cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: ÐÐ¿Ð¿ÑÐ¾ÐºÑÐ¸Ð¼Ð°ÑÐ¸Ñ ÑÑÐ°Ð½Ð´Ð°ÑÑÐ½Ð¾Ð¹ Ð±Ð¸Ð±Ð»Ð¸Ð¾ÑÐµÐºÐ¸ ÑÐ·ÑÐºÐ° C ÑÑÐµÐ´ÑÑÐ²Ð°Ð¼Ð¸ ÑÐ·ÑÐºÐ° LibSL
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: C standatd library approximation with LibSL language resources
Creators: name: ÐÐ½ÑÑÐ½Ð¾Ð²Ð¸Ñ, ÐÐ°Ð²ÐµÐ»
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: 2023
Subjects: Ð°Ð¿Ð¿ÑÐ¾ÐºÑÐ¸Ð¼Ð°ÑÐ¸Ñ
ÑÐ¾ÑÐ¼Ð°Ð»ÑÐ½Ð°Ñ ÑÐ¿ÐµÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¸Ñ
ÑÑÐ°Ð½Ð´Ð°ÑÑÐ½Ð°Ñ Ð±Ð¸Ð±Ð»Ð¸Ð¾ÑÐµÐºÐ° C
Ð³ÐµÐ½ÐµÑÐ°ÑÐ¸Ñ ÐºÐ¾Ð´Ð°
ÑÑÐ°ÑÐ¸ÑÐµÑÐºÐ¸Ð¹ Ð°Ð½Ð°Ð»Ð¸Ð·
cpproximation
formal specification
C standard library
code generation
static analysis

description: ÐÐ°Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° Ð½Ð°Ð¿Ð¸ÑÐ°Ð½Ð¸Ñ Ð°Ð¿Ð¿ÑÐ¾ÐºÑÐ¸Ð¼Ð°ÑÐ¸Ð¸ ÑÑÐ°Ð½Ð´Ð°ÑÑÐ½Ð¾Ð¹ Ð±Ð¸Ð±Ð»Ð¸Ð¾ÑÐµÐºÐ¸ C Ð½Ð° ÑÐ·ÑÐºÐµ ÑÐ¾ÑÐ¼Ð°Ð»ÑÐ½ÑÑ ÑÐ¿ÐµÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¹ LibSL. ÐÑÐ»Ð¸ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÐµ Ð¿Ð¾Ð´ÑÐ¾Ð´Ñ Ðº Ð½Ð°Ð¿Ð¸ÑÐ°Ð½Ð¸Ñ ÑÐ¾ÑÐ¼Ð°Ð»ÑÐ½ÑÑ ÑÐ¿ÐµÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¹, ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° ÑÐ¿ÐµÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¸Ñ ÑÑÐ°Ð½Ð´Ð°ÑÑÐ½Ð¾Ð¹ Ð±Ð¸Ð±Ð»Ð¸Ð¾ÑÐµÐºÐ¸, ÑÐ¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½ Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½ Ð³ÐµÐ½ÐµÑÐ°ÑÐ¾Ñ ÐºÐ¾Ð´Ð° Ð½Ð° Ð¡ Ð¸Ð· ÑÐ¿ÐµÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¸ Ð½Ð° LibSL, Ð½Ð°Ð¿Ð¸ÑÐ°Ð½Ñ ÑÐµÑÑÑ Ð´Ð»Ñ ÑÐ³ÐµÐ½ÐµÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð¹ ÑÑÐ°Ð½Ð´Ð°ÑÑÐ½Ð¾Ð¹ Ð±Ð¸Ð±Ð»Ð¸Ð¾ÑÐµÐºÐ¸ Ð¸ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¾ ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ðµ Ñ Ð¾ÑÐ¸Ð³Ð¸Ð½Ð°Ð»ÑÐ½Ð¾Ð¹ Ð±Ð¸Ð±Ð»Ð¸Ð¾ÑÐµÐºÐ¾Ð¹. Ð ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐµ Ð±ÑÐ»Ð° Ð¿Ð¾Ð»ÑÑÐµÐ½Ð° ÐºÐ¾ÑÑÐµÐºÑÐ½Ð°Ñ Ð°Ð¿Ð¿ÑÐ¾ÐºÑÐ¸Ð¼Ð°ÑÐ¸Ñ ÑÐ°ÑÑÐ¸ Ð±Ð¸Ð±Ð»Ð¸Ð¾ÑÐµÐºÐ¸ Ð¡, ÐºÐ¾ÑÐ¾ÑÐ°Ñ Ð¼Ð¾Ð¶ÐµÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°ÑÑÑÑ Ð² Ð´Ð°Ð»ÑÐ½ÐµÐ¹ÑÐµÐ¼ Ð´Ð»Ñ ÑÑÐ°ÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° ÐºÐ¾Ð´Ð°, Ð¸ÑÐ¿Ð¾Ð»ÑÐ·ÑÑÑÐµÐ³Ð¾ ÑÑÐ°Ð½Ð´Ð°ÑÑÐ½ÑÑ Ð±Ð¸Ð±Ð»Ð¸Ð¾ÑÐµÐºÑ.
description: This workâs purpose is to write an approximation of the C standard library functions using the formal specification language LibSL. Different approaches to designing formal specifications for the libraries were reviewed, C standard library formal specification was designed, the C programming code generator from the LibSL specification was developed, the generated standard library was tested and compared with the original library. As the result, the correct formal specification for the part of a standard library was made, which can be used for the static analysis of a code that uses standard library.
X-ray monitoring of classical novae in the central region of M 31. II. Autumn and winter 2007/2008 and 2008/2009
Creators: name: Henze, M.
name: Pietsch, W.
name: Haberl, F.
name: Hernanz, M.
name: Sala, G.
name: Hatzidimitriou, D.
name: Della Valle, M.
name: Rau, A.
name: Hartmann, D. H.
name: Burwitz, V.
Publisher: name: arXiv
Year: 2010
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: [Abridged] Classical novae (CNe) represent the major class of supersoft X-ray sources (SSSs) in the central region of our neighbouring galaxy M 31. We performed a dedicated monitoring of the M 31 central region with XMM-Newton and Chandra between Nov 2007 and Feb 2008 and between Nov 2008 and Feb 2009 respectively, in order to find SSS counterparts of CNe, determine the duration of their SSS phase and derive physical outburst parameters. We systematically searched our data for X-ray counterparts of CNe and determined their X-ray light curves and spectral properties. We detected in total 17 X-ray counterparts of CNe in M 31, only four of which were known previously. These latter sources are still active 12.5, 11.0, 7.4 and 4.8 years after the optical outburst. From the 17 X-ray counterparts 13 were classified as SSSs. Four novae displayed short SSS phases (< 100 d). Based on these results and previous studies we compiled a catalogue of all novae with SSS counterparts in M 31 known so far. We used this catalogue to derive correlations between the following X-ray and optical nova parameters: turn-on time, turn-off time, effective temperature (X-ray), t2 decay time and expansion velocity of the ejected envelope (optical). Furthermore, we found a first hint for the existence of a difference between SSS parameters of novae associated with the stellar populations of the M 31 bulge and disk. Additionally, we conducted a Monte Carlo Markov Chain simulation on the intrinsic fraction of novae with SSS phase. This simulation showed that the relatively high fraction of novae without detected SSS emission might be explained by the inevitably incomplete coverage with X-ray observations in combination with a large fraction of novae with short SSS states, as expected from the WD mass distribution. In order to verify our results with an increased sample further monitoring observations are needed.
description: 31 pages, 23 figures, 10 tables; submitted to A&A
Quenching of star-formation in cluster galaxies since z~1
Creators: name: Pintos-Castro, Irene
name: None
Publisher: name: Zenodo
Year: 2019

