cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
The Migration of Gap-Opening Planets is not Locked to Viscous Disk Evolution
Creators: name: Duffell, Paul C.
name: Haiman, Zoltan
name: MacFadyen, Andrew I.
name: D'Orazio, Daniel J.
name: Farris, Brian D.
Publisher: name: arXiv
Year: 2014
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Most standard descriptions of Type II migration state that massive, gap-opening planets must migrate at the viscous drift rate. This is based on the idea that the disk is separated into an inner and outer region and gas is considered unable to cross the gap. In fact, gas easily crosses the gap on horseshoe orbits, nullifying this necessary premise which would set the migration rate. In this work, it is demonstrated using highly accurate numerical calculations that the actual migration rate is dependent on disk and planet parameters, and can be significantly larger or smaller than the viscous drift rate. In the limiting case of a disk much more massive than the secondary, the migration rate saturates to a constant which is sensitive to disk parameters and is not necessarily of order viscous rate. In the opposite limit of a low-mass disk, the migration rate decreases linearly with disk mass. Steady-state solutions in the low disk mass limit show no pile-up outside the secondary's orbit, and no corresponding drainage of the inner disk.
description: ApJ Accepted
Generalized Heavy-to-Light Form Factors in Light-Cone Sum Rules
Creators: name: Meißner, Ulf-G.
name: Wang, Wei
Publisher: name: arXiv
Year: 2013
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: We study the form factors for a heavy meson into the S-wave $Kπ/ππ$ system with an invariant mass below 1~GeV. The mesonic final state interactions are described in terms of the scalar form factors, which are obtained from unitarized chiral perturbation theory. Employing generalized light-cone distribution amplitudes, we compute the heavy-to-light transition using light-cone sum rules. Our approach simultaneously respects constraints from analyticity and unitarity, and also takes advantage of the power expansion in the $1/m_b$ and the strong coupling constant.
description: 8 pages, 3 figures, v2: 11 pages, 3 figures, title changed, some clarifications and references added, matches version to appear in Physics Letters B
How do open infrastructures work together? - ROR
Creators: name: French, Amanda
Publisher: name: Zenodo
Year: 2022
Subjects: DataCite Member Meeting 2022
open infrastructure
Crossref
ROR
organization identifier

description: Providers of open infrastructures collaborate to enable seamless scholarly communication. But what are they actually doing to realize this? How do open infrastructures integrate metadata of other providers into their services? This open community session gives open infrastructures the opportunity to let us see scholarly communication through their eyes. Throughout the session you will be able to ask the panelists anything about their services. Speaker: Amanda French (Crossref/ROR) A recording of the presentation can be found at: https://www.youtube.com/watch?v=c43cb80WR2o&t=1526s
HUQUQIY SAVODXONLIKNI YUKSALTIRISHDA KONSTITUSIYANING O'RNI VA AXAMIYATI
Creators: name: Sayfitdinova, Madinabonu
Publisher: name: Zenodo
Year: 2023

description: Ushbu maqolada huquqiy savodxonlikni yuksaltirishda konstitusiyaning o'rni va axamiyati ilmiy dalillar asosida keng va atroflicha yoritib berilgan.
Spacetime singularity resolution in Snyder noncommutative space
Creators: name: Gorji, M. A.
name: Nozari, K.
name: Vakili, B.
Publisher: name: arXiv
Year: 2014
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Theory (hep-th)
subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: Inspired by quantum gravity proposal, we construct a deformed phase space which supports the UV and IR cutoffs. We show that the Liouville theorem is satisfied in the deformed phase space which allows us to formulate the thermodynamics of the early Universe in the semiclassical regime. Applying the proposed method to the Snyder noncommutative space, we find a temperature dependent equation of state which opens a new window for natural realization of inflation as a phase transition from quantum gravity regime to the standard radiation dominated era. Also we obtain finite energy and entropy densities for the Universe, when at least the Weak Energy Condition is satisfied. We show that there is a minimum size for the Universe which is proportional to the Planck length and consequently the Big Bang singularity is removed.
description: 11 pages, 4 figures, Revised for PRD, title changed
On conformal higher spin wave operators
Creators: name: Nutma, Teake
name: Taronna, Massimo
Publisher: name: arXiv
Year: 2014
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We analyze free conformal higher spin actions and the corresponding wave operators in arbitrary even dimensions and backgrounds. We show that the wave operators do not factorize in general, and identify the Weyl tensor and its derivatives as the obstruction to factorization. We give a manifestly factorized form for them on (A)dS backgrounds for arbitrary spin and on Einstein backgrounds for spin 2. We are also able to fix the conformal wave operator in d=4 for s=3 up to linear order in the Riemann tensor on generic Bach-flat backgrounds.
description: 26 pages, includes Mathematica notebook. Version published in JHEP
Supplementary document for A universal and effective variational method for destriping: application to light-sheet microscopy, FIB-SEM and remote sensing images - 7316521.pdf
Creators: name: Rottmayer, Niklas
name: Redenbach, Claudia
name: Fahrbach, Florian
Publisher: name: Optica Publishing Group
Year: 2025
Subjects: Uncategorized

description: Supplementary
Report
Creators: name: Satapathy, Sumit
Publisher: name: figshare
Year: 2023
Subjects: Particle and high energy physics not elsewhere classified

