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3D Simulations Capture the Persistent Low-Mode Asymmetries Evident in Laser-Direct-Drive Implosions on OMEGA

Authors :
A. Colaïtis
D. P. Turnbull
I. V. Igumenschev
D. Edgell
R. C. Shah
O. M. Mannion
C. Stoeckl
D. Jacob-Perkins
A. Shvydky
R. Janezic
A. Kalb
D. Cao
C. J. Forrest
J. Kwiatkowski
S. Regan
W. Theobald
V. N. Goncharov
D. H. Froula
Centre d'Etudes Lasers Intenses et Applications (CELIA)
Université de Bordeaux (UB)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Centre National de la Recherche Scientifique (CNRS)
Laboratory for lasers energetics - LLE (New-York, USA)
University of Rochester [USA]
European Project: 633053,H2020,EURATOM-Adhoc-2014-20,EUROfusion(2014)
Source :
Physical Review Letters, Physical Review Letters, 2022, 129 (9), pp.095001. ⟨10.1103/PhysRevLett.129.095001⟩
Publication Year :
2022
Publisher :
American Physical Society (APS), 2022.

Abstract

Spherical implosions in inertial confinement fusion are inherently sensitive to perturbations that may arise from experimental constraints and errors. Control and mitigation of low-mode (long wavelength) perturbations is a key milestone to improving implosion performances. We present the first 3D radiation-hydrodynamic simulations of directly driven inertial confinement fusion implosions with an inline package for polarized crossed-beam energy transfer. Simulations match bang times, yields (separately accounting for laser-induced high modes and fuel age), hot spot flow velocities and direction, for which polarized crossed-beam energy transfer contributes to the systematic flow orientation evident in the OMEGA implosion database. Current levels of beam mispointing, imbalance, target offset, and asymmetry from polarized crossed-beam energy transfer degrade yields by more than 40%. The effectiveness of two mitigation strategies for low modes is explored.

Details

ISSN :
10797114 and 00319007
Volume :
129
Database :
OpenAIRE
Journal :
Physical Review Letters
Accession number :
edsair.doi.dedup.....7f9c10d173d94d52d25797a93b58b808
Full Text :
https://doi.org/10.1103/physrevlett.129.095001