Search results for "Computer Science Application"

showing 10 items of 3998 documents

Emission of fragments in Ca+Ca reaction at 25 MeV/nucleon

2013

We discuss experimental data concerning 40,48Ca+ 40,48Ca reactions at 25 MeV/nucleon; the 4π multi-detector Chimera has been used as detection device. Effects that can be attributed to the neutron to proton ratios (N/Z) degree of freedom have been investigated. From the analysis of experimental data it seems that the neutron richness of the interacting system plays an important role on the evolution of fusion-like sources formed in semi-central collisions. In particular, it is observed that the larger is the neutron content and the larger is the emission of heavy residues. Experimental data have been compared with CoMD-II model calculations; a moderately stiff symmetry energy should be used…

PhysicsHistoryNuclear Theoryand isobaric spin 24.10.Pa Thermal and statistical modelsComputer Science ApplicationsEducationNuclear physicsPhysics and Astronomy (all)parityIsospin25.75.Gz Particle correlations and fluctuations 21.65.-f Nuclear matter 27.40.+z 39(less-than-or-equal-to)A(less-than-or-equal-to)58 21.10.Hw SpinIsobaric processNeutronAtomic physicsNuclear ExperimentNucleon
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Right-handed neutrino magnetic moments

2009

PACS numbers: 14.60.St, 13.15.+g, 13.35.Hb, 13.66.Hk

PhysicsHistoryNuclear and High Energy PhysicsParticle physicsMagnetic momentElectron–positron annihilationElectroweak interactionHigh Energy Physics::PhenomenologyVertex functionFOS: Physical sciencesPartícules (Física nuclear)Computer Science ApplicationsEducationHigh Energy Physics - PhenomenologyOperator (computer programming)High Energy Physics - Phenomenology (hep-ph)BibliographyCP violationHigh Energy Physics::ExperimentNeutrino
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Numerical viscosity in simulations of the two-dimensional Kelvin-Helmholtz instability

2020

The Kelvin-Helmholtz instability serves as a simple, well-defined setup for assessing the accuracy of different numerical methods for solving the equations of hydrodynamics. We use it to extend our previous analysis of the convergence and the numerical dissipation in models of the propagation of waves and in the tearing-mode instability in magnetohydrodynamic models. To this end, we perform two-dimensional simulations with and without explicit physical viscosity at different resolutions. A comparison of the growth of the modes excited by our initial perturbations allows us to estimate the effective numerical viscosity of two spatial reconstruction schemes (fifth-order monotonicity preservin…

PhysicsHistoryNumerical analysisFOS: Physical sciences010103 numerical & computational mathematicsMechanicsComputational Physics (physics.comp-ph)Dissipation01 natural sciencesInstabilityComputer Science ApplicationsEducationPiecewise linear functionViscositySimple (abstract algebra)0103 physical sciencesConvergence (routing)Magnetohydrodynamic drive0101 mathematicsAstrophysics - Instrumentation and Methods for AstrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Physics - Computational Physics010303 astronomy & astrophysicsJournal of Physics: Conference Series
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Relativistic MHD simulations of stellar core collapse and magnetars

2011

We present results from simulations of magneto-rotational stellar core collapse along with Alfven oscillations in magnetars. These simulations are performed with the CoCoA/CoCoNuT code, which is able to handle ideal MHD flows in dynamical spacetimes in general relativity. Our core collapse simulations highlight the importance of genuine magnetic effects, like the magneto-rotational instability, for the dynamics of the flow. For the modelling of magnetars we use the anelastic approximation to general relativistic MHD, which allows for an effective suppression of fluid modes and an accurate description of Alfven waves. We further compute Alfven oscillation frequencies along individual magneti…

PhysicsHistoryOscillationGeneral relativityCollapse (topology)MagnetarInstabilityComputer Science ApplicationsEducationMagnetic fieldClassical mechanicsHarmonicsQuantum electrodynamicsMagnetohydrodynamicsJournal of Physics: Conference Series
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On the local existence of maximal slicings in spherically symmetric spacetimes

2010

In this talk we show that any spherically symmetric spacetime admits locally a maximal spacelike slicing. The above condition is reduced to solve a decoupled system of first order quasi-linear partial differential equations. The solution may be accomplished analytical or numerically. We provide a general procedure to construct such maximal slicings.

