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A Classical Calculation Shows That the Critical Mass Density of the Universe

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A classical calculation shows that the critical mass density of the universe is given by A classical calculation shows that the critical mass density of the universe is given by   where H is the Hubble constant and G is the gravitation constant. If the density is below this value, the universe will expand forever, whereas if it is above this value the universe will eventually stop expanding and collapse. Approximately how many hydrogen atoms per m<sup>3</sup> is the critical density equivalent to? A)  4 B)  40 C)  400 D)  4000 E)  40,000 where H is the Hubble constant and G is the gravitation constant. If the density is below this value, the universe will expand forever, whereas if it is above this value the universe will eventually stop expanding and collapse. Approximately how many hydrogen atoms per m3 is the critical density equivalent to?


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