Non-linear hydrodynamical evolution of rotating relativistic stars: Numerical methods and code tests

Monthly Notices of the Royal Astronomical Society

Volumn 313, Issue 4, 2000, Pages 678-688

  Font, José A ^a   Stergioulas, Nikolaos ^a,b   Kokkotas, Kostas D ^b  

^a MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^b ARISTOTLE UNIVERSITY OF THESSALONIKI   (Greece)

Author keywords

Hydrodynamics; Methods: Numerical; Relativity; Stars: Neutron; Stars: Oscillations; Stars: Rotation

Indexed keywords

CODES (SYMBOLS); FINITE DIFFERENCE METHOD; FOURIER SERIES; HYDRODYNAMICS; LONG TERM EVOLUTION (LTE); NEUTRONS; NUMERICAL METHODS; RELATIVITY;

AXISYMMETRIC; HIGH RESOLUTION; LONG-TERM EVOLUTION; METHOD: NUMERICAL; NEUTRON STARS; NON LINEAR; RELATIVISTIC STARS; STAR OSCILLATIONS; STARS: NEUTRONS; STARS: ROTATION;

STARS;

EID: 0001402484     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2000.03254.x     Document Type: Article

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