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had recognized the expansion of the universe by late 1920s. He can be excused for making this mistake because astronomical observation in earlier time indicated a homogeneous distribution of objects in the sky and the view did not seem to change over "long" time. It induced him to assume a constant density in Eq.(18a). Simple mathematics as well as from solution of the equation§ shows that such model describes an expanding universe. In order to avoid this "unwanted" predicament, he introduced a repulsive term = 4 G /c2 to make d2R/dt2 = 0. The additional term would make dR/dt = 0 as well ifk = 4 G R2/c2 or k = R2. Thus, R = R0 = constant (see mathematical detail). However, this universe is unstable. A small perturbation would induce collapse or expansion forever. With the discovery of |
Figure 10l1 Einstein and His Cosmic Blunder |
cosmic acceleration, it is fashionable again to re-introduce the cosmological constant back into the model universe. The crucial difference is that we now know the density is not a constant; it varies with time as the universe expands. The two terms on the right-hand side of Eq.(20f) equal to each other only momentarily about 8 billion years after the Big Bang. |

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Figure 10l2 |
Figure 10l3 Hubble Tension [view large image] |
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= constant is:
(R0/2)eHt (as t
), the minimum size Rmin = R0;
(R0/2)eHt (as t
), the minimum size Rmin = 0;
G
/3)1/2, and R0 = (3|k|c2/8
G
)1/2 (for k
0), otherwise R0 = R(t = 0) (for k = 0).