Search results for "65"

showing 10 items of 1111 documents

Environmental and Product Contamination during the Preparation of Antineoplastic Drugs with Robotic Systems

2018

Abstract Background Robotic systems are designed to minimize the exposure to antineoplastic drugs during automated preparation. However, contamination cannot be completely excluded. The aim of the study was to evaluate the contamination with antineoplastic drugs on the working surfaces and on the outer surface of the ready-to-use products (infusion bags and syringes) during automated preparation with different versions of a robot and manual preparation. Methods Surface contamination with platinum (Pt) and 5-fluorouracil (5-FU) was measured by wipe sampling and quantified by voltammetry for Pt and GC-MS for 5-FU. Sampling was performed on pre-defined locations in the working areas before and…

PharmacyRM1-950030226 pharmacology & pharmacygas chromatography/mass spectrometryantineoplastic drugs03 medical and health sciences0302 clinical medicineMedicinePharmacology (medical)Pharmaceutical industryPharmacologyvoltammetryChromatographybusiness.industrysurface contaminationautomated compoundingContaminationwipe samplingRobotic systems030220 oncology & carcinogenesisProduct (mathematics)Antineoplastic DrugsTherapeutics. PharmacologyGas chromatography–mass spectrometryHD9665-9675businessWipe samplingPharmaceutical Technology in Hospital Pharmacy
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Nucleation and Collapse of the Superconducting Phase in Type-I Superconducting Films

2005

The phase transition between the intermediate and normal states in type-I superconducting films is investigated using magneto-optical imaging. Magnetic hysteresis with different transition fields for collapse and nucleation of superconducting domains is found. This is accompanied by topological hysteresis characterized by the collapse of circular domains and the appearance of lamellar domains. Magnetic hysteresis is shown to arise from supercooled and superheated states. Domain-shape instability resulting from long-range magnetic interaction accounts well for topological hysteresis. Connection with similar effects in systems with long-range magnetic interactions is emphasized.

Phase transitionnucleationNucleationFOS: Physical sciencesGeneral Physics and Astronomytopological hysteresis02 engineering and technology01 natural sciencesInstabilitySuperconductivity (cond-mat.supr-con)74.25.Ha 05.65.+b 75.70.KwCondensed Matter::SuperconductivityPhase (matter)0103 physical sciences010306 general physicsSupercoolingSuperconductivityPhysicsCondensed matter physicsCondensed Matter - Superconductivitysuperconductivitydomain pattern021001 nanoscience & nanotechnologyMagnetic hysteresis[PHYS.COND.CM-S]Physics [physics]/Condensed Matter [cond-mat]/Superconductivity [cond-mat.supr-con]Hysteresisphase transition0210 nano-technologyPhysical Review Letters
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Search for multiwavelength emission from the binary millisecond pulsar PSR J1836-2354A in the globular cluster M22

2019

We present a multi-band search for X-ray, optical and $\gamma$-ray emission of the radio binary millisecond pulsar J1836-2354A, hosted in the globular cluster M22. X-ray emission is significantly detected in two Chandra observations, performed in 2005 and 2014, at a luminosity of $\sim$2-3$\times$10$^{30}$ erg s$^{-1}$, in the 0.5-8 keV energy range. The radio and the X-ray source positions are found consistent within 1$\sigma$ error box. No detection is found in archival XMM-Newton and Swift/XRT observations, compatible with the Chandra flux level. The low statistics prevents us to assess if the X-ray source varied between the two observations. The X-ray spectrum is consistent with a power…

PhotonAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesBinary numberFluxAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesLuminosityX-rays: binariesMillisecond pulsarpulsars: general0103 physical sciences010303 astronomy & astrophysicsX-rays: individual: PSR J1836-2354AAstrophysics::Galaxy AstrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Physics010308 nuclear & particles physicsglobular clusters: individual: M22 (NGC 6656)Astronomy and AstrophysicsX-rays: binarie13. Climate actionSpace and Planetary ScienceGlobular clusterNo detectionAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Energy (signal processing)
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Prolonged sub-luminous state of the new transitional pulsar candidate CXOU J110926.4-650224

