  We explore the effects of anisotropic thermal conduction, anisotropic
pressure, and magnetic field strength on the hot accretion flows around black
holes by solving the axisymmetric, steady-state magnetohydrodynamic equations.
The anisotropic pressure is known as a mechanism for transporting angular
momentum in weakly collisional plasmas in hot accretion flows with extremely
low mass accretion rates. However, anisotropic pressure does not extensively
impact the transport of the angular momentum, it leads to shrinkage of the wind
region. Our results show that the strength of the magnetic field can help the
Poynting energy flux overcomes the kinetic energy flux. This result may be
applicable to understand the hot accretion flow in the Galactic Center Sgr A*
and M87 galaxy.

High Energy Astrophysical Phenomena