Bulletin of the American Physical Society
60th Annual Meeting of the APS Division of Plasma Physics
Volume 63, Number 11
Monday–Friday, November 5–9, 2018; Portland, Oregon
Session CO6: Hohlraum and X-ray Cavity Physics
2:00 PM–4:48 PM,
Monday, November 5, 2018
OCC
Room: B115-116
Chair: Pierre Michel, Lawrence Livermore National Laboratory
Abstract ID: BAPS.2018.DPP.CO6.14
Abstract: CO6.00014 : Re-evaluation of the Pulsed Power Indirect Drive Approach to Inertial Confinement Fusion
4:36 PM–4:48 PM
Presenter:
R. E. Olson
(Los Alamos National Laboratory)
Authors:
R. E. Olson
(Los Alamos National Laboratory)
R. R. Peterson
(Los Alamos National Laboratory)
S. H. Batha
(Los Alamos National Laboratory)
A. B. Zylstra
(Los Alamos National Laboratory)
P. A. Bradley
(Los Alamos National Laboratory)
R. J. Leeper
(Los Alamos National Laboratory)
Recently, the results of ICF experiments at the NIF have fostered discussions concerning a possible next generation ICF facility that could enable much higher levels of thermonuclear burn in the laboratory. Key questions include the type of driver that should be proposed and the power and energy parameters that would be required. In the 1990’s, LANL and SNL collaborated on a series of pulsed power experiments that demonstrated X ray driven hohlraums1,2. The X ray driven hohlraum experiments were motivated by an ICF concept that would use a 2-step radiation temperature to implode a high gain indirect-drive ICF capsule3,4. At that time, scaling studies indicated that the required driver size would be unfeasible with the existing pulsed power technology. However, with a new generation of efficient, reduced cost pulsed power technology, it is now feasible to envision a petawatt-class pulsed power facility5. Thus, it is timely to re-consider the pulsed power indirect drive approach to ICF.
1R. E. Olson et al., Phys. Plasmas 4, 1818 (1997).
2T. W. L. Sanford et al., Phys. Rev. Lett. 83, 5511 (1999).
3R. E. Olson et al., Bull. Am. Phys. Soc. 43, 1882 (1998)
4R. E. Olson et al., Fusion Technology 35, 260 (1999).
5W. A. Stygar et al., Phys. Rev. STAB 18, 110401 (2015).
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.DPP.CO6.14
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