Repository logo
Log in(current)
Repository logoMIT Open ScholarshipDSpace@MIT
  1. Home
  2. MIT Open Access Articles
  3. MIT Open Access Articles
  4. First Observations of Nonhydrodynamic Mix at the Fuel-Shell Interface in Shock-Driven Inertial Confinement Implosions

First Observations of Nonhydrodynamic Mix at the Fuel-Shell Interface in Shock-Driven Inertial Confinement Implosions

Thumbnail Image
Download
Name

Rinderknecht-2014-First observations of nonhydrodynamic mix.pdf

Size

816.51 KB

Format

Adobe PDF

Checksum (MD5)

62ea56e6d643021e48f38a1c0843b262

Author(s)
Amendt, P.
•
Delettrez, J. A.
•
Bellei, C.
•
Betti, R.
•
Glebov, V. Yu.
•
Meyerhofer, D. D.
•
Sangster, T. C.
•
Stoeckl, C.
•
Landen, O. L.
•
Smalyuk, V. A.
more
Date Issued
April 2014
Journal
Physical Review Letters
Publisher
American Physical Society
Citation
Rinderknecht, H. G., H. Sio, C. K. Li, A. B. Zylstra, M. J. Rosenberg, P. Amendt, J. Delettrez, et al. “First Observations of Nonhydrodynamic Mix at the Fuel-Shell Interface in Shock-Driven Inertial Confinement Implosions.” Physical Review Letters 112, no. 13 (April 2014). © 2014 American Physical Society
Version
Final published version
Abstract
A strong nonhydrodynamic mechanism generating atomic fuel-shell mix has been observed in strongly shocked inertial confinement fusion implosions of thin deuterated-plastic shells filled with [superscript 3]He gas. These implosions were found to produce D[superscript 3]He-proton shock yields comparable to implosions of identical shells filled with a hydroequivalent 50∶50 D[superscript 3]He gas mixture. Standard hydrodynamic mixing cannot explain this observation, as hydrodynamic modeling including mix predicts a yield an order of magnitude lower than was observed. Instead, these results can be attributed to ion diffusive mix at the fuel-shell interface.
MIT Department
Massachusetts Institute of Technology. Department of Physics
Massachusetts Institute of Technology. Plasma Science and Fusion Center
Terms of Use
Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.
Persistent DSpace Link
http://hdl.handle.net/1721.1/88999
DOI of Published Version
https://doi.org/10.1103/PhysRevLett.112.135001
Repository logo
PrivacyPermissionsAccessibilityContact us
Repository logo
Notify us about copyright concerns.