cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Common Envelope Evolution of Massive Stars
Creators: name: Ricker, Paul M.
name: Timmes, Frank X.
name: Taam, Ronald E.
name: Webbink, Ronald F.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: The discovery via gravitational waves of binary black hole systems with total masses greater than $60M_\odot$ has raised interesting questions for stellar evolution theory. Among the most promising formation channels for these systems is one involving a common envelope binary containing a low metallicity, core helium burning star with mass $\sim 80-90M_\odot$ and a black hole with mass $\sim 30-40M_\odot$. For this channel to be viable, the common envelope binary must eject more than half the giant star's mass and reduce its orbital separation by as much as a factor of 80. We discuss issues faced in numerically simulating the common envelope evolution of such systems and present a 3D AMR simulation of the dynamical inspiral of a low-metallicity red supergiant with a massive black hole companion.
description: 6 pages, 3 figures, oral contribution: IAU Symposium 346 "High Mass X-ray Binaries: illuminating the passage from massive binaries to merging compact objects", Vienna, Austria, 27-31 August 2018
Ameroseiidae Evans 1961
Creators: name: Khalili-Moghadam, Arsalan
name: Saboori, Alireza
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Arachnida
Mesostigmata
Ameroseiidae

description: Family Ameroseiidae Evans, 1961  Ameroseiidae Evans (in Hughes, 1961: 244).
 Type genus: Ameroseius Berlese, 1904, by inference.
For diagnosis of the family, see Mašán (2017).
description: Published as part of Khalili-Moghadam, Arsalan & Saboori, Alireza, 2021, World distribution and habitat scope of Ameroseiidae (Acari: Mesostigmata), pp. 403-450 in Persian Journal of Acarology 10 (4) on page 404, DOI: 10.22073/pja.v10i4.67440, http://zenodo.org/record/7173383
FITTING AND ADJUSTMENT OF PLATE PROSTHESES IN COMPLETE EDENTULISM: GUIDELINES FOR USE AND CORRECTION OF REMOVABLE DENTURES
Creators: name: Kosimova Dilafruz Samarkand State Medical University
name: Saidmaxmudov Shaxboz Samarkand State Medical University
Publisher: name: Zenodo
Year: 2025

description: The fitting and adjustment of plate prostheses are crucial for the successful rehabilitation of patients with complete edentulism. Ensuring a proper fit enhances comfort, functionality, and aesthetics. This article outlines the steps involved in the fitting process, the essential rules for patient use, and methods for correcting removable dentures to achieve optimal performance.
Additional file 3 of Expression profile analysis of the inflammatory response regulated by hepatocyte nuclear factor 4α
Creators: name: Zhongyan Wang
name: Bishop, Eric P
name: Burke, Peter A
Publisher: name: figshare
Year: 2020
Subjects: subject: Genetics
subject: FOS: Biological sciences

description: Additional file 3:siRNA rescue assay. This file shows the characterization of the HNF4α siRNA-resistant construct by Western blot, and the rescue effect of this construct on HNF4α knock-down responsive genes. (PDF 147 KB)
A water budget dichotomy of rocky protoplanets from $^{26}$Al-heating
Creators: name: Lichtenberg, Tim
name: Golabek, Gregor J.
name: Burn, Remo
name: Meyer, Michael R.
name: Alibert, Yann
name: Gerya, Taras V.
name: Mordasini, Christoph
Publisher: name: arXiv
Year: 2019
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Geophysics (physics.geo-ph)
subject: FOS: Physical sciences

description: In contrast to the water-poor inner solar system planets, stochasticity during planetary formation and order of magnitude deviations in exoplanet volatile contents suggest that rocky worlds engulfed in thick volatile ice layers are the dominant family of terrestrial analogues among the extrasolar planet population. However, the distribution of compositionally Earth-like planets remains insufficiently constrained, and it is not clear whether the solar system is a statistical outlier or can be explained by more general planetary formation processes. Here we employ numerical models of planet formation, evolution, and interior structure, to show that a planet's bulk water fraction and radius are anti-correlated with initial $^{26}$Al levels in the planetesimal-based accretion framework. The heat generated by this short-lived radionuclide rapidly dehydrates planetesimals prior to accretion onto larger protoplanets and yields a system-wide correlation of planet bulk abundances, which, for instance, can explain the lack of a clear orbital trend in the water budgets of the TRAPPIST-1 planets. Qualitatively, our models suggest two main scenarios of planetary systems' formation: high-$^{26}$Al systems, like our solar system, form small, water-depleted planets, whereas those devoid of $^{26}$Al predominantly form ocean worlds, where the mean planet radii between both scenarios deviate by up to about 10%.
description: Preprint version; free-to-read journal version at https://rdcu.be/bmdlw; blog article at https://t.co/p6SValG1ip
An exact learning algorithm for autoassociative neural networks with binary couplings
Creators: name: Milde, G.
name: Kobe, S.
Publisher: name: arXiv
Year: 1997
Subjects: subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: Quantitative Biology (q-bio)
subject: FOS: Physical sciences
subject: FOS: Biological sciences

description: Exact solutions for the learning problem of autoassociative networks with binary couplings are determined by a new method. The use of a branch-and-bound algorithm leads to a substantial saving of computational time compared with complete enumeration. As a result, fully connected networks with up to 40 neurons could be investigated. The network capacity is found to be close to 0.83.
description: LaTeX (ioplppt style), 5 pages, 2 (LaTeX) pictures
Afrocypholaelaps Elsen 1972
Creators: name: Khalili-Moghadam, Arsalan
name: Saboori, Alireza
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Arachnida
Mesostigmata
Ameroseiidae
Afrocypholaelaps

