A precessing magnetar model for GLEAM-X J162759.5-523504.3

TL;DR

This paper proposes a precessing magnetar model to explain the radio source GLEAM-X J162759.5-523504.3, linking observed periodicity to magnetar deformation and predicting observable precession in X-ray bands.

Contribution

It introduces a novel precessing magnetar model for GLEAM-X J162759.5-523504.3, connecting magnetic deformation to observed periodicity and making testable predictions.

Findings

Precession period of ~1 ks linked to magnetar deformation.

Predicted spin period of 0.1 s and period derivative of ~10^{-11} s/s.

Precession observable in hard X-ray band.

Abstract

We propose a precessing transient magnetar model for the recently discovered radio source GLEAM-X J162759.5-523504.3. We identify the observed period of $\sim 1$ ks as the precession period of the magnetar deformed due to its strong ($B_{\phi} \sim 10^{16}$ G) toroidal field. The resulting deformation of order $10^{-4}$ implies a spin period of $P_{\rm s} = 0.1$ s. Assuming a strong dipole field of $B_{\rm d} \sim 10^{14}$ G we predict a period derivative of $\dot{P}_{\rm s}\sim 10^{-11}$ s/s. We also predict that the precession period of the magnetar can be observed in the hard X-ray band just as the other three galactic magnetars exhibit precession.