monash University
Year: 2022

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.
PCORnet COVID-19 Common Data Model Design and Results
Creators: name: Carton, Thomas W.
name: Marsolo, Keith
name: Block, Jason Perry
Publisher: name: Zenodo
Year: 2020
Subjects: COVID-19
PCORnet
Common Data Model
CDM
Data Query
Health Disparities
Distributed data network

description: Original Post: NIH Collaboratory Key Points For data to be useful in research, they have to be standardized across systems. The PCORnet Common Data Model standardizes data into a single language, enabling fast insights. All the core data elements needed to support COVID-19 research and surveillance have a home in the PCORnet CDM. The goal for PCORnet is to characterize the cohort of COVID-19 patients and provide detailed information on demographics and pre-existing conditions. Discussion Themes Can PCORnet partners stand up a version of the CDM with more up-to-date information to allow for a faster characterization of the PCORnet COVID-19 population? Is there a query to discover and address COVID-19 health disparities and social determinants of health? Can PCORnet and NCATS’ National COVID Cohort Collaborative (N3C) work together? Read more about PCORnet’s code lists and case definitions on GitHub.
Sonnenfleckenzeichnung Nr. 183.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 01.08.1981, 08:15, erstellt von Sergio Cortesi, Sonnenobservatorium Specola Solare Ticinese in Locarno
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1981

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf dem Vordruck der Eidgenössischen Sternwarte Zürich. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 4.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)
Constraining models of twin peak quasi-periodic oscillations with realistic neutron star equations of state
Creators: name: Török, Gabriel
name: Goluchová, Kateřina
name: Urbanec, Martin
name: Šrámková, Eva
name: Adámek, Karel
name: Urbancová, Gabriela
name: Pecháček, Tomáš
name: Bakala, Pavel
name: Stuchlík, Zdeněk
name: Horák, Jiří
name: Juryšek, Jakub
Publisher: name: arXiv
Year: 2016
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Twin-peak quasi-periodic oscillations (QPOs) are observed in the X-ray power-density spectra of several accreting low-mass neutron star (NS) binaries. In our previous work we have considered several QPO models. We have identified and explored mass-angular-momentum relations implied by individual QPO models for the atoll source 4U 1636-53. In this paper we extend our study and confront QPO models with various NS equations of state (EoS). We start with simplified calculations assuming Kerr background geometry and then present results of detailed calculations considering the influence of NS quadrupole moment (related to rotationally induced NS oblateness) assuming Hartle-Thorne spacetimes. We show that the application of concrete EoS together with a particular QPO model yields a specific mass-angular-momentum relation. However, we demonstrate that the degeneracy in mass and angular momentum can be removed when the NS spin frequency inferred from the X-ray burst observations is considered. We inspect a large set of EoS and discuss their compatibility with the considered QPO models. We conclude that when the NS spin frequency in 4U 1636-53 is close to 580Hz we can exclude 51 from 90 of the considered combinations of EoS and QPO models. We also discuss additional restrictions that may exclude even more combinations. Namely, there are 13 EOS compatible with the observed twin peak QPOs and the relativistic precession model. However, when considering the low frequency QPOs and Lense-Thirring precession, only 5 EOS are compatible with the model.
description: 12 pages, 9 figures, 3 tables, accepted for publication in The Astrophysical Journal
Building the compliance of HAL, the French national open archive, with Open Science funders policies
Creators: name: Kuntziger, Bénédicte
Publisher: name: Zenodo
Year: 2023
Subjects: OR2023
National repositories
Research funding organizations
Open science policies
Funder registry
Repository integration

