cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Bubble quenches in the AdS/BCFT model
Creators: name: Cavalcanti, Arthur G.
name: Melnikov, Dmitry
Publisher: name: arXiv
Year: 2020
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: In this paper we construct time-dependent solutions of three-dimensional gravity in AdS space dual to systems with boundaries (BCFTs), following the AdS/BCFT prescription. Such solutions can be discussed in the context of the dynamics of first order phase transitions, or more generally, in the description of quantum quenches. As an example, we apply the holographic model to calculate the dynamics of the entanglement entropy of a local quench corresponding to a nucleation of a Euclidean bubble. As in the known 1+1 CFT examples of local cut and glue quenches, the holographic entanglement entropy grows logarithmically with time with the correct universal coefficient. However, in the bubble quench, the behavior is different at late times. The AdS/BCFT model exhibits the light-cone spreading of correlations and saturation at late times. We also find an analytical formula for the entropy at finite temperature. In the latter case the initial logarithmic growth is followed by the linear law at intermediate times.
description: 18 pages, 9 figures, In this version the relation between cut and glue quenches and the considered quench protocol was clarified. The title of the paper was changed to reflect the difference. Appropriate references added
The Evolution of Rotation and Magnetic Activity in 94 Aqr Aa from Asteroseismology with TESS
Creators: name: Metcalfe, Travis S.
name: van Saders, Jennifer L.
name: Basu, Sarbani
name: Buzasi, Derek
name: Chaplin, William J.
name: Egeland, Ricky
name: Garcia, Rafael A.
name: Gaulme, Patrick
name: Huber, Daniel
name: Reinhold, Timo
name: Schunker, Hannah
name: Stassun, Keivan G.
name: Appourchaux, Thierry
name: Ball, Warrick H.
name: Bedding, Timothy R.
name: Deheuvels, Sebastien
name: Gonzalez-Cuesta, Lucia
name: Handberg, Rasmus
name: Jimenez, Antonio
name: Kjeldsen, Hans
name: Li, Tanda
name: Lund, Mikkel N.
name: Mathur, Savita
name: Mosser, Benoit
name: Nielsen, Martin B.
name: Noll, Anthony
name: Orhan, Zeynep Celik
name: Ortel, Sibel
name: Santos, Angela R. G.
name: Yildiz, Mutlu
name: Baliunas, Sallie
name: Soon, Willie
Publisher: name: arXiv
Year: 2020
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Most previous efforts to calibrate how rotation and magnetic activity depend on stellar age and mass have relied on observations of clusters, where isochrones from stellar evolution models are used to determine the properties of the ensemble. Asteroseismology employs similar models to measure the properties of an individual star by matching its normal modes of oscillation, yielding the stellar age and mass with high precision. We use 27 days of photometry from the Transiting Exoplanet Survey Satellite to characterize solar-like oscillations in the G8 subgiant of the 94 Aqr triple system. The resulting stellar properties, when combined with a reanalysis of 35 yr of activity measurements from the Mount Wilson HK project, allow us to probe the evolution of rotation and magnetic activity in the system. The asteroseismic age of the subgiant agrees with a stellar isochrone fit, but the rotation period is much shorter than expected from standard models of angular momentum evolution. We conclude that weakened magnetic braking may be needed to reproduce the stellar properties, and that evolved subgiants in the hydrogen shell-burning phase can reinvigorate large-scale dynamo action and briefly sustain magnetic activity cycles before ascending the red giant branch.
description: 14 pages including 8 figures and 3 tables (updated Table 3 & Figure 6). ApJ in press
Exploring networks with traceroute-like probes: theory and simulations
Creators: name: Dall'Asta, Luca
name: Alvarez-Hamelin, Ignacio
name: Barrat, Alain
name: Vazquez, Alexei
name: Vespignani, Alessandro
Publisher: name: arXiv
Year: 2004
Subjects: subject: Networking and Internet Architecture (cs.NI)
subject: Other Condensed Matter (cond-mat.other)
subject: FOS: Computer and information sciences
subject: FOS: Physical sciences

description: Mapping the Internet generally consists in sampling the network from a limited set of sources by using traceroute-like probes. This methodology, akin to the merging of different spanning trees to a set of destination, has been argued to introduce uncontrolled sampling biases that might produce statistical properties of the sampled graph which sharply differ from the original ones. In this paper we explore these biases and provide a statistical analysis of their origin. We derive an analytical approximation for the probability of edge and vertex detection that exploits the role of the number of sources and targets and allows us to relate the global topological properties of the underlying network with the statistical accuracy of the sampled graph. In particular, we find that the edge and vertex detection probability depends on the betweenness centrality of each element. This allows us to show that shortest path routed sampling provides a better characterization of underlying graphs with broad distributions of connectivity. We complement the analytical discussion with a throughout numerical investigation of simulated mapping strategies in network models with different topologies. We show that sampled graphs provide a fair qualitative characterization of the statistical properties of the original networks in a fair range of different strategies and exploration parameters. Moreover, we characterize the level of redundancy and completeness of the exploration process as a function of the topological properties of the network. Finally, we study numerically how the fraction of vertices and edges discovered in the sampled graph depends on the particular deployements of probing sources. The results might hint the steps toward more efficient mapping strategies.
description: This paper is related to cond-mat/0406404, with explorations of different networks and complementary discussions
P.Oxy. LXXXVII 5581. Aristophanes, Thesmophoriazusae II (Addenda to II 212 + XXXVII 2808)
Creators: name: Oxford Papyrology
Publisher: name: University of Oxford
Year: 2023
Subjects: classificationCode: 470316
subject: Latin and classical Greek languages

