cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
TWIST-GAN: Towards Wavelet Transform and Transferred GAN for Spatio-Temporal Single Image Super Resolution
Creators: name: Dharejo, Fayaz Ali
name: Deeba, Farah
name: Zhou, Yuanchun
name: Das, Bhagwan
name: Jatoi, Munsif Ali
name: Zawish, Muhammad
name: Du, Yi
name: Wang, Xuezhi
Publisher: name: arXiv
Year: 2021
Subjects: subject: Image and Video Processing (eess.IV)
subject: Computer Vision and Pattern Recognition (cs.CV)
subject: FOS: Electrical engineering, electronic engineering, information engineering
subject: FOS: Computer and information sciences

description: Single Image Super-resolution (SISR) produces high-resolution images with fine spatial resolutions from aremotely sensed image with low spatial resolution. Recently, deep learning and generative adversarial networks(GANs) have made breakthroughs for the challenging task of single image super-resolution (SISR). However, thegenerated image still suffers from undesirable artifacts such as, the absence of texture-feature representationand high-frequency information. We propose a frequency domain-based spatio-temporal remote sensingsingle image super-resolution technique to reconstruct the HR image combined with generative adversarialnetworks (GANs) on various frequency bands (TWIST-GAN). We have introduced a new method incorporatingWavelet Transform (WT) characteristics and transferred generative adversarial network. The LR image hasbeen split into various frequency bands by using the WT, whereas, the transfer generative adversarial networkpredicts high-frequency components via a proposed architecture. Finally, the inverse transfer of waveletsproduces a reconstructed image with super-resolution. The model is first trained on an external DIV2 Kdataset and validated with the UC Merceed Landsat remote sensing dataset and Set14 with each image sizeof 256x256. Following that, transferred GANs are used to process spatio-temporal remote sensing images inorder to minimize computation cost differences and improve texture information. The findings are comparedqualitatively and qualitatively with the current state-of-art approaches. In addition, we saved about 43% of theGPU memory during training and accelerated the execution of our simplified version by eliminating batchnormalization layers.
description: Accepted: ACM TIST (10-03-2021)
One-rank interaction kernel of the two-nucleon system for medium and high energies
Creators: name: Bondarenko, S. G.
name: Burov, V. V.
name: Hwang, W-Y. Pauchy
name: Rogochaya, E. P.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: A new version of the separable kernel of the nucleon-nucleon interaction in the Bethe-Salpeter approach is presented. The phase shifts are fitted to recent experimental data for singlet and uncoupled triplet partial waves of the neutron-proton scattering with total angular momenta J=0,1. The results are compared with other model calculations.
description: 10 pages, 5 figures, 3 tables
Element-Specific Phonon Density of States of Iron in LaFeAsO_{1-x}F_{x} and La_{1-x}Ca_{x}FePO
Creators: name: Higashitaniguchi, S.
name: Seto, M.
name: Kitao, S.
name: Kobayashi, Y.
name: Saito, M.
name: Masuda, R.
name: Mitsui, T.
name: Yoda, Y.
name: Kamihara, Y.
name: Hirano, M.
name: Hosono, H.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: We have measured element-specific Fe-phonon densities of states (Fe-PDOS) of LaFeAsO_{1-x}F_{x} (x = 0, 0.11) and La_{1-x}Ca_{x}FePO (x = 0.13) by using nuclear resonant inelastic scattering of synchrotron radiation. The Fe-PDOS of superconductor LaFeAsO_{0.89}F_{0.11} (Tc = 26 K) and that of non-superconductor LaFeAsO have similar structures to both below Tc (15 K) and above Tc (298 K) and, therefore, fluorine doping does not have notable effect on the Fe-PDOS. As for the superconductor La_{0.87}Ca_{0.13}FePO (Tc = 5.4K), the entire structure of Fe-PDOS resembles with that of LaFeAsO_{1-x}F_{x}, but the energy of the highest peak is higher than that of LaFeAsO_{1-x}F_{x}. These peaks are attributed to vibrational modes between Fe and pnicogen (As and P) and the temperature-dependent energy shifts are observed for LaFeAsO_{1-x}F_{x}. Observed Fe-PDOS of LaFeAsO_{1-x}F_{x} agrees well with an previously calculated Fe-PDOS spectrum with a first-principles calculation and shows the structural resemblance with an calculated Eliashberg function #alpha^2F(x) giving small electron-phonon coupling. Therefore, our results indicate that phonons are not the main contributors to the Tc superconductivity of LaFeAsO_{1-x}F_{x}. From the experimental viewpoint, comparison of our observed Fe-PDOS and an experimentally obtained bosonic glue spectrum will be an important clue as to whether phonons are the main contributors to superconductivity in iron-pnictide superconductors.
Physical properties of Tolman-Bayin solutions: some cases of static charged fluid spheres in general relativity
Creators: name: Ray, Saibal
name: Das, Basanti
name: Rahaman, Farook
name: Ray, Subharthi
Publisher: name: arXiv
Year: 2007
Subjects: subject: Astrophysics (astro-ph)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: In this article, Einstein-Maxwell space-time has been considered in connection to some of the astrophysical solutions as previously obtained by Tolman (1939) and Bayin (1978). The effect of inclusion of charge into these solutions has been investigated thoroughly and also the nature of fluid pressure and mass density throughout the sphere have been discussed. Mass-radius and mass-charge relations have been derived for various cases of the charged matter distribution. Two cases are obtained where perfect fluid with positive pressures give rise to electromagnetic mass models such that gravitational mass is of purely electromagnetic origin.
description: 15 pages, 12 figures
Mapping an Island in the Landscape
Creators: name: Gmeiner, Florian
name: Honecker, Gabriele
Publisher: name: arXiv
Year: 2007
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We provide a complete classification and statistical analysis of all type IIA orientifold compactifications with intersecting D6-branes on the orbifold T^6/Z'_6. The total number of four dimensional N=1 supersymmetric models is found to be O(10^23). After a statistical analysis of the gauge sector properties of all possible solutions, we study three subsets of configurations which contain the chiral matter sector of the standard model, a Pati-Salam or SU(5) GUT model, respectively. We find O(10^15) compactifications with an MSSM and O(10^11) models with a Pati-Salam sector. Along the way we derive an explicit algebraic formulation for the computation of the non-chiral matter spectrum for all Z_N orbifolds.
