cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Study of the process $e^+ e^- \to K^0_{S}K^0_{L}$ in the center-of-mass energy range 1004--1060 MeV with the CMD-3 detector at the VEPP-2000 $e^+ e^-$ collider
Creators: name: Kozyrev, E. A.
Publisher: name: arXiv
Year: 2016
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: The $e^+ e^- \to K^0_{S}K^0_{L}$ cross section has been measured in the center-of-mass energy range 1004--1060 MeV at 25 energy points using $6.1 \times 10^5$ events with $K^0_{S}\to π^+π^-$ decay. The analysis is based on 5.9 pb$^{-1}$ of an integrated luminosity collected with the CMD-3 detector at the VEPP-2000 $e^+ e^-$ collider. To obtain $ϕ(1020)$ meson parameters the measured cross section is approximated according to the Vector Meson Dominance model as a sum of the $ρ, ω, ϕ$-like amplitudes and their excitations. This is the most precise measurement of the $e^+ e^- \to K^0_{S}K^0_{L}$ cross section with a 1.8\% systematic uncertainty.
description: 14 pages, 10 figures, journal paper
Observationally constraining gravitational wave emission from short gamma-ray burst remnants
Creators: name: Lasky, Paul D
name: Glampedakis, Kostas
Publisher: name: arXiv
Year: 2015
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: Observations of short gamma-ray bursts indicate ongoing energy injection following the prompt emission, with the most likely candidate being the birth of a rapidly rotating, highly magnetised neutron star. We utilise X-ray observations of the burst remnant to constrain properties of the nascent neutron star, including its magnetic field-induced ellipticity and the saturation amplitude of various oscillation modes. Moreover, we derive strict upper limits on the gravitational wave emission from these objects by looking only at the X-ray light curve, showing the burst remnants are unlikely to be detected in the near future using ground-based gravitational wave interferometers such as Advanced LIGO.
description: Accepted for publication in MNRAS
The minimal length and the Shannon entropic uncertainty relation
Creators: name: Pedram, Pouria
Publisher: name: arXiv
Year: 2016
Subjects: subject: Quantum Physics (quant-ph)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: In the framework of the generalized uncertainty principle, the position and momentum operators obey the modified commutation relation $[X,P]=i\hbar\left(1+βP^2\right)$ where $β$ is the deformation parameter. Since the validity of the uncertainty relation for the Shannon entropies proposed by Beckner, Bialynicki-Birula, and Mycieslki (BBM) depends on both the algebra and the used representation, we show that using the formally self-adjoint representation, i.e., $X=x$ and $P=\tan\left(\sqrtβp\right)/\sqrtβ$ where $[x,p]=i\hbar$, the BBM inequality is still valid in the form $S_x+S_p\geq1+\lnπ$ as well as in ordinary quantum mechanics. We explicitly indicate this result for the harmonic oscillator in the presence of the minimal length.
description: 9 pages, 3 figures
Scanning of the Supersymmetry Breaking Scale and the Gravitino Mass in Supergravity
Creators: name: Farakos, Fotis
name: Kehagias, Alex
name: Racco, Davide
name: Riotto, Antonio
Publisher: name: arXiv
Year: 2016
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We consider the minimal three-form ${\cal N}=1$ supergravity coupled to nilpotent three-form chiral superfields. The supersymmetry breaking is sourced by the three-forms of the chiral multiplets, while the value of the gravitino mass is controlled by the three-form of the supergravity multiplet. The three-forms can nucleate membranes which scan both the supersymmetry breaking scale and the gravitino mass. The peculiar supergravity feature that the cosmological constant is the sum of a positive contribution from the supersymmetry breaking scale and a negative contribution from the gravitino mass makes the cosmological constant jump. This can lead to a phenomenologically allowed small value of the cosmological constant even though the supersymmetry breaking scale and the gravitino mass are dynamically large.
description: 18 pages, 2 figures, JHEP version, citations added
Polarimetric Detection of Exoplanets Transiting T- and L- Brown Dwarfs
Creators: name: Sengupta, Sujan
Publisher: name: arXiv
Year: 2016
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: While scattering of light by atoms and molecules yields large amount of polarization at the B-band of both T- and L-dwarfs, scattering by dust grains in cloudy atmosphere of L-dwarfs gives rise to significant polarization at the far-optical and infra-red wavelengths where these objects are much brighter. However, the observable disk averaged polarization should be zero if the clouds are uniformly distributed and the object is spherically symmetric. Therefore, in order to explain the observed large polarization of several L-dwarfs, rotation-induced oblateness or horizontally inhomogeneous cloud distribution in the atmosphere is invoked. On the other hand, when an extra-solar planet of Earth-size or larger transits the brown dwarf along the line of sight, the asymmetry induced during the transit gives rise to a net non-zero, time dependent polarization. Employing atmospheric models for a range of effective temperature and surface gravity appropriate for T- and L-dwarfs, I derive the time dependent polarization profiles of these objects during transit phase and estimate the peak amplitude of polarization that occurs during the inner contact points of the transit ingress/egress phase. It is found that peak polarization in the range of 0.2-1.0 % at I- and J-band may arise of cloudy L dwarfs occulted by Earth-size or larger exoplanets. Such an amount of polarization is higher than that can be produced by rotation-induced oblateness of even the rapidly rotating L-dwarfs. Hence, I suggest that time resolved imaging polarization should be a potential technique to detect transiting exoplanets around L-dwarfs.
description: 17 pages (AASTEX) including 5 eps figures. Accepted for publication in The Astronomical Journal
title: WP2 Manchester Local Area Energy Strategy: Planning Briefing Notes Informing Stage 0 GM Spatial Energy Plan – Briefing Note 4
Creators: name: Jones Lang LaSalle Ltd (JLL)
Publisher: name: ETI
Year: 2016
Subjects: subject: Smart Systems and Heat
subject: ENERGY EFFICIENCY (Residential and commercial)
subject: OTHER CROSS-CUTTING TECHNOLOGIES or RESEARCH (Other Supporting Data)

