Colour-Spin, Dilaton-Spin and Hypermomentum Perfect Fluids as the Sources of non-Riemannian Cosmologies

Details Colour-Spin, Dilaton-Spin and Hypermomentum Perfect Fluids as the Sources of non-Riemannian Cosmologies Colour-Spin, Dilaton-Spin and Hypermomentum Perfect Fluids as the Sources of non-Riemannian Cosmologies

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998tx19.confe.171b&link_type=abstract

Abstracts of the 19th Texas Symposium on Relativistic Astrophysics and Cosmology, held in Paris, France, Dec. 14-18, 1998. Eds.:

Astronomy and Astrophysics

Astrophysics

Scientific paper

We consider the perfect fluid with intrinsic degrees of freedom, namely, the perfect colour-spin, dilaton-spin and hypermomentum fluids as the sources of the possible non-Riemannian spacetime structure. We develop the variational theories of the perfect fluids with intrinsic degrees of freedom on accounting the constraints in the Lagrangian density of the fluids with the help of Lagrange multipliers and taking into account the corresponding underlying geometrical structure. As a result we derive the expressions for the energy-momentum tensors. The consequences of the employing of these energy-momentum tensors to the development of early stage Universe models are investigated.

Affiliated with

Also associated with

No associations

Rating

Colour-Spin, Dilaton-Spin and Hypermomentum Perfect Fluids as the Sources of non-Riemannian Cosmologies 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 Colour-Spin, Dilaton-Spin and Hypermomentum Perfect Fluids as the Sources of non-Riemannian Cosmologies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Colour-Spin, Dilaton-Spin and Hypermomentum Perfect Fluids as the Sources of non-Riemannian Cosmologies will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-767881