Hamiltonian Fluids in Bianchi Universes

Details Hamiltonian Fluids in Bianchi Universes Hamiltonian Fluids in Bianchi Universes

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002nmgm.meet..798t&link_type=abstract

"THE NINTH MARCEL GROSSMANN MEETING On Recent Developments in Theoretical and Experimental General Relativity, Gravitation and R

Physics

Scientific paper

By using the integrand factors method we put enlightening on two particular problems :
• to classify dissipative cosmological solutions which preserve the isotropy and the homogeneity;
• to explore easily the consequences of an stress-energy tensor possessing anisotropic pressure which depends non linearly on the expansion parameter, and to show that the associated shear pass through a maximum and vanishes assymptotically.

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