Role of ionization potential depression for generation of strongly coupled plasmas in high-pressure supercritical fluids
摘要
The photosphere, one of the Sun’s inner layers, and white dwarfs exist as plasmas with high electron density and relatively low temperature, satisfying the strongly coupled condition that the Coulomb coupling parameter exceeds unity. While strongly coupled plasmas are prevalent throughout space, it is difficult to produce and sustain such states in the laboratory with a sufficiently long lifetime for investigation of basic transport processes. To surmount these obstacles, we have developed a laser-produced plasma experiment in supercritical fluids of He, Ar, and Kr. For helium at 100 bar, a nanosecond laser pulse generates a strongly coupled plasma with an electron density, estimated from ionization potential depression (IPD) modeling, of approximately