MAGNETIZED ROTATING NEUTRON STARS SIMULATED BY GENERAL-RELATIVISTIC POLYTROPIC MODELS: THE NUMERICAL TREATMENT

DOI10.1142/S0129183111016786zbMath1263.85021MaRDI QIDQ4911512

V. S. Geroyannis, A. G. Katelouzos, F. N. Valvi

Publication date: 15 March 2013

Published in: International Journal of Modern Physics C (Search for Journal in Brave)

zbMATH Keywords

MHDrotationnumerical methodsmagnetic fieldsgeneral relativityneutron starspolytropic modelsSturm--Liouville problemGrad--Shafranov equation

Mathematics Subject Classification ID

Magnetohydrodynamics and electrohydrodynamics (76W05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) PDEs in connection with relativity and gravitational theory (35Q75) Galactic and stellar structure (85A15) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30) PDEs in connection with astronomy and astrophysics (35Q85)

Cites Work

• ATOMFT: Solving ODEs and DAEs using Taylor series
• NUMERICAL TREATMENT OF ROTATING NEUTRON STARS SIMULATED BY GENERAL-RELATIVISTIC POLYTROPIC MODELS: A COMPLEX-PLANE STRATEGY
• NUMERICAL TREATMENT OF HARTLE'S PERTURBATION METHOD FOR DIFFERENTIALLY ROTATING NEUTRON STARS SIMULATED BY GENERAL-RELATIVISTIC POLYTROPIC MODELS
• The Equilibrium of Distorted Polytropes: (I). The Rotational Problem
• Algorithm 810: The SLEIGN2 Sturm-Liouville Code
• A SCILAB PROGRAM FOR COMPUTING GENERAL-RELATIVISTIC MODELS OF ROTATING NEUTRON STARS BY IMPLEMENTING HARTLE'S PERTURBATION METHOD

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