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Ken G
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- TL;DR Summary
- In the PF FAQ by @bcrowell, the remarkable point is made that the early universe had to be in a low entropy state or structure could not form spontaneously, but how does entropy rise when structure forms?
The FAQ by @bcrowell cites an explanation by physics netizen John Baez as to how entropy rises when a star loses heat and contracts. However, the linked explanation falls short of describing the key role that gravity must be playing. The FAQ by @bcrowell discusses why a low-entropy state of universal gravity must be playing a key role, since the matter in the universe is nearly thermalized (so is by itself in a state of high entropy). But the cited accounting of entropy rise in a contracting star by Baez includes gravity only as a source of energy, and talks about the entropy associated with the lost heat to the environment, but gives no direct entropic significance to the gravity itself.
Something must be missing here, because it is well known (via the Jeans instability) that isothermal gas can be made to spontaneously contract if the mass is high enough. In that situation, there is no entropy increase associated with heat transport from the ball of gas to its (isothermal) surroundings, yet there is the same entropy drop seen in the gas itself that Baez described (in essence, the loss in volume accessible to the particles reduces their entropy more than the increase in velocity space that their higher energy gives them access to). So the only thing left to account for the spontaneous entropy rise that must appear during an isothermal Jeans instability has to have something directly to do with entropy associated with gravity. What is this missing element, that surely must also be present in structure formation in the early universe?
Something must be missing here, because it is well known (via the Jeans instability) that isothermal gas can be made to spontaneously contract if the mass is high enough. In that situation, there is no entropy increase associated with heat transport from the ball of gas to its (isothermal) surroundings, yet there is the same entropy drop seen in the gas itself that Baez described (in essence, the loss in volume accessible to the particles reduces their entropy more than the increase in velocity space that their higher energy gives them access to). So the only thing left to account for the spontaneous entropy rise that must appear during an isothermal Jeans instability has to have something directly to do with entropy associated with gravity. What is this missing element, that surely must also be present in structure formation in the early universe?