AbstractIn this paper, we determine the relativistic and nonrelativistic energy levels for Dirac fermions in a spinning conical Gödel-type spacetime in(2+1)-dimensions, where we work with the curved Dirac equation in polar coordinates and we use the tetrads formalism. Solving a second-order differential equation for the two components of the Dirac spinor, we obtain a generalized Laguerre equation, and the relativistic energy levels of the fermion and antifermion, where such levels are quantized in terms of the radial and total magnetic quantum numbersnandmj, and explicitly depends on the spin parameters(describes the ‘spin’), spinorial parameteru(describes the two components of the spinor), curvature and rotation parametersαandβ(describes the conical curvature and the angular momentum of the spinning cosmic string), and on the vorticity parameter Ω (describes the Gödel-type spacetime). In particular, the quantization is a direct result of the existence of Ω (i.e. such quantity acts as a kind of ‘external field or potential’). We see that formj>0, the energy levels do not depend onsandu; however, depend onn,mj,α, andβ. In this case,αbreaks the degeneracy of the energy levels and such levels can increase infinitely in the limit4Ωβα→1. Already formj<0, we see that the energy levels depends ons,uandn; however, it no longer depends onmj,αandβ. In this case, it is as if the fermion/antifermion ‘lives only in a flat Gödel-type spacetime’. Besides, we also study the low-energy or nonrelativistic limit of the system. In both cases (relativistic and nonrelativistic), we graphically analyze the behavior of energy levels as a function of Ω,α, andβfor three different values ofn(ground state and the first two excited states).
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