Search results for "Hydrodynamics"

showing 10 items of 390 documents

Numerical treatment of radiation processes in the internal shocks of magnetized relativistic outflows

2017

Los blázares son un tipo de núcleo activo de galaxia (AGN, por sus siglas en inglés) que se encuentran entre los objetos astrofísicos más energéticos y violentos, a la par de los brotes de rayos gamma (GRB por sus siglas en inglés). Los procesos físicos y, en particular, el escenario del chorro relativista en el que se genera la radiación ultraenergética detectada por observatorios terrestres y en órbita, han conseguido atraer la atención e interés de los astrónomos y astrofísicos desde su descubrimiento. En la presente tesis investigamos el modelo de choques internos (IS) cuya hipótesis consta del choque de dos capas de plasma con geometría cilíndrica, formando dos ondas de choque que atra…

radiation mechanisms: thermalradiation mechanisms: nonthermalradiative transferthermal [radiation mechanisms]numerical methodsgeneral [bl lacertae objects]nonthermal [radiation mechanisms]shock wavesUNESCO::ASTRONOMÍA Y ASTROFÍSICAmagnetohydrodynamics:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]bl lacertae objects: general
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Enhancing the Iterative Smoothed Particle Hydrodynamics Method

2021

Motivated by recent research on the iterative approach proposed for the smoothed particle hydrodynamics (ISPH) method, some ideas to improve the process are introduced. The standard procedure is enhanced iterating on the residuals preserving the matrix-free nature of the process. The method is appealing providing reasonable results with disordered data distribution too and no kernel variations are needed in the approximation. This work moves forward with a novel formulation requiring a lower number of iterations to reach a desired accuracy. The computational procedure is described and some results are introduced to appreciate the proposed formulation.

smoothed particle hydrodynamics02 engineering and technologylcsh:Technology01 natural scienceslcsh:ChemistrySmoothed-particle hydrodynamicsSettore MAT/08 - Analisi Numerica0202 electrical engineering electronic engineering information engineeringGeneral Materials Science0101 mathematicslcsh:QH301-705.5InstrumentationFluid Flow and Transfer ProcessesPhysicslcsh:TProcess Chemistry and TechnologyGeneral Engineering020206 networking & telecommunicationsMechanicslcsh:QC1-999Computer Science Applications010101 applied mathematicskernel methodresidualslcsh:Biology (General)lcsh:QD1-999lcsh:TA1-2040lcsh:Engineering (General). Civil engineering (General)lcsh:PhysicsKernel method Residuals Smoothed particle hydrodynamicsApplied Sciences
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Study of thermoelectric magnetohydrodynamic convection on solute redistribution during laser additive manufacturing

2020

Abstract Melt pools formed in laser additive manufacturing (AM) are subject to large thermal gradients, resulting in the formation of thermoelectric currents due to the Seebeck effect. When in the presence of an external magnetic field, a Lorentz force is formed which drives fluid flow in the melt pool. This Thermoelectric Magnetohydrodynamics (TEMHD) phenomenon, can have a significant impact on the melt pool morphology and can alter the microstructural evolution of the solidification process. By coupling steady-state mesoscopic melt pool calculations to a microscopic solidification model, predictions of the resulting microstructure for multiple deposited layers have been obtained. The resu…

symbols.namesakeMaterials scienceCondensed matter physicsThermalThermoelectric effectFluid dynamicssymbolsMagnetohydrodynamic driveMagnetohydrodynamicsMicrostructureQALorentz forceMagnetic field
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Three-dimensional core-collapse supernovae with complex magnetic structures: I. Explosion dynamics

2021

Magnetic fields can play a major role in the dynamics of outstanding explosions associated to violent events such as GRBs and hypernovae, since they provide a natural mechanism to harness the rotational energy of the central proto-neutron star and power relativistic jets through the stellar progenitor. As the structure of such fields is quite uncertain, most numerical models of MHD-driven core-collapse supernovae consider an aligned dipole as initial magnetic field, while the field's morphology can actually be much more complex. We present three-dimensional simulations of core-collapse supernovae with more realistic magnetic structures, such as quadrupolar fields and, for the first time, an…

transients: supernovaeField (physics)MHDAstrophysics::High Energy Astrophysical Phenomenagamma-ray burst: generalFOS: Physical sciencesAstrophysics01 natural sciencesstars: magnetarsAstrophysical jet0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)relativistic processesPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsAstronomy and AstrophysicsRotational energyMagnetic fieldDipoleAstrophysics - Solar and Stellar AstrophysicsinstabilitiesSpace and Planetary ScienceMagnetohydrodynamicsAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]HypernovaDynamo
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The impact of non-dipolar magnetic fields in core-collapse supernovae

