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Studies of localized mix and asymmetry caused by the stalk in inertial fusion experiments at OMEGA

Title: Studies of localized mix and asymmetry caused by the stalk in inertial fusion experiments at OMEGA
Authors: Kunimune, J. H.; Reichelt, B. L.; Forrest, C. J.; Gerbsch, K.; Haines, B. M.; Luo, R.; McClow, H.; Schwemmlein, A.; Shuldberg, C.; Wink, C. W.; Gatu Johnson, M.; Frenje, J. A.
Contributors: Fusion Energy Sciences; EnergeticsNational Inertial Confinement Fusion Program; NNSA; Department of Energy National Nuclear Security Administration Laboratory Residency Graduate Fellowship
Source: Physics of Plasmas ; volume 33, issue 4 ; ISSN 1070-664X 1089-7674
Publisher Information: AIP Publishing
Publication Year: 2026
Description: In an inertially confined fusion experiment, a capsule of fusion fuel is compressed to high temperatures and densities using lasers, creating a hot plasma in which thermonuclear fusion reactions take place. To achieve efficient conversion of laser energy to fuel heating, the implosion must be as spherically symmetric as possible. One common source of asymmetry that degrades performance is the stalk and glue spot that hold the capsule in place before the experiment. The exact nature and magnitude of this perturbation had not been previously quantified. In this work, inertially confined fusion experiments were executed with an additional stalk on the capsule to measure and quantify the effect of the stalk and glue spot on the symmetry and performance. It is found that the stalk drives low-mode asymmetry by shadowing the laser drive on the part of the shell near the glue spot, enhancing the hot-spot velocity toward the stalk by 40–80 km/s and elongating the hot-spot along the stalk axis. It is also found that localized mix due to the additional stalk has a negligible effect on implosion performance. Two-dimensional radiation-hydrodynamic simulations using the xRAGE code reproduce the direction of the experimentally observed change to hot-spot velocity and implosion performance metrics, but not the observed elongation, suggesting that this feature results from an interaction between stalk perturbations and other preexisting asymmetry seeds, such as laser drive asymmetry.
Document Type: article in journal/newspaper
Language: English
DOI: 10.1063/5.0310230
DOI: 10.1063/5.0310230/20962583/042702_1_5.0310230.pdf
Availability: https://doi.org/10.1063/5.0310230; https://pubs.aip.org/aip/pop/article-pdf/doi/10.1063/5.0310230/20962583/042702_1_5.0310230.pdf
Rights: https://creativecommons.org/licenses/by/4.0/
Accession Number: edsbas.F51360C3
Database: BASE