cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
General practice access in regional and remote Australia for ageing populations
Creators: name: D Taylor
name: J Lange
name: C Laurence
name: Beilby, Justin
name: A Kitson
name: H Barrie
name: Visvanathan, Renuka
Publisher: name: Torrens University Australia
Year: 2020
Subjects: subject: 111702 Aged Health Care
subject: FOS: Health sciences

description: Identifying and removing access barriers to the timely provision of comprehensive health care is increasingly important for the wellbeing of Australia's rapidly ageing and frail populations, particularly those in non-metropolitan settings. This study has examined if current general practice (GP) locations in non-metropolitan South Australia and Western Australia (WA) are geographically accessible to the rapidly growing frail and prefrail populations known to have a high level of health service use and reduced mobility. Geospatial analysis linking 60-kilometre GP service catchments, 2016 population counts, and 2027 population projections has estimated that the size of the frail and prefrail population that live outside these GP service catchments will double, reaching 7,800 people by 2027. The maldistribution of GP locations was most evident in WA. As regional and remote populations continue to age, the challenge of health service provision, including geographic access to care, must be resolved to ensure that populations in these areas have the best opportunity to age well. Geospatial methods linking service and demographic information, such as the approach used in this analysis, can aid in planning the equitable provision of health care for older Australians.
Pelosia albifrons Rondani 1856
Creators: name: Sforzi, Alessandra
name: Sommaggio, Daniele
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Lepidoptera
Arctiidae
Pelosia
Pelosia albifrons

description: Pelosia albifrons Rondani, 1856
ORIGINAL DESCRIPTION: 1856: 185.
TYPE LOCALITY: Rondani gave no type locality in his original description but presumably it is Italy because the work deals with Italian species.
TYPE MATERIAL: 1 ♂, syntype (MZUF: Box 59): Pelosia Rndn. / albifrons Rndn., Parma / 3113.
CURRENT STATUS: doubtful species of Limoniidae (Savchenko et al. 1992: 369).
REMARKS: Rondani’s (1856: 185) key for the genus Pelosia Rondani, 1856 lists Pelosia albifrons as its type species, but he did not provide a detailed description, type locality, number or sex of the specimens. We found one syntype in this study.
description: Published as part of Sforzi, Alessandra & Sommaggio, Daniele, 2021, Catalog of the Diptera types described by Camillo Rondani, pp. 1-438 in Zootaxa 4989 (1) on page 136, DOI: 10.11646/zootaxa.4989.1.1, http://zenodo.org/record/4980621
Analysis of Dispersive Fourier Transform dataset using Dynamic Mode Decomposition: evidence of multiple vibrational modes, and their interplay in a three-soliton molecule
Creators: name: Sheveleva, Anastasiia
name: Hamdi, Saïd
name: Coillet, Aurélien
name: Finot, Christophe
name: Colman, Pierre
Publisher: name: arXiv
Year: 2023
Subjects: subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: We demonstrate that the Dynamic Mode Decomposition technique can effectively reduce the amount of noise in Dispersive Fourier Transform dataset; and allow for finer quantitative analysis of the experimental data. We therefore were able to demonstrate that the oscillation pattern of a soliton molecule actually results from the interplay of several elementary vibration modes.
Copious Amounts of Hot and Cold Dust Orbiting the Main Sequence A-type Stars HD 131488 and HD 121191
Creators: name: Melis, Carl
name: Zuckerman, B.
name: Rhee, Joseph H.
name: Song, Inseok
name: Murphy, Simon J.
name: Bessell, Michael S.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: We report two new dramatically dusty main sequence stars: HD 131488 (A1V) and HD 121191 (A8V). HD 131488 is found to have substantial amounts of dust in its terrestrial planet zone (L_IR/L_bol~4x10^-3), cooler dust further out in its planetary system, and an unusual mid-infrared spectral feature. HD 121191 shows terrestrial planet zone dust (L_IR/L_bol~2.3x10^-3), hints of cooler dust, and shares the unusual mid-infrared spectral shape identified in HD 131488. These two stars belong to sub-groups of the Scorpius-Centaurus OB association and have ages of ~10 Myr. HD 131488 and HD 121191 are the dustiest main sequence A-type stars currently known. Early-type stars that host substantial inner planetary system dust are thus far found only within the age range of 5-20 Myr.
description: 24 pages, 3 figures, 6 tables. Accepted for publication in ApJ
On Spectral Properties of Finite Population Processor Shared Queues
Creators: name: Zhen, Qiang
name: Knessl, Charles
Publisher: name: arXiv
Year: 2013
Subjects: subject: Probability (math.PR)
subject: FOS: Mathematics
subject: 60K25, 41A60, 35C20, 35P20

description: We consider sojourn or response times in processor-shared queues that have a finite population of potential users. Computing the response time of a tagged customer involves solving a finite system of linear ODEs. Writing the system in matrix form, we study the eigenvectors and eigenvalues in the limit as the size of the matrix becomes large. This corresponds to finite population models where the total population is $N\gg 1$. Using asymptotic methods we reduce the eigenvalue problem to that of a standard differential equation, such as the Hermite equation. The dominant eigenvalue leads to the tail of a customer's sojourn time distribution.
description: 28 pages, 7 figures and 5 tables
Allelopathic interference of wheat crop root exudates on germination, seedling growth and leaf chlorophyll attributes of purslane and annual ryegrass
Creators: name: M. Iftikhar Hussain
Publisher: name: Zenodo
Year: 2020
Subjects: Allelopathic crops, weed suppression, secondary metabolites, germination, growth bioassays, chlorophyll pigments

