- #1

jarekd

- 111

- 2

Not everyone likes the idea of Universe created from a point singularity, so recently grows in popularity the cyclic model - that our Universe will finally collapse and use obtained momentum to bounce (so-called Big Bounce) and become the new Big Bang.

One might criticize that we "know" that universe expansion is accelerating. But it is believed to be pushed away by "dark energy", so accordingly to energy conservation, this strength should decrease with volume: like 1/R^3 ... while attracting gravity weakens like 1/R^2 and so should finally win - leading to collapse.

But it seems there is a problem with the second law of thermodynamics here - on one hand entropy is said to be always increasing toward the future, on the other Big Bangs should intuitively 'reset the situation' - start new entropy growth from minimum.

I wanted to collect the possible approaches to handling this problem and discuss them - here is a schematic picture of the basic ones I can think of (to be extended):

http://dl.dropbox.com/u/12405967/cyclicun.jpg

The age of thermal death means that there are nearly no changes, because practically everything is in thermodynamical equilibrium, most of stars have extinguished.

1) The second law is sacred - succeeding Big Bangs have larger and larger entropy,

2) It is possible to break 2nd law, but only during the Great Bounce,

3) It is possible to break 2nd law in singularities like black holes - the Universe may be already in thermal death, while the entropy slowly "evaporates" with black holes (I think I've heard such concept in Penrose lecture in Cracow),

4) The second law of thermodynamics is not fundamental, but effective one - physics is fundamentally time/CPT symmetric. So Big Bounce is not only single Big Bang, but from time/CPT symmetry perspective, there is also second BB-like beginning of Universe reason-result chain in reverse time direction. The opposite evolutions would finally meet in the extremely long central thermal death age, which would probably destroy any low-entropic artifacts.

Personally,

I see 1) as a total nonsense - thermal death is near possible entropy maximum (like lg(N)).

Also 3) doesn't seem reasonable - hypothetical Hawking radiation is kind of thermal radiation - definitely not ordering energy (decreasing entropy), but rather equilibrating degrees of freedom - leading to thermalization of the Universe.

2) sounds worth considering - physics doesn't like discontinuities, but Big Bounce is kind of special - crushes everything, resetting the system.

And 4) seems the most reasonable, but requires accepting that thermodynamical time arrow is not fundamental principle, but statistical effect of e.g. low entropic BB-like situation: where/when everything is localized in small region.

Assuming our universe will eventually collapse, which thermodynamical scenario seems most reasonable? Why?

Perhaps above list requires expansion?

Did Universe started in a point, or maybe something ends - something begins?

One might criticize that we "know" that universe expansion is accelerating. But it is believed to be pushed away by "dark energy", so accordingly to energy conservation, this strength should decrease with volume: like 1/R^3 ... while attracting gravity weakens like 1/R^2 and so should finally win - leading to collapse.

But it seems there is a problem with the second law of thermodynamics here - on one hand entropy is said to be always increasing toward the future, on the other Big Bangs should intuitively 'reset the situation' - start new entropy growth from minimum.

I wanted to collect the possible approaches to handling this problem and discuss them - here is a schematic picture of the basic ones I can think of (to be extended):

http://dl.dropbox.com/u/12405967/cyclicun.jpg

The age of thermal death means that there are nearly no changes, because practically everything is in thermodynamical equilibrium, most of stars have extinguished.

1) The second law is sacred - succeeding Big Bangs have larger and larger entropy,

2) It is possible to break 2nd law, but only during the Great Bounce,

3) It is possible to break 2nd law in singularities like black holes - the Universe may be already in thermal death, while the entropy slowly "evaporates" with black holes (I think I've heard such concept in Penrose lecture in Cracow),

4) The second law of thermodynamics is not fundamental, but effective one - physics is fundamentally time/CPT symmetric. So Big Bounce is not only single Big Bang, but from time/CPT symmetry perspective, there is also second BB-like beginning of Universe reason-result chain in reverse time direction. The opposite evolutions would finally meet in the extremely long central thermal death age, which would probably destroy any low-entropic artifacts.

Personally,

I see 1) as a total nonsense - thermal death is near possible entropy maximum (like lg(N)).

Also 3) doesn't seem reasonable - hypothetical Hawking radiation is kind of thermal radiation - definitely not ordering energy (decreasing entropy), but rather equilibrating degrees of freedom - leading to thermalization of the Universe.

2) sounds worth considering - physics doesn't like discontinuities, but Big Bounce is kind of special - crushes everything, resetting the system.

And 4) seems the most reasonable, but requires accepting that thermodynamical time arrow is not fundamental principle, but statistical effect of e.g. low entropic BB-like situation: where/when everything is localized in small region.

Assuming our universe will eventually collapse, which thermodynamical scenario seems most reasonable? Why?

Perhaps above list requires expansion?

Did Universe started in a point, or maybe something ends - something begins?

Last edited by a moderator: