Search results for "methods [Magnetic Resonance Imaging]"

showing 10 items of 252 documents

'School adopts an experiment': the photoluminescence in extra-virgin olive oil and in tonic water

2011

We report a laboratory activity, carried out along with high- and secondary-school students, that can be done to increase the interest of the young in scientific studies. Groups of selected students ‘adopted’ experiments at physics research laboratories, under the guidance of university researchers. Subsequently, the students demonstrated the experiments to the public at large during the annual science festival organized in Palermo by the association PalermoScienza, in collaboration with the University of Palermo. Experiments on the magnetic levitation of superconductors and on the photoluminescence of several substances were proposed. We discuss the experiment on photoluminescence as a cas…

Physics education; Teaching methods and strategies; Fluorescence and phosphorescence spectraPhysicsScience instructionPhysics educationTeaching methodPhysics educationGeneral Physics and AstronomyTeaching methods and strategieEducationTonic waterfoodMathematics educationfood.beverageFluorescence and phosphorescence spectraOlive oil
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An inquiry-based approach to Maxwell distribution: a case study with engineering students

2013

The concept of distribution is a fundamental component of statistical thinking. This paper describes a teaching approach for it that uses a specific activity related to the field of statistical mechanics. The concept of the velocity distribution of a particle system is dealt with using an inquiry-based approach involving an experimental examination of Maxwell’s distribution. Some outcomes of a teaching experiment held at the Faculty of Engineering of the University of Palermo, Italy are described.

PhysicsDistribution (number theory)Research in physics education Teaching methods and strategies Laboratory experiments and apparatus Laboratory course design organization and evaluationClassical statistical mechanicsSettore FIS/08 - Didattica E Storia Della Fisica05 social sciences050301 educationGeneral Physics and AstronomyStatistical mechanics01 natural sciencesMaxwell–Boltzmann distributionField (geography)symbols.namesakeTheoretical physicsStatistical thinkingComponent (UML)0103 physical sciencessymbolsMathematics education010306 general physics0503 educationEuropean Journal of Physics
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Search for pulsations at high radio frequencies from accreting millisecond X-ray pulsars in quiescence

2010

It is commonly believed that millisecond radio pulsars have been spun up by transfer of matter and angular momentum from a low-mass companion during an X-ray active mass transfer phase. A subclass of low-mass X-ray binaries is that of the accreting millisecond X-ray pulsars, transient systems that show periods of X-ray quiescence during which radio emission could switch on. The aim of this work is to search for millisecond pulsations from three accreting millisecond X-ray pulsars, XTE J1751-305, XTE J1814-338, and SAX J1808.4-3658, observed during their quiescent X-ray phases at high radio frequencies (5 - 8 GHz) in order to overcome the problem of the free-free absorption due to the matter…

PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)MillisecondAstrophysics::High Energy Astrophysical PhenomenaX-ray binaryFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsLuminosityInterstellar medium85-05pulsars general methods data analysis methods observational stars neutron X-rays binariesNeutron starSettore FIS/05 - Astronomia E AstrofisicaPulsarSpace and Planetary ScienceMillisecond pulsarAstrophysics - High Energy Astrophysical PhenomenaX-ray pulsar
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On Relativistic Disk Spectroscopy in Compact Objects with X-ray CCD Cameras

2010

X-ray charge-coupled devices (CCDs) are the workhorse detectors of modern X-ray astronomy. Typically covering the 0.3-10.0 keV energy range, CCDs are able to detect photoelectric absorption edges and K shell lines from most abundant metals. New CCDs also offer resolutions of 30-50 (E/dE), which is sufficient to detect lines in hot plasmas and to resolve many lines shaped by dynamical processes in accretion flows. The spectral capabilities of X-ray CCDs have been particularly important in detecting relativistic emission lines from the inner disks around accreting neutron stars and black holes. One drawback of X-ray CCDs is that spectra can be distorted by photon "pile-up", wherein two or mor…

PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhotonSpectrometerAstrophysics::High Energy Astrophysical PhenomenaElectron shellFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum CosmologyRelativistic diskSpectral lineaccretion accretion disks black hole physics instrumentation spectrographs methods analytical X-rays binariesNeutron starSettore FIS/05 - Astronomia E AstrofisicaSpace and Planetary ScienceEmission spectrumAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaSpectroscopyAstrophysics::Galaxy Astrophysics
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Some analytical considerations on two-scale relations

1994

Scaling functions that generate a multiresolution analysis (MRA) satisfy, among other conditions, the so-called «two-scale relation» (TSR). In this paper we discuss a number of properties that follow from the TSR alone, independently of any MRA: position of zeros (mainly for continuous scaling functions), existence theorems (using fixed point and eigenvalue arguments) and orthogonality relation between integer translates. © 1994 Società Italiana di Fisica.

