cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Multi-neutron transfer coupling in sub-barrier 32S+90,96Zr fusion reactions
Creators: name: Richard, A.
name: Beck, C.
name: Zhang, H. Q.
Publisher: name: arXiv
Year: 2011
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: The role of neutron transfers is investigated in the fusion process below the Coulomb barrier by analyzing 32S+90Zr and 32S+96Zr as benchmark reactions. A full coupled-channel calculation of the fusion excitation functions has been performed for both systems by using multi-neutron transfer coupling for the more neutron-rich reaction. The enhancement of fusion cross sections for 32S+96Zr is well reproduced at sub-barrier energies by NTFus code calculations including the coupling of the neutron-transfer channels following the Zagrebaev semiclassical model. We found similar effects for 40Ca+90Zr and 40Ca+96Zr fusion excitation functions.
description: Minor corrections, 11 pages, 4 figures, Fusion11 Conference, Saint Malo, France, 2-6 mai 2011
Tunable correlation effects of magnetic impurities by the cubic Rashba spin-orbit couplings
Creators: name: Peng, Xiong-Tao
name: Lin, Fang
name: Chen, Liang
name: Li, Lin
name: Xu, Dong-Hui
name: Sun, Jin-Hua
Publisher: name: arXiv
Year: 2023
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We theoretically study the influence of the $k$-cubic Rashba spin-orbit coupling (SOC) on the correlation effects of magnetic impurities by combining the variational method and the Hirsch-Fye quantum Monte Carlo (HFQMC) simulations. Markedly different from the normal $k$-linear Rashba SOC, even a small cubic Rashba term can greatly alter the band structure and induce a Van Hove singularity in a wide range of energy, thus the single impurity local moment becomes largely tunable. The cubic Rashba SOC adopted in this work breaks the rotational symmetry, but the host material is still invariant under the operations $\mathcal{R}^z(π)$, $\mathcal{IR}^z(π/2)$, $\mathcal{M}_{xz}$, $\mathcal{M}_{yz}$, where $\mathcal{R}^z(θ)$ is the rotation of angle $θ$ about the $z$-axis, $\mathcal{I}$ is the inversion operator and $\mathcal{M}_{xz}$ ($\mathcal{M}_{yz}$) is the mirror reflection about the $x$-$z$ ($y$-$z$) principal plane. Saliently, various components of spin-spin correlation between the single magnetic impurity and the conduction electrons show three- or six-fold rotational symmetry. This unique feature is due to the triple winding of the spins with a $2π$ rotation of $\mathbf{k}$, which is a hallmark of the cubic Rashba effect and can possibly be an identifier to distinguish the cubic Rashba SOC from the normal $k$-linear Rashba term in experiments. Although the cubic Rashba term drastically alters the electronic properties of the host, we find that the spatial decay rate of the spin-spin correlation function remains essentially unchanged. Moreover, the carrier-mediated Ruderman-Kittel-Kasuya-Yosida interactions between two magnetic impurities show twisted features, the ferromagnetic diagonal terms dominate when two magnetic impurities are very close, but the off-diagonal terms become important at long distances.
description: 11 pages, 10 figures
New and consolidated therapeutic options for pubertal induction in hypogonadism: in-depth review of the literature - Supplementary Tables
Creators: name: Federici, Silvia
name: Goggi, Giovanni
name: Quinton, Richard
name: Giovanelli, Luca
name: Persani, Luca
name: Cangiano, Biagio
name: Bonomi, Marco
Publisher: name: Zenodo
Year: 2021

description: Supplementary Materials for "New and consolidated therapeutic options for pubertal induction in hypogonadism: in-depth review of the literature"
First Measurement of the Cross Section for Top-Quark Pair Production in Proton-Proton Collisions at sqrt(s)=7 TeV
Creators: name: CMS Collaboration
Publisher: name: arXiv
Year: 2010
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: The first measurement of the cross section for top-quark pair production in pp collisions at the LHC at center-of-mass energy sqrt(s)= 7 TeV has been performed using 3.1 {\pm} 0.3 inverse pb of data recorded by the CMS detector. This result utilizes the final state with two isolated, highly energetic charged leptons, large missing transverse energy, and two or more jets. Backgrounds from Drell-Yan and non-W/Z boson production are estimated from data. Eleven events are observed in the data with 2.1 {\pm} 1.0 events expected from background. The measured cross section is 194 {\pm} 72 (stat.) {\pm} 24 (syst.) {\pm} 21 (lumi.) pb, consistent with next-to-leading order predictions.
Poster - MIDA Kick-Off Meeting March 2019
Creators: name: Debargue Audrey
Publisher: name: Zenodo
Year: 2022
Subjects: ITN MIDA
POSTER
KICK-OFF MEETING
ISLAM
SOCIAL SCIENCES
GRAPHIC DESIGN

description: KICK-OFF MEETING 23rd March 2019 from 9:00 am to 6:30 pm Dear Members and Participants, Dear Ladies and Gentlemen, Welcome to the kick- off meeting of the European Innovative Training Network : MEDIATING ISLAM IN THE DIGITAL AGE
Simulation of CH$_3$OH ice UV photolysis under laboratory conditions
Creators: name: Rocha, W. R. M.
name: Woitke, P.
name: Pilling, S.
name: Thi, W. -F.
name: Jørgensen, J. K.
name: Kristensen, L. E.
name: Perotti, G.
name: Kamp, I.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Chemical Physics (physics.chem-ph)
subject: FOS: Physical sciences

