cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Stereo neutrino spectrum of 235U fission rejects sterile neutrino hypothesis
Creators: name: Almazán, H.
name: Bernard, L.
name: Blanchet, A.
name: Bonhomme, A.
name: Buck, C.
name: Chalil, A.
name: Sanchez, P. del Amo
name: Atmani, I. El
name: Labit, L.
name: Lhuillier, J. Lamblin A. Letourneau D.
name: Licciardi, M.
name: Lindner, M.
name: Materna, T.
name: Pessard, H.
name: Réal, J. -S.
name: Ricol, J. -S.
name: Roca, C.
name: Rogly, R.
name: Salagnac, T.
name: Savu, V.
name: Schoppmann, S.
name: Soldner, T.
name: Stutz, A.
name: Vialat, M.
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: Anomalies in past neutrino measurements have led to the discovery that these particles have non-zero mass and oscillate between their three flavors when they propagate. In the 2010's, similar anomalies observed in the antineutrino spectra emitted by nuclear reactors have triggered the hypothesis of the existence of a supplementary neutrino state that would be sterile i.e. not interacting via the weak interaction. The STEREO experiment was designed to study this scientific case that would potentially extend the Standard Model of Particle Physics. Here we present a complete study based on our full set of data with significantly improved sensitivity. Installed at the ILL (Institut Laue Langevin) research reactor, STEREO has accurately measured the antineutrino energy spectrum associated to the fission of 235U. This measurement confirms the anomalies whereas, thanks to the segmentation of the STEREO detector and its very short mean distance to the core (10~m), the same data reject the hypothesis of a light sterile neutrino. Such a direct measurement of the antineutrino energy spectrum suggests instead that biases in the nuclear experimental data used for the predictions are at the origin of the anomalies. Our result supports the neutrino content of the Standard Model and establishes a new reference for the 235U antineutrino energy spectrum. We anticipate that this result will allow to progress towards finer tests of the fundamental properties of neutrinos but also to benchmark models and nuclear data of interest for reactor physics and for observations of astrophysical or geo-neutrinos.
description: 34 pages, 13 figures. Final version submitted to Nature
A wide field map of intracluster globular clusters in Coma
Creators: name: Madrid, Juan P.
name: O'Neill, Conor R.
name: Gagliano, Alexander T.
name: Marvil, Joshua R.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: The large-scale distribution of globular clusters in the central region of the Coma cluster of galaxies is derived through the analysis of Hubble Space Telescope/Advanced Camera for Surveys data. Data from three different HST observing programs are combined in order to obtain a full surface density map of globular clusters in the core of Coma. A total of 22,426 Globular cluster candidates were selected through a detailed morphological inspection and the analysis of their magnitude and colors in two wavebands, F475W (Sloan g) and F814W (I). The spatial distribution of globular clusters defines three main overdensities in Coma that can be associated with NGC 4889, NGC 4874, and IC 4051 but have spatial scales five to six times larger than individual galaxies. The highest surface density of globular clusters in Coma is spatially coincidental with NGC 4889. The most extended overdensity of globular clusters is associated with NGC 4874. Intracluster globular clusters also form clear bridges between Coma galaxies. Red globular clusters, which agglomerate around the center of the three main subgroups, reach higher surface densities than blue ones.
description: STScI press release: https://media.stsci.edu/news_release/news/2018-44 contains beautiful HST images of the Coma cluster
Empirical Network Structure of Malicious Programs
Creators: name: Musgrave, John
name: Campan, Alina
name: Messay-Kebede, Temesguen
name: Kapp, David
name: Ralescu, Anca
Publisher: name: arXiv
Year: 2022
Subjects: subject: Social and Information Networks (cs.SI)
subject: Cryptography and Security (cs.CR)
subject: FOS: Computer and information sciences

description: A modern binary executable is a composition of various networks. Control flow graphs are commonly used to represent an executable program in labeled datasets used for classification tasks. Control flow and term representations are widely adopted, but provide only a partial view of program semantics. This study is an empirical analysis of the networks composing malicious binaries in order to provide a complete representation of the structural properties of a program. This is accomplished by the measurement of structural properties of program networks in a malicious binary executable dataset. We demonstrate the presence of Scale-Free properties of network structure for program data dependency and control flow graphs, and show that data dependency graphs also have Small-World structural properties. We show that program data dependency graphs have a degree correlation that is structurally disassortative, and that control flow graphs have a neutral degree assortativity, indicating the use of random graphs to model the structural properties of program control flow graphs would show increased accuracy. By providing an increase in feature resolution within labeled datasets of executable programs we provide a quantitative basis to interpret the results of classifiers trained on CFG graph features. An increase in feature resolution allows for the structural properties of program classes to be analyzed for patterns as well as their component parts. By capturing a complete picture of program graphs we can enable theoretical solutions for the mapping a program's operational semantics to its structure.
description: 13 pages, 7 figures
Metallic nanowires: multi-shelled or filled ?
Creators: name: Bilalbegovic, G.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: The room temperature structure of aluminum, copper and gold infinite nanowires is studied. The molecular dynamics simulation method and the same type of the embedded atom potentials made by Voter and coworkers are used. It was found that multi-shelled and various filled metallic nanowires exist depending on the metal and the initial configuration. The results were compared with previous simulations for gold nanowires using different type of the potential.
description: 6 jpg figures
Quantum Mechanics with Random Imaginary Scalar Potential
Creators: name: Izyumov, A. V.
name: Simons, B. D.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: We study spectral properties of a non-Hermitian Hamiltonian describing a quantum particle propagating in a random imaginary scalar potential. Cast in the form of an effective field theory, we obtain an analytical expression for the ensemble averaged one-particle Green function from which we obtain the density of complex eigenvalues. Based on the connection between non-Hermitian quantum mechanics and the statistical mechanics of polymer chains, we determine the distribution function of a self-interacting polymer in dimensions $d>4$.
description: 10 pages, 1 eps figure
Associated Permutations of Complete Non-Ambiguous Trees
Creators: name: Chen, Daniel
name: Ohlig, Sebastian
Publisher: name: arXiv
Year: 2022
Subjects: subject: Combinatorics (math.CO)
subject: FOS: Mathematics

