Late-time hohlraum pressure dynamics in supernova remnant experiments

Details Late-time hohlraum pressure dynamics in supernova remnant experiments Late-time hohlraum pressure dynamics in supernova remnant experiments

Jun 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001phpl....8.2609h&link_type=abstract

Physics of Plasmas, Volume 8, Issue 6, pp. 2609-2612 (2001).

Physics

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Shock Waves And Discontinuities, Plasma Production And Heating By Laser Beams, Laboratory Studies Of Space- And Astrophysical-Plasma Processes, Magnetohydrodynamics And Plasmas, Plasma Production And Heating By Shock Waves And Compression, Plasma Simulation, Supernova Remnants

Scientific paper

It is shown that laser driven hohlraums obtain significant internal pressures which affect the hydrodynamics of high-energy density shock-tube experiments. By incorporating this previously neglected hohlraum pressure effect (in addition to the usual x-ray drive) into computer simulations which model the NOVA laser driven supernova remnant experiment [R. P. Drake, S. G. Glendinning, K. Estabrook, B. A. Remington, R. McCray, R. J. Williams, L. J. Suter, T. B. Smith, J. J. Carroll III, R. A. London, and E. Liang, Phys. Rev. Lett. 81, 2068 (1998)], calculations are able to reproduce the observed structure of hydrodynamic features.

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