description: Methanol is the most complex molecule securely identified in interstellar ices and is a key chemical species for understanding chemical complexity in astrophysical environments. Important aspects of the methanol ice photochemistry are still unclear such as the branching ratios and photo-dissociation cross-sections at different temperatures and irradiation fluxes. This work aims at a quantitative agreement between laboratory experiments and astrochemical modelling of the CH3OH ice UV photolysis. This work also allows us to better understand which processes govern the methanol ice photochemistry present in laboratory experiments. We use ProDiMo to simulate the conditions of laboratory measurements. The simulations start with simple chemistry consisting only of methanol ice and helium to mimic the residual gas in the experimental chamber. A surface chemical network enlarged by photo-dissociation reactions is used to study the chemical reactions within the ice. Additionally, different surface chemistry parameters (surface competition, tunnelling, thermal diffusion and reactive desorption) are adopted to check those that reproduce the experimental results. The chemical models with ProDiMo can reproduce the methanol ice destruction via UV photodissociation at temperatures of 20, 30, 50 and 70 K as observed in the experiments. We note that the results are sensitive to different branching ratios after photolysis and to the mechanisms of reactive desorption. In the simulations of a molecular cloud at 20 K, we observed an increase in the methanol gas abundance of one order of magnitude, with a similar decrease in the solid-phase abundance. Comprehensive astrochemical models provide new insights into laboratory experiments as the quantitative understanding of the processes that govern the reactions within the ice. Ultimately, those insights can help to better interpret astronomical observations.
description: Accepted for publication in A&A on 08-Feb-2023
General moments of the inverse real Wishart distribution and orthogonal Weingarten functions
Creators: name: Matsumoto, Sho
Publisher: name: arXiv
Year: 2010
Subjects: subject: Statistics Theory (math.ST)
subject: Representation Theory (math.RT)
subject: FOS: Mathematics

description: Let $W$ be a random positive definite symmetric matrix distributed according to a real Wishart distribution and let $W^{-1}=(W^{ij})_{i,j}$ be its inverse matrix. We compute general moments $\mathbb{E} [W^{k_1 k_2} W^{k_3 k_4} ... W^{k_{2n-1}k_{2n}}]$ explicitly. To do so, we employ the orthogonal Weingarten function, which was recently introduced in the study for Haar-distributed orthogonal matrices. As applications, we give formulas for moments of traces of a Wishart matrix and its inverse.
description: 29 pages. The last version differs from the published version, but it includes Appendix
title: Camus’s Kierkegaardian Conception of a Good Life
Creators: name: Abel, Johannes
Publisher: name: Albert Camus Society
Year: 2019

description: The aim of this paper is to show, against contemporary comparative research, that Albert Camus' position in The Myth of Sisyphus does not correspond to the 'aesthetic stage' in the works of Søren Kierkegaard, but is structurally very close to Kierkegaard's own conception of a good life – in terms of methodology, relating to metaphysical truth via negation, the role of death, and the necessity of translation. In Camus, we see what a Kierkegaardian conception of a good life turns into when its foundational religious layer breaks away.
Herschel-ATLAS: counterparts from the UV--NIR in the science demonstration phase catalogue
Creators: name: Smith, D. J. B.
name: Dunne, L.
name: Maddox, S. J.
name: Eales, S.
name: Bonfield, D. G.
name: Jarvis, M. J.
name: Sutherland, W.
name: Fleuren, S.
name: Rigby, E. E.
name: Thompson, M. A.
name: Baldry, I. K.
name: Bamford, S.
name: Buttiglione, S.
name: Cava, A.
name: Clements, D.
name: Cooray, A
name: Croom, S.
name: Dariush, A.
name: de Zotti, G.
name: Driver, S. P.
name: Dunlop, J. S.
name: Fritz, J.
name: Hill, D. T.
name: Hopkins, A.
name: Hopwood, R.
name: Ibar, E.
name: Ivison, R. J.
name: Jones, D. H.
name: Kelvin, L.
name: Leeuw, L.
name: Liske, J.
name: Loveday, J.
name: Madore, B. F.
name: Norberg, P.
name: Panuzzo, P.
name: Pascale, E.
name: Pohlen, M.
name: Popescu, C. C.
name: Prescott, M.
name: Robotham, A.
name: Rodighiero, G.
name: Scott, D.
name: Seibert, M.
name: Sharp, R.
name: Temi, P.
name: Tuffs, R. J.
name: van der Werf, P.
name: van Kampen, E.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We present a technique to identify optical counterparts of 250 um-selected sources from the Herschel-ATLAS survey. Of the 6621 250 um > 32 mJy sources in our science demonstration catalogue we find that ~60 percent have counterparts brighter than r=22.4 mag in the Sloan Digital Sky Survey. Applying a likelihood ratio technique we are able to identify 2423 of the counterparts with a reliability R > 0.8. This is approximately 37 percent of the full 250 micron catalogue. We have estimated photometric redshifts for each of these 2423 reliable counterparts, while 1099 also have spectroscopic redshifts collated from several different sources, including the GAMA survey. We estimate the completeness of identifying counterparts as a function of redshift, and present evidence that 250 um-selected Herschel-ATLAS galaxies have a bimodal redshift distribution. Those with reliable optical identifications have a redshift distribution peaking at z ~ 0.25 +/- 0.05, while sub-mm colours suggest that a significant fraction with no counterpart above the r-band limit have z > 1. We also suggest a method for selecting populations of strongly-lensed high redshift galaxies. Our identifications are matched to UV--NIR photometry from the GAMA survey, and these data are available as part of the Herschel-ATLAS public data release.
description: 17 pages, 13 figures, MNRAS in press
A means-ends framework of acculturation
Creators: name: Vishkin Allon
name: Horenczyk Gabriel
name: Ben0Nun Bloom Pazit
Publisher: name: Zenodo
Year: 2021
Subjects: acculturation, motivation

