cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Exchange and correlation effects in the transmission phase through a few-electron quantum dot
Creators: name: Rontani, Massimo
Publisher: name: arXiv
Year: 2010
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: The transmission phase through a quantum dot with few electrons shows a complex, non-universal behavior. Here we combine configuration-interaction calculations ---treating rigorously Coulomb interaction--- and the Friedel sum rule to provide a rationale for the experimental findings. The phase evolution for more than two electrons is found to strongly depend on dot's shape and electron density, whereas from one to two the phase never lapses. In the Coulomb (Kondo) regime the phase shifts are significant fractions of pi (pi/2) for the second and subsequent charge addition if the dot is strongly correlated. These results are explained by the proper inclusion in the theory of Coulomb interaction, spin, and orbital degrees of freedom.
description: RevTeX 4.0, 6 pages, 3 b/w figures. Physical Review B (2010), in press
Studio sui nuovi metodi di stoccaggio: il caso SARIX SA
Creators: name: Feo, Emmanuel
Publisher: name: Scuola Universitaria della Svizzera Italiana (SUPSI)
Year: 2020

description: Attraverso differenti cambiamenti nel mercato e nelle aspettative del cliente, una crescente ondata di competitività da parte delle multinazionali sta portando al fallimento di moltissime piccole / medie imprese in tutto il territorio Svizzero e globale. L'innovazione rimane il punto fondamentale per sovrastare questa competitività attraverso piccoli cambiamenti aziendali che portino al miglioramente di ogni singolo processo interno ed esterno all'azienda: dalla produzione ai test di qualità, dall'amministrazione al sistema logistico. Differenti imprese stanno eseguendo il passo alla digitalizzazione attraverso nuovi sistemi collegati come IOT, l'Industry 4.0, software per la gestione della logistica e magazzini o più semplicemente nuove soluzioni di stoccaggio che permettano l'ottimizzazione dei movimenti degli operatori all'interno dei differenti magazzini, riduzione le metrature e riduzione di tempi dei processi di prelievo. Soluzioni spesso però sono ancora oscure alle piccole imprese in quanto non si sappia effettivamente la correttezza di questi risparmi e spesso risulta un investimento molto rischioso che porterebbe a differenti problemi finanziari se non studiata correttamente. Il seguente progetto di tesi ha l’obiettivo di analizzare correttamente tutte le soluzioni di stoccaggio automatico verticale, attraverso una attenta enfasi sui risparmi in fatto di tempi di prelievo e spazi ri-guadagnati da potere implementare all'interno dei magazzini dell'azienda SARIX SA di Sant'Antonino
Braided Tensor Products and the Covariance of Quantum Noncommutative Free Fields
Creators: name: Lukierski, Jerzy
name: Woronowicz, Mariusz
Publisher: name: arXiv
Year: 2011
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: We introduce the free quantum noncommutative fields as described by braided tensor products. The multiplication of such fields is decomposed into three operations, describing the multiplication in the algebra M of functions on noncommutative space-time, the product in the algebra H of deformed field oscillators, and the braiding by factor Psi_{M,H} between algebras M and H. For noncommutativity generated by the twist factor we shall employ the star-product realizations of the algebra M in terms of functions on standard Minkowski space. The covariance of single noncommutative quantum fields under deformed Poincare symmetries is described by the algebraic covariance conditions which are equivalent to the deformation of generalized Heisenberg equations on Poincare group manifold. We shall calculate the covariant braided field commutator, which for free quantum noncommutative fields provides the field quantization condition and is given by standard Pauli-Jordan function. For ilustration of our new scheme we present explicit calculations for the well-known case in the literature of canonically deformed free quantum fields.
description: 19 pages, v.4, final version
Cut-tag/ChIP-seq of AR/SP1 in prostate cancer cell lines
Creators: name: Xuanrong Chen
Publisher: name: CNGB
Year: 2021
Subjects: Genome sequencing
Epigenomics
Monoisolate
Medical

description: Genome binding/occupancy profiling by high throughput sequencing We examine total AR and SP1 chromatin-binding profiles in DHT-treated LNCaP and LNCaP-AI cells to address the molecular functions of SP1 on the chromatin.
Quantifying the tension between the Higgs mass and (g-2)_mu in the CMSSM
Creators: name: Cabrera, Maria Eugenia
name: Casas, J. Alberto
name: de Austri, Roberto Ruiz
name: Trotta, Roberto
Publisher: name: arXiv
Year: 2010
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Supersymmetry has been often invoqued as the new physics that might reconcile the experimental muon magnetic anomaly, a_mu, with the theoretical prediction (basing the computation of the hadronic contribution on e^+ e^- data). However, in the context of the CMSSM, the required supersymmetric contributions (which grow with decreasing supersymmetric masses) are in potential tension with a possibly large Higgs mass (which requires large stop masses). In the limit of very large m_h supersymmetry gets decoupled, and the CMSSM must show the same discrepancy as the SM with a_mu . But it is much less clear for which size of m_h does the tension start to be unbearable. In this paper, we quantify this tension with the help of Bayesian techniques. We find that for m_h > 125 GeV the maximum level of discrepancy given current data (~ 3.3 sigma) is already achieved. Requiring less than 3 sigma discrepancy, implies m_h < 120 GeV. For a larger Higgs mass we should give up either the CMSSM model or the computation of a_mu based on e^+ e^-; or accept living with such inconsistency.
Postnatal cytomegalovirus exposure in infants of antiretroviral-treated and untreated HIV-infected mothers
Creators: name: Kalilani, L.
name: Patel, E.
name: Swamy, G.K.
name: Meyer, S.A.
name: Ehlinger, E.P.
name: Permar, S.R.
name: Westreich, D.
name: Lovingood, R.V.
name: Denny, T.N.
Publisher: name: Hindawi Publishing Corporation
Year: 2014