description: We explore new connections between complete non-ambiguous trees (CNATs) and permutations. We give a bijection between tree-like tableaux and a specific subset of CNATs. This map is used to establish and solve a recurrence relation for the number of tree-like tableaux of a fixed size without occupied corners, proving a conjecture by Laborde-Zubieta. We end by establishing a row/column swapping operation on CNATs and identify new areas for future research.
Charger-mediated energy transfer for quantum batteries: an open system approach
Creators: name: Farina, Donato
name: Andolina, Gian Marcello
name: Mari, Andrea
name: Polini, Marco
name: Giovannetti, Vittorio
Publisher: name: arXiv
Year: 2018
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: The energy charging of a quantum battery is analyzed in an open quantum setting, where the interaction between the battery element and the external power source is mediated by an ancilla system (the quantum charger) that acts as a controllable switch. Different implementations are analyzed putting emphasis on the interplay between coherent energy pumping mechanisms and thermalization.
Egret (GeV) Blazars
Creators: name: Mukherjee, R.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The EGRET instrument on the Compton Gamma Ray Observatory (1991-2000) has positively detected high energy gamma-ray emission from more than 67 active galaxies of the blazar class. The majority of the EGRET blazars are flat-spectrum radio quasars, which are characterized by inferred isotropic luminosities often as high as 3E49 ergs/s. The remainder are BL Lac objects, some of which have been detected at TeV energies (> 250 GeV) by ground-based atmospheric Cherenkov telescopes. One of the remarkable characteristics observed in blazars is that the gamma-ray luminosity often dominates the bolometric power in these sources. The detection of blazars by EGRET has undoubtedly been one of the highlights of the mission, and has forever impacted upon our understanding of the emission mechanisms in these objects. In this article, we summarize the properties of EGRET blazars, and review the constraints that the EGRET observations place on the various models of gamma-ray production in these sources.
description: Invited review paper, to appear in the proceedings of the International Symposium on High Energy Gamma-Ray Astronomy, Heidelberg, June 2000, AIP Conference Proc. 14 pages, 5 figures
Clarkcomanthus littoralis
Creators: name: Kogo, Ichizo
name: Fujita, Toshihiko
name: Kubodera, Tsunemi
Publisher: name: Zenodo
Year: 2019
Subjects: Biodiversity
Taxonomy
Animalia
Echinodermata
Crinoidea
Comatulida
Comatulidae
Clarkcomanthus
Clarkcomanthus littoralis

description: Clarkcomanthus littoralis (Carpenter, 1888)
 Actinometra littoralis Carpenter, 1888: 346, pl. 67 figs 1, 2.
 Clarkcomanthus littoralis — Rowe et al. 1986: 236, fig. 7c–f; Fabricius 1994: 1228 (table); Messing 1994: 239 (list); 1998b: 189 (table); 2007: 97; Rowe and Gates 1995: 141; Kogo 1998: 51, fig. 40; MarshallCrossland and Price 1999: 25; Pilcher and Messing 2001: 16 (table); Kirkendale and Messing 2003: 529; Kogo and Fujita 2005: 335; Summers et al. 2014: 336.
 Material examined. 19 specimens. Ambon Is. NSMT E-8169 (1 specimen), E-8180 (1), Eri, 10 m, December 4, 1992. Lombok Is. NSMT E-8199 (3), Gili Air I., February 3, 1994; NSMT E-8206 (1), E-8212 (1), E-8216 (1), E-8222 (1), E-8223 (1), E-8225 (2), E-8229 (1), E-8230 (1), E-8234 (1), E-8238 (1), Gili Air I., February 5, 1994; NSMT E-8251 (2), E-8254 (1), Kodek, February 15, 1994.
 Description. Centrodorsal small, discoidal, circular, pentagonal or stellate in aboral view, 2–3 mm across, up to 0.5 mm thick, with 0–12 cirrus sockets in 1 aligned row. Cirri absent or weak, if present, up to X, 11–13, 6– 8 mm long. Longest cirrals (4 th –6 th) about 1.5 times longer than wide; 2–3 most distal cirrals with a small aboral spine or tubercle. Radials narrowly exposed, in contact laterally. IBr 2: Ibr 1 oblong, in contact laterally; Ibr 2 (axil) triangular or low pentagonal, free laterally. IIBr and IIIBr 4(3+4) or 2. Arms 14– c. 50; anterior arms 85–130 mm, posterior arms 35–80mm long; first syzygy at br 3+4. PII longest, 14–26 mm long, of 36–48 segments; combs of 6–11 teeth confluent with outer edge of pinnulars; distal pinnulars often with secondary tooth. Pinnule combs to P 2.
 Distribution. Western, northern, and eastern Australia, Indonesia, Melanesia (Rowe et al. 1986); Sulu Sea (Messing 1998b, 2007); Great Barrier Reef (Fabricius 1994); Papua New Guinea (Messing 1994); Micronesia (Messing 1998b, 2007; Kirkendale and Messing 2003; Japan (Kogo 1998; Pilcher and Messing 2001; Kogo and Fujita 2005). Depth range: 1–144 m (Rowe et al. 1986).
description: Published as part of Kogo, Ichizo, Fujita, Toshihiko & Kubodera, Tsunemi, 2019, Shallow-water Comatulids (Echinodermata: Crinoidea) from Ambon and Lombok Islands, Indonesia, pp. 229-246 in Species Diversity 24 on page 235, DOI: 10.12782/specdiv.24.229, http://zenodo.org/record/5738323
Journal of Molecular and Cellular Cardiology 123 (2018) 185–197.pdf
Creators: name: Chen, Mu
name: Dongzhu Xu
name: Wu, Adonis Z.
name: Kranias, Evangelia G.
name: Shien-Fong Lin
name: Peng-Sheng Chen
name: Zhenhui Chen
Publisher: name: Health Research Alliance
Year: 2019
Subjects: subject: 60802 Animal Cell and Molecular Biology
subject: FOS: Biological sciences

