cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Evidence for singular-phonon-induced nematic superconductivity in a topological superconductor candidate Sr$_{0.1}$Bi$_2$Se$_3$
Creators: name: Wang, Jinghui
name: Ran, Kejing
name: Li, Shichao
name: Ma, Zhen
name: Bao, Song
name: Cai, Zhengwei
name: Zhang, Youtian
name: Nakajima, Kenji
name: Ohira-Kawamura, Seiko
name: Cermak, P.
name: Schneidewind, A.
name: Savrasov, Sergey Y.
name: Wan, Xiangang
name: Wen, Jinsheng
Publisher: name: arXiv
Year: 2019
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: Superconductivity mediated by phonons is typically conventional, exhibiting a momentum-independent s-wave pairing function, due to the isotropic interactions between electrons and phonons along different crystalline directions. Here, by performing inelastic neutron scattering measurements on a superconducting single crystal of Sr0.1Bi2Se3, a prime candidate for realizing topological superconductivity by doping the topological insulator Bi2Se3, we find that there exist highly anisotropic phonons, with the linewidths of the acoustic phonons increasing substantially at long wavelengths, but only for those along the [001] direction. This observation indicates a large and singular electron-phonon coupling at small momenta, which we propose to give rise to the exotic p-wave nematic superconducting pairing in the MxBi2Se3 (M = Cu, Sr, Nb) superconductor family. Therefore, we show these superconductors to be example systems where electron-phonon interaction can induce more exotic superconducting pairing than the s-wave, consistent with the topological superconductivity.
description: Published in Nature Communications
Ionizing Photons and EUV Excesses in Clusters of Galaxies
Creators: name: Maloney, Philip R.
name: Bland-Hawthorn, J.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Observations with the Extreme Ultraviolet Explorer satellite are purported to show extreme ultraviolet (EUV) and soft X-ray excesses in several clusters of galaxies (Bonamente, Lieu & Mittaz 2001). If interpreted as thermal emission, this would imply the presence of warm (T\sim 10^6 K) gas in these clusters with a mass comparable to that of gas at coronal temperatures. If true, this would have profound implications for our understanding of galaxy clusters and the distribution of baryons in the universe. Here we show that because of the large ionizing photon emissivities of gas at such low temperatures, the ionizing photon fluxes seen by disk galaxies in the observed clusters can be very large, resulting in minimum emission measures from neutral gas in such disks as high as 100 cm^(-6) pc. This result is essentially independent of the mechanism actually responsible for producing the alleged EUV excesses. The predicted emission measures in Abell 1795 (z=0.063) are about an order of magnitude larger than seen in the Reynolds layer of the Galaxy, providing a straightforward observational test of the reality of the EUV excess. New tunable filter H alpha images and WFPC images from the Hubble Space Telescope archive do not support the existence of the claimed EUV excess.
description: To appear in ApJ Letters; 11 pages, 3 figures
Hot Settling Accretion Flow onto a Spinning Black Hole
Creators: name: Medvedev, Mikhail V.
name: Murray, Norman
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We study the structure and properties of hot MHD accretion onto a Kerr black hole. In such a system, the hole is magnetically coupled to the inflowing gas and exerts a torque onto the accretion flow. A hot settling flow can form around the hole and transport the angular momentum outward, to the outer edge of the flow. Unlike other hot flows, such as advection- and convection-dominated flows and inflow-outflow solutions (ADAFs, CDAFs, and ADIOS), the properties of the hot settling flow are determined by the spin of the central black hole, but are insensitive to the mass accretion rate. Therefore, it may be possible to identify rapidly spinning BHs simply from their broad-band spectra. Observationally, the hot settling flow around a Kerr hole is somewhat similar to other hot flows in that they all have hard, power-law spectra and relatively low luminosities. Thus, most black hole candidates in the low/hard and, perhaps, intermediate X-ray state may potentially accrete via the hot settling flow. However, a settling flow will be somewhat more luminous than ADAFs/CDAFs/ADIOS, will exhibit high variability in X-rays, and may have relativistic jets. This suggests that galactic microquasars and active galactic nuclei may be powered by hot settling flows. We identify several galactic X-ray sources as the best candidates.
description: 7 pages, 1 figure. Submitted to ApJ
Monoctenus juniperi
Creators: name: Schedl, W.
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Diprionidae
Monoctenus
Monoctenus juniperi

description: Monoctenus juniperi (LINNAEUS 1758)
M a t e r i a l: 1 Ex. Syrie, Brousse (=alte Bezeichnung von Bosra) (ABEILLE de PERRIN 1881; HARIRI 1971). Die Artzugehörigkeit ist nicht gesichert.
 B i o l o g i e: Die Larven fressen an Nadeln von Juniperus communis (ENSLIN 1917, BENSON 1951), die Imagines fliegen zur Zeit der Wacholderblüte (ENSLIN 1917).
V e r b r e i t u n g:M-u.N-Europa(BENSON 1951), S-Europa (PESARINI 2002).
description: Published as part of Schedl, W., 2009, Die Pflanzenwespen von Syrien (Hymenoptera: Symphyta) - ein Überblick, pp. 1609-1630 in Linzer biologische Beiträge 41 (2) on page 1611, DOI: 10.5281/zenodo.5279162
Open access.pdf
Creators: name: , Maryam
Publisher: name: figshare
Year: 2019
Subjects: subject: 130103 Higher Education
subject: FOS: Educational sciences

