Non-linear pulsations in differentially rotating neutron stars: Mass-shedding-induced damping and splitting of the fundamental mode

Monthly Notices of the Royal Astronomical Society

Volumn 352, Issue 4, 2004, Pages 1089-1101

  Stergioulas, Nikolaos ^a   Apostolatos, Theocharis A ^b   Font, José A ^c  

^a ARISTOTLE UNIVERSITY OF THESSALONIKI   (Greece)

^b UNIVERSITY OF ATHENS   (Greece)

^c UNIVERSITY OF VALENCIA   (Spain)

Author keywords

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

Indexed keywords

DAMPING; EIGENVALUES AND EIGENFUNCTIONS; FOURIER TRANSFORMS; GRAVITATIONAL EFFECTS; GRAVITY WAVES; HYDRODYNAMICS; NEUTRONS; NUMERICAL METHODS; RELATIVITY;

COWLING APPROXIMATION; METHOD: NUMERICAL; NEUTRON STARS; NON LINEAR; SPLITTINGS; STAR OSCILLATIONS; STARS: MASS; STARS: NEUTRONS; STARS: ROTATION; TWO-DIMENSIONAL;

STARS;

EID: 4344697784     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2004.07973.x     Document Type: Article

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