description: he Spatial Energy Plan for Greater Manchester Combined Authority project was commissioned as part of the Energy Technologies Institute (ETI) Smart Systems and Heat Programme and undertaken through collaboration between the Greater Manchester Combined Authority and the Energy Systems Catapult.The study has consolidated the significant data and existing evidence relating to the local energy system to provide a platform for future energy planning in the region and the development of suitable policies within the emerging spatial planning framework for Greater Manchester.

This Deliverable comprises one of a series of four briefing notes regarding the planning policy and related information to inform the production of a high level energy evidence base prior to the completion of a detailed EnergyPath modelling study with a local authority in Greater Manchester. It provides advice and recommendations relating to the current and future policy framework in GM which has informed the Catapult high level energy study for Greater Manchester. This Deliverable, Briefing Note 4, considers the possible policy levers and mechanisms that could be adopted and included within the Greater Manchester Spatial Framework to support energy system transformation and carbon reduction ambitions.
High-harmonic generation in liquids with few-cycle pulses: effect of laser-pulse duration on the cut-off energy
Creators: name: Mondal, Angana
name: Waser, Benedikt
name: Balciunas, Tadas
name: Neufeld, Ofer
name: Yin, Zhong
name: Tancogne-Dejean, Nicolas
name: Rubio, Angel
name: Wörner, Hans Jakob
Publisher: name: arXiv
Year: 2022
Subjects: subject: Optics (physics.optics)
subject: Atomic and Molecular Clusters (physics.atm-clus)
subject: Atomic Physics (physics.atom-ph)
subject: Chemical Physics (physics.chem-ph)
subject: FOS: Physical sciences

description: High-harmonic generation (HHG) in liquids is opening new opportunities for attosecond light sources and attosecond time-resolved studies of dynamics in the liquid phase. In gas-phase HHG, few-cycle pulses are routinely used to create isolated attosecond pulses and to extend the cut-off energy. Here, we study the properties of HHG in liquids, including water and several alcohols, by continuously tuning the pulse duration of a mid-infrared driver from the multi- to the sub-two-cycle regime. Similar to the gas phase, we observe the transition from discrete odd-order harmonics to continuous extreme-ultraviolet emission. However, the cut-off energy is shown to be entirely independent of the pulse duration. This observation is confirmed by ab-initio simulations of HHG in large clusters. Our results support the notion that the cut-off energy is a fundamental property of the liquid, independent of the driving-pulse properties. Combined with the recently reported wavelength-independence of the cutoff, these results confirm the direct sensitivity of HHG to the mean-free paths of slow electrons in liquids. Our results additionally imply that few-cycle mid-infrared laser pulses are suitable drivers for generating isolated attosecond pulses from liquids.
description: 9 pages, 5 figures
Theoretical uncertainty of the supersymmetric dark matter relic density from scheme and scale variations
Creators: name: Harz, J.
name: Herrmann, B.
name: Klasen, M.
name: Kovarik, K.
name: Steppeler, P.
Publisher: name: arXiv
Year: 2016
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: For particle physics observables at colliders such as the LHC at CERN, it has been common practice for many decades to estimate the theoretical uncertainty by studying the variations of the predicted cross sections with a priori unpredictable scales. In astroparticle physics, this has so far not been possible, since most of the observables were calculated at Born level only, so that the renormalization scheme and scale dependence could not be studied in a meaningful way. In this paper, we present the first quantitative study of the theoretical uncertainty of the neutralino dark matter relic density from scheme and scale variations. We first explain in detail how the renormalization scale enters the tree-level calculations through coupling constants, masses and mixing angles. We then demonstrate a reduction of the renormalization scale dependence through one-loop SUSY-QCD corrections in many different dark matter annihilation channels and enhanced perturbative stability of a mixed on-shell/$\bar{\rm DR}$ renormalization scheme over a pure $\bar{\rm DR}$ scheme in the top-quark sector. In the stop-stop annihilation channel, the Sommerfeld enhancement and its scale dependence are shown to be of particular importance. Finally, the impact of our higher-order SUSY-QCD corrections and their scale uncertainties are studied in three typical scenarios of the phenomenological Minimal Supersymmetric Standard Model with eleven parameters (pMSSM-11). We find that the theoretical uncertainty is reduced in many cases and can become comparable to the size of the experimental one in some scenarios.
description: 17 pages, 16 figures, 3 tables
Gromov-Hausdorff distance between vertex sets of regular polygons inscribed in a given circle
Creators: name: Talipov, Talant
Publisher: name: arXiv
Year: 2022
Subjects: subject: Metric Geometry (math.MG)
subject: Combinatorics (math.CO)
subject: FOS: Mathematics
subject: 51F99 (Primary)

