On the structure and stability of rapidly rotating fluid bodies in general relativity. I - The numerical method for computing structure and its application to uniformly rotating homogeneous bodies

Details On the structure and stability of rapidly rotating fluid bodies in general relativity. I - The numerical method for computing structure and its application to uniformly rotating homogeneous bodies On the structure and stability of rapidly rotating fluid bodies in general relativity. I - The numerical method for computing structure and its application to uniformly rotating homogeneous bodies

Feb 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976apj...204..200b&link_type=abstract

Astrophysical Journal, vol. 204, Feb. 15, 1976, pt. 1, p. 200-223. Research supported by the Louis Block Fund

Computer Science

Numerical Analysis

117

Neutron Stars, Relativistic Effects, Rotating Bodies, Stellar Models, Black Holes (Astronomy), Contraction, Kerr Effects, Maclaurin Series, Moments Of Inertia, Numerical Analysis, Radii, Rotary Stability, Stellar Evolution

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Abstract image available at:
http://adsabs.harvard.edu/abs/1976ApJ...204..200B

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