description: In this report we calculate necessary parameters related to Dark matter such as its relic density, its detection rate which is regarded as Direct detection, we do all these for a generic model as well as exclusively for Inert doublet model, we show how we can calculate these parameters using a software known as micromegas. At last we calculate the one loop correction to the tree level vertex.
The connections of pseudo-Finsler spaces
Creators: name: Minguzzi, E.
Publisher: name: arXiv
Year: 2014
Subjects: subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: We give an introduction to (pseudo-)Finsler geometry and its connections. For most results we provide short and self contained proofs. Our study of the Berwald non-linear connection is framed into the theory of connections over general fibered spaces pioneered by Mangiarotti, Modugno and other scholars. The main identities for the linear Finsler connection are presented in the general case, and then specialized to some notable cases like Berwald's, Cartan's or Chern-Rund's. In this way it becomes easy to compare them and see the advantages of one connection over the other. Since we introduce two soldering forms we are able to characterize the notable Finsler connections in terms of their torsion properties. As an application, the curvature symmetries implied by the compatibility with a metric suggest that in Finslerian generalizations of general relativity the mean Cartan torsion vanishes. This observation allows us to obtain dynamical equations which imply a satisfactory conservation law. The work ends with a discussion of yet another Finsler connection which has some advantages over Cartan's and Chern-Rund's.
description: 47 pages. v2: corrected several typos, some improved conclusions. To appear in Int. J. Geom. Meth. Mod. Phys
Scanning Doppler wind lidar for wind field measurements
Creators: name: Würth, Ines
name: Clifton, Andrew
Publisher: name: Zenodo
Year: 2022
Subjects: wind energy
wind lidar
scanning lidar
Doppler lidar

description: This is a short review of scanning Doppler wind lidar for wind energy applications. It is one of an ongoing series of publications by the wind energy technology transfer startup, enviConnect. To provide feedback, request modifications, or to have it customised to your needs, please write to info@enviconnect.de
description: This is published under the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International (CC BY-NC-ND 4.0) license https://creativecommons.org/licenses/by-nc-nd/4.0/
title: WP9 Progress, Results and Next Steps
title: WP9 Dissemination & Outreach
titleType: Subtitle
title: WP9 Project Management and Reporting
titleType: Subtitle
Creators: name: Hayashi, Erika
name: Bearzotti, Chiara
Publisher: name: Zenodo
Year: 2023

description: This presentation was given at the OCEAN:ICE Annual Meeting on October 25th, 2023 during the OCEAN:ICE Work Pacakges Progress, Results and Plans for the next 12 months session. 
Erika Hayashi (DMI) presented WP9 Dissemination and Outreach and the Equity, Diversity and Inclusivity Policy.
Chiara Bearzotti (DMI) presented WP9 Project Management, Reporting. 
The OCEAN:ICE Annual Meeting was part of a Joint Project meeting together with the EU Horizon 2020 project, SO-CHIC which took place at Sorbonne University in Paris from October 23rd to 26th, 2023. The Joint Project meeting included SO-CHIC's Annual Project Meeting, a Joint SO-CHIC and OCEAN:ICE Conference, and the OCEAN:ICE Annual Meeting.
Observational constraint on the interacting dark energy models including the Sandage-Loeb test
Creators: name: Zhang, Ming-Jian
name: Liu, Wen-Biao
Publisher: name: arXiv
Year: 2013
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Two types of interacting dark energy models are investigated using the type Ia supernova (SNIa), observational $H(z)$ data (OHD), cosmic microwave background (CMB) shift parameter and the secular Sandage-Loeb (SL) test. We find that the inclusion of SL test can obviously provide more stringent constraint on the parameters in both models. For the constant coupling model, the interaction term including the SL test is estimated at $δ=-0.01 \pm 0.01 (1σ) \pm 0.02 (2σ)$, which has been improved to be only a half of original scale on corresponding errors. Comparing with the combination of SNIa and OHD, we find that the inclusion of SL test directly reduces the best-fit of interaction from 0.39 to 0.10, which indicates that the higher-redshift observation including the SL test is necessary to track the evolution of interaction. For the varying coupling model, we reconstruct the interaction $δ(z)$, and find that the interaction is also negative similar as the constant coupling model. However, for high redshift, the interaction generally vanishes at infinity. The constraint result also shows that the $Λ$CDM model still behaves a good fit to the observational data, and the coincidence problem is still quite severe. However, the phantom-like dark energy with $w_X
description: 10 pages, 7 figures
Empis (Enoplempis) subgeneatis Sinclair, Brooks & Cumming, 2025, sp. nov.
Creators: name: Sinclair, Bradley J.
name: Brooks, Scott E.
name: Cumming, Jeffrey M.
Publisher: name: Zenodo
Year: 2025
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Empididae
Empis
Empis subgeneatis

