On the postNewtonian approximation of the EinsteinCartanSciamaKibble theory.
Abstract
The postNewtonian approximation of the EinsteinCartanSciamaKibble or ECSK theory is developed. It is used to obtain a drastic reduction on the density of the source needed to detect the spin. It is also proved that if we know the structure of the source, up to order ̄v, the spin can be detected, and if we know it up to order ̄v^{2} the theory can be verified.
 Publication:

General Relativity and Gravitation
 Pub Date:
 July 1985
 DOI:
 10.1007/BF00763029
 Bibcode:
 1985GReGr..17..683C
 Keywords:

 Cartan Space;
 Newton Theory;
 Relativity;
 Spin;
 Stellar Rotation;
 Acceleration (Physics);
 Density Distribution;
 Field Theory (Physics);
 Particle Trajectories;
 Rotating Fluids;
 Stellar Structure;
 Torsion;
 Astrophysics;
 Gravitation Theory