description: A talk given to the International Association for Cross-Cultural Psychology, Virtual. IACCP
X-ray softening in the new X-ray transient XTE J1719-291 during its 2008 outburst decay
Creators: name: Padilla, M. Armas
name: Degenaar, N.
name: Patruno, A.
name: Russell, D. M.
name: Linares, M.
name: Maccarone, T. J.
name: Homan, J.
name: Wijnands, R.
Publisher: name: arXiv
Year: 2011
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The X-ray transient XTE J1719-291 was discovered with RXTE/PCA during its outburst in 2008 March, which lasted at least 46 days. Its 2-10 keV peak luminosity is 7E35 erg/s assuming a distance of 8 kpc, which classifies the system as a very faint X-ray transient. The outburst was monitored with Swift, RXTE, Chandra and XMM-Newton. We analysed the X-ray spectral evolution during the outburst. We fitted the overall data with a simple power-law model corrected for absorption and found that the spectrum softened with decreasing luminosity. However, the XMM-Newton spectrum can not be fitted with a simple one-component model, but it can be fitted with a thermal component (black body or disc black body) plus power-law model affected by absorption. Therefore, the softening of the X-ray spectrum with decreasing X-ray luminosity might be due to a change in photon index or alternatively it might be due to a change in the properties of the soft component. Assuming that the system is an X-ray binary, we estimated a long-term time-averaged mass accretion rate of ~ 7.7E-13 M_sun/yr for a neutron star as compact object and ~ 3.7E10-13 M_sun/yr in the case of a black hole. Although no conclusive evidence is available about the nature of the accretor, based on the X-ray/optical luminosity ratio we tentatively suggest that a neutron star is present in this system.
description: Accepted for publication in MNRAS. 8 pages, 4 figures, 2 tables
Detection of Gravitational memory effect in LISA using triggers from ground-based detectors
Creators: name: Ghosh, Sourath
name: Weaver, Alexander
name: Sanjuan, Jose
name: Fulda, Paul
name: Mueller, Guido
Publisher: name: arXiv
Year: 2023
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Data Analysis, Statistics and Probability (physics.data-an)
subject: FOS: Physical sciences

description: The LIGO-Virgo-Kagra (LVK) collaboration has detected gravitational waves from 90 Compact Binary Coalescences. In addition to fortifying the linearized theory of General Relativity (GR), the statistical ensemble of detections also provides prospects of detecting nonlinear effects predicted by GR, one such prediction being the nonlinear gravitational memory effect. For detected stellar and intermediate mass compact binaries, the induced strain from the memory effect is one or two orders below the detector noise background. Additionally, since most of the energy is radiated at merger the strain induced by the memory effect resembles a step function at the merger time. These facts motivate the idea of coherently stacking up data streams from recorded GW events at these merger times so that the cumulative memory strain is detected with a sufficient SNR. GW detectors essentially record the integrated strain response at time scales of the round trip light travel time, making future space-based long arm interferometers like LISA ideal for detecting the memory effect at low frequencies. In this paper, we propose a method that uses the event catalog of ground-based detectors and searches for corresponding memory strains in the LISA data stream. Given LVK's O3 science run catalog, we use scaling arguments and assumptions on the source population models to estimate the run time required for LISA to accumulate a memory SNR of 5, using triggers from current and future ground-based detectors. Finally, we extend these calculations for using beyond LISA missions like ALIA, AMIGO, and Folkner to detect the gravitational memory effect. The results for LISA indicate a possible detection of the memory effect within the 10 year LISA mission lifetime and the corresponding results for beyond LISA missions are even more promising.
Poster - MIDA Training Paris 2019 A practical approach to acquiring, curating and publishing textual and visual data in an Open Source environment
Creators: name: Debargue Audrey
name: Galluccio Giulia
name: Buresi Pascal
Publisher: name: Zenodo
Year: 2019
Subjects: ITN MIDA
POSTER
GRAPHIC DESIGN
SOCIAL SCIENCES
ISLAM

description: MIDA Training Paris 2019 10th Dec. 2019 - 12th Dec. 2019 InVisu A practical approach to acquiring, curating and publishing textual and visual data in an Open Source environment
Gamma-ray energies and intensities observed in decay chain $^{83}Rb$/$^{83m}Kr$/$^{83}Kr$
Creators: name: Šefčík, M.
name: Vénos, D.
name: Lebeda, O.
name: Noll, C.
name: Ráliš, J.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: Radioactive sources of the monoenergetic low-energy conversion electrons from the decay of isomeric $^{83m}Kr$ are frequently used in the systematic measurements, particularly in the neutrino mass and dark matter experiments. For this purpose, the isomer is obtained by the decay of its parent radionuclide $^{83}Rb$. In order to get more precise data on the gamma-rays occuring in the $^{83}Rb$/$^{83m}Kr$ chain, we re-measured the relevant gamma-ray spectra, because the previous measurement took place in 1976. The obtained intensities are in fair agreement with this previous measurement. We have, however, improved the uncertainties by a factor of 4.3, identified a new gamma transition and determined more precisely energies of weaker gamma transitions.
description: 4 pages, 3 figures
Human head-neck biomechanical response to an active anti-whiplash automotive seat
Creators: name: Partovi, Reza
Publisher: name: University of British Columbia
Year: 2022

description: Whiplash injuries remain the most common injury associated with rear-end low-speed collisions despite improvements in head restraint designs and the introduction of innovative anti-whiplash seats. To address this problem, our research group developed an active car seat (RoboSeat) that controls seat hinge rotation and seatback cushion deformation. Preliminary experiments showed that the RoboSeat could reduce the kinematic and kinetic responses of an anthropometric test device. The aim of this study was to compare the performance of an actively controlled experimental anti-whiplash (RoboSeat) seat to passive control anti-whiplash seats in human volunteers: General Motor’s High Retention seat (GMHR) & Volvo’s Whiplash Protection Seat (WHIPS). Twelve healthy participants were exposed to a whiplash-like perturbation (4km/h speed change) while seated on each of the three seats. We recorded the electromyographic activity of sternocleidomastoid, neck paraspinals, splenius capitis, and multifidus along with the head/torso kinematics to quantify the participants’ responses to the whiplash-like perturbations. Given that excessive strain in cervical facet capsules is suggested as a cause of whiplash injury, we quantified cervical multifidus activation while head retraction occurred because both factors can potentially increase strains in the capsular ligaments. We hypothesized that the dynamic seatback rotation and cushion deformation of the RoboSeat prevents simultaneous activation of the neck multifidus muscle and head retraction. The RoboSeat reduced the combined multifidus activation and head retraction by 76% and 43% as well as 12/16 and 6/16 kinematic variables compared to the GMHR and WHIPS seats, respectively. Overall, our results suggest that the active seat can lower some head/torso kinematic responses compared to the current anti-whiplash seats and minimize combined activation of the multifidus muscle and head retraction. Our active RoboSeat represents a promising approach to potentially decrease the risk of whiplash injuries following low-speed rear-end collisions.
Ab initio calculations of the $2p_{3/2} \rightarrow 2s$ transition in He-, Li-, and Be-like uranium
Creators: name: Malyshev, A. V.
name: Kozhedub, Y. S.
name: Shabaev, V. M.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Atomic Physics (physics.atom-ph)
subject: FOS: Physical sciences