description: Reproduction requests: https://www.ees.ac.uk/reproduction-requests-and-fees
Additional file 2 of Parent-child communication about sexual issues in Zambia: a cross sectional study of adolescent girls and their parents
Creators: name: Isaksen, Katja Jezkova
name: Musonda, Patrick
name: Sandøy, Ingvild Fossgard
Publisher: name: figshare
Year: 2020
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Cancer
subject: Science Policy

description: Additional file 2 Additional data on distribution of responses for occurrence of parent-child communication about sexual issues and psychosocial variables used in the study. Table 1 presents the distribution of responses to ‘Occurrence of parent-child communication about sexual issues’ broken down by the five original response categories. This shows the distribution of responses before the variable was converted to a dichotomous variable. Table 2 shows the response patterns for the psychosocial variables according to the five original response options for the frequency of parent-child sexuality communication (“How many times have you talked about romantic relationships or sexual issues.”).
Additional file 1 of The role of contraception in preventing HIV-positive births: global estimates and projections
Creators: name: Sherwood, Jennifer
name: Lankiewicz, Elise
name: Beirne Roose-Snyder
name: Bergen Cooper
name: Jones, Austin
name: Honermann, Brian
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Biotechnology
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Cancer
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Additional file 1.
$d+1$ formalism in Einstein-scalar-Gauss-Bonnet gravity
Creators: name: Julié, Félix-Louis
name: Berti, Emanuele
Publisher: name: arXiv
Year: 2020
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We present the $d+1$ formulation of Einstein-scalar-Gauss-Bonnet (ESGB) theories in dimension $D=d+1$ and for arbitrary (spacelike or timelike) slicings. We first build an action which generalizes those of Gibbons-Hawking-York and Myers to ESGB theories, showing that they can be described by a Dirichlet variational principle. We then generalize the Arnowitt-Deser-Misner (ADM) Lagrangian and Hamiltonian to ESGB theories, as well as the resulting $d+1$ decomposition of the equations of motion. Unlike general relativity, the canonical momenta of ESGB theories are nonlinear in the extrinsic curvature. This has two main implications: (i) the ADM Hamiltonian is generically multivalued, and the associated Hamiltonian evolution is not predictable; (ii) the "$d+1$" equations of motion are quasilinear, and they may break down in strongly curved, highly dynamical regimes. Our results should be useful to guide future developments of numerical relativity for ESGB gravity in the nonperturbative regime.
description: 10 pages. v2: fixed references, no changes to the main text
Health care technology management (HCTM) : an assessment of its application in Canadian teaching hospitals
Creators: name: Eisler, George
Publisher: name: University of British Columbia
Year: 2009

description: The rate of technological change is often referred to as one of the drivers of change in Canada's health care system. However, the challenge of managing technology has not received extensive attention in the health care management literature. This study was conducted to provide a model for technology management and an assessment of the level of technology management practices in Canada's teaching hospitals. The research strategy involved an analysis of devebpments to date in the academic disciplines of Management of Technology (MOT) and Management of Medical Technology (MMT). An extensive literature content analysis generated a set of definitions and attributes of the conceptual construct 'technology management'. Through a formal survey design process involving expert input, pilot testing, and field testing a measurement instrument was developed. The Association of Canadian Academic Health Organizations (ACAHO) enthusiastically supported a web-based survey of senior administrators, representing many of Canada's technology intensive teaching hospitals. 324 CEOs, VPs, and managers reporting to the Executive responded. They each rated the importance and the extent of implementation of 26 indicators, which had been derived via the content analysis from the list of attributes. From each set of importance and implementation ratings, a gap score measure was calculated. Through a variety of statistical methods including factor analysis and cluster analysis of the gap scores, it was determined that there were significant differences between organizations relative to the gap between a benchmark level and their actual level of technology management practice. Two major clusters of hospitals emerged. One of the clusters performed significantly better than the other for each of the 26 measurement indicators.
Alternative Co-operative Structures for the Agri-food Sector: An Exploratory Study
Creators: name: Doyon, Maurice
name: Doyon, Maurice
Publisher: name: Unknown
Year: 2005
Subjects: subject: Agribusiness
subject: Marketing
subject: FOS: Economics and business