description: publication.
Magnetization of ferrofluids with dipolar interactions - a Born--Mayer expansion
Creators: name: Huke, B.
name: Lücke, M.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: For ferrofluids that are described by a system of hard spheres interacting via dipolar forces we evaluate the magnetization as a function of the internal magnetic field with a Born--Mayer technique and an expansion in the dipolar coupling strength. Two different approximations are presented for the magnetization considering different contributions to a series expansion in terms of the volume fraction of the particles and the dipolar coupling strength.
description: 19 pages, 11 figures submitted to PRE
Constraining Metallicity-dependent Mixing and Extra Mixing using [C/N] in Alpha-Rich Field Giants
Creators: name: Shetrone, Matthew
name: Tayar, Jamie
name: Johnson, Jennifer A.
name: Somers, Garrett
name: Pinsonneault, Marc H.
name: Holtzman, Jon A.
name: Hasselquist, Sten
name: Masseron, Thomas
name: Meszaros, Szabolcs
name: Jonsson, Henrik
name: Hawkins, Keith
name: Sobeck, Jennifer
name: Zamora, Olga
name: Garcia-Hernandez, D. A.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Internal mixing on the giant branch is an important process which affects the evolution of stars and the chemical evolution of the galaxy. While several mechanisms have been proposed to explain this mixing, better empirical constraints are necessary. Here, we use [C/N] abundances in 26097 evolved stars from the SDSS-IV/APOGEE-2 Data Release 14 to trace mixing and extra mixing in old field giants with -1.7< [Fe/H] < 0.1. We show that the APOGEE [C/N] ratios before any dredge-up occurs are metallicity dependent, but that the change in [C/N] at the first dredge-up is metallicity independent for stars above [Fe/H] ~ -1. We identify the position of the red giant branch (RGB) bump as a function of metallicity, note that a metallicity-dependent extra mixing episode takes place for low-metallicity stars ([Fe/H]
Alloeocomatella pectinifera
Creators: name: Kogo, Ichizo
name: Fujita, Toshihiko
name: Kubodera, Tsunemi
Publisher: name: Zenodo
Year: 2019
Subjects: Biodiversity
Taxonomy
Animalia
Echinodermata
Crinoidea
Comatulida
Comatulidae
Alloeocomatella
Alloeocomatella pectinifera

description: Alloeocomatella pectinifera (A. H. Clark, 1911c)
 Comissia pectinifer A. H. Clark, 1911c: 644; 1912a: 78; 1913: 6; 1929: 636; 1931: 255, pl. 25 figs 69, 70.
 Comissia pectinifera —A. M. Clark and Spencer Davis 1966: 598 (list); A. M. Clark and Rowe 1971: 14 (key); Messing 1994: 239 (list).
 Comissia magnifica (not of Gislén, 1922)— Kogo 1998: 20, fig. 15.
 Alloeocomatella pectinifera — Messing 1995: 445, figs 3e–g, i, j, 5, 6; 1998b: 189 (table); 2001: 291; 2007: 99; MarshallCrossland and Price 1999: 25; Kogo 2002: 6; Kogo and Fujita 2005: 328.
 Material examined. 4 specimens. Ambon Is. NSMT E-8151 (1 specimen), Silale, 15 m, December 2, 1992; NSMT E-8167 (1), Silale, 15 m, December 3, 1992; NSMT E-8170 (1), Eri, 10 m, December 4, 1992. Lombok Is. NSMT E-8194 (1), Gili Air I., February 3, 1994.
 Description. Centrodorsal thin discoidal, roundish or pentagonal in aboral view, 4–7 mm across, 1–1.5 mm thick, with cirrus sockets in 2 irregular rows. Cirri XXXII (or wholly lost), 18–19, about 15 mm long. Longest cirrals (4 th – 7 th) about 2 times longer than wide; cirrals beyond 6 th with aboral spine. Radials wholly concealed by centrodorsal. IBr 2: Ibr 1 trapezoidal, free laterally, Ibr 2 (axil) low pentagonal. IIBr not present. Arms 10, 90–130 mm long; first syzygy at br 3+4. P 1 longest, 15–18 mm long, of 40–50 segments; combs of 22–33 teeth confluent with outer edge of pinnulars, excessively long, nearly a half of pinnule length. Pinnule combs to P 4.
 Distribution. Indonesia, Philippines (A. M. Clark and Rowe 1971); Maldives, northern Australia, Papua New Guinea, Micronesia, Melanesia (Messing 1995, 1998b); Sumatra (MarshallCrossland and Price 1999); Japan (Kogo 1998, 2002; Kogo and Fujita 2005). Depth range: 3–23 m (Messing 1995).
description: Published as part of Kogo, Ichizo, Fujita, Toshihiko & Kubodera, Tsunemi, 2019, Shallow-water Comatulids (Echinodermata: Crinoidea) from Ambon and Lombok Islands, Indonesia, pp. 229-246 in Species Diversity 24 on page 231, DOI: 10.12782/specdiv.24.229, http://zenodo.org/record/5738323
(Semi-)leptonic decays of D Mesons at BESIII
Creators: name: Yang, Youhua
Publisher: name: arXiv
Year: 2018
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Leptonic and semi-leptonic $D$ decays at BESIII contribute the most precise experimental measurement of $|V_{cs(d)}|$ and form factor $f_{D_{(s)}}$ in the world based on 2.93 fb$^{-1}$ and 3.19 fb$^{-1}$ data taken at center-of-mass energies $\sqrt{s} = 3.773$ and 4.180~GeV, respectively. The largest samples at the mass threshold of the charmed hardons $D_{(s)}$ also provide chances to extract form factors of some semi-electronic decays for the first time and together with the semi-muonic decays we could understand lepton flavour universality better.
description: The International Workshop on the CKM Unitarity Triangle (2018) is a well-established workshop series which provides a venue for theorists and experimentalists to discuss the latest developments in the area of quark flavour physics, and to come up with ideas for improved analyses. This proceeding contains 7 pages and 10 figures
Tracking-based distributed equilibrium seeking for aggregative games
Creators: name: Carnevale, Guido
name: Fabiani, Filippo
name: Fele, Filiberto
name: Margellos, Kostas
name: Notarstefano, Giuseppe
Publisher: name: arXiv
Year: 2022
Subjects: subject: Systems and Control (eess.SY)
subject: Computer Science and Game Theory (cs.GT)
subject: Optimization and Control (math.OC)
subject: FOS: Electrical engineering, electronic engineering, information engineering
subject: FOS: Computer and information sciences
subject: FOS: Mathematics