description: HIV-1 and CMV are important pathogens transmitted via breastfeeding. Furthermore, perinatal CMV transmission may impact growth and disease progression in HIV-exposed infants. Although maternal antiretroviral therapy reduces milk HIV-1 RNA load and postnatal transmission, its impact on milk CMV load is unclear. We examined the relationship between milk CMV and HIV-1 load (4-6 weeks postpartum) and the impact of antiretroviral treatment in 69 HIV-infected, lactating Malawian women and assessed the relationship between milk CMV load and postnatal growth in HIV-exposed, breastfed infants through six months of age. Despite an association between milk HIV-1 RNA and CMV DNA load (0.39 log10 rise CMV load per log10 rise HIV-1 RNA load, 95% CI 0.13-0.66), milk CMV load was similar in antiretroviral-treated and untreated women. Higher milk CMV load was associated with lower length-for-age (-0.53, 95% CI: -0.96, -0.10) and weight-for-age (-0.40, 95% CI: -0.67, -0.13) Z-score at six months in exposed, uninfected infants. As the impact of maternal antiretroviral therapy on the magnitude of postnatal CMV exposure may be limited, our findings of an inverse relationship between infant growth and milk CMV load highlight the importance of defining the role of perinatal CMV exposure on growth faltering of HIV-exposed infants.
Three Dimensional Origin of AdS_2 Quantum Gravity
Creators: name: Castro, Alejandra
name: Keeler, Cynthia
name: Larsen, Finn
Publisher: name: arXiv
Year: 2010
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We study AdS_2 quantum gravity with emphasis on consistency with results from AdS_3. We lift AdS_2 black holes to three dimensions and map fluctuations around the solutions. Comparison with near extremal BTZ are discussed, with due emphasis on global aspects. The results confirm that parameters like central charges and conformal weights computed directly in 2D are consistent with standard results in 3D. Applying our results to the thermodynamics of near extreme Kerr black holes, we show that AdS_2 quantum gravity gives the correct central charge c=12J, and the entropy of excitations above the extremal limit is captured correctly.
description: 28 pages
C2D Spitzer-IRS spectra of disks around T Tauri stars V. Spectral decomposition
Creators: name: Olofsson, J.
name: Augereau, J. -C.
name: van Dishoeck, E. F.
name: Merín, B.
name: Grosso, N.
name: Ménard, F.
name: Blake, G. A.
name: Monin, J. -L.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: (Abridged) Dust particles evolve in size and lattice structure in protoplanetary disks, due to coagulation, fragmentation and crystallization, and are radially and vertically mixed in disks. This paper aims at determining the mineralogical composition and size distribution of the dust grains in disks around 58 T Tauri stars observed with Spitzer/IRS. We present a spectral decomposition model that reproduces the IRS spectra over the full spectral range. The model assumes two dust populations: a warm component responsible for the 10μm emission arising from the disk inner regions and a colder component responsible for the 20-30μm emission, arising from more distant regions. We show evidence for a significant size distribution flattening compared to the typical MRN distribution, providing an explanation for the usual boxy 10μm feature profile generally observed. We reexamine the crystallinity paradox, observationally identified by Olofsson et al. (2009), and we find a simultaneous enrichment of the crystallinity in both the warm and cold regions, while grain sizes in both components are uncorrelated. Our modeling results do not show evidence for any correlations between the crystallinity and either the star spectral type, or the X-ray luminosity (for a subset of the sample). The size distribution flattening may suggests that grain coagulation is a slightly more effective process than fragmentation in disk atmospheres, and that this imbalance may last over most of the T Tauri phase. This result may also point toward small grain depletion via strong stellar winds or radiation pressure in the upper layers of disk. The non negligible cold crystallinity fractions suggests efficient radial mixing processes in order to distribute crystalline grains at large distances from the central object, along with possible nebular shocks in outer regions of disks that can thermally anneal amorphous grains.
title: Ð£Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð¾ÑÐ²ÐµÑÐµÐ½Ð½Ð¾ÑÑÑÑ Ð½Ð° Ð±Ð°Ð·Ðµ ÐºÐ¾Ð½ÑÑÐ¾Ð»Ð»ÐµÑÐ° Siemens LÐ¾go!
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: Illumination control based on the Siemens Logo controller!
Creators: name: ÐÐ°Ð¹ÑÐµÐ²Ð°, ÐÐ¸Ð¾Ð»ÐµÑÑ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: 2022
Subjects: ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð¾ÑÐ²ÐµÑÐµÐ½Ð¸ÐµÐ¼
ÐºÐ¾Ð½ÑÑÐ¾Ð»Ð»ÐµÑ
Ð´Ð°ÑÑÐ¸Ðº Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ñ
ÑÐ¼Ð½ÑÐ¹ Ð´Ð¾Ð¼
lighting control
controller
motion sensor
smart home

description: Ð¢ÐµÐ¼Ð° Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ: Â«Ð£Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð¾ÑÐ²ÐµÑÐµÐ½Ð½Ð¾ÑÑÑÑ Ð½Ð° Ð±Ð°Ð·Ðµ ÐºÐ¾Ð½ÑÑÐ¾Ð»Ð»ÐµÑÐ° Siemens LÐ¾go!Â»Ð Ð°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐµ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¾ÑÐ²ÐµÑÐµÐ½Ð¸ÐµÐ¼ Ð´Ð»Ñ ÐºÐ¾Ð¼Ð¼ÐµÑÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿Ð¾Ð¼ÐµÑÐµÐ½Ð¸Ñ Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ ÐºÐ¾Ð½ÑÑÐ¾Ð»Ð»ÐµÑÐ° SiemensLOGO 12/24 RC. Ð ÑÐ¾Ð´Ðµ ÑÐ°Ð±Ð¾ÑÑ Ð±ÑÐ»Ð¸ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð²Ð¾Ð¿ÑÐ¾ÑÑ:ÐÐ·ÑÑÐµÐ½Ð¸Ðµ Ð¿ÑÐµÐ´Ð¼ÐµÑÐ½Ð¾Ð¹ Ð¾Ð±Ð»Ð°ÑÑÐ¸ÐÐ¾Ð´Ð¾Ð±ÑÐ°ÑÑ ÐºÐ¾Ð¼Ð¿Ð¾Ð½ÐµÐ½ÑÑ Ð´Ð»Ñ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ÐÑÐ¾Ð¸Ð·Ð²ÐµÑÑÐ¸ ÑÐ°ÑÑÐµÑÑ Ð´Ð»Ñ Ð¾ÑÐ²ÐµÑÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð¸ Ð¿Ð¾Ð´ÐºÐ»ÑÑÐµÐ½Ð¸Ñ ÑÐ¸ÑÑÐµÐ¼ÑÐ Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°ÑÑ ÑÐµÐ¶Ð¸Ð¼Ñ Ð¾ÑÐ²ÐµÑÐµÐ½Ð¸ÑÐ¡Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°ÑÑ ÑÐµÐ¶Ð¸Ð¼Ñ Ð² Ð¿Ð°ÐºÐµÑÐµ Ð´Ð»Ñ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸ÑÐ ÑÐ¾Ð´Ðµ ÑÐ°Ð±Ð¾ÑÑ Ð±ÑÐ»Ð° ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð° Ð¿ÑÐµÐ´Ð¼ÐµÑÐ½Ð°Ñ Ð¾Ð±Ð»Ð°ÑÑÑ, ÑÐ¸ÑÑÐµÐ¼ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¾ÑÐ²ÐµÑÐµÐ½Ð¸ÐµÐ¼ Ð¸ Ð²ÑÐ±ÑÐ°Ð½Ñ ÐºÐ¾Ð¼Ð¿Ð¾Ð½ÐµÐ½ÑÑ Ð´Ð»Ñ ÑÐ¸ÑÑÐµÐ¼Ñ. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ ÑÑÑÑÐºÑÑÑÐ½ÑÐµ ÑÑÐµÐ¼Ñ ÑÐµÐ¶Ð¸Ð¼Ð¾Ð² ÑÐ°Ð±Ð¾ÑÑ Ð¸ Ð² Ð¿Ð°ÐºÐµÑÐµ Ð´Ð»Ñ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ LOGO, ÑÐ¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ñ ÑÑÐ¸ ÑÐµÐ¶Ð¸Ð¼Ð° ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¾ÑÐ²ÐµÑÐµÐ½Ð½Ð¾ÑÑÑÑ, ÑÐ°ÐºÐ¶Ðµ Ð¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½Ñ ÑÐ°ÑÑÐµÑÑ Ð´Ð»Ñ Ð¾ÑÐ²ÐµÑÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð¿Ð¾Ð¼ÐµÑÐµÐ½Ð¸Ñ, ÑÐ°ÑÑÐµÑÑ Ð´Ð¾Ð¿ÑÑÑÐ¸Ð¼ÑÑ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÐ¾Ð² Ð¿Ð¾Ð´ÐºÐ»ÑÑÐ°ÐµÐ¼ÑÑ Ð»Ð°Ð¼Ð¿.
description: The topic of the final qualifying work: "Illumination control based on the Siemens Logo controller!".The work is devoted to the development of a lighting control system for a commercial premises using the SiemensLOGO 12/24 RC controller. During the work, the following issues were considered:1. Study of the subject area2. Select components for implementation3. Make calculations for illumination and system connection4. Develop lighting modes5. Simulate modes in a programming packageIn the course of the work, the subject area, lighting control systems were considered and components for the system were selected. Block diagrams of operating modes and in the LOGO programming package have been developed, three illumination control modes have been modeled, calculations for the illumination of the room, calculations of the permissible parameters of the connected lamps have also been made.
Large Dimensions and Small Curvatures from Supersymmetric Brane Back-reaction
Creators: name: Burgess, C. P.
name: van Nierop, L.
Publisher: name: arXiv
Year: 2011
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We compute the back-reaction of pairs of codimension-two branes within an explicit flux-stabilized compactification, to trace how its properties depend on the parameters that define the brane-bulk couplings. Both brane tension and magnetic couplings to the stabilizing flux play an important role in the resulting dynamics, with the magnetic coupling allowing some of the flux to be localized on the branes (thus changing the flux-quantization conditions). We find that back-reaction lifts the classical flat directions of the bulk supergravity, and we calculate both the scalar potential and changes to the extra-dimensional and on-brane geometries that result, as functions of the assumed brane couplings. When linearized about simple rugby-ball geometries the resulting solutions allow a systematic exploration of the system's response. Several of the systems we explore have remarkable properties. Among these are a propensity for the extra dimensions to stabilize at exponentially large sizes, providing a mechanism for generating extremely large volumes. In some circumstances the brane-dilaton coupling allows the bulk dilaton to adjust to suppress the on-brane curvature parametrically below the change in brane tension, potentially providing a mechanism for reducing the vacuum energy. We explore the stability of this suppression to quantum effects in the case where their strength is controlled by the value of the field along the classical flat direction, and find it can (but need not) be stable.
description: 32 pages + appendix. replacement: ref's updated
Genetic Analysis of Chinese Families with OCA2
Creators: name: 袁悉奥(YUAN Xiao)
Publisher: name: CNGB
Year: 2021
Subjects: Raw sequence reads
Exome
Monoisolate

