Hypermassive Neutron Stars 2

On the Properties of Hypermassive Neutron Stars Formed in Mergers of Spinning Binaries

Caption

Fig. 2: Gravitational wave signal of a merger of two NS with 1.5 solar masses each, assuming the Lattimer-Swesty EOS. The first part of the signal is caused the inspiral phase, the next stage is due to a hypermassive neutron star created in the merger, which then collapses to a BH (vertical line) responsible for the remaining signal (ring-down).

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