Cosmological parameters: Do we already know the final answer

نویسنده

  • MICHAEL ROWAN - ROBINSON
چکیده

Some of the arguments which support the strong concensus for an Ωo = 0.3, λo = 0.7 model are reexamined. Corrections for Malmquist bias, local flow and metallic-ity suggest a revised value for Ho of 63 ± 6 km/s/Mpc, improving the age problems for an Ωo = 1 universe. The latest CMB results may require a high baryon density and hence new physics, for example a strong lepton asymmetry. Difficulties for the Ωo = 1 model with cluster evolution, the baryon content of clusters, and the evidence from Type Ia supernovae favouring low Ωo, Λ > 0 models, are discussed critically.

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تاریخ انتشار 2001