Astronomy and Astrophysics – Astrophysics
Scientific paper
Nov 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988uill.rept.....r&link_type=abstract
Final Report, 30 Sep. 1985 - 29 Sep. 1988 Illinois Univ., Chicago. Lab. for Atomic Molecular and Radiation Physics.
Astronomy and Astrophysics
Astrophysics
Astrophysics, Coherent Radiation, Extreme Ultraviolet Radiation, Nonlinearity, Radiation Sources, Stellar Radiation, Thermonuclear Reactions, Gas Lasers, Photons, Rare Gases, Ultraviolet Lasers
Scientific paper
A laboratory means for the generation of ultrahigh energy density states of matter, corresponding approximately to 0.1 to 1.0 W/atom at solid density, is currently under development. This enables the production, in a convenient laboratory environment, of energy densities comparable to those occurring in the thermonuclear environments and stellar interiors. The method being developed involves a unique combination of three basic elements: (1) a new extremely high-peak-power ultraviolet laser technology (femtosecond rare gas halogen system), (2) energy deposition stemming from high-order multiphoton processes, and (3) a mode of channeled propagation that arises in the strong-field regime. The compatibility of these three independent considerations is a key and unique feature of the approach. The use of this technology will permit the study of new realms of atomic phenomena.
Boyer Keith
Luk Ting S.
Rhodes Charles K.
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