Is nuclear fusion possible on earth?

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Discussion Overview

The discussion revolves around the possibility of nuclear fusion occurring on Earth, both naturally and in hypothetical scenarios such as parallel universes. Participants explore the conditions required for fusion, the occurrence of fusion reactions in nature, and the challenges associated with observing these phenomena.

Discussion Character

  • Exploratory
  • Debate/contested
  • Technical explanation

Main Points Raised

  • Some participants assert that nuclear fusion cannot occur naturally on Earth due to insufficient temperatures and pressures, emphasizing the need for human-made environments like ITER and JET.
  • Others mention that there is a very small amount of muon-catalyzed fusion occurring in the oceans, although this is considered rare.
  • A participant requests references for the claim about muon-catalyzed fusion in seawater, indicating interest in further understanding this phenomenon.
  • Another participant elaborates on the rarity of fusion reactions, noting that cosmic rays can induce fusion in the atmosphere, but these events are infrequent.
  • Concerns are raised regarding the feasibility of muon-catalyzed fusion in seawater, particularly the challenges posed by the presence of oxygen and the complexity of the reactions involved.
  • One participant expresses skepticism about the mechanisms of muon-catalyzed fusion, questioning the conditions under which it could occur in seawater and suggesting the need for further research on muon interactions with water.

Areas of Agreement / Disagreement

Participants generally disagree on the possibility of natural nuclear fusion on Earth, with some asserting it cannot occur while others point to specific instances of fusion reactions. The discussion remains unresolved regarding the details and implications of muon-catalyzed fusion.

Contextual Notes

Limitations include the lack of consensus on the mechanisms of muon-catalyzed fusion and the specific conditions required for such reactions to occur in seawater. The discussion also highlights the complexity of fusion processes and the challenges in observing them.

steveJOBS
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Is nuclear fusion fusion possible on Earth naturally or can it be possible in an Earth in a parallel universe??
 
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steveJOBS said:
Is nuclear fusion fusion possible on Earth naturally or can it be possible in an Earth in a parallel universe??

It is not possible naturally, since the temperatures and pressures required do not occur naturally on Earth. We have to recreate them. Places like ITER and JET have undergone brief nuclear fusion. We aren't quite at the point where the energy out is more than the energy put in, but we are very close! :smile:

Here is ITER's website: https://www.iter.org/
And here is JET's website: https://www.euro-fusion.org/jet/

But no, it cannot occur naturally.
 
There is a very, very small amount of muon-catalyzed fusion in the oceans.
 
Vanadium 50 said:
There is a very, very small amount of muon-catalyzed fusion in the oceans.
Do you have a reference for that? That's something I'd like to have in the old mental filing cabinet, along with the Oklo fission reactor.
 
All sorts of reactions happen if you look close enough. About 1 in 1017 hydrogen atoms is tritium, about 1 in 7000 is deuterium, now imagine the probability that a muon gets stopped by a hydrogen molecule (those are rare enough in sea water) that has both together...

Fusion reactions from cosmic rays in the atmosphere happen more frequently, but still on the level of "oh, there was one fusion reaction here".
 
Ibix said:
Do you have a reference for that?

There was a Scientific American (I think) article many years back that calculated this. Basically, you get a mu- that slows down in seawater and is captured on deuterium. Then you get D-H fusion, or if you happen to hit some D2O, D-D. (While D2O is rarer than DHO by a factor of several thousand, the fusion rate is higher by a factor of several thousand) It's a hard process to observe, because there are many larger sources of helium.
 
Vanadium 50 said:
There was a Scientific American (I think) article many years back that calculated this. Basically, you get a mu- that slows down in seawater and is captured on deuterium. Then you get D-H fusion, or if you happen to hit some D2O, D-D. (While D2O is rarer than DHO by a factor of several thousand, the fusion rate is higher by a factor of several thousand) It's a hard process to observe, because there are many larger sources of helium.
I'm highly skeptical of this. The reason lab-observed muon-catalyzed fusion works so well is because the muon is captured by an exchange reaction, where H2+ (two nucleons and an electron) undergoes an electron-muon exchange to give H2μ+. The thing is, the only thing holding the H2+ system together is that one electron. When it's replaced by the muon, the bond length shortens by the mass factor of the muon. For D2O, on the other hand, you have a system of 10 electrons, 4 of which directly participate in bonding and 8 of which are valence electrons. Furthermore, if the fusion is D-D, you have to get the deuterons close enough together to fuse, but remember, there's an oxygen atom in the way. So the muon would have to either, as mfb said, encounter some dissolved D2 in the seawater, or it would have to 1) catalyze the breakup of D2O into something that was geometrically amenable to fusion, and 2) remain attached to that species to actually catalyze the fusion. I'd be interested in seeing the reference you're pulling from, if you can remember it.

EDIT (and I'm sure someone out there has looked at this): It would be informative to look at a paper on muon interactions with water. My guess is that the muon occupies a deep core orbital on the oxygen, giving a species that looks nominally like H2N- (assuming no electrons are ejected) (this is because the Oμ system behaves chemically like a nitrogen atom since the muon orbits so much closer into the oxygen nucleus than the electrons), a species whose bond length is probably comparable to that of NH3.
 

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