Search results for "WTO"

showing 10 items of 163 documents

Diffusion Acceleration in Randomly Switching Sawtooth Potential

2005

We investigate an overdamped Brownian motion in symmetric sawtooth periodic potential switched by Markovian dichotomous noise between two configurations. The two configurations differ each other by a translation of half of period. The calculation of the effective diffusion coefficient is reduced to the mean first‐passage time problem, and we obtain the exact expression valid for arbitrary mean rate of switchings and arbitrary intensity of white Gaussian noise. We find the area at parameters plane where acceleration of diffusion in comparison with the free diffusion case takes place.

Anomalous diffusionMathematical analysisSawtooth waveWhite noiseRATCHETSNoise (electronics)TIMESsymbols.namesakeAccelerationGaussian noiseQuantum mechanicssymbolsMOTORSDiffusion (business)Brownian motionMathematics
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A generalized Newton iteration for computing the solution of the inverse Henderson problem

2020

We develop a generalized Newton scheme IHNC for the construction of effective pair potentials for systems of interacting point-like particles.The construction is made in such a way that the distribution of the particles matches a given radial distribution function. The IHNC iteration uses the hypernetted-chain integral equation for an approximate evaluation of the inverse of the Jacobian of the forward operator. In contrast to the full Newton method realized in the Inverse Monte Carlo (IMC) scheme, the IHNC algorithm requires only a single molecular dynamics computation of the radial distribution function per iteration step, and no further expensive cross-correlations. Numerical experiments…

Applied MathematicsGeneral EngineeringInverseNumerical Analysis (math.NA)010103 numerical & computational mathematicsRadial distribution function01 natural sciencesComputer Science Applications010101 applied mathematicssymbols.namesakeScheme (mathematics)FOS: MathematicssymbolsApplied mathematicsMathematics - Numerical AnalysisGranularity0101 mathematicsNewton's method65Z05 82B21MathematicsInverse Problems in Science and Engineering
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A regularized Newton method for locating thin tubular conductivity inhomogeneities

2011

We consider the inverse problem of determining the position and shape of a thin tubular object, such as for instance a wire, a thin channel or a curve-like crack, embedded in some three-dimensional homogeneous body from a single measurement of electrostatic currents and potentials on the boundary of the body. Using an asymptotic model describing perturbations of electrostatic potentials caused by such thin objects, we reformulate the inverse problem as a nonlinear operator equation. We establish Frechet differentiability of the corresponding operator, compute its Frechet derivative and set up a regularized Newton scheme to solve the inverse problem numerically. We discuss our implementation…

Applied MathematicsOperator (physics)Mathematical analysisFréchet derivativeBoundary (topology)Inverse problemComputer Science ApplicationsTheoretical Computer Sciencesymbols.namesakeNewton fractalPosition (vector)Signal ProcessingsymbolsDifferentiable functionNewton's methodMathematical PhysicsMathematicsInverse Problems
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A White Paper on keV sterile neutrino Dark Matter

2017

We present a comprehensive review of keV-scale sterile neutrino Dark Matter, collecting views and insights from all disciplines involved - cosmology, astrophysics, nuclear, and particle physics - in each case viewed from both theoretical and experimental/observational perspectives. After reviewing the role of active neutrinos in particle physics, astrophysics, and cosmology, we focus on sterile neutrinos in the context of the Dark Matter puzzle. Here, we first review the physics motivation for sterile neutrino Dark Matter, based on challenges and tensions in purely cold Dark Matter scenarios. We then round out the discussion by critically summarizing all known constraints on sterile neutrin…

