van gogh
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can anyone explain how universe will end
I think he meant that the pressure of the vacuum due to the cosmological constant is equal to the negative of its density (x c2); it is three times as big (and the reverse sign) as the pressure of a photon gas of equivalent density.A cosmological constant with the right sign makes the energy density of the vacuum positive, but makes its pressure negative - and 3 times as big.
I don't know if it's exactly a subset--the Big Rip scenario says that the expansion rate goes to infinity in a finite time, which is a type of final singularity (though different from singularities with infinite density obviously).Chronos said:We will all be dead, so who cares? Seriously though, Harmony gives the three basic options [the Big Rip is a subset of eternal expansion].
Inflationary theory predicts the universe should be extremely close to flat.Chronos said:What is truly curious is how close the universe appears to being absolutely flat. There is no entirely satisfactory explanation for that apparent fact. It's like a coin flip that lands on its edge.