Search results for " MoM"

showing 10 items of 2281 documents

A second strain gradient elasticity theory with second velocity gradient inertia – Part II: Dynamic behavior

2013

Abstract This paper is the sequel of a companion Part I paper devoted to the constitutive equations and to the quasi-static behavior of a second strain gradient material model with second velocity gradient inertia. In the present Part II paper, a multi-cell homogenization procedure (developed in the Part I paper) is applied to a nonhomogeneous body modelled as a simple material cell system, in conjunction with the principle of virtual work (PVW) for inertial actions (i.e. momenta and inertia forces), which at the macro-scale level takes on the typical format as for a second velocity gradient inertia material model. The latter (macro-scale) PVW is used to determine the equilibrium equations …

Angular momentummedia_common.quotation_subjectRotary inertiaPolhodeContinuum thermodynamicsInertiaMoment of inertia factorsymbols.namesakeMaterials Science(all)Modelling and SimulationGeneral Materials ScienceEuler's equationsmedia_commonMathematicsWave propagationApplied MathematicsMechanical EngineeringMathematical analysisMoment of inertiaCondensed Matter PhysicsRigid body dynamicsDynamicsGradient elasticityClassical mechanicsHigher order inertiaMechanics of MaterialsModeling and SimulationsymbolsInternational Journal of Solids and Structures
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A gradient elasticity theory for second-grade materials and higher order inertia

2012

Abstract Second-grade elastic materials featured by a free energy depending on the strain and the strain gradient, and a kinetic energy depending on the velocity and the velocity gradient, are addressed. An inertial energy balance principle and a virtual work principle for inertial actions are envisioned to enrich the set of traditional theoretical tools of thermodynamics and continuum mechanics. The state variables include the body momentum and the surface momentum, related to the velocity in a nonstandard way, as well as the concomitant mass-accelerations and inertial forces, which do intervene into the motion equations and into the force boundary conditions. The boundary traction is the …

Angular momentummedia_common.quotation_subjectTraction (engineering)Continuum thermodynamicsInertiaMaterials Science(all)Modelling and SimulationWave dispersionGeneral Materials ScienceVirtual workBoundary value problemmedia_commonMathematicsContinuum mechanicsForce densityMechanical EngineeringApplied MathematicsMathematical analysisEquations of motionCondensed Matter PhysicsDynamicsGradient elasticityClassical mechanicsHigher order inertiaMechanics of MaterialsModeling and SimulationInternational Journal of Solids and Structures
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Local Berry curvature signatures in dichroic angle-resolved photoelectron spectroscopy from two-dimensional materials

2020

Orbital polarization and Berry curvature signatures are mapped out by circular dichroism in angle-resolved photoemission.

Angular momentumtopologyAb initioPhysics::OpticsPosition and momentum spaceAngle-resolved photoemission spectroscopy02 engineering and technologyDichroic glass01 natural sciencesSettore FIS/03 - Fisica Della MateriaCondensed Matter::Materials ScienceQuantum mechanicsCondensed Matter::Superconductivity0103 physical sciences010306 general physicsResearch ArticlesPhysicsMultidisciplinaryPhysicsSciAdv r-articles021001 nanoscience & nanotechnologyARPESCondensed Matter PhysicsDensity functional theoryCondensed Matter::Strongly Correlated ElectronsBerry connection and curvatureMathematics::Differential Geometry0210 nano-technologyGround stateResearch Article
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Electromagnetic Sensitivity Analysis and Shape Optimization Using Method of Moments and Automatic Differentiation

2009

Sensitivity analysis is an important part of gradient-based optimization of electromagnetic devices. We demonstrate how sensitivity analysis can be incorporated into an existing in-house method of moments solver with a relatively small amount of labor by using a technique called automatic differentiation (AD). This approach enables us to obtain (geometrical) sensitivities of the discrete solution with accuracy up to numerical precision. We compare the assembly time and memory usage of the modified and original solvers. Moreover, we optimize the shape of a dipole antenna and the dimensions of a Yagi-Uda array using the presented AD technique, traditional response level finite difference sens…

Antenna arrayMathematical optimizationAutomatic differentiationFinite difference methodShape optimizationSensitivity (control systems)Electrical and Electronic EngineeringMethod of moments (statistics)SolverAlgorithmGradient methodMathematicsIEEE Transactions on Antennas and Propagation
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Relativistic simulations of black hole-neutron star coalescence: the jet emerges

