How high energy fluxes may affect Rayleigh–Taylor instability growth in young supernova remnants

How high energy fluxes may affect Rayleigh–Taylor instability growth in young supernova remnants

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.

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Autores principales: 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
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Lenguaje:EN
Publicado: Nature Portfolio 2018
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Acceso en línea:https://doaj.org/article/f153b9b02a5a45d6934610dc34ba9b57
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spelling oai:doaj.org-article:f153b9b02a5a45d6934610dc34ba9b572021-12-02T16:49:17ZHow high energy fluxes may affect Rayleigh–Taylor instability growth in young supernova remnants10.1038/s41467-018-03548-72041-1723https://doaj.org/article/f153b9b02a5a45d6934610dc34ba9b572018-04-01T00:00:00Zhttps://doi.org/10.1038/s41467-018-03548-7https://doaj.org/toc/2041-1723Radiation 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.C. C. KuranzH.-S. ParkC. M. HuntingtonA. R. MilesB. A. RemingtonT. PlewaM. R. TranthamH. F. RobeyD. ShvartsA. ShimonyK. RamanS. MacLarenW. C. WanF. W. DossJ. KlineK. A. FlippoG. MalamudT. A. HandyS. PrisbreyC. M. KraulandS. R. KleinE. C. HardingR. WallaceM. J. GrosskopfD. C. MarionD. KalantarE. GiraldezR. P. DrakeNature PortfolioarticleScienceQENNature Communications, Vol 9, Iss 1, Pp 1-6 (2018)
institution DOAJ
collection DOAJ
language EN
topic Science
Q
spellingShingle Science
Q
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
How high energy fluxes may affect Rayleigh–Taylor instability growth in young supernova remnants
description 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.
format article
author 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
author_facet 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
author_sort C. C. Kuranz
title How high energy fluxes may affect Rayleigh–Taylor instability growth in young supernova remnants
title_short How high energy fluxes may affect Rayleigh–Taylor instability growth in young supernova remnants
title_full How high energy fluxes may affect Rayleigh–Taylor instability growth in young supernova remnants
title_fullStr How high energy fluxes may affect Rayleigh–Taylor instability growth in young supernova remnants
title_full_unstemmed How high energy fluxes may affect Rayleigh–Taylor instability growth in young supernova remnants
title_sort how high energy fluxes may affect rayleigh–taylor instability growth in young supernova remnants
publisher Nature Portfolio
publishDate 2018
url https://doaj.org/article/f153b9b02a5a45d6934610dc34ba9b57
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