description: 46 pages, 10 figures; v2: typos corrected, new examples and expanded study on chiral exotics
Effective Spin-1/2 Description of Transverse-Field-Induced Random Fields in Dipolar Spin Glasses with Strong Single-Ion Anisotropy
Creators: name: Tabei, S. M. A.
name: Vernay, F.
name: Gingras, M. J. P.
Publisher: name: arXiv
Year: 2007
Subjects: subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: We present analytical and numerical evidence for the validity of an effective S=1/2 approach to the description of random field generation in S>=1, and especially in an S=1, dipolar spin glass models with strong uniaxial Ising anisotropy and subject to weak external magnetic field Bx transverse to the Ising direction. Explicitely Bx-dependent random fields are shown to naturally emerge in the effective low-energy description of a microscopic S=1 toy model. We discuss our results in relation to recent theoretical studies pertaining to the topic of Bx-induced random fields in the LiHo$_x$Y$_{1-x}$F$_4$ magnetic materials with the Ho$^{3+}$ Ising moments subject to a transverse field. We show that the S_{eff}=1/2 approach is able to capture both the qualitative and quantitative aspects of the physics at small Bx, giving results that agree with those obtained using conventional second order perturbation theory.
description: 9 pages. 4 eps figures
Twist-3 Double Spin Asymmetries in Drell-Yan Processes
Creators: name: Hu, M. C.
name: Ma, J. P.
name: Pang, Z. Y.
name: Zhang, G. P.
Publisher: name: arXiv
Year: 2021
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We study double spin asymmetries in Drell-Yan processes in which one initial hadron is transversely polarized and another one is longitudinally polarized. The complete part of the hadronic tensor relevant to asymmetries is derived. This part consists of twist-2 and twist-3 parton distributions and is gauge invariant. We construct some observables which can be used to extract these parton distributions from experimental measurements.
description: Published version in Phys.Rev.D
Towards planetesimals: dense chondrule clumps in the protoplanetary nebula
Creators: name: Cuzzi, Jeffrey N.
name: Hogan, Robert C.
name: Shariff, Karim
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We outline a scenario which traces a direct path from freely-floating nebula particles to the first 10-100km-sized bodies in the terrestrial planet region, producing planetesimals which have properties matching those of primitive meteorite parent bodies. We call this "primary accretion". The scenario draws on elements of previous work, and introduces a new critical threshold for planetesimal formation. We presume the nebula to be weakly turbulent, which leads to dense concentrations of aerodynamically size-sorted particles having properties like those observed in chondrites. The fractional volume of the nebula occupied by these dense zones or clumps obeys a probability distribution as a function of their density, and the densest concentrations have particle mass density 100 times that of the gas. However, even these densest clumps are prevented by gas pressure from undergoing gravitational instability in the traditional sense (on a dynamical timescale). While in this state of arrested development, they are susceptible to disruption by the ram pressure of the differentially orbiting nebula gas. However, self-gravity can preserve sufficiently large and dense clumps from ram pressure disruption, allowing their entrained particles to sediment gently but inexorably towards their centers, producing 10-100 km "sandpile" planetesimals. Localized radial pressure fluctuations in the nebula, and interactions between differentially moving dense clumps, will also play a role that must be allowed for in future studies. The scenario is readily extended from meteorite parent bodies to primary accretion throughout the solar system.
description: Astrophys. J accepted April 11, 2008
Measurement of the Range Component Directional Signature in a DRIFT-II Detector using 252Cf Neutrons
Creators: name: Burgos, S.
name: Daw, E.
name: Forbes, J.
name: Ghag, C.
name: Gold, M.
name: Hagemann, C.
name: Kudryavtsev, V. A.
name: Lawson, T. B.
name: Loomba, D.
name: Majewski, P.
name: Muna, D.
name: Murphy, A. St. J.
name: Nicklin, G. G.
name: Paling, S. M.
name: Petkov, A.
name: Plank, S. J. S.
name: Robinson, M.
name: Sanghi, N.
name: Snowden-Ifft, D. P.
name: Spooner, N. J. C.
name: Turk, J.
name: Tziaferi, E.
Publisher: name: arXiv
Year: 2008
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The DRIFT collaboration utilizes low pressure gaseous detectors to search for WIMP dark matter with directional signatures. A 252Cf neutron source was placed on each of the principal axes of a DRIFT detector in order to test its ability to measure directional signatures from the three components of very low energy (~keV/amu) recoil ranges. A high trigger threshold and the event selection procedure ensured that only sulfur recoils were analyzed. Sulfur recoils produced in the CS2 target gas by the 252Cf source closely match those expected from massive WIMP induced sulfur recoils. For each orientation of the source a directional signal from the range components was observed, indicating that the detector is directional along all 3 axes. An analysis of these results yields an optimal orientation for DRIFT detectors when searching for a directional signature from WIMPs. Additional energy dependent information is provided to aid in understanding this effect.
description: 14 pages, 1 Table, 8 Figures
Additional file 1 of Diagnostic criteria for musculoskeletal disorders for use in occupational healthcare or research: a scoping review of consensus- and synthesised-based case definitions
Creators: name: Molen, Henk F. Van Der
name: Visser, Steven
name: Alfonso, Jose Hernán
name: Curti, Stefania
name: Mattioli, Stefano
name: Rempel, David
name: Roquelaure, Yves
name: P. Paul F. M. Kuijer
name: Tamminga, Sietske J.
Publisher: name: figshare
Year: 2021
Subjects: subject: Biophysics
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Biotechnology
subject: 69999 Biological Sciences not elsewhere classified
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Additional file 1. Search strategy.
Root cause prediction based on bug reports
Creators: name: Hirsch, Thomas
name: Hofer, Birgit
Publisher: name: arXiv
Year: 2021
Subjects: subject: Software Engineering (cs.SE)
subject: Artificial Intelligence (cs.AI)
subject: FOS: Computer and information sciences

