cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Evaporation-driven coalescence of two droplets undergoing freezing
Creators: name: Kavuri, Sivanandan
name: Karapetsas, George
name: Sharma, Chander Shekhar
name: Sahu, Kirti Chandra
Publisher: name: arXiv
Year: 2024
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: We examine the evaporation-induced coalescence of two droplets undergoing freezing by conducting numerical simulations employing the lubrication approximation. When two sessile drops undergo freezing in close vicinity over a substrate, they interact with each other through the gaseous phase and the simultaneous presence of evaporation/condensation. In an unsaturated environment, the evaporation flux over the two volatile sessile drops is asymmetric, with lower evaporation in the region between the two drops. This asymmetry in the evaporation flux generates an asymmetric curvature in each drop, which results in a capillary flow that drives the drops closer to each other, eventually leading to their coalescence. This capillary flow, driven by evaporation, competes with the upward movement of the freezing front, depending on the relative humidity in the surrounding environment. We found that higher relative humidity reduces the evaporative flux, delaying capillary flow and impeding coalescence by restricting contact line motion. For a constant relative humidity, the substrate temperature governs the coalescence phenomenon, and resulting condensation can accelerate this process. Interestingly, lower substrate temperatures are observed to facilitate faster propagation of the freezing front, which, in turn, restricts coalescence.
description: 36 pages, 17 figures. arXiv admin note: text overlap with arXiv:2312.03271
CJB910173_Supplemental_Material_CLN – Supplemental material for What Happens in Home Visits? Examining a Key Parole Activity
Creators: name: Meredith, Tammy
name: Hawk, Shila René
name: Johnson, Sharon
name: Prevost, John P.
name: Braucht, George
Publisher: name: SAGE Journals
Year: 2020
Subjects: subject: 111799 Public Health and Health Services not elsewhere classified
subject: FOS: Health sciences
subject: 160299 Criminology not elsewhere classified
subject: FOS: Law
subject: 170199 Psychology not elsewhere classified
subject: FOS: Psychology

description: Supplemental material, CJB910173_Supplemental_Material_CLN for What Happens in Home Visits? Examining a Key Parole Activity by Tammy Meredith, Shila René Hawk, Sharon Johnson, John P. Prevost and George Braucht in Criminal Justice and Behavior
Supplemental Material, Supplementary_material_Therapists_manual_J_Child_Health_Care_Fig_2_+_tiff - Therapy competence in delivering a brief cognitive behavioural therapy intervention to reduce maternal anxiety associated with child food allergy
Creators: name: Vickers, Bea
name: Boyle, Robert J
name: Thisanayagam Umasunthar
name: Smith, Jared G
name: Hodes, Matthew
Publisher: name: SAGE Journals
Year: 2019
Subjects: subject: 111708 Health and Community Services
subject: FOS: Health sciences
subject: 111099 Nursing not elsewhere classified
subject: 111403 Paediatrics
subject: FOS: Clinical medicine

description: Supplemental Material, Supplementary_material_Therapists_manual_J_Child_Health_Care_Fig_2_+_tiff for Therapy competence in delivering a brief cognitive behavioural therapy intervention to reduce maternal anxiety associated with child food allergy by Bea Vickers, Robert J Boyle, Thisanayagam Umasunthar, Jared G Smith and Matthew Hodes in Journal of Child Health Care
R4-Demand-Restricted_Growth_Theory-appendix – Supplemental material for A New Theory of Demand-Restricted Growth: The Basic Idea
Creators: name: Gries, Thomas
Publisher: name: SAGE Journals
Year: 2019
Subjects: subject: Economics
subject: 150310 Organisation and Management Theory
subject: FOS: Economics and business

description: Supplemental material, R4-Demand-Restricted_Growth_Theory-appendix for A New Theory of Demand-Restricted Growth: The Basic Idea by Thomas Gries in The American Economist
Supplementary_Table_1 – Supplemental material for Perinatal anxiety and depression: Awareness and attitudes in Australia
Creators: name: Smith, Terri
name: Gemmill, Alan W
name: Milgrom, Jeannette
Publisher: name: SAGE Journals
Year: 2019
Subjects: subject: 170199 Psychology not elsewhere classified
subject: FOS: Psychology
subject: 110319 Psychiatry (incl. Psychotherapy)
subject: FOS: Clinical medicine

