cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Antiferromagnetism and spin density waves in 3D Dirac semimetals
Creators: name: Bednik, Grigory
Publisher: name: arXiv
Year: 2019
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Materials Science (cond-mat.mtrl-sci)
subject: Other Condensed Matter (cond-mat.other)
subject: FOS: Physical sciences

description: We perform mean-field study of possible magnetic instabilities in Dirac semimetals. We find that Dirac electrons naturally host antiferromagnetic or spin density wave ground states, though their specific configurations may vary depending on specific model, as well as chemical potential and temperature. We also discuss paramagnetic susceptibility of Dirac semimetals. In the cases, when Dirac electrons do not have orbital momentum, the magnetic properties may be $μ$ and $T$ independent.
description: 12 pages
Gallup Poll # 681
Creators: name: Gallup
Publisher: name: Roper Center for Public Opinion Research
Year: 2021

description: Most admired woman in the world (2); most admired man in the world (2); Lyndon Johnson job performance (1); Johnson more/less favorable than Kennedy toward labor unions (1); Johnson more/less favorable than Kennedy toward business (1); possible 1964 presidential candidates (10); registered to vote (1); ever voted in district/precinct (1); 1964 presidential election (2); wrote to Congressman/Senator in last twelve months (1); attend religious services (3); ever pray (2); think people can/cannot be good Christians if they don't go to church (1); favour/oppose gun law requiring a person to get police permit before buying a gun (1); how often go out at various times of day/evening (3); 1960 presidential election (1).
Heat flow reversals without reversing the arrow of time: the role of internal quantum coherences and correlations
Creators: name: Latune, Camille L.
name: Sinayskiy, Ilya
name: Petruccione, Francesco
Publisher: name: arXiv
Year: 2019
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: One of the stunning consequences of quantum correlations in thermodynamics is the reversal of the arrow of time, recently shown experimentally in [K. Micadei, et al., Nat. Commun. 10:2456 (2019)], and manifesting itself by a reversal of the heat flow (from the cold system to the hot one). Here, we show that contrary to what could have been expected, heat flow reversal can happen without reversal of the arrow of time. Moreover, contrasting with previous studies, no initial correlations between system and bath is required. Instead, the heat flow reversal only relies on internal quantum coherences or correlations, which provides practical advantages over previous schemes: one does not need to have access to the bath in order to reverse the heat flow. The underlying mechanism is explained and shown to stem from the collective system-bath coupling and the impact of non-energetic coherences (coherences between degenerate energy levels) on apparent temperatures. The phenomenon is first uncovered in a broad framework valid for diverse quantum systems containing energy degeneracy. By the end of the paper, aiming at experimental realisations, more quantitative results are provided for a pair of two-level systems. Finally, as a curiosity, we mention that our scheme can be adapted as a correlations-to-energy converter, which have the particularity to be able to operate at constant entropy, similarly to ideal work sources.
description: 7 pages of main text, 3 figures, 4 pages of appendices and references
Feedback and the fudamental line of low-luminosity LSB/dwarf galaxies
Creators: name: Dekel, Avishai
name: Woo, Joanna
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We study in simple terms the role of feedback in establishing the scaling relations of low-surface-brightness and dwarf galaxies with stellar masses in the range 6x10^5 30km/s retain gas-rich discs with feedback-regulated star formation.
description: 12 pages including 6 figures, Latex, mn2e.cls, small revisions
Urochloa arrecta Morrone & Zuloaga, Darwiniana
Creators: name: Prunera-Olivé, Joan
name: Vorontsova, Maria S.
name: Williams, Emma V.
name: Mollel, Neduvoto P.
name: Hemp, Andreas
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Liliopsida
Poales
Poaceae
Urochloa
Urochloa arrecta

description: Urochloa arrecta (Hack.) Morrone & Zuloaga, Darwiniana 31: 69 (1992).
 Distribution: Ethiopia to S. Africa, Madagascar
 Specimens: MOSHI Hai area, Hemp, A. 2784 (NHT, UBT).
description: Published as part of Prunera-Olivé, Joan, Vorontsova, Maria S., Williams, Emma V., Mollel, Neduvoto P. & Hemp, Andreas, 2021, Checklist of Kilimanjaro grasses shows that both plot and herbarium methods are necessary to record diversity, pp. 201-244 in Phytotaxa 501 (2) on page 243, DOI: 10.11646/phytotaxa.501.2.1, http://zenodo.org/record/5424816
Drimys lenormandii P. Parm.
Creators: name: Turner, I. M.
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Canellales
Winteraceae
Drimys
Drimys lenormandii

description: 3. Drimys lenormandii Vieill. ex P.Parm.
Bulletin scientifique de la France et de la Belgique 27: 231-232, 308-309, 330, pl. X, fig. 35, pl. XI, figs 42, 43 (1896).
— Type: New Caledonia.
Zygogynum stipitatum Baill.: Adansonia 10: 334 (1872) (Vink 1990, 1993).
REMARKS
Parmentier indicates that he received a specimen labelled “ Drimys Lenormandii Vieill. ” from von Mueller in Melbourne. No such specimen has been located. It may represent a duplicate of Vieillard 2281 which bears this name, and one sheet of which has been annotated as an isotype of Drimys lenormandii Vieill. ex P.Parm by G. Buchheim (Deroin, pers. comm.).
description: Published as part of Turner, I. M., 2012, The taxa described by Paul Évariste Parmentier in Histoire des Magnoliacées, pp. 237-249 in Adansonia (3) (3) 34 (2) on page 239, DOI: 10.5252/a2012n2a3, http://zenodo.org/record/5205948
Additional file 1 of Prevalence and associated factors of metabolic syndrome in adults: a population-based epidemiological survey in Jiangxi province, China
Creators: name: Wu, Li
name: Shen, Yun
name: Hu, Lei
name: Zhang, Mei
name: Lai, Xiao
Publisher: name: figshare
Year: 2020
Subjects: subject: Medicine
subject: Environmental Sciences not elsewhere classified
subject: Ecology
subject: FOS: Biological sciences
subject: Biological Sciences not elsewhere classified
subject: Mathematical Sciences not elsewhere classified
subject: Developmental Biology
subject: Computational Biology

