Non-linear axisymmetric pulsations of rotating relativistic stars in the conformal flatness approximation

Monthly Notices of the Royal Astronomical Society

Volumn 368, Issue 4, 2006, Pages 1609-1630

  Dimmelmeier, Harald ^a   Stergioulas, Nikolaos ^b   Font, José A ^c  

^a MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^b ARISTOTLE UNIVERSITY OF THESSALONIKI   (Greece)

^c UNIVERSITY OF VALENCIA   (Spain)

Author keywords

Hydrodynamics; Methods: numerical; Relativity; Stars: neutron; Stars: oscillations; Stars: rotation

Indexed keywords

GRAVITATIONAL EFFECTS; GRAVITY WAVES; NUMERICAL METHODS; RELATIVITY; ROTATION; STARS;

AXISYMMETRIC; COWLING APPROXIMATION; METHOD: NUMERICAL; NON LINEAR; PULSATION FREQUENCY; RELATIVISTIC STARS; SPACE-TIME DYNAMICS; STAR OSCILLATIONS; STARS: NEUTRONS; STARS: ROTATION;

HYDRODYNAMICS;

EID: 33744529158     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2006.10274.x     Document Type: Article

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