A SCILAB PROGRAM FOR COMPUTING GENERAL-RELATIVISTIC MODELS OF ROTATING NEUTRON STARS BY IMPLEMENTING HARTLE'S PERTURBATION METHOD

DOI10.1142/S0129183103004516zbMath1082.85505OpenAlexW1995709032MaRDI QIDQ5716113

V. S. Geroyannis, P. J. Papasotiriou

Publication date: 9 January 2006

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

Full work available at URL: https://doi.org/10.1142/s0129183103004516

zbMATH Keywords

rotationneutron starsGRT methodsnumerical stars

Mathematics Subject Classification ID

Galactic and stellar structure (85A15) Approximation procedures, weak fields in general relativity and gravitational theory (83C25)

Related Items (3)

NUMERICAL METHODS FOR SOLVING THE RELATIVISTIC OPPENHEIMER–VOLKOFF EQUATIONS ⋮ MAGNETIZED ROTATING NEUTRON STARS SIMULATED BY GENERAL-RELATIVISTIC POLYTROPIC MODELS: THE NUMERICAL TREATMENT ⋮ NUMERICAL TREATMENT OF HARTLE'S PERTURBATION METHOD FOR DIFFERENTIALLY ROTATING NEUTRON STARS SIMULATED BY GENERAL-RELATIVISTIC POLYTROPIC MODELS

Uses Software

• Unnamed Item

Cites Work

• Slowly rotating general relativistic superfluid neutron stars
• Rotating compact objects with magnetic fields
• Equations of State of Elements Based on the Generalized Fermi-Thomas Theory

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