- #36
marcus
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So now I can tell the energy density of the universe, in metric units, just from knowing the two Hubble rates
the present rate 2.20 attohertz
the longterm rate 1.83 attohertz
I just have to square them and take the difference and divide by 6.22
H2 - H∞2 = const ρ
(2.20^2 - 1.83^2)/6.22 this will give ρ in nanopascal---or more exactly in nanojoules per cubic meter
when I put that in google it gives back:
((2.20^2) - (1.83^2)) / 6.22 =
0.2397266881
So the present energy density of the universe (radiation, ordinary matter and dark matter mass energy equiv) is 0.24 nanopascal. Or 0.24 nJ per m3
And in the far distant future when the energy density has thinned out to almost zero, the righthand side will be zero. so the lefthand will be, which means that H will have to almost equal H∞
which we know it has to because that is what H∞ (essentially a way of expressing the cosmological constant) is. It is the longterm eventual value of the distance growth rate.
that is to say, an intrinsic, residual spacetime curvature.
the present rate 2.20 attohertz
the longterm rate 1.83 attohertz
I just have to square them and take the difference and divide by 6.22
H2 - H∞2 = const ρ
(2.20^2 - 1.83^2)/6.22 this will give ρ in nanopascal---or more exactly in nanojoules per cubic meter
when I put that in google it gives back:
((2.20^2) - (1.83^2)) / 6.22 =
0.2397266881
So the present energy density of the universe (radiation, ordinary matter and dark matter mass energy equiv) is 0.24 nanopascal. Or 0.24 nJ per m3
And in the far distant future when the energy density has thinned out to almost zero, the righthand side will be zero. so the lefthand will be, which means that H will have to almost equal H∞
which we know it has to because that is what H∞ (essentially a way of expressing the cosmological constant) is. It is the longterm eventual value of the distance growth rate.
that is to say, an intrinsic, residual spacetime curvature.
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