AstrofísicaSterile neutrinocosmological modelCold dark mattercosmological neutrinosPhysics beyond the Standard Model[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]Dark matter theory01 natural sciencesCosmologyHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)White paperHigh Energy Physics - Phenomenology (hep-ph)X-RAY-EMISSIONMETALLIC MAGNETIC CALORIMETERSQUANTUM-FIELD THEORY[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]neutrino: dark matterCosmological neutrinos; Dark matter experiments; Dark matter theory; Particle physics - cosmology connection010303 astronomy & astrophysicsPhysicsdark matter theorynew physicsDOUBLE-BETA-DECAYhep-phneutrino: sterileCosmological neutrinos; Dark matter experiments; Dark matter theory; Particle physics - cosmology connection; Astronomy and AstrophysicsNuclear & Particles PhysicsHigh Energy Physics - Phenomenologyneutrino: detectorDark matter experimentsparticle physics - cosmology connectionastro-ph.COMILKY-WAY SATELLITESCosmological neutrinos3.5 KEV LINENeutrinoParticle Physics - ExperimentAstrophysics - Cosmology and Nongalactic AstrophysicsParticle physicsAstrophysics and AstronomyCosmology and Nongalactic Astrophysics (astro-ph.CO)astro-ph.GADark matterLY-ALPHA FORESTreviewFOS: Physical sciencesContext (language use)neutrino: productionX-raySettore FIS/05 - Astronomia e Astrofisica[ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex]RIGHT-HANDED NEUTRINOS0103 physical sciencesAstronomical And Space Sciencesnumerical calculationsDark matter experimentXMM-NEWTON OBSERVATIONSneutrino: modelParticle Physics - PhenomenologyDWARF SPHEROIDAL GALAXYCosmologia010308 nuclear & particles physicshep-exdark matter experimentsHigh Energy Physics::PhenomenologyAstronomy and AstrophysicsAtomic Molecular Nuclear Particle And Plasma PhysicsCosmological neutrinoAstrophysics - Astrophysics of Galaxies13. Climate actionAstrophysics of Galaxies (astro-ph.GA)[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]Particle physics - cosmology connection[ PHYS.HPHE ] Physics [physics]/High Energy Physics - Phenomenology [hep-ph]High Energy Physics::Experimentneutrino: oscillation[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Journal of Cosmology and Astroparticle Physics
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Experimental modeling of viscous inclusions in a circular high-strain shear rig: Implications for the interpretation of shape fabrics and deformed en…

2002

[1] Deformation experiments with initially spherical and prolate viscous inclusions suspended in a viscous Newtonian matrix in a circular high strain annular shear rig provide insights on the shape development of inclusions in high strain shear zones during progressive deformation. Inclusions with a specific viscosity ratio with respect to the matrix material show distinct types of three-dimensional shape development. For instance, at a high viscosity ratio between matrix and inclusion a pulsating ellipsoid develops, which both continuously rotates and changes its shape from a sphere to an ellipsoid and back to a sphere. The experiments show that the shape of an inclusion that has a viscosi…

Atmospheric ScienceEcologyPaleontologySoil ScienceMineralogyForestryMechanicsAquatic ScienceOceanographyEllipsoidPower lawPhysics::Fluid DynamicsViscosityGeophysicsShear (geology)RheologySpace and Planetary ScienceGeochemistry and PetrologyFinite strain theoryEarth and Planetary Sciences (miscellaneous)Newtonian fluidShear zoneGeologyEarth-Surface ProcessesWater Science and TechnologyJournal of Geophysical Research: Solid Earth
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Sawtooth-wave adiabatic-passage slowing of dysprosium

2018

We report on sawtooth wave adiabatic passage (SWAP) slowing of bosonic and fermionic dysprosium isotopes by using a 136 kHz wide transition at 626 nm. A beam of precooled atoms is further decelerated in one dimension by the SWAP force and the amount of atoms at near zero velocity is measured. We demonstrate that the SWAP slowing can be twice as fast as in a conventional optical molasses operated on the same transition. In addition, we investigate the parameter range for which the SWAP force is efficiently usable in our set-up, and relate the results to the adiabaticity condition. Furthermore, we add losses to the hyperfine ground-state population of fermionic dysprosium during deceleration …

Atomic Physics (physics.atom-ph)PopulationFOS: Physical scienceschemistry.chemical_elementSawtooth wave01 natural sciencesPhysics - Atomic Physics010305 fluids & plasmas0103 physical sciencesPhysics::Atomic Physics010306 general physicsAdiabatic processeducationHyperfine structurePhysicsQuantum PhysicsRange (particle radiation)education.field_of_studychemistryQuantum Gases (cond-mat.quant-gas)Optical molassesDysprosiumAtomic physicsQuantum Physics (quant-ph)Condensed Matter - Quantum GasesBeam (structure)Physical Review A
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New role of sawtooth transcription factors in the shift to photoautotrophic growth in plants

