Analysis of Spin-1/2 Particle Scattering in a Spinning Cosmic String Spacetime with Torsion, Curvature, and a Coulomb Potential
Abdelmalek Boumali

TL;DR
This paper analyzes how spin-1/2 particles scatter in a spinning cosmic string spacetime with torsion and curvature, revealing geometric effects on scattering patterns and potential applications in Dirac materials like graphene.
Contribution
It provides exact solutions for Dirac particles in complex cosmic-string geometries, including effects of torsion, rotation, and Coulomb interaction, with implications for condensed matter systems.
Findings
Geometry modifies effective azimuthal quantum number
Strong rotation introduces a radial cutoff acting as a hard wall
Conical curvature and torsion produce Aharonov-Bohm-like effects
Abstract
This paper investigates the scattering states of spin-1/2 particles in the spacetime of a spinning cosmic string with spacelike disclination and dislocation, with and without a Coulomb interaction. Working within the tetrad formalism, we solve the Dirac equation for several configurations of the angular momentum density and the torsion parameter that are relevant from a physical perspective. These configurations include balanced torsion (), pure spinning strings (), pure screw dislocations () and the general case. In all cases, the geometry modifies an effective azimuthal quantum number, and for strong rotation it introduces a geometric radial cutoff that acts as a hard wall. These factors lead to closed-form expressions for the radial wave functions, phase shifts and differential cross sections, which are expressed in terms of confluent…
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