cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Thermal smearing of the magneto-Kohn anomaly for Dirac materials and comparison with the two-dimensional electron liquid
Creators: name: Gumbs, Godfrey
name: Balassis, Antonios
name: Dahal, Dipendra
name: Glasser, M. L.
Publisher: name: arXiv
Year: 2015
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We compute and compare the effects due to a uniform perpendicular magnetic field as well as temperature on the static polarization functions for monolayer graphene (MLG), associated with the Dirac point, with that for the two-dimensional electron liquid (2DEL) with the use of comprehensive numerical calculations. Previous results for the 2DEL are discussed and, in particular, we point out a flaw in a reported analytic derivation which was carried out to exhibit the smearing of the Fermi surface for 2DEL. The relevance of our study to the Kohn anomaly in low-dimensional structures and the Friedel oscillations for the screening of the potential for a dilute distribution of impurities is reported. Our results show substantial differences due to screening for the 2DEL and MLG which have not been given adequate attention previously.
Stellungnahme der Physikalisch-Technischen Bundesanstalt (PTB) zur Frage, ob bei Laserscannern der PoliScan-Familie, mit denen aus einem stehenden Messfahrzeug heraus gemessen wird, das Ein- und Aussteigen oder Bewegungen des Messpersonals im Messfahrzeug zu Falschmessungen führen können
Creators: name: Physikalisch-Technische Bundesanstalt (PTB), Fachbereich 1.3 "Geschwindigkeit"
Publisher: name: Physikalisch-Technische Bundesanstalt (PTB)
Year: 2016
Subjects: amtliche Geschwindigkeitsüberwachung
technische Stellungnahme

description: Es kommt immer mal wieder die Frage auf, welchen Einfluss es hat, wenn bei einer Laserscanner-Geschwindigkeitsmessung aus einem stehenden Fahrzeug heraus das Messpersonal ins Fahrzeug ein- und aussteigt oder sich darin bewegt. Nun, die resultierenden Wackelbewegungen sind viel zu klein, um irgendeinen Einfluss auf die Messrichtigkeit zu haben. Neben einer einfachen Berechnung zeigen wir auch, wie man ganz leicht mit einem Handy und einer Wasserwaagen-App zu diesem Ergebnis kommen kann.
title: NATSUSHIMA Cruise Report NT11-17
Creators: name: Fukuba, Tatsuhiro
Publisher: name: JAMSTEC
Year: 2011
Subjects: subject: oceans
subject: Cruise report
subject: R/V NATSUSHIMA

description: [CRUISE REPORT] This document is a preliminary report of NT11-17 on R/V NATSUSHIMA from 2011-09-05 to 2011-09-10.
On the compressibility effect in test particle acceleration by magnetohydrodynamic turbulence
Creators: name: González, C. A.
name: Dmitruk, P.
name: Mininni, P. D.
name: Matthaeus, W. H.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Plasma Physics (physics.plasm-ph)
subject: FOS: Physical sciences

description: The effect of compressibility in charged particle energization by magnetohydrodynamic (MHD) fields is studiedin the context of test particle simulations. This problem is relevant to the solar wind and the solar corona due to the compressible nature of the flow in those astrophysical scenarios. We consider turbulent electromagnetic fields obtained from direct numerical simulations of the MHD equations with a strong background magnetic field. In order to explore the flow compressibilty effect over the particle dynamics we performed different numerical experiments: an incompressible case, and two weak compressible cases with Mach number M = 0.1 and M = 0.25. We analyze the behavior of protons and electrons in those turbulent fields, which are well known to form aligned current sheets in the direction of the guide magnetic field. What we call protons and electrons are test particles with scales comparable to (for protons) and much smaller than (for electrons) the dissipative scale of MHD turbulence, maintaining the correct mass ratio me /mi. For these test particles we show that compressibility enhances the efficiency of proton acceleration, and that the energization is caused by perpendicular electric fields generated between currents sheets. On the other hand, electrons remain magnetized and display an almost adiabatic motion, with no effect of compressibility observed. Another set of numerical experiments takes into account two fluid modifications, namely electric field due to Hall effect and electron pressure gradient. We show that the electron pressure has an important contribution to electron acceleration allowing highly parallel energization. In contrast, no significant effect of these additional terms is observed for the protons.
description: 10 pages
Interpreting B-anomalies within an extended 331 gauge theory
Creators: name: Addazi, Andrea
name: Ricciardi, Giulia
name: Scarlatella, Simone
name: Srivastava, Rahul
name: Valle, José W. F.
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: In light of the recent $R_{K^{(*)}}$ data on neutral current flavour anomalies in $B \to K^{(*)} \ell^+ \ell^-$ decays, we re-examine their quantitative interpretation in terms of an extended 331 gauge theory framework. We achieve this by adding two extra lepton species with novel 331 charges, while ensuring that the model remains anomaly free. In contrast to the canonical 331 models, the gauge charges of the first and second lepton families differ from each other, allowing lepton flavour universality violation. We further expand the model by adding the neutral fermions required to provide an adequate description for small neutrino masses.
description: 26 pages, 5 tables, 3 figures. Title modified, typos corrected, conclusions unchanged. Matches published Phys. Rev. D version
title: R/V Natsushima "Cruise Report" NT11-16
Creators: name: Kawagucci, Shinsuke
Publisher: name: JAMSTEC
Year: 2011
Subjects: subject: oceans
subject: Cruise report
subject: R/V NATSUSHIMA

