What is the required value for the density parameter ($\Omega_0$) that corresponds to a perfectly flat universe?

Answer

$\Omega_0 = 1$

A perfectly flat geometry occurs when the actual mass-energy density exactly matches the critical density required to balance expansion, resulting in the density parameter being equal to one.

What is the required value for the density parameter ($\Omega_0$) that corresponds to a perfectly flat universe?
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