cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
COSMIC MIND AND CREATIVITY
Creators: name: καρπούζος,
Publisher: name: figshare
Year: 2020
Subjects: subject: Anthropology
subject: FOS: Sociology
subject: 130103 Higher Education
subject: FOS: Educational sciences
subject: Sociology

description: We live in a universe that can be seen and experienced from many different perspectives. We therefore need to look at the universe from many different angles. Everything and everyone is a form of the universe being expressed in a particular way. In other words, each one of us can say with absolute certainly "We are the Universe!" Since we are the universe, each one of us provides a valuable perspective that complements the contributions of everyone and everything else around us.Each of us is the universe being expressed in a particular location in a specific way. We're all part of the same moving and evolving cosmos, but the view of it is unique from each of our respective locations. This suggests that the universe is not only omnicentric, but that it is also multiperspectival-there are many different, and equally valid, viewpoints on this. Each one of us is a cosmic laboratory within which we can discover the secrets of the universe.We speak in various ways, we are each the universe having become aware of itself in our own unique way. The insights that the universe has many different perspectives and is both cosmic and personal has great transformative potential, and is worth reflecting on deeply. Creativity and Modern Science Creativity and Theory of relativity In Einstein's theory of relativity, the notions of events (space and time simultaneity), mass and energy equivalence (special relativity), space expansion (big bang) as well as space and energy-mass equivalence, are introduced. General theory of relativity combined to quantum mechanics leads to the emergence of the whole universe from zero and absolute nothingness. Such "emergence-creation" of the universe from zero does not take place in space or time, since both are identical to the universe, space as energy expansion of the vacant space and time as a measurement unit of movement and change. Hence, the event, as "something" that takes place, and since it takes place, creates space, time and matter-mass-energy,
Runaway and walkaway stars from the ONC with Gaia DR2
Creators: name: Schoettler, Christina
name: de Bruijne, Jos
name: Vaher, Eero
name: Parker, Richard J.
Publisher: name: arXiv
Year: 2020
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Theory predicts that we should find fast, ejected (runaway) stars of all masses around dense, young star-forming regions. $N$-body simulations show that the number and distribution of these ejected stars could be used to constrain the initial spatial and kinematic substructure of the regions. We search for runaway and slower walkaway stars within 100 pc of the Orion Nebula Cluster (ONC) using $Gaia$ DR2 astrometry and photometry. We compare our findings to predictions for the number and velocity distributions of runaway stars from simulations that we run for 4 Myr with initial conditions tailored to the ONC. In $Gaia$ DR2, we find 31 runaway and 54 walkaway candidates based on proper motion, but not all of these are viable candidates in three dimensions. About 40 per cent are missing radial velocities, but we can trace back 9 3D-runaways and 24 3D-walkaways to the ONC, all of which are low/intermediate-mass (<8 M$_{\odot}$). Our simulations show that the number of runaways within 100 pc decreases the older a region is (as they quickly travel beyond this boundary), whereas the number of walkaways increases up to 3 Myr. We find fewer walkaways in $Gaia$ DR2 than the maximum suggested from our simulations, which may be due to observational incompleteness. However, the number of $Gaia$ DR2 runaways agrees with the number from our simulations during an age of $\sim$1.3-2.4 Myr, allowing us to confirm existing age estimates for the ONC (and potentially other star-forming regions) using runaway stars.
description: 19 pages, 7 figures, accepted for publication in MNRAS
Food Consumption Highlights
Creators: name: Rogers, Anne
name: Rogers, Anne
Publisher: name: Unknown
Year: 1984
Subjects: Food Consumption/Nutrition/Food Safety

description: Per capita food consumption dropped 7 pounds in 1982 to an average of 1,387 pounds, reflecting a decline in animal product use of 9 pounds from 1981. Reductions in pork, eggs, and dairy products offset increased poultry consumption. We consumed almost 2 pounds more of crop products per person, with increases in vegetables and potatoes offsetting decreases in cereal and bakery items, sugar and sweeteners, and fruits and melons.
Two-dimensional PIC-MCC simulations of capacitively coupled radio-frequency discharge in methane
Creators: name: Alexandrov, A L
name: Schweigert, I V
Publisher: name: arXiv
Year: 2004
Subjects: subject: Plasma Physics (physics.plasm-ph)
subject: FOS: Physical sciences

