my2cts said:
What a mistake. I bet you don't have a reference for this to a real scientific paper or textbook.
So are you saying you dispute that P = 2/3 E/V for both degenerate and ideal gases? Goodness, I thought we had established that a long time ago. So if you realize that expression is correct, just ask yourself this: does the "magic wand" that makes the electrons distinguishable change the E, or the V, or neither? Of course, the answer is
neither, so nothing happens to P at first. It's just obvious, it's very hard to find references for statements of basic math. Of course, I already said that things will begin to evolve over a radiative diffusion time.
What would happen is that all the extra energy that was required by PEP now becomes available as thermal energy.
What happens is just what I said-- nothing at all to the pressure, but a big jump in temperature.
The star would suddenly become much hotter, gravitationally implode under emission of huge amounts of radiation and explosively reject its outer parts.
If you reread my last post, you will find a more careful accounting of the timescales here.
Yes--
eventually. But not for quite a long time, and certainly not on a sound crossing time, as I said above. The star will need to wait for many radiative diffusion times in order to lose that energy that is now freed up. But this is all what I stressed above-- the primary effects of the PEP are on
heat transport. You are only repeating what I already said, but exaggerating how quickly it would happen.
What would happen is the extreme opposite of "almost nothing".
Again, if you would quote me, it is important to quote my
entire statement, or you will miss the important parts, as you have done here. You have missed the
timescales involved.