A 266 nm Mach-Zehnder interferometer with ICCD imaging and Fourier analysis was developed to measure line-integrated electron densities in nanosecond-resolved dense plasmas generated in 100-bar supercritical helium, yielding a peak local density of ~2.5e18 cm^{-3} after Abel inversion.
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Simulations show that intermediate-mass progenitors with non-degenerate cores before helium burning produce a mass-orbital period relation for massive white dwarfs that accounts for long-period systems.
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Nanosecond-resolved 266 nm Mach-Zehnder interferometry for electron-density measurements of dense plasmas generated in supercritical fluids
A 266 nm Mach-Zehnder interferometer with ICCD imaging and Fourier analysis was developed to measure line-integrated electron densities in nanosecond-resolved dense plasmas generated in 100-bar supercritical helium, yielding a peak local density of ~2.5e18 cm^{-3} after Abel inversion.
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Mass-Orbital Period Distribution of Massive White Dwarfs Formed Through Stable Mass Transfer
Simulations show that intermediate-mass progenitors with non-degenerate cores before helium burning produce a mass-orbital period relation for massive white dwarfs that accounts for long-period systems.