description: Genus Afrocypholaelaps Elsen, 1972
 Afrocypholaelaps Elsen, 1972b: 159. Type species: Neocypholaelaps africana Evans, 1963, by original designation.
For diagnosis of the genus, see Mašán (2017).
description: Published as part of Khalili-Moghadam, Arsalan & Saboori, Alireza, 2021, World distribution and habitat scope of Ameroseiidae (Acari: Mesostigmata), pp. 403-450 in Persian Journal of Acarology 10 (4) on page 404, DOI: 10.22073/pja.v10i4.67440, http://zenodo.org/record/7173383
A Primal Decomposition Method with Suboptimality Bounds for Distributed Mixed-Integer Linear Programming
Creators: name: Camisa, Andrea
name: Notarnicola, Ivano
name: Notarstefano, Giuseppe
Publisher: name: arXiv
Year: 2018
Subjects: subject: Systems and Control (eess.SY)
subject: Distributed, Parallel, and Cluster Computing (cs.DC)
subject: Multiagent Systems (cs.MA)
subject: Optimization and Control (math.OC)
subject: FOS: Electrical engineering, electronic engineering, information engineering
subject: FOS: Computer and information sciences
subject: FOS: Mathematics

description: In this paper we deal with a network of agents seeking to solve in a distributed way Mixed-Integer Linear Programs (MILPs) with a coupling constraint (modeling a limited shared resource) and local constraints. MILPs are NP-hard problems and several challenges arise in a distributed framework, so that looking for suboptimal solutions is of interest. To achieve this goal, the presence of a linear coupling calls for tailored decomposition approaches. We propose a fully distributed algorithm based on a primal decomposition approach and a suitable tightening of the coupling constraints. Agents repeatedly update local allocation vectors, which converge to an optimal resource allocation of an approximate version of the original problem. Based on such allocation vectors, agents are able to (locally) compute a mixed-integer solution, which is guaranteed to be feasible after a sufficiently large time. Asymptotic and finite-time suboptimality bounds are established for the computed solution. Numerical simulations highlight the efficacy of the proposed methodology.
description: 57th IEEE Conference on Decision and Control
Einstellungen zur Akzeptanz räumlicher Distanz in erwerbsbedingt multilokalen Lebensformen
Creators: name: Rüger, Heiko
name: Schier, Michaela
name: Feldhaus, Michael
name: Ries, Tammy
Publisher: name: JFR - Journal of Family Research
Year: 2014

description: Work-related multi-local living arrangements describe those living arrangements in which, due to occupational reasons, at least one partner is absent from the communal residence of the partners or the family for a substantial part of the year. In the context of high requirements concerning spatial flexibility of employees, such living arrangements have become increasingly important. Against this background, this paper examines the acceptance of spatial distance in intimate relationships. Analyses are based on panel data of the “Job Mobilities and Family Lives in Europe” study (2007 and 2010/11), collected in Germany, France, Spain and Switzerland (N=1.189). We used path modelling to conduct a cross-lagged panel analysis. Results show a higher acceptance of spatial distance in intimate relationships in individuals living multi-locally due to work-related spatial mobility requirements. Longitudinal analyses suggest that this correlation is primarily based on adaptation processes. Experiences of multi-local living arrangements lead to attitude changes towards a higher acceptance of spatial distance. However, further selection processes could not be detected, which might partially be explained by a high degree of selectivity at the first point of data collection. Zusammenfassung Im Kontext hoher Anforderungen an die räumliche Flexibilität von Erwerbstätigen werden erwerbsbedingt multilokale Lebensformen, in denen mindestens ein Partner aus beruflichen Gründen einen Teil des Jahres nicht an dem gemeinsamen Hauptwohnort des Paares oder der Familie verbringt, zunehmend bedeutsam. Vor diesem Hintergrund untersucht der Beitrag die Rolle der Einstellungen zur akzeptierten räumlichen Distanz in Paarbeziehungen. Grundlage sind Paneldaten der Studie „Job Mobilities and Family Lives in Europe“ (2007 und 2010/11), die in Deutschland, Frankreich, Spanien und der Schweiz erhoben wurden (N=1.189). Berechnet werden Pfadmodelle im Cross-Lagged-Panel-Design. Die Ergebnisse zeigen zunächst eine höhere räumliche Distanzakzeptanz in Paarbeziehungen bei Personen, die berufsbedingt multilokal leben. Die Längsschnittanalysen legen nahe, dass dieser Zusammenhang in erster Linie auf Anpassungsprozessen zu beruhen scheint. So führen Multilokalitätserfahrungen zu Veränderungen der Einstellungen in Richtung einer stärkeren Distanzakzeptanz. Weitere Selektionsprozesse konnten im Zeitverlauf hingegen nicht nachgewiesen werden, wofür unter anderem ein bereits zum ersten Erhebungszeitpunkt hoher Grad an Selektivität verantwortlich sein könnte.
description: JFR - Journal of Family Research, Vol 26 No 2 (2014)
Gravomagnetic Lensing by NUT Space
Creators: name: Nouri-Zonoz, Mohammad
name: Lynden-Bell, Donald
Publisher: name: arXiv
Year: 1998
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: Using the fact that the null geodesics in NUT space lie on spatial cones, we consider the gravomagnetic lens effect on light rays passing a NUT deflector. We show that this effect changes the observed shape, size and orientation of a source. Compared to the Schwarzschild lens, there is an extra shear (a differential twist around the lens axis) due to the gravomagnetic field which shears the shape of the source. Gravomagnetic monopoles can thus be recognized by the spirality that they produce in the lensing pattern. All the results obtained in this case (magnification factor, orientation of images, multiplicity of images, etc.) depend on $Q$, the strength of the gravomagnetic monopole represented by NUT metric. One recovers the results of the usual Schwarzschild lens effect by putting this factor equal to zero.
description: 29 pages including 15 figures, MNRAS format
The induced metric on the boundary of the convex hull of a quasicircle in hyperbolic and anti de Sitter geometry
Creators: name: Bonsante, Francesco
name: Danciger, Jeffrey
name: Maloni, Sara
name: Schlenker, Jean-Marc
Publisher: name: arXiv
Year: 2019
Subjects: subject: Geometric Topology (math.GT)
subject: FOS: Mathematics
subject: 57M50, 53B30, 53C50, 53C45, 30F40, 37F30, 30C62

