Orlenys Troconis, Viviane Alfradique, Rodrigo Negreiros

International Journal of Modern Physics: Conference Series

01/01/2017

Abstract

We consider the analytical Bonnor solution for a relativistic neutron star and discuss about the limit in which this solution satisfies Einstein-Maxwell equations. We study the gravitational redshift for Bonnor solution without electric charge. We find that for stars with magnetic fields up to [Formula: see text] in the center, the gravitational redshift for Bonnor metric differs from the Schwarzschild solution on a term that depends on magnetic dipole moment and the polar angle of the emission signal.

10.1142/s2010194517600485