Search results for "DOMAIN"

showing 10 items of 2485 documents

Meson exchange currents in kaon scattering on the lightest nuclei

1997

The K^+ scattering on the lightest nuclei, d, 3He and 4He is studied in the framework of multiple scattering theory. Effects from MEC tied to the K^+N-->KNpi reaction are evaluated. We found that at momentum transfers Q^2<0.5 (GeV/c)^2 contributions from MEC are much smaller than kaon rescattering corrections. This makes the conventional multiple scattering picture a reliable tool to study these reactions in this kinematical domain and to extract the K^+n scattering amplitude from the K^+d data. At larger transferred momentum MEC can become more relevant.

PhysicsNuclear and High Energy PhysicsParticle physicsNuclear TheoryMesonScatteringNuclear TheoryMomentum transferFOS: Physical sciencesFísicaNuclear Theory (nucl-th)Nuclear physicsMomentumScattering amplitudeDomain (ring theory)Nuclear forceNuclear ExperimentNuclear theoryPhysical Review C
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Search for heavy charged scalars in Z$^0$ Decays

1990

Using a sample of Z0's corresponding to about 12 000 events, we have searched for the production of charged scalars, primarily charged Higgs particles, decaying into c̄scs̄, τν+jets, and τντν. The average detection efficiency is 20%. No candidate was found in the leptonic modes. Masses in the range up to 30-36 GeV/c2 are excluded, extending the mass domain covered by previous e+e- machines.

PhysicsNuclear and High Energy PhysicsParticle physicsRange (particle radiation)Internet010308 nuclear & particles physicsElectron–positron annihilation01 natural sciencesteachingNuclear physics0103 physical sciencesDomain (ring theory)course packsPhysique des particules élémentairesHiggs bosonComputingMilieux_COMPUTERSANDEDUCATIONeditors[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]High Energy Physics::ExperimentFísica nuclear010306 general physicsParticle Physics - Experiment
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Production of transverse energy from minijets in next-to-leading order perturbative QCD

2000

We compute in next-to-leading order (NLO) perturbative QCD the transverse energy carried into the central rapidity unit of hadron or nuclear collisions by the partons freed in the few-GeV subcollisions. The formulation is based on a rapidity window and a measurement function of a new type. The behaviour of the NLO results as a function of the minimum transverse momentum and as a function of the scale choice is studied. The NLO results are found to be stable relative to the leading-order ones even in the few-GeV domain.

PhysicsNuclear and High Energy PhysicsParticle physicsScale (ratio)High Energy Physics::PhenomenologyHadronFOS: Physical sciencesPerturbative QCDPartonFunction (mathematics)High Energy Physics - PhenomenologyTransverse planeHigh Energy Physics - Phenomenology (hep-ph)Domain (ring theory)High Energy Physics::ExperimentRapidityNuclear ExperimentParticle Physics - PhenomenologyPhysics Letters B
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Fracture processes studied in CRESST

2005

In the early stages of running of the CRESST dark matter search with sapphire crystals as detectors, an unexpectedly high rate of signal pulses appeared. Their origin was finally traced to fracture events in the sapphire due to the very tight clamping of the detectors. During extensive runs the energy and time of each event was recorded, providing large data sets for such phenomena. We believe this is the first time that the energy release in fracture has been accurately measured on a microscopic event-by-event basis. The energy distributions appear to follow a power law, dN/dE proportional to E-beta, similar to the Gutenberg-Richter power law for earthquake magnitudes, and after appropriat…

PhysicsNuclear and High Energy Physics[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]AutocorrelationDark matter01 natural sciencesPower law010305 fluids & plasmasComputational physicsNuclear physics[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]81.05.-t; 05.40; 07.90.+c; 29.40.-v0103 physical sciencesFracture (geology)Time domain[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsInstrumentationEvent (particle physics)Energy (signal processing)Noise (radio)
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Electrical analogous in viscoelasticity

2014

In this paper, electrical analogous models of fractional hereditary materials are introduced. Based on recent works by the authors, mechanical models of materials viscoelasticity behavior are firstly approached by using fractional mathematical operators. Viscoelastic models have elastic and viscous components which are obtained by combining springs and dashpots. Various arrangements of these elements can be used, and all of these viscoelastic models can be equivalently modeled as electrical circuits, where the spring and dashpot are analogous to the capacitance and resistance, respectively. The proposed models are validated by using modal analysis. Moreover, a comparison with numerical expe…

PhysicsNumerical AnalysisEigenvalues analysiEigenvalues analysis Fractional calculus Fractional capacitor Viscoelastic modelsApplied MathematicsModal analysisMathematical analysisFinite-difference time-domain methodViscoelastic modelFractional calculuDashpotViscoelasticityFractional calculuslaw.inventionMathematical OperatorsFractional capacitorSettore ING-IND/31 - ElettrotecnicaSettore MAT/08 - Analisi NumericaSpring (device)lawModeling and SimulationElectrical networkCalculusSettore ICAR/08 - Scienza Delle Costruzioni
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Pulsating B and Be Stars in the Magellanic Clouds

