Evolution of scale factor for a Lemaitre model close to the "loitering" condition where
matter's pull and the vacuum's push are nearly balanced. The condition is
found by setting both da/dt and d2a/dt2 to zero.
The condition is: k = 1 - (v + m) = -3/2 (2 v m2)1/3. Just one example is plotted
from close to the loitering sequence. It has m = 0.3 and v = 1.71 and an age of 3.6 tH. To achieve significantly longer ages than tH requires fine tuning. Notice also
that in these kinds of models we always live at a rather special time just before a rapid exponential runaway. This arises because of demanding a current Hubble constant which is
significant.
Figure made for this website.
Include figure 7.7 in Longair (or the equivalents from Carroll et al)
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