description: The bound-state QED approach is applied to calculations of the $2p_{3/2} \rightarrow 2s$ transition energies in He-, Li-, and Be-like uranium. For U$^{90+}$ and U$^{89+}$, standard perturbation theory for a single level is employed, while the calculations of U$^{88+}$ have required its counterpart for quasidegenerate levels. The utilized approach merges the rigorous QED treatment up to the second order of perturbation theory with the higher-order electron-correlation contributions evaluated within the Breit approximation. The higher-order screened QED effects are estimated by means of the model-QED operator. The nuclear recoil, nuclear polarization, and nuclear deformation effects are taken into account as well. Along with the transition energies, their pairwise differences are calculated. The comprehensive analysis of the uncertainties due to uncalculated effects is carried out, and the most accurate theoretical predictions, which are in perfect agreement with available experimental data, are obtained.
description: 1 figure, 8 tables
On the finite inverse problem in iterative differential Galois theory
Creators: name: Maurischat, Andreas
Publisher: name: arXiv
Year: 2010
Subjects: subject: Commutative Algebra (math.AC)
subject: Algebraic Geometry (math.AG)
subject: FOS: Mathematics
subject: 12H20 (Primary), 12F15 (Secondary)

description: In positive characteristic, nearly all Picard-Vessiot extensions are inseparable over some intermediate iterative differential extensions. In the Galois correspondence, these intermediate fields correspond to nonreduced subgroup schemes of the Galois group scheme. Moreover, the Galois group scheme itself may be nonreduced, or even infinitesimal. In this article, we investigate which finite group schemes occur as iterative differential Galois group schemes over a given ID-field. For a large class of ID-fields, we give a description of all occuring finite group schemes.
description: 8 pages, v2: added "finite" in the title to be more precise. Changed some typos and also did some more explanations in some proofs
title: ÐÑÐ¾Ð±Ð»ÐµÐ¼Ð° Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ Ð²Ð·ÑÐ¾ÑÐ»ÑÑ Ð¸Ð½Ð¾ÑÑÑÐ°Ð½Ð½Ð¾Ð¼Ñ ÑÐ·ÑÐºÑ Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ Ð³ÑÐ°Ð¼Ð¼Ð°ÑÐ¸ÐºÐ¸ Ð½ÐµÐ¼ÐµÑÐºÐ¾Ð³Ð¾ ÑÐ·ÑÐºÐ° (Ð½Ð°ÑÐ°Ð»ÑÐ½ÑÐ¹ ÑÑÐ°Ð¿)
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
title: The problem of teaching adults a foreign language on the example of German grammar (for starters)
Creators: name: ÐÐ¸Ð»ÑÐºÐ¸, ÐÐ°ÑÐ°Ð»ÑÑ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2021
Subjects: Ð¿ÐµÐ´Ð°Ð³Ð¾Ð³Ð¸ÐºÐ°
Ð°Ð½Ð´ÑÐ¾Ð³Ð¾Ð³Ð¸ÐºÐ°
Ð·ÑÐµÐ»ÑÐ¹ ÑÐµÐ»Ð¾Ð²ÐµÐº
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Ð°Ð½Ð´ÑÐ¾Ð³Ð¾Ð³Ð¸ÑÐµÑÐºÐ°Ñ Ð¼Ð¾Ð´ÐµÐ»Ñ Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ
Ð³ÑÐ°Ð¼Ð¼Ð°ÑÐ¸ÐºÐ° Ð½ÐµÐ¼ÐµÑÐºÐ¾Ð³Ð¾ ÑÐ·ÑÐºÐ° Ð½Ð°ÑÐ°Ð»ÑÐ½ÑÐ¹ ÑÑÐ°Ð¿
pedagogy
androgogy
mature person
methods of teaching the second foreign language to adults
first FL
second FL
interference
transposition
androgogical model of learning
grammar of the German language for starters

