cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Eriesthis Burmeister 1844
Creators: name: Allsopp, Peter G.
name: Schoolmeesters, Paul
Publisher: name: Zenodo
Year: 2024
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Scarabaeidae
Eriesthis

description: Eriesthis Burmeister, 1844
[21 species].
Type species Eriesthis vestita Burmeister, 1844, by subsequent designation of Schein (1959).
Eriesthis: Dejean 1833. Unavailable name.
description: Published as part of Allsopp, Peter G. & Schoolmeesters, Paul, 2024, All genera of the world: Subfamilies Prototroginae, Cretoscarabaeinae, Dynamopodinae, Electrorubesopsinae, Phaenomeridinae, Orphninae, Allidiostomatinae, Aclopinae, Lichniinae, Melolonthinae, Oncerinae, Podolasiinae, Sericinae, Sericoidinae (Animalia: Arthropoda: Insecta: Coleoptera: Scarabaeidae), pp. 104-175 in Megataxa 12 (1) on page 114, DOI: 10.11646/megataxa.12.1.2, http://zenodo.org/record/14984437
Euknemoplia Lacroix 1997
Creators: name: Allsopp, Peter G.
name: Schoolmeesters, Paul
Publisher: name: Zenodo
Year: 2024
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Scarabaeidae
Euknemoplia

description: Euknemoplia Lacroix, 1997b
[4 species].
Type species Hoplia semisulphurea Fairmaire, 1900, by original designation.
description: Published as part of Allsopp, Peter G. & Schoolmeesters, Paul, 2024, All genera of the world: Subfamilies Prototroginae, Cretoscarabaeinae, Dynamopodinae, Electrorubesopsinae, Phaenomeridinae, Orphninae, Allidiostomatinae, Aclopinae, Lichniinae, Melolonthinae, Oncerinae, Podolasiinae, Sericinae, Sericoidinae (Animalia: Arthropoda: Insecta: Coleoptera: Scarabaeidae), pp. 104-175 in Megataxa 12 (1) on page 114, DOI: 10.11646/megataxa.12.1.2, http://zenodo.org/record/14984437
Additional file 1 of iPNHOT: a knowledge-based approach for identifying protein-nucleic acid interaction hot spots
Creators: name: Zhu, Xiaolei
name: Liu, Ling
name: He, Jingjing
name: Fang, Ting
name: Xiong, Yi
name: Mitchell, Julie C.
Publisher: name: figshare
Year: 2020
Subjects: subject: Biophysics
subject: Biochemistry
subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Chemical Sciences not elsewhere classified
subject: Biological Sciences not elsewhere classified
subject: Information Systems not elsewhere classified
subject: Cancer
subject: Inorganic Chemistry
subject: FOS: Chemical sciences

description: Additional file 1. Supplementary Materials for iPNHOT: A knowledge-based approach for identifying protein-nucleic acid interaction hot spots. This file provides more detailed data for protein-nucleic acids complexes, all the features generated in this study, and other tables for analysis and discussion. Table S1: Protein-nucleic acid complexes in the training dataset. Table S3: Protein-nucleic acid complexes in the independent test set. Table S5: All features generated for building our model to predict hotspot on protein-NA interfaces. Table S6: The numerical values of 10 different kinds of properties of the 20 amino acids. Table S7: Features selected and the corresponding cross validation performance in the SFS process. Table S8: The features selected and the corresponding cross validation performance in the SFS process based on the original 97 features. Description of Statistically analysis of the correlations between hotspots and different features: This section also includes 6 figures (Figure S1-S6) which visually show the results of the statistically analysis of the 20 features selected by decision tree.
Search for new physics with neutrinos at Radioactive Ion Beam facilities
Creators: name: Espinoza, Catalina
name: Lazauskas, Rimantas
name: Volpe, Cristina
Publisher: name: arXiv
Year: 2012
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We propose applications of Radioactive Ion Beam facilities to investigate physics beyond the Standard Model. In particular, we focus on the possible measurement of coherent neutrino-nucleus scattering and on a search for sterile neutrinos, by means of a low energy beta-beam with a Lorentz boost factor $γ\approx 1$. In the considered setup the collected radioactive ions are sent inside a 4$π$ detector. For the first application we provide the number of events associated with neutrino-nucleus coherent scattering, when the detector is filled in with a noble liquid. For the sterile search we consider that the spherical detector is filled in with a liquid scintillator, and that the neutrino detection channel is inverse-beta decay. We provide the exclusion curves for the sterile neutrino mixing parameters, based upon the 3+1 formalism, depending upon the achievable ion intensity. Our results are obtained both from total rates, and including spectral information with binning in energy and in distance. The proposed experiment represents a possible alternative to clarify the current anomalies observed in neutrino experiments.
description: 9 pages, 6 figures. v2 - added 2 figures
On the regional dose susceptibility of parotid gland function loss and recovery : an effort toward amelioration of radiotherapy-induced xerostomia
Creators: name: Clark, Haley
Publisher: name: University of British Columbia
Year: 2013