description: This paper has been published in Encyclopedia of Library and Information Science in Persian. It is a brief paper on history, models, benefits, search and challenges of open access publishing. یک مقاله دائره المعارفی است که به پیشینه، انواع، مدلها و مزایای نشر دسترسی آزاد؛ جستجوی مقالات دسترسی آزاد و مسائل و چالش های دسترسی آزاد می پردازد
Tantalizing New Physics from the Cosmic Purview
Creators: name: Melia, Fulvio
Publisher: name: arXiv
Year: 2019
Subjects: subject: General Physics (physics.gen-ph)
subject: FOS: Physical sciences

description: The emergence of a highly improbable coincidence in cosmological observations speaks to a remarkably simple cosmic expansion. Compelling evidence now suggests that the Universe's gravitational horizon, coincident with the better known Hubble sphere, has a radius improbably equal to the distance light could have travelled since the Big Bang. The confirmation of this unexpected result would undoubtedly herald the influence of new physics, yet appears to be unavoidable after a recent demonstration that the Friedmann-Lemaitre-Robertson-Walker metric is valid only for the so-called zero active mass equation of state. As it turns out, a cosmic fluid with this property automatically produces the aforementioned equality, leaving little room for a cosmological constant. The alternative---a dynamical dark energy---would suggest an extension to the standard model of particle physics, and a serious re-evaluation of the Universe's early history.
description: 23 pages, 9 figures, Review article accepted for publication in Modern Physics Letters A
Additional file 1 of Transcriptomic analysis of glucosidase II beta subunit (GluIIß) knockout A549 cells reveals its roles in regulation of cell adhesion molecules (CAMs) and anti-tumor immunity
Creators: name: Khaodee, Worapong
name: Xiyuan, Guo
name: Han, Moe Thi Thi
name: Tayapiwatana, Chatchai
name: Chiampanichayakul, Sawitree
name: Anuchapreeda, Songyot
name: Cressey, Ratchada
Publisher: name: figshare
Year: 2024
Subjects: subject: Biochemistry
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Genetics
subject: Molecular Biology
subject: Physiology
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer
subject: Hematology
subject: Computational Biology

description: Additional file 1: Figure 1A. Western blot analysis showing GluIIß expression levels in GluIIß KO and non-target transfected cells. Figure 5A. Image of cytokine array signals containing 42 different anti-cytokine antibodies spotted in duplicate, including 3 positive and 2 negative controls, hybridized with co-culture media. Supplementary table 1. List of primers used in this study.
Crystalline membrane morphology beyond polyhedra
Creators: name: Yuan, Hang
name: de la Cruz, Monica Olvera
Publisher: name: arXiv
Year: 2019
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Elastic crystalline membranes exhibit a buckling transition from sphere to polyhedron. However, their morphologies are restricted to convex polyhedra and are difficult to externally control. Here, we study morphological changes of closed crystalline membrane of super-paramagnetic particles. The competition of magnetic dipole-dipole interactions with the elasticity of this magnetoelastic membrane leads to concave morphologies. Interestingly, as the magnetic field strength increases, the symmetry of the buckled membrane decreases from 5-fold to 3-fold, to 2-fold and, finally, to 1-fold rotational symmetry. This gives the ability to switch the membrane morphology between convex and concave shapes with specific symmetry and provides promising applications for membrane shape control in the design of actuatable micro-containers for targeted delivery systems.
Submillimeter lines from circumstellar disks around pre-main sequence stars
Creators: name: van Zadelhoff, Gerd-Jan
name: van Dishoeck, Ewine F.
name: Thi, Wing-Fai
name: Blake, Geoffrey A.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Observations of submillimeter lines of CO (up to J=6-5), HCO+, HCN (up to J=4-3) and their isotopes from circumstellar disks around low mass pre-main sequence stars are presented. The different line ratios and optical depths indicate that most of the observed line emission arises from an intermediate disk layer with high densities of 1E6-1E8 cm-3 and moderately warm temperatures in the outer regions. The data are compared with three disk models from the literature using a full 2D Monte Carlo radiative transfer code. The abundances of the molecules are constrained from the more optically thin 13C species and indicate depletions of 1-30 for LkCa 15 and very high depletions of > 100 for TW Hya with respect to dark cloud abundances. Evidence for significant freeze-out (factors 10 or larger) of CO and HCO+ onto grain surfaces at temperatures below 22 K is found, but the abundances of these molecules must also be low in the warmer upper layer, most likely as a result of photodissociation. A warm upper layer near the surface of a flaring disk heated by stellar and interstellar radiation is an appropriate description of the observations of TW Hya. LkCa 15 seems to be cooler at the surface, perhaps due to dust settling.
description: 15 pages, 8 figures. Accepted for publication in A&A
Arge auripennis KONOW 1891
Creators: name: Schedl, W.
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Argidae
Arge
Arge auripennis

description: Arge auripennis KONOW 1891
 M a t e r i a l 13 Syrie, als „ Hylotoma sanguinicollis ANDRÉ“ in ABEILLE de PERRIN (1881), bestätigt in BENSON (1968); 1♀ 13 Syria NW, 20 km NE Latakia, 25.5.1996, leg. M. Halada, in coll. OÖLM, det. W.Sch. 2009.
B i o l o g i e: unbekannt.
V e r b r e i t u n g SO-Europa, Transkaukasien, Kaukasus, Türkei, Syrien (BENSON 1968; SMITH 1982).
description: Published as part of Schedl, W., 2009, Die Pflanzenwespen von Syrien (Hymenoptera: Symphyta) - ein Überblick, pp. 1609-1630 in Linzer biologische Beiträge 41 (2) on page 1613, DOI: 10.5281/zenodo.5279162
Introducing Certified Compilation in Education by a Functional Language Approach
Creators: name: Lindgren, Per
name: Lindner, Marcus
name: Fitinghoff, Nils
Publisher: name: arXiv
Year: 2019
Subjects: subject: Programming Languages (cs.PL)
subject: Logic in Computer Science (cs.LO)
subject: FOS: Computer and information sciences

