Abstract:
This report considers the five-dimensional gravitational solutions that arise within the framework of holographic quantum chromodynamics anisotropic models. These holographic models are supported by the Einstein action with the dilaton field and Maxwell fields. Maxwell's first field is associated with the introduction of a chemical potential. The second field is characterized by the parameter $\nu$ and is responsible for spatial anisotropy. The third field describes the anisotropy associated with an external magnetic field.
