Abstract
For the region after the recombination era of the Universe the hydrodynamical density waves are analyzed including shear viscosity and heat conduction for ρ=ρc as well as for ρ<ρc(ρc is the critical density of the Universe). Very near to the end of the recombination era (z=1200) we find the well-known Jeans instability. It is shown that the influence of the shear viscosity on the instabilities in negligible, however, a visible influence of the bulk viscosity is present.
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References
Allen, C. W.: 1973,Astrophysical Quantities (3rd ed.), University of London, The Athlone Press, London.
Chapman, S. and Cowling, T. G.: 1970,The Mathematical Theory of Non-Uniform Gases, Cambridge University Press, Cambridge.
Corona-Galindo, M. G.: 1985, ‘Hydrodynamical Approach of Galaxy Formation on the Basis of a Fluid Model of Two and Three Components’, Konstanzer Dissertation.
Jeans, J.: 1928,Astronomy and Cosmogony, reprinted by Dover Publications, New York, 1961.
Lifshitz, E. M. and Pitaevskii, L. P.: 1981,Physical Kinetics, Pergamon Press, Oxford.
Nowotny, E. and Corona, M. G.: 1982,Astrophys. Space Sci. 84, 401.
Peebles, P. J. E. and Dicke, R. H.: 1968,Astrophys. J. 154, 891.
Simon, R.: 1970,Astron. Astrophys. 6, 151.
Simon, R.: 1971,Astron. Astrophys. 11, 161 (Erratum).
Weinberg, S.: 1972,Gravitation and Cosmology, J. Wiley and Sons, New York.
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Corona-Galindo, M.G., Dehnen, H. The jeans instability criterion for a compressible fluid including viscosity and heat conduction. Astrophys Space Sci 153, 87–94 (1989). https://doi.org/10.1007/BF00643614
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DOI: https://doi.org/10.1007/BF00643614