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ñ Ð¾ÑÐ»Ð¸ÑÐ¸Ñ Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ Ð´ÐµÑÐµÐ¹ Ð¸ Ð²Ð·ÑÐ¾ÑÐ»ÑÑ Ð¿ÑÑÐµÐ¼ ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ñ Ð¿ÐµÐ´Ð°Ð³Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð¸ Ð°Ð½Ð´ÑÐ°Ð³Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð¼Ð¾Ð´ÐµÐ»ÐµÐ¹ Ð¾Ð±ÑÑÐµÐ½Ð¸Ñ. ÐÑÐ¿Ð¾Ð»Ð½ÐµÐ½ ÑÐ¾Ð¿Ð¾ÑÑÐ°Ð²Ð¸ÑÐµÐ»ÑÐ½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐ¸ÑÑÐµÐ¼ ÑÐ¾Ð½ÐµÑÐ¸ÐºÐ¸, Ð»ÐµÐºÑÐ¸ÐºÐ¸ Ð¸ Ð³ÑÐ°Ð¼Ð¼Ð°ÑÐ¸ÐºÐ¸ Ð°Ð½Ð³Ð»Ð¸Ð¹ÑÐºÐ¾Ð³Ð¾ Ð¸ Ð½ÐµÐ¼ÐµÑÐºÐ¾Ð³Ð¾ ÑÐ·ÑÐºÐ¾Ð². ÐÑÑÐ²Ð»ÐµÐ½Ñ ÑÐ»ÑÑÐ°Ð¸ Ð¸Ð½ÑÐµÑÑÐµÑÐµÐ½ÑÐ¸Ð¸ Ð¸ ÑÑÐ°Ð½ÑÐ¿Ð¾Ð·Ð¸ÑÐ¸Ð¸ Ð¿ÑÐ¸ Ð¾Ð±ÑÑÐµÐ½Ð¸Ð¸ Ð²ÑÐ¾ÑÐ¾Ð¼Ñ Ð¸Ð½Ð¾ÑÑÑÐ°Ð½Ð½Ð¾Ð¼Ñ ÑÐ·ÑÐºÑ.
description: The research is devoted to the differences between children's and adults' learning by comparing pedagogical and andragogical models of learning. A comparative analysis of the phonetic systems, vocabulary, and grammar of English and German is performed. Cases of interference and transposition in teaching a second foreign language have been identified.
High precision numerical sequences of rotating hairy black holes
Creators: name: García, Gustavo
name: Gourgoulhon, Eric
name: Grandclément, Philippe
name: Salgado, Marcelo
Publisher: name: arXiv
Year: 2023
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We analyze numerically the existence of regular stationary rotating hairy black holes within the framework of general relativity, which are the result of solving the Einstein-Klein-Gordon system for a complex-valued scalar field under suitable boundary (regularity and asymptotically flat) conditions. To that aim we solve the corresponding system of elliptic partial differential equations using spectral methods which are specially suited for such a numerical task. In order to obtain such system of equations we employ a parametrization for the metric that corresponds to quasi-isotropic coordinates (QIC) that have been used in the past for analyzing different kinds of stationary rotating relativistic systems. Our findings are in agreement with those reported originally by Herdeiro \& Radu ite{Herdeiro2014,Herdeiro2015}. The method is submitted to several analytic and numerical tests, which include the recovery of the Kerr solution in QIC and the cloud solutions in the Kerr background. We report different global quantities that allow us to determine the contribution of the boson hair to the spacetime, as well as relevant quantities at the horizon, like the surface gravity. The latter indicates to what extent the hairy solutions approach the extremal limit, noting that for this kind of solutions the ratio of the angular momentum per squared mass $J_\infty/M^2_{\rm ADM}$ can be larger than unity due to the contribution of the scalar hair, a situation which differs from the Kerr metric where this parameter is bounded according to $0\leq |J/M^2| \leq 1$ with the upper bound corresponding to the extremal case.
description: 28 pages, 36 figures
Bulk viscosity coefficients due to phonons and kaons in superfluid color-flavor locked quark matter
Creators: name: Bierkandt, Robert
name: Manuel, Cristina
Publisher: name: arXiv
Year: 2011
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We evaluate the three bulk viscosity coefficients $ζ_1, ζ_2$ and $ζ_3$ in the color-flavor locked (CFL) superfluid phase due to phonons and kaons, which are the lightest modes in that system. We first show that the computation is rather analogous to the computation of the same coefficients in superfluid $^4$He, as due to phonons and rotons. For astrophysical applications, we also find the value of the viscosities when there is a periodic disturbance, and the viscosities also depend on the frequency of the disturbance. In a temperature regime that might be of astrophysical relevance, we find that the contributions of both the phonons and kaons should be considered, and that $ζ_2$ is much less that the same coefficient in unpaired quark matter
description: 13 pages, 6 figures; Explanations and one reference added; version to be published in Phys. Rev. D
Resolution of Infrared Divergences in Gluon-Gluon Scattering Regulated on a Lightcone Worldsheet Lattice
Creators: name: Thorn, Charles B.
Publisher: name: arXiv
Year: 2010
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We improve and update the discussion, given some years ago by my collaborators and me, of infrared divergences and Bremsstrahlung in one-loop gluon scattering probabilities in lightcone gauge. In that work, we showed that adding soft and collinear gluon radiation, satisfying simple Lorentz invariant constraints, not only cancelled all IR divergences, but resulted in compact expressions for the consequent scattering probabilities. Here we impose less restrictive (albeit noncovariant) constraints on the unobserved radiation, which increases the high energy (s) fixed momentum transfer (t) behavior of the total probabilities from -ln^2s to ln s ln t, a behavior shared by the (IR divergent) elastic probabilities. Using this new treatment we also make a much more detailed comparison of the lightcone results to covariant calculations using dimensional regularization, finding complete agreement between the two styles of calculation.
description: 14 pages, 1 figure
title: ÐÐµÑÐµÐ²Ð¾Ð´ Ð¸Ð¼ÑÐ½ ÑÐ¾Ð±ÑÑÐ²ÐµÐ½Ð½ÑÑ Ð² ÑÐ¾Ð¼Ð°Ð½Ðµ Ð§. ÐÐ¸ÐºÐºÐµÐ½ÑÐ° "ÐÐ¾ÑÐ¼ÐµÑÑÐ½ÑÐµ Ð·Ð°Ð¿Ð¸ÑÐºÐ¸ ÐÐ¸ÐºÐ²Ð¸Ð½ÑÐºÐ¾Ð³Ð¾ ÐºÐ»ÑÐ±Ð°"
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
title: Translation of proper names in the novel "Posthumous Notes of the Pickwine Club" by Charles Dickens
Creators: name: ÐÐ¾ÑÑÑÐ½Ð¾Ð²Ð°, ÐÑÐµÐ½Ð¸Ñ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2021
Subjects: Ð¸Ð¼Ñ ÑÐ¾Ð±ÑÑÐ²ÐµÐ½Ð½Ð¾Ðµ
Ð°Ð½ÑÑÐ¾Ð¿Ð¾Ð½Ð¸Ð¼
Ñ ÑÐ´Ð¾Ð¶ÐµÑÑÐ²ÐµÐ½Ð½ÑÐ¹ Ð¿ÐµÑÐµÐ²Ð¾Ð´
ÑÑÐ°Ð½ÑÐ»Ð¸ÑÐµÑÐ°ÑÐ¸Ñ
ÑÑÐ°Ð½ÑÐºÑÐ¸Ð¿ÑÐ¸Ñ
proper name
anthroponym
literaly translation
transliteration
transcription