description: In a context of internationalisation and concentration, bio-foods co-operatives often face problems of capital access and governance. According to Spear (2001), limited access to capital, management structure, governance conflicts, and the local, regional or national focus of co-operatives limit their expansion. Recent events in Canada, such as Agricore going public and Dairyworld being absorbed by a corporation, have reinforced this perception (Thibault and Dupuis, 2003). In this evolving competitive environment, the traditional co-operative model cannot thrive and succeed if static. New hybrid co-operative models are emerging, and an analysis of these models should contribute to an understanding of the trade-off between co-operative values and other attributes necessary for survival in an increasingly competitive environment.
AG Carinae: a Luminous Blue Variable with a high rotational velocity
Creators: name: Groh, J. H.
name: Hillier, D. J.
name: Damineli, A.
Publisher: name: arXiv
Year: 2005
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We report the detection of broad absorptions due to Si IV 4088-4116 A in the Luminous Blue Variable (LBV) AG Carinae during its last hot phase (2001-2003). Our NLTE spectral analysis, with the radiative transfer code CMFGEN, revealed the photospheric nature of these lines predicting, however, much narrower and deeper absorption profiles than observed. Using a recently-developed code to compute synthetic spectra in 2D geometry allowing for the effects of rotation, we could match the broad absorptions with a high projected rotational velocity of 190 +/- 30 km/s on 2001 April. Analysis of spectra obtained on 2002 March and 2003 January, when the star was cooling, yielded to a projected rotational velocity of 110 +/- 10 km/s and 85 +/- 10 km/s, respectively. The derived rotational velocities are proportional to R^-1, as expected from angular momentum conservation. We discuss the effects of such high rotation on the spectral analysis of AG Car, and on the wind terminal velocity. Our results show direct spectroscopic evidence, for the first time, that a LBV may rotate at a significant fraction of its break-up velocity. Thus, AG Car (and possibly other LBVs) is indeed close to the Gamma-Omega limit, as predicted by theoretical studies of LBVs.
description: 15 pages, 4 figures, submitted to ApJ Letters
The Carnegie Supernova Project II. Observations of SN 2014ab possibly revealing a 2010jl-like SN IIn with pre-existing dust
Creators: name: Moriya, T. J.
name: Stritzinger, M. D.
name: Taddia, F.
name: Morrell, N.
name: Suntzeff, N. B.
name: Contreras, C.
name: Gall, C.
name: Hjorth, J.
name: Ashall, C.
name: Burns, C. R.
name: Busta, L.
name: Campillay, A.
name: Castellon, S.
name: Corco, C.
name: Davis, S.
name: Galbany, L.
name: Gonzalez, C.
name: Holmbo, S.
name: Hsiao, E. Y.
name: Maund, J. R.
name: Phillips, M. M.
Publisher: name: arXiv
Year: 2020
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We present optical and near-infrared photometry and spectroscopy of the Type IIn supernova (SN) 2014ab, obtained by the Carnegie Supernova Project II (CSP-II) and initiated immediately after its optical discovery. We also present mid-infrared photometry obtained by the Wide-field Infrared Survey Explorer (WISE) satellite extending from 56 days prior to the optical discovery to over 1600 days. The light curve of SN 2014ab evolves slowly, while the spectra exhibit strong emission features produced from the interaction between rapidly expanding ejecta and dense circumstellar matter. The light curve and spectral properties are very similar to those of SN 2010jl. The estimated mass-loss rate of the progenitor of SN 2014ab is of the order of 0.1 Msun/yr under the assumption of spherically symmetric circumstellar matter and steady mass loss. Although the mid-infrared luminosity increases due to emission from dust, which is characterized by a blackbody temperature close to the dust evaporation temperature (~ 2000 K), no clear signatures of in situ dust formation within the cold dense shell located behind the forward shock are observed in SN 2014ab in early phases. Mid-infrared emission of SN 2014ab may originate from pre-existing dust located within dense circumstellar matter that is heated by the SN shock or shock-driven radiation. Finally, for the benefit of the community, we also present in an Appendix five near-infrared spectra of SN 2010jl obtained between 450 to 1300 days post discovery.
description: 22 pages, 13 figures, 6 tables, accepted by Astronomy & Astrophysics, proofed
CAIS Program Structure and Performance: Evidence from Ontario
Creators: name: Mussell, Al
name: Martin, Larry J.
name: Mussell, Al
name: Martin, Larry J.
Publisher: name: Unknown
Year: 2005
Subjects: Agricultural and Food Policy

