Search results for "methods [Neuroimaging]"

showing 10 items of 244 documents

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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Swift follow-up of IceCube triggers, and implications for the Advanced-LIGO era

2015

Between 2011 March and 2014 August Swift responded to 20 triggers from the IceCube neutrino observatory, observing the IceCube 50% confidence error circle in X-rays, typically within 5 hours of the trigger. No confirmed counterpart has been detected. We describe the Swift follow up strategy and data analysis and present the results of the campaign. We discuss the challenges of distinguishing the X-ray counterpart to a neutrino trigger from serendipitous uncatalogued X-ray sources in the error circle, and consider the implications of our results for future strategies for multi-messenger astronomy, with particular reference to the follow up of gravitational wave triggers from the advanced-era…

PhysicsSwiftHigh Energy Astrophysical Phenomena (astro-ph.HE)Astrophysics::High Energy Astrophysical PhenomenaAstronomyLibrary scienceFOS: Physical sciencesAstronomy and AstrophysicsMethods observationalLIGOSpace and Planetary Scienceddc:520Astrophysics - High Energy Astrophysical Phenomenacomputercomputer.programming_language
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Real-time Fluorescence Measurement of Enterovirus Uncoating

2019

Viruses need to open, i.e., uncoat, in order to release their genomes for efficient replication and translation. Especially for non-enveloped viruses, such as enteroviruses, the cues leading to uncoating are less well known. The status of the virus has previously been observed mainly by transmission electron microscopy using negative staining, cryo electron microscopy, X-ray crystallography or gradient separation (reviewed in Tuthill et al., 2010, Myllynen et al., 2016, Ruokolainen et al., 2019). However, monitoring of uncoating has been limited by the lack of methods detecting dynamic changes of the virions. Here, we present a real-time fluorescence based protocol, which detects the viral …

PicornavirusRNase PCryo-electron microscopyStrategy and ManagementvirusesspektroskopiainfektiotIndustrial and Manufacturing EngineeringVirusMethods ArticletutkimusmenetelmätRNaseNucleic acid structuregenomeEnterovirusbiologyChemistryMechanical EngineeringSYBR Green IIVirus UncoatingPicornavirusMetals and AlloysfluoresenssiRNAfluorescence spectroscopybiology.organism_classificationNegative stainCell biologyenteroviruksetRNAuncoating
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