description: The introduction of intensity-modulated radiotherapy treatment has produced a small surplus of treatment planning flexibility compared to conventional techniques. Target volumes containing cancerous tumours are given a prescribed dose, but the surrounding normal tissue can sometimes be selectively irradiated. Therefore, as tissue-sparing techniques improve, the knowledge of complication risk in normal tissue becomes increasingly important. Xerostomia is one of the most common normal tissue complications in head-and-neck cancer patients. It refers to the non-distinct symptom of dry mouth. In the case of radiotherapy-induced xerostomia, it is generally due to the loss of salivary function resulting from radiation damage to the parotid parenchyma. In severe cases it can drastically reduce oral hygiene and is known to strongly detract from a patient's quality of life. We investigate the regional dose susceptibility of salivary function loss and recovery in the parotid gland with the intent of more precisely quantifying the risk of xerostomia. Reports have indicated regional dose susceptibility of loss in rat parotid glands. Similar results have been seen in human, though they seem to indicate primarily a morphological dependence on the shape of the dose distribution, not specific regional dependence. Further, they consider only subjective xerostomia, not objective salivary function loss nor recovery. The quantification of the regional dependence of loss and recovery of salivary function would substantially benefit our understanding of the complication risk of xerostomia. Immediate improvements in patient outcomes may follow. To this end, we investigate the functional relation between dose delivered to sub-segments of the parotid and whole mouth saliva measurements. To enable the investigation, we have developed a contour recognition system which is able to identify embedded planar organ contours with minimal human effort. Additionally, we have developed a sub-segmentation system capable of partitioning organ contours into arbitrarily-complex sub-segments.
Additional file 1: of Sleep duration and the risk of cancer: a systematic review and meta-analysis including doseâ response relationship
Creators: name: Chen, Yuheng
name: Tan, Fengwei
name: Wei, Luopei
name: Li, Xin
name: Lyu, Zhangyan
name: Feng, Xiaoshuang
name: Wen, Yan
name: Guo, Lanwei
name: He, Jie
name: Dai, Min
name: Li, Ni
Publisher: name: figshare
Year: 2018
Subjects: subject: Molecular Biology
subject: Physiology
subject: FOS: Biological sciences
subject: Pharmacology
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Science Policy

description: PRISMA 2009 Checklist. (DOCX 25Â kb)
Phase transition and scaling behavior of topological charged black holes in Horava-Lifshitz gravity
Creators: name: Majhi, Bibhas Ranjan
name: Roychowdhury, Dibakar
Publisher: name: arXiv
Year: 2012
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Gravity can be thought as an emergent phenomenon and it has a nice "thermodynamic" structure. In this context, it is then possible to study the thermodynamics without knowing the details of the underlying microscopic degrees of freedom. Here, based on the ordinary thermodynamics, we investigate the phase transition of the static, spherically symmetric charged black hole solution with arbitrary scalar curvature $2k$ in Hořava-Lifshitz gravity at the Lifshitz point $z=3$. The analysis is done using the canonical ensemble frame work; i.e. the charge is kept fixed. We find (a) for both $k=0$ and $k=1$, there is no phase transition, (b) while $k=-1$ case exhibits the second order phase transition within the {\it physical region} of the black hole. The critical point of second order phase transition is obtained by the divergence of the heat capacity at constant charge. Near the critical point, we find the various critical exponents. It is also observed that they satisfy the usual thermodynamic scaling laws.
description: Minor corrections, refs. added, to appear in Class. Quant. Grav. arXiv admin note: text overlap with arXiv:1111.0973 by other authors
Acoustic waves: should they be propagated forward in time, or forward in space?
Creators: name: Kinsler, Paul
Publisher: name: arXiv
Year: 2012
Subjects: subject: Classical Physics (physics.class-ph)
subject: FOS: Physical sciences

description: The evolution of acoustic waves can be evaluated in two ways: either as a temporal, or a spatial propagation. Propagating in space provides the considerable advantage of being able to handle dispersion and propagation across interfaces with remarkable efficiency; but propagating in time is more physical and gives correctly behaved reflections and scattering without effort. Which should be chosen in a given situation, and what compromises might have to be made? Here the natural behaviors of each choice of propagation are compared and contrasted for an ordinary second order wave equation, the time-dependent diffusion wave equation, an elastic rod wave equation, and the Stokes'/ van Wijngaarden's equations, each case illuminating a characteristic feature of the technique. Either choice of propagation axis enables a partitioning the wave equation that gives rise to a directional factorization based on a natural "reference" dispersion relation. The resulting exact coupled bidirectional equations then reduce to a single unidirectional first-order wave equation using a simple "slow evolution" assumption that minimizes effect of subsequent approximations, while allowing a direct term-to-term comparison between exact and approximate theories.
description: 12 pages, v2 corrected
Dohrniphora seriata Kung & Brown, 2006: 1939 - 1941
Creators: name: Brown, Brian V.
name: Kung, Giar-Ann
Publisher: name: Zenodo
Year: 2010
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Phoridae
Dohrniphora
Dohrniphora seriata

description: Dohrniphora seriata group
 Diagnosis. Peglike setae in small basal line or group. The extra pair of scutellar setae might be a synapomorphy as well, if they arose independently in the apparently unrelated D. scutellaris.
 Included species. This possibly monophyletic group includes D. hexaseta, D. lafondaensis, D. seriata, and D. sexspinosa.
description: Published as part of Brown, Brian V. & Kung, Giar-Ann, 2010, 2699, pp. 1-142 in Zootaxa 2699 on page 17
Eulaiades Fairmaire 1899
Creators: name: Allsopp, Peter G.
name: Schoolmeesters, Paul
Publisher: name: Zenodo
Year: 2024
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Scarabaeidae
Eulaiades

