Lecture Note: Cosmology II
Termes manquants :
Early galaxy formation and its large-scale effectsStandard big bang nucleosynthesis production of H, He, Li, Be, and. B isotopes as a function of time, for the baryon density taken from WMAP7. The hot, early universe - Haus der AstronomieTdS = Td(sa3) = d(?a3) + Pda3. (2.8) ... properties than the classical theory: this particularity allows us to get rid of the Big Bang. Impacts of cosmic inhomogeneities on the CMBBig Bang. < 10-43 sec. ~infinity. All four forces (Gravity, Strong, Electromagnetic, and Weak) are united. Quantum Gravity Era. ~ 10-43 sec.
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