Colliding Beam Fusion Reactors
Tóm tắt
The recirculating power for virtually all types of fusion reactors has previously been calculated [1] with the Fokker–Planck equation. The reactors involve non-Maxwellian plasmas. The calculations are generic in that they do not relate to specific confinement devices. In all cases except for a Tokamak with D–T fuel the recirculating power was found to exceed the fusion power by a large factor. In this paper we criticize the generality claimed for this calculation. The ratio of circulating power to fusion power is calculated for the Colliding Beam Reactor with fuels D–T, D–He3 and p–B11. The results are respectively, 0.070, 0.141 and 0.493.
Tài liệu tham khảo
Todd H. Rider, Phys. Plasmas, 4, 1039 (1997); also 1998 APS/DPP General Meeting, invited paper R8M3-7, New Orleans Nov. 19, 1998.
W. Heidbrink and G. J. Sadler, Nuclear Fusion, 34, 535 (1994).
3.H. Monkhorst and N. Rostoker, US Patent 6, 611, 106 B-2 Aug 26, 2003 and 6,628,740 B-2 Sept. 30, 2003.
J. Dawson in Fusion edited by E. Teller Vol. 1, p. 489, Academic Press New York (1981); also J. Dawson in EPRI-ER-429-SR a special report on p-B11 fusion reactor, May (1977).
H. J. Monkhorst, M. W. Binderbauer, and N. Rostoker, in 2nd Conference on Current Trends in International Fusion Research, March 10-14, 1997. Proceedings published by NRC Research Press, Ottawa, Canada, (1999).
M. Tuszewski, Nuclear Fusion, 28, 2033 (1988).
N. Rostoker, M. Binderbauer, and H. J. Monkhorst, 1998 APS/DPP General meeting, invited paper R8M3-4, New Orleans, Nov. 19, (1998); N. Rostoker and M. Binderbauer, US Patent # 6,664,740 B-2 Dec. 16, 2003.
L. Landau, Phys. Z. Soviet Union, 10, 154 (1936).
N. Rostoker et al., Phys. Rev. Lett., 70, 1818 (1993).
N. Rostoker and M. Binderbauer, J. Plasma Phys., 56, 451 (1996).
H. Naitou, T. Kamimura, and J. Dawson, J. Phys. Soc. Jpn., 46, 258 (1997); G. Manfredi and R. O. Dendy, Phys. Rev. Lett., 76, 4360 (1996).
N. Rostoker and A. Qerushi, Phys. Plasmas, 9, 3057 (2002).
H. Berk, H. Momota, and T. Tajima, Phys. Fluids, 30, 3548 (1987).
R. Svensson, Astro. Phys. J. 258, 335 (1982).