cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Production d'eau purifiée par évaporation solaire à partir de structures 3D imprégnées de charbon actif : étude numérique du système
Creators: name: Fillet, Romain
name: Nicolas, Vincent
name: Celzard, Alain
name: Fierro, Vanessa
Publisher: name: Société Française de Thermique
Year: 2023
Subjects: Simulation
matériaux biosourcés
évaporation solaire
transferts de chaleur et de masse
charbon actif
impression 3D

description: En raison de l'augmentation de la population, de la pollution des rivières et du réchauffement climatique, on estime que d'ici 2050, 3,9 milliards de personnes, soit plus de 40\% de la population mondiale, vivront dans des zones de stress hydrique. Il est donc nécessaire de développer de nouvelles solutions pour produire de l'eau purifiée en utilisant moins d'énergie. L'énergie solaire est prometteuse à exploiter, car la quantité qui atteint la terre en une heure peut couvrir les besoins énergétiques de l'humanité pendant un an. Comme cela a été prouvé, cette énergie est bien adaptée à la production d'eau purifiée par évaporation. Le système d'évaporation consiste à placer un matériau à la surface d'eau non potable pour en accélérer l'évaporation. Ce matériau doit capter suffisamment bien le rayonnement solaire, tout en permettant à l'eau de diffuser vers la surface d'évaporation. Le matériau doit aussi limiter les transferts thermiques vers l'eau liquide afin de conserver l'énergie en surface. Le carbone est un matériau de choix pour cette application : dans la littérature, différents matériaux carbonés ont été utilisés à cette fin, comme la biomasse carbonisée, les nanotubes de carbone, le graphène ou le charbon actif. Dans ce travail, des architectures ont été imprimées en 3D et imprégnées de charbon actif pour améliorer le transport de l'eau et la conversion photothermique lorsqu'elles sont utilisées comme évaporateurs solaires. L'accent a été mis sur la modélisation du processus d'évaporation pour étudier les différents aspects affectant les performances. En effet, l'évaporation étant un processus endothermique, la maîtrise des transferts de chaleur et de masse est essentielle pour optimiser l'efficacité du système. Nous présentons ainsi un modèle numérique 3D permettant de simuler les transferts de vapeur d'eau et de chaleur vers l'air extérieur en modélisant l'écoulement autour des évaporateurs. La simulation de l'écoulement forcé autour de l'évaporateur a pour objectif de développer un modèle plus représentatif des conditions expérimentales. Ainsi, une surface plane 2D et quatre structures 3D présentant une surface concave qui concentre le flux solaire ont été modélisées. A partir de ce modèle, les effets sur le taux d'évaporation du rayonnement de surface à surface d'une part, et de l'aire d'évaporation d'autre part, ont été analysés. De plus, le percement latéral des structures 3D comme piste d'amélioration des performances d'évaporation a été étudié.
Bessel Process and Conformal Quantum Mechanics
Creators: name: Rajabpour, M. A.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Other Condensed Matter (cond-mat.other)
subject: High Energy Physics - Theory (hep-th)
subject: Probability (math.PR)
subject: FOS: Physical sciences
subject: FOS: Mathematics

description: Different aspects of the connection between the Bessel process and the conformal quantum mechanics (CQM) are discussed. The meaning of the possible generalizations of both models is investigated with respect to the other model, including self adjoint extension of the CQM. Some other generalizations such as the Bessel process in the wide sense and radial Ornstein- Uhlenbeck process are discussed with respect to the underlying conformal group structure.
description: 28 Pages
title: ÐÐ½Ð°Ð»Ð¸Ð· Ð¸ Ð¾ÑÐµÐ½ÐºÐ° ÑÑÐµÑÑ ÑÐ¾Ð·Ð½Ð¸ÑÐ½Ð¾Ð¹ ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ð¸ Ð² ÑÑÐ»Ð¾Ð²Ð¸ÑÑ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð³Ð¾ ÐºÑÐ¸Ð·Ð¸ÑÐ°
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: Ð¡Ð°Ð»Ð¸ÑÐ¾Ð²Ð°, ÐÐ½Ð½Ð°
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: 2016
Subjects: ÑÐ¾Ð·Ð½Ð¸ÑÐ½Ð°Ñ ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ñ
Ð¿ÑÐ¸Ð±ÑÐ»Ñ
Ð·Ð°ÑÑÐ°ÑÑ
ÐºÑÐ¸Ð·Ð¸Ñ
retail trade
profit
cost
crisis

description: ÐÐ°Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÑÐµÑ ÑÐ¾Ð±Ð¾Ð¹ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¼ÐµÑÐ¾Ð´Ð¾Ð² ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð¾ÑÐµÐ½ÐºÐ¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¹ ÑÐ¾Ð·Ð½Ð¸ÑÐ½Ð¾Ð¹ ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ð¸ Ð² Ð¿ÐµÑÐ¸Ð¾Ð´ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÐºÑÐ¸Ð·Ð¸ÑÐ°. Ð Ð°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑÑÑ Ð¼ÐµÑÐ¾Ð´Ñ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð¾ÑÐµÐ½ÐºÐ¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¹, Ð° ÑÐ°ÐºÐ¶Ðµ ÑÐ±Ð°Ð»Ð°Ð½ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð½Ð°Ñ ÑÐ¸ÑÑÐµÐ¼Ð° Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»ÐµÐ¹ Ð¸ ÑÐ¾ÑÐ¼Ð¸ÑÑÐµÑÑÑ Ð½Ð¾Ð²ÑÐ¹ Ð¼ÐµÑÐ¾Ð´, Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð½ÑÐ¹ Ð½Ð° ÐºÐ¾Ð¼Ð±Ð¸Ð½Ð°ÑÐ¸Ð¸ Ð´Ð²ÑÑ Ð¿ÑÐµÐ´ÑÐ´ÑÑÐ¸Ñ. Ð Ð°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÐµÑÑÑ ÑÑÐµÑÐ° ÑÐ¾Ð·Ð½Ð¸ÑÐ½Ð¾Ð¹ ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ð¸ Ð¿Ð¾ÑÐ»Ðµ Ð²Ð²ÐµÐ´ÐµÐ½Ð¸Ñ Ð·Ð°Ð¿Ð°Ð´Ð½ÑÑ ÑÐ°Ð½ÐºÑÐ¸Ð¹ Ð¸ Ð½Ð°ÑÑÑÐ¿Ð»ÐµÐ½Ð¸Ñ ÐºÑÐ¸Ð·Ð¸ÑÐ°, ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑÑÑ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¾ÑÐ½Ð¾Ð²Ñ Ð²ÐµÐ´ÐµÐ½Ð¸Ñ ÑÐ¾Ð·Ð½Ð¸ÑÐ½Ð¾Ð¹ ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ð¸ Ð² Ð Ð¤.
description: This paper presents an analysis of the economic evaluation methods of retailers during the economic crisis. It contains the methods of economic evaluation of companies, the balanced scorecard, and forming a new method based on a combination of the previous two. We consider the sphere of retail trade after the introduction of Western sanctions and the onset of the crisis and examine the theoretical bases of conducting retail procedures in Russia.
Additional file 5 of Papillary thyroid cancer organoids harboring BRAFV600E mutation reveal potentially beneficial effects of BRAF inhibitor-based combination therapies
Creators: name: Chen, Dong
name: Su, Xi
name: Zhu, Lizhang
name: Jia, Hao
name: Han, Bin
name: Chen, Haibo
name: Liang, Qingzhuang
name: Hu, Chenchen
name: Yang, Hao
name: Liu, Lisa
name: Li, Peng
name: Wei, Wei
name: Zhao, Yongsheng
Publisher: name: figshare
Year: 2023
Subjects: subject: Biochemistry
subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Pharmacology
subject: Biotechnology
subject: Chemical Sciences not elsewhere classified
subject: Biological Sciences not elsewhere classified
subject: Cancer
subject: Virology