description: Eulaiades Fairmaire, 1899
[5 species].
Type species Eulaiades inflatipes Fairmaire, 1899, by monotypy.
description: Published as part of Allsopp, Peter G. & Schoolmeesters, Paul, 2024, All genera of the world: Subfamilies Prototroginae, Cretoscarabaeinae, Dynamopodinae, Electrorubesopsinae, Phaenomeridinae, Orphninae, Allidiostomatinae, Aclopinae, Lichniinae, Melolonthinae, Oncerinae, Podolasiinae, Sericinae, Sericoidinae (Animalia: Arthropoda: Insecta: Coleoptera: Scarabaeidae), pp. 104-175 in Megataxa 12 (1) on page 114, DOI: 10.11646/megataxa.12.1.2, http://zenodo.org/record/14984437
Electron performance measurements with the ATLAS detector using the 2010 LHC proton-proton collision data
Creators: name: ATLAS Collaboration
Publisher: name: arXiv
Year: 2011
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: Detailed measurements of the electron performance of the ATLAS detector at the LHC are reported, using decays of the Z, W and J/psi particles. Data collected in 2010 at sqrt(s)=7 TeV are used, corresponding to an integrated luminosity of almost 40 pb^-1. The inter-alignment of the inner detector and the electromagnetic calorimeter, the determination of the electron energy scale and resolution, and the performance in terms of response uniformity and linearity are discussed. The electron identification, reconstruction and trigger efficiencies, as well as the charge misidentification probability, are also presented.
description: 34 pages plus author list (46 pages total), 24 figures, 12 tables, matches published version in EPJC
The Convenient Setting for Denjoy--Carleman Differentiable Mappings of Beurling and Roumieu Type
Creators: name: Kriegl, Andreas
name: Michor, Peter W.
name: Rainer, Armin
Publisher: name: arXiv
Year: 2011
Subjects: subject: Functional Analysis (math.FA)
subject: Classical Analysis and ODEs (math.CA)
subject: FOS: Mathematics
subject: 26E10, 46A17, 46E50, 58B10, 58B25, 58C25, 58D05, 58D15

description: We prove in a uniform way that all Denjoy--Carleman differentiable function classes of Beurling type $C^{(M)}$ and of Roumieu type $C^{\{M\}}$, admit a convenient setting if the weight sequence $M=(M_k)$ is log-convex and of moderate growth: For $\mathcal C$ denoting either $C^{(M)}$ or $C^{\{M\}}$, the category of $\mathcal C$-mappings is cartesian closed in the sense that $\mathcal C(E,\mathcal C(F,G))\cong \mathcal C(E\times F, G)$ for convenient vector spaces. Applications to manifolds of mappings are given: The group of $\mathcal C$-diffeomorphisms is a regular $\mathcal C$-Lie group if $\mathcal C \supseteq C^ω$, but not better.
description: 41 pages; numbering changed in order to make it consistent with the published version; to appear in Rev. Mat. Complut. arXiv admin note: text overlap with arXiv:0909.5632
Comparison Between Turbulent Helical Dynamo Simulations and a Nonlinear Three-Scale Theory
Creators: name: Park, Kiwan
name: Blackman, E. G.
Publisher: name: arXiv
Year: 2011
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Plasma Physics (physics.plasm-ph)
subject: FOS: Physical sciences

description: Progress toward understanding principles of nonlinear growth and saturation of large scale magnetic fields has emerged from comparison of theoretical models that incorporate the evolution of magnetic helicity with numerical simulations for problems that are more idealized than expected in astrophysical circumstances, but still fully non-linear. We carry out a new comparison of this sort for the magnetic field growth from forced isotropic helical turbulence in a periodic box. Previous comparisons be- tween analytic theory and simulations of this problem have shown that a two-scale model compares well with the simulations in agreeing that the driver of large scale field growth is the difference between kinetic and current helicities associated with the small scale field, and that the backreaction that slows the growth of the large scale field as the small scale current helicity grows. However, the two-scale model artificially re- stricts the small scale current helicity to reside at the same scale as the driving kinetic helicity. In addition, previous comparisons have focused on the late time saturation regime, and less on the early-time growth regime. Here we address these issues by comparing a three scale model to new simulations for both early and late time growth regimes. We find that the minimalist extension to three scales provides a better model for the field evolution than the two-scale model because the simulations show that the small scale current helicity does not reside at the same scale as that of the driving kinetic helicity. The simulations also show that the peak of the small scale current helicity migrates toward lower wave numbers as the growth evolves from the fast to saturated growth regimes.
description: This paper has been withdrawn by the author due to some typos
Fairmairoplia Lacroix 1997
Creators: name: Allsopp, Peter G.
name: Schoolmeesters, Paul
Publisher: name: Zenodo
Year: 2024
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Scarabaeidae
Fairmairoplia