description: Supplemental material, Supplementary_Table_1 for Perinatal anxiety and depression: Awareness and attitudes in Australia by Terri Smith, Alan W Gemmill and Jeannette Milgrom in International Journal of Social Psychiatry
LavAtmos 2.0: Incorporating Volatiles Species in Vaporization Models
Creators: name: van Buchem, Christiaan P. A.
name: Zilinskas, Mantas
name: Miguel, Yamila
name: van Westrenen, Wim
Publisher: name: arXiv
Year: 2024
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: Due to strong irradiation, hot rocky exoplanets are able to sustain lava oceans. Direct interaction between these oceans and overlying atmospheres can provide insight into planetary interiors. In order to fully understand how the composition of the atmosphere of such planets are affected by the properties of the oceans, comprehensive chemical equilibrium models are required. Thus far, most models have only taken non-volatile species into account when calculating lava vaporisation. We investigate the effect of including C-, H-, N-, S-, and P-bearing species in the equilibrium lava vaporisation calculations on the overall atmospheric composition of hot rocky exoplanets by expanding our LavAtmos code. In LavAtmos 2.0 we integrate the chemical equilibrium code FastChem to expand the considered gas phase species to 523. We apply this new approach to calculate the composition of "pure" atmospheres which contain only a single volatile element and more complex atmospheres which contain C, H, N, S, and P. We also test two proposed compositions for the atmosphere of 55-Cnc e. We find that the inclusion of volatile elements in vaporisation calculations increases the partial pressures of vaporised species for all tested atmospheric compositions. Our models indicate that the tested volatile atmospheres above a lava ocean have a relatively low C-O ratio. This demonstrates the utility of complex chemical models that better describe the chemical behavior of atmospheres across a wide range of pressures and temperatures. Volatile elements must be taken into account for comprehensive modeling of vaporisation from a surface lava ocean into a volatile atmosphere. Vaporised species such as SiO, TiO, and Na may be present in greater abundances than previously estimated. A low atmospheric C/O ratio may be able to function as a new tracer for the presence of surface lava oceans on hot rocky exoplanets.
description: In rev. A&A (16 pages, 14 figures)
Identification of resistance to Eurygaster integriceps Put. on some bread wheat genotypes
Creators: name: Aykut Tonk, Fatma
name: Kaya, Ekrem
name: İştipliler, Deniz
name: İlker, Emre
name: Turanlı, Ferit
name: Tosun, Muzaffer
name: Yılmaz, Erkan
name: Ersin, Firdevs
name: Savran Takak, Ebru
name: Çakır, Mehmet
Publisher: name: Journal of Applied Botany and Food Quality
Year: 2017
Subjects: Sunn pest; bread wheat; resistance; sedimentation; delayed sedimentation

description: Sunn pest (Eurygaster integriceps Put.) is one of the most important pests of wheat in Eastern Europe including Turkey, West and Cen-tral Asia. Its damage on leaves, stems, spikes and grains reduce the baking quality of flour made from damaged grains. In this study, some wheat genotypes from Turkey and ICARDA were evaluated for the pest resistance. The genotypes were planted in a randomized block design using hill plots in nylon mesh screening cages in wheat growing season of 2011-2012 and 2012-2013. Sunn pest population was collected from Çanakkale province, where the pest was intensely found in recent years. The plants of each hill plots were infested with one male and one female Sunn pest adults. The results with 12.5% sucking damage showed that the genotypes from ICARDA had higher resistance than the landraces from Turkey to Sunn pest. Especially, the genotypes IC3 and IC4 from ICARDA and TR7 from Turkey with respect to their SED and DSED values were found the most promising genotypes resistant to Sunn pest for future breeding programs.
description: Journal of Applied Botany and Food Quality, Vol 90 (2017): Journal of Applied Botany and Food Quality
Supplementary_files_rev – Supplemental material for The Role of Pets in Supporting Cognitive-Behavioral Chronic Pain Self-Management: Perspectives of Older Adults
Creators: name: Janevic, Mary R.
name: Varick Shute
name: Connell, Cathleen M
name: Piette, John D.
name: Goesling, Jenna
name: Fynke, Julie
Publisher: name: SAGE Journals
Year: 2019
Subjects: subject: 110306 Endocrinology
subject: FOS: Clinical medicine
subject: 110308 Geriatrics and Gerontology
subject: 111799 Public Health and Health Services not elsewhere classified
subject: FOS: Health sciences

description: Supplemental material, Supplementary_files_rev for The Role of Pets in Supporting Cognitive-Behavioral Chronic Pain Self-Management: Perspectives of Older Adults by Mary R. Janevic, Varick Shute, Cathleen M Connell, John D. Piette, Jenna Goesling and Julie Fynke in Journal of Applied Gerontology
Die Römischen Schreibtafeln (Tabulae Ceratae) Aus Tasgetium/Eschenz
Creators: name: Hartmann, Benjamin
Publisher: name: Zenodo
Year: 2011
Subjects: epigraphy
inscription
graffiti
writing tablet
writing material
writing
classical studies
history
roman history
tabula cerata