description: HAL is the French open archive produced by the center for direct scientific communications (CCSD). ANR, which is the main funding agency in France and a member of the Coalition S, asks researchers to submit ‘at the time of publication at the latest, the full text of the scientific publications (version Author Accepted Manuscript or Version of Record) in the national open archive HAL, and mention the ANR research project reference (e.g. ANR-22-CE64-0001)’. With this in mind, ANR and CCSD have been conducted a project in 2021 to improve the current technical situation. The common work allowed an automatic update of the list of the ANR projects and an accurate description of the projects features. It has also led to the opening of an ANR portal to promote projects and their related publications. ANR works now to use HAL APIs to feed another information systems too. This collaboration should serve as a model for other funders, and led to a new project of funders and projects registries integration in HAL
Nonequilibrium self-organization of colloidal particles on substrates: adsorption, relaxation, and annealing
Creators: name: Araújo, N. A. M.
name: Dias, C. S.
name: da Gama, M. M. Telo
Publisher: name: arXiv
Year: 2016
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: Colloidal particles are considered ideal building blocks to produce materials with enhanced physical properties. The state-of-the-art techniques for synthesizing these particles provide control over shape, size, and directionality of the interactions. In spite of these advances, there is still a huge gap between the synthesis of individual components and the management of their spontaneous organization towards the desired structures. The main challenge is the control over the dynamics of self-organization. In their kinetic route towards thermodynamically stable structures, colloidal particles self-organize into intermediate (mesoscopic) structures that are much larger than the individual particles and become the relevant units for the dynamics. To follow the dynamics and identify kinetically trapped structures, one needs to develop new theoretical and numerical tools. Here we discuss the self-organization of functionalized colloids (also known as patchy colloids) on attractive substrates. We review our recent results on the adsorption and relaxation and explore the use of annealing cycles to overcome kinetic barriers and drive the relaxation towards the targeted structures.
Sonnenfleckenzeichnung Nr. 122.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 23.05.1981, 07:00, erstellt von Sergio Cortesi, Sonnenobservatorium Specola Solare Ticinese in Locarno
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1981

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf dem Vordruck der Eidgenössischen Sternwarte Zürich. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 3.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)
Theoretical design and circuit implementation of integer domain chaotic systems
Creators: name: Wang, Qianxue
name: Yu, Simin
name: Guyeux, Christophe
name: Bahi, Jacques
name: Fang, Xiaole
Publisher: name: arXiv
Year: 2016
Subjects: subject: Chaotic Dynamics (nlin.CD)
subject: Cryptography and Security (cs.CR)
subject: Dynamical Systems (math.DS)
subject: Pattern Formation and Solitons (nlin.PS)
subject: FOS: Physical sciences
subject: FOS: Computer and information sciences
subject: FOS: Mathematics

description: In this paper, a new approach for constructing integer domain chaotic systems (IDCS) is proposed, and its chaotic behavior is mathematically proven according to the Devaney's definition of chaos. Furthermore, an analog-digital hybrid circuit is also developed for realizing the designed basic IDCS. In the IDCS circuit design, chaos generation strategy is realized through a sample-hold circuit and a decoder circuit so as to convert the uniform noise signal into a random sequence, which plays a key role in circuit implementation. The experimental observations further validate the proposed systematic methodology for the first time.
Sonnenfleckenzeichnung Nr. 137.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 11.06.1981, 08:45, erstellt von Roberto Cortesi, Sonnenobservatorium Specola Solare Ticinese in Locarno
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1981

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf dem Vordruck der Eidgenössischen Sternwarte Zürich. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 3.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)
Parametric studies on the cavity micro-bioreactor via computational fluid dynamics simulations
Creators: name: Tan, Wei Leng.
Publisher: name: Monash University
Year: 2022

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.
Construction of Perturbatively Correct Light Front Hamiltonian for (2+1)-Dimensional Gauge Theory
Creators: name: Malyshev, M. Yu.
name: Prokhvatilov, E. V.
name: Zubov, R. A.
name: Franke, V. A.
Publisher: name: arXiv
Year: 2016
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: In this paper we consider (2+1)-dimensional SU(N)-symmetric gauge theory within light front perturbation theory, regularized by the method analogous to Pauli-Villars regularization. This enables us to construct correct renormalized light front Hamiltonian.
description: LaTeX, 15 pages, 3 figures. Article will be published in Theoretical and Mathematical Physics, the final publication will be available at http://link.springer.com/journal/11232
Numerical analysis and assessment of thermoplastically welded joints
Creators: name: Kreikemeier, Janko
name: Abdulkadir, Agit
Publisher: name: Zenodo
Year: 2019
Subjects: thermoplastic welding, cohesive zone modelling, finite element method

description: The work is dedicated to the numerical analysis and assessment of thermoplastically welded carbon fibre reinforced polymer laminates.
Impact of Cosmic Variance on the Galaxy-Halo Connection for Lyman-$α$ Emitters
Creators: name: Mejia-Restrepo, Julian E.
name: Forero-Romero, Jaime E.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: In this paper we study the impact of cosmic variance and observational uncertainties in constraining the mass and occupation fraction, $f_{\rm occ}$, of dark matter halos hosting Ly-$α$ Emitting Galaxies (LAEs) at high redshift. To this end, we construct mock catalogs from an N-body simulation to match the typical size of observed fields at $z=3.1$ ($\sim 1 {\rm deg^2}$). In our model a dark matter halo with mass in the range $M_{\rm min}
description: 7 Pages, 5 figures. Accepted for publication in ApJ
Sonnenfleckenzeichnung Nr. 171.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 17.07.1981, 09:00, erstellt von Roberto Cortesi, Sonnenobservatorium Specola Solare Ticinese in Locarno
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1981

