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Demonstration of Fuel Hot-Spot Pressure in Excess of 50 Gbar for Direct-Drive, Layered Deuterium-Tritium Implosions on OMEGA.

Authors :
Regan SP
Goncharov VN
Igumenshchev IV
Sangster TC
Betti R
Bose A
Boehly TR
Bonino MJ
Campbell EM
Cao D
Collins TJ
Craxton RS
Davis AK
Delettrez JA
Edgell DH
Epstein R
Forrest CJ
Frenje JA
Froula DH
Gatu Johnson M
Glebov VY
Harding DR
Hohenberger M
Hu SX
Jacobs-Perkins D
Janezic R
Karasik M
Keck RL
Kelly JH
Kessler TJ
Knauer JP
Kosc TZ
Loucks SJ
Marozas JA
Marshall FJ
McCrory RL
McKenty PW
Meyerhofer DD
Michel DT
Myatt JF
Obenschain SP
Petrasso RD
Radha PB
Rice B
Rosenberg MJ
Schmitt AJ
Schmitt MJ
Seka W
Shmayda WT
Shoup MJ
Shvydky A
Skupsky S
Solodov AA
Stoeckl C
Theobald W
Ulreich J
Wittman MD
Woo KM
Yaakobi B
Zuegel JD
Source :
Physical review letters [Phys Rev Lett] 2016 Jul 08; Vol. 117 (2), pp. 025001. Date of Electronic Publication: 2016 Jul 07.
Publication Year :
2016

Abstract

A record fuel hot-spot pressure P_{hs}=56±7  Gbar was inferred from x-ray and nuclear diagnostics for direct-drive inertial confinement fusion cryogenic, layered deuterium-tritium implosions on the 60-beam, 30-kJ, 351-nm OMEGA Laser System. When hydrodynamically scaled to the energy of the National Ignition Facility, these implosions achieved a Lawson parameter ∼60% of the value required for ignition [A. Bose et al., Phys. Rev. E 93, 011201(R) (2016)], similar to indirect-drive implosions [R. Betti et al., Phys. Rev. Lett. 114, 255003 (2015)], and nearly half of the direct-drive ignition-threshold pressure. Relative to symmetric, one-dimensional simulations, the inferred hot-spot pressure is approximately 40% lower. Three-dimensional simulations suggest that low-mode distortion of the hot spot seeded by laser-drive nonuniformity and target-positioning error reduces target performance.

Details

Language :
English
ISSN :
1079-7114
Volume :
117
Issue :
2
Database :
MEDLINE
Journal :
Physical review letters
Publication Type :
Academic Journal
Accession number :
27447511
Full Text :
https://doi.org/10.1103/PhysRevLett.117.025001