cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Validation of the Eriksen Method of the Exact Foldy-Wouthuysen Representation
Creators: name: Silenko, Alexander J.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences
subject: J.2
subject: 81-XX Quantum theory

description: The Eriksen method is proven to yield a correct and exact result when a sufficient condition of exact transformation to the Foldy-Wouthuysen (FW) representation is satisfied. Therefore, the Eriksen method is confirmed as valid. This makes it possible to establish the limits within which the approximate "step-by-step" methods are applicable. The latter is done by comparing the relativistic formulas for a Hamiltonian operator in the FW representation (obtained using those methods) and the known expression for the first terms of a series, which defines the expansion of this operator in powers of v/c as found by applying the Eriksen method.
description: 7 pages
Chameleonic inflation
Creators: name: Hinterbichler, Kurt
name: Khoury, Justin
name: Nastase, Horatiu
name: Rosenfeld, Rogerio
Publisher: name: arXiv
Year: 2013
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We attempt to incorporate inflation into a string theory realization of the chameleon mechanism. Previously, it was found that the volume modulus, stabilized by the supersymmetric potential used by Kachru, Kallosh, Linde and Trivedi (KKLT) and with the right choice of parameters, can generically work as a chameleon. In this paper, we ask whether inflation can be realized in the same model. We find that we need a large extra dimensions set-up, as well as a semi-phenomenological deformation of the Kahler potential in the quantum region. We also find that an additional KKLT term is required so that there are now two pieces to the potential, one which drives inflation in the early universe, and one which is responsible for chameleon screening at late times. These two pieces of the potential are separated by a large flat desert in field space. The scalar field must dynamically traverse this desert between the end of inflation and today, and we find that this can indeed occur under the right conditions.
description: 27 pages, 4 figures
Almost sure global well posedness for the radial nonlinear Schrödinger equation on the unit ball II: the 3D case
Creators: name: Bourgain, Jean
name: Bulut, Aynur
Publisher: name: arXiv
Year: 2013
Subjects: subject: Analysis of PDEs (math.AP)
subject: Mathematical Physics (math-ph)
subject: FOS: Mathematics
subject: FOS: Physical sciences

description: We extend the convergence method introduced in our works [8]-[10] for almost sure global well-posedness of Gibbs measure evolutions of the nonlinear Schrödinger (NLS) and nonlinear wave (NLW) equations on the unit ball in R^d to the case of the three dimensional NLS. This is the first probabilistic global well-posedness result for NLS with supercritical data on the unit ball in R^3. The initial data is taken as a Gaussian random process lying in the support of the Gibbs measure associated to the equation, and results are obtained almost surely with respect to this probability measure. The key tools used include a class of probabilistic a priori bounds for finite-dimensional projections of the equation and a delicate trilinear estimate on the nonlinearity, which - when combined with the invariance of the Gibbs measure - enables the a priori bounds to be enhanced to obtain convergence of the sequence of approximate solutions.
description: 39 pages
Asteroid rotation excitation by subcatastrophic impacts
Creators: name: Henych, T.
name: Pravec, P.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Photometric observations of asteroids show that some of them are in non-principal axis rotation state (free precession), called tumbling. Collisions between asteroids have been proposed as a possible asteroid rotation excitation mechanism. We simulated subcatastrophic collisions between asteroids of various physical and material parameters to find out whether they could be responsible for the excited rotation. For every simulated target body after the collision, we computed its rotational lightcurve and we found that tumbling was photometrically detectable for the rotational axis misalignment angle βgreater than about 15 deg. We found that subcatastrophic collisions are a plausible cause of non-principal axis rotation for small slowly rotating asteroids. The determining parameter is the ratio of the projectile orbital angular momentum to the target rotational angular momentum and we derived an approximate relation between this ratio and the angle β. We also compared the limiting energy for the onset of tumbling with the shattering energy. Slowly rotating asteroids of diameter 100 m and larger can be rotationally excited by collisions with energies below the shattering limit.
description: 10 pages, 12 figures
Additional file 1 of Does teaching medical ethics ensure good knowledge, attitude, and reported practice? An ethical vignette-based cross-sectional survey among doctors in a tertiary teaching hospital in Nepal
Creators: name: Shrestha, Carmina
name: Shrestha, Ashma
name: Joshi, Jasmin
name: Karki, Shuvechchha
name: Acharya, Sajan
name: Joshi, Suchita
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Pharmacology
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Cancer
subject: Science Policy

description: Additional file 1. Supplementary Results and Findings.
What do leaders know?
Creators: name: Livan, Giacomo
name: Marsili, Matteo
Publisher: name: arXiv
Year: 2013
Subjects: subject: Physics and Society (physics.soc-ph)
subject: Social and Information Networks (cs.SI)
subject: FOS: Physical sciences
subject: FOS: Computer and information sciences