description: We study the star-forming (SF) population of galaxies within a sample of 209 IR-selected galaxy clusters from the SpARCS survey at 0.3$\leq$z$\leq$1.1 in the ELAIS-N1 and XMM-LSS fields, exploiting the first HSC-SSP data release. The large area and depth of these data allows us to analyze the dependence of the SF fraction, $f_{SF}$, on stellar mass and environment separately. Using $R/R_{200}$ to trace environment, we observe a decrease in $f_{SF}$ from the field towards the cluster core, which strongly depends on stellar mass and redshift. The data show an accelerated growth of the quiescent population within the cluster environment: the $f_{SF}$ vs. stellar mass relation of the cluster core ($R<0.4R_{200}$) is always below that of the field (4$
Dileptons from the nonequilibrium Quark-Gluon Plasma
Creators: name: Bratkovskaya, E. L.
name: Linnyk, O.
name: Cassing, W.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: According to the dynamical quasiparticle model (DQPM) -- matched to reproduce lattice QCD results in thermodynamic limit, -- the constituents of the strongly interacting quark-gluon plasma (sQGP) are massive and off-shell quasi-particles (quarks and gluons) with broad spectral functions. In order to address the electromagnetic radiation of the sQGP, we derive off-shell cross sections of $q\bar q\toγ^*$, $q\bar q\toγ^*+g$ and $qg\toγ^*q$($\bar q g\toγ^* \bar q$) reactions taking into account the effective propagators for quarks and gluons from the DQPM. Dilepton production in In+In collisions at 158 AGeV is studied by implementing these processes into the parton-hadron-string dynamics (PHSD) transport approach. The microscopic PHSD transport approach describes the full evolution of the heavy-ion collision: from the dynamics of quasi-particles in the sQGP phase (when the local energy density is above $\sim 1$ GeV/fm$^3$) through hadronization and to the following hadron interactions and off-shell propagation after the hadronization. A comparison to the data of the NA60 Collaboration shows that the low mass dilepton spectra are well described by including a collisional broadening of vector mesons, while the spectra in the intermediate mass range are dominated by off-shell quark-antiquark annihilation, quark Bremsstrahlung and gluon-Compton scattering in the nonperturbative QGP. In particular, the observed softening of the $m_T$ spectra at intermediate masses (1 GeV $\le M \le$ 3 GeV) is approximately reproduced.
description: 8 pages, 8 figures, to be published in the Proceedings of the 26th Winter Workshop on `Nuclear Dynamics', Ochto Rios, Jamaica, 2-9 January, 2010
Classifying topology of consistent thermodynamics of the four-dimensional neutral Lorentzian NUT-charged spacetimes
Creators: name: Wu, Di
Publisher: name: arXiv
Year: 2023
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: In this paper, via employing the uniformly modified form of the generalized off-shell Helmholtz free energy, we investigate the topological numbers for the four-dimensional neutral Lorentzian Taub-NUT, Taub-NUT-AdS and Kerr-NUT spacetimes, and find that these solutions can also be classified into one of three types of those well-known black hole solutions, which implies that these spacetimes should be viewed as generic black holes from the viewpoint of the thermodynamic topological approach.
description: 19 pages, 6 figures, 1 table, to appear in EPJC
A small quotient of the big absolute Galois group (joint work with Ido Efrat and Ján Mináč)
Creators: name: Chebolu, Sunil K.
Publisher: name: arXiv
Year: 2011
Subjects: subject: Number Theory (math.NT)
subject: FOS: Mathematics

description: This is a report of a talk given at the Oberwolfach workshop on "cohomology of finite groups: Interactions and applications" which was held during July 25th - July 31st, 2010. It is an announcement of some of the results (with motivation) and their applications from the paper "Quotients of absolute Galois groups which determine the entire Galois cohomology"; see arXiv:0905.1364.
description: to appear in Oberwolfach Report
The First Comprehensive Photometric Study of the Algol-type System CL Aurigae
Creators: name: Lee, Jae Woo
name: Kim, Chun-Hwey
name: Kim, Duck Hyun
name: Kim, Seung-Lee
name: Lee, Chung-Uk
name: Koch, Robert H.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We present the first extensive photometric results of CL Aur from our BVRI CCD photometry made on 22 nights from 2003 November through 2005 February. Fifteen new timings of minimum light were obtained. During the past 104 years, the orbital period has varied due to a periodic oscillation superposed on a continuous period increase. The period and semi-amplitude of the oscillation are about 21.6 yrs and 0.0133 d, respectively. This detail is interpreted as a light-travel-time effect due to a low-luminosity K-type star gravitationally bound to the CL Aur close system. Our photometric study indicates that CL Aur is a relatively short-period Algol-type binary with values of q=0.602 and i=88$^\circ$.2. Mass transfer from the secondary to the primary eclipsing component is at least partly responsible for the observed secular period change with a rate of dP/dt = +1.4$\times10^{-7}$ d yr$^{-1}$. A cool spot model has been calculated but we think that an alternative hot-spot model resulting from a gas stream impact on the hot star is more reasonable despite two difficulties with the explanation. Absolute dimensions of the eclipsing system are deduced and its present state is compared with tracks for single star and conservative close binary evolution. Finally, we examine the possible reconciliation of two different calculations of the luminosity of the hot spot and a re-interpretation of the secular term of the period variability.
description: 26 pages, including 5 figures and 9 tables, accepted for publication in AJ
Can a Carbon Nanotube Pierce through a Phospholipid Bilayer?
Creators: name: Pogodin, Sergey
name: Baulin, Vladimir A.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: Great efficiency to penetrate into living cells is attributed to carbon nanotubes due to a number of direct and indirect observations of carbon nanotubes inside the cells. However, a direct evidence of physical translocation of nanotubes through phospholipid bilayers and the exact microscopic mechanism of their penetration into cells are still lacking. In order to test one of the inferred translocation mechanisms, namely the spontaneous piercing through the membrane induced only by thermal motion, we calculate the energy cost associated with the insertion of a carbon nanotube into a model phospholipid bilayer using the Single Chain Mean Field theory which is particularly suitable for the accurate measurements of equilibrium free energies. We find that the energy cost of the bilayer rupture is quite high compared to the energy of thermal motion. This conclusion may indirectly support other energy dependent translocation mechanisms such as, for example, endocytosis.
description: Published in ACS Nano
Additional file 5 of Impact of universal home visits on child health in Bauchi State, Nigeria: a stepped wedge cluster randomised controlled trial
Creators: name: Omer, Khalid
name: Joga, Altine
name: Dutse, Umar
name: Hasan, Khalid
name: Aziz, Amar
name: Ansari, Umaira
name: Gidado, Yagana
name: Baba, Muhd Chadi
name: Gamawa, Adamu Ibrahim
name: Mohammad, Rilwanu
name: Andersson, Neil
name: Cockcroft, Anne
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Cell Biology
subject: Sociology
subject: FOS: Sociology
subject: Cancer
subject: Science Policy
subject: Computational Biology

