Rotation of a fluid with rheological equation of state in special andgeneral theory of relativity.
Abstract
The rotation of a real fluid with a rheological equation of state is studied in the framework of special and general relativity with reference to the internal structure of pulsars (neutron stars) rotating at high velocity and consisting of a fluid contained between a massive core and a solid shell (the crust). Particular attention is given to the rotation of a fluid between two coaxial cylinders on the background of a Minkowski metric written in a cylindrical system of coordinates, and to the rotation of a fluid between two concentric spheres on the background of a Minkowski metric written in a spherical system of coordinates.
 Publication:

Trudy Kazanskaia Gorodkoj Astronomicheskoj Observatorii
 Pub Date:
 1983
 Bibcode:
 1983TrKaz..47..114T
 Keywords:

 Pulsars;
 Relativity;
 Rheology;
 Rotating Fluids;
 Rotating Plasmas;
 Stellar Rotation;
 Equations Of State;
 Minkowski Space;
 Relativistic Plasmas;
 Stellar Cores;
 Stellar Models;
 Stellar Structure;
 Astrophysics;
 Fluid Dynamics:Relativity;
 Relativity:Fluid Dynamics