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Energy loss in anisotropic hot dense QGP in external magnetic field isstudied within holographic approach. Energy loss is calculated by estimation ofbehaviour of the spatial Wilson loops using the effective potential technique.We examine the dependence of the effective potential on the spatial Wilsonloops orientation in fully anisotropic background. For this purpose we obtaingeneral formulas for the effective potential and study appearance of theeffective potential dynamical wall. We consider particular fully anisotropicmodel [arXiv:2011.07023] supported by Einstein-Dilaton-three-Maxwell action.The effective potential strongly depends on the parameters of anisotropy andmagnetic field, therefore the energy loss depends on physical parameters $-$$T$, $\mu$, $c_B$ and orientation. Orientation is determined by angles betweenthe moving heavy quark velocity, the axis of heavy ions collision and theirimpact parameter vector.

Energy Loss in Holographic Anisotropic Model for Heavy Quarks in External Magnetic Field