  We investigate black holes with toroidal horizons in (d +1)-dimensional
space-time. Using the solution phase space method, we calculated conserved
charges for these black holes before exploring some features of this metric
including its entropy and thermodynamic quantities. Another aspect of the study
involves obtaining a general exact static interior solution for uncharged black
holes with toroidal horizons in (d+1)-dimensional space-time. Finally, an
interior solution for charged black holes is obtained.
