Simon Bridge said:
There are no observation on the "whole Universe", only that bit we can see, That is what the word "observable Universe" means. Therefore there is no way to tell if the whole Universe is bigger than what we see. How do you know that all we see is not all there is?
Do you really think that there is no way to tell if the universe is bigger than what we can see?
If current theory is correct, we can only see back to the time light could begin to travel freely, leaving us something like 380,000 years of expansion beyond the observable universe. What was the universe doing for that first 380,000 years?
According to this Wikipedia article (
http://en.wikipedia.org/wiki/Observable_universe#The_universe_versus_the_observable_universe) Alan Guth has an estimate for the size of the whole at 3x10^23 times the observable. I think it is about 10^243 times larger. The whole is much larger than what we can see, and I am sure you agree, despite this pedantic question.
Simon Bridge said:
How do you know that the Rest of the Universe is not infinite?
That comment treats infinity like a number. If the universe had a start, it cannot be infinite now. How big was the universe when it was half the current age, or a quarter, or one hundreth, etc? The universe had a start, and is growing still. It is big, but not infinite, because it cannot be infinite. Infinite implies it cannot grow more. What are you going to do, multiply infinity by two every time it doubles?
Simon Bridge said:
Please summarize the main points of the derivation for those who do not have access to the journal.
Carvalho starts out discussing the standard density solution, as a point of reference, showing the mass of the observable universe to be c^3/(GH). He then considers the case when the radius of the universe was about the size of the wavelength of an elementary particle.
$$R \sim l_p=\frac{\hbar }{m_\pi c}$$
The density should be the Planck density:
$$\rho =\frac{c^{5}}{G^{2}\hbar }$$
He then computes the mass inside the volume of R, which is $$\rho R^{3}$$
using the above two equations:
$$\rho R^{3}=\left( \frac{c^{5}}{G^{2}\hbar }\right) \left( \frac{\hbar }{%
m_{\pi }c}\right) ^{3}=\frac{c^{2}\hbar ^{2}}{G^{2}m_{\pi }^{3}}$$
He inserts the numerical values and gets about 1.5 x 10*52 kg
"which is of the order of the mass of the visible universe"
Then Carvalho uses a relation given by Weinberg (from his Gravitation and
Cosmology book):
$$m_{\pi }=\left( \frac{\hbar ^{2}H_{0}}{Gc}\right) ^{\frac{1}{3}}$$
He inserts that relation into $$\frac{c^{2}\hbar ^{2}}{G^{2}m_{\pi }^{3}}$$ to get:
$$\frac{c^{2}\hbar ^{2}}{G^{2}m_{\pi }^{3}}=\frac{c^{2}\hbar ^{2}}{%
G^{2}\left( \left( \frac{\hbar ^{2}H_{0}}{Gc}\right) ^{\frac{1}{3}}\right)
^{3}}= \frac{c^{3}}{GH_{0}}$$
which is the same mass derived by the standard density approach.
He does a bit more math and concludes: "We have seen that, from a very simple argument, a new derivation of the mass of the universe is possible which involves only microscopic quantities. This strengthens the idea that there must exsist a deep relation between the microscopic and the macroscopic world within a complete and unified theory of the forces of nature."
Simon Bridge said:
... and yet for everyone else it is trivial: an artifact of the calculation process..
Let me again try to get the point across... these constants give the observable mass, not the whole mass. To get the whole mass, we would have to multiply the observable mass equation by yet another value, probably a scaled up version of one of these constants, meaning at least one of the constants is scaled to the observable.
Simon Bridge said:
The reason the mass formulas come out as some nice combination of universal constants is because they all assume some simplicity in the symmetry of the Universe.
"assume some simplicity in the symmetry ..." what??
If the universe generates these constants, why is it that observable does it, and not the whole? One of these constants, at least, is scaled to the observable.