Search results for "Equations"

showing 10 items of 955 documents

Determination of the stochastic evolution equation from noisy experimental data

2003

We have determined the coefficients of the Kardar-Parisi-Zhang equation as functions of coarse graining, which best describe the time evolution and spatial behavior observed for slow-combustion fronts in sheets of paper and magnetic flux fronts in a thin-film high-Tc superconductor. Reconstruction of the relevant equation of motion and its coefficients was mainly based on the inverse method proposed by Lam and Sander [Phys. Rev. Lett. 71, 561 (1993)]. The coefficient of the nonlinear term was also determined from the local slope-dependence of the front velocity.

PhysicsNonlinear systemStochastic processCondensed Matter::Statistical MechanicsFront velocityTime evolutionEquations of motionStatistical physicsInverse problemCondensed Matter PhysicsMagnetic fluxElectronic Optical and Magnetic MaterialsKardar–Parisi–Zhang equationThe European Physical Journal B - Condensed Matter
researchProduct

Ansatz-independent solution of a soliton in a strong dispersion-management system

2000

We introduce a theoretical approach to the study of propagation in systems with periodic strong-management dispersion. Our approach does not assume any ansatz about the form of the solution nor does it make use of any average procedure. We find an explicit solution for the pulse evolution in the fast dynamics regime (distances smaller than the dispersion period). We also establish the equation of motion governing the slow dynamics of an arbitrary pulse and prove that the pulse evolution is nonlinear and Hamiltonian. We solve this equation and find that a nonlinear solitonlike solution occurs self-consistently in the form of an asymptotic stationary eigenfunction of the Hamiltonian.

PhysicsNonlinear systemsymbols.namesakeClassical mechanicsWave propagationsymbolsEquations of motionRadiowave propagationEigenfunctionHamiltonian (quantum mechanics)AnsatzPhysical review. E, Statistical physics, plasmas, fluids, and related interdisciplinary topics
researchProduct

IMEX Finite Volume Methods for Cloud Simulation

2017

We present new implicit-explicit (IMEX) finite volume schemes for numerical simulation of cloud dynamics. We use weakly compressible equations to describe fluid dynamics and a system of advection-diffusion-reaction equations to model cloud dynamics. In order to efficiently resolve slow dynamics we split the whole nonlinear system in a stiff linear part governing the acoustic and gravitational waves as well as diffusive effects and a non-stiff nonlinear part that models nonlinear advection effects. We use a stiffly accurate second order IMEX scheme for time discretization to approximate the stiff linear operator implicitly and the non-stiff nonlinear operator explicitly. Fast microscale clou…

PhysicsNonlinear systemsymbols.namesakeFinite volume methodComputer simulationDiscretizationCompressibilityFluid dynamicssymbolsApplied mathematicsNavier–Stokes equationsEuler equations
researchProduct

Gravitational waves in dynamical spacetimes with matter content in the fully constrained formulation

2012

The Fully Constrained Formulation (FCF) of General Relativity is a novel framework introduced as an alternative to the hyperbolic formulations traditionally used in numerical relativity. The FCF equations form a hybrid elliptic-hyperbolic system of equations including explicitly the constraints. We present an implicit-explicit numerical algorithm to solve the hyperbolic part, whereas the elliptic sector shares the form and properties with the well known Conformally Flat Condition (CFC) approximation. We show the stability andconvergence properties of the numerical scheme with numerical simulations of vacuum solutions. We have performed the first numerical evolutions of the coupled system of…

PhysicsNuclear and High Energy Physics010308 nuclear & particles physicsGeneral relativityGravitational waveRotational symmetryFOS: Physical sciencesSpherical coordinate systemGeneral Relativity and Quantum Cosmology (gr-qc)Neutron-star oscillationSystem of linear equations01 natural sciencesGeneral Relativity and Quantum CosmologyNeutron starNumerical relativityClassical mechanicsAstrophysics - Solar and Stellar Astrophysics0103 physical sciences010306 general physicsSolar and Stellar Astrophysics (astro-ph.SR)Physical Review D
researchProduct

Real-time calibration of the A4 electromagnetic lead fluoride (PbF2) calorimeter

2011

Abstract Sufficient energy resolution is the key issue for the calorimetry in particle and nuclear physics. The calorimeter of the A4 parity violation experiment at MAMI is a segmented calorimeter where the energy of an event is determined by summing the signals of neighboring channels. In this case, the precise matching of the individual modules is crucial to obtain a good energy resolution. We have developed a calibration procedure for our total absorbing electromagnetic calorimeter which consists of 1022 lead fluoride (PbF 2 ) crystals. This procedure reconstructs the single-module contributions to the events by solving a linear system of equations, involving the inversion of a 1022×1022…

PhysicsNuclear and High Energy Physics010308 nuclear & particles physicsPhysics::Instrumentation and DetectorsLead fluorideCalorimetry[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]System of linear equations7. Clean energy01 natural sciencesParticle detectorComputational physicsCalorimeterNuclear physicsElectromagnetic calorimeter0103 physical sciencesMeasuring instrument010306 general physicsInstrumentationBeam (structure)
researchProduct

A Lemaitre-Tolman-Bondi cosmological wormhole

2010

We present a new analytical solution of the Einstein field equations describing a wormhole shell of zero thickness joining two Lema{\i}tre-Tolman-Bondi universes, with no radial accretion. The material on the shell satisfies the energy conditions and, at late times, the shell becomes comoving with the dust-dominated cosmic substratum.