description: Additional file 1: Table S1. Criteria of metabolic syndrome diagnosis in the IDF and CDS systems.
Bumpy Power Spectra and Galaxy Clusters
Creators: name: Knebe, Alexander
name: Islam, Ranty
name: Silk, Joseph
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The evolution of the abundance of galaxy clusters is not a reliable measure of Omega if there are features on scales of a few Mpc in the primordial power spectrum. Conversely, if we know the cosmological model parameters from other measurements, the cluster abundance evolution permits us to probe features in the power spectrum that are in the nonlinear regime at the present epoch, and hence difficult to discern directly from current epoch measurements. We have investigated the influence of an artificially introduced Gaussian feature on an otherwise unperturbed SCDM power spectrum. Using these modified spectra as an input to cosmological N-body simulations, we are able to show that in terms of the cluster abundance evolution, a SCDM model displays characteristics similar to an OCDM model. However, strong modifications would also be visible at a redshift z=0 in the dark matter power spectrum whereas minor alterations to the usual SCDM spectrum are washed away by non-linear evolution effects. We therefore conclude that features with characteristics such as discussed here might not be detectable using observations of the galaxy power spectrum, the local cluster abundance or the large-scale velocity field as measured by the velocity distribution of galaxy clusters. The only quantity that shows a pronounced difference at the present epoch between our models under investigation is the halo-halo correlation function which appears to be strongly biased with respect to an unmodified SCDM model. This is due to a lack of power on certain scales which subsequently modifies the relative amplitude of high-and low-k waves. Apart from observations of the evolution of cluster abundance, measurements of the Lyman-alpha forest at high redshift could put constraints on possible features in the power spectrum, too.
description: 9 pages, 13 figures, MNRAS accepted version
Gallup Poll # 682
Creators: name: Gallup
Publisher: name: Roper Center for Public Opinion Research
Year: 2021

description: Lyndon Johnson job performance (1); Barry Goldwater vs. Lyndon Johnson (2); Henry Cabot Lodge vs. Lyndon Johnson (2); Richard Nixon vs. Lyndon Johnson (2); Nelson Rockefeller vs. Lyndon Johnson (2); George Romney vs. Lyndon Johnson (2); partisan opinions (1); Republican candidates (2); foreign aid (1); Vietnam (2); handling Communist countries (3); Social Security (1); medical insurance (2); taxes (2); labor unions (2); compulsory arbitration (1); federal aid to education (3); civil rights (2); juvenile delinquency (1); obscene magazines (2); church and state (1); aiding development (3); Dwight Eisenhower (1); presidential qualities (1).
On the duality of ring and ladder diagrams and its importance for many-electron perturbation theories
Creators: name: Irmler, Andreas
name: Hummel, Felix
name: Grüneis, Andreas
Publisher: name: arXiv
Year: 2019
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: Chemical Physics (physics.chem-ph)
subject: FOS: Physical sciences

description: We present a diagrammatic decomposition of the transition pair correlation function for the uniform electron gas. We demonstrate explicitly that ring and ladder diagrams are dual counterparts that capture significant long- and short-ranged interelectronic correlation effects, respectively. Our findings help to guide the further development of approximate many-electron theories and reveal that the contribution of the ladder diagrams to the electronic correlation energy can be approximated in an effective manner using second-order perturbation theory. We employ the latter approximation to reduce the computational cost of coupled cluster theory calculations for insulators and semiconductors by two orders of magnitude without compromising accuracy.
description: 6 pages, 2 figures, 1 table
Urochloa brachyura Stapf
Creators: name: Prunera-Olivé, Joan
name: Vorontsova, Maria S.
name: Williams, Emma V.
name: Mollel, Neduvoto P.
name: Hemp, Andreas
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Liliopsida
Poales
Poaceae
Urochloa
Urochloa brachyura

description: Urochloa brachyura (Hack.) Stapf in D.Oliver & auct. suc. (eds.), Fl. Trop. Afr. 9: 592 (1920).
 Distribution: Ethiopia to S. Africa
 Specimens: MOSHI Lerang’wa, Grimshaw, J.M. 94247 (K).
description: Published as part of Prunera-Olivé, Joan, Vorontsova, Maria S., Williams, Emma V., Mollel, Neduvoto P. & Hemp, Andreas, 2021, Checklist of Kilimanjaro grasses shows that both plot and herbarium methods are necessary to record diversity, pp. 201-244 in Phytotaxa 501 (2) on page 243, DOI: 10.11646/phytotaxa.501.2.1, http://zenodo.org/record/5424816
Attractive versus truncated repulsive supercooled liquids: The dynamics is encoded in the pair correlation function
Creators: name: Landes, François P.
name: Biroli, Giulio
name: Dauchot, Olivier
name: Liu, Andrea J.
name: Reichman, David R.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: Soft Condensed Matter (cond-mat.soft)
subject: Machine Learning (cs.LG)
subject: FOS: Physical sciences
subject: FOS: Computer and information sciences