description: Celebrated work of Alexandrov and Pogorelov determines exactly which metrics on the sphere are induced on the boundary of a compact convex subset of hyperbolic three-space. As a step toward a generalization for unbounded convex subsets, we consider convex regions of hyperbolic three-space bounded by two properly embedded disks which meet at infinity along a Jordan curve in the ideal boundary. In this setting, it is natural to augment the notion of induced metric on the boundary of the convex set to include a gluing map at infinity which records how the asymptotic geometry of the two surfaces compares near points of the limiting Jordan curve. Restricting further to the case in which the induced metrics on the two bounding surfaces have constant curvature $K \in [-1,0)$ and the Jordan curve at infinity is a quasicircle, the gluing map is naturally a quasisymmetric homeomorphism of the circle. The main result is that for each value of $K$, every quasisymmetric map is achieved as the gluing map at infinity along some quasicircle. We also prove analogous results in the setting of three-dimensional anti de Sitter geometry. Our results may be viewed as universal versions of the conjectures of Thurston and Mess about prescribing the induced metric on the boundary of the convex core of quasifuchsian hyperbolic manifolds and globally hyperbolic anti de Sitter spacetimes.
description: 55 pages, 9 figures
Localizing the $E_2$ page of the Adams spectral sequence
Creators: name: Belmont, Eva
Publisher: name: arXiv
Year: 2019
Subjects: subject: Algebraic Topology (math.AT)
subject: FOS: Mathematics
subject: 55T15

description: There is only one nontrivial localization of $π_*S_{(p)}$ (the chromatic localization at $v_0=p$), but there are infinitely many nontrivial localizations of the Adams $E_2$ page for the sphere. The first non-nilpotent element in the $E_2$ page after $v_0$ is $b_{10}\in \mathrm{Ext}_A^{2p(p-1)-2}(\mathbb{F}_p,\mathbb{F}_p)$. We work at $p=3$ and study $b_{10}^{-1}\mathrm{Ext}_P(\mathbb{F}_3,\mathbb{F}_3)$ (where $P$ is the algebra of dual reduced powers), which agrees with the infinite summand $\mathrm{Ext}_P(\mathbb{F}_3,\mathbb{F}_3)$ of $\mathrm{Ext}_A(\mathbb{F}_3,\mathbb{F}_3)$ above a line of slope ${1\over 23}$. We compute up to the $E_9$ page of an Adams spectral sequence in the category $\mathrm{Stable}(P)$ converging to $b_{10}^{-1}\mathrm{Ext}_P(\mathbb{F}_3,\mathbb{F}_3)$, and conjecture that the spectral sequence collapses at $E_9$. We also give a complete calculation of $b_{10}^{-1}\mathrm{Ext}_P^*(\mathbb{F}_3,\mathbb{F}_3[ξ_1^3])$.
An Upper Limit on the Coalescence Rate of Double Neutron-Star Binaries in the Galaxy
Creators: name: Kalogera, Vassiliki
name: Lorimer, Duncan
Publisher: name: arXiv
Year: 1999
Subjects: subject: Astrophysics (astro-ph)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: In the context of assessing the detectability of the coalescence of two neutron stars (NS) by currently built gravitational-wave experiments, we present a way of obtaining an upper limit to the coalescence rate in the Galaxy. We consider the NS/NS progenitors just before the second supernova explosion. By combining our theoretical understanding of orbital dynamics at NS formation with methods of empirically estimating pulsar birth rates we derive an upper limit of a few mergers every 100,000 yr. Such a Galactic rate implies a possible detection by the ``enhanced'' LIGO of up to a few to ten mergers per year.
description: Revised version with small changes in the text (16 pages, 3 figures, 1 table); accepted for publication in The Astrophysical Journal
Interplay between spin-density-wave and superconducting states in quasi-one-dimensional conductors
Creators: name: Duprat, Raphael
name: Bourbonnais, C.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: The interference between spin-density-wave and superconducting instabilities in quasi-one-dimensional correlated metals is analyzed using the renormalization group method. At the one-loop level, we show how the interference leads to a continuous crossover from a spin-density-wave state to unconventional superconductivity when deviations from perfect nesting of the Fermi surface exceed a critical value. Singlet pairing between electrons on neighboring stacks is found to be the most favorable symmetry for superconductivity. The consequences of non uniform spin-density-wave pairing on the structure of phase diagram within the crossover region is also discussed.
description: 10 pages RevTex,4 Figures, submitted to EPJB
Ameroseiella Bregetova 1977
Creators: name: Khalili-Moghadam, Arsalan
name: Saboori, Alireza
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Arachnida
Mesostigmata
Ameroseiidae
Ameroseiella

description: Genus Ameroseiella Bregetova, 1977
 Ameroseiella Bregetova, 1977: 167. Type species: Ameroseius apodius Karg, 1971a (syn.: A. macrochelae Westerboer, 1963), by original designation.
For diagnosis of the genus see Mašán (2017).
description: Published as part of Khalili-Moghadam, Arsalan & Saboori, Alireza, 2021, World distribution and habitat scope of Ameroseiidae (Acari: Mesostigmata), pp. 403-450 in Persian Journal of Acarology 10 (4) on page 405, DOI: 10.22073/pja.v10i4.67440, http://zenodo.org/record/7173383
Die Veränderung der Hausarbeitsteilung in Paarbeziehungen. Ein Überblick über die Längsschnittforschung und neue empirische Befunde auf Basis der pairfam-Daten
Creators: name: Dechant, Anna
name: Rost, Harald
name: Schulz, Florian
Publisher: name: JFR - Journal of Family Research
Year: 2014

