Search results for "Boundary value problem"

showing 10 items of 551 documents

Size effects of small-scale beams in bending addressed with a strain-difference based nonlocal elasticity theory

2019

Abstract A strain-difference based nonlocal elasticity model devised by the authors elsewhere (Polizzotto et al., Int. J. Solids Struct. 25 (2006) 308–333) is applied to small-scale homogeneous beam models in bending under static loads in the purpose to describe the inherent size effects. With this theory —belonging to the strain-integral nonlocal model family, but exempt from anomalies typical of the Eringen nonlocal theory— the relevant beam problem is reduced to a set of three mutually independent Fredholm integral equations of the second kind (each independent of the beam’s ordinary boundary conditions, only one depends on the given load), which can be routinely solved numerically. Appl…

PhysicsMechanical EngineeringMathematical analysis02 engineering and technologyStrain differenceElasticity (physics)021001 nanoscience & nanotechnologyCondensed Matter PhysicsStrain gradientIntegral equation020303 mechanical engineering & transports0203 mechanical engineeringMechanics of MaterialsHomogeneousGeneral Materials ScienceBoundary value problem0210 nano-technologyBeam (structure)Civil and Structural EngineeringInternational Journal of Mechanical Sciences
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Study of the anomalous magnetic moment of the muon computed from the Adler function

2014

We compute the Adler function on the lattice from vacuum polarization data with twisted boundary conditions using numerical derivatives. The study is based on CLS ensembles with two flavours of $O(a)$ improved Wilson fermions. We extrapolate the lattice data for the Adler function to the continuum limit and to the physical pion mass and analyze its dependence on the momentum transfer. We discuss the application of this method to the extraction of the $u,d$ contribution to $a_\mu^{\mathrm{HLO}}$.

PhysicsMuonAnomalous magnetic dipole moment010308 nuclear & particles physicsHigh Energy Physics::LatticeMomentum transferHigh Energy Physics - Lattice (hep-lat)FOS: Physical scienceshep-latFermion01 natural sciencesPionHigh Energy Physics - LatticeQuantum electrodynamicsLattice (order)0103 physical sciencesBoundary value problemVacuum polarization010306 general physicsPoS(LATTICE2014)162
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Linear and non-linear flow mode in Pb–Pb collisions at sNN=2.76 TeV

2017

The second and the third order anisotropic flow, V2 and V3, are mostly determined by the corresponding initial spatial anisotropy coefficients, e2 and e3, in the initial density distribution. In addition to their dependence on the same order initial anisotropy coefficient, higher order anisotropic flow, Vn (n > 3), can also have a significant contribution from lower order initial anisotropy coefficients, which leads to mode-coupling effects. In this Letter we investigate the linear and non-linear modes in higher order anisotropic flow Vn for n = 4, 5, 6 with the ALICE detector at the Large Hadron Collider. The measurements are done for particles in the pseudorapidity range |η| < 0.8 and the…

PhysicsNuclear and High Energy Physics010308 nuclear & particles physicsHadron01 natural sciencesNuclear physicsThird orderViscosityFlow (mathematics)Pseudorapidity0103 physical sciencesRapidityBoundary value problem010306 general physicsAnisotropyPhysics Letters B
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Fully relativistic non-linear cosmological evolution in spherical symmetry using the BSSN formalism

2014

We present a fully relativistic numerical method for the study of cosmological problems using the Baumgarte-Shapiro-Shibata-Nakamura formalism on a dynamical Friedmann-Lema\^itre-Robertson-Walker background. This has many potential applications including the study of the growth of structures beyond the linear regime. We present one such application by reproducing the Lema\^itre-Tolman-Bondi solution for the collapse of pressureless matter with arbitrary lapse function. The regular and smooth numerical solution at the center of coordinates proceeds in a natural way by relying on the Partially Implicit Runge-Kutta algorithm described in Montero and Cordero-Carri\'on [arXiv:1211.5930]. We gene…

PhysicsNuclear and High Energy Physics010308 nuclear & particles physicsNumerical analysisFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyCosmologyGeneral Relativity and Quantum CosmologyNonlinear systemTheoretical physicsNumerical relativityDe Sitter universe0103 physical sciencesRadiative transferCircular symmetryBoundary value problemAstrophysics - Instrumentation and Methods for Astrophysics010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Physical Review D
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String fields as limit of functions and surface terms in string field theory

1989

We consider the String Field Theory proposed by Witten in the discretized approach, where the string is considered as the limit N → ∞ of a collection of N points. In this picture the string functional is the limit of a succession of functions of an increasing number of variables; an object with some resemblances to distributions. Attention is drawn to the fact that the convergence is not of the uniform kind, and that therefore exchanges of limits, sums and integral signs can cause problems, and be ill defined. In this context we discuss some surface terms found by Woodard, which arise in integrations by parts, and argue that they depend crucially on the choice of the successions of functio…