description: Additional file 5: Figure S5. The Combination Index (CI) versus Fractional Effect plot for the indicated drug combinations, according to the Chou-Talalay dose-effect method. The CI < 1.0, CI = 1.0, and CI > 1.0 indicate synergism, additivity, and antagonism, respectively.
Can the zero-point energy of the quantized harmonic oscillator be lower? Possible implications for the physics of 'dark energy' and 'dark matter'
Creators: name: Kastrup, Hans
Publisher: name: Deutsches Elektronen-Synchrotron, DESY, Hamburg
Year: 2020
Subjects: * Automatic Keywords *
energy: zero-point
oscillator: harmonic
energy: quantization
wave: electromagnetic
dark energy: density
dark matter
symplectic
nucleus
cosmological model
phase space
Hamiltonian
topological
radio wave
structure
infrared
hydrogen
SO(1,2)
WIMP

description: Replacing the canonical pair q and p of the harmonic oscillator (HO) by the locally and symplectically equivalent pair angle phi and action variable I implies a qualitative change of the global topological structure of the associated phase spaces: the pair (q,p) is an element of a topologically trivial plane R^2 whereas the pair (phi,I>0) is an element of a topologically non-trivial, infinitely connected, punctured plane R^2-{0}, which has the group SO(1,2) as its 'canonical' group. Due to its infinitely many covering groups the resulting ('symplectic') spectrum of the associated quantum Hamiltonian is given by {hbar omega (n+b), n =0,1,...; b in (0,1]}, in contrast to the 'orthodox' spectrum {hbar omega (n+1/2)}. The potentially most important implications concern the vibrations of diatomic molecules in the infrared, e.g. those of molecular hydrogen H_2. Those symplectic spectra of the HO may provide a simultaneous key to two outstanding astrophysical puzzles, namely the nature of dark (vacuum) energy and that of dark matter: To the former because the zero-point energy b hbar omega of free electromagnetic wave oscillator modes can be extremely small > 0 (b ca. exp(-35) for the measured dark energy density). And a key to the dark matter problem because the quantum zero-point energies of the Born-Oppenheimer potentials in which the two nuclei of H_2 or the nuclei of other primordial diatomic molecules vibrate can be lower, too, and, therefore, may lead to spectrally detuned 'dark' H_2 molecules during the 'Dark Ages' of the universe and forming WIMPs in the hypothesized sense. All results appear to be in surprisingly good agreement with the LambdaCDM model of the universe. Besides laboratory experiments the search for 21-cm radio signals from the Dark Ages of the universe and other astrophysical observations can help to explore those hypothetical implications.
Structure and History of Dark Matter Halos Probed with Gravitational Lensing
Creators: name: Lapi, A.
name: Cavaliere, A.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We test with gravitational lensing data the dark matter (DM) halos embedding the luminous baryonic component of galaxy clusters; our benchmark is provided by their two-stage cosmogonical development that we compute with its variance, and by the related 'α-profiles' we derive. The latter solve the Jeans equation for the self-gravitating, anisotropic DM equilibria, and yield the radial runs of the density ρ(r) and the velocity dispersion σ_r^2(r) in terms of the DM 'entropy' K = σ_r^2/ρ^(2/3) ~ r^(α) highlighted by recent N-body simulations; the former constrains the slope to the narrow range α~ 1.25 - 1.3. These physically based α-profiles meet the overall requirements from gravitational lensing observations, being intrinsically flatter at the center and steeper in the outskirts relative to the empirical NFW formula. Specifically, we project them along the l.o.s. and compare with a recent extensive dataset from strong and weak lensing observations in and around the cluster A1689. We find an optimal fit at both small and large scales in terms of a halo constituted by an early body with α~ 1.25 and by recent extensive outskirts, that make up an overall mass 10^15 M_sun with a concentration parameter c ~ 10 consistent with the variance we compute in the \LambdaCDM cosmogony. The resulting structure corresponds to a potential well shallow in the outskirts as that inferred from the X rays radiated from the hot electrons and baryons constituting the intracluster plasma.
description: 5 pages, 3 figures, uses RevTeX4 + emulateapj.cls and apjfonts.sty. Accepted by ApJL
title: ÐÑÐ½Ð¾Ð²Ð½ÑÐµ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐµÐ³ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÑÑÐ°Ñ Ð¾Ð²Ð¾Ð³Ð¾ ÑÑÐ½ÐºÐ° Ð² Ð Ð¤
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: ÐÐµÐ»ÑÑÐ¸Ð½, Ð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: 2017
Subjects: ÑÑÑÐ°Ñ Ð¾Ð²Ð°Ð½Ð¸Ðµ
ÑÑÑÐ°Ñ Ð¾Ð²Ð¾Ð¹ ÑÑÐ½Ð¾Ðº
ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÐµ ÑÑÐ½ÐºÐ¸
ÑÑÑÐ°Ñ Ð¾Ð²Ð¾Ð¹ Ð½Ð°Ð´Ð·Ð¾Ñ
Ð±Ð»Ð¾ÐºÑÐµÐ¹Ð½