2010

Stellar pulsations in main-sequence B-type stars are driven by the κ-mechanism due to the Fe-group opacity bump. The current models do not predict the presence of instability strips in the B spectral domain at very low metallicities. As the metallicity of the Magellanic Clouds (MC) has been measured to be around Z = 0. 002 for the Small Magellanic Cloud (SMC) and Z = 0. 007 for the Large Magellanic Cloud (LMC), they constitute a very suitable objects to test these predictions. The aim of this work is to investigate the existence of B-type pulsators at low metallicities, searching for short-term periodic variability in a large sample of B and Be stars from the MC with accurately determined f…

PhysicsOpacityAstrophysics::High Energy Astrophysical PhenomenaMetallicitySpectral domainAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsInstabilityLarge sampleStars13. Climate actionAstrophysics::Solar and Stellar AstrophysicsSmall Magellanic CloudLarge Magellanic CloudAstrophysics::Galaxy Astrophysics
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Spectral incoherent solitons: a localized soliton behavior in the frequency domain

2008

We show both theoretically and experimentally in an optical fiber system that a noninstantaneous nonlinear environment supports the existence of spectral incoherent solitons. Contrary to conventional solitons, spectral incoherent solitons do not exhibit a confinement in the spatiotemporal domain, but exclusively in the frequency domain. The theory reveals that the causality condition inherent to the nonlinear response function is the key property underlying the existence of spectral incoherent solitons. These solitons constitute nonequilibrium stable states of the incoherent field and are shown to be robust with respect to binary collisions.

PhysicsOptical fiberField (physics)General Physics and AstronomyNon-equilibrium thermodynamics01 natural scienceslaw.invention010309 opticsCausality (physics)Nonlinear systemNonlinear Sciences::Exactly Solvable and Integrable SystemslawQuantum mechanicsFrequency domain0103 physical sciencesDomain (ring theory)Soliton010306 general physicsNonlinear Sciences::Pattern Formation and SolitonsComputingMilieux_MISCELLANEOUS
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Analysis method for detecting topological defect dark matter with a global magnetometer network

2019

Abstract The Global Network of Optical Magnetometers for Exotic physics searches (GNOME) is a network of time-synchronized, geographically separated, optically pumped atomic magnetometers that is being used to search for correlated transient signals heralding exotic physics. GNOME is sensitive to exotic couplings of atomic spins to certain classes of dark matter candidates, such as axions. This work presents a data analysis procedure to search for axion dark matter in the form of topological defects: specifically, walls separating domains of discrete degenerate vacua in the axion field. An axion domain wall crossing the Earth creates a distinctive signal pattern in the network that can be d…

PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Field (physics)Spins010308 nuclear & particles physicsMagnetometerDark matterFOS: Physical sciencesAstronomy and Astrophysics01 natural sciencesTopological defectlaw.inventionDomain wall (string theory)Space and Planetary Sciencelaw0103 physical sciencesAstrophysics - Instrumentation and Methods for Astrophysics010303 astronomy & astrophysicsAxionInstrumentation and Methods for Astrophysics (astro-ph.IM)GnomeAstrophysics - Cosmology and Nongalactic Astrophysics
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Spontaneous Breaking of Lepton Number and Cosmological Domain Wall Problem

2019

We show that if global lepton number symmetry is spontaneously broken in a post inflation epoch, then it can lead to the formation of cosmological domain walls. This happens in the well-known "Majoron paradigm" for neutrino mass generation. We propose some realistic examples which allow spontaneous lepton number breaking to be safe from such domain walls.

PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Mass generationHigh Energy Physics::PhenomenologyGeneral Physics and AstronomyFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesLepton numberSymmetry (physics)High Energy Physics - PhenomenologyDomain wall (string theory)High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesDomain (ring theory)High Energy Physics::ExperimentNeutrino010306 general physicsAstrophysics - Cosmology and Nongalactic Astrophysics
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An invisible axion model with controlled FCNCs at tree level

2015

We derive the necessary conditions to build a class of invisible axion models with Flavor Changing Neutral Currents at tree-level controlled by the fermion mixing matrices and present an explicit model implementation. A horizontal Peccei-Quinn symmetry provides a solution to the strong CP problem via the Peccei-Quinn mechanism and predicts a cold dark mater candidate, the invisible axion or familon. The smallness of active neutrino masses can be explained via a type I seesaw mechanism, providing a dynamical origin for the heavy seesaw scale. The possibility to avoid the domain wall problem stands as one of the most interesting features of the type of models considered. Experimental limits r…

PhysicsParticle physicsNuclear and High Energy PhysicsPhysics::Instrumentation and DetectorsDark matterHigh Energy Physics::PhenomenologyFOS: Physical scienceslcsh:QC1-999Domain wall (string theory)High Energy Physics - PhenomenologySeesaw mechanismHigh Energy Physics - Phenomenology (hep-ph)Seesaw molecular geometryStrong CP problemNeutrinoAxionMixing (physics)lcsh:PhysicsPhysics Letters B
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