Asymptotic self-similar solutions with a characteristic time-scale

TL;DR

This paper broadens the understanding of self-similar solutions in adiabatic gas flows, showing that more general forms, including exponential solutions, are physically relevant and analyzing their behavior in blast-wave scenarios.

Contribution

It introduces a generalized form of self-similar solutions that includes exponential behavior, extending previous assumptions and analyzing their physical relevance in blast-wave dynamics.

Findings

Exponential self-similar solutions occur at a critical density slope.

Flow behavior changes at a critical density exponent $\omega_c$.

New solutions describe the asymptotic behavior for $\omega extgreater\omega_c$.

Abstract

For a wide variety of initial and boundary conditions, adiabatic one dimensional flows of an ideal gas approach self-similar behavior when the characteristic length scale over which the flow takes place, $R$, diverges or tends to zero. It is commonly assumed that self-similarity is approached since in the $R\to\infty(0)$ limit the flow becomes independent of any characteristic length or time scales. In this case the flow fields $f(r,t)$ must be of the form $f(r,t)=t^{\alpha_f}F(r/R)$ with $R\propto(\pm t)^\alpha$. We show that requiring the asymptotic flow to be independent only of characteristic length scales imply a more general form of self-similar solutions, $f(r,t)=R^{\delta_f}F(r/R)$ with $\dot{R}\propto R^\delta$, which includes the exponential ($\delta=1$) solutions, $R\propto e^{t/\tau}$. We demonstrate that the latter, less restrictive, requirement is the physically relevant one by showing that the asymptotic behavior of accelerating blast-waves, driven by the release of energy at the center of a cold gas sphere of initial density $\rho\propto r^{-\omega}$, changes its character at large $\omega$: The flow is described by $0\le\delta<1$, $R\propto t^{1/(1-\delta)}$, solutions for $\omega<\omega_c$, by $\delta>1$ solutions with $R\propto (-t)^{1/(\delta-1)}$ diverging at finite time ($t=0$) for $\omega>\omega_c$, and by exponential solutions for $\omega=\omega_c$ ($\omega_c$ depends on the adiabatic index of the gas, $\omega_c\sim8$ for $4/3<\gamma<5/3$). The properties of the new solutions obtained here for $\omega\ge\omega_c$ are analyzed, and self-similar solutions describing the $t>0$ behavior for $\omega>\omega_c$ are also derived.