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Derive the relationship between the deceleration parameter q0 and the cosmological density parameter (z = 0) in: (1) a matter-dominated Universe ( = R =
Derive the relationship between the deceleration parameter q0 and the cosmological density parameter (z = 0) in: (1) a matter-dominated Universe ( = R = 0); (2) a radiation-dominated Universe ( = M = 0); (3) a Universe with both matter and vacuum energy densities.
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