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- W3100274681 abstract "GRB 111005A, one long duration gamma-ray burst (GRB) occurred within a metal-rich environment that lacks massive stars with $M_{rm ZAMS}geq 15M_odot$, is not coincident with supernova emission down to stringent limit and thus should be classified as a long-short GRB (lsGRB; also known as SN-less long GRB or hybrid GRB), like GRB 060505 and GRB 060614. In this work we show that in the neutron star merger model, the non-detection of the optical/infrared emission of GRB 111005A requires a sub-relativistic neutron-rich ejecta with the mass of $leq 0.01~M_odot$, (significantly) less massive than that of GRB 130603B, GRB 060614 and GRB 050709. The lsGRBs are found to have a high rate density and the neutron star merger origin model can be unambiguously tested by the joint observations of the second generation gravitational wave (GW) detectors and the full-sky gamma-ray monitors such as Fermi-GBM and the proposing GECAM. If no lsGRB/GW association is observed in 2020s, alternative scenarios have to be systematically investigated. With the detailed environmental information achievable for the very-nearby events, a novel kind of merger or explosion origin may be identified." @default.
- W3100274681 created "2020-11-23" @default.
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- W3100274681 date "2017-12-08" @default.
- W3100274681 modified "2023-10-15" @default.
- W3100274681 title "GRB 111005A at z = 0.0133 and the Prospect of Establishing Long–Short GRB/GW Association" @default.
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- W3100274681 doi "https://doi.org/10.3847/2041-8213/aa9d7f" @default.
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