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 BP11: Poster Session I: HEDP; General Stellarator; Wendelstein 7-X; Heating, Current Drive, and Energetic Ions (9:30am-12:30pm)
Monday, November 5, 2018
OCC
Room: Exhibit Hall A1&A
Abstract ID: BAPS.2018.DPP.BP11.9
Abstract: BP11.00009 : X-ray diagnostic development for electron beam driven WDM studies*
Presenter:
Nicholas Ramey
(Los Alamos Natl Lab, Univ of Michigan - Ann Arbor)
Authors:
Nicholas Ramey
(Los Alamos Natl Lab, Univ of Michigan - Ann Arbor)
Joshua Coleman
(Los Alamos Natl Lab)
James P Colgan
(Los Alamos Natl Lab)
John Perry
(Los Alamos Natl Lab)
Heidi E Morris
(Los Alamos Natl Lab)
Ronald Matthew Gilgenbach
(Univ of Michigan - Ann Arbor)
Ryan D McBride
(Univ of Michigan - Ann Arbor)
A platform for characterizing the equation-of-state of the warm dense matter (WDM) regime is being developed on an intense, relativistic electron accelerator1,2. An 80-ns (FWHM) electron pulse with a beam current of 1.7 kA and energy of 19.8 MeV deposits energy into a thin, low-Z metal foil heating it to a warm dense plasma. LASNEX hydrodynamic simulations suggest the relatively large scale (~100 μm) WDM lasts 100 ns after the beam pulse providing a background-free measurement window for deploying X-ray diagnostics. Time-resolved X-ray shadowgraphy will be used to measure the spatial extent of the WDM. X-ray absorption spectroscopy can measure the temperature and density of the WDM by tailoring backlighter/crystal pairs to the plasma under interrogation. Calculations and simulations will be presented to evaluate the feasibility of different X-ray sources and detection techniques for each diagnostic. Full scale Geant4 simulations to estimate photon yields and guide experimental deployment are underway.
1. J.E. Coleman and J. Colgan, Phys. Rev. E 96, 013208 (2017).
2. J.E. Coleman and J. Colgan, Physics of Plasmas 24, 083302 (2017).
*This work was supported by the National Nuclear Security Administration of the U.S. Department of Energy under Contract No. DE-AC52-06NA25396.
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.DPP.BP11.9
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