Observational Cosmology - Unit 3 Solutions

2. From the lecture 2 notes,  kc2/a2H2=Omega-1.  Given a(t)~t2/3, we have H=(da/dt)/a ~ t-1 .
Therefore aH~t-1/3, and so  Omega-1 ~ 1/(aH)2 ~ t2/3 ~ a .
Hence at z=1000, a=1/(1+z) is 1001 times smaller than at present, and so too is Omega-1.
If Omega-1 were 0.6 at the present, then it would have been only 0.0006 at z=1000, i.e. Omega would have been 0.9994, very close to unity.