Testing dispersion relations of quantum κ-Poincaré algebra on cosmological ground

Following the procedure proposed recently by Martin and Brandenberger we investigate the spectrum of the cosmological perturbations in the case when the “trans-Plackian” dispersion relations are motivated by the quantum κ-Poincaré algebra. We find that depending on the choice of initial conditions of the perturbations, the spectrum either differs from the flat one for instantaneous Minkowski vacuum or, in the case of initial conditions minimizing energy density, leads to the observed scale-invariant Harrison–Zelʹdovich spectrum in the Friedmann epoch.