description: Classes on compiler technology are commonly found in Computer Science curricula, covering aspects of parsing, semantic analysis, intermediate transformations and target code generation. This paper reports on introducing certified compilation techniques through a functional language approach in an introductory course on Compiler Construction. Targeting students with little or no experience in formal methods, the proof process is highly automated using the Why3 framework. Underlying logic, semantic modelling and proofs are introduced along with exercises and assignments leading up to a formally verified compiler for a simplistic imperative language. This paper covers the motivation, course design, tool selection, and teaching methods, together with evaluations and suggested improvements from the perspectives of both students and teachers.
description: In Proceedings TFPIE 2018, arXiv:1906.10757
Cometary compositions compared with protoplanetary disk midplane chemical evolution. An emerging chemical evolution taxonomy for comets
Creators: name: Eistrup, Christian
name: Walsh, Catherine
name: van Dishoeck, Ewine F.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: [Abridged] With a growing number of molecules observed in many comets, and an improved understanding of chemical evolution in protoplanetary disk midplanes, comparisons can be made between models and observations that could potentially constrain the formation histories of comets. A $χ^{2}$-method was used to determine maximum likelihood surfaces for 14 different comets that formed at a given time (up to 8 Myr) and place (out to beyond the CO iceline) in the pre-solar nebula midplane. This was done using observed volatile abundances for the 14 comets and the evolution of volatile abundances from chemical modelling of disk midplanes. Considering all parent species (ten molecules) in a scenario that assumed reset initial chemistry, the $χ^{2}$ likelihood surfaces show a characteristic trail in the parameter space with high likelihood of formation around 30 AU at early times and 12 AU at later times for ten comets. This trail roughly traces the vicinity of the CO iceline in time. The formation histories for all comets were thereby constrained to the vicinity of the CO iceline, assuming that the chemistry was partially reset early in the pre-solar nebula. This is found, both when considering carbon-, oxygen-, and sulphur-bearing molecules (ten in total), and when only considering carbon- and oxygen-bearing molecules (seven in total). Since these 14 comets did not previously fall into the same taxonomical categories together, this chemical constraint may be proposed as an alternative taxonomy for comets. Based on the most likely time for each of these comets to have formed during the disk chemical evolution, a formation time classification for the 14 comets is suggested.
description: 16 pages, accepted for publication in Astronomy & Astrophysics
M-type Vega-like stars
Creators: name: Song, Inseok
name: Weinberger, A.
name: Becklin, E.
name: Zuckerman, B.
name: Chen, C.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We carried out a search for M-type Vega-like stars by correlating the IRAS Faint Source Catalog with Hipparcos selected M-type stars. Three stars with apparent IRAS 25mu excess emission are shown instead to be non-IR-excess stars from ground-based 11.7 and 17.9mu photometry. Two stars previously suggested to have Vega-like mid-IR excess are also shown to be non-excess stars. These results imply that other suggested mid-IR excess stars in the literature may also be false excess stars. Detection threshold bias is apparently responsible for these bogus IR excesses. Sixty micron excess emission from a previously known M-type Vega-like star (GJ 803) is identified again.
description: 3 figures, 1 table. Accepted in AJ
Open access publishing: history, models, search, challenges دسترسی آزاد: پیشینه، مدلها، جستجو، چالشها
Creators: name: , Maryam
Publisher: name: figshare
Year: 2019
Subjects: subject: 130103 Higher Education
subject: FOS: Educational sciences

description: This paper has been published in Encyclopedia of Library and Information Science in Persian. It is a brief paper on history, models, benefits, search and challenges of open access publishing. یک مقاله دائره المعارفی است که به پیشینه، انواع، مدلها و مزایای نشر دسترسی آزاد؛ جستجوی مقالات دسترسی آزاد و مسائل و چالش های دسترسی آزاد می پردازد
Additional file 1 of The outcome of conversion total hip arthroplasty following acetabular fractures: a systematic review and meta-analysis of comparative studies
Creators: name: Shaker, Farhad
name: Esmaeili, Sina
name: Nakhjiri, Mobina Taghva
name: Azarboo, Alireza
name: Shafiei, Seyyed Hossein
Publisher: name: figshare
Year: 2024
Subjects: Space Science
Medicine
Cell Biology
Environmental Sciences not elsewhere classified
Biological Sciences not elsewhere classified
Science Policy

description: Additional file 1 : Fig. S1. Risk of bias assessment of eligible studies using base on Newcastle Ottawa scale (NOS). Fig. S2. Forest plots demonstrating the revision rate in those who underwent cTHA versus pTHA. Fig. S3. Forest plots demonstrating the operation time (A), blood loss (B), and bone graft need (C) in those who underwent cTHA versus pTHA. Fig. S4. Forest plots demonstrating the revision rate in those who underwent ORIF versus conservative. Fig. S5. Forest plots demonstrating the operation time (A), blood loss (B), and bone graft need C in those who underwent ORIF versus conservative. Fig. S6. Forest plots demonstrating the operation time (A) and blood loss B in those who underwent acute THA versus delayed THA. Fig. S7. Funnel plot of the group A studies reporting infection rate. Fig. S8. Funnel plot of the group B studies reporting heterotopic ossification. Fig. S9. Funnel plot of the group C studies reporting dislocation rate.
An isomorphism between polynomial eigenfunctions of the transfer operator and the Eichler cohomology for modular groups
Creators: name: Mayer, D.
name: Neunhaeuserer, J.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Number Theory (math.NT)
subject: Mathematical Physics (math-ph)
subject: Dynamical Systems (math.DS)
subject: FOS: Mathematics
subject: FOS: Physical sciences
subject: 11F11, 30F35, 37C30

