Table 1 The exact form of functions used to define models 1–9.
From: Supernova Ia observations in the Lemaître-Tolman model
Model | Pair of functions |
|---|---|
model 1 | t B = 0; ρ/ρ b = 0.5 + 0.2 cos(10-5πrMpc-1) + 0.5 cos2(10-5πrMpc-1) |
model 2 | t B = 0; ρ/ρ b = 0.4 + 0.6 cos(2 × 10-5πrMpc-1) + 1.8 cos2(2 × 10-5πrMpc-1) |
model 3 | t B = 0; ρ/ρ b = 1 + 0.4 cos(10-5πrMpc-1) |
model 4 | t B = 0; ρ/ρ b = 1 + (8 × 10-6rMpc-1)0.55 |
model 5 | ρ/ρ b = 1; |
H/H0 – not an analytic functions, see Fig. 4.1.2 | |
model 6 | t B = 0; H/H0 = 1 |
model 7 | as in model 1 |
model 8 | as in model 2 |
model 9 | as in model 3 |