2019

The magnetic field is believed to play an important role in at least some core-collapse supernovae if its magnitude reaches $10^{15}\,\rm{G}$, which is a typical value for a magnetar. In the presence of fast rotation, such a strong magnetic field can drive powerful jet-like explosions if it has the large-scale coherence of a dipole. The topology of the magnetic field is, however, probably much more complex with strong multipolar and small-scale components and the consequences for the explosion are so far unclear. We investigate the effects of the magnetic field topology on the dynamics of core-collapse supernovae and the properties of forming proto-neutron star (PNS) by comparing pre-collap…

transients: supernovaeMHDAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCompact starMagnetar01 natural sciencesstars: magnetars0103 physical sciences010303 astronomy & astrophysicsrelativistic processesPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Toroid010308 nuclear & particles physicsgamma-ray burststurbulenceAstronomy and AstrophysicsRotational energyComputational physicsMagnetic fieldSupernovaDipoleSpace and Planetary ScienceMagnetohydrodynamicsAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Monthly Notices of the Royal Astronomical Society
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Parametric sensitivity of a CFD model concerning the hydrodynamics of trickle-bed reactor (TBR)

2016

Abstract The aim of the present study was to investigate the sensitivity of a multiphase Eulerian CFD model with respect to relations defining drag forces between phases. The mean relative error as well as standard deviation of experimental and computed values of pressure gradient and average liquid holdup were used as validation criteria of the model. Comparative basis for simulations was our own data-base obtained in experiments carried out in a TBR operating at a co-current downward gas and liquid flow. Estimated errors showed that the classical equations of Attou et al. (1999) defining the friction factors Fjk approximate experimental values of hydrodynamic parameters with the best agre…

trickle-flow regimeMaterials sciencebusiness.industryThermodynamicslcsh:TP155-156pressure gradient02 engineering and technologyMechanicsTrickle-bed reactorComputational fluid dynamics021001 nanoscience & nanotechnologyliquid holdupPhysics::Fluid Dynamicsphases interaction020401 chemical engineeringhydrodynamicsSensitivity (control systems)0204 chemical engineeringlcsh:Chemical engineering0210 nano-technologybusinessCFDPressure gradientLiquid holdupParametric statisticsChemical and Process Engineering
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Разработка и применение специальных численных методов для решения задач математической физики, гидродинамики и магнитной гидродинамики

1993

Математическая физикаMagnetohydrodynamics:NATURAL SCIENCES::Physics::Other physics::Mathematical physics [Research Subject Categories]МагнитогидродинамикаMatemātiskā fizikaMagnetohidrodinamikaHydrodynamicsГидродинамикаHidrodinamika
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Прикладные задачи математической физики: Математическое моделирование

1990

Настоящий сборник содержит работы по математическому моделированию различных физических и технологических процессов. Анализируются процессы тепло- и массопереноса в расплавах и жидкостях, задачи термоупругости и упругопластического деформирования в кристаллах.

Математическая физикаПроцессы массопереносаТермоупругостьMatemātiskā modelēšanaПроцессы теплопереносаГидродинамикаHidrodinamikaДеформирование:NATURAL SCIENCES::Physics::Other physics::Mathematical physics [Research Subject Categories]КристаллыТепломассообменMatemātiskā fizikaHydrodynamicsМатематическое моделирование
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Прикладные задачи математической физики: Математическое моделирование

1991

Сборник содержит работы, посвященные математическому моделированию различных физических и технологических процессов. Анализируются процессы тепло- и массопереноса в расплавах и жидкостях, задачи термоупругости и упругопластического деформирования в кристаллах.

Математическая физикаТермоупругостьПроцессы масссопереносаMatemātiskā modelēšanaПроцессы теплопереносаГидродинамикаHidrodinamikaДеформирование:NATURAL SCIENCES::Physics::Other physics::Mathematical physics [Research Subject Categories]ТепломассообменКристаллыMatemātiskā fizikaHydrodynamicsМатематическое моделирование
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Магнитные взаимодействия и ориентационные явления в гидродинамике намагничивающихся жидкостей

1985

Ферромагнетики:NATURAL SCIENCES::Physics::Condensed matter physics [Research Subject Categories]Механика сплошных средMagnetohydrodynamicsPlūsmas mehānikaМагнитная гидродинамикаMagnetohidrodinamikaMagnetismElectromagnetic fieldFluid mechanicsГидродинамикаЭлектромагнитное поле
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