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- W3105803150 abstract "GW170817/GRB170817A probably marks a double neutron star coalescence. Extended Emission $t_ssimeq (0.67pm0.03)$,s post-merger shows an estimated energy output ${cal E}simeq (3.5pm1)%M_odot c^2$ determined by response curves to power-law signal injections, where $c$ is the velocity of light. It provides calorimetric evidence for a rotating black hole of $sim 3M_odot$, inheriting the angular momentum $J$ of the merged hyper-massive neutron star in the immediate aftermath of GW170817 following core-collapse about or prior to $t_s$. Core collapse greatly increases the central energy reservoir to $E_Jlesssim 1M_odot c^2$, accounting for ${cal E}$ even at modest efficiencies in radiating gravitational waves through a non axisymmetric thick torus. The associated multi-messenger output in ultra-relativistic outflows and sub-relativistic mass-ejecta is consistent with observational constraints from the GRB-afterglow emission of GRB170817A and accompanying kilonova." @default.
- W3105803150 created "2020-11-23" @default.
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- W3105803150 date "2019-04-25" @default.
- W3105803150 modified "2023-09-25" @default.
- W3105803150 title "Multi-messenger Extended Emission from the Compact Remnant in GW170817" @default.
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- W3105803150 doi "https://doi.org/10.3847/2041-8213/ab18a2" @default.
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