description: The Canadian Agricultural Income Stabilization (CAIS) program was approved in late 2003. It now serves as Canada’s sole farm safety net program, having replaced the Net Income Stabilization Account (NISA), Canadian Farm Income Program (CFIP), and provincial companion programs. However, the mechanisms of operation and actual performance of CAIS in providing stability to farm incomes are relatively unknown. In particular, to develop expectations of future farm costs and returns and to determine their support for CAIS as the sole safety net under the federal-provincial Agricultural Policy Framework (APF), farmers and their representatives need a concrete understanding of how CAIS can be expected to work relative to its predecessors.
A Note on High Energy Neutrinos from AGN Cores
Creators: name: Stecker, F. W.
Publisher: name: arXiv
Year: 2005
Subjects: subject: Astrophysics (astro-ph)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Taking into account new physics and astronomy developments I give a revised high energy neutrino flux for the AGN core model of Stecker, Done, Salamon and Sommers
description: Accepted for publication in Physical Review D
The Surprising Anisotropy of Fast Rotating, Disky Elliptical Galaxies
Creators: name: Burkert, Andreas
name: Naab, Thorsten
Publisher: name: arXiv
Year: 2005
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The projected kinematical properties of unequal-mass merger remnants of disk galaxies are analysed and shown to agree well with observations of disky, fast rotating elliptical galaxies. This supports the major merger hypothesis of early-type galaxy formation. However, in contrast to previous claims, the merger remnants are very anisotropic with values of the anisotropy parameter that are similar to equal-mass merger remnants that form boxy, slowly rotating ellipticals. Including gas in the simulations does not change this result although the line-of-sight velocity profile and the intrinsic orbital structure are strongly affected by the presenceof gas. The kinematical difference between boxy and disky ellipticals appears not to be the amount of anisotropy but rather rotation and the shape of the velocity dispersion tensor. The apparent isotropy of observed disky ellipticals is shown to result from inclination effects. Even small inclination angles strongly reduce the measured anisotropy of fast rotating systems, seen in projection. A second problem is the limited amount of information that is available when measuring only the central velocity dispersion and a characteristic rotation and ellipticity. Methods are investigated that allow a better determination of the intrinsic anisotropy of fast rotating early-type galaxies with known inclination angles.
description: 7 pages, 6 figures, submitted to MNRAS
Additional file 1 of Transplantation of a kidney with a heterozygous mutation in the SLC22A12 (URAT1) gene causing renal hypouricemia: a case report
Creators: name: Kiyokazu Tsuji
name: Kitamura, Mineaki
name: Muta, Kumiko
name: Mochizuki, Yasushi
name: Mori, Takayasu
name: Eisei Sohara
name: Uchida, Shinichi
name: Sakai, Hideki
name: Mukae, Hiroshi
name: Nishino, Tomoya
Publisher: name: figshare
Year: 2020
Subjects: subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Physiology
subject: Immunology
subject: FOS: Clinical medicine
subject: Developmental Biology
subject: Marine Biology
subject: Cancer
subject: Hematology
subject: 60506 Virology

description: Additional file 1: Supplemental Material 1. The American College of Medical Genetics and Genomics variant classifications variant classifications to (NM_144585.4:c.269G > A:p.(Arg90His).
Scale Invariance in the Spectral Action
Creators: name: Chamseddine, Ali H.
name: Connes, Alain
Publisher: name: arXiv
Year: 2005
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: The arbitrary mass scale in the spectral action for the Dirac operator in the spectral action is made dynamical by introducing a dilaton field. We evaluate all the low-energy terms in the spectral action and determine the dilaton couplings. These results are applied to the spectral action of the noncommutative space defined by the standard model. We show that the effective action for all matter couplings is scale invariant, except for the dilaton kinetic term and Einstein-Hilbert term. The resulting action is almost identical to the one proposed for making the standard model scale invariant as well as the model for extended inflation and has the same low-energy limit as the Randall-Sundrum model. Remarkably, all desirable features with correct signs for the relevant terms are obtained uniquely and without any fine tuning.
description: 27 pages, spectral function defined, one reference added. Form to be published in Journal Mathematical Physics
A Solution to Symmetric Teleparallel Gravity
Creators: name: Adak, Muzaffer
name: Sert, Ozcan
Publisher: name: arXiv
Year: 2004
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: Teleparallel gravity models, in which the curvature and the nonmetricity of spacetime are both set zero, are widely studied in the literature. We work a different teleparallel theory, in which the curvature and the torsion of spacetime are both constrained to zero, but the nonmetricity is nonzero. After reformulating the general relativity in this spacetime we find a solution and investigate its singularity structure.
description: 7 pages, LaTeX, original part of O. Sert's M.Sc. thesis
V453 Oph: a s-process enriched, but carbon-deficient RV Tauri star of low intrinsic metallicity
Creators: name: Deroo, Pieter
name: Reyniers, Maarten
name: Van Winckel, Hans
name: Goriely, Stephane
name: Siess, Lionel
Publisher: name: arXiv
Year: 2005
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: This paper reports the detection of a heavy element enriched RV Tauri variable with an abundance pattern that differs significantly from a standard s-process enriched object: V453 Oph. Based on optical high-resolution spectra, we determined that this object of low intrinsic metallicity ([Fe/H] = -2.2) has a mild, but significant, enrichment ([s/Fe] ~ +0.5) of heavy elements for which the distribution points to slow neutron capture nucleosynthesis. This result is strengthened by a comparative analysis to the non-enriched RV Tauri star DS Aqr ([s/Fe] = 0.0). Although V453 Oph is the first RV Tauri star showing a strong s-process signature, it is NOT accompanied by C enhancement, challenging our current nucleosynthetic models of post-AGB stars that predict a simultaneous enrichment in C and s-process elements. The low N abundance excludes CN cycling as being responsible for the low C abundance. We explore three different scenarios to explain the heavy element distribution in this evolved object: an enrichment of the parental cloud, an accretion scenario in which the chemical patterns were acquired by mass transfer in a binary system and an intrinsic enrichment by dredge-up.
description: Accepted for publication in A&A
[Utkast til Sidste Blade] / Camilla Collett
Creators: name: Collett, Camilla
Publisher: name: Unknown
Year: 1868

