Abstract
An exact solution of Einstein's equation is stated in which the density (ϱ), pressure (p), scale factorS and metric coefficients are functions of only one dimensionless self-similar variable,ct/R, wheret is cosmic time andR is a co-moving radial coordinate. The solution represents a cosmology that begins as a static sphere having ϱ ∝R −2 and evolves into an expanding model which is pressure-free and has a hierarchical type of density law (ϱ ∝R −θ, approximately, with θ=a number, 0≤θ≤2). It is suggested that this model should supersede the previous models of Wesson and other workers, since it appears to be the simplest cosmology for a hierarchy.
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References
Barenblatt, G. E. and Zel'dovich, Ya. B.: 1972,Ann. Rev. Fluid Mech. 4, 285.
Bonner, W. B.: 1972,Monthly Notices Roy. Astron. Soc. 159, 261.
Cahill, M. E. and Taub, A. H.: 1971,Comm. Math. Phys. 21, 1.
Carrus, P. A., Fox, P. A., Haas, F. and Kopal, Z.: 1951,Astrophys. J. 113, 193, 496.
De Vaucouleurs, G.: 1970,Science 167, 1203.
Henriksen, R. N. and Wesson, P. S.: 1978a,Astrophys, Space Sci. 53, 429.
Henriksen, R. N. and Wesson, P. S.: 1978b,Astrophys. Space Sci. 53, 445.
Kopal, Z.: 1954,Astrophys. J. 120, 159.
Peebles, P. J. E.: 1974,Astrophys. Space Sci. 31, 403.
Podurets, M. A.: 1964,Soviet Astron. (A.J.) 8, 19.
Sedov, L. I.: 1949,Similarity and Dimensional Methods, Academic Press, London.
Wertz, J. R.: 1971,Astrophys. J. 164, 227.
Wesson, P. S.: 1975,Astrophys. Space Sci. 32, 273, 305, 315.
Wilson, A. C.: 1967,Astron. J. 72, 326.
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Wesson, P.S. General-relativistic hierarchical cosmology: An exact model. Astrophys Space Sci 54, 489–495 (1978). https://doi.org/10.1007/BF00639451
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DOI: https://doi.org/10.1007/BF00639451