cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Tineobius (Tineobius) indicus Lucian Fusu & Antoni Ribes 2017, stat. nov.
Creators: name: Lucian Fusu
name: Antoni Ribes
Publisher: name: Zenodo
Year: 2017
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Eupelmidae
Tineobius
Tineobius indicus

description: 17. Tineobius (Tineobius) indicus (Ferrière, 1938) stat. nov. [new subgeneric status]
Anastatoidea indica Ferrière, 1938: 49–50, 58, fg. 6.
Holotype ♀, unique specimen (BMNH type no. 5.937, examined by LF). Type locality: India [now Pakistan]: Punjab, Lyallpur.
Anastatoïdea indica – Risbec 1952: 66 (keyed).
Tineobius indicus – Bouček 1988: 565.
description: Published as part of Lucian Fusu & Antoni Ribes, 2017, Description of the first Palaearctic species of Tineobius Ashmead, 1896 with DNA data, a checklist of world species, and nomenclatural changes in Eupelmidae (Hymenoptera, Chalcidoidea), pp. 1-19 in European Journal of Taxonomy 263 on page 13, DOI: 10.5852/ejt.2017.263, http://zenodo.org/record/889169
Nuclear astrophysics researches in an ion trap apparatus
Creators: name: Donets, E. D.
name: Donets, E. E.
name: Itahashi, T.
name: Kudomi, N.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: At low energies, far below Coulumb barrier, fusion nuclear reactions are very sensitive to its shape, which is usually in experiments modified by atomic electrons of targer or both projectile and target particles. This article describes proposal on construction of an installation and measurements of excitation functions for d(d,p)t reaction in the region 1.5
description: 12 pages, 2 figures
Exact Chromatic Polynomials for Toroidal Chains of Complete Graphs
Creators: name: Chang, Shu-Chiuan
Publisher: name: arXiv
Year: 2001
Subjects: subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: We present exact calculations of the partition function of the zero-temperature Potts antiferromagnet (equivalently, the chromatic polynomial) for graphs of arbitrarily great length composed of repeated complete subgraphs $K_b$ with $b=5,6$ which have periodic or twisted periodic boundary condition in the longitudinal direction. In the $L_x \to \infty$ limit, the continuous accumulation set of the chromatic zeros ${\cal B}$ is determined. We give some results for arbitrary $b$ including the extrema of the eigenvalues with coefficients of degree $b-1$ and the explicit forms of some classes of eigenvalues. We prove that the maximal point where ${\cal B}$ crosses the real axis, $q_c$, satisfies the inequality $q_c \le b$ for $2 \le b$, the minimum value of $q$ at which ${\cal B}$ crosses the real $q$ axis is $q=0$, and we make a conjecture concerning the structure of the chromatic polynomial for Klein bottle strips.
description: 36 pages, latex, 2 postscript figures included
Classical spiral spin liquids as a possible route to quantum spin liquids
Creators: name: Niggemann, Nils
name: Hering, Max
name: Reuther, Johannes
Publisher: name: arXiv
Year: 2019
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: Quantum spin liquids are long-range entangled phases whose magnetic correlations are determined by strong quantum fluctuations. While an overarching principle specifying the precise microscopic coupling scenarios for which quantum spin-liquid behavior arises is unknown, it is well-established that they are preferably found in spin systems where the corresponding classical limit of spin magnitudes $S\rightarrow\infty$ exhibits a macroscopic ground state degeneracy, so-called classical spin liquids. Spiral spin liquids represent a special family of classical spin liquids where degenerate manifolds of spin spirals form closed contours or surfaces in momentum space. Here, we investigate the potential of spiral spin liquids to evoke quantum spin-liquid behavior when the spin magnitude is tuned from the classical $S\rightarrow\infty$ limit to the quantum $S=1/2$ case. To this end, we first use the Luttinger-Tisza method to formulate a general scheme which allows one to construct new spiral spin liquids based on bipartite lattices. We apply this approach to the two-dimensional square lattice and the three-dimensional hcp lattice to design classical spiral spin-liquid phases which have not been previously studied. By employing the pseudofermion functional renormalization group (PFFRG) technique we investigate the effects of quantum fluctuations when the classical spins are replaced by quantum $S=1/2$ spins. We indeed find that extended spiral spin-liquid regimes change into paramagnetic quantum phases possibly realizing quantum spin liquids. Remnants of the degenerate spiral surfaces are still discernible in the momentum-resolved susceptibility, even in the quantum $S=1/2$ case. In total, this corroborates the potential of classical spiral spin liquids to induce more complex non-magnetic quantum phases.
description: 11 pages, 6 figures
Classifications of the Host Galaxies of Supernovae
Creators: name: Bergh, Sidney van den
name: Li, Weidong
name: Filippenko, Alexei V.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Classifications on the DDO system are given for the host galaxies of 177 supernovae (SNe) that have been discovered since 1997 during the course of the Lick Observatory Supernova Search with the Katzman Automatic Imaging Telescope. Whereas SNe Ia occur in all galaxy types, it is found, at a high level of statistical confidence, that SNe Ib, Ic, and II are strongly concentrated in late-type galaxies. However, attention is drawn to a possible exception provided by SN 2001I. This SN IIn occurred in the E2 galaxy UGC 2836, which was not expected to harbor a massive young supernova progenitor.
description: Accepted to be published in PASP
Ferinestrix Bjork 1970
Creators: name: Wolsan, Mieczyslaw
name: Sotnikova, Marina
Publisher: name: Zenodo
Year: 2013
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Carnivora
Mustelidae
Ferinestrix

