2nd law of thermodynamics and the big bang

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Discussion Overview

The discussion revolves around the relationship between the second law of thermodynamics and the conditions of the universe at the time of the Big Bang. Participants explore concepts of entropy, its implications for the early universe, and the nature of dimensions in relation to thermodynamic principles.

Discussion Character

  • Debate/contested
  • Conceptual clarification
  • Exploratory

Main Points Raised

  • Some participants reference Victor Stenger's assertion that the universe had maximum entropy at the Big Bang, suggesting that entropy has decreased since then due to the expansion of the universe.
  • Others challenge this view, arguing that the early universe actually had low entropy, which has increased over time, aligning with the thermodynamic arrow of time.
  • One participant introduces the idea that the laws of thermodynamics may be emergent properties rather than fundamental, raising questions about the nature of the universe and the quest for a theory of everything (TOE).
  • Another participant questions whether adding more spacetime dimensions has effectively reduced degrees of freedom in theoretical models.
  • There is a discussion about the relationship between entropy and black holes, with references to how the event horizon relates to entropy and disorder.
  • A participant mentions Roger Penrose's perspective that conditions at the Big Bang were characterized by low entropy, particularly due to the gravitational field, which contrasts with the idea of maximum entropy.

Areas of Agreement / Disagreement

Participants express differing views on the entropy of the universe at the time of the Big Bang, with no consensus reached. Some support the idea of maximum entropy, while others argue for low entropy, indicating a fundamental disagreement on this topic.

Contextual Notes

The discussion highlights the complexity of defining entropy in the context of the early universe and black holes, as well as the implications of emergent versus fundamental properties in theoretical physics. There are unresolved assumptions regarding the definitions and interpretations of entropy and dimensions.

huyen_vyvy
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I read from Victor Stenger's books that maximum entropy exists in black holes or singularities. So, at the Big bang, the universe had its maximum entropy. Does it mean that entropy has DECREASED since then? Stenger explained that since the universe expands, it has more space for entropy. However, this doesn't really make sense to me.
 
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Could you give a precise reference please? It was my understanding that the early universe contained a small entropy, which has increased as time increased (this is something like that thermodynamical arrow of time). I'd like to take a look at the given reference though, or at least an exact quotation, before commenting on it (especially since I'm not too sure what's meant by "the maximum entropy is found in a black hole).
 
Further complicating matters is whether or not the laws of thermodynamics are a transcendental property of the 'oververse', or an emergent property of this universe. If an emergent property [which is an arguably difficult proposition to avoid], it is conceivable this is the only kind of universe possible - i.e., one whose fundamental properties happen to be sufficiently fine tuned to enable a very long lived incarnation [the only kind where observers like us could emerge]. In that sense, the quest for a TOE is an 18th century classical hangover. We will be forever stuck with some number [greater than one] of fundamental constants that defy all efforts to further reduce. I find it curious the current number of fundamental constants of nature [26] is the same as the number of dimension proposed by heterotic string theory.
 
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Chronos,
totally in line with you. I would add the question, "isn't it a fact that, so far, adding more spacetime dimensions has done nothing in reducing the degrees of freedom ?".
Having said that, if we had a theory that could enable to derive the 26 parameters from one, would you say that this gets closer in the way of a TOE ?
 
Have a look at Victor Stenger's book called "God: the failed hypothesis", in which he argues that although at the big bang, the universe had maximum entropy, the universe has ever since expanded so it has more space to "throw" its entropy.
 
I think, chrisina, we need to think outside the box when it comes to defining what constitutes a 'dimension'. Classical spacetime, IMO, is emergent, not fundamental, arising from quantum imbalances in the initial conditions. I would argue that quantum principles are transcendental properties of the 'oververse', but have no preferred value. Think of it as looking for dimensions in all the wrong places.
 
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cristo said:
Could you give a precise reference please? It was my understanding that the early universe contained a small entropy, which has increased as time increased (this is something like that thermodynamical arrow of time). I'd like to take a look at the given reference though, or at least an exact quotation, before commenting on it (especially since I'm not too sure what's meant by "the maximum entropy is found in a black hole).

actually in a black hole the event horizon is compared to the antropy. antropy increases as disorder increases.in the same way matter falling inside a black hole is the disorder and the increasing eventhorizon is the antropy.we can say that the disorder(acretion disc)in a black hole increases the antropy(eventhorizon).another example the total antropy of a system is the sum of the reactant antropies of the two systems. similarly if two black holes collide the event horizon of the resultant black hole will be the sum of the event horizons of the colliding black holes.therefore it is said that black has the max antropy.thanks for reading
 
huyen_vyvy said:
Have a look at Victor Stenger's book called "God: the failed hypothesis", in which he argues that although at the big bang, the universe had maximum entropy, the universe has ever since expanded so it has more space to "throw" its entropy.

Unfortunately I don't have Stenger's book handy, so i cannot follow this argument.
there is a talk about the Big Bang and entropy and the 2nd Law by Roger Penrose,
that is free online (voice and slides).

Penrose says that from the standpoint of someone in our universe looking back at the Big Bang, conditions at that time had very LOW ENTROPY. He says people are mistaken to say it was high entropy because that does not count the extremely low entropy of the gravitational field at that era.

It is a very clear, wide-audience talk. I respect Penrose a lot although i don't always understand his arguments, or agree in every case (where i do follow.)

the talk can be googled using information like "Penrose before the big bang"
http://www.Newton.cam.ac.uk/webseminars/pg+ws/2005/gmr/gmrw04/1107/penrose/
 
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