English

Spherical explosion with central energy source

High Energy Astrophysical Phenomena 2016-03-09 v1 Solar and Stellar Astrophysics

Abstract

We present a novel semi-analytic solution describing the propagation of a spherical blast wave driven by a central energy source. The initial density profile has a power-law function of the distance from the center and the energy is injected only into the central region at a rate given by a power-law function of time. This solution is composed of three regions separated by the contact surface and the shock front. The innermost region is assumed to be uniform and the outside of the contact surface includes the shocked matter described by self-similar solutions. We analytically derive the applicable range of parameters of this solution from requirements to satisfy boundary conditions. We perform numerical simulations for flows with various values of parameters, some of which reside out of the thus derived applicable range, and compare with the semi-analytic solutions.

Cite

@article{arxiv.1512.06952,
  title  = {Spherical explosion with central energy source},
  author = {Miyu Masuyama and Toshikazu Shigeyama and Yoichiro Tsuboki},
  journal= {arXiv preprint arXiv:1512.06952},
  year   = {2016}
}

Comments

11 pages, 3 figures, accepted for publication in PASJ

R2 v1 2026-06-22T12:15:36.552Z