description: ÐÐ±ÑÐµÐºÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ - ÑÑÑÐ°ÑÐ¾Ð²Ð¾Ð¹ ÑÑÐ½Ð¾Ðº Ð Ð¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð¹ Ð¤ÐµÐ´ÐµÑÐ°ÑÐ¸Ð¸. Ð¦ÐµÐ»Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ð¸ - ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐµÐ³ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÑÑÐ°ÑÐ¾Ð²Ð¾Ð³Ð¾ ÑÑÐ½ÐºÐ° Ð² Ð Ð¾ÑÑÐ¸Ð¸ Ð´Ð»Ñ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ¸ ÑÑÑÐ°Ð½Ñ Ð¸ Ð¿ÑÐµÐ´Ð¾ÑÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð½Ð°Ð´ÐµÐ¶Ð½ÑÑ Ð³Ð°ÑÐ°Ð½ÑÐ¸Ð¹ ÑÑÑÐ°ÑÐ¾Ð²Ð°ÑÐµÐ»ÑÐ¼. Ð Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ¾Ð¹ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ð¸ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð·Ð½Ð°ÑÐµÐ½Ð¸Ðµ, ÑÑÑÐ½Ð¾ÑÑÑ ÑÑÑÐ°ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¸ ÑÑÐ½ÐºÐ° ÑÑÑÐ°ÑÐ¾Ð²ÑÑ ÑÑÐ»ÑÐ³, Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÐµÐ³ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÑÑÐ°ÑÐ¾Ð²Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¸ ÑÐ¿ÐµÑÐ¸ÑÐ¸ÐºÐ° Ð¾ÑÐ³Ð°Ð½Ð¾Ð² ÑÑÑÐ°ÑÐ¾Ð²Ð¾Ð³Ð¾ Ð½Ð°Ð´Ð·Ð¾ÑÐ° Ð² Ð Ð¾ÑÑÐ¸Ð¸. ÐÑÐ¸Ð²ÐµÐ´ÐµÐ½ Ð¾Ð±Ð·Ð¾Ñ Ð¿ÑÐ¸Ð¼ÐµÐ½ÑÐµÐ¼ÑÑ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² ÑÐµÐ³ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÑÑÐ°ÑÐ¾Ð²Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸, Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ñ ÑÑÑÐ°ÑÐ¾Ð²Ð¾Ð³Ð¾ ÑÑÐ½ÐºÐ° Ð² Ð¿ÐµÑÐ¸Ð¾Ð´ Ñ 2014-2016 Ð³. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð° Ð¾ÑÐµÐ½ÐºÐ° Ð²Ð»Ð¸ÑÐ½Ð¸Ñ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÐµÐ³ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð½Ð° ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÑÑÑÐ°ÑÐ¾Ð²Ð¾Ð³Ð¾ ÑÑÐ½ÐºÐ° Ð¸ Ð²ÑÑÐ²Ð»ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐµÐ³ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÑÑÐ°ÑÐ¾Ð²Ð¾Ð³Ð¾ ÑÑÐ½ÐºÐ° Ð Ð¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð¹ Ð¤ÐµÐ´ÐµÑÐ°ÑÐ¸Ð¸.Ð ÑÐ°ÐºÐ¶Ðµ Ð²ÑÑÐ²Ð»ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐµÐ³ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÑÑÐ°ÑÐ¾Ð²Ð¾Ð³Ð¾ ÑÑÐ½ÐºÐ°, Ð° Ð¸Ð¼ÐµÐ½Ð½Ð¾ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ðµ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð±Ð»Ð¾ÐºÑÐµÐ¹Ð½ Ð² ÑÑÐµÑÐµ ÑÑÐ½ÐºÐ° ÑÑÑÐ°ÑÐ¾Ð²ÑÑ ÑÑÐ»ÑÐ³, Ð° ÑÐ°ÐºÐ¶Ðµ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ðµ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¿Ð¾ÑÐ°ÑÐ¾Ð²Ð¾Ð³Ð¾ ÑÑÑÐ°ÑÐ¾Ð²Ð°Ð½Ð¸Ñ.
Flora diversity survey and establishment of a plant DNA barcode database of Lomas ecosystems in Peru
Creators: name: Song, Feng
name: Deng, Yun-Fei
name: Yan, Hai-Fei
name: Ge, Xue-Jun
name: Lin, Zhe-Li
name: Delgado, Amalia
name: Trinidad, Huber
name: Arce, Paul Gonzales
name: Riva, Sebastián
name: Cano-Echevarría, sunción
name: Ramos, Elmer
name: Aroni, Yaquelin Pamela
name: Rivera, Soledad
name: Arakaki, Mónica
name: Ge, Xue-Jun
Publisher: name: figshare
Year: 2023
Subjects: Plant biology not elsewhere classified

description: Dataset for "Flora diversity survey and establishment of a plant DNA barcode database of Lomas ecosystems in Peru "
Additional file 3 of Papillary thyroid cancer organoids harboring BRAFV600E mutation reveal potentially beneficial effects of BRAF inhibitor-based combination therapies
Creators: name: Chen, Dong
name: Su, Xi
name: Zhu, Lizhang
name: Jia, Hao
name: Han, Bin
name: Chen, Haibo
name: Liang, Qingzhuang
name: Hu, Chenchen
name: Yang, Hao
name: Liu, Lisa
name: Li, Peng
name: Wei, Wei
name: Zhao, Yongsheng
Publisher: name: figshare
Year: 2023
Subjects: subject: Biochemistry
subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Pharmacology
subject: Biotechnology
subject: Chemical Sciences not elsewhere classified
subject: Biological Sciences not elsewhere classified
subject: Cancer
subject: Virology