description: This paper proposes a supervised machine learning approach for predicting the root cause of a given bug report. Knowing the root cause of a bug can help developers in the debugging process - either directly or indirectly by choosing proper tool support for the debugging task. We mined 54755 closed bug reports from the issue trackers of 103 GitHub projects and applied a set of heuristics to create a benchmark consisting of 10459 reports. A subset was manually classified into three groups (semantic, memory, and concurrency) based on the bugs' root causes. Since the types of root cause are not equally distributed, a combination of keyword search and random selection was applied. Our data set for the machine learning approach consists of 369 bug reports (122 concurrency, 121 memory, and 126 semantic bugs). The bug reports are used as input to a natural language processing algorithm. We evaluated the performance of several classifiers for predicting the root causes for the given bug reports. Linear Support Vector machines achieved the highest mean precision (0.74) and recall (0.72) scores. The created bug data set and classification are publicly available.
description: 6 pages
Evolving center-vortex loops
Creators: name: Moosmann, Julian
name: Hofmann, Ralf
Publisher: name: arXiv
Year: 2008
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We consider coarse-graining applied to nonselfintersecting planar center-vortex loops as they emerge in the confining phase of an SU(2) Yang-Mills theory. Well-established properties of planar curve-shrinking predict that a suitably defined, geometric effective action exhibits (mean-field) critical behavior when the conformal limit of circular points is reached. This suggests the existence of an asymptotic mass gap. We demonstrate that the initially sharp mean center-of-mass position in a given ensemble of curves develops a variance under the flow as is the case for a position eigenstate in free-particle quantum mechanics under unitary time evolution. A possible application of these concepts is an approach to high-$T_c$ superconductivity based (a) on the nonlocal nature of the electron (1-fold selfintersecting center-vortex loop) and (b) on planar curve-shrinking flow representing the decrease in thermal noise in a cooling cuprate.
description: 15 pages, 8 figures
Additional file 1 of Strategies to improve the implementation of preventive care in primary care: a systematic review and meta-analysis
Creators: name: Heath, Laura
name: Stevens, Richard
name: Nicholson, Brian D.
name: Wherton, Joseph
name: Gao, Min
name: Callan, Caitriona
name: Haasova, Simona
name: Aveyard, Paul
Publisher: name: figshare
Year: 2024
Subjects: subject: Medicine
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Science Policy

description: Additional file 1: Database search strategy.
Ισορροπία οικογενειακής και επαγγελματικής ζωής εργαζομένων κηδεμόνων και πρακτικές διοίκησης ανθρωπίνων πόρων φιλικές προς την οικογένεια.
Creators: name: Μολά, Αϊσέ Βεντάτ
Publisher: name: Aristotle University of Thessaloniki
Year: 2023
Subjects: Ισορροπία επαγγελματικής και οικογενειακής ζωής
Πρακτικές διοίκησης φιλικές προς την οικογένεια
Ευέλικτα ωράρια εργασίας
Work-life balance
Family-friendly management practices
Flexible working arrangements

