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Why does the low entropy at the big bang require an explanation? (cosmological arrow of time)

+ 6 like - 0 dislike
114 views

I have read Sean Carrol's book. I have listened to Roger Penrose talk on "Before the Big Bang". Both are offering to explain the mystery of low entropy, highly ordered state, at the Big Bang. Since the second law of thermodynamics is considered a fundamental law of nature, and since it states that in a closed system entropy either must stay the same or increase, the entropy at the time of the Big Bang must have been much lower than it is now. Also, the thermodynamic arrow was explained by Boltzmann in 1896 embodied in $S=k\ln W$ which was inscribed on his tombstone. $W$ is the number of distinct microstates of the system. It seems to me that trivially this number will be less in the past than in the future since entropy obeys the 2nd law. This determines the thermodynamic arrow of time. Why do we need more explanation of a "fundamental law"?

This post imported from StackExchange Physics at 2014-05-14 20:00 (UCT), posted by SE-user Gordon
asked Jan 30, 2011 in Theoretical Physics by Gordon (400 points) [ no revision ]
I see that Lubos has posted this great link on another question: "Is it physically meaningful to talk about the arrow of time in other universes?"--:"Robert Wald arxiv.org/abs/gr-qc/0507094 who argued that the thermodynamic arrow of time - or low entry of the early Universe - can't have a dynamical origin. – Luboš Motl Jan 21 at 18:34" Many thanks, Lubos. I am not going to argue with Robert Wald.

This post imported from StackExchange Physics at 2014-05-14 20:00 (UCT), posted by SE-user Gordon
Thanks, Gordon, for your good contributions. Just a link so that people may simply click: arxiv.org/abs/gr-qc/0507094

This post imported from StackExchange Physics at 2014-05-14 20:00 (UCT), posted by SE-user Luboš Motl
All these arguments hinge on the assumption that the Universe is a closed system. If you abandon that assumption the whole ball-game changes. So one has to seriously consider whether this assumption is warranted in the first place. After all no closed systems exist in the world that we observe. Not even black holes. Why should the Universe be any different?

This post imported from StackExchange Physics at 2014-05-14 20:00 (UCT), posted by SE-user user346
related: physics.stackexchange.com/questions/18702/…

This post imported from StackExchange Physics at 2014-05-14 20:00 (UCT), posted by SE-user Ben Crowell

3 Answers

+ 1 like - 0 dislike

Because this violates the assumption that every state ought to be equally likely.

The low entropy of the big bang leads to the second law of thermodynamics, not the other way around.

In fact, as Boltzmann had shown, for almost all states constrained to have a given macroscopic description at a given time, entropy will increase both toward the past as well as the future. For the entropy to have been continually decreasing as we move back to the past for billions of years requires an incredible amount of fine-tuning of the correlations between almost all the particles in the present.

This post imported from StackExchange Physics at 2014-05-14 20:00 (UCT), posted by SE-user QGR
answered Jan 30, 2011 by QGR (250 points) [ no revision ]
I still don't follow (agree). I do agree that the initial conditions lead to the 2nd law, but it is a bit of a tautology.

This post imported from StackExchange Physics at 2014-05-14 20:00 (UCT), posted by SE-user Gordon
What leads to the 2nd law and the arrow is the difference in entropy between then and now. I don't see how incredible fine tuning is required. If (say) the universe started as a bubble (say, Linde's eternal inflation model), it must start in a highly ordered state, and inflation can explain the fine tuning. Or not?

This post imported from StackExchange Physics at 2014-05-14 20:00 (UCT), posted by SE-user Gordon
That is, "the correlation between almost all the particles in the present" could be explained by eternal inflation?

This post imported from StackExchange Physics at 2014-05-14 20:00 (UCT), posted by SE-user Gordon
(The -1 wasn't me :) )

This post imported from StackExchange Physics at 2014-05-14 20:00 (UCT), posted by SE-user Gordon
I think it would require a lot of fine tuning to start with eternal inflation, but once we have eternal inflation, it will continue indefinitely.

This post imported from StackExchange Physics at 2014-05-14 20:00 (UCT), posted by SE-user QGR
+ 1 like - 0 dislike

This is somewhat controversial issue. But let me present the reasons, as far as I understood, why people like Sir Penrose thinks so. Their arguments are roughly as follows:

1) The basic microscopic laws of physics are perfectly time symmetric. They are not biased in any time direction past or future.

2) Second law follows from the fact that that given an initial condition of a system which is not in the most probable state will tend to go towards the most probable state by the same microscopic laws. Since number of disordered states are much higher the system will become more and more disordered with time. Accordingly its entropy will increase until a maximum value when the system comes to the thermal equilibrium.

