cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Tenebrio impressus Linnaeus
Creators: name: Ferrer, Julio
name: Holston, Kevin
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Tenebrionidae
Tenebrio
Tenebrio impressus

description: 6. Tenebrio impressus Linnaeus, in litteris.
 Sex indeterminate, probably female, det. Erodius sp. Linnaeus Coll., UUZM.
 Remarks. This name is unpublished, and the specimen does not represent any published Linnean species. The specimen is not mentioned by Thunberg (1804) in the list of insects described by Linnaeus and donated to the Academy of the University of Uppsala, nor is it mentioned in subsequent papers by Thunberg on darkling beetles (1814, 1821, 1827). Tenebrio impressus Fabricius, 1801, is a species of the genus Promethis Pascoe, 1869, from the Indo-Malaysian region (Gebien 1906, Kaszab 1988), verified after examination of the two ZMUC types, whereas the UUZM “ Tenebrio impressus ” is a species of the Mediterranean genus Erodius impossible to identify without further revision of this genus.
 FIGURES 11–12. Illustrations from Pallas (1781). Fig. 11. Tenebrio glandiformis Pallas, det. Psammodes gibbus (L.), in lateral (“11.b”) and dorsal (“11.a”) view. Fig. 12. of Tenebrio gibbus Pallas, det. Moluris gibbus (Pallas), in lateral view.
description: Published as part of Ferrer, Julio & Holston, Kevin, 2009, Identities of Tenebrio Linnaeus types at Uppsala, and the resulting changes in old darkling beetle names (Insecta: Coleoptera: Tenebrionidae), pp. 29-42 in Zootaxa 2308 (1) on pages 38-39, DOI: 10.11646/zootaxa.2308.1.2, http://zenodo.org/record/5305799
Limits on $ν_τ$ mass by DELPHI
Creators: name: Perego, Davide
Publisher: name: arXiv
Year: 2002
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: A limit on the tau neutrino mass is obtained using all the $Z^{0} \to τ^{+} τ^{-}$ data collected at LEP by the DELPHI detector between 1992 and 1995. In this analysis events in which one of the taus decays into one charged particle, while the second $τ$ decays into f{}ive charged pions (1-5 topology) have been used. The neutrino mass is determined from a bidimensional \fit ~on the invariant mass $m^{*}_{5 π}$ and on the energy $E_{5 π}$ of the f{}ive $π^{\pm}$ system. The result found is $m_{ν_τ}
description: Invited talk at the 7th International Workshop on Tau Lepton Physics (TAU02), Santa Cruz, Ca, USA, Sept 2002, 9 pages, LaTex, espcrc2.sty, 9 eps figures
Asymptotic behavior of dispersive electromagnetic waves in bounded domains
Creators: name: Nicaise, Serge
name: Pignotti, Cristina
Publisher: name: arXiv
Year: 2019
Subjects: subject: Analysis of PDEs (math.AP)
subject: FOS: Mathematics

description: We analyze the stability of Maxwell equations in bounded domains taking into account electric and magnetization effects. Well-posedness of the model is obtained by means of semigroup theory. A passitivity assumption guarantees the boundedness of the associated semigroup. Further the exponential or polynomial decay of the energy is proved under suitable sufficient conditions. Finally, several illustrative examples are presented.
EdgeFool: An Adversarial Image Enhancement Filter
Creators: name: Shamsabadi, Ali Shahin
name: Oh, Changjae
name: Cavallaro, Andrea
Publisher: name: arXiv
Year: 2019
Subjects: subject: Machine Learning (cs.LG)
subject: Computer Vision and Pattern Recognition (cs.CV)
subject: Machine Learning (stat.ML)
subject: FOS: Computer and information sciences

description: Adversarial examples are intentionally perturbed images that mislead classifiers. These images can, however, be easily detected using denoising algorithms, when high-frequency spatial perturbations are used, or can be noticed by humans, when perturbations are large. In this paper, we propose EdgeFool, an adversarial image enhancement filter that learns structure-aware adversarial perturbations. EdgeFool generates adversarial images with perturbations that enhance image details via training a fully convolutional neural network end-to-end with a multi-task loss function. This loss function accounts for both image detail enhancement and class misleading objectives. We evaluate EdgeFool on three classifiers (ResNet-50, ResNet-18 and AlexNet) using two datasets (ImageNet and Private-Places365) and compare it with six adversarial methods (DeepFool, SparseFool, Carlini-Wagner, SemanticAdv, Non-targeted and Private Fast Gradient Sign Methods). Code is available at https://github.com/smartcameras/EdgeFool.git.
MOESM5 of â We are responsible for the violence, and prevention is up to usâ : a qualitative study of perceived risk factors for gender-based violence among Ethiopian university students
Creators: name: Kaufman, Michelle
name: Williams, Ashlie
name: Graziele Grilo
name: Marea, Christina
name: Fasil Fentaye
name: Lakew Gebretsadik
name: Shifera Yedenekal
Publisher: name: figshare
Year: 2019
Subjects: subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Additional file 5. focus group guide for faculty/staff.
Homogeneous models and their toposes of supported sets
Creators: name: Faber, Eric Ernst
Publisher: name: Apollo - University of Cambridge Repository
Year: 2020
Subjects: topos theory
category theory
model theory
intuitionism
constructive mathematics
mathematical logic
sheaves
Fraïssé theory
set theory

