Figure 3. Sampled (108 histories) energy spectra S(ω) as in Figure 2 for (A) a Gaussian distribution (stars transparent), (B) a Planck distribution (stars opaque, exponentially accelerated expansion), and (C) a Planck-type distribution with distorted tail (stars opaque, but no accelerated expansion)

From

Dark Energy, Exponential Expansion, CMB, Wave/Particle Duality All Result from Lorentz-Covariance of Boltzmann’s Transport Equation

Arne Bergstrom

International Journal of Physics. 2014, 2(4), 112-117 doi:10.12691/ijp-2-4-4