N-body simulations show degenerate effects of momentum exchange parameter β and scalar field slope λ on mean pairwise peculiar velocity and velocity dispersion in Type 3 dark energy models.
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Probing the Type 3 interacting dark-energy model using matter pairwise velocity
N-body simulations show degenerate effects of momentum exchange parameter β and scalar field slope λ on mean pairwise peculiar velocity and velocity dispersion in Type 3 dark energy models.