description: Two-dimensional capacitively coupled radio frequency discharge in methane is simulated by PIC-MCC method. The results were obtained in pressure range 50-300 mTorr and voltage range 40-180 V for discharge frequency 13.56 MHz. The electron energy and electron--methane reaction rates spatial distributions show existence of two regimes of discharge glow: a) with active sheaths, when electrons are hot in electrode sheaths and cold in the middle of discharge so the electron-neutral reactions strongly dominate in sheaths regions; b) with volume domination, when the electron energy is more uniform and the reactions take place in all discharge volume. The second regime is usually observed for low discharge voltages, and turns to the first one with voltage increasing. Besides, simulation of chemical reactions in methane plasma was also fulfilled to find the gas mixture composition in discharge volume. The results are in agreement with the known experimental data.
description: 24 pages, 11 figures submitted to Plasma Sourses Science and Technology in May, 2004
Recurrent fourth-order interference dips and peaks with a comb-like two-photon entangled state
Creators: name: Zavatta, Alessandro
name: Viciani, Silvia
name: Bellini, Marco
Publisher: name: arXiv
Year: 2003
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We demonstrate full selective control over the constructive or destructive character of fourth-order recurring interferences in a modified version of a HOM interferometer using comb-like two-photon states. The comb spectral/temporal structure is obtained by inserting an etalon cavity in the signal path of an entangled photon pair obtained by pulsed spontaneous parametric down-conversion. Both a simple qualitative discussion and a complete theoretical derivation are used to explain and analyze the experimental data.
description: 4 pages, 4 figures. Revised version, to appear in Physical Review A
Generalized Kinetic Theory of Electrons and Phonons: Models, Equilibrium, Stability
Creators: name: Rossani, A.
name: Scarfone, A. M.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: In the present paper our aim is to introduce some models for the generalization of the kinetic theory of electrons and phonons (KTEP), as well as to study equilibrium solutions and their stability for the generalized KTEP (GKTEP) equations. We consider a couple of models, relevant to non standard quantum statistics, which give rise to inverse power law decays of the distribution function with respect to energy. In the case of electrons in a phonon background, equilibrium and stability are investigated by means of Lyapounov theory. Connections with thermodynamics are pointed out.
description: 10 pages, 2 figures, (RevTeX4), to appear in Physica B (2003)
Rotational and pulsational variability in the TESS light curve of HD27463
Creators: name: Khalack, V.
name: Lovekin, C.
name: Bowman, D. M.
name: Kobzar, O.
name: David-Uraz, A.
name: Paunzen, E.
name: Sikora, J.
name: Lenz, P.
name: Kochukhov, O.
name: Holdsworth, D. L.
name: Wade, G. A.
Publisher: name: arXiv
Year: 2019
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: The new photometric data on pulsating Ap star HD~27463 obtained recently with the Transiting Exoplanet Survey Satellite (\textit{TESS}) are analysed to search for variability. Our analysis shows that HD~27463 exhibits two types of photometric variability. The low frequency variability with the period $P$ =~2.834274 $\pm$ 0.000008 d can be explained in terms of axial stellar rotation assuming the oblique magnetic rotator model and presence of surface abundance/brightness spots, while the detected high-frequency variations are characteristics of $δ$~Scuti pulsations. From the analysis of Balmer line profiles visible in two FEROS spectra of HD~27463 we have derived its effective temperature and surface gravity, finding values that are close to those published for this star in the \textit{TESS} Input Catalogue (TIC). Knowing the rotation period and the v$\sin{i}$ value estimated from the fitting of Balmer line profiles we found that the rotational axis is inclined to the line of sight with an angle of $i=33\pm8°$. Our best-fitting model of the observed pulsation modes results in an overshoot parameter value $f_{ov} = 0.014$ and values of global stellar parameters that are in good agreement with the data reported in the TIC and with the data derived from fitting Balmer line profiles. This model indicates an age of 5.0 $\pm$~0.4 $\times 10^8$~yrs, which corresponds to a core hydrogen fraction of 0.33.
description: 9 pages, 12 figures
Low mass AGB stellar models for 0.003 < Z < 0.02: basic formulae for nucleosynthesis calculations
Creators: name: Straniero, Oscar
name: Dominguez, Inma
name: Cristallo, Sergio
name: Gallino, Roberto
Publisher: name: arXiv
Year: 2003
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We have extended our published set of low mass AGB stellar models to lower metallicity. Different mass loss rates have been explored. Interpolation formulae for luminosity, effective temperature, core mass, mass of dredge up material and maximum temperature in the convective zone generated by thermal pulses are provided. Finally, we discuss the modifications of these quantities as obtained when an appropriate treatment of the inward propagation of the convective instability, caused by the steep rise of the radiative opacity occurring when the convective envelope penetrates the H-depleted region, is taken into account.
description: 11 pages, 4 figures, accepted for publication in Publications of the Astronomical Society of Australia (PASA)
High-Resolution Spectral Discriminants of Ocean Loss for M Dwarf Terrestrial Exoplanets
Creators: name: Leung, Michaela
name: Meadows, Victoria S.
name: Lustig-Yaeger, Jacob
Publisher: name: arXiv
Year: 2020
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: In the near future, extremely-large ground-based telescopes may conduct some of the first searches for life beyond the solar system. High-spectral resolution observations of reflected light from nearby exoplanetary atmospheres could be used to search for the biosignature oxygen. However, while Earth's abundant O$_2$is photosynthetic, early ocean loss may also produce high atmospheric O$_2$ via water vapor photolysis and subsequent hydrogen escape. To explore how to use spectra to discriminate between these two oxygen sources, we generate high-resolution line-by-line synthetic spectra of both a habitable Earth-like, and post-ocean-loss Proxima Centauri b. We examine the strength and profile of four bands of O$_2$ from 0.63 to 1.27 $μ$m, and quantify their relative detectability. We find that 10 bar O$_2$ post-ocean-loss atmospheres have strong suppression of oxygen bands, and especially the 1.27$μ$m band. This suppression is due to additional strong, broad O$_2$-O$_2$ collisionally-induced absorption (CIA) generated in these more massive O$_2$atmospheres, which is not present for the smaller amounts of oxygen generated by photosynthesis. Consequently, any detection of the 1.27$μ$m band in reflected light indicates lower Earth-like O$_2$ levels, which suggests a likely photosynthetic origin. However, the 0.69 $μ$m O$_2$ band is relatively unaffected by O$_2$-O$_2$ CIA, and the presence of an ocean-loss high-O$_2$ atmosphere could be inferred via detection of a strong 0.69 $μ$m O$_2$ band, and a weaker or undetected 1.27 $μ$m band. These results provide a strategy for observing and interpreting O$_2$ in exoplanet atmospheres, that could be considered by future ground-based telescopes.
