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Interpreting the X-ray afterglows of gamma-ray bursts with radiative losses and millisecond magnetars

By Nikhil Sarin, Paul D. Lasky and Gregory Ashton

Abstract

The spin-down energy of millisecond magnetars has been invoked to explain X-ray afterglow observations of a significant fraction of short and long gamma-ray bursts. Here, we extend models previously introduced in the literature, incorporating radiative losses with the spin down of a magnetar central engine through an arbitrary braking index. Combining this with a model for the tail of the prompt emission, we show that our model can better explain the data than millisecond-magnetar models without radiative losses or those that invoke spin down solely through vacuum dipole radiation. We find that our model predicts a subset of X-ray flares seen in some gamma-ray bursts. We can further explain the diversity of X-ray plateaus by altering the radiative efficiency and measure the braking index of newly-born millisecond magnetars. We measure the braking index of GRB061121 as $n=4.85^{+0.11}_{-0.15}$ suggesting the millisecond-magnetar born in this gamma-ray burst spins down predominantly through gravitational-wave emission.Comment: Submitted to MNRA

Topics: Astrophysics - High Energy Astrophysical Phenomena
Year: 2020
OAI identifier: oai:arXiv.org:2008.05745

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