description: In this study, we reviewed the records of OCA2 patients who had conducted albinism genetic testing, and then analyzed the clinical and genetic information of OCA2 patients who had been genetically diagnosed as OCA2 by using Sanger sequencing and next-generation sequencing. Our results were beneficial for diagnosis and precision clinical management for OCA2-related disorder, and this study expanded the mutation spectrum of oculocutaneous albinism.
Ca' Rossa (Grono), Alloggio per sportivi
Creators: name: Romano, Irina
Publisher: name: Scuola Universitaria della Svizzera Italiana (SUPSI)
Year: 2018

description: La Cà Rossa verrà adibita ad un alloggio per sportivi. Gli ospiti saranno persone a cui piace stare all’aria aperta, sempre pronti a nuove sfide e senza il timore di sporcarsi le mani. Questa casa è caratterizzata da alte stanze con stucchi, affreschi e decori, ma per questo tipo di ospiti mi piacerebbe invece ottenere un’atmosfera informale e accogliente, un luogo dove potersi sentire a proprio agio. Per questo motivo è nata l’idea di realizzare una fascia a scala d’uomo che possa far sentire i visitatori a proprio agio inserendoli in uno spazio informale volto ad incorniciare il prezioso apparato decorativo-storico del palazzo.
Manipulation of the Land$\acute{\text{e}}$ g-factor in InAs quantum dots through the application of anisotropic gate potentials: Exact diagonalization, numerical and perturbation methods
Creators: name: Prabhakar, Sanjay
name: Raynolds, James E
name: Melnik, Roderick
Publisher: name: arXiv
Year: 2010
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We study the variation in the Land$\acute{\text{e}}$ g-factor of electron spins induced by both anisotropic gate potentials and magnetic fields in InAs quantum dots for possible implementation towards solid state quantum computing. In this paper, we present analytical expressions and numerical simulations of the variation in the Land$\acute{\text{e}}$ g-factor for both isotropic and anisotropic quantum dots. Using both analytical techniques and numerical simulations, we show that the Rashba spin-orbit coupling has a major contribution in the variation of the g-factor with electric fields before the regime, where level crossing or anticrossing occurs. In particular, the electric field tunability is shown to cover a wide range of g-factor through strong Rashba spin-orbit interaction. Another major result of this paper is that the anisotropic gate potential gives quenching effect in the orbital angular momentum that reduces the variation in the E-field and B-field tunability of the g-factor if the area of the symmetric and asymmetric quantum dots is held constant. We identify level crossings and anticrossings of the electron states in the variation of the Land$\acute{\text{e}}$ g-factor. We model the wavefunctions of electron spins and estimate the size of the anticrossing for the spin states $|0,-1,+1/2>$ and $|0,0,-1/2>$ corresponding to a quantum dot that has been recently studied experimentally (Phys. Rev. Lett. \textbf{104}, 246801 (2010)).
description: 9 pages and 8 figures
title: ÐÐ½Ð°Ð»Ð¸Ð· ÑÐºÐ¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð¿Ð°ÑÐ¿Ð¾ÑÑÐ¸Ð·Ð°ÑÐ¸Ð¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¹ ÐºÐ°Ðº Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÐ° ÑÐµÑÐµÐ½Ð¸Ñ ÑÐºÐ¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ñ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼
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: Analysis of environmental certification of enterprises as a tool for solving environmental problems
Creators: name: ÐÐ²Ð°Ð½Ð¾Ð², ÐÐ»ÑÑ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2019
Subjects: ÑÐºÐ¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ°Ñ Ð¿Ð°ÑÐ¿Ð¾ÑÑÐ¸Ð·Ð¸ÑÐ¸Ñ
ÑÐºÐ¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð¿Ð°ÑÐ¿Ð¾ÑÑ
ÑÐºÐ¾Ð»Ð¾Ð³Ð¸Ñ
Ð¾Ñ ÑÐ°Ð½Ð° Ð¾ÐºÑÑÐ¶Ð°ÑÑÐµÐ¹ ÑÑÐµÐ´Ñ
ecological certification
ecological pasport
ecology
enviromental protection