description: We propose fully-distributed algorithms for Nash equilibrium seeking in aggregative games over networks. We first consider the case where local constraints are present and we design an algorithm combining, for each agent, (i) the projected pseudo-gradient descent and (ii) a tracking mechanism to locally reconstruct the aggregative variable. To handle coupling constraints arising in generalized settings, we propose another distributed algorithm based on (i) a recently emerged augmented primal-dual scheme and (ii) two tracking mechanisms to reconstruct, for each agent, both the aggregative variable and the coupling constraint satisfaction. Leveraging tools from singular perturbations analysis, we prove linear convergence to the Nash equilibrium for both schemes. Finally, we run extensive numerical simulations to confirm the effectiveness of our methods and compare them with state-of-the-art distributed equilibrium-seeking algorithms.
Design of cycloidal rays in optical waveguides in analogy to the fastest descent problem
Creators: name: Hui, Xiong
name: He, Zijun
name: Liu, Yangjie
Publisher: name: arXiv
Year: 2022
Subjects: subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: In this work, we present the design of cycloidal waveguides from a gradient refractive index (GRIN) medium in analogy to the fastest descending problem in classical mechanics. Light rays propagate along cycloids in this medium, of which the refractive index can be determined from relating to the descending speed under gravity force. It can be used as GRIN lenses or waveguides, and the frequency specific focusing and imaging properties have been discussed. The results suggest that the waveguide can be viewed as an optical filter. Its frequency response characteristics change with the refractive index profile and the device geometries.
description: 6 pages, 6 figures
A Hybrid Approach to Joint Estimation of Channel and Antenna impedance
Creators: name: Wu, Shaohan
name: Hughes, Brian L.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Signal Processing (eess.SP)
subject: FOS: Electrical engineering, electronic engineering, information engineering

description: This paper considers a hybrid approach to joint estimation of channel information and antenna impedance, for single-input, single-output channels. Based on observation of training sequences via synchronously switched load at the receiver, we derive joint maximum a posteriori and maximum-likelihood (MAP/ML) estimators for channel and impedance over multiple packets. We investigate important properties of these estimators, e.g., bias and efficiency. We also explore the performance of these estimators through numerical examples.
description: 6 pages, two columns, 6 figures. References updated
Comment to the CPT-symmetric Universe: Two possible extensions
Creators: name: Volovik, G. E.
Publisher: name: arXiv
Year: 2019
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Other Condensed Matter (cond-mat.other)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: In Ref.1 (L. Boyle, K. Finn and N. Turok, CPT-Symmetric Universe, Phys. Rev. Lett. {\bf 121}, 251301 (2018)) the antispacetime Universe was suggested as the analytic continuation of our Universe across the Big Bang singularity in conformal time. We consider two different scenarios of analytic continuation. In one of them the analytic continuation is extended to the temperature of the system. This extension suggests that if such analytic continuation is valid, then it is possible that the initial stage of the evolution of the Universe on our side of the Big Bang was characterized by the negative temperature. In the second scenario, the analytic continuation is considered in the proper time. In this scenario the Big Bang represents the bifurcation point at which the $Z_2$ symmetry between the spacetime and antispacetime is spontaneously broken.
description: 2 pages, 1 figure, comment to PRL 121, 251301 (2018), accepted in JETP Letters
Clarkcomanthus mirabilis
Creators: name: Kogo, Ichizo
name: Fujita, Toshihiko
name: Kubodera, Tsunemi
Publisher: name: Zenodo
Year: 2019
Subjects: Biodiversity
Taxonomy
Animalia
Echinodermata
Crinoidea
Comatulida
Comatulidae
Clarkcomanthus
Clarkcomanthus mirabilis

description: Clarkcomanthus mirabilis   (Rowe, Hoggett, Birtles, and Vail, 1986)
 Comanthus mirabilis Rowe et al., 1986: 226, fig. 6B, C. Clarkcomanthus mirabilis — Summers et al. 2014: 336.
 Material examined. 1 specimen. Lombok Is. NSMT E-8232 (1 specimen), Gili Air I., February 5, 1994.
 Description. Centrodorsal small, stellate in aboral view, 3 mm across, reduced to level with radial-circlet, lacking cirrus sockets and cirri. Radials trapezoidal, 2 mm long, in contact laterally. IBr 2: Ibr 1 trapezoidal, in contact laterally; Ibr 2 (axil) pentagonal, free laterally. IIBr 4(3+4). IIIBr 2, rarely 4(3+4). Arms 39; anterior arms 110 mm, posterior arms 85 mm long; first syzygy at br 3+4. PII longest, 18 mm long, of 49 segments; combs of 12–14 teeth confluent with outer edge of pinnulars, some pinnulars with secondary tooth; most proximal tooth transverse. Pinnule combs to P 2, rarely to P 3 –P 9. Disc covered with many nodules.
 Distribution. Philippines, Papua New Guinea (Messing 1994); northern and eastern Australia, Indonesia, New Caledonia. Depth range: 3–18 m (Rowe et al. 1986).
description: Published as part of Kogo, Ichizo, Fujita, Toshihiko & Kubodera, Tsunemi, 2019, Shallow-water Comatulids (Echinodermata: Crinoidea) from Ambon and Lombok Islands, Indonesia, pp. 229-246 in Species Diversity 24 on page 235, DOI: 10.12782/specdiv.24.229, http://zenodo.org/record/5738323
Distribution Grid Monitoring Based on Widely Available Smart Plugs
Creators: name: Grafenhorst, Simon
name: Förderer, Kevin
name: Hagenmeyer, Veit
Publisher: name: arXiv
Year: 2022
Subjects: subject: Networking and Internet Architecture (cs.NI)
subject: FOS: Computer and information sciences
subject: H.4.3

