Stability of stagnation via an expanding accretion shock wave
A. L. Velikovich, M. Murakami, B. D. Taylor, J. L. Giuliani, S. T., Zalesak, and Y. Iwamoto

TL;DR
This paper theoretically analyzes the stability of stagnation via an expanding accretion shock wave in plasma physics, demonstrating that such stagnation is stable with perturbations decaying over time, supported by simulations.
Contribution
It provides the first theoretical stability analysis of stagnation via an expanding shock wave in ideal-gas flows, including explicit eigenvalue formulas and simulation validation.
Findings
Stagnation flow is stable with perturbations decaying over time.
Eigenmodes exhibit power-law, oscillatory, or monotonic decay.
Results support hydro code verification in 2D and 3D simulations.
Abstract
Stagnation of a cold plasma streaming to the center or axis of symmetry via an expanding accretion shock wave is ubiquitous in inertial confinement fusion (ICF) and high-energy-density plasma physics, the examples ranging from plasma flows in x-ray-generating Z pinches [Y. Maron et al., Phys. Rev. Lett. 111, 035001 (2013)] to the experiments in support of the recently suggested concept of impact ignition in ICF [H. Azechi et al., Phys. Rev. Lett. 102, 235002 (2009); M. Murakami et al., Nucl. Fusion 54, 054007 (2014)]. Some experimental evidence indicates that stagnation via an expanding shock wave is stable, but its stability has never been studied theoretically. We present such analysis for the stagnation that does not involve a rarefaction wave behind the expanding shock front and is described by the classic ideal-gas Noh solution in spherical and cylindrical geometry. In either case…
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