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Cosmology

Steady state.Λ > 0k = +1 ; no ΛExpands then recollapses. Spatially closed (finite).k = −1 ; no Λk = 0 ; Λ = 0Critical densityΛ > 0 ; Λ > |Gravity|William H. McCrea, 1930s

[ "Astronomy", "Astrophysics", "Quantum mechanics", "Cosmological constant", "Friedmann–Lemaître–Robertson–Walker metric", "Inflation (cosmology)", "Epic of evolution", "Cosmological perturbation theory" ]
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