description: The growing popularity of e-mobility, heat pumps, and renewable generation such as photovoltaics is leading to scenarios which the distribution grid was not originally designed for. Moreover, parts of the distribution grid are only sparsely instrumented, leaving the distribution system operator unaware of possible bottlenecks resulting from the introduction of such loads and renewable generation. To overcome this lack of information, we propose the use of widely available smart home devices, such as smart plugs, for grid monitoring. We detail the aggregation and storage of smart plug measurements for distribution grid monitoring and examine the accuracy of the measurements. A case study shows how the average monitoring error in a distribution grid area decreases the more measurement devices are installed. Hence, simple smart plugs can help with distribution grid monitoring and provide valuable information to the DSO.
description: 18 pages,
NEUMONIA ADQUIRIDA EN LA COMUNIDAD REVISIÓN DE TEMA BASADA EN GUÍAS PRACTICAS CLÍNICAS
Creators: name: Ortiz, Gillian Stefany Blanco
name: Pedroza, Jose Rubiano
Publisher: name: figshare
Year: 2019
Subjects: subject: 111712 Health Promotion
subject: FOS: Health sciences

description: La neumonía adquirida en la comunidad (NAC), en una patología caracterizada por un proceso infeccioso a nivel de parénquima pulmonar que puede ser activada por agentes o microorganismos, el cual es las partes distales del sistema respiratorio, produciendo una respuesta inflamatoria que puede haber A ser sistémica, manifestándose con algunas complicaciones como sepsis, choque séptico, disfunción orgánica e incluso la muerte. Cuando se presenta un caso de NAC, el organismo se trata de una respuesta ante los agentes patógenos, la producción de esta forma una serie de compuestos o sustancias un fin de erradicar el proceso y continuar en un estado basal no patológico. Al presentarse esta respuesta inmune, se origina una muestra de estadísticas, paraclínicas y / o radiológicas que son la parte fundamental para realizar un diagnóstico oportuno y preciso. Además de realizar una adecuada exploración de nuestro paciente, actualmente tenemos una serie de herramientas que nos facilitan la toma de decisiones en el lugar más oportuno para dar un tratamiento a estos pacientes, las escalas o los índices, las que forman parte del diario uso de todo medico al que le presenten estos casos. Es importante realizar un diagnóstico temprano,
Why energy democracy can enhance landscape democracy in the energy transition: some reflections on the Italian case
Creators: name: Picchi, Paolo
Publisher: name: Ri-Vista
Year: 2019

description: The energy transition towards renewable energy sources is unavoidable in order to reduce gas emissions by 40-70% within 2050 (Paris, 2015). In the last two decades, we assisted at frequent oppositions and block to the installation of renewable energy technologies by local communities, because of the associated landscape change. Local initiatives aiming at the 100% self-sufficiency can be a challenging approach for a sustainable energy transition, safeguarding bot the landscape democracy and the energy democracy. According to studies in sociology, the success of these bottom-up processes at community level depends on the socio-historical backgrounds and in the consequent capacity of acting in a cooperative perspective for the management of common goods. A special attention will be deserved to the Italian regional contexts. According to present literature, landscape architects are called to be facilitators for knowledge integration and reflections among different disciplines and backgrounds, this contribution want to address the role of research and practice in landscape architecture as facilitator, supporting communities in envisioning their own energy transition towards renewable energy.
description: Ri-Vista, Vol 16 No 2 (2018)
The temperature-mass relation in magnetized galaxy clusters
Creators: name: Dolag, Klaus
name: Evrard, August
name: Bartelmann, Matthias
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We use cosmological, magneto-hydrodynamic simulations of galaxy clusters to quantify the dynamical importance of magnetic fields in these clusters. The set-up of initial magnetic field strengths at high redshifts is chosen such that observed Faraday-rotation measurements in low-redshift clusters are well reproduced in the simulations. We compute the radial profiles of the intracluster gas temperature and of the thermal and magnetic pressure in a set of clusters simulated in the framework of an Einstein-de Sitter and a low-density, spatially-flat CDM cosmological model. We find that, for a realistic range of initial magnetic field strengths, the temperature of the intracluster gas changes by less than $\approx5%$.
description: Accepted for publication in A&A
Charge, Orbital and Magnetic Order in Nd0.5Ca0.5MnO3
Creators: name: millange, F.
name: de Brion, S.
name: Chouteau, G.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: In the manganite Nd0.5Ca0.5MnO3, charge ordering occurs at much higher temperature than the antiferromagnetic order (TCO=250K,TN=160K). The magnetic behavior of the phase TN
description: 17 pages, 11 Figures to appear in Phys. Rev. B
High-mass X-ray binaries and OB-runaway stars
Creators: name: Kaper, Lex
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: High-mass X-ray binaries (HMXBs) represent an important phase in the evolution of massive binary systems. HMXBs provide unique diagnostics to test massive-star evolution, to probe the physics of radiation-driven winds, to study the process of mass accretion, and to measure fundamental parameters of compact objects. As a consequence of the supernova explosion that produced the neutron star (or black hole) in these systems, HMXBs have high space velocities and thus are runaways. Alternatively, OB-runaway stars can be ejected from a cluster through dynamical interactions. Observations obtained with the Hipparcos satellite indicate that both scenarios are at work. Only for a minority of the OB runaways (and HMXBs) a wind bow shock has been detected. This might be explained by the varying local conditions of the interstellar medium.
description: 15 pages, latex (sty file included) with 5 embedded figures (one in jpg format), to appear in Proc. "Influence of binaries on stellar population studies", Eds. Vanbeveren, Van Rensbergen
Comatula pectinata
Creators: name: Kogo, Ichizo
name: Fujita, Toshihiko
name: Kubodera, Tsunemi
Publisher: name: Zenodo
Year: 2019
Subjects: Biodiversity
Taxonomy
Animalia
Echinodermata
Crinoidea
Comatulida
Comasteridae
Comatula
Comatula pectinata

