Scattering and bound states of a spin--1/2 neutral particle in the cosmic string spacetime

TL;DR

This paper investigates the relativistic quantum behavior of a neutral spin-1/2 particle in cosmic string spacetime, revealing new bound states and scattering properties influenced by a point interaction and boundary conditions.

Contribution

It introduces the effects of spin-charge interaction in cosmic string spacetime using self-adjoint extensions, uncovering bound states not previously discussed.

Findings

Bound states are identified via S-matrix poles.

Scattering amplitude depends on energy, indicating non-conservation of helicity.

The approach incorporates point interactions through boundary conditions.

Abstract

In this paper the relativistic quantum dynamics of a spin-1/2 neutral particle with a magnetic moment $\mu$ in the cosmic string spacetime is reexamined by applying the von Neumann theory of self--adjoint extensions. Contrary to previous studies where the interaction between the spin and the line of charge is neglected, here we consider its effects. This interaction gives rise to a point interaction: $\boldsymbol{\nabla} \cdot \mathbf{E}= (2\lambda/\alpha)\delta(r)/r$. Due to the presence of the Dirac delta function, by applying an appropriated boundary condition provided by the theory of self--adjoint extensions, irregular solutions for the Hamiltonian are allowed. We address the scattering problem obtaining the phase shift, S-matrix and the scattering amplitude. The scattering amplitude obtained shows a dependency with energy which stems from the fact that the helicity is not conserved in this system. Examining the poles of the S-matrix we obtain an expression for the bound states. The presence of bound states for this system has not been discussed before in the literature.