Mechanisms of shape transfer and preheating in indirect-drive double shell collisions

Author:

Loomis E. N.1ORCID,Robey H. F.1,Haines B. M.1ORCID,Morrow T.1ORCID,Montgomery D. S.1,Wilson D. C.1ORCID,Xu H.2,Millot M.3ORCID,Celliers P.3ORCID,Sacks R.1ORCID,Sauppe J. P.1ORCID,Quintana T.1,Heinbockel C.2ORCID,Kroll J.3,Randolph B.1,Fierro F.1,Wilson C.1,Daughton W.1ORCID,Merritt E.1ORCID,Finnegan S. M.1ORCID,Kot L.1ORCID,Keiter P.1ORCID,Sagert I.1,Stark D. J.1ORCID,Amendt P.3ORCID,Ping Y.3ORCID,Smalyuk V. A.3,Patel M. V.3ORCID,Salmonson J. D.3

Affiliation:

1. Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA

2. General Atomics, San Diego, California 92186, USA

3. Lawrence Livermore National Laboratory, Livermore, California 94550, USA

Abstract

Implosions of Hohlraum-driven double shell targets as an alternative inertial confinement fusion concept are underway at the National Ignition Facility. The double shell system relies on a series of energy transfer processes starting from thermal x-ray absorption by the outer shell, followed by collisional transfer of kinetic energy to a heavy metal inner shell, and finally, conversion to the internal energy of the deuterium-tritium fuel. During each of these energy transfer stages, low-mode asymmetries can act to reduce the ideal transfer efficiency degrading double shell performance. Mechanisms, such as hard x-ray preheat from the Hohlraum, not only decrease the efficiency of kinetic energy transfer but may also be a source of low-mode asymmetry. In this article, we evaluate the shape transfer processes through the time of shell collision using two-dimensional integrated Hohlraum and capsule computations. We find that the dominant mode of the shape transfer is well described using a “radial impulse” model from the shape of the foam pressure reservoir. To evaluate the importance of preheat on inner shell shape, we also report on first measurements of Au L-shell preheat asymmetry in a double shell with a tungsten pusher. These measurements showed a 65% higher preheat velocity at the pole of the capsule relative to the equator. We also found that the experiments provided rigorous constraints by which to test the Hohlraum model settings that impact the amount and symmetry of Au L-shell preheat via the plasma conditions inside the outer cone Au bubble.

Funder

Los Alamos National Laboratory

Lawrence Livermore National Laboratory

General Atomics

Publisher

AIP Publishing

Subject

Condensed Matter Physics

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