Robustness of IFE relevant implosions to low-mode asymmetries
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Conditions for neutrino emission processes domination of highly evolved star luminosity, disputing Fowler-Hoyle collapse temperature for 30 solar mass stars
Shock tube with cylindrical explosive to implode glass wall and produce high velocity glass particle jet, studying jet velocity and behavior and test gas pressure effects
Cold wall and multibody collision effects on reflection of imploding shock waves using Monte Carlo method and molecular dynamics
Spectroscopic study of imploding shock waves in hemispherical chamber filled with O-H-He mixture at high pressure
An approximate analytical solution is developed for the evolution of an interstellar neutral cloud exposed to the ionizing radiation of a newly formed star. The structure of a steady photoevaporation gas flow off a spherical ionization front is derived even for cases where the ionization front cannot be considered thin, and the downstream flow is not in ionization and thermal equilibrium. Under a wide range of conditions, the ionization front is approximately D-critical, and the ionized gas expands supersonically into the intercloud medium. The ionization front typically drives a strong shock into the initial cloud.
Compression by a spherical solid liner of a gold target surrounded by a hydrogen plasma is simulated. Two-dimensional simulations that treat only a subset of the physics included in the one-dimensional code were performed in an attempt to assess multidimensional effects. A one-dimensional numerical code has been developed to study the effects of thermal radiation and conduction. Results of pressure, density, and energy deposited for different initial plasma conditions are presented and discussed. Results from both one- and two-dimensional codes show that the average target density at peak compression is 39-43 g/cu cm, using the SHIVA Star facility at 90 kV discharge.
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