Numerical study of rotating relativistic stars

Details Numerical study of rotating relativistic stars Numerical study of rotating relativistic stars

Aug 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975pans.procq....w&link_type=abstract

Meeting phys. astrophys. neutron stars black holes, Varenna, Italy, 14 July 1975, 54 p.

Astronomy and Astrophysics

Astrophysics

Gravitational Collapse, Relativity, Stellar Rotation, Equilibrium Equations, Gravitational Fields, Magnetic Stars, Neutron Stars, Quasars

Scientific paper

The equations of structure for rotating stars in general relativity are presented and put in a form suitable for computer calculations. The results of equilibrium calculations for supermassive stars, neutron stars and magnetically supported stars are reported, as are calculations of collapsing, rotating, and magnetized stars in the slowly changing gravitational field approximation.

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