Search results for "Models"

showing 10 items of 8211 documents

Advanced models for nonlocal magneto-electro-elastic multilayered plates based on Reissner mixed variational theorem

2019

In the present work, nonlocal layer-wise models for the analysis of magneto-electro-elastic multilayered plates are formulated. An Eringen non-local continuum behaviour is assumed for the layers material; in particular, as usual in plate theories, partial in-plane nonlocality is assumed whereas local constitutive behaviour is considered in the thickness direction. The proposed plate theories are obtained via the Reissner Mixed Variational Theorem, assuming the generalized displacements and generalized out-of-plane stresses as primary variables, and expressing them as through-the-thickness expansions of suitably selected functions, considering the expansion order as a free parameter. In the …

PhysicsWork (thermodynamics)Classical mechanicsMechanics of MaterialsContinuum (topology)Advanced plate theories Nonlocal plate theories Carrera Unified Formulation Reissner Mixed Variational Theorem Smart plates Layerwise modelsMechanical EngineeringGeneral MathematicsGeneral Materials ScienceSettore ING-IND/04 - Costruzioni E Strutture AerospazialiMagnetoCivil and Structural EngineeringMechanics of Advanced Materials and Structures
researchProduct

The 2014 KIDA network for interstellar chemistry

2015

Chemical models used to study the chemical composition of the gas and the ices in the interstellar medium are based on a network of chemical reactions and associated rate coefficients. These reactions and rate coefficients are partially compiled from data in the literature, when available. We present in this paper kida.uva.2014, a new updated version of the kida.uva public gas-phase network first released in 2012. In addition to a description of the many specific updates, we illustrate changes in the predicted abundances of molecules for cold dense cloud conditions as compared with the results of the previous version of our network, kida.uva.2011.

Physics[PHYS]Physics [physics][ PHYS ] Physics [physics]Chemical models[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]FOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsChemical reactionAstrophysics - Astrophysics of GalaxiesInterstellar medium13. Climate actionSpace and Planetary ScienceChemical physics[ SDU.ASTR.CO ] Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Astrophysics of Galaxies (astro-ph.GA)MoleculeChemical compositionComputingMilieux_MISCELLANEOUS
researchProduct

Dissipative soliton resonance in a passively mode-locked fiber laser

2011

The phenomenon of dissipative soliton resonance (DSR) predicts that an increase of pulse energy by orders of magnitude can be obtained in laser oscillators. Here, we prove that DSR is achievable in a realistic ring laser cavity using nonlinear polarization evolution as the mode-locking mechanism, whose nonlinear transmission function is adjusted through a set of waveplates and a passive polarizer. The governing model accounts explicitly for the arbitrary orientations of the waveplates and the polarizer, as well as the gain saturation in the amplifying medium. It is shown that DSR is achievable with realistic laser settings. Our findings provide an excellent design tool for optimizing the mo…

Physicsbusiness.industryLasersNonlinear opticsRing laserModels TheoreticalPolarizerPolarization (waves)LaserAtomic and Molecular Physics and Opticslaw.inventionDissipative solitonNonlinear systemOpticslawFiber laserbusinessOptics Letters
researchProduct

About the link between the detailed description of transitions in an ion and the average-ion models

2009

We study the link which exists between microscopic (detailed) models for the evolution of the electronic configurations in a population of ions and the macroscopic (average ion) models. Rigorous asymptotics are presented in situations where they exist (large temperature; almost empty or almost full shells), and numerical simulations are presented.

Physicseducation.field_of_studyApplied MathematicsGeneral MathematicsAverage-ion modelsrigorous asymptoticsPopulationcomparison of solutions34C11Ion37M0535Q40Statistical physicsElectron configurationmicroscopic models82D10Link (knot theory)education
researchProduct

Population dynamics based on ladder bosonic operators

2021

Abstract We adopt an operatorial method, based on truncated bosons, to describe the dynamics of populations in a closed region with a non trivial topology. The main operator that includes the various mechanisms and interactions between the populations is the Hamiltonian, constructed with the density and transport operators. The whole evolution is derived from the Schrodinger equation, and the densities of the populations are retrieved from the normalized expected values of the density operators. We show that this approach is suitable for applications in very large domain, solving the computational issues that typically occur when using an Hamiltonian based on fermionic ladder operators.

Physicseducation.field_of_studyPopulation dynamicsApplied MathematicsPopulation02 engineering and technologyExpected value01 natural sciencesSchrödinger equationsymbols.namesake020303 mechanical engineering & transportsOperator (computer programming)Ladder operator0203 mechanical engineeringTrivial topologySchrödinger dynamicsModeling and Simulation0103 physical sciencessymbolsStatistical physicsOperatorial modelseducationHamiltonian (quantum mechanics)010301 acousticsBosonApplied Mathematical Modelling
researchProduct

Working group report: Neutrino physics

2009

This is the report of the neutrino physics working group at WHEPP-X. We summarize the problems selected and discussed at the workshop and the papers which have resulted subsequently.

