cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Enhanced persistent photoconductivity in $δ$-doped LaAlO$_{3}$/SrTiO$_{3}$ heterostructures
Creators: name: Rastogi, A.
name: Pulikkotil, J. J.
name: Budhani, R. C.
Publisher: name: arXiv
Year: 2014
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We report the effect of $δ$-doping at LaAlO$_{3}$/SrTiO$_{3}$ interface with LaMnO$_{3}$ monolayers on the photoconducting (PC) state. The PC is realized by exposing the samples to broad band optical radiation of a quartz lamp and 325 and 441 nm lines of a He-Cd laser. Along with the significant modification in electrical transport which drives the pure LaAlO$_{3}$/SrTiO$_{3}$ interface from metal-to-insulator with increasing LaMnO$_{3}$ sub-monolayer thickness, we also observe an enhancement in the photo-response and relaxation time constant. Possible scenario for the PC based on defect-clusters, random potential fluctuations and large lattice relaxation models have been discussed. For pure LaAlO$_{3}$/SrTiO$_{3}$, the photoconductivity appears to originate from inter-band transitions between Ti-derived $3d$ bands which are $e_{g}$ in character and O 2p - Ti $t_{2g}$ hybridized bands. The band structure changes significantly when fractional layers of LaMnO$_{3}$ are introduced. Here the Mn $e_{g}$ bands ($\approx1.5$ eV above the Fermi energy) within the photo-conducting gap lead to a reduction in the photo-excitation energy and a gain in overall photoconductivity.
description: 9 pages, 5 figures
500 Jahre Reformation – wo steht die Ökumene?, hg. v. Bertram Stubenrauch / Athanasios Vletsis / Friederike Nüssel / Michael Huber
Creators: name: Oeldemann, Johannes
Publisher: name: Theologische Revue
Year: 2020

description: Theologische Revue, Bd. 116 (2020): November
title: L’homme qui voulait prendre la femme de son fils
title: Lo ba-nuu ma mi nii
Creators: name: Leguy, Cécile
Publisher: name: Pangloss
Year: 2022
Subjects: subject: Linguistique
subject: Boomu

description: Chanté, Accompagnement : musical à la harpe-luth à 8 cordes (’uanni) avec un accompagnateur qui frappe sur la caisse de résonnance de l’instrument, mais ne dit rien. Le conteur alterne des passages chantés et des passages dits, mais toujours accompagnés de la harpe-luth et du rythme frappé sur la caisse de l’instrument.
General multicomponent Yajima-Oikawa system: Painlevé analysis, soliton solutions, and energy-sharing collisions
Creators: name: Kanna, T.
name: Sakkaravarthi, K.
name: Tamilselvan, K.
Publisher: name: arXiv
Year: 2014
Subjects: subject: Pattern Formation and Solitons (nlin.PS)
subject: Exactly Solvable and Integrable Systems (nlin.SI)
subject: FOS: Physical sciences

description: We consider the multicomponent Yajima-Oikawa (YO) system and show that the two-component YO system can be derived in a physical setting of three-coupled nonlinear Schrödinger (3-CNLS) type system by the asymptotic reduction method. The derivation is further generalized to multicomponent case. This set of equations describes the dynamics of nonlinear resonant interaction between one-dimensional long-wave and multiple short-waves. The Painlevé analysis of the general multicomponent YO system shows that the underlying set of evolution equations is integrable for arbitrary nonlinearity coefficients which will result in three different sets of equations corresponding to positive, negative and mixed nonlinearity coefficients. We obtain general bright $N$-soliton solution of multicomponent YO system in the Gram determinant form by using Hirota's bilinearization method and explicitly analyze the one- and two-soliton solutions of the multicomponent YO system for the above mentioned three choices of nonlinearity coefficients. We also point out that the 3-CNLS system admits special asymptotic solitons of bright, dark, anti-dark and grey types, when the long-wave--short-wave resonance takes place. The short-wave component solitons undergo two types of energy sharing collisions. The solitons appearing in the long-wave component always exhibit elastic collision whereas that of short-wave components exhibit standard elastic collisions only for specific choice of parameters. We have also investigated the collision dynamics of asymptotic solitons in the original 3-CNLS system. For completeness, we explore the three-soliton interaction and demonstrate the pair-wise nature of collision and unravel fascinating state restoration property.
description: 14 pages, 9 figures
On the notion of Laplacian bounds on $\mathrm{RCD}$ spaces and applications
Creators: name: Gigli, Nicola
name: Mondino, Andrea
name: Semola, Daniele
Publisher: name: arXiv
Year: 2023
Subjects: subject: Differential Geometry (math.DG)
subject: Analysis of PDEs (math.AP)
subject: Metric Geometry (math.MG)
subject: FOS: Mathematics

description: We show that several different interpretations of the inequality $Δf\leqη$ are equivalent in the setting of $\mathrm{RCD}(K,N)$ spaces. With respect to previously available results in this direction, we improve both on the generality of the underlying space and in terms of regularity to be assumed on the function $f$. Applications are presented.
description: Comments are welcome!
On Safety of Passengers Entering a Bus Rapid Transit System from Scheduled Stops
Creators: name: Valencia, Alejandra
name: Malikopoulos, Andreas A.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Systems and Control (eess.SY)
subject: FOS: Electrical engineering, electronic engineering, information engineering

