Pressureless matter obeys the cosmological perfect-fluid continuity equation, . Integrating gives . Define the present critical density and cosmological density parameters byHere and the curvature contribution is an effective density parameter, not an additional matter fluid. Substitution into the Friedmann equation givesUsing the Hubble parameter therefore yieldsAt the same equation implies . The power in the matter term is ; the converted TeX's is an error not present in the original PDF.
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