Anisotropic holographic models supported by Einstein-dilaton-four-Maxwell action

This talk 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 four Maxwell fields. Maxwell's first field is associated with the introduction of a chemical potential. The second field is responsible for the spatial anisotropy. The third and fourth fields describe the anisotropy associated with an external magnetic field. It is shown that we have only 6 independent equations out of 7 in the fully anisotropic case due to the Bianchi identity and EOM connection. The scheme of finding a solution is presented.