Physicsline-experiment-simulatorParticle physicsGroup (mathematics)Solar neutrinooscillation experimentsGeneral Physics and AstronomyNeutrino Mass ModelsSolar neutrino problemPhysics and Astronomy(all)Oscillation ExperimentsNeutrino OscillationsNuclear physicsLeptogenesisLine-Experiment-SimulatorLeptogenesisPhysical Sciences and MathematicsMeasurements of neutrino speedNeutrinoLepton Flavour ViolationNeutrino oscillation
researchProduct

Collective rotation of an oblate nucleus at very high spin

2019

International audience; A sequence of nine almost equidistant quadrupole transitions is observed in Nd137. The sequence represents an extremely regular rotational band that extends to a spin of about 75/2 and an excitation energy of ≈4.5MeV above yrast. Cranked mean-field calculations of the Nilsson-Strutinsky type suggest an oblate shape for the band. They reproduce the observed I(I+1) dependence of the rotational energy whereas predicting a pronounced decrease in the deformation, which is the hallmark of antimagnetic rotation.

Physicsnuclear spinta114010308 nuclear & particles physicsNuclear Theorycollective models[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]RotationNuclear Structure01 natural sciencesmedicine.anatomical_structureelectromagnetic transitions0103 physical sciencesQuadrupoleOblate spheroidmedicineEquidistantcollective levelsAtomic physics010306 general physicsSpin (physics)ydinfysiikkaNucleusSequence (medicine)
researchProduct

Filaments in observed and mock galaxy catalogues

2010

Context. The main feature of the spatial large-scale galaxy distribution is an intricate network of galaxy filaments. Although many attempts have been made to quantify this network, there is no unique and satisfactory recipe for that yet. Aims. The present paper compares the filaments in the real data and in the numerical models, to see if our best models reproduce statistically the filamentary network of galaxies. Methods. We apply an object point process with interactions (the Bisous process) to trace and describe the filamentary network both in the observed samples (the 2dFGRS catalogue) and in the numerical models that have been prepared to mimic the data.We compare the networks. Result…

Physicsstatistical [Methods]Cosmology and Nongalactic Astrophysics (astro-ph.CO):ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::Otras [UNESCO]FOS: Physical scienceslarge [Cosmology]Astronomy and AstrophysicsContext (language use)Scale structure of UniverseAstrophysicsNumerical models:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]Cosmology : large; Scale structure of Universe; Methods : data analysis; Methods : statisticalGalaxyObject pointSpace and Planetary ScienceUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::OtrasUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogoniadata analysis [Methods]Astrophysics - Cosmology and Nongalactic Astrophysics
researchProduct

Elasticity of Poissonian fiber networks

2000

An effective-medium model is introduced for the elasticity of two-dimensional random fiber networks. These networks are commonly used as basic models of heterogeneous fibrous structures such as paper. Using the exact Poissonian statistics to describe the microscopic geometry of the network, the tensile modulus can be expressed by a single-parameter function. This parameter depends on the network density and fiber dimensions, which relate the macroscopic modulus to the relative importance of axial and bending deformations of the fibers. The model agrees well with simulation results and experimental findings. We also discuss the possible generalizations of the model. Peer reviewed

Physicssymbols.namesakePhysicssymbolsModulusYoung's modulusStatistical physicseffective-medium modelselastic propertiesElasticity (economics)Network densityinhomogeneous materials
researchProduct

Neutron halos in the excited states of B12

2018

The differential cross sections of the $^{11}\mathrm{B}(d,p)\phantom{\rule{0.16em}{0ex}}^{12}\mathrm{B}$ reaction leading to formation of the ${1}^{+}$ ground state and the 0.95-MeV ${2}^{+}$, 1.67-MeV ${2}^{\ensuremath{-}}$, 2.62-MeV ${1}^{\ensuremath{-}}$, 2.72-MeV ${0}^{+}$, and 3.39-MeV ${3}^{\ensuremath{-}}$ excited states of $^{12}\mathrm{B}$ are measured at ${E}_{d}$ = 21.5 MeV. The analysis of the data is carried out within the coupled-reaction-channels method for the direct neutron transfer and the Hauser-Feshbach formalism of the statistical compound-nucleus model. The spectroscopic factors, asymptotic normalization coefficients, and rms radii of the last neutron in all states stu…

Physicsta114electromagnetic moments010308 nuclear & particles physicsNuclear Theorynucleon distributiondirect reactions01 natural sciencescluster modelsExcited state0103 physical sciencesbooritransfer reactionsPhysics::Accelerator PhysicsNeutronspectroscopic factorsHaloAtomic physicsydinfysiikkaNuclear Experiment010306 general physicsGround statePhysical Review C
researchProduct