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð° Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ð° Ð¿ÐµÑÐµÐ²Ð¾Ð´Ð° Ð°Ð½ÑÑÐ¾Ð¿Ð¾Ð½Ð¸Ð¼Ð¾Ð² Ð² ÑÐ¾Ð¼Ð°Ð½Ðµ Ð§. ÐÐ¸ÐºÐºÐµÐ½ÑÐ° Â«ÐÐ¾ÑÐ¼ÐµÑÑÐ½ÑÐµ Ð·Ð°Ð¿Ð¸ÑÐºÐ¸ ÐÐ¸ÐºÐ²Ð¸ÐºÑÐºÐ¾Ð³Ð¾ ÐºÐ»ÑÐ±Ð°Â» Ñ Ð°Ð½Ð³Ð»Ð¸Ð¹ÑÐºÐ¾Ð³Ð¾ Ð½Ð° ÑÑÑÑÐºÐ¸Ð¹ ÑÐ·ÑÐº. Ð ÑÐ°Ð±Ð¾ÑÐµ Ð´Ð°ÐµÑÑÑ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ° Ð¾Ð±ÑÐ¸Ñ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼ Ð¿ÐµÑÐµÐ²Ð¾Ð´Ð° Ð¸Ð¼ÑÐ½ ÑÐ¾Ð±ÑÑÐ²ÐµÐ½Ð½ÑÑ Ð¸ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÑÑÑÑÑ ÑÐ¿Ð¾ÑÐ¾Ð±Ñ Ð¿ÐµÑÐµÐ´Ð°ÑÐ¸ Ð°Ð½Ð³Ð»Ð¸Ð¹ÑÐºÐ¸Ñ Ð¸Ð¼ÑÐ½ ÑÐ¾Ð±ÑÑÐ²ÐµÐ½Ð½ÑÑ Ð¸ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐµÐ¹ ÑÑÐ½ÐºÑÐ¸Ð¾Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¸Ð¼ÐµÐ½ ÑÐ¾Ð±ÑÑÐ²ÐµÐ½Ð½ÑÑ Ð² ÑÐ¾Ð¼Ð°Ð½Ðµ. ÐÑÐµÐ´Ð»Ð°Ð³Ð°ÐµÑÑÑ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ° Ð°Ð½ÑÑÐ¾Ð¿Ð¾Ð½Ð¸Ð¼Ð¾Ð² ÑÐ¾Ð¼Ð°Ð½Ð° Ð¸ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÑÑÑÑÑ ÑÑÑÐ°ÑÐµÐ³Ð¸Ð¸ Ð¸ Ð¿ÑÐ¸ÑÐ¼Ñ Ð¿ÐµÑÐµÐ²Ð¾Ð´Ð° Ð°Ð½ÑÑÐ¾Ð¿Ð¾Ð½Ð¸Ð¼Ð¾Ð² Ð² ÑÐ¾Ð¼Ð°Ð½Ðµ.
description: This work discusses the problems of English to Russian translation of the anthroponyms from Â«The Posthumous Papers of the Pickwick ClubÂ» by Ch. Dickens. The paper addresses the general problems of translating English proper names. The specificity of the proper names and their functions in the novel are analysed. The strategies and techniques for translating anthroponyms in the novel are provide.
Additional file 3 of Efficacy and safety of upadacitinib over 84 weeks in Japanese patients with rheumatoid arthritis (SELECT-SUNRISE)
Creators: name: Kameda, Hideto
name: Takeuchi, Tsutomu
name: Yamaoka, Kunihiro
name: Oribe, Motohiro
name: Kawano, Mitsuhiro
name: Yokoyama, Masayuki
name: Pangan, Aileen L.
name: Konishi, Yuko
name: Meerwein, Sebastian
name: Tanaka, Yoshiya
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Pharmacology
subject: Ecology
subject: FOS: Biological sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Additional file 3. Supplementary Table 1.
HF=HM I : Heegaard Floer homology and Seiberg--Witten Floer homology
Creators: name: Kutluhan, Cagatay
name: Lee, Yi-Jen
name: Taubes, Clifford Henry
Publisher: name: arXiv
Year: 2010
Subjects: subject: Geometric Topology (math.GT)
subject: Symplectic Geometry (math.SG)
subject: FOS: Mathematics

description: Let M be a closed, connected and oriented 3-manifold. This article is the first of a five part series that constructs an isomorphism between the Heegaard Floer homology groups of M and the corresponding Seiberg-Witten Floer homology groups of M.
description: 25 pages. This version includes a minor revision to Theorem 3.3
Improving the availability of fine-scale forest fuel and fire severity information using innovative remote sensing data
Creators: name: Arkin, Jeremy Benjamin
Publisher: name: University of British Columbia
Year: 2022

description: Due to climate change and historic land management practices, wildfires are becoming more prevalent, with increases in fire sizes, frequencies, and intensities. As a result, there is an increased need to accurately understand the environmental drivers of these wildfires, as well as their impacts. The primary objective of this dissertation was to meet this need by developing a suite of workflows that examine the utility provided by newly available remote sensing data that provide greater levels of detail than conventional data. This research was divided between pre- and post-fire management stages. The post-fire research questions evaluated the ability of remote sensing data acquired from cost-effective, remotely piloted aerial systems (RPAS) to create detailed pixel- and individual tree-based fire severity maps. The data used to produce these maps were acquired exclusively post-fire and included high resolution orthomosaics and dense digital aerial photogrammetric (DAP) point clouds. The pixel-based fire severity maps were produced at 5- and 1-meter resolutions using a supervised random forest classification approach, whereas the individual tree-approach estimated crown scorch height across segmented trees that were classified as having fire damage. The pre-fire questions were focused on characterizing the amount and arrangement of combustible fuels that drive wildfire behaviour, and did so at the plot- and individual tree-level. The plot-level approach estimated a full suite of canopy and surface fuel metrics that are commonly used in fire behaviour models. Due to the complex nature of these fuels, these estimations were carried out separately using RPAS-acquired light detection and ranging (LiDAR) and DAP point clouds, as well as ground-based mobile laser scanning (MLS) point clouds. The individual tree-based fuel characterizations were carried out by automatically segmenting and evaluating continuous portions of crown fuels from RPAS LiDAR point clouds and comparing against measurements collected from more detailed MLS point clouds. Through the investigation of these research questions, I provide detailed information that describes both the strengths and weaknesses of these data as well as a suite of methodologies that can be incorporated in conventional and next generation forest management frameworks.
Linear response of entanglement entropy to $T\bar{T}$ in massive QFTs
Creators: name: Ashkenazi, Shachar
name: Chakraborty, Soumangsu
name: Ma, Zhanyu
name: Shachar, Tom
Publisher: name: arXiv
Year: 2023
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We compute the leading correction to entanglement entropy in $T\bar{T}$ deformed massive QFTs. We show that both for massive scalar and Dirac fermion, the leading order correction to the entanglement entropy of half-space comes from the boundary of the entangling surface. For the case of massive scalar, the boundary term is finite while for massive fermion, it diverges logarithmically giving rise to an additional log-square divergence in the entanglement entropy.
description: 15 pages
Poster - MIDA Networkwide Activity x Campus Condorcet 16→24 SEPTEMBER 2021
Creators: name: Debargue Audrey
name: Galluccio Giulia
name: Buresi Pascal
Publisher: name: Zenodo
Year: 2021
Subjects: ITN MIDA
GRAPHIC DESIGN
ISLAM
CAMPUS CONDORCET