description: Common purslane (Portulaca oleracea) and annual ryegrass (Lolium rigidum) are important infesting weeds of field crops. Furthermore, prospects of herbicide resistance also demands considering alternative options such as the use of allelopathic crops for weed management. Wheat is an important allelopathic crop and present research was conducted to evaluate the allelopathic prospects of four wheat varieties on P. oleracea and L. rigidum in a laboratory-based germination and seedling growth bioassays. The Equal-Compartment-Agar (ECA) method was used to check the allelopathic effects of wheat genotypes while the interference in weed leaf chlorophyll pigments was measured by HPLC. Germination, radicle length and weed biomass were reduced following co-growth of weeds with wheat genotypes for 10-days. Wheat root exudates reduced the seedling growth of L. rigidum but it varies from 29% to 60%, depending on the wheat genotype, e.g. ‘Ursita’ showed a stronger allelopathic potential than ‘Glosa’ to inhibit the germination and radicle length of L. rigidum. Wheat also caused damage to xanthophyll pigments in weed leaves. The reduction of chlorophyll pigments was more prominent in L. rigidum than P. oleracea. The results conclude that wheat genotypes are allelopathic in nature and can be an alternate option to control L. rigidum and P. oleracea. However, wheat varieties differ considerably in their allelopathic potential and their performance should be checked against weeds under the natural field conditions.
Einstein-Yang-Mills theory : I. Asymptotic symmetries
Creators: name: Barnich, Glenn
name: Lambert, Pierre-Henry
Publisher: name: arXiv
Year: 2013
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: Asymptotic symmetries of the Einstein-Yang-Mills system with or without cosmological constant are explicitly worked out in a unified manner. In agreement with a recent conjecture, one finds a Virasoro-Kac-Moody type algebra not only in three dimensions but also in the four dimensional asymptotically flat case.
description: 12 pages Latex file
Beleuchtung der "Denkschrift des sächsischen Central-Zweig-Vereins zum Schutz vaterländischer Arbeit" zu Chemnitz; [um 1850]
Creators: name: Junghanns, Carl
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2018

description: Kopftitel
The Solar Orientation of the Lion Rock Complex in Sri Lanka
Creators: name: Sparavigna, Amelia Carolina
Publisher: name: arXiv
Year: 2013
Subjects: subject: History and Philosophy of Physics (physics.hist-ph)
subject: FOS: Physical sciences

description: This paper discusses the solar orientation of the archaeological complex of Sigiriya, the Lion Rock, in Sri Lanka. We can see that the axis of this complex is oriented with the sunset of the zenithal sun.
description: Keywords: Satellite Maps, Solar orientation, Archaeoastronomy
Self-Organized Synchronization and Voltage Stability in Networks of Synchronous Machines
Creators: name: Schmietendorf, Katrin
name: Peinke, Joachim
name: Friedrich, Rudolf
name: Kamps, Oliver
Publisher: name: arXiv
Year: 2013
Subjects: subject: Adaptation and Self-Organizing Systems (nlin.AO)
subject: Systems and Control (eess.SY)
subject: FOS: Physical sciences
subject: FOS: Electrical engineering, electronic engineering, information engineering

description: The integration of renewable energy sources in the course of the energy transition is accompanied by grid decentralization and fluctuating power feed-in characteristics. This raises new challenges for power system stability and design. We intend to investigate power system stability from the viewpoint of self-organized synchronization aspects. In this approach, the power grid is represented by a network of synchronous machines. We supplement the classical Kuramoto-like network model, which assumes constant voltages, with dynamical voltage equations, and thus obtain an extended version, that incorporates the coupled categories voltage stability and rotor angle synchronization. We compare disturbance scenarios in small systems simulated on the basis of both classical and extended model and we discuss resultant implications and possible applications to complex modern power grids.
description: 9 pages, 9 figures
Dasiops loncheus Rondani 1856
Creators: name: Sforzi, Alessandra
name: Sommaggio, Daniele
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Lonchaeidae
Dasiops
Dasiops loncheus