description: Ο σκοπός της παρούσας διατριβής ήταν να εξεταστεί ο αντίκτυπος των φιλικών προς την οικογένεια πρακτικών διοίκησης ανθρώπινων πόρων στην ισορροπία μεταξύ επαγγελματικής και οικογενειακής ζωής των εργαζόμενων γονέων. Συγκεκριμένα, η διατριβή χρησιμοποίησε ποσοτικά δεδομένα από μια έρευνα που πραγματοποιήθηκε σε εργαζόμενους γονείς που εργάζονταν σε διεθνείς ευρωπαϊκούς οργανισμούς. Στόχος ήταν να αξιολογηθεί πώς οι φιλικές προς την οικογένεια πρακτικές διοίκησης ανθρώπινων πόρων επηρέαζαν την ισορροπία μεταξύ των επαγγελματικών και προσωπικών υποχρεώσεων των εργαζομένων, καθώς και πώς αυτό επηρέαζε την ευημερία, την ικανοποίηση από την εργασία και την παραγωγικότητά τους. Με αυτόν τον τρόπο, η διατριβή προσέφερε σημαντική κατανόηση των πρακτικών που μπορούν να βοηθήσουν τους εργαζόμενους γονείς να επιτύχουν μια πιο ισορροπημένη και ικανοποιητική συνδυασμένη επαγγελματική και οικογενειακή ζωή.
description: The purpose of this thesis was to examine the impact of family-friendly human resource management practices on the work-life balance of working parents. Specifically, the thesis used quantitative data from a survey of parents working in international European organisations. The aim was to assess how family-friendly human resource management practices affected employees' work-life balance and how this affected their well-being, job satisfaction and productivity. In doing so, the thesis provided an important understanding of practices that can help working parents achieve a more balanced and satisfying work-life balance and family life balance.
Approximation Algorithms for the NFV Service Distribution Problem
Creators: name: Feng, Hao
name: Llorca, Jaime
name: Tulino, Antonia M.
name: Raz, Danny
name: Molisch, Andreas F.
Publisher: name: arXiv
Year: 2021
Subjects: subject: Networking and Internet Architecture (cs.NI)
subject: FOS: Computer and information sciences

description: Distributed cloud networking builds on network functions virtualization (NFV) and software defined networking (SDN) to enable the deployment of network services in the form of elastic virtual network functions (VNFs) instantiated over general purpose servers at distributed cloud locations. We address the design of fast approximation algorithms for the NFV service distribution problem (NSDP), whose goal is to determine the placement of VNFs, the routing of service flows, and the associated allocation of cloud and network resources that satisfy client demands with minimum cost. We show that in the case of load-proportional costs, the resulting fractional NSDP can be formulated as a multi-commodity-chain flow problem on a cloud augmented graph, and design a queue-length based algorithm, named QNSD, that provides an O(ε) approximation in time O(1/ε). We then address the case in which resource costs are a function of the integer number of allocated resources and design a variation of QNSD that effectively pushes for flow consolidation into a limited number of active resources to minimize overall cloud network cost.
description: This 11-page draft is a modified long version of the conference paper "Approximation Algorithms for the NFV Service Distribution Problem" published in IEEE Infocom 2017 and contains the complete proof referred by the conference paper. This draft is listed as Ref. [15] in the conference paper
Magnetic-Field Dependence of the YbRh2Si2 Fermi Surface
Creators: name: Rourke, P. M. C.
name: McCollam, A.
name: Lapertot, G.
name: Knebel, G.
name: Flouquet, J.
name: Julian, S. R.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: Magnetic-field-induced changes of the Fermi surface play a central role in theories of the exotic quantum criticality of YbRh2Si2. We have carried out de Haas-van Alphen measurements in the magnetic-field range 8 T <= H <= 16 T, and directly observe field dependence of the extremal Fermi surface areas. Our data support the theory that a low-field "large" Fermi surface, including the Yb 4f quasihole, is increasingly spin split until a majority-spin branch undergoes a Lifshitz transition and disappears at H0 ~ 10 T, without requiring 4f localization at H0.
description: 4 pages, 5 figures, 1 table
Packing dimension of mean porous measures
Creators: name: Beliaev, D.
name: Järvenpää, E.
name: Järvenpää, M.
name: Käenmäki, A.
name: Rajala, T.
name: Smirnov, S.
name: Suomala, V.
Publisher: name: arXiv
Year: 2007
Subjects: subject: Classical Analysis and ODEs (math.CA)
subject: FOS: Mathematics
subject: 28A75, 28A80

description: We prove that the packing dimension of any mean porous Radon measure on $\mathbb R^d$ may be estimated from above by a function which depends on mean porosity. The upper bound tends to $d-1$ as mean porosity tends to its maximum value. This result was stated in \cite{BS}, and in a weaker form in \cite{JJ1}, but the proofs are not correct. Quite surprisingly, it turns out that mean porous measures are not necessarily approximable by mean porous sets. We verify this by constructing an example of a mean porous measure $μ$ on $\mathbb R$ such that $μ(A)=0$ for all mean porous sets $A\subset\mathbb R$.
description: Revised version
Pseudo Nambu-Goldstone Boson Inflation
Creators: name: Rodrigues Sandner, Stefan Marinus
Publisher: name: Deutsches Elektronen-Synchrotron, DESY, Hamburg
Year: 2019

description: Masterarbeit, University of Hamburg, 2019; 108 pp. (2019). = Masterarbeit, University of Hamburg, 2019
description: We investigate an early Universe inflationary phase driven by a pseudo Nambu-Goldstone boson. The setup is not only naturally protected in the sense of t’Hooft, but such particles are also ubiquitous in quantum and string theories. In particular, we may adopt the interpretation of an axion. We derive phenomenological interesting consequences by couplings to (non-) Abelian gauge fields. The only interaction term which respects the axion shift symmetry in this setup is of Chern-Simons form. Starting from the Bunch-Davies vacuum, we show that tachyonic enhanced gauge field modes source gravitational waves strong enough to be detectable at various stages of the inflationary phase. However, agreement with cosmic microwave background (CMB) observations require a super-Planckian periodicity scale of the potential. We try to recover a viable effective field theory (EFT) description by distinguishing between the axion decay constant and the periodicity scale. This may be achieved by e.g. aligning multiple axion fields. Nonetheless, we present a bottom-up EFT approach which puts stringent bounds on the non-Abelian model − almost entirely closing the parameter space. Additionally, we show that field excursions in the remaining viable window of large gauge couplings are of order $10^4$ times larger than the axion decay constant − indicating a difficult string theoretical realization. We propose a novel more realistic model of simultaneous axion couplings to both Abelian and non-Abelian gauge fields. In the case of a coupling hierarchy, such a degenerated gauge field unification gracefully circumvents the EFT bound. This complex gauge group structure is indeed desirable to provide a natural Standard Model connection to reheat the Universe through the Adler-Bell-Jackiv anomaly. We discuss that only gauge field self-interactions may lead to a formation of a thermal bath. Moreover, we introduce distortions of the CMB as a new strong constraint and simultaneously show that tensor contributions to them are generically highly suppressed.
A proposed microwave system for on-line measurement of specific gravity and moisture content of dimension lumber
Creators: name: Loo, James
Publisher: name: University of British Columbia
Year: 2010