description: The ability of a society to make the right decisions on relevant matters relies on its capability to properly aggregate the noisy information spread across the individuals it is made of. In this paper we study the information aggregation performance of a stylized model of a society whose most influential individuals - the leaders - are highly connected among themselves and uninformed. Agents update their state of knowledge in a Bayesian manner by listening to their neighbors. We find analytical and numerical evidence of a transition, as a function of the noise level in the information initially available to agents, from a regime where information is correctly aggregated to one where the population reaches consensus on the wrong outcome with finite probability. Furthermore, information aggregation depends in a non-trivial manner on the relative size of the clique of leaders, with the limit of a vanishingly small clique being singular.
description: 10 pages, 3 figures
What is Visualization Really for?
Creators: name: Chen, Min
name: Floridi, Luciano
name: Borgo, Rita
Publisher: name: arXiv
Year: 2013
Subjects: subject: Human-Computer Interaction (cs.HC)
subject: FOS: Computer and information sciences

description: Whenever a visualization researcher is asked about the purpose of visualization, the phrase "gaining insight" by and large pops out instinctively. However, it is not absolutely factual that all uses of visualization are for gaining a deep understanding, unless the term insight is broadened to encompass all types of thought. Even when insight is the focus of a visualization task, it is rather difficult to know what insight is gained, how much, or how accurate. In this paper, we propose that "saving time" in accomplishing a user's task is the most fundamental objective. By giving emphasis to saving time, we can establish a concrete metric, alleviate unnecessary contention caused by different interpretations of insight, and stimulate new research efforts in some aspects of visualization, such as empirical studies, design optimisation and theories of visualization.
Additional file 2 of Does teaching medical ethics ensure good knowledge, attitude, and reported practice? An ethical vignette-based cross-sectional survey among doctors in a tertiary teaching hospital in Nepal
Creators: name: Shrestha, Carmina
name: Shrestha, Ashma
name: Joshi, Jasmin
name: Karki, Shuvechchha
name: Acharya, Sajan
name: Joshi, Suchita
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Pharmacology
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Cancer
subject: Science Policy

description: Additional file 2. Informed Consent form and Survey questionnaire for Study 1.
Additional file 3 of Does teaching medical ethics ensure good knowledge, attitude, and reported practice? An ethical vignette-based cross-sectional survey among doctors in a tertiary teaching hospital in Nepal
Creators: name: Shrestha, Carmina
name: Shrestha, Ashma
name: Joshi, Jasmin
name: Karki, Shuvechchha
name: Acharya, Sajan
name: Joshi, Suchita
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Pharmacology
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Cancer
subject: Science Policy

description: Additional file 3. Informed Consent form and Survey questionnaire for Study 2.
MPEC 2023-W04 : 2023 VB10
Creators: name: Minor Planet Center Staff
Publisher: name: The Minor Planet Center
Year: 2023
Subjects: subject: Small Solar System bodies
valueUri: http://astrothesaurus.org/uat/1469
subject: 2023 VB10

description: The Minor Planet Electronic Circulars contain information on unusual minor planets, routine data on comets and natural satellites, and occasional editorial announcements.  They are published on behalf of Division F of the International Astronomical Union by the Minor Planet Center, Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A.
Disentangling satellite galaxy populations using orbit tracking in simulations
Creators: name: Oman, Kyle A.
name: Hudson, Michael J.
name: Behroozi, Peter S.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: Physical processes regulating star formation in satellite galaxies represent an area of ongoing research, but the projected nature of observed coordinates makes separating different populations of satellites (with different processes at work) difficult. The orbital history of a satellite galaxy leads to its present-day phase space coordinates; we can also work backwards and use these coordinates to statistically infer information about the orbital history. We use merger trees from the MultiDark Run 1 N-body simulation to compile a catalog of the orbits of satellite haloes in cluster environments. We parameterize the orbital history by the time since crossing within 2.5 rvir of the cluster centre and use our catalog to estimate the probability density over a range of this parameter given a set of present-day projected (i.e. observable) phase space coordinates. We show that different populations of satellite haloes, e.g. infalling, backsplash and virialized, occupy distinct regions of phase space, and semi-distinct regions of projected phase space. This will allow us to probabilistically determine the time since infall of a large sample of observed satellite galaxies, and ultimately to study the effect of orbital history on star formation history (the topic of a future paper). We test the accuracy of our method and find that we can reliably recover this time within +/-2.58 Gyr in 68 per cent of cases by using all available phase space coordinate information, compared to +/-2.64 Gyr using only position coordinates and +/-3.10 Gyr guessing 'blindly', i.e. using no coordinate information, but with knowledge of the overall distribution of infall times. In some regions of phase space, the accuracy of the infall time estimate improves to +/-1.85 Gyr. Although we focus on time since infall, our method is easily generalizable to other orbital parameters (e.g. pericentric distance and time).
description: 10 pages, 9 figures, submitted to MNRAS
Schwinger-Dyson Renormalization Group
Creators: name: Veschgini, Kambis
name: Salmhofer, Manfred
Publisher: name: arXiv
Year: 2013
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We use the Schwinger-Dyson equations as a starting point to derive renormalization flow equations. We show that Katanin's scheme arises as a simple truncation of these equations. We then give the full renormalization group equations up to third order in the irreducible vertex. Furthermore, we show that to the fifth order, there exists a functional of the self-energy and the irreducible four-point vertex whose saddle point is the solution of Schwinger-Dyson equations.
The effect of Coulomb interactions on the disorder driven superconductor-insulator transition: THz versus tunneling spectroscopy
Creators: name: Sherman, Daniel
name: Gorshunov, Boris
name: Poran, Shachaf
name: Jesudasan, John
name: Raychaudhuri, Pratap
name: Trivedi, Nandini
name: Dressel, Martin
name: Frydman, Aviad
Publisher: name: arXiv
Year: 2013
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: The interplay between disorder and superconductivity has intrigued physicists for decades. Of particular interest is the influence of disorder on the superconducting energy gap $Δ$. In the absence of Coulomb interactions between electrons, disorder leads to emergent granularity of the local order parameter resulting in a pseudogap at temperatures above the critical temperature $T_c$, as well as a finite gap $Δ$ on the insulating side of the disorder-driven superconductor-insulator transition (SIT). At the same time, disorder also enhances the Coulomb interactions, which subsequently may influence $Δ$ in a manner that is still not fully understood. Here we investigate the evolution of the energy gap through the SIT by two different experimental methods: tunneling spectroscopy, in which a metallic electrode is placed close to the studied sample thus screening the Coulomb interactions, and terahertz (THz) spectroscopy, which probes the unscreened sample. The comparison between the two methods illustrates the role played by electronic interactions in determining the nature of the phases across the SIT and sheds light on the mechanisms involved in the destruction of superconductivity.
description: 17 pages, 5 figures
Additional file 1 of Retained particle surface area dose drives inflammation in rat lungs following acute, subacute, and subchronic inhalation of nanomaterials
Creators: name: Cosnier, Frédéric
name: Seidel, Carole
name: Valentino, Sarah
name: Schmid, Otmar
name: Bau, Sébastien
name: Vogel, Ulla
name: Devoy, Jérôme
name: Gaté, Laurent
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Pharmacology
subject: Biotechnology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: 69999 Biological Sciences not elsewhere classified
subject: Hematology