description: Dasiops loncheus Rondani, 1856
ORIGINAL DESCRIPTION: 1856: 120.
TYPE LOCALITY: Meigen (1826: 308) gave no type locality in the original description of Lonchea dasyops, but presumably it is Europe because the work deals with European species
TYPE MATERIAL: see Remarks.
CURRENT STATUS: junior synonym of Dasiops latifrons (Meigen, 1826) (Kovalev & Morge 1984: 249).
REMARKS: Rondani’s (1856: 120) key for the new genus Dasiops Rondani, 1856 identifies Lonchea dasyops Meigen, 1826 as the type species. Having used the species’ epithet for his new genus and thinking that the name Dasiops dasiops was incorrect, he erroneously substituted it with Dasiops loncheus, but did not provide a detailed description (Rondani 1856: 120). In his redescriptions of Dasiops loncheus, Rondani (1875a: 272, 1878b: 165) placed it in synonymy with Lonchaea parvicornis Meigen, 1826, Chorthophila lasiophtalma Macquart, 1835 and Lasiops aenescens Meigen, 1838. Dasiops loncheus is considered as a synonym of Dasiops lasiophthalmus (Macquart, 1835) by Bezzi (1892: 48), Becker (1895: 322), Pandellé (1902: 421) and Bezzi & Stein (1907: 88), and as a synonym of Dasiops latifrons (Meigen, 1826) by Czerny (1934: 7), Collin (1953: 181), Morge (1959a: 39) and Kovalev & Morge (1984: 249), but never as a valid species. The type material for Dasiops loncheus will be the same as for the name it was proposed to replace, i. e., Lonchea dasyops Meigen, 1826. Morge (1959a: 923) reported the holotype of Lonchaea dasiops in the MNHN. Muséum national d’Histoire naturelle (2020) did not list this latter species. Morge (1959a: 44) incorrectly considered the female of Dasiops loncheus in the MZUB as the lectotype. Under the name Dasiops loncheus there are four males and five females in the MZUF and two specimens in the MZUB (all are non-types). The type species of Dasiops is Lonchaea latifrons Meigen, 1826. The species name dasiops published as Lonchea [sic!] dasiops Rondani, 1856 (an incorrect spelling for dasyops, Lonchaea, Meigen, 1826) is considered as a rejected name (China 1961; I.C.Z.N. 1963: 114 [Opinion 652]).
description: Published as part of Sforzi, Alessandra & Sommaggio, Daniele, 2021, Catalog of the Diptera types described by Camillo Rondani, pp. 1-438 in Zootaxa 4989 (1) on page 136, DOI: 10.11646/zootaxa.4989.1.1, http://zenodo.org/record/4980621
Search for doubly charmed hadron at B factory
Creators: name: Jin, Yi
name: Li, Shi-Yuan
name: Liu, Yan-Rui
name: Si, Zong-Guo
name: Yao, Tao
Publisher: name: arXiv
Year: 2014
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The doubly charmed hadron production at B factories is of special importance for the study of the hadron structure and the color connections before hadronization. To suppress the combination background fluctuations of the reconstructed hadron mass spectra, we suggest a three-jet event shape trigger. After these three jets are identified by their energy and angular distributions, it is found that: 1) The background process $e^+ e^- \to c\bar {c} \to h's$ in consideration of the final hadron system $Λ_c^+K^-π^+ +X$ are significantly suppressed. 2) For the selected events, about half of the particles, $Λ_c^+$, $K^-$, $π^+$, which obviously can not belong to the decay products of doubly charmed hadron, can be vetoed. The relevant hadronization is investigated.
description: 14 pages, 8 figures. arXiv admin note: text overlap with arXiv:1309.5849
Asymptotic Analysis of Spectral Properties of Finite Capacity Processor Shared Queues
Creators: name: Zhen, Qiang
name: Knessl, Charles
Publisher: name: arXiv
Year: 2013
Subjects: subject: Probability (math.PR)
subject: FOS: Mathematics
subject: 60K25, 41A60, 35C20, 35P20

description: We consider sojourn (or response) times in processor-shared queues that have a finite customer capacity. Computing the response time of a tagged customer involves solving a finite system of linear ODEs. Writing the system in matrix form, we study the eigenvectors and eigenvalues in the limit as the size of the matrix becomes large. This corresponds to finite capacity models where the system can only hold a large number $K$ of customers. Using asymptotic methods we reduce the eigenvalue problem to that of a standard differential equation, such as the Airy equation. The dominant eigenvalue leads to the tail of a customer's sojourn time distribution. Some numerical results are given to assess the accuracy of the asymptotic results.
description: 30 pages, 7 figures, and 3 tables
On the growth of supermassive black holes formed from the gravitational collapse of fermionic dark matter cores
Creators: name: Argüelles, C. R.
name: Boshkayev, K.
name: Krut, A.
name: Nurbakhyt, G.
name: Rueda, J. A.
name: Ruffini, R.
name: Uribe-Suárez, J. D.
name: Yunis, R.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Observations support the idea that supermassive black holes (SMBHs) power the emission at the center of active galaxies. However, contrary to stellar-mass BHs, there is a poor understanding of their origin and physical formation channel. In this article, we propose a new process of SMBH formation in the early Universe that is not associated with baryonic matter (massive stars) or primordial cosmology. In this novel approach, SMBH seeds originate from the gravitational collapse of fermionic dense dark matter (DM) cores that arise at the center of DM halos as they form. We show that such a DM formation channel can occur before star formation, leading to heavier BH seeds than standard baryonic channels. The SMBH seeds subsequently grow by accretion. We compute the evolution of the mass and angular momentum of the BH using a geodesic general relativistic disk accretion model. We show that these SMBH seeds grow to $\sim 10^9$-$10^{10} M_\odot$ in the first Gyr of the lifetime of the Universe without invoking unrealistic (or fine-tuned) accretion rates.
description: 11 pages, 9 figures, 2 appendices. Accepted for publication in MNRAS
Electromagnetic Shower Properties in a Lead-Scintillator Sampling Calorimeter
Creators: name: Kotwal, Ashutosh V.
name: Hays, Christopher
Publisher: name: arXiv
Year: 2013
Subjects: subject: Instrumentation and Detectors (physics.ins-det)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: The Collider Detector at Fermilab (CDF) is a general-purpose experimental apparatus with an inner tracking detector for measuring charged particles, surrounded by a calorimeter for measurements of electromagnetic and hadronic showers. We describe a {\sc geant4} simulation and parameterization of the response of the CDF central electromagnetic calorimeter (CEM) to incident electrons and photons. The detector model consists of a detailed description of the CEM geometry and material in the direction of the incident particle's trajectory, and of the passive material between the tracker and the CEM. We use {\sc geant4} to calculate the distributions of: the energy that leaks from the back of the CEM, the energy fraction sampled by the scintillators, and the energy dependence of the response. We parameterize these distributions to accurately model electron and photon response and resolution in a custom simulation for the measurement of the $W$ boson mass.
Lonchea scutellaris Rondani 1875
Creators: name: Sforzi, Alessandra
name: Sommaggio, Daniele
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Lonchaeidae
Lonchea
Lonchea scutellaris

