Search results for "methods [Biological Assay]"

showing 10 items of 243 documents

Non-thermal processes in coronae and beyond

2013

This contribution summarizes the splinter session “Non-thermal processes in coronae and beyond” held at the Cool Stars 17 workshop in Barcelona in 2012. It covers new developments in high energy non-thermal effects in the Earth's exosphere, solar and stellar flares, the diffuse emission in star forming regions and reviews the state and the challenges of the underlying atomic databases. (© 2013 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim)

PhysicsHigh energyStarsSolar flareSpace and Planetary ScienceThermalAstronomyAstronomy and AstrophysicsMethods laboratoryExosphereAtomic dataAstronomische Nachrichten
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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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Rotational spectra of CF+and13CF+: accurate rest frequencies and spectroscopic parameters

2010

Context. The astrophysical relevance of the fluoromethylidynium ion and its importance for the interstellar chemistry of fluorine motivated the present laboratory spectroscopic investigation of both 12 CF + and the corresponding 13 C-containing isotopologue, 13 CF + . Aims. This investigation has been carried out to provide accurate rest frequencies for future (radioastronomical) observations, to improve the accuracy of the values for the spectroscopic parameters available in the literature for CF + , and to provide them for the first time for 13 CF + . Methods. Rotational spectra of CF + and 13 CF + were recorded in the millimeter- and submillimeter-wave frequency ranges. Their investigati…

PhysicschemistrySpace and Planetary ScienceFluorinechemistry.chemical_elementAstronomy and AstrophysicsContext (language use)IsotopologueMethods laboratoryAtomic physicsAstrophysics::Galaxy AstrophysicsSpectral lineIonAstronomy and Astrophysics
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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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