description: Additional file 1 : Supplemental 1. Inhalation set-up for P25 and Printex-90 aerosol exposures. Supplemental 2. Inhalation set-up for MWNT-7 aerosols exposure. Supplemental 3. Representative transmission electron microscopy images of (A) P25, (B) Printex-90 and (C) MWNT-7 aerosols. Supplemental 4. Number (left panel) and mass (right panel) particle size distributions of (A) agglomerated P25, (B) nebulized P25, (C) Printex-90, and (D) MWNT-7 aerosols. Supplemental 5. Cytology of bronchoalveolar lavage fluid (left lung) and lung and body weights for control animals and rats exposed to the different aerosols (n = 6 per group). Supplemental 6. Lung burden and clearance of P25 TiO2 (normalized to the airborne TiO2 concentration and fitted with a first order kinetic model) for the different exposure conditions (RBG: dry powder; AGK: dried nebulized suspension of powder). Supplemental 7. Lung burden and clearance of Printex-90 CB (normalized to airborne CB concentration) for the different exposure conditions (dry powder). Supplemental 8. Details of the post-exposure times for TiO2 material-induced effects on neutrophil influx as a function of retained surface area dose for different exposure times as depicted in Fig. 2: 1-week (triangle), 2-week (diamond), 4-week (square) or 13-week (circle). Both nanoparticles (unicolor) and fine particles (bicolor) were considered. Supplemental 9. Details of the post-exposure times for CB-induced effects on neutrophil influx as a function of retained surface area dose for different exposure times as depicted in Fig. 4: 4-week (or 6-week for Monarch 880 and Elftex 12) (square) or 13-week (circle). Supplemental 10. Details of the post-exposure times for MWCNT-induced effects on neutrophil influx as a function of retained surface area dose for different exposure times as depicted in Fig. 5: 1-week (triangle), 2-week (diamond), 4-week (square), or13-week (circle). Open symbols indicate that the retained surface area dose was estimated.
The helium-rich cataclysmic variable SBSS 1108+574
Creators: name: Carter, P. J.
name: Steeghs, D.
name: de Miguel, E.
name: Goff, W.
name: Koff, R. A.
name: Krajci, T.
name: Marsh, T. R.
name: Gänsicke, B. T.
name: Breedt, E.
name: Groot, P. J.
name: Nelemans, G.
name: Roelofs, G. H. A.
name: Rau, A.
name: Koester, D.
name: Kupfer, T.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We present time-resolved spectroscopy and photometry of the dwarf nova SBSS 1108+574, obtained during the 2012 outburst. Its quiescent spectrum is unusually rich in helium, showing broad, double-peaked emission lines from the accretion disc. We measure a line flux ratio HeI 5875/Halpha = 0.81 +/- 0.04, a much higher ratio than typically observed in cataclysmic variables (CVs). The outburst spectrum shows hydrogen and helium in absorption, with weak emission of Halpha and HeI 6678, as well as strong HeII emission. From our photometry, we find the superhump period to be 56.34 +/- 0.18 minutes, in agreement with the previously published result. The spectroscopic period, derived from the radial velocities of the emission lines, is found to be 55.3 +/- 0.8 minutes, consistent with a previously identified photometric orbital period, and significantly below the normal CV period minimum. This indicates that the donor in SBSS 1108+574 is highly evolved. The superhump excess derived from our photometry implies a mass ratio of q = 0.086 +/- 0.014. Our spectroscopy reveals a grazing eclipse of the large outbursting disc. As the disc is significantly larger during outburst, it is unlikely that an eclipse will be detectable in quiescence. The relatively high accretion rate implied by the detection of outbursts, together with the large mass ratio, suggests that SBSS 1108+574 is still evolving towards its period minimum.
description: 12 pages, 13 figures. Accepted for publication in MNRAS
Influence mechanism of commuter’s low-carbon literacy on the intention of mode choice: a case study in Shanghai, China
Creators: name: Huang, Yuqiao
name: Gao, Linjie
Publisher: name: Taylor & Francis
Year: 2021
Subjects: subject: Medicine
subject: Sociology
subject: FOS: Sociology
subject: 59999 Environmental Sciences not elsewhere classified
subject: FOS: Earth and related environmental sciences
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Ecology
subject: FOS: Biological sciences
subject: Inorganic Chemistry
subject: Science Policy

