NUMERICAL TREATMENT OF ROTATING NEUTRON STARS SIMULATED BY GENERAL-RELATIVISTIC POLYTROPIC MODELS: A COMPLEX-PLANE STRATEGY

DOI10.1142/S0129183111016269zbMath1217.85002OpenAlexW2038619973MaRDI QIDQ3011498

I. E. Sfaelos, V. S. Geroyannis

Publication date: 29 June 2011

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

Full work available at URL: https://doi.org/10.1142/s0129183111016269

zbMATH Keywords

rotationnumerical methodsrelativityneutron starspolytropic models

Mathematics Subject Classification ID

Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Galactic and stellar structure (85A15) Software, source code, etc. for problems pertaining to astronomy and astrophysics (85-04)

Related Items (1)

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

Cites Work

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• ATOMFT: Solving ODEs and DAEs using Taylor series
• NUMERICAL METHODS FOR SOLVING THE RELATIVISTIC OPPENHEIMER–VOLKOFF EQUATIONS
• NUMERICAL TREATMENT OF HARTLE'S PERTURBATION METHOD FOR DIFFERENTIALLY ROTATING NEUTRON STARS SIMULATED BY GENERAL-RELATIVISTIC POLYTROPIC MODELS
• Ratio-Like and Recurrence Relation Tests for Convergence of Series

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