description: Fairmairoplia Lacroix, 1997b
[12 species].
Type species Hoplia plicata Fairmaire, 1903, by original designation.
description: Published as part of Allsopp, Peter G. & Schoolmeesters, Paul, 2024, All genera of the world: Subfamilies Prototroginae, Cretoscarabaeinae, Dynamopodinae, Electrorubesopsinae, Phaenomeridinae, Orphninae, Allidiostomatinae, Aclopinae, Lichniinae, Melolonthinae, Oncerinae, Podolasiinae, Sericinae, Sericoidinae (Animalia: Arthropoda: Insecta: Coleoptera: Scarabaeidae), pp. 104-175 in Megataxa 12 (1) on page 114, DOI: 10.11646/megataxa.12.1.2, http://zenodo.org/record/14984437
Effect of radiative transfer on damped Lyman-alpha and Lyman limit systems in cosmological SPH simulations
Creators: name: Yajima, Hidenobu
name: Choi, Jun-Hwan
name: Nagamine, Kentaro
Publisher: name: arXiv
Year: 2011
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We study the effect of local stellar radiation and UVB on the physical properties of DLAs and LLSs at z=3 using cosmological SPH simulations. We post-process our simulations with the ART code for radiative transfer of local stellar radiation and UVB. We find that the DLA and LLS cross sections are significantly reduced by the UVB, whereas the local stellar radiation does not affect them very much except in the low-mass halos. This is because clumpy high-density clouds near young star clusters effectively absorb most of the ionizing photons from young stars. We also find that the UVB model with a simple density threshold for self-shielding effect can reproduce the observed column density distribution function of DLAs and LLSs very well, and we validate this model by direct radiative transfer calculations of stellar radiation and UVB with high angular resolution. We show that, with a self-shielding treatment, the DLAs have an extended distribution around star-forming regions typically on ~ 10-30 kpc scales, and LLSs are surrounding DLAs on ~ 30-60 kpc scales. Our simulations suggest that the median properties of DLA host haloes are: Mh = 2.4*10^10 Msun, SFR = 0.3 Msun/yr, M* = 2.4*10^8 Msun, and Z/Zsun = 0.1. About 30 per cent of DLAs are hosted by haloes having SFR = 1 - 20 Msun/yr, which is the typical SFR range for LBGs. More than half of DLAs are hosted by the LBGs that are fainter than the current observational limit. Our results suggest that fractional contribution to LLSs from lower mass haloes is greater than for DLAs. Therefore the median values of LLS host haloes are somewhat lower with Mh = 9.6*10^9 Msun, SFR = 0.06 Msun/yr, M* = 6.5*10^7 Msun and Z/Zsun = 0.08. About 80 per cent of total LLS cross section are hosted by haloes with SFR < 1 Msun/yr, hence most LLSs are associated with low-mass halos with faint LBGs below the current detection limit.
description: 18 pages, 12 figures, accepted for publication in MNRAS
Goniaspidius Burmeister 1844
Creators: name: Allsopp, Peter G.
name: Schoolmeesters, Paul
Publisher: name: Zenodo
Year: 2024
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Scarabaeidae
Goniaspidius

description: Goniaspidius Burmeister, 1844 (not Goniaspidius Péringuey, 1902)
[2 species].
Type species Goniaspidius brevis Burmeister, 1844, by subsequent designation of Lucas (1920).
description: Published as part of Allsopp, Peter G. & Schoolmeesters, Paul, 2024, All genera of the world: Subfamilies Prototroginae, Cretoscarabaeinae, Dynamopodinae, Electrorubesopsinae, Phaenomeridinae, Orphninae, Allidiostomatinae, Aclopinae, Lichniinae, Melolonthinae, Oncerinae, Podolasiinae, Sericinae, Sericoidinae (Animalia: Arthropoda: Insecta: Coleoptera: Scarabaeidae), pp. 104-175 in Megataxa 12 (1) on page 114, DOI: 10.11646/megataxa.12.1.2, http://zenodo.org/record/14984437
Global Gyrokinetic Simulation of Tokamak Edge Pedestal Instabilities
Creators: name: Wan, Weigang
name: Parker, Scott E.
name: Chen, Yang
name: Yan, Zheng
name: Groebner, Richard J.
name: Snyder, Philip B.
Publisher: name: arXiv
Year: 2012
Subjects: subject: Plasma Physics (physics.plasm-ph)
subject: FOS: Physical sciences

description: Global electromagnetic gyrokinetic simulations show the existence of near threshold conditions for both a high-$n$ kinetic ballooning mode (KBM) and an intermediate-$n$ kinetic version of peeling-ballooning mode (KPBM) in the edge pedestal of two DIII-D H-mode discharges. When the magnetic shear is reduced in a narrow region of steep pressure gradient, the KPBM is significantly stabilized, while the KBM is weakly destabilized and hence becomes the most-unstable mode. Collisions decrease the KBM's critical $β$ and increase the growth rate.
description: 4 pages, 6 figures
Aluminium in an ocean general circulation model compared with the West Atlantic Geotraces cruises
Creators: name: van Hulten, Marco
name: Sterl, Andreas
name: Tagliabue, Alessandro
name: Dutay, Jean-Claude
name: Gehlen, Marion
name: de Baar, Hein J. W.
name: Middag, Rob
Publisher: name: arXiv
Year: 2012
Subjects: subject: Atmospheric and Oceanic Physics (physics.ao-ph)
subject: FOS: Physical sciences

description: A model of aluminium has been developed and implemented in an Ocean General Circulation Model (NEMO-PISCES). In the model, aluminium enters the ocean by means of dust deposition. The internal oceanic processes are described by advection, mixing and reversible scavenging. The model has been evaluated against a number of selected high-quality datasets covering much of the world ocean, especially those from the West Atlantic Geotraces cruises of 2010 and 2011. Generally, the model results are in fair agreement with the observations. However, the model does not describe well the vertical distribution of dissolved Al in the North Atlantic Ocean. The model may require changes in the physical forcing and the vertical dependence of the sinking velocity of biogenic silica to account for other discrepancies. To explore the model behaviour, sensitivity experiments have been performed, in which we changed the key parameters of the scavenging process as well as the input of aluminium into the ocean. This resulted in a better understanding of aluminium in the ocean, and it is now clear which parameter has what effect on the dissolved aluminium distribution and which processes might be missing in the model, among which boundary scavenging and biological incorporation of aluminium into diatoms.
description: J. Mar. Syst. (2012), ISSN 0924-7963. 22 pages, 30 figures, on the occasion of the May 2011 GEOTRACES colloquium
Observation of a narrow structure in p(gamma,K_s)X via interference with phi-meson production
Creators: name: Amaryan, M. J.
name: Gavalian, G.
name: Nepali, C.
name: Polyakov, M. V.
name: Azimov, Ya.
name: Briscoe, W. J.
name: Dodge, G. E.
name: Hyde, C. E.
name: Klein, F.
name: Kuznetsov, V.
name: Strakovsky, I.
name: Zhang, J.
Publisher: name: arXiv
Year: 2011
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: We report observation of a narrow peak structure at ~1.54 GeV with a Gaussian width sigma=6 MeV in the missing of K_s in the reaction gamma+p = pK_sK_L. The observed structure may be due to the interference between a strange (or anti-strange) baryon resonance in the pK_L system and the phi(K_sK_L) photoproduction leading to the same final state. The statistical significance of the observed excess of events estimated as the log likelihood ratio of the resonant signal+background hypothesis and the phi-production based background only hypothesis corresponds to 5.3 sigma.
description: Accepted for publication in Physical Review C, 9 pages, 11 figures, 1 table added, revised
Gouna Peringuey 1902
Creators: name: Allsopp, Peter G.
name: Schoolmeesters, Paul
Publisher: name: Zenodo
Year: 2024
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Scarabaeidae
Gouna

