English

Self-similar solutions to isothermal shock problems

Fluid Dynamics 2018-02-20 v3 High Energy Astrophysical Phenomena

Abstract

We investigate exact solutions for isothermal shock problems in different one-dimensional geometries. These solutions are given as analytical expressions if possible, or are computed using standard numerical methods for solving ordinary differential equations. We test the numerical solutions against the analytical expressions to verify the correctness of all numerical algorithms. We use similarity methods to derive a system of ordinary differential equations (ODE) yielding exact solutions for power law density distributions as initial conditions. Further, the system of ODEs accounts for implosion problems (IP) as well as explosion problems (EP) by changing the initial or boundary conditions, respectively. Taking genuinely isothermal approximations into account leads to additional insights of EPs in contrast to earlier models. We neglect a constant initial energy contribution but introduce a parameter to adjust the initial mass distribution of the system. Moreover, we show that due to this parameter a constant initial density is not allowed for isothermal EPs. Reasonable restrictions for this parameter are given. Both, the (genuinely) isothermal implosion as well as the explosion problem are solved for the first time.

Keywords

Cite

@article{arxiv.1610.07879,
  title  = {Self-similar solutions to isothermal shock problems},
  author = {Stephan C. Deschner and Tobias F. Illenseer and Wolfgang J. Duschl},
  journal= {arXiv preprint arXiv:1610.07879},
  year   = {2018}
}

Comments

24 pages, 15 figures

R2 v1 2026-06-22T16:31:02.660Z