Direct-drive double-shell implosion: A platform for burning-plasma physics studies

S. X. Hu, R. Epstein, W. Theobald, H. Xu, H. Huang, V. N. Goncharov, S. P. Regan, P. W. McKenty, R. Betti, E. M. Campbell, and D. S. Montgomery
Phys. Rev. E 100, 063204 – Published 12 December 2019

Abstract

Double-shell ignition designs have been studied with the indirect-drive inertial confinement fusion (ICF) scheme in both simulations and experiments in which the inner-shell kinetic energy was limited to ∼10–15 kJ, even driven by megajoule-class lasers such as the National Ignition Facility. Since direct-drive ICF can couple more energy to the imploding shells, we have performed a detailed study on direct-drive double-shell (D3S) implosions with state-of-the-art physics models implemented in radiation-hydrodynamic codes (lilac and draco), including nonlocal thermal transport, cross-beam energy transfer (CBET), and first-principles−based material properties. To mitigate classical unstable interfaces, we have proposed the use of a tungsten-beryllium–mixed inner shell with gradient-density layers that can be made by magnetron sputtering. In our D3S designs, a 70-μm-thick beryllium outer shell is driven symmetrically by a high-adiabat (α10), 1.9-MJ laser pulse to a peak velocity of ∼240 km/s. Upon spherical impact, the outer shell transfers ∼30–40 kJ of kinetic energy to the inner shell filled with deuterium-tritium gas or liquid, giving neutron-yield energies of ∼6 MJ in one-dimensional simulations. Two-dimensional high-mode draco simulations indicated that such high-adiabat D3S implosions are not susceptible to laser imprint, but the long-wavelength perturbations from the laser port configuration along with CBET can be detrimental to the target performance. Nevertheless, neutron yields of ∼0.3–1.0-MJ energies can still be obtained from our high-mode draco simulations. The robust α-particle bootstrap is readily reached, which could provide a viable platform for burning-plasma physics studies. Once CBET mitigation and/or more laser energy becomes available, we anticipate that break-even or moderate energy gain might be feasible with the proposed D3S scheme.

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  • Received 25 September 2019

DOI:https://doi.org/10.1103/PhysRevE.100.063204

©2019 American Physical Society

Physics Subject Headings (PhySH)

Plasma Physics

Authors & Affiliations

S. X. Hu1,*, R. Epstein1, W. Theobald1, H. Xu2, H. Huang2, V. N. Goncharov1, S. P. Regan1, P. W. McKenty1, R. Betti1, E. M. Campbell1, and D. S. Montgomery3

  • 1Laboratory for Laser Energetics, University of Rochester, 250 E. River Road, Rochester, New York 14623, USA
  • 2General Atomics, San Diego, California 92121, USA
  • 3Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA

  • *shu@lle.rochester.edu

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Vol. 100, Iss. 6 — December 2019

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