Post-Newtonian Equilibrium Configurations of Rotating Polytropes

Details Post-Newtonian Equilibrium Configurations of Rotating Polytropes Post-Newtonian Equilibrium Configurations of Rotating Polytropes

Oct 1972

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1972ap%26ss..18..437m&link_type=abstract

Astrophysics and Space Science, Volume 18, Issue 2, pp.437-448

Astronomy and Astrophysics

Astrophysics

5

Scientific paper

Post-Newtonian equations are solved numerically for stellar models with a polytropic pressure-density relation for the case of uniform rotation, no meridional currents, and axial symmetry. The solution is obtained by following Stoeckly's numerical technique. Parameters characterizing the critical configuration are determined and compared with the values obtained recently by Fahlman and Anand, who followed Chandrasekhar's series expansion method.

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