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- W3100986087 abstract "Two plateaus and one following bump in the X-ray light curve of GRB 170714A have been detected by the textit{Swift}/X-Ray Telescope, which could be very meaningful for the central engine of gamma-ray bursts (GRBs), implying that the origin of this burst might be different from that of other ultra-long GRBs. We propose that merging two neutron stars into a hyper-massive quark star (QS) and then collapsing into a black hole (BH), with a delay time around $10^4$~s, could be responsible for those X-ray components. The hyper-massive QS is initially in a fluid state, being turbulent and differentially rotating, but would be solidified and release its latent heat injected into the GRB fireball (lasting about $10^3$~s during the liquid-solid phase transition). Magnetic field as high as $sim 10^{15}$~G could be created by dynamo action of the newborn liquid QS, and a magnetar-like central engine (after solidification) supplies significant energy for the second plateau. More energy could be released during a fall-back accretion after the post-merger QS collapses to a BH, and the X-ray bump forms. This post-merger QS model might be tested by future observations, with either advanced gravitational wave detectors (e.g., advanced LIGO and VIRGO) or X-ray/optical telescopes." @default.
- W3100986087 created "2020-11-23" @default.
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- W3100986087 date "2018-02-16" @default.
- W3100986087 modified "2023-10-16" @default.
- W3100986087 title "The X-Ray Light Curve in GRB 170714A: Evidence for a Quark Star?" @default.
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- W3100986087 doi "https://doi.org/10.3847/1538-4357/aaabba" @default.
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