Abstract
The three lectures I presented at the NATO Advanced Study Institute 2000 covered the following topics: I. Cosmological Parameters, II. Cold Dark Matter Cosmology: Status and Open Questions, and III. Probing Galaxy Formation with High Energy Gamma-Rays. In this first lecture, the cosmological parameters that I will emphasize are the Hubble parameter H0 ≡ 100h km s-1 Mpc-1, the age of the universe t0, the average matter density Ωm, the baryonic matter density Ωb, the neutrino density Ωv, and the cosmological constant ΩΛ. The evidence currently favors t0 ≈ 13 Gyr, h ≈ 0.65, Ωm ≈ 0.4 ± 0.1, Ωb = 0.02h-2, 0.001 < Ωv < 0.1, and ΩΛ ≈ 0.7.
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Primack, J.R. (2001). Dark Matter and Large Scale Structure I.. In: Branco, G.C., Shafi, Q., Silva-Marcos, J.I. (eds) Recent Developments in Particle Physics and Cosmology. NATO Science Series, vol 34. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-0676-7_13
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DOI: https://doi.org/10.1007/978-94-010-0676-7_13
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