cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Pain assessments for procedural pain in neonates at risk of neonatal opioid withdrawal syndrome: A scoping review
Creators: name: Langman, Erin
name: Mansell, Deborah
name: West, Claire
name: Lavergne, Julianna
name: Benoit, Britney
name: Dol, Justine
Publisher: name: Open Science Framework
Year: 2023
Subjects: subject: Maternal, Child Health and Neonatal Nursing
subject: Pediatric Nursing
subject: Medicine and Health Sciences
subject: Substance Abuse and Addiction
subject: Medical Sciences
subject: Nursing
subject: FOS: Health sciences
subject: Mental and Social Health

description: The purpose of this scoping review is to identify evidence for pain assessment during acute procedures in hospitalized neonates at risk of neonatal opioid withdrawal syndrome (NOWS).
Bound states on the lattice with partially twisted boundary conditions
Creators: name: Agadjanov, D.
name: Guo, F. -K.
name: Ríos, G.
name: Rusetsky, A.
Publisher: name: arXiv
Year: 2014
Subjects: subject: High Energy Physics - Lattice (hep-lat)
subject: FOS: Physical sciences

description: We propose a method to study the nature of exotic hadrons by determining the wave function renormalization constant $Z$ from lattice simulations. It is shown that, instead of studying the volume-dependence of the spectrum, one may investigate the dependence of the spectrum on the twisting angle, imposing twisted boundary conditions on the fermion fields on the lattice. In certain cases, e.g., the case of the $DK$ bound state which is addressed in detail, it is demonstrated that the partial twisting is equivalent to the full twisting up to exponentially small corrections.
Scroll Waves Pinned to Moving Heterogeneities
Creators: name: Ke, Hua
name: Zhang, Zhihui
name: Steinbock, Oliver
Publisher: name: arXiv
Year: 2014
Subjects: subject: Pattern Formation and Solitons (nlin.PS)
subject: Soft Condensed Matter (cond-mat.soft)
subject: Adaptation and Self-Organizing Systems (nlin.AO)
subject: FOS: Physical sciences

description: Three-dimensional excitable systems can selforganize vortex patterns that rotate around one-dimensional phase singularities called filaments. In experiments with the Belousov-Zhabotinsky reaction and numerical simulations, we pin these scroll waves to moving heterogeneities and demonstrate the controlled repositioning of their rotation centers. If the pinning site extends only along a portion of the filament, the phase singularity is stretched out along the trajectory of the heterogeneity which effectively writes the singularity into the system. Its trailing end point follows the heterogeneity with a lower velocity. This velocity, its dependence on the placement of the anchor, and the shape of the filament are explained by a curvature flow model.
Superconductivity in multiorbital systems with repulsive interactions: Hund's pairing vs. spin-fluctuation pairing
Creators: name: Roig, Mercè
name: Rømer, Astrid T.
name: Kreisel, Andreas
name: Hirschfeld, P. J.
name: Andersen, Brian M.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: Hund's pairing refers to Cooper pairing generated by onsite interactions that become attractive due to large Hund's exchange $J$. This is possible in multiorbital systems even when all local bare interactions are repulsive, since attraction in specific channels are given by certain linear combinations of interaction parameters. On the other hand, pairing processes such as the exchange of spin fluctuations, are also present. We compare these two mechanisms on an equal footing using electronic bands appropriate for different classes of multiorbital systems over a wide range of interaction parameters. We find that for systems without clear nesting features, the superconducting state generated by the Hund's mechanism agrees well with that from the full fluctuation exchange vertex when Hund's exchange and spin-orbit coupling are sufficiently large. On the other hand, for systems characterized by a peaked finite-momentum particle-hole susceptibility, spin-fluctuation pairing generally dominates over Hund's pairing. We conclude that Hund's pairing states are unlikely to be realized in systems like Sr$_2$RuO$_4$ and generic iron-based superconductors.
description: 6 pages, 2 figures, including supplemental material
Limit distributions of Gaussian block ensembles
Creators: name: Lenczewski, Romuald
Publisher: name: arXiv
Year: 2015
Subjects: subject: Operator Algebras (math.OA)
subject: Probability (math.PR)
subject: FOS: Mathematics
subject: 46L54, 15B52