description: Predicting the intention of mode choice is indispensable for policymakers to develop sustainable transportation in large cities. This paper constructs a conceptual framework and tests it in the travel mode sector to investigate the influence mechanism between commuter’s low-carbon literacy and intention of mode choice. Commuter’s low-carbon literacy (LCL) was assessed through four critical attributes: low-carbon knowledge (LCK), low-carbon awareness (LCAW), low-carbon habits (LCH) and low-carbon affection (LCAF). Based on a questionnaire survey in Shanghai, empirical evidence was concluded using the Structural Equation Model of Partial Least Square (PLS-SEM). The results of this study are as follows: (1) low-carbon knowledge, habits and affection have direct influences on commuter’s intention of mode choice, whereas low-carbon awareness influences commuter’s intention through these three low-carbon attributes indirectly; (2) low-carbon affection has the highest impact rating on the intention of mode choice in both performance and importance; (3) commuting trips are less closely associated with the influence of low-carbon literacy than other trips. These findings have several implications for transportation demand management and are beneficial for urban trip structure optimization.
Additional file 10 of Adverse childhood experiences and child mental health: an electronic birth cohort study
Creators: name: Lowthian, Emily
name: Anthony, Rebecca
name: Evans, Annette
name: Daniel, Rhian
name: Long, Sara
name: Bandyopadhyay, Amrita
name: John, Ann
name: Bellis, Mark A.
name: Paranjothy, Shantini
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Biotechnology
subject: Science Policy
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Additional file 10: Table 8. Adult Mental Health codes for Common Mental Disorder (CMD) and Serious Mental Illness (SMI).
การศึกษาผลการใช้บอร์ดเกมการศึกษาเพื่อส่งเสริมพฤติกรรมการอนุรักษ์สิ่งแวดล้อมของนักเรียนชั้นอนุบาลปีที่ 2
Creators: name: ณัฐธิดา  รัตนบวรสถิตย์
Publisher: name: คณะเทคโนโลยีคหกรรมศาสตร์ มหาวิทยาลัยเทคโนโลยีราชมงคลธัญบุรี
Year: 2022
Subjects: บอร์ดเกมการศึกษา
พฤติกรรมการอนุรักษ์สิ่งแวดล้อม
นักเรียนชั้นอนุบาลปีที่ 2

description: วารสารเทคโนโลยีคหกรรมศาสตร์และนวัตกรรม, 1, 2(December), 57-70
title: Investigation of ultrasonic transducer responses when coupled with solid materials
Creators: name: Joyce, Katelyn
Publisher: name: Memorial University of Newfoundland
Year: 2023

