https://doi.org/10.1140/epjc/s10052-025-14866-8
Regular Article - Theoretical Physics
Quantum dynamics of scalar particles in a spinning cosmic string background with topological defects: a Feshbach–Villars formalism perspective
Laboratory of Theoretical and Applied Physics, Echahid Cheikh Larbi Tebessi University, Tebessa, Algeria
a
boumali.abdelmalek@gmail.com
Received:
22
July
2025
Accepted:
27
September
2025
Published online:
5
November
2025
We study the relativistic quantum dynamics of spin-0 particles in the spacetime of a spinning cosmic string that carries both spacelike disclination (conical deficit
) and screw dislocation (torsion
) together with frame dragging (
). Using the Feshbach–Villars (FV) reformulation of the Klein–Gordon equation, we obtain a first-order Hamiltonian with a positive-definite density, enabling a clean probabilistic interpretation for bosons in curved/topologically nontrivial backgrounds. In the weak-field regime (retaining terms
and discarding the
contribution that would otherwise lead to (double)-confluent Heun behavior), separation of variables in a finite cylinder of radius
yields a Bessel radial equation with an effective index
that mixes rotation and torsion. The hard-wall condition
quantizes the spectrum,
Working in the stationary positive-energy sector, we derive closed-form normalized eigenfunctions and FV densities, and we evaluate information-theoretic indicators (Fisher information and Shannon entropy) directly from the FV probability density. We find that increased effective confinement (via geometry/torsion) enhances Fisher information and reduces position-space Shannon entropy, quantitatively linking defect parameters to localization/complexity. The FV framework thus provides a robust, computationally transparent route to spectroscopy and information measures for scalar particles in rotating/torsional string backgrounds, and it smoothly reproduces the pure-rotation, pure-torsion, and flat-spacetime limits.
© The Author(s) 2025
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Funded by SCOAP3.