2016

BioengineeringGeneral MedicineSawtooth waveBiologyMolecular BiologyTranscription factorBiotechnologyCell biologyNew Biotechnology
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Blokķēžu tehnoloģijas ieviešana numuru pārnesamības sistēmā

2022

Darba mērķis: Izstrādāt sistēmas prototipu modernizētai mobilo numuru pārnesamības (MNP) sistēmai, kas atbilstu izvirzītajām sistēmas prasībām un būtu saskaņā ar visu iesaistīto pušu interesēm. Darbs sastāv no 3 daļām, kur pirmajā tiek aprakstīts mobilo numuru pārnešanas process un tiek apskatītas iespējamās alternatīvas pašreiz lietotajai sistēmai, otrajā tiek padziļināti izpētīta blokķēžu tehnoloģijas būtība, kā arī tiek izpētīti pieejamie risinājumi un sagatavoti piemēri kā būtu jāizskatās MNP procesiem, izmantojot izpētītos risinājumus, bet trešajā daļā tiek izstrādāts prototips MNP procesam, kas tiek darbināts Hyperledger Sawtooth platformā. Rezultātā tiek izstrādāts sistēmas prototips…

BlokķēdeDatorzinātneHyperledger sawtoothViedie līgumiNumuru pārnešana
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Oscillatory integrals and fractal dimension

2021

Theory of singularities has been closely related with the study of oscillatory integrals. More precisely, the study of critical points is closely related to the study of asymptotic of oscillatory integrals. In our work we investigate the fractal properties of a geometrical representation of oscillatory integrals. We are motivated by a geometrical representation of Fresnel integrals by a spiral called the clothoid, and the idea to produce a classification of singularities using fractal dimension. Fresnel integrals are a well known class of oscillatory integrals. We consider oscillatory integral $$ I(\tau)=\int_{; ; \mathbb{; ; R}; ; ^n}; ; e^{; ; i\tau f(x)}; ; \phi(x) dx, $$ for large value…

Box dimensionGeneral Mathematics010102 general mathematicsMathematical analysisPhase (waves)Resolution of singularitiesOscillatory integral ; Box dimension ; Minkowski content ; Critical points ; Newton diagramCritical points01 natural sciencesFractal dimensionCritical point (mathematics)Oscillatory integralAmplitudeDimension (vector space)Mathematics - Classical Analysis and ODEsMinkowski contentClassical Analysis and ODEs (math.CA)FOS: Mathematics0101 mathematicsMinkowski contentOscillatory integralNewton diagram[MATH]Mathematics [math]fractal dimension; box dimension; oscillatory integrals; theory of singularitiesMathematics
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MILES extended: Stellar population synthesis models from the optical to the infrared

2016

We present the first single-burst stellar population models which covers the optical and the infrared wavelength range between 3500 and 50000 Angstrom and which are exclusively based on empirical stellar spectra. To obtain these joint models, we combined the extended MILES models in the optical with our new infrared models that are based on the IRTF (Infrared Telescope Facility) library. The latter are available only for a limited range in terms of both age and metallicity. Our combined single-burst stellar population models were calculated for ages larger than 1 Gyr, for metallicities between [Fe/H] = -0.40 and 0.26, for initial mass functions of various types and slopes, and on the basis …

CAII TRIPLETStellar populationInfraredMetallicityINITIAL MASS FUNCTIONBROWN DWARFSInfrared telescopeFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesAstronomical spectroscopyinfrared: galaxiesATMOSPHERIC PARAMETERS0103 physical sciencesRange (statistics)Astrophysics::Solar and Stellar Astrophysics2.5 MU-MGIANT BRANCH STARS010303 astronomy & astrophysicsinfrared: starsEMPIRICAL CALIBRATIONAstrophysics::Galaxy AstrophysicsPhysics010308 nuclear & particles physicsNear-infrared spectroscopyHIGH-SPECTRAL-RESOLUTIONAstronomy and AstrophysicsEVOLUTIONARY SYNTHESISAstrophysics - Astrophysics of GalaxiesGalaxySpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)NEWTON-TELESCOPE LIBRARYgalaxies: stellar contentAstrophysics::Earth and Planetary Astrophysics
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