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐ¾Ð²Ð¾Ð´Ð¸ÑÑÑ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¾Ð¹ Ð±Ð°Ð·Ñ Ð¸ Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¿Ð¾Ð´ÑÐ¾Ð´Ð¾Ð² Ð² Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ð¸ ÑÐºÐ¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð¿Ð°ÑÐ¿Ð¾ÑÑÐ¸Ð·Ð°ÑÐ¸Ð¸. Ð ÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¾Ð¼ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¿ÑÐ¸Ð¼ÐµÑÐ° Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð´Ð¾Ð¿Ð¾Ð»Ð½Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð¹ Ð´Ð¾ÐºÑÐ¼ÐµÐ½ÑÐ°ÑÐ¸Ð¸ Ð´Ð»Ñ Ð·Ð°Ð¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ ÑÐºÐ¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿Ð°ÑÐ¿Ð¾ÑÑÐ° Ð¸ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð¸Ðµ ÑÐ¿Ð¾ÑÐ¾Ð±Ð° ÑÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¿ÑÐ¾ÑÐµÑÑÐ° Ð¿Ð°ÑÐ¿Ð¾ÑÑÐ¸Ð·Ð°ÑÐ¸Ð¸ Ñ ÑÐµÐ»ÑÑ ÐµÐ³Ð¾ ÑÐ¿ÑÐ¾ÑÐµÐ½Ð¸Ñ.
description: This work contains analysis of the theoretical and practical part of the process of ecological certification. The result of the work is to give an example of using other documentation to fill out an ecological passport and suggest a way to improve the certification process to facilitate this process.
title: ÐÐ½Ð°Ð»Ð¸Ð· Ð¿ÑÐ¸ÑÐ¸Ð½ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð´ÐµÑÐµÐºÑÐ¾Ð² ÑÑÑÑÐºÑÑÑÑ ÑÑÐ°Ð»Ð¸ 12Ð¥18Ð10Ð¢ Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¹ Ð¿Ð¾ Ð¸Ñ ÑÑÑÑÐ°Ð½ÐµÐ½Ð¸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
title: Analysis of the causes of microstructure defects of steel 12H18N10T and development of recommendations for their elimination
Creators: name: ÐÐ¸ÑÐ½Ð¾Ð²Ð°, Ð¢Ð°ÑÑÑ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: 2019
Subjects: Ð¡ÑÐ°Ð»Ñ
ÐÑÑÑÐµÐ½Ð¸Ñ
Ð´ÐµÑÐµÐºÑÑ Ð¼Ð¸ÐºÑÐ¾ÑÑÑÑÐºÑÑÑÑ
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ÑÐµÑÑÐ¸ÑÐ½Ð°Ñ Î-ÑÐ°Ð·Ð°

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¸ Ð¿ÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ñ Ð¾Ð´Ð½Ð¸ Ð¸Ð· ÑÐ°Ð¼ÑÑ ÑÐ°ÑÐ¿ÑÐ¾ÑÑÑÐ°Ð½ÐµÐ½Ð½ÑÑ Ð´ÐµÑÐµÐºÑÐ¾Ð² Ð¼Ð¸ÐºÑÐ¾ÑÑÑÑÐºÑÑÑÑ ÑÑÐ°Ð»Ð¸ 12Ð¥18Ð10Ð¢. ÐÑÐ¸Ð²ÐµÐ´ÐµÐ½Ð° Ð¾Ð±ÑÐ°Ñ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ñ Ð¾ ÑÐ¿Ð¾ÑÐ¾Ð±Ð°Ñ Ð²ÑÐ¿Ð»Ð°Ð²ÐºÐ¸ ÑÑÐ°Ð»Ð¸ Ð´Ð°Ð½Ð½Ð¾Ð¹ Ð¼Ð°ÑÐºÐ¸. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¿ÑÐ¸ÑÐ¸Ð½ Ð²Ð¾Ð·Ð½Ð¸ÐºÐ½Ð¾Ð²ÐµÐ½Ð¸Ñ Ð´ÐµÑÐµÐºÑÐ¾Ð² Ð¼Ð¸ÐºÑÐ¾ÑÑÑÑÐºÑÑÑÑ Ð¿Ð¾Ð»ÑÑÐ°Ð±ÑÐ¸ÐºÐ°ÑÐ¾Ð² Ð¸Ð· ÑÑÐ°Ð»Ð¸ Ð¼Ð°ÑÐºÐ¸ 12Ð¥18Ð10Ð¢. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ ÐºÐ¾Ð½ÐºÑÐµÑÐ½ÑÐµ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¿Ð¾ Ð¿ÑÐµÐ´Ð¾ÑÐ²ÑÐ°ÑÐµÐ½Ð¸Ñ Ð¸ ÑÑÑÑÐ°Ð½ÐµÐ½Ð¸Ñ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð½ÑÑ Ð´ÐµÑÐµÐºÑÐ¾Ð².
description: In the given work consider and analyze some of the most common defects of microstructure of steel 12X18H10T. General information about the methods of smelting of this steel is given. The analysis of the causes of defects of microstructure of steel 12Ð¥18Ð10T. Specific recommendations on prevention and elimination of the considered defects are developed.
Incident Pregnancy and Time to Death or AIDS among HIV-Positive Women Receiving Antiretroviral Therapy
Creators: name: Firnhaber, C.
name: Sanne, I.
name: Maskew, M.
name: Majuba, P.
name: Westreich, D.
name: Evans, D.
Publisher: name: Public Library of Science
Year: 2013

description: Background: Little is known about the impact of pregnancy on response to highly active antiretroviral therapy (HAART) in sub-Saharan Africa. We examined the effect of incident pregnancy after HAART initiation on clinical response to HAART. Methods: We evaluated a prospective clinical cohort of adult women initiating HAART in Johannesburg, South Africa between 1 April 2004 and 31 March 2011, and followed up until an event, transfer, drop-out, or administrative end of follow-up on 30 September 2011. Women over age 45 and women who were pregnant at HAART initiation were excluded from the study. Main exposure was having experienced pregnancy after HAART initiation; main outcome was death and (separately) death or new AIDS event. We calculated adjusted hazard ratios (HRs) and 95% confidence limits (CL) using marginal structural Cox proportional hazards models. Results: The study included 7,534 women, and 20,813 person-years of follow-up; 918 women had at least one recognized pregnancy during follow-up. For death alone, the weighted (adjusted) HR was 0.84 (95% CL 0.44, 1.60). Sensitivity analyses confirmed main results, and results were similar for analysis of death or new AIDS event. Incident pregnancy was associated with a substantially reduced hazard of drop-out (HR = 0.62, 95% CL 0.51, 0.75). Conclusions: Recognized incident pregnancy after HAART initiation was not associated with increases in hazard of clinical events, but was associated with a decreased hazard of drop-out. High rates of pregnancy after initiation of HAART may point to a need to better integrate family planning services into clinical care for HIV-infected women.
Thermodynamic potentials and Thermodynamic Relations in Nonextensive Thermodynamics
Creators: name: Gu, Lina
name: Du, Jiulin
Publisher: name: arXiv
Year: 2010
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Classical Physics (physics.class-ph)
subject: FOS: Physical sciences