description: Gouna Péringuey, 1902
[3 species].
Type species Gymnoloma lineolata Burmeister, 1844, by subsequent designation of Dombrow in Dombrow et al. (2022).
description: Published as part of Allsopp, Peter G. & Schoolmeesters, Paul, 2024, All genera of the world: Subfamilies Prototroginae, Cretoscarabaeinae, Dynamopodinae, Electrorubesopsinae, Phaenomeridinae, Orphninae, Allidiostomatinae, Aclopinae, Lichniinae, Melolonthinae, Oncerinae, Podolasiinae, Sericinae, Sericoidinae (Animalia: Arthropoda: Insecta: Coleoptera: Scarabaeidae), pp. 104-175 in Megataxa 12 (1) on page 114, DOI: 10.11646/megataxa.12.1.2, http://zenodo.org/record/14984437
Dohrniphora hexaseta Brown & Kung 2010, sp. n.
Creators: name: Brown, Brian V.
name: Kung, Giar-Ann
Publisher: name: Zenodo
Year: 2010
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Diptera
Phoridae
Dohrniphora
Dohrniphora hexaseta

description: Dohrniphora hexaseta sp. n.
(Figs 17–18)
 Species recognition. This species is most similar to D. seriata, from which it differs by the emargination of the ventral margin of the hind femur, basal to the peglike setae, as well as the position and shape of the basal tooth.
Description. Body length: 1.88–2.38 mm. Head: Frons dark brown, second row of setae slightly concave. Flagellomere 1 round to rounded-oval, brown. Palpus of normal size, yellow. Thorax: Scutum brown, darker posteriorly. Scutellum dark brown, with 3 pairs of setae; middle pair longest; anterior seta one-third length of middle seta; posterior seta one-half length of middle seta. Pleuron light brown. Mean costal length 0.54 wing length, range 0.53–0.54. Halter light brown. Legs yellowish-brown, darker on dorsal margin and apex of hind femur. Forecoxa in lateral view yellowish-brown. Foretibia with 3–4 dorsal setae. Foretarsomeres slender, elongate. Midcoxa yellowish-brown. Hind coxa yellowish-brown. Hind coxal lobe yellow, short, narrow, dorsally curved. Posterior face of hind femur with short row of peglike setae; ventral margin of hind femur emarginate basal to peglike setae; with broad basal tooth at mid-depth (Figs 17–18). Abdomen: Abdominal tergite 1 light brown, tergites 2–6 dark brown with lighter posterior seam. Venter of abdomen gray, with few longer setae on segment 5. Male terminalia brown, cercus yellow.
Distribution. Colombia and Mexico.
 Derivation of specific epithet. From Greek hex for six, referring to the six scutellar setae.
Holotype. ♂, COLOMBIA: Magdalena: PNN Tayrona, Neguanje, 11.33°N, 74.03°W, 21.ii–5.iii.2001, R. Henriquez, Malaise trap CAP-1351, 10 m [LACM ENT 180860] (IAVH).
Paratypes. COLOMBIA: Cauca: Isla Gorgona, 2.97°N, 78.18°W, 1♂, 1–4.iii.2000, B. Brown, G. Kung, M. Sharkey, Malaise trap #11 (LACM); Magdalena: PNN Tayrona, Neguanje, 11.33°N, 74.03°W, 7♂ 21.ii– 5.iii.2001, R. Henriquez, Malaise trap CAP-1351, 10 m (LACM, IAVH). MEXICO: Jalisco: Puerto Vallarta, 1♂, 15.xii.1987, G. E. Bohart (EMUS).
Other material examined. 32♂ specimens from the type locality, but 5–21.iii.2001, R. Henriquez, Malaise trap CAP-1481 (EMUS, IAVH, LACM, MCZC, USNM).
description: Published as part of Brown, Brian V. & Kung, Giar-Ann, 2010, 2699, pp. 1-142 in Zootaxa 2699 on pages 17-19
Total Hadronic Cross Section Data and the Froissart-Martin Bound
Creators: name: Fagundes, D. A.
name: Menon, M. J.
name: Silva, P. V. R. G.
Publisher: name: arXiv
Year: 2011
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: The energy dependence of the total hadronic cross section at high energies is investigated with focus on the recent experimental result by the TOTEM Collaboration at 7 TeV and the Froissart-Martin bound. On the basis of a class of analytical parametrization with the exponent $γ$ in the leading logarithm contribution as a free parameter, different variants of fits to $pp$ and $\bar{p}p$ total cross section data above 5 GeV are developed. Two ensembles are considered, the first comprising data up to 1.8 TeV, the second also including the data collected at 7 TeV. We shown that in all fit variants applied to the first ensemble the exponent is statistically consistent with $γ$ = 2. Applied to the second ensemble, however, the same variants yield $γ$'s above 2, a result already obtained in two other analysis, by U. Amaldi \textit{et al}. and by the UA4/2 Collaboration. As recently discussed by Ya. I. Azimov, this faster-than-squared-logarithm rise does not necessarily violate unitarity. Our results suggest that the energy dependence of the hadronic total cross section at high energies still constitute an open problem.
description: 20 pages, 10 figures, introduction extended and general references added to match editorial style, to appear in the Brazilian Journal of Physics
Two kinds of peaked solitary waves of the KdV, BBM and Boussinesq equations
Creators: name: Liao, Shijun
Publisher: name: arXiv
Year: 2012
Subjects: subject: Pattern Formation and Solitons (nlin.PS)
subject: FOS: Physical sciences

