ONCE upon a TIME in the UNIVERSE

Those 26 seconds that seem like eternity.

Those 26 seconds that will decide which theory lives, or dies.

Those 26 seconds where only the interstellar wind can stop the emptiness.

Those 26 seconds before a parameter falls onto the ground to be forgotten.

LMU & CP-3 proudly presents a MATHEMATICA FILM directed by FELIX BERKHAHN, DENNIS D. DIETRICH, STEFAN HOFMANN, FLORIAN KÜHNEL and PARVIN MOYASSARI story by and of THE UNIVERSE starring THE COLOURED DOTS and "RUNNING-T"

This movie presents a stability scan of the deformation's (eq. (4) in arXiv:1106.3566) parameter space over the entire cosmological expansion history for earlier and earlier times. Concretely, for a given value of the earliest time t_min, the parameter plot shows the stability analysis of the deformed gravitational wave theory for the time interval [t_min ,∞]. Here t_min decreases gradually from  10³H₀^-1 to 10^-10H₀^-1. One can see that there is always a region (the green area) in which the deformed theory is strictly stable. For details, in particular about the deformation parameters α, β, see the paper arXiv:1106.3566