description: Edition of Roman wooden wax tablets from the vicus Tasgetium (Eschenz, CH). (in German)
Gravity from entropy
Creators: name: Bianconi, Ginestra
Publisher: name: arXiv
Year: 2024
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: High Energy Physics - Theory (hep-th)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Gravity is derived from an entropic action coupling matter fields with geometry. The fundamental idea is to relate the metric of Lorentzian spacetime to a quantum operator, playing the role of an renormalizable effective density matrix and to describe the matter fields topologically, according to a Dirac-Kähler formalism, as the direct sum of a zero-form, a one-form and a two-form. While the geometry of spacetime is defined by its metric, the matter fields can be used to define an alternative metric, the metric induced by the matter fields, which geometrically describes the interplay between spacetime and matter. The proposed entropic action is the quantum relative entropy between the metric of spacetime and the metric induced by the matter fields. The modified Einstein equations obtained from this action reduce to the Einstein equations with zero cosmological constant in the regime of low coupling. By introducing the G-field, which acts as a set of Lagrangian multipliers, the proposed entropic action reduces to a dressed Einstein-Hilbert action with an emergent small and positive cosmological constant only dependent on the G-field. The obtained equations of modified gravity remain second order in the metric and in the G-field. A canonical quantization of this field theory could bring new insights into quantum gravity while further research might clarify the role that the G-field could have for dark matter.
description: (16 pages, 1 figure)
Massive star cluster formation III. Early mass segregation during cluster assembly
Creators: name: Polak, Brooke
name: Mac Low, Mordecai-Mark
name: Klessen, Ralf S.
name: Zwart, Simon Portegies
name: Andersson, Eric P.
name: Appel, Sabrina M.
name: Cloutier, Claude Cournoyer
name: Glover, Simon C. O.
name: McMillan, Stephen L. W.
Publisher: name: arXiv
Year: 2024
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Mass segregation is seen in many star clusters, but whether massive stars form in the center of a cluster or migrate there dynamically is still debated. N-body simulations have shown that early dynamical mass segregation is possible when sub-clusters merge to form a dense core with a small crossing time. However, the effect of gas dynamics on both the formation and dynamics of the stars could inhibit the formation of the dense core. We aim to study the dynamical mass segregation of star cluster models that include gas dynamics and self-consistently form stars from the dense substructure in the gas. Our models use the Torch framework, which is based on AMUSE and includes stellar and magnetized gas dynamics, as well as stellar evolution and feedback from radiation, stellar winds, and supernovae. Our models consist of three star clusters forming from initial turbulent spherical clouds of mass $10^{4,5,6}\rm~M_\odot$ and radius $11.7\rm~pc$ that have final stellar masses of $3.6\times10^3\rm~M_\odot$, $6.5\times10^4\rm~M_\odot$, and $8.9\times10^5\rm~M_\odot$, respectively. There is no primordial mass segregation in the model by construction. All three clusters become dynamically mass segregated at early times via collapse confirming that this mechanism occurs within sub-clusters forming directly out of the dense substructure in the gas. The dynamics of the embedded gas and stellar feedback do not inhibit the collapse of the cluster. We find that each model cluster becomes mass segregated within $2~$Myr of the onset of star formation, reaching the levels observed in young clusters in the Milky Way. However, we note that the exact values are highly time-variable during these early phases of evolution. Massive stars that segregate to the center during core collapse are likely to be dynamically ejected, a process that can decrease the overall level of mass segregation again.
description: Submitted to A&A. 8 pages, 4 figures
New ultracool dwarf candidates from multi-epoch WISE data
Creators: name: Karpov, Sergey
name: Malkov, Oleg
name: Avdeeva, Aleksandra
Publisher: name: arXiv
Year: 2024
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Thirty years after the discovery of brown dwarfs, the search for these objects continues, particularly in the vicinity of the Sun. Objects near the Sun are characterized by large proper motions, making them seen as fast-moving objects. While the Gaia DR3 catalogue is a comprehensive source of proper motions, it lacks the depth needed for discovering fainter objects. Modern multi-epoch surveys, with their greater depth, offer a new opportunity for systematic search for ultracool dwarfs. The study aims to systematically search for high proper motion objects using the newly released catalogue of epochal WISE data in order to identify new brown dwarf candidates in the solar neighborhood, estimate their spectral types, distances and spatial velocities. We used recently released unTimely catalogue of epochal detections in unWISE coadds to search for objects with high proper motions using simple motion detection algorithm, combined with machine learning based artefact rejection routine. This method was used to identify objects with proper motions exceeding approximately 0.3 arcseconds per year. The identified objects were then cross-referenced with data from other large-scale sky surveys to further analyze their characteristics. The search yielded 21,885 moving objects with significant proper motions, 258 of which had not been previously published. All except 6 of them are compatible with being ultracool dwarfs. Among these, at least 33 were identified as most promising new T dwarf candidates, with estimated distances closer than about 40 parsecs, and effective temperatures less than 1300 K.
description: Table 2 is available online at https://doi.org/10.5281/zenodo.14651236. Submitted to A&A
Online_appendix_16.5 – Supplemental material for Coalitions and counter-coalitions in online contestation: An analysis of the German and British climate change debate
Creators: name: Adam, Silke
name: Häussler, Thomas
name: Schmid-Petri, Hannah
name: Reber, Ueli
Publisher: name: SAGE Journals
Year: 2019
Subjects: subject: 200199 Communication and Media Studies not elsewhere classified
subject: FOS: Media and communications

description: Supplemental material, Online_appendix_16.5 for Coalitions and counter-coalitions in online contestation: An analysis of the German and British climate change debate by Silke Adam, Thomas Häussler, Hannah Schmid-Petri and Ueli Reber in New Media & Society
Additional file 1 of Efficacy and safety of particle therapy for inoperable stage II-III non-small cell lung cancer: a systematic review and meta-analysis
Creators: name: Chen, Yanliang
name: Luo, Hongtao
name: Liu, Ruifeng
name: Tan, Mingyu
name: Wang, Qian
name: Wu, Xun
name: Du, Tianqi
name: Liu, Zhiqiang
name: Sun, Shilong
name: Zhang, Qiuning
name: Wang, Xiaohu
Publisher: name: figshare
Year: 2024
Subjects: subject: Physical Sciences not elsewhere classified
subject: Medicine
subject: Ecology
subject: FOS: Biological sciences
subject: Cancer
subject: Infectious Diseases
subject: FOS: Health sciences