description: It is well-known that the celebrated Camassa-Holm equation has the peaked solitary waves, which have been not reported for other mainstream models of shallow water waves. In this letter, the closed-form solutions of peaked solitary waves of the KdV equation, the BBM equation and the Boussinesq equation are given for the first time. All of them have either a peakon or an anti-peakon. Each of them exactly satisfies the corresponding Rankine-Hogoniot jump condition and should be understood as weak solution. Therefore, the peaked solitary waves might be common for most of shallow water wave models, no matter whether or not they are integrable and/or admit breaking-wave solutions.
description: 13 pages, 2 figures, accepted by Science China - Physics, Mechanics & Astronomy
Grammodoplia Lacroix 1997
Creators: name: Allsopp, Peter G.
name: Schoolmeesters, Paul
Publisher: name: Zenodo
Year: 2024
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Scarabaeidae
Grammodoplia

description: Grammodoplia Lacroix, 1997b
[1 species].
Type species Hoplia asperata Fairmaire, 1903, by original designation.
description: Published as part of Allsopp, Peter G. & Schoolmeesters, Paul, 2024, All genera of the world: Subfamilies Prototroginae, Cretoscarabaeinae, Dynamopodinae, Electrorubesopsinae, Phaenomeridinae, Orphninae, Allidiostomatinae, Aclopinae, Lichniinae, Melolonthinae, Oncerinae, Podolasiinae, Sericinae, Sericoidinae (Animalia: Arthropoda: Insecta: Coleoptera: Scarabaeidae), pp. 104-175 in Megataxa 12 (1) on page 114, DOI: 10.11646/megataxa.12.1.2, http://zenodo.org/record/14984437
Manipulation of the motion of polyatomic molecules in the rotational ground state : microwave lens effect by AC Stark dipole force
Creators: name: Zhong, Wei
Publisher: name: University of British Columbia
Year: 2013

description: The main contribution of this project to the field of cold and ultracold molecules is we firstly demonstrated successful manipulation of the motion of polyatomic molecular beam in the rotational ground state, which has the lowest temperature of all possible states. Chapter 1 gives a summary of this field, including the application of cold and ultracold molecules, the methods to obtain them, and each method’s advantages and disadvantages. Once we decelerate molecular ensembles, we would like to trap the cold and ultracold molecules in electric trap, megnetic trap and megneto-optical trap. Chapter 2 starts with an introduction of the concept of supersonic beam and the basic knowledge of it, such as the specific features. The experimental setup will also be presented and explained in this chapter. The main highlight of this project is that we are manipulating molecules in the real ground state. Our molecular source is a Counter Rotating Nozzle(CRN), which can precool (or slow in alternate terminology) molecules in all states including the rotational ground state. The principle and performance of CRN will be presented and explained in Chapter 3. After obtaining a well precooled molecular beam, the microwave lens effect on various species is presented in Chapter 4. Meanwhile, the principle of AC Stark shift, AC dipole force and the microwave standing wave modes, such as TE modes and TM modes, will be explained in this chapter as well. Finally, I’ll summarize, draw conclusion of this work and describe the future expectation of this project in Chapter 5.
Massive gravity from bimetric gravity
Creators: name: Baccetti, Valentina
name: Martin-Moruno, Prado
name: Visser, Matt
Publisher: name: arXiv
Year: 2012
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We discuss the subtle relationship between massive gravity and bimetric gravity, focusing particularly on the manner in which massive gravity may be viewed as a suitable limit of bimetric gravity. The limiting procedure is more delicate than currently appreciated. Specifically, this limiting procedure should not unnecessarily constrain the background metric, which must be externally specified by the theory of massive gravity itself. The fact that in bimetric theories one always has two sets of metric equations of motion continues to have an effect even in the massive gravity limit, leading to additional constraints besides the one set of equations of motion naively expected. Thus, since solutions of bimetric gravity in the limit of vanishing kinetic term are also solutions of massive gravity, but the contrary statement is not necessarily true, there is not complete continuity in the parameter space of the theory. In particular, we study the massive cosmological solutions which are continuous in the parameter space, showing that many interesting cosmologies belong to this class.
description: v1: 25 pages; v2: 6 references added, discussion streamlined; v3: 24 pages, 20 references added, section 2 summarized, new comments added to section 3, conclusions improved but unchanged. This version accepted for publication in Classical and Quantum Gravity
X-ray absorption and resonant inelastic X-ray scattering calculations with ligand field single cluster method on praseodymium nickel oxide
Creators: name: Balandeh, Shadi
Publisher: name: University of British Columbia
Year: 2013

