In this work the dynamics of a 2D Dirac oscillator in the spacetime of a
magnetic cosmic string is considered. It is shown that earlier approaches to
this problem have neglected a δ function contribution to the full
Hamiltonian, which comes from the Zeeman interaction. The inclusion of spin
effects leads to results which confirm a modified dynamics. Based on the
self-adjoint extension method, we determined the most relevant physical
quantities, such as energy spectrum, wave functions and the self-adjoint
extension parameter by applying boundary conditions allowed by the system.Comment: 9 pages, 2 figures, published versio