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Ramo
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Austin, Texas, USA
Oct 1999 time: 23:37
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quote: What does R(t) mean? Is t any arbitrarily point? |
R is the scale factor of the line element of the constant time hypersurface of the metric for a homogenous, isotropic universe.
Your metric looks somethign like this:
ds^2 = -dt^2 + R^2(h_ij)dx^i*dx^j
It's important because well...
When the universe was radiation dominated, rho*R^4 was a constant, when it's matter domianted, rho*R^3 is a constant (take the covariant derivitive of the energy momentum tensor for a perfect fluid, etc., etc.). So, we're only talking about the second regime. So, if you plug in your metric and the previously mentioned expression for density, into Einstein's equations, you eventually get some expression for R which I can't possibly remeber.
Anyways, you can relate luminosity with distance, and eventually get an expression for Hubble's constant, H = R'(t)/R(t). So, you'd be able to find out an expression for R if you happened to know H. So I think there's some missing info on question 1.
For question 2, you can, through adiabatic expansion, say that the microwave background ratiation temperature is inversely proportional to R. So, you'd need the answer to question 1 for that, and thus be able to say T(t1)/T(t0) = R(t0)/R(t1). And you plug the T(t1) into the equation you posted to get t1.
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Vince278
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quote: Originally posted by Sava
lies
none of this was in the bible |
"The universe was without form..."
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All times are GMT. The time now is 05:37. Apolyton Time is 00:37. |
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