description: Lonchea scutellaris Rondani, 1875
ORIGINAL DESCRIPTION:1875a: 269 (key), 271 (description).
TYPE LOCALITY: “ in collibus agri parmensis, et … etruscum [Parmese hills, and … Etruria (= Tuscany) (Italy)]”.
TYPE MATERIAL: 1 ♀, lectotype (glued to a cardboard stage, covered with mold) (MZUF: Box 35): Lonchea Fall. / scutellaris n. / 1830 / Lectotypus [not designated] Lonchea scutellaris Rondani, ♀, det. G. Morge, Ex. 525; 1 ♂, paralectotype (MZUF: Box 35): Lonchea Fall. / scutellaris n. / 1830 / Paratypus Lonchea scutellaris Rondani, ♂, det. G. Morge, Ex. 524; 1 ♂, paralectotype (MZUF: Box 35): Lonchea Fall. / scutellaris n. / 1830 / Paratypus Lonchea scutellaris Rondani, ♂, det. G. Morge, Ex. 526.
CURRENT STATUS: valid species as Lonchaea scutellaris (Kovalev & Morge 1984: 257, Belcari et al. 1995b: 5).
REMARKS: Rondani (1875a: 271) described Lonchea scutellaris from four specimens without specifying their sex: “ Specimina tria legi in collibus agri parmensis, et unum a D. Piccioli etruscum, accepi [I collected three specimens in the Parmese hills, and received one from Etruria from D. Piccioli]”. Günter Morge examined the MZUF type series, adding the label “ lectotypus ” under one female and “ paratypus ” under each of the two males, without, as far as we know, publishing a lectotype designation (Morge 1959a, 1962a, 1963). We also found just three syntypes in this study. In order to promote nomenclatural stability, we give credit to G. Morge and here designate as a lectotype for Lonchea scutellaris Rondani, 1875 the female labeled as such by him. Rondani described this nominal species under the generic name “ Lonchea ”, which is an incorrect subsequent spelling of Lonchaea Fallén, 1820 (O’Hara et al. 2011: 108).
description: Published as part of Sforzi, Alessandra & Sommaggio, Daniele, 2021, Catalog of the Diptera types described by Camillo Rondani, pp. 1-438 in Zootaxa 4989 (1) on page 137, DOI: 10.11646/zootaxa.4989.1.1, http://zenodo.org/record/4980621
Bound states of spatially dependent mass Dirac equation with the Eckart potential including Coulomb tensor interaction
Creators: name: Ikhdair, S. M.
name: Falaye, B. J.
Publisher: name: arXiv
Year: 2014
Subjects: subject: Nuclear Theory (nucl-th)
subject: Mathematical Physics (math-ph)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We investigate the approximate solutions of the Dirac equation with the position-dependent mass particle in the Eckart potential field including the Coulomb tensor interaction by using the parametric Nikiforov-Uvarov method. Taking an appropriate approximation to deal with the centrifugal term, the Dirac energy states and the corresponding normalized two-spinor components of the wave function are obtained in closed form. Some special cases of our solution are investigated. Furthermore, we present the correct solutions obtained via the asymptotic iteration method which are in agreement with the parametric Nikiforov-Uvarov method results.
description: 24 pages, 1 figure
Nanofatigue behaviour of single struts of cast A356.0 foam: cyclic deformation, nanoindent characteristics and sub-surface microstructure
Creators: name: Schmahl, Merle
name: Märten, Anke
name: Zaslansky, P.
name: Fleck, Claudia
Publisher: name: Technische Universität Berlin
Year: 2020
Subjects: subject: 600 Technik, Technologie
subject: Al-Si-Mg alloy
subject: open-cell metal foam
subject: nanoindentation
subject: nano-fatigue
subject: cyclic deformation behaviour
subject: phase-contrast enhanced microcomputed tomography
subject: PCE-μCT
subject: transmission electron microscopy
subject: indent morphology

description: Struts are the main load carrying elements in cyclically loaded open cell metal foams. Little is known about the local fatigue behaviour and the influence of the microstructure on nanoscale deformation mechanisms. Different to the bulk counterpart, the millimetre-sized struts in precision-cast AlSi7Mg0.3 foams contain only 1–2 Al-dendrites, Si-Al-eutectic and intermetallic phases. We applied cyclic nanoindentation to N = 105 to assess nanofatigue. The change in minimum depth per cycle and the ratio of minimum to maximum indentation depths versus the number of cycles correspond to cyclic plastic processes. These and the indent and pile-up morphologies were correlated with the microstructure and dislocation formations revealed by phase-contrast-enhanced micro-computed tomography and transmission electron microscopy. Our results reveal that Si-particles affect deformation within 5 to 10 μm from the indent, and that they favour the formation of fatigue induced dislocation cells in the affected volume. We believe that this interaction is mediated through residual stresses. Furthermore, local variations in microstructure strongly influence the cyclic deformation behaviour and the indent pile-up size and morphology. Interestingly, the results well coincide with observations during fatigue of the bulk alloy reported in the literature.
title: Die deutsche Einheit; [1849]
title: Wie kann eine wahre deutsche Einheit erzweckt werden? Einzig und allein durch nachstehende deutsche Staats-Verfassung ; [München im Mai 1849]
titleType: Subtitle
Creators: name: Direnberger, Max
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2018

description: Kopftitel
Micropeza formicaria Rondani 1863
Creators: name: Sforzi, Alessandra
name: Sommaggio, Daniele
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Micropezidae
Micropeza
Micropeza formicaria