PhysicsNuclear and High Energy PhysicsAccretion (meteorology)010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical PhenomenaShell (structure)Zero (complex analysis)FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Mathematical Physics (math-ph)Astrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesCosmologyGeneral Relativity and Quantum CosmologyStarsGeneral Relativity and Quantum CosmologyClassical mechanics0103 physical sciencesEinstein field equationsAstrophysics::Earth and Planetary AstrophysicsWormholeField equation010303 astronomy & astrophysicsMathematical Physics
researchProduct

Microscopic description of α-like resonances

2000

A description of $\ensuremath{\alpha}$-like resonances is given in terms of single-particle states including narrow Gamow resonances in continuum. The equations of motion are derived within the multistep shell-model approach; the lowest collective two-particle eigenmodes are used as building blocks for the four-particle states. A good agreement with the low-lying states in ${}^{212}\mathrm{Po}$ is obtained. A new technique to estimate the $\ensuremath{\alpha}$-particle formation amplitude for any multipolarity is proposed. The spectroscopic factor of the $\ensuremath{\alpha}$-decay between ground states is reproduced, but the total width is by two orders of magnitude less than the experimen…

PhysicsNuclear and High Energy PhysicsAmplitudeMolecular geometryScatteringEquations of motionContinuum (set theory)Alpha decayMicroscopic descriptionAtomic physicsOrder of magnitudePhysical Review C
researchProduct

Microscopic description of low-lying two-phonon states: Electromagnetic transitions

2003

Microscopic description of low-lying two-phonon states in even-even nuclei is introduced. The main building blocks are the quasiparticle random-phase approximation (QRPA) phonons. A realistic microscopic nuclear Hamiltonian, based on the Bonn one-boson-exchange potential, is diagonalized in a basis containing one-phonon and two-phonon components, coupled to a given angular momentum and parity. The QRPA equations are directly used in deriving the equations of motion for the two-phonon states. The Pauli principle is taken into account by diagonalizing the metric matrix and discarding the zero-norm states. The electromagnetic transition matrix elements are derived in terms of the metric matrix…

PhysicsNuclear and High Energy PhysicsAngular momentumPhononNuclear TheoryStochastic matrixEquations of motionParity (physics)symbols.namesakePauli exclusion principleQuantum mechanicssymbolsQuasiparticleHamiltonian (quantum mechanics)Physical Review C
researchProduct

A model study of Hartree-Fock and Linear Response in coordinate space

1979

A fast procedure for spherical Hartree-Fock is obtained by coordinate space representation and a modification of gradient iteration. Along similar lines, the corresponding Linear Response equations are derived and solved, in order to achieve a fully consistent treatment. The Linear Response equations are applied to a change in particle numbers, i.e. to the description of isotopic differences. In a model study we look for their physical and numerical properties, i.e. linearity of the response, numerical stability and consistency requirements for the Hartree-Fock basis.

PhysicsNuclear and High Energy PhysicsBasis (linear algebra)Consistency (statistics)Mathematical analysisHartree–Fock methodLinearityPhysics::Atomic PhysicsCoordinate spaceSystem of linear equationsRepresentation (mathematics)Numerical stabilityZeitschrift f�r Physik A Atoms and Nuclei
researchProduct

Low-lying collective states inRu98–106isotopes studied using a microscopic anharmonic vibrator approach

2003

Anharmonic features of the low-lying collective states in the $^{98--106}\mathrm{Ru}$ isotopes have been investigated systematically by using the microscopic anharmonic vibrator approach (MAVA). MAVA is based on a realistic microscopic $G$-matrix Hamiltonian, only slightly renormalized in the adopted large realistic single-particle spaces. This Hamiltonian is used to derive equations of motion for the mixing of one- and two-phonon degrees of freedom starting from collective phonons of the quasiparticle random-phase approximation. Analysis of the level energies and the electric quadrupole decays of the two-phonon type of states indicates that $^{100}\mathrm{Ru}$ can be interpreted as being a…

PhysicsNuclear and High Energy PhysicsCondensed matter physicsPhononAnharmonicityDegrees of freedom (physics and chemistry)Equations of motionType (model theory)symbols.namesakeQuadrupoleQuasiparticlesymbolsAtomic physicsHamiltonian (quantum mechanics)Physical Review C
researchProduct