There was lots of radiation, and lots of very fast moving elementary particles (which you might want to call "matter" - it's a matter of taste

). If you were to stick a chunk of, say, iron in there, it would vaporize almost instantaneously into a cloud of very energetic photons, quarks, electrons, gluons, etc.
Ah ok, I had thought that it was purely radiation, that makes more sense to talk about heat then.
And yes, all that energy couples to gravity (gravity acts on all forms of energy, democratically).
I was trying to get MM to acknowledge that for his bomb thought experiment, which he's abandoned now I guess
As for this issue of net zero energy:
...
In a closed universe, the energy is strictly zero, because the "sphere at infinity" actually has zero size, and so there's nowhere for the flux to escape. But closed universes can have plenty of matter and energy in them, can be hot, etc. Ergo, the gravitational contribution to the total energy is negative definite - which is no surprise at all, as the same thing is true in Newtonian gravity.
In a flat or open universe I don't know a good way to define a conserved, non-zero energy (because no matter how big the sphere is there is always energy flowing in or out).
And we don't know if the universe is open or closed.
As usual the real answer is "it depends" and "it's more complicated than that" lol.. thanks!
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So MM, you didn't respond to anything but the first part of my post, so I'll post it again so you don't have to scroll back.
If I have an electron and a proton (or whatever you want), and the closer I bring them together, the attractive force between them increases right?
Do you agree with Coulomb's law?
[latex]$$ F=k_e\frac{q_1q_2}{r^2} $$[/latex]
As r approaches zero, what's going to happen to the force? What's the upper limit of that attraction? You can't produce one for the Casimir effect, but you should be able to do so for this since this is your home turf so to speak.
Hypothetically it approaches infinity, do you agree?
How is this any different than the formula for pressure? What do you think happens to the pressure as the distance between the plates goes to zero, if the distance is in the denominator? In an ideal situation with impossibly flat and impossibly parallel and impossibly close plates?
Nah. The folks that wrote the WIKI article and created the images on the Casimir effect got it right. This negative pressure in a vacuum is almost exclusive limited to your group. Most scientists I meet seem to have a better grasp of QM than this crew.
Here again you agree with the wiki article for the Casimir effect.
Let me ask again, for the dozenth time or something, what is the sign for pressure in this forumula?
[latex]$$ \frac{F_c}{A}=-\frac{\hbar c \pi^2}{240a^4} $$[/latex]
If you disagree with the derived formula, at which point does the derivation go wrong in your opinion?
What textbook *besides on related to Lambda-CDM theory* claims that a vacuum contains "negative pressure".
Well the wiki article you say is written by people that got it right claims it. What's the sign on the formula above?
Actually, in the case of the Casimir article, the WIKI presentation was correct. Only your crew seems to be incapable of distinguishing between a QM "force" and pressure and not being able to recognize that there is *force* on both sides of the plates.
And according to the crew that wrote the wiki article, what's the sign on the formula above?