description: Comatula pectinata (Linnaeus, 1758)
 Asterias pectinata Linnaeus, 1758: 663.
 Comatula pectinata —A. H. Clark 1909a: 394; 1909b: 148; 1931: 339, pl. 20 fig. 49, pl. 33 fig. 100, pl. 34 fig. 101, pl. 35 fig. 102, pl. 36 fig. 103, pl. 37 fig. 104, pl. 38 figs 105– 107; H. L. Clark 1915: 101; A. M. Clark and Rowe 1971: 14 (key); A. M. Clark 1972: 85; Gibbs et al. 1976: 110; Fabricius 1994: 1228 (table); Liao and A. M. Clark 1995: 28, fig. 13; Rowe and Gates 1995: 148; Kogo 1998: 23, fig. 17; 2002: 7; Lane et al. 2000: 476 (table).
 Comatula cf. pectinata — Messing and Tay 2016: 631, fig. 3D–F.
 Actinometra pectinata — Carpenter 1888: 284, pl. 53 figs 15– 22.
 Alecto purpurea Müller, 1843: 132.
 Comatula purpurea —A. H. Clark 1911a: 532; 1918: 271, pl. 14 fig. 16; 1931: 360, pl. 39 fig. 109, pl. 40 fig. 111, pl. 41 fig. 114.
 Material examined. 3 specimens. Ambon Is. NSMT E-8143 (1 specimen, juvenile), E-8147 (2), Latuhalat, 10 m, December 1, 1992.
 Description. Centrodorsal thin discoidal, 1–2.2 mm across, up to 0.6 mm thick, roundish in aboral view, with cirrus sockets in 1 aligned row. Cirri VII–VIII, 11–14, 5– 8 mm long. Longest cirrals (4 th –5 th) 1.2 times longer than wide; cirrals smooth without aboral tubercle. Radials narrowly exposed, in contact laterally. IBr 2(1+2): Ibr 1 trapezoidal, in contact laterally; Ibr 2 (axil) triangular, free laterally. IIBr not present. Arms 10; anterior arms 85 mm, posterior arms 50 mm long; first syzygy at br 1+2, second usually at br 3+4. P 1 longest, 7–8 mm long, of 30–32 segments; combs of 4–7 teeth confluent with outer edge of pinnulars. Pinnule combs to P 2.
 Remarks. Comatula purpurea (Müller, 1843) was synonymized with Comatula pectinata by Rowe and Gates (1995: 148). These two species had been distinguished mainly by the arrangement of cirri (A. H. Clark 1931: 320, in key): cirri are segregated in the interradial angles in the former species, while not in the latter. The specimens (NSMT E-8143 and E-8147) show both types of cirri arrangement. We agree the synonymization by Rowe and Gates (1995).
 Distribution. Singapore (Messing and Tay 2016); Indonesia, northern Australia, Philippines (A. M. Clark and Rowe 1971); Great Barrier Reef (Gibbs et al. 1976; Fabricius 1994); South China Sea (Lane et al. 2000). Depth range: 0–120 m (Lane et al. 2000).
description: Published as part of Kogo, Ichizo, Fujita, Toshihiko & Kubodera, Tsunemi, 2019, Shallow-water Comatulids (Echinodermata: Crinoidea) from Ambon and Lombok Islands, Indonesia, pp. 229-246 in Species Diversity 24 on pages 231-232, DOI: 10.12782/specdiv.24.229, http://zenodo.org/record/5738323
Anisotropic compact stars in f(T) gravity under Karmarkar condition
Creators: name: Deb, Debabrata
name: Ghosh, Shounak
name: Maurya, S. K.
name: Khlopov, Maxim
name: Ray, Saibal
Publisher: name: arXiv
Year: 2018
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: In this study, we present a generalized spherically symmetric, anisotropic and static compact stellar model in $f(T)$ gravity, where $T$ represents the torsion scalar. By employing the Karmarkar condition we have obtained embedding class 1 metric from the general spherically metric of class 2 and the solutions of the Einstein field equations (EFE) has been presented with the choice of suitable parametric values of $n$ under a simplified linear form of $f(T)$ gravity reads as $f(T)=A+BT$, where $A$ and $B$ are two constants. By matching the interior spacetime metric with the exterior Schwarzschild metric at the surface and considering the values of mass and radius of the compact stars we obtain the values of the unknown constants. We have presented further a detailed analysis of the physical acceptability and examined the stability of the stellar configuration by studying the energy conditions, generalized Tolman-Oppenheimer-Volkov (TOV) equation, Herrera cracking concept, adiabatic index, etc. In the investigation, we predict numerical values of the central density, surface density, central pressure, etc., in a tabular form taking different values of $n$ specifically for $LMC~X-4$, $Cen~X-3$ and $SMC~X-1$ as the representative of compact star candidates.
description: 20 pages, 11 figures, 4 tables
Frictional Mechanics of Wet Granular Material
Creators: name: Geminard, J. -C.
name: Losert, W.
name: Gollub, J. P.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: The mechanical response of a wet granular layer to imposed shear is studied experimentally at low applied normal stress. The granular material is immersed in water and the shear is applied by sliding a plate resting on the upper surface of the layer. We monitor simultaneously the horizontal and the vertical displacements of the plate to submicron accuracy with millisecond time resolution. The relations between the plate displacement, the dilation of the layer and the measured frictional force are analyzed in detail. When slip begins, the dilation increases exponentially over a slip distance comparable to the particle radius. We find that the total dilation and the steady state frictional force do not depend on the driving velocity, but do depend linearly on the applied normal stress. The frictional force also depends linearly on the dilation rate (rather than the dilation itself), and reaches a maximum value during the transient acceleration. We find that the layer can temporarily sustain a shear stress that is in excess of the critical value that will eventually lead to slip. We describe an empirical model that describes much of what we observe. This model differs in some respects from those used previously at stresses 10^6 times larger.
description: 17 pages, 15 figures, revised version, to appear in Phys. Rev. E, May 1999
Calculation of photoemission spectra of the doped Mott insulator La_{1-x}Sr_xTiO_3 using LDA+DMFT(QMC)
Creators: name: Nekrasov, I. A.
name: Held, K.
name: Blümer, N.
name: Poteryaev, A. I.
name: Anisimov, V. I.
name: Vollhardt, D.
Publisher: name: arXiv
Year: 2000
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: The spectral properties of La$_{1-x}$Sr$_{x}$TiO$_{3}$, a doped Mott insulator with strong Coulomb correlations, are calculated with the ab initio computational scheme LDA+DMFT(QMC). It starts from the non-interacting electronic band structure as calculated by the local density approximation (LDA), and introduces the missing correlations by the dynamical mean-field theory (DMFT), using numerically exact quantum Monte-Carlo (QMC) techniques to solve the resulting self-consistent multi-band single-impurity problem. The results of the LDA+DMFT(QMC) approach for the photoemission spectra of La$_{1-x}$Sr$_{x}$TiO$_{3}$ are in good agreement with experiment and represent a considerable qualitative and quantitative improvement on standard LDA calculations.
description: 6 pages, 4 figures
Comanthus gisleni Rowe, Hoggett, Birtles, and Vail 1986
Creators: name: Kogo, Ichizo
name: Fujita, Toshihiko
name: Kubodera, Tsunemi
Publisher: name: Zenodo
Year: 2019
Subjects: Biodiversity
Taxonomy
Animalia
Echinodermata
Crinoidea
Comatulida
Comasteridae
Comanthus
Comanthus gisleni