description: [CRUISE REPORT] This document is a preliminary report of NT11-16 on R/V NATSUSHIMA from 2011-08-25 to 2011-09-02.
Bifurcations of lunisolar secular resonances for space debris orbits
Creators: name: Celletti, Alessandra
name: Galeş, Cătălin
name: Pucacco, Giuseppe
Publisher: name: arXiv
Year: 2015
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Dynamical Systems (math.DS)
subject: FOS: Physical sciences
subject: FOS: Mathematics
subject: 37N05, 37L10, 70F15

description: Using bifurcation theory, we study the secular resonances induced by the Sun and Moon on space debris orbits around the Earth. In particular, we concentrate on a special class of secular resonances, which depend only on the debris' orbital inclination. This class is typically subdivided into three distinct types of secular resonances: those occurring at the critical inclination, those corresponding to polar orbits, and a third type resulting from a linear combination of the rates of variation of the argument of perigee and the longitude of the ascending node. The model describing the dynamics of space debris includes the effects of the geopotential, as well as the Sun's and Moon's attractions, and it is defined in terms of suitable action-angle variables. We consider the system averaged over both the mean anomaly of the debris and those of the Sun and Moon. Such multiply-averaged Hamiltonian is used to study the lunisolar resonances which depend just on the inclination. Borrowing the technique from the theory of bifurcations of Hamiltonian normal forms, we study the birth of periodic orbits and we determine the energy thresholds at which the bifurcations of lunisolar secular resonances take place. This approach gives us physically relevant information on the existence and location of the equilibria, which help us to identify stable and unstable regions in the phase space. Besides their physical interest, the study of inclination dependent resonances offers interesting insights from the dynamical point of view, since it sheds light on different phenomena related to bifurcation theory.
description: 39 pages, 10 figures
title: NT11-15 Cruise Report
Creators: name: Ishibashi, Jun-ichiro
Publisher: name: JAMSTEC
Year: 2011
Subjects: subject: oceans
subject: Cruise report
subject: R/V NATSUSHIMA

description: [CRUISE REPORT] This document is a preliminary report of NT11-15 on R/V NATSUSHIMA from 2011-08-14 to 2011-08-23.
Antworten auf häufige Fragen zum Laserscanner-Geschwindigkeitsüberwachungsgerät PoliScanspeed der Fa. VITRONIC
Creators: name: Physikalisch-Technische Bundesanstalt (PTB), Fachbereich 1.3 "Geschwindigkeit"
Publisher: name: Physikalisch-Technische Bundesanstalt (PTB)
Year: 2017
Subjects: amtliche Geschwindigkeitsüberwachung
technische Stellungnahme
Laserscanner
PoliScan

description: Im Zusammenhang mit der Messwertbildung des PoliScan-Geschwindigkeitsmessgerätes der Firma VITRONIC legen wir grundlegende Zusammenhänge dar. Die Zulassung des Gerätes ist unverändert gültig, denn das Gerät funktioniert genau wie vorgesehen, die Messrichtigkeit ist gegeben und unter gleichen Bedingungen sind gleiche Ergebnisse zu erwarten.
Indistinguishability-enhanced entanglement recovery by spatially localized operations and classical communication
Creators: name: Piccolini, Matteo
name: Nosrati, Farzam
name: Morandotti, Roberto
name: Franco, Rosario Lo
Publisher: name: arXiv
Year: 2022
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We extend a procedure exploiting spatial indistinguishability of identical particles to recover the spoiled entanglement between two qubits interacting with Markovian noisy environments. Here, the spatially localized operations and classical communication (sLOCC) operational framework is used to activate the entanglement restoration from the indistinguishable constituents. We consider the realistic scenario where noise acts for the whole duration of the process. Three standard types of noises are considered: a phase damping, a depolarizing, and an amplitude damping channel. Within this general scenario, we find the entanglement to be restored in an amount proportional to the degree of spatial indistinguishability. These results elevate sLOCC to a practical framework for accessing and utilizing quantum state protection within a quantum network of spatially indistinguishable subsystems.
description: 13 pages, 10 figures. Submitted to a Special Issue in memoriam of Prof. Andrzej Kossakowski
Many-body localization phase transition: A simplified strong-randomness approximate renormalization group
Creators: name: Zhang, Liangsheng
name: Zhao, Bo
name: Devakul, Trithep
name: Huse, David A.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: FOS: Physical sciences

description: We present a simplified strong-randomness renormalization group (RG) that captures some aspects of the many-body localization (MBL) phase transition in generic disordered one-dimensional systems. This RG can be formulated analytically, and the critical fixed point distribution and critical exponents (that satisfy the Chayes inequality) are obtained to numerical precision by solving integro-differential equations. This reproduces many, but not all, of the qualitative features of the MBL phase transition that are suggested by previous numerical work and approximate RG studies: our RG might serve as a "zeroth-order" approximation for future RG studies. One interesting feature that we highlight is that the rare Griffiths regions are fractal. For thermal Griffiths regions within the MBL phase, this feature might be qualitatively correctly captured by our RG. If this is correct beyond our approximations, then these Griffiths effects are stronger than has been previously assumed.
description: 10 pages, 5 figures; added references; as in journal
Historische Kritik und theologische Exegese der synoptischen Evangelien
Creators: name: Schierse, Franz Joseph
Publisher: name: Scholastik
Year: 1970

