Signature of Triaxially Precessing Magnetars in Gamma-ray Burst X-Ray Afterglows
Biao Zhang, Shu-Qing Zhong, Long Li, Zi-Gao Dai

TL;DR
This paper identifies and models quasi-periodic oscillations in the X-ray afterglows of certain gamma-ray bursts, attributing them to the precession of newborn millisecond magnetars, thus providing evidence for early magnetar precession.
Contribution
The study introduces a model of magnetic dipole radiation from a triaxially precessing magnetar to explain observed flux variations in GRB afterglows, supporting the presence of early magnetar precession.
Findings
Successfully fitted four GRB afterglow light curves with the precession model.
Identified three categories of GRBs based on periodicity evidence.
Provided observational support for early precession in newborn magnetars.
Abstract
The X-ray afterglows of some gamma-ray bursts (GRBs) exhibit plateaus, which can be explained by the internal dissipation of a newborn millisecond magnetar wind. In the early phase of these newborn magnetars, the magnetic inclination angle undergoes periodic changes due to precession, leading to periodic modulation of the injection luminosity due to magnetic dipole radiation. This may result in quasi-periodic oscillations (QPOs) on the plateaus. In this paper, we identify four GRBs with regular flux variations on their X-ray afterglow plateaus from Swift/XRT data before November 2023, three of which exhibit periodicity. Based on the likelihood of supporting a precessing magnetar as the central engine, we classify them into three categories: Gold (GRB 060202 and GRB 180620A), Silver (GRB 050730), and Bronze (GRB 210610A). We invoke a model of magnetic dipole radiation emitted by a…
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Taxonomy
TopicsGamma-ray bursts and supernovae
