English

3D modeling of collisionless shocks

High Energy Astrophysical Phenomena 2015-05-19 v1 Cosmology and Nongalactic Astrophysics

Abstract

Two dimensional modeling of collisionless shocks has been of tremendous importance in understanding the physics of the non-linear evolution, momentum transfer and particle acceleration, but current computer capacities have now reached a point where three dimensional modeling is becoming feasible. We present the first three dimensional model of a fully developed and relaxed relativistic ion-electron shock, and analyze and compare it to similar 2D models. Quantitative and qualitative differences are found with respect to the two-dimensional models. The shock jump conditions are of course different, because of the extra degree of freedom, but in addition it is found that strong parallel electric fields develop at the shock interface, the level of magnetic field energy is lower, and the non-thermal particle distribution is shallower with a powerlaw index of ~2.2.

Keywords

Cite

@article{arxiv.1007.5082,
  title  = {3D modeling of collisionless shocks},
  author = {Troels Haugboelle},
  journal= {arXiv preprint arXiv:1007.5082},
  year   = {2015}
}

Comments

4 pages, 5 figures, submitted to ApJL

R2 v1 2026-06-21T15:54:23.826Z