description: For the group PSL(2,Z) it is known that there is an isomorphism between polynomial eigenfunctions of the transfer operator for the geodesic flow and the Eichler cohomology in the theory of modular forms. In a recent paper by Chang and Mayer it is indicated that such an isomorphism exists as well for certain subgroups of PSL(2,Z). We prove this and provide some evidence by computer aided algebraic calculations that such an isomorphism exists for all principal congruence subgroups and all congruence subgroups of Hecke type.
description: 18 pages
Arge pleuritica
Creators: name: Schedl, W.
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Argidae
Arge
Arge pleuritica

description: Arge pleuritica (KLUG 1834)
M a t e r i a l:? Ex. Syria ohne Fundortangabe (ABEILLE de PERRIN 1881; HARIRI 1971).
B i o l o g i e: unbekannt.
V e r b r e i t u n g Südosteuropa, Halbinsel Krim, Anatolien, Transkaukasus, Kaukasus, Mittelasien (BENSON 1968; MUCHE 1977), Griechenland (PESARINI 2002).
description: Published as part of Schedl, W., 2009, Die Pflanzenwespen von Syrien (Hymenoptera: Symphyta) - ein Überblick, pp. 1609-1630 in Linzer biologische Beiträge 41 (2) on page 1613, DOI: 10.5281/zenodo.5279162
The Kṣatrīya Odissey Continues
Creators: name: RODRIGUES, TENSING CARLOS
Publisher: name: figshare
Year: 2019
Subjects: subject: History
subject: Anthropology
subject: FOS: Sociology
subject: Archaeology
subject: Geography
subject: Sociology

description: But, like the ephemeral Sarasvatī, the fall of Kāṭhīyāvāḍ was written in its making. Set on the land created by the receding sea, it got submerged when the Ice Age ended. And the kāṭhīyāvāḍī kṣatrīya had to flee. They had to find another Kāṭhīyāvāḍ. The natural course was to move south along the western coast. That is what brought them to Kōṁkaṇ. As we have said earlier, Kāṭhīyāvāḍ was not just a single port, it was a massive port complex; its replacement had to be equally massive. What eventually came to be built was a ‘belt’ of ports spanning the entire littoral of Kōṁkaṇ, from Saṁjāṇ in Gujarat (outside modern Daman) to Kuśasthaḷi in Goa. [Ancient God Of A Modern Metropolis, 15 Apr 18; A Survey Of Ancient Kōṁkaṇ Ports, 29 Apr 18] Of course we do not know whether these were built from the scratch, or whether they captured and expanded existing ports. [The Shells Of Khirsara, 23 Jun 19]We find strong evidence to back such a hypothesis. One of the new port they founded was at the mouth of river Zuari in Goa, which not only looked very much like the Kuśasthaḷi port the kāṭhīyāvāḍī kṣatrīya had left behind, but was promising – fertile land, lush vegetation and plenty of water; and a sheltered harbour. In keeping with the nostalgic practice we find common in history, they named the place Kuśasthaḷi. They occupied several villages around – Sāṁkhavāḷi (Sancoale), probably naming it after Shankhodhar (also called Bet Dwarka) that they had left behind; Kēḷaśī (Quelossim); Loṭli (Loutulim), probably naming it after Lothal, whose remains have been found; and so on. [The Lost Ports of Goa, 20 May 18]
Cold-Tip Temperature Control of Space-borne SatelliteStirlingCryocooler: Mathematical Modeling and Control Investigation
Creators: name: Nagarsheth, Shaival H.
name: Bhatt, Jiten H.
name: Barve, Jayesh J.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Optimization and Control (math.OC)
subject: Systems and Control (eess.SY)
subject: FOS: Mathematics
subject: FOS: Electrical engineering, electronic engineering, information engineering

