String fluid dynamical models in the Einstein-Cartan theory

Details String fluid dynamical models in the Einstein-Cartan theory String fluid dynamical models in the Einstein-Cartan theory

Mar 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999cqgra..16.1011s&link_type=abstract

Classical and Quantum Gravity, Volume 16, Issue 3, pp. 1011-1019 (1999).

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Using the general, energy-momentum tensor for a dynamical, string fluid developed from the Ray-Hilbert variational principle, physically motivated applications to Riemann-Cartan spacetime are given within the framework of the Einstein-Cartan theory. The string density is considered for the cases when it is or is not a thermodynamical variable of the fluid. Solutions are given for both cases and compared with other models in both general relativity and the Einstein-Cartan theory. The use of a string fluid as a contributer to galactic halo density is also discussed.

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