description: We calculate the Gromov-Hausdorff distance between vertex sets of regular polygons endowed with the round metric. We give a full answer for the case of n- and m-gons with m divisible by n. Also, we calculate all distances to 2-gons and 3-gons
description: 7 pages, 0 figures, submitted to Moscow University Mathematics Bulletin
Biblische Perspektiven zum Verhältnis von Homosexualität und sexueller Identität
Creators: name: Gagnon, Robert A. J.
Publisher: name: Jahrbuch für evangelikale Theologie
Year: 2025

description: 1646907493
description: Jahrbuch für evangelikale Theologie, V. 24 (2010): Jahrbuch für evangelikale Theologie, Band 24
Kriminalitätsbericht 2006. Statistik und Analyse
Creators: name: (:Unkn) Unknown
Publisher: name: Universität Tübingen
Year: 2006
Subjects: subject: Österreich , Kriminalität , Statistik
subject: 360

description: Mit dem vorliegenden Kriminalitätsbericht werden die von den Sicherheitsbehörden und Sicherheitsdienststellen im Berichtsjahr gemeldeten Daten über die bekannt gewordenen gerichtlich strafbaren Handlungen veröffentlicht. Der Kriminalitätsbericht ist eine Anzeigenstatistik, das heißt, die Daten werden anlässlich der Vorlage der Anzeige über eine strafbare Handlung an die Strafverfolgungsbehörde in die Datenbank der EDV-Zentrale des Bundesministeriums für Inneres gespeichert, dort aufbereitet und vom Bundeskriminalamt zu den veröffentlichten Tabellen verarbeitet. Ziel des Kriminalitätsberichtes ist es, unter sinnvoller Beschränkung der zu erfassenden Daten und mit ökonomisch vertretbarem Arbeitsaufwand ein möglichst umfassendes und realitätsgerechtes Bild des bekannt gewordenen kriminellen Geschehens zu bieten.
Motion Matters: A Novel Motion Modeling For Cross-View Gait Feature Learning
Creators: name: Li, Jingqi
name: Gao, Jiaqi
name: Zhang, Yuzhen
name: Shan, Hongming
name: Zhang, Junping
Publisher: name: arXiv
Year: 2022
Subjects: subject: Computer Vision and Pattern Recognition (cs.CV)
subject: FOS: Computer and information sciences

description: As a unique biometric that can be perceived at a distance, gait has broad applications in person authentication, social security, and so on. Existing gait recognition methods suffer from changes in viewpoint and clothing and barely consider extracting diverse motion features, a fundamental characteristic in gaits, from gait sequences. This paper proposes a novel motion modeling method to extract the discriminative and robust representation. Specifically, we first extract the motion features from the encoded motion sequences in the shallow layer. Then we continuously enhance the motion feature in deep layers. This motion modeling approach is independent of mainstream work in building network architectures. As a result, one can apply this motion modeling method to any backbone to improve gait recognition performance. In this paper, we combine motion modeling with one commonly used backbone~(GaitGL) as GaitGL-M to illustrate motion modeling. Extensive experimental results on two commonly-used cross-view gait datasets demonstrate the superior performance of GaitGL-M over existing state-of-the-art methods.
A parametrized quasi-normal mode framework for non-Schwarzschild metrics
Creators: name: Franchini, Nicola
name: Völkel, Sebastian H.
Publisher: name: arXiv
Year: 2022
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: In this work we comment in more detail on what happens to the parametrized framework first presented by Cardoso et al. when there are departures from the Schwarzschild background metric, as well as possible deviations in the "dynamics". We treat possible deviations in the background metric with additional coefficients with respect to the original works. The advantages of this reformulation are clear when applied to a parameter estimation problem, since the coefficients are always real, and many of them do not depend on the overtone number and angular momentum of the frequency, thus eventually reducing the total amount of parameters to be inferred.
description: 5 pages, 2 figures
Bericht Internet-Sicherheit Österreich 2014
Creators: name: (:Unkn) Unknown
Publisher: name: Universität Tübingen
Year: 2015
Subjects: subject: Österreich , Internet , Sicherheit , Bericht
subject: 360

description: Der Bericht zur Internet-Sicherheit Österreich 2014 von CERT.at und GovCERT Austria fasst die wichtigsten Themen des Jahres zusammen und gibt einen Überblick über die Aktivitäten der CERTs. Neben Statistiken aus der technischen Arbeit wird auch der aktuelle Stand der Umsetzung von Österreichs Strategie für Cyber Sicherheit präsentiert.
Diffusion towards a nanoforest of absorbing pillars
Creators: name: Grebenkov, Denis S.
name: Skvortsov, Alexei T.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Chemical Physics (physics.chem-ph)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: Spiky coatings (also known as nanoforests or Fakir-like surfaces) have found many applications in chemical physics, material sciences and biotechnology, such as superhydrophobic materials, filtration and sensing systems, selective protein separation, to name but a few. In this paper, we provide a systematic study of steady-state diffusion towards a periodic array of absorbing cylindrical pillars protruding from a flat base. We approximate a periodic cell of this system by a circular tube containing a single pillar, derive an exact solution of the underlying Laplace equation, and deduce a simple yet exact representation for the total flux of particles onto the pillar. The dependence of this flux on the geometric parameters of the model is thoroughly analyzed. In particular, we investigate several asymptotic regimes such as a thin pillar limit, a disk-like pillar, and an infinitely long pillar. Our study sheds a light onto the trapping efficiency of spiky coatings and reveals the roles of pillar anisotropy and diffusional screening.
title: WP2 Manchester Local Area Energy Strategy: Assessment of Domestic Low Carbon Transition Pathways in Bury
Creators: name: De La Cruz, M.
Publisher: name: ETI
Year: 2017
Subjects: subject: Smart Systems and Heat
subject: ENERGY EFFICIENCY (Residential and commercial)
subject: OTHER CROSS-CUTTING TECHNOLOGIES or RESEARCH (Other Supporting Data)

