Physics
Scientific paper
Mar 1975
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975pthph..53..656n&link_type=abstract
Progress of Theoretical Physics, Vol. 53, No. 3, pp. 656-670
Physics
2
Scientific paper
The previous formalism for dealing with the average effect of a highly supersonic turbulent gravito-hydrodynamic field in the hadron era of the universe is extended so as to take into consideration various dissipative processes in the hadronic substratum. After a phenomenological fixation of the coefficients of bulk viscosity, shear viscosity and heat conduction, it is shown that those dissipative processes have a considerable influence upon the three characteristic mean-value quantities (at the bounce epoch of our regular model-universe) corresponding to metric, velocity and density fluctuations. A possibility of fixing the dissipation coefficients of the hadronic matter under consideration, i.e., the one based on the concept of statistical bootstrap, in a more well-founded manner is also conjectured.
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