description: Supplementary Material 1
On the Linear Stability of Partially and Fully Saturated Atmospheres to Moist Convection
Creators: name: Oishi, Jeffrey S.
name: Brown, Benjamin P.
Publisher: name: arXiv
Year: 2024
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: Atmospheric and Oceanic Physics (physics.ao-ph)
subject: FOS: Physical sciences

description: We present a linear analysis of a minimal model of moist convection under a variety of atmospheric conditions. The stationary solutions that we analyze include both fully saturated and partially unsaturated atmospheres in both unconditionally and conditionally unstable cases. We find that all of the solutions we consider are linearly unstable via exchange of stability when sufficiently driven. The critical Rayleigh numbers vary by over an order of magnitude between unconditionally unstable and conditionally unstable atmospheres. The unsaturated atmospheres are notable for the presence of linear gravity wave-like oscillations even in unstable conditions. We study their eigenfunction structure and find that the buoyancy and moisture perturbations are anticorrelated in $z$, such that regions of negative buoyancy have positive moisture content. We suggest that these features in unsaturated atmospheres may explain the phenomenon of gravity wave shedding by moist convective plumes.
description: 27 pages, 18 figures
Supplemental material for Use of real-time videoconferencing to deliver physical therapy services: A scoping review of published and emerging evidence
Creators: name: Horsley, Stephanie
name: Schock, Gunnar
name: Grona, Stacey L
name: Montieth, Kara
name: Bryttnee Mowat
name: Stasiuk, Kiara
name: Boden, Catherine
name: Bath, Brenna
Publisher: name: SAGE Journals
Year: 2019
Subjects: subject: 111708 Health and Community Services
subject: FOS: Health sciences
subject: 111799 Public Health and Health Services not elsewhere classified

description: Supplemental Material for Use of real-time videoconferencing to deliver physical therapy services: A scoping review of published and emerging evidence by Stephanie Horsley, Gunnar Schock, Stacey L Grona, Kara Montieth, Bryttnee Mowat, Kiara Stasiuk, Catherine Boden and Brenna Bath in Journal of Telemedicine and Telecare
Supplemental Material, DS_10.1177_0022242919857698 - Brand Coolness
Creators: name: Warren, Caleb
name: Batra, Rajeev
name: Loureiro, Sandra Maria Correia
name: Bagozzi, Richard P.
Publisher: name: SAGE Journals
Year: 2019
Subjects: subject: 150402 Hospitality Management
subject: FOS: Economics and business

description: Supplemental Material, DS_10.1177_0022242919857698 for Brand Coolness by Caleb Warren, Rajeev Batra, Sandra Maria Correia Loureiro and Richard P. Bagozzi in Journal of Marketing
Interaction imbalanced spin-orbit coupled quantum droplets
Creators: name: Gangwar, Sonali
name: Ravisankar, Rajamanickam
name: Mistakidis, S. I.
name: Muruganandam, Paulsamy
name: Mishra, Pankaj Kumar
Publisher: name: arXiv
Year: 2024
Subjects: subject: Quantum Gases (cond-mat.quant-gas)
subject: FOS: Physical sciences

