I How would the laws of thermodynamics change in a contracting universe?

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In a contracting universe, the laws of thermodynamics, particularly entropy, are debated with varying interpretations. Some argue that entropy will still increase or remain constant, while others suggest it may decrease as the universe approaches a "big crunch." The discussion highlights the complexity of defining entropy in a deterministic model like the closed Friedmann-Robertson-Walker (FRW) universe, where entropy is theoretically zero. There is a call for specific references to ground the discussion in established physics, as current models may not adequately address the differing properties of the universe's expansion and contraction phases. Ultimately, the conversation emphasizes the need for a proper framework to explore these speculative ideas meaningfully.
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How would the laws of thermodynamics change in a contracting universe?On the internet, I get different answers: Most say that entropy will still increase or stay the same. Some say the second law will be reversed. Some say that there will be a local decrease in entropy.
The universe as a whole will increase in temperature. Is that considered an increase in entropy?
How would the laws of thermodynamics change in a contracting universe?
(Of course we live in an accelerating and expanding universe. So the questions are hypothetical.)
On the internet, I get different answers: Most say that entropy will still increase or stay the same, but no explanations or mathematics were given. Some say the second law will be reversed. Some say that there will be local decreases in entropy.
The universe as a whole will increase in temperature. Is that considered an increase in entropy?
But as the universe continues toward the "big crunch", entropy need to decease, since at the beginning of the "big bang" entropy was low?
I believe that since the universe is getting smaller, at least the definition of disorder will need to be modified.
Is it all semantics? I wonder what the members of physics forums think?
 
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In physics hypothethis should be proved/denied by observation or experiment. I don't think we have a chance of experiment on this issue though I would like to.
 
KurtLudwig said:
On the internet, I get different answers
You need to give specific references. Particularly for a topic like this, we need to have some kind of mainstream reference as a basis for discussion. If there are no such references, that means the topic is too speculative to be usefully discussed here.
 
KurtLudwig said:
The universe as a whole will increase in temperature. Is that considered an increase in entropy?
But as the universe continues toward the "big crunch", entropy need to decease, since at the beginning of the "big bang" entropy was low?
As far as an idealized closed FRW model that expands and then contracts is concerned, the question of "entropy" is meaningless, because the model is an exact deterministic solution, whose "entropy" is zero at all times since there is no uncertainty about its state.

Of course what you are trying to envision is a more realistic model in which the FRW solution is just an approximation. But that is where we need actual references as a basis for discussion: what kind of approximation is being used? Does it allow for the "Big Bang" and "Big Crunch" ends of the universe to have different properties? (Note that the idealized FRW model does not; they have to be the same.) Without an actual reference as a basis for discussion, questions like there are not even answerable.
 
Thank you for your answers.
 
anuttarasammyak said:
In physics hypothethis should be proved/denied by observation or experiment. I don't think we have a chance of experiment on this issue though I would like to.
I think that this is too reductive. Sure it is good to attach hypothesis to observation but sometimes not-so-real models can help build an intuition. What I think this question is missing is a proper framework. Using model "insert specific model name here" what happens with "insert variable here" when "variable here" decreases.
 
https://en.wikipedia.org/wiki/Recombination_(cosmology) Was a matter density right after the decoupling low enough to consider the vacuum as the actual vacuum, and not the medium through which the light propagates with the speed lower than ##({\epsilon_0\mu_0})^{-1/2}##? I'm asking this in context of the calculation of the observable universe radius, where the time integral of the inverse of the scale factor is multiplied by the constant speed of light ##c##.
The formal paper is here. The Rutgers University news has published a story about an image being closely examined at their New Brunswick campus. Here is an excerpt: Computer modeling of the gravitational lens by Keeton and Eid showed that the four visible foreground galaxies causing the gravitational bending couldn’t explain the details of the five-image pattern. Only with the addition of a large, invisible mass, in this case, a dark matter halo, could the model match the observations...
Hi, I’m pretty new to cosmology and I’m trying to get my head around the Big Bang and the potential infinite extent of the universe as a whole. There’s lots of misleading info out there but this forum and a few others have helped me and I just wanted to check I have the right idea. The Big Bang was the creation of space and time. At this instant t=0 space was infinite in size but the scale factor was zero. I’m picturing it (hopefully correctly) like an excel spreadsheet with infinite...
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