description: Scholastik, Bd. 29 Nr. 4 (1954): Scholastik. Vierteljahresschrift für Theologie und Philosophie, Band 29, Heft 4
Parametrising CCQE uncertainties in the Spectral Function model for neutrino oscillation analyses
Creators: name: Chakrani, Jaafar
name: Avanzini, Margherita Buizza
name: Dolan, Stephen
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: A substantial fraction of systematic uncertainties in neutrino oscillation experiments stems from the lack of precision in modeling the nucleus when describing the neutrino-nucleus interactions. The Spectral Function (SF) model features a distribution of momenta and removal energies of nucleons inside the nucleus within the shell-model picture, and also accounts for short-range correlations between nucleons. These characteristics offer significant improvements with respect to the more commonly used Fermi gas-based models. Electron scattering experiments offer a precise probe of the structure of the nucleus and have been used to both construct and validate the SF model. SF is thus an interesting reference model for long baseline neutrino experiments. Based on constraints from electron scattering data, we develop a set of parameters that can alter the occupancy of the nuclear shells and the distribution of the nucleon momentum within each shell. In addition, the impact of final-state interactions on the outgoing lepton and nucleon kinematics, the contribution of short-range correlations and the effect of Pauli blocking can also be modified. In this document, we will first describe the development of these parameters, partially based on a comparison with electron scattering data. We then show fits of these parameters to available T2K and MINER$ν$A cross-section data and discuss how they can be used to constrain the systematic uncertainties related to the SF model in neutrino oscillation analyses.
title: R/V Natsushima Cruise Report NT11-13
Creators: name: Ichihara, Hiroshi
Publisher: name: JAMSTEC
Year: 2011
Subjects: subject: oceans
subject: Cruise report
subject: R/V NATSUSHIMA

description: [CRUISE REPORT] This document is a preliminary report of NT11-13 on R/V NATSUSHIMA from 2011-07-25 to 2011-07-30.
A measurement of the time profile of scintillation induced by low energy gamma-rays in liquid xenon with the XMASS-I detector
Creators: name: XMASS Collaboration
name: Takiya, H.
name: Abe, K.
name: Hiraide, K.
name: Ichimura, K.
name: Kishimoto, Y.
name: Kobayashi, K.
name: Kobayashi, M.
name: Moriyama, S.
name: Nakahata, M.
name: Norita, T.
name: Ogawa, H.
name: Sekiya, H.
name: Takachio, O.
name: Takeda, A.
name: Tasaka, S.
name: Yamashita, M.
name: Yang, B. S.
name: Kim, N. Y.
name: Kim, Y. D.
name: Itow, Y.
name: Kegasa, R.
name: Kobayashi, K.
name: Masuda, K.
name: Fushimi, K.
name: Martens, K.
name: Suzuki, Y.
name: Fujita, R.
name: Hosokawa, K.
name: Miuchi, K.
name: Oka, N.
name: Onishi, Y.
name: Takeuchi, Y.
name: Kim, Y. H.
name: Lee, J. S.
name: Lee, K. B.
name: Lee, M. K.
name: Fukuda, Y.
name: Nishijima, K.
name: Nakamura, S.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Instrumentation and Detectors (physics.ins-det)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Physics - Experiment (hep-ex)
subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: We report the measurement of the emission time profile of scintillation from gamma-ray induced events in the XMASS-I 832 kg liquid xenon scintillation detector. Decay time constant was derived from a comparison of scintillation photon timing distributions between the observed data and simulated samples in order to take into account optical processes such as absorption and scattering in liquid xenon. Calibration data of radioactive sources, $^{55}$Fe, $^{241}$Am, and $^{57}$Co were used to obtain the decay time constant. Assuming two decay components, $τ_1$ and $τ_2$, the decay time constant $τ_2$ increased from 27.9 ns to 37.0 ns as the gamma-ray energy increased from 5.9 keV to 122 keV. The accuracy of the measurement was better than 1.5 ns at all energy levels. A fast decay component with $τ_1 \sim 2$ ns was necessary to reproduce data. Energy dependencies of $τ_2$ and the fraction of the fast decay component were studied as a function of the kinetic energy of electrons induced by gamma-rays. The obtained data almost reproduced previously reported results and extended them to the lower energy region relevant to direct dark matter searches.
description: 7 pages, 3 figures, accepted for publication in Nucl. Instrum. Meth. A
Deep Learning based Coverage and Rate Manifold Estimation in Cellular Networks
Creators: name: Mondal, Washim Uddin
name: Mankar, Praful D.
name: Das, Goutam
name: Aggarwal, Vaneet
name: Ukkusuri, Satish V.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Networking and Internet Architecture (cs.NI)
subject: Machine Learning (cs.LG)
subject: FOS: Computer and information sciences