description: GENUS FERINESTRIX BJORK, 1970
 Ferinestrix – Bjork, 1970: 19.
 Ferinestris – Kalmykov & Maschenko, 2007: 182 (incorrect subsequent spelling); Maschenko, Takai & Kalmykov, 2007: 204 (incorrect subsequent spelling).
 Firenestrix – Sotnikova, 2008a: 298 (incorrect subsequent spelling).
 Etymology: Derived from the Latin ferina meaning ‘flesh of wild animals’ and estrix meaning ‘eater’; feminine in gender.
 Revised diagnosis: Stem melines differing from all other taxa of the total clade of Melinae in the following features: body size larger; facial and palatal skull region rostrocaudally shorter relative to its transverse breadth; P2, P3, M1, and p2–p4 mesiodistally shorter relative to their vestibulolingual widths; m1 talonid smaller relative to the trigonid.
 Type species: Ferinestrix vorax Bjork, 1970. Referred species: Ferinestrix rapax sp. nov.
 Phylogenetic relationships: Phylogenetic analysis recovered Ferinestrix as closely related to Arctomeles, Arctonyx, and Meles to the exclusion of Melodon (Fig. 2).
description: Published as part of Wolsan, Mieczyslaw & Sotnikova, Marina, 2013, Systematics, evolution, and biogeography of the Pliocene stem meline badger Ferinestrix (Carnivora: Mustelidae), pp. 208-226 in Zoological Journal of the Linnean Society 167 (1) on pages 212-213, DOI: 10.1111/j.1096-3642.2012.00868.x, http://zenodo.org/record/5292120
Accessible tourism services in the North Great Plain region
Creators: name: Tatár, András
name: Puskás, Andrea
name: Biró, Melinda
name: Pucsok, József Márton
name: Hidvégi, Péter
Publisher: name: Debreceni Egyetem
Year: 2019

description: Különleges Bánásmód, vol. 5. issue 1. ISSN 2498-5368
Tineobius (Tineobius) lamborni Lucian Fusu & Antoni Ribes 2017, comb. nov.
Creators: name: Lucian Fusu
name: Antoni Ribes
Publisher: name: Zenodo
Year: 2017
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Eupelmidae
Tineobius
Tineobius lamborni

description: 18. Tineobius (Tineobius) lamborni (Ferrière, 1938) comb. nov.
Anastatoidea lamborni Ferrière, 1938: 56, 58.
Holotype ♀, unique specimen (BMNH type no. 5.947, examined by LF). Type locality: East Africa: Nyasaland, Kota-kotu.
Anastatoïdea lamborni – Risbec 1952: 67 (keyed).
description: Published as part of Lucian Fusu & Antoni Ribes, 2017, Description of the first Palaearctic species of Tineobius Ashmead, 1896 with DNA data, a checklist of world species, and nomenclatural changes in Eupelmidae (Hymenoptera, Chalcidoidea), pp. 1-19 in European Journal of Taxonomy 263 on page 13, DOI: 10.5852/ejt.2017.263, http://zenodo.org/record/889169
Semantic Preserving Bijective Mappings for Expressions involving Special Functions in Computer Algebra Systems and Document Preparation Systems
Creators: name: Greiner-Petter, Andre
name: Schubotz, Moritz
name: Cohl, Howard S.
name: Gipp, Bela
Publisher: name: arXiv
Year: 2019
Subjects: subject: Digital Libraries (cs.DL)
subject: Symbolic Computation (cs.SC)
subject: FOS: Computer and information sciences

description: Purpose: Modern mathematicians and scientists of math-related disciplines often use Document Preparation Systems (DPS) to write and Computer Algebra Systems (CAS) to calculate mathematical expressions. Usually, they translate the expressions manually between DPS and CAS. This process is time-consuming and error-prone. Our goal is to automate this translation. This paper uses Maple and Mathematica as the CAS, and LaTeX as our DPS. Design/methodology/approach: Bruce Miller at the National Institute of Standards and Technology (NIST) developed a collection of special LaTeX macros that create links from mathematical symbols to their definitions in the NIST Digital Library of Mathematical Functions (DLMF). We are using these macros to perform rule-based translations between the formulae in the DLMF and CAS. Moreover, we develop software to ease the creation of new rules and to discover inconsistencies. Findings: We created 396 mappings and translated 58.8% of DLMF formulae (2,405 expressions) successfully between Maple and DLMF. For a significant percentage, the special function definitions in Maple and the DLMF were different. Therefore, an atomic symbol in one system maps to a composite expression in the other system. The translator was also successfully used for automatic verification of mathematical online compendia and CAS. Our evaluation techniques discovered two errors in the DLMF and one defect in Maple. Originality: This paper introduces the first translation tool for special functions between LaTeX and CAS. The approach improves error-prone manual translations and can be used to verify mathematical online compendia and CAS.
description: This work was supported by the German Research Foundation (DFG, grant GI-1259-1)
Mass-Metallicity Relation for the Local Group Dwarf Spheroidal Galaxies: A New Picture for the Chemical Enrichment of Galaxies in the Lowest Mass Range
Creators: name: Tamura, Naoyuki
name: Hirashita, Hiroyuki
name: Takeuchi, Tsutomu T.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The virial mass ($M_{\rm vir}$)-metallicity relation among the Local Group dwarf spheroidal galaxies (dSphs) is examined. Hirashita, Takeuchi, & Tamura showed that the dSphs can be divided into two distinct classes with respect to the relation between their virial masses and luminosities: low-mass ($M_{\rm vir} \la 10^8 M_\odot$) and high-mass ($M_{\rm vir} \ga 10^8 M_\odot$) groups. We see that both the mass-metallicity and the mass-luminosity relations of the high-mass dSphs are understood as a low-mass extension of giant ellipticals. On the contrary, we find that the classical galactic-wind model is problematic to apply to the low-mass dSphs, whose low binding energy is comparable to that released by several supernova explosions. A strongly regulated star formation in their formation phase is required to reproduce their observed metallicity. Such regulation is naturally expected in a gas cloud with the primordial elemental abundance according to Nishi & Tashiro. A significant scatter in the mass-metallicity relation for the low-mass dSphs is also successfully explained along with the scenario of Hirashita and coworkers. We not only propose a new picture for a chemical enrichment of the dSphs, but also suggest that the mass-metallicity and the mass-luminosity relations be understood in a consistent context.
description: 14 pages LaTeX, 1 PostScript figure, to appear in ApJ Letter
Linking and causality in (2+1)-dimensional static spacetimes
Creators: name: Natario, Jose
Publisher: name: arXiv
Year: 2001
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: Given a (d+1)-dimensional spacetime (M,g), one can consider the set N of all its null geodesics. If (M,g) is globally hyperbolic then this set is naturally a smooth (2d-1)-manifold. The sky of an event x in M is the set X of all null geodesics through x, and is an embedded submanifold of N diffeomorphic to S^{d-1}. Low conjectured that if d=2 then x,y are causally related in M iff X,Y are linked in N. We prove Low's conjecture for a (large) class of static spacetimes.
description: 13 pages, 3 figures; typos corrected, 2 figures added
Tineobius (Tineobius) longfellowi Lucian Fusu & Antoni Ribes 2017, stat. nov.
Creators: name: Lucian Fusu
name: Antoni Ribes
Publisher: name: Zenodo
Year: 2017
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Eupelmidae
Tineobius
Tineobius longfellowi