description: This paper examines the changes in the division of housework over the course of relationships, first providing a detailed and comprehensive overview of the current status of longitudinal research on the subject matter. The findings available to date, revealing a largely gendered division of labor among German couples, were then confirmed using pairfam data and fixed-effects panel regression models: routine household tasks, such as cooking, cleaning, and doing laundry, remain predominantly “women’s work”. This division of housework is reinforced considerably with the transition to parenthood. Furthermore, effects of the couples’ levels of education and the women’s labor market participation could be illustrated in accordance with well-established theories. In conclusion, we suggest that this current state of knowledge can highly benefit from qualitative longitudinal studies, allowing for a detailed representation of new contextual dimensions such as attitudes towards gender roles, socialization experiences or negotiation processes among couples. Zusammenfassung Der Beitrag untersucht die Veränderung der Hausarbeitsteilung im Partnerschaftsverlauf und gibt hierfür zunächst einen ausführlichen und umfassenden Überblick über den aktuellen Stand der Längsschnittforschung. Eigene Panelregressionsmodelle mit fixen Effekten auf Basis der pairfam-Daten bestätigen die bisher bekannten Befunde, dass in Deutschland eine weitgehend geschlechtsspezifische Arbeitsteilung in Paaren vorliegt: Haushaltsroutinen wie Kochen, Putzen und Wäsche machen liegen überwiegend im Zuständigkeitsbereich der Frauen. Der Übergang zur Elternschaft verstärkt diese Hausarbeitsteilung deutlich. Darüber hinaus konnten Effekte des Bildungsniveaus im Paar und der Erwerbstätigkeit der Frau gezeigt werden, die im Einklang mit den gängigen Theorien stehen. Wir schließen mit der These, dass dieser Erkenntnisstand vor allem durch qualitative Längsschnittstudien erweitert werden kann, weil dadurch neue inhaltliche Dimensionen wie beispielsweise Einstellungen zu den Geschlechterrollen, Sozialisationserfahrungen oder Aushandlungsprozesse in Paaren detailliert abgebildet werden können.
description: JFR - Journal of Family Research, Vol 26 No 2 (2014)
Feynman's proof of the commutativity of the Calogero integrals of motion
Creators: name: Polychronakos, Alexios P.
Publisher: name: arXiv
Year: 2018
Subjects: subject: History and Philosophy of Physics (physics.hist-ph)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: High Energy Physics - Theory (hep-th)
subject: Mathematical Physics (math-ph)
subject: Exactly Solvable and Integrable Systems (nlin.SI)
subject: FOS: Physical sciences

description: During his last year of life Feynman became interested in integrable models. In the course of his study of one dimensional particles with inverse square-type potentials (the Calogero class of models) he came up with a field theory-inspired proof of the commutativity of the integrals of motion of the system, which remained unpublished. I present an exact transcript of the proof together with a scan of the first page of Feynman's original manuscript and some historical background.
description: 10 pages plus one scanned page
Metal-superconductor transition at zero temperature: A case of unusual scaling
Creators: name: Kirkpatrick, T. R.
name: Belitz, D.
Publisher: name: arXiv
Year: 1997
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: An effective field theory is derived for the normal metal-to-superconductor quantum phase transition at T=0. The critical behavior is determined exactly for all dimensions d>2. Although the critical exponents βand νdo not exist, the usual scaling relations, properly reinterpreted, still hold. A complete scaling description of the transition is given, and the physics underlying the unusual critical behavior is discussed. Quenched disorder leads to anomalously strong T_c-fluctuations which are shown to explain the experimentally observed broadening of the transition in low-T_c thin films.
description: 4 pp., no figs, final version as published
Leucophlebia afra Karsch 1891
Creators: name: Mbata, Keith J.
name: Prins, Jurate De
Publisher: name: Zenodo
Year: 2023
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Lepidoptera
Sphingidae
Leucophlebia
Leucophlebia afra

description: Leucophlebia afra Karsch, 1891
COMMON NAME(S): Rosy banded hawkmoth.
SYNONYM(S): None.
IUCN STATUS: Not Evaluated (NE).
DISTRIBUTION: Angola, Burkina Faso, Cameroon, Central African Republic, Côte d’Ivoire, Democratic Republic of Congo, Gabon, Malawi, Nigeria, Republic of Congo, Senegal, South Sudan, Sudan, Tanzania, Uganda, Zambia, Zimbabwe.
LOCALITY IN ZAMBIA: ‘Lusaka’, in Lusaka Province.
LARVAL HOSTPLANT(S): Larval foodplants are grasses (Poaceae) including Hyparrhenia subplumosa (African Moths 2019).
SOURCES: African Moths 2019; D’Abrera 1987; De Prins & De Prins 2022.
description: Published as part of Mbata, Keith J. & Prins, Jurate De, 2023, Annotated checklist of moths of Zambia (Insecta: Lepidoptera), pp. 1-503 in Zootaxa 5354 (1) on page 193, DOI: 10.11646/zootaxa.5354.1.1, http://zenodo.org/record/10130434
title: Xanthium albinum (Widder) H. Scholz subsp. albinum
Creators: name: :None
Publisher: name: Universitätsbibliothek Braunschweig
Year: 2023
Subjects: subject: Digitale Pflanzenbilder: Sammlung Dietmar Brandes
subject: 58

description: Pflanzensammlung Dietmar Brandes: Digitale Pflanzenbilder
Ameroseiella macrochelae
Creators: name: Khalili-Moghadam, Arsalan
name: Saboori, Alireza
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Arachnida
Mesostigmata
Ameroseiidae
Ameroseiella
Ameroseiella macrochelae