description: In this paper, we address the vehicle scheduling problem for improving passenger safety in bus rapid transit systems. Our focus is on passengers waiting at street stops to enter terminal stations. To enhance their safety, we minimize deviations from the proposed timetable, thereby minimizing passengers' initial waiting time. We formulate an optimization problem considering the position, speed deviation, and passenger count at each stop, solved using dynamic programming. Numerical simulations validate the effectiveness of our approach in enhancing passenger safety. Our work is the first attempt to minimize waiting time for improved safety and the first to utilize position tracking for departure time matching.
description: 6 pages, 5 figures, 7th IEEE Conference on Control Technology and Applications (CCTA) 2023
Testing the Asteroseismic Mass Scale Using Metal-Poor Stars Characterized with APOGEE and Kepler
Creators: name: Epstein, Courtney R.
name: Elsworth, Yvonne P.
name: Johnson, Jennifer A.
name: Shetrone, Matthew
name: Mosser, Benoît
name: Hekker, Saskia
name: Tayar, Jamie
name: Harding, Paul
name: Pinsonneault, Marc
name: Aguirre, Víctor Silva
name: Basu, Sarbani
name: Beers, Timothy C.
name: Bizyaev, Dmitry
name: Bedding, Timothy R.
name: Chaplin, William J.
name: Frinchaboy, Peter M.
name: García, Rafael A.
name: Pérez, Ana E. García
name: Hearty, Fred R.
name: Huber, Daniel
name: Ivans, Inese I.
name: Majewski, Steven R.
name: Mathur, Savita
name: Nidever, David
name: Serenelli, Aldo
name: Schiavon, Ricardo P.
name: Schneider, Donald P.
name: Schönrich, Ralph
name: Sobeck, Jennifer S.
name: Stassun, Keivan G.
name: Stello, Dennis
name: Zasowski, Gail
Publisher: name: arXiv
Year: 2014
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Fundamental stellar properties, such as mass, radius, and age, can be inferred using asteroseismology. Cool stars with convective envelopes have turbulent motions that can stochastically drive and damp pulsations. The properties of the oscillation frequency power spectrum can be tied to mass and radius through solar-scaled asteroseismic relations. Stellar properties derived using these scaling relations need verification over a range of metallicities. Because the age and mass of halo stars are well-constrained by astrophysical priors, they provide an independent, empirical check on asteroseismic mass estimates in the low-metallicity regime. We identify nine metal-poor red giants (including six stars that are kinematically associated with the halo) from a sample observed by both the Kepler space telescope and the Sloan Digital Sky Survey-III APOGEE spectroscopic survey. We compare masses inferred using asteroseismology to those expected for halo and thick-disk stars. Although our sample is small, standard scaling relations, combined with asteroseismic parameters from the APOKASC Catalog, produce masses that are systematically higher (=0.17+/-0.05 Msun) than astrophysical expectations. The magnitude of the mass discrepancy is reduced by known theoretical corrections to the measured large frequency separation scaling relationship. Using alternative methods for measuring asteroseismic parameters induces systematic shifts at the 0.04 Msun level. We also compare published asteroseismic analyses with scaling relationship masses to examine the impact of using the frequency of maximum power as a constraint. Upcoming APOKASC observations will provide a larger sample of ~100 metal-poor stars, important for detailed asteroseismic characterization of Galactic stellar populations.
description: 4 figures; 1 table. Accepted to ApJL
Dès le début. Die Friedensnote Papst Benedikts XV. von 1917, hg. v. Birgit Aschmann / Heinz-Gerhard Justenhoven
Creators: name: Simperl, Matthias
Publisher: name: Theologische Revue
Year: 2020

description: Theologische Revue, Bd. 116 (2020): November
MOND as a peculiar case of the SIV theory
Creators: name: Maeder, Andre
Publisher: name: arXiv
Year: 2023
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The scale invariant theory is preserving the fundamental physical properties of General Relativity, while enlarging the group of invariances subtending gravitation theory (Dirac1973; Canuto et al.1977). The Scale Invariant Vacuum (SIV) theory assumes, as gauging condition, that:"The macroscopic empty space is scale invariant, homogeneous and isotropic". Some basic properties in Weyl's Integrable Geometry and cotensor calculus are examined in relation with scalar-tensor theories. Possible scale invariant effects are strongly reduced by matter density, both at the cosmological and local levels. The weak feld limit of SIV tends to MOND, when the scale factor is taken as constant, an approximation valid (<1%) over the last 400 Myr. A better understanding of the a0-parameter is obtained: it corresponds to the equilibrium point of the Newtonian and SIV dynamical acceleration. Parameter a0 is not a universal constant, it depends on the density and age of the Universe. As MOND is doing, SIV theory avoids the call to dark matter, moreover the cosmological models predict accelerated expansion.
description: 9 pages, 2 figures
Supplementary document for Millimeter waves alter DNA secondary structures and modulate the transcriptome in human fibroblasts - 5799791.pdf
Creators: name: Lawler, Nicholas
name: Evans, Cameron
name: Romanenko, Sergii
name: Chaudhari, Nutan
name: Fear, Mark
name: Wood, Fiona
name: Smith, Nicole
name: Wallace, Vincent
name: Iyer, K. Swaminathan
Publisher: name: Optica Publishing Group
Year: 2022
Subjects: Uncategorized