description: A 10 GHz microwave bridge measurement system has been developed to automatically measure the electromagnetic field parameters transmitted through a dielectric material. These parameters are used to calculate the complex dielectric constant with the free-space transmission technique. The system is used to measure the field parameters transmitted through dimension lumber and a correlation is made with two strength determining factors of lumber: specific gravity and moisture content. Hemlock and Douglas Fir wood samples were tested and a grading technique was implemented. The system is capable of estimating the specific gravity to ±0.05 accuracy and the moisture content to ±3.0% accuracy.
Hemispheric Tectonics on super-Earth LHS 3844b
Creators: name: Meier, Tobias G.
name: Bower, Dan J.
name: Lichtenberg, Tim
name: Tackley, Paul J.
name: Demory, Brice-Olivier
Publisher: name: arXiv
Year: 2021
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Geophysics (physics.geo-ph)
subject: FOS: Physical sciences

description: The tectonic regime of rocky planets fundamentally influences their long-term evolution and cycling of volatiles between interior and atmosphere. Earth is the only known planet with active plate tectonics, but observations of exoplanets may deliver insights into the diversity of tectonic regimes beyond the solar system. Observations of the thermal phase curve of super-Earth LHS 3844b reveal a solid surface and lack of a substantial atmosphere, with a temperature contrast between the substellar and antistellar point of around 1000 K. Here, we use these constraints on the planet's surface to constrain the interior dynamics and tectonic regimes of LHS 3844b using numerical models of interior flow. We investigate the style of interior convection by assessing how upwellings and downwellings are organized and how tectonic regimes manifest. We discover three viable convective regimes with a mobile surface: (1) spatially uniform distribution of upwellings and downwellings, (2) prominent downwelling on the dayside and upwellings on the nightside, and (3) prominent downwelling on the nightside and upwellings on the dayside. Hemispheric tectonics is observed for regimes (2) and (3) as a direct consequence of the day-to-night temperature contrast. Such a tectonic mode is absent in the present-day solar system and has never been inferred from astrophysical observations of exoplanets. Our models offer distinct predictions for volcanism and outgassing linked to the tectonic regime, which may explain secondary features in phase curves and allow future observations to constrain the diversity of super-Earth interiors.
description: Accepted for publication in The Astrophysical Journal Letters; 9 pages, 5 figures; summary available at http://exoplanet-talks.org/talk/263
Sterile neutrino dark matter with dipole interaction
Creators: name: Cho, Wonsub
name: Choi, Ki-Young
name: Seto, Osamu
Publisher: name: arXiv
Year: 2021
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We consider the possibility of the lightest sterile neutrino dark matter which has dipole interaction with heavier sterile neutrinos. The lifetime can be long enough to be a dark matter candidate without violating other constraints and the correct amount of relic abundance can be produced in the early Universe. We find that a sterile neutrino with the mass of around MeV and the dimension-five non-renormalisable dipole interaction suppressed by $Λ_5 \gtrsim 10^{15}$ GeV can be a good candidate of dark matter, while heavier sterile neutrinos with masses of the order of GeV can explain the active neutrino oscillations.
description: 20 pages, 6 figures
Additional file 2 of Diagnostic criteria for musculoskeletal disorders for use in occupational healthcare or research: a scoping review of consensus- and synthesised-based case definitions
Creators: name: Molen, Henk F. Van Der
name: Visser, Steven
name: Alfonso, Jose Hernán
name: Curti, Stefania
name: Mattioli, Stefano
name: Rempel, David
name: Roquelaure, Yves
name: P. Paul F. M. Kuijer
name: Tamminga, Sietske J.
Publisher: name: figshare
Year: 2021
Subjects: subject: Biophysics
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Biotechnology
subject: 69999 Biological Sciences not elsewhere classified
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Additional file 2. Reasons for excluding studies based on full text.
Cosmic ray protons and electrons from supernova remnants
Creators: name: Cristofari, P.
name: Blasi, P.
name: Caprioli, D.
Publisher: name: arXiv
Year: 2021
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: The spectrum of cosmic ray protons and electrons released by supernova remnants throughout their evolution is poorly known, because of the difficulty in accounting for particle escape and confinement in the downstream of a shock front, where both adiabatic and radiative losses are present. Here we calculate the spectrum of cosmic ray protons released during the evolution of supernovae of different types, accounting for the escape from upstream and for adiabatic losses of particles advected downstream of the shock and liberated at later times. The same calculation is carried out for electrons. The magnetic field in the post-shock region is calculated by using an analytic treatment of the magnetic field amplification due to non--resonant and resonant streaming instability and their saturation. We find that when the field is the result of the growth of the cosmic-ray--driven non--resonant instability alone, the spectrum of electrons and protons released by a supernova remnant are indeed different, but such a difference becomes appreciable only at energies $\gtrsim 100-1000$ GeV, while observations of the electron spectrum require such a difference to be present at energies as low as $\sim 10$ GeV. An effect at such low energies requires substantial magnetic field amplification in the late stages of the supernova remnant evolution (shock velocity $\ll 1000$ km/s), perhaps not due to streaming instability but hydrodynamical processes. We comment on the feasibility of such conditions and speculate on the possibility that the difference in spectral shape between electrons and protons may reflect either some unknown acceleration effect, or additional energy losses in cocoons around the sources.
description: 11 pages, 5 figures, Accepted for publication in Astronomy \& Astrophysics
Additional file 3 of Diagnostic criteria for musculoskeletal disorders for use in occupational healthcare or research: a scoping review of consensus- and synthesised-based case definitions
Creators: name: Molen, Henk F. Van Der
name: Visser, Steven
name: Alfonso, Jose Hernán
name: Curti, Stefania
name: Mattioli, Stefano
name: Rempel, David
name: Roquelaure, Yves
name: P. Paul F. M. Kuijer
name: Tamminga, Sietske J.
Publisher: name: figshare
Year: 2021
Subjects: subject: Biophysics
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Biotechnology
subject: 69999 Biological Sciences not elsewhere classified
subject: Science Policy
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Additional file 3. Study characteristics and MSD case definitions of included studies.
The Existence of Einstein Static Universes and their Stability in Fourth order Theories of Gravity
Creators: name: Goswami, Rituparno
name: Goheer, Naureen
name: Dunsby, Peter K. S.
Publisher: name: arXiv
Year: 2008
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We investigate whether or not an Einstein Static universe is a solution to the cosmological equations in $f(R)$ gravity. It is found that only one class of $f(R)$ theories admits an Einstein Static model, and that this class is neutrally stable with respect to vector and tensor perturbations for all equations of state on all scales. Scalar perturbations are only stable on all scales if the matter fluid equation of state satisfies $c_s^2>\frac{\sqrt{5}-1}{6}\approx 0.21$. This result is remarkably similar to the GR case, where it was found that the Einstein Static model is stable for $c_s^2>{1/5}$.
description: Minor changes, To appear in PRD
MOESM7 of A benchmark of batch-effect correction methods for single-cell RNA sequencing data
Creators: name: Tran, Hoa
name: Ang, Kok
name: Chevrier, Marion
name: Zhang, Xiaomeng
name: Lee, Nicole
name: Goh, Michelle
name: Chen, Jinmiao
Publisher: name: figshare
Year: 2020
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Chemical Sciences not elsewhere classified
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Information Systems not elsewhere classified
subject: Mathematical Sciences not elsewhere classified