description: This thesis studies homogeneous models by looking at their topos of finitely supported sets. Of various well-known toposes, such as cubical sets and simplicial sets, it is shown that they can be presented as a topos of this kind. It is argued that these examples can be understood as coming from a homogeneous model, in the sense of model theory, but formulated in topos-theoretical terms. It is shown that the connecting structure between the two is a factorizing prime site and the notion of a principal model. This is further substantiated by demonstrating that the Fraïssé-Hrushovski construction can be formulated in terms of such sites. The notion of finite support is abstracted and a general calculus of orbits for toposes of supported sets is developed. It is shown that these form a factorizing prime site and that they can be compared to the age of structure as in classical model theory, and can be given a topos-theoretic characterization in terms of the hyperconnected-localic factorization of a geometric morphism. The theory is then applied by revisiting and generalizing the Ryll-Nardzewski theorem to the new setting and by constructing a very general class of Fraenkel-Mostowki models of intuitionistic set theory. Lastly, a notion of a Kan fibration for such toposes is studied and shown to generalize the familiar notions in simplicial sets and cubical sets. Under particular assumptions, it is proved that these Kan fibrations are closed under dependent product and hence interpret a version of Martin-Löf intensional dependent type theory. For simplicial sets, a different approach using simplicial Moore paths and its connection to the present work is announced.
Quark and Gluon Propagators in Covariant Gauges
Creators: name: Giusti, L.
name: Paciello, M. L.
name: Petrarca, S.
name: Taglienti, B.
name: Tantalo, N.
Publisher: name: arXiv
Year: 2001
Subjects: subject: High Energy Physics - Lattice (hep-lat)
subject: FOS: Physical sciences

description: We present data for the gluon and quark propagators computed in the standard lattice Landau's gauge and for three values of the covariant gauge-fixing parameter lambda=0,8,16. Our results are obtained using the SU(3) Wilson action in the quenched approximation at beta=6.0 and volume=16^3x32.
description: Lattice2001(theorydevelop)
Assessing the Political Economy of the 2014 U.S. Farm Bill
Creators: name: Zulauf, Carl R.
name: Orden, David
name: Zulauf, Carl R.
name: Orden, David
Publisher: name: Unknown
Year: 2014
Subjects: subject: Agricultural and Food Policy
subject: Agricultural policy
subject: 2014 farm bill
subject: farm subsidies
subject: commodity programs
subject: crop insurance
subject: conservation
subject: WTO

description: This chapter assesses the political economy of the 2014 farm bill, which eliminated annual fixed direct payments but offers enhanced downside risk protection against low prices or declining revenue. The farm bill secured substantial bipartisan majorities in a politically contentious Congress. The countercyclical structure of U.S. support is reaffirmed and crop insurance is enhanced as a safety net pillar. Open policy issues include the distribution of benefits among crops, the design of multiple year support around moving-average revenue benchmarks versus fixed references prices, and questions related to crop insurance, including the overall level of premium subsidies. In an international context, we conclude the 2014 farm safety net likely would not have been enacted had multilateral agreement been reached on the 2008 Doha Round negotiating documents; conversely, the 2014 safety net makes achieving those limits more difficult.
Supplementary Materials from The Goldilocks Effect: female geladas in mid-sized groups have higher fitness
Creators: name: Johnson, Elizabeth Tinsley
name: Feder, Jacob A.
name: Bergman, Thore J.
name: Lu, Amy
name: Snyder-Mackler, Noah
name: Beehner, Jacinta C.
Publisher: name: The Royal Society
Year: 2021
Subjects: subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: 60801 Animal Behaviour

description: Figures and tables presenting full results from statistical analyses
Spin-polarized neutron matter, the maximum mass of neutron stars, and GW170817
Creators: name: Tews, I.
name: Schwenk, A.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Nuclear Theory (nucl-th)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We investigate how a phase transition from neutron-star matter to spin-polarized neutron matter affects the equation of state and mass-radius relation of neutron stars. While general extension schemes for the equation of state allow for high pressures inside neutron stars, we find that a phase transition to spin-polarized neutron matter excludes extreme regimes. Hence, such a transition limits the maximum mass of neutron stars to lie below 2.6$-$$2.9 \, M_{\odot}$, depending on the microscopic nuclear forces used, while significantly larger masses could be reached without these constraints. These limits are in good agreement with recent constraints extracted from the neutron-star merger GW170817 and its electromagnetic counterpart. Assuming the description in terms of spin-polarized neutron matter to be valid in the center of neutron stars, we find that stars with a large spin-polarized domain in their core are ruled out by GW170817.
description: 10 pages, 3 figures, published version
Tegonotini Bagdasarian 1978
Creators: name: Wei, Suigai
name: Wang, Guoquan
name: Qin, Aizhi
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Arachnida
Trombidiformes
Eriophyidae