description: Additional file 5. Other initiatives in Toro LGA potentially related to the measured child health outcomes. This file contains a description and relevant web links to view details about other initiatives in Toro LGA during the period of the home visits
Nuova edificazione “Residenza al Fiume” Riva San Vitale
Creators: name: Lamberti, Davide
Publisher: name: Scuola Universitaria della Svizzera Italiana (SUPSI)
Year: 2018

description: Il tema della tesi di Bachelor riguarda la progettazione di un edificio residenziale di tre piani con annessa autorimessa nel comune di Riva San Vitale, a ridosso del Fiume Laveggio. Le caratteristiche geotecniche del terreno sfavorevoli rendono il lavoro intrigante, in quanto, permettono di comparare vari sistemi costruttivi e valutare quale meglio si addica alle esigenze richieste.
Additional file 1 of Intra-patient stability of tumor mutational burden from tissue biopsies at different time points in advanced cancers
Creators: name: Pham, Timothy V.
name: Goodman, Aaron M.
name: Sivakumar, Smruthy
name: Frampton, Garrett
name: Kurzrock, Razelle
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Cell Biology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Cancer

description: Additional file 1: Figure S1. CONSORT Diagram for UCSD clinically curated cohort. Figure S2. Additional correlation analysis between earlier and later TMB for UCSD clinically curated cohort. Figure S3. Linear Regression Analysis of Paired Biopsies in the Foundation Medicine Cohort. Figure S4. Difference in TMB from paired biopsies in Foundation Medicine Cohort
Macromolecular Dynamics in Red Blood Cells Investigated Using Neutron Spectroscopy
Creators: name: Stadler, Andreas Maximilian
name: van Eijck, Lambert
name: Demmel, Franz
name: Artmann, Gerhard
Publisher: name: arXiv
Year: 2011
Subjects: subject: Biological Physics (physics.bio-ph)
subject: Biomolecules (q-bio.BM)
subject: FOS: Physical sciences
subject: FOS: Biological sciences

