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56Ni Production in Long-lived Binary Neutron Star Merger Remnants

  • Authors: Maximilian Jacobi, Fabio Magistrelli, Eleonora Loffredo, Giacomo Ricigliano, Leonardo Chiesa, Sebastiano Bernuzzi, Albino Perego, Almudena Arcones

Maximilian Jacobi et al 2026 The Astrophysical Journal Letters 999 .

  • Provider: AAS Journals

Caption: Figure 1.

Top panel: mass-ejection rate for the considered BNS models. Bottom panel: 56Ni mass fraction that the fluid elements will achieve after 10 s as a function of their ejection time. The x-axis shows the time of ejection defined as the time at which the fluid elements cross the sphere at ∼450 km.

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