description: Key to the genera of Tegonotini from China  1. Dorsal opisthosoma with anterior dorsal annuli fused forming a broad plate.............................................................. 2
- Dorsal opisthosoma without anterior dorsal annuli fused, not forming a plate............................................................ 3
 2. Dorsal pedipalp genual setae d bifurcated, ventral setae d absent .......................................... Asetidicrothrix gen. nov.
 - Dorsal pedipalp genual setae d not bifurcated, ventral setae d present......... Phyllocoptacus Mohanasundaram, 1984
 3. Dorsal annuli 2, 5, 7, 9 and 11 with large spines .................................................. Spinaetergum Hong & Kuang, 1989
- Dorsal annuli not as above............................................................................................................................................ 4
 4. Coxae setae 1b absent ........................................................................................................ Parategonotus Kuang, 1991
 - Coxae setae 1b present..................................................................................................................................................5
5. Genu II setae absent...................................................................................................................................................... 6
- Genu II setae present..................................................................................................................................................... 7
 6. Scapular setae ahead of rear shield margin, tibial setae absent ................................................. Gongella Kuang, 2005
 - Scapular setae on rear shield margin, tibial setae present. .............................Neoshevtchenkella Kuang & Zhuo, 1989
 7. Scapular setae ahead of rear shield margin .............................................................................. Tegonotus Nalepa, 1890
 - Scapular setae on rear shield margin ....................................................................... Shevtchenkella Bagdasarian, 1978
description: Published as part of Wei, Suigai, Wang, Guoquan & Qin, Aizhi, 2009, One new genus and four new species of Tegonotini (Acari: Eriophyidae) from Guangxi, South China, pp. 60-68 in Zootaxa 2312 on page 61
Noise and the strong signal limit in radio astronomical measurement
Creators: name: Liszt, H.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The random error of radioastronomical measurements is usually computed in the weak-signal limit, which assumes that the system temperature is sensibly the same on and off source, or with and without a spectral line. This assumption is often very poor. We give examples of common situations in which it is important to distinguish the system noise in signal-bearing and signal-free regions.
description: To appear in PASP, 2002 October
Expansion of General Relativity via the  Temporal Oscillation Theory
Creators: name: Marques, Daniel
Publisher: name: Zenodo
Year: 2025
Subjects: subject: Physical cosmology

description: Extending General Relativity through the Temporal Oscillation Theory (TOT)

General Relativity (GR) provides a geometric framework for gravity, describing it as the curvature of spacetime. While extensively validated through astrophysical observations and precision experiments, GR faces persistent challenges in cosmology and high-energy physics. These include the unexplained need for dark matter in galactic dynamics, the introduction of a cosmological constant to justify cosmic acceleration, and the presence of singularities in black holes.

The Temporal Oscillation Theory (TOT) proposes a dynamical extension of GR, incorporating gravitational oscillations in the spacetime metric. This novel framework enables:Singularity resolution – Black hole interiors exhibit dynamically oscillating gravitational fields rather than absolute singularities.Dark matter alternative – Instead of hypothesizing unknown particles, TOT modifies gravity at galactic scales to naturally reproduce observed rotation curves.Cosmic acceleration without Λ\LambdaΛ – The universe's accelerated expansion arises naturally from an intrinsic oscillatory effect, removing the need for a cosmological constant.

This paper presents a rigorous mathematical derivation of the TOT-modified metric and field equations, systematically comparing its predictions with GR and alternative gravity models. We explore its implications for black hole physics and cosmology, providing testable observational predictions. These include possible deviations in gravitational lensing, corrections to the Hawking radiation spectrum, and measurable effects on atomic clocks in strong gravitational fields.

A stability analysis is conducted, confirming the mathematical robustness of TOT and its compatibility with experimental constraints. By maintaining the core principles of General Relativity while addressing its major limitations, TOT provides a novel and physically motivated extension of gravitational theory with broad implications for astrophysics, cosmology, and quantum gravity.
Asetidicrothrix Wei & Wang & Qin 2009, gen. nov.
Creators: name: Wei, Suigai
name: Wang, Guoquan
name: Qin, Aizhi
Publisher: name: Zenodo
Year: 2009
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Arachnida
Actinedida
Eriophyidae
Asetidicrothrix

description: Asetidicrothrix gen. nov.
 Diagnosis. Dorsal pedipalp genual setae (d) bifurcated, prodorsal shield with frontal lobe, scapular tubercles set ahead of rear shield margin; coxae I with 2 pairs of setae, coxae II with 1 pair of setae; tibial setae (l ΄), genu II setae (l''), setae d and setae e absent; tarsal empodium entire; dorsal opisthosoma with anterior annuli fused forming a broad plate, median and lateral ridges present; anterior ventral annuli narrower than dorsal annuli, posterior ventral annuli broad and equal to dorsal annuli.
 Type species. Asetidicrothrix luculiae sp. nov.
 Etymology. Aseti, referring to ventral setae e absent, and the generic name Dicrothrix Keifer, 1966, to which the new genus is similar.
 Remarks. The new genus is similar to Dicrothrix Keifer, 1966, but can be differentiated from the latter by the ventral setae e being absent and the anterior ventral annuli narrower than the dorsal annuli. In Dicrothrix, the ventral setae e are present and all the ventral annuli are broad and equal to dorsal annuli (Keifer 1966).
description: Published as part of Wei, Suigai, Wang, Guoquan & Qin, Aizhi, 2009, One new genus and four new species of Tegonotini (Acari: Eriophyidae) from Guangxi, South China, pp. 60-68 in Zootaxa 2312 on page 61
Using Big Data Sets to Analyse Human Behaviour Patterns and Urban Spatial Structure - A Case Study of the Spatial-Temporal Dynamics in Shanghai
Creators: name: Xiao, Chaowei
Publisher: name: Apollo - University of Cambridge Repository
Year: 2020
Subjects: Big Data
Urban Spatial Structure
Mobile Phone Signal Data
Shanghai
Activity Patterns
OD
Dynamic Matrices
Housing Price