description: Micropeza formicaria Rondani, 1863
ORIGINAL DESCRIPTION: 1863: 42.
TYPE LOCALITY: “ Chiliae [Chile]”.
TYPE MATERIAL: 1 ♂, 1 ♀, syntypes (couple pinned together) (MZUN: Box Coll. entomol. extra-europea - Gen. Grallomya a Celiphus): Micropeza formicaria Rnd., Chili [= Chile] / M. Zool. N° 11468.
CURRENT STATUS: valid species, as Cryogonus formicarius (Steyskal 1968a: 2).
REMARKS: Rondani (1863: 42) described Micropeza formicaria, without specifying either the number or the sex of the specimens and not giving a range of lengths, from material received from R.A. Philippi, to whom he attributed the species name. Costa (1866: 35) listed a single MZUN specimen (as Micropeza formicaria Phil.) numbered “748”. We found two syntypes in this study.
description: Published as part of Sforzi, Alessandra & Sommaggio, Daniele, 2021, Catalog of the Diptera types described by Camillo Rondani, pp. 1-438 in Zootaxa 4989 (1) on page 138, DOI: 10.11646/zootaxa.4989.1.1, http://zenodo.org/record/4980621
Aspilia alpestris Rondani 1871
Creators: name: Sforzi, Alessandra
name: Sommaggio, Daniele
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Muscidae
Aspilia
Aspilia alpestris

description: Aspilia alpestris Rondani, 1871
ORIGINAL DESCRIPTION: 1871a: 318.
TYPE LOCALITY: “ in Alpibus … prope Varallum [Alps … near Varallo (= Vercelli, Italy)]”.
TYPE MATERIAL: 2 ♀♀, syntypes (one covered with mold) (MZUF: Box 22): Aspilia Rnd. / alpestris Rnd., Varallo, Alpi / 1167.
CURRENT STATUS: junior synonym of Phaonia angelicae (Scopoli, 1763) (Pont 1986b: 117, Gorodkov et al. 1995: 12).
REMARKS: Rondani (1871a: 318) described Aspilia alpestris from just the female sex, without specifying the exact number of specimens: “ legi specimina aliqua foeminea [I collected some female specimens]”. He later (Rondani 1877c: 87) reported two females: “ Mas ignotus. Faeminas duas alpinas possideo [Male unknown. I have two females from the Alps]”.
description: Published as part of Sforzi, Alessandra & Sommaggio, Daniele, 2021, Catalog of the Diptera types described by Camillo Rondani, pp. 1-438 in Zootaxa 4989 (1) on page 140, DOI: 10.11646/zootaxa.4989.1.1, http://zenodo.org/record/4980621
Aspilia funeralis Rondani 1866
Creators: name: Sforzi, Alessandra
name: Sommaggio, Daniele
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Muscidae
Aspilia
Aspilia funeralis

description: Aspilia funeralis Rondani, 1866
ORIGINAL DESCRIPTION: 1866a: 87 (key), 88 (description).
TYPE LOCALITY: “ in Apennino parmensi [Parmese Apennines (Italy)]”.
TYPE MATERIAL: 3 ♂♂, syntypes (two partially destroyed by the pin) (MZUF: Box 22): Aspilia Rnd. / funeralis Rnd., Apenn. [= Apennines] / 1161.
CURRENT STATUS: junior synonym of Spilogona dispar (Fallén, 1823) (Pont 1986b: 168, Gorodkov et al. 1995: 15).
REMARKS: Rondani (1866a: 88) described Aspilia funeralis from just the male sex, without specifying the exact number of specimens and not giving a range of lengths: “ Raro lecta a Doct. Berteo et a me in Apennino parmensi, …, specimina mascula tantum [Rarely collected by Dr. Berteo and me in the Parma Apennines … only male specimens]”. We found three syntypes in this study.
description: Published as part of Sforzi, Alessandra & Sommaggio, Daniele, 2021, Catalog of the Diptera types described by Camillo Rondani, pp. 1-438 in Zootaxa 4989 (1) on page 140, DOI: 10.11646/zootaxa.4989.1.1, http://zenodo.org/record/4980621
Plasmonic-enhanced bright single spin defects in silicon carbide membranes
Creators: name: Zhou, Ji-Yang
name: Li, Qiang
name: Hao, Zhi-He
name: Lin, Wu-Xi
name: He, Zhen-Xuan
name: Liang, Rui-Jian
name: Guo, Liping
name: Li, Hao
name: You, Lixing
name: Tang, Jian-Shun
name: Xu, Jin-Shi
name: Li, Chuan-Feng
name: Guo, Guang-Can
Publisher: name: arXiv
Year: 2023
Subjects: subject: Optics (physics.optics)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Optically addressable spin defects in silicon carbide (SiC) have emerged as attractable platforms for various quantum technologies. However, the low photon count rate significantly limits their applications. We strongly enhanced the brightness by 7 times and spin-control strength by 14 times of single divacancy defects in 4H-SiC membranes using surface plasmon generated by gold film coplanar waveguides. The mechanism of the plasmonic-enhanced effect is further studied by tuning the distance between single defects and the surface of the gold film. A three-energy-level model is used to determine the corresponding transition rates consistent with the enhanced brightness of single defects. Lifetime measurements also verified the coupling between defects and surface plasmons. Our scheme is low-cost, without complicated microfabrication and delicate structures, which is applicable for other spin defects in different materials. This work would promote developing spin defect-based quantum applications in mature SiC materials.
Spontaneously quenched gamma-ray spectra from compact sources
Creators: name: Petropoulou, Maria
name: Arfani, Dafni
name: Mastichiadis, Apostolos
Publisher: name: arXiv
Year: 2013
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We study a mechanism for producing intrinsic broken power-law gamma-ray spectra in compact sources. This is based on the principles of automatic photon quenching, according to which, gamma-rays are being absorbed on spontaneously produced soft photons, whenever the injected luminosity in gamma-rays lies above a certain critical value. We derive an analytical expression for the critical gamma-ray compactness in the case of power-law injection. For the case where automatic photon quenching is relevant, we calculate analytically the emergent steady-state gamma-ray spectra. We perform also numerical calculations in order to back up our analytical results. We show that a spontaneously quenched power-law gamma-ray spectrum obtains a photon index 3Γ/2, where Γ is the photon index of the power-law at injection. Thus, large spectral breaks of the gamma-ray photon spectrum, e.g. $ΔΓ\gtrsim 1$, can be obtained by this mechanism. We also discuss additional features of this mechanism that can be tested observationally. Finally, we fit the multiwavelength spectrum of a newly discovered blazar (PKS 0447-439) by using such parameters, as to explain the break in the gamma-ray spectrum by means of spontaneous photon quenching, under the assumption that its redshift lies in the range 0.1
description: 14 pages, 9 figures, 2 tables, accepted for publication in A&A
Flugschrift vom politischen Greisler in Wien in der Leopold-Vorstadt. Das magistratisch-politische Raubnest, oder: Die Wiener magistratische Beamten-Bureaukratie; [1848]
Creators: name: Ullmeyer, Anton
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2018