description: It has been shown by Voiculescu that important classes of square independent random matrices are asymptotically free, where freeness is a noncommutative analog of classical independence. Recently, we introduced the concept of matricial freeness, which is similar to freeness in free probability, but it also has some matricial features. Using this new concept of noncommutative independence, we described the asymptotics of blocks and symmetric blocks of certain classes of independent random matrices. In this paper, we present the main results obtained in this framework, concentrating on the ensembles of blocks of Gaussian random matrices.
description: 14 pages
Dark Matter constraints from Planck observations of the Galactic polarized synchrotron emission
Creators: name: Manconi, Silvia
name: Cuoco, Alessandro
name: Lesgourgues, Julien
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Dark Matter (DM) annihilation in our Galaxy may produce a linearly polarized synchrotron signal. We use, for the first time, synchrotron polarization to constrain the DM annihilation cross section by comparing theoretical predictions with the latest polarization maps obtained by the Planck satellite collaboration. We find that synchrotron polarization is typically more constraining than synchrotron intensity by about one order of magnitude, independently of uncertainties in the modeling of electron and positron propagation, or of the Galactic magnetic field. Our bounds compete with Cosmic Microwave Background limits in the case of leptophilic DM.
description: 6+11 pages, 3+9 figures. Minor comments added, results unchanged. Matches the version accepted by PRL
Antisymmetric tensor field and spontaneous magnetization in holographic duality
Creators: name: Cai, Rong-Gen
name: Yang, Run-Qiu
Publisher: name: arXiv
Year: 2015
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: A real anti-symmetric tensor field was introduced to realize a holographic magnetic ordered phase in our previous works. However, a more careful analysis shows there is a vector ghost in the model. In this paper we present a modified Lagrangian density for the anti-symmetric tensor, which is ghost free and causality is well-defined, and keeps all the significant results in the original model qualitatively. We show this modified Lagrangian density could come from the dimensional compactification of $p$-form field in String/M-theory. For static curved space-time, we also prove that this modified model is ghost free and dose not violate causality. This new model offers a solid foundation for the application of antisymmetric tensor field in holographic duality, especially for the spontaneous magnetization.
description: minor revision
Exuviae Alexandri: slittamenti del significato allegorico della spoglia elefantina
Creators: name: Bonoldi Lorenzo
Publisher: name: La Rivista di Engramma
Year: 2005
Subjects: Exuviae elephantis
Alexander the Great
Iconography

description: The term exuviae elephantis indicates the iconographic attribute of the elephantine bare worn to cover the head. In the repertoire of classical art there are mainly three figures to whom this attribute is precisely: Alexander the Great, the personification of Africa and that of the city of Alexandria in Egypt. Alongside these three figures, others must also be enumerated (including the effigies of some Hellenistic sovereigns and the personifications of some African nations and, later, some other allegories by Cesare Ripa) which have made the attribute of the elephant scalp their own. by imitation and / or by analogy. In this essay we will try to outline the history of the iconographic attribute, investigating the reasons for its passage from one figure to another, along a path, more tortuous than linear, which winds through the centuries and which crosses three continents - Asia, Africa and Europe - leads from India to Rome.
Deformation and tidal evolution of close-in planets and satellites using a Maxwell viscoelastic rheology
Creators: name: Correia, Alexandre C. M.
name: Boué, Gwenaël
name: Laskar, Jacques
name: Rodríguez, Adrián
Publisher: name: arXiv
Year: 2014
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Dynamical Systems (math.DS)
subject: Geophysics (physics.geo-ph)
subject: FOS: Physical sciences
subject: FOS: Mathematics

description: In this paper we present a new approach to tidal theory. Assuming a Maxwell viscoelastic rheology, we compute the instantaneous deformation of celestial bodies using a differential equation for the gravity field coefficients. This method allows large eccentricities and it is not limited to quasi-periodic perturbations. It can take into account an extended class of perturbations, including chaotic motions and transient events. We apply our model to some already detected eccentric hot Jupiters and super-Earths in planar configurations. We show that when the relaxation time of the deformation is larger than the orbital period, spin-orbit equilibria arise naturally at half-integers of the mean motion, even for gaseous planets. In the case of super-Earths, these equilibria can be maintained for very low values of eccentricity. Our method can also be used to study planets with complex internal structures and other rheologies.
description: 16 pages, 13 figures, 2 tables
Thermodynamics of the Reissner-Nordström-de Sitter Spacetime with Quintessence
Creators: name: Zhang, Yang
name: Ma, Yu-Bo
name: Du, Yun-Zhi
name: Li, Huai-Fan
name: Zhang, Li-Chun
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: For Anti-de Sitte (AdS) black holes, the isochoric heat capacity of system is vanished, while the isobaric heat capacity is not. However, this situation does not hold on for de Sitter (dS) black holes. In this work, by introducing the interaction between the black hole horizon and the cosmological horizon of the Reissner-Nordström-de Sitter (RNdS) spacetime with quintessence, we discuss the phase transition of this system. The results show that the spacetime not only has the similar phase transition behavior to that of Van der Waals (VdW) system, and the non-vanishing isochoric heat capacity fulfills the whole thermodynamics system. Through the discussion of the entropic force between two horizons, we find out the role of entropic force in the evolution of spacetime. In addition, we also study the influence of various parameters on the phase transition and entropic force, which will provide a new method for exploring the interaction among black hole molecules from a micro perspective.
Gravitational instability with a dark matter background: Exploring the different scenarios
Creators: name: Ourabah, Kamel
Publisher: name: arXiv
Year: 2022
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We study the Jeans-type gravitational instability for a self-gravitating medium composed of two species, baryonic (bright) and dark matter particles, using a hybrid quantum-classical fluid approach. Baryonic matter is treated classically, which is appropriate for most astrophysical environments, e.g., Bok globules, while dark matter is treated through a quantum hydrodynamic approach allowing for possible nonlinearities. These nonlinearities may arise in bosonic dark matter due to attractive or repulsive short-range self-interaction (attractive interaction being more relevant for axions) or from the Pauli exclusion principle for fermionic dark matter, e.g., massive neutrinos. This allows us to explore, in a very broad context, the impact of a dark matter background on the Jeans process for different scenarios discussed in the literature. In the simplest case, it is shown that the effect of a dark matter background on the Jeans mass depends only on the ratio of densities and velocity dispersions of baryonic and dark matter particles. Taking advantage of that, we confront the established stability criterion with Bok globule stability observations and show that the model adequately accounts for the data with dark matter parameters close to those predicted independently from numerical simulations.
A multiple--resolution strategy for Direct Numerical Simulation of scalar turbulence
Creators: name: Ostilla-Mónico, Rodolfo
name: Yang, Yantao
name: van der Poel, Erwin P.
name: Lohse, Detlef
name: Verzicco, Roberto
Publisher: name: arXiv
Year: 2015
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: Computational Physics (physics.comp-ph)
subject: FOS: Physical sciences