description: We compare glassy dynamics in two liquids that differ in the form of their interaction potentials. Both systems have the same repulsive interactions but one has also an attractive part in the potential. These two systems exhibit very different dynamics despite having nearly identical pair correlation functions. We demonstrate that a properly weighted integral of the pair correlation function, which amplifies the subtle differences between the two systems, correctly captures their dynamical differences. The weights are obtained from a standard machine learning algorithm.
description: 6 pages, 5 figures
BZ Cam during its 1999/2000 optical low state
Creators: name: Greiner, J.
name: Tovmassian, G.
name: Orio, M.
name: Lehmann, H.
name: Chavushyan, V.
name: Rau, A.
name: Schwarz, R.
name: Casalegno, R.
name: Scholz, R. -D.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report optical observations of the VY Scl star BZ Cam during its previous optical low state in 1999/2000. We find drastic variations in the line profiles. Narrow-band imaging observations show that its nebula extends farther than previously known and seems to be composed of two components. We determine the [OIII] line intensity of BZ Cam's nebula to 4.8 * 10^-13 erg/cm^2/s. We discover a proper motion of BZ Cam of 25+-2 mas/yr which together with the systemic radial velocity yields a space velocity of 125 km/s. We re-interpret the nebula as being photo-ionized by hypothesized transient, luminous, supersoft X-ray emission during optical low states, and shaped by the transverse motion of BZ Cam.
description: 8 pages with aa.sty, 8 figures, to appear in A&A
Effects of Youth Educational Aspirations on Academic Outcomes and Racial Differences: A Propensity Score Matching Approach
Creators: name: Lanier, Paul
name: Kainz, Kirsten
name: Eisensmith, Sarah Rabiner
name: Chung, Gerard
Publisher: name: Springer Nature
Year: 2022

description:
This study examined how 7th to 12th grade students’ educational aspirations influenced their school engagement and grade point average (GPA) a year later. Using data (n = 4368) from the National Longitudinal Study of Adolescent to Adult Health, this study used propensity score matching to address confounders due to family, parenting, and individual-level background characteristics, allowing for a minimally biased effect of educational aspirations on the academic performances of White, African American, and Hispanic youths. We found that high educational aspirations helped youths to have better school engagement behaviors above and beyond the positive effects of school climate. White and African American youths with high aspirations attained a higher GPA than those with low aspirations. Yet, even with high aspirations boosting GPA, racial/ethnic group differences in GPA scores persisted. Supporting youths to develop and maintain high levels of aspirations would have a positive effect on their academic performances regardless of racial groups. But improving school learning environment would be important in reducing racial differences in academic performances.
A Density Functional Extension to Excited State Mean-Field Theory
Creators: name: Zhao, Luning
name: Neuscamman, Eric
Publisher: name: arXiv
Year: 2019
Subjects: subject: Chemical Physics (physics.chem-ph)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We investigate an extension of excited state mean-field theory in which the energy expression is augmented with density functional components in an effort to include the effects of weak electron correlations. The approach remains variational and entirely time-independent, allowing it to avoid some of the difficulties associated with linear response and the adiabatic approximation. In particular, all of the electrons' orbitals are relaxed state specifically and there is no reliance on Kohn-Sham orbital energy differences, both of which are important features in the context of charge transfer. Preliminary testing shows clear advantages for single-component charge transfer states, but the method, at least in its current form, is less reliable for states in which multiple particle-hole transitions contribute significantly.
Non-Axisymmetric g-Mode and p-Mode Instability in a Hydrodynamic Thin Accretion Disk
Creators: name: Li, Li-Xin
name: Goodman, Jeremy
name: Narayan, Ramesh
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: It has been suggested that quasi-periodic oscillations of accreting X-ray sources may relate to the modes named in the title. We consider non-axisymmetric linear perturbations to an isentropic, isothermal, unmagnetized thin accretion disk. The radial wave equation, in which the number of vertical nodes (n) appears as a separation constant, admits a wave-action current that is conserved except, in some cases, at corotation. Waves without vertical nodes amplify when reflected by a barrier near corotation. Their action is conserved. As was previously known, this amplification allows the n=0 modes to be unstable under appropriate boundary conditions. In contrast, we find that waves with n >0 are strongly absorbed at corotation rather than amplified; their action is not conserved. Therefore, non-axisymmetric p-modes and g-modes with n>0 are damped and stable even in an inviscid disk. This eliminates a promising explanation for quasi-periodic oscillations in neutron-star and black-hole X-ray binaries.
description: A new version of the paper. The technical error in version 1 has been corrected
Microscopic Reversibility and Macroscopic Irreversibility: From a viewpoint of Algorithmic Randomness
Creators: name: Hiura, Ken
name: Sasa, Shin-ichi
Publisher: name: arXiv
Year: 2019
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: Emergence of deterministic and irreversible macroscopic behavior from deterministic and reversible microscopic dynamics is understood as a result of the law of large numbers. In this paper, we prove on the basis of the theory of algorithmic randomness that Martin-Löf random initial microstates satisfy an irreversible macroscopic law in the Kac infinite chain model. We find that the time-reversed state of a random state is not random as well as violates the macroscopic law.
description: 21 pages
A Simple Model for r-Process Scatter and Halo Evolution
Creators: name: Fields, Brian D.
name: Truran, James W.
name: Cowan, John J.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Recent observations of heavy elements produced by rapid neutron capture (r-process) in the halo have shown a striking and unexpected behavior: within a single star, the relative abundances of r-process elements heavier than Eu are the same as the same as those of solar system matter, while across stars with similar metallicity Fe/H, the r/Fe ratio varies over two orders of magnitude. In this paper we present a simple analytic model which describes a star's abundances in terms of its ``ancestry,'' i.e., the number of nucleosynthesis events (e.g., supernova explosions) which contributed to the star's composition. This model leads to a very simple analytic expression for the abundance scatter versus Fe/H, which is in good agreement with the data and with more sophisticated numerical models. We investigate two classes of scenarios for r-process nucleosynthesis, one in which r-process synthesis events occur in only \sim 4% of supernovae but iron synthesis is ubiquitous, and one in which iron nucleosynthesis occurs in only about 9% of supernovae. (the Wasserburg- Qian model). We find that the predictions in these scenarios are similar for [Fe/H] \ga -2.5, but that these models can be readily distinguished observationally by measuring the dispersion in r/Fe at [Fe/H] \la -3.
description: AASTeX, 21 pages, includes 4 figures
Additional file 2: of Assessing the national capacity for disaster research response (DR2) within the NIEHS Environmental Health Sciences Core Centers
Creators: name: Errett, Nicole
name: Haynes, Erin N.
name: Wyland, Nancy
name: Everhart, Ali
name: Pendergrast, Claire
name: Parker, Edith
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Evolutionary Biology
subject: FOS: Biological sciences
subject: Ecology
subject: Marine Biology
subject: Science Policy
subject: 111714 Mental Health
subject: FOS: Health sciences
subject: 110309 Infectious Diseases

