cesiumfrog said:
That's very interesting. There's obviously some truth to entropy being observer dependent, but to say it accounts for the problem of improbable state at the (worse: each) start of the universe is surprising.
I should have put a paragraph break in there. HE says entropy is observer dependent. But he does not apply that idea to bounce cosmology.
What follows is my continuation. It was MY suggestion that the second law is not being broken if no one can observe a violation.
BTW I wouldn't call the start of expansion an "improbable" state. It happens naturally in LQC models, both the analytical versions and the numerical simulations. Intuitively all structure melts---geometry and matter become indistinguishable and uniform.
The LQC also initiates inflation naturally.
What you call "improbable" turns out to be
inevitable---using this QG model. All I am pointing out is that it is not against the law.
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As I recall this is your field of research (or one of them.) Didn't you say you took part in the Sydney GR conference in 2007? If so (I could be mis-remembering) then you know the interesting and unintuitive fact that
the uniform gravitational field is the lowest entropy state.
It is just the opposite from, say, a gas. When the gas is all spread out, that's high entropy. It naturally wants to spread out. But when the gravitational field is uniform and even it means things haven't clumped yet, and they want to clump---so even and level is low entropy.
Intuitively, in a bounce, the crunch destroys clumps---so you start with a clean slate.
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Ashtekar (a familiar name

) has a paper about inflation in LQG. It might interest you. I'll get the link.
http://arxiv.org/abs/0912.4093
Loop quantum cosmology and slow roll inflation
Abhay Ashtekar, David Sloan
"In loop quantum cosmology the big bang is replaced by a quantum bounce which is followed by a robust phase of super-inflation. We show that this phase has an unforeseen implication: in presence of suitable inflationary potentials it funnels all dynamical trajectories to conditions which virtually guarantee a slow roll inflation with more than 68 e-foldings, without any input from the pre-big bang regime. This is in striking contrast to the situation in general relativity where it has been argued that the a priori probability of obtaining a slow roll inflation with N e-foldings is suppressed by a factor Exp(-3N)."