3) Since the microscopic laws are time symmetric the same argument can be made towards the past time direction as well. Given an an initial condition of a system which is not in the most probable state should go towards more disordered (high entropy) states towards past as well. That's what the mathematics of the laws tells us.

4) This is against our experience. Either all the parts of the universe we are observing (including our memories of past) has just undergone a HUGE fluctuation right now to give the impression that there was a more ordered past (which is crazy) OR the system was already even more ordered (low entropy) and more special in the past. But that means even more huge a fluctuation. This reasoning will lead us to conclude that at the moment of big bang the universe was extra ordinarily ordered and most special. It should be so special that it requires explanation.

Critics often point out that prediction and retrodiction is not the same thing forgetting that when one talks about the very "arrow of time" no one can say with justification which is prediction and which is retrodiction. Other than that it is also questionable whether second law can be applied this way to the whole universe or not.

This post imported from StackExchange Physics at 2014-05-14 20:00 (UCT), posted by SE-user user1355
answered Jan 30, 2011 by user1355 (75 points) [ no revision ]
See the link to the paper by Robert Wald:arxiv.org/find/all/1/…

This post imported from StackExchange Physics at 2014-05-14 20:00 (UCT), posted by SE-user Gordon
OT: (I went to some of the Waldfest in 2006 with my son...it was fun.)

This post imported from StackExchange Physics at 2014-05-14 20:00 (UCT), posted by SE-user Gordon
I have just read the paper and I agree with it. I agree that the specialness of the big bang is required and one can not invoke dynamical theories like chaotic inflation to explain the specialness, which assumes the universe started with a random initial condition.

This post imported from StackExchange Physics at 2014-05-14 20:00 (UCT), posted by SE-user user1355
@sbi Yes, Wald does argue that, but the point of my posting the link is that he also does not hold that a cosmological explanation is known or perhaps required. He says that cosmological arguments become circular and uses inflation and anthropic examples. Ultimately, he says that the universe came into existence in a special state, period. He has an addendum saying he disagrees with Carrol and Chen. In my view Wald answers the above question I asked as "It doesn't".. He does agree with you about inflation though.

This post imported from StackExchange Physics at 2014-05-14 20:00 (UCT), posted by SE-user Gordon
Well, I will leave it with Wald's paper and we will disagree.

This post imported from StackExchange Physics at 2014-05-14 20:00 (UCT), posted by SE-user Gordon
+ 0 like - 1 dislike

The key issue is: To allow galaxy and star formation, the universe had to start up in an extremely (but not perfectly) homogeneous state. The fact that the initial inhomogeneities were of size 1 part in a gadzillion (as opposed to zero) is what is puzzling.

This post imported from StackExchange Physics at 2014-05-14 20:00 (UCT), posted by SE-user Johannes
answered Jan 30, 2011 by Johannes (280 points) [ no revision ]
Most voted comments show all comments
Not really. Quantum vacuum fluctuations were inflated by the inflaton field.

This post imported from StackExchange Physics at 2014-05-14 20:00 (UCT), posted by SE-user Gordon
Not sure what you are commenting on. Are you disputing that the initial universe must have had very small but nonzero inhomogeneity?

This post imported from StackExchange Physics at 2014-05-14 20:00 (UCT), posted by SE-user Johannes
No, I am not disputing that. I am saying that. The inhomogeneities were due to "1 part in a gazillion" quantum fluctuations(as opposed to zero). Zero would be puzzling. Nothing is unstable. The infinitesimal fluctuations were stretched out by inflation---voila, galaxy formation.

This post imported from StackExchange Physics at 2014-05-14 20:00 (UCT), posted by SE-user Gordon
Inflation will increase the entropy. So the initial entropy has to be even smaller.

This post imported from StackExchange Physics at 2014-05-14 20:00 (UCT), posted by SE-user Johannes
Yes. I agree. So?. As above, see arxiv.org/find/all/1/…

This post imported from StackExchange Physics at 2014-05-14 20:00 (UCT), posted by SE-user Gordon
Most recent comments show all comments
@Gordon: Wald is wrong. Inflation in the physically proper causal patch picture produces low entropy initial conditions, as explained by Davies.

This post imported from StackExchange Physics at 2014-05-14 20:00 (UCT), posted by SE-user Ron Maimon
This doesn't answer the question and doesn't make sense. A maximum-entropy big bang would have been one in which the gravitational-wave degrees of freedom were in equilibrium with the other degrees of freedom.

This post imported from StackExchange Physics at 2014-05-14 20:00 (UCT), posted by SE-user Ben Crowell

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