bill alsept said:
Thanks, but I'm not sure if I follow. I am suggesting a system such as our universe does not always increase it's entropy. It may increase and decrease in the short run but stays the same in the long run. If it truly cycles then its entropy will always come back to where it started...
I think what you say here is absolutely right. There are several arguments to be made justifying LQG "bounce" cosmology on entropy grounds.
I am not a Loop cosmology expert (by any means!) and don't have time to write a long post right now. I will just try to suggest some of the reasoning, and get back to this later today.
This is a really interesting question!
1. One idea is that entropy of U is not well-defined right at the bounce.
2. The whole 2nd law business is meaningless unless you can define the entropy of the gravitational field because that is a BIG part of the total. The grav field means the geometry of the U. What is the entropy of geometry. People still working on that.
3. LQG quantizes GR (the modern law of gravity) and when it does so it turns out that at very high density quantum effects take over and gravity
repels instead of attracting!
This means that uniformly spread out geometry is favored.
But at ordinary density, gravity attracts, and clumpy geometry is favored.
Therefore at the bounce the entropy of U geometry cannot possible be well defined.
4. Right at that moment, density changes abruptly from the usual (attractive gravity) range up to the extreme (Planck scale) density range, and then in a split second changes back down into the usual range again. No consistent definition of the geometrical (i.e. grav. field) entropy is possible.
5. A fundamental requirement of the 2nd Law is an observer, who defines the macrostate regions of the phase space. What defines the observer's map of phase space is what the observer can see and measure. A region of microstates which all look the same to that observer is lumped together into a single macrostate. This necessarily assumes an observer. Coarsegraining requires a point of view.
But at the bounce there is no well-defined observer! There is only the "before" observer who looks forward to the bounce in his future, and the "after" observer for whom the bounce is the big bang beginning of his era, who looks back to it in the past.
At the very moment of the bounce it is not possible to define an observer.
6. I suspect that in the quantum regime right around the bounce, time itself may not be well defined. Normal distinctions between what is matter and what is geometry may be difficult to make. But that is just a matter for speculation at this point. In any case I think it would be a naive/simple-minded point of view to expect the 2nd to apply there in a straightforward manner. One still has not even defined what the terms and quantities mean there.