2019

We report on a multi-wavelength study of the unclassified X-ray source CXOU J110926.4-650224 (J1109). We identified the optical counterpart as a blue star with a magnitude of $\sim$20.1 (3300-10500 $\require{mediawiki-texvc} \AA$). The optical emission was variable on timescales from hundreds to thousands of seconds. The spectrum showed prominent emission lines with variable profiles at different epochs. Simultaneous XMM-Newton and NuSTAR observations revealed a bimodal distribution of the X-ray count rates on timescales as short as tens of seconds, as well as sporadic flaring activity. The average broad-band (0.3-79 keV) spectrum was adequately described by an absorbed power law model with…

PhotonX-rays: BinarieAstrophysics::High Energy Astrophysical PhenomenaFluxFOS: Physical sciencesAstrophysicsMethods: Data analysiAstrophysics::Cosmology and Extragalactic Astrophysics7. Clean energy01 natural sciencesLuminosityAccretion accretion diskSettore FIS/05 - Astronomia E AstrofisicaPulsarMethods: Observational0103 physical sciencesEmission spectrum010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsAstronomy and AstrophysicsStars: neutronX-rays: Individuals: CXOU J110926.4-650224Neutron star13. Climate actionSpace and Planetary ScienceMagnitude (astronomy)Astrophysics - High Energy Astrophysical PhenomenaFermi Gamma-ray Space Telescope
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A 1D coupled Schrödinger drift-diffusion model including collisions

2005

We consider a one-dimensional coupled stationary Schroedinger drift-diffusion model for quantum semiconductor device simulations. The device domain is decomposed into a part with large quantum effects (quantum zone) and a part where quantum effects are negligible (classical zone). We give boundary conditions at the classic-quantum interface which are current preserving. Collisions within the quantum zone are introduced via a Pauli master equation. To illustrate the validity we apply the model to three resonant tunneling diodes.

Physics and Astronomy (miscellaneous)Quantum dynamics34L40Pauli master equationinterface conditionsQuantum mechanicsPrincipal quantum numberQuantum operation65Z05quantum-classical couplingAmplitude damping channelscattering states82D37PhysicsNumerical Analysis82C70Applied Mathematics34L30Quantum numberComputer Science Applications34L25Computational MathematicsModeling and SimulationQuantum process78A35Schroedinger equationdrift-diffusionQuantum algorithmQuantum dissipation
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Efficient numerical integration of neutrino oscillations in matter

2016

A special purpose solver, based on the Magnus expansion, well suited for the integration of the linear three neutrino oscillations equations in matter is proposed. The computations are speeded up to two orders of magnitude with respect to a general numerical integrator, a fact that could smooth the way for massive numerical integration concomitant with experimental data analyses. Detailed illustrations about numerical procedure and computer time costs are provided.

Physics010308 nuclear & particles physicsComputationNumerical analysisFOS: Physical sciencesNumerical Analysis (math.NA)65L05 65L20Computational Physics (physics.comp-ph)Solver01 natural sciencesNumerical integrationHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Classical mechanicsIntegratorMagnus expansion0103 physical sciencesFOS: MathematicsApplied mathematicsMathematics - Numerical Analysis010306 general physicsNeutrino oscillationPhysics - Computational PhysicsNumerical stability
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Dynamics of correlations due to a phase noisy laser

2012

We analyze the dynamics of various kinds of correlations present between two initially entangled independent qubits, each one subject to a local phase noisy laser. We give explicit expressions of the relevant quantifiers of correlations for the general case of single-qubit unital evolution, which includes the case of a phase noisy laser. Although the light field is treated as classical, we find that this model can describe revivals of quantum correlations. Two different dynamical regimes of decay of correlations occur, a Markovian one (exponential decay) and a non-Markovian one (oscillatory decay with revivals) depending on the values of system parameters. In particular, in the non-Markovia…