description: The Spatial Energy Plan for Greater Manchester Combined Authority project was commissioned as part of the Energy Technologies Institute (ETI) Smart Systems and Heat Programme and undertaken through collaboration between the Greater Manchester Combined Authority and theEnergy Systems Catapult.The study has consolidated the significant data and existing evidence relating to the local energy system to provide a platform for future energy planning in the region and the development of suitable policies within the emerging spatial planning framework for Greater Manchester.

Arup was commissioned to undertake a high-level desktop screening of potential constraints not considered by the Energy Path Networks (EPN) tool to 15 specific low carbon, domestic pathways in different clusters in Bury.The factors assessed for constraints to the pathways were technical feasibility, flood risk, ground conditions, air quality, heritage and planning, and noise impact.The technologies considered were district heating, high temperature air source heat pumps (HT ASHP), hybrid heat pumps and low temperature air source heat pumps (LT ASHP). Each pathway was allocated a risk rating based on the constraints found to the implementation of these technologies at a domestic level.
Extending Velocity Channel Analysis for Studying Turbulence Anisotropies
Creators: name: Kandel, Dinesh
name: Lazarian, Alex
name: Pogosyan, Dmitri
Publisher: name: arXiv
Year: 2016
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We extend the velocity channel analysis (VCA), introduced by Lazarian & Pogosyan, of the intensity fluctuations in the velocity slices of position-position-velocity (PPV) spectroscopic data from Doppler broadened lines to study statistical anisotropy of the underlying velocity and density that arises in a turbulent medium from the presence of magnetic field. In particular, we study analytically how the anisotropy of the intensity correlation in the channel maps changes with the thickness of velocity channels. In agreement with the earlier VCA studies we find that the anisotropy in the thick channels reflects the anisotropy of the density field, while the relative contribution of density and velocity fluctuations to the thin velocity channels depends on the density spectral slope. We show that the anisotropies arising from Alfven, slow and fast magnetohydrodynamical modes are different, in particular, the anisotropy in PPV created by fast modes is opposite to that created by Alfven and slow modes, and this can be used to separate their contributions. We successfully compare our results with the recent numerical study of the PPV anisotropies measured with synthetic observations. We also extend our study to the medium with self-absorption as well as to the case of absorption lines. In addition, we demonstrate how the studies of anisotropy can be performed using interferometers.
description: 36 pages, 16 figures, Accepted to MNRAS, minor changes to match the accepted version
Auxo: Efficient Federated Learning via Scalable Client Clustering
Creators: name: Liu, Jiachen
name: Lai, Fan
name: Dai, Yinwei
name: Akella, Aditya
name: Madhyastha, Harsha
name: Chowdhury, Mosharaf
Publisher: name: arXiv
Year: 2022
Subjects: subject: Machine Learning (cs.LG)
subject: Distributed, Parallel, and Cluster Computing (cs.DC)
subject: FOS: Computer and information sciences