description: In this paper a numerical procedure to simulate low diffusivity scalar turbulence is presented. The method consists of using a grid for the advected scalar with a higher spatial resolutions than that of the momentum. The latter usually requires a less refined mesh and integrating both fields on a single grid tailored to the most demanding variable, produces an unnecessary computational overhead. A multiple resolution approach is used also in the time integration in order to maintain the stability of the scalars on the finer grid. The method is the more advantageous the less diffusive the scalar is with respect to momentum, therefore it is particularly well suited for large Prandtl or Schmidt number flows. However, even in the case of equal diffusivities the present procedure gives CPU time and memory occupation savings. The reason is that the absence of the pressure term in the scalar equation leads to much steeper gradients in the scalar field as compared to the velocity field.
Capacitively coupled distinct mechanical resonators for room temperature phonon-cavity electromechanics
Creators: name: Pokharel, Alok
name: Xu, Hao
name: Venkatachalam, Srisaran
name: Collin, Eddy
name: Zhou, Xin
Publisher: name: arXiv
Year: 2022
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Coupled electromechanical resonators that can be independently driven/detected and easily integrated with external circuits are essential for exploring mechanical modes based signal processing. Here, we present a room temperature phonon-cavity electromechanical system, consisting of two distinct resonators: a silicon nitride electromechanical drum capacitively coupled to an aluminum one. We demonstrate electromechanically induced transparency and amplification in a two-tone driving scheme and observe the phonon-cavity force affecting the mechanical damping rates of both movable objects. We also develop an analytical model based on linearly coupled motion equations, which captures the optomechanical features in the classical limit and enables to fit quantitatively our measurements. Our results open up new possibilities in the study of phonon-cavity based signal processing in the classical and potentially in the future in the quantum regimes.
Exploring the landscape of (anti-) de Sitter and Minkowski solutions: group manifolds, stability and scale separation
Creators: name: Andriot, David
name: Horer, Ludwig
name: Marconnet, Paul
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: We classified in arXiv:2201.04152 certain 10d supergravity solutions with a 4d de Sitter, Minkowski or anti-de Sitter spacetime. We then found new solutions in previously unexplored classes. In this paper we study their properties, compare them to swampland conjectures, and make new observations. Using new numerical tools, we first identify all Lie algebras underlying the 6d group manifolds, allowing us to discuss their compactness. We then investigate scale separation, and prove related no-go theorems. Last but not least, we automatize and analyze the stability of all solutions. This leads us to propose the Massless Minkowski Conjecture, claiming the systematic presence of a 4d massless scalar field.
description: v1: 30 pages + appendices. The numerical codes AlgId, AlgIso and MaxSymSolSpec developed are provided here as ancillary files; v2: minor modifications, published version; v3: clarification on the Massless Minkowski Conjecture
Bayesian optimization with experimental failure for high-throughput materials growth
Creators: name: Wakabayashi, Yuki K.
name: Otsuka, Takuma
name: Krockenberger, Yoshiharu
name: Sawada, Hiroshi
name: Taniyasu, Yoshitaka
name: Yamamoto, Hideki
Publisher: name: arXiv
Year: 2022
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: A crucial problem in achieving innovative high-throughput materials growth with machine learning and automation techniques, such as Bayesian optimization (BO) and robotic experimentation, has been a lack of an appropriate way to handle missing data due to experimental failures. Here, we propose a new BO algorithm that complements the missing data in the optimization of materials growth parameters. The proposed method provides a flexible optimization algorithm capable of searching a wide multi-dimensional parameter space. We demonstrate the effectiveness of the method with simulated data as well as in its implementation for actual materials growth, namely machine-learning-assisted molecular beam epitaxy (ML-MBE) of SrRuO3, which is widely used as a metallic electrode in oxide electronics. Through the exploitation and exploration in a wide three-dimensional parameter space, while complementing the missing data, we attained tensile-strained SrRuO3 film with a high residual resistivity ratio of 80.1, the highest among tensile-strained SrRuO3 films ever reported, in only 35 MBE growth runs.
Geometric post-Newtonian description of spin-half particles in curved spacetime
Creators: name: Alibabaei, Ashkan
Publisher: name: arXiv
Year: 2022
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Theory (hep-th)
subject: Mathematical Physics (math-ph)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Einstein Equivalence Principle (EEP) requires all matter components to universally couple to gravity via a single common geometry: that of spacetime. This relates quantum theory with geometry as soon as interactions with gravity are considered. In this work, I study the geometric theory of coupling a spin-1/2 particle to gravity in a twofold expansion scheme: First with respect to the distance based on Fermi normal coordinates around a preferred worldline (e.g., that of a clock in the laboratory), second with respect to 1/c (post-Newtonian expansion). I consider the one-particle sector of a massive spinor field in QFT, here described effectively by a classical field. The formal expansion in powers of 1/c yields a systematic and complete generation of GR corrections for quantum systems. I find new terms that were overlooked in the literature at order 1/c^2 and extended the level of approximation to the next order. These findings are significant for a consistent inclusion of gravity corrections in the description of quantum experiments of corresponding sensitivities, and also for testing aspects of GR, like the EEP, in the quantum realm.
description: Master's thesis, 8+77 pages, 3 figures. v2: corrected typos, updated discussion in chapter 5, removed double references. v3: corrected further typos
CAD_bioreactor_side_view.pdf from Nutrients and flow shape the cyclic dominance games between Escherichia coli strains
Creators: name: Kuhn, Thierry
name: Pilar, Junier
name: Bshary, Redouan
name: Terrettaz, Céline
name: Gonzalez, Diego
name: Richter, Xiang-Yi Li
Publisher: name: The Royal Society
Year: 2023
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: Evolutionary Biology
subject: Ecology
subject: 60102 Bioinformatics
subject: FOS: Computer and information sciences
subject: Computational Biology
subject: 10202 Biological Mathematics
subject: FOS: Mathematics