description: This research focuses on ultrasonic transducer responses and elastic wave propagation in solid materials. This work was inspired by previous studies in geophysics, and its applications span several disciplines, such as material science, medicine and civil engineering. Previous geophysical work used a non-destructive testing method to investigate whether the frequency of a single-cycle ultrasonic pulse is related to the magnitude of its non-linear interactions. This work was inconclusive because the elastic wave frequency before and after propagating through the material was inconsistent. Hence, this research focuses on the fundamentals of how to analyze single-cycle pulses after they've travelled through solids using the Fast Fourier Transform and attempts to identify the source of the reported frequency discrepancy. This unexpected frequency discrepancy leads us to two hypotheses: (1) the examined material possesses the capacity for frequency conversion, or (2) aws in the experimental setup led to misleading results. To investigate these hypotheses, we conducted a series of experiments to establish the capabilities and limitations of our instruments. Before examining frequency conversion, it was essential to establish our setup's ability to generate and measure desired frequencies in the range of 50 kHz to 1 MHz. Using ultrasonic transducers to trigger wave propagation in various solid materials, we develop optimal operating parameters when coupling transducers to solid samples. The significance of this research lies in the understanding of how ultrasonic transducers couple with different materials. Although the motivation for this research lies in non-linear elasticity, these understandings apply to a diverse variety of fields. This contribution to the field of physics and instrumentation will lead to improved protocols for non-linear elastic data collection, ultimately enhancing our ability to measure and understand elastic wave propagation.
Extremal Horizons with Reduced Symmetry: Hyperscaling Violation, Stripes, and a Classification for the Homogeneous Case
Creators: name: Iizuka, Norihiro
name: Kachru, Shamit
name: Kundu, Nilay
name: Narayan, Prithvi
name: Sircar, Nilanjan
name: Trivedi, Sandip P.
name: Wang, Huajia
Publisher: name: arXiv
Year: 2012
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: Classifying the zero-temperature ground states of quantum field theories with finite charge density is a very interesting problem. Via holography, this problem is mapped to the classification of extremal charged black brane geometries with anti-de Sitter asymptotics. In a recent paper [1], we proposed a Bianchi classification of the extremal near-horizon geometries in five dimensions, in the case where they are homogeneous but, in general, anisotropic. Here, we extend our study in two directions: we show that Bianchi attractors can lead to new phases, and generalize the classification of homogeneous phases in a way suggested by holography. In the first direction, we show that hyperscaling violation can naturally be incorporated into the Bianchi horizons. We also find analytical examples of "striped" horizons. In the second direction, we propose a more complete classification of homogeneous horizon geometries where the natural mathematics involves real four-algebras with three dimensional sub-algebras. This gives rise to a richer set of possible near-horizon geometries, where the holographic radial direction is non-trivially intertwined with field theory spatial coordinates. We find examples of several of the new types in systems consisting of reasonably simple matter sectors coupled to gravity, while arguing that others are forbidden by the Null Energy Condition. Extremal horizons in four dimensions governed by three-algebras or four-algebras are also discussed.
description: 58 pages, 1 figure and 1 cartoon. v2: references added
Streaming instability in the quasi-global protoplanetary discs
Creators: name: Kowalik, Kacper
name: Hanasz, Michal
name: Wóltański, Dominik
name: Gawryszczak, Artur
Publisher: name: arXiv
Year: 2013
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: We investigate streaming instability using two-fluid approximation (neutral gas and dust) in a quasi-global, unstratified protoplanetary disc, with the help of PIERNIK code. We compare amplification rate of the eigen-mode in numerical simulations, with the corresponding growth resulting from the linear stability analysis of full system of Euler's equation including aerodynamic drag. Following Youdin & Goodman (2005) we show that (1) rapid dust clumping occurs due to the difference in azimuthal velocities of gas and dust, coupled by the drag force, (2) initial density perturbations are amplified by several orders of magnitude. We demonstrate that the multi-fluid extension of the simple and efficient Relaxing TVD scheme, implemented in PIERNIK, leads to results, which are compatible with those obtained with other methods.
description: 9 pages, 10 figures, accepted for publication in MNRAS; correct title and typos
Additional file 11 of Adverse childhood experiences and child mental health: an electronic birth cohort study
Creators: name: Lowthian, Emily
name: Anthony, Rebecca
name: Evans, Annette
name: Daniel, Rhian
name: Long, Sara
name: Bandyopadhyay, Amrita
name: John, Ann
name: Bellis, Mark A.
name: Paranjothy, Shantini
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Biotechnology
subject: Science Policy
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Additional file 11: Table 9. Codes for Externalising and Internalising categories.
Rare Decays and CP Violation in the $B_s$ System
Creators: name: Borissov, Guennadi
name: Fleischer, Robert
name: Schune, Marie-Hélène
Publisher: name: arXiv
Year: 2013
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: CP violating phenomena and rare decays of $B_s$ mesons offer interesting probes to test the quark-flavor sector of the Standard Model. In view of plenty of data reported in particular from the Large Hadron Collider, this topic has received a lot of attention in 2012. We give an overview of the the most recent experimental results, new theoretical developments, and discuss the prospects for the future exploration of the $B_s$-meson system.
description: 40 pages, 10 figures, Invited contribution to Annual Review of Nuclear and Particle Science, Vol. 63 (2013)
ผลของการทดแทนไขมันบางส่วนด้วยเนื้ออะโวคาโดต่อคุณสมบัติทางกายภาพและทางประสาทสัมผัสของคุกกี้เนย
Creators: name: อภิเดช พงษ์ประจักษ์
Publisher: name: คณะเทคโนโลยีคหกรรมศาสตร์ มหาวิทยาลัยเทคโนโลยีราชมงคลธัญบุรี
Year: 2022
Subjects: อะโวคาโด
คุกกี้
เนย