description: We present neutron scattering measurements on the dynamics of hemoglobin (Hb) in human red blood cells in vivo. Global and internal Hb dynamics were measured in the ps to ns time- and Å length-scale using quasielastic neutron backscattering spectroscopy. We observed the cross-over from global Hb short-time to long-time self-diffusion. Both short- and long-time diffusion coefficients agree quantitatively with predicted values from hydrodynamic theory of non-charged hard-sphere suspensions when a bound water fraction of around 0.23g H2O/ g Hb is taken into account. The higher amount of water in the cells facilitates internal protein fluctuations in the ps time-scale when compared to fully hydrated Hb powder. Slower internal dynamics of Hb in red blood cells in the ns time-range were found to be rather similar to results obtained with fully hydrated protein powders, solutions and E. coli cells.
Langevin simulation of dark matter kinetic equilibration
Creators: name: Kim, Seyong
name: Laine, M.
Publisher: name: arXiv
Year: 2023
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Recently it has been questioned, notably in the context of the scalar singlet dark matter model with $m_φ^{ }\simeq 60$ GeV, how efficiently kinetic equilibrium is maintained if freeze-out dynamics is pushed down to low temperatures by resonant effects. We outline how Langevin simulations can be employed for addressing the non-equilibrium momentum distribution of non-relativistic particles in a cosmological background. For a scalar singlet mass $m_φ^{ }\simeq 60$ GeV, these simulations suggest that kinetic equilibrium is a good approximation down to $T \sim 1$ GeV, with the deviation first manifesting itself as a red-tilted spectrum. This reduces the annihilation cross section, confirming findings from other methods that a somewhat larger ($ < 20\%$) coupling than in equilibrium is needed for obtaining the correct abundance.
description: 15 pages. v2: clarifications added
title: ÐÐ¿ÑÐ¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ñ ÑÑÑÑÐºÑÑÑÑ Ð½Ð¾Ð²Ð¾Ð¹ ÑÐºÐ¾Ð½Ð¾Ð¼Ð½Ð¾Ð»ÐµÐ³Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð¹ ÑÑÐ°Ð»Ð¸ Ð´Ð»Ñ Ð±Ð¾Ð»ÑÑÐµÐ³ÑÑÐ·Ð½Ð¾Ð¹ ÑÐµÑ Ð½Ð¸ÐºÐ¸ Ñ ÑÐµÐ»ÑÑ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÐµÐµ ÑÐºÑÐ¿Ð»ÑÐ°ÑÐ°ÑÐ¸Ð¾Ð½Ð½ÑÑ ÑÐ²Ð¾Ð¹ÑÑÐ²
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¼Ð°Ð³Ð¸ÑÑÑÐ°
titleType: Subtitle
title: Optimization of the structure of new economically alloyed steel for heavy equipment in order to improve its performance properties
Creators: name: ÐÐ¼Ð¸ÑÑÐ¸ÐµÐ², ÐÑÑÐ°Ð¿
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: 2019
Subjects: Ð¡ÑÐ°Ð»Ñ Ñ Ð»Ð°Ð´Ð½Ð¾ÑÑÐ¾Ð¹ÐºÐ°Ñ
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ÑÐ´Ð°ÑÐ½Ð°Ñ Ð²ÑÐ·ÐºÐ¾ÑÑÑ
Ð¾Ð¿ÑÐ¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ñ
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description: Ð Ð±Ð¾Ð»ÑÑÐµÐ³ÑÑÐ·Ð½Ð¾Ð¹ ÑÐµÑÐ½Ð¸ÐºÐµ Ð¾Ð´Ð½Ð¾Ð¹ Ð¸Ð· Ð³Ð»Ð°Ð²Ð½ÑÑ ÑÐ¾ÑÑÐ°Ð²Ð»ÑÑÑÐ¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÑÐ°Ð¼Ð°. ÐÐ°ÑÐµÑÐ¸Ð°Ð», Ð¸Ð· ÐºÐ¾ÑÐ¾ÑÐ¾Ð³Ð¾ Ð¾Ð½Ð° Ð´ÐµÐ»Ð°ÐµÑÑÑ, Ð´Ð¾Ð»Ð¶ÐµÐ½ Ð¾Ð±Ð»Ð°Ð´Ð°ÑÑ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÑÐ½Ð½ÑÐ¼ Ð½Ð°Ð±Ð¾ÑÐ¾Ð¼ ÑÐ²Ð¾Ð¹ÑÑÐ², Ð° Ð¸Ð¼ÐµÐ½Ð½Ð¾ Ð²ÑÑÐ¾ÐºÐ¾Ð¹ Ð¿ÑÐ¾ÑÐ½Ð¾ÑÑÑÑ Ð¸ Ð¿Ð»Ð°ÑÑÐ¸ÑÐ½Ð¾ÑÑÑÑ, Ð¸Ð·Ð½Ð¾ÑÐ¾ÑÑÐ¾Ð¹ÐºÐ¾ÑÑÑÑ Ð¸ ÑÐ²Ð°ÑÐ¸Ð²Ð°ÐµÐ¼Ð¾ÑÑÑÑ. ÐÑÐ½ÐµÑÐ½Ð¸Ðµ Ð°Ð½Ð°Ð»Ð¾Ð³Ð¸ ÑÑÐ°Ð»ÐµÐ¹ Ð¾Ð±Ð»Ð°Ð´Ð°ÑÑ Ð²ÑÐµÐ¼ ÑÐ¿ÐµÐºÑÑÐ¾Ð¼ Ð´Ð°Ð½Ð½ÑÑ ÑÐ²Ð¾Ð¹ÑÑÐ², Ð½Ð¾ Ð¸Ð¼ÐµÑÑ Ð½Ð¸Ð·ÐºÑÑ ÑÐ»Ð°Ð´Ð¾ÑÑÐ¾Ð¹ÐºÐ¾ÑÑÑ Ð¸ Ð½Ðµ Ð¼Ð¾Ð³ÑÑ ÑÐ°Ð±Ð¾ÑÐ°ÑÑ Ð¿ÑÐ¸ Ð½Ð¸Ð·ÐºÐ¸Ñ ÑÐµÐ¼Ð¿ÐµÑÐ°ÑÑÑÐ°Ñ Ð´Ð¾ -70 Ð³ÑÐ°Ð´ÑÑÐ¾Ð². ÐÑÐ»Ð° Ð¸Ð·Ð¾Ð±ÑÐµÑÐµÐ½Ð° Ð½Ð¾Ð²Ð°Ñ ÑÑÐ°Ð»Ñ 09Ð¥ÐÐ2ÐÐ. ÐÑÐ» Ð¸Ð·ÑÑÐµÐ½ ÑÐ¾ÑÑÐ°Ð² ÐµÑ ÑÑÑÑÐºÑÑÑÐ½ÑÑ ÑÐ°Ð· Ð¿Ð¾ ÑÑÐµÐ´ÑÑÐ²Ð°Ð¼ Ð¾Ð¿ÑÐ¸ÑÐµÑÐºÐ¾Ð¹ Ð¼Ð¸ÐºÑÐ¾ÑÐºÐ¾Ð¿Ð¸Ð¸. ÐÑÐ»Ð¸ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ñ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÐµÐµ Ð¼ÐµÑÐ°Ð½Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ²Ð¾Ð¹ÑÑÐ² Ð¸ Ð²Ð»Ð¸ÑÐ½Ð¸Ðµ ÑÐµÐ¶Ð¸Ð¼Ð¾Ð² ÑÐµÑÐ¼Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð½Ð° Ð½Ð¸Ñ. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¾ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¿Ð¾Ð²ÐµÑÑÐ½Ð¾ÑÑÐµÐ¹ ÑÐ°Ð·ÑÑÑÐµÐ½Ð¸Ñ Ð¾Ð±ÑÐ°Ð·ÑÐ¾Ð² Ð¿ÑÑÐµÐ¼ ÑÐ°ÑÑÑÐ¾Ð²Ð¾Ð¹ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½Ð¾Ð¹ Ð¼Ð¸ÐºÑÐ¾ÑÐºÐ¾Ð¿Ð¸Ð¸.
description: In heavy equipment, one of the main components is the frame. The material from which it is made must have a certain set of properties, namely high strength and ductility, wear resistance and weldability. Current steel analogues have the full range of these properties, but have low cold resistance and can not operate at low temperatures up to -70 degrees. Had invented a new steel 09Ð¥Ð2ÐÐ. The composition of its structural phases was studied by means of optical microscopy. Researches of its mechanical properties and influence of modes of heat treatment on them were carried out. The study of fracture surfaces of samples by scanning electron microscopy.
A vector equilibrium problem for the two-matrix model in the quartic/quadratic case
Creators: name: Duits, Maurice
name: Geudens, Dries
name: Kuijlaars, Arno B. J.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Classical Analysis and ODEs (math.CA)
subject: Mathematical Physics (math-ph)
subject: FOS: Mathematics
subject: FOS: Physical sciences

description: We consider the two sequences of biorthogonal polynomials (p_{k,n})_k and (q_{k,n})_k related to the Hermitian two-matrix model with potentials V(x) = x^2/2 and W(y) = y^4/4 + ty^2. From an asymptotic analysis of the coefficients in the recurrence relation satisfied by these polynomials, we obtain the limiting distribution of the zeros of the polynomials p_{n,n} as n tends to infinity. The limiting zero distribution is characterized as the first measure of the minimizer in a vector equilibrium problem involving three measures which for the case t=0 reduces to the vector equilibrium problem that was given recently by two of us. A novel feature is that for t < 0 an external field is active on the third measure which introduces a new type of critical behavior for a certain negative value of t. We also prove a general result about the interlacing of zeros of biorthogonal polynomials.
description: 60 pages, 9 figures
Compression and information entropy of binary strings from the collision history of three hard balls
Creators: name: Vedak, Matej
name: Ackland, Graeme J
Publisher: name: arXiv
Year: 2023
Subjects: subject: Computational Physics (physics.comp-ph)
subject: FOS: Physical sciences
subject: 82-10 (Primary) 82-04, 70F07 (Secondary)