description: Federated learning (FL) is an emerging machine learning (ML) paradigm that enables heterogeneous edge devices to collaboratively train ML models without revealing their raw data to a logically centralized server. However, beyond the heterogeneous device capacity, FL participants often exhibit differences in their data distributions, which are not independent and identically distributed (Non-IID). Many existing works present point solutions to address issues like slow convergence, low final accuracy, and bias in FL, all stemming from client heterogeneity. In this paper, we explore an additional layer of complexity to mitigate such heterogeneity by grouping clients with statistically similar data distributions (cohorts). We propose Auxo to gradually identify such cohorts in large-scale, low-availability, and resource-constrained FL populations. Auxo then adaptively determines how to train cohort-specific models in order to achieve better model performance and ensure resource efficiency. Our extensive evaluations show that, by identifying cohorts with smaller heterogeneity and performing efficient cohort-based training, Auxo boosts various existing FL solutions in terms of final accuracy (2.1% - 8.2%), convergence time (up to 2.2x), and model bias (4.8% - 53.8%).
description: 18 pages
Adiabaticity and gravity theory independent conservation laws for cosmological perturbations
Creators: name: Romano, Antonio Enea
name: Mooij, Sander
name: Sasaki, Misao
Publisher: name: arXiv
Year: 2015
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We carefully study the implications of adiabaticity for the behavior of cosmological perturbations. There are essentially three similar but different definitions of non-adiabaticity: one is appropriate for a thermodynamic fluid $δP_{nad}$, another is for a general matter field $δP_{c,nad}$, and the last one is valid only on superhorizon scales. The first two definitions coincide if $c_s^2=c_w^2$ where $c_s$ is the propagation speed of the perturbation, while $c_w^2=\dot P/\dotρ$. Assuming the adiabaticity in the general sense, $δP_{c,nad}=0$, we derive a relation between the lapse function in the comoving sli\-cing $A_c$ and $δP_{nad}$ valid for arbitrary matter field in any theory of gravity, by using only momentum conservation. The relation implies that as long as $c_s\neq c_w$, the uniform density, comoving and the proper-time slicings coincide approximately for any gravity theory and for any matter field if $δP_{nad}=0$ approximately. In the case of general relativity this gives the equivalence between the comoving curvature perturbation $R_c$ and the uniform density curvature perturbation $ζ$ on superhorizon scales, and their conservation. We then consider an example in which $c_w=c_s$, where $δP_{nad}=δP_{c,nad}=0$ exactly, but the equivalence between $R_c$ and $ζ$ no longer holds. Namely we consider the so-called ultra slow-roll inflation. In this case both $R_c$ and $ζ$ are not conserved. In particular, as for $ζ$, we find that it is crucial to take into account the next-to-leading order term in $ζ$'s spatial gradient expansion to show its non-conservation, even on superhorizon scales. This is an example of the fact that adiabaticity (in the thermodynamic sense) is not always enough to ensure the conservation of $R_c$ or $ζ$.
description: 6 pages, accepted in Physics Letters B
Impact of Dietary Conditions in Diabetic Adults: Integrative Review
Creators: name: Santos, Jair
name: Ribeiro, Chan
name: Costa, João
name: Ferreira, Luís
Publisher: name: figshare
Year: 2023
Subjects: Public health nutrition
Health surveillance
Social determinants of health
Behavioural epidemiology
Nutritional epidemiology

description: This reaseach is a integrative review of literature about the following theme "Impact of Dietary Conditions in Diabetic Adults: Integrative Review"
Equation of state for neutron stars with hyperons by the variational method
Creators: name: Togashi, H.
name: Hiyama, E.
name: Yamamoto, Y.
name: Takano, M.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Nuclear Theory (nucl-th)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We investigate the effects of the odd-state part of bare $ΛΛ$ interactions on the structure of neutron stars (NSs) by constructing equations of state (EOSs) for uniform nuclear matter containing $Λ$ and $Σ^-$ hyperons with use of the cluster variational method. The isoscalar part of the Argonne v18 two-nucleon potential and the Urbana IX three-nucleon potential are employed as the interactions between nucleons, whereas, as the bare $ΛN$ and even-state $ΛΛ$ interactions, two-body central potentials that are determined so as to reproduce the experimental data on single- and double-$Λ$ hypernuclei are adopted. In addition, the $Σ^- N$ interaction is constructed so as to reproduce the empirical single-particle potential of $Σ^-$ in symmetric nuclear matter. Since the odd-state part of the $ΛΛ$ interaction is not known owing to lack of experimental data, we construct four EOSs of hyperonic nuclear matter, each with a different odd-state part of the $ΛΛ$ interaction. The EOS obtained for NS matter becomes stiffer as the odd-state $ΛΛ$ interaction becomes more repulsive, and correspondingly the maximum mass of NSs increases. It is interesting that the onset density of $Σ^-$ depends strongly on the repulsion of the odd-state $ΛΛ$ interaction. Furthermore, we take into account the three-baryon repulsive force to obtain results that are consistent with observational data on heavy NSs.
description: 12 pages, 6 figures, accepted for publication in Phys. Rev. C
Electronic structure of FeSe monolayer superconductors
Creators: name: Nekrasov, I. A.
name: Pavlov, N. S.
name: Sadovskii, M. V.
name: Slobodchikov, A. A.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: We review a variety of theoretical and experimental results concerning electronic band structure of superconducting materials based on FeSe monolayers. Three type of systems are analyzed: intercalated FeSe systems A_xFe_2Se_{2-x}S_x and [Li_{1-x}Fe_xOH]FeSe as well as the single FeSe layer films on SrTiO_3 substrate. We present the results of detailed first principle electronic band structure calculations for these systems together with comparison with some experimental ARPES data. The electronic structure of these systems is rather different from that of typical FeAs superconductors, which is quite significant for possible microscopic mechanism of superconductivity. This is reflected in the absence of hole pockets of the Fermi surface at Γ-point in Brillouin zone, so that there are no "nesting" properties of different Fermi surface pockets. LDA+DMFT calculations show that correlation effects on Fe-3d states in the single FeSe layer are not that strong as in most of FeAs systems. As a result, at present there is no theoretical understanding of the formation of rather "shallow" electronic bands at M points. LDA calculations show that the main difference in electronic structure of FeSe monolayer on SrTiO_3 substrate from isolated FeSe layer is the presence of the band of O-2p surface states of TiO_2 layer on the Fermi level together with Fe-3d states, which may be important for understanding the enhanced T_c values in this system. We briefly discuss the implications of our results for microscopic models of superconductivity.
description: 21 pages, 13 figures, minor typos corrected
title: Impfhindernisse und ihr Einfluss auf das Praxismanagement und die Impfquoten in Deutschland
Creators: name: Englert, L.
name: Sanftenberg, L.
name: Schrörs, H.-J.
name: Schelling, J.
Publisher: name: German Medical Science GMS Publishing House
Year: 2016
Subjects: subject: Impfquote
subject: Praxismanagement
subject: 610 Medical sciences; Medicine

