Аннотация:
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.
