Constraining properties of GRB magnetar central engines using the observed plateau luminosity and duration correlation

An intrinsic correlation has been identified between the luminosity and duration of plateaus in the X-ray afterglows of gamma-ray bursts (GRBs; Dainotti et al. 2008), suggesting a central engine origin. The magnetar central engine model predicts an observable plateau phase, with plateau durations an...

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Bibliographic Details
Published in:Monthly notices of the Royal Astronomical Society 2014-09, Vol.443 (2), p.1779-1787
Main Authors: Rowlinson, A., Gompertz, B. P., Dainotti, M., O'Brien, P. T., Wijers, R. A. M. J., van der Horst, A. J.
Format: Article
Language:English
Subjects:
Correlation
Emission
Engines
Gamma ray astronomy
Gamma ray bursts
Gamma rays
Luminosity
Mathematical models
Spreads
Starbursts
Stars & galaxies
Statistical methods
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Summary:An intrinsic correlation has been identified between the luminosity and duration of plateaus in the X-ray afterglows of gamma-ray bursts (GRBs; Dainotti et al. 2008), suggesting a central engine origin. The magnetar central engine model predicts an observable plateau phase, with plateau durations and luminosities being determined by the magnetic fields and spin periods of the newly formed magnetar. This paper analytically shows that the magnetar central engine model can explain, within the 1σ uncertainties, the correlation between plateau luminosity and duration. The observed scatter in the correlation most likely originates in the spread of initial spin periods of the newly formed magnetar and provides an estimate of the maximum spin period of ∼35 ms (assuming a constant mass, efficiency and beaming across the GRB sample). Additionally, by combining the observed data and simulations, we show that the magnetar emission is most likely narrowly beamed and has ≲20 per cent efficiency in conversion of rotational energy from the magnetar into the observed plateau luminosity. The beaming angles and efficiencies obtained by this method are fully consistent with both predicted and observed values. We find that short GRBs and short GRBs with extended emission lie on the same correlation but are statistically inconsistent with being drawn from the same distribution as long GRBs, this is consistent with them having a wider beaming angle than long GRBs.
ISSN:0035-8711
1365-2966
DOI:10.1093/mnras/stu1277