description: 14 pages, 11 figures
Geometric phase shift for detection of gravitational radiation
Creators: name: Mitskievich, N V
name: Nesterov, A I
Publisher: name: arXiv
Year: 2004
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Theory (hep-th)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: An effect of geometrical phase shift is predicted for a light beam propagating in the field of a gravitational wave. Gravitational radiation detection experiments are proposed using this new effect, the corresponding estimates being given.
description: LaTeX2e, 12 pp
Space-time analysis of reaction at RHIC
Creators: name: Retiere, F.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: Space-time information about the Au-Au collisions produced at RHIC are key tools to understand the evolution of the system and especially assess the presence of collective behaviors. Using a parameterization of the system's final state relying on collective expansion, we show that pion source radii can be tied together with transverse mass spectra and elliptic flow within the same framework. The consistency between these different measures provide a solid ground to understand the characteristics of collective flow and especially the possible peculiar behavior of particles such as Xi, Omega or phi. The validity of the short time scales that are extracted from fits to the pion source size is also addressed. The wealth of new data that will soon be available from Au-Au collisions at sqrt{s_{NN}} = 200 GeV, will provide a stringet test of the space-time analysis framework developped in these proceedings.
description: Invited talk given at the SQM2003 conference (March 2003), to be published in Journal of Physics G. 10 pages, 3 figures
The Effect of the LISA Response Function on Observations of Monochromatic Sources
Creators: name: Vecchio, A.
name: Wickham, E. D. L.
Publisher: name: arXiv
Year: 2004
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: The Laser Interferometer Space Antenna (LISA) is expected to provide the largest observational sample of binary systems of faint sub-solar mass compact objects, in particular white-dwarfs, whose radiation is monochromatic over most of the LISA observational window. Current astrophysical estimates suggest that the instrument will be able to resolve about 10000 such systems, with a large fraction of them at frequencies above 3 mHz, where the wavelength of gravitational waves becomes comparable to or shorter than the LISA arm-length. This affects the structure of the so-called LISA transfer function which cannot be treated as constant in this frequency range: it introduces characteristic phase and amplitude modulations that depend on the source location in the sky and the emission frequency. Here we investigate the effect of the LISA transfer function on detection and parameter estimation for monochromatic sources. For signal detection we show that filters constructed by approximating the transfer function as a constant (long wavelength approximation) introduce a negligible loss of signal-to-noise ratio -- the fitting factor always exceeds 0.97 -- for f below 10mHz, therefore in a frequency range where one would actually expect the approximation to fail. For parameter estimation, we conclude that in the range 3mHz to 30mHz the errors associated with parameter measurements differ from about 5% up to a factor of 10 (depending on the actual source parameters and emission frequency) with respect to those computed using the long wavelength approximation.
description: replacement version with typos corrected
Stacking Order in Graphite Films Controlled by Van der Waals Technology
Creators: name: Yang, Yaping
name: Zou, Yi-Chao
name: Woods, Colin R.
name: Shi, Yanmeng
name: Yin, Jun
name: Xu, Shuigang
name: Ozdemir, Servet
name: Taniguchi, Takashi
name: Watanabe, Kenji
name: Geim, Andre K.
name: Novoselov, Kostya S.
name: Haigh, Sarah J.
name: Mishchenko, Artem
Publisher: name: arXiv
Year: 2019
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: In graphite crystals, layers of graphene reside in three equivalent, but distinct, stacking positions typically referred to as A, B, and C projections. The order in which the layers are stacked defines the electronic structure of the crystal, providing an exciting degree of freedom which can be exploited for designing graphitic materials with unusual properties including predicted high-temperature superconductivity and ferromagnetism. However, the lack of control of the stacking sequence limits most research to the stable ABA form of graphite. Here we demonstrate a strategy to control the stacking order using van der Waals technology. To this end, we first visualise the distribution of stacking domains in graphite films and then perform directional encapsulation of ABC-rich graphite crystallites with hexagonal boron nitride (hBN). We found that hBN-encapsulation which is introduced parallel to the graphite zigzag edges preserves ABC stacking, while encapsulation along the armchair edges transforms the stacking to ABA. The technique presented here should facilitate new research on the important properties of ABC graphite.
Astrophysical Insights into Radial Velocity Jitter from an Analysis of 600 Planet-search Stars
Creators: name: Luhn, Jacob K.
name: Wright, Jason T.
name: Howard, Andrew W.
name: Isaacson, Howard
Publisher: name: arXiv
Year: 2020
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Radial velocity (RV) detection of planets is hampered by astrophysical processes on the surfaces of stars that induce a stochastic signal, or "jitter", which can drown out or even mimic planetary signals. Here, we empirically and carefully measure the RV jitter of more than 600 stars from the California Planet Search (CPS) sample on a star-by-star basis. As part of this process we explore the activity-RV correlation of stellar cycles and include appendices listing every ostensibly companion-induced signal we removed and every activity cycle we noted. We then use precise stellar properties from Brewer et al. (2017) to separate the sample into bins of stellar mass and examine trends with activity and with evolutionary state. We find RV jitter tracks stellar evolution and that in general, stars evolve through different stages of RV jitter: the jitter in younger stars is driven by magnetic activity, while the jitter in older stars is convectively-driven and dominated by granulation and oscillations. We identify the "jitter minimum" -- where activity-driven and convectively-driven jitter have similar amplitudes -- for stars between 0.7 and 1.7 $M_{\odot}$ and find that more massive stars reach this jitter minimum later in their lifetime, in the subgiant or even giant phases. Finally, we comment on how these results can inform future radial velocity efforts, from prioritization of follow-up targets from transit surveys like TESS to target selection of future RV surveys.
description: 44 pages, 11 figures, published in The Astronomical Journal
Cloud futures for CMIP data – Evaluating object storage models and re-evaluating federation for data distribution
Creators: name: Stephens, Ag
name: Kershaw, Philip
name: Iwi, Alan
name: Jones, Matthew
name: Lawrence, Bryan
name: Massey, Neil
name: Petrie, Ruth
name: Pryor, Matt
name: Smith, Eleanor
Publisher: name: Zenodo
Year: 2020