description: The generalized Gibbs free energy and enthalpy is derived in the framework of nonextensive thermodynamics by using the so-called physical temperature and the physical pressure. Some thermodynamical relations are studied by considering the difference between the physical temperature and the inverse of Lagrange multiplier. The thermodynamical relation between the heat capacities at a constant volume and at a constant pressure is obtained using the generalized thermodynamical potential, which is found to be different from the traditional one in Gibbs thermodynamics. But, the expressions for the heat capacities using the generalized thermodynamical potentials are unchanged.
description: 7 pages
XrBridge: un wrapper OpenXR-OpenGL per applicazioni VR
Creators: name: Piazza, Lorenzo Adam
Publisher: name: Scuola Universitaria della Svizzera Italiana (SUPSI)
Year: 2024
Subjects: C++
virtual reality
education

description: XrBridge è una libreria C++ che semplifica l’interfacciamento di applicazioni 3D con i visori da realtà virtuale appoggiandosi al nuovo e complesso standard adottato nel settore: OpenXR. L’obiettivo di XrBridge è quello di permettere a studenti e ricercatori di accedere ai benefici di OpenXR attraverso uno strumento che ne astrae significativamente le funzionalità, riducendo la curva di apprendimento e lo sforzo richiesto a livelli compatibili con i percorsi formativi SUPSI. ____ XrBridge is a C++ library that simplifies the interfacing of 3D applications with virtual reality headsets by relying on the new and complex standard adopted in the industry: OpenXR. The goal of XrBridge is to allow students and researchers to access the benefits of OpenXR through a tool that significantly abstracts its functionalities, reducing the learning curve and effort required to levels compatible with SUPSI educational programs.
Detections of C2H, cyclic-C3H2, and H13CN in NGC 1068
Creators: name: Nakajima, Taku
name: Takano, Shuro
name: Kohno, Kotaro
name: Inoue, Hirofumi
Publisher: name: arXiv
Year: 2011
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We used the Nobeyama 45-m telescope to conduct a spectral line survey in the 3-mm band (85.1-98.4 GHz) toward one of the nearest galaxies with active galactic nucleus NGC 1068 and the prototypical starburst galaxy NGC 253. The beam size of this telescope is ~18", which was sufficient to spatially separate the nuclear molecular emission from the emission of the circumnuclear starburst region in NGC 1068. We detected rotational transitions of C2H, cyclic-C3H2, and H13CN in NGC 1068. These are detections of carbon-chain and carbon-ring molecules in NGC 1068. In addition, the C2H N = 1-0 lines were detected in NGC 253. The column densities of C2H were determined to be 3.4 x 10^15 cm^-2 in NGC 1068 and 1.8 x 10^15 cm^-2 in NGC 253. The column densities of cyclic-C3H2 were determined to be 1.7 x 10^13 cm^-2 in NGC 1068 and 4.4 x 10^13 cm^-2 in NGC 253. We calculated the abundances of these molecules relative to CS for both NGC 1068 and NGC 253, and found that there were no significant differences in the abundances between the two galaxies. This result suggests that the basic carbon-containing molecules are either insusceptible to AGN, or are tracing cold (T_rot ~10 K) molecular gas rather than X-ray irradiated hot gas.
description: 10 pages, 3 figures, Accepted for publication in ApJ Letter. After the submission of this manuscript, we found two relevant papers. Snell et al. detected C2H in NGC 1068 (astro-ph 1101.0132). It was very recently published in The Astronomical Journal 141 38. Costagliola et al. detected C2H and H13CN in NGC 1068 (astro-ph 1101.2122)
1st Place Floral Arrangement by Mrs. Martha Strong Turner, Dahlia Show of The Garden Club of East Hampton , September 16th, 1924
Creators: name: (:Unas)
Publisher: name: Garden Club of East Hampton
Year: 1924
Subjects: Gardening
Gardens
Social organizations
Organizations
Flowers
Flower shows
Flower arrangements
East Hampton (N.Y.)

description: This photo shows a table arrangement by Mrs. Martha Strong Turner, wife of Mr. Harold Turner, at the Dahlia Show of the Garden Club of East Hampton on September 16th, 1924
title: ÐÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð·Ð°ÑÑÐ´Ð½Ð¾Ð³Ð¾ ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð° Ð´Ð»Ñ ÑÐ»ÐµÐºÑÑÐ¾Ð¼Ð¾Ð±Ð¸Ð»Ñ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð¼Ð¾ÑÑÐ¾Ð²Ð¾Ð³Ð¾ Ð¿ÑÐµÐ¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»Ñ Ñ ÑÐ°Ð·Ð¾Ð²ÑÐ¼ ÑÐ´Ð²Ð¸Ð³Ð¾Ð¼ Ð¼Ð¾ÑÐ½Ð¾ÑÑÑÑ 10 ÐºÐÑ
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: Designing a charger for an electric vehicle based on a 10 kW phase shift bridge converter
Creators: name: ÐÐ¾ÑÐ¾ÑÐºÐ¾Ð², Ð¡ÑÐµÐ¿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: 2023
Subjects: Ð·Ð°ÑÑÐ´Ð½Ð¾Ðµ ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð¾ Ð´Ð»Ñ ÑÐ»ÐµÐºÑÑÐ¾Ð¼Ð¾Ð±Ð¸Ð»Ñ
li-ion Ð°ÐºÐºÑÐ¼ÑÐ»ÑÑÐ¾Ñ
Ð¼Ð¾ÑÑÐ¾Ð²Ð¾Ð¹ Ð¿ÑÐµÐ¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»Ñ Ñ ÑÐ°Ð·Ð¾Ð²ÑÐ¼ ÑÐ´Ð²Ð¸Ð³Ð¾Ð¼
Ð·Ð°ÑÑÐ´ÐºÐ° ÑÐ»ÐµÐºÑÑÐ¾Ð¼Ð¾Ð±Ð¸Ð»Ñ
electric car charger
li-ion battery
bridge converter with phase shift
electric car charging

