Search results for "Grad–Shafranov equation"

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Numerically solving the relativistic Grad–Shafranov equation in Kerr spacetimes: numerical techniques

2018

The study of the electrodynamics of static, axisymmetric and force-free Kerr magnetospheres relies vastly on solutions of the so called relativistic Grad-Shafranov equation (GSE). Different numerical approaches to the solution of the GSE have been introduced in the literature, but none of them has been fully assessed from the numerical point of view in terms of efficiency and quality of the solutions found. We present a generalization of these algorithms and give detailed background on the algorithmic implementation. We assess the numerical stability of the implemented algorithms and quantify the convergence of the presented methodology for the most established setups (split-monopole, parab…

High Energy Astrophysical Phenomena (astro-ph.HE)Physics010308 nuclear & particles physicsGeneralizationRotational symmetryFOS: Physical sciencesAstronomy and AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyMagnetic fieldGrad–Shafranov equationQuality (physics)Space and Planetary Science0103 physical sciencesConvergence (routing)Applied mathematicsPoint (geometry)Astrophysics - High Energy Astrophysical Phenomena010303 astronomy & astrophysicsNumerical stabilityMonthly Notices of the Royal Astronomical Society
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The force-free twisted magnetosphere of a neutron star – II. Degeneracies of the Grad–Shafranov equation

2017

We extend our previous study of equilibrium solutions of non-rotating force-free magnetospheres of neutron stars. We show that multiple solutions exist for the same sets of parameters, implying that the solutions are degenerate. We are able to obtain configurations with disconnected field lines, however, in nearly all cases these correspond to degenerate higher energy solutions. We carry out a wide parametric search in order to understand the properties of the solutions. We confirm our previous results that the lower energy solutions have up to $\sim 25\%$ more energy than the vacuum case, helicity of the order of $\sim 5$ (in some defined units), maximum twist of $\sim 1.5$ rad, and a dipo…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsWork (thermodynamics)MHDFOS: Physical sciencesMagnetosphereneutron [Stars]Astronomy and Astrophysics01 natural sciencesMagnetic fieldmagnetars [Stars]magnetic field [Stars]Neutron starGrad–Shafranov equationClassical mechanicsSpace and Planetary ScienceMagnetic fieldsQuantum electrodynamics0103 physical sciencesCost actionMagnetohydrodynamicsAstrophysics - High Energy Astrophysical Phenomena010306 general physics010303 astronomy & astrophysicsAstronomía y AstrofísicaMonthly Notices of the Royal Astronomical Society
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