# Dirac states of an electron in a circular intense magnetic field

**Authors:** Guillaume Voisin (LUTH), Silvano Bonazzola (LUTH), Fabrice Mottez, (CNRS, LUTH)

arXiv: 1703.05193 · 2017-04-12

## TL;DR

This paper models Dirac electron states in intense, curved magnetic fields relevant to neutron-star magnetospheres, extending Landau states to curved geometries and setting the stage for analyzing quantum curvature radiation.

## Contribution

It introduces a theoretical framework for Dirac particles in curved magnetic fields, generalizing Landau states to curved geometries in neutron-star environments.

## Key findings

- Derived Dirac states in curved magnetic fields with small Larmor radius.
- Connected curved magnetic field states to relativistic Landau states as a limit.
- Laid groundwork for future analysis of quantum curvature radiation.

## Abstract

Neutron-star magnetospheres are structured by very intense magnetic fields extending from 100 to 10 5 km traveled by very energetic electrons and positrons with Lorentz factors up to $\sim$ 10 7. In this context, particles are forced to travel almost along the magnetic field with very small gyro-motion, potentially reaching the quantified regime. We describe the state of Dirac particles in a locally uniform, constant and curved magnetic field in the approximation that the Larmor radius is very small compared to the radius of curvature of the magnetic field lines. We obtain a result that admits the usual relativistic Landau states as a limit of null curvature. We will describe the radiation of these states, that we call quantum curvature or synchro-curvature radiation, in an upcoming paper.

## Full text

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## Figures

2 figures with captions in the complete paper: https://tomesphere.com/paper/1703.05193/full.md

## References

18 references — full list in the complete paper: https://tomesphere.com/paper/1703.05193/full.md

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Source: https://tomesphere.com/paper/1703.05193