description: CAD drawing of the mini-bioreactor – side view
New insight into the Solar System's transition disk phase provided by the unusual meteorite Isheyevo
Creators: name: Morris, Melissa A.
name: Garvie, Laurence A. J.
name: Knauth, L. Paul
Publisher: name: arXiv
Year: 2014
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Many aspects of planet formation are controlled by the amount of gas remaining in the natal protoplanetary disk (PPDs). Infrared observations show that PPDs undergo a transition stage at several Myr, during which gas densities are reduced. Our Solar System would have experienced such a stage. However, there is currently no data that provides insight into this crucial time in our PPD's evolution. We show that the Isheyevo meteorite contains the first definitive evidence for a transition disk stage in our Solar System. Isheyevo belongs to a class of metal-rich meteorites whose components have been dated at almost 5 Myr after the first solids in the Solar System, and exhibits unique sedimentary layers that imply formation through gentle sedimentation. We show that such layering can occur via gentle sweep-up of material found in the impact plume resulting from the collision of two planetesimals. Such sweep-up requires gas densities consistent with observed transition disks. As such, Isheyevo presents the first evidence of our own transition disk and provides new constraints on the evolution of our solar nebula.
description: submitted to The Astrophysical Journal Letters
Complete nonlinear action for supersymmetric multiple D$0$-brane system
Creators: name: Bandos, Igor
name: Sarraga, Unai D. M.
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: We present a complete nonlinear action for the dynamical system of nearly coincident multiple D$0$-branes (mD$0$) which possesses, besides manifest spacetime (target superspace) supersymmetry, also the worldline supersymmetry, a counterpart of the local fermionic $κ$-symmetry of single D$0$-brane (Dirichlet superparticle). The action contains an arbitrary non-vanishing function ${\cal M}({\cal H})$ of the relative motion Hamiltonian ${\cal H}$. The $D=10$ mD$0$ model with particular form of ${\cal M}({\cal H})$ can be obtained by dimensional reduction from the action of eleven-dimensional ($D=11$) multiple M-wave (mM$0$) system.
description: 5 pages, revtex4. V2: Appendices added, 11 pages
Unwinding the hairball graph: pruning algorithms for weighted complex networks
Creators: name: Dianati, Navid
Publisher: name: arXiv
Year: 2015
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: Empirical networks of weighted dyadic relations often contain noisy edges that alter the global characteristics of the network and obfuscate the most important structures therein. Graph pruning is the process of identifying the most significant edges according to a generative null model, and extracting the subgraph consisting of those edges. Here, we focus on integer-weighted graphs commonly arising when weights count the occurrences of an "event" relating the nodes. We introduce a simple and intuitive null model related to the configuration model of network generation, and derive two significance filters from it: the Marginal Likelihood Filter (MLF) and the Global Likelihood Filter (GLF). The former is a fast algorithm assigning a significance score to each edge based on the marginal distribution of edge weights whereas the latter is an ensemble approach which takes into account the correlations among edges. We apply these filters to the network of air traffic volume between US airports and recover a geographically faithful representation of the graph. Furthermore, compared with thresholding based on edge weight, we show that our filters extract a larger and significantly sparser giant component.
Stream-based Active Learning with Verification Latency in Non-stationary Environments
Creators: name: Castellani, Andrea
name: Schmitt, Sebastian
name: Hammer, Barbara
Publisher: name: arXiv
Year: 2022
Subjects: subject: Machine Learning (cs.LG)
subject: Artificial Intelligence (cs.AI)
subject: FOS: Computer and information sciences