description: We explore the ground states and quench dynamics of one-dimensional quantum droplets with spin-orbit coupling (SOC) and an imbalance in intracomponent interactions. A plethora of miscible ground state stripe and standard (i.e., non-modulated) droplets is found depending on the SOC wavenumber and building upon Gaussian to flat-top background for increasing (decreasing) atom number (interactions). Deformations among the states were accompanied by spin population transfer caused by the Rabi coupling and could be controlled by adjusting the interactions or the SOC parameters. When considering a trap, we identified a transition from a bound to a trapped gas many-body state, characterized by a sign change of the chemical potential, which occurred at lower (larger) atom numbers for tighter traps (stronger interactions). The droplet's breathing motion was accompanied by minor population transfer, and its frequency increases for a larger intracomponent interaction ratio or reaching a maximum at SOC wavenumbers, where the transition from non-modulated flat-top to stripe droplets occurred. We witness droplet fragmentation for abrupt changes in the Rabi coupling while large amplitude quenches of the SOC wavenumber trigger spin-demixing, resulting in constant amplitude but opposite direction motion of untrapped droplets or in-trap out-of-phase oscillating droplets. Our findings have implications for controlled spin-demixing processes of droplets and the excitation of relevant magnetic bound states.
description: Published version
The Hierarchical Growth of Bright Central Galaxies and Intracluster Light as Traced by the Magnitude Gap
Creators: name: Golden-Marx, Jesse B.
name: Zhang, Y.
name: Ogando, R. L. C.
name: Yanny, B.
name: Pereira, M. E. S.
name: Hilton, M.
name: Aguena, M.
name: Allam, S.
name: Andrade-Oliveira, F.
name: Bacon, D.
name: Brooks, D.
name: Rosell, A. Carnero
name: Carretero, J.
name: Cheng, T. -Y.
name: da Costa, L. N.
name: De Vicente, J.
name: Desai, S.
name: Doel, P.
name: Everett, S.
name: Ferrero, I.
name: Frieman, J.
name: García-Bellido, J.
name: Gatti, M.
name: Giannini, G.
name: Gruen, D.
name: Gruendl, R. A.
name: Gutierrez, G.
name: Hinton, S. R.
name: Hollowood, D. L.
name: Honscheid, K.
name: James, D. J.
name: Kuehn, K.
name: Lee, S.
name: Mena-Fernández, J.
name: Menanteau, F.
name: Mohr, J.
name: Miquel, R.
name: Palmese, A.
name: Pieres, A.
name: Malagón, A. A. Plazas
name: Samuroff, S.
name: Sanchez, E.
name: Schubnell, M.
name: Sevilla-Noarbe, I.
name: Smith, M.
name: Suchyta, E.
name: Tarle, G.
name: Vikram, V.
name: Walker, A. R.
name: Weaverdyck, N.
name: Wiseman, P.
Publisher: name: arXiv
Year: 2024
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Using a sample of 2800 galaxy clusters identified in the Dark Energy Survey across the redshift range $0.20 < z < 0.60$, we characterize the hierarchical assembly of Bright Central Galaxies (BCGs) and the surrounding intracluster light (ICL). To quantify hierarchical formation we use the stellar mass - halo mass (SMHM) relation, comparing the halo mass, estimated via the mass-richness relation, to the stellar mass within the BCG+ICL system. Moreover, we incorporate the magnitude gap (M14), the difference in brightness between the BCG (measured within 30 kpc) and 4th brightest cluster member galaxy within 0.5 $R_{200,c}$, as a third parameter in this linear relation. The inclusion of M14, which traces BCG hierarchical growth, increases the slope and decreases the intrinsic scatter, highlighting that it is a latent variable within the BCG+ICL SMHM relation. Moreover, the correlation with M14 decreases at large radii. However, the stellar light within the BCG+ICL transition region (30 kpc - 80 kpc) most strongly correlates with halo mass and has a statistically significant correlation with M14. Since the transition region and M14 are independent measurements, the transition region may grow due to the BCG's hierarchical formation. Additionally, as M14 and ICL result from hierarchical growth, we use a stacked sample and find that clusters with large M14 values are characterized by larger ICL and BCG+ICL fractions, which illustrates that the merger processes that build the BCG stellar mass also grow the ICL. Furthermore, this may suggest that M14 combined with the ICL fraction can identify dynamically relaxed clusters.
description: 16 pages, 5 Figures, Accepted for Publication in MNRAS on 2/2025
Pareto-Optimal Peer-to-Peer Risk Sharing with Robust Distortion Risk Measures
Creators: name: Ghossoub, Mario
name: Zhu, Michael B.
name: Chong, Wing Fung
Publisher: name: arXiv
Year: 2024
Subjects: subject: Risk Management (q-fin.RM)
subject: FOS: Economics and business

description: We study Pareto optimality in a decentralized peer-to-peer risk-sharing market where agents' preferences are represented by robust distortion risk measures that are not necessarily convex. We obtain a characterization of Pareto-optimal allocations of the aggregate risk in the market, and we show that the shape of the allocations depends primarily on each agent's assessment of the tail of the aggregate risk. We quantify the latter via an index of probabilistic risk aversion, and we illustrate our results using concrete examples of popular families of distortion functions. As an application of our results, we revisit the market for flood risk insurance in the United States. We present the decentralized risk sharing arrangement as an alternative to the current centralized market structure, and we characterize the optimal allocations in a numerical study with historical flood data. We conclude with an in-depth discussion of the advantages and disadvantages of a decentralized insurance scheme in this setting.
Additional file 3 of A genetic tool to express long fungal biosynthetic genes
Creators: name: Kirchgaessner, Leo
name: Wurlitzer, Jacob M.
name: Seibold, Paula S.
name: Rakhmanov, Malik
name: Gressler, Markus
Publisher: name: figshare
Year: 2024
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 3: Table S2. Organisms used in this study.
Seven decades of exploring planetary interiors with rotating convection experiments
Creators: name: Pothérat, Alban
name: Horn, Susanne
Publisher: name: arXiv
Year: 2024
Subjects: subject: Geophysics (physics.geo-ph)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: The interiors of many planets consist mostly of fluid layers. When these layers are subject to superadiabatic temperature or compositional gradients, turbulent convection transports heat and momentum. In addition, planets are fast rotators. Thus, the key process that underpins planetary evolution, the dynamo action, flow patterns and more, is rotating convection. Because planetary interiors are inaccessible to direct observation, experiments offer physically consistent models that are crucial to guide our understanding. If we can fully understand the laboratory model, we may eventually fully understand the original. Experimentally reproducing rotating thermal convection relevant to planetary interiors comes with specific challenges, e.g. modelling the central gravity field of a planet that is parallel to the temperature gradient. Three classes of experiments tackle this challenge. One approach consists of using an alternative central force field, such as the electric force. These are, however, weaker than gravity and require going to space. Another method entails rotating the device fast enough so that the centrifugal force supersedes Earth's gravity. This mimics the equatorial regions of a planet. Lastly, by using the actual lab gravity aligned with the rotation axis, insight into the polar regions is gained. These experiments have been continuously refined during the past seven decades. We review their evolution, from the early days of visualising the onset patterns of convection, over central force field experiments in spacecrafts, liquid metal experiments, to the latest optical velocity mapping of rotating magnetoconvection in sulfuric acid inside high-field magnets. We show how innovative experimental design and emerging experimental techniques advanced our understanding and painted a more realistic picture of planetary interiors, including Earth's liquid metal outer core.
description: 55 pages, 17 figures
Higher-genus Fay-like identities from meromorphic generating functions
Creators: name: Baune, Konstantin
name: Broedel, Johannes
name: Im, Egor
name: Lisitsyn, Artyom
name: Moeckli, Yannis
Publisher: name: arXiv
Year: 2024
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Algebraic Geometry (math.AG)
subject: FOS: Physical sciences
subject: FOS: Mathematics