description: Big Data is changing the traditional way of data collection. As an example of Big Data, mobile phone signal data can be used in geography and urban planning analysis. The approximate spatial position of the mobile-phone user can be calculated according to the signal data sent by a mobile-phone and the location of the base station. This research demonstrates that it is possible to use the mobile-phone signal data to calculate the spatial distribution of urban population. It also tests the suitability of existent metrics and tries to evaluate change by creating new metrics. In Shanghai, by using existent metrics, this study finds that the spatial distribution of the city’s population calculated by mobile-phone signal data generally corresponds to the demographic census. Moreover, this research also employs mobile phone signal data to analyse the spatial correlation between facilities, housing price and other variables and population density distribution in Shanghai. Finally, this study calculates the individual’s origin-destination (OD) flows of Shanghai, gets the job housing distance, and identifies the difference of job-living spatial movement pattern of Shanghai residents. This research also intends to figure out the factors that cause the difference in job-housing spatial relationships between four groups of people in different types of urban functional areas. This research corroborates David Harvey’s time-space compression theory and spatial fix theory by using Big Data set. Going beyond that, it extends these theories by arguing the interchangeability between exploitation in the time dimension, and that in the spatial dimension, resulting in dual exploitation. This study has important policy implications for optimizing the urban spatial system of Shanghai, as it advocates that in addition to strengthening the enforcement of labour law, the government also needs to improve the public service such as strengthening the public transportation systems capacity, and construct affordable houses, so as to alleviate the employees’ sufferings caused by temporal and spatial exploitation.
Building a CCD Spectrograph for Educational or Amateur Astronomy
Creators: name: Kannappan, Sheila J.
name: Fabricant, Daniel G.
name: Hughes, Charles B.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We discuss the design of an inexpensive, high-throughput CCD spectrograph for a small telescope. By using optical fibers to carry the light from the telescope focus to a table-top spectrograph, one can minimize the weight carried by the telescope and simplify the spectrograph design. We recently employed this approach in the construction of IntroSpec, an instrument built for the 16-inch Knowles Telescope on the Harvard College campus.
description: 17 pages including 7 figures, PASP, accepted (higher resolution figures at http://cfa-www.harvard.edu/~sheila/introspec.ps.gz)
Semi-analytic modelling of AGNs: auto-correlation function and halo occupation
Creators: name: Oogi, Taira
name: Shirakata, Hikari
name: Nagashima, Masahiro
name: Nishimichi, Takahiro
name: Kawaguchi, Toshihiro
name: Okamoto, Takashi
name: Ishiyama, Tomoaki
name: Enoki, Motohiro
Publisher: name: arXiv
Year: 2019
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: The spatial clustering of active galactic nuclei (AGNs) is considered to be one of the important diagnostics for the understanding of the underlying processes behind their activities complementary to measurements of the luminosity function (LF). We analyse the AGN clustering from a recent semi-analytic model performed on a large cosmological $N$-body simulation covering a cubic gigaparsec comoving volume. We have introduced a new time-scale of gas accretion on to the supermassive black holes to account for the loss of the angular momentum on small scales, which is required to match the faint end of the observed X-ray LF. The large simulation box allows us accurate determination of the auto-correlation function of the AGNs. The model prediction indicates that this time-scale plays a significant role in allowing massive haloes to host relatively faint population of AGNs, leading to a higher bias factor for those AGNs. The model predictions are in agreement with observations of X-ray selected AGNs in the luminosity range $10^{41.5}~\mathrm{erg} \ \mathrm{s}^{-1} \leq L_{2-10\mathrm{keV}} \leq 10^{44.5}~\mathrm{erg} \ \mathrm{s}^{-1}$, with the typical host halo mass of $10^{12.5-13.5} h^{-1}\,{\rm M}_{\odot}$ at $z \lesssim 1$. This result shows that the observational clustering measurements impose an independent constraint on the accretion time-scale complementary to the LF measurements. Moreover, we find that not only the effective halo mass corresponding to the overall bias factor, but the extended shape of the predicted AGN correlation function shows remarkable agreement with those from observations. Further observational efforts towards the low luminosity end at $z \sim 1$ would give us stronger constraints on the triggering mechanisms of AGN activities through their clustering.
description: 20 pages, 13 figures, accepted in MNRAS. Error estimates of the 2PCFs and the fitting to them have been improved. Further discussions and references have been added. Main results remain unchanged
GCM Analysis of the collective properties of lead isotopes with exact projection on particle numbers
Creators: name: Heenen, P. -H.
name: Valor, A.
name: Bender, M.
name: Bonche, P.
name: Flocard, H.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We present a microscopic analysis of the collective behaviour of the lead isotopes in the vicinity of Pb208. In this study, we rely on a coherent approach based on the Generator Coordinate Method including exact projection on N and Z numbers within a collective space generated by means of the constrained Hartree-Fock BCS method. With the same Hamiltonian used in HF+BCS calculations, we have performed a comprehensive study including monopole, quadrupole and octupole excitations as well as pairing vibrations. We find that, for the considered nuclei, the collective modes which modify the most the conclusions drawn from the mean-field theory are the octupole and pairing vibrations.
description: 10 pages LATEX, 8 figures, submitted to EPJA
MOESM4 of â We are responsible for the violence, and prevention is up to usâ : a qualitative study of perceived risk factors for gender-based violence among Ethiopian university students
Creators: name: Kaufman, Michelle
name: Williams, Ashlie
name: Graziele Grilo
name: Marea, Christina
name: Fasil Fentaye
name: Lakew Gebretsadik
name: Shifera Yedenekal
Publisher: name: figshare
Year: 2019
Subjects: subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Additional file 4. focus group guide for male students.
Additional file 1 of Scaling-up filariasis lymphoedema management into the primary health care system in Kerala State, Southern India: a case study in healthcare equity
Creators: name: Krishnasastry, Suma T.
name: Mackenzie, Charles D.
name: Sadanandan, Rajeev
Publisher: name: figshare
Year: 2022
Subjects: subject: Medicine
subject: Biotechnology
subject: Cancer
subject: 111714 Mental Health
subject: FOS: Health sciences
subject: 110309 Infectious Diseases
subject: Computational Biology

