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Revisiting the Strong Shock Problem: Converging and Diverging Shocks in Different Geometries

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arxiv 2102.07235 v2 pith:ZFEWKDRK submitted 2021-02-14 astro-ph.HE physics.flu-dyn

classification astro-ph.HEphysics.flu-dyn
keywords convergingshockself-similarshockssolutionsdifferentdivergingentirety
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abstract

Self-similar solutions to converging (implosions) and diverging (explosions) shocks have been studied before, in planar, cylindrical or spherical symmetry. Here we offer a unified treatment of these apparently disconnected problems . We study the flow of an ideal gas with adiabatic index $\gamma$ with initial density $\rho\sim r^{-\omega}$, containing a strong shock wave. We characterize the self-similar solutions in the entirety of the parameter space $\gamma,\omega$, and draw the connections between the different geometries. We find that only type II self-similar solutions are valid in converging shocks, and that in some cases, a converging shock might not create a reflected shock after its convergence. Finally, we derive analytical approximations for the similarity exponent in the entirety of parameter space.

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Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Cold Stream Penetration of Virial Shocks: Fragmentation, Coagulation, and Disruption in the Hot Circumgalactic Medium

    astro-ph.GA 2026-07 conditional novelty 6.0 of 10

    Cold streams penetrating virial shocks survive and fragment at z>2 but are shock-heated and suppressed at z<0.5, depending on whether the post-shock gas cools before the halo-crossing time.

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