description: วารสารเทคโนโลยีคหกรรมศาสตร์และนวัตกรรม, 1, 2(December), 77-86
Additional file 12 of Adverse childhood experiences and child mental health: an electronic birth cohort study
Creators: name: Lowthian, Emily
name: Anthony, Rebecca
name: Evans, Annette
name: Daniel, Rhian
name: Long, Sara
name: Bandyopadhyay, Amrita
name: John, Ann
name: Bellis, Mark A.
name: Paranjothy, Shantini
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Biotechnology
subject: Science Policy
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Additional file 12: Table 10. Codes for Other and Developmental delay.
First evidence of interaction between longitudinal and transverse waves in solar magnetic elements
Creators: name: Stangalini, M.
name: Solanki, S. K.
name: Cameron, R.
name: Pillet, V. Martìnez
Publisher: name: arXiv
Year: 2013
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Small-scale magnetic fields are thought to play an important role in the heating of the outer solar atmosphere. By taking advantage of the unprecedented high-spatial and temporal cadence of IMaX, the filter vector polarimeter on board the Sunrise balloon-borne observatory, we study the transversal and longitudinal velocity oscillations in small magnetic elements. The results of this analysis are then compared to MHD simulations, showing excellent agreement. We found buffeting-induced transverse oscillations with velocity amplitudes of the order of 1-2 km/s, to be common along with longitudinal oscillations with amplitudes 0.4 km/s. Moreover, we also found an interaction between transverse oscillations and longitudinal velocity oscillations, showing a +-90 degrees phase lag at the frequency at which they exhibit the maximum coherence in the power spectrum. Our results are consistent with the theoretical picture in which MHD longitudinal waves are excited inside small magnetic elements as a response of the flux tube to the forcing action of the granular flows.
description: 9 pages, 7 figures, A&A accepted
Baryon and meson screening masses
Creators: name: Wang, Kun-lun
name: Liu, Yu-xin
name: Chang, Lei
name: Roberts, Craig D.
name: Schmidt, Sebastian M.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Nuclear Theory (nucl-th)
subject: High Energy Physics - Lattice (hep-lat)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: In a strongly-coupled quark-gluon plasma, collective excitations of gluons and quarks should dominate over the excitation of individual quasi-free gluon and quark modes. To explore this possibility, we computed screening masses for ground-state light-quark mesons and baryons at leading-order in a symmetry-preserving truncation scheme for the Dyson-Schwinger equations using a confining formulation of a contact-interaction at nonzero temperature. Meson screening masses are obtained from Bethe-Salpeter equations; and baryon analogues from a novel construction of the Faddeev equation, which employs an improved quark-exchange approximation in the kernel. Our treatment implements a deconfinement transition that is coincident with chiral symmetry restoration in the chiral limit, when both transitions are second order. Despite deconfinement, in all T=0 bound-state channels, strong correlations persist above the critical temperature, T>T_c; and, in the spectrum defined by the associated screening masses, degeneracy between parity-partner correlations is apparent for T >1.3T_c. Notwithstanding these results, there are reasons (including Golberger-Treiman relations) to suppose that the inertial masses of light-quark bound-states, when they may be defined, vanish at the deconfinement temperature; and that this is a signal of bound-state dissolution. Where a sensible comparison is possible, our predictions are consistent with results from contemporary numerical simulations of lattice-regularised QCD.
description: 21 pages, 12 figures, 1 table
EuFe2(As1-xPx)2: reentrant spin glass and superconductivity
Creators: name: Zapf, S.
name: Jeevan, H. S.
name: Ivek, T.
name: Pfister, F.
name: Klingert, F.
name: Jiang, S.
name: Wu, D.
name: Gegenwart, P.
name: Kremer, R. K.
name: Dressel, M.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: By systematic investigations of the magnetic, transport and thermodynamic properties of single crystals of EuFe2(As1-xPx)2 we explore the complex interplay of superconductivity and Eu2+ magnetism. Below 30K, two magnetic transitions are observed for all P substituted crystals suggesting a revision of the phase diagram. In addition to the canted A-type antiferromagnetic order of Eu2+ at approximately 20K, a spin glass transition is discovered at lower temperatures. Most remarkably, the reentrant spin glass state of EuFe2(As1-xPx)2 coexists with superconductivity around x = 0.2.
description: accepted by Physical Review Letters
Additional file 14 of Adverse childhood experiences and child mental health: an electronic birth cohort study
Creators: name: Lowthian, Emily
name: Anthony, Rebecca
name: Evans, Annette
name: Daniel, Rhian
name: Long, Sara
name: Bandyopadhyay, Amrita
name: John, Ann
name: Bellis, Mark A.
name: Paranjothy, Shantini
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Biotechnology
subject: Science Policy
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Additional file 14: Table 12. Table of national population statistics.
Additional file 13 of Adverse childhood experiences and child mental health: an electronic birth cohort study
Creators: name: Lowthian, Emily
name: Anthony, Rebecca
name: Evans, Annette
name: Daniel, Rhian
name: Long, Sara
name: Bandyopadhyay, Amrita
name: John, Ann
name: Bellis, Mark A.
name: Paranjothy, Shantini
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Biotechnology
subject: Science Policy
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Additional file 13: Table 11. ICD-10 codes for victimisation, taken from Lee, Gonzalez-Izquierod, and Gilbert (2012) [27].
La Participación Ciudadana como Componente Fundamental de la Gestión Social del Agua
Creators: name: Sinisterra Rodriguez, Mónica Maria
Publisher: name: Zenodo
Year: 2024
Subjects: subject: Water management
subject: water utilities
subject: citizen participation

