From the Einstein-de Sitter cosmological model, the critical density of the universe(the density required for the universe to be closed to that expansion stops asymptotically at infinite time) is
where H is the Hubble constant and G is the gravitational constant.
The quantity is defined as
so a closed universe satisfies .
where H is the Hubble constant and G is the gravitational constant.
The quantity is defined as
so a closed universe satisfies .
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