description: This article proposes Convolutional Neural Network-based Auto Encoder (CNN-AE) to predict location-dependent rate and coverage probability of a network from its topology. We train the CNN utilising BS location data of India, Brazil, Germany, and the USA and compare its performance with stochastic geometry (SG) based analytical models. In comparison to the best-fitted SG-based model, CNN-AE improves the coverage and rate prediction errors by a margin of as large as $40\%$ and $25\%$ respectively. As an application, we propose a low complexity, provably convergent algorithm that, using trained CNN-AE, can compute locations of new BSs that need to be deployed in a network in order to satisfy pre-defined spatially heterogeneous performance goals.
Stellar mass functions of galaxies, disks and spheroids at z~0.1
Creators: name: Thanjavur, Karun
name: Simard, Luc
name: Bluck, Asa F. L.
name: Mendel, Trevor
Publisher: name: arXiv
Year: 2016
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present the stellar mass functions (SMF) and mass densities of galaxies, and their spheroid and disk components in the local (z~0.1) universe over the range 8.9 <= log(M/M_solar) <= 12 from spheroid+disk decompositions and corresponding stellar masses of a sample of over 600,000 galaxies in the SDSS-DR7 spectroscopic sample. The galaxy SMF is well represented by a single Schechter function (M* = 11.116+/-0.011, alpha = -1.145+/-0.008), though with a hint of a steeper faint end slope. The corresponding stellar mass densities are (2.670+/-0.110), (1.687+/-0.063) and (0.910+/-0.029)x10^8 M_solar Mpc^-3 for galaxies, spheroids and disks respectively. We identify a crossover stellar mass of log(M/M_solar) = 10.3+/-0.030 at which the spheroid and disk SMFs are equal. Relative contributions of four distinct spheroid/disk dominated sub-populations to the overall galaxy SMF are also presented. The mean disk-to-spheroid stellar mass ratio shows a five fold disk dominance at the low mass end, decreasing monotonically with a corresponding increase in the spheroidal fraction till the two are equal at a galaxy stellar mass, log(M/M_solar)=10.479+/-0.013, the dominance of spheroids then grows with increasing stellar mass. The relative numbers of composite disk and spheroid dominated galaxies show peaks in their distributions, perhaps indicative of a preferred galaxy mass. Our characterization of the low redshift galaxy population provides stringent constraints for numerical simulations to reproduce.
description: 30 pages, 18 figures, 5 tables (2 online), Accepted for publication in MNRAS
Scanning SQUID susceptometers with sub-micron spatial resolution
Creators: name: Kirtley, John R.
name: Paulius, Lisa
name: Rosenberg, Aaron J.
name: Palmstrom, Johanna C.
name: Holland, Connor M.
name: Spanton, Eric M.
name: Schiessl, Daniel
name: Jermain, Colin L.
name: Gibbons, Jonathan
name: Fung, Y. -K. -K.
name: Huber, Martin E.
name: Ralph, Daniel C.
name: Ketchen, Mark B.
name: Gibson, Gerald W.
name: Moler, Kathryn A.
Publisher: name: arXiv
Year: 2016
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: Superconducting QUantum Interference Device (SQUID) microscopy has excellent magnetic field sensitivity, but suffers from modest spatial resolution when compared with other scanning probes. This spatial resolution is determined by both the size of the field sensitive area and the spacing between this area and the sample surface. In this paper we describe scanning SQUID susceptometers that achieve sub-micron spatial resolution while retaining a white noise floor flux sensitivity of $\approx 2μΦ_0/Hz^{1/2}$. This high spatial resolution is accomplished by deep sub-micron feature sizes, well shielded pickup loops fabricated using a planarized process, and a deep etch step that minimizes the spacing between the sample surface and the SQUID pickup loop. We describe the design, modeling, fabrication, and testing of these sensors. Although sub-micron spatial resolution has been achieved previously in scanning SQUID sensors, our sensors not only achieve high spatial resolution, but also have integrated modulation coils for flux feedback, integrated field coils for susceptibility measurements, and batch processing. They are therefore a generally applicable tool for imaging sample magnetization, currents, and susceptibilities with higher spatial resolution than previous susceptometers.
description: 13 figures
PageRank Pipeline Benchmark: Proposal for a Holistic System Benchmark for Big-Data Platforms
Creators: name: Dreher, Patrick
name: Byun, Chansup
name: Hill, Chris
name: Gadepally, Vijay
name: Kuszmaul, Bradley
name: Kepner, Jeremy
Publisher: name: arXiv
Year: 2016
Subjects: subject: Performance (cs.PF)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: Distributed, Parallel, and Cluster Computing (cs.DC)
subject: Data Analysis, Statistics and Probability (physics.data-an)
subject: FOS: Computer and information sciences
subject: FOS: Physical sciences

description: The rise of big data systems has created a need for benchmarks to measure and compare the capabilities of these systems. Big data benchmarks present unique scalability challenges. The supercomputing community has wrestled with these challenges for decades and developed methodologies for creating rigorous scalable benchmarks (e.g., HPC Challenge). The proposed PageRank pipeline benchmark employs supercomputing benchmarking methodologies to create a scalable benchmark that is reflective of many real-world big data processing systems. The PageRank pipeline benchmark builds on existing prior scalable benchmarks (Graph500, Sort, and PageRank) to create a holistic benchmark with multiple integrated kernels that can be run together or independently. Each kernel is well defined mathematically and can be implemented in any programming environment. The linear algebraic nature of PageRank makes it well suited to being implemented using the GraphBLAS standard. The computations are simple enough that performance predictions can be made based on simple computing hardware models. The surrounding kernels provide the context for each kernel that allows rigorous definition of both the input and the output for each kernel. Furthermore, since the proposed PageRank pipeline benchmark is scalable in both problem size and hardware, it can be used to measure and quantitatively compare a wide range of present day and future systems. Serial implementations in C++, Python, Python with Pandas, Matlab, Octave, and Julia have been implemented and their single threaded performance has been measured.
description: 9 pages, 7 figures, to appear in IPDPS 2016 Graph Algorithms Building Blocks (GABB) workshop
Mapping Class Group Representations Derived from Stated Skein Algebras
Creators: name: Korinman, Julien
Publisher: name: arXiv
Year: 2022
Subjects: subject: Quantum Algebra (math.QA)
subject: Algebraic Topology (math.AT)
subject: FOS: Mathematics

description: We construct finite-dimensional projective representations of the mapping class groups of compact connected oriented surfaces having one boundary component using stated skein algebras.
description: Parts of the exposition of Sections 2-4 already appeared in the author's unpublished survey arXiv:2105.09563
Ist der „historische" Gottesbeweis ein Zirkelschluß?
Creators: name: Keilbach, Wilhelm
Publisher: name: Scholastik
Year: 1970

description: Scholastik, Bd. 29 Nr. 4 (1954): Scholastik. Vierteljahresschrift für Theologie und Philosophie, Band 29, Heft 4
title: R/V Natsushima Cruise Report NT11-12
Creators: name: Shimomura, Norio
Publisher: name: JAMSTEC
Year: 2011
Subjects: subject: oceans
subject: Cruise report
subject: R/V NATSUSHIMA

