Approaches to the Monopole-Dynamic Dipole Vacuum Solution Concerning the Structure of Its Ernst Potential on the Symmetry Axis

The FHP (Fodor, Hoenselaers, Perjés) algorithm 1] allows to obtain the relativistic multipole moments of a vacuum stationary axisymmetric solution in terms of coefficients which appear in the expansion of its Ernst potential on the symmetry axis. First of all, we will use this result in order to determine, at a certain approximation degree, the Ernst potential on the symmetry axis of the metric whose only multipole moments are mass and angular momentum. By using Sibgatullin's method 2] we then analyse a series of exact solutions with the afore mentioned multipole characteristic; besides, we present an approximate solution whose Ernst potential is introduced as a power series of a dimensionless parameter. The calculation of its multipole moments allows us to understand the existing differences between both approximations to the proposed pure multipole solution.