Could the Universe's Infinite Nature Align with Thermodynamics?

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SUMMARY

The discussion centers on the relationship between the infinite nature of the universe and thermodynamics, specifically referencing Newton's Second Law of Thermodynamics and the heat death of the universe. Participants clarify that the universe is currently understood to be infinite based on cosmological models, with no definitive evidence supporting its finiteness. The conversation also touches on the implications of potential energy pooling into black holes and the subsequent transformation of energy forms, while emphasizing the distinction between conjecture and evidence in cosmological theories.

PREREQUISITES
  • Understanding of Newton's Laws of Motion and Thermodynamics
  • Familiarity with cosmological models and the concept of heat death
  • Knowledge of black hole physics and energy transformations
  • Basic grasp of the Friedmann equations and cosmological parameters
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  • Study the implications of the heat death of the universe on cosmic structures
  • Explore the Friedmann equations and their role in cosmology
  • Investigate the nature of black holes and their energy dynamics
  • Examine current research on the curvature of the universe and its implications
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Astrophysicists, cosmologists, and students of physics interested in the interplay between thermodynamics and the structure of the universe.

  • #31
I suspect there's not enough available information to assign probabilities to any of the imagined "possibilities" regarding whether the universe is infinite or not. ["Possibilities" such as a) vast, yet closed, finite universe with slightly positive curvature, b) flat and infinite, c) flat and finite (e.g., torus shaped), d) open and infinite with a slightly negative curvature.]

Here's a tale of caution regarding probabilities which involve infinity. It's a purely mathematical story and doesn't even touch on the physical unknowns that are pertinent to this thread. If it's even on topic at all, it doesn't become on-topic until 13:30 or so of the second video.





Forgive me if this isn't on topic. This isn't exactly my area of expertise.
 
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  • #32
Buzz Bloom said:
Hi @Hornbein:

I am puzzled by the statement that seems to imply that a finite universe has a curvature Ωk which gets larger as the universe expands. Ωk is inversely proportional to the radius R of the finite universe. Since the radius gets bigger over time, Ωk gets closer to zero, that is closer to flatness. I think that the statement that the critical density (assumed to be greater than 1) approaches 1 (and then is larger as the size is smaller) is also incorrect. This was the case for ΩΛ = 0, but not so for the currently best fit where ΩΛ ~= 0.7.

Regards,
Buzz
I don't understand it. I just quote experts. There are discussions on this topic elsewhere at PF, I would suppose under Cosmology.
 
  • #33
Hi @collinsmark:

Wikipedia has a very clear explanation of the paradox.
It is an excellent example that the probability distribution of a variable depends on the method used to define an instance of the variable. A different method results in a different distribution.

I do not think this paradox is applicable to the topic of calculating the distribution of a cosmological variable, but I could be mistaken. I would be only moderately surprised if it should be found out that the recent strange difference in results between two methods of calculating H0 is an example of this paradox.

Regards,
Buzz
 
  • #34
Sorry, we really do not allow philosophy at PF, with the exception in Quantum Physics, at the mentors discretion in that forum, it's a fine line.

So thanks again to everyone for keeping the thread from going off the rails, but alas, time to close it before people outside of PF find the thread and begin quoting unicorns and fairies. :nb)
 

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