Star and planet formation according to the 2nd Law of Thermodynamics

Click For Summary

Discussion Overview

The discussion revolves around the relationship between the second law of thermodynamics and the formation of stars and planets from the early universe. Participants explore the implications of entropy, the initial conditions of the universe, and the nature of gravitational systems in the context of thermodynamic principles.

Discussion Character

  • Exploratory
  • Debate/contested
  • Conceptual clarification

Main Points Raised

  • Some participants question how stars and planets could form from a state of high entropy without violating the second law of thermodynamics, suggesting that this might imply a misunderstanding of entropy.
  • Others argue that the early universe was in a low-entropy state, contrary to the notion of it being disordered, and that this low entropy is necessary for the existence of stars and life.
  • A participant notes that the second law implies that if the early universe had been in a maximum entropy state, it would have experienced heat death immediately, which contradicts current observations of the universe.
  • Some contributions highlight that the cosmic microwave background radiation indicates thermal equilibrium for matter but not for gravitational degrees of freedom, suggesting a nuanced understanding of entropy in cosmological contexts.
  • One participant proposes the need for a new model that accommodates thermodynamic laws in a way that might explain the universe's behavior without relying on concepts like dark energy and dark matter.

Areas of Agreement / Disagreement

Participants express differing views on the nature of the early universe's entropy and its implications for star and planet formation. There is no consensus on the interpretations of entropy or the necessity of new models to explain these phenomena.

Contextual Notes

Some claims rely on specific interpretations of gravitational systems and thermodynamic principles, which may not be universally accepted. The discussion includes references to complex models and theories that are not fully resolved within the conversation.

mess1n
Messages
24
Reaction score
0
In the first part of Brian Cox's documentary series 'Wonders of the Universe', he explains how the entropy of the universe always increases, and that we are therefore headed for a state of total 'disorder' where all is left of the universe is photons and dying black holes.

But wasn't this essentially the initial state of the universe after the big bang? Minus the black holes. If it was, how did stars and planets form from this without violating the second law? It seems to be a situation where the splattered egg reforms into a perfect egg. When stars and planets formed, it seems as though the universe became more orderly. Was matter formation just massively unlikely? Or am I misinterpreting entropy?


Andrew
 
Space news on Phys.org
mess1n said:
But wasn't this essentially the initial state of the universe after the big bang?

No, the early universe was in a very low-entropy state. A maximum-entropy state would have been dominated by gravitational waves. A good popular-level book that covers this is Cycles of Time by Roger Penrose.
 
Since this seems to be a FAQ, I've written a FAQ entry for it.

FAQ: Wasn't the early universe in a disordered state?

No. The second law of thermodynamics says that entropy can only increase, so if the early universe had been in a state of maximum entropy, then the cosmos would have experienced its heat death immediately after being born. This contradicts the observation that the present universe contains burning stars, heat engines, and life. These observations imply that the early universe was in a very low-entropy state, which shows that its initial conditions were extremely finely tuned. The reasons for this fine-tuning are not explained by general relativity or the standard model. I'm not an expert on inflation, but apparently adding inflation to the model does not cure this fine-tuning problem.[Penrose 2005]

These ideas are strongly counterintuitive to most people, since we picture the early universe as an undifferentiated soup of hot gas, very much like what we might imagine a heat-dead universe to be like. In what way is the early universe *not* equilibrated?

We observe that the cosmic microwave background radiation's spectrum is a blackbody curve, which would normally be interpreted as evidence of thermal equilibrium. However, this observation only really tells us that the *matter* degrees of freedom were in thermal equilibrium. The gravitational degrees of freedom were not. In standard cosmological models, which are constructed to be as simple as possible, there are no gravitational waves. Although the real universe presumably does have gravitational waves in it, they are apparently very weak. In a maximum-entropy universe, the gravitational modes would be equilibrated with the matter degrees of freedom, and they would be very strong, as in Misner's mixmaster universe cosmology.[Misner 1969]

Even in Newtonian mechanics, gravitating systems violate most people's intuition about entropy. If we psssssht a bunch of helium atoms into a box through an inlet valve, they will quickly reach a maximum-entropy state in which their density is nearly constant everywhere. But in an imaginary Newtonian "box" full of gravitating particles, the maximum-entropy state is one in which the particles have all glommed onto each other and formed a single blob. This is because of the attractive nature of the gravitational force.