description: Ameroseiella macrochelae (Westerboer, 1963)
 Ameroseius macrochelae Westerboer (in Westerboer & Bernhard 1963: 501).
 Ameroseius apodius Karg, 1971a: 226. Synonymy by Mašán (2017: 20).
 Ameroseiella macrochelae. — Mašán 2017: 20.
More information about the synonyms of this species are available in Mašán (2017: 20).
 Distribution and habitats – Finland, from mink, farm waste and compost (Huhta 2016); France, from compost (Westerboer and Bernhard 1963; Karg 1971a; 1993); Germany, from compost soil (Karg 1971a; 1993); Ireland, unspecified substrate (Evans and Till 1979); Poland, from nests of the white-tailed sea eagle Haliaeetus albicilla L. (Accipitriformes: Accipitridae) (Gwiazdowicz et al. 2006), nests of birds (Bloszyk et al. 2009; 2011); Russia, Moscow, Novosibirsk Oblast and Rostov Oblast, from soil and litter (Bregetova 1977); Slovakia, from nest of Passer domesticus L. (Passeriformes: Passeridae), Haliaeetus albicilla L. (Accipitriformes: Accipitridae) and Passer montanus (Passeriformes: Passeridae) (Mašán 2017); United Kingdom, unspecified substrate (Evans and Till 1979); Europe (country not mentioned), from nest of birds (Aves, Columbiformes: Columbidae) and nests of hoopoe (Upupa epops L.) (Bucerotiformes: Upupidae) (Sixl 1975; Krištofík et al. 2013).
description: Published as part of Khalili-Moghadam, Arsalan & Saboori, Alireza, 2021, World distribution and habitat scope of Ameroseiidae (Acari: Mesostigmata), pp. 403-450 in Persian Journal of Acarology 10 (4) on page 405, DOI: 10.22073/pja.v10i4.67440, http://zenodo.org/record/7173383
Approximate Analytical Solutions to the Initial Data Problem of Black Hole Binary Systems
Creators: name: Marronetti, P.
name: Huq, M.
name: Laguna, P.
name: Lehner, L.
name: Matzner, R.
name: Shoemaker, D.
name: .
Publisher: name: arXiv
Year: 2000
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We present approximate analytical solutions to the Hamiltonian and momentum constraint equations, corresponding to systems composed of two black holes with arbitrary linear and angular momentum. The analytical nature of these initial data solutions makes them easier to implement in numerical evolutions than the traditional numerical approach of solving the elliptic equations derived from the Einstein constraints. Although in general the problem of setting up initial conditions for black hole binary simulations is complicated by the presence of singularities, we show that the methods presented in this work provide initial data with $l_1$ and $l_\infty$ norms of violation of the constraint equations falling below those of the truncation error (residual error due to discretization) present in finite difference codes for the range of grid resolutions currently used. Thus, these data sets are suitable for use in evolution codes. Detailed results are presented for the case of a head-on collision of two equal-mass M black holes with specific angular momentum 0.5M at an initial separation of 10M. A straightforward superposition method yields data adequate for resolutions of $h=M/4$, and an "attenuated" superposition yields data usable to resolutions at least as fine as $h=M/8$. In addition, the attenuated approximate data may be more tractable in a full (computational) exact solution to the initial value problem.
description: 6 pages, 5 postscript figures. Minor changes and some points clarified. Accepted for publication in Phys. Rev. D
A New Transport Regime in the Quantum Hall Effect
Creators: name: Shahar, D.
name: Hilke, M.
name: Li, C. C.
name: Tsui, D. C.
name: Sondhi, S. L.
name: Razeghi, M.
Publisher: name: arXiv
Year: 1997
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: This paper describes an experimental identification and characterization of a new low temperature transport regime near the quantum Hall-to-insulator transition. In this regime, a wide range of transport data are compactly described by a simple phenomenological form which, on the one hand, is inconsistent with either quantum Hall or insulating behavior and, on the other hand, is also clearly at odds with a quantum-critical, or scaling, description. We are unable to determine whether this new regime represents a clearly defined state or is a consequence of finite temperature and sample-size measurements.
description: Revtex, 3 pages, 2 figures
Ameroseius Berlese 1904
Creators: name: Khalili-Moghadam, Arsalan
name: Saboori, Alireza
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Arachnida
Mesostigmata
Ameroseiidae
Ameroseius

