NUMERICAL TREATMENT OF HARTLE'S PERTURBATION METHOD FOR DIFFERENTIALLY ROTATING NEUTRON STARS SIMULATED BY GENERAL-RELATIVISTIC POLYTROPIC MODELS

DOI10.1142/S0129183108013370zbMath1173.85304MaRDI QIDQ3631052

V. S. Geroyannis, A. G. Katelouzos

Publication date: 5 June 2009

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

zbMATH Keywords

starsmethodsdifferential rotationneutronnumerical

Mathematics Subject Classification ID

Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Galactic and stellar structure (85A15) Exact solutions to problems in general relativity and gravitational theory (83C15) Software, source code, etc. for problems pertaining to astronomy and astrophysics (85-04)

Related Items (2)

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

Cites Work

• NUMERICAL METHODS FOR SOLVING THE RELATIVISTIC OPPENHEIMER–VOLKOFF EQUATIONS
• Rapidly rotating general relativistic stars - I. Numerical method and its application to uniformly rotating polytropes
• A SCILAB PROGRAM FOR COMPUTING GENERAL-RELATIVISTIC MODELS OF ROTATING NEUTRON STARS BY IMPLEMENTING HARTLE'S PERTURBATION METHOD

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