description: Data stream classification is an important problem in the field of machine learning. Due to the non-stationary nature of the data where the underlying distribution changes over time (concept drift), the model needs to continuously adapt to new data statistics. Stream-based Active Learning (AL) approaches address this problem by interactively querying a human expert to provide new data labels for the most recent samples, within a limited budget. Existing AL strategies assume that labels are immediately available, while in a real-world scenario the expert requires time to provide a queried label (verification latency), and by the time the requested labels arrive they may not be relevant anymore. In this article, we investigate the influence of finite, time-variable, and unknown verification delay, in the presence of concept drift on AL approaches. We propose PRopagate (PR), a latency independent utility estimator which also predicts the requested, but not yet known, labels. Furthermore, we propose a drift-dependent dynamic budget strategy, which uses a variable distribution of the labelling budget over time, after a detected drift. Thorough experimental evaluation, with both synthetic and real-world non-stationary datasets, and different settings of verification latency and budget are conducted and analyzed. We empirically show that the proposed method consistently outperforms the state-of-the-art. Additionally, we demonstrate that with variable budget allocation in time, it is possible to boost the performance of AL strategies, without increasing the overall labeling budget.
description: ENNS Best Paper Award at ICANN 2022
การพัฒนาโปรแกรมสำเร็จรูปเพื่อการคำนวณวันครบกำหนดคลอด
Creators: name: วัฒนา ชยธวัช
Publisher: name: ศูนย์สนับสนุนและพัฒนาการเรียนการสอน มหาวิทยาลัยรังสิต
Year: 2012
Subjects: Calculation Sofware
date of confinement
Midwifery
Naegele's rule
Parikh's formula
กฎของเนเกล
ผดุงครรภ์
วันครบกำหนดคลอด
สูตรของพาริกฮ์
โปรแกรมสำเร็จรูปเพื่อการคำนวณ

description: วารสารพัฒนาการเรียนการสอน, 6, 2, 30-38
Survival probability of random walks and Lévy flights with stochastic resetting
Creators: name: Godrèche, Claude
name: Luck, Jean-Marc
Publisher: name: arXiv
Year: 2022
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Probability (math.PR)
subject: FOS: Physical sciences
subject: FOS: Mathematics

description: We perform a thorough analysis of the survival probability of symmetric random walks with stochastic resetting, defined as the probability for the walker not to cross the origin up to time $n$. For continuous symmetric distributions of step lengths with either finite (random walks) or infinite variance (Lévy flights), this probability can be expressed in terms of the survival probability of the walk without resetting, given by Sparre Andersen theory. It is therefore universal, i.e., independent of the step length distribution. We analyze this survival probability at depth, deriving both exact results at finite times and asymptotic late-time results. We also investigate the case where the step length distribution is symmetric but not continuous, focussing our attention onto arithmetic distributions generating random walks on the lattice of integers. We investigate in detail the example of the simple Polya walk and propose an algebraic approach for lattice walks with a larger range.
description: 19 pages, 5 figures
Supplementary Materials and Methods.pdf from Nutrients and flow shape the cyclic dominance games between Escherichia coli strains
Creators: name: Kuhn, Thierry
name: Pilar, Junier
name: Bshary, Redouan
name: Terrettaz, Céline
name: Gonzalez, Diego
name: Richter, Xiang-Yi Li
Publisher: name: The Royal Society
Year: 2023
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: Evolutionary Biology
subject: Ecology
subject: 60102 Bioinformatics
subject: FOS: Computer and information sciences
subject: Computational Biology
subject: 10202 Biological Mathematics
subject: FOS: Mathematics

