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We suggest a short-lived supermassive magnetar model to account for the X-ray flares following short γ-ray bursts. In this model the central engine of the short γ-ray bursts is a supermassive millisecond magnetar, formed in coalescence of double neutron stars. The X-ray flares are powered by the dipole radiation of the magnetar. When the magnetar has lost a significant part of its angular momentum, it collapses to a black hole and the X-ray flares cease abruptly.
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Gao, W. H., & Fan, Y. (2006). Short-living Supermassive Magnetar Model for the Early X-ray Flares Following Short GRBs. 天文和天体物理学研究：英文版, 6(5), 513–516. https://doi.org/10.1088/1009-9271/6/5/01
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