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High-energy emissions from neutron star mergers

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Figure

Figure 1.Neutrino fluences from extended emissions (EEs),plateau emission, prompt emission, and X-ray flare of SGRBsat the luminosity distance dL = 300 Mpc
Table 1. Used parameters for each component of SGRBs. Γ is the Lorentz factor of the jet, L∗γ,iso and E ∗γ,iso are the isotropic equivalentluminosity and energy fluence in the observed energy band, rdiss is the dissipation radius, Eγ,pk is the observed brea
Figure 2. Schematic picture of the choked jet system. This figureis reproduced from [20].
Table 4. The used parameters for the internal shock models.Lorentz factor of the downstream of the internal shocks,time from the ejecta (for model C), Lk,iso is the isotropic equivalent kinetic luminosity of the jets, Γ j is the tdur or tbois the duration

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