description: Presented at AGU Fall Meeting 2020, Session IN032-02.
Mimicking Time Evolution within a Quantum Ground State: Ground-State Quantum Computation, Cloning, and Teleportation
Creators: name: Mizel, Ari
Publisher: name: arXiv
Year: 2003
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Ground-state quantum computers mimic quantum mechanical time evolution within the amplitudes of a time-independent quantum state. We explore the principles that constrain this mimicking. A no-cloning argument is found to impose strong restrictions. It is shown, however, that there is flexibility that can be exploited using quantum teleportation methods to improve ground-state quantum computer design.
description: 10 pages, 7 figures
Reporte de Lectura: “El método científico y la nueva Filosofía de la Ciencia” y rescatar el planteamiento que hace el autor sobre la relación del método científico con el nuevo enfoque filosófico de la ciencia.
Creators: name: TIMANA, EDGAR ALFREDO MONTANO
Publisher: name: figshare
Year: 2020
Subjects: Education

description: Reporte de Lectura: Leer el texto “El método científico y la nueva Filosofía de la Ciencia” y rescatar el planteamiento que hace el autor sobre la relación del método científico con el nuevo enfoque filosófico de la ciencia.
Spin Effects in a Quantum Ring
Creators: name: Ihn, T.
name: Fuhrer, A.
name: Ensslin, K.
name: Bichler, M.
name: Wegscheider, W.
Publisher: name: arXiv
Year: 2004
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: Recent experiments are reviewed that explore the spin states of a ring-shaped many-electron quantum dot. Coulomb-blockade spectroscopy is used to access the spin degree of freedom. The Zeeman effect observed for states with successive electron number allows to select possible sequences of spin ground states of the ring. Spin-paired orbital levels can be identified by probing their response to magnetic fields normal to the plane of the ring and electric fields caused by suitable gate voltages. This narrows down the choice of ground-state spin sequences. A gate-controlled singlet--triplet transition is identified and the size of the exchange interaction matrix element is determined.
description: 13 pages, 3 figures, Proceedings of the QD2004 conference in Banff
Additional file 1 of Patient-derived xenograft models capture genomic heterogeneity in endometrial cancer
Creators: name: Bonazzi, Vanessa F.
name: Kondrashova, Olga
name: Smith, Deborah
name: Nones, Katia
name: Sengal, Asmerom T.
name: Ju, Robert
name: Packer, Leisl M.
name: Koufariotis, Lambros T.
name: Kazakoff, Stephen H.
name: Davidson, Aimee L.
name: Ramarao-Milne, Priya
name: Lakis, Vanessa
name: Newell, Felicity
name: Rogers, Rebecca
name: Davies, Claire
name: Nicklin, James
name: Garrett, Andrea
name: Chetty, Naven
name: Perrin, Lewis
name: Pearson, John V.
name: Patch, Ann-Marie
name: Waddell, Nicola
name: Pollock, Pamela M.
Publisher: name: figshare
Year: 2022
Subjects: subject: Biochemistry
subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Cancer

description: Additional file 1: Supplementary Methods, Supplementary Tables 1-3,5 and Supplementary Figures.
2020 MÜNİH GÜVENLİK KONFERANSI "YAPICI AVRASYACILIĞIN" GEREKLİLİĞİNİ ORTAYA KOYUYOR
Creators: name: Tulun, Teoman Ertuğrul
Publisher: name: figshare
Year: 2020
Subjects: subject: 160607 International Relations
subject: FOS: Political science