description: RNiO3 perovskites (R=rare earth) are one of the most interesting compounds in condensed matter physics presenting various unusual physical properties. The detailed electronic structure of these materials are very controversial at the present time. The charge transfer energy and the d-d Coulomb interaction are the two very important parameters which can explain their electronic behaviours nicely. However, predicting their values has been a challenge to the science society so far. X-ray Absorption Spectroscopy (XAS) and Resonant Inelastic Scattering (RIXS) are the two very useful techniques to probe the electronic structure of a solid state system in general and predict these two energies in particular. In this thesis Multiplet Ligand Field Cluster Calculation (MLFCC) is used to calculate these two spectra, then the charge transfer energy (Δ), the covalent hopping integral(pds), and the d-d Coulomb repulsion energy Udd are obtained by fitting the calculated spectra to the experiment. In this work, the calculated XAS results are compared with the experiment and the adjusted values are introduced as Δ=2.5eV , pds=-1.9eV, Udd=7.5eV and 10Dq=0.5 eV. The low spin to high spin transition is also studied and the critical charge transfer energies and covalent hopping integrals are calculated at which the abrupt transition happens. It is also found that in almost all low spin cases the d8L9 configuration has the largest contribution to the ground state. Since the best fit of XAS is not satisfactory and displays considerable differences with the experiment, the study is followed with the RIXS calculations. Finally, the calculated RIXS results for different polarizations are compared with the experiment.It results in a smaller Δ=0.8eV and a smaller absolute value of pds=-1.4eV at which the double peak structure in XAS L3 vanishes. This could be an evidence to the fact that XAS should not be interpreted in the conventional way and the Δ should not be fitted to keep the double peak which probably has another source than the multiplet structure.
Switching nonlinearity in a superconductor-enhanced metamaterial
Creators: name: Kurter, Cihan
name: Tassin, Philippe
name: Zhuravel, Alexander P.
name: Zhang, Lei
name: Koschny, Thomas
name: Ustinov, Alexey V.
name: Soukoulis, Costas M.
name: Anlage, Steven M.
Publisher: name: arXiv
Year: 2011
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: Superconductivity (cond-mat.supr-con)
subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: We demonstrate a nonlinear metamaterial that can be switched between low and high transmission by controlling the power level of the incident beam. The origin of this nonlinear response is the superconducting Nb thin film employed in the metamaterial structure. We show that with moderate RF power of about 22 dBm it is possible to quench the superconducting state as a result of extremely strong current densities at the corners of the metamaterial's split-ring resonators. We measure a transmission contrast of 10 dB and a change in group delay of 70 ns between the low and high power states.
description: 4 pages, 4 figures
Additional file 2: of Sleep duration and the risk of cancer: a systematic review and meta-analysis including doseâ response relationship
Creators: name: Chen, Yuheng
name: Tan, Fengwei
name: Wei, Luopei
name: Li, Xin
name: Lyu, Zhangyan
name: Feng, Xiaoshuang
name: Wen, Yan
name: Guo, Lanwei
name: He, Jie
name: Dai, Min
name: Li, Ni
Publisher: name: figshare
Year: 2018
Subjects: subject: Medicine
subject: Physiology
subject: FOS: Biological sciences
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Science Policy

description: Characteristics of studies included in the meta-analysis. (DOCX 39Â kb)
Gymnoloma Dejean 1833
Creators: name: Allsopp, Peter G.
name: Schoolmeesters, Paul
Publisher: name: Zenodo
Year: 2024
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Scarabaeidae
Gymnoloma

description: Gymnoloma Dejean, 1833
[12 species].
Type species Melolontha atomaria Fabricius, 1781, by monotypy.
description: Published as part of Allsopp, Peter G. & Schoolmeesters, Paul, 2024, All genera of the world: Subfamilies Prototroginae, Cretoscarabaeinae, Dynamopodinae, Electrorubesopsinae, Phaenomeridinae, Orphninae, Allidiostomatinae, Aclopinae, Lichniinae, Melolonthinae, Oncerinae, Podolasiinae, Sericinae, Sericoidinae (Animalia: Arthropoda: Insecta: Coleoptera: Scarabaeidae), pp. 104-175 in Megataxa 12 (1) on page 114, DOI: 10.11646/megataxa.12.1.2, http://zenodo.org/record/14984437
Nonrelativistic quantum dynamics on a cone with and without a constraining potential
Creators: name: Filgueiras, C.
name: Silva, E. O.
name: Andrade, F. M.
Publisher: name: arXiv
Year: 2012
Subjects: subject: Quantum Physics (quant-ph)
subject: High Energy Physics - Theory (hep-th)
subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: In this paper we investigate the bound state problem of nonrelativistic quantum particles on a conical surface. This kind of surface appears as a topological defect in ordinary semiconductors as well as in graphene sheets. Specifically, we compare and discuss the results stemming from two different approaches. In the first one, it is assumed that the charge carriers are bound to the surface by a constraining potential, while the second one is based on the Klein-Gordon type equation on surfaces, without the constraining potential. The main difference between both theories is the presence/absence of a potential which contains the mean curvature of a given surface. This fact changes the dependence of the bound states on the angular momentum $l$. Moreover, there are bound states that are absent in the Klein-Gordon theory, which instead appear in the Schrödinger one.
description: Accepted for publication in Journal of Mathematical Physics, 14 pages, 1 figure
Project Dissemination and Communication Plan (D6.1 )
Creators: name: Javier Fernandez Hidalgo,
name: Sanjuan, Jose Miguel
name: Shuaib Siddiqui
Publisher: name: Zenodo
Year: 2019
Subjects: 5g
dissemination