description: IR (Infra-Red) detectors are widely used in Space-borne remote sensing satellites. In order to achieve a high signal to noise ratio, the IR detectors need to be operated at cryogenic temperatures. Traditionally, the cryogenic cooling of these detectors is achieved using passive cooling techniques. However recent trend is to employ Stirling-cycle based miniaturized active cryocoolers. An accurate and stringent control of active cryocooler cold-tip temperature is essential to accomplish high signal & image quality from the IR detectors. This paper presents work on investigations and comparison of performance of proposed 2-DOF (2-Degrees-of-Freedom) versus traditional 1-DOF feedback-control structures for the control of cryocooler cold-tip temperature used in IR (Infra-Red) detectors of Space Satellites. Towards this, first-principle based control oriented mathematical model simulated in Matlab/Simulink is proposed to support such investigation and controller tuning. Open-loop (system) and closed-loop (controls) simulation results are tuned & validated with the experimental data obtained from the Lab-scale test-setup of a commercial Stirlingcryocooler. The performance of 2-DOF feedback control structures are analyzed with the help of experiment results offering a better cold-tip temperature control performance.
description: 7 pages, 16 figures, 5th IFAC Conference on Advances in Control and Optimization of Dynamical Systems ACODS 2018
ASCA X-ray source catalogue in the Galactic Center region
Creators: name: Sakano, Masaaki
name: Koyama, Katsuji
name: Murakami, Hiroshi
name: Maeda, Yoshitomo
name: Yamauchi, Shigeo
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The ASCA satellite made 107 pointing observations on a 5 x 5 deg^2 region around the center of our Milky Way Galaxy (the Galactic Center) from 1993 to 1999. In the X-ray images of the 0.7--3 keV or 3--10 keV bands, we found 52 point sources and a dozen diffuse sources. All the point sources are uniformly fitted with an absorbed power-law model. For selected bright sources, Sgr A*, AX J1745.6-2901, A 1742-294, SLX 1744-300, GRO J1744-28, SLX 1737-282, GRS 1734-292, AX J1749.2-2725, KS 1741-293, GRS 1741.9-2853, and an unusual flare source XTE J1739-302, we present further detailed spectral and timing analyses, and discuss their nature. The dozen extended X-ray sources comprise radio supernova remnants, giant molecular clouds, and some new discoveries. Most show emission lines from either highly ionized atoms or low-ionized irons. The X-ray spectra were fitted with either a thin thermal or power-law model. This paper summarizes the results and provides the ASCA X-ray source catalogue in the Galactic Center region.
description: 33 pages, 8 figures, Accepted for publication in ApJS, also found in http://www.star.le.ac.uk/~mas/research/paper/#Sakano2001apjs
Security of 5G-Mobile Backhaul Networks: A Survey
Creators: name: Choudhary, Gaurav
name: Kim, Jiyoon
name: Sharma, Vishal
Publisher: name: arXiv
Year: 2019
Subjects: subject: Networking and Internet Architecture (cs.NI)
subject: Cryptography and Security (cs.CR)
subject: Social and Information Networks (cs.SI)
subject: FOS: Computer and information sciences

description: The rapid involution of the mobile generation with incipient data networking capabilities and utilization has exponentially increased the data traffic volumes. Such traffic drains various key issues in 5G mobile backhaul networks. Security of mobile backhaul is of utmost importance; however, there are a limited number of articles, which have explored such a requirement. This paper discusses the potential design issues and key challenges of the secure 5G mobile backhaul architecture. The comparisons of the existing state-of-the-art solutions for secure mobile backhaul, together with their major contributions have been explored. Furthermore, the paper discussed various key issues related to Quality of Service (QoS), routing and scheduling, resource management, capacity enhancement, latency, security-management, and handovers using mechanisms like Software Defined Networking and millimeter Wave technologies. Moreover, the trails of research challenges and future directions are additionally presented.
description: 30 pages, 6 figures, 6 tables, Journal of Wireless Mobile Networks, Ubiquitous Computing, and Dependable Applications (JoWUA)
Additional file 2: of Health, not weight loss, focused programmes versus conventional weight loss programmes for cardiovascular risk factors: a systematic review and meta-analysis
Creators: name: Khasteganan, Nazanin
name: Lycett, Deborah
name: Furze, Gill
name: Turner, Andy
Publisher: name: figshare
Year: 2019
Subjects: Medicine
Developmental Biology
Science Policy
Computational Biology

description: Additional Meta-analysis. (DOCX 975 kb)
Arge scita
Creators: name: Schedl, W.
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Argidae
Arge
Arge scita

description: Arge scita (MOCSÁRY 1880)
 M a t e r i a l: 2 Ex. Syrien, Umgebung Damaskus, als " Hylotoma proxima nov.spec." (ANDRÉ 1881; ABEILLE de PERRIN, 1881; MAGRETTI 1890); 1♀ Syria (GHIGI 1904) 1♀ 233 Syria, 40 km NE Damaskus, 13.5.1996, leg. M. Halada, in OÖLM, det. W. Sch. 2009.
 B i o l o g i e: Adulte auf Euphorbien gefunden (ABEILLE de PERRIN 1881), Larven an Blättern von Prunus (MUCHE 1977), gezogen vom Verfasser und GEORGHIOU (1977) von Prunus dulcis (Mandelbaumblättern).
V e r b r e i t u n g Griechenland, Türkei, Syrien, Libanon, Israel, Transkaukasus, Iran, Turkmenien (BENSON 1968), Kreta (SCHEDL 1985), Zákynthos 1♀ 13 leg. et in coll. W. Sch.
description: Published as part of Schedl, W., 2009, Die Pflanzenwespen von Syrien (Hymenoptera: Symphyta) - ein Überblick, pp. 1609-1630 in Linzer biologische Beiträge 41 (2) on page 1614, DOI: 10.5281/zenodo.5279162
Additional file 1 of Insights into estrogen impact in oral health & microbiome in COVID-19
Creators: name: Bayardo-González, Rubén Alberto
name: Peña-Rodríguez, Marcela
name: Pereira-Suárez, Ana Laura
name: Rubio-Sánchez, Alina Xcaret
name: García-Chagollán, Mariel
name: Valenzuela-Orozco, Daniel Natividad
name: Lizarazo-Taborda, Melida del Rosario
name: Mora-Mora, Jesús
name: Vega-Magaña, Natali
Publisher: name: figshare
Year: 2024
Subjects: subject: Medicine
subject: Physiology
subject: FOS: Biological sciences
subject: Biotechnology
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Mathematical Sciences not elsewhere classified
subject: Science Policy
subject: Infectious Diseases
subject: FOS: Health sciences