description: Münih Güvenlik Konferansı (MSC), 1963'ten beri Münih'te uluslararası güvenlik politikası konusunda düzenlenen yıllık bir konferanstır. MSC başkanlar, başbakanlar, dışişleri ve savunma bakanları, askeri liderler arasında uluslararası güvenlik politikası konusunda gayrı resmi bir ortamda görüş alışverişinde bulunulmasına yönelik en önemli resmi olmayan forumlardan biridir. Bu yılki konferans, siyaset dünyasından, uluslararası örgütlerden, iş dünyası ve sivil toplumdan yüzlerce üst düzey liderin ve düşünürün katılımıyla 14-16 Şubat tarihleri arasında yapılmıştır.
RAQAMLI TEXNOLOGIYALAR ELEMENTI: MOBIL ILOVANING, ILM FAN TARAQQIYOTI RIVOJIGA TA'SIRI VA SAMARASI
Creators: name: Pazilova, Dilnoza X.
Publisher: name: Zenodo
Year: 2025

description: Ushbu ilmiy maqolada raqamli texnologiyalar elementi sifatida mobil ilova olingan. Bunda xozirgi kun messengerlaridan Telegram ilovasida talabalarning mutaxasislik fanidan biri Web dasturlashga kirish fanidan talabalarni baholash haqida ilmiy qarashlar zamonaviy ta’lim ped texnologiyalaridan Vizual dasturlash metodi asosida dastur tuzishning sodda va tushunarli usuli va messenger orqali baholash usulidan misol keltirilgan. Bu usul natijasi diagramma ko’rinishidagi statistik tahlilini ko’rish mumkin
Adiabatic landscape and optimal paths in ergodic systems
Creators: name: Sugiura, Sho
name: Claeys, Pieter W.
name: Dymarsky, Anatoly
name: Polkovnikov, Anatoli
Publisher: name: arXiv
Year: 2020
Subjects: subject: Quantum Physics (quant-ph)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Whether one is interested in quantum state preparation or in the design of efficient heat engines, adiabatic (reversible) transformations play a pivotal role in minimizing computational complexity and energy losses. Understanding the structure of these transformations and identifying the systems for which such transformations can be performed efficiently and quickly is therefore of primary importance. In this paper we focus on finding optimal paths in the space of couplings controlling the system's Hamiltonian. More specifically, starting from a local Hamiltonian we analyze directions in the space of couplings along which adiabatic transformations can be accurately generated by local operators, which are both realizable in experiments and easy to simulate numerically. We consider a non-integrable 1D Ising model parametrized by two independent couplings, corresponding to longitudinal and transverse magnetic fields. We find regions in the space of couplings characterized by a very strong anisotropy of the variational adiabatic gauge potential (AGP), generating the adiabatic transformations, which allows us to define optimal adiabatic paths. We find that these paths generally terminate at singular points characterized by extensive degeneracies in the energy spectrum, splitting the parameter space into adiabatically disconnected regions. The anisotropy follows from singularities in the AGP, and we identify special robust weakly-thermalizing and non-absorbing many-body "dark" states which are annihilated by the singular part of the AGP and show that their existence extends deep into the ergodic regime.
description: 23 pages, 13 figures
Additional file 4 of A clinical decision support system improves antibiotic therapy for upper urinary tract infection in a randomized single-blinded study
Creators: name: M. Neugebauer
name: M. Ebert
name: R. Vogelmann
Publisher: name: figshare
Year: 2020
Subjects: subject: Space Science
subject: Medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Developmental Biology
subject: Computational Biology

description: Additional file 4: Figure S4. Questionnaire Part 1 â€“ case description.
Additional file 2 of Development of the Inner City attitudinal assessment tool (ICAAT) for learners across Health care professions
Creators: name: McKinney, Mark
name: Smith, Katherine
name: Dong, Kathryn
name: Babenko, Oksana
name: Ross, Shelley
name: Kelly, Martina
name: Salvalaggio, Ginetta
Publisher: name: figshare
Year: 2020
Subjects: subject: Medicine
subject: Molecular Biology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Developmental Biology
subject: Science Policy
subject: Computational Biology

description: Additional file 2. List of tools selected for preliminary item generation.
Additional file 1 of Upper crustal shear-wave velocity structure Beneath Western Java, Indonesia from seismic ambient noise tomography
Creators: name: Rosalia, Shindy
name: Widiyantoro, Sri
name: Cummins, Phil R.
name: Yudistira, Tedi
name: Nugraha, Andri Dian
name: Zulfakriza, Zulfakriza
name: Setiawan, Ahmad
Publisher: name: figshare
Year: 2022
Subjects: subject: Geology
subject: FOS: Earth and related environmental sciences
subject: Geophysics

description: Additional file 1: Figure S1. A–c) Examples of 1D P-wave velocity profile inverted using dinver package of Geopsy at points 1, 2, 3 shown in Figure 3, respectively. The red line in the 1D velocity model shows the optimum velocity model. The black to gray lines represent the generated ensemble models with their corresponding misfit values. Figure S2. The distribution of the ensemble models generated at point 3 (longitude 107.8o and latitude 7.2o) at depth 2–20 km. The red dashed line is the mean value of the ensemble.
Generics Revisited
Creators: name: Seigle, Naaman
name: Seigle, Naaman
Publisher: name: Unknown
Year: 1979
Subjects: Food Consumption/Nutrition/Food Safety

