Statistics – Computation
Scientific paper
Dec 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986acaps...6..208d&link_type=abstract
(Acta Astrophysica Sinica, vol. 6, 1986, p. 208-219) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 10, Dec. 1986, p.
Statistics
Computation
Computational Astrophysics, Equilibrium Equations, Gravitational Effects, Relativistic Effects, Stellar Rotation, Angular Velocity, Equations Of State, Hydrostatics, Red Shift, Self Consistent Fields, Stellar Mass
Scientific paper
In this paper, the equilibrium configurations of rapid rotating compact stars and some gravitational effects are studied within the general relativity by use of the Harrison-Wheeler equation of state and by the self-consistent field method. Numerical calculations show that the equilibrium configuration of a rotating star is a spheroid. For large spin velocities (greater than 300 per sec), the eccentricity and mass increase vary rapidly as the angular velocity increases; for the critical angular velocity of the rotating star, the eccentricity is about 0.7, the increase in mass is about 10-35 percent. The difference of the gravitational redshifts at the surface of the star caused by rotation, and the difference of the light bending when the beam moves in the direction of rotation or in the opposite direction are obvious.
Dong Jun
Sun Jing-Li
Zhu Pei-Chen
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