description: Empis (Enoplempis) subgeneatis sp. nov.
urn:lsid:zoobank.org:act: BF8CC15F-C0A9-450A-81E1-5713DED3EA09
(Figs 187, 192)
Type material. HOLOTYPE ♂, labelled: “Alsea [44°22′N 123°35′W]/ Ore. 4-26-29”; J.E. Davis / Coll.”; “ Empis / (Pogoenempis)/ geneatis/ Melander/ det. WJ Turner 1978”; “ HOLOTYPE / Empis (Enoplempis) / subgeneatis Sinclair,/ Brooks & Cumming [red label]” [dissected] (OSAC). PARATYPE: USA. Oregon: Washington County: Banks [45°36′N 123°06′W], 20.v.1964, Blk. light trap, K. Goeden (ODAC).
Possible additional material (unassociated females). USA. Oregon: Benton County: Corvalis, Lewisburg Saddle ck below Old Growth Tr., 44.6423°N 123.2891°W, MT, 29.iii–23.iv.2013, SJF (1♀, CNC); same data except, 44°38′32.28″N 123°17′20.76″W, MT over ck, 23.iv–6.v.2013 (1♀, CNC); Marys Peak, 12 mi. W Corvallis, 3800 ft, 10.vi.1984, Darling (1♀, ROM).
Diagnosis. This species is very similar to E. (En.) geneatis, distinguished by its larger size (wing length more than 6 mm), dense dorsal setae on the male hind femur, length more than twice femur width, and the male cercus is more rounded dorsally.
Description. Wing length 6.2–6.5 mm. Male. Similar to E. (En.) geneatis, except as follows: head with ocellar triangle with several pairs of posterior setulae. Scape 5× longer than pedicel.
Scutum without pair of greyish vittae. Postpronotum with numerous short, silky setae. Notopleuron clothed in long silky setae; 1 long pal and short silky setulae. Scutellum with pair of long sctl, with numerous pairs of long silky marginal setae.
Fore femur clothed in long, wavy setae, longer dorsally and posteriorly. Fore tibia with long posterodorsal setae, 3× longer than width of tibia; ventrally with fine, dense setae, subequal to width of segment. Hind tibia evenly expanded apically, not broader than femur distally.
Terminalia (Fig. 187): cercus broader than epandrium, suboval, rounded dorsally.
Female. Not confirmed.
Geographical distribution and seasonal occurrence (Fig. 192). Empis (En.) subgeneatis sp. nov. is known from Oregon. Adults have been collected in April and May and also possibly March and June.
Etymology. The species name is in reference to the similarity of this species with E. geneatis.
Nuptial gift presentation. Form unknown.
description: Published as part of Sinclair, Bradley J., Brooks, Scott E. & Cumming, Jeffrey M., 2025, Revision of the western Nearctic species of Empis subgenus Enoplempis (Diptera: Empididae), pp. 1-200 in Zootaxa 5615 (1) on pages 96-97, DOI: 10.11646/zootaxa.5615.1.1, http://zenodo.org/record/15217957
Magnetic ordering of three-component ultracold fermionic mixtures in optical lattices
Creators: name: Sotnikov, Andrii
name: Hofstetter, Walter
Publisher: name: arXiv
Year: 2014
Subjects: subject: Quantum Gases (cond-mat.quant-gas)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We study finite-temperature magnetic phases of three-component mixtures of ultracold fermions with repulsive interactions in optical lattices with simple cubic or square geometry by means of dynamical mean-field theory (DMFT). We focus on the case of one particle per site (1/3 band filling) at moderate interaction strength, where we observe a sequence of thermal phase transitions into two- and three-sublattice ordered states by means of the unrestricted real-space generalization of DMFT. From our quantitative analysis we conclude that long-range ordering in three-component mixtures should be observable at comparable temperatures as in two-component mixtures.
description: 7 pages, 4 figures
Ion Bernstein instability dependence on the proton-to-electron mass ratio: Linear dispersion theory
Creators: name: Min, Kyungguk
name: Liu, Kaijun
Publisher: name: Auburn University
Year: 2016

description: Fast magnetosonic waves, which have as their source ion Bernstein instabilities driven by tenuous ring-like proton velocity distributions, are frequently observed in the inner magnetosphere. One major difficulty in the simulation of these waves is that they are excited in a wide frequency range with discrete harmonic nature and require time-consuming computations. To overcome this difficulty, recent simulation studies assumed a reduced proton-to-electron mass ratio, m(p)/m(e), and a reduced light-to-Alfven speed ratio, c/v(A), to reduce the number of unstable modes and, therefore, computational costs. Although these studies argued that the physics of wave-particle interactions would essentially remain the same, detailed investigation of the effect of this reduced system on the excited waves has not been done. In this study, we investigate how the complex frequency, = (r)+i, of the ion Bernstein modes varies with m(p)/m(e) for a sufficiently large c/v(A) (such that pe2/e2(me/mp)(c/vA)2 >> 1) using linear dispersion theory assuming two different types of energetic proton velocity distributions, namely, ring and shell. The results show that low- and high-frequency harmonic modes respond differently to the change of m(p)/m(e). For the low harmonic modes (i.e., (r)approximate to(p)), both (r)/(p) and /(p) are roughly independent of m(p)/m(e), where (p) is the proton cyclotron frequency. For the high harmonic modes (i.e., p<<r less than or similar tolh, where (lh) is the lower hybrid frequency), /(lh) (at fixed (r)/(lh)) stays independent of m(p)/m(e) when the parallel wave number, k(vertical bar), is sufficiently large and becomes inversely proportional to (m(p)/m(e))(1/4) when k(vertical bar) goes to zero. On the other hand, the frequency range of the unstable modes normalized to (lh) remains independent of m(p)/m(e), regardless of k(vertical bar).
General Use SOP for Compressed Gases
Creators: name: Stanford EH&S
Publisher: name: Stanford Digital Repository
Year: 2024
Subjects: chemical safety
compressed gasses
simple asphyxiant

