Search results for "methods"

showing 10 items of 4526 documents

Mauro Picone, Sandro Faedo, and the numerical solution of partial differential equations in Italy (1928-1953)

2013

In this paper we revisit the pioneering work on the numerical analysis of partial differential equations (PDEs) by two Italian mathematicians, Mauro Picone (1885-1977) and Sandro Faedo (1913-2001). We argue that while the development of constructive methods for the solution of PDEs was central to Picone's vision of applied mathematics, his own work in this area had relatively little direct influence on the emerging field of modern numerical analysis. We contrast this with Picone's influence through his students and collaborators, in particular on the work of Faedo which, while not the result of immediate applied concerns, turned out to be of lasting importance for the numerical analysis of …

Partial differential equationNumerical analysisApplied MathematicsConstructiveSettore MAT/08 - Analisi NumericaIstituto per le Applicazioni del CalcoloHistory of numerical analysi Istituto per le Applicazioni del Calcolo Evolution problems Faedo–Galerkin method Spectral methodsHistory of numerical analysiCalculusApplied mathematicsEvolution problemFaedo-Galerkin methodAlgebra over a fieldSpectral methodSturm–Picone comparison theoremSpectral methodNumerical partial differential equationsMathematics
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Multiplicity results for Sturm-Liouville boundary value problems

2009

Multiplicity results for Sturm-Liouville boundary value problems are obtained. Proofs are based on variational methods.

Partial differential equationSturm-Liouville problem variational methodsApplied MathematicsNumerical analysisMultiplicity resultsMathematical analysisSturm–Liouville theoryMixed boundary conditionMathematics::Spectral TheoryMathematical proofCritical point (mathematics)Computational MathematicsSettore MAT/05 - Analisi MatematicaBoundary value problemMathematics
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Urban Innovation Through Co-design Scenarios. Lessons from Palermo

2019

This paper aims to contribute to current research on learning through designing for urban innovation. It provides a framework methodology for a multidisciplinary ecosystem as a participatory method developed in the context of Mobility Urban Values (MUV), an EU Horizon 2020 project (2017–2020), that addresses the issue of behavioral change towards (more) sustainable mobility lifestyle in EU cities. The paper frames the MUV method through the combination of theories on collaborative urban planning and participatory design with a background rooted on governance of public participation, as the interplay between co-creation (thick participation) and co-design (thin participation). MUV participat…

Participatory methods Capacity building Loop learning
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Multi-PeV Signals from a New Astrophysical Neutrino Flux beyond the Glashow Resonance.

2016

The IceCube neutrino discovery was punctuated by three showers with $E_\nu$ ~ 1-2 PeV. Interest is intense in possible fluxes at higher energies, though a marked deficit of $E_\nu$ ~ 6 PeV Glashow resonance events implies a spectrum that is soft and/or cutoff below ~few PeV. However, IceCube recently reported a through-going track event depositing 2.6 $\pm$ 0.3 PeV. A muon depositing so much energy can imply $E_{\nu_\mu} \gtrsim$ 10 PeV. We show that extending the soft $E_\nu^{-2.6}$ spectral fit from TeV-PeV data is unlikely to yield such an event. Alternatively, a tau can deposit this much energy, though requiring $E_{\nu_\tau}$ ~10x higher. We find that either scenario hints at a new flu…

Particle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Astrophysics::High Energy Astrophysical PhenomenaGeneral Physics and AstronomyFOS: Physical sciencesCosmic ray01 natural sciencesHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)Flux (metallurgy)High Energy Physics - Phenomenology (hep-ph)0103 physical sciences010303 astronomy & astrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Muon010308 nuclear & particles physicsGlashow resonanceHigh Energy Physics::PhenomenologyAstrophysics::Instrumentation and Methods for AstrophysicsAstrophysics - Astrophysics of GalaxiesHigh Energy Physics - PhenomenologyAstrophysics of Galaxies (astro-ph.GA)High Energy Physics::ExperimentNeutrinoAstrophysics - High Energy Astrophysical PhenomenaEvent (particle physics)Energy (signal processing)Astrophysics - Cosmology and Nongalactic AstrophysicsPhysical review letters
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A test of electric charge conservation with Borexino

2015

Borexino is a liquid scintillation detector located deep underground at the Laboratori Nazionali del Gran Sasso (LNGS, Italy). Thanks to the unmatched radio-purity of the scintillator, and to the well understood detector response at low energy, a new limit on the stability of the electron for decay into a neutrino and a single mono-energetic photon was obtained. This new bound, tau > 6.6 10**28 yr at 90 % C.L., is two orders of magnitude better than the previous limit.

Particle physicsPhysics - Instrumentation and DetectorsOrders of magnitude (temperature)Physics::Instrumentation and DetectorsGeneral Physics and AstronomyFOS: Physical sciencesElectronScintillatorElectric chargeHigh Energy Physics - ExperimentNuclear physicsPhysics and Astronomy (all)High Energy Physics - Experiment (hep-ex)ddc:550Nuclear ExperimentBorexinoComputingMilieux_MISCELLANEOUSPhysics[PHYS]Physics [physics]Liquid scintillation countingDetectorAstrophysics::Instrumentation and Methods for AstrophysicsInstrumentation and Detectors (physics.ins-det)High Energy Physics::ExperimentNeutrino[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Axion search with BabyIAXO in view of IAXO