description: Additional file 1: S1. Table of symptoms. S2. Questionnaire for demographic and clinical data. S3. Table accession numbers to sequences NCBI repository.
Nucleosynthesis and mixing on the Asymptotic Giant Branch. III. Predicted and observed s-process abundances
Creators: name: Busso, M.
name: Gallino, R.
name: Lambert, D. L.
name: Travaglio, C.
name: Smith, V. V.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present the results of s-process nucleosynthesis calculations for AGB stars of different metallicities and initial masses. The computations were based on previously published stellar evolutionary models that account for the III dredge up phenomenon occurring late on the AGB. Neutron production is driven by the 13C(alpha,n)16O reaction during the interpulse periods in a tiny layer in radiative equilibrium at the top of the He- and C-rich shell. The s-enriched material is subsequently mixed with the envelope by the III dredge up, and the envelope composition is computed after each thermal pulse. We follow the changes in the photospheric abundance of the Ba-peak elements (heavy s, or `hs') and that of the Zr-peak ones (light s, or `ls'), whose logarithmic ratio [hs/ls] has often been adopted as an indicator of the s-process efficiency. The theoretical predictions are compared with published abundances of s elements for Galactic AGB giants of classes MS, S, SC, post-AGB supergiants, and for various classes of binary stars. The observations in general confirm the complex dependence of n captures on metallicity. They suggest that a moderate spread exists in the abundance of 13C that is burnt in different stars. Although additional observations are needed, a good understanding has been achieved of s-process operation in AGB. The detailed abundance distribution including the light elements (CNO) of a few s-enriched stars at different metallicity are examined.
description: Accepted for ApJ, 59 pages, 19 figures, 5 tables
Competing Active and Passive Interactions Drive Amoeba-like Living Crystallites and Ordered Bands
Creators: name: Mauleon-Amieva, Abraham
name: Mosayebi, Majid
name: Hallett, James E.
name: Turci, Francesco
name: Liverpool, Tanniemola B.
name: van Duijneveldt, Jeroen S.
name: Royall, C. Patrick
Publisher: name: arXiv
Year: 2019
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: Swimmers and self-propelled particles are physical models for the collective behaviour and motility of a wide variety of living systems, such as bacteria colonies, bird flocks and fish schools. Such artificial active materials are amenable to physical models which reveal the microscopic mechanisms underlying the collective behaviour. Here we study colloids in a DC electric field. Our quasi-two-dimensional system of electrically-driven particles exhibits a rich and exotic phase behaviour. At low field strengths, electrohydrodynamic flows lead to self-organisation into crystallites with hexagonal order. Upon self-propulsion of the particles due to Quincke rotation, we find an ordered phase of active matter in which the motile crystallites constantly change shape and collide with one another. At higher field strengths, this "dissolves" to an active gas. We parameterise a particulate simulation model which reproduces the experimentally observed phases and, at higher field strengths predicts an activity-driven demixing to band-like structures.
Additional file 1: of Health, not weight loss, focused programmes versus conventional weight loss programmes for cardiovascular risk factors: a systematic review and meta-analysis
Creators: name: Khasteganan, Nazanin
name: Lycett, Deborah
name: Furze, Gill
name: Turner, Andy
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Developmental Biology
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Search strategies. (DOCX 31 kb)
Dynamical mode coupling and coherence in spin Hall nano-oscillator with perpendicular magnetic anisotropy
Creators: name: Chen, Lina
name: Urazhdin, S.
name: Du, Youwei
name: Liu, R. H.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We experimentally study the dynamical modes excited by spin current in Spin Hall nano-oscillators based on the Pt/[Co/Ni] multilayers with perpendicular magnetic anisotropy. Both propagating spin wave and localized solitonic modes of the oscillation are achieved and controlled by varying the applied magnetic field and current. At room temperature, the generation linewidth broadening associated with mode hopping was observed at currents close to the transition between different modes and in the mode coexistence regimes. The mode hopping was suppressed at cryogenic temperatures, confirming that the coupling between modes is mediated by thermal magnons. We also demonstrate that coherent single-mode oscillations with linewidth of 5 MHz can be achieved without applying external magnetic field. Our results provide insight into the mechanisms controlling the dynamical coherence in nanomagnetic oscillators, and guidance for optimizing their applications in spin wave-based electronics.
description: 6 pages, 5 figures
Chemical significance of different temperature regimes for cosmic-ray-induced heating of whole interstellar grains
Creators: name: Kalvans, Juris
name: Kalnin, Juris Roberts
Publisher: name: arXiv
Year: 2019
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Cosmic-ray-induced whole-grain heating induces evaporation and other processes that affect the chemistry of interstellar clouds. With recent data on grain heating frequencies as an input for a modified rate-equation astrochemical model, this study examines, which whole-grain heating temperature regime is the most efficient at altering the chemical composition of gas and ices. Such a question arises because low-temperature heating, albeit less effective at inducing evaporation of adsorbed species, happens much more often than high-temperature grain heating. The model considers a delayed gravitational collapse of a Bonnor-Ebert sphere, followed by a quiescent cloud core stage. It was found that the whole-grain heating regimes can be divided in three classes, depending on their induced physico-chemical effects. Heating to low-temperature thresholds of 27 and 30 K induce desorption of the most volatile of species - N2 and O2 ices, and adsorbed atoms. The medium-temperature thresholds 40, 50, and 60 K allow effective evaporation of CO and CH4, delaying their accumulation in ices. We find that the 40 K threshold is the most effective cosmic-ray induced whole-grain heating regime because its induced evaporation of CO promotes major abundance changes also for other compounds. An important role in grain cooling may be played by molecular nitrogen as the most volatile of the abundant species in the icy mantles. Whole-grain heating determines the sequence of accretion for different molecules on to grain surface, which plays a key role in the synthesis of complex organic molecules.
description: 13 pages, 7 figures, +1 appendix
Eddington limit and radiative transfer in highly inhomogeneous atmospheres
Creators: name: Ruszkowski, Mateusz
name: Begelman, Mitchell C.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Radiation dominated accretion disks are likely to be subject to the ``photon bubble'' instability, which may lead to strong density inhomogeneities on scales much shorter than the disk scale height. Such disks -- and magnetized, radiation-dominated atmospheres in general -- could radiate well above the Eddington limit without being disrupted. When density contrasts become large over distances of order the photon mean free path, radiative transfer cannot be described adequately using either the standard diffusion approximation or existing prescriptions for flux-limited diffusion. Using analytical and Monte Carlo techniques, we consider the effects of strong density gradients deep within radiation- and scattering-dominated atmospheres. We find that radiation viscosity -- i.e., the off-diagonal elements of the radiation stress tensor -- has an important effect on radiative transfer under such conditions. We compare analytical and numerical results in the specific case of a plane-parallel density wave structure and calculate Eddington enhancement factors due to the porosity of the atmosphere. Our results can be applied to the study of dynamical coupling between radiation forces and density inhomogeneities in radiation dominated accretion disks in two or three dimensions.
description: 7 pages, 2 figures, accepted for The Astrophysical Journal
Additional file 1 of Safety levels for organophosphate pesticide residues on fruits, vegetables, and nuts
Creators: name: Jara, Elizabeth
name: Winter, Carl
Publisher: name: figshare
Year: 2019
Subjects: subject: Molecular Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Developmental Biology
subject: Inorganic Chemistry
subject: FOS: Chemical sciences
subject: Plant Biology

