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??
Nuclear fusion is not possible naturally on Earth due to insufficient temperatures and pressures. Current experimental facilities like ITER and JET have achieved brief instances of fusion but have not yet produced a net energy gain. While there are minor occurrences of muon-catalyzed fusion in seawater and cosmic rays, these are exceedingly rare and not significant for practical energy production. The scientific community continues to explore these phenomena, but the focus remains on controlled fusion experiments.
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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??
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.Vanadium 50 said:There is a very, very small amount of muon-catalyzed fusion in the oceans.
Ibix said:Do you have a reference for that?
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.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.