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf dem Vordruck der Eidgenössischen Sternwarte Zürich. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 3.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)
Universality of the ion flux to the JET outer wall
Creators: name: Walkden, N. R.
name: Wynn, A.
name: Militello, F.
name: Lipschultz, B.
name: Matthews, G.
name: Guillemaut, C.
name: Harrison, J.
name: Moulton, D.
name: Contributors, JET
Publisher: name: arXiv
Year: 2016
Subjects: subject: Plasma Physics (physics.plasm-ph)
subject: FOS: Physical sciences

description: Universality in the ion flux to the JET outer-wall is observed in outerwall limiter mounted Langmuir probe (OLP) time-series across a large range of plasma current and line-averaged density during Ohmically heated horizontal target L-mode plasmas. The mean, M, and the standard deviation, sigma, of the ion-saturation current measured by the OLP show systematic variation with plasma current and density. Both increase as either plasma current decreases and/or density increases. Upon renormalization, achieved by subtraction of M and rescaling by sigma, the probability distribution functions (PDFs) of each signal collapse approximately onto a single curve. The shape of the curve deviates from a distribution in the tail of the PDF and is better described by a log-normal distribution. The collapse occurs over 4 decades of the ordinate which, given the wide parameter space over which the data spans, is a strong indication of universality.
description: 10 pages, 6 figures. This is an author-created, un-copyedited version of an article submitted for publication in Nuclear Fusion Letter. IoP Publishing Ltd is not responsible for any errors or omissions in this version of the manuscript or any version derived from it
NTU Research Data Repository's assessment and certification
Creators: name: Ishak, Yuyun Wirawati
Publisher: name: Zenodo
Year: 2023
Subjects: OR2023
CoreTrustSeal certification
data repositories

description: DR-NTU (Data), the research repository of Nanyang Technological University, was launched in 2017 as a data repository where NTU community can archive and publicly share the research data from projects carried out at the University. The repository uses Dataverse, an open-source software. After five years, the repository contains more than 1,000 published datasets and it was timely to assess it, to ensure that the repository is aligned with industry's best practices and to identify possible gaps in workflows, technology, and documentation. CoreTrustSeal Certification was chosen as a framework that not only allows repository to performs self-assessment, but also gives positive signal to stakeholders, that an independent authority has evaluated the research data repository and endorsed its trustworthiness. It ensures reliability and durability of data repository and therefore affirms repository's potential for storing and sharing data over a long period of time. In addition, journals and funders also encourage deposit of research data in a trusted repository (Center for Open Science, 2015). The certification process was rigorous, with preparation works that took place way before the certification application was even submitted. The review from CoreTrustSeal identified a few gaps which we see as opportunities for continuous improvements.
Sonnenfleckenzeichnung Nr. 41.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 12.02.1981, 08:00, erstellt von Sergio Cortesi, Sonnenobservatorium Specola Solare Ticinese in Locarno
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1981

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf dem Vordruck der Eidgenössischen Sternwarte Zürich. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 3.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)
Sonnenfleckenzeichnung Nr. 25.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 27.01.1981, 08:30, erstellt von Sergio Cortesi, Sonnenobservatorium Specola Solare Ticinese in Locarno
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1981

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf dem Vordruck der Eidgenössischen Sternwarte Zürich. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 3.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)
Sonnenfleckenzeichnung Nr. 141.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 15.06.1981, 06:00, erstellt von Sergio Cortesi, Sonnenobservatorium Specola Solare Ticinese in Locarno
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1981

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf dem Vordruck der Eidgenössischen Sternwarte Zürich. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 3.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)
Development of active radio frequency identification system and anti-collision algorithm
Creators: name: Teoh, Qi Jing.
Publisher: name: Monash University
Year: 2022