description: A possible way of constructing polylogarithms on Riemann surfaces of higher genera facilitates integration kernels, which can be derived from generating functions incorporating the geometry of the surface. Functional relations between polylogarithms rely on identities for those integration kernels. In this article, we derive identities for Enriquez' meromorphic generating function and investigate the implications for the associated integration kernels. The resulting identities are shown to be exhaustive and therefore reproduce all identities for Enriquez' kernels conjectured in arXiv:2407.11476 recently.
description: 31+8 pages
title: The Catholic Church in the Nicaraguan Revolution: Interdependence and Social Movements
Creators: name: Firth, Eric W.
Publisher: name: Old Dominion University
publisherIdentifier: https://ror.org/04zjtrb98
publisherIdentifierScheme: ROR
Year: 2001

description: In July 1979, Anastasio Somoza Garcia fled Nicaragua, signaling the beginning of a true revolution, in every sense of the word. The triumph of the Nicaraguan Revolution hinged primarily on the development of a broad-based opposition coalition that included workers, peasants, the bourgeoisie and conservative upper-classes, students, and Catholic Christians. For centuries the Catholic Church in Nicaragua had maintained a mutually supportive relationship with the State. In the mid-1960s, however, a social movement began to sweep through the Church at the grassroots, causing the foundations of the Church-State relationship to shift dramatically. This social movement manifested itself in a common sense of injustice and emerging solidarity among Catholics, based on a revised interpretation of common Christian symbols, themes, and concerns. It spread through novel base organizations and pastoral methods, capitalizing on political opportunity offered not only by the regime but also by the hierarchy of Nicaraguan bishops. By the late 1970s elements the Catholic Church had fostered and participated in both the radical vanguard of the Revolution and its more cautious support, contributing to the momentous changes that engulfed Nicaraguan society throughout the 1970s and 1980s. Yet the origin of this key Catholic social movement was not Nicaraguan. In fact, all of its basic components were imported from the movement in the worldwide Catholic Church known as Liberation Theology. Only by using the analytical tools of both social movement theory and interdependence theory can we fully understand the changes in the Nicaraguan Church, and how those changes redounded to changes in Nicaraguan society.
Supplementary_Material – Supplemental material for Institutions, contexts, and ethnic violence in comparative perspective
Creators: name: Lee, Feng-Yu
name: Tse-Min Lin
Publisher: name: SAGE Journals
Year: 2020
Subjects: subject: 160607 International Relations
subject: FOS: Political science

description: Supplemental material, Supplementary_Material for Institutions, contexts, and ethnic violence in comparative perspective by Feng-yu Lee and Tse-min Lin in International Political Science Review
Supplemental Material, Appendix - Spending the pupil premium: What influences leaders’ decision-making?
Creators: name: Morris, Rebecca
name: Dobson, Graeme
Publisher: name: SAGE Journals
Year: 2020
Subjects: subject: Education
subject: 150310 Organisation and Management Theory
subject: FOS: Economics and business

description: Supplemental Material, Appendix for Spending the pupil premium: What influences leaders’ decision-making? by Rebecca Morris and Graeme Dobson in Educational Management Administration & Leadership
Principles of hydrodynamic particle manipulation in internal Stokes flow
Creators: name: Liu, Xuchen
name: Das, Partha Kumar
name: Hilgenfeldt, Sascha
Publisher: name: arXiv
Year: 2024
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: Manipulation of small-scale particles across streamlines is the elementary task of microfluidic devices. Many such devices operate at very low Reynolds numbers and deflect particles using arrays of obstacles, but a systematic quantification of relevant hydrodynamic effects has been lacking. Here, we explore an alternate approach, rigorously modeling the displacement of force-free spherical particles in vortical Stokes flows under hydrodynamic particle-wall interaction. Certain Moffatt-like eddy geometries with broken symmetry allow for systematic deflection of particles across streamlines, leading to particle accumulation at either Faxen field fixed points or limit cycles. Moreover, particles can be forced onto trajectories approaching channel walls exponentially closely, making quantitative predictions of particle capture (sticking) by short-range forces possible. This rich, particle size-dependent behavior suggests the versatile use of inertial-less flow in devices with a long particle residence time for concentration, sorting, or filtering.
title: Cultivating a Culture of Food Justice
title: Impacts of Community Based Economies on Farmers and Neighborhood Leaders in the Case of Fresh Stop Markets in Kentucky
titleType: Subtitle
Creators: name: Hyden, Heather
Publisher: name: University of Kentucky
Year: 2017
Subjects: subject: Civic and Community Engagement
subject: Community-Based Research
subject: Food Security
subject: Human Geography
subject: FOS: Social and economic geography
subject: Inequality and Stratification
subject: Leadership Studies
subject: Place and Environment
subject: Rural Sociology