description: 19. Tineobius (Tineobius) longfellowi (Girault, 1923) stat. nov. [new subgeneric status]
Metapelma longfellowi Girault, 1923: 99.
Holotype ♀, unique specimen (QMBA T.4209, not examined). Type locality: Australia: Kuranda.
Metapelma longfellowi – Girault 1926: 64. — Girault 1930a: 3 (compared with M. beenleighi). — Dahms 1984: 764 (type information).
Anastatoidea longfellowi – Gahan 1927: 15 (keyed). — Ferrière 1938: 45, 57 (keyed). — Risbec 1952: 67 (catalogued).
Tineobius longfellowi – Bouček 1988: 565.
description: Published as part of Lucian Fusu & Antoni Ribes, 2017, Description of the first Palaearctic species of Tineobius Ashmead, 1896 with DNA data, a checklist of world species, and nomenclatural changes in Eupelmidae (Hymenoptera, Chalcidoidea), pp. 1-19 in European Journal of Taxonomy 263 on page 13, DOI: 10.5852/ejt.2017.263, http://zenodo.org/record/889169
Ferinestrix vorax Bjork 1970
Creators: name: Wolsan, Mieczyslaw
name: Sotnikova, Marina
Publisher: name: Zenodo
Year: 2013
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Mammalia
Carnivora
Mustelidae
Ferinestrix
Ferinestrix vorax