description: We investigate how to measure and define the entropy of a simple chaotic system, three hard spheres on a ring. A novel approach is presented, which does not assume the ergodic hypothesis. It consists of transforming the particles collision history into a sequence of binary digits. We then investigate three approaches which should demonstrate the non-randomness of these collision-generated strings compared with random number generator created strings: Shannon entropy, diehard randomness tests and compression percentage. We show that the Shannon information entropy is unable to distinguish random from deterministic strings. The Diehard test performs better, but for certain mass-ratios the collision-generated strings are misidentified as random with high confidence. The zlib and bz2 compression algorithms are efficient at detecting non-randomness and low information content, with compression efficiencies that tend to 100% in the limit of infinite strings. Thus compression algorithm entropy is non-extensive for this chaotic system, in marked contrast to the extensive entropy determined from phase-space integrals by assuming ergodicity.
description: 15 pages, 7 figures, submitted to Journal of Physics Communications
Lessons Learned from the Definitive Spectral Atlas of Star-forming Galaxies at Cosmic Noon
Creators: name: Bayliss, Matthew
name: None
Publisher: name: Zenodo
Year: 2019

description: Dedicated searches for bright, strongly lensed galaxies have revealed large samples of highly magnified sources that will forever constitute a unique and finite number of opportunities for probing distant galaxies at high signal-to-noise. As such, the brightest lensed galaxies are invaluable laboratories in which to compare the detailed properties of distant starburst galaxies with local, well-studied star-forming galaxies. In this talk I will present the Magellan Evolution of Galaxies Spectroscopic and Ultraviolet Reference Atlas (MEGaSaURA), the definitive look at the rest-frame UV spectra of star-forming galaxies at cosmic noon. The MEGaSaURA sample, primarily drawn from the Sloan Giant Arcs Survey, is selected from the brightest known lensed galaxies, with redshifts between 1.6 < z < 3.6. The MEGaSAURA spectra capture dozens of lines that reveal the physical properties of the population of massive stars, the elemental abundances and physical properties of the nebular gas ionized by those stars, and the wind-driven gas outflows that they power. We analyze nebular emission lines, ISM and stellar wind outflows, and the best-fit properties of the young stellar populations with an eye toward informing studies of the first galaxies with the next generation of observational facilities (JWST and 30m-class telescopes). We find remarkable similarity between the properties of vigorously star-forming galaxies at Cosmic Noon and in the local universe. In galaxies dominated by extremely young (<50 Myr) stellar populations the precise stellar age is most important physical property, independent of redshift. Combining MEGaSaURA with similarly young z~0 star-forming galaxies, we quantify strong relationships between simple observable quantities, such as rest-UV emission line equivalent widths, and important underling properties of the stellar continuum emission.
Observation of Supercurrent in PbIn-Graphene-PbIn Josephson Junction
Creators: name: Jeong, Dongchan
name: Choi, Jae-Hyun
name: Lee, Gil-Ho
name: Jo, Sanghyun
name: Doh, Yong-Joo
name: Lee, Hu-Jong
Publisher: name: arXiv
Year: 2011
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: Superconductor-graphene-superconductor (SGS) junction provides a unique platform to study relativistic electrodynamics of Dirac fermions combined with proximity-induced superconductivity. We report observation of the Josephson effect in proximity-coupled superconducting junctions of graphene in contact with Pb1-xInx (x=0.07) electrodes for temperatures as high as T = 4.8K, with a large IcRn (~ 255 microV). This demonstrates that Pb1-xInx SGS junction would facilitate the development of the superconducting quantum information devices and superconductor-enhanced phase-coherent transport of graphene.
description: 8 pages, 7 figures, accepted in PRB
Early childhood educators' dialogical engagement in an artmaking space
Creators: name: Chung, Kwang Dae
Publisher: name: University of British Columbia
Year: 2021

description: Early childhood educators nowadays are encouraged to pedagogically engage with children, materials, and their given environments (Jardine et al., 2011; van Manen, 2017; Vintimilla, 2017) and to practice the “pedagogy of listening” (Kind, 2008, 2020; Rinaldi, 2006). However, neither dialogue nor the creation of a space for practicing the pedagogy of listening have received considerable attention (Aoki, 2004; Jardine et al., 2011; Wilson, 2007). Wilson (2007) and Thompson (2015) have suggested that understanding children’s ways of being and of making in an art space requires educators to encounter children in “the pedagogical third space” (Aoki, 2004; Wilson, 2007). The aim of this study is to examine the dialogical engagement of early childhood educators in an artmaking space. Dialogical engagement involves responsible listening, encountering, dwelling, asking questions, thinking with others, engaging in conversations, and learning from and with others (Dahlberg & Moss, 2005; Kind, 2020; Pacini-Ketchabaw et al., 2017; Rinaldi, 2006). This study was guided by the following primary research question: How do early childhood educators dialogically engage with children during an artmaking process?” A descriptive-qualitative research model was utilized for this phenomenological descriptive case study (van Manen, 2007, 2014; Yazan, 2015; Yin, 2009). I observed the art/drawing events of three early childhood educators in two different early childhood centres and interviewed them to understand how they were attentively attuned to their engagement with children and materials during children’s artmaking sessions and to determine whether they had been purposefully making dialogue to learn something from the children in their art spaces. I discovered that pedagogical listening could facilitate dialogue among educators and children. Moreover, dialogical engagement supported children’s creativity, imagination, and wonderment in the process of making and drawing. The significance of the research is that it demonstrates how early childhood educators implement the pedagogy of listening in their everyday practice. Furthermore, this research reveals the potential impact of educators’ multiple ways of being, dwelling, encountering, and slowing, as well as their responsibility within children’s artmaking spaces.
title: ÐÑÐ²Ð¾Ð´ Ð¸ Ð¿ÑÐ¾Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ðµ Ð½Ð° Ð¼Ð¸ÑÐ¾Ð²Ð¾Ð¹ ÑÑÐ½Ð¾Ðº ÑÐ»Ð¾Ð¶Ð½Ð¾Ð³Ð¾ ÑÐµÑ Ð½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ° (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐ¡-21 â ÑÐµÐ¼ÐµÐ¹ÑÑÐ²Ð° Ð¿Ð°ÑÑÐ°Ð¶Ð¸ÑÑÐºÐ¸Ñ ÑÐ°Ð¼Ð¾Ð»ÐµÑÐ¾Ð² Ð½Ð¾Ð²Ð¾Ð³Ð¾ Ð¿Ð¾ÐºÐ¾Ð»ÐµÐ½Ð¸Ñ)
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¼Ð°Ð³Ð¸ÑÑÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¾Ð±ÑÐ»ÐºÐ¾, ÐÑÐ¸Ð½Ð°
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: 2020
Subjects: Ð¡Ð°Ð¼Ð¾Ð»ÐµÑÐ¾ÑÑÑÐ¾ÐµÐ½Ð¸Ðµ
ÑÐ»Ð¾Ð¶Ð½ÑÐ¹ ÑÐµÑ Ð½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑ
ÐÐ¡-21
Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð¾Ð²Ð°Ñ ÑÑÑÐ°ÑÐµÐ³Ð¸Ñ
Ð¶Ð¸Ð·Ð½ÐµÐ½Ð½ÑÐ¹ ÑÐ¸ÐºÐ»
Ð³ÑÐ°Ñ
Ð³ÑÐ°Ð¶Ð´Ð°Ð½ÑÐºÐ°Ñ Ð°Ð²Ð¸Ð°ÑÐ¸Ñ

