English

Analytical solution for the structure of ADAFs

High Energy Astrophysical Phenomena 2015-06-19 v1 Astrophysics of Galaxies

Abstract

The standard Advection-Dominated Accretion Flow (ADAF) is studied using a set of self-similar analytical solutions in the spherical coordinates. Our new solutions are useful for studying ADAFs without dealing with the usual mathematical complexity. We assume the rφr\varphi component of the stress tensor dominates and the latitudinal component of the velocity is negligible. Moreover, the fluid is incompressible and the solutions are radially self-similar. We show that our analytical solutions display most of the important properties of ADAFs which have already been obtained by the detailed numerical solutions. According to our solutions, the density and the pressure of the flow decreases from the equator to the polar regions and this reduction depends on the amount of the advected energy. We also show analytically that an ADAF tends to a quasi-spherical configuration as more energy is advected with the radial flow.

Keywords

Cite

@article{arxiv.1405.7934,
  title  = {Analytical solution for the structure of ADAFs},
  author = {Mohsen Shadmehri},
  journal= {arXiv preprint arXiv:1405.7934},
  year   = {2015}
}

Comments

Accepted for publication in MNRAS

R2 v1 2026-06-22T04:27:12.534Z