description: [CRUISE REPORT] This document is a preliminary report of NT11-12 on R/V NATSUSHIMA from 2011-07-15 to 2011-07-23.
Asymptotic normality of linear statistics of zeros of random polynomials
Creators: name: Bayraktar, Turgay
Publisher: name: arXiv
Year: 2016
Subjects: subject: Complex Variables (math.CV)
subject: Probability (math.PR)
subject: FOS: Mathematics

description: In this note, we prove a central limit theorem for smooth linear statistics of zeros of random polynomials which are linear combinations of orthogonal polynomials with iid standard complex Gaussian coefficients. Along the way, we obtain Bergman kernel asymptotics for weighted $L^2$-space of polynomials endowed with varying measures of the form $e^{-2nφ_n(z)}dz$ under suitable assumptions on the weight functions $φ_n$.
description: Minor revisions, references added. To appear in Proc. of Amer. Math. Soc
title: NATSUSHIMA Cruise Report NT11-11
Creators: name: Shiobara, Hajime
Publisher: name: JAMSTEC
Year: 2011
Subjects: subject: oceans
subject: Cruise report
subject: R/V NATSUSHIMA

description: [CRUISE REPORT] This document is a preliminary report of NT11-11 on R/V NATSUSHIMA from 2011-07-08 to 2011-07-11.
A Critical Review of Educational Psychologist Engagement with the Black Community: A Diverse Group Within a Local United Kingdom Community Context
Creators: name: Ajewole, Selone
Publisher: name: School of Psychology, University of East London
Year: 2023

description: A diverse group within a community is described as a collective of individuals that are different from others within that same community (Pickup, 2021). Burnham (2012) highlights that these differences may pertain to factors such as gender, identity, class, sexual orientation or ethnicity. This perception of difference can lead to prejudice by the dominant group. The mere threat of deviation from societal norms can result in the marginalisation of diverse groups whereby they are overtly or covertly dispelled to live on the fringes of society (Pickup, 2021). Such groups often experience reduced functioning and disadvantage compared with the rest of the community (Brind et al., 2008). This paper provides a critical review of educational psychologists’ (EPs’) engagement with the Black community within the United Kingdom (UK); a diverse group within a predominantly White local community Educational Psychology Service (EPS) placement context. Relevant literature, insight into the experiences of the Black community and ways to promote group participation in professional practice are underscored. Critical analysis of factors that lead to underachievement, disaffection and exclusion among this group is also examined. A reflective writing style is incorporated throughout as I critically consider placement practice experiences of engagement with the Black community as a Black thirdyear Trainee Educational Psychologist (TEP) at the University of East London at the time of writing.
title: Natsushima Cruise Report NT11-10 (Leg2)
Creators: name: Usui, Akira
Publisher: name: JAMSTEC
Year: 2011
Subjects: subject: oceans
subject: Cruise report
subject: R/V NATSUSHIMA

description: [CRUISE REPORT] This document is a preliminary report of NT11-10 Leg2 on R/V NATSUSHIMA from 2011-07-02 to 2011-07-07.
title: Natsushima "Cruise Report" NT11-10 Leg1
Creators: name: Iizasa, Kokichi
Publisher: name: JAMSTEC
Year: 2011
Subjects: subject: oceans
subject: Cruise report
subject: R/V NATSUSHIMA

description: [CRUISE REPORT] This document is a preliminary report of NT11-10 Leg1 on R/V NATSUSHIMA from 2011-06-28 to 2011-07-02.
Griffiths effects of the susceptible-infected-susceptible epidemic model on random power-law networks
Creators: name: Cota, Wesley
name: Ferreira, Silvio C.
name: Ódor, Géza
Publisher: name: arXiv
Year: 2015
Subjects: subject: Physics and Society (physics.soc-ph)
subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: We provide numerical evidence for slow dynamics of the susceptible-infected-susceptible model evolving on finite-size random networks with power-law degree distributions. Extensive simulations were done by averaging the activity density over many realizations of networks. We investigated the effects of outliers in both highly fluctuating (natural cutoff) and non-fluctuating (hard cutoff) most connected vertices. Logarithmic and power-law decays in time were found for natural and hard cutoffs, respectively. This happens in extended regions of the control parameter space $λ_1
description: 10 pages, 8 figures
Das Versprechen der Dinge. Aspekte einer kulturwissenschaftlichen Epistemologie
Creators: name: Keller-Drescher, Lioba
Publisher: name: Universität Tübingen
Year: 2010
Subjects: subject: Sachkulturforschung , Sachkultur , Kulturanalyse , Episteme , Materialität
subject: 000
subject: 300
subject: Materielle Kultur
subject: Episteme der Dinge
subject: Theory of Things
subject: Epistemologie der Kulturwissenschaften
subject: Epistemology
subject: Material Culture Studies

description: Thematisiert werden hier die komplexen Zusammenhängen, in die die Dinge in den historischen und gegenwartsbezogenen Kulturwissenschaften verwickelt sind. Auf der Grundlage eingeführter Analysemodelle der Empirischen Kulturwissenschaft, erweitert um Positionen der philosophischen Phänomenologie und der Wissenschaftstheorie, versucht der Beitrag Aspekte einer kulturwissenschaftlichen Epistemologie des Materiellen herauszuarbeiten. Diskutiert wird der Status der Dinge selbst, ihre Rolle im Forschungsprozess, ihre spezifische Geschichtlichkeit und die Bedingungen und Ansprüche einer kulturwissenschaftlichen Analyse des Materiellen.
title: RV Natsushima Cruise Report NT11-09
Creators: name: Inoue, Koji
Publisher: name: JAMSTEC
Year: 2011
Subjects: subject: oceans
subject: Cruise report
subject: R/V NATSUSHIMA