description: FERINESTRIX VORAX BJORK, 1970 (FIG. 3)
 Ferinestrix vorax – Bjork, 1970: 19–21, 48, 49, 51, fig. 11; Galbreath, 1972: 786; Hibbard, 1972: 128; Kurtén & Anderson, 1980: 155; Anderson, 1984: 258, 261; McDonald, Link & Lee, 1996: 42; Baskin, 1998: 164; Ruez, 2005: 107 A; Sotnikova, 2006: 84; Ogino et al., 2007: 125 A; Ruez, 2009a: 70; Ruez, 2009b: 2, 49, 112; Matishov & Kalmykov, 2011a: 819, 821; Matishov & Kalmykov, 2011b: 1467, 1469.
 Etymology: Derived from the Latin vorax meaning ‘voracious’.
 Revised diagnosis: Differs from Ferinestrix rapax in the following features: condyloid and angular processes of the dentary situated more ventrally (condy- loid process is at the level of the m1 crown; angular process is ventral to the level of the m1 crown); mental foramina closer to each other and located more rostrally (caudal mental foramen is in front of p4); space between c1 and p4 relatively smaller (shortest distance between the alveolar rims of c1 and p4 is smaller than the mesiodistal length of the p4 crown); lower cheek-tooth series more arcuate; lingual wall of the m1 talonid higher with a series of larger elevations relative to the vestibular wall; m1 hypoconulid smaller and positioned more basally relative to the hypoconid; m2 placed more ventrally relative to m1.
 Holotype: UMMP 53343, an incomplete right dentary with p4, partial m1, and m2 (Fig. 3).
 Type locality: Hagerman Fossil Beds National Monument (HAFO) locality 63 [University of Michigan Museum of Paleontology Idaho locality (UM-Ida) 1-65], Glenns Ferry Formation, HAFO, near the town of Hagerman, Idaho, USA (Bjork, 1970; Ruez, 2009a).
 Referred specimen: Bjork (1970) referred to this species a femur, UMMP 49941, collected from the HAFO locality 153 (UM-Ida 76-64). As this specimen was not associated with the holotype and no other femur referable to Ferinestrix is known, this referral is disputable.
 Distribution and age: Known only from the HAFO localities 63 (holotype) and 153 (referred femur). Approximate ages for these localities are 3.2 and 3.6 Mya, respectively, both within Blancan III, Pliocene (Ruez, 2009a).
 Description: The morphological characteristics and size of the holotype dentary and lower teeth are similar to or within the range of variation of those in Ferinestrix rapax except for the features indicated in the revised diagnosis (compare Fig. 3 with Figs 4–6; see Tables 3, 4). For a detailed description of the holotype and referred femur, see Bjork (1970).
description: Published as part of Wolsan, Mieczyslaw & Sotnikova, Marina, 2013, Systematics, evolution, and biogeography of the Pliocene stem meline badger Ferinestrix (Carnivora: Mustelidae), pp. 208-226 in Zoological Journal of the Linnean Society 167 (1) on page 213, DOI: 10.1111/j.1096-3642.2012.00868.x, http://zenodo.org/record/5292120
A Real-Time, All-Sky, High Time Resolution, Direct Imager for the Long Wavelength Array
Creators: name: Kent, James
name: Dowell, Jayce
name: Beardsley, Adam
name: Thyagarjan, Nithyanandan
name: Taylor, Greg
name: Bowman, Judd
Publisher: name: arXiv
Year: 2019
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: The future of radio astronomy will require instruments with large collecting areas for higher sensitivity, wide fields of view for faster survey speeds, and efficient computing and data rates relative to current capabilities. We describe the first successful deployment of the E-field Parallel Imaging Correlator (EPIC) on the LWA station in Sevilleta, New Mexico, USA (LWA-SV). EPIC is a solution to the computational problem of large interferometers. By gridding and spatially Fourier transforming channelised electric fields from the antennas in real-time, EPIC removes the explicit cross multiplication of all pairs of antenna voltages to synthesize an aperture, reducing the computational scaling from $\mathcal{O}(n_a^2)$ to $\mathcal{O}(n_g \log_2 n_g)$, where $n_a$ is the number of antennas and $n_g$ is the number of grid points. Not only does this save computational costs for dense arrays but it produces very high time resolution images in real time. The GPU-based implementation uses existing LWA-SV hardware and the high performance streaming framework, Bifrost. We examine the practical details of the EPIC deployment and verify the imaging performance by detecting a meteor impact on the atmosphere using continuous all-sky imaging at 50 ms time resolution.
description: 10 pages
title: CERN Yellow Reports: Monographs, Vol 2 (2019): A Facility for Tumour Therapy and Biomedical Research in South-Eastern Europe
title: A Facility for Tumour Therapy and Biomedical Research in South-Eastern Europe
titleType: AlternativeTitle
Creators: name: CERN
Publisher: name: CERN
Year: 2019

description: In 2016 the South East European International Institute for Sustainable Technologies (SEEIIST) was proposed by Herwig Schopper and brought to the political level by Sanja Damjanovic, Minister of Science of Montenegro. In this framework two design studies have been completed by two groups of European experts: a "4th Generation Synchrotron Light Source for Science and Technology" (SRL) and a "Facility for Tumour Hadron Therapy and Biomedical Research" (HTR). A preliminary report was presented and discussed at the Workshop on "New International Research Facilities for South East Europe" held in January 2017 at ICTP (Trieste). In March 2018 the Steering Committee came unanimously to the conclusion that the first facility to be built should be the HTR. This report contains the HTR study, which was completed in July 2018; the Executive Summary has been written for the readers who are not interested in the details.
A New Way of Visualizing Quantum Fields
Creators: name: Linde, Helmut
Publisher: name: arXiv
Year: 2019
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Quantum Field Theory (QFT) is the basis of some of the most fundamental theories in modern physics, but it is not an easy subject to learn. In the present article we intend to pave the way from quantum mechanics to QFT for students at early graduate or advanced undergraduate level. More specifically, we propose a new way of visualizing the wave function $Ψ$ of a linear chain of interacting quantum harmonic oscillators, which can be seen as a model for a simple one-dimensional bosonic quantum field. The main idea is to draw randomly chosen classical states of the chain superimposed upon each other and use a \BW{gray}\color{color} scale to represent the value of $Ψ$ at the corresponding coordinates of the quantized system. Our goal is to establish a better intuitive understanding of the mathematical objects underlying quantum field theories and solid state physics.
description: This is an author-created, un-copyedited version of an article accepted for publication/published in European Journal of Physics. IOP Publishing Ltd is not responsible for any errors or omissions in this version of the manuscript or any version derived from it. The Version of Record is available online at https://doi.org/10.1088/1361-6404/aaa032
SO(5) structure of p-wave superconductivity for spin-dipole interaction model
Creators: name: Zhang, Hong-Biao
name: Ge, Mo-Lin
name: Xue, Kang
Publisher: name: arXiv
Year: 2001
Subjects: subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: A closed SO(5) algebraic structure in the the mean-field form of the Hamiltonian the pure p-wave superconductivity is found that can help to diagonalized by making use of the Bogoliubov rotation instead of the Balian-Werthamer approach. we point out that the eigenstate is nothing but SO(5)-coherent state with fermionic realization. By applying the approach to the Hamiltonian with dipole interaction of Leggett the consistency between the diagonalization and gap equation is proved through the double-time Green function. The relationship between the s-wave and p-wave superconductivities turns out to be recognized through Yangian algebra, a new type of infinite-dimensional algebra.
description: 7 pages, no figures. Accepted Journal of Physcis A: Mathematical and General
Thermal Hall signatures of non-Kitaev spin liquids in honeycomb Kitaev materials
Creators: name: Gao, Yong Hao
name: Hickey, Ciarán
name: Xiang, Tao
name: Trebst, Simon
name: Chen, Gang
Publisher: name: arXiv
Year: 2019
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences
subject: https://arxiv.org/a/chen_g_4.html

