A Numerical Method of Studying the Evolution of Spherically Symmetric Superdense Celestial Bodies

Details A Numerical Method of Studying the Evolution of Spherically Symmetric Superdense Celestial Bodies A Numerical Method of Studying the Evolution of Spherically Symmetric Superdense Celestial Bodies

Oct 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ap.....37..372g&link_type=abstract

Astrophysics, Vol. 37, NO.4/OCT-DEC, P.372, 1994

Astronomy and Astrophysics

Astrophysics

Scientific paper

For fully relativistic strong gravitational fields we obtain a
consistent set of hydrodynamic and field equations that describe the
propagation of all types of waves in matter (from small perturbations to
shock waves). We obtain an algorithm for numerical solution of these
equations for certain equations of state of degenerate matter.

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