description: [CRUISE REPORT] This document is a preliminary report of NT11-09 on R/V NATSUSHIMA from 2011-06-15 to 2011-06-26.
Arbeiten zur frühen Geschichte der Dominikaner und Franziskaner in England: ...
Creators: name: Pelster, Franz
Publisher: name: Scholastik
Year: 1970

description: Scholastik, Bd. 29 Nr. 3 (1954): Scholastik. Vierteljahresschrift für Theologie und Philosophie, Band 29, Heft 3
Indexical Shifting in Dhaasanac and Somali
Creators: name: Nishiguchi, Sumiyo
Publisher: name: Universität Tübingen
Year: 2017
Subjects: subject: Linguistik , Semantik , Feldforschung , Somali , Dasenech , Afrikanische Sprachen
subject: 400
subject: 490

description: It has been claimed that there are three kinds of Kaplanian monsters selected by dif- ferent attitude verbs in Slave (Anand and Nevins 2004, Anand 2006) as well as in Uyghur (Sudo 2010). This paper shows, on the basis of the collected data, that Dhaasanac has a fourth kind of monster that shifts person and temporal parameters optionally, but does not shift the locative parameter.
title: R/V Natsushima Cruise Report NT11-E02
Creators: name: Ito, Aki
Publisher: name: JAMSTEC
Year: 2011
Subjects: subject: oceans
subject: Cruise report
subject: R/V NATSUSHIMA

description: [CRUISE REPORT] This document is a preliminary report of NT11-E02 on R/V NATSUSHIMA from 2011-06-01 to 2011-06-10.
Combinatorial formulas for arithmetic density
Creators: name: Schneider, Robert
name: Sills, Andrew V.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Number Theory (math.NT)
subject: Combinatorics (math.CO)
subject: FOS: Mathematics

description: Let $d_S$ denote the arithmetic density of a subset $S \subseteq \mathbb N$. We derive a power series in $q\in \mathbb C$, $|q|<1$, with coëfficients related to integer partitions and integer compositions, that yields $1/d_S$ in the limit as $q\to 1$ radially.
description: 5 pages
title: R/V Natsushima Cruise Report NT11-08
Creators: name: Ichihara, Hiroshi
Publisher: name: JAMSTEC
Year: 2011
Subjects: subject: oceans
subject: Cruise report
subject: R/V NATSUSHIMA

description: [CRUISE REPORT] This document is a preliminary report of NT11-08 on R/V NATSUSHIMA from 2011-05-22 to 2011-05-28.
title: CRUISE REPORT NT11-05
Creators: name: Matsumoto, Hiroyuki
Publisher: name: JAMSTEC
Year: 2011
Subjects: subject: oceans
subject: Cruise report
subject: R/V NATSUSHIMA

description: [CRUISE REPORT] This document is a preliminary report of NT11-05 on R/V NATSUSHIMA from 2011-04-21 to 2011-05-04.
Stability analysis of fixed point of fractional-order coupled map lattices
Creators: name: Bhalekar, Sachin
name: Gade, Prashant M.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Dynamical Systems (math.DS)
subject: Chaotic Dynamics (nlin.CD)
subject: FOS: Mathematics
subject: FOS: Physical sciences
subject: 39A30

description: We study the stability of synchronized fixed-point state for linear fractional-order coupled map lattice(CML). We observe that the eigenvalues of the connectivity matrix determine the stability as for integer-order CML. These eigenvalues can be determined exactly in certain cases. We find exact bounds in one-dimensional lattice with translationally invariant coupling using the theory of circulant matrices. This can be extended to any finite dimension. Similar analysis can be carried out for the synchronized fixed point of nonlinear coupled fractional maps where eigenvalues of the Jacobian matrix play the same role. The analysis is generic and demonstrates that the eigenvalues of connectivity matrix play a pivotal role in stability analysis of synchronized fixed point even in coupled fractional maps.
description: 26 pages. 19 figures
Origin of in-plane anisotropic resistivity in the antiferromagnetic phase of Fe$_{1+x}$Te
Creators: name: Kaneshita, Eiji
name: Tohyama, Takami
Publisher: name: arXiv
Year: 2016
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: Motivated by a recent experimental report on in-plane anisotropic resistivity in the double-striped antiferromagnetic phase of FeTe, we theoretically calculate in-plane resistivity by applying a memory function approach to the ordered phase. We find that the resistivity is larger along an antiferromagnetically ordered direction than along a ferromagnetically ordered one, consistent with experimental observation. The anisotropic results are mainly contributed from Drude weight, whose behavior is attributed to Fermi surface topology of the ordered phase.
Non-linear Transport by Bethe Bound States
Creators: name: Urichuk, A.
name: Klümper, A.
name: Sirker, J.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: We consider non-linear ballistic spin transport in the XXZ spin chain and derive an analytical result for the non-linear Drude weight $D^{(3)}$ at infinite temperatures. In contrast to the linear Drude weight $D^{(1)}$, we find that the result not only depends on anisotropy but also on the string length of the quasiparticles transporting the spin current. Our result provides further insights into transport by quasiparticles and raises questions about Luttinger liquid universality.
description: Appendices added
title: NT11-04 R/V Natsushima Cruise Report
Creators: name: Ura, Tamaki
Publisher: name: JAMSTEC
Year: 2011
Subjects: subject: oceans
subject: Cruise report
subject: R/V NATSUSHIMA

