Relativistic Shock Reflection using Integral Conservation Laws
Jonathan Granot, Michael Rabinovich

TL;DR
This paper develops a new integral conservation law approach in the lab frame to analyze relativistic shock wave reflection, especially in super-luminal regimes where traditional steady-state methods fail, with implications for astrophysics.
Contribution
It introduces a novel method using integral conservation laws in the lab frame to study relativistic shock reflection, including super-luminal regimes, unifying sub-luminal and super-luminal analysis.
Findings
Bounded parameter space for weak and strong shock solutions.
Existence of critical lines (detachment and luminal) defining solution regimes.
Strong shock solutions only exist within specific incidence angle ranges.
Abstract
Shock wave reflection from a rigid wall has been thoroughly studied in the Newtonian limit, simplifying the problem by analyzing it in a steady-state frame, , where the point of the shock's intersection with the wall is at rest. However, a "super-luminal" regime emerges when the velocity of point () exceeds the speed of light (), where no steady-state frame exists. It occurs predominantly in the relativistic regime, relevant in astrophysics, where it encompasses nearly all of the shock incidence angles. To study this regime, we introduce a new approach. We formulate integral conservation laws in the lab frame (where the unshocked fluid is at rest) for regular reflection (RR), using two methods: a. fixed volume analysis and b. fixed fluid analysis. We show the equivalence between the two methods, and also to the steady-state oblique shock jump conditions…
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Taxonomy
TopicsAstrophysics and Star Formation Studies · Computational Fluid Dynamics and Aerodynamics · Astrophysical Phenomena and Observations
