Art Carlson wrote:D Tibbets wrote:....
Does Rider figure bremsstrahlung on a thermalized electron population, or a dominantly radial electron direction that is cold in the center and hot on the periphery? I believe this is one of the necessary conditions for Polywell to work. If so, Rider's conclusions are presumably correct for the assumptions he made, but does not match the Polywell assumptions.
Rider quickly dismissed using electric fields to reflect the electrons lost through the cusps using much the same arguments as I did: What reduces problems with the electrons aggravates problem with the ions. If recirculation helps anyway, then it helps reduce the cusp losses, but not the bremsstrahlung. The bremsstrahlung power he cites is for Maxwellian electrons, but only after he first shows that the the electron distribution will rapidly thermalize. He mentions that trying to maintain a non-thermal distribution by bleeding off particles will aggravate energy losses that are already too high. I think he has all the bases covered.
D Tibbets wrote:Also, a 5 to 1 ratio of P to B11 was quoted. I think (?) I have heard of a 10 to 1 ratio proposed by someone. This would presumably help the bremsstrahlung some but also decrease the fusion rate, so I don't know if there would be any net gain.
The optimum fuel ratio to minimize P_brem/P_fus is n_1:n_2 = Z_1:Z_2.
D Tibbets wrote:Is the 'Phi_well = 900 kV' the potential well depth? This seems high if it is.......
Rider goes to a good deal of effort at the beginning to explain why you can't really take advantage of any resonances in the cross section. I'm not sure, but his well depth may have been optimized in light of ion losses through up-scattering.
Does bleeding off high energy electrons waste too much energy? If an escaping electron has an energy of 50.000eV and the magrid is 20,000 volts, then 30,000 eV is lost. But if the escaping electron has an energy of 20,100 eV, then only 100 eV is lost. So, I'm supposing there is some relationship between the rate of electron upscattering to higher energies and the lifefime of the electron. In other words, the upscattered electrons have a progressively shorter amount of time to pick up more energy before they escape (assuming the electrons have ~ the same number of transits befor escaping-eg: 100,000). This might keep the lost energy of most of the escaping (nonrecirculating) electrons low. Or another way to look at it is that the electrons are removed at low cost when those electrons are only a modest distance past the average (mean?) peak of the maxwell distribution, rather than waiting till they reach the much higher energy tail.
As far as ions and electrons having equal but opposite responces to conservation attempts in the cusps, I'm guessing that this would only fully apply if the cusp flows are ambipolar, which they are claimed not to be.
Rider's optamistic estimate of a ~ 10 fold shortfall in the energy balance is actually fairly close to what Bussard was saying, up untill the claimed breakthrough with electron recirculation in WB6.
Bremsstrulung radiation could be modeled on the BIG hole in the center. I don't see why this would cost energy. It is dependant on the non thermalized assumption. I capitalized the adjative BIG to emphasize that the core region not only removes some of the area aviable to brem generation in a thermalized model, but also due to convergance and slowing of the electrons in the middle (again assuming some significant degree of non thermalization over the life time of the electrons) which results in a disproportionate concentration of the electrons in the core region. It seems odd that there is (?) a central concentration of both electrons and ions (I assume this correlates to an elliptical potential well -vs- a square well). I'm guessing that it is due to the dynamic time dependant distribution of the electrons, and the convergence of the ions overcomeing the greater time they spend in the perifery.
Brem -vs- fusion rate based on your formula makes sense. But only if the slopes of both curves have the same slope. At 900 KeV the slope of the P-B11 crossection is pretty shallow compared to what it is at say 200 KeV.
Does the brem curve follow the same profile? I'm guessing that this may be one reason why a larger reactor is needed for P-B11 compared to a D-D. The cross section matches or slightly favors P-B11 compared to D-D at higher voltages. Increasing the size presumably could compensate for a lower fusion rate due to higher proton to boron ratios, but a disproportionate decrease in brem radiation.
Why a 900 KeV well to reduce upscattered ion losses? If the potential well equals X eV: then theoretically, any ion upscattered to X+1 eV could potentially escape if it hits a cusp. I assume that the higher electron potential and probably stronge magnets to adequatly containe electrons at that energy would result in a more efficient wiffleball. Did Rider believe in or at least accept the wiffleball argument in his 900KeV calculation. If the wiffleball is real, does it even apply to this required well depth argument?
I'm supposing the ion loss rate would be the same weather you had a 20 KeV potential well or a 900KeV well, everything else being equal. Would this change if it was a thermalized ion population? Are the Maxwell curves different at these different temperatures?
I wonder how many of these questions have been at least tenatively answered by EMC's unpublished data (thermalization times, annealing, cusp energy losses -vs- particle losses, confluence, other transport losses, fusion collision types, etc.)
Dan Tibbets
To error is human... and I'm very human.