2020

Axions are a natural consequence of the Peccei-Quinn mechanism, the most compelling solution to the strong-CP problem. Similar axion-like particles (ALPs) also appear in a number of possible extensions of the Standard Model, notably in string theories. Both axions and ALPs are very well motivated candidates for Dark Matter, and in addition, they would be copiously produced at the sun's core. A relevant effort during the last decade has been the CAST experiment at CERN, the most sensitive axion helioscope to-date. The International Axion Observatory (IAXO) is a large-scale 4th generation helioscope. As its primary physics goal, IAXO will look for solar axions or ALPs with a signal to backgro…

Particle physicsPhysics - Instrumentation and Detectorssolar axion[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]experimental methodsDark matterFOS: Physical sciences7. Clean energyString (physics)Standard Modelaxion helioscopedesign [detector]International Axion Observatory (IAXO)ObservatoryPeccei-Quinn mechanismDark Matterdetector design[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Detectors and Experimental TechniquesAxionsun-tracking systemsphysics.ins-detactivity reportdetector: designPhysicsinstrumentationHelioscopeLarge Hadron Colliderdetectorsolar [axion]DESYInstrumentation and Detectors (physics.ins-det)[PHYS.ASTR.SR]Physics [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]IAXOmagnetopticsaxion: solar
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Search for Dark Matter Annihilations in the Sun with the 79-String IceCube Detector

2012

We have performed a search for muon neutrinos from dark matter annihilation in the center of the Sun with the 79-string configuration of the IceCube neutrino telescope. For the first time, the DeepCore sub-array is included in the analysis, lowering the energy threshold and extending the search to the austral summer. The 317 days of data collected between June 2010 and May 2011 are consistent with the expected background from atmospheric muons and neutrinos. Upper limits are therefore set on the dark matter annihilation rate, with conversions to limits on spin-dependent and spin-independent WIMP-proton cross-sections for WIMP masses in the range 20 - 5000 GeV. These are the most stringent s…

Particle physicsPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaDark matterFOS: Physical sciencesGeneral Physics and AstronomyCosmic rayddc:500.2MASSIVE PARTICLESAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics7. Clean energy01 natural sciencesIceCubeHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)LIMITSWIMP0103 physical sciencesddc:550010306 general physicsLight dark matterCANDIDATESHigh Energy Astrophysical Phenomena (astro-ph.HE)Physics010308 nuclear & particles physicsAstrophysics::Instrumentation and Methods for AstrophysicsCONSTRAINTSCAPTURENEUTRINOSPhysics and AstronomyNeutrino detector13. Climate actionWeakly interacting massive particlesHigh Energy Physics::ExperimentCryogenic Dark Matter SearchNeutrinoAstrophysics - High Energy Astrophysical PhenomenaPhysical Review Letters
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General Introduction to Computer Simulation Methods

1986

Computer simulation methods are now an established tool in many branches of science. The motivation for computer simulations of physical systems are manifold. One of the main motivations is that one eliminates approximations with computer simulations. Usually to treat a problem analytically (if it can be done at all) one needs to resort to some kind of approximation; for exam- ple a mean-field-type approximation. With a computer simulation we have the ability to study systems not yet tractable with analytical methods. The computer simulation approach allows one to study complex systems and gain insight into their behaviour. Indeed, the complexity can go far beyond the reach of present analy…

Partition function (quantum field theory)Theoretical computer sciencelawComputer sciencePhase spaceComplex systemPhysical systemManifold (fluid mechanics)Simulation methodslaw.invention
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Pasaku tulkošanas specifika. Brāļu Grimmu "Hansel und Gretel" un krievu tulkojums valodu kontrastīvā skatījumā

2016

Bakalaura darbs Pasaku tulkošanas specifika.Brāļu Grimmu "Hänsel und Gretel" un krievu tulkojums valodu kontrastīvā skatījumā rakstīts ar mērķi izpētīt literāra teksta specifiku un to tulkošanas problēmas, kā arī tulkojumu daudzveidību un dažādas uztveres pieejas. Darbā ir tuvāk aplūkotas tulkošanas tehniskās metodes, literāra teksta, proti, pasaku adaptācijas grūtības tulkošanas procesā, kas saistītas ar nacionālās kultūras atšķirībām un vācu autoru pasakas žanra īpatnībām. Ļoti plaši analizēti tulkojumu stilistisko atšķirību cēloņi. Pētījumā ir izmantota grāmatu formātā un internetā atrodamā nozares literatūra.

Pasaku specifikaValodniecībaTulkojuma metodesTranslations methodsAdaptācija
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Minimization of a rectangular patch using genetic algorithms

2002

In recent years, the miniaturization of antennas have become more and more important, especially in connection with subscriber transceivers for cellular systems. Due to the multiple scattering environments and the almost indefinable operating scenario, the crosspolarization characteristics of the antenna are less important, however its physical size is critical. The attempts to reduce the physical size of the antenna made in the past, used classical methods, such as embedding the antenna in a dielectric medium of a high permittivity, adding a resistive element in series with the antenna, etc., but little effort was invested in simply generating other geometries, which by their intrinsic pro…

Patch antennaEngineeringReconfigurable antennaDirectional antennabusiness.industryConformal antennaAntenna measurementAstrophysics::Instrumentation and Methods for AstrophysicsElectrical engineeringEvolved antennaMicrostripAntenna efficiencylaw.inventionMicrostrip antennaElectrical lengthlawElectronic engineeringAntenna (radio)businessOmnidirectional antennaComputer Science::Information TheoryIEEE Antennas and Propagation Society International Symposium. 2001 Digest. Held in conjunction with: USNC/URSI National Radio Science Meeting (Cat. No.01CH37229)
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