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Constraining properties of GRB magnetar central engines using the observed plateau luminosity and duration correlation
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Constraining properties of GRB magnetar central engines using the observed plateau luminosity and duration correlation
Bibliographic description
| title: | Constraining properties of GRB magnetar central engines using the observed plateau luminosity and duration correlation |
| author: | Rowlinson Antonia, Gompertz Ben P., Dainotti Maria  , O'Brien Paul T., Wijers Ralph A. M. J., van der Horst Alexander J. |
| journal title: | Monthly Notices of the Royal Astronomical Society |
| volume: | 443 |
| issue: | 2 |
| date of publication : | 2014 |
| pages: | 1779-1787 |
| ISSN: |
0035-8711 |
| eISSN: |
1365-2966 |
| DOI: | |
| language: | English |
| journal language: | English |
| abstract in English: | 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. |
| keywords in English: | gamma-ray bursts: general, stars: magnetars |
| affiliation: | Wydział Fizyki, Astronomii i Informatyki Stosowanej : Instytut – Obserwatorium Astronomiczne |
| type: | journal article |
| subtype: | academic paper |
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Projekt „Repozytorium otwartego dostępu do dorobku naukowego i dydaktycznego UJ” współfinansowany w ramach poddziałania 2.3.1 „Cyfrowe udostępnianie zasobów nauki” Programu Operacyjnego Polska Cyfrowa z Europejskiego Funduszu Rozwoju Regionalnego i budżetu państwa na podstawie umowy o dofinansowanie nr POPC.02.03.01-00-0030/17-00