description: Supplemental document containing supplemental figures and tables
Tagging Boosted Ws with Wavelets
Creators: name: Rentala, Vikram
name: Shepherd, William
name: Tait, Tim M. P.
Publisher: name: arXiv
Year: 2014
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: We present a new technique for distinguishing the hadronic decays of boosted heavy particles from QCD backgrounds based on wavelet transforms. As an initial exploration, we illustrate the technique in the particular case of hadronic $W$ boson decays, comparing it to the ``mass drop'' cut currently used by the LHC experiments. We apply wavelet cuts, which make use of complementary information, and in combination with the mass drop cut results in an improvement of $\sim$7% in discovery reach of hadronic $W$ boson final states over a wide range of transverse momenta.
description: 14 pages, 5 figures
Corrections for the Geometric Distortion of the Tube Detectors on SANS Instruments at ORNL
Creators: name: He, Lilin
name: Do, Changwoo
name: Qian, Shuo
name: Wignall, George D.
name: Heller, William T.
name: Littrell, Kenneth C.
name: Smith, Gregory S.
Publisher: name: arXiv
Year: 2014
Subjects: subject: Instrumentation and Detectors (physics.ins-det)
subject: FOS: Physical sciences

description: The small-angle neutron scattering instruments at the Oak Ridge National Laboratory High Flux Isotope Reactor recently upgraded the area detectors from the large, single volume crossed-wire detectors originally installed to staggered arrays of linear position-sensitive detectors, based on the design used on the EQ-SANS instrument at ORNL Spallation Neutron Source. The specific geometry of the LPSD array requires that approaches to data reduction traditionally employed be modified. Here, two methods for correcting the geometric distortion produced by the LPSD array are presented and compared. The first method applies a correction derived from a detector sensitivity measurement performed using the same configuration as the samples are measured. In the second method presented here, a solid angle correction derived for the LPSDs is applied to data collected in any instrument configuration during the data reduction process in conjunction with a detector sensitivity measurement collected at a sufficiently long camera length where the geometric distortions are negligible. Both methods produce consistent results and yield a maximum deviation of corrected data from isotropic scattering samples of less than 0.05 for momentum transfers up to a maximum of 0.8 A-1. The results are broadly applicable to any SANS instrument employing LPSD array detectors, which will be increasingly common as instruments having higher incident flux are constructed at various neutron scattering facilities around the world.
description: L.H., C. D. and S. Q. contributed equally to this work
Entropy conserving/stable schemes for a vector-kinetic model of hyperbolic systems
Creators: name: Anandan, Megala
name: Rao, S. V. Raghurama
Publisher: name: arXiv
Year: 2023
Subjects: subject: Numerical Analysis (math.NA)
subject: Mathematical Physics (math-ph)
subject: FOS: Mathematics
subject: FOS: Physical sciences

description: The moment of entropy equation for vector-BGK model results in the entropy equation for macroscopic model. However, this is usually not the case in numerical methods because the current literature consists only of entropy conserving/stable schemes for macroscopic model (to the best of our knowledge). In this paper, we attempt to fill this gap by developing an entropy conserving scheme for vector-kinetic model, and we show that the moment of this results in an entropy conserving scheme for macroscopic model. With the numerical viscosity of entropy conserving scheme as reference, the entropy stable scheme for vector-kinetic model is developed in the spirit of [33]. We show that the moment of this scheme results in an entropy stable scheme for macroscopic model. The schemes are validated on several benchmark test problems for scalar and shallow water equations, and conservation/stability of both kinetic and macroscopic entropies are presented.
The Effect of Sad Mood and Depressive Rumination on Autobiographical Memory: A Pre-Registration of Study Protocol
Creators: name: Hatami, Javad
name: Jahanitabesh, Azra
name: Boutimaz, Samaneh
Publisher: name: Open Science Framework
Year: 2023
Subjects: subject: Clinical Psychology
subject: Social and Behavioral Sciences
subject: Personality and Social Contexts
subject: Psychology
subject: FOS: Psychology
subject: autobiographical memory
subject: sad mood
subject: rumination
subject: trait versus state
subject: depression
subject: memory specificity

description: A Pre-Registration of a double-blind, parallel-group, randomized controlled experiment regarding state/chronic sad mood and state/trait depressive rumination effect on the specificity and overgenerality of autobiographical memory.
Radiation Feedback in ULIRGS: Are Photons Movers and Shakers?
Creators: name: Davis, Shane W.
name: Jiang, Yan-Fei
name: Stone, James M.
name: Murray, Norman
Publisher: name: arXiv
Year: 2014
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We use our variable Eddington tensor (VET) radiation hydrodynamics code to perform two-dimensional simulations to study the impact of radiation forces on atmospheres composed of dust and gas. Our setup closely follows that of Krumholz & Thompson, assuming that dust and gas are well-coupled and that the radiation field is characterized by blackbodies with temperatures >~ 80 K, as might be found in ultraluminous infrared galaxies. In agreement with previous work, we find that Rayleigh-Taylor instabilities develop in radiation supported atmospheres, leading to inhomogeneities that limit momentum exchange between radiation and dusty gas, and eventually providing a near balance of the radiation and gravitational forces. However, the evolution of the velocity and spatial distributions of the gas differs significantly from previous work, which utilized a less accurate flux-limited diffusion (FLD) method. Our VET simulations show continuous net acceleration of the gas, with no steady-state reached by the end of the simulation. In contrast, FLD results show little net acceleration of the gas and settle in to a quasi-steady, turbulent state with low velocity dispersion. The discrepancies result primarily from the inability of FLD to properly model the variation of the radiation field around structures that are less than a few optical depths across. We conclude that radiation feedback remains a viable mechanism for driving high-Mach number turbulence. We discuss implications for observed systems and global numerical simulations of feedback, but more realistic setups are needed to make robust observational predictions and assess the prospect of launching outflows with radiation.
description: 16 pages, 11 figures, submitted to ApJ
A New Causal Ideal Internal Dynamics Generator
Creators: name: Quan, Quan
name: Cai, Kai-Yuan
Publisher: name: arXiv
Year: 2014
Subjects: subject: Systems and Control (eess.SY)
subject: FOS: Electrical engineering, electronic engineering, information engineering

