The JCDM model yields H0 of 66.95 plus or minus 0.51 km/s/Mpc and Omega_m of 0.3419 plus or minus 0.0065 in a flat universe, rising to H0 of 69.13 plus or minus 0.56 with slight positive curvature, fitting late-time data but struggling with full early-universe consistency.
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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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Cosmological constraints on the big bang quantum cosmology model
The JCDM model yields H0 of 66.95 plus or minus 0.51 km/s/Mpc and Omega_m of 0.3419 plus or minus 0.0065 in a flat universe, rising to H0 of 69.13 plus or minus 0.56 with slight positive curvature, fitting late-time data but struggling with full early-universe consistency.
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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.