The unusual X-ray emission of the short Swift GRB 090515: Evidence for the formation of a magnetar?

TL;DR

This paper analyzes the unusual X-ray emission of the short GRB 090515, proposing it may be due to a forming magnetar, which challenges the typical black hole formation model for short gamma-ray bursts.

Contribution

It presents Swift and Gemini observations of GRB 090515 and suggests the unusual emission is caused by an unstable millisecond pulsar, providing constraints on its spin and magnetic field.

Findings

High initial X-ray flux observed for a short GRB

Unusual plateau and steep decay in X-ray light curve

Constraints on magnetar spin period and magnetic field

Abstract

The majority of short gamma-ray bursts (SGRBs) are thought to originate from the merger of compact binary systems collapsing directly to form a black hole. However, it has been proposed that both SGRBs and long gamma-ray bursts (LGRBs) may, on rare occasions, form an unstable millisecond pulsar (magnetar) prior to final collapse. GRB 090515, detected by the Swift satellite was extremely short, with a T_90 of 0.036 +/- 0.016 s, and had a very low fluence of 2 x 10^-8 erg cm^-2 and faint optical afterglow. Despite this, the 0.3 - 10 keV flux in the first 200 s was the highest observed for a SGRB by the Swift X-ray Telescope (XRT). The X-ray light curve showed an unusual plateau and steep decay, becoming undetectable after ~500 s. This behaviour is similar to that observed in some long bursts proposed to have magnetars contributing to their emission. In this paper, we present the Swift observations of GRB 090515 and compare it to other gamma-ray bursts (GRBs) in the Swift sample. Additionally, we present optical observations from Gemini, which detected an afterglow of magnitude 26.4 +/- 0.1 at T+ 1.7 hours after the burst. We discuss potential causes of the unusual 0.3 - 10 keV emission and suggest it might be energy injection from an unstable millisecond pulsar. Using the duration and flux of the plateau of GRB 090515, we place constraints on the millisecond pulsar spin period and magnetic field.