description: Kopftitel
Aspilia pubicheta Rondani 1871
Creators: name: Sforzi, Alessandra
name: Sommaggio, Daniele
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Muscidae
Aspilia
Aspilia pubicheta

description: Aspilia pubicheta Rondani, 1871
ORIGINAL DESCRIPTION: 1871a: 317.
TYPE LOCALITY: “ in Alpibus Pedemontii [Piedmont, Italy, Alps]”.
TYPE MATERIAL: 1 ♀, syntype (MRSN): 21.64 / 682 / Aspilia Rond. / pubicheta Rond., Alpi, ♀; 1 ♀, syntype (MRSN): 93 56 / 688 / Aspilia Rond. / pubicheta Rond., Alpi, ♀; 1 ♀, syntype (MRSN): [illegible label] / 687 / Aspilia Rond. / pubicheta Rond., Alpi, ♀.
CURRENT STATUS: junior synonym of Thricops aculeipes (Zetterstedt, 1838) (Pont 1986b: 65).
REMARKS: Rondani (1871a: 317) described Aspilia pubicheta without specifying the number, the sex or the length of the specimens, received from L. Bellardi. Hennig (1961: 228) reported three female types in the MRSN. We also found three female syntypes in this study.
description: Published as part of Sforzi, Alessandra & Sommaggio, Daniele, 2021, Catalog of the Diptera types described by Camillo Rondani, pp. 1-438 in Zootaxa 4989 (1) on page 140, DOI: 10.11646/zootaxa.4989.1.1, http://zenodo.org/record/4980621
Conversion efficiency in the process of co-polarized spontaneous four-wave mixing
Creators: name: Garay-Palmett, Karina
name: U'Ren, Alfred B.
name: Rangel-Rojo, Raúl
Publisher: name: arXiv
Year: 2013
Subjects: subject: Quantum Physics (quant-ph)
subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: We study the process of co-polarized spontaneous four-wave mixing in single-mode optical fibers, with an emphasis on an analysis of the conversion efficiency. We consider both the monochromatic-pumps and pulsed-pumps regimes, as well as both the degenerate-pumps and non-degenerate-pumps configurations. We present analytical expressions for the conversion efficiency, which are given in terms of double integrals. In the case of pulsed pumps we take these expressions to closed analytical form with the help of certain approximations. We present results of numerical simulations, and compare them to values obtained from our analytical expressions, for the conversion efficiency as a function of several key experimental parameters.
An Introduction to Noncommutative Physics
Creators: name: Liang, Shi-Dong
name: Lake, Matthew J.
Publisher: name: arXiv
Year: 2023
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: In recent years, many new developments in theoretical physics, and in practical applications rely on different techniques of noncommutative algebras. In this review, we introduce the basic concepts and techniques of noncommutative physics in a range of areas, including classical physics, condensed matter systems, statistical mechanics, and quantum mechanics, and we present some important examples of noncommutative algebras, including the classical Poisson brackets, the Heisenberg algebra, Lie and Clifford algebras, the Dirac algebra, and the Snyder and Nambu algebras. Potential applications of noncommutative structures in high-energy physics and gravitational theory are also discussed. In particular, we review the formalism of noncommutative quantum mechanics based on the Seiberg--Witten map and propose a parameterization scheme to associate the noncommutative parameters with the Planck length and the cosmological constant. We show that noncommutativity gives rise to an effective gauge field, in the Schrödinger and Pauli equations. This term breaks translation and rotational symmetries in the noncommutative phase space, generating intrinsic quantum fluctuations of the velocity and acceleration, even for free particles. This review is intended as an introduction to noncommutative phenomenology for physicists, as well as a basic introduction to the mathematical formalisms underlying these effects.
description: 31 pages, no tables, no figures. Published version (v1). Minor changes and updated references (v2)
Woronowicz construction of compact quantum groups for functions on permutations. Classification result for N=3
Creators: name: Kula, Anna
Publisher: name: arXiv
Year: 2014
Subjects: subject: Operator Algebras (math.OA)
subject: Quantum Algebra (math.QA)
subject: FOS: Mathematics
subject: 81R50 (Primary), 46L65, 18D10 (Secondary)

description: We provide a classification of compact quantum groups, which can be obtained by the Woronowicz construction, when the arrays used in the twisted determinant condition are extensions of functions on permutations. General properties of such quantum groups are revealed with the aid of operators intertwining tensor powers of the fundamental corepresentation. Two new families of quantum groups appear: three versions of the quantum group $SU_q(3)$ with complex $q$ and a non-commutative analogue of the semi-direct product of two-dimensional torus with the alternating group $A_3$.
description: 34 pages
title: Effect of biochar on soil fertility, nitrate losses, dissolved organic carbon, forage crop production and greenhouse gas (GHG) emissions
Creators: name: Eissa, Riad Omar Abosalahe Omar
Publisher: name: Memorial University of Newfoundland
Year: 2022