description: Community Engagement Core Director Interview Questions. (DOCX 15 kb)
title: Evaluation of the Effects of Vegetated Buffer Strips on Fate of Sediment with Mathematical Models
Creators: name: Akram, Sina
Publisher: name: Griffith University
Year: 2014
Subjects: subject: Vegetated Buffer Strips
subject: Sediment transport
subject: Gradually varied flow equation

description: Several mathematical models have been developed in recent years to simulate hydrologic and sediment transport processed through vegetated buffer strips. Some of these models are empirically-based equations with limited applicability to conditions other than those under which they have been developed and the input data collected and used. There is a considerable amount of uncertainty in the application of existing process-based models as they consist of empirical sub-models in their structure. The inconsistency between the assumed section of erosion and deposition in and around the grass strip beds in the existing models is also a major limitation. Three independent predictive models are developed and presented in this thesis to fill in the gaps and to improve our predictive capabilities for hydrology and sediment transport across grass strips. The first model developed in this study is a process-based one capable of simulating surface water profile in the upstream section and within grass strips. The data from the experiments carried out earlier in Griffith University’s GUTSR facilities were used to develop a relationship between the hydraulic roughness and flow characteristics and to develop the model itself. The gradually varied flow equation was used to apply the new relationship and to calculate the flow characteristics in the upstream section and within the grass strip bed.
null Universität Rostock zwischen Sozialismus und Hochschulerneuerung
Creators: name: Krüger, Kersten
Publisher: name: Universität Rostock Rostock
Year: 2007
Subjects: subject: 943 General history of Europe Central Europe Germany

description: Unter dem Titel "Universitätsgeschichte und Zeitzeugen" fand im Fach Geschichte seit dem Wintersemester 2006/2007 eine Serie von drei Seminaren statt, die im Wintersemester 2007/2008 zum Abschluss kam. Methodischer Ausgangspunkt ist die Erfahrung, dass in den schriftlich überlieferten Quellen überwiegend die großen Haupt- und Staatsaktionen dokumentiert sind, nicht die Lebenswirklichkeit, nicht der Alltag der einzelnen Menschen, die sich in den politisch und gesellschaftlich gesetzten Rahmenbedingungen zurechtfinden und ihre Existenz gestalten mussten und wollten. War die (Wilhelm-Pieck-)Universität Rostock eine sozialistische Hochschule oder eine Hochschule im Sozialismus? Welche wissenschaftlichen Leistungen wurden an ihr erbracht? Wer trug die Hochschulerneuerung nach 1990? Welche Bedeutung hatte die Wiedereinführung der Freiheit von Forschung und Lehre?
Additional file 2: of Under pressure: force resistance measurements in box mites (Actinotrichida, Oribatida)
Creators: name: Schmelzle, Sebastian
name: BlĂźthgen, Nico
Publisher: name: figshare
Year: 2019
Subjects: subject: Space Science
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Pharmacology
subject: Evolutionary Biology
subject: Ecology
subject: 69999 Biological Sciences not elsewhere classified
subject: Computational Biology

description: Table S2. Body properties of the Euphthiracaroidea specimens where first the prodorsum popped open and the legs were extruded before they were crushed. (DOCX 19 kb)
Baryonic pollution in gamma-ray bursts: the case of a magnetically driven wind emitted from a disk orbiting a stellar mass black hole
Creators: name: Daigne, Frederic
name: Mochkovitch, Robert
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Most models for the central engine of gamma-ray bursts involve a stellar mass black hole surrounded by a thick disk formed after the merging of a system of compact objects or the collapse of a massive star. Energy released from the accretion of disk material by the black hole or from the rotation of the hole itself extracted by the Blandford-Znajek mechanism powers a relativistic wind along the system axis. Lorentz factors of several hundreds are needed to solve the compactness problem in the wind which implies the injection of a tremendous power into a very small amount of matter. The Blandford-Znajek mechanism, where the outflow follows magnetic field lines anchored to the black hole is probably the best way to prevent baryonic pollution and can even initially produce a purely leptonic wind. In this paper we rather study the wind emitted from the inner part of the disk where the risk of baryonic pollution is much larger since the outflow originates from high density regions. We show that the baryonic load of this wind sensitively depends on the disk temperature and magnetic field geometry and that the outflow can become ultra-relativistic (Lorentz factor Gamma>100) under quite restrictive conditions only. Conversely, if Gamma remains of the order of unity the dense wind emitted from the inner disk could help to confine the central jet but may also represent a source of baryon contamination for the Blandford-Znajek mechanism.
description: 13 pages, 8 figures, to be published in A&A
Zakanocoris aceri V. G. Putshkov 1970
Creators: name: Linnavuori, Rauno E.
Publisher: name: Zenodo
Year: 2007
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Hemiptera
Miridae
Zakanocoris
Zakanocoris aceri