description: The design of ideal internal dynamics (IID) generators, namely solving IID, is a fundamental problem, which is a key step to handle the nonminimum-phase output tracking problem. In this paper, for a class of unstable matrix differential equations, a new causal dynamic IID generator is proposed, whose parameters are partly chosen via H_2/H_inf optimization. Compared with existing similar generators, it is applicable to matrix differential equations with singular system matrices and is easily extended to slowly time-varying matrix differential equations without extra computation.
description: 16 pages
Steiner, Niccolo: Diego Laínez und Alfonso Salmerón auf dem Konzil von Trient. Ihr Beitrag zur Eucharistie- und Messopferthematik
Creators: name: Dahlke, Benjamin
Publisher: name: Theologische Revue
Year: 2020

description: Theologische Revue, Bd. 116 (2020): November
Cooling antihydrogen ions for the free-fall experiment GBAR
Creators: name: Hilico, Laurent
name: Karr, Jean-Philippe
name: Douillet, Albane
name: Indelicato, Paul
name: Wolf, Sebastian
name: Kaler, Ferdinand Schmidt
Publisher: name: arXiv
Year: 2014
Subjects: subject: Atomic Physics (physics.atom-ph)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We discuss an experimental approach allowing to prepare antihydrogen atoms for the GBAR experiment. We study the feasibility of all necessary experimental steps: The capture of incoming $\bar{\rm H}^+$ ions at keV energies in a deep linear RF trap, sympathetic cooling by laser cooled Be$^+$ ions, transfer to a miniaturized trap and Raman sideband cooling of an ion pair to the motional ground state, and further reducing the momentum of the wavepacket by adiabatic opening of the trap. For each step, we point out the experimental challenges and discuss the efficiency and characteristic times, showing that capture and cooling are possible within a few seconds.
description: 10 pages, 5 figures
Halpha and [S II] emission from warm ionized gas in the Scutum-Centaurus Arm
Creators: name: Hill, Alex S.
name: Benjamin, Robert A.
name: Haffner, L. Matthew
name: Gostisha, Martin
name: Barger, Kathleen A.
Publisher: name: arXiv
Year: 2014
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present Wisconsin H-Alpha Mapper [S II] λ6716 and Hα spectroscopic maps of the warm ionized medium (WIM) in the Scutum-Centaurus Arm at Galactic longitudes 310° < l < 345°. Using extinction-corrected Hα intensities (IHαc), we measure an exponential scale height of electron density-squared in the arm of H_ne^2 = 0.30 kpc (assuming a distance of 3.5 kpc), intermediate between that observed in the inner Galaxy and in the Perseus Arm. The [S II]/Hα line ratio is enhanced at large |z| and in sightlines with faint IHαc. We find that the [S II]/Hα line ratio has a power law relationship with IHαc from a value of ~=1.0 at IHαc < 0.2 R (Rayleighs) to a value of ~=0.08 at IHαc >= 100 R. The line ratio is better correlated with Hα intensity than with height above the plane, indicating that the physical conditions within the WIM vary systematically with electron density. We argue that the variation of the line ratio with height is a consequence of the decrease of electron density with height. Our results reinforce the well-established picture in which the diffuse Hα emission is due primarily to emission from in situ photoionized gas, with scattered light only a minor contributor.
description: ApJ in press. 8 pages in emulateapj format
Agbagnon, Jean Prosper: „Und die Nacht wird leuchten wie der Tag“. Weltbild, Gottesbeziehung und Bewusstsein des Beters in Psalm 139
Creators: name: Eder, Sigrid
Publisher: name: Theologische Revue
Year: 2020

