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2.2. Dynamics of the Friedmann model

Let us now turn to the second assumption which determines the dynamics of the universe. When several non interacting sources are present in the universe, the total energy momentum tensor which appear on the right hand side of the Einstein's equation will be the sum of the energy momentum tensor for each of these sources. Spatial homogeneity and isotropy imply that each Tba is diagonal and has the form Tba = dia [rhoi(t), - Pi(t), - Pi(t), - Pi(t)] where the index i = 1, 2,..., N denotes N different kinds of sources (like radiation, matter, cosmological constant etc.). Since the sources do not interact with each other, each energy momentum tensor must satisfy the relation Tb;aa = 0 which translates to the condition d (rhoi a3) = - Pi da3. It follows that the evolution of the energy densities of each component is essentially dependent on the parameter wi ident (Pi / rhoi) which, in general, could be a function of time. Integrating d (rhoi a3) = - wi rhoi da3, we get

Equation 19 (19)

which determines the evolution of the energy density of each of the species in terms of the functions wi(a).

This description determines rho(a) for different sources but not a(t). To determine the latter we can use one of the Einstein's equations:

Equation 20 (20)

This equation shows that, once the evolution of the individual components of energy density rhoi(a) is known, the function H(a) and thus the line element in equation (13) is known. (Evaluating this equation at the present epoch one can determine the value of k; hence it is not necessary to provide this information separately.) Given H0, the current value of the Hubble parameter, one can construct a critical density, by the definition:

Equation 21 (21)

and parameterize the energy density, rhoi(a0), of different components at the present epoch in terms of the critical density by rhoi(a0) ident Omegai rhoc. [Observations [49, 50] give h = 0.72 ± 0.03 (statistical) ± 0.07 (systematic)]. It is obvious from equation (20) that k = 0 corresponds to Omegatot = sumi Omegai = 1 while Omegatot > 1 and Omegatot < 1 correspond to k = ± 1. When Omegatot neq 1, equation (20), evaluated at the current epoch, gives (k / a02) = H02(Omegatot - 1), thereby fixing the value of (k / a02); when, Omegatot = 1, it is conventional to take a0 = 1 since its value can be rescaled.

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