PhysicsNuclear and High Energy PhysicsCompactification (physics)DiscretizationFísicaAstronomy and AstrophysicsString field theoryTopological string theoryRelationship between string theory and quantum field theoryAtomic and Molecular Physics and OpticsNon-critical string theoryTheoretical physicsQuantum mechanicsString cosmologyBoundary value problem
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Mathematical Issues in a Fully-Constrained Formulation of Einstein Equations

2008

Bonazzola, Gourgoulhon, Grandcl\'ement, and Novak [Phys. Rev. D {\bf 70}, 104007 (2004)] proposed a new formulation for 3+1 numerical relativity. Einstein equations result, according to that formalism, in a coupled elliptic-hyperbolic system. We have carried out a preliminary analysis of the mathematical structure of that system, in particular focusing on the equations governing the evolution for the deviation of a conformal metric from a flat fiducial one. The choice of a Dirac's gauge for the spatial coordinates guarantees the mathematical characterization of that system as a (strongly) hyperbolic system of conservation laws. In the presence of boundaries, this characterization also depen…

PhysicsNuclear and High Energy PhysicsConservation lawPartial differential equationSpace timeMathematical analysisFOS: Physical sciencesConformal mapGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum CosmologyNumerical relativityClassical mechanicsEinstein field equationsBoundary value problemMathematical structure
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Trapping Horizons as inner boundary conditions for black hole spacetimes

2007

We present a set of inner boundary conditions for the numerical construction of dynamical black hole space-times, when employing a 3+1 constrained evolution scheme and an excision technique. These inner boundary conditions are heuristically motivated by the dynamical trapping horizon framework and are enforced in an elliptic subsystem of the full Einstein equation. In the stationary limit they reduce to existing isolated horizon boundary conditions. A characteristic analysis completes the discussion of inner boundary conditions for the radiative modes.

PhysicsNuclear and High Energy PhysicsEvent horizonWhite holeBoundary conformal field theoryFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum CosmologyGeneral Relativity and Quantum CosmologyClassical mechanicsRotating black holeNonsingular black hole modelsExtremal black holeFree boundary problemBoundary value problem
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Effect of three-body cluster on the healing properties of the Jastrow Correlation function

1973

A variational equation for the Jastrow Correlation function is derived from the energy functional expanded up to three-body cluster terms. The asymptotic behaviour of this nonlinear equation is studied. The solutions show a healing at least of the type cos(tαr)/r2. The influence of higher cluster contributions is studied. Finally, it is discussed, how one can reduce the many-body cluster contributions to healing conditions to be used in the two-body cluster treatment.

PhysicsNuclear and High Energy PhysicsNonlinear systemCorrelation functionVariational equationQuantum electrodynamicsCluster (physics)Boundary value problemStatistical physicsEnergy functionalZeitschrift für Physik A Hadrons and nuclei
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Event-by-event distributions of azimuthal asymmetries in ultrarelativistic heavy-ion collisions

2012

Relativistic dissipative fluid dynamics is a common tool to describe the space-time evolution of the strongly interacting matter created in ultrarelativistic heavy-ion collisions. For a proper comparison to experimental data, fluid-dynamical calculations have to be performed on an event-by-event basis. Therefore, fluid dynamics should be able to reproduce, not only the event-averaged momentum anisotropies, $$, but also their distributions. In this paper, we investigate the event-by-event distributions of the initial-state and momentum anisotropies $\epsilon_n$ and $v_n$, and their correlations. We demonstrate that the event-by-event distributions of relative $v_n$ fluctuations are almost eq…

PhysicsNuclear and High Energy PhysicsNuclear Theoryta114FOS: Physical sciencesNuclear Theory (nucl-th)MomentumViscosityQuantum electrodynamicsQuark–gluon plasmaDissipative systemFluid dynamicsBoundary value problemAnisotropyEvent (particle physics)Physical Review C
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FlexibleSUSY - a meta spectrum generator for supersymmetric models

2016

FlexibleSUSY is a software package that takes as input descriptions of (non-)minimal supersymmetric models written in Wolfram/Mathematica and generates a set of spectrum generator libraries and executables, with the aid of SARAH. The design goals are precision, reliability, modularity, speed, and readability of the code. The boundary conditions are independent C++ objects that are plugged into the boundary value problem solver together with the model objects. This clean separation makes it easy to adapt the generated code for individual projects. The current status of the interface and implementation is sketched.

PhysicsNuclear and High Energy PhysicsParticle physicsModularity (networks)010308 nuclear & particles physicsInterface (Java)renormalization group equationsFOS: Physical sciencescomputer.file_formatSolver01 natural sciencesSet (abstract data type)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesCode (cryptography)Boundary value problemExecutablesupersymmetry010306 general physicscomputersparticleGenerator (mathematics)Higgs
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