description: In this thesis, I focus on two tensions within the alternative agro-food movement. First is a question of who/what community is allowed to define food systems problems and then implement solutions. For example, food desert metaphors rely discursively on defining communities as being “without”, which perpetuates needs-based narratives, in which only professional “experts” know how to solve problems of food access. These representations ignore the creativity, agency, and resiliency of everyday food justice mobilizations happening at the grassroots level. Second, what form can solutions take within hegemonic constructions of development? I build a theoretical model based on Black geographies (McKittrick, 2013) and feminist economic geography (Gibson-Graham, 2006) and apply it to an unique model of a grassroots-driven alternative agriculture initiative in Kentucky, Fresh Stop Markets (FSM). Further, with the use of the Community Capitals Framework (Flora & Flora, 2008), I analyze the value(s) of participating in FSM for both farmers and procurement organizers (farmer liaisons). My conclusions signal a need for increased investment in human, social, and cultural capital systems to create a culture of food justice in our communities. These investments allow for both farmers and limited-income consumers to benefit and create long-term sustainability, which center equity and cooperation.
Three-dimensional coherent structures in a curved pipe flow
Creators: name: Song, Runjie
name: Deguchi, Kengo
Publisher: name: arXiv
Year: 2024
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: Dean's approximation for curved pipe flow, valid under loose coiling and high Reynolds numbers, is extended to study three-dimensional travelling waves. Two distinct types of solutions bifurcate from the Dean's classic two-vortex solution. The first type arises through a supercritical bifurcation from inviscid linear instability, and the corresponding self-consistent asymptotic structure aligns with the vortex-wave interaction theory. The second type emerges from a subcritical bifurcation by curvature-induced instabilities and satisfies the boundary region equations. Despite the subcritical nature of the second type of solutions, it is not possible to connect their solution branches to the zero-curvature limit of the pipe. However, by continuing from known self-sustained exact coherent structures in the straight pipe flow problem, another family of three-dimensional travelling waves can be shown to exist across all Dean numbers. The self-sustained solutions also possess the two high-Reynolds-number limits. While the vortex-wave interaction type of solutions can be computed at large Dean numbers, their branch remains unconnected to the Dean vortex solution branch.
description: 24 pages, 14 figures
WALLABY Pilot Survey: HI source-finding with a machine learning framework
Creators: name: Wang, Li
name: Wong, O. Ivy
name: Westmeier, Tobias
name: Murugeshan, Chandrashekar
name: Lee-Waddell, Karen
name: Cai, Yuanzhi.
name: Liu, Xiu.
name: Shen, Austin Xiaofan
name: Rhee, Jonghwan
name: Dénes, Helga
name: Deg, Nathan
name: Kamphuis, Peter
name: Catinella, Barbara
Publisher: name: arXiv
Year: 2024
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: The data volumes generated by the WALLABY atomic Hydrogen (HI) survey using the Australiian Square Kilometre Array Pathfinder (ASKAP) necessitate greater automation and reliable automation in the task of source-finding and cataloguing. To this end, we introduce and explore a novel deep learning framework for detecting low Signal-to-Noise Ratio (SNR) HI sources in an automated fashion. Specfically, our proposed method provides an automated process for separating true HI detections from false positives when used in combination with the Source Finding Application (SoFiA) output candidate catalogues. Leveraging the spatial and depth capabilities of 3D Convolutional Neural Networks (CNNs), our method is specifically designed to recognise patterns and features in three-dimensional space, making it uniquely suited for rejecting false positive sources in low SNR scenarios generated by conventional linear methods. As a result, our approach is significantly more accurate in source detection and results in considerably fewer false detections compared to previous linear statistics-based source finding algorithms. Performance tests using mock galaxies injected into real ASKAP data cubes reveal our method's capability to achieve near-100% completeness and reliability at a relatively low integrated SNR~3-5. An at-scale version of this tool will greatly maximise the science output from the upcoming widefield HI surveys.
description: 14 pages, 12 figures, accepted for publication in the Publications of the Astronomical Society of Australia
Mueller_OpenPracticesDisclosure_rev – Supplemental material for Aversive Imagery Causes De Novo Fear Conditioning
Creators: name: Mueller, Erik M.
name: Sperl, Matthias F. J.
name: Panitz, Christian
Publisher: name: SAGE Journals
Year: 2019
Subjects: subject: 110904 Neurology and Neuromuscular Diseases
subject: FOS: Clinical medicine
subject: 170199 Psychology not elsewhere classified
subject: FOS: Psychology
subject: 110319 Psychiatry (incl. Psychotherapy)
subject: Neuroscience

description: Supplemental material, Mueller_OpenPracticesDisclosure_rev for Aversive Imagery Causes De Novo Fear Conditioning by Erik M. Mueller, Matthias F. J. Sperl and Christian Panitz in Psychological Science
AppendixA.rjf_online_supp – Supplemental material for Simulation Analysis and Comparison of Point of Care Testing and Central Laboratory Testing
Creators: name: Harder, Reed
name: Keji Wei
name: Vikrant Vaze
name: Stahl, James E.
Publisher: name: SAGE Journals
Year: 2019
Subjects: subject: 111799 Public Health and Health Services not elsewhere classified
subject: FOS: Health sciences