description: Table S1: Organophosphate (OP) Pesticide Safety Levels (PSLs) for 80 fruit, vegetable, and nut commodities (DOCX 806 kb)
Η αναστήλωσις των μνημείων της Ακροπόλεως: Προπύλαια, Ερέχθειον, Παρθενών. Κείμενο
Creators: name: (:Unkn) Unknown
Publisher: name: Εργαστήριον Γραφικών Τεχνών " Στεφ. Ν. Ταρουσόπουλος"
Year: 2024
Subjects: Acropolis (Athens, Greece) - Conservation and restoration
Monuments - Athens, Greece

description: 145 σ.
Η αναστήλωσις των μνημείων της Ακροπόλεως: Προπύλαια Ερεχθείον Παρθενών. Σχέδια
Creators: name: (:Unkn) Unknown
Publisher: name: Εργαστήριον Γραφικών Τεχνών "Στεφ. Ν. Ταρουσόπουλος"
Year: 2025
Subjects: Acropolis (Athens, Greece) - Conservation and restoration
Monuments - Athens, Greece

description: πιν., 147 εικ.
Arge simulatrix KONOW 1887
Creators: name: Schedl, W.
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Argidae
Arge
Arge simulatrix

description: Arge simulatrix KONOW 1887
M a t e r i a l:? Ex. Syria (BENSON 1968).
B i o l o g i e: unbekannt.
V e r b r e i t u n g: Griechenland, Türkei, Syrien,Transkaukasus, Iran (BENSON 1968; PESARINI 2002).
description: Published as part of Schedl, W., 2009, Die Pflanzenwespen von Syrien (Hymenoptera: Symphyta) - ein Überblick, pp. 1609-1630 in Linzer biologische Beiträge 41 (2) on page 1614, DOI: 10.5281/zenodo.5279162
Network properties of healthy and Alzheimer's brains
Creators: name: Coninck, José C. P.
name: Ferrari, Fabiano A. S.
name: Reis, Adriane S.
name: Iarosz, Kelly C.
name: Batista, Antonio M.
name: Viana, Ricardo L.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Neurons and Cognition (q-bio.NC)
subject: Physics and Society (physics.soc-ph)
subject: FOS: Biological sciences
subject: FOS: Physical sciences

description: Small-world structures are often used to describe structural connections in the brain. In this work, we compare the structural connection of cortical areas of a healthy brain and a brain affected by Alzheimer's disease with artificial small-world networks. Based on statistics analysis, we demonstrate that similar small-world networks can be constructed using Newman-Watts procedure. The network quantifiers of both structural matrices are identified inside the probabilistic valley. Despite of similarities between structural connection matrices and sampled small-world networks, increased assortativity can be found in the Alzheimer brain. Our results indicate that network quantifiers can be helpful to identify abnormalities in real structural connection matrices.
Fluctuations in the Bose Gas with Attractive Boundary Conditions
Creators: name: Lauwers, J.
name: Verbeure, A.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Mathematical Physics (math-ph)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: In this paper limiting distribution functions of field and density fluctuations are explicitly and rigorously computed for the different phases of the Bose gas. Several Gaussian and non-Gaussian distribution functions are obtained and the dependence on boundary conditions is explicitly derived. The model under consideration is the free Bose gas subjected to attractive boundary conditions, such boundary conditions yield a gap in the spectrum. The presence of a spectral gap and the method of the coupled thermodynamic limits are the new aspects of this work, leading to new scaling exponents and new fluctuation distribution functions.
description: 42 pages, 5 figures
Additional file 1 of Cost-consequence analysis of continuous denosumab therapy for osteoporosis treatment in South Korea
Creators: name: Cha, Seungju
name: Sohn, Minjeong
name: Yang, Hyowon
name: Yeh, Eric J.
name: Baek, Ki-Hyun
name: Ha, Jeonghoon
name: Ku, Hyemin
Publisher: name: figshare
Year: 2024
Subjects: subject: Medicine
subject: Biotechnology
subject: Ecology
subject: FOS: Biological sciences
subject: Cancer
subject: Science Policy
subject: Hematology