description: Additional file 3: Figure S3. Drug response to 13 anticancer agents. PTC organoids were subjected to the targeted drugs vemurafenib, dabrafenib, selumetinib, trametinib, sorafenib, lenvatinib, cabozantinib, vandetanib, and sunitinib, and chemotherapy drugs doxorubicin, vincristine, paclitaxel, and cisplatin. Organoid viability was measured and plotted as percentage of untreated organoids.
Small-spatial scale variations of nebular properties and the abundance discrepancy in three Galactic HII regions
Creators: name: Mesa-Delgado, A.
name: Esteban, C.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present results of long-slit spectroscopy in several slit positions that cover different morphological structures of the central parts of three bright Galactic HII regions: M8, M17 and NGC7635. We study the spatial distributions of a large number of nebular parameters such as the extinction coefficient, line fluxes, physical conditions and ionic abundances at the maximum spatial resolution attainable with our instrumentation. Particularly, our goal is to study the behaviour of the abundance discrepancy factor of O^{2+}, ADF(O^{2+}), defined as the logarithmic difference of the O^{2+} abundances derived from collisionally excited and recombination lines. We find that the ADF(O^{2+}) remains fairly constant along the slit positions of M8 and M17. In the case of NGC7635, we only detect the OII recombination lines in the integrated spectrum along the whole slit, where the ADF(O^{2+}) reaches a remarkably high value of about 0.59 dex. We compare our results with previous ones obtained for the Orion Nebula. We find several evidences that suggest the presence of a candidate to Herbig-Haro object in M8.
description: 18 pages, 9 figures. Table A1 available only in the online version. Accepted for publication in MNRAS.
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¸ ÑÐµÑÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¿ÑÐ¾ÑÐ¸Ð²Ð¾Ð°Ð²Ð°ÑÐ¸Ð¹Ð½Ð¾Ð³Ð¾ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¸Ð·Ð¾Ð»Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð¹ ÑÐ½ÐµÑÐ³Ð¾ÑÐ¸ÑÑÐµÐ¼Ð¾Ð¹
title: ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÑ 05.14.02 â Ð­Ð»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÑÐ°Ð½ÑÐ¸Ð¸ Ð¸ ÑÐ»ÐµÐºÑÑÐ¾ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÐ¸ÑÑÐµÐ¼Ñ
titleType: Subtitle
Creators: name: ÐÐ½Ð´ÑÐ°Ð½Ð¾Ð²Ð¸Ñ, ÐÐ¾Ð³Ð´Ð°Ð½
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: 2022
Subjects: ÐÐ°Ð·Ð¾ÑÑÑÐ±Ð¸Ð½Ð½ÑÐµ ÑÑÑÐ°Ð½Ð¾Ð²ÐºÐ¸
ÐÐ°ÑÐ¾Ð³Ð°Ð·Ð¾Ð²ÑÐµ ÑÑÑÐ°Ð½Ð¾Ð²ÐºÐ¸
Ð­Ð½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÐ¸ÑÑÐµÐ¼Ñ
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description: ÐÐ¸ÑÑÐµÑÑÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° Ð²Ð¾Ð¿ÑÐ¾ÑÐ°Ð¼ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¿ÑÐ¾ÑÐ¸Ð²Ð¾Ð°Ð²Ð°ÑÐ¸Ð¹Ð½Ð¾Ð³Ð¾ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð² Ð¸Ð·Ð¾Ð»Ð¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÑ ÑÐ½ÐµÑÐ³Ð¾ÑÐ¸ÑÑÐµÐ¼Ð°Ñ Ñ Ð¿ÑÐµÐ¾Ð±Ð»Ð°Ð´Ð°Ð½Ð¸ÐµÐ¼ Ð² ÑÑÑÑÐºÑÑÑÐµ Ð³ÐµÐ½ÐµÑÐ¸ÑÑÑÑÐ¸Ñ Ð¼Ð¾ÑÐ½Ð¾ÑÑÐµÐ¹ Ð³Ð°Ð·Ð¾ÑÑÑÐ±Ð¸Ð½Ð½ÑÑ Ð¸ Ð¿Ð°ÑÐ¾Ð³Ð°Ð·Ð¾Ð²ÑÑ ÑÑÑÐ°Ð½Ð¾Ð²Ð¾Ðº. Ð ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð° Ð½Ð¾Ð²Ð°Ñ ÑÐ¸ÑÑÐµÐ¼Ð° Ð¿ÑÐ¾ÑÐ¸Ð²Ð¾Ð°Ð²Ð°ÑÐ¸Ð¹Ð½Ð¾Ð¹ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸ÐºÐ¸, Ð¾ÑÑÑÐµÑÑÐ²Ð»ÑÑÑÐ°Ñ Ð² ÑÐµÐ¶Ð¸Ð¼Ðµ ÑÐµÐ°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð²ÑÐµÐ¼ÐµÐ½Ð¸ ÑÐ°ÑÑÑÑ Ð¸ ÑÐ¸Ð·Ð¸ÑÐµÑÐºÑÑ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ Ð¾Ð±ÑÑÐ¼Ð¾Ð² ÑÐ¿ÑÐ°Ð²Ð»ÑÑÑÐ¸Ñ Ð²Ð¾Ð·Ð´ÐµÐ¹ÑÑÐ²Ð¸Ð¹, ÐºÐ¾ÑÐ¾ÑÑÐµ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ñ Ð½Ð° Ð¿ÑÐµÐ´Ð¾ÑÐ²ÑÐ°ÑÐµÐ½Ð¸Ðµ ÑÑÐ°Ð±Ð°ÑÑÐ²Ð°Ð½Ð¸Ñ ÑÑÑÑÐ¾Ð¹ÑÑÐ² Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÑÐ°ÑÑÐ¾ÑÐ½Ð¾Ð¹ ÑÐ°Ð·Ð³ÑÑÐ·ÐºÐ¸ Ð² Ð¿ÐµÑÐµÑÐ¾Ð´Ð½Ð¾Ð¼ Ð¿ÑÐ¾ÑÐµÑÑÐµ Ð¸ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ðµ Ð´Ð¾Ð¿ÑÑÑÐ¸Ð¼ÑÑ Ð¿Ð¾ÑÐ»ÐµÐ°Ð²Ð°ÑÐ¸Ð¹Ð½ÑÑ Ð·Ð½Ð°ÑÐµÐ½Ð¸Ð¹ ÑÐ°ÑÑÐ¾ÑÑ Ð¿ÐµÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÐ¾ÐºÐ°. ÐÐ¿ÑÐ¾Ð±Ð°ÑÐ¸Ñ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¾Ð² Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ Ð±ÑÐ»Ð° Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð° Ð²Ð¾ Ð²ÑÐµÐ¼Ñ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ Ð½Ð°ÑÑÑÐ½ÑÑ Ð¸ÑÐ¿ÑÑÐ°Ð½Ð¸Ð¹ Ð¿Ð¾ Ð²ÑÐ´ÐµÐ»ÐµÐ½Ð¸Ñ ÑÐ½ÐµÑÐ³Ð¾ÑÐ¸ÑÑÐµÐ¼Ñ ÐÐ°Ð»Ð¸Ð½Ð¸Ð½Ð³ÑÐ°Ð´ÑÐºÐ¾Ð¹ Ð¾Ð±Ð»Ð°ÑÑÐ¸ Ð½Ð° Ð¸Ð·Ð¾Ð»Ð¸ÑÐ¾Ð²Ð°Ð½Ð½ÑÑ ÑÐ°Ð±Ð¾ÑÑ.
Feshbach Shape Resonance for High Tc Pairing in Superlattices of Quantum Stripes and Quantum Wells
Creators: name: Bianconi, Antonio
Publisher: name: arXiv
Year: 2008
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: The Feshbach shape resonances in the interband pairing in superconducting superlattices of quantum wells or quantum stripes is shown to provide the mechanism for high Tc superconductivity. This mechanism provides the Tc amplification driven by the architecture of material: superlattices of quantum wells (intercalated graphite or diborides) and superlattices of quantum stripes (doped high Tc cuprate perovskites) where the chemical potential is tuned to a Van Hove-Lifshitz singularity (vHs) in the electronic energy spectrum of the superlattice associated with the change of the Fermi surface dimensionality in one of the subbands.
description: 15 pages, 13 figures
Effelsberg 100-m polarimetric observations of a sample of Compact Steep-Spectrum sources
Creators: name: Mantovani, F.
name: Mack, K. -H.
name: Montenegro-Montes, F. M.
name: Rossetti, A.
name: Kraus, A.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We completed observations with the Effelsberg 100-m radio telescope to measure the polarised emission from a complete sample of Compact Steep-Spectrum sources. We observed the sources at four different frequencies. We complemented these measurements with polarisation parameters at 1.4 GHz derived from the NVSS. Previous single dish measurements were taken from the catalogue of Tabara and Inoue. The depolarisation index DP was computed for four pairs of frequencies. A drop in the fractional polarisation appeared in the radio emission when observing at frequencies below about 2 GHz. Rotation measures were derived for about 25% of the sources in the sample. The values range from about -20 rad/m**2} found for 3C138 to 3900 rad/m**2 in 3C119. In all cases, the lambda**2 law is closely followed. The presence of a foreground screen as predicted by the Tribble model or with ``partial coverage'' as defined by ourselves can explain the polarimetric behaviour of the CSS sources detected in polarisation by the present observations. Indication of repolarisation at lower frequencies was found for some sources. A case of possible variability in the fractional polarisation is also suggested. The most unexpected result was found for the distribution of the fractional polarisations versus the linear sizes of the sources. Our results appear to disagree with the findings of Cotton and collaborators and Fanti and collaborators for the B3-VLA sample of CSS sources, the so-called ``Cotton effect''. This apparent contradiction may, however, be caused by the large contamination of the sample by quasars with respect to the B3-VLA.
description: Astronomy and Astrophysycs, in press
title: ÐÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð²Ð½Ð¾-ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¿Ð¾ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ ÑÑÐµÑÐ¸Ð½Ð¾ÑÑÐ¾Ð¹ÐºÐ¾ÑÑÐ¸ Ð¸ Ð¼Ð¾Ð½Ð¾Ð»Ð¸ÑÐ½Ð¾ÑÑÐ¸ Ð¼Ð°ÑÑÐ¸Ð²Ð½ÑÑ Ð±ÐµÑÐ¾Ð½Ð½ÑÑ Ð³Ð¸Ð´ÑÐ¾ÑÐµÑ Ð½Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ¾Ð¾ÑÑÐ¶ÐµÐ½Ð¸Ð¹
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: Ð¢ÐµÐ»ÐµÑÐµÐ², ÐÐ¸ÐºÑÐ¾Ñ
Publisher: name: ÐÐÐ
Year: 1983
Subjects: ÐÐ¸Ð´ÑÐ¾ÑÐµÑ Ð½Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐ¾Ð¾ÑÑÐ¶ÐµÐ½Ð¸Ñ Ð±ÐµÑÐ¾Ð½Ð½ÑÐµ

