Search results for "Computational physics"

showing 10 items of 725 documents

Core collapse with magnetic fields and rotation

2018

We study the effects of magnetic fields and rotation on the core collapse of a star of an initial mass of M = 20 solar masses using axisymmetric simulations coupling special relativistic magnetohydrodynamics, an approximately relativistic gravitational potential, and spectral neutrino transport. We compare models of the same core with different, artificially added profiles of rotation and magnetic field. A model with weak field and slow rotation does not produce an explosion, while stronger fields and fast rotation open the possibility of explosions. Whereas the neutrino luminosities of the exploding models are the same as or even less than those of the non-exploding model, magnetic fields …

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsNuclear and High Energy PhysicsField (physics)010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesRotation01 natural sciences7. Clean energyInstabilityMagnetic fieldComputational physicsGravitational potentialAstrophysics - Solar and Stellar Astrophysics0103 physical sciencesGravitational collapseMagnetohydrodynamicsNeutrinoAstrophysics - High Energy Astrophysical Phenomena010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Journal of Physics G: Nuclear and Particle Physics
researchProduct

Dynamical efficiency of collisionless magnetized shocks in relativistic jets

2010

The so-called internal shock model aims to explain the light-curves and spectra produced by non-thermal processes originated in the flow of blazars and gamma-ray bursts. A long standing question is whether the tenuous collisionless shocks, driven inside a relativistic flow, are efficient enough to explain the amount of energy observed as compared with the expected kinetic power of the outflow. In this work we study the dynamic efficiency of conversion of kinetic-to- thermal/magnetic energy of internal shocks in relativistic magnetized outflows. We find that the collision between shells with a non-zero relative velocity can yield either two oppositely moving shocks (in the frame where the co…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsShock waveShock (fluid dynamics)Magnetic energyAstrophysics::High Energy Astrophysical PhenomenaRelative velocityFOS: Physical sciencesRarefaction020206 networking & telecommunications02 engineering and technologyKinetic energyComputational physicsAstrophysical jet0202 electrical engineering electronic engineering information engineering020201 artificial intelligence & image processingAstrophysics - High Energy Astrophysical PhenomenaBlazarAstrophysics::Galaxy AstrophysicsAIP Conference Proceedings
researchProduct

Observability and diagnostics in the X-ray band of shock-cloud interactions in supernova remnants

2010

X-ray emitting features originating from the interaction of supernova shock waves with small interstellar gas clouds are revealed in many X-ray observations of evolved supernova remnants (e.g. Cygnus Loop and Vela), but their interpretation is not straightforward. We develop a self-consistent method for the analysis and interpretation of shock-cloud interactions in middle-aged supernova remnants, which can provide the key parameters of the system and the role of relevant physical effects like the thermal conduction, without the need to run ad-hoc numerical simulations and to bother of morphology details. We explore all the possible values of the shock speed and cloud density contrast releva…

High Energy Astrophysical Phenomena (astro-ph.HE)Shock wavePhysicsCygnus LoopRadiative coolingAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstronomy and AstrophysicsHydrodynamicThermal conductionVelaX-rays: ISMComputational physicsShock (mechanics)SupernovaShock waveISM: cloudSpace and Planetary ScienceDensity contrastAstrophysics - High Energy Astrophysical PhenomenaISM: supernova remnantAstrophysics::Galaxy AstrophysicsAstronomy and Astrophysics
researchProduct

EFFICIENCY OF INTERNAL SHOCKS IN MAGNETIZED RELATIVISTIC JETS

2011

We study the dynamic and radiative efficiency of conversion of kinetic-to-thermal/magnetic energy by internal shocks in relativistic magnetized outflows. A parameter study of a large number of collisions of cylindrical shells is performed. We explore how, while keeping the total flow luminosity constant, the variable fluid magnetization influences the efficiency and find that the interaction of shells in a mildly magnetized jet yields higher dynamic, but lower radiative efficiency than in a non-magnetized flow. A multi-wavelength radiative signature of different shell magnetization is computed assuming that relativistic particles are accelerated at internal shocks.

High Energy Astrophysical Phenomena (astro-ph.HE)Shock wavePhysicsJet (fluid)Luminosity (scattering theory)010504 meteorology & atmospheric sciencesMagnetic energyAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciences01 natural sciencesRelativistic particleComputational physicsMagnetizationAstrophysical jet0103 physical sciencesRadiative transferAstrophysics - High Energy Astrophysical Phenomena010303 astronomy & astrophysics0105 earth and related environmental sciencesInternational Journal of Modern Physics: Conference Series
researchProduct

Galactic rotation curves in hybrid metric-Palatini gravity

2013

Generally, the dynamics of test particles around galaxies, as well as the corresponding mass deficit, is explained by postulating the existence of a hypothetical dark matter. In fact, the behavior of the rotation curves shows the existence of a constant velocity region, near the baryonic matter distribution, followed by a quick decay at large distances. In this work, we consider the possibility that the behavior of the rotational velocities of test particles gravitating around galaxies can be explained within the framework of the recently proposed hybrid metric-Palatini gravitational theory. The latter is constructed by modifying the metric Einstein-Hilbert action with an f(R) term in the P…

High Energy Physics - TheoryModified gravityMass deficitDark matterFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesGeneral Relativity and Quantum CosmologyGravitationGeneral Relativity and Quantum Cosmology0103 physical sciencesDark matterSurface brightness010303 astronomy & astrophysicsGalaxy rotation curvePhysics010308 nuclear & particles physicsAstronomy and AstrophysicsObservableGalactic rotation curvesAstrophysics - Astrophysics of GalaxiesGalaxyComputational physicsClassical mechanicsHigh Energy Physics - Theory (hep-th)Astrophysics of Galaxies (astro-ph.GA)Scalar field
researchProduct