description: Genus Ameroseius Berlese, 1904
 Ameroseius Berlese, 1904: 258. Type species: Seius echinatus C. L. Koch, 1839 (syn.: Acarus corbicula Sowerby, 1806), by original designation. Synonymy by Vitzthum (1942).
 Cornubia Turk, 1943: 858. Type species: Cornubia ornata Turk, 1943 (syn.: Acarus corbicula Sowerby, 1806), by original designation. Synonymy by Turk (1953).
 Ameroseius. — Evans 1963: 230.
For diagnosis of the genus see Mašán (2017).
description: Published as part of Khalili-Moghadam, Arsalan & Saboori, Alireza, 2021, World distribution and habitat scope of Ameroseiidae (Acari: Mesostigmata), pp. 403-450 in Persian Journal of Acarology 10 (4) on page 406, DOI: 10.22073/pja.v10i4.67440, http://zenodo.org/record/7173383
Dark Matter Search Results from the Complete Exposure of the PICO-60 C$_3$F$_8$ Bubble Chamber
Creators: name: Amole, C.
name: Ardid, M.
name: Arnquist, I. J.
name: Asner, D. M.
name: Baxter, D.
name: Behnke, E.
name: Bressler, M.
name: Broerman, B.
name: Cao, G.
name: Chen, C. J.
name: Chowdhury, U.
name: Clark, K.
name: Collar, J. I.
name: Cooper, P. S.
name: Coutu, C. B.
name: Cowles, C.
name: Crisler, M.
name: Crowder, G.
name: Cruz-Venegas, N. A.
name: Dahl, C. E.
name: Das, M.
name: Fallows, S.
name: Farine, J.
name: Felis, I.
name: Filgas, R.
name: Girard, F.
name: Giroux, G.
name: Hall, J.
name: Hardy, C.
name: Harris, O.
name: Hillier, T.
name: Hoppe, E. W.
name: Jackson, C. M.
name: Jin, M.
name: Klopfenstein, L.
name: Krauss, C. B.
name: Laurin, M.
name: Lawson, I.
name: Leblanc, A.
name: Levine, I.
name: Licciardi, C.
name: Lippincott, W. H.
name: Loer, B.
name: Mamedov, F.
name: Mitra, P.
name: Moore, C.
name: Nania, T.
name: Neilson, R.
name: Noble, A. J.
name: Oedekerk, P.
name: Ortega, A.
name: Piro, M. -C.
name: Plante, A.
name: Podviyanuk, R.
name: Priya, S.
name: Robinson, A. E.
name: Sahoo, S.
name: Scallon, O.
name: Seth, S.
name: Sonnenschein, A.
name: Starinski, N.
name: Štekl, I.
name: Sullivan, T.
name: Tardif, F.
name: Vázquez-Jáuregui, E.
name: Walkowski, N.
name: Weima, E.
name: Wichoski, U.
name: Wierman, K.
name: Yan, Y.
name: Zacek, V.
name: Zhang, J.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Physics - Experiment (hep-ex)
subject: Instrumentation and Detectors (physics.ins-det)
subject: FOS: Physical sciences

description: Final results are reported from operation of the PICO-60 C$_3$F$_8$ dark matter detector, a bubble chamber filled with 52 kg of C$_3$F$_8$ located in the SNOLAB underground laboratory. The chamber was operated at thermodynamic thresholds as low as 1.2 keV without loss of stability. A new blind 1404-kg-day exposure at 2.45 keV threshold was acquired with approximately the same expected total background rate as the previous 1167-kg-day exposure at 3.3 keV. This increased exposure is enabled in part by a new optical tracking analysis to better identify events near detector walls, permitting a larger fiducial volume. These results set the most stringent direct-detection constraint to date on the WIMP-proton spin-dependent cross section at 2.5 $\times$ 10$^{-41}$ cm$^2$ for a 25 GeV WIMP, and improve on previous PICO results for 3-5 GeV WIMPs by an order of magnitude.
description: 9 pages, 8 figures
Bond-order-wave phase and quantum phase transitions in the one-dimensional extended Hubbard model
Creators: name: Sengupta, Pinaki
name: Sandvik, Anders W.
name: Campbell, David K.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We use a stochastic series expansion quantum Monte Carlo method to study the phase diagram of the one-dimensional extended Hubbard model at half filling for small to intermediate values of the on-site (U) and nearest-neighbor (V) repulsions. We confirm the existence of a novel, long-range-ordered bond-order-wave (BOW) phase recently predicted by Nakamura (J. Phys. Soc. Jpn. 68, 3123 (1999)) in a small region of the parameter space between the familiar charge-density-wave (CDW) state for V > U/2 and the state with dominant spin-density-wave (SDW) fluctuations for V < U/2. We discuss the nature of the transitions among these states and evaluate some of the critical exponents. Further, we determine accurately the position of the multi-critical point, (U_m,V_m)= (4.7 +/- 0.1, 2.51 +/- 0.04) (in energy units where the hopping integral is normalized to unity), above which the two continuous SDW-BOW-CDW transitions are replaced by one discontinuous (first-order) direct SDW-CDW transition. We also discuss the evolution of the CDW and BOW states upon hole doping. We find that in both cases the ground state is a Luther-Emery liquid, i.e., the spin gap remains but the charge gap existing at half-filling is immediately closed upon doping. The charge and bond-order correlations decay with distance r as r^{-K_rho}, where K_rho is approximately 0.5 for the parameters we have considered. We also discuss advantages of using parallel tempering (or exchange Monte Carlo) -- an extended ensemble method that we here combine with quantum Monte Carlo -- in studies of quantum phase transitions.
description: New results for doped systems added. Accepted for publication in Phys. Rev. B
title: Xanthoceras sorbifolium Bunge
Creators: name: :None
Publisher: name: Universitätsbibliothek Braunschweig
Year: 2023
Subjects: subject: Digitale Pflanzenbilder: Sammlung Dietmar Brandes
subject: 58

description: Pflanzensammlung Dietmar Brandes: Digitale Pflanzenbilder
Remagnetization in the array of ferromagnetic nanowires with periodic and quasiperiodic order
Creators: name: Szulc, K.
name: Lisiecki, F.
name: Makarov, A.
name: Zelent, M.
name: Kuświk, P.
name: Głowiński, H.
name: Klos, J. W.
name: Munzenberg, M.
name: Gieniusz, R.
name: Dubowik, J.
name: Stobiecki, F.
name: Krawczyk, M.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We investigate experimentally and theoretically the magnetization reversal process in one-dimensional magnonic structures composed of permalloy nanowires of the two different widths and finite length arranged in a periodic and quasiperiodic order. The main features of the hysteresis loop are determined by different shape anisotropies of the component elements and the dipolar interactions between them. We showed, that the dipolar interactions between nanowires forming a ribbon can be controlled by change a distance between the neighboring ribbons. The quasiperiodic order can influence the hysteresis loop by introduction additional tiny switching steps when the dipolar interactions are sufficiently strong.
description: 10 pages, 7 figures
Stability of self-gravitating magnetic monopoles
Creators: name: Arreaga, Guillermo
name: Cho, Inyong
name: Guven, Jemal
Publisher: name: arXiv
Year: 2000
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: The stability of a spherically symmetric self-gravitating magnetic monopole is examined in the thin wall approximation: modeling the interior false vacuum as a region of de Sitter space; the exterior as an asymptotically flat region of the Reissner-Nordström geometry; and the boundary separating the two as a charged domain wall. There remains only to determine how the wall gets embedded in these two geometries. In this approximation, the ratio $k$ of the false vacuum to surface energy densities is a measure of the symmetry breaking scale $η$. Solutions are characterized by this ratio, the charge on the wall $Q$, and the value of the conserved total energy $M$. We find that for each fixed $k$ and $Q$ up to some critical value, there exists a unique globally static solution, with $M\simeq Q^{3/2}$; any stable radial excitation has $M$ bounded above by $Q$, the value assumed in an extremal Reissner-Nordström geometry and these are the only solutions with $M
description: 19 pages, RevTex two cols., 11 eps figs. Submitted to Phys. Rev. D
Ameroseius aegypticus El-Badry, Nasr & Hafez 1979
Creators: name: Khalili-Moghadam, Arsalan
name: Saboori, Alireza
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Arachnida
Mesostigmata
Ameroseiidae
Ameroseius
Ameroseius aegypticus