PhysicsHistoryPartial differential equationFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)First orderSpherically symmetric spacetimeGeneral Relativity and Quantum CosmologyComputer Science ApplicationsEducationMathematical physics
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Master Majorana neutrino mass parametrization

2019

After introducing a master formula for the Majorana neutrino mass matrix, we present a master parametrization for the Yukawa matrices automatically in agreement with neutrino oscillation data. This parametrization can be used for any model that induces Majorana neutrino masses. The application of the master parametrization is also illustrated in an example model, with special focus on its lepton flavor violating phenomenology.

PhysicsHistoryParticle physics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyYukawa potentialFOS: Physical sciencesMass matrix01 natural sciencesComputer Science ApplicationsEducationHigh Energy Physics - PhenomenologyMAJORANAHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesHigh Energy Physics::ExperimentNeutrino010306 general physicsNeutrino oscillationPhenomenology (particle physics)ParametrizationLeptonJournal of Physics: Conference Series
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Automation of NLO processes and decays and POWHEG matching in WHIZARD

2016

Journal of physics / Conference Series 762, 012059 (2016). doi:10.1088/1742-6596/762/1/012059

PhysicsHistoryParticle physics010308 nuclear & particles physicsScatteringMonte Carlo methodHigh Energy Physics::PhenomenologyFOS: Physical sciencesObservable01 natural sciences530Computer Science ApplicationsEducationHigh Energy Physics - PhenomenologyAmplitudeHigh Energy Physics - Phenomenology (hep-ph)Phase space0103 physical sciencesddc:530High Energy Physics::Experiment010306 general physicsParton showerNuclear ExperimentEvent generatorLepton
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New Atomic Methods for Dark Matter Detection

2015

We calculate the parity and time-reversal violating effects that are induced in atoms, nuclei, and molecules by their interaction with various background cosmic fields, such as axion dark matter or dark energy.

PhysicsHistoryParticle physicsAxion Dark Matter ExperimentHot dark matterHigh Energy Physics::PhenomenologyDark matterScalar field dark matterAstrophysics::Cosmology and Extragalactic AstrophysicsComputer Science ApplicationsEducationMixed dark matterWarm dark matterLight dark matterDark fluidJournal of Physics: Conference Series
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Study of theZb(10610) andZb(10650) states through $B\bar{B}^*$ and $B^*\bar{B}^*$ interactions using local hidden gauge approach

2016

We have studied the $B\bar{B}^*$ and $B^*\bar{B}^*$ interactions for isospin I = 1 using the Local Hidden gauge approach. Since both interactions via one light meson exchange are not allowed by Okubo-Zweig-Iizuka (OZI) rule, we investigated the contributions for those interactions coming from two pions, interacting and noninteracting among themselves, and also due to the heavy vector meson exchange, in which the OZI rule no longer holds. From the amplitudes calculated by these mechanism, we determine an effective potential which is used as a kernel of the Bethe-Salpeter equation. Our goal is look for poles in the T-matrix in attemp to relate them with the charged Zb (10610) and Zb (10650) s…

PhysicsHistoryParticle physicsBethe–Salpeter equationMesonBar (music)Nuclear TheoryHigh Energy Physics::PhenomenologyComputer Science ApplicationsEducationNuclear physicsPionOZI ruleIsospinBound stateHigh Energy Physics::ExperimentVector mesonNuclear ExperimentJournal of Physics: Conference Series
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Right Handed Sneutrino Dark Matter in Inverse and Linear seesaw scenarios

2012

We consider supersymmetric models in which the right-handed sneutrino is a viable WIMP dark matter candidate. These are either simple extensions of the Minimal Supersymmetric Standard Model or models with the addition of an extra U(1) group. All of them can explain small neutrino masses, through either the Inverse or the Linear Seesaw mechanism. We investigate the properties of the dark matter candidate naturally arising in these scenarios. We check for phenomenological bounds, such as correct relic abundance, consistency with direct detection cross section limits and laboratory constraints. Especially, we comment on limitations of the model space due to lepton flavour violating charged lep…

PhysicsHistoryParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Dark matterHigh Energy Physics::PhenomenologyFOS: Physical sciencesSupersymmetryLightest Supersymmetric ParticleComputer Science ApplicationsEducationHigh Energy Physics - PhenomenologySeesaw mechanismHigh Energy Physics - Phenomenology (hep-ph)Seesaw molecular geometryHigh Energy Physics::ExperimentNeutrinoLeptonMinimal Supersymmetric Standard ModelAstrophysics - Cosmology and Nongalactic Astrophysics
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