description: Ð¦ÐµÐ»ÑÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¹ Ð¿Ð¾ ÑÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð¾Ð²Ð¾Ð¹ ÑÑÑÐ°ÑÐµÐ³Ð¸Ð¸ Ð²ÑÐ²Ð¾Ð´Ð° ÐÐ¡-21 Ð½Ð° Ð¼Ð¸ÑÐ¾Ð²Ð¾Ð¹ ÑÑÐ½Ð¾Ðº. ÐÑÐ½Ð¾Ð²Ð½ÑÐ¼Ð¸ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ°Ð¼Ð¸ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÑÑÑÑ Ð¾ÑÑÐ°Ð¶ÐµÐ½Ð¸Ðµ ÑÑÐ°Ð¿Ð¾Ð² Ð¶Ð¸Ð·Ð½ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÐ¸ÐºÐ»Ð° ÐÐ¡-21 Ð² Ð²Ð¸Ð´Ðµ Ð°Ð»ÑÑÐµÑÐ½Ð°ÑÐ¸Ð²Ð½Ð¾Ð³Ð¾ Ð³ÑÐ°ÑÐ°; Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð¸Ðµ Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð¾Ð²Ð¾Ð¹ ÑÑÑÐ°ÑÐµÐ³Ð¸Ð¸ Ð´Ð»Ñ ÑÐ»Ð¾Ð¶Ð½Ð¾Ð³Ð¾ ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ° ÐÐ¡-21; ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¾ÑÐ½Ð¾Ð²Ð½ÑÑ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹ Ð´Ð»Ñ Ð²ÑÐ²Ð¾Ð´Ð° ÐÐ¡-21 Ð½Ð° ÑÑÐ½Ð¾Ðº.
description: The purpose of the study is development of practical recommendations for improving the marketing strategy of introducing MC-21 to the world market. The main results of the paper are that the stages of the life cycle of MC-21 are reflected in the form of an alternative graph; the methodology of developing a marketing strategy for the compound technical complex MC-21; developed the main activities for bringing the MC-21 to the market.
Star forming galaxies and AGN at the peak of cosmic star formation
Creators: name: Herrera-Camus, Rodrigo
name: None
Publisher: name: Zenodo
Year: 2019

description: In this talk I will review our current  knowledge on the molecular gas masses  (from CO and dust observations), depletion timescales, gas fractions, and demographics of  outflows in galaxies at z~1-3, the time when the cosmic star formation rate density and the frequency of nuclear activity in galaxies peaked.
Quenching of spectroscopic factors for proton removal in oxygen isotopes
Creators: name: Jensen, Ø.
name: Hagen, G.
name: Hjorth-Jensen, M.
name: Brown, B. Alex
name: Gade, A.
Publisher: name: arXiv
Year: 2011
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We present microscopic coupled-cluster calculations of the spectroscopic factors for proton removal from the closed-shell oxygen isotopes $^{14,16,22,24,28}$O with the chiral nucleon-nucleon interaction at next-to-next-to-next-to-leading order. We include coupling-to-continuum degrees of freedom by using a Hartree-Fock basis built from a Woods-Saxon single-particle basis. This basis treats bound and continuum states on an equal footing. We find a significant quenching of spectroscopic factors in the neutron-rich oxygen isotopes, pointing to enhanced many-body correlations induced by strong coupling to the scattering continuum above the neutron emission thresholds.
description: 3 figures
Additional file 3 of Intra-patient stability of tumor mutational burden from tissue biopsies at different time points in advanced cancers
Creators: name: Pham, Timothy V.
name: Goodman, Aaron M.
name: Sivakumar, Smruthy
name: Frampton, Garrett
name: Kurzrock, Razelle
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Cell Biology
subject: 39999 Chemical Sciences not elsewhere classified
subject: FOS: Chemical sciences
subject: Cancer

description: Additional file 3:. PREDICT Study Protocol and Consent Form. Study Protocol. Consent Form
ARPES signature of the competition between magnetic order and Kondo effect in CeCoGe3
Creators: name: Li, Peng
name: Ye, Huiqing
name: Hu, Yong
name: Fang, Yuan
name: Xiao, Zhiguang
name: Wu, Zhongzheng
name: Shan, Zhaoyang
name: Singh, Ravi P.
name: Balakrishnan, Geetha
name: Shen, Dawei
name: Yang, Yi-feng
name: Cao, Chao
name: Plumb, Nicholas C.
name: Smidman, Michael
name: Shi, Ming
name: Kroha, Johann
name: Yuan, Huiqiu
name: Steglich, Frank
name: Liu, Yang
Publisher: name: arXiv
Year: 2023
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: The competition between magnetic order and Kondo effect is essential for the rich physics of heavy fermion systems. Nevertheless, how such competition is manifested in the quasiparticle bands in a real periodic lattice remains elusive in spectroscopic experiments. Here we report a high-resolution photoemission study of the antiferromagnetic Kondo lattice system CeCoGe3 with a high TN1 of 21K. Our measurements reveal a weakly dispersive 4f band at the Fermi level near the Z point, arisingfrom moderate Kondo effect. The intensity of this heavy 4f band exhibits a logarithmic increase with lowering temperature and begins to deviate from this Kondo-like behavior below 25 K, just above TN1, and eventually ceases to grow below 12 K. Our work provides direct spectroscopic evidence for the competition between magnetic order and the Kondo effect in a Kondo lattice system with local-moment antiferromagnetism, indicating a distinct scenario for the microscopic coexistence and competition of these phenomena, which might be related to the real-space modulation.
description: 7 pages, 4 figures
Cosmic-Ray Acceleration Efficiency vs Temperature Equilibration: the Case of SNR 0509-67.5
Creators: name: Helder, E. A.
name: Kosenko, D.
name: Vink, J.
Publisher: name: arXiv
Year: 2010
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: We study the 0509-67.5 supernova remnant in the Large Magellanic Cloud with the VLT/FORS2 spectrograph. We detect a broad component in the H-alpha emission with a FWHM of 2680 \pm 70 km/s and 3900 \pm 800 km/s for the southwest (SW) and northeast (NE) shocks respectively. For the SW, the proton temperature appears to be too low for the shock velocity, which we attribute to a cosmic-ray pressure behind the shock front of at least 20% of the total pressure. For the NE, the post-shock proton temperature and the shock velocity are compatible, only if the plasma behind the shock front has a degree of thermal equilibrium of over 20%, which is at odds with current models for temperature equilibration behind fast shocks, which do not accelerate cosmic rays. If we assume the electron temperature to be less than 10% of the proton temperature, we find a post-shock cosmic-ray pressure of at least 7%.
description: Accepted for publication in ApJ Letters, 5 pages, 4 figures and 1 table
Formation of Young Massive Clusters with Multiple Stellar Populations in Galaxy-Galaxy Merging Process
Creators: name: Matsui, Hidenori
name: None
Publisher: name: Zenodo
Year: 2019

