|
In this article, I intentionally open the proverbial 'can of worms' on the energy of the Universe. During a recent (lengthy) discussion[1] between jonmtkisco (Jon) and myself, we came to the preliminary conclusion that at least some of the energy components of the present observable universe are changing. It is almost as if energy is lost at certain times and gained at other times.
According to the present standard cosmological theory, an inflationary epoch imparted an enormous 'kinetic energy' of expansion upon the embryo universe. It also says that in the beginning there was no matter or radiation, just the energy of the 'false vacuum', brought about by a quantum fluctuation.
At around 10-32 seconds after 'time zero', a phase transition happened that converted a very small portion of the enormous expansion energy into radiation and matter. Immediately following inflation, radiation energy was the dominant form due to the astronomical density and temperature. Later other energy forms took over. What follows is a rather 'engineering-like' effort to quantify those energy components.
An Engineering Approach
Using simple Friedmann cosmological principles to calculate the evolution of the energy of the observable universe over time,[2] one can obtain at least order of magnitude values. Our 'purist' Physics Forum friends do not agree and they argue that General Relativity's Friedmann solution cannot be used to calculate the energy content of the universe at large.
They are probably right, but because we are not here looking at the universe as a whole, just the finite observable part, one can approximate the situation by rather simple considerations and learn quite a lot. This is an example of the 'engineering approach': good enough for practical purposes, whatever that may mean in cosmology.
Figure 1 shows the approximate static and expansion energies of the observable universe as log-log plots, stretching from the end of the inflation epoch (~10-41 years or ~10-32 seconds after 'time zero') into the distant future. We are now at ~1.4 x 1010 (14 billion) years and the curves are cut off at ~1012 (one trillion) years after the big bang.
The magnitudes may be out by an order of magnitude, but on 10100, does it matter?
Figure 1: 
Radiation Energy
In the beginning, both energy curves were totally dominated by radiation energy due to the immense temperature of ~1027 deg. Kelvin.[3] Due to the enormous expansion rate, the expansion energy was many orders of magnitude higher than the static energy. Both static and expansion energies got diluted due to the redshift that each photon suffered with the expansion. The expansion energy decreased more rapidly, because the expansion rate also dropped dramatically during this 'radiation epoch'.
Matter Energy
This 'loss of energy' lasted until at around 105 (100 thousand) years, when the total radiation energy was redshifted to below the total matter (ordinary and dark matter) energy level. In reality no energy was actually lost, because negative gravitational potential energy got less negative by an equal amount. This ensured a constant total energy for the observable universe – by Newtonian conventions, the total energy of the observable universe is zero.
Then followed a horizontal (constant energy) portion on the blue static energy curve. This indicates the next epoch: matter domination. Total matter energy is not redshifted by expansion, as far as we know. The red kinetic energy curve did not go horizontal at the same time as the static energy, because the expansion rate kept dropping, hence less expansion energy. Then, at around 5 billion years, the expanding universe entered the vacuum energy (or dark energy) epoch.
Vacuum Energy
Vacuum energy has a constant density, so the more the universe expands, the more total vacuum energy there is. Taken at face value, this would have rapidly decreased the expansion rate, because vacuum energy acts like a brake on expansion, just like any other form of energy. However, vacuum energy also has an anti-gravity (negative gravitational pressure) effect that accelerates the expansion of the universe.
The original inflationary expansion epoch is thought to have occurred as a very high 'false vacuum' energy content. This caused a runaway expansion that was somehow stopped by one or more phase transitions. The log-log graph seems to show that we are probably at the beginning of another runaway expansion epoch. The only difference is that in the beginning the inflationary time constant was something like 10-32 seconds, while today that time constant is a few billion years. Lucky for us!
The Ratio of Things
This brings us to the enormous difference there was between expansion energy and static energy right at after inflation. Hold your breath: the kinetic energy started out more than 40 orders of magnitude higher than the static (E=mc2) energy - yes, we are talking of a factor >1040. Unimaginable! Just goes to show how insignificant we (and the matter that we see around us) really are. If that ratio has changed by a little bit, the universe at large would not have noticed. But would we have noticed?
An Observation
So far, all was a bit of speculation and not pure science, but now for an interesting and technically sound observation. Vacuum energy is today taken as roughly 73% of the total rest energy, with ordinary plus dark matter making up about 27%. This gives the standard expansion curve like the red one in figure 2 below.
Figure 2: 
Note that the expansion rate (the slope of the red curve) has visibly increased in the recent past. The 'present' is indicated by the red dotted line, around 13.7 Gy, where the red curve reaches unity expansion factor. The change in slope of the red curve during the recent past made it possible for the Hubble telescope to detect the increasing expansion rate during the late 1990s.
A What If?
Now consider what would have happened if, instead of the observed ~30:70 energy split of today, nature conspired against us and made the energy split ~50:50. Not a big change, but this would have resulted in the green expansion curve, cutting the unity expansion factor line at about 11.5 Gy. The change in slope in the recent past would have been very small and hence difficult to detect with present technology.
I wonder how the cosmologists would have interpreted this almost linear expansion curve. Probably not by bringing in 'dark energy', or would they?
What do you think?
Jorrie
[1] http://cr4.globalspec.com/blogentry/2468/Age-and-Size-of-the-Universe. Jon and I don't quite agree om some points, but we got more or less to the gist of it.
[2] See this Relativity 4 Engineers web page for some of the math used. It is still a bread-board page, a work in progress, but for those interested, it has real nice equations and a little explanation.
[3] Smoot G, et. al, Wrinkles in Time, 1993, Abacus, London.
|
Users who posted comments:
BlueAussieBoy (3), bmorrow492 (1), cashman68bam (1), guitarhunter (2), Johnjohn (5), jonmtkisco (11), Jorrie (21), Roger Pink (2), StandardsGuy (3)