Bulletin of the American Physical Society
60th Annual Meeting of the APS Division of Plasma Physics
Volume 63, Number 11
Monday–Friday, November 5–9, 2018; Portland, Oregon
Session UP11: Poster Session VIII: MST; DIII-D Tokamak; SPARC, C-Mod, and High Field Tokamaks; HBT-EP; Transport and LPI in ICF Plasmas, Hydrodynamic Instability; HEDP Posters; Space and Astrophysical Plasmas (2:00pm-5:00pm)
Thursday, November 8, 2018
OCC
Room: Exhibit Hall A1&A
Abstract ID: BAPS.2018.DPP.UP11.115
Abstract: UP11.00115 : Modelling electron transport through laser-driven compression of CH plasma with HYDRA**
Presenter:
Krish A Bhutwala
(Univ of California - San Diego)
Authors:
Krish A Bhutwala
(Univ of California - San Diego)
John D Moody
(Lawrence Livermore Natl Lab)
Bradley Pollock
(Lawrence Livermore Natl Lab)
Nathan Meezan
(Lawrence Livermore Natl Lab)
Marty Marinak
(Lawrence Livermore Natl Lab)
Joohwan Kim
(Univ of California - San Diego)
Scott Wilks
(Lawrence Livermore Natl Lab)
Frank R Graziani
(Lawrence Livermore Natl Lab)
Farhat N Beg
(Univ of California - San Diego)
The Fast Ignition (FI) scheme of Inertial Confinement Fusion (ICF) involves fusion fuel compression to high densities via long pulse lasers, followed by fuel heating via electron energy deposition. These electrons are produced by irradiating a metal foil with a high intensity short-pulse laser, producing a beam of 1-10 MeV “hot” electrons. Applying an external magnetic field parallel to the electron beam can prolong the confinement of the hot electrons within the dense plasma, increasing the heating efficiency. We use the radiation-hydrodynamics code HYDRA to investigate the laser-driven compression of cylindrical CH foam and determine the macroscopic plasma properties (temperature, density, etc.). We may then input these properties to the hybrid-PIC code LSP to simulate the electron propagation and energy deposition into the plasma. We compare the results with a recent experiment performed at LLE, where Omega-60 was used to compress CH foam and Omega EP was used to produce hot electrons to propagate with and without a magnetic field.
This work was performed under the auspices of the U.S. Department of Energy by Lawrence Livermore National Laboratory under contract DE-AC52-07NA27344.
LLNL-ABS-XXXXXXXXX
*This work is funded by the NNSA under contracts DE-NA0002728 (NLUF)
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.DPP.UP11.115
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