description: Este folleto presenta los distintos mecanismos de participación ciudadana existentes en el marco de la legislación colombiana que favorecen al mejoramiento de la provisión del servicio de agua potable. Su principal objetivo es difundir conocimiento relevante que permite a la ciudadanía contribuir a la mejor prestación del servicio y al mejoramiento de la calidad de vida.
Error control of a numerical formula for the Fourier transform by Ooura's continuous Euler transform and fractional FFT
Creators: name: Tanaka, Ken'ichiro
Publisher: name: arXiv
Year: 2013
Subjects: subject: Numerical Analysis (math.NA)
subject: FOS: Mathematics
subject: 65D30, 65G99, 65T50

description: In this paper, we consider a method for fast numerical computation of the Fourier transform of a slowly decaying function with given accuracy in given ranges of the frequency. In these decades, some useful formulas for the Fourier transform are proposed to recover difficulty of the computation due to the slow decay and the oscillation of the integrand. In particular, Ooura proposed formulas with continuous Euler transformation and showed their effectiveness. It is, however, also reported that errors of them become large outside some ranges of the frequency. Then, for an illustrating representative of the formulas, we choose parameters in the formula based on its error analysis to compute the Fourier transform with given accuracy in given ranges of the frequency. Furthermore, combining the formula and fractional FFT, a generalization of the fast Fourier transform (FFT), we execute the computation in the same order of computation time as the FFT.
description: 15 pages, 13 figures
Techniques for Measuring Aerosol Attenuation using the Central Laser Facility at the Pierre Auger Observatory
Creators: name: Pierre Auger Collaboration
Publisher: name: arXiv
Year: 2013
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: The Pierre Auger Observatory in Malargüe, Argentina, is designed to study the properties of ultra-high energy cosmic rays with energies above 1018 eV. It is a hybrid facility that employs a Fluorescence Detector to perform nearly calorimetric measurements of Extensive Air Shower energies. To obtain reliable calorimetric information from the FD, the atmospheric conditions at the observatory need to be continuously monitored during data acquisition. In particular, light attenuation due to aerosols is an important atmospheric correction. The aerosol concentration is highly variable, so that the aerosol attenuation needs to be evaluated hourly. We use light from the Central Laser Facility, located near the center of the observatory site, having an optical signature comparable to that of the highest energy showers detected by the FD. This paper presents two procedures developed to retrieve the aerosol attenuation of fluorescence light from CLF laser shots. Cross checks between the two methods demonstrate that results from both analyses are compatible, and that the uncertainties are well understood. The measurements of the aerosol attenuation provided by the two procedures are currently used at the Pierre Auger Observatory to reconstruct air shower data.
description: 28 pages, 13 figures
Additional file 15 of Adverse childhood experiences and child mental health: an electronic birth cohort study
Creators: name: Lowthian, Emily
name: Anthony, Rebecca
name: Evans, Annette
name: Daniel, Rhian
name: Long, Sara
name: Bandyopadhyay, Amrita
name: John, Ann
name: Bellis, Mark A.
name: Paranjothy, Shantini
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Biotechnology
subject: Science Policy
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Additional file 15: Table 13. Moderation analysis for ACEs, deprivation, and child mental health.
Perturbative and Non-Perturbative Aspects in Vector Model/Higher Spin Duality
Creators: name: Jevicki, Antal
name: Jin, Kewang
name: Ye, Qibin
Publisher: name: arXiv
Year: 2012
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We review some recent work on AdS/CFT duality involving the 3d O(N) Vector Model and AdS4 Higher Spin Gravity. Our construction is based on bi-local collective field theory which provides an off-shell formulation of Higher Spin Gravity with G = 1/N playing the role of a coupling constant. Consequently perturbative and non-perturbative issues of the theory can be studied. For the correspondence based on free CFT's we discuss the nature of bulk 1/N interactions through an S-matrix which is argued to be equal to 1 (Coleman-Mandula theorem). As a consequence in this class of theories nonlinearities are removable, through a nonlinear field transformation which we show at the exact level. We also describe a geometric (Kahler space) framework for the bi-local theory which applies equally simple to Sp(2N) fermions and the de Sitter correspondence. We discuss in this framework the structure and size of the bi-local Hilbert space and the implementation of (finite N) exclusion principle.
description: 21 pages, 3 figures; Contribution to J. Phys. A special volume on "Higher Spin Theories and AdS/CFT" edited by M. R. Gaberdiel and M. Vasiliev; v2: references updated
Spitzer Transits of the Super-Earth GJ1214b and Implications for Its Atmosphere
Creators: name: Fraine, Jonathan D.
name: Deming, Drake
name: Gillon, Michaël
name: Jehin, Emmanuël
name: Demory, Brice-Olivier
name: Benneke, Bjoern
name: Seager, Sara
name: Lewis, Nikole K.
name: Knutson, Heather
name: Desert, Jean-Michel
Publisher: name: arXiv
Year: 2013
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: We observed the transiting super-Earth exoplanet GJ1214b using Warm Spitzer at 4.5 microns wavelength during a 20-day quasi-continuous sequence in May 2011. The goals of our long observation were to accurately define the infrared transit radius of this nearby super-Earth, to search for the secondary eclipse, and to search for other transiting planets in the habitable zone of GJ1214. We here report results from the transit monitoring of GJ1214b, including a re-analysis of previous transit observations by Desert et al. (2011). In total, we analyse 14 transits of GJ1214b at 4.5 microns, 3 transits at 3.6 microns, and 7 new ground-based transits in the I+z band. Our new Spitzer data by themselves eliminate cloudless solar composition atmospheres for GJ1214b, and methane-rich models from Howe & Burrows (2012). Using our new Spitzer measurements to anchor the observed transit radii of GJ1214b at long wavelengths, and adding new measurements in I+z, we evaluate models from Benneke & Seager (2012) and Howe & Burrows (2012) using a chi-squared analysis. We find that the best-fit model exhibits an increase in transit radius at short wavelengths due to Rayleigh scattering. Pure water atmospheres are also possible. However, a flat line (no atmosphere detected) remains among the best of the statistically acceptable models, and better than pure water atmospheres. We explore the effect of systematic differences among results from different observational groups, and we find that the Howe & Burrows (2012) tholin-haze model remains the best fit, even when systematic differences among observers are considered.
Additional file 1 of Adverse childhood experiences and child mental health: an electronic birth cohort study
Creators: name: Lowthian, Emily
name: Anthony, Rebecca
name: Evans, Annette
name: Daniel, Rhian
name: Long, Sara
name: Bandyopadhyay, Amrita
name: John, Ann
name: Bellis, Mark A.
name: Paranjothy, Shantini
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Biotechnology
subject: Science Policy
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Additional file 1: Figure 1. Participant Selection.
Entropic Forms and Related Algebras
Creators: name: Scarfone, A. M.
Publisher: name: arXiv
Year: 2013
Subjects: subject: Mathematical Physics (math-ph)
subject: Data Analysis, Statistics and Probability (physics.data-an)
subject: FOS: Physical sciences