description: Theologische Revue, Bd. 116 (2020): November
The internal clock of many-body delocalization
Creators: name: Evers, Ferdinand
name: Modak, Ishita
name: Bera, Soumya
Publisher: name: arXiv
Year: 2023
Subjects: subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: After a decade of many claims to the opposite, there now is a growing consensus that generic disordered quantum wires, e.g. the XXZ-Heisenberg chain, do not exhibit many-body localization (MBL) - at least not in a strict sense within a reasonable window of disorder values $W$. Specifically, computational studies of short wires exhibit an extremely slow but unmistakable flow of physical observables with increasing time and system size (``creep") that is consistently directed away from (strict) localization. Our work sheds fresh light on delocalization physics: Strong sample-to-sample fluctuations indicate the absence of a generic time scale, i.e. of a naive ``clock rate"; however, the concept of an ``internal clock" survives, at least in an ensemble sense. Specifically, we investigate the relaxation of the imbalance $\mathcal{I}(t)$ and its temporal fluctuations $\mathcal{F}(t)$, the entanglement and Renyi entropies, $\mathcal{S}_{\mathrm{e}}(t)$ and $ \mathcal{S}_2(t)$, in a 1D system of interacting disordered fermions. We observe that adopting $\mathcal{S}_{\mathrm{e}}(t), \mathcal{S}_2(t)$ as a measure for the internal time per sample reduces the sample-to-sample fluctuations but does not eliminate them. However, a (nearly) perfect collapse of the average $\overline{\mathcal{I}}(t)$ and $\overline{\mathcal{F}}(t)$ for different $W$ is obtained when plotted against $\overline{\mathcal{S}}_{\mathrm{e}}(t)$ or $\overline{\mathcal{S}}_2(t)$, indicating that the average entropy appropriately models the ensemble-averaged internal clock. We take the tendency for faster-than-logarithmic growth of $\overline{\mathcal{S}}_{\mathrm{e}}(t)$ together with smooth dependency on $W$ of all our observables within the entire simulation window as support for the cross-over scenario, discouraging an MBL transition within the traditional parametric window of computational studies.
description: 15 pages, 12+5 figures, published version
The SDSS-2MASS-WISE Ten Dimensional Stellar Color Locus
Creators: name: Davenport, James R. A.
name: Ivezic, Zeljko
name: Becker, Andrew C.
name: Ruan, John J.
name: Hunt-Walker, Nicholas M.
name: Covey, Kevin R.
name: Lewis, Alexia R.
name: AlSayyad, Yusra
name: Anderson, Lauren M.
Publisher: name: arXiv
Year: 2014
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present the fiducial main sequence stellar locus traced by 10 photometric colors observed by SDSS, 2MASS, and WISE. Median colors are determined using 1,052,793 stars with r-band extinction less than 0.125. We use this locus to measure the dust extinction curve relative to the r-band, which is consistent with previous measurements in the SDSS and 2MASS bands. The WISE band extinction coefficients are larger than predicted by standard extinction models. Using 13 lines of sight, we find variations in the extinction curve in H, Ks, and WISE bandpasses. Relative extinction decreases towards Galactic anti-center, in agreement with prior studies. Relative extinction increases with Galactic latitude, in contrast to previous observations. This indicates a universal mid-IR extinction law does not exist due to variations in dust grain size and chemistry with Galactocentric position. A preliminary search for outliers due to warm circumstellar dust is also presented, using stars with high signal-to-noise in the W3-band. We find 199 such outliers, identified by excess emission in Ks-W3. Inspection of SDSS images for these outliers reveals a large number of contaminants due to nearby galaxies. Six sources appear to be genuine dust candidates, yielding a fraction of systems with infrared excess of 0.12$\pm$0.05%.
description: 11 pages, 10 figures, MNRAS Accepted. Tables 1 and 2 available online: https://github.com/jradavenport/wise_locus
Unveiling the impact of temperature on magnon diffuse scattering detection in the transmission electron microscope
Creators: name: Castellanos-Reyes, José Ángel
name: Zeiger, Paul
name: Bergman, Anders
name: Kepaptsoglou, Demie
name: Ramasse, Quentin M.
name: Idrobo, Juan Carlos
name: Rusz, Ján
Publisher: name: arXiv
Year: 2023
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Magnon diffuse scattering (MDS) signals could be studied with high spatial resolution in scanning transmission electron microscopy (STEM), thanks to recent technological progress in electron energy loss spectroscopy. However, detecting MDS signals in STEM is challenging due to their overlap with stronger thermal diffuse scattering (TDS) signals. In bcc Fe at 300 K, MDS signals greater than or comparable to TDS signals occur under the central Bragg disk, into a currently inaccesible energy-loss region. Therefore, to detect MDS in STEM, it is necessary to find conditions in which TDS and MDS signals can be separated. Temperature may be a key factor due to the distinct thermal signatures of magnon and phonon signals. In this work, we present a study on the effects of temperature on MDS and TDS in bcc Fe -- considering a detector outside the central Bragg disk and a fixed convergent electron probe -- using the frozen phonon and frozen magnon multislice methods. Our study reveals that neglecting the effects of atomic vibrations causes the MDS signal to grow approximately linearly up to the Curie temperature of Fe, after which it exhibits less variation. The MDS signal displays an alternating behavior due to dynamical diffraction, instead of increasing monotonically as a function of thickness. Including the effects of atomic vibrations through a complex atomic electrostatic potential causes the linear growth of the MDS signal to change to a non-linear behavior that exhibits a predominant peak for a sample of thickness 16.072 nm at 1100 K. In contrast, the TDS signal grows more linearly than the MDS signal but still exhibits appreciable dynamical diffraction effects. An analysis of the signal-to-noise ratio (SNR) shows that the MDS signal can be a statistically significant contribution to the total scattering intensity under realizable measurement conditions and acquisition times.
description: *) Changed title to "Unveiling the impact of temperature on magnon diffuse scattering detection in the transmission electron microscope." *) Incorporated the effects of absorption due to phonons in the magnon-diffuse-scattering calculations through a complex atomic electrostatic potential
title: Η χωρική εμπειρία μέσα από τα κινηματογραφικά πλάνα των πόλεων: Αναπαραστάσεις και ψευδαισθήσεις
title: Spatial experience through cinematic footage of cities: Representations and illusions
Creators: name: Δουρελιαδου Δημητρα-Θεοδωρα
Publisher: name: Technical University of Crete
Year: 2023

