Initial data for general relativity containing a marginally outer trapped torus

Asymptotically flat, time-symmetric, axially symmetric, and conformally flat initial data for vacuum general relativity are studied numerically on R(3) With the interior of a standard torus cut out. By the choice of boundary condition the torus is marginally outer trapped, and thus a surface of minimal area. Apart from pure scaling the standard tori are parametrized by a radius a is an element of[0,1], where a=0 corresponds to the limit where the boundary torus degenerates to a circle and a=1 to a torus that touches the axis of symmetry. Noting that these tori are the orbits of a U(1)XU(1) conformal isometry allows for a simple scheme to solve the constraint, involving numerical solution of only ordinary differential equations. Regular solutions can be constructed for a is an element of]a(0) similar to 0.14405,1[. The tori are unstable minimal surfaces (i.e., only saddle points of the area functional) and thus cannot be apparent horizons, but they are always surrounded by an apparent horizon of spherical topology, which is analyzed in the context of the hoop conjecture and isoperimetric inequality for black holes.