[TML] RTT FGMP
Jerry W Barrington
jerry.barrington at gmail.com
Sun Jul 13 21:32:31 MDT 2008
On 7/13/08 10:25 PM, "Grimmund" <grimmund at gmail.com> wrote:
> Once the plasma cools and stops fusing, so does the radioactivity.
Not entirely. Other atoms that absorb the neutrons may thus become unstable
isotopes.
> Fusion produces relatively little radioactivity, mostly fast
> particles.
Again, fusion tends to emit a lot of neutron. See above.
> But if you pick your fuel carefully, fusion doesn't produce ANY
> radioactive isotopes. It produces fast particles while the fusion
> reaction is happening, but when it stops, so does the radioactivity.
> The classic example is hydrogen fusion, which produces helium.
Likely, most of the criteria for a fusion power reactor will apply. Plus we
don't want the neutrons mentioned. That doesn't leave many good choices:
H-2 + He-3; He-3 + He-3; after that you start getting into heavier elements
like Li and B.
If you mean the proton-proton chain or CNO cycle, only in stars. Even in
stellar cores (15,000,000 K, 160g/cm^3), the energy production per volume is
only a quarter of that of the same volume of a *resting* human. Hardly
weapon-level energy.
There's lots of other complicating factors. But if we look too hard at
them, PGMP & FGMP will be show to simply be impractical as weapons.
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