Chrismb's interpretation seems misleading (or at least confusing for me), though the numbers may be accurate.
To give a perspective on the rates/ lifetimes involved, lock at this link.
A straight forward method to calculate the fusion rate and a comparison of ion lifetimes before fusion in three systems:
http://fusedweb.llnl.gov/CPEP/Chart_pag ... Works.html
"Plasma Fusion Reaction Rate = R * n1 * n2
n1,n2 = Densities of reacting species (particles/m3); R = Rate Coefficient (m3/s).
Multiply by Ef to get fusion power density.
Discussion:
To calculate the rate of reactions per unit volume, multiply the rate coefficient, R, by the particle densities of the two reacting species (divide by two if there is only one species, in order to avoid double-counting the reaction possibilities). The p + p => D reaction rate coefficient in the sun is much lower than that achievable with a deuterium-tritium fuel mix, because the p + p reaction proceeds by the weak nuclear interaction. Despite the sun's high density, the low rate coefficient means a proton in the sun will exist for an average of billions of years before it fuses. By comparison, a deuteron in a magnetic fusion power plant would only exist for about 100 seconds, and a deuteron in an imploding, fully-burned inertial confinement pellet only for 1.0E-9 seconds".
These are all Maxwellian systems and do not incorporate the narrow energy spread and confluence benifits claimed for the Polywell
To see some real world numbers perhaps Chrismb can crunch some numbers from Jet. It produced ~ 15MW of fusion, Assume this would represent ~ 10 ^16 D-T fusions per second. Assume that Jet had a density of ~ 10^20 ions per cubic meter (generous number?), a volume of ~ 100 cubic meters (?) and a temperature of 5,000 eV ( actually I believe only a small tail of the Maxwellian distribution would have had an energy approaching this in Jet). Using 20 MW of input power to maintain this reaction should allow the effective containment time for the system to be calculated.
Compare the resultant numbers with the above.
Then throw in the added benefits in energy density that the Polywell can achieve (Dr Nebel mentioned ~ 60,000 fold advantage-due, I guess, to the increased particle density thanks to the Wiffleball trapping factor and some degree of ion focusing). For simplicity, assume the narrow energy distribution (non Maxwellian) claimed for the Polywell is counterbalanced by the advantages of burning D-T fuel in the Tokamac with a thermalized Maxwellian plasma.
Crunching these numbers should show the relations between real performance and things like derived perameters like MFP and fusion crossections. If they don't add up there is something wrong or missing.
As for neutral recombinations, I speculate that with the claimed narrow energy spreads at energies well above 10's of KeV, recombinations would be uncommon and short lived enough so that their effects would be tolerable. If most collisions occur the core or the border regions as claimed, and not in the mantle (in between regions) the effects on radial and angular spread would be further reduced. In the core collisions (weather between ions, or ions and neutrals) could not introduce much angular momentum. In the border the claimed annealing effects would also help the upscatering and down scattering effects (I'm uncertain if the claimed annealing effect has much effect on angular momentum spread(?).
Another way of stating it, is that in a large enough machine the distance a recombined neutral would travel before being re ionized would be so short in comparison to the diameter of a large machine, the effects would not be much different than the backgrounf ion- ion collisions. This is why Bussard claimed that the diassadvantages of the neutral gas puffers in WB 6 would dissappear once the machine grew to dimensions necessary for net power production.
I might (will) add that the distance traveled by a neutral before re ionization is so short compared to the machine diameter that a neutral created deep inside the machine would re ionize before escaping the machine. Only those neutrals that are born from recombined ions in the border (edge) regions could survive long enough to escape and the ions that birthed the neutral are at their lowest energies there so this would not be a path for significant energy loss.
Dan Tibbets