Multi-boson block factorization of fermions

2017

The numerical computations of many quantities of theoretical and phenomenological interest are plagued by statistical errors which increase exponentially with the distance of the sources in the relevant correlators. Notable examples are baryon masses and matrix elements, the hadronic vacuum polarization and the light-by-light scattering contributions to the muon g-2, and the form factors of semileptonic B decays. Reliable and precise determinations of these quantities are very difficult if not impractical with state-of-the-art standard Monte Carlo integration schemes. I will review a recent proposal for factorizing the fermion determinant in lattice QCD that leads to a local action in the g…

High Energy Physics::Latticeaction: local01 natural sciencesHigh Energy Physics - Phenomenology (hep-ph)Vacuum polarizationcorrelation functionQuantum Chromodynamics Lattice gauge theory Computational PhysicsMonte CarloBosonPhysicsform factorPhysicsHigh Energy Physics - Lattice (hep-lat)lattice field theoryPropagatorpropagator [quark]hep-phParticle Physics - Latticestatistical [error]Lattice QCDFIS/02 - FISICA TEORICA MODELLI E METODI MATEMATICIHigh Energy Physics - Phenomenologyerror: statisticalquark: factorizationquark: propagatorMonte Carlo integrationQuarkParticle physicsQC1-999fermion: determinantdeterminant [fermion]FOS: Physical scienceshep-latbaryon: massHigh Energy Physics - LatticeFactorization0103 physical sciencesmagnetic moment [muon]hadronic [vacuum polarization]010306 general physicsnumerical calculationsParticle Physics - Phenomenologymuon: magnetic moment010308 nuclear & particles physicsvacuum polarization: hadronicHigh Energy Physics::Phenomenologyphoton photon: scatteringB: decaylocal [action]Fermiondecay [B]mass [baryon]scattering [photon photon]gauge field theoryHigh Energy Physics::Experimentfactorization [quark]
researchProduct

Fundamentals of metastability exchange optical pumping in helium

2010

21 pages; International audience; Advances in metastability exchange optical pumping (MEOP) at high laser powers, but also at high gas pressures and high magnetic field strengths, has provided strong motivation for revisiting the understanding of the limitations of this powerful technique. A comprehensive model has been developped for improved description of the combined effects of OP, ME, and relaxation, and of detailed MEOP features observed over the broad range of operating conditions. A brief description is provided, with illustrative comparisons of computed and experimental results. This improved tool is used to explain the excellent photon efficiency of OP obtained at all field streng…

HistoryAngular momentumPhotonCondensed matter physicsField (physics)[PHYS.PHYS.PHYS-ATOM-PH]Physics [physics]/Physics [physics]/Atomic Physics [physics.atom-ph]ChemistryRelaxation (NMR)chemistry.chemical_elementLaser01 natural sciences010305 fluids & plasmasComputer Science ApplicationsEducationComputational physicslaw.inventionOptical pumpinglawMetastability0103 physical sciences010306 general physicsHelium
researchProduct

Bichromatic field propagation in a resonant medium: Floquet analysis

2011

We study the propagation of a bichromatic field in a resonant medium. The two modes of the incoming fields are pulsed and delayed with respect to each other. It is shown that in the course of the propagation, new Raman sidebands will be generated. The achievable frequency spacing between the sidebands is determined from experimental data. A numerical example is shown for realistic physical parameters.

HistoryEngineeringField propagationField (physics)business.industryComputer Science ApplicationsEducationComputational physicssymbols.namesakesymbolsElectronic engineeringFloquet analysisRaman spectroscopybusinessJournal of Physics: Conference Series
researchProduct

Results from the Project 8 phase-1 cyclotron radiation emission spectroscopy detector

2017

The Project 8 collaboration seeks to measure the absolute neutrino mass scale by means of precision spectroscopy of the beta decay of tritium. Our technique, cyclotron radiation emission spectroscopy, measures the frequency of the radiation emitted by electrons produced by decays in an ambient magnetic field. Because the cyclotron frequency is inversely proportional to the electron's Lorentz factor, this is also a measurement of the electron's energy. In order to demonstrate the viability of this technique, we have assembled and successfully operated a prototype system, which uses a rectangular waveguide to collect the cyclotron radiation from internal conversion electrons emitted from a ga…

HistoryPhysics - Instrumentation and DetectorsCyclotronFOS: Physical sciencesElectronRadiationEducationlaw.inventionHigh Energy Physics - Experimentsymbols.namesakeHigh Energy Physics - Experiment (hep-ex)Internal conversionlawddc:530Cyclotron radiationEmission spectrumNuclear Experiment (nucl-ex)Nuclear ExperimentPhysicsPhysicsInstrumentation and Detectors (physics.ins-det)Computer Science ApplicationsComputational physicsLorentz factorsymbolsNeutrino
researchProduct

Progress in Modelling Coherently Pumped Far-Infrared Laser Dynamics

1990

Coherently pumped lasers (CPL) operating in the far-infrared spectral region shown a wealth of instabilities1, including a behavior remarkably similar2,3 with the predictions of the paradigmatic Lorenz-Haken model of a single-mode homogeneously broadened laser4,5. The qualitative agreement; between theory and experiments2,3 was rather surprising, for the model4,5 refers to a two-level system whereas the CPL operate on a three-level scheme, where the pumping and lasing transitions share a common upper level. Dupertuis et al.6 have identified conditions for the mathematical reduction of the CPL equations to the Lorenz-Haken equations4, but these conditions were not all fulfilled in the experi…

Hopf bifurcationReduction (complexity)Physicssymbols.namesakelawFar-infrared laserDynamics (mechanics)symbolsBifurcation diagramLaserLasing thresholdComputational physicslaw.invention
researchProduct