description: Additional file 7: Table S6. Simulation statistical test. Statistical significance test results of the DEG recovery with simulated data.
The Effective Field Theory of Large Scale Structure at Three Loops
Creators: name: Konstandin, Thomas
name: Porto, Rafael A.
name: Rubira, Henrique
Publisher: name: Deutsches Elektronen-Synchrotron, DESY, Hamburg
Year: 2019

description: We study the power spectrum of dark matter density fluctuations in the framework of the Effective Field Theory of Large Scale Structures (EFTofLSS) up to three loop orders. In principle, several counter-terms may be needed to handle the short-distance sensitivity in perturbation theory. However, we show that a small number of extra coefficients are sufficient to match numerical simulations with percent accuracy when a generic renormalization prescription is implemented (allowing for running of the individual counter-terms). We show that the level of accuracy increases with respect to the two loop results, up to $k \simeq 0.4\, h$Mpc$^{-1}$ at redshift $z=0$, although the overall improvement is somewhat marginal. At the same time, we argue there is evidence that the behavior of the loop expansion in the EFTofLSS is typical of an asymptotic series, already on the brink of its maximum predictive power (at $z=0$). Hence, the inclusion of higher orders will likely deteriorate the matching to data, even at moderate values of $k$. Part of the reason for this behavior is due to large contributions to the (renormalized) power spectrum at three loop order from mildly non-linear scales, even after the UV counter-terms are included. In conclusion, the EFTofLSS to three loop orders provides the best approximation to the (deterministic part of the) power spectrum in the weakly non-linear regime at $z=0$, and higher loops are not expected to improve our level of accuracy.
Multilevel Global-Local techniques for adaptive ductile phase-field fracture
Creators: name: Aldakheel, Fadi
name: Noii, Nima
name: Wick, Thomas
name: Allix, Olivier
name: Wriggers, Peter
Publisher: name: arXiv
Year: 2021
Subjects: subject: Numerical Analysis (math.NA)
subject: FOS: Mathematics

