Unpacking Entropy Bounds and Their Violations

In summary, the Bekenstein bound states that the entropy of an object with externally measured mass ##M## and enclosed within a surface with surface area ##A## must be less than or equal to the entropy of a black hole with mass ##M## and horizon area ##A##. The precise definition involves the use of a center of mass frame and either the ADM mass or the Bondi mass for asymptotically flat systems. However, without a theory of quantum gravity, the precise microscopic degrees of freedom of a system including the spacetime geometry are unknown.
  • #1
martinbn
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There is something that is unclear to me, and because entropy bounds and their violations were discussed in the other thread, I thought it is a good opportunity to learn something. The problem is essentially a matter of impression. The statements go roughly in the following way: for a system with entropy ##S## and energy ##E##, which is contain in space of radius ##R## a certain inequality involving the above must hold. The problem for me is that the ##E## and the ##R## are never defined (well, I haven't seen it, it might very well be explained somewhere). And in a general relativistic setting they are meaningless.

So the question is how does one make the statements precise?
 
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  • #2
The precise definition of the Bekenstein bound is that the entropy of an object with externally measured mass ##M## and enclosed within a surface with surface area ##A## must be less than or equal to the entropy of a black hole with mass ##M## and horizon area ##A##. The latter has a precise formula first derived by Hawking, which amounts to the entropy being the log of the horizon area divided by the Planck area.
 
  • #3
The surface area is better than the vague ##R##, but it still depends on the space-like slice. And how is the mass defined?
 
  • #4
martinbn said:
The surface area is better than the vague ##R##, but it still depends on the space-like slice.

Technically, yes, but for an asymptotically flat (i.e., isolated) system, one can define what amounts to a center of mass frame and use that to define the spacelike slices. Until we get a proper theory of quantum gravity, that's probably the best we're going to be able to do, since without one we simply don't know the precise microscopic degrees of freedom of a system including the spacetime geometry.

martinbn said:
how is the mass defined?

The ADM mass or the Bondi mass would be the simplest definitions, since they apply to any asymptotically flat system. I would lean towards the latter since it takes into account radiation emitted out to infinity.
 
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1. What is entropy and why is it important in science?

Entropy is a measure of the disorder or randomness in a system. It is a fundamental concept in physics, chemistry, and information theory, and plays a key role in understanding the behavior of systems at the atomic and molecular level. It is an important concept in science because it helps us understand and predict the behavior of complex systems.

2. What are entropy bounds?

Entropy bounds are theoretical limits on the amount of disorder or randomness that can exist in a system. These bounds are based on the laws of thermodynamics and statistical mechanics, and provide a framework for understanding the behavior of systems at the atomic and molecular level.

3. How can entropy bounds be violated?

Entropy bounds can be violated when a system is not in equilibrium, meaning that it is not at a stable state with a uniform distribution of energy and particles. Violations of entropy bounds can also occur in systems with strong interactions or in systems undergoing phase transitions.

4. What are some examples of entropy violations?

Some examples of entropy violations include the formation of ordered structures in non-equilibrium systems, such as crystals or snowflakes, and the emergence of complex patterns in biological systems, such as the organization of cells in tissues and organs. Violations of entropy bounds can also occur in black holes and other extreme environments.

5. How do violations of entropy bounds impact our understanding of the universe?

Violations of entropy bounds challenge our understanding of the universe and the laws that govern it. They suggest that there may be new physical laws at play in complex systems, and that our current understanding of entropy may need to be revised. These violations also have important implications for fields such as cosmology, where the study of entropy and its violations can provide insights into the evolution and structure of the universe.

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