description: [CRUISE REPORT] This document is a preliminary report of NT11-04 on R/V NATSUSHIMA from 2011-03-05 to 2011-03-21.
Noise Thresholds for the [[4, 2, 2]]-concatenated Toric Code
Creators: name: Criger, Ben
name: Terhal, Barbara
Publisher: name: arXiv
Year: 2016
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We analyze the properties of a 2D topological code derived by concatenating the [[4, 2, 2]] code with the toric/surface code, or alternatively by removing check operators from the 2D square-octagon or 4.8.8 color code. We show that the resulting code has a circuit-based noise threshold of $\sim 0.41\%$ (compared to $\sim 0.6\%$ for the toric code in a similar scenario), which is higher than any known 2D color code. We believe that the construction may be of interest for hardware in which one wants to use both long-range two-qubit gates as well as short-range gates between small clusters of qubits.
description: 19 pages, 22 figures
Lehmann, Hartmut (Hrsg.), Geschichte des Pietismus
Creators: name: Padberg, Lutz Von
Publisher: name: Jahrbuch für evangelikale Theologie
Year: 2025

description: 1822610826
description: Jahrbuch für evangelikale Theologie, V. 18 (2004): Jahrbuch für evangelikale Theologie, Band 18
Constraining dark energy with Hubble parameter measurements: an analysis including future redshift-drift observations
Creators: name: Guo, Rui-Yun
name: Zhang, Xin
Publisher: name: arXiv
Year: 2015
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Dark energy affects the Hubble expansion rate (namely, the expansion history) $H(z)$ by an integral over $w(z)$. However, the usual observables are the luminosity distances or the angular diameter distances, which measure the distance-redshift relation. Actually, dark energy affects the distances (and the growth factor) by a further integration over functions of $H(z)$. Thus, the direct measurements of the Hubble parameter $H(z)$ at different redshifts are of great importance for constraining the properties of dark energy. In this paper, we show how the typical dark energy models, for example, the $Λ$CDM, $w$CDM, CPL, and holographic dark energy (HDE) models, can be constrained by the current direct measurements of $H(z)$ (31 data in total, covering the redshift range of $z\in [0.07,2.34]$). In fact, the future redshift-drift observations (also referred to as the Sandage-Loeb test) can also directly measure $H(z)$ at higher redshifts, covering the range of $z\in [2,5]$. We thus discuss what role the redshift-drift observations can play in constraining dark energy with the Hubble parameter measurements. We show that the constraints on dark energy can be improved greatly with the $H(z)$ data from only a 10-year observation of redshift drift.
description: 20 pages, 5 figures; final version published in EPJC
Fittkau, G., Der Begriff des Mysteriums bei Johannes Chrysostomus
Creators: name: Stenzel, A.
Publisher: name: Scholastik
Year: 1970

description: Scholastik, Bd. 29 Nr. 3 (1954): Scholastik. Vierteljahresschrift für Theologie und Philosophie, Band 29, Heft 3
Characterizing the aerosol atmosphere above the Observatorio del Roque de los Muchachos by analyzing seven years of data taken with an GaAsP HPD-readout, absolutely calibrated elastic LIDAR
Creators: name: Fruck, Christian
name: Gaug, Markus
name: Hahn, Alexander
name: Acciari, Victor
name: Besenrieder, Jürgen
name: Prester, Dijana Dominis
name: Dorner, Daniela
name: Fink, David
name: Font, Lluís
name: Mićanović, Saša
name: Mirzoyan, Razmik
name: Müller, Dominik
name: Pavletić, Lovro
name: Schmuckermaier, Felix
name: Will, Martin
Publisher: name: arXiv
Year: 2022
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences
subject: J.2.3; J.2.5

description: We present a new elastic LIDAR concept, based on a bi-axially mounted Nd:YAG laser and a telescope with HPD readout, combined with fast FADC signal digitization and offline pulse analysis. The LIDAR return signals have been extensively quality checked and absolutely calibrated. We analyze seven years of quasi-continuous LIDAR data taken during those nights when the MAGIC telescopes were operating. Characterization of the nocturnal ground layer yields zenith and azimuth angle dependent aerosol extinction scale heights for clear nights. We derive aerosol transmission statistics for light emitted from various altitudes throughout the year and separated by seasons. We find further seasonal dependencies of cloud base and top altitudes, but none for the LIDAR ratios of clouds. Finally, the night sky background light is characterized using the LIDAR photon backgrounds. abstract.txt
description: 40 pages, submitted to MNRAS
Kornfeld, W., Studien zum Heiligkeitsgesetz (Lev 17-26)
Creators: name: Haspecker, Josef
Publisher: name: Scholastik
Year: 1970

description: Scholastik, Bd. 29 Nr. 3 (1954): Scholastik. Vierteljahresschrift für Theologie und Philosophie, Band 29, Heft 3
title: Natsushima+Deep Tow DT-4C Cruise Report NT11-02
Creators: name: Takagawa, Shinichi
Publisher: name: JAMSTEC
Year: 2011
Subjects: subject: oceans
subject: Cruise report
subject: R/V NATSUSHIMA

description: [CRUISE REPORT] This document is a preliminary report of NT11-02 on R/V NATSUSHIMA from 2011-01-30 to 2011-02-10.
Rich gauge structures from an unitary approach of some massless gauge fields of spins one and two
Creators: name: Cioroianu, E. M.
Publisher: name: arXiv
Year: 2016
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Considering a bosonic ($1$-)form-valued $k$-form with a second-order Lagrangian dynamics [depending on two arbitrary real constants] we firstly perform the Dirac analysis. The procedure implies a partition of cardinally seven for the plane of the real parameters that label the starting Lagrangian. In each of the seven partition's components one determines the number and the nature of independent degrees of freedom and also a generating set of gauge transformations. Secondly, with the help of some auxiliary gauge/matter tensor gauge fields, in each of the seven situations, we construct the first-order Lagrangian density corresponding to the second-order one.
description: 24 pages
Beumer, J., S. J., Theologie als Glaubensverständnis
Creators: name: Buuck, F.
Publisher: name: Scholastik
Year: 1970