description: MIDA Networkwide Activity  Campus Condorcet 16→24 SEPTEMBER 2021
Energy response and spatial alignment of the perturbed electron gas
Creators: name: Dornheim, Tobias
name: Tolias, Panagiotis
name: Moldabekov, Zhandos
name: Vorberger, Jan
Publisher: name: arXiv
Year: 2023
Subjects: subject: Quantum Gases (cond-mat.quant-gas)
subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: We present extensive new \emph{ab initio} path integral Monte Carlo (PIMC) simulations of the harmonically perturbed uniform electron gas (UEG) for different densities and temperatures. This allows us to study the linear response of the UEG with respect to different contributions to the total energy for different wave numbers. We find that the induced change in the interaction energy exhibits a non-monotonic behaviour, and becomes negative for intermediate wave numbers. This effect is strongly dependent on the coupling strength and can be traced back to the spatial alignment of electrons introduced in earlier works [T.~Dornheim \emph{et al.}, Communications Physics \textbf{5}, 304 (2022)]. The observed quadratic dependence on the perturbation amplitude in the limit of weak perturbations and the quartic dependence of the perturbation amplitude corrections are consistent with linear and non-linear versions of the density stifness theorem. All PIMC simulation results are freely available online and can be used to benchmark new methods, or as input for other calculations.
Pressure-tunable magnetic topological phases in magnetic topological insulator MnSb4Te7
Creators: name: Gao, Lingling
name: Wu, Juefei
name: Xi, Ming
name: Pei, Cuiying
name: Wang, Qi
name: Zhao, Yi
name: Tian, Shangjie
name: Li, Changhua
name: Cao, Weizheng
name: Chen, Yulin
name: Lei, Hechang
name: Qi, Yanpeng
Publisher: name: arXiv
Year: 2023
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: Magnetic topological insulators, possessing both magnetic order and topological electronic structure, provides an excellent platform to research unusual physical properties. Here, we report a high-pressure study on the anomalous Hall effect of magnetic TI MnSb4Te7 through transports measurements combined with first-principle theoretical calculations. We discover that the ground state of MnSb4Te7 experiences a magnetic phase transition from the A-type antiferromagnetic state to ferromagnetic dominating state at 3.78 GPa, although its crystal sustains a rhombohedral phase under high pressures up to 8 GPa. The anomalous Hall conductance σxyA keeps around 10 Ω-1 cm-1, dominated by the intrinsic mechanism even after the magnetic phase transition. The results shed light on the intriguing magnetism in MnSb4Te7 and pave the way for further studies of the relationship between topology and magnetism in topological materials.
description: 10 pages, 4 figures
Particle and guiding-center orbits in crossed electric and magnetic fields
Creators: name: Brizard, Alain J.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Plasma Physics (physics.plasm-ph)
subject: FOS: Physical sciences

description: The problem of the charged-particle motion in crossed electric and magnetic fields is investigated, and the validity of the guiding-center representation is assessed in comparison with the exact particle dynamics. While the magnetic field is considered to be straight and uniform, the (perpendicular) radial electric field is nonuniform. The Hamiltonian guiding-center theory of charged-particle motion is presented for arbitrary radial electric fields, and explicit examples are provided for the case of a linear radial electric field.
description: 13 pages, 6 figures
New and consolidated therapeutic options for pubertal induction in hypogonadism: in-depth review of the literature (Supplementary Tables)
Creators: name: Federici, Silvia
name: Goggi, Giovanni
name: Quinton, Richard
name: Giovanelli, Luca
name: Persani, Luca
name: Cangiano, Biagio
name: Bonomi, Marco
Publisher: name: Zenodo
Year: 2021

description: Supplementary Tables for the paper "New and consolidated therapeutic options for pubertal induction in hypogonadism: in-depth review of the literature"
HST viewing of spectacular star-forming trails behind ESO 137-001
Creators: name: Waldron, William
name: Sun, Ming
name: Luo, Rongxin
name: Laudari, Sunil
name: Chatzikos, Marios
name: Sivanandam, Suresh
name: Kenney, Jeffrey D. P.
name: Jachym, Pavel
name: Voit, G. Mark
name: Donahue, Megan
name: Fossati, Matteo
Publisher: name: arXiv
Year: 2023
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We present the results from the HST WFC3 and ACS data on an archetypal galaxy undergoing ram pressure stripping (RPS), ESO 137-001, in the nearby cluster Abell 3627. ESO 137-001 is known to host a prominent stripped tail detected in many bands from X-rays, Halpha to CO. The HST data reveal significant features indicative of RPS such as asymmetric dust distribution and surface brightness as well as many blue young star complexes in the tail. We study the correlation between the blue young star complexes from HST, HII regions from Halpha (MUSE) and dense molecular clouds from CO (ALMA). The correlation between the HST blue star clusters and the HII regions is very good, while their correlation with the dense CO clumps are typically not good, presumably due in part to evolutionary effects. In comparison to the Starburst99+Cloudy model, many blue regions are found to be young (< 10 Myr) and the total star formation (SF) rate in the tail is 0.3 - 0.6 M_Sun/yr for sources measured with ages less than 100 Myr, about 40% of the SF rate in the galaxy. We trace SF over at least 100 Myr and give a full picture of the recent SF history in the tail. We also demonstrate the importance of including nebular emissions and a nebular to stellar extinction correction factor when comparing the model to the broadband data. Our work on ESO 137-001 demonstrates the importance of HST data for constraining the SF history in stripped tails.
description: 22 pages, 20 figures, 4 tables, published in MNRAS 06/2023
title: Fracture parameters for buried cast iron pipes subjected to internal and external corrosions and crackings
Creators: name: Akhi, Atika Hossain
Publisher: name: Memorial University of Newfoundland
Year: 2021

