Equilibrium and stability of rotating stellar cores with finite entropy

Details Equilibrium and stability of rotating stellar cores with finite entropy Equilibrium and stability of rotating stellar cores with finite entropy

Jan 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981a%26a....93..395g&link_type=abstract

Astronomy and Astrophysics, vol. 93, no. 1-2, Jan. 1981, p. 395-402. Deutsche Forschungsgemeinschaft

Astronomy and Astrophysics

Astrophysics

4

Entropy, Equilibrium Equations, Stellar Cores, Stellar Rotation, Supermassive Stars, Gravitational Collapse, Pulsars, Rotary Stability

Scientific paper

The stability of rapidly rotating stellar cores of evolved massive stars having finite entropy is tested. Maclaurin spheroids are used to describe the mechanical equilibrium and stability. Adopting a realistic equation of state generalized Chandrasekhar limits as functions of angular momentum are obtained for specific entropies and electron concentrations taken from advanced stellar evolution calculations. The significance of the results for pulsar formation and gravitational radiation bursts is stressed.

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