Figure. 3. The cumulative distribution function F(R, t0) in (6) as function of t0 for values of R = 1, 2, 3, 4…, illustrating that for values of R greater than R ≈ 5, the function F(R, t0) is well approximated by the function F(t0) = 1 – exp (-t0 ) in (7)

From

Is CMB just an Observational Effect of a Universe in Accelerated Expansion?

Arne Bergstrom

International Journal of Physics. 2013, 1(6), 133-137 doi:10.12691/ijp-1-6-1