description: Teksten er ikke identisk med den trykte, men den svarer til Sidste Blade [1], 1868, s. 13-27, 34-41, 42-50 (med større avvik fra den trykte tekst), 170-176.
Conformational Properties of an Adsorbed Charged Polymer
Creators: name: Cheng, Chi-Ho
name: Lai, Pik-Yin
Publisher: name: arXiv
Year: 2004
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: Chemical Physics (physics.chem-ph)
subject: FOS: Physical sciences

description: The behavior of a strongly charged polymer adsorbed on an oppositely charged surface of low-dielectric constant is formulated by the functional integral method. By separating the translational, conformational, and fluctuational degrees of freedom, the scaling behaviors for both the height of the polymer and the thickness of the diffusion layer are determined. Unlike the results predicted by scaling theory, we identified the continuous crossover from the weak compression to the compression regime. All teh analytical results are found to be consistent with Monte-Carlo simulations. Finally, an alternative (operational) definition of a charged polymer adsorption is proposed.
description: 4 pages, 3 figures
Additional file 2 of The role of contraception in preventing HIV-positive births: global estimates and projections
Creators: name: Sherwood, Jennifer
name: Lankiewicz, Elise
name: Beirne Roose-Snyder
name: Bergen Cooper
name: Jones, Austin
name: Honermann, Brian
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Biotechnology
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Cancer
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Additional file 2.
Torsional Landau levels and geometric anomalies in condensed matter Weyl systems
Creators: name: Laurila, Sara
name: Nissinen, Jaakko
Publisher: name: arXiv
Year: 2020
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We consider the role of coordinate dependent tetrads ("Fermi velocities"), momentum space geometry, and torsional Landau levels (LLs) in condensed matter systems with low-energy Weyl quasiparticles. In contrast to their relativistic counterparts, they arise at finite momenta and an explicit cutoff to the linear spectrum. Via the universal coupling of tetrads to momentum, they experience geometric chiral and axial anomalies with gravitational character. More precisely, at low-energy, the fermions experience background fields corresponding to emergent anisotropic Riemann-Cartan and Newton-Cartan spacetimes, depending on the form of the low-energy dispersion. On these backgrounds, we show how torsion and the Nieh-Yan (NY) anomaly appear in condensed matter Weyl systems with a ultraviolet (UV) parameter with dimensions of momentum. The torsional NY anomaly arises in simplest terms from the spectral flow of torsional LLs coupled to the nodes at finite momenta and the linear approximation with a cutoff. We carefully review the torsional anomaly and spectral flow for relativistic fermions at zero momentum and contrast this with the spectral flow, non-zero torsional anomaly and the appearance the dimensionful UV-cutoff parameter in condensed matter systems at finite momentum. We apply this to chiral transport anomalies sensitive to the emergent tetrads in non-homogenous chiral superconductors, superfluids and Weyl semimetals under elastic strain. This leads to the suppression of anomalous density at nodes from geometry, as compared to (pseudo)gauge fields. We also briefly discuss the role torsion in anomalous thermal transport for non-relativistic Weyl fermions, which arises via Luttinger's fictitious gravitational field corresponding to thermal gradients.
description: 21 pages, several figures, minor changes and updated refs
THE FATALITY OF LOVE IN THE STORY 'TRICKS' BY ALICE MUNRO
Creators: name: Ibodova Maknuna Bahodirovna
Publisher: name: Zenodo
Year: 2024

description: Critical readings of Munro’s work have been prolific, throughout her writing life, especially in the form of academic articles. Already in the mid 1970s, articles on separate stories began to appear in academic journals.  Since the beginning of Munro’s career critics have continued to be fascinated and puzzled by her particular twist of realism, but no one has exposed the realism as connected to her exploration of possibility as arising out of fatality, no critic has explored the tension between possibility and fatality that we see at the heart of Munro’s writing.
A Review on Machine Learning for Neutrino Experiments
Creators: name: Psihas, Fernanda
name: Groh, Micah
name: Tunnell, Christopher
name: Warburton, Karl
Publisher: name: arXiv
Year: 2020
Subjects: subject: Computational Physics (physics.comp-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: Neutrino experiments study the least understood of the Standard Model particles by observing their direct interactions with matter or searching for ultra-rare signals. The study of neutrinos typically requires overcoming large backgrounds, elusive signals, and small statistics. The introduction of state-of-the-art machine learning tools to solve analysis tasks has made major impacts to these challenges in neutrino experiments across the board. Machine learning algorithms have become an integral tool of neutrino physics, and their development is of great importance to the capabilities of next generation experiments. An understanding of the roadblocks, both human and computational, and the challenges that still exist in the application of these techniques is critical to their proper and beneficial utilization for physics applications. This review presents the current status of machine learning applications for neutrino physics in terms of the challenges and opportunities that are at the intersection between these two fields.
Additional file 3 of The role of contraception in preventing HIV-positive births: global estimates and projections
Creators: name: Sherwood, Jennifer
name: Lankiewicz, Elise
name: Beirne Roose-Snyder
name: Bergen Cooper
name: Jones, Austin
name: Honermann, Brian
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Biotechnology
subject: 19999 Mathematical Sciences not elsewhere classified
subject: FOS: Mathematics
subject: Cancer
subject: 110309 Infectious Diseases
subject: FOS: Health sciences
subject: Computational Biology