description: Στην παρούσα ερευνητική εργασία ο κινηματογραφημένος χώρος αξιοποιείται ως μέσο άντλησης χωρικών πληροφοριών της αρχιτεκτονικής μορφής και της αισθητηριακής αντίληψης που διαμορφώνουν τα ποιοτικά χαρακτηριστικά αυτής της οπτικοακουστικής εμπειρίας. Μέσα από την ανάλυση των χωρικών και ποιοτικών στοιχείων που συνθέτουν την εικόνα και τη δομή του χώρου που προβάλλεται στην οθόνη, προκύπτει ένας ανθρωποκεντρικός χαρακτηρισμός που περιγράφει το κάθε case study. Η αποδόμηση της εικόνας και η παρατήρηση των αρχιτεκτονικών μορφών, και των επιμέρους στοιχείων του πραγματικού και του κινηματογραφημένου χώρου -χρωμάτων, υφών, ήχου, δομής των κάδρων που επιλέγονται σε κάθε δράση- αποτελούν τη βασική μέθοδο κατηγοριοποίησης της πληροφορίας. Ο τρόπος που ο δημιουργός συνθέτει τα στοιχεία μεταξύ τους και τα διαφορετικά νοήματα που προκύπτουν από τη ροή μέσα στον φιλμικό χώρο οδηγούν σε αντιθέσεις και πολλές φορές παραπλανούν τον θεατή. Από την αντικειμενική αποκωδικοποίηση των χωρικών συστατικών θα δημιουργηθεί μια “Εργαλειοθήκη” που θα ανταποκρίνεται στην ανάλυση του κινηματογραφημένου χώρου αλλά και σε μια μεθοδολογία σχεδιασμού και επεξεργασίας του χώρου.
Summary of Gila Monster sample and genetic information collected for individuals sequenced in Nevada and Utah
Creators: name: Wood, Dustin A
Publisher: name: Zenodo
Year: 2022
Subjects: Heloderma suspectum
Gila Monster

description: Summary of Gila Monster sample and genetic information collected for individuals sequenced in Nevada and Utah. For all measurements an ‘NA’ indicates that no measurements were available. Sample, unique sample name Site Abbv, abbreviated name of collection site State, State where sample was collected County, county where the site occurs Locality, more detailed information of collection site Zone, projection UTM_N, UTM northing coordinates (meters) UTM_E, UTM easting coordinates (meters) Lat, Latitude Long, Longitude Date, date of tissue collection Sex, M=Male, F=Female, U=Unknown Other ident; other identifier used to label tissue sample Vial label, unique alpha-numeric code for each individual Filter, whether sample 'Passed' or 'Failed' bioinformatic filtering n_loci, the number of loci recovered mean_cov, mean coverage per sample missing, frequency of missing data.
Daemonic ergotropy in continuously-monitored open quantum batteries
Creators: name: Morrone, Daniele
name: Rossi, Matteo A. C.
name: Genoni, Marco G.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: The amount of work that can be extracted from a quantum system can be increased by exploiting the information obtained from a measurement performed on a correlated ancillary system. The concept of daemonic ergotropy has been introduced to properly describe and quantify this work extraction enhancement in the quantum regime. We here explore the application of this idea in the context of continuously-monitored open quantum systems, where information is gained by measuring the environment interacting with the energy-storing quantum device. We first show that the corresponding daemonic ergotropy takes values between the ergotropy and the energy of the corresponding unconditional state. The upper bound is achieved by assuming an initial pure state and a perfectly efficient projective measurement on the environment, independently of the kind of measurement performed. On the other hand, if the measurement is inefficient or the initial state is mixed, the daemonic ergotropy is generally dependent on the measurement strategy. This scenario is investigated via a paradigmatic example of an open quantum battery: a two-level atom driven by a classical field and whose spontaneously emitted photons are continuously monitored via either homodyne, heterodyne, or photo-detection.
description: 6 pages, 4 figures
HATS-5b: A Transiting hot-Saturn from the HATSouth Survey
Creators: name: Zhou, G.
name: Bayliss, D.
name: Penev, K.
name: Bakos, G. Á.
name: Hartman, J. D.
name: Jordán, A.
name: Mancini, L.
name: Mohler, M.
name: Csubry, Z.
name: Ciceri, S.
name: Brahm, R.
name: Rabus, M.
name: Buchhave, L.
name: Henning, T.
name: Suc, V.
name: Espinoza, N.
name: Béky, B.
name: Noyes, R. W.
name: Schmidt, B.
name: Butler, R. P.
name: Shectman, S.
name: Thompson, I.
name: Crane, J.
name: Sato, B.
name: Csák, B.
name: Lázár, J.
name: Papp, I.
name: Sári, P.
name: Nikolov, N.
Publisher: name: arXiv
Year: 2014
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: We report the discovery of HATS-5b, a transiting hot-Saturn orbiting a G type star, by the HAT-South survey. HATS-5b has a mass of Mp=0.24 Mj, radius of Rp=0.91 Rj, and transits its host star with a period of P=4.7634d. The radius of HATS-5b is consistent with both theoretical and empirical models. The host star has a V band magnitude of 12.6, mass of 0.94 Msun, and radius of 0.87 Rsun. The relatively high scale height of HATS-5b, and the bright, photometrically quiet host star, make this planet a favourable target for future transmission spectroscopy follow-up observations. We reexamine the correlations in radius, equilibrium temperature, and metallicity of the close-in gas-giants, and find hot Jupiter-mass planets to exhibit the strongest dependence between radius and equilibrium temperature. We find no significant dependence in radius and metallicity for the close-in gas-giant population.
description: 10 pages, submitted to AJ
Exploitation Plan (D8.12)
Creators: name: Miller, Raeanne
name: Bearzotti, Chiara
Publisher: name: Zenodo
Year: 2018