description: This deliverable provides an exhaustive dissemination plan that will be used as guideline during the project and structures a first set of actions that will be implemented during the project. The ultimate objective of this plan is to coordinate the effort of the partners and to implement a coherent and uniform message to the different stakeholders.
Gyroplia Brenske 1894
Creators: name: Allsopp, Peter G.
name: Schoolmeesters, Paul
Publisher: name: Zenodo
Year: 2024
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Scarabaeidae
Gyroplia

description: Gyroplia Brenske, 1894c
[1 species].
Type species Gyroplia bimaculata Brenske, 1894, by monotypy.
description: Published as part of Allsopp, Peter G. & Schoolmeesters, Paul, 2024, All genera of the world: Subfamilies Prototroginae, Cretoscarabaeinae, Dynamopodinae, Electrorubesopsinae, Phaenomeridinae, Orphninae, Allidiostomatinae, Aclopinae, Lichniinae, Melolonthinae, Oncerinae, Podolasiinae, Sericinae, Sericoidinae (Animalia: Arthropoda: Insecta: Coleoptera: Scarabaeidae), pp. 104-175 in Megataxa 12 (1) on page 114, DOI: 10.11646/megataxa.12.1.2, http://zenodo.org/record/14984437
Mass assembly of galaxies: Smooth accretion versus mergers
Creators: name: L'Huillier, Benjamin
name: Combes, Francoise
name: Semelin, Benoit
Publisher: name: arXiv
Year: 2011
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Galaxies accrete their mass by means of both smooth accretion from the cosmic web, and the mergers of smaller entities. We wish to quantify the respective role of these two modes of accretion, which could determine the morphological types of galaxies observed today. Multi-zoom cosmological simulations are used to estimate as a function of time the evolution of mass in bound systems, for dark matter as well as baryons. The baryonic contents of dark matter haloes are studied. Merger histories are followed as a function of external density, and the different ways in which mass is assembled in galaxies and the stellar component accumulated are quantified. We find that most galaxies assemble their mass through smooth accretion, and only the most massive galaxies also grow significantly through mergers. The mean fraction of mass assembled by accretion is 77 %, and by mergers 23 %. We present typical accretion histories of hundreds of galaxies: masses of the most massive galaxies increase monotonically in time, mainly through accretion, many intermediate-mass objects also experience mass-loss events such as tidal stripping and evaporation. However, our simulations suffer from the overcooling of massive galaxies caused by the neglect of active galaxy nuclei (AGN) feedback. The time by which half of the galay mass has assembled, both in dark matter and baryons, is a decreasing function of mass, which is compatible with the observations of a so-called downsizing. At every epoch in the universe, there are low-mass galaxies actively forming stars, while more massive galaxies form their stars over a shorter period of time within half the age of the universe.
description: A&A Accepted, 19 pages, 17 figures
Supplementary Information from A discordance of seasonally covarying cues uncovers misregulated phenotypes in the heterophyllous pitcher plant Cephalotus follicularis
Creators: name: FUKUSHIMA, Kenji
name: Narukawa, Hideki
name: Palfalvi, Gergo
name: Hasebe, Mitsuyasu
Publisher: name: The Royal Society
Year: 2021
Subjects: subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: Plant Biology

description: Supplementary Texts 1-2; Supplementary Methods; Figs. S1–S12; Supplementary References
Fluctuating noise drives Brownian transport
Creators: name: Hasegawa, Yoshihiko
name: Arita, Masanori
Publisher: name: arXiv
Year: 2011
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: The transport properties of Brownian ratchet was studied in the presence of stochastic intensity noise (SIN) in both overdamped and underdamped regimes. In the overdamped case, analytical solution using the matrix continued fraction method revealed the existence of a maximum current when the noise intensity fluctuates on intermediate time scale regions. Similar effects were observed for the underdamped case by Monte Carlo simulations. The optimal time-correlation for the Brownian transport coincided with the experimentally observed time-correlation of the extrinsic noise in Esherichia coli gene expression and implied the importance of environmental noise for molecular mechanisms.
description: 22 pages, 8 figures
Global one-sample tests for high-dimensional covariance matrices
Creators: name: Wang, Xiaoyi
name: Liu, Baisen
name: Shi, Ning-Zhong
name: Tian, Guo-Liang
name: Zheng, Shurong
Publisher: name: Taylor & Francis
Year: 2021
Subjects: subject: Biochemistry
subject: Cell Biology
subject: Biotechnology
subject: Chemical Sciences not elsewhere classified
subject: Ecology
subject: FOS: Biological sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Mathematical Sciences not elsewhere classified
subject: Marine Biology
subject: Cancer
subject: Infectious Diseases
subject: FOS: Health sciences

description: Testing high-dimensional covariance matrix plays an important role in multivariate statistical analysis. Many statisticians used the statistics based on tr[(ΣΣ0−1−Ip)2] to test H0:Σ=Σ0 with Σ being the covariance matrix. However, none have proposed a statistic based on tr[(Σ−Σ0)2] for this purpose. In fact, neither of the two tests is superior to the other based on their powers because they target different kinds of dense alternatives. Furthermore, some maximum-type tests were proposed to accommodate sparse alternatives. By using the advantages of these tests, we propose two new tests for one-sample covariance matrix when the sample size and data dimension increase proportionally. One is suitable for dense alternatives, the other is powerful against a wide range of situations, such as dense, sparse or a mixture of both alternatives. Extensive simulation results show that our proposed tests maintain high powers against various alternatives while the existing tests fail in at least one situation.