description: In the year since this topic was last covered in the National Food Review generic labels have become big business. I Today, approximately 125 grocery firms sell generic labeled items in about 11,000 stores. These stores sell from I to over 150 food and nonfood generic labeled items. The nonfood items have been more popular than food items. Recent interviews with representatives of grocery firms found divergent views on proportionate sales of generic labels. About half of those interviewed stated that generic products were increasing in sales; others said that sales of such products have reached a plateau. This article investigates the reasons for the apparent differences in views.
Betreuung im Alter : Herausforderungen und Lösungsansätze
Creators: name: Derrer, Roxane
name: Laube, Ramona
Publisher: name: ZHAW Zürcher Hochschule für Angewandte Wissenschaften
Year: 2024
Subjects: 305: Personengruppen (Alter, Herkunft, Geschlecht, Einkommen)
361: Sozialarbeit und Sozialhilfe

description: Diese Masterarbeit untersucht die Herausforderungen und Lösungsansätze bei der Reintegration älterer Menschen mit begrenzten finanziellen Ressourcen in ihr häusliches Umfeld nach einem Spitalaufenthalt. Der Fokus liegt auf der Rolle der Spitalsozialarbeit als Schnittstelle zwischen medizinischer Versorgung und sozialer Umwelt. Die Arbeit analysiert spezifische Hürden im Bereich Betreuung, evaluiert bestehende Projekte zur Förderung des autonomen Wohnens und entwickelt Strategien für eine erfolgreiche Unterstützung durch die Spitalsozialarbeit. Mittels umfassender Literaturrecherche und Analyse aktueller politischer Bestrebungen werden konkrete Handlungsempfehlungen erarbeitet. Die Ergebnisse zeigen die Komplexität der Thematik auf, insbesondere hinsichtlich der Finanzierung von Betreuungsleistungen und des Nichtbezugs von Sozialversicherungsleistungen. Bestehende Projekte in verschiedenen Kantonen bieten vielversprechende Ansätze, bedürfen jedoch weiterer Evaluation und Anpassung. Diese Erkenntnisse unterstreichen die Notwendigkeit einer ganzheitlichen Betrachtung der Problematik und die zentrale Bedeutung der Spitalsozialarbeit in der Bewältigung der demografischen Herausforderungen. Sie bieten eine Grundlage für die Weiterentwicklung von Unterstützungsangeboten und politischen Massnahmen zur Förderung der Autonomie im Alter.
Analytical System with Decision Tree for Economic Benefit
Creators: name: Tyrychtr, J.
name: Tyrychtr, J.
Publisher: name: Unknown
Year: 2017
Subjects: subject: Agricultural Finance
subject: Analytical system
subject: decision tree
subject: decision rules
subject: economic value
subject: agriculture

description: Data processing is an important aspect of business decision support systems (DSS). A good analytical system to process these data is essential to implement as a primary pillar for the development of complex expert systems. Businesses themselves are constantly confronted with deciding on investment opportunities to improve their performance. An important criterion for selecting investment is its profitability which cannot be easily determined when investing in analytical systems. Currently, there are two types of approaches to evaluating investments into information systems: normative and positive approaches. The simplest form of decisional analytical modeling is the decision tree (normative approach). The purpose of the article is to illustrate decision tree analysis as a component of an analytical system for evaluating two decision alternatives. The test case is demonstrated on an example of decision-making in agriculture.
Additional file 1 of Healthcare institutions’ recommendation regarding the use of FFP-2 masks and SARS-CoV-2 seropositivity among healthcare workers: a multicenter longitudinal cohort study
Creators: name: Szajek, Katarzyna
name: Fleisch, Felix
name: Hutter, Sandra
name: Risch, Martin
name: Bechmann, Theresa
name: Luyckx, Valerie A.
name: Güsewell, Sabine
name: Hirzel, Cédric
name: Cusini, Alexia
name: Group, AMICO Study
Publisher: name: figshare
Year: 2022
Subjects: subject: Medicine
subject: Biotechnology
subject: Cancer
subject: 111714 Mental Health
subject: FOS: Health sciences
subject: 110309 Infectious Diseases
subject: 60506 Virology
subject: FOS: Biological sciences
subject: Computational Biology