description: Deliverable: D8.12 Exploitation Plan Work package in charge: WP8 Communication, Dissemination, Engagement and Exploitation Actual delivery date for this deliverable: Project-month 12 Dissemination level: The general public (PU) Lead author SAMS Research Services Ltd (SRSL): Raeanne Miller Other contributing author Danish Meteorological Institute(DMI): Chiara Bearzotti
description: We support the Blue Growth! Visit us on: www.blue-action.eu Follow us on Twitter: @BG10Blueaction
Scaling limit for line ensembles of random walks with geometric area tilts
Creators: name: Serio, Christian
Publisher: name: arXiv
Year: 2023
Subjects: subject: Probability (math.PR)
subject: Mathematical Physics (math-ph)
subject: FOS: Mathematics
subject: FOS: Physical sciences
subject: 60G50, 60F17, 82B41, 82B20

description: We consider line ensembles of non-intersecting random walks constrained by a hard wall, each tilted by the area underneath it with geometrically growing pre-factors $\mathfrak{b}^i$ where $\mathfrak{b}>1$. This is a model for the level lines of the $(2+1)$D SOS model above a hard wall, which itself mimics the low-temperature 3D Ising interface. A similar model with $\mathfrak{b}=1$ and a fixed number of curves was studied by Ioffe, Velenik, and Wachtel (2018), who derived a scaling limit as the time interval $[-N,N]$ tends to infinity. Line ensembles of Brownian bridges with geometric area tilts ($\mathfrak{b}>1$) were studied by Caputo, Ioffe, and Wachtel (2019), and later by Dembo, Lubetzky, and Zeitouni (2022). Their results show that as the time interval and the number of curves $n$ tend to infinity, the top $k$ paths converge to a limiting measure $μ$. In this paper we address the open problem of proving existence of a scaling limit for random walk ensembles with geometric area tilts. We prove that with mild assumptions on the jump distribution, under suitable scaling the top $k$ paths converge to the same measure $μ$ as $N\to\infty$ followed by $n\to\infty$. We do so both in the case of bridges fixed at $\pm N$ and of walks fixed only at $-N$.
description: Corrected a few typos and added new references. 12 pages
Project website www.blue-action.eu (D8.3)
Creators: name: Bearzotti, Chiara
name: Paterson, Euan
Publisher: name: Zenodo
Year: 2017
Subjects: Blue-Action

description: About this document
 Deliverable: D8.3
 Work package in charge: WP8 Communication, Dissemination, Engagement and Exploitation
 Actual delivery date for this deliverable: Project-month 2
 Dissemination level: The general public (PU)
 Lead author(s)
 Danish Meteorological Institute: Chiara Bearzotti
 Other contributing author(s)
 SAMS: Euan Paterson Summary The website www.blue-action.eu has been set up in December 2016 for ensuring that we “promote the action and its results, by providing targeted information to multiple audiences (including the media and the public) in a strategic and effective manner” (Art. 38.1 of the Grant Agreement).
 The website has been set up by the Project Office at DMI, with tools made available by MPI-M. During the lifetime of the project, the website will be populated with additional sections related to the presentation of the project tools and results.
description: We support the Blue Growth! Visit us on: www.blue-action.eu Follow us on Twitter: @BG10Blueaction
Protoplanetary disc evolution affected by star-disc interactions in young stellar clusters
Creators: name: Rosotti, Giovanni P.
name: Dale, James E.
name: Ovelar, Maria de Juan
name: Hubber, David A.
name: Kruijssen, J. M. Diederik
name: Ercolano, Barbara
name: Walch, Stefanie
Publisher: name: arXiv
Year: 2014
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Most stars form in a clustered environment. Therefore, it is important to assess how this environment influences the evolution of protoplanetary discs around young stars. In turn, this affects their ability to produce planets and ultimately life. We present here for the first time 3D SPH/N-body simulations that include both the hydrodynamical evolution of the discs around their natal stars, as well as the dynamics of the stars themselves. The discs are viscously evolving, accreting mass onto the central star and spreading. We find penetrating encounters to be very destructive for the discs as in previous studies, although the frequency of such encounters is low. We also find, however, that encounter influence the disc radii more strongly than other disc properties such as the disc mass. The disc sizes are set by the competition between viscous spreading and the disruptive effect of encounters. As discs spread, encounters become more and more important. In the regime of rapid spreading encounters simply truncate the discs, stripping the outer portions. In the opposite regime, we find that the effect of many distant encounters is able to limit the disc size. Finally, we predict from our simulations that disc sizes are limited by encounters at stellar densities exceeding $\sim 2-3 \times 10^3 \ \mathrm{pc}^{-2}$.
description: 18 pages, 13 figures; accepted by MNRAS
Final Thesis- Effect of Different Management Scenarios on Key Nutrients for Algae Growth in the Lago Ypacarai Watershed
Creators: name: Price, Thomas
Publisher: name: figshare
Year: 2022
Subjects: subject: 70402 Aquatic Ecosystem Studies and Stock Assessment
subject: FOS: Agriculture, forestry and fisheries
subject: 70301 Agro-ecosystem Function and Prediction
subject: 50102 Ecosystem Function
subject: FOS: Earth and related environmental sciences
subject: 60204 Freshwater Ecology
subject: FOS: Biological sciences
subject: 90903 Geospatial Information Systems
subject: FOS: Environmental engineering
subject: 70104 Agricultural Spatial Analysis and Modelling
subject: FOS: Other agricultural sciences
subject: 149902 Ecological Economics
subject: FOS: Economics and business
subject: 140205 Environment and Resource Economics