description: This standard operating procedure (SOP) is intended to provide general guidance on how to safely work with compressed gases. This general use SOP only addresses safety issues specific to compressed gases. In some instances, several general use SOPs may be applicable for a specific chemical (i.e., for flammable gases, both this general use SOP and the general use SOP for flammables would apply). If you have questions concerning the applicability of any item listed in this procedure contact the Principal Investigator/Laboratory Supervisor of your laboratory or Environmental Health and Safety (EHS_Research_SOP@lists.stanford.edu)
Dust formation in macronovae
Creators: name: Takami, Hajime
name: Nozawa, Takaya
name: Ioka, Kunihito
Publisher: name: arXiv
Year: 2014
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We examine dust formation in macronovae (as known as kilonovae), which are the bright ejecta of neutron star binary mergers and one of the leading sites of r-process nucleosynthesis. We find that dust grains of r-process elements are difficult to form because of the low number density of the r-process atoms, while carbon or elements lighter than irons can condense into dust if they are abundant, in light of the first macronova candidate associated with GRB 130603B. Dust grains absorb emission from ejecta with opacity even greater than that of the r-process elements, and re-emit photons at infrared wavelengths. Such dust emission can potentially account for the macronova without r-process nucleosynthesis as an alternative model. This dust scenario predicts a more featureless spectrum than the r-process model and day-scale optical-to-ultraviolet emission.
description: 5 pages, 4 figures, 1 table, accepted for publication in ApJ Letters
Multi-Event Studies of Sudden Energetic Electron Enhancements in the Inner Magnetosphere and Its Association With Plasmapause Positions
Creators: name: Li, X
name: Khoo, L
name: Thaller, S
name: Hogan, B
Publisher: name: Auburn University
Year: 2021

description: Sudden enhancements of energetic electrons (tens of keV to <500 keV) at low L-shells have been frequently observed by Van Allen Probes. It is, however, still unclear how deep these electrons can reach and what the responsible mechanisms are. Here we seek to determine the inner boundary of initial enhancements of these energetic electrons and its link with the plasmapause location to offer a new, insightful perspective on this topic. Previous statistical studies have revealed a remarkably consistent observation that initial enhancements of energetic electrons occur mostly at higher L-shell than the innermost plasmapause locations (L-pp), though a few outlier events were also identified. In this study, we examine the identified outlier events where electron enhancements were reported inside the plasmapause (either in situ L-pp or simulated innermost L-pp). More detailed investigation indicates that the appearance of enhancements inside the in situ L-pp is often associated with duskside observations where the actual initial enhancement likely occurs somewhere else, outside the innermost plasmapause location. We thereby urge caution when using the relationship between the observed enhancement locations and the in situ L-pp to infer the effect of electric fields on energetic electrons. In summary, our findings suggest that the innermost L-pp remains the innermost limit of the initial sudden enhancements of energetic electrons. Combining with phase space density analysis, our result implies the role of a large-scale electric field that leads to sudden electron enhancements and the erosion of the plasmasphere.
The Cross-pollination of Memories between Black and LGBT+ Activism
Creators: name: Salerno, Daniele
Publisher: name: figshare
Year: 2023
Subjects: Multicultural, intercultural and cross-cultural studies
Global and world history
Histories of race
Latin and South American history
Transnational history
Feminist and queer theory

description: Text for the blog "Remembering Activism" on the cultural and rhetorical intersections between Black and LGBT+ activism.
Radiation-pressure-driven dust waves inside bursting interstellar bubbles
Creators: name: Ochsendorf, B. B.
name: Verdolini, S.
name: Cox, N. L. J.
name: Berné, O.
name: Kaper, L.
name: Tielens, A. G. G. M.
Publisher: name: arXiv
Year: 2014
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Massive stars drive the evolution of the interstellar medium through their radiative and mechanical energy input. After their birth, they form bubbles of hot gas surrounded by a dense shell. Traditionally, the formation of bubbles is explained through the input of a powerful stellar wind, even though direct evidence supporting this scenario is lacking. Here we explore the possibility that interstellar bubbles seen by the Spitzer- and Herschel space telescopes, blown by stars with log(L/L_sun) < 5.2, form and expand due to the thermal pressure accompanying ionization of the surrounding gas. We show that density gradients in the natal cloud or a puncture in the swept up shell lead to an ionized gas flow through the bubble into the general interstellar medium, which is traced by a dust wave near the star, demonstrating the importance of radiation pressure during this phase. Dust waves provide a natural explanation for the presence of dust inside H II bubbles, offer a novel method to study dust in H II regions and provide direct evidence that bubbles are relieving their pressure into the ISM through a champagne flow, acting as a probe of the radiative interaction of a massive star with its surroundings. We create a parameter space connecting the ambient density, the ionizing source luminosity, and the position of the dust wave, while using the well-studied H II bubbles RCW 120 and RCW 82 as benchmarks of our model. Finally, we briefly examine the implications of our study for the environments of super star clusters formed in UltraLuminous InfraRed Galaxies (ULIRGs), merging galaxies and the early Universe, which occur in very luminous and dense environments and where radiation pressure is expected to dominate the dynamical evolution.
description: 9 pages, 6 figures: corrected typos
Interface Problems for Dispersive equations
Creators: name: Sheils, Natalie E
name: Deconinck, Bernard
Publisher: name: arXiv
Year: 2014
Subjects: subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: The interface problem for the linear Schrödinger equation in one-dimensional piecewise homogeneous domains is examined by providing an explicit solution in each domain. The location of the interfaces is known and the continuity of the wave function and a jump in their derivative at the interface are the only conditions imposed. The problem of two semi-infinite domains and that of two finite-sized domains are examined in detail. The problem and the method considered here extend that of an earlier paper by Deconinck, Pelloni and Sheils (2014). The dispersive nature of the problem presents additional difficulties that are addressed here.
description: 18 pages, 6 figures. arXiv admin note: text overlap with arXiv:1402.3007, Studies in Applied Mathematics 2014
Signatures of electron Landau resonant interactions with chorus waves from THEMIS observations
Creators: name: Min, Kyungguk
name: Kaijun, Liu
name: Li, Wen
Publisher: name: Auburn University
Year: 2014