description: Hintergrund: Bis zum Jahr 2015 sollten die Masern in Deutschland eliminiert sein [1], jedoch wurden im Jahr 2015 immer noch 2065 Masernfälle gemeldet [2]. Fragestellung: Diese Arbeit beschäftigt sich mit den Impfhindernissen (IH), mit denen sich niedergelassene Ärzte[zum vollständigen Text gelangen Sie über die oben angegebene URL]
description: 50. Kongress für Allgemeinmedizin und Familienmedizin
title: WP2 Manchester Local Area Energy Strategy: Non-Domestic Decentralised Energy and District Heating Deployment, Bury. Metrics
Creators: name: Korais, E.
Publisher: name: ETI
Year: 2017
Subjects: subject: Smart Systems and Heat
subject: ENERGY EFFICIENCY (Residential and commercial)
subject: OTHER CROSS-CUTTING TECHNOLOGIES or RESEARCH (Energy system analysis)
subject: OTHER CROSS-CUTTING TECHNOLOGIES or RESEARCH (Energy Models)
subject: OTHER CROSS-CUTTING TECHNOLOGIES or RESEARCH (Other Supporting Data)

description: The Spatial Energy Plan for Greater Manchester Combined Authority project was commissioned as part of the Energy Technologies Institute (ETI) Smart Systems and Heat Programme and undertaken through collaboration between the Greater Manchester Combined Authority and theEnergy Systems Catapult.The study has consolidated the significant data and existing evidence relating to the local energy system to provide a platform for future energy planning in the region and the development of suitable policies within the emerging spatial planning framework for Greater Manchester.

This study provides a desktop review of the EnergyPath Networks (EPN) Decentralised Energy and District Heating deployment in Bury, considering the connection of non-domestic buildings to heat networks.The EPN model develops heat network deployment across cluster area, with connections to both domestic and non-domestic buildings. This report provides general recommendations on nondomestic building connection to a heat network based on their use type and size.The aim of this report is to define metrics on which the connection policy applied by the model can be tested and refined.
Statistical static timing analysis via modern optimization lens: I. Histogram-based approach
Creators: name: Bosak, Adam
name: Mishagli, Dmytro
name: Marecek, Jakub
Publisher: name: arXiv
Year: 2022
Subjects: subject: Optimization and Control (math.OC)
subject: Hardware Architecture (cs.AR)
subject: FOS: Mathematics
subject: FOS: Computer and information sciences

description: Statistical static timing analysis (SSTA) is studied from the point of view of mathematical optimization. We present two formulations of the problem of finding the critical path delay distribution that were not known before: (i) a formulation of the SSTA problem using Binary--Integer Programming and (ii) a practical formulation using Geometric Programming. For simplicity, we use histogram approximation of the distributions. Scalability of the approaches is studied and possible generalizations are discussed.
description: 26 pages, 7 figures
Possible identification of massive and evolved galaxies At z > 5
Creators: name: Mawatari, Ken
name: Yamada, Toru
name: Fazio, Giovanni
name: Huang, Jiasheng
name: Ashby, Matthew
Publisher: name: arXiv
Year: 2016
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We report on the identification of the old stellar population galaxy candidates at z > 5. We developed a new infrared color selection scheme to isolate galaxies with the strong Balmer breaks at z > 5, and applied it to the ultra-deep and wide infrared survey data from the Spitzer Extended Deep Survey (SEDS) and the UKIRT Infrared Deep Sky Survey. The eight objects satisfying K - [3.6] > 1.3 and K - [3.6] > 2.4 ([3.6] - [4.5]) + 0.6 are selected in the 0.34 deg^2 SEDS Ultra Deep Survey field. Rich multi-wavelength imaging data from optical to far-infrared are also used to reject blending sources and strong nebular line emitters, and we finally obtained the three most likely evolved galaxies at z > 5. Their stacked spectral energy distribution is fitted well with the old stellar population template with M_{*} = (7.5+-1.5) x 10^{10} Msun, star formation rate = 0.9 +- 0.2 Msun yr^{-1}, dust A_V < 1, and age = 0.7+-0.4 Gyr at z = 5.7+-0.6, where the dusty star-forming galaxies at z ~ 2.8 are disfavored because of the faintness in the 24um. The stellar mass density of these evolved galaxy candidates, (6+-4) x 10^4 Msun Mpc^{-3}, is much lower than that of star-forming galaxies, but the non-zero fraction suggests that initial star-formation and quenching have been completed by z ~ 6.
description: 13 pages, 9 figures, 4 tables, and accepted for publication in PASJ
title: Prävalenz von Burnout in einer deutschen Hausarztpopulation: Gibt es Unterschiede zwischen Einzel- und Gemeinschaftspraxen?
Creators: name: Möller, M.
name: Weltermann, B.
name: Viehmann, A.
Publisher: name: German Medical Science GMS Publishing House
Year: 2016
Subjects: subject: Burnout
subject: Gemeinschaftspraxis vs. Einzelpraxis
subject: Hausärzte
subject: 610 Medical sciences; Medicine