description: We have analized simulation data of a galaxy-galaxy merger (Matsui et al. 2012) and researched stellar age in young massive clusters (YMCs). We find that whereas most YMCs have single stellar population, the rest YMCs have multiple stellar populations. Such YMCs with multiple stellar populations are formed by capturing dense gas and forming next generation stars when they pass dense gas region. Since the captured gas is contaminated with metal ejected from TypeII supernovae, the YMC consists of stars with different metallicity.
Additional file 1 of Falls associated with indoor and outdoor environmental hazards among community-dwelling older adults between men and women
Creators: name: Lee, Sungmin
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Biotechnology
subject: Ecology
subject: 111714 Mental Health
subject: FOS: Health sciences
subject: Computational Biology

description: Additional file 1 Appendix Table 1. Robust check: Construction of indoor and outdoor environmental hazards variables.
A spin model for intrinsic antiferromagnetic skyrmions on a triangular lattice
Creators: name: Aldarawsheh, Amal
name: Sallermann, Moritz
name: Abusaa, Muayad
name: Lounis, Samir
Publisher: name: arXiv
Year: 2023
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: Skyrmions are prospected as the potential future of data storage due to their topologically protected spin structures. However, traditional ferromagnetic (FM) skyrmions experience deflection when driven with an electric current, hindering their usage in spintronics. Antiferromagnetic (AFM) skyrmions, consisting of two FM solitons coupled antiferromagnetically, are predicted to have a zero Magnus force, making them promising candidates for spintronic racetrack memories. Currently, they have been stabilized in synthetic AFM structures, i.e. multilayers hosting FM skyrmions, which couple antiferromagnetically through a non-magnetic spacer, while recent first-principles simulations predict their emergence in an intrinsic form, within an row-wise AFM single monolayer of Cr deposited on PdFe bilayer grown on Ir(111) surfaces. The latter material forms a triangular lattice, where single and interlinked AFM skyrmions can be stabilized. Here, we explore the minimal Heisenberg model enabling the occurrence of such AFM solitons and the underlying phase diagrams by accounting for the interplay between the Dzyaloshinskii-Moriya and Heisenberg exchange interactions, as well as the magnetic anisotropy and impact of magnetic field. By providing the fundamental basis to identify and understand the behavior of intrinsic AFM skyrmions, we anticipate our model to become a powerful tool for exploring and designing new topological magnetic materials to conceptualize devices for AFM spintronics.
description: 21 pages, 3 figures
Detection of mechanical resonance of a single-electron transistor by direct current
Creators: name: Pashkin, Yu. A.
name: Li, T. F.
name: Pekola, J. P.
name: Astafiev, O.
name: Knyazev, D. A.
name: Hoehne, F.
name: Im, H.
name: Nakamura, Y.
name: Tsai, J. S.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We have suspended an Al based single-electron transistor whose island can resonate freely between the source and drain leads forming the clamps. In addition to the regular side gate, a bottom gate with a larger capacitance to the SET island is placed underneath to increase the SET coupling to mechanical motion. The device can be considered as a doubly clamped Al beam that can transduce mechanical vibrations into variations of the SET current. Our simulations based on the orthodox model, with the SET parameters estimated from the experiment, reproduce the observed transport characteristics in detail.
description: 4 pages, 3 figures
Programming nonreciprocity and harmonic beam steering via a digitally space-time-coded metamaterial antenna
Creators: name: Vosoughitabar, Shaghayegh
name: Wu, Chung-Tse Michael
Publisher: name: arXiv
Year: 2023
Subjects: subject: Applied Physics (physics.app-ph)
subject: Systems and Control (eess.SY)
subject: FOS: Physical sciences
subject: FOS: Electrical engineering, electronic engineering, information engineering

description: Recent advancement in digital coding metasurfaces incorporating spatial and temporal modulation has enabled simultaneous control of electromagnetic (EM) waves in both space and frequency domains by manipulating incident EM waves in a transmissive or reflective fashion, resulting in time-reversal asymmetry. Here we show in theory and experiment that a digitally space-time-coded metamaterial (MTM) antenna with spatiotemporal modulation at its unit cell level can be regarded as a radiating counterpart of such digital metasurface, which will enable nonreciprocal EM wave transmission and reception via surface-to-leaky-wave transformation and harmonic frequency generation. Operating in the fast wave (radiation) region, the space-time-coded MTM antenna is tailored in a way such that the propagation constant of each programmable unit cell embedded with varactor diodes can toggle between positive and negative phases, which is done through providing digital sequences by using a field-programmable gate array (FPGA). Owing to the time-varying coding sequence, harmonic frequencies are generated with different main beam directions. Furthermore, the space time modulation of the digitally coded MTM antenna allows for nonreciprocal transmission and reception of EM waves by breaking the time-reversal symmetry, which may enable many applications, such as simultaneous transmit and receive, unidirectional transmission, radar sensing, and multiple-input and multiple-output (MIMO) beamformer.
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÐ¸ÑÑÐµÐ¼Ñ Ð´Ð»Ñ Ð³ÐµÐ½ÐµÑÐ°ÑÐ¸Ð¸ Ð´ÐµÐ¹ÑÐµÑÐ¸Ñ Ð¸ Ð³Ð°Ð·Ð¾Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ¾Ð² Ð¿Ð¾Ð»ÑÑÐ¸Ð·Ð¾Ð²Ð°Ð½Ð½ÑÑ Ð°ÑÐ¾Ð¼Ð¾Ð² Ð¸ Ð¸Ð¾Ð½Ð¾Ð² Ð² Ð¿ÑÐ¾ÐµÐºÑÐµ Ð¿Ð¾ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐµÐ°ÐºÑÐ¸Ð¸ ÑÐ´ÐµÑÐ½Ð¾Ð³Ð¾ dd-ÑÐ¸Ð½ÑÐµÐ·Ð° Ñ Ð¿Ð¾Ð»ÑÑÐ¸Ð·Ð°ÑÐ¸ÐµÐ¹ Ð¸ÑÑ Ð¾Ð´Ð½ÑÑ ÑÐ°ÑÑÐ¸Ñ Ð¿ÑÐ¸ Ð½Ð¸Ð·ÐºÐ¸Ñ ÑÐ½ÐµÑÐ³Ð¸ÑÑ (PolFusion)
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: Development of a system for the generation of deuterium and gas supply system to sources of polarized atoms and ions in the experiment aimsto study dd-fusionreactions with the low beam energy (PolFusion)
Creators: name: Ð Ð¾Ð¶Ð´ÐµÑÑÐ²ÐµÐ½ÑÐºÐ¸Ð¹, ÐÐ½ÑÐ¾Ð½
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: 2020
Subjects: dd-ÑÐ¸Ð½ÑÐµÐ·
polfusion
Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ¸ Ð¸Ð¾Ð½Ð¾Ð²
Ð³ÐµÐ½ÐµÑÐ°ÑÐ¾Ñ Ð´ÐµÐ¹ÑÐµÑÐ¸Ñ
ÑÐ¸ÑÑÐµÐ¼Ð° Ð³Ð°Ð·Ð¾Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ
dd-fusion
ion sorces
deuterium generator
gas sustem