description: Additional file 1: Objectives and description of various sessions on LF MMDP training in Kerala.
title: Table des matières_Manuel du jardinier-fleuriste et de l'amateur de fleurs
Creators: name: AmauetrS
Publisher: name: NAKALA - https://nakala.fr (Huma-Num - CNRS)
publisherIdentifier: https://ror.org/04ces3204
publisherIdentifierScheme: ROR
Year: 2020

description: Table des matières
Physical and match performance characteristics of male university field hockey players
Creators: name: Lam, Elliot
Publisher: name: Loughborough University
Year: 2023
Subjects: classificationCode: 420799
subject: Sports science and exercise not elsewhere classified

description: Field hockey is predominantly an amateur sport in the United Kingdom and many players will choose to study an academic degree at university. This period of academic study coincides with a key period in the talent identification and development pathway of players, where they can be selected for or progress into junior international and senior international programmes during their studies. Engaging in a high-performance university programme may facilitate the development of players. The aim of the present thesis was to quantify the physical and match performance characteristics of male university field hockey players competing at UK national level, and to examine whether these characteristics developed as players progressed through university.Quantifying the physical and match performance characteristics of male university field hockey players competing at UK national level revealed comparable profiles to senior international level players reported in the literature. This may reflect the high proportion of junior international players attending university and suggest that high-performance university programmes prepare players well for the potential transition into senior international competition. Whilst physical characteristics such as intermittent endurance capacity and lower body strength were higher in 3rd year undergraduate/postgraduate players compared to 1st year undergraduate players, the match performance characteristics (total and high-speed running distance) of 3rd year players were lower compared to 1st and 2nd year players. Whilst the concurrent development of game understanding (tactical and technical characteristics) in more experienced university players may reduce the running output required to perform at national level, the development of physical characteristics at university may prepare players to achieve this high level of performance repeatedly at senior international level where shorter in-match rotations and between-match periods are likely apparent in tournament matchplay.
The influence of a top-heavy integrated galactic IMF and dust on the chemical evolution of high-redshift starbursts
Creators: name: Palla, Marco
name: Calura, Francesco
name: Matteucci, Francesca
name: Fan, XiLong
name: Vincenzo, Fiorenzo
name: Lacchin, Elena
Publisher: name: arXiv
Year: 2019
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We study the effects of the integrated galactic initial mass function (IGIMF) and dust evolution on the abundance patterns of high redshift starburst galaxies. In our chemical models, the rapid collapse of gas clouds triggers an intense and rapid star formation episode, which lasts until the onset of a galactic wind, powered by the thermal energy injected by stellar winds and supernova explosions. Our models follow the evolution of several chemical elements (C, N, $α$-elements and Fe) both in the gas and dust phases. %The most recent stellar yield and dust prescriptions are adopted. We test different values of $β$, the slope of the embedded cluster mass function for the IGIMF, where lower $β$ values imply a more top-heavy initial mass function (IMF). The computed abundances are compared to high-quality abundance measurements obtained in lensed galaxies and from composite spectra in large samples of star-forming galaxies in the redshift range $2 \lesssim z \lesssim 3$. The adoption of the IGIMF causes a sensible increase of the rate of star formation with respect to a standard Salpeter IMF, with a strong impact on chemical evolution. We find that in order to reproduce the observed abundance patterns in these galaxies, either we need a very top-heavy IGIMF ($β< 2$) or large amounts of dust. In particular, if dust is important, the IGIMF should have $β\ge 2$, which means an IMF slightly more top-heavy than the Salpeter one. The evolution of the dust mass with time for galaxies of different mass and IMF is also computed, highlighting that the dust amount increases with a top-heavier IGIMF.
description: 21 pages, 14 Figures. Accepted for publication in MNRAS
Additional file 1 of Production of succinic acid through the fermentation of Actinobacillus succinogenes on the hydrolysate of Napier grass
Creators: name: Lee, Jhih-Sing
name: Lin, Cheng-Jia
name: Lee, Wen-Chien
name: Teng, Hsin-Yi
name: Chuang, Meng-Hsin
Publisher: name: figshare
Year: 2022
Subjects: subject: Biophysics
subject: Biochemistry
subject: Space Science
subject: Microbiology
subject: FOS: Biological sciences
subject: Biotechnology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology

description: Additional file 1: Figure S1. PCR conditions, primers and DNA sequence alignment of alcohol dehydrogenase (Asuc_0403) in Mu-B7 mutant. “Query” is the DNA sequence of Asuc_0403 in the chromosome of Actinobacillus succinogenes 130Z (GenBank accession number CP000746.1), while “Sbjct” is the DNA sequence of Asuc_0403 in Mu-B7 mutant. Figure S2. Succinic acid fermentation on hydrolysate of glucose (a), xylose (b), and hydrolysate of Napier grass supplemented with glycerol at the mass ratio of 10:1 (c), 5:1 (d), and 2:1 (e). The ratios are based on the amount of glucose in hydrolysate to the amount of glycerol added, w/w. Figure S3. HPLC spectra of fermentation broth compositions: (a) fermentation on glucose for 8 h and (b) fermentation on the hydrolysate of Napier grass supplemented with glycerol at the hydrolysate-to-glycerol ratio of 2:1 for 8 h.
Who Will Feed China in the 21st Century? Income
Creators: name: Martin, William J.
name: Fukase, Emiko
name: Martin, William J.
name: Fukase, Emiko
Publisher: name: Unknown
Year: 2014
Subjects: subject: International Development
subject: International Relations/Trade
subject: cereal equivalents
subject: China
subject: food self-sufficiency
subject: livestock
subject: income growth

description: This paper uses resource-based cereal equivalent measures to explore the evolution of China’s demand and supply for food. Although demand for food calories is probably close to its peak level in China, the ongoing dietary shift to animal-based foods, induced by income growth, is likely to impose considerable pressure on agricultural resources. Estimating the relationship between income growth and food demand with data from a wide range of countries, China’s demand growth appears to have been broadly similar to the global trend. On the supply side, output of food depends strongly on the productivity growth associated with income growth and on the country’s agricultural land endowment, with China appearing to be an out-performer. The analyses of income-consumption-production dynamics suggest that China’s current income level falls in the range where consumption growth outstrips production growth, but that the gap is likely to begin to decline as China’s population growth and dietary transition slow down. Continued agricultural productivity growth through further investment in research and development, and expansion in farm size and increased mechanization, as well as sustainable management of agricultural resources, are vital for ensuring that it is primarily China that will feed China in the 21st century.
Searches for Diboson New Physics and the L1Calo Software Development with the ATLAS Detector
Creators: name: Lin, Chiao-Ying
Publisher: name: Apollo - University of Cambridge Repository
Year: 2020
Subjects: ATLAS
Diboson
electroweak
exotics
Standard Model
DAQ
Trigger
L1Calo
LHC

description: The Standard Model has been a successful theory in describing the behaviour of fundamental particles, but there are still problems remaining unsolved. New theoretical models are therefore proposed to answer those questions with either new interactions or new particles. This thesis is presenting the searches for new physics with diboson signatures in these two ways from LHC $\sqrt{s}=13~TeV$ collisions with the ATLAS detector with the data collected in 2015 and 2016 corresponding to an integrated luminosity of $36.1~fb^{-1}$. The searching strategy was performed with the Monte Carlo simulation for the SM background modelling and a data-driven method for the multijet background estimation. The final result was interpreted by a comparison between background modelling and data by a CLs method. For the resonance search, no new particle was discovered, and mass limits are therefore set on the new particles from models taken as the interpretation benchmarks. For the study on new interactions in the signatures of vector boson scattering, the first measurement of this process with the semileptonic decay was given with a significance of $2.7\sigma$ in reasonable agreement with the SM prediction Both the LHC and ATLAS detector are now going through the upgrades for operations in 2021 with the $\sqrt{s}=14~TeV$ collisions. The ATLAS hardware calorimeter trigger is part of the upgrade project for the implementation of three new object processors: eFex, jFex, and gFex. This thesis will also present the construction of simulation system along with the expected performance of proposed object reconstruction algorithms for this new infrastructure.
description: Peterhouse Studentship
O'ZBEKISTONDA BIZNES MUHITINI YAXSHILASH VA INVESTITSION LOYIHALARDAN FOYDALANISH JARAYONLARINI TAKOMILLASHTIRISH
Creators: name: Mirsalixova, N.A.
Publisher: name: Zenodo
Year: 2024

