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GRB 130831a: Rise and demise of a magnetar at z = 0.5

De Pasquale, M; Page, MJ; Zane, S; Breeveld, AA; Oates, SR; Castro-Tirado, AJ; Gorosabel, J; ... Burkhonov, O; + view all (2017) GRB 130831a: Rise and demise of a magnetar at z = 0.5. In: Bianchi, M and Jantzen, RT and Ruffini, R, (eds.) Proceedings of the MG14 Meeting on General Relativity: On Recent Developments in Theoretical and Experimental General Relativity, Astrophysics, and Relativistic Field Theories. (pp. pp. 2981-2988). World Scientific Publishing Green open access

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Abstract

Gamma-ray bursts (GRBs) are the brightest explosions in the universe, yet the properties of their energy sources are far from understood. Very important clues, however, can be deduced by studying the afterglows of these events. We present observations of GRB 130831A and its afterglow obtained with Swift, Chandra, and multiple ground-based observatories. This burst shows an uncommon drop in the X-ray light curve at about 100 ks after the trigger, with a decay slope of α 7. The standard Forward Shock (FS) model offers no explanation for such a behaviour. Instead, a model in which a newly born magnetar outflow powers the early X-ray emission is found to be viable. After the drop, the X-ray afterglow resumes its decay with a slope typical of FS emission. The optical emission, on the other hand, displays no clear break across the X-ray drop and its decay is consistent with that of the late X-rays. Using both the X-ray and optical data, we show that the FS model can explain the emission after 100 ks. We model our data to infer the kinetic energy of the ejecta and thus estimate the efficiency of a magnetar “central engine” of a GRB. Furthermore, we break down the energy budget of this GRB into prompt emission, late internal dissipation, kinetic energy of the relativistic ejecta, and compare it with the energy of the accompanying supernova, SN 2013fu.

Type: Proceedings paper
Title: GRB 130831a: Rise and demise of a magnetar at z = 0.5
Event: The Fourteenth Marcel Grossmann Meeting
ISBN-13: 9789813226593
Open access status: An open access version is available from UCL Discovery
DOI: 10.1142/9789813226609_0375
Publisher version: https://doi.org/10.1142/9789813226609_0375
Language: English
Additional information: This is an Open Access article distributed under the terms of the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
UCL classification: UCL
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Space and Climate Physics
URI: https://discovery.ucl.ac.uk/id/eprint/10065516
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