Galaxy pairwise peculiar velocities from Cosmicflows-4 yield M_ν = 0.24^{+0.34}_{-0.18} eV and η² = 2.14^{+0.30}_{-0.32} (7σ non-zero asymmetry) in the CMB framework, consistent with prior Planck results.
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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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Measuring neutrino mass and asymmetry through galaxy pairwise peculiar velocity
Galaxy pairwise peculiar velocities from Cosmicflows-4 yield M_ν = 0.24^{+0.34}_{-0.18} eV and η² = 2.14^{+0.30}_{-0.32} (7σ non-zero asymmetry) in the CMB framework, consistent with prior Planck results.
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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.