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Note on solving for the dynamics of the Universe
1.V. Faraoni, “Solving for the dynamics of the universe,” Am. J. Phys. 67 (8), 732–734 (1999).
2.M. J. D. Assad and J. A. S. Lima, “General and unified solution for perfect fluid homogeneous and isotropic cosmological models,” Gen. Relativ. Gravit. 20, 527–538 (1988).
3.L. D. Landau and E. M. Lifshitz, The Classical Theory of Fields (Pergamon, Oxford, 1989), pp. 363–367.
4.R. D’Inverno, Introducing Einstein’s Relativity (Clarendon, Oxford, 1992), p. 322.
5.H. Stephani, General Relativity (Cambridge U.P., Cambridge, 1990), pp. 265–271.
6.Ya. B. Zeldovich and I. D. Novikov, Stars and Relativity (Dover, New York, 1996), pp. 186–187.
7.Actually, the case should be separately discussed because from (5) one has This means that the solution, is valid for all values of K. Taking the first integral as given by (7), the particular closed expansionist solution is lost.
8.J. A. S. Lima, Notes in Cosmology 1990 (in Portuguese, unpublished).
9.J. A. S. Lima, A. M. Moreira, and J. Santos, “Particle-like description for FRW cosmologies,” Gen. Relativ. Gravit. 30, 425–434 (1998).
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