description: Zakanocoris aceri V. G. Putshkov, 1970
 Material examined. GILAN: Gyssom, 1 specimen, 30.vi.-10.v.1996; 45-50 km E of Khalkhal, several specimens, 27.vi.1995, 1.-21.vii.1996; Manjil, 1 specimen, 8.-10.v.2001.
 Comments. On Acer monspessulanum. Known from Caucasus, Turkmenistan, and the Golestan province in Iran.
description: Published as part of Linnavuori, Rauno E., 2007, Studies on the Miridae (Heteroptera) of Gilan and the adjacent provinces in northern Iran. II. List of species, pp. 17-56 in Acta Entomologica Musei Nationalis Pragae 47 on page 55, DOI: 10.5281/zenodo.5328235
Urochloa brizantha R. D. Webster, Austral. Paniceae
Creators: name: Prunera-Olivé, Joan
name: Vorontsova, Maria S.
name: Williams, Emma V.
name: Mollel, Neduvoto P.
name: Hemp, Andreas
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Liliopsida
Poales
Poaceae
Urochloa
Urochloa brizantha

description: Urochloa brizantha (A.Rich.) R.D.Webster, Austral. Paniceae: 233 (1987).
 Distribution: Trop. & S. Africa, W. Indian Ocean, SW. Arabian Pen.
 Specimens: MOSHI Kirua, Hemp, A. 1686 (NHT, UBT); Moshi, Haarer, A.E. 742 (K); Mwika, Hemp, A. 2054 (B, NHT, UBT); Rombo, Greenway, P.J. 7835 (K); s. loc., Endlich, R. 33A (NH).
description: Published as part of Prunera-Olivé, Joan, Vorontsova, Maria S., Williams, Emma V., Mollel, Neduvoto P. & Hemp, Andreas, 2021, Checklist of Kilimanjaro grasses shows that both plot and herbarium methods are necessary to record diversity, pp. 201-244 in Phytotaxa 501 (2) on page 243, DOI: 10.11646/phytotaxa.501.2.1, http://zenodo.org/record/5424816
Five-Dimensional Brane World Theory
Creators: name: Carmeli, Moshe
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present a five-dimensional gravitational theory in a space-time-velocity Riemannian manifold. The equations of motion of a star moving around a galaxy are shown to be the Tully-Fisher law. The problem of the cosmological constant is discussed, and a new formula for the cosmological redshift is derived.
description: 27 pages LaTeX, to be published
Additional file 1: of Under pressure: force resistance measurements in box mites (Actinotrichida, Oribatida)
Creators: name: Schmelzle, Sebastian
name: BlĂźthgen, Nico
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Physiology
subject: FOS: Biological sciences
subject: Evolutionary Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: Science Policy
subject: Computational Biology

description: Table S1. Results of Kruskal-Wallis test for equal medians and Mann-Whitney pairwise post-hoc test with assumed sequential Bonferroni significance of different body properties between groups. (DOCX 19 kb)
FUSE and HST STIS Observations of Hot and Cold Gas in the AB Aurigae System
Creators: name: Roberge, A.
name: Etangs, A. Lecavelier des
name: Grady, C. A.
name: Vidal-Madjar, A.
name: Bouret, J. -C.
name: Feldman, P. D.
name: Deleuil, M.
name: Andre, M.
name: Boggess, A.
name: Bruhweiler, F. C.
name: Ferlet, R.
name: Woodgate, B.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present the first observations of a Herbig Ae star with a circumstellar disk by the Far Ultraviolet Spectroscopic Explorer (FUSE), as well as a simultaneous observation of the star obtained with the Hubble Space Telescope Space Telescope Imaging Spectrograph (STIS). The spectra of AB Aurigae show emission and absorption features arising from gasses that have a wide range in temperature, from hot OVI emission to cold molecular hydrogen and CO absorption. Emissions from the highly ionized species OVI and CIII present in the FUSE spectrum are redshifted, while absorption features arising from low-ionization species like OI, NI, and SiII are blueshifted and show characteristic stellar wind line-profiles. We find the total column density of molecular hydrogen toward AB Aur from the FUSE apectrum, N(H_2) = (6.8 +/- 0.5) x 10^19 cm^-2. The gas kinetic temperature of the molecular hydrogen derived from the ratio N(J=1)/N(J=0) is 65 +/- 4 K. The column density of the CO observed in the STIS spectrum is N(CO) = (7.1 +/- 0.5) x 10^13 cm^-2, giving a CO/H_2 ratio of (1.04 +/- 0.11) x 10^-6. We also use the STIS spectrum to find the column density of HI, permitting us to calculate the total column density of hydrogen atoms, the fractional abundance of H_2, and the gas-to-dust ratio.
description: 5 pages, including 6 figures. LaTex2e (emulateapj5.sty). Accepted for publication in ApJ Letters
MPEC 2024-C163 : DAILY ORBIT UPDATE (2024 February 14)
Creators: name: Minor Planet Center Staff
Publisher: name: The Minor Planet Center
Year: 2024
Subjects: subject: Small Solar System bodies
valueUri: http://astrothesaurus.org/uat/1469