description: Simultaneous observations of electron phase space density (PSD) and chorus waves for more than 4 years by the Time History of Events and Macroscale Interactions during Substorms (THEMIS) are analyzed to identify signatures of the electron Landau resonant interactions with chorus waves in the radiation belts. Chorus waves play an important role in the radiation belt dynamics by effectively interacting with electrons. Landau resonant interactions arise when the waves are not exactly parallel propagating. Such interactions lead to plateaus along v(II) in the electron velocity distributions, where v(II) is the parallel (with respect to the background magnetic field) component of the electron velocity. The analyzed electron PSDs often demonstrate local minima in the derivative of the velocity distribution along v(II) near the Landau resonant velocity calculated from the simultaneous in situ wave observations. These minima are, therefore, direct signatures and solid evidence of the electron Landau resonant interactions with chorus waves.
RID study AutoNOM
Creators: name: Gatin, Laure
name: Yannou, Bernard
name: Abdelatif, Naila
name: Jankovic, Marija
name: Sahin, Evren
Publisher: name: Zenodo
Year: 2024

description: According to a recent study, about 22% of residents in retirement homes suffer from troublesome acquired deforming hypertonia (ADH). Very few of them benefit from the necessary care due to the difficulties inherent to travel and hospitalisation. A novel procedure has been developed to reduce the medical impact of such a procedure and lower hospitalisation duration. The advantage of this procedure based on a needle tenotomy is that it does not require a full surgery room. Actual situations are deficient in detecting and treating these patients. Hence, the idea of developing a mobile unit has been seen as a possibility to address the issue of accessibility for such a procedure near retirement homes and reduce hospitalisation time. To explore the lack of effective solutions in the care of patients suffering from AHD in France, and assess the potential advantages of this new concept, we used Radical Innovation Design (RID) methodology, well adapted to supporting usage-based innovation projects. The RID study AutoNOM has allowed us to identify a refined understanding of the existing pain points of different ADH stakeholders (AHD patients, medical staff, retirement home staff) and investigate how existing solutions address these pain points. We found value buckets which were starting points to imagine innovative solutions. The study allowed identifying eight novel scenarios for logistic solutions to reduce ADH patients’ suffering and assess them against their ability to alleviate the RID whole “quantity of pains” of ADH issue. One of the significant results of this study is the decree allowing the use of the botulinum toxin in home healthcare in France.

This AutoNOM RID study has borne fruit: recently, on December 22, 2022, the French General Secretariat of the Social Affairs Ministry gave the official go-ahead for a 30-month trial in 4 French regions with 8 AutoNOM mobile units. This experiment will soon lead to an evaluation of the solution's effectiveness.
Art_03_424_2024.pdf
Creators: name: Franco, Manuel
Publisher: name: figshare
Year: 2024
Subjects: classificationCode: 390303
subject: Higher education

description: There exists a scarcity of neurocognitive research that has successfully used electrophysiology as an objective tool to assess different learning modalitiesthat are commonly used in anatomy. The objective of this study was to explore the trend in the expression of brain waves in medical students when using different didactic strategies in learning anatomy. An exploratory, observational, cross-sectional study was conducted on 22 first- semester medical students in anatomy. Using didactic strategies with different pedagogical tools such as biological models (human skulls and pig hearts) and/or digital application (Visible Body software), and different evaluation methods, students were grouped into three groups: "EOR1" students who learned using a skull and were evaluated with it; "EOV1" students who learned using a pig heart and were evaluated with the Visible Body software; and "EOV2" for students who learned through the Visible Body software and were evaluated with it. During the evaluation, each student was monitored in real-time using an electroencephalogram and the Emotiv EPOC brain-computer interface system to record the electro-physiological activity of beta (B), theta (T), and gamma (G) waves. The data obtained (the trend of the electrical activity of each wave and its relationship with students' performance in each didactic strategy) were analyzed using Pearson's correlation coefficient. Groups EOR1 and EOV1 had satisfactory results in their evaluations and showed a predominance of B waves (x=67.33) and T waves (x=57.67). Additionally, a strongly positive correlation (r=0.82) was found between the presence of B waves and the duration of T waves. Students who used three-dimensional biological models as a pedagogical tool showed a predominance of B and T waves, which are associated with sensorimotor and exploratory learning necessary for studying anatomy.
A study of the electromagnetic proton cyclotron instability as a generation mechanism for EMIC waves in the Earth's magnetosphere using SCATHA data
Creators: name: Nguyen, Son
name: Perez, J
name: Fennell, Joseph
Publisher: name: Auburn University
Year: 2007