description: ÐÐ°Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° Ð¿ÑÐ¾ÑÐµÑÑÑ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ ÑÐ¸ÑÑÐµÐ¼Ñ Ð´Ð»Ñ Ð³ÐµÐ½ÐµÑÐ°ÑÐ¸Ð¸ Ð´ÐµÐ¹ÑÐµÑÐ¸Ñ Ð¸ Ð³Ð°Ð·Ð¾Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ¾Ð² Ð¿Ð¾Ð»ÑÑÐ¸Ð·Ð¾Ð²Ð°Ð½Ð½ÑÑ Ð°ÑÐ¾Ð¼Ð¾Ð² Ð¸ Ð¸Ð¾Ð½Ð¾Ð². Ð Ð°Ð±Ð¾ÑÐ° Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð° Ð² ÑÐ°Ð¼ÐºÐ°Ñ ÑÐ´ÐµÑÐ½Ð¾-ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐºÑÐ¿ÐµÑÐ¸Ð¼ÐµÐ½ÑÐ° PolFusion, Ð¾ÑÑÑÐµÑÑÐ²Ð»ÑÐµÐ¼Ð¾Ð³Ð¾ Ð² ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¾Ð¼ Ð¸Ð½ÑÑÐ¸ÑÑÑÐµ ÑÐ´ÐµÑÐ½Ð¾Ð¹ ÑÐ¸Ð·Ð¸ÐºÐ¸ (ÐÐ°ÑÑÐ¸Ð½Ð°), ÑÐµÐ»ÑÑ ÐºÐ¾ÑÐ¾ÑÐ¾Ð³Ð¾ ÑÐ²Ð»ÑÐµÑÑÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐµÐ°ÐºÑÐ¸Ð¸ ÑÐ»Ð¸ÑÐ½Ð¸Ñ 2H (d, p) 3H Ð¸ 2H (d, n) 3He Ñ Ð¿Ð¾Ð»ÑÑÐ¸Ð·Ð°ÑÐ¸ÐµÐ¹ Ð¸ÑÑÐ¾Ð´Ð½ÑÑ ÑÐ°ÑÑÐ¸Ñ Ð¿ÑÐ¸ Ð½Ð¸Ð·ÐºÐ¸Ñ ÑÐ½ÐµÑÐ³Ð¸ÑÑ Ð² Ð¾Ð±Ð»Ð°ÑÑÐ¸ 10-100 ÐºÑÐ.
description: This work is devoted to the process of creating a system for the generation of deuterium and gas supply to sources of polarized atoms and ions. This work was carried out as part of the PolFusion nuclear physics experiment carried out at the Petersburg Nuclear Physics Institute (Gatchina), the purpose of which is to study the fusion reaction of 2H (d, p) 3H and 2H (d, n) 3He with polarization of the initial particles at low energies in the range of 10-100 keV.
Nonlocal extension of the dispersive-optical-model to describe data below the Fermi energy
Creators: name: Dickhoff, W. H.
name: Van Neck, D.
name: Waldecker, S. J.
name: Charity, R. J.
name: Sobotka, L. G.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Nuclear Theory (nucl-th)
subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: Present applications of the dispersive-optical-model analysis are restricted by the use of a local but energy-dependent version of the generalized Hartree-Fock potential. This restriction is lifted by the introduction of a corresponding nonlocal potential without explicit energy dependence. Such a strategy allows for a complete determination of the nucleon propagator below the Fermi energy with access to the expectation value of one-body operators (like the charge density), the one-body density matrix with associated natural orbits, and complete spectral functions for removal strength. The present formulation of the dispersive optical model (DOM) therefore allows the use of elastic electron-scattering data in determining its parameters. Application to ${}^{40}$Ca demonstrates that a fit to the charge radius leads to too much charge near the origin using the conventional assumptions of the functional form of the DOM. A corresponding incomplete description of high-momentum components is identified, suggesting that the DOM formulation must be extended in the future to accommodate such correlations properly. Unlike the local version, the present nonlocal DOM limits the location of the deeply-bound hole states to energies that are consistent with (\textit{e,e}$^{\prime}$\textit{p}) and (\textit{p,2p}) data.
description: 14 pages, 10 figures, submitted to Physical Review C
Additional file 1 of Multi-component cognitive intervention for older adults with mixed cognitive levels: implementation and preliminary effectiveness in real-world settings
Creators: name: Mao, Hui-Fen
name: Tsai, Athena Yi-Jung
name: Chang, Ling-Hui
name: Tsai, I-Lu
Publisher: name: figshare
Year: 2021
Subjects: subject: Medicine
subject: Neuroscience
subject: Physiology
subject: FOS: Biological sciences
subject: Biotechnology
subject: 111714 Mental Health
subject: FOS: Health sciences

description: Additional file 1.
Higher-order statistics and intermittency of a two-fluid HVBK quantum turbulent flow
Creators: name: Zhang, Zhentong
name: Danaila, Ionut
name: Lévêque, Emmanuel
name: Danaila, Luminita
Publisher: name: arXiv
Year: 2023
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: The Hall-Vinen-Bekharevich-Khalatnikov (HVBK) model is widely used to numerically study quantum turbulence in superfluid helium. Based on the two-fluid model of Tisza and Landau, the HVBK model describes the normal (viscous) and superfluid (inviscid) components of the flow using two Navier-Stokes type equations, coupled through a mutual friction force term. This feature makes the HVBK model very appealing in applying statistical tools used in classical turbulence to study properties of quantum turbulence. A large body of literature used low-order statistics (spectra, or second-order structure functions in real space) to unravel exchanges between the two fluids at several levels. The novelty in this study is to use a theoretical approach based on first principles to derive transport equations for the third-order moments for each component of velocity.
description: 27 pages, 10 figures, accepted for publication in Journal of Fluid Mechanics