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In the introductory part, the shape of the cosmic expansion parabola and 'tear drop' shape of the observable universe were shown. The parabola depends on the expansion model used - in this case the so-called "Einstein-De Sitter" model, which is a universe with enough matter to make it 'flat', with no cosmological constant.
The 'expansion law' of the Einstein-De Sitter model is particularly simple, given by:

where dt is a time differential, a the expansion factor and H0 the Hubble constant. The expansion factor is a linear scalar that today has the value a = 1. At the Big Bang, a = 0 and when the observable universe was half as large as it is now, a was 0.5.
This equation can be easily integrated against time, from t = 0 to t, to get:

which can be used to get the age of the "Einstein-De Sitter universe". In the days when it was believed that H0 = 50 km/s/Mpc, this gave an age of the universe of about 13 Gy. (A Mpc is about 3.2 million light-years).
Surprisingly, this is more or less the age that cosmologists agree upon today, except that it is coming from a different value for H0 (about 72 km/s/Mpc) and a very different model! In the coming parts of this mini-series, the reasons why a different model was required will be discussed.
PS. I am taking a long-weekend, away from projects and computers. Will be back on Tuesday 24th. If you have questions, I'll attempt answers them then! The equations obviously come from Relativity 4 Engineers (where else? )
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