description: Using 59 days of magnetic field data from SCATHA, a study of the electromagnetic proton cyclotron instability as a generation mechanism for EMIC waves in the Earth's magnetosphere has been conducted. From 1181 events found, we selected 373 events that were not influenced by the presence of He+ and O+ ions, i.e.,events with frequency above the local He+ cyclotron frequency and that had all the required accompanying data. These events occurred in all magnetic local times (MLT) sectors, with L ranging from 5.6 to 8.1 and magnetic latitudes (MLAT) from -13.7 degrees to 15.6 degrees. Assuming a pure proton plasma, the proton temperature anisotropy, Ap, is determined from the maximum normalized frequency at which power is emitted. Using measured parameters and estimated total number density, the convective growth rate, S, of Electromagnetic Ion Cyclotron (EMIC) waves as a function of frequency depends only on the parallel proton temperature, T-parallel to. Matching the observed peak in the frequency spectrum and the calculated peak in S allows the determination of T-parallel to and the proton perpendicular temperature, T-perpendicular to, for each event. Analysis of the results yields a new empirical expression for A(p) as a function of the hot proton parallel beta, beta(parallel to h), and the maximum value of the wave temporal growth rate. The relationship between A(p) and beta(parallel to h) is consistent with theoretical predictions. The dependence of A(p) on T-parallel to is consistent with the expectation that the free energy source of EMIC waves is energetic protons with T-perpendicular to > T-parallel to.
Evolution of the universe in entropic cosmologies via different formulations
Creators: name: Komatsu, Nobuyoshi
name: Kimura, Shigeo
Publisher: name: arXiv
Year: 2014
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We study two types of entropic-force models in a homogeneous, isotropic, spatially flat, matter-dominated universe. The first type is a `$Λ(t)$ type' similar to $Λ(t)$CDM (varying-lambda cold dark matter) models in which both the Friedmann equation and the acceleration equation include an extra driving term. The second type is a `BV type' similar to bulk viscous models in which the acceleration equation includes an extra driving term whereas the Friedmann equation does not. In order to examine the two types systematically, we consider an extended entropic-force model that includes a Hubble parameter ($H$) term and a constant term in entropic-force terms. The $H$ term is derived from a volume entropy whereas the constant term is derived from an entropy proportional to the square of an area entropy. Based on the extended entropic-force model, we examine four models obtained from combining the $H$ and constant terms with the $Λ(t)$ and BV types. The four models agree well with the observed supernova data and describe the background evolution of the late universe properly. However, the evolution of first-order density perturbations is different in each of the four models, especially for low redshift, assuming that an effective sound speed is negligible. The $Λ(t)$ type is found to be consistent with the observed growth rate of clustering, in contrast with the BV type examined in this study. A unified formulation is proposed as well, in order to examine density perturbations of the two types systematically.
description: Final version accepted for publication in PRD. References are corrected. [21 pages, 4 figures, and 2 tables]
Generation of near-Earth reconnection by divergent flows in the plasma sheet
Creators: name: Lin, Y
name: Swift, D
Publisher: name: Auburn University
Year: 2002

description: [1] A global two-dimensional hybrid simulation is carried out to study the evolution of the near-Earth plasma sheet. It is shown that reconnection X lines and plasmoids can be generated by diverging flows in the plasma sheet. These diverging flows can be caused by variations in the Maxwell stress due to variations of B-x and B-z components of the magnetic field outside the current sheet. In addition, the flow acceleration/deceleration in the plasma sheet can also be caused by variations in the local plasma mass density. Comparison runs have been made with a Harris model current sheet with zero B-z, and no evidence of reconnection is found. The results indicate that divergent plasma flow is a sufficient condition for reconnection even in a dissipation-less plasma.
FACCE SURPLUS PREAR project – Farmer questionnaire
Creators: name: Forster, Matthieu
name: Bane, Miranda
name: Derocles, Stephane
name: Oudoire, Geoffroy
name: Pocock, Michael JO
name: Bohan, David A
Publisher: name: Zenodo
Year: 2020