description: Ameroseius aegypticus El-Badry, Nasr & Hafez, 1979
 Ameroseius aegypticus El-Badry, Nasr & Hafez, 1979: 2.
 Ameroseius aegypticus. — Zaher 1986: 401; Narita et al. 2015: 395; Mašán 2017: 26.
 Distribution and habitats – Egypt, from decayed debris under wild-sage (Lantana camara L.) (Lamiales: Verbenaceae), water weeds and barley grain (El-Badry et al. 1979; Nasr et al. 2011; ElSayed Gad et al. 2020).
 Published material from Iran – Chaharmahal va Bakhtiari Province, Shahrekord, Saman, Farokhshahr, Boldaji and Choghakhor, from soil and decaying wood; Esfahan Province, Esfahan, from soil; Guilan Province, from stored rice, rice dust and debris (Roodbar), soil in olive orchards, (Sangar), rice hulls,; Sangar, Eslamabad (Shaqaji) Village, from woodchips, from soil, stored products, debris, plant foliage, leaves, wood, and manure; Kerman Province, Kerman, from cow manure and sheep manure; Khorasan Razavi Province, Kashmar, from soil of vineyards; Khuzestan Province, Izeh, from soil; Mazandaran Province, in honey bee hives; Khuzestan and Golestan Provinces, from soil, debris, soil of ants nests and fungi (Kazemi and Rajaei 2013; Nemati et al. 2018).
 Note – In all above refreences, this species has been reported as Sertitympanum aegypticus.
description: Published as part of Khalili-Moghadam, Arsalan & Saboori, Alireza, 2021, World distribution and habitat scope of Ameroseiidae (Acari: Mesostigmata), pp. 403-450 in Persian Journal of Acarology 10 (4) on page 406, DOI: 10.22073/pja.v10i4.67440, http://zenodo.org/record/7173383
title: Xanthorrhoea australis R. Br.
Creators: name: :None
Publisher: name: Universitätsbibliothek Braunschweig
Year: 2023
Subjects: subject: Digitale Pflanzenbilder: Sammlung Dietmar Brandes
subject: 58

description: Pflanzensammlung Dietmar Brandes: Digitale Pflanzenbilder
title: Arabian Gulf in the Era of Portuguese Dominance: A Study in Historical Sources/ Mohamed Hameed Al-Salman
Creators: name: Al-Salman, Mohamed Hameed
Publisher: name: National Library and Archives
Year: 2012
Subjects: Arabian Gulf Region - Relations - Portugal.
Portugal - Relations - Arabian Gulf Region.
Arabian Gulf Region - History - 16th century.
Arabian Gulf Region - History - 17th century.

This study of the era of Portuguese dominance in the Arabian Gulf is an attempt at delving deeper into such facts to verify whether they speak for themselves or they come to light through disputes and disagreements. The paper examines historical facts gleaned from important Portuguese, British, French, Persian and Arabic documentary sources and references covering the period of the Portuguese invasion of the Gulf region, and her political as well as military predominance in that region from 1507 to 1650.
title: Xerochrysum bracteatum (Vent.) Tzvelev
Creators: name: :None
Publisher: name: Universitätsbibliothek Braunschweig
Year: 2023
Subjects: subject: Digitale Pflanzenbilder: Sammlung Dietmar Brandes
subject: 58