description: Motivated by the recent surge of field-driven phenomena discussed for Kitaev materials, in particular the experimental observation of a finite thermal Hall effect and theoretical proposals for the emergence of additional spin liquid phases beyond the conventional Kitaev spin liquid, we develop a theoretical understanding of the thermal Hall effect in honeycomb Kitaev materials in magnetic fields. Our focus is on gapless U(1) spin liquids with a spinon Fermi surface, which have been shown to arise as field-induced phases. We demonstrate that in the presence of symmetry-allowed, second-neighbor Dzyaloshinskii-Moriya interactions these spin liquids give rise to a finite, non-quantized, thermal Hall conductance in a magnetic field. The microscopic origin of this thermal Hall effect can be traced back to an interplay of Dzyaloshinskii-Moriya interaction and Zeeman coupling, which generates an internal U(1) gauge flux that twists the motion of the emergent spinons. We argue that such a non-quantized thermal Hall effect is a generic response in Kitaev models for a range of couplings.
description: 8+4 pages, 8+1 figures
Magnetorotational Instability in Liquid Metal Couette Flow
Creators: name: Noguchi, K.
name: Pariev, V. I.
name: Colgate, S. A.
name: Nordhaus, J.
name: Beckley, H. F.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Despite the importance of the magnetorotational instability (MRI) as a fundamental mechanism for angular momentum transport in magnetized accretion disks, it has yet to be demonstrated in the laboratory. A liquid sodium alpha-omega dynamo experiment at the New Mexico Institute of Mining and Technology provides an ideal environment to study the MRI in a rotating metal annulus (Couette flow). A local stability analysis is performed as a function of shear, magnetic field strength, magnetic Reynolds number, and turbulent Prandtl number. The later takes into account the minimum turbulence induced by the formation of an Ekman layer against the rigidly rotating end walls of a cylindrical vessel. Stability conditions are presented and unstable conditions for the sodium experiment are compared with another proposed MRI experiment with liquid gallium. Due to the relatively large magnetic Reynolds number achievable in the sodium experiment, it should be possible to observe the excitation of the MRI for a wide range of wavenumbers and further to observe the transition to the turbulent state.
description: 12 pages, 22 figures, 1 table. To appear in the Astrophysical Journal
MOESM5 of De novo transcriptome sequencing and analysis revealed the molecular basis of rapid fat accumulation by black soldier fly (Hermetia illucens, L.) for development of insectival biodiesel
Creators: name: Zhaolu Zhu
name: Rehman, Kashif Ur
name: Yongqiang Yu
name: Liu, Xiu
name: Wang, Hui
name: Tomberlin, Jeffery
name: Sing-Hoi Sze
name: Minmin Cai
name: Jibin Zhang
name: Ziniu Yu
name: Jinshui Zheng
name: Longyu Zheng
Publisher: name: figshare
Year: 2019
Subjects: subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Physiology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Plant Biology
subject: Computational Biology

description: Additional file 5: Figure S3. Gene ontology (GO) classification of BSF unigenes. The left side and the right side of the panel show the percentage of genes and the number of genes that are classified to the three main categories, including biological process, cellular component, and molecular function.
Luminous and Dark Matter in the Milky Way
Creators: name: Olling, R. P.
name: Merrifield, M. R.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: (Abridged) Axisymmetric models of the Milky Way exhibit strong interrelations between the Galactic constants (R_0 and T_0), the stellar columndensity (S_*) and the shape of the dark matter (DM) halo. Here we present analytical relations that can be used to investigate the effects of the uncertain gaseous velocity dispersion on the HI flaring constraints. The contribution of cosmic rays and magnetic fields to the pressure gradients is small. A significantly flattened dark matter halo is only possible if R_0 ~ 170 km/s, we can rule out two DM candidates that require a highly flattened DM halo: 1) decaying massive neutrinos; and 2) a disk of cold molecular hydrogen. It is only possible to construct self-consistent models of the Galaxy based on the IAU-recommended values for the Galactic constants in the unlikely case that the the stellar columndensity is smaller than ~18 M_sun/pc^2. If we assume that the halo is oblate and S_* = 35 +/- 5 M_sun/pc^2, R_0
description: Accepted for publication in MNRAS
Origin of the "Disk-Line" Feature in the X-Ray Energy Spectrum of a Seyfert Galaxy, NGC4151
Creators: name: Takahashi, Kazuki
name: Inoue, Hajime
name: Dotani, Tadayasu
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have studied the origin of the broad and skewed feature at 4.5-7.5 keV in the energy spectra of NGC4151 using the ASCA and RXTE data. The feature consists of a narrow peak at 6.4 keV and a broad wing extended between 4.5-7.5 keV. An analysis of the long-term variations revealed that the feature became variable only on a time scale longer than 1.5x10^6 s. Through a comparison with the continuum variabilities, we found that the emission region of the excess flux at 4.5-7.5 keV has an extent of 10^17 cm. The broad and skewed feature at 4.5-7.5 keV may be explained by the so-called ``disk-line'' model. If so, the size of the line-emitting region, 10^17 cm, should be equal to several or ten-times the Schwarzschild radius of the central black hole. This results in a black hole mass of 10^11 solar mass, which may be too large for NGC4151. We propose an alternative explanation for the broad and skewed feature, i.e. a ``reflection'' model, which can also reproduce the overall energy spectra very well. In this model, cold matter with a sufficiently large column density is irradiated by X-rays to produce a reflected continuum, which constitutes the broad wing of the feature, and narrow fluorescent lines. The equivalent width of the iron fluorescent line (~2 keV) and the upper limit of its width (sigma < 92 eV) are also consistent with this model. From these results and considerations, we conclude that the ``disk-line'' model has difficulty to explain the spectral variations of NGC4151, and the reflection model is more plausible.
description: 19 pages, 16 figures, PASJ accepted
Neoproxius gypsatus
Creators: name: Heiss, E.
name: Moragues, G.
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Aradidae
Neoproxius
Neoproxius gypsatus