description: Supplementary Materials and Methods
Magnetic properties of triangular lattice antiferromagnets Ba3RB9O18 (R = Yb, Er)
Creators: name: Khatua, J.
name: Pregelj, M.
name: Elghandour, A.
name: Jaglicic, Z.
name: Klingeler, R.
name: Zorko, A.
name: Khuntia, P.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Frustration, spin correlations and interplay between competing degrees of freedom are some of the key ingredients that underlie exotic states with fractional excitations in quantum materials. Rare-earth based two dimensional magnetic lattice wherein crystal electric field, spin-orbit coupling, anisotropy and electron correlation between rare-earth moments offer a new paradigm in this context. Herein, we present crystal structure, magnetic susceptibility and specific heat accompanied by crystal electric field calculations on the polycrystalline sample of Ba3RB9O18 (R = Yb, Er) in which R3+ ions form a perfect triangular lattice without anti-site disorder. The localized R3+ spins show neither long-range order nor spin-glass state down to 1.9 K in Ba3RB9O18. Magnetization data reveal a pseudospin Jeff = 1/2 ( Yb3+) in the Kramers doublet state and a weak antiferromagnetic interaction between Jeff = 1/2 moments in the Yb variant. On the other hand, the effective moment μeff = 8.8 μB was obtained from the Curie-Weiss fit of the low-temperature susceptibility data of Er variant suggests the admixture of higher crystal electric field states with the ground state. The Curie-Weiss fit of low-temperature susceptibility data for Er system unveils the presence of a relatively strong antiferromagnetic interaction between Er3+ moments compared to its Yb3+ analog. Ba3ErB9O18 does not show long-range magnetic ordering down to 500 mK. Furthermore, our crystal electric field calculations based on magnetization data of Ba3ErB9O18 suggest the presence of a small gap between the ground and first excited Kramers doublets. The broad maximum around 4 K in magnetic specific heat in zero-field is attributed to the thermal population of the first CEF excited state in Ba3ErB9O18, which is consistent with our CEF calculations.
Axion domain wall baryogenesis
Creators: name: Daido, Ryuji
name: Kitajima, Naoya
name: Takahashi, Fuminobu
Publisher: name: arXiv
Year: 2015
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We propose a new scenario of baryogenesis, in which annihilation of axion domain walls generates a sizable baryon asymmetry. Successful baryogenesis is possible for a wide range of the axion mass and decay constant, $m \simeq 10^8 -10^{13}$ GeV and $f \simeq 10^{13} - 10^{16}$ GeV. Baryonic isocurvature perturbations are significantly suppressed in our model, in contrast to various spontaneous baryogenesis scenarios in the slow-roll regime. In particular, the axion domain wall baryogenesis is consistent with high-scale inflation which generates a large tensor-to-scalar ratio within the reach of future CMB B-mode experiments. We also discuss the gravitational waves produced by the domain wall annihilation and its implications for the future gravitational wave experiments.
description: 25 pages, 3 figures; v2: accepted for publication in JCAP
SupplementaryFigures.pdf from Nutrients and flow shape the cyclic dominance games between Escherichia coli strains
Creators: name: Kuhn, Thierry
name: Pilar, Junier
name: Bshary, Redouan
name: Terrettaz, Céline
name: Gonzalez, Diego
name: Richter, Xiang-Yi Li
Publisher: name: The Royal Society
Year: 2023
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: Evolutionary Biology
subject: Ecology
subject: 60102 Bioinformatics
subject: FOS: Computer and information sciences
subject: Computational Biology
subject: 10202 Biological Mathematics
subject: FOS: Mathematics

description: Supplementary figures
Detection of Yarkovsky acceleration in the context of precovery observations and the future Gaia catalogue
Creators: name: Desmars, Josselin
Publisher: name: arXiv
Year: 2015
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: The Yarkovsky effect is a weak non-gravitational force leading to a small variation of the semi-major axis of an asteroid. Using radar measurements and astrometric observations, it is possible to measure a drift in semi-major axis through orbit determination. This paper aims to detect a reliable drift in semi-major axis of near-Earth asteroids (NEAs) from ground-based observations and to investigate the impact of precovery observations and the future Gaia catalogue in the detection of a secular drift in semi-major axis. We have developed a precise dynamical model of an asteroid's motion taking the Yarkovsky acceleration into account and allowing the fitting of the drift in semi-major axis. Using statistical methods, we investigate the quality and the robustness of the detection. By filtering spurious detections with an estimated maximum drift depending on the asteroid's size, we found 46 NEAs with a reliable drift in semi-major axis in good agreement with the previous studies. The measure of the drift leads to a better orbit determination and constrains some physical parameters of these objects. Our results are in good agreement with the 1/D dependence of the drift and with the expected ratio of prograde and retrograde NEAs. We show that the uncertainty of the drift mainly depends on the length of orbital arc and in this way we highlight the importance of the precovery observations and data mining in the detection of consistent drift. Finally, we discuss the impact of Gaia catalogue in the determination of drift in semi-major axis.
description: 11 pages, 5 figures, accepted in A&A
Majorana bound states with chiral magnetic textures
Creators: name: Güngördü, Utkan
name: Kovalev, Alexey A.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Superconductivity (cond-mat.supr-con)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: The aim of this Tutorial is to give a pedagogical introduction into realizations of Majorana fermions, usually termed as Majorana bound states (MBS), in condensed matter systems with magnetic textures. We begin by considering the Kitaev chain model of 'spinless' fermions and show how two 'half' fermions can appear at chain ends due to interactions. By considering this model and its two-dimensional generalization, we emphasize intricate relation between topological superconductivity and possible realizations of MBS. We further discuss how 'spinless' fermions can be realized in more physical systems, e.g., by employing the spin-momentum locking. Next, we demonstrate how magnetic textures can be used to induce synthetic or fictitious spin-orbit interactions, and, thus, stabilize MBS. We describe a general approach that works for arbitrary textures and apply it to skyrmions. We show how MBS can be stabilized by elongated skyrmions, certain higher order skyrmions, and chains of skyrmions. We also discuss how braiding operations can be performed with MBS stabilized on magnetic skyrmions. This Tutorial is aimed at students at graduate level.
description: 18 pages, 21 figures
Bioenergy cropping systems of tomorrow
Creators: name: Von Cossel, Moritz
name: Wagner, Moritz
name: Lask, Jan
name: Magenau, Elena
name: Bauerle, Andrea
name: Von Cossel, Viktoria
name: Warrach-Sagi, Kirsten
name: Elbersen, Berien
name: Staritsky, Igor
name: Van Eupen, Michiel
name: Iqbal, Yasir
name: Jablonowski, Nicolai David
name: Happe, Stefan
name: Fernando, Ana Luisa
name: Scordia, Danilo
name: Cosentino, Salvatore Luciano
name: Wulfmeyer, Volker
name: Lewandowski, Iris
name: Winkler, Bastian
Publisher: name: Zenodo
Year: 2020
Subjects: agrobiodiversity
bioeconomy
bioenergy
biomass production
castor bean
climate change
climate change adaptation
climate change mitigation
cropping system
cup plant
diversification
erosion mitigation
groundwater protection
growth suitability
industrial crop
marginal agricultural land
marginal land
miscanthus
perennial crop
precipitation
resilience
social-ecological sustainability
temperature sum
wild plant
wild plant mixture

