Radiation from fast rotating neutron stars

The radiation field of an arbitrarily fast rotating magnetic star is investigated, using the 4-vector formalism in the Deutsch analysis, for a two-fold purpose. The first is to verify that the radiation field of an arbitrarily fast rotating magnetic dipole, obtained by Belinsky et al, corresponds to a relativistically corrected expression for the Deutsch analysis. The second is to investigate the differences between the radiation fields of a fast rotating magnetic dipole and Deutsch star