description: Hintergrund: Stress, Depression und Burnout können sich negativ auf die Gesundheit und Jobzufriedenheit auswirken. Hohe Burnout-Prävalenzwerte bei Hausärzten wurden in einer großen europäischen Studie [43% emotionale Erschöpfung, 35,4% Depersonalisation (Zynismus),[zum vollständigen Text gelangen Sie über die oben angegebene URL]
description: 50. Kongress für Allgemeinmedizin und Familienmedizin
Wearables At Work
Creators: name: Pandey, Santosh
Publisher: name: figshare
Year: 2023
Subjects: Cardiology (incl. cardiovascular diseases)
Respiratory diseases
Exercise physiology
Motor control
Sports science and exercise not elsewhere classified
Biomechanics
Digital electronic devices
Analog electronics and interfaces
Electronic sensors
Industrial electronics
Microelectronics
Radio frequency engineering
Quantum engineering systems (incl. computing and communications)
Intelligent robotics
Knowledge representation and reasoning
Modelling and simulation
Natural language processing
Speech recognition

description: The multitude of workplaces come with their inherent distractions, risks, and dangers. Timely identification and remediation of the potential risk factors is critical for the safety, health, and productivity of workers. For this purpose, employers’ resort to key enabling technologies (KETs) to monitor, manage, and optimize their workplace assets (e.g., tools, machines, inventory, safety equipment, supporting technologies, and workers). On one hand, workplace wearables (i.e., smart, on-body accessories, and personal protective equipment [PPE]) track the activities, behavior and body status of individual workers. On the other hand, connected worker solutions (i.e., intelligent computing, data analytics, and storage platforms) serve as the central hub for extracting contextual information from distributed networks of workplace wearables for better workflow organization, asset management, and predictive maintenance. Our objective here is to provide a comprehensive review of commercial wearables and connected worker solutions for occupational safety, health, and productivity. Our intent is to cover workplace technologies that are already in use or have the potential for use at different worksites.
Additional file 1 of Toll-like receptor and C-type lectin receptor agonists attenuate osteogenic differentiation in human dental pulp stem cells
Creators: name: Bulanawichit, Wajathip
name: Sinsareekul, Chanakarn
name: Kornsuthisopon, Chatvadee
name: Chansaenroj, Ajjima
name: Trachoo, Vorapat
name: Nowwarote, Nunthawan
name: Osathanon, Thanaphum
Publisher: name: figshare
Year: 2024
Subjects: subject: Biochemistry
subject: Medicine
subject: Molecular Biology
subject: Pharmacology
subject: Biotechnology
subject: Chemical Sciences not elsewhere classified
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Computational Biology

description: Supplementary Material 1
Spatially resolved detection of complex ferromagnetic dynamics using optically detected NV spins
Creators: name: Wolfe, Chris. S.
name: Manuilov, Sergei. A.
name: Purser, Carola. M.
name: Teeling-Smith, Richelle
name: Dubs, Carsten.
name: Hammel, P. Chris
name: Bhallamudi, Vidya Praveen
Publisher: name: arXiv
Year: 2015
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We demonstrate optical detection of a broad spectrum of ferromagnetic excitations using nitrogen-vacancy (NV) centers in an ensemble of nanodiamonds. Our recently developed approach exploits a straightforward CW detection scheme using readily available diamond detectors, making it easily implementable. The NV center is a local detector, giving the technique spatial resolution, which here is defined by our laser spot, but in principle can be extended far into the nanoscale. Among the excitations we observe are propagating dipolar and dipolar-exchange spinwaves, as well as dynamics associated with the multi-domain state of the ferromagnet at low fields. These results offer an approach, distinct from commonly used ODMR techniques, for spatially resolved spectroscopic study of magnetization dynamics at the nanoscale.
description: 6 pages and 1 page supplmentary information
Characterising Strong Lensing Galaxy Clusters using the Millennium-XXL and MOKA simulations
Creators: name: Giocoli, Carlo
name: Bonamigo, Mario
name: Limousin, Marceau
name: Meneghetti, Massimo
name: Moscardini, Lauro
name: Angulo, Raul E.
name: Despali, Giulia
name: Jullo, Eric
Publisher: name: arXiv
Year: 2016
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: In this paper we investigate the strong lensing statistics in galaxy clusters. We extract dark matter haloes from the Millennium-XXL simulation, compute their Einstein radius distribution, and find a very good agreement with Monte Carlo predictions produced with the MOKA code. The distribution of the Einstein radii is well described by a log-normal distribution, with a considerable fraction of the largest systems boosted by different projection effects. We discuss the importance of substructures and triaxiality in shaping the size of the critical lines for cluster size haloes. We then model and interpret the different deviations, accounting for the presence of a Bright Central Galaxy (BCG) and two different stellar mass density profiles. We present scaling relations between weak lensing quantities and the size of the Einstein radii. Finally we discuss how sensible is the distribution of the Einstein radii on the cosmological parameters Ω_M-σ_8 finding that cosmologies with higher Ω_M and σ_8 possess a large sample of strong lensing clusters. The Einstein radius distribution may help distinguish Planck13 and WMAP7 cosmology at 3σ.
description: replaced to match the accepted version for publication on MNRAS
title: Das Verhalten von niedergelassenen Ärzten im eigenen Krankheitsfall
Creators: name: Schulz, S.
name: Einsle, F.
name: Schneider, N.
name: Hänsch, S.
name: Bungenberg, G.
name: Gensichen, J.
Publisher: name: German Medical Science GMS Publishing House
Year: 2016
Subjects: subject: Ärztegesundheit
subject: Krankheitsverhalten
subject: Selbstbehandlung
subject: 610 Medical sciences; Medicine

