Geometric properties of rotating stars in general relativity

Details Geometric properties of rotating stars in general relativity Geometric properties of rotating stars in general relativity

Oct 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998cqgra..15.3203k&link_type=abstract

Classical and Quantum Gravity, Volume 15, Issue 10, pp. 3203-3214 (1998).

Physics

1

Scientific paper

We prove precise a priori estimates from above for the equatorial radius, the mass and the angular momentum of a rotating star in general relativity, provided that the star is stationary and axisymmetric with perfect fluid matter satisfying the dominant energy condition and possesses an equatorial plane which is stable in the sense of minimal surfaces.

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