Nature Communications (Apr 2018)
How high energy fluxes may affect Rayleigh–Taylor instability growth in young supernova remnants
- C. C. Kuranz,
- H.-S. Park,
- C. M. Huntington,
- A. R. Miles,
- B. A. Remington,
- T. Plewa,
- M. R. Trantham,
- H. F. Robey,
- D. Shvarts,
- A. Shimony,
- K. Raman,
- S. MacLaren,
- W. C. Wan,
- F. W. Doss,
- J. Kline,
- K. A. Flippo,
- G. Malamud,
- T. A. Handy,
- S. Prisbrey,
- C. M. Krauland,
- S. R. Klein,
- E. C. Harding,
- R. Wallace,
- M. J. Grosskopf,
- D. C. Marion,
- D. Kalantar,
- E. Giraldez,
- R. P. Drake
Affiliations
- C. C. Kuranz
- University of Michigan
- H.-S. Park
- Lawrence Livermore National Laboratory
- C. M. Huntington
- Lawrence Livermore National Laboratory
- A. R. Miles
- Lawrence Livermore National Laboratory
- B. A. Remington
- Lawrence Livermore National Laboratory
- T. Plewa
- Florida State University
- M. R. Trantham
- University of Michigan
- H. F. Robey
- Lawrence Livermore National Laboratory
- D. Shvarts
- Ben Gurion University of the Negev
- A. Shimony
- Ben Gurion University of the Negev
- K. Raman
- Lawrence Livermore National Laboratory
- S. MacLaren
- Lawrence Livermore National Laboratory
- W. C. Wan
- University of Michigan
- F. W. Doss
- Los Alamos National Laboratory
- J. Kline
- Los Alamos National Laboratory
- K. A. Flippo
- Los Alamos National Laboratory
- G. Malamud
- University of Michigan
- T. A. Handy
- University of Michigan
- S. Prisbrey
- Lawrence Livermore National Laboratory
- C. M. Krauland
- General Atomics
- S. R. Klein
- University of Michigan
- E. C. Harding
- Sandia National Laboratory
- R. Wallace
- Lawrence Livermore National Laboratory
- M. J. Grosskopf
- Simon Fraser University
- D. C. Marion
- University of Michigan
- D. Kalantar
- Lawrence Livermore National Laboratory
- E. Giraldez
- General Atomics
- R. P. Drake
- University of Michigan
- DOI
- https://doi.org/10.1038/s41467-018-03548-7
- Journal volume & issue
-
Vol. 9,
no. 1
pp. 1 – 6
Abstract
Radiation and conduction are generally considered as the main energy transport mechanisms for the evolution of early supernova remnants. Here the authors experimentally show the role of electron heat transfer on the growth of Rayleigh–Taylor instability in young supernova remnants.