description: Hintergrund: Ärzte haben aufgrund ihrer Ausbildung und beruflichen Tätigkeit besondere Bedingungen hinsichtlich des Verhaltens im eigenen Krankheitsfall. Entsprechend internationalen Empfehlungen sind die eigene Registrierung bei einem Hausarzt sowie Selbstdiagnostik und -therapie von besonderer[zum vollständigen Text gelangen Sie über die oben angegebene URL]
description: 50. Kongress für Allgemeinmedizin und Familienmedizin
Toward extracting $γ$ from $B \to DK$ without binning
Creators: name: Backus, Jeffrey V.
name: Freytsis, Marat
name: Grossman, Yuval
name: Schacht, Stefan
name: Zupan, Jure
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: $B^\pm \to DK^\pm$ transitions are known to provide theoretically clean information about the CKM angle $γ$, with the most precise available methods exploiting the cascade decay of the neutral $D$ into $CP$ self-conjugate states. Such analyses currently require binning in the $D$ decay Dalitz plot, while a recently proposed method replaces this binning with the truncation of a Fourier series expansion. In this paper, we present a proof of principle of a novel alternative to these two methods, in which no approximations at the level of the data representation are required. In particular, our new strategy makes no assumptions about the amplitude and strong phase variation over the Dalitz plot. This comes at the cost of a degree of ambiguity in the choice of test statistic quantifying the compatibility of the data with a given value of $γ$, with improved choices of test statistic yielding higher sensitivity. While our current proof-of-principle implementation does not demonstrate optimal sensitivity to $γ$, its conceptually novel approach opens the door to new strategies for $γ$ extraction. More studies are required to see if these can be competitive with the existing methods.
description: v2: 18 pages, 1 figure, modified discussion in Introduction and Conclusions, improved simulations and numerical results, references added, version accepted for publication in EPJC
On fractional Schrodinger systems of Choquard type
Creators: name: Bhattarai, Santosh
Publisher: name: arXiv
Year: 2016
Subjects: subject: Analysis of PDEs (math.AP)
subject: Mathematical Physics (math-ph)
subject: FOS: Mathematics
subject: FOS: Physical sciences
subject: 35R11, 35Q55, 35Q40, 35B35

description: In this article, we first employ the concentration compactness techniques to prove existence and stability results of standing waves for nonlinear fractional Schrödinger-Choquard equation \[ i\partial_tΨ+ (-Δ)^αΨ= a |Ψ|^{s-2}Ψ+λ\left( \frac{1}{|x|^{N-β}} \star |Ψ|^p \right)|Ψ|^{p-2}Ψ \ \ \mathrm{in}\ \mathbb{R}^{N+1}, \] where $N\geq 2$, $α\in (0,1)$, $β\in (0, N)$, $s\in (2, 2+\frac{4α}{N})$, $p\in [2, 1+\frac{2α+β}{N})$, and the constants $a, λ$ are nonnegative satisfying $a+λ> 0.$ We then extend the arguments to establish similar results for coupled standing waves of nonlinear fractional Schrödinger systems of Choquard type. The same argument works for equations with an arbitrary number of combined nonlinearities and when $|x|^{β-N}$ is replaced by a more general convolution potential $\mathcal{K}:\mathbb{R}^N\to [0, \infty)$ under certain assumptions. The same arguments can be applied and the results are identical for the case $α=1$ as well.
description: 31 pages, revised version
title: SL-Bandrekonstruktion: 4-Jahresergebnisse nach durchgeführter modifizierter Brunelli Bandplastik
Creators: name: Brockamp, Thomas
name: Bayer-Sandow, Thomas
name: Von Maydell, Bernd
name: Richter, Martin
Publisher: name: German Medical Science GMS Publishing House
Year: 2016
Subjects: subject: SL-Band
subject: modifizierte Brunelli SL-Band Rekonstruktion
subject: 610 Medical sciences; Medicine

description: Fragestellung: Das SL-Band ist eines der wesentlichen Stabilisatoren im Handgelenk. Eine Ruptur des Bandes verursacht in der Regel eine Karpale Instabilität, die eine Handgelenksarthrose (SLAC-Wrist) zur Folge haben kann. Die operative Therapie ist aufgrund der häufig frustranen Ergebnisse[zum vollständigen Text gelangen Sie über die oben angegebene URL]
description: 57. Kongress der Deutschen Gesellschaft für Handchirurgie
title: Progranulin promotes peripheral nerve regeneration and reinnervation: role of Notch signaling
Creators: name: Altmann, Christine
Publisher: name: German Medical Science GMS Publishing House
Year: 2016
Subjects: subject: 610 Medical sciences; Medicine

description: Background: Peripheral nerve injury is a frequent cause of lasting motor deficits and chronic pain. Although peripheral nerves are capable of regrowth they often fail to re-innervate target tissues. Results: Using newly generated transgenic mice with inducible neuronal progranulin overexpression [for full text, please go to the a.m. URL]
description: Joint-Meeting of the German Society for Neuropathology and Neuroanatomy (DGNN) and the Scandinavian Neuropathological Society (SNS)