description: This paper outlines a rigorous variational-based multilevel Global-Local formulation for ductile fracture. Here, a phase-field formulation is used to resolve failure mechanisms by regularizing the sharp crack topology on the local state. The coupling of plasticity to the crack phase-field is realized by a constitutive work density function, which is characterized through a degraded stored elastic energy and the accumulated dissipated energy due to plasticity and damage. Two different Global-Local approaches based on the idea of multiplicative Schwarz' alternating method are proposed: (i) A global constitutive model with an elastic-plastic behavior is first proposed, while it is enhanced with a single local domain, which, in turn, describes an elastic-plastic fracturing response. (ii) The main objective of the second model is to introduce an adoption of the Global-Local approach toward the multilevel local setting. To this end, an elastic-plastic global constitutive model is augmented with two distinct local domains; in which, the first local domain behaves as an elastic-plastic material and the next local domain is modeled due to the fracture state. To further reduce the computational cost, predictor-corrector adaptivity within Global-Local concept is introduced. An adaptive scheme is devised through the evolution of the effective global plastic flow (for only elastic-plastic adaptivity), and through the evolution of the local crack phase-field state (for only fracture adaptivity). Thus, two local domains are dynamically updated during the computation, resulting with two-way adaptivity procedure. The overall response of the Global-Local approach in terms of accuracy/robustness and efficiency is verified using single-scale problems. The resulting framework is algorithmically described in detail and substantiated with numerical examples.
description: 50 pages, 24 Figures, 4 Tables
Η πνευματική ζωή και τα ιερά μυστήρια στη διδασκαλία του Οσίου Παϊσίου του Αγιορείτη
Creators: name: Βοτάνης, Πασχάλης Χαραραλάμπους
Publisher: name: Aristotle University of Thessaloniki
Year: 2023
Subjects: Πνευματική ζωή
Άγιος Παΐσιος
Ιερά μυστήρια
Spiritual life
Saint Paisios
Holy mysteries

description: Σκοπός της παρούσας εργασίας είναι η ανάδειξη της πνευματικής ζωής και των ιερών μυστηρίων της εκκλησίας σύμφωνα με τη διδασκαλία του Οσίου Παϊσίου του Αγιορείτη. Πιο συγκεκριμένα η εργασία διαρθρώνεται σε δύο μέρη. Το πρώτο αναφέρεται στην πνευματική ζωή του χριστιανού. Αφού γίνεται μια σύντομη αναφορά στον βίο του Αγίου, στη συνέχεια προσεγγίζεται η ορθόδοξη χριστιανική αγωγή καθώς και οι φορείς της αγωγής. Στη συνέχεια αναφέρονται τα πάθη και οι αρετές στην πνευματική τελείωση του ανθρώπου αλλά και η σχέση του με τον πλησίον. Το δεύτερο μέρος πραγματεύεται τη στάση του Αγίου επάνω σε θέματα πίστης όπως αυτό των μυστηρίων της εκκλησίας. Αρχικά γίνεται αναφορά στα μυστήρια της εκκλησίας και για τον ρόλο που διαδραματίζουν, προκειμένου ο άνθρωπος να σώσει την ψυχή του, ενώ παράλληλα παρουσιάζονται και οι διδαχές του, όπως αυτές αποκαλύπτονται μέσα από τους λόγους του και αφορούν τα μυστήρια της εκκλησίας. Ο τόνος που χρησιμοποιεί είναι συμβουλευτικός, οικείος, ζεστός και σε καμία περίπτωση αυστηρός, βλέποντας τους αμέτρητους πιστούς που τον επισκέπτονταν σαν παιδιά του.
description: The purpose of this work is to highlight the spiritual life and the sacred mysteries of the church according to the teaching of Saint Paisios of Holy Mountain. More specifically, it is structured in two parts. The first refers to the spiritual life of the christian. After a brief reference is made to the life of the Saint, then the orthodox christian education and the institutions of the education are approached. Then the passions and virtues are mentioned in the spiritual perfection of man as well as his relationship with his nearby. The second part deals with the attitude of the Saint on matters of faith such as that of the mysteries of the church. First, reference is made to the mysteries of the church and the role they play in order for man to save his soul, while at the same time his teachings are also presented, as they are revealed through his speeches and concern the mysteries of the church. The tone he uses is consultative, intimate, warm and in no way strict, seeing the countless devotees who visit him as his children.
Baryogenesis from axion inflation
Creators: name: Domcke, Valerie
name: Von Harling, Benedict
name: Morgante, Enrico
name: Mukaida, Kyohei
Publisher: name: Deutsches Elektronen-Synchrotron, DESY, Hamburg
Year: 2019

description: The coupling of an axion-like particle driving inflation to the Standard Model particle content through a Chern-Simons term generically sources a dual production of massless helical gauge fields and chiral fermions. We demonstrate that the interplay of these two components results in a highly predictive baryogenesis model, which requires no further ingredients beyond the Standard Model. If the helicity stored in the hyper magnetic field and the effective chemical potential induced by the chiral fermion production are large enough to avoid magnetic diffusion from the thermal plasma but small enough to sufficiently delay the chiral plasma instability, then the non-vanishing helicity survives until the electroweak phase transition and sources a net baryon asymmetry which is in excellent agreement with the observed value. If any of these two conditions is violated, the final baryon asymmetry vanishes. The observed baryon asymmetry can be reproduced if the energy scale of inflation is around $H_\text{inf} \sim 10^{10}$--$10^{12}$ GeV with a moderate dependence on inflation model parameters.
Additional file 2 of Strategies to improve the implementation of preventive care in primary care: a systematic review and meta-analysis
Creators: name: Heath, Laura
name: Stevens, Richard
name: Nicholson, Brian D.
name: Wherton, Joseph
name: Gao, Min
name: Callan, Caitriona
name: Haasova, Simona
name: Aveyard, Paul
Publisher: name: figshare
Year: 2024
Subjects: subject: Medicine
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Science Policy

