My first reply seems to have been eaten by the board (what was that about “trusting the CGI”? ). So, being too stupid to do otherwise, let me try again.
We will look at deuterium-tritium (D-T) fusion, this being the only kind that’s likely to be achieved in my lifetime[sup]1,2[/sup].
Deuterium is, I believe, available from ordinary water as a proportion of about 0.016% of the hydrogen (due to gravitational enrichment). Unless we’re planning on building Sol II, then, we don’t have to worry about it in the foreseeable future.
Tritium, OTOH, does not exist in nature save in vanishingly small quantities, as it is weakly radioactive with a half-life of 12.3 years. We’ll have to make it (more on this below).
The D-T reaction is: D + T -> [sup]4[/sup]He + n. About 18MeV of energy is released by this reaction, of which 80% is carried by the neutron.
Now the neutron can actually be useful. Two reactions can be used to make tritium:[ul]
[li][sup]6[/sup]Li + n -> [sup]4[/sup]He + T[/li][li][sup]7[/sup]Li + n -> [sup]4[/sup]He + T + n[/li][/ul]
The first assumes a thermal (slow) neutron, and is exothermic; the second assumes a fast neutron (as is produced by the D-T reaction) and is endothermic. [sup]7[/sup]Li is about 13 times as abundant as the lighter isotope; depending on how we tweak our tritium production, we have sufficient lithium to supply with tritium for several thousands to several tens of thousands of years, so we’ll stamp this problem “Solved”, too.
The problem comes with the total neutron flux. Assume that the reactor is producing 1GW of power. Then, depending on power recovery from the tritium-making blanket, we’re producing 1-4 GW of neutron flux; call it 2.5 GW. Assume that the blanket is 99.9% efficient at capturing neutrons, so only 2.5 MW gets through. If someone is standing 10 meters outside of the blanket, he’s intercepting about 0.04% of this flux (assumption: he presents a surface of about one-half square meter). 1 rad is 0.01J/kg; if he weighs 70 kg, then the dose rate is about 1430 rad/s. A ‘Q’ factor of 20 is safe to assume for fast neutrons, so that we’re talking over 28,000 rem/s. Can you say, “dead before he hits the floor”?
Of course, we can deal with this the same way in which we deal with neutron flux from fission reactors, but we’ll also have the same problems (neutron embrittlement of materials, generation of LLW).
A fusion reactor won’t generate HLW (unless we’re talking here about something exotic like a fusion-fission breeder using [sup]238[/sup]U outside the tritium blanket), so I suppose that we can say that fusion won’t suck as badly as fission. OTOH, we have fission now; a working
inertial fusion reactor (IFR) using D-T is probably 20-50 years away. Research on this should continue, and at about an order of magnitude greater of funding, but you can’t get a baby in a month by impregnating nine women; don’t expect that, even if that extra funding is provided, we’ll be seeing an IFR on-line before 2010 at the earliest.
[sup]1[/sup][sub]Of course, “my lifetime” is not equivalent to “the lifetime of any of the Teeming Thousands”. OTOH, I will really need to see some evidence before I concede that any of them will live to the age of 250.[/sub]
[sup]2[/sup][sub]Don’t even talk to me about weak-force-mediated reactions like p-p.[/sub]