description: Ð£ÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð¿ÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð²ÑÐµÑ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐµÐ¹ Ð³Ð¸Ð´ÑÐ¾ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ°ÐºÑÐ»ÑÑÐµÑÐ° Ð¿ÑÐ¸ Ð¸Ð·ÑÑÐµÐ½Ð¸Ð¸ Ð¸Ð¼Ð¸ ÑÐ°Ð·Ð´ÐµÐ»Ð° Â«ÐÐµÑÐ¾Ð½Ð½ÑÐµ ÑÐ°Ð±Ð¾ÑÑÂ» Ð² ÐºÑÑÑÐµ Â«Ð¢ÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ñ Ð³Ð¸Ð´ÑÐ¾ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ°Ð±Ð¾ÑÂ», Ð° ÑÐ°ÐºÐ¶Ðµ Ð¼Ð¾Ð¶ÐµÑ Ð±ÑÑÑ Ð¿Ð¾Ð»ÐµÐ·Ð½Ð¾ Ð´Ð»Ñ Ð¸Ð½Ð¶ÐµÐ½ÐµÑÐ½Ð¾-ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ°Ð±Ð¾ÑÐ½Ð¸ÐºÐ¾Ð² Ð¿ÑÐ¾ÐµÐºÑÐ½ÑÑ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¹, Ð·Ð°Ð½Ð¸Ð¼Ð°ÑÑÐ¸ÑÑÑ Ð²Ð¾Ð¿ÑÐ¾ÑÐ°Ð¼Ð¸ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¼Ð°ÑÑÐ¸Ð²Ð½ÑÑ Ð±ÐµÑÐ¾Ð½Ð½ÑÑ Ð³Ð¸Ð´ÑÐ¾ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ¾Ð¾ÑÑÐ¶ÐµÐ½Ð¸Ð¹. Ð Ð¿Ð¾ÑÐ¾Ð±Ð¸Ð¸ Ð¾ÑÐ²ÐµÑÐµÐ½Ñ Ð¾Ð±ÑÐ¸Ðµ ÑÑÐµÐ±Ð¾Ð²Ð°Ð½Ð¸Ñ Ðº Ð³Ð¸Ð´ÑÐ¾ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð¼Ñ Ð±ÐµÑÐ¾Ð½Ñ, ÑÑÐµÐ±Ð¾Ð²Ð°Ð½Ð¸Ñ Ðº ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¸ Ð¼Ð°ÑÑÐ¸Ð²Ð½ÑÑ Ð±ÐµÑÐ¾Ð½Ð½ÑÑ ÑÐ¾Ð¾ÑÑÐ¶ÐµÐ½Ð¸Ð¹ Ð¸ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð¸Ñ Ð²Ð¾Ð·Ð²ÐµÐ´ÐµÐ½Ð¸Ñ Ð´Ð»Ñ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ Ð¸Ñ ÑÑÐµÑÐ¸Ð½Ð¾ÑÑÐ¾Ð¹ÐºÐ¾ÑÑÐ¸ Ð¸ Ð¼Ð¾Ð½Ð¾Ð»Ð¸ÑÐ½Ð¾ÑÑÐ¸. ÐÐ·Ð»Ð¾Ð¶ÐµÐ½Ñ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ°Ð·ÑÐµÐ·ÐºÐ¸ ÑÐ¾Ð¾ÑÑÐ¶ÐµÐ½Ð¸Ð¹ Ð½Ð° Ð±Ð»Ð¾ÐºÐ¸ Ð±ÐµÑÐ¾Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¸ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¿Ð¾ Ð¸Ñ Ð¾Ð¼Ð¾Ð½Ð¾Ð»Ð¸ÑÐ¸Ð²Ð°Ð½Ð¸Ñ, ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¿Ð¾ ÑÐµÐ³ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐµÐ¼Ð¿ÐµÑÐ°ÑÑÑÐ½Ð¾Ð³Ð¾ ÑÐµÐ¶Ð¸Ð¼Ð° Ð±Ð»Ð¾ÐºÐ¾Ð² Ð±ÐµÑÐ¾Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ. ÐÑÐ¾Ð±Ð¾Ðµ Ð²Ð½Ð¸Ð¼Ð°Ð½Ð¸Ðµ ÑÐ´ÐµÐ»ÐµÐ½Ð¾ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ð¼ Ð¾ÑÐ½Ð¾Ð²Ð°Ð¼ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ ÑÑÐµÐ±Ð¾Ð²Ð°Ð½Ð¸Ð¹ Ðº ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð±ÐµÑÐ¾Ð½Ð½ÑÑ ÑÐ°Ð±Ð¾Ñ Ð´Ð»Ñ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ ÑÑÐµÑÐ¸Ð½Ð¾ÑÑÐ¾Ð¹ÐºÐ¾ÑÑÐ¸ Ð¸ Ð¼Ð¾Ð½Ð¾Ð»Ð¸ÑÐ½Ð¾ÑÑÐ¸ Ð¼Ð°ÑÑÐ¸Ð²Ð½ÑÑ Ð±ÐµÑÐ¾Ð½Ð½ÑÑ Ð³Ð¸Ð´ÑÐ¾ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ¾Ð¾ÑÑÐ¶ÐµÐ½Ð¸Ð¹.
Secondary Parameters of Type Ia Supernova Light Curves
Creators: name: Hoeflich, P.
name: Krisciunas, K.
name: Khokhlov, A. M.
name: Baron, E.
name: Folatelli, G.
name: Hamuy, M.
name: Phillips, M. M.
name: Suntzeff, N.
name: Wang, L.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: High-quality observations of $B$ and $V$ light curves obtained at Las Campanas Observatory for local Type Ia Supernovae (SNe Ia) show clear evidence that SNe Ia with the same brightness decline or stretch may have systematic and independent deviations at times < 5 days before and at times > 30 days after maximum light. This suggests the existence of two independent secondary parameters which control the shape of SN Ia light curves in addition to the brightness decline relation. stretch. The differences are consistent in morphology of the time dependence and size with predictions by models within the delayed detonation scenario. The secondary parameters may reflect two independent physical effects caused by variations in the progenitor and accretion rates, and link the LC variations in shape with the intrinsic, absolute brightness.
description: 32 pages, 9 Figures, ApJ accepted
title: ÐÑÐµÐ½ÐºÐ° Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿Ð¾ÑÐµÐ½ÑÐ¸Ð°Ð»Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð¡Ð¸Ð²ÑÑÐ°, ÐÐ¸ÐºÑÐ¾ÑÐ¸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: 2016
Subjects: ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð¿Ð¾ÑÐµÐ½ÑÐ¸Ð°Ð»
Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ðµ
Ð±Ð°Ð½ÐºÐ¸
economic potential
enterprise
banks