PhysicsMathematics::Functional AnalysisScale (ratio)mathematical methods in physicsFixed pointIntegerProbability theoryOrthogonalityPosition (vector)Computer Science::Computer Vision and Pattern RecognitionQuantum mechanicsApplied mathematicsSettore MAT/07 - Fisica MatematicaScalingEigenvalues and eigenvectorsIl Nuovo Cimento B
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Time characteristics of Lévy flights in a steep potential well

2013

Using the method previously developed for ordinary Brownian diffusion, we derive a new formula to calculate the correlation time of stationary Lévy flights in a steep potential well. For the symmetric quartic potential, we obtain the exact expression of the correlation time of steady-state Lévy flights with index α = 1. The correlation time of stationary Lévy flights decreases with an increasing noise intensity and steepness of potential well.

PhysicsMathematics::ProbabilityLévy flightQuartic functionGeneral Physics and AstronomyNoise intensityGeneral Materials ScienceLévy flights Kolmogorov equation Frcational Fokker-Planck equation Stochastic Dynamics (theory) Methods of Stochastic Analysis Exact resultsStatistical physicsPhysical and Theoretical ChemistrySettore FIS/03 - Fisica Della MateriaBrownian motionThe European Physical Journal Special Topics
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Low energy collective modes of deformed superfluid nuclei within the finite amplitude method

2013

Background: The major challenge for nuclear theory is to describe and predict global properties and collective modes of atomic nuclei. Of particular interest is the response of the nucleus to a time-dependent external field that impacts the low-energy multipole and beta-decay strength. Purpose: We propose a method to compute low-lying collective modes in deformed nuclei within the finite amplitude method (FAM) based on the quasiparticle random-phase approximation (QRPA). By using the analytic property of the response function, we find the QRPA amplitudes by computing the residua of the FAM amplitudes by means of a contour integration around the QRPA poles in a complex frequency plane. Metho…

PhysicsNuclear and High Energy Physicsta114Nuclear TheoryIsoscalarNuclear TheoryMagnetic monopoleFOS: Physical sciencesMethods of contour integrationNuclear Theory (nucl-th)Matrix (mathematics)Classical mechanicsQuantum mechanicsAtomic nucleusQuasiparticleMultipole expansionNuclear ExperimentNuclear density
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Kinematics of Magnetic Bright Features in the Solar Photosphere

2016

S. Jafarzadeh et. al.

PhysicsPhotospherephotosphere [Sun]FOS: Physical sciencesSun: photosphereAstronomy and AstrophysicsSolar photosphereAstrophysicsKinematics01 natural sciencesMethods observationalmagnetic fields [Sun]Methods: observationalAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary Science0103 physical sciencesAstrophysics::Solar and Stellar Astrophysicsobservational [Methods]010306 general physics010303 astronomy & astrophysicsSun: magnetic fieldsSolar and Stellar Astrophysics (astro-ph.SR)
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Nonadiabatic quantum search algorithms

2007

7 pages, 4 figures.-- PACS nrs.: 03.67.Lx, 05.45.Mt, 72.15.Rn.-- ISI Article Identifier: 000251326400049.-- ArXiv pre-print available at: http://arxiv.org/abs/0706.1139

PhysicsQuantum PhysicsFOS: Physical sciences[PACS] Semiclassical methods in quantum chaosAdiabatic quantum computationAtomic and Molecular Physics and OpticsQuantum chaosCromodinàmica quànticaAmplitude amplificationSearch algorithm[PACS] Localization effects (metals/alloys) including Anderson or weak localizationGrover's algorithmQuantum algorithmCamps Teoria quàntica deQuantum informationQuantum Physics (quant-ph)AlgorithmQuantum computer[PACS] Quantum computation
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A pedagogical approach to the Boltzmann factor through experiments and simulations

2009

The Boltzmann factor is the basis of a huge amount of thermodynamic and statistical physics, both classical and quantum. It governs the behaviour of all systems in nature that are exchanging energy with their environment. To understand why the expression has this specific form involves a deep mathematical analysis, whose flow of logic is hard to see and is not at the level of high school or college students' preparation. We here present some experiments and simulations aimed at directly deriving its mathematical expression and illustrating the fundamental concepts on which it is grounded. Experiments use easily available apparatuses, and simulations are developed in the Net-Logo environment…

PhysicsScience instructionBasis (linear algebra)Interface (Java)Settore FIS/08 - Didattica E Storia Della FisicaPhysics::Physics EducationGeneral Physics and AstronomyStatistical mechanicsComputer in educationLaboratory experiments and apparatusBoltzmann distributionExpression (mathematics)Teaching methods and strategieEducationFlow (mathematics)ComputingMilieux_COMPUTERSANDEDUCATIONStatistical physicsQuantum
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