description: The Minor Planet Electronic Circulars contain information on unusual minor planets, routine data on comets and natural satellites, and occasional editorial announcements.  They are published on behalf of Division F of the International Astronomical Union by the Minor Planet Center, Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A.
title: Eliciting Fear in Psycho (1960), Halloween (1978) and The Shining (1980)
Creators: name: Long, Rosemary
Publisher: name: Griffith University
Year: 2020
Subjects: subject: Film
subject: Fear

description: Psycho (1960), Halloween (1978) and The Shining (1980) are seminal films that have been instrumental in both shaping the horror genre and eliciting the emotional response of fear in the viewer. Their respective directors, Alfred Hitchcock, John Carpenter and Stanley Kubrick, each employed and developed specific techniques for producing fear. This research identifies those techniques by close analyses of the formal elements of each film and considers why the they effective. A common core of techniques is shared by all three films: the primary technique for inducing fear is the employment of the subjective camera. Freud’s notion of the uncanny is also significant and each film takes considerable measures to arouse ‘uncanny’ sensations in the viewer through a variety of cinematic techniques. Both Carpenter and Kubrick built on Hitchcock as well as developed new techniques, with the aid of new technology, in order to keep up with changing audience perceptions and expectations.
Cossyphus (Acontodactylus) limbatus Pascoe 1887
Creators: name: Háva, Jiří
Publisher: name: Zenodo
Year: 2007
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Tenebrionidae
Cossyphus
Cossyphus limbatus

description: 1. Cossyphus (Acontodactylus) limbatus Pascoe, 1887
 Cossyphus (Acontodactylus) limbatus Pascoe, 1887: SCUPOLA (2000): 207.
 Material examined. CAMBODIA: ‘ Cambodia mer., Takeo, 5.v.[19]84, Frühbauer lgt.’, 2 spec. (1 NMPC, 1 JHAC); ‘ Cambodia centr., Phnom Penh, 20.12.[19]84, Frühbauer lgt.’, 1 spec. (NMPC).
 Distribution. Species known from Cambodia, Laos, Thailand, Vietnam, and probably also from the Philippines (SCUPOLA 2000).
description: Published as part of Háva, Jiří, 2007, List of specimens of the tribe Cossyphini (Coleoptera: Tenebrionidae) kept in the National Museum, Praha, pp. 183-187 in Acta Entomologica Musei Nationalis Pragae 47 on page 184, DOI: 10.5281/zenodo.5328309
Maximal energy extraction via quantum measurement
Creators: name: Solfanelli, Andrea
name: Buffoni, Lorenzo
name: Cuccoli, Alessandro
name: Campisi, Michele
Publisher: name: arXiv
Year: 2019
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We study the maximal amount of energy that can be extracted from a finite quantum system by means of projective measurements. For this quantity we coin the expression "metrotropy" $\mathcal{M}$, in analogy with "ergotropy" $\mathcal{W}$, which is the maximal amount of energy that can be extracted by means of unitary operations. The study is restricted to the case when the system is initially in a stationary state, and therefore the ergotropy is achieved by means of a permutation of the energy eigenstates. We show that i) the metrotropy is achieved by means of an even combination of the identity and an involution permutation; ii) it is $\mathcal{M}\leq\mathcal{W}/2$, with the bound being saturated when the permutation that achieves the ergotropy is an involution.
description: 12 pages, 3 figures. Contribution to the special issue of JSTAT "New Trends in Nonequilibrium Statistical Mechanics: Classical and Quantum Systems - nesmcq18". v2 = published version
Gallup Poll # 683
Creators: name: Gallup
Publisher: name: Roper Center for Public Opinion Research
Year: 2021

description: Lyndon Johnson job performance (1); sickness within the family (5); civil rights (2); presidential succession (2); Republican candidate (3); Democratic candidate (2); voting intent (4); Barry Goldwater vs. Lyndon Johnson (2); William Scranton vs. Lyndon Johnson (2); Henry Cabot Lodge vs. Lyndon Johnson (2); Richard Nixon vs. Lyndon Johnson (2); Nelson Rockefeller vs. Lyndon Johnson (2); George Romney vs. Lyndon Johnson (2).
Using Human Ratings for Feedback Control: A Supervised Learning Approach with Application to Rehabilitation Robotics
Creators: name: Menner, Marcel
name: Neuner, Lukas
name: Lünenburger, Lars
name: Zeilinger, Melanie N.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Robotics (cs.RO)
subject: Systems and Control (eess.SY)
subject: FOS: Computer and information sciences
subject: FOS: Electrical engineering, electronic engineering, information engineering

description: This paper presents a method for tailoring a parametric controller based on human ratings. The method leverages supervised learning concepts in order to train a reward model from data. It is applied to a gait rehabilitation robot with the goal of teaching the robot how to walk patients physiologically. In this context, the reward model judges the physiology of the gait cycle (instead of therapists) using sensor measurements provided by the robot and the automatic feedback controller chooses the input settings of the robot to maximize the reward. The key advantage of the proposed method is that only a few input adaptations are necessary to achieve a physiological gait cycle. Experiments with nondisabled subjects show that the proposed method permits the incorporation of human expertise into a control law and to automatically walk patients physiologically.
Running Measurement Protocol for the Quantum First-detection problem
Creators: name: Meidan, Dror
name: Barkai, Eli
name: Kessler, David A.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: The problem of the detection statistics of a quantum walker has received increasing interest, connected as it is to the problem of quantum search. We investigate the effect of employing a moving detector, using a projective measurement approach with fixed sampling time $τ$, with the detector moving right before every detection attempt. For a tight-binding quantum walk on the line, the moving detector allows one to target a specific range of group velocities of the walker, qualitatively modifying the behavior of the quantum first-detection probabilities. We map the problem to that of a stationary detector with a modified unitary evolution operator and use established methods for the solution of that problem to study the first-detection statistics for a moving detector on a finite ring and on an infinite 1D lattice. On the line, the system exhibits a dynamical phase transition at a critical value of $τ$, from a state where detection decreases exponentially in time and the total detection is very small, to a state with power-law decay and a significantly higher probability to detect the particle. The exponent describing the power-law decay of the detection probability at this critical $τ$ is 10/3, as opposed to 3 for every larger $τ$. In addition, the moving detector strongly modifies the Zeno effect.
Drimys muelleri P. Parm.
Creators: name: Turner, I. M.
Publisher: name: Zenodo
Year: 2012
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Magnoliopsida
Canellales
Winteraceae
Drimys
Drimys muelleri

