paper

Dirac fermions in a spinning conical Gödel-type spacetime

arXiv:2405.11334 · doi:10.1088/1361-6382/ad69f5

Abstract

In this paper, we determine the relativistic and nonrelativistic energy levels for Dirac fermions in a spinning conical Gödel-type spacetime in -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 numbers and , and explicitly depends on the spin parameter (describes the ``spin''), spinorial parameter (describes the two components of the spinor), curvature and rotation parameters and (describes the conical curvature and the angular momentum of the spinning cosmic string), and on the vorticity parameter (describes the Gödel-type spacetime). In particular, the quantization is a direct result of the existence of (i.e. acts as a kind of ``external field or potential''). We see that for , the energy levels do not depend on and ; however, depend on , , , and . In this case, breaks the degeneracy of the energy levels and such levels can increase infinitely in the limit . Already for , we see that the energy levels depends on , and ; however, it no longer depends on , and . In this case, it is as if the fermion ``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 , , and for three different values of (ground state and the first two excited states).

15 pages, 6 figures. arXiv admin note: text overlap with arXiv:2402.15720

Dirac fermions in a spinning conical Gödel-type spacetime · wovepaper