description: We developed a rotational questionnaire, co-constructed with farmers, to explore whether farmers use rotations and are interested in using them to mitigate climate change, but also to understand better farmer attitudes and decision-making for rotations, particularly in respect of climate change. We applied this questionnaire along an approximately North to South transect, running from the Southern United Kingdom to Occitanie in Southern France, covering regions we expected would vary in their current exposure to and experience of climate change. The farmer sites are presented in the attached figure. Attached are the two questionnaires, respectively in English and French, as used in the UK and France.
Millimetre-wave Site Characteristics at the Australia Telescope Compact Array
Creators: name: Indermuehle, Balthasar T.
name: Burton, Michael G.
Publisher: name: arXiv
Year: 2014
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: We present a millimetre-wave site characterisation for the Australia Telescope Compact Array (ATCA) based on nearly 9 years of data from a seeing monitor operating at this facility. The seeing monitor, which measures the phase fluctuations in the signal from a geosynchronous satellite over a 230\,m baseline caused by water vapour fluctuations along their sight lines, provides an almost gapless record since 2005, with high time resolution. We determine the root mean square (rms) of the path length variations as a function of time of day and season. Under the assumption of the "frozen screen" hypothesis, we also determine the Kolomogorov exponent, $α$, for the turbulence and the phase screen speed. From these, we determine the millimetre-wave seeing at $λ= 3.3$\,mm. Based on the magnitude of the rms path length variations, we estimate the expected fraction of the available observing time when interferometry could be successfully conducted using the ATCA, as a function of observing frequency and antenna baseline, for the time of day and the season. We also estimate the corresponding observing time fractions when using the water vapour radiometers (WVRs) installed on the ATCA in order to correct for the phase fluctuations occurring during the measurement of an astronomical source.
New Constraints on Cosmic Polarization Rotation from B-Mode Polarization in Cosmic Microwave Background
Creators: name: Alighieri, Sperello di Serego
name: Ni, Wei-Tou
name: Pan, Wei-Ping
Publisher: name: arXiv
Year: 2014
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: STPpol, POLARBEAR and BICEP2 have recently measured the cosmic microwave background (CMB) B-mode polarization in various sky regions of several tens of square degrees and obtained BB power spectra in the multipole range 20-3000, detecting the components due to gravitational lensing and to inflationary gravitational waves. We analyze jointly the results of these three experiments and propose modifications of their analysis of the spectra to include in the model, in addition to the gravitational lensing and the inflationary gravitational waves components, also the effects induced by the cosmic polarization rotation (CPR), if it exists within current upper limits. Although in principle our analysis would lead also to new constraints on CPR, in practice these can only be given on its fluctuations , since constraints on its mean angle are inhibited by the de-rotation which is applied by current CMB polarization experiments, in order to cope with the insufficient calibration of the polarization angle. The combined data fits from all three experiments (with 29% CPR-SPTpol correlation, depending on theoretical model) gives constraint ^1/2 < 27.3 mrad (1.56°) with r = 0.194 \pm 0.033. These results show that the present data are consistent with no CPR detection and the constraint on CPR fluctuation is about 1.5°. This method of constraining the cosmic polarization rotation is new, is complementary to previous tests, which use the radio and optical/UV polarization of radio galaxies and the CMB E-mode polarization, and adds a new constraint for the sky areas observed by SPTpol, POLARBEAR and BICEP2.
description: Accepted for publication by The Astrophysical Journal
Riccati equations for holographic 2-point functions
Creators: name: Papadimitriou, Ioannis
name: Taliotis, Anastasios
Publisher: name: arXiv
Year: 2013
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Any second order homogeneous linear ordinary differential equation can be transformed into a first order non-linear Riccati equation. We argue that the Riccati form of the linearized fluctuation equations that determine the holographic 2-point functions simplifies considerably the numerical computation of such 2-point functions and of the corresponding transport coefficients by computing directly the response functions, eliminating the arbitrary source from the start. Moreover, it provides a neat criterion for the infrared regularity of the fluctuations. In particular, it is shown that the infrared regularity conditions for scalar and tensor fluctuations coincide, and hence they are either both regular or both singular. We demonstrate our numerical recipe based on the Riccati equations by computing the holographic 2-point functions for the stress tensor and a scalar operator in a number of asymptotically anti de Sitter backgrounds of bottom up scalar-gravity models. Analytical results are obtained for the 2-point function of the transverse traceless part of the stress tensor in two confining geometries, including a geometry that belongs to the class of IHQCD. We find that in this background the spin-2 spectrum is linear and, as expected, the position space 2-point function decays exponentially at large distances at a rate proportional to the confinement scale.
description: 33 pages, 5 figures, 2 appendices. Changes with respect to V1: major extension of the numerical and analytical analysis. Added lemma 5.1, appendices A and B and references. Corrected typos
Systematics of small parahydrogen clusters in two dimensions
Creators: name: Idowu, Saheed
name: Boninsegni, Massimo
Publisher: name: arXiv
Year: 2014
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We studied by means of computer simulations the low temperature properties of two-dimensional parahydrogen clusters comprising between 7 and 30 molecules. Computed energetics is in quantitative agreement with that reported in the only previous study [Phys. Rev. B 65, 174527 (2002)], but a generally stronger superfluid response is obtained here for clusters with more than ten molecules. Moreover, all the clusters, including the smallest one, display a well-defined, clearly identifiable solidlike structure; with only one possible exception, those with fewer than 25 molecules are (almost) entirely superfluid at the lowest temperature considered here (i.e., 0.25 K), and can thus be regarded as nanoscale "supersolids". The implications of these results on a possible bulk two-dimensional superfluid phase of parahydrogen are discussed.
Impact of Biofield Energy Treated Herbomineral Formulation (The Trivedi Effect®) on Mouse Dendritic and Splenocyte Cells for Modulation of Pro-inflamm
Creators: name: Hancharuk, Aksana
Publisher: name: SMN - The ScienceMedia Network
Year: 2019
Subjects: Natural Sciences
Biology

