Classical solutions in five dimensional induced matter theory and its relation to an imperfect fluid

Details Classical solutions in five dimensional induced matter theory and its relation to an imperfect fluid Classical solutions in five dimensional induced matter theory and its relation to an imperfect fluid

1996-05-07

arxiv.org/abs/gr-qc/9605012v1

Int.J.Mod.Phys. A11 (1996) 5495-5504

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

16 pages, latex, no figures

Scientific paper

10.1142/S0217751X96002510

We study five dimensional cosmological models with four dimensional hypersufaces of the Bianchi type I and V. In this way the five dimensional vacuum field equations $\rm G_{AB} = 0$, led us to four dimensional matter equations $\rm G_{\mu\nu}=T_{\mu\nu}$ and the matter is interpreted as a purely geometrical property of a fifth dimension. Also, we find that the energy-momentum tensor induced from the fifth dimension has the structure of an imperfect fluid that has dissipative terms.

Affiliated with

Also associated with

No associations

Rating

Classical solutions in five dimensional induced matter theory and its relation to an imperfect fluid 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 Classical solutions in five dimensional induced matter theory and its relation to an imperfect fluid, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Classical solutions in five dimensional induced matter theory and its relation to an imperfect fluid will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-80580