Investigating the detection rates and inference of gravitational-wave and radio emission from black hole neutron star mergers

Open Access

Fig. 2.

Same as Fig. 1 except now the final kinetic energy of the jet in Eq. (10) is visualised. The regions of the parameter space with no colour indicate either that M_disk = 0 or that the minimal accreted disk mass for sGRB creation, M_acc = 0.03 M_⊙, is not reached.

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