description: The use of herbomineral formulation in the healthcare sector for different chronic diseases is gaining popularity due to its fewer side effects, high safety profile, and cost effectiveness. A new proprietary herbomineral formulation was formulated, consisting of four essential ingredients viz. herbal root extract (ashwagandha), and minerals (zinc, magnesium, and selenium). The study aims to evaluate the in vitro effect of Biofield Energy Healing (The Trivedi Effect®) on the test formulation using murine dendritic (DCs) and splenocyte cells. The herbomineral formulation was divided into two parts; one was represented as control, while the other part was treated with the Biofield Energy Healing Treatment remotely by eighteen renowned Biofield Energy Healers (The Trivedi Effect®) and defined as the Biofield Treated formulation. The effect of the test formulation on these cells were monitored by an estimation of pro-inflammatory cytokines level such as tumor necrosis factor (TNF-α), macrophage inflammatory protein (MIP-1α), and interleukin (IL-1β) in cell culture supernatants at the non-cytotoxic concentrations of the test formulation using MTT assay. The DCs were treated with the Biofield Energy Treated test formulation at different concentrations (i.e. 1.05 to 1052.5 µg/mL) for 24 hours, and the results showed significant (p≤0.001) suppression of TNF-α levels at all the tested concentrations with a maximum percentage decrease by 43.64% at 5.2 µg/mL concentration in the Biofield Treated formulation as compared with the untreated test formulation. Further, the Biofield Treated formulation also demonstrated inhibition of MIP-1α and IL-1β at a concentration range of 0.0000105 to 10.5 µg/mL in LPS stimulated splenocyte cells. There was a significant (p≤0.001) inhibition of MIP-1α (26.52%) and IL-1β (35.28%) in the Biofield Treated test formulation at concentration 0.000105 µg/mL and 0.0000105 µg/mL, respectively in comparison to the untreated test formulation. Overall, these results suggest that the Biofield Energy Healing based herbomineral formulation (The Trivedi Effect®) significantly down-regulated the tested cytokines expression in DCs and splenocyte cells as compared to the untreated formulation. Therefore, the Biofield Healing based formulation might be useful as a better anti-inflammatory product for many chronic and acute inflammatory disease conditions and autoimmune disorders. The Biofield Energy Treatment based formulation can also be effectively applied in cases of organ transplants, stress management and anti-aging by improving overall health.
Ontology Development in Catalysis: Status of NFDI4Cat-TA1
Creators: name: Behr, Alexander
name: Linke, David
name: Dörr, Mark
name: Kockmann, Norbert
Publisher: name: Zenodo
Year: 2022
Subjects: Katalytikertreffen
Conference presentation
TA1-status

description: Presentation held by David Linke at the 55. Katalytikertreffen in Weimar regarding the current state of NFDI4Cat TA1. First, an introduction to ontologies in general is given. Then the current state of TA1 regarding already found ontologies and workflow of SKOS-Taxonomies is given. Manual and automated ways of conducting the task of taxonomy creation are elaborated.
title: К вопросу о применении аппаратного Т-образного тонкокишечного анастомоза
Creators: name: Ильканич, Андрей
name: Дарвин, Владимир
name: Алиев, Фуад
name: Воронин, Юрий
Publisher: name: Новгородский государственный университет имени Ярослава Мудрого (НовГУ)
Year: 2020

description: Для оценки эффективности применения аппаратного Т-образного тонкокишечного анастомоза проведен одноцентровой ретроспективный анализ результатов лечения 53 пациентов с превентивными илестомами. Они были пролечены в период 2015-2020 гг. по поводу злокачественных новообразований толстой кишки и органов малого таза. По типу накладываемого анастомоза 53 (100,0%) пациента были разделены на основную и контрольную группы. Для оценки возможности проведения сравнительного анализа эти группы были сопоставлены по полу, возрасту, тяжести коморбидной патологии, среднему ИМТ. При анализе результатов применения аппаратного Т-образного анастомоза было установлено, что метод позволяет сократить продолжительность реконструктивно-восстановительного вмешательства с 70 (55;120) до 45 (30;65) минут, снизить число послеоперационных осложнений с 36,0% до 14,3%, уменьшить сроки нахождения пациентов в стационаре с 11 (9;13) до 7 (6;9) суток.
How do open infrastructures work together? - Crossref
Creators: name: Feeney, Patrica
Publisher: name: Zenodo
Year: 2022
Subjects: DataCite Member Meeting 2022
open infrastructure
Crossref

description: Providers of open infrastructures collaborate to enable seamless scholarly communication. But what are they actually doing to realize this? How do open infrastructures integrate metadata of other providers into their services? This open community session gives open infrastructures the opportunity to let us see scholarly communication through their eyes. Throughout the session you will be able to ask the panelists anything about their services. Speaker: Patrica Feeney (Crossref) A recording of the presentation can be found at: https://www.youtube.com/watch?v=c43cb80WR2o&t=200s