description: Comanthus gisleni Rowe, Hoggett, Birtles, and Vail, 1986
 Comanthus gisleni Rowe et al., 1986: 219, figs 4b, 5d; Vail 1987: 555; Fabricius 1994: 1228 (table); Messing 1994: 239 (list), 1998b: 189 (table); Rowe and Gates 1995: 144; Kogo 1998: 35, fig. 28; 2002: 10; MarshallCrossland and Price 1999: 26; Lane et al. 2000: 476 (table); Kogo and Fujita 2005: 332; Mekhova and Britayev 2012: 915, fig. 6; Summers et al. 2014: 337.
 Material examined. 1 specimen. Ambon Is. NSMT E-8179 (1 specimen), Eri, 10 m, December 4, 1992.
 Description. Centrodorsal thin discoidal, roundish in aboral view, 3 mm across, 0.3 mm thick, with cirrus sockets in 1 aligned row. Cirri XIV, including 2 rudimentary ones, 13– 14, 7– 8 mm long. Longest cirrals (5 th –6 th) 1.3 times longer than wide; cirrals beyond 7 th shorter than wide with blunt aboral crest. Radials trapezoidal, in contact laterally. IBr 2: Ibr 1 trapezoidal, in contact laterally at base; Ibr 2 (axil) low triangular, free laterally. IIBr 2, rarely 4(3+4). IIIBr 4(3+4), rarely 2. Arms 28, 65–85 mm long; first syzygy at br 3+4. PII longest, 14 mm long, of about 40 segments; combs of about 6 teeth confluent with outer edge of pinnulars; first comb tooth transverse. Pinnule combs to middle, often to distal pinnules. Middle pinnulars of distal pinnule fringed with small distal spines.
 Distribution. Sri Lanka, Sumatra (MarshallCrossland and Price 1999); southern Vietnam (Mekhova and Britayev 2012); Thailand, western, northern, and eastern Australia, Coral Sea, Melanesia (Rowe et al. 1986); Timor Sea (Rowe and Gates 1995); Borneo (Lane et al. 2000); Sulu Sea, Papua New Guinea (Messing 1994, 1998b); Great Barrier Reef (Vail 1987; Fabricius 1994); Japan (Rowe et al. 1986; Kogo 2002; Kogo and Fujita 2005). Depth range: 0–32 m (Rowe et al. 1986).
description: Published as part of Kogo, Ichizo, Fujita, Toshihiko & Kubodera, Tsunemi, 2019, Shallow-water Comatulids (Echinodermata: Crinoidea) from Ambon and Lombok Islands, Indonesia, pp. 229-246 in Species Diversity 24 on page 238, DOI: 10.12782/specdiv.24.229, http://zenodo.org/record/5738323
Bandgap Change of Carbon Nanotubes: Effect of Small Tensile and Torsional Strain
Creators: name: Yang, Liu
name: Anantram, M. P.
name: Han, Jie
name: Lu, J. P.
Publisher: name: arXiv
Year: 1998
Subjects: subject: Condensed Matter (cond-mat)
subject: FOS: Physical sciences

