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.CO6.9
Abstract: CO6.00009 : Advanced Hohlraum Designs on the NIF for High Coupling Efficiency*
3:36 PM–3:48 PM
Presenter:
Peter Andrew Amendt
(Lawrence Livermore Natl Lab)
Authors:
Peter Andrew Amendt
(Lawrence Livermore Natl Lab)
Darwin Ho
(Lawrence Livermore Natl Lab)
William Kruer
(Lawrence Livermore Natl Lab)
John D Lindl
(Lawrence Livermore Natl Lab)
Nathan Meezan
(Lawrence Livermore Natl Lab)
The coupling of 3ω laser light to the capsule in hohlraum designs for the NIF is typically <10%, resulting in an absorbed energy Ecap of 200 kJ or less in cylindrical hohlraums driven at 2 MJ. Ignition thresholds or performance margins scale linearly with Ecap, so that a significant improvement in these metrics may require considering non-standard hohlraum shapes, e.g., rugbys [1] or a “frustraum”. The frustraum is formed by joining a pair of frusta (or truncated right-circular cones) above the capsule. The low surface area of the frustraum allows for a tradeoff in increased volume above the capsule to facilitate inner beam propagation and accommodate a far larger capsule than the nominal ~1 mm radius size. Integrated hohlraum simulations suggest Ecap~ 500 kJ at only 1.8 MJ laser energy and 460 TW peak power for HDC capsules of radius 1.5 mm may be achievable under conditions of adequate drive symmetry and low backscatter risk. The greatest modeling uncertainty in these candidate hohlraum geometries is the relative balance of specular and diffuse reflection of the outer cones from the oblique hohlraum wall and its high impact on drive symmetry. [1] P. Amendt et al., PoP 21, 112703 (2014)
*Prepared by LLNL under Contract DE-AC52-07NA27344 and supported by LDRD-17-ERD-119.
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.DPP.CO6.9
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