description: Neoproxius gypsatus (BERGROTH 1898)
L i t e r a t u r e d a t a:describedfromVenezuela.
M a t e r i a l e x a m i n e d 1♀ PK 37.5 Montagne de Kaw, 20.V.2001, piège malaise; 1♀ same locality PK 35, 12.XI.2002, piège malaise, both lg. J.A.Cerda (CGMM).
D i s t r i b u t i o n: Panama, Guatemala, Brazil, Venezuela.
description: Published as part of Heiss, E. & Moragues, G., 2009, Flat Bugs of French Guyana - a preliminary faunal list (Heteroptera, Aradidae), pp. 1659-1675 in Linzer biologische Beiträge 41 (2) on page 1664, DOI: 10.5281/zenodo.5279382
Y(so(5)) symmtry of the nonlinear Schr$\ddot{o}$dinger model with four-cmponents
Creators: name: Zhang, Hong-Biao
name: Ge, Mo-Lin
name: Xue, Kang
Publisher: name: arXiv
Year: 2001
Subjects: subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: The quantum nonlinear Schr$\ddot{o}$dinger(NLS) model with four-component fermions exhibits a $Y(so(5))$ symmetry when considered on an infintite interval. The constructed generators of Yangian are proved to satisfy the Drinfel'd formula and furthermore, the $RTT$ relation with the general form of rational R-matrix given by Yang-Baxterization associated with $so(5)$ algebraic structure.
description: 10 pages, no figures
Are the observed gaps in protoplanetary discs caused by growing planets?
Creators: name: Ndugu, Nelson
name: Bitsch, Bertram
name: Jurua, Edward
Publisher: name: arXiv
Year: 2019
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Recent detailed observations of protoplanetary discs revealed a lot of sub-structures which are mostly ring-like. One interpretation is that these rings are caused by growing planets. These potential planets are not yet opening very deep gaps in their discs. These planets instead form small gaps in the discs to generate small pressure bumps exterior to their orbits that stop the inflow of the largest dust particles. In the pebble accretion paradigm, this planetary mass corresponds to the pebble isolation mass, where pebble accretion stops and efficient gas accretion starts. We perform planet population synthesis via pebble and gas accretion including type-I and type-II migration. In the first stage of our simulations, we investigate the conditions necessary for planets to reach the pebble isolation mass and compare their position to the observed gaps. We find that in order to match the gap structures 2000 M E in pebbles is needed, which would be only available for the most metal rich stars. We then follow the evolution of these planets for a few My to compare the resulting population with the observed exoplanet populations. Planet formation in discs with these large amounts of pebbles result in mostly forming gas giants and only very little super-Earths, contradicting observations. This leads to the conclusions that either (i) the observed discs are exceptions, (ii) not all gaps in observed discs are caused by planets or (iii) that we miss some important ingredients in planet formation related to gas accretion and/or planet migration.
description: 9 pages, accepted for publication in MNRAS
The First Detection of Co in a Damped Lyman Alpha System
Creators: name: Ellison, Sara L.
name: Ryan, Sean G.
name: Prochaska, Jason X.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The study of elemental abundances in Damped Lyman Alpha systems (DLAs) at high redshift represents one of our best opportunities to probe galaxy formation and chemical evolution at early times. By coupling measurements made in high z DLAs with our knowledge of abundances determined locally and with nucleosynthetic models, we can start to piece together the star formation histories of these galaxies. Here, we discuss the clues to galactic chemical evolution that may be gleaned from studying the abundance of Co in DLAs. We present high resolution echelle spectra of two QSOs, Q2206-199 and Q1223+17, both already known to exhibit intervening damped systems. These observations have resulted in the first ever detection of Co at high redshift, associated with the z= 1.92 DLA in the sightline towards Q2206-199. We find that the abundance of Co is approximately 1/4 solar and that there is a clear overabundance relative to iron, [Co/Fe] = +0.31 +/- 0.05. From the abundance of Zn, we determine that this is a relatively metal-rich DLA, with a metallicity approximately 1/3 solar. Therefore, this first detection of Co is similar to the marked overabundance relative to Fe seen in Galactic bulge and thick disk stars.
description: Accepted for publication in MNRAS, 10 pages
Tineobius (Tineobius) longicauda Lucian Fusu & Antoni Ribes 2017, stat. nov.
Creators: name: Lucian Fusu
name: Antoni Ribes
Publisher: name: Zenodo
Year: 2017
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Eupelmidae
Tineobius
Tineobius longicauda