description: We use a simple picture based on the $π$ electron approximation to study the bandgap variation of carbon nanotubes with uniaxial and torsional strain. We find (i) that the magnitude of slope of bandgap versus strain has an almost universal behaviour that depends on the chiral angle, (ii) that the sign of slope depends on the value of $(n-m) \bmod 3$ and (iii) a novel change in sign of the slope of bandgap versus uniaxial strain arising from a change in the value of the quantum number corresponding to the minimum bandgap. Four orbital calculations are also presented to show that the $π$ orbital results are valid.
description: Revised. Method explained in detail
Intermediate State in Type I superconducting sphere: pinning and size effect
Creators: name: Shapiro, I.
name: Shapiro, B. Ya.
Publisher: name: arXiv
Year: 2018
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: Simulations, based on the time dependent Ginzburg-Landau equations, show that the magnetization and spatial structure of the intermediate state strongly affected both by the radius of the sphere and by pinning center concentration. The intermediate states undergoes transformation from one-domain state in small clean sphere to multi-domain structure in big spheres. In spheres where part of the superconducting material replaced by the 0.5% randomly distributed normal phase (dirty case) the intermediate state demonstrates a well pronounced turbulence behavior.
description: 14 pages, 11 figures
Detection by high-throughput sequencing and molecular characterization of complexes of fabaviruses infecting ‘Staccato(R)’ sweet cherry (Prunus avium) in Canada
Creators: name: James, Delano
name: DELANO JAMES
name: Phelan, James
name: JAMES PHELAN
name: Sanderson, Daniel
name: DANIEL SANDERSON
Publisher: name: Taylor & Francis
Year: 2019
Subjects: subject: Biochemistry
subject: Space Science
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Molecular Biology
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: 60506 Virology

description: High throughput sequencing (HTS) revealed the existence of complexes of fabaviruses infecting two ‘Staccato(R) ’ sweet cherry plants (Prunus avium). Species classified as members of the genus Fabavirus are positive sense RNA viruses that possess bipartite genomes. The cherry plants Stac-3B (symptomatic) and Stac-4B (asymptomatic) were each determined to be infected with multiple RNA1 and RNA2 segments of Prunus virus F (PrVF) and the putative cherry virus F (CVF). The RNA1 and RNA2 segments Stac-3B_C3 and Stac-3B_c11, respectively, are proposed to represent an isolate identified as PrVF-CP1; while the RNA1 and RNA2 segments Stac-3B_C4 and Stac-3B_c7 are proposed to represent an isolate CVF-CC1. The termini of these four RNA segments were confirmed by RACE revealing that the first 28 nucleotides of the 5ʹuntranslated region (UTR) of all four RNA segments is conserved and is predicted to form a hairpin structure. The 3ʹUTRs possess various repeat sequences. Very interestingly, a group of PrVF sequences, exemplified by SwC 74_2c, were identified as the products of an interspecies recombination event, with PrVF 8816_s1 as a possible major parent and an isolate of CVF being the minor parent. This was supported by all methods in the RDP4 program. No association was made of any of the fabavirus complexes with any disease symptoms. This is the first description of the detection of CVF in Canada.
Clarkcomanthus alternans
Creators: name: Kogo, Ichizo
name: Fujita, Toshihiko
name: Kubodera, Tsunemi
Publisher: name: Zenodo
Year: 2019
Subjects: Biodiversity
Taxonomy
Animalia
Echinodermata
Crinoidea
Comatulida
Comatulidae
Clarkcomanthus
Clarkcomanthus alternans

description: Clarkcomanthus alternans (Carpenter, 1881)
 Actinometra alternans Carpenter, 1881: 208; 1888: 330 (key).
 Comantheria alternans —A. H. Clark 1912a: 90; 1913: 13; 1931: 488; Reichensperger 1913: 87.
 Comanthus alternans —A. H. Clark 1908c: 206; H. L. Clark 1915: 101; 1921: 16; Rowe et al. 1986: 224, fig. 6a; Fabricius 1994: 1228; Messing 1994: 239 (list); 1998b: 189 (table); 2007: 97; Rowe and Gates 1995: 143; Kogo 1998: 33, fig. 26; 2002: 9; Lane et al. 2000: 476 (table); Kirkendale and Messing 2003: 530; Kogo and Fujita 2005: 332; Mekhova and Britayev 2012: 915.
 Clarkcomanthus alternans — Summers et al. 2014: 336.
 Material examined. 8 specimens. Ambon Is. NSMT E-8110 (1 specimen), Pombo I., lagoon, November 27, 1992; NSMT E-8114 (1), Pombo I., 10 m, November 28, 1992. Lombok Is. NSMT E-8197 (1), Gili Air I., February 3, 1994; NSMT E-8242 (1), Gili Air I., February 5, 1994; NSMT E-8255 (2), E-8256 (1), E-8260 (1), Kodek, February 15, 1994.
 Description. Centrodorsal thin, small, pentagonal or stellate in aboral view, 2.5–3.5 mm across, up to 0.4 mm thick, lacking cirrus sockets and cirri. Radials trapezoidal, in contact laterally. IBr 2: Ibr 1 oblong, in contact laterally; Ibr 2 (axil) low pentagonal, free laterally. IIBr 4(3+4). IIIBr 2, rarely 4(3+4); outer brachials twisted outward. IVBr and VBr 4(3+4). Arms 48–122, 60– 100 mm long; first syzygy at br 3+4. PII longest, 9–16 mm long, of 32–44 segments; combs of 6–10 teeth confluent with outer edge of pinnulars; 2–3 distal pinnulars with small secondary tooth. Pinnule combs to P 4, rarely to P 5 –P 7.
 Distribution. Southern Vietnam (Mekhova and Britayev 2012); western, northern and eastern Australia, Indonesia, New Guinea, New Caledonia, Philippines (Rowe et al. 1986); Sulu Sea, Papua New Guinea, Micronesia (Messing 1994, 1998b, 2007; Kirkendale and Messing 2003); South China Sea (Lane et al. 2000); Japan (Rowe et al. 1986; Kogo 1998, 2002; Kogo and Fujita 2005). Depth range: 0–90 m (Lane et al. 2000).
description: Published as part of Kogo, Ichizo, Fujita, Toshihiko & Kubodera, Tsunemi, 2019, Shallow-water Comatulids (Echinodermata: Crinoidea) from Ambon and Lombok Islands, Indonesia, pp. 229-246 in Species Diversity 24 on page 235, DOI: 10.12782/specdiv.24.229, http://zenodo.org/record/5738323