Implosion velocity enhancement by M-band preheating: a non-ablative hydrodynamic mechanism
ID:91 View Protection:ATTENDEE Updated Time:2025-04-03 14:26:45 Hits:201 Oral Presentation

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Abstract
The hohlraum hard X-ray flux, like the M-band radiation of gold, may preheat the ICF target and alter the implosion dynamics significantly. Besides its the widely discussed influence on the fuel/ablator interface Atwood number, numerical studies have suggested that higher M-band fraction would also lead to higher implosion velocity (vimp) of the cryogenic DT fuel (by a few percent), accompanied by a decrease in the remaining ablator mass. Very often, this phenomenon is simply attributed to an increase of ablative rocket efficiency.

However, we found with 1-D simulations that even if the radiation module is completely shut down for the final stage of implosion (after shell radius ≈ 1/2 initial radius), vimp of the DT fuel is basically not affected – it will continue rising for about 30%, and shows the difference caused by M-band radiation. Especially, it is in this final stage of acceleration, rather than the earlier times with ablation on, that the difference in vimp emerges.

By a careful investigation of the 1-D radiation hydrodynamic simulation results, we think the increase in DT velocity due to M-band preheating is primarily a hydrodynamic effect, caused by the radial expansion of the remaining ablator material – with entropy set mainly by the M-band energy deposited earlier in these matters. In this manner, the difference in remaining mass is more likely to be the result of this hydrodynamic process, rather than its cause.

Based on these understandings, we propose that the difference in DT vimp caused by M-band radiation may be largely suppressed by increasing the dopant level – if the final chunks of ablator material were well protected from M-band preheating for most of the implosion time, their entropy as well as hydrodynamic behavior would be similar in the final stage, insensitive to the M-band flux screened by the outer layers. i.e., higher ablator opacity may not only alleviate the high-mode hydrodynamic instability at the fuel/ablator interface, but also help to reduces the overall low-mode asymmetry introduced by asymmetric M-band flux.
 
Keywords
inertial confinement fusion,implosion,preheating effect,1-D Simulation
Speaker
ShenJingxiang
博士后 北京应用物理与计算数学研究所

Submission Author
ShenJingxiang 北京应用物理与计算数学研究所
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  • Conference Date

    May 12

    2025

    to

    May 15

    2025

  • Mar 26 2025

    Draft paper submission deadline

  • Apr 30 2025

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  • May 15 2025

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Sponsored By
Institute of Applied Physics and Computational Mathematics, Beijing, China
Shaanxi Normal University, Xi’an, China
Organized By
陕西师范大学
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