description: Maqolada bozor iqtisodiyoti sharoitida olib borilayotgan islohotlar natijasida ishlab chiqarish korxonalarini keng ko‘lamli rivojlantirish asosida kichik biznes, kasanachilik, hunarmandchilik, oilaviy va yakka tadbirkorlikning boshqa yo‘nalishlariga davlatimiz tomonidan yaratilayotgan sharoitlar tahlil qilingan. Bugungi kunda, O‘zbekistonda biznes muhitini yaxshilash va investitsion loyihalardan foydalanish jarayonlarini takomillashtirish bo‘yicha takliflar ishlab chiqilgan.
MOESM1 of Role of protein arginine methyltransferase 5 in group 3 (MYC-driven) Medulloblastoma
Creators: name: Nagendra Chaturvedi
name: Sidharth Mahapatra
name: Varun Kesherwani
name: Kling, Matthew
name: Shukla, Mamta
name: Ray, Sutapa
name: Kanchan, Ranjana
name: Naveenkumar Perumal
name: McGuire, Timothy
name: J. Sharp
name: Shantaram Joshi
name: Coulter, Don
Publisher: name: figshare
Year: 2019
Subjects: subject: Biochemistry
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Science Policy

description: Additional file 1: Figure S1. The expression correlation of PRMT5gene with MYCgene in medulloblastoma. These data were analyzed using a Pifster(nÂ =â 223) cohort at R2-Genomics platform.
qubit-ADAPT-VQE: An adaptive algorithm for constructing hardware-efficient ansatze on a quantum processor
Creators: name: Tang, Ho Lun
name: Shkolnikov, V. O.
name: Barron, George S.
name: Grimsley, Harper R.
name: Mayhall, Nicholas J.
name: Barnes, Edwin
name: Economou, Sophia E.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Quantum simulation, one of the most promising applications of a quantum computer, is currently being explored intensely using the variational quantum eigensolver. The feasibility and performance of this algorithm depend critically on the form of the wavefunction ansatz. Recently in Nat. Commun. 10, 3007 (2019), an algorithm termed ADAPT-VQE was introduced to build system-adapted ansätze with substantially fewer variational parameters compared to other approaches. This algorithm relies heavily on a predefined operator pool with which it builds the ansatz. However, Nat. Commun. 10, 3007 (2019) did not provide a prescription for how to select the pool, how many operators it must contain, or whether the resulting ansatz will succeed in converging to the ground state. In addition, the pool used in that work leads to state preparation circuits that are too deep for a practical application on near-term devices. Here, we address all these key outstanding issues of the algorithm. We present a hardware-efficient variant of ADAPT-VQE that drastically reduces circuit depths using an operator pool that is guaranteed to contain the operators necessary to construct exact ansätze. Moreover, we show that the minimal pool size that achieves this scales linearly with the number of qubits. Through numerical simulations on $\text{H}_4$, LiH and $\text{H}_6$, we show that our algorithm ("qubit-ADAPT") reduces the circuit depth by an order of magnitude while maintaining the same accuracy as the original ADAPT-VQE. A central result of our approach is that the additional measurement overhead of qubit-ADAPT compared to fixed-ansatz variational algorithms scales only linearly with the number of qubits. Our work provides a crucial step forward in running algorithms on near-term quantum devices.
description: 15 pages, 6 figures; v2 includes a new proof that the minimal operator pool size scales linearly in the number of qubits. Explicit examples of such pools are also now included
Search for a low mass CP-odd Higgs boson in e+e- collisions with the OPAL detector at LEP2
Creators: name: The OPAL Collaboration
name: Abbiendi, G.
Publisher: name: arXiv
Year: 2002
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: We have analysed the data collected by OPAL at centre-of-mass energies between 189 and 209 GeV searching for Higgs boson candidates from the process e+e- -> h0Z0 followed by the decay of h0 -> A0A0 where A0 is the CP-odd Higgs boson. The search is done in the region where the A0 mass, mA, is below the production threshold for bbbar, and the CP-even Higgs boson mass mh is within the range 45-86 GeV/c^2. In this kinematic range, the decay of h0 -> A0A0 may be dominant and previous Higgs boson searches have very small sensitivities. This search can be interpreted within any model that predicts the existence of at least one scalar and one pseudoscalar Higgs boson. No excess of events is observed above the expected Standard Model backgrounds. Model-independent limits on the cross-section for the process e+e- -> h0Z0 are derived assuming 100% decays of the h0 into A0A0 and 100% decays of the A0A0 into each of the following final states: ccbarccbar, gggg, tau+tau-tau+tau-, ccbargg ggtau+tau- and ccbartau+tau-. The results are also interpreted in the CP-conserving no-mixing MSSM scenario, where the region 45 <= mh <= 85 GeV/c^2 and 2<= mA <= 9.5 GeV/c^2 is excluded.
description: 26 pages, 8 figures, Submitted to Eur. Phys. J.C
Clear Evidence of a Continuum Theory of 4D Euclidean Simplicial Quantum Gravity
Creators: name: Egawa, H. S.
name: Horata, S.
name: Yukawa, T.
Publisher: name: arXiv
Year: 2001
Subjects: subject: High Energy Physics - Lattice (hep-lat)
subject: FOS: Physical sciences

