Evolution of Radiative Blast Waves

Details Evolution of Radiative Blast Waves Evolution of Radiative Blast Waves

Oct 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aps..dppup1047k&link_type=abstract

American Physical Society, 43rd Annual Meeting of the APS Division of Plasma Physics October 29 - November 2, 2001 Long Beach, C

Physics

Plasma Physics

Scientific paper

We simulate experiments performed with the Falcon laser at Lawrence Livermore National Laboratory to generate strong blast waves expanding in cylindrical geometry of relevance to astrophysics. In particular, we are interested in producing and modeling radiative shocks. Our goal is to develop a laboratory setting for studying radiative shocks of relevance to supernova remnants. In previous work we have demonstrated that it is possible to generate radiative shocks in the laboratory. In additions, we have shown how we can determine the energy-loss rate of the shock from the blast wave evolution using a simple analytic method that is independent of the details of radiative cooling and is scalable to both the laboratory and astrophysical blast waves. Our current work deals with instabilities associated with radiative blast waves and their application to the laboratory and to astrophysics. In addition, we describe our work in generating a self-similar solution to the expansion of a radiative blast wave, both in the ISM and in the laboratory.

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