description: Additional file 3.
Van den Oudenrijn, Mark-Antoine: Gamaliel
Creators: name: Engberding, Hieronymus
Publisher: name: Oriens christianus : Hefte für die Kunde des christlichen Orients
Year: 2024

description: Oriens christianus : Hefte für die Kunde des christlichen Orients, Bd. 44 (1960): Oriens christianus, Band 44
A time-scale modification dataset with subjective quality labels
Creators: name: Roberts, Timothy
name: Paliwal, Kuldip K.
Publisher: name: arXiv
Year: 2020
Subjects: subject: Audio and Speech Processing (eess.AS)
subject: Sound (cs.SD)
subject: FOS: Electrical engineering, electronic engineering, information engineering
subject: FOS: Computer and information sciences

description: Time Scale Modification (TSM) is a well-researched field; however, no effective objective measure of quality exists. This paper details the creation, subjective evaluation, and analysis of a dataset for use in the development of an objective measure of quality for TSM. Comprised of two parts, the training component contains 88 source files processed using six TSM methods at 10 time scales, while the testing component contains 20 source files processed using three additional methods at four time scales. The source material contains speech, solo harmonic and percussive instruments, sound effects, and a range of music genres. Ratings (42 529) were collected from 633 sessions using laboratory and remote collection methods. Analysis of results shows no correlation between age and quality of rating; expert and non-expert listeners to be equivalent; minor differences between participants with and without hearing issues; and minimal differences between testing modalities. A comparison of published objective measures and subjective scores shows the objective measures to be poor indicators of subjective quality. Initial results for a retrained objective measure of quality are presented with results approaching average root mean squared error loss and Pearson correlation values of subjective sessions. The labeled dataset is available at http://ieee-dataport.org/1987.
description: 12 Pages, 13 Figures, Published in The Journal of the Acoustical Society of America (Vol.148, Issue 1), For associated dataset, see http://ieee-dataport.org/1987
Positive Market Effects from a Meatpacking Plant Opening: Perceptions and Reality
Creators: name: Hornung, Jonathan T.
name: Ward, Clement E.
name: Hornung, Jonathan T.
name: Ward, Clement E.
Publisher: name: Unknown
Year: 2005
Subjects: Agribusiness
Demand and Price Analysis

description: Economic theory suggests that adding a competitive buyer to a market should have positive effects on competition and prices, ceteris paribus. An additional buyer increases market demand, shifting demand to the right, and expands the number of active buyers, reducing average market shares of existing buyers while intensifying bidding competition. Whether or not these positive impacts occur in reality is an empirical question. The largest pork processor in Canada, Maple Leaf Foods Inc., opened a 45,000 head/week hog processing facility in August 1999 in Brandon, Manitoba. The plant opened during a period of expanding hog production in Canada, of increasing hog exports to the United States, and of increasingly tight processing capacity in the United States (Luby, 1999; Parcell, Mintert, and Plain, 2004). Most previous research on the impacts of meat processing plants has focused on plant closings, and none has estimated the effects of a plant opening under conditions of expanding production and tight processing capacity. Research reported here expands previous work by taking a dual approach to the question. First, two models were used to estimate market price impacts from the plant opening. Second, a survey of Manitoba pork producers provided insight into the perceived market dynamics of the plant opening.
Schenke, Hans-Martin: Die Herkunft des sogenannten Evangelium Veritatis
Creators: name: Hammerschmidt, Ernst
Publisher: name: Oriens christianus : Hefte für die Kunde des christlichen Orients
Year: 2024

description: Oriens christianus : Hefte für die Kunde des christlichen Orients, Bd. 44 (1960): Oriens christianus, Band 44
Supernovae: Explosions in the Cosmos
Creators: name: Suresh, P K
name: Kumar, V H Satheesh
Publisher: name: arXiv
Year: 2005
Subjects: subject: Astrophysics (astro-ph)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: In this article, a broad perspective of supernovae, their classification and mechanism is given. Later, the astrophysical significance of supernovae is discussed in brief.
description: 8 pages, 8 figures, submitted to Science Reporter
Animal spectacula of the Roman Empire
Creators: name: Epplett, William Christopher
Publisher: name: University of British Columbia
Year: 2009