description: Pflanzensammlung Dietmar Brandes: Digitale Pflanzenbilder
Ultra-bright CO and [CI] emission in a lensed z=2.04 submillimeter galaxy with extreme molecular gas properties
Creators: name: Dannerbauer, H.
name: Harrington, K.
name: Diaz-Sanchez, T.
name: Iglesias-Groth, S.
name: Rebolo, R.
name: Genova-Santos, R.
name: Krips, M.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We report the very bright detection of cold molecular gas with the IRAM NOEMA interferometer of the strongly lensed source WISE J132934.18+224327.3 at z=2.04, the so-called Cosmic Eyebrow. This source has a similar spectral energy distribution from optical-mid/IR to submm/radio but significantly higher fluxes than the well-known lensed SMG SMMJ 2135, the Cosmic Eyelash at z=2.3. The interferometric observations identify unambiguously the location of the molecular line emission in two components, component CO32-A with I_CO(3-2)=52.2+-0.9 Jy km s^-1 and component CO32-B with I_CO(3-2)=15.7+-0.7 Jy km s^-1. Thus, our NOEMA observations of the CO(3-2) transition confirm the SMG-nature of WISE J132934.18+224327.3, resulting in the brightest CO(3-2) detection ever of a SMG. In addition, we present follow-up observations of the brighter component with the Green Bank Telescope (CO(1-0) transition) and IRAM 30m telescope (CO(4-3) and [CI](1-0) transitions). The star-formation efficiency of ~100 L_sun (K km s^-1 pc^2) is at the overlap region between merger-triggered and disk-like star-formation activity and the lowest seen for lensed dusty star-forming galaxies. The determined gas depletion time ~60~Myr, intrinsic infrared star-formation SFR_IR approx. 2000 M_sun yr^-1 and gas fraction M_mol/M_star=0.44 indicates a starburst/merger triggered star-formation. The obtained data of the cold ISM - from CO(1-0) and dust continuum - indicates a gas mass M_mol~15x10^11 M_sun for component CO32-A. Its unseen brightness offers the opportunity to establish the Cosmic Eyebrow as a new reference source at z=2 for galaxy evolution.
description: Accepted by AJ. 14 pages, 10 figures and 3 tables
Understanding mechanism of performance improvement in nitrogen-doped niobium superconducting radio frequency cavity
Creators: name: Fang, Xiaotian
name: Oh, Jin-Su
name: Kramer, Matt
name: Romanenko, A.
name: Grassellino, A.
name: Zasadzinski, John
name: Zhou, Lin
Publisher: name: Taylor & Francis
Year: 2022
Subjects: subject: Space Science
subject: Microbiology
subject: FOS: Biological sciences
subject: Physiology
subject: Environmental Sciences not elsewhere classified
subject: Chemical Sciences not elsewhere classified
subject: Ecology
subject: Immunology
subject: FOS: Clinical medicine
subject: Developmental Biology
subject: Hematology
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Niobium superconducting radiofrequency cavities enable applications in modern accelerators and quantum computers. However, the surface resistance significantly deteriorates the cavities’ performance. Nitrogen doping surface treatment can consistently increase cavity performance by reducing surface resistance, but the improvement mechanism is not fully understood. Herein, we employed transmission electron microscopy and spectroscopy to uncover the structural and chemical differences of the Nb/air interface between the non-doped and nitrogen-doped cavities. The results indicate that nitrogen doping passivates the Nb surface by introducing a compressive stress/strain close to the Nb/air interface, which impedes the diffusion of oxygen and hydrogen atoms and reduces surface oxide thickness. A comprehensive structural and chemical study of the Nb/air interface from the non-doped and nitrogen-doped niobium cavity helps to understand the performance improvement mechanisms of the nitrogen-doped cavity.
Discretization based Solutions for Secure Machine Learning against Adversarial Attacks
Creators: name: Panda, Priyadarshini
name: Chakraborty, Indranil
name: Roy, Kaushik
Publisher: name: arXiv
Year: 2019
Subjects: subject: Machine Learning (cs.LG)
subject: Cryptography and Security (cs.CR)
subject: Computer Vision and Pattern Recognition (cs.CV)
subject: Machine Learning (stat.ML)
subject: FOS: Computer and information sciences

description: Adversarial examples are perturbed inputs that are designed (from a deep learning network's (DLN) parameter gradients) to mislead the DLN during test time. Intuitively, constraining the dimensionality of inputs or parameters of a network reduces the 'space' in which adversarial examples exist. Guided by this intuition, we demonstrate that discretization greatly improves the robustness of DLNs against adversarial attacks. Specifically, discretizing the input space (or allowed pixel levels from 256 values or 8-bit to 4 values or 2-bit) extensively improves the adversarial robustness of DLNs for a substantial range of perturbations for minimal loss in test accuracy. Furthermore, we find that Binary Neural Networks (BNNs) and related variants are intrinsically more robust than their full precision counterparts in adversarial scenarios. Combining input discretization with BNNs furthers the robustness even waiving the need for adversarial training for certain magnitude of perturbation values. We evaluate the effect of discretization on MNIST, CIFAR10, CIFAR100 and Imagenet datasets. Across all datasets, we observe maximal adversarial resistance with 2-bit input discretization that incurs an adversarial accuracy loss of just ~1-2% as compared to clean test accuracy.
description: 8 pages, 8 Figures, 6 Tables
Suppression of Low-mass Galaxy Formation around Quasars at z~2-3
Creators: name: Uchiyama, H.
name: Kashikawa, N.
name: Overzier, R.
name: Toshikawa, J.
name: Onoue, M.
name: Ishikawa, S.
name: Kubo, M.
name: Ito, K.
name: Namiki, S.
name: Liang, Y.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We have carried out deep and wide field imaging observations with narrow bands targeting 11 quasar fields to systematically study the possible photoevaporation effect of quasar radiation on surrounding low mass galaxies at $z\sim2-3$. We focused on Lyman alpha emitters (LAEs) at the same redshifts as the quasars that lie within the quasar proximity zones, where the ultra-violet radiation from the quasars is higher than the average background at that epoch. We found that LAEs with high rest-frame equivalent width of Ly$α$ emission ($EW_0$) of $\gtrsim 150$Å$~$ with low stellar mass ($\lesssim 10^8 M_{\odot}$), are predominantly scarce in the quasar proximity zones, suggesting that quasar photoevaporation effects may be taking place. The halo mass of LAEs with $EW_0>150$Å$~$ is estimated to be $3.6^{+12.7}_{-2.3}\times10^9 M_{\odot}$ either from the Spectral Energy Distribution (SED) fitting or the main sequence. Based on a hydrodynamical simulation, the predicted delay in star formation under a local UV background intensity with $J (ν_L)\gtrsim10^{-21}$ erg s$^{-1}$ cm$^{-2}$ Hz$^{-1}$ sr$^{-1}$ for galaxies having less than this halo mass is about $>20$ Myr, which is longer than the expected age of LAEs with $EW_0>150$Å. On the other hand, the photoevaporation seems to be less effective around very luminous quasars, which is consistent with the idea that these quasars are still in an early stage of quasar activity.
description: 18 pages, 9 figures