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð±ÑÐ»Ð¾ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¾ Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð¾ Ð·Ð°ÑÑÐ´Ð½Ð¾Ðµ ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð¾ Ð´Ð»Ñ ÑÐ»ÐµÐºÑÑÐ¾Ð¼Ð¾Ð±Ð¸Ð»ÐµÐ¹ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð¼Ð¾ÑÑÐ¾Ð²Ð¾Ð³Ð¾ Ð¿ÑÐµÐ¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»Ñ Ñ ÑÐ°Ð·Ð¾Ð²ÑÐ¼ ÑÐ´Ð²Ð¸Ð³Ð¾Ð¼. ÐÐ°Ð´Ð°ÑÐ¸, ÐºÐ¾ÑÐ¾ÑÑÐµ ÑÐµÑÐ°Ð»Ð¸ÑÑ Ð² ÑÐ¾Ð´Ðµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ: 1. ÐÐ½Ð°Ð»Ð¸Ð· Ð¿ÑÐ±Ð»Ð¸ÐºÐ°ÑÐ¸Ð¹ Ð¿Ð¾ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÐ¼ Ð·Ð°ÑÑÐ´Ð½ÑÐ¼ ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð°Ð¼ ÑÐ»ÐµÐºÑÑÐ¾Ð¼Ð¾Ð±Ð¸Ð»ÐµÐ¹. 2. ÐÐ·ÑÑÐµÐ½Ð¸Ðµ Ð·Ð°ÑÑÐ´Ð½ÑÑ ÑÑÑÑÐ¾Ð¹ÑÑÐ² Ð´Ð»Ñ ÑÐ»ÐµÐºÑÑÐ¾Ð¼Ð¾Ð±Ð¸Ð»ÐµÐ¹. 3. ÐÐ·ÑÑÐµÐ½Ð¸Ðµ Ð¿ÑÐµÐ¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÐµÐ¹ ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÑÐ½ÐµÑÐ³Ð¸Ð¸. 4. ÐÐ·ÑÑÐµÐ½Ð¸Ðµ Ð¿ÑÐ¸Ð½ÑÐ¸Ð¿Ð° ÑÐ°Ð±Ð¾ÑÑ Ð¸ ÐºÐ¾Ð¼Ð¿Ð¾Ð½ÐµÐ½ÑÐ¾Ð² Ð¿ÑÐµÐ¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÐµÐ¹ ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÑÐ½ÐµÑÐ³Ð¸Ð¸. 5. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¼Ð¾Ð´ÐµÐ»Ð¸ Ð² ÑÑÐµÐ´Ðµ MATLAB Simulink. 6. Ð Ð°ÑÑÐµÑ Ð¸ Ð²ÑÐ±Ð¾Ñ ÐºÐ¾Ð¼Ð¿Ð¾Ð½ÐµÐ½ÑÐ¾Ð² Ð¼Ð¾Ð´ÐµÐ»Ð¸.
description: In this work, a charger for electric vehicles based on a phase-shifted bridge converter was investigated and developed. Tasks that were solved during the study: 1. Analysis of publications on modern electric car chargers. 2. Study of chargers for electric vehicles. 3. Study of electrical energy converters. 4. Study of the principle of operation and components of electric energy converters. 5. Model development in the MATLAB Simulink environment. 6. Calculation and selection of model components.
Floating wind turbine motion suppression using an active wave energy converter
Creators: name: Webler Soares, Anderson Ricardo
Publisher: name: University of British Columbia
Year: 2020

description: This thesis proposes a new concept of an actively-controlled wave energy converter for suppressing the pitch and roll motions of the floating offshore wind turbines. The wave energy converter consists of several floating bodies which receive the wave energy, actuators which convert the wave energy into electrical energy and generate the mechanical forces, and rigid bars which connect the floating bodies and the wind turbine platform and deliver the actuator forces to the platform. The rotational torques to minimize the platform pitch and roll motions are determined by the linear quadratic regulator, while the determined torques are realized by the actuator forces that maximize the wave power capture. The performance of the proposed wave energy converter in simultaneously suppressing the platform pitch and roll motions and extracting the wave energy is validated in simulations.
The distance and internal composition of the neutron star in EXO 0748-676 with XMM-Newton
Creators: name: Zhang, Guobao
name: Mendez, Mariano
name: Jonker, Peter
name: Hiemstra, Beike
Publisher: name: arXiv
Year: 2010
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Recently, the neutron star X-ray binary EXO 0748-676 underwent a transition to quiescence. We analyzed an XMM-Newton observation of this source in quiescence, where we fitted the spectrum with two different neutron-star atmosphere models. From the fits we constrained the allowed parameter space in the mass-radius diagram for this source for an assumed range of distances to the system. Comparing the results with different neutron-star equations of state, we constrained the distance to EXO 0748-676. We found that the EOS model 'SQM1' is rejected by the atmosphere model fits for the known distance, and the 'AP3' and 'MS1' is fully consistent with the known distance.
description: 6 pages, 7 figures, 2 tables, submitted to MNRAS on June 20, 1010
Cappuccetto Rosso, hai paura del lupo? Conoscere la paura attraverso la fiaba di Cappuccetto Rosso
Creators: name: Barra, Jessica
Publisher: name: Scuola Universitaria della Svizzera Italiana (SUPSI)
Year: 2014

description: La ricerca è volta a verificare se una fiaba della tradizione possa aiutare i bambini a riconoscere, comprendere e verbalizzare l’emozione della paura, una delle sei emozioni chiave riscontrate nell’infanzia. Per rispondere a questo interrogativo, è stata svolta un’indagine in due classi della scuola dell’Infanzia di Ascona, una sperimentale e una di controllo. Nella prima è stata utilizzata la fiaba come strumento di supporto, seguito da attività di analisi e di discussione; nella seconda è stata invece proposta solo la discussione riguardante tale emozione. Dalla ricerca è emerso che i bambini della classe sperimentale non hanno avuto difficoltà a riconoscere l’emozione nella storia e a parlarne; al contrario, i bambini della sezione di controllo hanno mostrato maggiori difficoltà a definire una loro paura e soprattutto a parlarne. È stato quindi ipotizzato che la lettura di una fiaba possa favorire nei bambini la capacità di riconoscere e di verbalizzare le proprie emozioni, partendo dalle emozioni provate dal protagonista della storia e identificandosi con lui. Relatore: Luca Cignetti.
The Mass Distribution of Stellar-Mass Black Holes
Creators: name: Farr, Will M.
name: Sravan, Niharika
name: Cantrell, Andrew
name: Kreidberg, Laura
name: Bailyn, Charles D.
name: Mandel, Ilya
name: Kalogera, Vicky
Publisher: name: arXiv
Year: 2010
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We perform a Bayesian analysis of the mass distribution of stellar-mass black holes using the observed masses of 15 low-mass X-ray binary systems undergoing Roche lobe overflow and five high-mass, wind-fed X-ray binary systems. Using Markov Chain Monte Carlo calculations, we model the mass distribution both parametrically---as a power law, exponential, gaussian, combination of two gaussians, or log-normal distribution---and non-parametrically---as histograms with varying numbers of bins. We provide confidence bounds on the shape of the mass distribution in the context of each model and compare the models with each other by calculating their relative Bayesian evidence as supported by the measurements, taking into account the number of degrees of freedom of each model. The mass distribution of the low-mass systems is best fit by a power-law, while the distribution of the combined sample is best fit by the exponential model. We examine the existence of a "gap" between the most massive neutron stars and the least massive black holes by considering the value, M_1%, of the 1% quantile from each black hole mass distribution as the lower bound of black hole masses. The best model (the power law) fitted to the low-mass systems has a distribution of lower-bounds with M_1% > 4.3 Msun with 90% confidence, while the best model (the exponential) fitted to all 20 systems has M_1% > 4.5 Msun with 90% confidence. We conclude that our sample of black hole masses provides strong evidence of a gap between the maximum neutron star mass and the lower bound on black hole masses. Our results on the low-mass sample are in qualitative agreement with those of Ozel, et al (2010).
description: 56 pages, 22 figures, 9 tables, as accepted by ApJ
title: ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐµÐ³Ð½ÐµÑÐ¾ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÐ²Ð¾Ð¹ÑÑÐ² ÐºÑÐ¸ÑÑÐ°Ð»Ð»Ð¾Ð² ÑÐ¸ÑÐºÐ¾Ð½Ð°Ñ-ÑÐ¸ÑÐ°Ð½Ð°ÑÐ° ÑÐ²Ð¸Ð½ÑÐ° (PZT) Ð¸ ÐºÐµÑÐ°Ð¼Ð¸Ðº Ð¼Ð°Ð³Ð½Ð¾-Ð½Ð¸Ð¾Ð±Ð°ÑÐ° ÑÐ²Ð¸Ð½ÑÐ° (PMN)
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: Ferroelectric properties of lead zirconate-titanate (PZT) single crystals and lead magnesium-niobate (PMN) ceramics
Creators: name: ÐÐ°ÑÑÐº, Ð¢Ð°ÑÑÑ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: 2021
Subjects: ÐÑÐ¸ÑÑÐ°Ð»Ð»Ñ
Ð¡Ð²Ð¸Ð½ÐµÑ
Ð¡Ð¿ÐµÐºÑÑÐ¾ÑÐºÐ¾Ð¿Ð¸Ñ
Ð¡ÐµÐ³Ð½ÐµÑÐ¾ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÑÐ²Ð¾
ÐÑÐµÐ·Ð¾ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÑÐ²Ð¾
ÐÐ¸ÐºÑÐ¾ÑÐºÐ¾Ð¿Ð¸Ñ