description: Supplementary Material 1
Sterictophora furcata
Creators: name: Schedl, W.
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Argidae
Sterictophora
Sterictophora furcata

description: Sterictophora furcata (VILLERS 1789)
M a t e r i a l:? Ex. Syria (BENSON 1968).
 B i o l o g i e: Larven an Blättern von Prunus spinosa (MUCHE 1977); Rubus idaeus agg. (LISTON 1995).
V e r b r e i t u n g:Europa, Türkei, Syrien,Transkaukasien, Iran (BENSON 1968).
description: Published as part of Schedl, W., 2009, Die Pflanzenwespen von Syrien (Hymenoptera: Symphyta) - ein Überblick, pp. 1609-1630 in Linzer biologische Beiträge 41 (2) on page 1614, DOI: 10.5281/zenodo.5279162
RX J1643.7+3402 : a new bright cataclysmic variable
Creators: name: Mickaelian, A. M.
name: Balayan, S. K.
name: Ilovaisky, S. A.
name: Chevalier, C.
name: Veron-Cetty, M. -P.
name: Veron, P.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report the discovery of a new bright (V$\sim$12.6) cataclysmic variable star identified with the ROSAT X-ray source RX J1643.7+3402. Spectroscopic and photometric observations show it to be a novalike variable sharing some of the characteristics of the SW Sex sub-class of novalike CVs. The spectroscopic period may be either 2\fh575 or 2\fh885, within the period "gap." A photometric modulation with a probable period of 2\fh595 and an amplitude of $\sim$ 0.1 mag in V is present on most nights and could be either a "positive" or a "negative" superhump modulation (depending on the exact spectroscopic period), indicating the presence of a precessing accretion disk in this system. Rapid variations of 0.1 to 0.2 mag amplitude in V repeat with a time scale of $\sim$ 15 min.
description: 11 pages, 12 figures, accepted in Astronomy & Astrophysics
Supplementary Material from NFIL3 contributes to cytotoxic T lymphocyte-mediated killing
Creators: name: Douanne, Tiphaine
name: Strege, Katharina
name: Del Castillo Velasco-Herrera, Martin
name: Rochussen, Adam M.
name: Adams, David J.
name: Griffiths, Gillian M.
Publisher: name: The Royal Society
Year: 2024
Subjects: classificationCode: 310199
subject: Biochemistry and cell biology not elsewhere classified

description: Figures S1, S2 and Table 4
Horndeski model in nonlinearly realized supergravity
Creators: name: Yamada, Yusuke
name: Yokoyama, Jun'ichi
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We construct the Horndeski Lagrangian within non-linearly realized supergravity. We will show that the bosonic part of the Horndeski Lagrangian can be realized. Gravitino naturally couples to Horndeski sector in a super-covariant way. Such gravitino couplings are also free from ghosts.
description: 5 pages
MOESM1 of Shaping the lipid composition of bacterial membranes for membrane protein production
Creators: name: Kanonenberg, Kerstin
name: Royes, Jorge
name: Kedrov, Alexej
name: Poschmann, Gereon
name: Angius, Federica
name: Solgadi, Audrey
name: Spitz, Olivia
name: Kleinschrodt, Diana
name: StĂźhler, Kai
name: Miroux, Bruno
name: Schmitt, Lutz
Publisher: name: figshare
Year: 2019
Subjects: subject: Biochemistry
subject: Cell Biology
subject: Molecular Biology
subject: Pharmacology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Developmental Biology
subject: Marine Biology

description: Additional file 1. The file contains detailed protocols for the lipidomics analyses, supplementary data for lipid species quantification, and detailed procedures supplementing the materials and methods section of the main manuscript.
A Comparison of Independent Star Formation Diagnostics for a UV-Selected Sample of Nearby Galaxies
Creators: name: Sullivan, Mark
name: Mobasher, Bahram
name: Chan, Ben
name: Cram, Lawrence
name: Ellis, Richard
name: Treyer, Marie
name: Hopkins, Andrew
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present results from a decimetric radio survey undertaken with the Very Large Array as part of a longer term goal to inter-compare star formation and dust extinction diagnostics, on a galaxy by galaxy basis, for a representative sample of nearby galaxies. For our survey field, Selected Area 57, star formation rates derived from 1.4GHz luminosities are compared with earlier nebular emission line and ultraviolet (UV) continuum diagnostics. We find broad correlations, over several decades in luminosity, between H-alpha, the UV continuum and 1.4GHz diagnostics. However, the scatter in these relations is found to be larger than observational errors, with offsets between the observed relations and those expected assuming constant star-formation histories and luminosity-independent extinction models. We investigate the physical origin of the observed relations, and conclude the discrepancies between different star-formation diagnostics can only be partly explained by simple models of dust extinction in galaxies. These models cannot by themselves explain all the observed differences, introducing the need for temporally varying star-formation histories and/or more complex models of extinction, to explain the entire dataset.
description: 25 pages, 6 Figures. Accepted for publication in ApJ