description: Supplemental material, AppendixA.rjf_online_supp for Simulation Analysis and Comparison of Point of Care Testing and Central Laboratory Testing by Reed Harder, Keji Wei, Vikrant Vaze and James E. Stahl in MDM Policy & Practice
Supplemental Material, EA_Suppl_material_table_1 - Linking Family Financial Socialization With Its Proximal and Distal Outcomes: Which Socialization Dimensions Matter Most for Emerging Adults’ Financial Identity, Financial Behaviors, and Financial Anxiety?
Creators: name: Vosylis, Rimantas
name: Erentaitė, Rasa
Publisher: name: SAGE Journals
Year: 2019
Subjects: subject: 170199 Psychology not elsewhere classified
subject: FOS: Psychology

description: Supplemental Material, EA_Suppl_material_table_1 for Linking Family Financial Socialization With Its Proximal and Distal Outcomes: Which Socialization Dimensions Matter Most for Emerging Adults’ Financial Identity, Financial Behaviors, and Financial Anxiety? by Rimantas Vosylis and Rasa Erentaitė in Emerging Adulthood
Additional file 1 of Impact of the COVID-19 pandemic on children and adolescents: determinants and association with quality of life and mental health—a cross-sectional study
Creators: name: Richard, Viviane
name: Dumont, Roxane
name: Lorthe, Elsa
name: Loizeau, Andrea
name: Baysson, Hélène
name: Zaballa, María-Eugenia
name: Pennacchio, Francesco
name: Barbe, Rémy P.
name: Posfay-Barbe, Klara M.
name: Guessous, Idris
name: Stringhini, Silvia
Publisher: name: figshare
Year: 2024
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: Science Policy
subject: Mental Health

description: Additional file 1: Figure S1. Flow chart of the study participants. Figure S2. Directed acyclic graph of the potential determinants of the COVID-19 pandemic impact. Age and sex were deemed covariates for all other variables (see Methods); arrows are not drawn for readability purpose. Figure S3. Individual item responses to the Coronavirus Impact scale. Parents reported on behalf of their children how each domain had been impacted by the COVID-19 pandemic, n=2101. Table S1. Physical and mental health condition distribution in the sample as reported by parents (n=2101). Table S2. Outcomes comparison according to recruitment period (n=2101). Table S3. Determinants of a severe COVID-19 pandemic impact score among children and adolescents. Sensitivity analyses with data imputation and severe impact definition. Table S4. Association between having been severely impacted by the pandemic and health-related quality of life (HRQoL) or mental health of children and adolescents. Sensitivity analyses with data imputation and severe impact definition. Table S5. Association between having been severely impacted by the pandemic and health-related quality of life (HRQoL) or mental health of children and adolescents, stratified by sex. Table S6. Association between the COVID-19 pandemic impact score and the health-related quality of life of children of adolescents according to different adjustment strategies (n=2043). Table S7. Association between the COVID-19 pandemic impact score and the mental health of children of adolescents according to different adjustment strategies (n=2043).
Quantum heat engine based on quantum interferometry: the SU(1,1) Otto cycle
Creators: name: Ferreri, Alessandro
name: Wang, Hui
name: Nori, Franco
name: Wilhelm, Frank K.
name: Bruschi, David Edward
Publisher: name: arXiv
Year: 2024
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We present a quantum heat engine based on a quantum Otto cycle, whose working substance reproduces the same outcomes of a SU(1,1) interference process at the end of each adiabatic transformation. This device takes advantage of the extraordinary quantum metrological features of the SU(1,1) interferometer to better discriminate the sources of uncertainty of relevant observables during each adiabatic stroke of the cycle. Applications to circuit QED platforms are also discussed.
Online_supplementary_figure – Supplemental material for Using Online Survey Software to Enhance Rigor and Efficiency of Knowledge Synthesis Reviews
Creators: name: Lopez, Karen Dunn
name: Gephart, Sheila M.
name: Hershberger, Patricia E.
Publisher: name: SAGE Journals
Year: 2020
Subjects: subject: 111099 Nursing not elsewhere classified
subject: FOS: Health sciences

description: Supplemental material, Online_supplementary_figure for Using Online Survey Software to Enhance Rigor and Efficiency of Knowledge Synthesis Reviews by Karen Dunn Lopez, Sheila M. Gephart and Patricia E. Hershberger in Western Journal of Nursing Research
Geometric contribution to adiabatic amplification in non-Hermitian systems
Creators: name: Ozawa, Tomoki
name: Schomerus, Henning
Publisher: name: arXiv
Year: 2024
Subjects: subject: Quantum Physics (quant-ph)
subject: Other Condensed Matter (cond-mat.other)
subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: Concepts from non-Hermitian quantum mechanics have proven useful in understanding and manipulating a variety of classical systems, such as those encountered in optics, classical mechanics, and metamaterial design. Recently, the non-Hermitian analog of the Berry phase for adiabatic processes was experimentally measured. In non-Hermitian systems, the Berry phase can have an imaginary part, which contributes to the amplification or decay of the total wave intensity. When the imaginary part of the Berry curvature is zero, this geometric amplification factor is determined solely by the initial and final points of the adiabatic path in parameter space, and it does not depend on how these points are connected by the path. We list classes of non-Hermitian Hamiltonians where this path independence is guaranteed by suitable symmetries, and we find that, for some of these classes, the amplification factor can be written only in terms of the Petermann factors of the initial and final points. Our result can, in turn, be used to experimentally obtain the Petermann factor by observing how the norm of the wave function changes under adiabatic processes. We validate our theory using a couple of concrete examples of physical relevance.
description: 15 pages, 4 figures