description: Four-dimensional (4D) simplicial quantum gravity coupled to both scalar fields (N_X) and gauge fields (N_A) has been studied using Monte-Carlo simulations. The matter dependence of the string susceptibility exponent gamma^{(4)} is estimated. Furthermore, we compare our numerical results with Background-Metric-Independent (BMI) formulation conjectured to describe the quantum field theory of gravity in 4D. The numerical results suggest that the 4D simplicial quantum gravity is related to the conformal gravity in 4D. Therefore, we propose a phase structure in detail with adding both scalar and gauge fields and discuss the possibility and the property of a continuum theory of 4D Euclidean simplicial quantum gravity.
description: 3 pages, LaTeX, Lattice2001(surfaces)
Minnesota's Nonmetro Cities Use Revolving Loans as a Development Tool
Creators: name: Stinson, Thomas F.
name: Lubov, Andrea
name: Stinson, Thomas F.
name: Lubov, Andrea
Publisher: name: Unknown
Year: 1992
Subjects: Community/Rural/Urban Development
Public Economics

description: Nearly 100 of Minnesota's nonmetro towns use revolving loan funds as a way to spur local economic development. Here's how they work: a town makes the initial loans to qualified businesses, and as the loans are repaid, the money is loaned out again and again to other businesses. A few problems need to be worked out: default rates somewhat higher than those experienced by other lenders, slow accumulation of funds needed to make second-generation loans, and slow turnover in "revolving" the funds to the next round of businesses. In city-based programs, there is also the risk that viable projects are going unfunded in towns without access to a revolving fund.
Docker Image file of MARCOVul
Creators: name: Zhang, Jixian
Publisher: name: Zenodo
Year: 2025
Subjects: Code vulnerability detection
Docker image

description: ``zjx-cvd-v1.tar`` is the docker image file of MARCOVul.

``requirements.txt`` and ``freeze-conda-env.yml`` are the ``bugdetect`` environment configurations exported by conda.
Coordinated thermal and optical observations of Trans-Neptunian object (20000) Varuna from Sierra Nevada
Creators: name: Lellouch, E.
name: Moreno, R.
name: Ortiz, J. L.
name: Paubert, G.
name: Doressoundiram, A.
name: Peixinho, N.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report on coordinated thermal and optical measurements of trans-Neptunian object (20000) Varuna obtained in January-February 2002, respectively from the IRAM 30-m and IAA 1.5 m telescopes. The optical data show a lightcurve with a period of 3.176+/-0.010 hr, a mean V magnitude of 20.37+/-0.08 and a 0.42+/-0.01 magnitude amplitude. They also tentatively indicate that the lightcurve is asymmetric and double-peaked. The thermal observations indicate a 1.12+/-0.41 mJy flux, averaged over the object's rotation. Combining the two datasets, we infer that Varuna has a mean 1060(+180/-220) km diameter and a mean 0.038(+0.022/-0.010) V geometric albedo, in general agreement with an earlier determination using the same technique.
description: Accepted for publication in Astronomy & Astrophysics (7 pages, including 3 figures)
Gradient sub-grid-scale model for relativistic MHD Large Eddy Simulations
Creators: name: Carrasco, Federico
name: Viganò, Daniele
name: Palenzuela, Carlos
Publisher: name: arXiv
Year: 2019
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: MHD turbulence is likely to play an important role in several astrophysical scenarios where the magnetic Reynolds is very large. Numerically, these cases can be studied efficiently by means of Large Eddy Simulations, in which the computational resources are used to evolve the system only up to a finite grid size. The resolution is not fine enough to capture all the relevant small-scale physics at play, which is instead effectively modeled by a set of additional terms in the evolution equations, dubbed as sub-grid-scale model. Here we extend such approach, commonly used in non-relativistic/non-magnetic/incompressible fluid dynamics, applying the so-called gradient model to a general set of balance-law equations, that includes the relevant case in which a non-trivial inversion of conserved to primitive fields is needed. In particular, we focus on the relativistic compressible ideal MHD scenario, providing for the first time (and for any equation of state) all the additional sub-grid-scale terms. As an application, we consider box simulations of the relativistic Kelvin-Helmholtz instability, which is also the first mechanism responsible for the magnetic field amplification in binary neutron star mergers and cannot yet be fully captured by the finest-grid and longest simulations available. The performance of our model is numerically assessed by comparing it to the residuals arising from the filtering of high-resolution simulations. We find that the model can fit very well those residuals from resolutions a few times higher. Although the application shown here explicitly considers the Minkowski metric, it can be directly extended to general relativity, thus settling the basis to implement the gradient sub-grid model in a GRMHD binary merger. Our results suggest that this approach will be potentially able to unveil much better the small-scale dynamics achievable in full GRMHD simulations.
description: 15 pages, 6 figures. Final version. arXiv admin note: text overlap with arXiv:1904.04099
MOESM3 of â We are responsible for the violence, and prevention is up to usâ : a qualitative study of perceived risk factors for gender-based violence among Ethiopian university students
Creators: name: Kaufman, Michelle
name: Williams, Ashlie
name: Graziele Grilo
name: Marea, Christina
name: Fasil Fentaye
name: Lakew Gebretsadik
name: Shifera Yedenekal
Publisher: name: figshare
Year: 2019
Subjects: subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Science Policy
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Additional file 3. focus group guide for female students.