description: Cast iron water main represents a significant portion of municipal infrastructure in North America and worldwide. The aging cast-iron pipes are subjected to deterioration due to corrosion, resulting in cracking and failure. The municipalities face problems with pipe breakage or leakage and associated socio-economic issues caused by water loss, service disruption, and damages to the nearby facilities. For a proper maintenance decision of the pipes, it requires evaluating the remaining strength of the deteriorating structure. Fracture mechanics is being preferred to assess the remaining strength of the deteriorating structure over the conventional strength-based method due to its ability to capture crack initiation and propagation. However, determining fracture parameters, such as Stress Intensity Factor (SIF), is a challenge in applying the fracture mechanics for evaluating the structure. This study presents an evaluation of the SIF for buried cast iron pipes subjected to internal and external corrosions and cracks. Semi-elliptical surface defects (crack only and crack with corrosion) are considered for a wide range of aspect ratios (crack-depth to crack-length ratio) and relative crack depths (crack-depth to pipe thickness ratio) to evaluate the SIFs. The SIFs are assessed for invert/crown and springline position cracks under internal pressure and vertical surface loads. The study revealed that the SIF for a crack due to internal pressure is not affected by the presence of surrounding soil and therefore can be calculated using the available solution for in-air pipes. The SIF due to surface load depends on its geometry and location of the crack. A design equation is proposed to calculate the SIFs due to the surface load using an influence coefficient. The influence coefficient is presented for internal and external semi-elliptical defects as a function of crack aspect ratios, depths and locations. A method is proposed to determine the SIFs for buried pipes as a sum of the SIFs due to the internal pressure and the surface loads.
Integration by parts: An introduction
Creators: name: Grozin, A. G.
Publisher: name: arXiv
Year: 2011
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Integration by parts is used to reduce scalar Feynman integrals to master integrals.
description: Lectures at CAPP-2011 (Zeuthen), 47 p; v2: small improvements, references added; v3: small improvements, 1 reference added; v4: a few typos in formulas fixed
Investigating the superorbital modulations in 4U 1909+07, IGR J16418-4532 and IGR J16479-4514 with Swift XRT, BAT and NuSTAR observations
Creators: name: Islam, Nazma
name: Corbet, Robin H. D.
name: Coley, Joel B.
name: Pottschmidt, Katja
name: Fuerst, Felix
Publisher: name: arXiv
Year: 2023
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: A puzzling variety of superorbital modulations have been discovered in several supergiant High-Mass X-ray binaries (sgHMXBs). To investigate the mechanisms driving these superorbital modulations, we have analyzed long-term Neil Gehrels Swift Observatory (Swift) Burst Alert Telescope (BAT) observations of three sgHMXBs: 4U 1909+07, IGR J16418-4532 and IGR J16479-4514 and constructed their dynamic power spectra and superorbital intensity profiles. These Swift BAT observations are complemented by pointed Swift X-ray Telescope (XRT) and Nuclear Spectroscopic Telescope Array (NuSTAR) observations performed near the predicted maximum and minimum phase of a single superorbital cycle for each of these sources. The BAT dynamic power spectra show changes in the strength of the superorbital modulation on timescales of years, with either the peak at the fundamental frequency and/or the second harmonic present at different times for all three sources. The pointed Swift XRT and NuSTAR observations show no significant differences between the pulse profiles and spectral parameters at the superorbital maximum and minimum phase. This is likely due to the fact the superorbital modulation had weakened significantly during the times when the NuSTAR observations were carried out for all three sources. The results from the Swift XRT, BAT and NuSTAR analysis indicate the possible presence of multiple co-rotating interaction regions (CIRs) in the stellar winds of the supergiant stars, although a structured stellar wind from the supergiant star due to tidal oscillations cannot be ruled out.
description: Accepted for publication in the Astrophysical Journal
Additional file 2 of Efficacy and safety of upadacitinib over 84 weeks in Japanese patients with rheumatoid arthritis (SELECT-SUNRISE)
Creators: name: Kameda, Hideto
name: Takeuchi, Tsutomu
name: Yamaoka, Kunihiro
name: Oribe, Motohiro
name: Kawano, Mitsuhiro
name: Yokoyama, Masayuki
name: Pangan, Aileen L.
name: Konishi, Yuko
name: Meerwein, Sebastian
name: Tanaka, Yoshiya
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Pharmacology
subject: Ecology
subject: FOS: Biological sciences
subject: Immunology
subject: FOS: Clinical medicine
subject: 110309 Infectious Diseases
subject: FOS: Health sciences

description: Additional file 2. Supplementary Text 1.
Spectroscopic signatures of tetralayer graphene polytypes
Creators: name: McEllistrim, Andrew
name: Garcia-Ruiz, Aitor
name: Goodwin, Zachary A. H.
name: Fal`ko, Vladimir I.
Publisher: name: arXiv
Year: 2023
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: Tetralayer graphene has recently become a new addition to the family of few-layer graphene with versatile electronic properties. This material can be realised in three distinctive stacking configurations, for which we determine spectroscopic signatures in angle-resolved photoemission spectroscopy (ARPES), dynamical optical conductivity, and Raman spectra of inter-band excitations. The reported library of spectral features of tetralayer graphenes can be used for the non-invasive identification of the stacking order realised in a particular film.
description: Pages 11, figures 7