description: Scholastik, Bd. 29 Nr. 3 (1954): Scholastik. Vierteljahresschrift für Theologie und Philosophie, Band 29, Heft 3
Limitations of the background field method applied to Rayleigh-Bénard convection
Creators: name: Nobili, Camilla
name: Otto, Felix
Publisher: name: arXiv
Year: 2016
Subjects: subject: Analysis of PDEs (math.AP)
subject: FOS: Mathematics

description: We consider Rayleigh-Bénard convection as modeled by the Boussinesq equations, in case of infinite Prandtl number. There is a broad interest in bounds of the upwards heat flux, as given by the Nusselt number ${\rm Nu}$, in terms of the forcing via the imposed temperature difference, as given by the Rayleigh number in the turbulent regime ${\rm Ra}\gg 1$. In several works, the background field method applied to the temperature field has been used to provide upper bounds on ${\rm Nu}$ in terms of ${\rm Ra}$. In these applications, the background field method comes in form of a variational problem where one optimizes a stratified temperature profile subject to a certain stability condition; the method is believed to capture marginal stability of the boundary layer. The best available upper bound via this method is ${\rm Nu}$ $\lesssim {\rm Ra}^\frac{1}{3}(\ln {\rm Ra})^\frac{1}{15}$; it proceeds via the construction of a stable temperature background profile that increases logarithmically in the bulk. In this paper, we show that the background temperature field method cannot provide a tighter upper bound in terms of the power of the logarithm. However, by another method one does obtain the tighter upper bound ${\rm Nu}\lesssim {\rm Ra}^\frac{1}{3}(\ln\ln {\rm Ra})^\frac{1}{3}$, so that the result of this paper implies that the background temperature field method is unphysical in the sense that it cannot provide the optimal bound.
description: 54 pages, 5 figures, 25 references
Rensch, B., Neuere Probleme der Abstammungslehre
Creators: name: Haas, Alois
Publisher: name: Scholastik
Year: 1970

description: Scholastik, Bd. 29 Nr. 3 (1954): Scholastik. Vierteljahresschrift für Theologie und Philosophie, Band 29, Heft 3
Direct Collapse to Supermassive Black Hole Seeds: Comparing the AMR and SPH Approaches
Creators: name: Luo, Yang
name: Nagamine, Kentaro
name: Shlosman, Isaac
Publisher: name: arXiv
Year: 2015
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We provide detailed comparison between the AMR code Enzo-2.4 and the SPH/N- body code GADGET-3 in the context of isolated or cosmological direct baryonic collapse within dark matter (DM) halos to form supermassive black holes. Gas flow is examined by following evolution of basic parameters of accretion flows. Both codes show an overall agreement in the general features of the collapse, however, many subtle differences exist. For isolated models, the codes increase their spatial and mass resolutions at different pace, which leads to substantially earlier collapse in SPH than in AMR cases due to higher gravitational resolution in GADGET-3. In cosmological runs, the AMR develops a slightly higher baryonic resolution than SPH during halo growth via cold accretion permeated by mergers. Still, both codes agree in the buildup of DM and baryonic structures. However, with the onset of collapse, this difference in mass and spatial resolution is amplified, so evolution of SPH models begins to lag behind. Such a delay can have effect on formation/destruction rate of H2 due to UV background, and on basic properties of host halos. Finally, isolated non-cosmological models in spinning halos, with spin parameter λ ~ 0.01 - 0.07, show delayed collapse for greater λ, but pace of this increase is faster for AMR. Within our simulation setup, GADGET-3 requires significantly larger computational resources than Enzo- 2.4 during collapse, and needs similar resources, during the pre-collapse, cosmological structure formation phase. Yet it benefits from substantially higher gravitational force and hydrodynamic resolutions, except at the end of collapse.
description: 19 pages, 14 figures, Referees' comments incorporated. Accepted for publication in MNRAS
Binswanger, L., Grundformen und Erkenntnis menschlichen Daseins
Creators: name: Gilen, Leonhard
Publisher: name: Scholastik
Year: 1970

description: Scholastik, Bd. 29 Nr. 3 (1954): Scholastik. Vierteljahresschrift für Theologie und Philosophie, Band 29, Heft 3
title: R/V Natsushima Cruise Report NT11-01
Creators: name: Kamiya, Shinichiro
Publisher: name: JAMSTEC
Year: 2011
Subjects: subject: oceans
subject: Cruise report
subject: R/V NATSUSHIMA

description: [CRUISE REPORT] This document is a preliminary report of NT11-01 on R/V NATSUSHIMA from 2011-01-04 to 2011-01-22.
title: R/V Mirai Cruise Report MR11-08
Creators: name: Kumamoto, Yuichiro
name: Murata, Akihiko
Publisher: name: JAMSTEC
Year: 2012
Subjects: subject: oceans
subject: Cruise report
subject: R/V MIRAI

description: [CRUISE REPORT] This document is a preliminary report of MR11-08 Leg1 on R/V MIRAI from 2011-12-04 to 2011-12-20, MR11-08 Leg2 on R/V MIRAI from 2011-12-20 to 2012-01-12 and MR11-08 Leg3 on R/V MIRAI from 2012-01-12 to 2012-02-09.