Rotational phase dependence of magnetar bursts

Abstract

The trigger for the short bursts observed in $\gamma$-rays from many magnetar sources remains unknown. One particular open question in this context is the localization of burst emission to a singular active region or a larger area across the neutron star. While several observational studies have attempted to investigate this question by looking at the phase dependence of burst properties, results have been mixed. At the same time, it is not obvious a priori that bursts from a localized active region would actually give rise to a detectable phase-dependence, taking into account issues such as geometry, relativistic effects, and intrinsic burst properties such brightness and duration. In this paper, we build a simple theoretical model to investigate the circumstances under which the latter effects could affect detectability of a dependence of burst emission on rotational phase. We find that even for strongly phase-dependent emission, inferred burst properties may not show a rotational phase dependence depending on the geometry of the system and the observer. Furthermore, the observed properties of bursts with durations short as 10-20% of the spin period can vary strongly depending on the rotational phase at which the burst was emitted. We also show that detectability of a rotational phase dependence depends strongly on the minimum number of bursts observed, and find that existing burst samples may simply be too small to rule out a phase dependence.

arXiv comment15 pages, 17 figures

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• Repeating Fast Radio Bursts from Magnetars with Low Magnetospheric Twist
• The NICER View of the 2020 Burst Storm and Persistent Emission of SGR 1935+2154
• The Fast Radio Burst Luminosity Function and Death Line in the Low-Twist Magnetar Model
• Burst phase distribution of SGR J1935+2154 based on Insight-HXMT