# The Dirac oscillator in a spinning cosmic string spacetime

**Authors:** Mansoureh Hosseinpour, Hassan Hassanabadi, Marc de Montigny

arXiv: 1904.05889 · 2019-04-15

## TL;DR

This paper investigates how a Dirac oscillator behaves in a spinning cosmic string spacetime, analyzing energy levels and eigenfunctions affected by gravitational and topological parameters.

## Contribution

It provides a novel analysis of the Dirac oscillator in a spinning cosmic string background, deriving eigenfunctions and energy spectra considering various physical parameters.

## Key findings

- Eigenfunctions and energy levels are derived for the Dirac oscillator in this spacetime.
- The energy spectrum depends on the string density, rotation frequency, and oscillator parameters.
- The study highlights the influence of topological defects on relativistic quantum systems.

## Abstract

We examine the effects of gravitational fields produced by topological defects on a Dirac field and a Dirac oscillator in a spinning cosmic string spacetime. We obtain the eigenfunctions and the energy levels of the relativistic field in that background and consider the effect of various parameters, such as the frequency of the rotating frame, the oscillator's frequency, the string density and other quantum numbers.

## Full text

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## Figures

3 figures with captions in the complete paper: https://tomesphere.com/paper/1904.05889/full.md

## References

60 references — full list in the complete paper: https://tomesphere.com/paper/1904.05889/full.md

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Source: https://tomesphere.com/paper/1904.05889