description: The research objective of this study is the development of long-term sustainable Marginal Agricultural Land Low-Input Systems for industrial crop cultivation. And the research question of this study is: How bioenergy cropping systems of tomorrow could be made more sustainable under social-ecological terms. It was found that there are five main requirements for the development of social-ecologically more sustainable bioenergy cropping systems. And here, four of them are presented and discussed.
description: This research received funding from the European Union's Horizon 2020 research and innovation programme under grant agreement No 727698 and the University of Hohenheim. N.D.J. received funding from the Bioeconomy Science Center (BioSC), supported in the project AP3 Focus Lab. The scientific activities of the Bioeconomy Science Center were financially supported by the Ministry of Innovation, Science and Research within the framework of the NRW Strategieprojekt BioSC (no. 313/323‐400‐002 13).
description: {"references": ["https://www.mdpi.com/1996-1073/12/16/3123", "https://www.mdpi.com/2073-4395/9/10/605", "https://onlinelibrary.wiley.com/doi/10.1002/adsu.202000037", "https://link.springer.com/article/10.1007/s12155-015-9690-2"]}
Creating an Open-source Hardware Ecosystem for Research and Sustainable Development
Creators: name: Sanli Faez
name: Urra, Jose
name: Saggiomo, Vittorio
name: De Vos, Jerry
name: Illamparuthi, Santosh
Publisher: name: Zenodo
Year: 2023
Subjects: Open Hardware
Open Source Hardware

description: At the core of education, engineering, and science lies the quest to better understand and improve the world. This document aims to explain the essential role of open-source hardware for this mission and why it should be considered an essential pillar of the ongoing open science programmes in Dutch Universities. Open-source hardware is hardware whose design is made publicly available so that anyone can study, modify, distribute, make, and sell the design or other hardware and products based on that design. Ideally, the design of open source hardware is available in the preferred format for making modifications and uses widely available components and materials, standard processes, open infrastructure, unrestricted content, and open-source design tools to maximize the ability of other individuals to make and use hardware. Open-source hardware gives people the freedom to control their technology while sharing knowledge and encouraging commerce through the open exchange of (compatible) designs. Open Science practices are becoming the norm in academia, and are rightly encouraged by funders and policymakers of higher education. Open-source hardware is an essential pillar of Open Science. Sharing hardware designs openly both enables more people and teams to access it, and through encouraging replication it makes science more reproducible. But it is also an area of contention because of the exclusive knowledge transfer practices and (not always justified) confidentiality clauses in research partnerships or contract defaults.  Beyond academia, open hardware has the potential to radically transform science, education, and society by facilitating collaborative innovation and democratizing access to technology. It can massively accelerate the transition of an invention into a useful product, and simultaneously reduce costs and promote sustainable practices. By promoting open-source hardware initiatives, the Netherlands can solidify its position as a leader in Open Science and contribute to the global effort of achieving the sustainable development goals. 
Kitaev Chain with a Fractional Twist
Creators: name: Basa, Bora
name: La Nave, Gabriele
name: Phillips, Philip W.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: The topological non-triviality of insulating phases of matter is by now well understood through topological K-theory where the indices of the Dirac operators are assembled into topological classes. We consider in the context of the Kitaev chain a notion of a generalized Dirac operator where the associated Clifford algebra is centrally extended. We demonstrate that the central extension is achieved via taking rational operator powers of Pauli matrices that appear in the corresponding BdG Hamiltonian. Doing so introduces a pseudo-metallic component to the topological phase diagram within which the winding number is valued in $\mathbb Q$. We find that this phase hosts a mode that remains extended in the presence of weak disorder, motivating a topological interpretation of a non-integral winding number. We remark that this is in correspondence with Ref.[J. Differential Geom. 74(2):265-292] demonstrating that projective Dirac operators defined in the absence of spin$^\mathbb C$ structure have rational indices.
description: 8 pages, 4 figures
Potential Vorticity in the 1/60° Labrador Sea model
Creators: Pennelly, Clark
Publisher: name: University of Alberta Library
Year: 2023