description: ÐÐ°Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° Ð¸Ð·ÑÑÐµÐ½Ð¸Ñ Ð¾Ð±ÑÐ°Ð·ÑÐ¾Ð² Ð¼Ð¾Ð½Ð¾ÐºÑÐ¸ÑÑÐ°Ð»Ð»Ð° Pb[Zr â. â â âTi â. âââ]Oâ (PZT 1.1) Ð¸ ÐºÐµÑÐ°Ð¼Ð¸ÐºÐ¸ 0.8Pb[Mg â/âNb â/â]Oâ - 0.2PbTiOâ (PMN PT20). ÐÐµÑÐ°Ð¼Ð¸ÐºÐ° PMN PT20 Ð¸Ð·Ð¼ÐµÑÑÐ»Ð°ÑÑ Ð¼ÐµÑÐ¾Ð´Ð¾Ð¼ Ð´Ð¸ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÑÐ¿ÐµÐºÑÑÐ¾ÑÐºÐ¾Ð¿Ð¸Ð¸. ÐÐ»Ñ PMN PT20 Ð¾Ð±Ð½Ð°ÑÑÐ¶ÐµÐ½Ñ Ð´Ð²Ð° ÑÐ°Ð·Ð¾Ð²ÑÑ Ð¿ÐµÑÐµÑÐ¾Ð´Ð°, Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ñ Ð¸Ñ ÑÐµÐ¼Ð¿ÐµÑÐ°ÑÑÑÑ Ð¸ Ð·Ð°Ð²Ð¸ÑÐ¸Ð¼Ð¾ÑÑÑ Ð¾Ñ Ð²Ð½ÐµÑÐ½ÐµÐ³Ð¾ Ð¿Ð¾Ð»Ñ. ÐÐ±Ð° Ð¾Ð±ÑÐ°Ð·ÑÐ° Ð±ÑÐ»Ð¸ Ð¸Ð·Ð¼ÐµÑÐµÐ½Ñ Ñ Ð¿Ð¾Ð¼Ð¾ÑÑÑ Ð¿ÑÐµÐ·Ð¾ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÑÐ¸Ð»Ð¾Ð²Ð¾Ð¹ Ð¼Ð¸ÐºÑÐ¾ÑÐºÐ¾Ð¿Ð¸Ð¸. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½Ñ Ð¿Ð¾Ð»ÑÑÐ¸Ð·Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐµ ÑÐºÑÐ¿ÐµÑÐ¸Ð¼ÐµÐ½ÑÑ. ÐÑÐ¸ÑÑÐ°Ð»Ð» PZT Ð¿Ð¾ÐºÐ°Ð·Ð°Ð» ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÐ¹ Ð¿ÑÐµÐ·Ð¾ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ð¹ Ð¾ÑÐºÐ»Ð¸Ðº Ð½Ð° ÑÐ°Ð·Ð½ÑÑ ÑÑÐ°ÑÑÐºÐ°Ñ Ð¿Ð¾Ð²ÐµÑÑÐ½Ð¾ÑÑÐ¸ Ð¾Ð±ÑÐ°Ð·ÑÐ°, ÑÑÐ¾ Ð³Ð¾Ð²Ð¾ÑÐ¸Ñ Ð¾ ÐµÐ³Ð¾ Ð½ÐµÐ¾Ð´Ð½Ð¾ÑÐ¾Ð´Ð½Ð¾ÑÑÐ¸.
description: The samples of Pb[Zr â. â â âTi â. âââ]Oâ (PZT 1.1) single crystal and 0.8Pb[Mg â/âNb â/â]Oâ - 0.2PbTiOâ (PMN PT20) ceramics were investigated. PMN PT20 ceramics was measured with the dielectric spectroscopy method. For PMN PT20 two phase transitions were observed, their temperatures were determined, and their dependence on an external field. Both samples were measured with piezoresponse force microscopy (PFM). Polarization experiments were provided. The PZT crystal showed a different piezoelectric response at different areas of the sample surface, which corresponds to its inhomogeneity.
Sky subtraction at the Poisson limit with fibre-optic multi-object spectroscopy
Creators: name: Sharp, Robert
name: Parkinson, Hannah
Publisher: name: arXiv
Year: 2010
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: We report on the limitations of sky subtraction accuracy for long duration fibre-optic multi-object spectroscopy of faint astronomical sources during long duration exposures. We show that while standard sky subtraction techniques yield accuracies consistent with the Poisson noise limit for exposures of 1 hour duration, there are large scale systematic defects that inhibit the sensitivity gains expected on the summation of longer duration exposures. For the AAOmega system at the Anglo-Australian Telescope we identify a limiting systematic sky subtraction accuracy which is reached after integration times of 4-10 hours. We show that these systematic defects can be avoided through the use of the fibre nod-and-shuffle observing mode, but with potential cost in observing efficiency. Finally we demonstrate that these disadvantages can be overcome through the application of a Principle Components Analysis sky subtraction routine. Such an approach minimise systematic residuals across long duration exposures allowing deep integrations. We apply the PCA approach to over 200 hours of on-sky observations and conclude that for the AAOmega system the residual error in long duration observations falls at a rate proportional to t^-0.32 in contrast to the t^-0.5 rate expected from theoretical considerations. With this modest rate of decline, the PCA approach represents a more efficient mode of observation than the nod-and-shuffle technique for observations in the sky limited regime with durations of 10-100 hours (even before accounting for the additional signal-to-noise and targeting efficiency losses often associated with the N+S technique).[abridged]
description: 18 pages, 13 figures, accepted for publication MNRAS July 2010
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¼Ð¾Ð±Ð¸Ð»ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐ¸Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ð´Ð»Ñ ÑÑÑÐ°Ñ Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ½ÑÑ ÑÑÐµÐ´ÑÑÐ² Ð¿Ð¾Ð´ ÐÐ¡ Android
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 mobile application for vehicle insurance for Android OS
Creators: name: Ð¨Ð°Ð¿Ð¾Ð²Ð°Ð», ÐÐ¾Ð»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: 2021
Subjects: Ð¼Ð¾Ð±Ð¸Ð»ÑÐ½Ð¾Ðµ Ð¿ÑÐ¸Ð»Ð¾Ð¶ÐµÐ½Ð¸Ðµ
Android
MVVM
ÑÑÑÐ°Ñ Ð¾Ð²Ð°Ð½Ð¸Ðµ
ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ½Ð¾Ðµ ÑÑÐµÐ´ÑÑÐ²Ð¾
mobile app
insurance
vehicle