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.
DigtaX Archive some stories of more than 200 years of tax resources
Creators: name: Beberweil, Katharina
Publisher: name: Zenodo
Year: 2023
Subjects: OR2023
Digital tax law resources
digital archive
preservation
repository for tax law

description: The title of my presentation shows what I will be talking about: DigitaX = Digital and Tax. I am planning to present our work on digital resources on tax law, thereby looking back at more than 200 years of materials collected. I will present the way towards setting up our digital archive, with the challenges experienced and lessons learned as part of this initial project in 2013. By now, the initial scanning project has turned into a biennial activity, through which we regularly add materials that we cannot keep in paper due to space constraints. In addition, I will also show how we successfully opened the content of one prestigious tax journal via the archive when this journal turned 75 years.
Sonnenfleckenzeichnung Nr. 176.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 25.07.1981, 06:30, erstellt von Sergio Cortesi, Sonnenobservatorium Specola Solare Ticinese in Locarno
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1981

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf dem Vordruck der Eidgenössischen Sternwarte Zürich. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 2.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)
Lessons learnt during the establishment of an Oral History Channel on how to make oral histories more accessible
Creators: name: Hartzenberg, Reinhardt
name: Khumalo, Vukile
Publisher: name: Zenodo
Year: 2023
Subjects: OR2023
Oral History Channel
Repository access
System design
Oral Interviews

description: The purpose of this paper is to share recent developments and practices implemented by the KwaZulu-Natal Archives and Records Service in South Africa in order to discover inventive new approaches for making Oral History interviews available to a wider audience. With assistance from AVP in the United States, the KwaZulu-Natal Archives and Records Service has launched an Oral History Channel to increase access to oral interviews from its archive. As technology evolve, the KwaZulu-Natal Oral History unit is exploring new approaches to aid researchers and the general public in gaining access to their decade-long oral collection. In South Africa, publishing interviews on a dedicated Oral History platform has been relatively unheard of, and the KwaZulu-Natal Archives had to overcome certain particular obstacles in order to create a holistic system that would improve oral history access for South African audiences. Language, metadata, interactive access, and publishing were some of the most problematic areas in building a successful system. This short presentation will overview some of the unique solutions that was applied to the challenge in building the Oral history ecosystem.
Roadmap for the Implementation of OPERAS National Nodes (OPERAS-PLUS Deliverable 7.2)
Creators: name: Caliman, Lorena
name: Leão, Delfim
Publisher: name: Zenodo
Year: 2023
Subjects: open scholarly communication
OPERAS-PLUS
social sciences
humanities
research infrastructure
SSH
OPERAS

description: This document provides a first roadmap for the implementation of OPERAS national nodes, communities built with the aim of establishing a connection point to outside the OPERAS community, connecting relevant stakeholders in individual countries. The document defines a common approach to all 12 existing nodes for engaging communities and providing OPERAS services nationally, establishing some minimum requirements. An update of this initial document will be provided at M33 (May 2025). 
Wind-driven Accretion in Transitional Protostellar Disks
Creators: name: Wang, Lile
name: Goodman, Jeremy J.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Transitional protostellar disks have inner cavities heavily depleted in dust and gas, yet most show signs of ongoing accretion, often at rates comparable to full disks. We show that recent constraints on the gas surface density in a few well-studied disk cavities imply that the accretion speed is at least transsonic. We propose that this is the natural result of accretion driven by magnetized winds. Typical physical conditions of the gas inside such cavities are estimated for plausible X-ray and FUV radiation fields. The gas is molecular and predominantly neutral, with a dimensionless ambipolar parameter in the right general range for wind solutions of the type developed by Königl, Wardle, and others. That is to say, the density of ions and electrons is sufficient for moderately good coupling to the magnetic field, but not so good that the magnetic flux need be dragged inward by the accreting neutrals.
description: 7 pages, 2 figures; submitted to ApJ
Sonnenfleckenzeichnung Nr. 33.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 04.02.1981, 10:30, erstellt von Sergio Cortesi, Sonnenobservatorium Specola Solare Ticinese in Locarno
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1981

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf dem Vordruck der Eidgenössischen Sternwarte Zürich. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 3.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)
A quantitative interpretation of the frequent hypercyclicity criterion
Creators: name: Ernst, Romuald
name: Mouze, A
Publisher: name: arXiv
Year: 2016
Subjects: subject: Functional Analysis (math.FA)
subject: FOS: Mathematics

description: We give a quantitative interpretation of the Frequent Hypercyclicity Criterion. Actually we show that an operator which satisfies the Frequent Hypercyclicity Criterion is necessarily A-frequently hypercyclic, where A refers to some weighted densities sharper than the natural lower density. In that order, we exhibit different scales of weighted densities that are of interest to quantify the "frequency" measured by the Frequent Hypercyclicity Criterion. Moreover we construct an example of unilateral weighted shift which is frequently hypercyclic but not A-frequently hypercyclic on a particular scale.
Sonnenfleckenzeichnung Nr. 109.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 08.05.1981, 07:15, erstellt von Sergio Cortesi, Sonnenobservatorium Specola Solare Ticinese in Locarno
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1981