description: 20. Tineobius (Tineobius) longicauda (Ferrière, 1938) stat. nov. [new subgeneric status]
Anastatoidea longicauda Ferrière, 1938: 49, 57.
Holotype ♀, unique specimen (BMNH 5.938, examined by LF). Type locality: Siam: Bangkok.
Anastatoïdea longicauda – Risbec 1952: 67 (catalogued).
Tineobius longicauda – Bouček 1988: 565.
description: Published as part of Lucian Fusu & Antoni Ribes, 2017, Description of the first Palaearctic species of Tineobius Ashmead, 1896 with DNA data, a checklist of world species, and nomenclatural changes in Eupelmidae (Hymenoptera, Chalcidoidea), pp. 1-19 in European Journal of Taxonomy 263 on page 13, DOI: 10.5852/ejt.2017.263, http://zenodo.org/record/889169
Supplementary document for A method to derive the infrared complex refractive indices n(λ) and k(λ) for organic solids from KBr pellet absorption measurements - 6753502.pdf
Creators: name: Peterson, Kelly
name: Francis, Ryan
name: Banach, Catherine
name: Bradley, Ashley
name: Burton, Sarah
name: Erickson, Jeremy
name: Lockwood, Schuyler
name: Jensen, Karissa
name: Yokosuk, Michael
name: Johnson, Timothy
Publisher: name: Optica Publishing Group
Year: 2024
Subjects: Optical Properties of Materials

description: Table S1
Dynamical condition of neutral hydrogen envelopes of dwarf galaxies and their possible morphological evolution
Creators: name: Tajiri, Yuka Y.
name: Kamaya, Hideyuki
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We investigate the star-formation history of gas-rich dwarf galaxies, taking account of the dynamical evolution of their neutral hydrogen (H{\sc i}) envelope. Gas-rich dwarfs are classified into blue compact dwarfs (BCDs) and dwarf irregulars (dIrrs). In this paper, their H{\sc i} envelope is clearly shown not to be blown away by their stellar feedback. This is concluded since the observed star-formation rate (SFR) of gas-rich dwarfs is generally smaller than a critical SFR, $ψ_{\rm crit}$, at which stellar feedback accelerates the H{\sc i} envelope to the escape velocity. From this standpoint and the chemical property of sample BCDs, we suggest two possibilities; (1) The H{\sc i} gas in the envelope of BCDs is consumed to fuel their star-formation; and (2) BCDs have a similar star-formation history. We also discuss morphological evolution among dwarf galaxies. As long as gas-rich dwarfs are isolated, it is difficult for them to evolve into dwarf ellipticals (dEs). When the H{\sc i} envelope in gas-rich dwarfs is consumed in subsequent star-formation, a morphological exchange between BCDs and dIrrs is still expected, consistent with previous studies. If the SFR of gas-rich dwarfs was much higher than $ψ_{\rm crit}$ in the past, interestingly, an evolutionary scenario from dEs to gas-rich dwarfs is possible.
description: 15 pages, 2 figures, accepted by A&Ap
MOESM4 of De novo transcriptome sequencing and analysis revealed the molecular basis of rapid fat accumulation by black soldier fly (Hermetia illucens, L.) for development of insectival biodiesel
Creators: name: Zhaolu Zhu
name: Rehman, Kashif Ur
name: Yongqiang Yu
name: Liu, Xiu
name: Wang, Hui
name: Tomberlin, Jeffery
name: Sing-Hoi Sze
name: Minmin Cai
name: Jibin Zhang
name: Ziniu Yu
name: Jinshui Zheng
name: Longyu Zheng
Publisher: name: figshare
Year: 2019
Subjects: subject: Biochemistry
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Molecular Biology
subject: Pharmacology
subject: Evolutionary Biology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Marine Biology
subject: Inorganic Chemistry
subject: FOS: Chemical sciences
subject: Plant Biology
subject: Computational Biology

description: Additional file 4: Figure S2. Similarity analysis between BSF unigenes and NR database. (A) e value (â 17%) of BSF putative proteins with known proteins in NR database. (C) Top-hit species distribution of BLAST matches for BSF unigenes.
Quantum simulation of non-Markovianity using the quantum Zeno effect
Creators: name: Patsch, Sabrina
name: Maniscalco, Sabrina
name: Koch, Christiane P.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We suggest a quantum simulator that allows to study the role of memory effects in the dynamics of open quantum systems. Our proposal is based on a bipartite quantum system consisting, for simplicity, of a harmonic oscillator and a few-level system; it exploits the formal analogy between dissipation and quantum measurements. The interaction between the subsystems gives rise to quantum Zeno dynamics, and the dissipation strength experienced by the harmonic oscillator can be tuned by changing the parameters of the measurement, i.e., the interaction with the few-level system. Extension of the proposal to anharmonic systems is straightforward.
description: 10 pages, 7 figures
Neoproxius magdalenae
Creators: name: Heiss, E.
name: Moragues, G.
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Aradidae
Neoproxius
Neoproxius magdalenae

