The perfect-fluid tensor in the non-symmetric theory of gravitation

Details The perfect-fluid tensor in the non-symmetric theory of gravitation The perfect-fluid tensor in the non-symmetric theory of gravitation

May 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985cqgra...2..409v&link_type=abstract

Classical and Quantum Gravity (ISSN 0264-9381), vol. 2, May 1, 1985, p. 409-418. Research supported by the Natural Sciences and

Physics

10

Gravitation Theory, Ideal Fluids, Relativity, Tensors, Conservation Equations, Equations Of State, Euler Equations Of Motion, Variational Principles

Scientific paper

The perfect-fluid energy-momentum tensor in the non-symmetric gravitation theory (NGT) is derived using a fluid variational technique. Two different approaches are used. The first involves conservation of rest mass as a fundamental fluid constraint in the total Lagrangian while the second involves the assumption of an equation of state P = P(rho sub zero). The relativistic fluid conservation equation and the Euler equation of motion for NGT are obtained using the derived fluid tensor.

Affiliated with

Also associated with

No associations

Rating

The perfect-fluid tensor in the non-symmetric theory of gravitation does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The perfect-fluid tensor in the non-symmetric theory of gravitation, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The perfect-fluid tensor in the non-symmetric theory of gravitation will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1631759