description: Additional file 1. Supplementary Data.
Correlation lengths and scaling functions in the three-dimensional O(4) model
Creators: name: Engels, J.
name: Fromme, L.
name: Seniuch, M.
Publisher: name: arXiv
Year: 2003
Subjects: subject: High Energy Physics - Lattice (hep-lat)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: We investigate numerically the transverse and longitudinal correlation lengths of the three-dimensional O(4) model as a function of the external field H. From our data we calculate the scaling function of the transverse correlation length, and that of the longitudinal correlation length for T>T_c. We show that the scaling functions do not only describe the critical behaviours of the correlation lengths but encompass as well the predicted Goldstone effects, in particular the H^{-1/2}-dependence of the transverse correlation length for T
description: 24 pages, 13Ps-figures, Latex2e,one page added,version to appear in Nucl. Phys. B[FS]
Selected Aspects of the Internalisation Process of the Czech Agricultural SMEs with Focus on the Success Factors
Creators: name: Tuzova, Marcela
name: Toulova, Martina
name: Kubickova, Lea
name: Tuzova, Marcela
name: Toulova, Martina
name: Kubickova, Lea
Publisher: name: Unknown
Year: 2016
Subjects: subject: Agricultural and Food Policy
subject: International Development
subject: Marketing
subject: FOS: Economics and business
subject: internationalisation
subject: small- and medium-sized enterprises
subject: agriculture
subject: success factors
subject: networks

description: Enterprises from all over the world face the pressure of strengthening international competition because of the globalisation of markets. Therefore, enterprises should react promptly to all these changes. One of the ways how enterprises can sustain their competitiveness or achieve further growth is their involvement in internationalisation, which means their foreign expansion. This paper deals with agricultural enterprises which also try to look for new ways how to sell their production even beyond the national borders, it means that they try to internationalise. There are a lot of factors which can influence the success of enterprises in foreign markets. What factors can contribute to the success of agricultural enterprises in foreign trade operations? It is the main question addressed in this paper.
Comparison of Agricultural Costs Prediction Approaches
Creators: name: Hloušková, Z.
name: Ženíšková, P.
name: Prášilová, M.
name: Hloušková, Z.
name: Ženíšková, P.
name: Prášilová, M.
Publisher: name: Unknown
Year: 2018
Subjects: subject: Agricultural Finance
subject: Research Methods/ Statistical Methods
subject: Time series analysis
subject: exponential smoothing
subject: ARIMA models
subject: cost inputs in agriculture
subject: Farm Accountancy Data Network (FADN)

description: The paper submitted offers an assessment and comparison of three approaches to agricultural cost inputs short-term forecasting, that have been proposed as possible alternatives to tackle the problem. The data applied have been taken from the Czech Statistical Office and the Farm Accountancy Data Network data sources. The forecasts were prepared using time series analyses based on methods of exponential smoothing and Box-Jenkins methodology of autoregressive integrated process moving averages. The proposed change index numbers for the 2012, 2013 and 2014 years from three approaches were confronted with the real development of costs time series as it was found in the statistical FADN survey results. The main conclusion drawn pointed out that, for the purpose of economic income estimation based on the FADN database, the cost prediction approach based on the same database, i.e., on time series analysis of the FADN panel data, is the most applicable one. However, it is recommended, too, to use other approaches for crops protection products cost and labour cost development.
Additional file 1 of Combined driving: task-specific position impacts grip strength of equestrian athletes
Creators: name: Keener, Michaela M.
name: Tumlin, Kimberly I.
name: Heebner, Nicholas R.
Publisher: name: figshare
Year: 2022
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: FOS: Biological sciences
subject: Cancer

description: Additional file 1.
Gamma-ray Emission Properties from Mature Pulsars in the Galaxy and in the Gould Belt
Creators: name: Cheng, K. S.
name: Zhang, L.
name: Leung, P.
name: Jiang, Z. J.
Publisher: name: arXiv
Year: 2004
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We study the $γ$-ray emission properties of pulsars by using a new self-consistent outer gap model. The outer gap can exist in pulsars with age over million years old if the effect of magnetic inclination angle as well as the average properties of the outer gap are considered. The mature $γ$-ray pulsars, whose ages are between 0.3 to 3 million years old, are able to move up to high galactic latitude. Moreover, their $γ$-ray luminosity are weaker and their spectra are softer than those of younger $γ$-ray pulsars in the galactic plane significantly. We use a Monte Carlo method to simulate the statistical properties of $γ$-ray pulsars in the Galaxy as well as in the Gould Belt. We find that $γ$-ray pulsars located at $\mid b \mid < 5^{\circ}$ and located at $\mid b \mid > 5^{\circ}$ have very different properties. High galactic latitude $γ$-ray pulsars are dominated by mature pulsars with longer periods, weaker fluxes and softer spectra. If the pulsar birth rate in the Galaxy and the Gould Belt are $\sim 10^{-2}yr^{-1}$ and $\sim 2\times 10^{-5}yr^{-1}$ respectively, there are 42 and 35 radio-quiet $γ$-ray pulsars for $\mid b \mid < 5^{\circ}$ and $\mid b \mid > 5^{\circ}$ respectively. Radio-quiet $γ$-ray pulsars from the Gould Belt are 2 and 13 for $\mid b \mid < 5^{\circ}$ and $\mid b \mid > 5^{\circ}$ respectively. We suggest that a good fraction of unidentified EGRET $γ$-ray sources may be these radio-quiet $γ$-ray pulsars. Furthermore $γ$-ray pulsars located at $\mid b \mid > 5^{\circ}$ satisfies $L_γ \propto L^β_{sd}$ whereas $L_γ \propto L^δ_{sd}$ for $γ$-ray pulsars in the galactic plane, where $β\sim 0.6$ and $δ\sim 0.3$ respectively.
description: 24 pages, 21 figures, accepted to be published in ApJ
Additional file 1 of Development of the Inner City attitudinal assessment tool (ICAAT) for learners across Health care professions
Creators: name: McKinney, Mark
name: Smith, Katherine
name: Dong, Kathryn
name: Babenko, Oksana
name: Ross, Shelley
name: Kelly, Martina
name: Salvalaggio, Ginetta
Publisher: name: figshare
Year: 2020
Subjects: subject: Biochemistry
subject: Medicine
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: Ecology
subject: FOS: Biological sciences
subject: Sociology
subject: FOS: Sociology
subject: 69999 Biological Sciences not elsewhere classified
subject: 80699 Information Systems not elsewhere classified
subject: FOS: Computer and information sciences
subject: Developmental Biology
subject: Science Policy
subject: Computational Biology

