Entropy in a Black Hole: A Thermodynamic Paradox

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Discussion Overview

The discussion revolves around the concept of entropy in the context of black holes and its implications for the second law of thermodynamics. Participants explore the paradox of how black holes, which seemingly condense matter and prevent heat loss, might lead to a decrease in total entropy, challenging established thermodynamic principles.

Discussion Character

  • Debate/contested
  • Conceptual clarification
  • Exploratory

Main Points Raised

  • One participant notes that while the entropy of the universe must increase, black holes seem to condense matter without heat loss, suggesting a decrease in entropy for the black hole system.
  • The same participant proposes that when a gas cloud collides with a black hole, the resulting condensation could lead to a decrease in entropy in the surroundings, potentially violating the second law of thermodynamics.
  • Another participant references Hawking Radiation as a mechanism that might help reconcile the entropy paradox, suggesting it could re-balance entropy in accordance with thermodynamic laws.
  • Further contributions mention that black holes possess maximal entropy in a given region, contrasting with the low entropy associated with the big bang, hinting at deeper implications for understanding entropy in cosmological contexts.
  • There is a discussion about the relationship between the entropy of a black hole and its event horizon, which leads to considerations of the holographic principle and the idea that minimal units of space may carry specific amounts of entropy.

Areas of Agreement / Disagreement

Participants express differing views on the implications of black holes for entropy and thermodynamics. While some suggest mechanisms like Hawking Radiation may resolve the paradox, others raise questions about the fundamental understanding of entropy in extreme conditions, indicating that the discussion remains unresolved.

Contextual Notes

Participants highlight the complexity of entropy in black holes, including the dependence on definitions of entropy and the conditions under which these discussions occur. The implications of the holographic principle and the nature of singularities are also noted as areas requiring further exploration.

Bacat
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In thermodynamics we have a law that says that the entropy of the universe must always increase, though the entropy of sub-system can temporarily decrease. This increase of entropy generally happens through work -> heat processes (ie friction). We also think of the diffusion of atoms in a disorganized way as an increase of entropy. So if I have 1 mole of gas in a box and I open the box, the gas expands freely and entropy is increased.

I was thinking about the theory of black holes the other day; the immense gravity of a black hole condenses matter so completely that light cannot escape. If this is the case, then it is reasonable to assume that matter with mass certainly cannot escape either, therefore heat cannot escape (which is transferred by the kinetic motion of matter). Therefore, a black hole condenses matter without heat loss. This seems to be a decrease in entropy (of the black hole system). But what about the surroundings?

Let a gas cloud collide with the black hole. Now the mole of gas which had expanded freely in a vacuum is condensed into a much smaller volume without heat loss. The pressure will increase so much that the gas will condense into a solid, thus we have lost 1 mole of gas. This implies a decrease in entropy in the surroundings.

[tex]\Delta S_{total} = \Delta S_{surr} + \Delta S_{sys}[/tex]

So the total entropy of the universe has decreased due to the black hole, which seems to violate the second law of thermodynamics.

Can anyone shed light on this problem?
 
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That's very interesting and I think offers a way out of the paradox. I appreciate the time you took to write all of that out and now to have linked to it. It looks as if Hawking Radiation manages to re-balance the entropy so that thermodynamics still hold.

Do you have information critical mass and the expansion of the universe also?

Cheers.
 
There are all sorts of interesting implications...black holes have maximal entropy (in a given region of space) while the other major singularity, the big bang, has low entropy. I just know there is something that hasn't been fully appreciated yet.

Further, since the entropy of a black hole is proportional to its event horizon (rather than its volume) that leads into the holographic principle as well as a minimal size to space...suggesting Planck size nuggets of one Planck unt area carry one unit of entropy (information).
 

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