description: The growing need to improve soil fertility and enhance crop production has led to increase in the nitrogenous (N) fertilizer use, which could result in detrimental effects due to the possible increase in greenhouse gas (GHG) emissions and nitrate leaching losses. Therefore, there is a pressing need to address the negative environmental effects of nitrogen fertilizer use through better management practices. Biochar applications to the agricultural soils have been recognized as a unique strategy for improving soil fertility, mitigating GHG emission, enhancing carbon sequestration, and plant nutrient use efficiencies by increasing nutrients uptake while reducing the leachate losses. Considering multidimensional benefits of biochar, the current study investigated the effects of different biochar application rates on podzolic soil fertility, GHGs mitigation potential, soil nitrogen dynamics, crop productivity and forage quality in eastern Newfoundland podzolic soils. The first experiment was conducted to assess the nitrate adsorption potential of four different biochar feedstocks including, spruce-bark biochar at 550⁰C (SB550), hardwood biochar at 500⁰C (HW500), fir/spruce biochar at 427⁰C (FS427), and softwood biochar at 500⁰C (SW500). The results showed that SB550 has the highest nitrate adsorption capacity (184 mg g⁻¹) among others. The second experiment was conducted in a greenhouse with five rates of SB550 and two N application levels to (i) investigate the capability of biochar application for improving the soil fertility, forage production, forage quality, and nutrient uptake, (ii) assess their effects on soil total nitrogen (TN), nitrate (NO₃⁻), ammonium (NH₄⁺) dynamics and dissolved organic carbon (DOC). Results indicated that biochar application significantly improved soil pH, Soil Organic Matter (SOM), Cation Exchange Capacity (CEC), and available nutrients in the soil. Moreover, SB550 biochar has significantly reduced NO₃⁻, NH₄⁺, TN, and DOC in the leachate compared to the control treatment. The third experiment was conducted under field conditions. Four rates of HW500 biochar applications, with three levels of nitrogen fertilizer applications (Urea 46-0-0) that were applied at the rates of 0, 65 and 130 N kg/ha to the Festulolium forage crop field. Biochar application has significantly reduced GHG emissions and increased the Festulolium productions. Thus, biochar application has shown to be a promising technique for sustainable agricultural management practices in the eastern Newfoundland Podzolic soil.
The Formation of Population III Stars in Gas Accretion Stage: Effects of Magnetic Fields
Creators: name: Machida, Masahiro N.
name: Doi, Kentaro
Publisher: name: arXiv
Year: 2013
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: The formation of Population III stars is investigated using resistive magnetohydrodynamic simulations. Starting from a magnetized primordial prestellar cloud, we calculate the cloud evolution several hundreds of years after first protostar formation, resolving the protostellar radius. When the natal minihalo field strength is weaker than B \lesssim 10^-13 (n/1 cm^-3)^-2/3 G (n is the hydrogen number density), magnetic effects can be ignored. In this case, fragmentation occurs frequently and a stellar cluster forms, in which stellar mergers and mass exchange between protostars contribute to the mass growth of these protostars. During the early gas accretion phase, the most massive protostar remains near the cloud centre, whereas some of the less massive protostars are ejected. The magnetic field significantly affects Population III star formation when B_amb \gtrsim 10^-12 (n/1 cm^-3)^-2/3 G. In this case, because the angular momentum around the protostar is effectively transferred by both magnetic braking and protostellar jets, the gas falls directly onto the protostar without forming a disk, and only a single massive star forms. In addition, a massive binary stellar system appears when B_amb \sim 10^-12 (n/1cm^-3)^-2/3 G. Therefore, the magnetic field determines the end result of the formation process (cluster, binary or single star) for Population III stars. Moreover, no persistent circumstellar disk appears around the protostar regardless of the magnetic field strength, which may influence the further evolution of Population III stars.
description: 59 pages, 21 figures, Accepted for publication in MNRAS. For high resolution figures see http://jupiter.geo.kyushu-u.ac.jp/machida/arxiv/PopIII/
Aspilia rupestris Rondani 1866
Creators: name: Sforzi, Alessandra
name: Sommaggio, Daniele
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Muscidae
Aspilia
Aspilia rupestris

description: Aspilia rupestris Rondani, 1866
ORIGINAL DESCRIPTION: 1866a: 87 (key), 89 (description).
TYPE LOCALITY: “ in Apennino parmensi … in alpina plaga agri Tirolensis [Parmese Apennines (Italy) … Tyrolean alpine locality]”.
TYPE MATERIAL: not found in this study. See Remarks.
CURRENT STATUS: junior synonym of Thricops nigrifrons (Robineau-Desvoidy, 1830) (Pont 1986b: 68, Gorodkov et al. 1995: 10).
REMARKS: Rondani (1866a: 89) described Aspilia rupestris from two females: “ Foeminam unicam legi … in Apennino parmensi, et aliam possideo … lectam a Prof. Strobel [I collected one female … in Parmese Apennines and have another one collected by Prof. Strobel]”. Rondani (1877c: 90) considered the female received from Strobel as a different species, which he named Spilogaster tirolensis. Hennig (1961: 228) incorrectly considered the specimen from “ Tirol ” [= Tyrol] as the type of Atherigona rupestris. We did not find the specimen from “Parma”, the true type of Aspilia rupestris but, under the name Atherigona rupestris in the MZUF, did find the single specimen from “ Tirol ” [= Tyrol], which we consider as the holotype of Spilogaster tirolensis.
description: Published as part of Sforzi, Alessandra & Sommaggio, Daniele, 2021, Catalog of the Diptera types described by Camillo Rondani, pp. 1-438 in Zootaxa 4989 (1) on page 141, DOI: 10.11646/zootaxa.4989.1.1, http://zenodo.org/record/4980621
Compressible Turbulence in the Near-Sun Solar Wind: Parker Solar Probe's First Eight Perihelia
Creators: name: Cuesta, Manuel Enrique
name: Chhiber, Rohit
name: Fu, Xiangrong
name: Du, Senbei
name: Yang, Yan
name: Pecora, Francesco
name: Matthaeus, William H.
name: Li, Hui
name: Steinberg, John
name: Guo, Fan
name: Gan, Zhaoming
name: Conrad, Emma
name: Swanson, Diana
Publisher: name: arXiv
Year: 2023
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Plasma Physics (physics.plasm-ph)
subject: Space Physics (physics.space-ph)
subject: FOS: Physical sciences