description: Ð ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÐµÑÑÑ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð¿Ð¾ÑÐµÐ½ÑÐ¸Ð°Ð», ÑÐ¿Ð¾ÑÐ¾Ð±Ñ ÐµÐ³Ð¾ Ð¾ÑÐµÐ½ÐºÐ¸. ÐÐ½Ð°Ð»Ð¸Ð·Ð¸ÑÑÐµÑÑÑ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ðµ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ðµ Ð±Ð°Ð½ÐºÐ° ÐÐ¢Ð 24, Ð²ÑÑÐ²Ð»ÑÑÑÑÑ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ Ð¸ Ð´Ð°ÑÑÑÑ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¿Ð¾ ÑÐ²ÐµÐ»Ð¸ÑÐµÐ½Ð¸Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸.
description: In work the economic potential, ways of his assessment is considered. The financial condition of VTB 24 bank is analyzed, the main problems come to light and recommendations about increase in efficiency of activity of the company are made.
title: Ð¢ÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð¿ÑÐ¾ÑÐµÑÑ Ð¸Ð·Ð³Ð¾ÑÐ¾Ð²Ð»ÐµÐ½Ð¸Ñ Ð´ÐµÑÐ°Ð»Ð¸ Â«ÐÐ°Ð»Â»
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
Creators: name: Ð¡Ð°Ð²Ð¸Ð½Ð¾Ð²Ð°, ÐÐ»ÐµÐ½Ð°
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: 2018
Subjects: ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ñ Ð¼Ð°ÑÐ¸Ð½Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ñ
ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð¿ÑÐ¾ÑÐµÑÑ
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description: Ð¢ÐµÐ¼Ð° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ - Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð¸Ð·Ð³Ð¾ÑÐ¾Ð²Ð»ÐµÐ½Ð¸Ñ Ð²Ð°Ð»Ð°, Ð´Ð»Ñ ÐºÐ¾ÑÐ¾ÑÐ¾Ð¹ Ð±ÑÐ»Ð¸ ÑÐ¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ñ Ð·Ð°Ð³Ð¾ÑÐ¾Ð²ÐºÐ°, ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¾Ð¿ÐµÑÐ°ÑÐ¸Ð¸ Ð¸ Ð¿ÐµÑÐµÑÐ¾Ð´Ñ, Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ñ ÑÐµÐ¶Ð¸Ð¼Ñ ÑÐµÐ·Ð°Ð½Ð¸Ñ, Ð¿Ð¾ÑÑÐ¸ÑÐ°Ð½Ñ Ð½Ð°Ð»Ð°Ð´Ð¾ÑÐ½ÑÐµ ÑÐ°Ð·Ð¼ÐµÑÑ.ÐÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ°:
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The independent contribution of muscle strength or cardiorespiratory fitness to cognitive health in aging adults.
Creators: name: Zou, Jammy
Publisher: name: University of British Columbia
Year: 2024

description: As the world’s population ages, the number of people affected by dementia and the overall burden of the disease continues to grow. Research dedicated to refining strategies to reduce the risk of cognitive decline and dementia are of vital importance to promote cognitive health. Exercise can play a neuroprotective role by mitigating the consequences of physical inactivity such as low muscle strength and cardiorespiratory fitness. However, limited studies have focused on examining the contribution of muscle strength and cardiorespiratory fitness for maintaining cognitive function in mid-to-late life. In this thesis, I conducted a secondary analysis using the Canadian Space Agency (CSA) Inactivity Study, a randomized controlled trial (RCT) of either: 1) 14 days 6° head-down tilt bed rest (HDBR); or 2) HDBR with daily resistance training (RT) and aerobic training (AT) to examine the independent and relative contribution of change in muscle strength and change in cardiorespiratory fitness on cognitive function in adults aged over 55 years. Results from multiple linear regressions showed that change in muscle strength, but not cardiorespiratory fitness was significantly associated with improved executive function following 14 days of HDBR. This finding prompted the inclusion of the Reshaping the Path of Vascular Cognitive Impairment (RVCI) trial, a RCT of 12-month, twice-weekly RT vs. active control in community-dwelling adults with vascular cognitive impairment to further examine the relationship between change muscle strength and cognitive function. Using data from RVCI, results from multiple linear regressions showed that muscle strength was positively associated with processing speed and working memory. The RVCI dataset addresses the limitations of the CSA study by providing a larger sample size, a non-HDBR sample, and a greater RT stimulus. This thesis provides preliminary evidence that maintaining muscle strength may be critical for preserving cognitive function in aging adults who experience bed rest or have cerebral small vessel disease. Importantly, this thesis prompts future research to examine: 1) the effect of exercise modality; and 2) the mediating factors between exercise and cognitive health. A better understanding will inform public health policies to help provide more precise exercise recommendations that focus on promoting healthy cognitive aging.
title: ÐÐ½Ð°Ð»Ð¸Ð· ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÑÐ°Ð±Ð¾ÑÑ ÑÐµÐ½ÑÑÐ°Ð»Ð¸Ð·Ð¾Ð²Ð°Ð½Ð½Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¿ÑÐ¾ÑÐ¸Ð²Ð¾Ð°Ð²Ð°ÑÐ¸Ð¹Ð½Ð¾Ð¹ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸ÐºÐ¸ Ð² ÐÐ­Ð¡ Ð¡ÐµÐ²ÐµÑÐ¾-ÐÐ°Ð¿Ð°Ð´Ð°
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Ð¸ÐºÑÐ»Ð¸Ð½Ð°, ÐÐºÐ°ÑÐµÑ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: 2018
Subjects: Ð­Ð½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÐ¸ÑÑÐµÐ¼Ñ
Ð­Ð»ÐµÐºÑÑÐ¾ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÐ¸ÑÑÐµÐ¼Ñ

description: Ð ÑÐ°Ð±Ð¾ÑÐµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð° ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ ÑÐ°Ð±Ð¾ÑÑ ÑÐµÐ½ÑÑÐ°Ð»Ð¸Ð·Ð¾Ð²Ð°Ð½Ð½Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¿ÑÐ¾ÑÐ¸Ð²Ð¾Ð°Ð²Ð°ÑÐ¸Ð¹Ð½Ð¾Ð¹ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸ÐºÐ¸ Ð² ÐÐ­Ð¡ Ð¡ÐµÐ²ÐµÑÐ¾-ÐÐ°Ð¿Ð°Ð´Ð°. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð° ÑÑÑÑÐºÑÑÑÐ° Ð¦Ð¡ÐÐ, ÐµÐµ Ð°Ð¿Ð¿Ð°ÑÐ°ÑÐ½ÑÐ¹ Ð¸ ÑÑÐ½ÐºÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½ÑÐ¹ ÑÐ¾ÑÑÐ°Ð². ÐÑÐ¸Ð²ÐµÐ´ÐµÐ½Ñ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð¦Ð¡ÐÐ ÐÐ­Ð¡ Ð¡ÐµÐ²ÐµÑÐ¾-ÐÐ°Ð¿Ð°Ð´Ð°. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ ÑÐµÐ¶Ð¸Ð¼Ñ ÑÐ°Ð±Ð¾ÑÑ ÐÐ¢Ð Ð¦Ð¡ÐÐ. ÐÑÐ¸Ð²ÐµÐ´ÐµÐ½Ñ Ð¿ÑÑÐºÐ¾Ð²ÑÐµ Ð¾ÑÐ³Ð°Ð½Ñ, Ð·Ð°Ð²ÐµÐ´ÐµÐ½Ð½ÑÐµ Ð½Ð° ÐºÐ»ÐµÐ¼Ð¼Ñ Ð½Ð¸Ð·Ð¾Ð²Ð¾Ð³Ð¾ ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð°, Ð¸ ÑÐ¿ÑÐ°Ð²Ð»ÑÑÑÐ¸Ðµ Ð²Ð¾Ð·Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ, Ð´Ð¾ÑÑÑÐ¿Ð½ÑÐµ Ð´Ð»Ñ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¾Ñ Ð¦Ð¡ÐÐ ÐÐ­Ð¡ Ð¡ÐµÐ²ÐµÑÐ¾-ÐÐ°Ð¿Ð°Ð´Ð°. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÐºÐ¾ÑÑÐµÐºÑÐ½Ð¾ÑÑÐ¸ Ð²ÑÐ±Ð¾ÑÐ° ÑÐ¿ÑÐ°Ð²Ð»ÑÑÑÐ¸Ñ Ð²Ð¾Ð·Ð´ÐµÐ¹ÑÑÐ²Ð¸Ð¹.
Thermal and quantum fluctuations in chains of ultracold polar molecules
Creators: name: Astrakharchik, G. E.
name: De Chiara, Gabriele
name: Morigi, Giovanna
name: Boronat, Jordi
Publisher: name: arXiv
Year: 2009
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Ultracold polar molecules, in highly anisotropic traps and interacting via a repulsive dipolar potential, may form one-dimensional chains at high densities. According to classical theory, at low temperatures there exists a critical value of the density at which a second order phase transition from a linear to a zigzag chain occurs. We study the effect of thermal and quantum fluctuations on these self-organized structures using classical and quantum Monte Carlo methods, by means of which we evaluate the pair correlation function and the static structure factor. Depending on the parameters, these functions exhibit properties typical of a crystalline or of a liquid system. We compare the thermal and the quantum results, identifying analogies and differences. Finally, we discuss experimental parameter regimes where the effects of quantum fluctuations on the linear - zigzag transition can be observed.
description: Submitted to the Special issue on modern applications of trapped ions, J. Phys. B: At. Mol. Opt. Phys
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÑÑÐ°ÑÐµÐ³Ð¸Ð¸ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐÐ Â«Ð¢Ð°Ð¹Ð¼ Ð¢ÑÐ¸Ð°Ð»Â»
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
Creators: name: Ð£Ð¿Ð°Ð´ÑÑÐµÐ²Ð°, Ð®Ð»Ð¸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: 2018
Subjects: Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³
ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÑ
Ð¿Ð¾ÑÑÐ°Ð²ÑÐ¸ÐºÐ¸
ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾-Ñ Ð¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½Ð°Ñ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ

description: Ð¦ÐµÐ»Ñ ÑÐ°Ð±Ð¾ÑÑ â Ð¿ÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°ÑÑ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ðµ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ðµ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ ÐÐÐ Â«Ð¢Ð°Ð¹Ð¼ Ð¢ÑÐ¸Ð°Ð»Â» Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°ÑÑ ÑÑÑÐ°ÑÐµÐ³Ð¸Ñ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ.
ÐÐ±ÑÐµÐºÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ â ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾-ÑÐ¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½Ð°Ñ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ ÐÐÐ Â«Ð¢Ð°Ð¹Ð¼ Ð¢ÑÐ¸Ð°Ð»Â», Ð¿ÑÐµÐ´Ð¼ÐµÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ â ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð°Ñ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÑ Ð¸ Ð´ÐµÐ»Ð¾Ð²Ð°Ñ Ð°ÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ ÐÐÐ Â«Ð¢Ð°Ð¹Ð¼ Ð¢ÑÐ¸Ð°Ð»Â».
Ð ÑÐ°Ð¼ÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÑ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð¿Ð¾Ð»Ð½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· Ð²Ð½ÑÑÑÐµÐ½Ð½ÐµÐ³Ð¾ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ñ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸, Ð¾Ð¿Ð¸ÑÐ°Ð½Ð° Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸, Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´Ð¸Ð¼Ð°Ñ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¸Ñ. ÐÐ¿Ð¸ÑÐ°Ð½Ñ Ð¿Ð¾ÑÑÐ°Ð²ÑÐ¸ÐºÐ¸, Ð¿Ð¾ÑÑÐµÐ±Ð¸ÑÐµÐ»Ð¸, ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÑ. ÐÑÑÐ²Ð»ÐµÐ½Ñ ÑÐ»Ð°Ð±ÑÐµ Ð¸ ÑÐ¸Ð»ÑÐ½ÑÐµ ÑÑÐ¾ÑÐ¾Ð½Ñ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ Ð¸ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½ÑÐµ Ð¿ÑÑÐ¸ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ.
ÐÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½Ð° Ð¾ÑÐµÐ½ÐºÐ° ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾-ÑÐ¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ, ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° ÑÑÑÐ°ÑÐµÐ³Ð¸Ñ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸.
Electronic self-organization in the single-layer manganite $\rm Pr_{\it 1-x}Ca_{\it 1+x}MnO_4$
Creators: name: Ye, F.
name: Chi, Songxue
name: Fernandez-Baca, J. A.
name: Moreo, A.
name: Dagotto, E.
name: Lynn, J. W.
name: Mathieu, R.
name: Kaneko, Y.
name: Tokura, Y.
name: Dai, Pengcheng
Publisher: name: arXiv
Year: 2009
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: We use neutron scattering to investigate the doping evolution of the magnetic correlations in the single-layer manganite $\rm Pr_{\it 1-x}Ca_{\it 1+x}MnO_4$, away from the $x=0.5$ composition where the CE-type commensurate antiferromagnetic (AF) structure is stable. We find that short-range incommensurate spin correlations develop as the system is electron doped ($x<0.5$), which coexist with the CE-type AF order. This suggests that electron doping in this system induces an inhomogeneous electronic self-organization, where commensurate AF patches with $x=0.5$ are separated by electron-rich domain walls with short range magnetic correlations. This behavior is strikingly different than for the perovksite $\rm Pr_{\it 1-x}Ca_{\it x}MnO_3$, where the long-range CE-type commensurate AF structure is stable over a wide range of electron or hole doping around $x=0.5$.
description: 4 figures. To be published in Phys. Rev. Lett
Modélisation d'une serre couplée à un système de stockage thermique : développement d'un modèle et étude de validité
Creators: name: Maheux, Timothée
name: Monfet, Danielle
name: Gibout, Stéphane
name: Haillot, Didier
Publisher: name: Société Française de Thermique
Year: 2023
Subjects: Stockage thermique
Serre nordique
Modèle numérique

description: Les communautés nordiques du Nunavik, le territoire du nord du Québec, font face à des contraintes alimentaires fortes liées notamment à l'appauvrissement des ressources halieutiques et terrestres. Afin de développer l'offre alimentaire locale, une serre communautaire est installée à Kuujjuaq (2 668 habitants en 2021, latitude 58$^{\circ}$ nord et longitude 68$^{\circ}$ ouest). Cette serre étant conçue pour les climats continentaux, elle n'est pas thermiquement adaptée au climat nordique. Il en découle une saison de culture courte et des rendements faibles. La serre a été instrumentée en juin 2016 afin de définir les améliorations à apporter. Les mesures ont montré que malgré une ressource solaire riche, les pertes thermiques nocturnes provoquaient une chute de la température importante. Ceci freine le développement des plantes et est engendré par la faible isolation ainsi que le peu d'inertie thermique des matériaux formant la serre : les températures nocturnes intérieures restent proches des températures nocturnes extérieures. Un système de stockage thermique de l'énergie (STE) a donc été conçu, construit et testé par l'équipe afin de stocker l'énergie thermique diurne et la réinjecter dans la serre la nuit. Bien qu'efficace, des améliorations sont envisagées et à ce titre, il est nécessaire de développer un outil d'analyse. Un modèle numérique de la serre de Kuujjuaq et de son STE a donc été développé à l'aide de l'outil Modelica. L'objectif de ce travail est d'évaluer la validité de ce modèle : une étude comparative sera présentée sur la température intérieure de la serre avec ou sans STE pendant des semaines de culture typiques. Ceci permettra à terme de définir les différents paramètres géométriques et thermiques optimaux pour la construction de futurs systèmes de stockage. L'article complet présentera les modèles de serre et de stockage, puis la méthodologie de couplage. Nous présenterons ensuite l'étude des résultats de simulation du modèle couplé en évaluant la cohérence physique des résultats puis leur précision sur plusieurs échelles temporelles.
title: ÐÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ñ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½Ð¾-ÑÐ¾ÑÐ³Ð¾Ð²Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÐºÐ°ÑÐµ-ÐºÐ¾Ð½Ð´Ð¸ÑÐµÑÑÐºÐ¾Ð¹ Ð½Ð° 50 Ð¼ÐµÑÑ Ð² ÐÐ°ÑÑÐ¸Ð½ÑÐºÐ¾Ð¼ ÑÐ°Ð¹Ð¾Ð½Ðµ ÐÐµÐ½Ð¸Ð½Ð³ÑÐ°Ð´ÑÐºÐ¾Ð¹ Ð¾Ð±Ð»Ð°ÑÑÐ¸
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð¡ÑÑÐ¾ÑÑÐºÐ¾Ð²Ð°, Ð®Ð»Ð¸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: 2016
Subjects: ÐºÐ°ÑÐµ
Ð¼ÐµÐ½Ñ
Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½Ð¾-ÑÐ¾ÑÐ³Ð¾Ð²Ð°Ñ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ

description: ÐÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¾ Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð¾Ð²Ð¾Ðµ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼Ð¾ÑÑÐ¸ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÐºÐ°ÑÐµ-ÐºÐ¾Ð½Ð´Ð¸ÑÐµÑÑÐºÐ¾Ð¹ Ð½Ð° 50 Ð¼ÐµÑÑ Ð² ÐÐ°ÑÑÐ¸Ð½ÑÐºÐ¾Ð¼ ÑÐ°Ð¹Ð¾Ð½Ðµ ÐÐµÐ½Ð¸Ð½Ð³ÑÐ°Ð´ÑÐºÐ¾Ð¹ Ð¾Ð±Ð»Ð°ÑÑÐ¸, Ð¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½Ñ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐ°ÑÑÐµÑÑ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ, Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð° Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÑÑÑÐºÑÑÑÐ° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¿Ð¾ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÑÐµÐ¼Ð¾Ð³Ð¾ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ, ÐµÐ³Ð¾ Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð¾ÑÐ½Ð¾Ðµ ÑÐµÑÐµÐ½Ð¸Ðµ Ð¸ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸.
From devices to data and back again : a tale of computationally modelling affective touch
Creators: name: Cang, Xi Laura
Publisher: name: University of British Columbia
Year: 2024

description: Emotionally responsive Human-Robot Interaction (HRI) has captured our curiosity and imagination in fantastical ways throughout much of modern media. With touch being a valuable yet sorely missed emotion communication channel when in-person interaction is unrealistic for practical reasons, we could look to machine-mediated ways to bridge that distance. In this thesis, we investigate how we might enable machines to recognize natural and spontaneous emotional touch expressions in two parts. First, we take a close look at ways machines engage with human emotion by examining examples of machines in three emotionally communicative roles: as a passive witness receiving and logging the emotional state of their (N=30) human counterparts, as an influential actor whose own breathing behaviour alters human fear response (N=103), and as a conduit for the transmission of emotion expression between human users (N=10 dyads and N=21 individuals). Next, we argue that in order for devices to be truly emotionally reactive, they should address the time-varying and dynamic nature of emotional lived experience. Any computational or emotion recognition engine intended for use under realistic conditions should acknowledge that emotions will evolve over time. Machine responses may change with changing ‘emotion direction’ – acting in an encouraging way when the user is `happy and getting happier' vs. presenting calming behaviours for `happy but getting anxious'. To that end, we develop a multi-stage emotion self-reporting procedure for collecting N=16 users’ dynamic emotion expression during videogame play. From their keypress force controlling their in-game character, we benchmark individualized recognition performance for emotion direction, even finding it to exceed that of brain activity (as measured by continuous Electroencephalography (EEG)). For a proof-of-concept of a training process that generates models of true and spontaneous emotion expression evolving with the user, we then revise our protocol to be more flexible to naturalistic emotion expression. We build a custom tool to help with data collection and labelling of personal storytelling sessions and evaluate user impressions (N=5 with up to 3 stories each for a total of 10 sessions). Finally, we conclude with actionable recommendations for advancing the training and machine recognition of naturalistic and dynamic emotion expression.
The Birth and Growth of Neutralino Haloes
Creators: name: Angulo, R. E.
name: White, S. D. M.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We use the Extended-Press-Schechter (EPS) formalism to study halo assembly histories in a standard $Λ$CDM cosmology. A large ensemble of Monte Carlo random walks provides the {\it entire} halo membership histories of a representative set of dark matter particles, which we assume to be neutralinos. The first generation halos of most particles do not have a mass similar to the free-streaming cut-off $M_{f.s.}$ of the neutralino power spectrum, nor do they form at high redshift. Median values are $M_1 = 10^5$ to $10^7M_{f.s.}$ and $z_1 = 13$ to 8 depending on the form of the collapse barrier assumed in the EPS model. For almost a third of all particles the first generation halo has $M_1>10^9M_{f.s.}$. At redshifts beyond 20, most neutralinos are not yet part of any halo but are still diffuse. These numbers apply with little modification to the neutralinos which are today part of halos similar to that of the Milky Way. Up to 10% of the particles in such halos were never part of a smaller object; the typical particle has undergone $\sim 5$ "accretion events' where the halo it was part of falls into a more massive object. Available N-body simulations agree well with the EPS predictions for an "ellipsoidal" collapse barrier, so these may provide a reliable extension of simulation results to smaller scales. The late formation times and large masses of the first generation halos of most neutralinos imply that they will be disrupted with high efficiency during halo assembly.
description: 7 pages, 7 figures
Optimisation géométrique pour la réhabilitation thermique des enveloppes des bâtiments
Creators: name: Alpar, Sultan
name: Berger, Julien
name: Belarbi, Rafik
Publisher: name: Société Française de Thermique
Year: 2023
Subjects: transfert de chaleur
problème inverse
problème d'optimisation
matériau d'isolation

description: The building sector represents a major source of energy savings and greenhouse gas reduction. It is also a major societal concern linked to the improvement of the living environment of the occupants through the use of energy-efficient solutions with a low environmental footprint. However, a main barrier to the success of the act of rehabilitation of the built heritage is the fact that all the existing tools for designing an energy renovation generate flat walls by combining layers of materials. Thus, the scientific problem is therefore the following: improvement of the energy performance of existing walls by optimizing their geometry. In particular, achieving an optimal distribution of the insulation with regard to the asymmetry of the incident radiative flux. In the present investigation, the boundary element method is applied to solve two-dimensional steady heat conduction problem. The boundary element method is a numerical technique which has been receiving growing attention for solving heat transfer problems because of its unique ability to confine the discretization process to the boundaries of the problem region. The boundary integral equation (BIE) and boundary element equation (BEE) are derived heat conduction. This work will allow an important advance on the optimization of the energy performance of the walls by proposing a theoretical and numerical framework and experimental investigations to validate the reliability of the predictions of the proposed models. From a socio-economic point of view, the proposed approach would make it possible to renovate old buildings by developing walls with high energy performance. This work would therefore have an impact on the sustainable construction sector and the rehabilitation of buildings. This work fits perfectly into the many societal challenges. It responds to the challenge dedicated to “Sustainable mobility and urban systems” and more particularly in the axis “From building to sustainable built living environment”. It also contributes to the “Clean, safe and efficient energy” challenge. Indeed, current thermal regulations recommend designing buildings that are more and more thermally insulated with a very low permeability of the envelope. Admittedly, this makes it possible to limit the energy and environmental impact but brings up new challenges because it risks altering summer comfort and the quality of indoor air.