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Two-dimensional simulations of plastic-shell, direct-drive implosions on OMEGA

  • P. B. Radha
  • , V. N. Goncharov
  • , T. J.B. Collins
  • , J. A. Delettrez
  • , Y. Elbaz
  • , V. Yu Glebov
  • , R. L. Keck
  • , D. E. Keller
  • , J. P. Knauer
  • , J. A. Marozas
  • , F. J. Marshall
  • , P. W. McKenty
  • , D. D. Meyerhofer
  • , S. P. Regan
  • , T. C. Sangster
  • , D. Shvarts
  • , S. Skupsky
  • , Y. Srebro
  • , R. P.J. Town
  • , C. Stoeckl

Research output: Contribution to journalArticlepeer-review

155 Scopus citations

Abstract

Multidimensional hydrodynamic properties of high-adiabat direct-drive plastic-shell implosions on the OMEGA laser system [T. R. Boehly, Opt. Commun. 133, 495 (1997)] are investigated using the multidimensional hydrodynamic code, DRACO [D. Keller, Bull. Am. Phys. Soc. 44, 37 (1999)]. Multimode simulations including the effects of nonuniform illumination and target roughness indicate that shell stability during the acceleration phase plays a critical role in determining target performance. For thick shells that remain integral during the acceleration phase, target yields are significantly reduced by the combination of the long-wavelength (ℓ<10) modes due to surface roughness and beam imbalance and the intermediate modes (20≤ℓ≤50) due to single-beam nonuniformities. The neutron-production rate for these thick shells truncates relative to one-dimensional (1D) predictions. The yield degradation in the thin shells is mainly due to shell breakup at short wavelengths (λ~Δ, where Δ is the in-flight shell thickness). The neutron-rate curves for the thinner shells have significantly lower amplitudes and a fall-off that is less steep than 1D rates. DRACO simulation results are consistent with experimental observations.

Original languageEnglish
Article number032702
Pages (from-to)1-18
Number of pages18
JournalPhysics of Plasmas
Volume12
Issue number3
DOIs
StatePublished - 25 Apr 2005
Externally publishedYes

ASJC Scopus subject areas

  • Condensed Matter Physics

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