Lecture Notes on the General Theory of Relativity pp 207-244 | Cite as
Cosmology
Chapter
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We will consider expanding homogeneous and isotropic models of the universe. We introduce an expanding frame of reference with the galactic clusters as reference particles. Then we introduce a “comoving coordinate system” in this frame of reference with spatial coordinates χ, θ φ. We use time measured on standard clocks carried by the galactic clusters as coordinate time (cosmic time).
Keywords
Hubble Parameter Vacuum Energy Critical Density Universe Model Expansion Factor
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