description: Although gladiatorial spectacles in ancient Rome have been the subject of a great deal of recent scholarly literature, comparatively little attention has been paid to the contemporary animal spectacles and staged beast-hunts (venationes), the events most closely associated with gladiatorial combat in the imperial period. A number of different works have dealt with such topics as the origins and organization of gladiatorial combat in ancient Rome, but relatively few scholars have attempted to address similar questions concerning the venationes. Only a single monograph in English, written approximately 60 years ago, has been produced on the phenomenon of Roman animal spectacles. The purpose of .this thesis is to give a comprehensive account of Roman venationes and animal displays, incorporating, in certain cases, evidence that has only recently become available or has largely been overlooked by previous scholars. A wide variety of evidence will be used in this study, ranging from literary sources to archaeological data. The paper will trace the historical development of these spectacles, from Republican displays staged in imitation of contemporary Greek events, to the beasthunts of the Byzantine empire. Another major focus of the thesis will be the infrastructure and organization behind Roman animal spectacles, in particular the methods by which the Romans captured and transported the large numbers of animals necessary for events staged throughout the empire.
Additional file 2 of Optical microscopy reveals the dynamic nature of B. pseudomallei morphology during β-lactam antimicrobial susceptibility testing
Creators: name: McLaughlin, Heather P.
name: Bugrysheva, Julia
name: Sue, David
Publisher: name: figshare
Year: 2020
Subjects: subject: Biophysics
subject: Biochemistry
subject: Space Science
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Molecular Biology
subject: Pharmacology
subject: Biotechnology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Ecology
subject: Developmental Biology
subject: Cancer
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Additional file 2: Figure S2. Cell morphology ofB. pseudomallei6788 in the presence and absence of AMC (μg/ml). Optical screen images were captured after 6 h. Amoxicillin-clavulanic acid (AMC), CLSI breakpoints for susceptibility (green dotted line), MIC (blue line).
Epistler [5 del, 1. epistel] s. 24 : derav et stykke som censor prof. J.P. Anchersen ikke ville tillate trykt da epistlene etter forfatterens død ble utgitt
Creators: name: Holberg, Ludvig
Publisher: name: Unknown
Year: 1740

description: Avskrift ved Benjamin Dass.
description: Trykt i A.E. Boye: Holbergiana, 2. del s. 46-50.
description: Se også Frederik Fabricius: 120 af Holbergs Epistler, s. 383-387.
A deep learning view of the census of galaxy clusters in IllustrisTNG
Creators: name: Su, Y.
name: Zhang, Y.
name: Liang, G.
name: ZuHone, J. A.
name: Barnes, D. J.
name: Jacobs, N. B.
name: Ntampaka, M.
name: Forman, W. R.
name: Nulsen, P. E. J.
name: Kraft, R. P.
name: Jones, C.
Publisher: name: arXiv
Year: 2020
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: The origin of the diverse population of galaxy clusters remains an unexplained aspect of large-scale structure formation and cluster evolution. We present a novel method of using X-ray images to identify cool core (CC), weak cool core (WCC), and non cool core (NCC) clusters of galaxies, that are defined by their central cooling times. We employ a convolutional neural network, ResNet-18, which is commonly used for image analysis, to classify clusters. We produce mock Chandra X-ray observations for a sample of 318 massive clusters drawn from the IllustrisTNG simulations. The network is trained and tested with low resolution mock Chandra images covering a central 1 Mpc square for the clusters in our sample. Without any spectral information, the deep learning algorithm is able to identify CC, WCC, and NCC clusters, achieving balanced accuracies (BAcc) of 92%, 81%, and 83%, respectively. The performance is superior to classification by conventional methods using central gas densities, with an average BAcc = 81%, or surface brightness concentrations, giving BAcc = 73%. We use Class Activation Mapping to localize discriminative regions for the classification decision. From this analysis, we observe that the network has utilized regions from cluster centers out to r~300 kpc and r~500 kpc to identify CC and NCC clusters, respectively. It may have recognized features in the intracluster medium that are associated with AGN feedback and disruptive major mergers.
description: Accepted for publication in MNRAS
Additional file 7 of Influence of particle aggregation on the tephra dispersal and sedimentation from the October 8, 2016, eruption of Aso volcano
Creators: name: Tsuji, Tomohiro
name: Nishizaka, Naoki
name: Ohnishi, Kozo
Publisher: name: figshare
Year: 2020
Subjects: subject: Biotechnology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Ecology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: Inorganic Chemistry

description: Additional file 7. Particle density and terminal fall velocity as a function of grain size. Grain densities were calculated from the linear trend in Additional file 5.
Aandelig Samtale imellem Troen og en beængsted Siæl / af Samuel Slatter
Creators: name: Slatter, Samuel
Publisher: name: Unknown
Year: 1750