description: The watershed of Lago (lake) Ypacaraí is a hotspot for biodiversity and tourism in Paraguay. Currently the lake and its surrounding tributaries are in a eutrophic state. This study uses the Resource Investment Optimization System (RIOS) 1.1.16 and Integrated Valuation of Ecosystem Services and Tradeoffs (InVEST) 3.6.0 nutrient retention models to value the retention levels of the primary contributors to the eutrophication process (phosphorous and nitrogen) from different habitats and management scenarios. This study analyzed the management practices of sustainable agriculture, reforestation, payment for ecosystem services and wetland restoration for their effect on nutrient retention under various restoration scenarios and degradation scenarios. The findings were at the municipal, departmental and watershed level for the different management practices. At the municipal level this study found that Pirayu in the Paraguari department was the most important municipality to implement sustainable management practices. At the watershed level the study found that the most important watershed to implement sustainable management practices was the Salado. The most important department to implement sustainable management practices was found to be Central where PES could mitigate around 10 grams per dollar invested of nutrient export and load. We also found that implementing sustainable agriculture in the Salado could mitigate around 3 grams of load and 1 gram of export of nutrients per dollar invested. The most important management practice at the watershed level was found to be sustainable agriculture with around .003 kilos mitigated per dollar on nutrient load and 1 gram mitigated per dollar on nutrient export. This study found that with each hectare that is deforested an average 2,000 grams of nutrients per hectare is lost. Ultimately these results can help land managers decide what sustainable management practices to focus on and in what key areas.
Presentation: Geothermal Well Drilling Plan In Consideration To Geological Structures Of Mataloko Geothermal Field, Flores
Creators: name: Yudistian Yunis
name: Fajar Hendrasto
name: Pudyastuti, Kris
name: Sammuel, Evan R.
name: Dhany Rizky
Publisher: name: Zenodo
Year: 2020

description: This material presented in 2nd ICESE 2020
A direct way to observe absolute molecular handedness
Creators: name: Vager, Zeev
Publisher: name: arXiv
Year: 2014
Subjects: subject: Chemical Physics (physics.chem-ph)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: Unique labeling of chiral stereo-centers must include their handedness. The conventional method that has been developed to do this was originated by three chemists: R.S. Cahn, C. Ingold, and V. Prelog (CIP) and is formally known as R,S nomenclature. It requires knowledge of the spatial absolute configuration of that center. Traditionally, experimental methods of extracting handedness go through the absolute configuration and only then through the application of the CIP convention. Here we show that a direct experimental method of determination of the natural handedness by the polarization of tunneling electrons is almost always compatible with the CIP convention. By the sole use of symmetry arguments we show that the chiral molecule symmetry withdraws the need of fine structure splitting. As a consequence, the polarization of electrons tunneling through the molecular electric dipole direction uniquely determines their handedness. The symmetry breaking argument that induces lack of fine-structure splitting eliminates the need for a precise value of the spin-orbit interaction.
WEARDA: Recording Wearable Sensor Data for Human Activity Monitoring
Creators: name: van Dijk, Richard M. K.
name: Gawehns, Daniela
name: van Leeuwen, Matthijs
Publisher: name: arXiv
Year: 2023
Subjects: subject: Human-Computer Interaction (cs.HC)
subject: Computers and Society (cs.CY)
subject: FOS: Computer and information sciences

description: We present WEARDA, the open source WEARable sensor Data Acquisition software package. WEARDA facilitates the acquisition of human activity data with smartwatches and is primarily aimed at researchers who require transparency, full control, and access to raw sensor data. It provides functionality to simultaneously record raw data from four sensors -- tri-axis accelerometer, tri-axis gyroscope, barometer, and GPS -- which should enable researchers to, for example, estimate energy expenditure and mine movement trajectories. A Samsung smartwatch running the Tizen OS was chosen because of 1) the required functionalities of the smartwatch software API, 2) the availability of software development tools and accessible documentation, 3) having the required sensors, and 4) the requirements on case design for acceptance by the target user group. WEARDA addresses five practical challenges concerning preparation, measurement, logistics, privacy preservation, and reproducibility to ensure efficient and errorless data collection. The software package was initially created for the project "Dementia back at the heart of the community", and has been successfully used in that context.
description: Submitted 20 January 2023; Accepted 6 July 2023; Published 26 October 2023 by the Journal of Open Research Software JORS, 11 pages, 5 figures, 3 tables