Physics03.67.Mn Entanglement measures witnesses and other characterizationQuantum discordQuantum PhysicsPhase (waves)Markov processFOS: Physical sciencesQuantum entanglement03.65.Ud Entanglement and quantum nonlocality (e.g. EPR paradox Bell's inequalities GHZ states etc.)Condensed Matter PhysicsAtomic and Molecular Physics and OpticsSettore FIS/03 - Fisica Della Materiasymbols.namesake02.50.Ga Markov processeQubit42.50.Dv Quantum state engineering and measurementsymbolsStatistical physicsExponential decayQuantum Physics (quant-ph)QuantumMathematical PhysicsLight field03.67.Lx Quantum computation architectures and implementations03.65.Ud Entanglement and quantum nonlocality (e.g. EPR paradox Bell's inequalities GHZ states etc.); 42.50.Dv Quantum state engineering and measurements; 03.67.Mn Entanglement measures witnesses and other characterizations; 02.50.Ga Markov processes; 03.67.Lx Quantum computation architectures and implementations
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Towards the time-optimal control of dissipative spin-1/2 particles in nuclear magnetic resonance

2011

International audience; We consider the time-optimal control of a spin 1/2 particle whose dynamics is governed by the Bloch equations with both longitudinal and transverse relaxation terms. We solve this control problem by using geometric optimal control techniques. We show the crucial role of singular extremals in the time-optimal synthesis. This role can mainly be attributed to the presence of dissipation. We also analyze the robustness of the optimal control sequence when both the maximum amplitude of the control field and the dissipative parameters are varied. Finally, we present an experimental implementation of the different solutions using techniques of Nuclear Magnetic Resonance.

Physics32.80.QkDissipationCondensed Matter PhysicsTime optimalOptimal control01 natural sciencesAtomic and Molecular Physics and Optics010305 fluids & plasmasNuclear magnetic resonanceBloch equationsTransverse relaxationRobustness (computer science)0103 physical sciences03.65.Yz78.20.BhDissipative system010306 general physicsMaximum amplitude
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An algorithm for computing geometric relative velocities through Fermi and observational coordinates

2013

We present a numerical method for computing the \textit{Fermi} and \textit{observational coordinates} of a distant test particle with respect to an observer. We apply this method for computing some previously introduced concepts of relative velocity: \textit{kinematic}, \textit{Fermi}, \textit{spectroscopic} and \textit{astrometric} relative velocities. We also extend these concepts to non-convex normal neighborhoods and we make some convergence tests, studying some fundamental examples in Schwarzschild and Kerr spacetimes. Finally, we show an alternative method for computing the Fermi and astrometric relative velocities.

Physics83C10 83-08 65Z05Physics and Astronomy (miscellaneous)Numerical analysisMathematical analysisRelative velocityFOS: Physical sciencesKinematicsGeneral Relativity and Quantum Cosmology (gr-qc)Mathematical Physics (math-ph)Observer (physics)General Relativity and Quantum CosmologyConvergence testsTest particleSchwarzschild radiusMathematical PhysicsFermi Gamma-ray Space Telescope
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The Role Of General Relativity in the Evolution of Low-Mass X-ray Binaries

2005

We study the evolution of Low Mass X-ray Binaries (LMXBs) and of millisecond binary radio pulsars (MSPs), with numerical simulations that keep into account the evolution of the companion, of the binary system and of the neutron star. According to general relativity, when energy is released, the system loses gravitational mass. Moreover, the neutron star can collapse to a black hole if its mass exceeds a critical limit, that depends on the equation of state. These facts have some interesting consequences: 1) In a MSP the mass-energy is lost with a specific angular momentum that is smaller than the one of the system, resulting in a positive contribution to the orbital period derivative. If th…

Physics:relativityX-rays : binariesGeneral relativityAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)pulsars : generalFOS: Physical sciencesrelativity; binaries : close; stars : individual : SAX J1808.4-3658; stars : neutron; pulsars : general; X-rays : binariesAstronomy and AstrophysicsAstrophysicsMoment of inertiaOrbital periodAstrophysicsSpecific relative angular momentumstars : neutronBlack holeNeutron starPulsarstars : individual : SAX J1808.4-3658Space and Planetary Sciencebinaries : closeLow Mass
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