description: ÐÐ°Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐµ Ð¼Ð¾Ð±Ð¸Ð»ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐ¸Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ð´Ð»Ñ ÑÑÑÐ°ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ½ÑÑ ÑÑÐµÐ´ÑÑÐ² Ð½Ð° ÐºÑÐ°ÑÐºÐ¾ÑÑÐ¾ÑÐ½ÑÐ¹ Ð¿ÐµÑÐ¸Ð¾Ð´. Ð ÐµÑÐ°ÐµÐ¼ÑÐµ Ð·Ð°Ð´Ð°ÑÐ¸: 1. ÐÐ½Ð°Ð»Ð¸Ð· Ð¿ÑÐµÐ´Ð¼ÐµÑÐ½Ð¾Ð¹ Ð¾Ð±Ð»Ð°ÑÑÐ¸; 2. Ð¡Ð¾ÑÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ ÑÐ¿ÐµÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¸; 3. Ð ÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ Ð¿ÑÐ¸Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ. Ð ÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¾Ð¼ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ Ð¿Ð¾Ð»Ð½Ð¾ÑÑÑÑ ÑÑÐ½ÐºÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ðµ Ð¼Ð¾Ð±Ð¸Ð»ÑÐ½Ð¾Ðµ Ð¿ÑÐ¸Ð»Ð¾Ð¶ÐµÐ½Ð¸Ðµ, ÐºÐ¾ÑÐ¾ÑÐ¾Ðµ Ð¿Ð¾Ð·Ð²Ð¾Ð»Ð¸Ñ Ð¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ¼ ÑÑÑÐ°ÑÐ¾Ð²Ð°ÑÑ ÑÐ²Ð¾Ð¸ ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ½ÑÐµ ÑÑÐµÐ´ÑÑÐ²Ð° Ð¿Ð¾ Ð½ÐµÑÐºÐ¾Ð»ÑÐºÐ¸Ð¼ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð½ÑÐ¼ ÑÐ°ÑÐ¸ÑÐ°Ð¼, Ð° ÑÐ°ÐºÐ¶Ðµ Ð±ÑÐ´ÐµÑ ÑÐ¾Ð±Ð¸ÑÐ°ÑÑ ÑÐµÐ»ÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð´Ð°Ð½Ð½ÑÐµ Ð½ÐµÐ¿Ð¾ÑÑÐµÐ´ÑÑÐ²ÐµÐ½Ð½Ð¾ Ð²Ð¾ Ð²ÑÐµÐ¼Ñ Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ñ.
description: The given work is devoted to the development of a mobile application for short-term vehicle insurance. Tasks to be solved: 1. Analysis of the subject area; 2. Drawing up a specification; 3. Development of the application. The study resulted into the fully functional mobile application that will allow users to insure their vehicles at several proposed tariffs, and will also collect telematic data directly while driving.
Anisotropic Fluid and Bianchi Type III Model in f(R) Gravity
Creators: name: Sharif, M.
name: Kausar, H. Rizwana
Publisher: name: arXiv
Year: 2011
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: This paper is devoted to study the Bianchi type III model in the presence of anisotropic fluid in f(R) gravity. Exponential and power-law volumetric expansions are used to obtain exact solutions of the field equations. We discuss the physical behavior of the solutions and anisotropy behavior of the fluid, the expansion parameter and the model in future evolution of the universe.
description: 18 pages, accepted for publication in Phys. Lett. B
Unidirectional Electronic Structure in the Parent State of Iron-Chalcogenide Superconductor Fe$_{1+δ}$Te
Creators: name: Machida, Tadashi
name: Kogure, Kazuho
name: Kato, Takuya
name: Nakamura, Hiroshi
name: Takeya, Hiroyuki
name: Mochiku, Takashi
name: Ooi, Shuuichi
name: Mizuguchi, Yoshikazu
name: Takano, Yoshihiko
name: Hirata, Kazuto
name: Sakata, Hideaki
Publisher: name: arXiv
Year: 2011
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: We use scanning tunnelling microscopy and spectroscopy to explore the electronic structure of Fe$_{1.07}$Te which is the parent compound of the iron-chalcogenide superconductors. A unidirectional electronic structure with a period of $a_{0}$ (where $a_{0}$ is the lattice constant) along the a-axis is observed. The unidirectional pattern is visible within an energy range from approximately -200 to +130 meV. Since the direction of the unidirectional electronic structure coincides with those of the underlying antiferromagnetic and the predicted orbital orders, it is presumable that the observed unidirectional structure is closely tied to these orders and is peculiar to the parent state in iron-based superconductors.
description: 6 pages 5 figures
Enstatite-rich Warm Debris Dust around HD165014
Creators: name: Fujiwara, Hideaki
name: Onaka, Takashi
name: Ishihara, Daisuke
name: Yamashita, Takuya
name: Fukagawa, Misato
name: Nakagawa, Takao
name: Kataza, Hirokazu
name: Ootsubo, Takafumi
name: Murakami, Hiroshi
Publisher: name: arXiv
Year: 2010
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: We present the Spitzer/Infrared Spectrograph spectrum of the main-sequence star HD165014, which is a warm (>~ 200 K) debris disk candidate discovered by the AKARI All-Sky Survey. The star possesses extremely large excess emission at wavelengths longer than 5 \mum. The detected flux densities at 10 and 20 \mum are ~ 10 and ~ 30 times larger than the predicted photospheric emission, respectively. The excess emission is attributable to the presence of circumstellar warm dust. The dust temperature is estimated as 300-750 K, corresponding to the distance of 0.7-4.4 AU from the central star. Significant fine-structured features are seen in the spectrum and the peak positions are in good agreement with those of crystalline enstatite. Features of crystalline forsterite are not significantly seen. HD165014 is the first debris disk sample that has enstatite as a dominant form of crystalline silicate rather than forsterite. Possible formation of enstatite dust from differentiated parent bodies is suggested according to the solar system analog. The detection of an enstatite-rich debris disk in the current study suggests the presence of large bodies and a variety of silicate dust processing in warm debris disks.
description: 10 pages, 2 tables, 3 figures, accepted for publication in The Astrophysical Journal Letters
Additional file 1 of Effect of appropriate empirical antimicrobial therapy on mortality of patients with Gram-negative bloodstream infections: a retrospective cohort study
Creators: name: Xu, Shanshan
name: Song, Zhihui
name: Han, Furong
name: Zhang, Chao
Publisher: name: figshare
Year: 2023
Subjects: subject: Space Science
subject: Medicine
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Mathematical Sciences not elsewhere classified
subject: Cancer
subject: Science Policy
subject: Infectious Diseases
subject: FOS: Health sciences
subject: Virology
subject: Computational Biology

description: Supplementary Material 1