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf dem Vordruck der Eidgenössischen Sternwarte Zürich. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 3.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)
Thermochemical production of biofuels from Australian forestry resources : literature review and theoretical case study
Creators: name: Melendez, Jose.
Publisher: name: Monash University
Year: 2022

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.
Sonnenfleckenzeichnung Nr. 143.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 17.06.1981, 60:30, erstellt von Sergio Cortesi, Sonnenobservatorium Specola Solare Ticinese in Locarno
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1981

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf dem Vordruck der Eidgenössischen Sternwarte Zürich. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 3.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)
Tall sections from non-minimal transformations
Creators: name: Morrison, David R.
name: Park, Daniel S.
Publisher: name: arXiv
Year: 2016
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: In previous work, we have shown that elliptic fibrations with two sections, or Mordell-Weil rank one, can always be mapped birationally to a Weierstrass model of a certain form, namely, the Jacobian of a $\mathbb{P}^{112}$ model. Most constructions of elliptically fibered Calabi-Yau manifolds with two sections have been carried out assuming that the image of this birational map was a "minimal" Weierstrass model. In this paper, we show that for some elliptically fibered Calabi-Yau manifolds with Mordell-Weil rank-one, the Jacobian of the $\mathbb{P}^{112}$ model is not minimal. Said another way, starting from a Calabi-Yau Weierstrass model, the total space must be blown up (thereby destroying the "Calabi-Yau" property) in order to embed the model into $\mathbb{P}^{112}$. In particular, we show that the elliptic fibrations studied recently by Klevers and Taylor fall into this class of models.
description: 16 pages
The process is the work scribe at the side sectional infrastructure
Creators: name: Vials Moore, Adam
name: Evans, Jenny
name: Kaye, John
name: Fellows, Tim
name: McLaughlin, Scott
Publisher: name: Zenodo
Year: 2023
Subjects: OR2023
Practice research
sectional outputs
metadata
novel infrastructure

description: Repositories are currently typically the destination of outputs of the final stages of research. New infrastructure and standards are supporting the capture of a more fine-grained view of the research process. As these novel output types and research capture practices evolve and become a part of the wider landscape, repositories and the technical / policy milieu will also need to evolve to respond. This short talk will look at the current state of the art and discuss how practice, technical platforms and policy might progress.
Sonnenfleckenzeichnung Nr. 74.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 23.03.1981, 08:30, erstellt von Sergio Cortesi, Sonnenobservatorium Specola Solare Ticinese in Locarno
Creators: name: [s.n.]
Publisher: name: [s.n.]
Year: 1981

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf dem Vordruck der Eidgenössischen Sternwarte Zürich. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 3.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)
Hybrid Models in Loop Quantum Cosmology
Creators: name: Navascués, B. Elizaga
name: Martín-Benito, M.
name: Marugán, G. A. Mena
Publisher: name: arXiv
Year: 2016
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: In the framework of Loop Quantum Cosmology, inhomogeneous models are usually quantized by means of a hybrid approach that combines loop quantization techniques with standard quantum field theory methods. This approach is based on a splitting of the phase space in a homogeneous sector, formed by global, zero-modes, and an inhomogeneous sector, formed by the remaining, infinite number of modes, that describe the local degrees of freedom. Then, the hybrid quantization is attained by adopting a loop representation for the homogeneous gravitational sector, while a Fock representation is used for the inhomogeneities. The zero-mode of the Hamiltonian constraint operator couples the homogeneous and inhomogeneous sectors. The hybrid approach, therefore, is expected to provide a suitable quantum theory in regimes where the main quantum effects of the geometry are those affecting the zero-modes, while the inhomogeneities, still being quantum, can be treated in a more conventional way. This hybrid strategy was first proposed for the simplest cosmological midisuperspaces: the Gowdy models, and it has been later applied to the case of cosmological perturbations. This paper reviews the construction and main applications of hybrid Loop Quantum Cosmology
description: Invited review article for the special issue of the International Journal of Modern Physics D on Loop Quantum Cosmology