description: SAdditional file 2: Imputed calculations.
Classification of coastal grizzly bear habitat for forestry interpretations and the role of food in habitat use by coastal grizzly bears
Creators: name: Hamilton, Anthony Neil
Publisher: name: University of British Columbia
Year: 2010

description: A grizzly bear habitat classification was developed by modifying and expanding the climax-based Biogeoclimatic Ecosystem Classification (BEC) to accommodate serai vegetation. Locations of radio-collared bears were assigned to a large number (N=110) of structurally and floristically unique habitats. An interpretive classification of 14 Bear Habitat Units (BHUs) was derived from the taxa of the BEC system; units were amalgamated on the basis of grizzly bear habitat value and similarity of response to forest management practices. Fifteen climax forest, three subalpine, three wetland, and three avalanche chute units were identified and described in the lower Kimsquit River. Two adult female grizzly bears (numbers 08 and 25) were monitored for 1238 and 1196 days, respectively, from April 1982 to October 1985 and had multi-annual minimum convex polygon (MCP) home ranges of 85 km² (N=23 6), and 60 km² (N=241). River floodplain BHUs were used most heavily by bears 08 and 25 during their active seasons (65% of locations and 51% of time for bear 08; 75% of locations and 63% of time for bear 25) followed by avalanche chutes and sidehill climax and old-growth forests. Rank testing between quality/quantity indices (food plant nutrient content, biomass, berry abundance) and grizzly bear use indicated that movements were generally correlated with food availability at the higher, or BHU, level of the classification (rs=0.61 and 0.83, p<.05 for bears 08 and 25, respectively). Salmon (Oncorhynchus spp.) and insects were the only common non-plant items in a diet of over 3 0 species, although food habits differed between bears. It is concluded that, although food plays a critical role in habitat selection of coastal grizzly bears, a relatively rich environment precludes the need for individuals to forage optimally at a micro-habitat level. Except for the early spring and late fall, food can be found in a number of units that collectively meet life requisites. These analyses were used in combination with other use and habitat quality information to develop seasonal habitat values. Assigned values allowed predictions about the effects of forest management practices on habitat capability.
Additional file 3 of Strategies to improve the implementation of preventive care in primary care: a systematic review and meta-analysis
Creators: name: Heath, Laura
name: Stevens, Richard
name: Nicholson, Brian D.
name: Wherton, Joseph
name: Gao, Min
name: Callan, Caitriona
name: Haasova, Simona
name: Aveyard, Paul
Publisher: name: figshare
Year: 2024
Subjects: subject: Medicine
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Biological Sciences not elsewhere classified
subject: Science Policy

description: Additional file 3: Figures S1-S7. FigS1 – Meta-analysis summary diamonds as random effects (main analysis), Hartung-Knapp-Sidik-Jonkman (HKSJ) and inverse variance heterogeneity (IVhet) models for process outcomes. FigS2 - Meta-analysis summary diamonds as random effects (main analysis), Hartung-Knapp-Sidik-Jonkman (HKSJ) and inverse variance heterogeneity model (IVhet) models for behavioural outcomes. FigS3 - Random effects meta-analysis summary diamonds excluding studies at high risk of bias and those that required data imputation for process outcomes. FigS4 - Random effects meta-analysis summary diamonds excluding studies at high risk of bias and those that required data imputation for behavioural outcomes. FigS5 - Random effects meta-analysis of behavioural outcomes, excluding Moore 2003, Welzel 2021 and Goodfellow 2016. FigS6 - Random effects meta-analysis summary diamonds of health behaviour subgroups for process outcomes. FigS7 - Random effects meta-analysis summary diamonds of health behaviour subgroups for behavioural outcomes.
Extreme-ultraviolet Late Phase in Homologous Solar Flares from a Complex Active Region
Creators: name: Zhong, Y.
name: Dai, Y.
name: Ding, M. D.
Publisher: name: arXiv
Year: 2021
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Recent observations in extreme-ultraviolet (EUV) wavelengths reveal a new late phase in some solar flares, which is seen as a second peak in warm coronal emissions ($\sim3$ MK) several tens of minutes to a few hours after the soft X-ray (SXR) peak. The origin of the EUV late phase (ELP) is explained by either a long-lasting cooling process in the long ELP loops, or a delayed energy ejection into the ELP loops well after the main flare heating. Using the observations with the \emph{Solar Dynamics Observatory} (\emph{SDO}), we investigate the production of the ELP in six homologous flares (F1--F6) originating from a complex active region (AR) NOAA 11283, with an emphasis on the emission characteristics of the flares. It is found that the main production mechanism of the ELP changes from additional heating in flare F1 to long-lasting cooling in flares F3--F6, with both mechanisms playing a role in flare F2. The transition is evidenced by an abrupt decrease of the time lag of the ELP peak, and the long-lasting cooling process in the majority of the flares is validated by a positive correlation between the flare ribbon fluence and the ELP peak intensity. We attribute the change in ELP production mechanism to an enhancement of the envelope magnetic field above the AR, which facilitates a more prompt and energetic heating of the ELP loops. In addition, the last and the only confined flare F6 exhibits an extremely large ELP. The different emission pattern revealed in this flare may reflect a different energy partitioning inside the ELP loops, which is due to a different magnetic reconnection process.
description: 26 pages, 12 figures, 3 tables, accepted for publication in ApJ