description: 4. Drimys muelleri P.Parm.
Bulletin scientifique de la France et de la Belgique 27: 227, 300, pl. X, figs 36, 37 (1896).
— Type: Australia, Tasmania, Mt Victoria, C. Glover s.n. (holo-, P [P00750497]; iso-, MEL).
Persoonia muelleri (P.Parm.) Orchard: Brunonia 6: 226 (1984) (Proteaceae) (Weston 1995).
description: Published as part of Turner, I. M., 2012, The taxa described by Paul Évariste Parmentier in Histoire des Magnoliacées, pp. 237-249 in Adansonia (3) (3) 34 (2) on page 239, DOI: 10.5252/a2012n2a3, http://zenodo.org/record/5205948
Urochloa comata Sosef, Fl.
Creators: name: Prunera-Olivé, Joan
name: Vorontsova, Maria S.
name: Williams, Emma V.
name: Mollel, Neduvoto P.
name: Hemp, Andreas
Publisher: name: Zenodo
Year: 2021
Subjects: Biodiversity
Taxonomy
Plantae
Tracheophyta
Liliopsida
Poales
Poaceae
Urochloa
Urochloa comata

description: Urochloa comata (Hochst. ex A.Rich.) Sosef, Fl. Gabon 5bis: 64 (1999).
 Distribution: Trop. Africa, SW. Arabian Pen.
 Specimens: MOSHI Kidia, Hemp, A. 1677 (NHT, UBT); Lerang’wa, Hemp, A. 3055 (NHT, UBT); Mandara Hut (=Bismark Hut), Hitchcock, A.S. 24622 (K); Marangu, Hitchcock, A.S. 24660 (K, NH); s. loc., Volkens, G. 657 (MO); Sanya Juu, Hemp, A. 4454 (NHT, UBT).
description: Published as part of Prunera-Olivé, Joan, Vorontsova, Maria S., Williams, Emma V., Mollel, Neduvoto P. & Hemp, Andreas, 2021, Checklist of Kilimanjaro grasses shows that both plot and herbarium methods are necessary to record diversity, pp. 201-244 in Phytotaxa 501 (2) on page 243, DOI: 10.11646/phytotaxa.501.2.1, http://zenodo.org/record/5424816
Evolutionary Synthesis Models for the Formation of S0 Galaxies in Clusters
Creators: name: Bicker, J.
name: Alvensleben, U. Fritze - v.
name: Fricke, K. J.
Publisher: name: arXiv
Year: 2002
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Rich galaxy clusters in the local Universe show a large population of S0 galaxies (~ 40%) of all luminous galaxies). With increasing redshift the fraction of this S0 galaxy population is observed to strongly decrease (e.g. by a factor ~2-3 to z = 0.5) in favor of the spiral galaxy fraction while the number of bright ellipticals does not seem to change. The infalling field galaxy population that successively builds up the cluster also is spiral rich and S0 poor. It has hence been suspected that galaxy transformation processes, either due to galaxy -- galaxy or to galaxy -- ICM interactions, are responsible for this change. Complementing dynamical and morphological studies, we use evolutionary synthesis models describing various possible effects of those interactions on the star formation rates of the infalling spirals. We study the effects of starbursts of various strengths as well as of the truncation of star formation on the color and luminosity evolution of model galaxies of various spectral types. Comparison with observed properties of the local S0 galaxy population is used to constrain possible S0 formation mechanisms. We find that star formation truncation in spiral galaxies earlier than Sd-type, if occurring not too long ago, as well as starbursts more than 3 Gyr ago and followed by complete star formation extinction in spirals -- again earlier than Sd-- may well account for the observed average S0 luminosities and colors. Late-type galaxies (Sd), even after a strong burst, remain either too blue or too faint. Our results are in agreement with studies of spectral features of cluster S0s but allow for stronger constraints.
description: 10 pages, accepted (A&A)
Nuclear and global X-ray properties of LINER galaxies: Chandra and BeppoSAX results for Sombrero and NGC 4736
Creators: name: Pellegrini, S.
name: Fabbiano, G.
name: Fiore, F.
name: Trinchieri, G.
name: Antonelli, A.
Publisher: name: arXiv
Year: 2001
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report on the 0.1--100 keV BeppoSAX observations of two nearby LINER galaxies, Sombrero and NGC 4736. Chandra ACIS-S observations supplement this broad-beam spectral study with a high resolution look into the nuclear region, and show a dominating central point source in Sombrero and a complex X-ray binary dominated/starburst region in NGC 4736. A compact non-thermal radio source, present in the nucleus of both galaxies, coincides with the central source in Sombrero, while in NGC 4736 its X-ray counterpart is a much fainter point source, not the brightest of the central region. On the basis of these and other results, we conclude that the LINER activity is linked to the presence of a low luminosity AGN in Sombrero and to a recent starburst in NGC 4736, and that Chandra's spectroscopic capabilities coupled to high resolution imaging are essential to establish the origin of the nuclear activity.
description: 13 pages, 12 figures (Fig. 4 and Fig. 5 are colour figures), to be published in Astronomy & Astrophysics
Gallup Poll # 684
Creators: name: Gallup
Publisher: name: Roper Center for Public Opinion Research
Year: 2021

