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Onset of Hydrodynamic Mix in High-Velocity, Highly Compressed Inertial Confinement Fusion Implosions

Authors :
S. Le Pape
Damien Hicks
V. A. Smalyuk
J. D. Moody
E. L. Dewald
D. A. Callahan
T. Ma
M. H. Key
Joseph Ralph
G. A. Kyrala
Daniel Clark
Harry Robey
Otto Landen
Edward I. Moses
Brian Spears
Jason Ross
B. A. Hammel
D. K. Bradley
Nobuhiko Izumi
S. V. Weber
Siegfried Glenzer
Laura Robin Benedetti
Richard Town
Shahab Khan
P. T. Springer
A. J. Mackinnon
Sean Regan
S. N. Dixit
L. J. Suter
O. S. Jones
T. G. Parham
Bruce Remington
H.-S. Park
Tilo Döppner
Art Pak
Gary Grim
R. Tommasini
L. J. Atherton
J. D. Kilkenny
W. W. Hsing
S. W. Haan
P. M. Celliers
Melissa Edwards
S. M. Glenn
P. K. Patel
D. H. Edgell
Andrew MacPhee
Nathan Meezan
John Kline
C. J. Cerjan
J. D. Lindl
Reuben Epstein
B. J. MacGowan
Source :
Physical Review Letters. 111
Publication Year :
2013
Publisher :
American Physical Society (APS), 2013.

Abstract

Deuterium-tritium inertial confinement fusion implosion experiments on the National Ignition Facility have demonstrated yields ranging from 0.8 to $7\ifmmode\times\else\texttimes\fi{}{10}^{14}$, and record fuel areal densities of 0.7 to $1.3\text{ }\text{ }\mathrm{g}/{\mathrm{cm}}^{2}$. These implosions use hohlraums irradiated with shaped laser pulses of 1.5--1.9 MJ energy. The laser peak power and duration at peak power were varied, as were the capsule ablator dopant concentrations and shell thicknesses. We quantify the level of hydrodynamic instability mix of the ablator into the hot spot from the measured elevated absolute x-ray emission of the hot spot. We observe that DT neutron yield and ion temperature decrease abruptly as the hot spot mix mass increases above several hundred ng. The comparison with radiation-hydrodynamic modeling indicates that low mode asymmetries and increased ablator surface perturbations may be responsible for the current performance.

Details

ISSN :
10797114 and 00319007
Volume :
111
Database :
OpenAIRE
Journal :
Physical Review Letters
Accession number :
edsair.doi.dedup.....f2b5d8cf1a57cdb90a034bcc82502918