description: På tittelbladet: Af Samuel Slatters Engl. Poems P. II efter Philander von der Lindes tydske Oversættelse i det danske Sprog oversat ved Ole Molde, sogneprest i Maasøe menighed i Vest-Finmarken.
Turbulent Origin of the Galactic-Center Magnetic Field: Nonthermal Radio Filaments
Creators: name: Boldyrev, Stanislav
name: Yusef-Zadeh, Farhad
Publisher: name: arXiv
Year: 2005
Subjects: subject: Astrophysics (astro-ph)
subject: Fluid Dynamics (physics.flu-dyn)
subject: Plasma Physics (physics.plasm-ph)
subject: FOS: Physical sciences

description: A great deal of study has been carried out over the last twenty years on the origin of the magnetic activity in the Galactic center. One of the most popular hypotheses assumes milli-Gauss magnetic field with poloidal geometry, pervading the inner few hundred parsecs of the Galactic-center region. However, there is a growing observational evidence for the large-scale distribution of a much weaker field of B \lesssim 10 micro G in this region. Here, we propose that the Galactic-center magnetic field originates from turbulent activity that is known to be extreme in the central hundred parsecs. In this picture the spatial distribution of the magnetic field energy is highly intermittent, and the regions of strong field have filamentary structures. We propose that the observed nonthermal radio filaments appear in (or, possibly, may be identified with) such strongly magnetized regions. At the same time, the large-scale diffuse magnetic field is weak. Both results of our model can explain the magnetic field measurements of the the Galactic-center region. In addition, we discuss the role of ionized outflow from stellar clusters in producing the long magnetized filaments perpendicular to the Galactic plane.
description: 11 pages, accepted to ApJ Letters
Predicting the Activity and Selectivity of Bimetallic Metal Catalysts for Ethanol Reforming using Machine Learning
Creators: name: Artrith, Nongnuch
name: Lin, Zhexi
name: Chen, Jingguang G.
Publisher: name: arXiv
Year: 2020
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Machine learning is ideally suited for the pattern detection in large uniform datasets, but consistent experimental datasets on catalyst studies are often small. Here we demonstrate how a combination of machine learning and first-principles calculations can be used to extract knowledge from a relatively small set of experimental data. The approach is based on combining a complex machine-learning model trained on a computational library of transition-state energies with simple linear regression models of experimental catalytic activities and selectivities from the literature. Using the combined model, we identify the key C-C bond scission reactions involved in ethanol reforming and perform a computational screening for ethanol reforming on monolayer bimetallic catalysts with architectures TM-Pt-Pt(111) and Pt-TM-Pt(111) (TM = 3d transition metals). The model also predicts four promising catalyst compositions for future experimental studies. The approach is not limited to ethanol reforming but is of general use for the interpretation of experimental observations as well as for the computational discovery of catalytic materials.
description: 29 pages, 10 figures, 2 Tables
P.Oxy. LXXXVII 5583. Antiphon, On Truth 1 (?)
Creators: name: Oxford Papyrology
Publisher: name: University of Oxford
Year: 2023
Subjects: classificationCode: 470316
subject: Latin and classical Greek languages

description: Reproduction requests: https://www.ees.ac.uk/reproduction-requests-and-fees
New constraint on the cosmological background of relativistic particles
Creators: name: Hannestad, Steen
Publisher: name: arXiv
Year: 2005
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have derived new bounds on the relativistic energy density in the Universe from cosmic microwave background (CMB), large scale structure (LSS), and type Ia supernova (SNI-a) observations. In terms of the effective number of neutrino species a bound of N_ν= 4.2^{+1.2}_{-1.7} is derived at 95% confidence. This bound is significantly stronger than previous determinations, mainly due to inclusion of new CMB and SNI-a observations. The absence of a cosmological neutrino background (N_ν= 0) is now excluded at 5.4 σ. The value of N_νis compatible with the value derived from big bang nucleosynthesis considerations, marking one of the most remarkable successes of the standard cosmological model. In terms of the cosmological helium abundance, the CMB, LSS, and SNI-a observations predict a value of 0.240 < Y < 0.281.
description: 10 pages, 3 figures, references added
Additional file 1 of Optical microscopy reveals the dynamic nature of B. pseudomallei morphology during β-lactam antimicrobial susceptibility testing
Creators: name: McLaughlin, Heather P.
name: Bugrysheva, Julia
name: Sue, David
Publisher: name: figshare
Year: 2020
Subjects: subject: Biophysics
subject: Biochemistry
subject: Space Science
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Molecular Biology
subject: Pharmacology
subject: Biotechnology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Ecology
subject: Developmental Biology
subject: Cancer
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Additional file 1: Figure S1. Growth kinetics ofB. pseudomalleistrains evaluated over 18 h in the presence and absence of β-lactams. Bp1651 exposed to AMC (A) and IPM (B), MSHR1655 exposed to CAZ (C) and 724644 exposed to IPM (D). Drug concentrations (μg/ml) corresponding to the CLSI breakpoint for susceptibility (green dots) and MICs (blue dots). Graphs represent the average ± standard deviation from triplicate samples. Amoxicillin-clavulanic acid (AMC), ceftazidime (CAZ), and imipenem (IPM)