description: Starting from a very general trace-form entropy, we introduce a pair of algebraic structures endowed by a generalized sum and a generalized product. These algebras form, respectively, two Abelian fields in the realm of the complex numbers isomorphic each other. We specify our results to several entropic forms related to distributions recurrently observed in social, economical, biological and physical systems including the stretched exponential, the power-law and the interpolating Bosons-Fermions distributions. Some potential applications in the study of complex systems are advanced.
description: 20 pages, no figures
Additional file 3 of Adverse childhood experiences and child mental health: an electronic birth cohort study
Creators: name: Lowthian, Emily
name: Anthony, Rebecca
name: Evans, Annette
name: Daniel, Rhian
name: Long, Sara
name: Bandyopadhyay, Amrita
name: John, Ann
name: Bellis, Mark A.
name: Paranjothy, Shantini
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Biotechnology
subject: Science Policy
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Additional file 3: Table 1. Sociodemographic and perinatal characteristics in each exposure.
Adaptive confidence intervals for regression functions under shape constraints
Creators: name: Cai, T. Tony
name: Low, Mark G.
name: Xia, Yin
Publisher: name: arXiv
Year: 2013
Subjects: subject: Statistics Theory (math.ST)
subject: FOS: Mathematics

description: Adaptive confidence intervals for regression functions are constructed under shape constraints of monotonicity and convexity. A natural benchmark is established for the minimum expected length of confidence intervals at a given function in terms of an analytic quantity, the local modulus of continuity. This bound depends not only on the function but also the assumed function class. These benchmarks show that the constructed confidence intervals have near minimum expected length for each individual function, while maintaining a given coverage probability for functions within the class. Such adaptivity is much stronger than adaptive minimaxity over a collection of large parameter spaces.
description: Published in at http://dx.doi.org/10.1214/12-AOS1068 the Annals of Statistics (http://www.imstat.org/aos/) by the Institute of Mathematical Statistics (http://www.imstat.org)
A modified W-W interatomic potential based on ab initio calculations
Creators: name: Wang, Jun
name: Zhou, Yulu
name: Li, Min
name: Hou, Qing
Publisher: name: arXiv
Year: 2013
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Based on ab initio calculations, a Finnis-Sinclair-type interatomic potential for W-W interactions has been developed. The modified potential is able to reproduce the correct formation energies of self-interstitial atom defects in tungsten, offering a significant improvement over the Ackland-Thetford tungsten potential. Using the modified potential, the thermal expansion is calculated in a temperature range from 0 K to 3500 K, and the results are in reasonable agreement with the experimental data, thus overcoming the shortcoming of the negative thermal expansion using the Derlet-Nguyen-Manh-Dudarev tungsten potential. The present W-W potential is also applied to study in detail the diffusion of self-interstitial atoms in tungsten. It is revealed that the initial self-interstitial atom initiates a sequence of W atom displacements and replacements in the <111> direction. An Arrhenius fit to the diffusion data at temperatures below 550 K indicates a migration energy of 0.022 eV, in reasonable agreement with the experimental data.
description: 27 pages,5 figures