The LAB60 simulation is a coupled ocean sea-ice model (NEMO) that uses grid refinement to achieve high resolution (1/60 of a degree) within the Labrador Sea. This video shows the surface relative vorticity from 2004 through the end of 2018.
CAD_bioreactor_top_view.pdf from Nutrients and flow shape the cyclic dominance games between Escherichia coli strains
Creators: name: Kuhn, Thierry
name: Pilar, Junier
name: Bshary, Redouan
name: Terrettaz, Céline
name: Gonzalez, Diego
name: Richter, Xiang-Yi Li
Publisher: name: The Royal Society
Year: 2023
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: Evolutionary Biology
subject: Ecology
subject: 60102 Bioinformatics
subject: FOS: Computer and information sciences
subject: Computational Biology
subject: 10202 Biological Mathematics
subject: FOS: Mathematics

description: CAD drawing of the mini-bioreactor – top view
Field-Assisted Sub-Terahertz Spin Pumping and Auto-Oscillation in NiO
Creators: name: Guo, Mingda
name: Cheng, Ran
Publisher: name: arXiv
Year: 2022
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: Spin pumping converting sub-terahertz electromagnetic waves to DC spin currents has recently been demonstrated in antiferromagnets (AFMs) with easy-axis magnetic anisotropy. However, easy-plane AFMs such as NiO, which are easier to prepare experimentally, are considered to be bad candidates for spin pumping because the Néel vector oscillation is linearly polarized, placing a major restriction on the material choice for practical applications. Through a case study of NiO, we show that an applied magnetic field below the spin-flop transition can substantially modify the polarization of the resonance eigenmodes, which enables coherent sub-terahertz spin pumping as strong as that in easy-axis AFMs. In addition, we find that an applied magnetic field can significantly reduce the threshold of Néel vector auto-oscillation triggered by spin-transfer torques. These prominent field-assisted effects can greatly facilitate spintronic device engineering in the sub-terahertz frequency regime.
Supplementary document for Noncollinear, inelastic four-wave mixing in the extreme ultraviolet - 6593183.pdf
Creators: name: Mincigrucci, Riccardo
name: Cannizzo, Andrea
name: capotondi, flavio
name: Cinquegrana, Paolo
name: Cucini, Riccardo
name: Dallari, Francesco
name: Danailov, M
name: de Ninno, Giovanni
name: Di Mitri, Simone
name: Feurer, Thomas
Publisher: name: Optica Publishing Group
Year: 2023
Subjects: Uncategorized

description: Supplementary document
Spacetime evolution during moduli stabilization in radiation dominated era beyond 4D effective theory
Creators: name: Otsuka, Hajime
name: Sakamura, Yutaka
Publisher: name: arXiv
Year: 2022
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We investigate the time evolution of the background spacetime during the moduli stabilization process, which is assumed to occur in the radiation dominated era. The setup is basically the Salam-Sezgin model, but we add a potential term for the dilaton in order to stabilize the moduli completely. We numerically solve the higher-dimensional background field equations, including a case that the stabilization process cannot be described within the 4D effective theory. In contrast to the conventional 4D effective theory analysis, we find that when the mass scale of the stabilization is larger than the compactification scale, the radiation contribution to the total energy density remains to be non-negligible for a much longer time than the stabilization time scale. As a result, the non-compact 3D space expands slower than the matter dominated universe. We also find the equation of state for the radiation $w_{\rm rad}$ remains to be smaller than 1/3 for a long time, which indicates that the radiation still feels the extra dimensions for a while even after the moduli are stabilized.
description: 28 pages, 14 figures, v2: published version
ผลสัมฤทธ์ิของการใช้สื่อการสอนอิเล็กทรอนิกส์ รายวิชา THA 106 ในหัวข้อเรื่อง การเขียนย่อหน้า
Creators: name: จิรพร รักษาพล
Publisher: name: ศูนย์สนับสนุนและพัฒนาการเรียนการสอน มหาวิทยาลัยรังสิต
Year: 2012
Subjects: e-Learning
e-Learning Media Instruction
Learning Achievement
Paragraph Writing
การเขียนย่อหน้า
การใช้สื่อการสอนอิเล็กทรอนิกส์
ผลสัมฤทธิ์
อีเลิรน์นิ่ง

description: วารสารพัฒนาการเรียนการสอน, 6, 2, 39-55
21st Century Skills of Secondary School Principals in Nakhorn Nayok, thailand
Creators: name: Pada, Willard Jeff Villablanca
name: Doctor, Teresita
Publisher: name: figshare
Year: 2020
Subjects: subject: 130304 Educational Administration, Management and Leadership
subject: FOS: Educational sciences

description: Assessment of 21st Century Skills quotient of principals in secondary schools , descriptive -quantitative method of research, data was collected with the permission of the ministry of education and the principals in Nakhorn Nayok thailand