description: Neoproxius magdalenae (KORMILEV 1982)
L i t e r a t u r e d a t a: described from Nicaragua.
M a t e r i a l e x a m i n e d: 13 Forêt de St-Jean du Maroni, 5°405.85N, 54°063.34W, 70m, 1.5km layon en sous bois, Philodendron, J.C. Streito lg. and coll.
N o t e KORMILEV & FROESCHNER 1987: 85 erroneously indicated Costa Rica as type locality, however in the original description holo- and allotype are reported from Nicaragua. No further records are published since.
description: Published as part of Heiss, E. & Moragues, G., 2009, Flat Bugs of French Guyana - a preliminary faunal list (Heteroptera, Aradidae), pp. 1659-1675 in Linzer biologische Beiträge 41 (2) on page 1664, DOI: 10.5281/zenodo.5279382
The inclusive production of charged pion pairs in proton-antiproton collisions
Creators: name: Ahmadov, A. I.
name: Aydin, C.
name: Uzun, O.
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: In this study, we have considered the contribution of the higher-twist (HT) effects of the subprocesses to inclusive pion pair production cross section in the high energy proton-antiproton collisions by using various pion distribution amplitudes (DAs) within the frozen coupling constant approach and compared them with the leading-twist contributions. The feature of the HT effects may help the theoretical interpretation of the future PANDA experiment. The dependencies of the HT contribution on the transverse momentum $p_T$, the center of mass energy $\sqrt s$, and the variable $x_T$ are discussed numerically with special emphasis put on DAs. Moreover, the obtained analytical and numerical results for the differential cross section of the pion pair production are compared with the elastic backward scattering of the pion on the proton. We show that the main contribution to the inclusive cross section comes from the HT direct production process via gluon-gluon fusion. Also, it is strongly dependent on the pion DAs, momentum cut-off parameter $\triangle p$ and $$ which is the mean square of the intrinsic momentum of either initial parton.
description: 26 pages, 16 figures. arXiv admin note: text overlap with arXiv:hep-ph/9808229 by other authors
Local U(1) symmetry in Y(so(5)) associated with Massless Thirring Model and its Bethe Ansatz
Creators: name: Zhang, Hong-Biao
name: Ge, Mo-Lin
name: Xue, Kang
Publisher: name: arXiv
Year: 2001
Subjects: subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: The Massless Thirring model associated with SO(5) is solved in terms of the local U(1) symmetry. The local U(1) symmetry is related to q-deformation of four-component field operators due to the nonlinear interaction for differently internal degree of freedom. The Bethe ansatz wavefunction is also discussed. In addition, the local U(1) symmetry in the Yangian associated with SO(5)(Y(SO(5))) is explored.
description: 10 pages, no figures
Additional file 1 of The efficacy of a cyclin dependent kinase 9 (CDK9) inhibitor, FIT039, on verruca vulgaris: study protocol for a randomized controlled trial
Creators: name: Nomura, Takashi
name: Sumi, Eriko
name: Gyohei Egawa
name: Nakajima, Saeko
name: Toichi, Eiko
name: Uozumi, Ryuji
name: Tada, Harue
name: Nakagawa, Takayuki
name: Hagiwara, Masatoshi
name: Kabashima, Kenji
Publisher: name: figshare
Year: 2019
Subjects: subject: Biochemistry
subject: Medicine
subject: Biotechnology
subject: Developmental Biology
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: : SPIRIT 2013 checklist: recommended items to address in a clinical trial protocol and related documents. (DOC 126 kb)
Discrete Spectra of Semirelativistic Hamiltonians
Creators: name: Hall, Richard
name: Lucha, Wolfgang
name: Schoeberl, F. F.
Publisher: name: arXiv
Year: 2002
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: Mathematical Physics (math-ph)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We review various attempts to localize the discrete spectra of semirelativistic Hamiltonians of the form H = β\sqrt{m^2 + p^2} + V(r) (w.l.o.g. in three spatial dimensions) as entering, for instance, in the spinless Salpeter equation. Every Hamiltonian in this class of operators consists of the relativistic kinetic energy β\sqrt{m^2 + p^2} (where β> 0 allows for the possibility of more than one particles of mass m) and a spherically symmetric attractive potential V(r), r = |x|. In general, accurate eigenvalues of a nonlocal Hamiltonian operator can only be found by the use of a numerical approximation procedure. Our main emphasis, however, is on the derivation of rigorous semi-analytical expressions for both upper and lower bounds to the energy levels of such operators. We compare the bounds obtained within different approaches and present relationships existing between the bounds.
description: 21 pages, 3 figures
Aphleboderrhis pubescens
Creators: name: Heiss, E.
name: Moragues, G.
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Aradidae
Aphleboderrhis
Aphleboderrhis pubescens

description: Aphleboderrhis pubescens (WALKER 1873)
L i t e r a t u r e d a t a:describedfromBrazil.
M a t e r i a l e x a m i n e d: 13 Montagne de Kaw PK 37.5 + 2, 18.VIII.2004, à vue, lg. G. Moragues CGMM); 1♀ Régina, Montagne de Kaw PK 36, malaise trap, 5.I.1998 lg. J.A. Cerda (CEHI)
D i s t r i b u t i o n: Recorded from Mexico, Guatemala, Panama to Brazil.
description: Published as part of Heiss, E. & Moragues, G., 2009, Flat Bugs of French Guyana - a preliminary faunal list (Heteroptera, Aradidae), pp. 1659-1675 in Linzer biologische Beiträge 41 (2) on page 1665, DOI: 10.5281/zenodo.5279382
Tineobius (Tineobius) madagascariensis Lucian Fusu & Antoni Ribes 2017, nom. nov.
Creators: name: Lucian Fusu
name: Antoni Ribes
Publisher: name: Zenodo
Year: 2017
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hymenoptera
Eupelmidae
Tineobius
Tineobius madagascariensis

description: 21. Tineobius (Tineobius) madagascariensis Fusu & Ribes nom. nov.
Metapelma seyrigi Risbec, 1952: 63–66, fg. 16e, f.
Holotype ♀, unique specimen (MNHN, examined by LF). Type locality: Madagascar: Ranomafana. Secondary homonym of Tineobius seyrigi (Ferrière, 1938).
description: Published as part of Lucian Fusu & Antoni Ribes, 2017, Description of the first Palaearctic species of Tineobius Ashmead, 1896 with DNA data, a checklist of world species, and nomenclatural changes in Eupelmidae (Hymenoptera, Chalcidoidea), pp. 1-19 in European Journal of Taxonomy 263 on page 13, DOI: 10.5852/ejt.2017.263, http://zenodo.org/record/889169