Charles W. Misner, "Mixmaster Universe", Physical Review Letters 22(1969)1071. http://astrophysics.fic.uni.lodz.pl/100yrs/pdf/07/036.pdf

Roger Penrose, 2005 talk at the Isaac Newton Institute, http://www.Newton.ac.uk/webseminars/pg+ws/2005/gmr/gmrw04/1107/penrose/
 
Last edited by a moderator:
bcrowell said:
Since this seems to be a FAQ, I've written a FAQ entry for it.

FAQ: Wasn't the early universe in a disordered state?

No. The second law of thermodynamics says that entropy can only increase, so if the early universe had been in a state of maximum entropy, then the cosmos would have experienced its heat death immediately after being born. This contradicts the observation that the present universe contains burning stars, heat engines, and life. These observations imply that the early universe was in a very low-entropy state, which shows that its initial conditions were extremely finely tuned. The reasons for this fine-tuning are not explained by general relativity or the standard model. I'm not an expert on inflation, but apparently adding inflation to the model does not cure this fine-tuning problem.[Penrose 2005]

These ideas are strongly counterintuitive to most people, since we picture the early universe as an undifferentiated soup of hot gas, very much like what we might imagine a heat-dead universe to be like. In what way is the early universe *not* equilibrated?

We observe that the cosmic microwave background radiation's spectrum is a blackbody curve, which would normally be interpreted as evidence of thermal equilibrium. However, this observation only really tells us that the *matter* degrees of freedom were in thermal equilibrium. The gravitational degrees of freedom were not. In standard cosmological models, which are constructed to be as simple as possible, there are no gravitational waves. Although the real universe presumably does have gravitational waves in it, they are apparently very weak. In a maximum-entropy universe, the gravitational modes would be equilibrated with the matter degrees of freedom, and they would be very strong, as in Misner's mixmaster universe cosmology.[Misner 1969]

Even in Newtonian mechanics, gravitating systems violate most people's intuition about entropy. If we psssssht a bunch of helium atoms into a box through an inlet valve, they will quickly reach a maximum-entropy state in which their density is nearly constant everywhere. But in an imaginary Newtonian "box" full of gravitating particles, the maximum-entropy state is one in which the particles have all glommed onto each other and formed a single blob. This is because of the attractive nature of the gravitational force.

Charles W. Misner, "Mixmaster Universe", Physical Review Letters 22(1969)1071. http://astrophysics.fic.uni.lodz.pl/100yrs/pdf/07/036.pdf

Roger Penrose, 2005 talk at the Isaac Newton Institute, http://www.Newton.ac.uk/webseminars/pg+ws/2005/gmr/gmrw04/1107/penrose/

I think we need a new model where Thermodynamics laws are almost perfect. The place where Universes are created and despaired as smooth as a hurricane or Typhons do in our planet. Thermodynamics are ok for engineering inside the planet and when u can have limit (e: gasoline engine). Either the universe is the last frontere or there is other system where it can have entropy almost zero so will increased to the despairing state of max entropy. Observing jupiter. mass gravity and energy such system must exist so the 98 % that was needed to adjust the actual model (dark energy and dark mass?) would not be necessary
 
Last edited by a moderator:

Similar threads

  • · Replies 27 ·
Replies
27
Views
6K
  • · Replies 33 ·
2
Replies
33
Views
3K
  • · Replies 6 ·
Replies
6
Views
3K
  • · Replies 3 ·
Replies
3
Views
6K
  • · Replies 1 ·
Replies
1
Views
2K
  • · Replies 1 ·
Replies
1
Views
2K
  • · Replies 5 ·
Replies
5
Views
1K
  • · Replies 18 ·
Replies
18
Views
5K
  • · Replies 15 ·
Replies
15
Views
3K
  • · Replies 15 ·
Replies
15
Views
3K