description: Many questions remain about the compressibility of solar wind turbulence with respect to its origins and properties. Low plasma beta (ratio of thermal to magnetic pressure) environments allow for the easier generation of compressible turbulence, enabling study of the relationship between density fluctuations and turbulent Mach number. Utilizing Parker Solar Probe plasma data, we examine the normalized proton density fluctuations $\langle δn_p^2 \rangle ^{1/2}/\langle n_p\rangle = δ{n_p}_{rms}/\langle n_p\rangle$ as a function of turbulent Mach number $M_t$ conditioned on plasma beta and cross helicity. With consideration of statistical error in the parameters computed from in-situ data, we find a general result that $δ{n_p}_{rms}/\langle n_p\rangle \sim M_t^{1.18 \pm 0.04}$, consistent with both linear-wave theory, and nearly-incompressible turbulence in an inhomogeneous background field. We compare observational results conditioned on plasma beta and cross helicity with 3D magnetohydrodynamic simulations, and observe rather significant similarities with respect to how those parameters affect the proportionality between density fluctuations and turbulent Mach number. This study further investigates the complexity of compressible turbulence as viewed by the density scaling relationship, and may help better understand the compressible environment of the near-Sun solar wind.
description: 8 pages, 3 figures, 1 table, submitted to ApJL
Atherigona soccata Rondani 1871
Creators: name: Sforzi, Alessandra
name: Sommaggio, Daniele
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Muscidae
Atherigona
Atherigona soccata

description: Atherigona soccata Rondani, 1871
ORIGINAL DESCRIPTION: 1871a: 332.
TYPE LOCALITY: “ in Etruria [Etruria (= Tuscany, Italy)]”.
TYPE MATERIAL: 1 ♀, syntype (missing fore- and left mid-legs) (MZUF: Box 24): Atherigona Rndn. / soccata Rnd., ♀, Etruria / 1273.
CURRENT STATUS: valid species (Pont 1986b: 114, Gorodkov et al. 1995: 12).
REMARKS: Rondani (1871a: 332) described Atherigona soccata from just the female sex, without specifying either the number or the length of the specimens: “ Semel foeminam legit in Etruria D. Piccioli [the female once collected in Etruria by D. Piccioli]”. We found one syntype in this study.
description: Published as part of Sforzi, Alessandra & Sommaggio, Daniele, 2021, Catalog of the Diptera types described by Camillo Rondani, pp. 1-438 in Zootaxa 4989 (1) on page 141, DOI: 10.11646/zootaxa.4989.1.1, http://zenodo.org/record/4980621
title: Der Gewerbe-Ausschuß an seine Mitbürger; [um 1848]
title: In einer Zeit, wie in der gegenwärtigen, wo abseiten der außerordentlichen Ereignisse in unserem deutschen Vaterlande, es sich auch darum handelt, unserem kleinen Freistaat anstatt der Institutionen ...
titleType: Subtitle
Creators: name: (:Unav)
Publisher: name: Universitätsbibliothek der Ludwig-Maximilians-Universität München
Year: 2018

description: Kopftitel
Caricea pardalina Rondani 1871
Creators: name: Sforzi, Alessandra
name: Sommaggio, Daniele
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Muscidae
Caricea
Caricea pardalina

description: Caricea pardalina Rondani, 1871
ORIGINAL DESCRIPTION: 1871a: 334.
TYPE LOCALITY: “ In Sardinia [Sardinia, Italy]”.
TYPE MATERIAL: not found in this study.
CURRENT STATUS: junior synonym of Helina ciliatocosta (Zetterstedt, 1845) (Pont 1986b: 139, Gorodkov et al. 1995: 13).
REMARKS: Rondani (1871a: 334) described Caricea pardalina, without specifying the number, the sex or the length of the specimens, from material received from L. Bellardi. We could not locate any type specimens of this nominal species during our study.
description: Published as part of Sforzi, Alessandra & Sommaggio, Daniele, 2021, Catalog of the Diptera types described by Camillo Rondani, pp. 1-438 in Zootaxa 4989 (1) on page 146, DOI: 10.11646/zootaxa.4989.1.1, http://zenodo.org/record/4980621
Legendre scalarization in gravity and cosmology
Creators: name: Cotsakis, Spiros
name: Mimoso, Jose P.
name: Miritzis, John
Publisher: name: arXiv
Year: 2023
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We propose a new formulation of $f(R)$ gravity, dubbed scalarized $f(R)$ gravity, in which the Legendre transform is included as a dynamical term. This leads to a theory with second-order field equations that describes general relativity with a self-interacting scalar field, without requiring the introduction of conformal frames. We demonstrate that the quadratic version of scalarized $f(R)$ gravity reduces to general relativity with a massive scalar field, and we explore its implications for Friedmann cosmology. Our findings suggest that scalarized $f(R)$ gravity may lead to simplified descriptions of cosmological applications, while the proposed formulation could offer a new perspective on the relationship between $f(R)$ gravity and scalar-tensor theories.
description: v2: 14 pages, 3 figures, matches published version