Studying radiative shocks using laser driven blast waves in clustered gases

We report on the creation of radiative blast waves by irradiating gases of atomic clusters with intense short pulse laser light. The efficient absorption of the cluster medium leads to high energy deposition and development into a cylindrical shock. These non-equilibrium, optically thin shocks have...

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Main Authors: Symes, DR, Hohenberger, M, Doyle, H, Smith, R, Moore, A, Gumbrell, E, Rodriguez, R, Gil, J
Format: Journal article
Language:English
Published: 2011
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author Symes, DR
Hohenberger, M
Doyle, H
Smith, R
Moore, A
Gumbrell, E
Rodriguez, R
Gil, J
author_facet Symes, DR
Hohenberger, M
Doyle, H
Smith, R
Moore, A
Gumbrell, E
Rodriguez, R
Gil, J
author_sort Symes, DR
collection OXFORD
description We report on the creation of radiative blast waves by irradiating gases of atomic clusters with intense short pulse laser light. The efficient absorption of the cluster medium leads to high energy deposition and development into a cylindrical shock. These non-equilibrium, optically thin shocks have great potential for hydrodynamic scaling with astrophysical relevance, particularly for supernova remnants. We discuss how cluster blast waves may become susceptible to spatial and temporal instabilities and the application of the RAPCAL atomic physics code to determine our plasma conditions. © 2010 Elsevier B.V.
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spelling oxford-uuid:9300c545-b246-4233-a0e1-694cf8e1b0a52022-03-26T23:29:23ZStudying radiative shocks using laser driven blast waves in clustered gasesJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:9300c545-b246-4233-a0e1-694cf8e1b0a5EnglishSymplectic Elements at Oxford2011Symes, DRHohenberger, MDoyle, HSmith, RMoore, AGumbrell, ERodriguez, RGil, JWe report on the creation of radiative blast waves by irradiating gases of atomic clusters with intense short pulse laser light. The efficient absorption of the cluster medium leads to high energy deposition and development into a cylindrical shock. These non-equilibrium, optically thin shocks have great potential for hydrodynamic scaling with astrophysical relevance, particularly for supernova remnants. We discuss how cluster blast waves may become susceptible to spatial and temporal instabilities and the application of the RAPCAL atomic physics code to determine our plasma conditions. © 2010 Elsevier B.V.
spellingShingle Symes, DR
Hohenberger, M
Doyle, H
Smith, R
Moore, A
Gumbrell, E
Rodriguez, R
Gil, J
Studying radiative shocks using laser driven blast waves in clustered gases
title Studying radiative shocks using laser driven blast waves in clustered gases
title_full Studying radiative shocks using laser driven blast waves in clustered gases
title_fullStr Studying radiative shocks using laser driven blast waves in clustered gases
title_full_unstemmed Studying radiative shocks using laser driven blast waves in clustered gases
title_short Studying radiative shocks using laser driven blast waves in clustered gases
title_sort studying radiative shocks using laser driven blast waves in clustered gases
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