2014

We perform magnetohydrodynamic simulations in full general relativity (GRMHD) of a binary black hole-neutron star on a quasicircular orbit that undergoes merger. The binary mass ratio is 3:1, the black hole initial spin parameter $a/m=0.75$ ($m$ is the black hole Christodoulou mass) aligned with the orbital angular momentum, and the neutron star is an irrotational $\Gamma=2$ polytrope. About two orbits prior to merger (at time $t=t_B$), we seed the neutron star with a dynamically weak interior dipole magnetic field that extends into the stellar exterior. At $t=t_B$ the exterior has a low-density atmosphere with constant plasma parameter $\beta\equiv P_{\rm gas}/P_{\rm mag}$. Varying $\beta$…

AstrofísicaAngular momentumGeneral relativityAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesGeneral Relativity and Quantum CosmologyGeneral Relativity and Quantum Cosmology0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsGravitational waveAstronomy and AstrophysicsMass ratioPolytropeBlack holeNeutron starSpace and Planetary ScienceAstronomiaAstrophysics::Earth and Planetary AstrophysicsGamma-ray burstAstrophysics - High Energy Astrophysical Phenomena
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New horizons for fundamental physics with LISA

2022

K. G. Arun et al.

AstrofísicaPROTOPLANET MIGRATIONFísica-Modelos matemáticosPhysics and Astronomy (miscellaneous)gr-qcFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)GRAVITATIONAL-WAVEShorizonFundamental physicGeneral Relativity and Quantum CosmologyPhysics Particles & FieldsGravitational wavesLIGO (Observatory)Tests of general relativitySettore FIS/05 - Astronomia e AstrofisicaDARK-MATTERFísica matemáticaKOZAI MECHANISMHigh Energy PhysicsGENERAL-RELATIVITYFundamental physics; Gravitational waves; LISA; Tests of general relativityFundamental physicsPRIMORDIAL BLACK-HOLESLISAScience & TechnologyGeneral Relativity and Cosmology83CXXPhysicsgravitation: interactiongravitational radiationFísicaCompactQUANTUM-GRAVITYPhysical SciencesAstronomia[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]fundamental physics; gravitational waves; LISA; test of general relativityMODIFIED GRAVITYtest of general relativityGravitational waveMULTIPOLE MOMENTSHUBBLE CONSTANT
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Multiple expansions for energy and momenta carried by gravitational waves

2007

We present expressions for the energy, linear momentum and angular momentum carried away from an isolated system by gravitational radiation based on spin-weighted spherical harmonics decomposition of the Weyl scalar $\Psi_4$. We also show that the expressions derived are equivalent to the common expressions obtained when using a framework based on perturbations of a Schwazschild background. The main idea is to collect together all the different expressions in a uniform and consistent way. The formulae presented here are directly applicable to the calculation of the radiated energy, linear momentum and angular momentum starting from the gravitational waveforms which are typically extracted f…

AstrofísicaPhysicsAngular momentumPhysics and Astronomy (miscellaneous)Gravitational waveScalar (physics)FOS: Physical sciencesSpherical harmonicsGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum CosmologyIsolated systemGravitationQuantum electrodynamicsAstronomiaMultipole expansionEnergy (signal processing)General Relativity and Gravitation
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"Table 29" of "Measurement of the jet fragmentation function and transverse profile in proton-proton collisions at a center-of-mass energy of 7 TeV w…

2011

Charged particle ptRel distribution in the jet-Pt range 310 TO 400 GeV.

Astrophysics::High Energy Astrophysical Phenomena7000.0Single Differential DistributionJet ProductionP P --> CHARGED XP P --> JET XDN/DPTInclusiveSingle Differential Cross SectionProton-Proton ScatteringHigh Energy Physics::ExperimentDSIG/DPTNuclear ExperimentTransverse Momentum Dependence
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"Table 28" of "Measurement of the jet fragmentation function and transverse profile in proton-proton collisions at a center-of-mass energy of 7 TeV w…

2011

Charged particle ptRel distribution in the jet-Pt range 260 TO 310 GeV.

Astrophysics::High Energy Astrophysical Phenomena7000.0Single Differential DistributionJet ProductionP P --> CHARGED XP P --> JET XDN/DPTInclusiveSingle Differential Cross SectionProton-Proton ScatteringHigh Energy Physics::ExperimentDSIG/DPTNuclear ExperimentTransverse Momentum Dependence
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"Table 25" of "Measurement of the jet fragmentation function and transverse profile in proton-proton collisions at a center-of-mass energy of 7 TeV w…

2011

Charged particle ptRel distribution in the jet-Pt range 110 TO 160 GeV.

Astrophysics::High Energy Astrophysical Phenomena7000.0Single Differential DistributionJet ProductionP P --> CHARGED XP P --> JET XDN/DPTInclusiveSingle Differential Cross SectionProton-Proton ScatteringHigh Energy Physics::ExperimentDSIG/DPTNuclear ExperimentTransverse Momentum Dependence
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