description: Lyndon Johnson job performance (3); racial integration (1); Communist China admitted into United Nations (2); 1964 Republican presidential candidates (2); Barry Goldwater vs. Nelson Rockefeller (1); 1964 Democratic vice-presidential candidates (1); partisan opinions (1); Congress (1); finances of Senate and House of representatives (1); law limiting terms of senators and representatives (2); Barry Goldwater vs. Lyndon Johnson (2); Henry Cabot Lodge vs. Lyndon Johnson (2); Richard Nixon vs. Lyndon Johnson (2); selling to Russia (5); voted in precinct in the past (1); voting intent (2).
Cossyphus (Cossyphus) dejeani Breme 1846
Creators: name: Háva, Jiří
Publisher: name: Zenodo
Year: 2007
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Insecta
Coleoptera
Tenebrionidae
Cossyphus
Cossyphus dejeani

description: 2. Cossyphus (Cossyphus) dejeani Brême, 1846
 Cossyphus (Cossyphus) dejeani Brême, 1846: SCUPOLA (2000): 226.
 Material examined. MOROCCO: ‘ Tetuan, J. Váca’, 2 spec. (NMPC); ‘ Casablanca, Maroc’ // ‘6302’ // ‘ Cossyphus dejeani, B. Kouřil det.’, 4 spec. (3 NMPC, 1 JHAC). ITALY: ‘Sardinia’ // ‘dejeani’, 1 spec. (NMPC). SPAIN: ‘ Andalusia, Hispania’ // ‘ Cossyphus dejeani Br., det. Hlisnikowski 1942 ’, 2 spec. (NMPC); ‘ Algeciras, C. Bolivar’ // ‘ Cossyphus hoffmannseggi Hbst’, 3 spec. (NMPC); ‘ Algeciras, Hispania’ // ‘ Cossyphus dejeani Br., det. Hlisnikowski 1942 ’, 2 spec. (NMPC); ‘ Algeciras, Andalusien, Prof. G. Strobl’ // ‘ Cossyphus dejeani Br., det. Hlisnikowski 1942 ’, 1 spec. (NMPC); ‘ Tarifa, 11-4-[19]06, coll. Schramm’ // ‘ Cossyphus dejeani Br., det. Hlisnikowski 1942 ’, 3 spec. (NMPC); ‘ Guadarrama, Cercedilla,V.M. Duchon’, 3 spec. (NMPC); ‘ Spanien. ’, 3 spec. (2 NMPC, 1 JHAC); ‘ Hispan. ’, 6 spec. (NMPC); ‘ Andalusia’ // ‘ Mus. Pragense, col. Kamberský’ // ‘ Cossyphus dejeani Br., Det. Schuster’, 2 spec. (NMPC); ‘ Kelecsényi, Madrid’ // ‘ dejeani Br., Det. Obenberger’, 2 spec. (NMPC); ‘ Hispania’, 1 spec. (NMPC); ‘ Andalusien’, 4 spec. (NMPC); ‘ Algeciras, C. Bolivar’, 3 spec. (NMPC).
 Distribution. Species known from Algeria, Morocco, and Spain (SCUPOLA 2000). New species for Italy (Sardinia).
description: Published as part of Háva, Jiří, 2007, List of specimens of the tribe Cossyphini (Coleoptera: Tenebrionidae) kept in the National Museum, Praha, pp. 183-187 in Acta Entomologica Musei Nationalis Pragae 47 on page 185, DOI: 10.5281/zenodo.5328309
Additional file 1 of Exploring the information transmission properties of noise-induced dynamics: application to glioma differentiation
Creators: name: Sai, Aditya
name: Kong, Nan
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Neuroscience
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Supplementary Information. Section S1 AN Model Description. Section S2 CLE Model Description. Figure S1. AN response dynamics. Figure S2. Heatmaps for summary descriptors of AN model. Figure S3. CLE- response dynamics. Figure S4. Heatmaps for summary descriptors of CLE- model.Figure S5. Channel capacities for summary descriptors of AN model as a function of k specified in k-nearest neighbors algorithm. Figure S6. Channel capacities for summary descriptors of CLE model as a function of k specified in k-nearest neighbors algorithm. Figure S7. Channel capacities for summary descriptors of CLE- model as a function of k specified in k-nearest neighbors algorithm. Figure S8. Channel capacities for multivariate response vectors of AN, CLE, and CLE- models as a function of vector dimension d specified in channel capacity algorithm. Table S1. Initial conditions for model states. Table S2. Parameter values for mathematical model. (PDF 548 kb)
Conditioned two-dimensional simple random walk: Green's function and harmonic measure
Creators: name: Popov, Serguei
Publisher: name: arXiv
Year: 2019
Subjects: subject: Probability (math.PR)
subject: FOS: Mathematics
subject: Primary 60J10. Secondary 60G50, 82C41

description: We study the Doob's $h$-transform of the two-dimensional simple random walk with respect to its potential kernel, which can be thought of as the two-dimensional simple random walk conditioned on never hitting the origin. We derive an explicit formula for the Green's function of this random walk, and also prove a quantitative result on the speed of convergence of the (conditional) entrance measure to the harmonic measure (for the conditioned walk) on a finite set.
description: 23 pages, 4 figures