Relativistic disk
In general relativity, the relativistic disk expression refers to a class of axi-symmetric self-consistent solutions to Einstein's field equations corresponding to the gravitational field generated by axi-symmetric isolated sources. To find such solutions, one has to pose correctly and solve together the 'outer' problem, a boundary value problem for vacuum Einstein's field equations whose solution determines the external field, and the 'inner' problem, whose solution determines the structure and the dynamics of the matter source in its own gravitational field.