description: Additional file 1. Search strategy to identify tools used to measure attitudes to inner city populations.
Investigation of two colliding solitonic cores in Fuzzy Dark Matter models
Creators: name: Maleki, Alireza
name: Baghram, Shant
name: Rahvar, Sohrab
Publisher: name: arXiv
Year: 2019
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: One of the challenging questions in cosmology is the nature of dark matter particles. Fuzzy Dark Matter (FDM) is one of the candidates which is made of very light ($m_{FDM}\simeq 10^{-22}-10^{-21}$ eV) bosonic particles with no self-interaction. It is introduced by the motivation to solve the core-cusp problem in the galactic halos. In this work, we investigate the observational features from FDM halo collisions. Taking into account the quantum wave-length of the condensed bosonic structure, we determine the interference of the wave function of cores after collision. The fringe formation in the wave function is associated to the density contrast of the dark matter inside the colliding galaxies. The observational signatures of the fringes of the distribution of the dark matter are (i) on the lensing of the background sources, (ii) accumulation of the baryonic plasma tracking the interference of the FDM potential and (iii) excess in the X-ray emission from dense regions. Finally, we provide prospects for the observations of quantum wave features of FDM in the colliding galaxies. The NGC6240 colliding galaxy at the redshift of $z=0.024$ is a suitable candidate for this study. No signal is detected from the fringes in the Chandra data and taking into account the angular resolution of the telescope, we put constrain of $m> 7 \times10^{-23}$ eV on the mass of FDM particles.
description: 15 pages, 16 figures. Comments are welcome
A comparative study of productivity bargaining in the United Kingdom Margarine and Edible Fats Group of Unilever Ltd: an examination of bargaining in progress
Creators: name: J.P. Reason
Publisher: name: Loughborough University
Year: 2021
Subjects: subject: 150399 Business and Management not elsewhere classified
subject: FOS: Economics and business

description: A comparative study of productivity bargaining in the United Kingdom Margarine and Edible Fats Group of Unilever Ltd: an examination of bargaining in progress
Accretion driven turbulence in filaments II: Effects of self-gravity
Creators: name: Heigl, Stefan
name: Gritschneder, Matthias
name: Burkert, Andreas
Publisher: name: arXiv
Year: 2020
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We extend our previous work on simulations with the code RAMSES on accretion driven turbulence by including self-gravity and study the effects of core formation and collapse. We show that radial accretion onto filaments drives turbulent motions which are not isotropic but radially dominated. In contrast to filaments without gravity, the velocity dispersion of self-gravitating filaments does not settle in an equilibrium. Despite showing similar amounts of driven turbulence, they continually dissipate their velocity dispersion until the onset of core formation. This difference is connected to the evolution of the radius as it determines the dissipation rate. In the non-gravitational case filament growth is not limited and its radius grows linearly with time. In contrast, there is a maximum extent in the self-gravitational case resulting in an increased dissipation rate. Furthermore, accretion driven turbulence shows a radial profile which is anti-correlated with density. This leads to a constant turbulent pressure throughout the filament. As the additional turbulent pressure does not have a radial gradient it does not contribute to the stability of filaments and does not increase the critical line-mass. However, this radial turbulence does affect the radius of a filament, adding to the extent and setting its maximum value. Moreover, the radius evolution also affects the growth timescale of cores which compared to the timescale of collapse of an accreting filament limits core formation to high line-masses.
A low-loss fiber accessible plasmon photonic crystal waveguide for planar energy guiding and sensing
Creators: name: Maier, Stefan A.
name: Barclay, Paul E.
name: Johnson, Thomas J.
name: Friedman, Michelle D.
name: Painter, Oskar J.
Publisher: name: arXiv
Year: 2003
Subjects: subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: A metal nanoparticle plasmon waveguide for electromagnetic energy transport utilizing dispersion engineering to dramatically increase lateral energy confinement via a two-dimensional pattern of Au dots on an optically thin Si membrane is described. Using finite-difference time-domain simulations and coupled-mode theory, we show that phase-matched evanescent excitation from conventional fiber tapers is possible with efficiencies > 90 % for realistic geometries. Energy loss in this waveguide is mainly due to material absorption, allowing for 1/e energy decay distances of about 2 mm for excitation at telecommunication frequencies. This concept can be extended to the visible regime and promises applications in optical energy guiding, optical sensing, and switching.
description: 10 pages, 2 figures